Introduction

Let F=Q(−3)F=\mathbb{Q}(\sqrt{-3}), let O\mathcal{O} be its ring of integers, and write Na=∣O/a∣N\mathfrak a=|\mathcal O/\mathfrak a| for the norm of a nonzero integral ideal. A finite-order Hecke character η\eta modulo a nonzero integral ideal f\mathfrak{f} is a character of the ray class group modulo f\mathfrak{f}, extended by zero to ideals not coprime to f\mathfrak{f}. This agrees with the usual finite-order idelic definition: the complex place contributes no nontrivial finite-order continuous character [22 Chapter VI, Section 1]. For ℜs>1\Re s>1, put

LF(s,η)=∑a≠0η(a)(Na)s=∏p(1−η(p)(Np)−s)−1.L_F(s,\eta)=\sum_{\mathfrak a\ne0} \frac{\eta(\mathfrak a)}{(N\mathfrak a)^s} =\prod_{\mathfrak p} \left(1-\eta(\mathfrak p)(N\mathfrak p)^{-s}\right)^{-1}.

The same notation denotes its meromorphic continuation. For a Dirichlet character χ\chi modulo qq, extended by zero on nonunits, we likewise write

L(s,χ)=∑n≥1χ(n)ns(ℜs>1).L(s,\chi)=\sum_{n\ge1}\frac{\chi(n)}{n^s}\qquad(\Re s>1).

and then continue meromorphically; the character modulo 11 gives the Riemann zeta function ζ(s)\zeta(s). The problem here is uniform exclusion: to find a constant σ0<1\sigma_0<1, independent of the character, its conductor, and the height, such that these functions have no zeros in ℜs>σ0\Re s>\sigma_0.

For ζ\zeta alone, the existence of a fixed σ0<1\sigma_0<1 for which ζ(s)≠0\zeta(s)\ne0 in ℜs>σ0\Re s>\sigma_0 is called the quasi-Riemann hypothesis [3 Section 1]. It asks for one gap valid at every height, not merely nonvanishing on ℜs=1\Re s=1. The corresponding uniform formulation over all Dirichlet characters appears in [9 p. 288, Equation (1.4) and the following paragraph].

The connection between these functions and prime distribution has a long history. Dirichlet’s 1837 proof of infinitude of primes in every reduced arithmetic progression introduced the character LL-series that separate residue classes [7]. Riemann’s 1859 memoir related the zeros of ζ\zeta to the distribution of primes and formulated the critical-line conjecture [25]. Hadamard and de la Vallée Poussin independently proved in 1896 that ζ\zeta has no zero on ℜs=1\Re s=1, obtaining the prime number theorem [15, 28]. Hecke subsequently developed the character zeta functions and their analytic theory over number fields [18].

Classical zero-free regions for Hecke LL-functions approach the line ℜs=1\Re s=1 as the conductor or height increases and can allow one simple real exceptional zero; a precise form for abelian extensions is given by [27 Theorem 3.1]. Such regions do not give uniform exclusion in a fixed half-plane. Zero-density estimates address a different question: they bound the number of zeros to the right of a given vertical line. For example, Guth and Maynard’s large-value estimates improve zero-density bounds for ζ\zeta [14 Theorem 1.2], but these zero-density bounds do not exclude every zero.

Theorem 1.1. Every finite-order Hecke LL-function over F=Q(−3)F=\mathbb{Q}(\sqrt{-3}) has no zero in ℜs>7/8\Re s>7/8. The same holds for every Dirichlet LL-function, including ζ(s)\zeta(s). A pole at s=1s=1 for a principal character is allowed.

In particular, Theorem 1.1 resolves the quasi-Riemann hypothesis affirmatively: the supremum of the real parts of the nontrivial zeros of ζ\zeta, namely its zeros in 0<ℜs<10<\Re s<1, is at most 7/87/8. The boundary ℜs=7/8\Re s=7/8 is not included, while any exceptional real zero in (7/8,1)(7/8,1) is excluded. The theorem does not establish the Riemann hypothesis or its generalized versions, which place nontrivial zeros on ℜs=1/2\Re s=1/2. The Riemann hypothesis remains open [5].

Kubota’s metaplectic theory and Patterson’s cubic theta series provide the automorphic setting [20, 24]. We use the unconditional explicit cusp expansions recorded by Dunn and Radziwiłł [8 Section 5 and Appendix A]; their GRH-conditional prime asymptotic is not an input. The corresponding first-moment asymptotic is proved unconditionally in an independent manuscript [23 Theorem 1.1]; that result is also not used here. Proposition 5.1 derives the reflection used here while retaining the characters’ zero-on-nonunit restrictions.

The character large-sieve arguments build on the quadratic Hecke-family estimate of Goldmakher and Louvel [13 Definition 1 and Theorem 1.1], the higher-order norm recursion of Blomer, Goldmakher, and Louvel [4 Theorem 1.3 and Section 3], and Heath-Brown’s cubic estimate [17 Theorem 2]. We prove the precise sextic specialization needed here in Lemma 9.1, using paired residue characters to carry out that recursion in the primary-generator convention. An Eisenstein-integer form is also recorded by Gao and Zhao [12 Lemma 2.9]. The recursive moment arguments are related to the framework of Heath-Brown’s quadratic method [16 Section 2]. We also use the ordinary Hecke functional equation [11 Equation (1.1)] and prime counting in a fixed ray class [27 Theorem 1.1].

The planar additive large sieve used in the first stage is classical; compare Huxley’s multivariable and number-field inequality [19] and the Poisson proof in [1 Section 3, Theorem 3]. We include a direct Eisenstein-lattice proof to record the normalization needed for the reduced-fraction expansion. David, de Faveri, Dunn, and Stucky combine Patterson’s coefficients, the cubic large sieve, and mollified moments to prove nonvanishing at s=1/2s = 1/2 for a positive proportion of a cubic Hecke family [6 Theorem 1.1 and Section 1.2]. The zero detector below uses the classical truncated-inverse mechanism; compare [21 Appendix C], and for a higher-order-character density application [4 Corollary 1.6 and Section 5].

The proof has two stages, each comparing two representations of a completed cubic-theta sum but using a different normalized sum in the continuation argument. Part I proves the corresponding 11/1211/12 assertion in Theorem 3.1, already obtaining a fixed zero-free half-plane for both families. Part II starts from that conclusion and introduces prime compensation, asymmetric scales, and two additional moment estimates. The contribution developed here is the construction of these compatible reflected and Poisson comparisons, including the principal residues, with positive exponent margins chosen independently of the target character.

Proof overview

A common continuation principle. The analytic argument begins with the family of primitive finite-order Hecke characters over FF. Let β∗\beta_* be the supremum of 1/21/2 and the real parts of their zeros in 1/2≤ℜs≤11/2 \le\Re s \le1; poles are not included. Imprimitive characters have the same possible zeros in ℜs>0\Re s > 0, because the finitely omitted Euler factors are nonzero there. If β∗\beta_* exceeds a proposed boundary σ0\sigma_0, the task is to continue every target reciprocal across a common positive distance to the left of β∗\beta_*.

Section 2 gives the precise criterion. For each target η\eta and large real scale ZZ, it compares a normalized character sum with a Mellin integral containing 1/LF(s,η)1/L_F(s,\eta), after deletion of finitely many Euler factors and multiplication by a holomorphic factor bounded away from zero. A direct bound for the sum and a power-saving bound for its difference from that integral imply the required continuation. The two parts use this same principle with different affine powers of ZZ in the Mellin integral:

CI(s)=s−23,CII(s)=s−1116.C_{\mathrm{I}}(s)=s-\frac{2}{3}, \qquad C_{\mathrm{II}}(s)=s-\frac{11}{16}.

Thus the common analytic principle does not identify the two normalized sums. Only the positive power margins must be independent of η\eta; fixed-character constants and lower thresholds may depend on it.

The completed sum. Section 4 sets up the sextic residue characters over O\mathcal{O}, always retaining their zero values on nonunits. The base sum in Section 6 averages smoothed cubic-theta Fourier coefficients against these characters and a fixed target η\eta. After the fixed rescaling in the theta expansion, the completed indices are cn3cn^3, where c,n∈Oc,n \in\mathcal{O} are congruent to 1 modulo 3 and cc is squarefree. The variables cc and nn may share prime factors. Here completion means retaining the full cubic factor n3n^3, rather than restricting the index to its squarefree part. The target character and a finite ray-class phase act on the whole product cn3cn^3, rather than separately on its two factors.

The resulting completed base sum has two exact representations. The reflection in Proposition 5.1 transforms its theta coefficients while retaining the character zeros in the resulting formula. Poisson summation transforms the averaging variable. Its nonzero frequencies have the form ua6ua^6, where u,a∈Ou,a \in\mathcal{O} and uu is sixth-power-free: every prime valuation of uu is at most five. Section 7.2 then expresses the contribution of each such row through a quotient of Hecke LL-functions and a controlled Euler product. For u=1u=1, this quotient contains the reciprocal of the target function.

The balanced first stage. In Part I, the two averaging scales are both Z1/2Z^{1/2}. On the reflected side, the base sum separates into a completed theta row and an additive polynomial. The quadratic large sieve bounds the mean square of the reflected rows. Expanding the additive polynomial produces reduced fractions in C/O\mathbb{C}/\mathcal{O}; their separation and coefficient mass give the required planar large-sieve bound. The Cauchy–Schwarz inequality combines the two norms in Proposition 6.3. This direct estimate does not use the later inverse-moment recursion.

On the Poisson side, the intermediate rows are grouped by their norm and by the location of zeros in bounded-height rectangles for the finite family of Hecke twists that each row determines. Section 8 assigns zero-free rectangles to these families. When a row has a selected zero above the detector’s fixed floor for the real part, it produces two large Dirichlet polynomials: one with ideal Möbius coefficients, representing a truncated reciprocal, and one without those coefficients. They have one common row character and one common twist height. Part I uses only the inverse polynomial in its row count. After the part of the row with prime valuations at least two is fixed, the sextic large sieve applies to its squarefree factor; Proposition 9.2 gives the resulting count. Rows at the floor and the remaining small and large norm ranges are bounded directly.

The principal row is treated separately. Its residues, together with the local Euler identity, give a nonzero scalar multiple of the target Mellin integral. After normalization, the direct estimate and the remaining-row estimate verify the common continuation criterion with CI(s)=s−2/3C_{\mathrm{I}}(s)=s-2/3. This proves Theorem 3.1. The entire family is needed even for the consequence about ζ\zeta, because the Poisson rows introduce finite-order Hecke twists of the target.

The refined second stage. Part II retains the completed support and the shared arithmetic identities, but it modifies the base sum. Selected prime factors provide a local compensation that cancels an unwanted Euler contribution, and the two averaging scales are no longer equal. After the new residue calculation and scalar normalization, the corresponding Mellin signal uses CII(s)=s−11/16C_{\mathrm{II}}(s)=s-11/16. The low estimate for the normalized sum again follows directly from reflected energy and an additive mean-square estimate; Section 15 proves it for the modified sum.

The high estimate uses both polynomials supplied by the zero detector. For a smooth compactly supported WW on (0,∞)(0,\infty), a scale D>0D>0, and a finite-order Hecke character ψ\psi, their basic forms are

D−1/2∑a≠0μ(a)ψ(a)W(Na/D),D−1/2∑a≠0ψ(a)W(Na/D),D^{-1/2}\sum_{\mathfrak a\ne0}\mu(\mathfrak a)\psi(\mathfrak a) W(N\mathfrak a/D),\qquad D^{-1/2}\sum_{\mathfrak a\ne0}\psi(\mathfrak a)W(N\mathfrak a/D),

where μ\mu is the ideal Möbius function. In the specified intermediate norm ranges above the detector floor, each retained row has a large inverse polynomial and a large plain polynomial with one common row character and twist height. Bounds for their moments limit the number of such rows. Section 19 combines the two bounds, using integer powers and selected prime factors in the larger intermediate norm ranges. Small and large norm ranges, and the floor class, remain direct estimates.

The two moment bounds require separate inductions. Section 17 proves the second-moment estimate for an inverse polynomial multiplied by sums over disjoint prime sets (Lemma 17.1). Its recursive step uses two finite Poisson transformations to shorten the row range, with reflected energy providing the terminal bound. Section 18 proves a mean-square estimate for products of two plain polynomials, again with permitted prime factors (Lemma 18.1). Ordinary Hecke reflection reduces the length ranges at each stage; the recursive step uses two finite Poisson transformations.

The plain estimate retains different row families according to whether prime factors are present. With them, it excludes rows whose primitive inducing character belongs to the fixed finite group generated by the target and the auxiliary ray characters; without them, it excludes only principal inducing characters. Transformed rows in that finite family are treated separately within the induction. Direct volume bounds handle uncentered products. For a difference of two products with the same two profiles and equal products of scales, the common main terms cancel. This cancellation is used only for that centered expression, not for every row in the finite inducing-character family.

Section 20 combines the resulting row counts with the compensated expansion, its local errors, the contour tails, and the principal residue. After normalization, their bound verifies the second comparison in the continuation criterion at 7/87/8.

Transfer to Dirichlet LL-functions. The final transfer is the same at both boundaries. Composing a Dirichlet character χ\chi with the ideal norm gives a Hecke character over FF. Away from finitely many Euler factors, quadratic factorization writes its LL-function as the product of the Dirichlet LL-functions attached to χ\chi and to χχ−3\chi\chi_{-3}, where χ−3\chi_{-3} is the quadratic character of F/QF/\mathbb{Q}. The omitted factors are nonzero in ℜs>0\Re s > 0, and the principal pole is handled separately. Thus each Hecke half-plane transfers to all Dirichlet characters, completing the two stages.

Least nonresidues and square roots over prime fields

The fixed Dirichlet zero-free half-plane also makes the following classical consequences unconditional.

Corollary 1.2. There are absolute constants A,C>0A,C>0 such that, for every odd prime pp, the least positive quadratic nonresidue n(p)n(p) satisfies

n(p)≤C(log⁡p)A.n(p) \le C(\log p)^A.

In particular, n(p)≪δpδn(p) \ll_{\delta} p^{\delta} for every δ>0\delta>0, proving Vinogradov’s least quadratic nonresidue conjecture [26 Conjecture 1.1] [Conjecture 1.1]. Given an odd prime pp and a∈Fpa \in\mathbb{F}_p in binary representation, there is a deterministic algorithm, with running time polynomial in log⁡p\log p, that returns a square root of aa or reports that none exists.

Proof. By Theorem 1.1 and the functional equation, the nontrivial zeros of every primitive Dirichlet LL-function lie in 1/8≤ℜs≤7/81/8 \le\Re s \le7/8. They therefore lie in the strictly larger strip 1/16<ℜs<15/161/16 < \Re s < 15/16. This supplies the weak-GRH hypothesis of Bhargava, Ivanyos, Mittal, and Saxena [2 Conjecture 6.3 and Theorem 6.7] with ϵ=7/16\epsilon=7/16. Their bound for the least quadratic nonresidue gives the asserted inequality, for example with A=32A=32; no optimization is needed here. The assertion for each δ>0\delta>0 follows because every fixed power of log⁡p\log p is Oδ(pδ)O_{\delta}(p^{\delta}).

For the algorithm, first handle a=0a=0 and test a nonzero aa by Euler’s criterion. If aa is a square, scan 2,3,…2,3,\ldots until a quadratic nonresidue is found, testing each candidate by its Legendre symbol. The bound just proved makes this a polynomial-time deterministic search; its stopping rule does not require knowing CC. Use the resulting nonresidue in the Tonelli–Shanks algorithm [10 Section 2.9, Algorithm 3 and Lemma 2.9.5]. All remaining steps are deterministic and polynomial in log⁡p\log p. Writing p−1=2eup-1=2^e u with uu odd only requires removing factors of two, not factoring uu. ☐

From a common signal to a zero-free half-plane

Both parts of the proof use the same analytic principle. A character sum is bounded directly and is also compared with a Mellin integral containing the reciprocal of a target LL-function. A power saving in both comparisons then continues that reciprocal across the rightmost possible zeros. We prove this principle for a variable boundary, so that it can be applied at 11/1211/12 and at 7/87/8 without repeating the argument.

Throughout the paper, F=Q(−3)F = \mathbb{Q}(\sqrt{-3}). It suffices to consider primitive target characters. Indeed, a character induced from a primitive character η\eta has LL-function differing from LF(s,η)L_F(s,\eta) by finitely many factors 1−η(p)Np−s1-\eta(\mathfrak{p})N\mathfrak{p}^{-s}, all nonzero for ℜs>0\Re s > 0. Define

β∗=sup⁡({1/2}∪{ℜρ:12≤ℜρ≤1, LF(ρ,η)=0 for some primitive finite-order Hecke character η}).\beta_* = \sup\left(\{1/2\}\cup\left\{\Re\rho:\frac{1}{2}\le\Re\rho\le1,\ L_F(\rho,\eta)=0\text{ for some primitive finite-order Hecke character }\eta\right\}\right).

Poles are not included. Absolute convergence of the Euler product excludes zeros in ℜs>1\Re s > 1, so 1/2≤β∗≤11/2\le\beta_*\le1.

For a finite set S\mathcal{S} of prime ideals, a superscript S\mathcal{S} means that the corresponding Euler factors have been deleted:

LFS(s,η)=LF(s,η)∏p∈S(1−η(p)Np−s).L_F^{\mathcal{S}}(s,\eta)=L_F(s,\eta)\prod_{\mathfrak{p}\in\mathcal{S}}\left(1-\eta(\mathfrak{p})N\mathfrak{p}^{-s}\right).

The local value is zero at a ramified prime. Each displayed factor is nonzero for ℜs>0\Re s > 0, so deleting finitely many factors neither creates nor removes a zero there.

Proposition 2.1 (Continuation from a common signal). Fix σ0∈(1/2,1)\sigma_0\in(1/2,1) and suppose Δ0=β∗−σ0>0\Delta_0=\beta_*-\sigma_0>0. Let C(s)=s+cC(s)=s+c, where c∈Rc\in\mathbb{R} is fixed. Suppose that numbers ω,σ\omega,\sigma satisfying

0<ω<Δ0,σ>00<\omega<\Delta_0,\qquad\sigma>0

can be chosen independently of the target character. For every primitive finite-order Hecke character η\eta, suppose there exist a finite set S\mathcal{S}, a holomorphic function HηH_\eta on ℜs>σ0\Re s>\sigma_0, and a function Jη(Z)J_\eta(Z) defined for all sufficiently large real ZZ, such that

sup⁡ℜs>σ0∣Hη(s)−1∣≤12.\sup_{\Re s>\sigma_0}|H_\eta(s)-1|\le\frac{1}{2}.

For Z>0Z>0, define

fη(Z)=12πi∫ℜs=2ZC(s)e(s−5/6)2Hη(s)LFS(s,η) ds.f_\eta(Z)=\frac{1}{2\pi i}\int_{\Re s=2}Z^{C(s)}e^{(s-5/6)^2}\frac{H_\eta(s)}{L_F^{\mathcal{S}}(s,\eta)}\,ds.

Assume that, as Z→∞Z\to\infty,

∣Jη(Z)∣≪ηZC(σ0)+ω,|J_\eta(Z)|\ll_\eta Z^{C(\sigma_0)+\omega},
∣Jη(Z)−fη(Z)∣≪ηZC(β∗)−σ.|J_\eta(Z)-f_\eta(Z)|\ll_\eta Z^{C(\beta_*)-\sigma}.

The implied constants, lower thresholds, excluded set, and function HηH_\eta may depend on η\eta. Then these assumptions contradict β∗>σ0\beta_*>\sigma_0.

Proof. Put

ϵ∗:=min⁡{Δ0−ω,σ}>0.\epsilon_*:=\min\{\Delta_0-\omega,\sigma\}>0.

Because CC has slope one, the triangle inequality gives

∣fη(Z)∣≪ηZC(β∗)−ϵ∗(Z≥Z0,η).|f_\eta(Z)|\ll_\eta Z^{C(\beta_*)-\epsilon_*}\qquad(Z\ge Z_{0,\eta}).

Moreover ϵ∗≤Δ0−ω<Δ0\epsilon_*\le\Delta_0-\omega<\Delta_0, so β∗−ϵ∗>σ0\beta_*-\epsilon_*>\sigma_0. We also need control as Z↓0Z \downarrow0. By (2.2), HηH_\eta is bounded on ℜs>σ0\Re s > \sigma_0. The reciprocal Euler product is absolutely and uniformly bounded on ℜs≥2\Re s \ge2. On every fixed strip 2≤ℜs≤B2 \le\Re s \le B, the Gaussian in (2.3) is OB(e−(ℑs)2)O_B(e^{-(\Im s)^2}). Cauchy’s theorem on rectangles therefore moves the contour to any fixed B>2B > 2, with horizontal integrals tending to zero. Hence

∣fη(Z)∣≪η,BZB+c(0<Z≤1).\lvert f_\eta(Z)\rvert\ll_{\eta,B} Z^{B+c} \qquad(0 < Z \le1).

Since BB is arbitrary, the signal has arbitrarily rapid power decay at zero. This bound and (2.6) show that

Fη(s):=∫0∞fη(Z)Z−C(s)dZZF_\eta(s) := \int_0^\infty f_\eta(Z)Z^{-C(s)}\frac{dZ}{Z}

converges locally uniformly on ℜs>β∗−ϵ∗\Re s > \beta_* - \epsilon_*. On each compact subset, choose BB larger than all occurring real parts for the integral near zero, and use (2.6) near infinity. Thus FηF_\eta is holomorphic on that half-plane.

We identify this Mellin transform without moving a contour across a zero. Set

Aη(s)=e(s−5/6)2Hη(s)LFS(s,η)(ℜs>1).A_\eta(s)=e^{(s-5/6)^2} \frac{H_\eta(s)}{L_F^{\mathcal S}(s,\eta)} \qquad(\Re s>1).

The function Aη(2+it)A_\eta(2+it) is continuous and integrable in tt. Writing Z=euZ=e^u, (2.3) becomes

e−(2+c)ufη(eu)=12π∫ReituAη(2+it) dt.e^{-(2+c)u}f_\eta(e^u)=\frac{1}{2\pi}\int_{\mathbb{R}}e^{itu}A_\eta(2+it)\,dt.

The left side is integrable in uu by the two endpoint estimates. Ordinary Fourier inversion therefore gives Fη(2+it)=Aη(2+it)F_\eta(2+it)=A_\eta(2+it) for every real tt. Both sides are holomorphic on ℜs>1\Re s > 1, so the identity theorem gives

Fη(s)=e(s−5/6)2Hη(s)LFS(s,η)(ℜs>1).F_\eta(s)=e^{(s-5/6)^2} \frac{H_\eta(s)}{L_F^{\mathcal S}(s,\eta)} \qquad(\Re s>1).

(2.2) implies ∣Hη(s)∣≥1/2\lvert H_\eta(s)\rvert\ge1/2 on ℜs>σ0\Re s > \sigma_0. Consequently

e−(s−5/6)2Fη(s)Hη(s)(ℜs>β∗−ϵ∗)e^{-(s-5/6)^2}\frac{F_\eta(s)}{H_\eta(s)} \qquad(\Re s > \beta_*-\epsilon_*)

is a holomorphic continuation of 1/LFS(s,η)1/L_F^{\mathcal S}(s,\eta). The number ϵ∗\epsilon_* was chosen independently of η\eta. By the definition of β∗\beta_*, some target has a zero ρ\rho with ℜρ>β∗−ϵ∗\Re\rho> \beta_*-\epsilon_*. Its reciprocal has a pole at ρ\rho, and the deleted factors are nonzero there. This contradicts the continuation.

The high estimate in Proposition 2.1 is measured relative to C(β∗)C(\beta_*), not to C(σ0)C(\sigma_0). This distinction matters when a row contribution reaches the low scale but still has a power saving relative to the hypothetical rightmost zero. Part I uses

σ0=1112,C(s)=s−23,C(σ0)=14.\sigma_0=\frac{11}{12},\qquad C(s)=s-\frac{2}{3},\qquad C(\sigma_0)=\frac{1}{4}.

whereas Part II uses

σ0=78,C(s)=s−1116,C(σ0)=316.\sigma_0=\frac{7}{8},\qquad C(s)=s-\frac{11}{16},\qquad C(\sigma_0)=\frac{3}{16}.

Only the positive power margins must be uniform in the target. Fixed-character constants, excluded sets, and sufficiently large lower thresholds may depend on it in both applications.

Part I

The quasi-Riemann hypothesis

A first zero-free half-plane

We first prove a fixed zero-free half-plane using the basic completed cubic-theta sum. This isolates the mechanism that excludes zeros before the additional estimates needed for the sharper boundary are introduced.

Theorem 3.1 (The 11/12 half-plane). Every finite-order Hecke LL-function over F=Q(−3)F = \mathbb{Q}(\sqrt{-3}) has no zero in ℜs>11/12\Re s > 11/12. The same holds for every Dirichlet LL-function, including ζ(s)\zeta(s). A pole at s=1s = 1 for a principal character is allowed.

For the Hecke assertion, suppose for contradiction that

Δ1:=β∗−1112>0.\Delta_1 := \beta_* - \frac{11}{12} > 0.

The proof will construct one character sum with two exact representations. Cubic-theta reflection bounds the sum after an elementary additive large-sieve estimate. Poisson summation expresses the same sum as a principal Mellin signal and a family of remaining character rows. A zero detector and the sextic large sieve control those rows. These estimates verify Proposition (2.1) with boundary 11/1211/12.

The fixed family in Equation (2.1) is essential even when the desired consequence concerns ζ\zeta: the Poisson representation introduces finite-order Hecke twists of the target. Proving the family-wide assertion also supplies the precise input used at the beginning of Part II.

Arithmetic and analytic preliminaries

The two parts use the same arithmetic conventions and analytic estimates. This section fixes the residue symbols, retaining their zero values even for principal powers, and proves the Gauss and reciprocity identities used to transform character sums. It then establishes a calculus for smooth norm profiles and uniform bounds for a Hecke LL-function on a disk known to be zero-free. These are the common preliminaries for the balanced argument.

Arithmetic notation and coefficient classes

Let F=Q(−3)F = \mathbb{Q}(\sqrt{-3}), let ω=e2πi/3\omega= e^{2\pi i/3}, and put

O=Z[ω],λ=−3=ω−ω2=1+2ω.\mathcal{O} = \mathbb{Z}[\omega], \qquad\lambda= \sqrt{-3} = \omega- \omega^2 = 1 + 2\omega.

For an element aa write qa=∣a∣2=NF/Q(a)q_a = |a|^2 = N_{F/\mathbb{Q}}(a), and for a≠0a \ne0 write α(a)=a/∣a∣\alpha(a) = a/|a|. The same notation qaq_{\mathfrak a} denotes the norm of a nonzero ideal. The ring O\mathcal{O} is Euclidean for this norm: a point of C\mathbb{C} is at distance at most 1/3<11/\sqrt{3} < 1 from the triangular lattice O\mathcal{O}, which gives Euclidean division. In particular every ideal is principal. The six units are {±1,±ω,±ω2}\{\pm1, \pm\omega, \pm\omega^2\}, and their images are the six units of O/3O\mathcal{O}/3\mathcal{O}. Consequently every ideal coprime to 33 has a unique generator congruent to 11 (mod 33); we call this generator primary. Products of primary generators are primary.

In the character-polynomial estimates below, a row is an outer index for a character polynomial, while a column is an ideal index, or a tuple of ideal indices, summed inside it. A label is an auxiliary index distinguishing parts of the family. Whether a label is averaged or locally frozen refers to the current sum; freezing it does not make it part of the fixed arithmetic datum.

For the arithmetic datum in any given invocation, fix from the outset a finite set SS of prime ideals containing the primes above 66 and the prime supports of the defining moduli of every finite-order character presentation in that datum and of the fixed finite ray group used to present them. For a character presentation, its defining-modulus support consists exactly of the primes at which it is extended by zero, including any redundant primes of an imprimitive presentation. A fixed character includes its entire zero-extended presentation and the finite ray group through which it is presented, all fixed independently of ZZ, the current rows, and the averaged labels. The fixed datum may depend on a target fixed beforehand. In particular every such character has modulus one at every prime outside SS. We also write S=S\mathcal{S}=S. We call primes outside SS good, and call an ideal good if all its prime divisors lie outside SS. Unless a different support is specified, ideal sums exclude SS and use primary generators. We write “sf” for squarefree and μ\mu for the ideal Möbius function. Element rows, in contrast, may have arbitrary prime powers and unit factors.

For z∈Fz\in F define

e(z)=exp⁡(2πiTr⁡F/Q(z/λ)).e(z)=\exp(2\pi i\operatorname{Tr}_{F/\mathbb{Q}}(z/\lambda)).

Its extension to C\mathbb{C} is e(z)=exp⁡(4πiIm⁡z/3)e(z)=\exp(4\pi i\operatorname{Im}z/\sqrt{3}). The measure dμ(z)=(2/3) dx dyd\mu(z)=(2/\sqrt{3})\,dx\,dy makes O\mathcal{O} self-dual for the pairing (z,y)↦e(zy)(z,y)\mapsto e(zy). Indeed, writing y=u+vωy=u+v\omega with real u,vu,v, the conditions e(y)=e(ωy)=1e(y)=e(\omega y)=1 say v,u−v∈Zv,u-v\in\mathbb{Z}, hence y∈Oy\in\mathcal{O}; and the covolume of O\mathcal{O} for dμd\mu is one. Lattice point counting in a disk, followed by division by the six units, gives the unrestricted ideal count

#{a:qa≤H}=πH33+O(H+1)(H≥0).\#\{\mathfrak{a}:q_{\mathfrak{a}}\le H\}=\frac{\pi H}{3\sqrt{3}}+O(\sqrt{H}+1)\qquad(H\geq0).

For example, the error follows by covering the boundary of the disk with O(H+1)O(\sqrt{H}+1) fixed fundamental parallelograms.

If p∉Sp\notin S is prime, its residue field has order P=qp≡1(mod6)P=q_p\equiv1\pmod6: the six roots of unity remain distinct in that field. Define the sextic symbol χp(a)=(a/p)6\chi_p(a)=(a/p)_6 to be the unique sixth root of unity satisfying

χp(a)≡a(P−1)/6(modp)(p∤a),χp(a)=0(p∣a).\chi_p(a)\equiv a^{(P-1)/6}\pmod p\quad(p\nmid a), \qquad \chi_p(a)=0\quad(p\mid a).

For a primary c=∏pvp(c)c=\prod p^{v_p(c)} outside SS, define χc(a)=∏p∣cχp(a)vp(c)\chi_c(a)=\prod_{p\mid c}\chi_p(a)^{v_p(c)}, and put χ1(a)=1\chi_1(a)=1 for every aa. For every integer jj, including j=0j=0 and negative jj, the notation χc(a)j\chi_c(a)^j means its usual power when (a,c)=1(a,c)=1 and means zero otherwise. Thus an exponent divisible by six is the function 1(a,c)=11_{(a,c)=1}, not the constant function one. The square χc2\chi_c^2 is the cubic symbol. For squarefree cc set

γj(c)=qc−1/2∑v mod cχc(v)je(v/c),γj(1)=1.\gamma_j(c)=q_c^{-1/2}\sum_{v\bmod c}\chi_c(v)^j e(v/c), \qquad \gamma_j(1)=1.

Lemma 4.1 (Fixed numerators give ray characters). Fix 0≠a∈O0\ne a\in\mathcal{O}. At a prime ideal p∤6a\mathfrak{p}\nmid6a, let (a/p)6(a/\mathfrak{p})_6 be the unique sixth root of unity congruent to a(qp−1)/6(modp)a^{(q_{\mathfrak{p}}-1)/6}\pmod{\mathfrak{p}}; at a prime outside SS this is χp(a)\chi_p(a). The extension F(a1/6)/FF(a^{1/6})/F is finite abelian and unramified outside the primes dividing 6a6a, and

Frob⁡p(a1/6)a1/6=(a/p)6,\frac{\operatorname{Frob}_{\mathfrak{p}}(a^{1/6})}{a^{1/6}}=(a/\mathfrak{p})_6,

where Frob⁡p\operatorname{Frob}_{\mathfrak{p}} is arithmetic Frobenius. Hence the multiplicative extension of this symbol to ideals coprime to 6a6a is a finite-order ray character whose conductor is supported on the primes dividing 6a6a. No bound on its conductor exponents at those primes is asserted. This identification is only on ideals coprime to 6a6a; it does not erase the prescribed zero of χA(a)\chi_A(a) when a good ideal AA meets aa.

In particular, choose one generator πp\pi_{\mathfrak{p}} for each p∈S\mathfrak{p}\in S. On primary ideals outside SS, the characters

A⟼χA(u∏p∈Sπpvp),u∈O×,vp≥0,A\longmapsto\chi_A\left(u\prod_{\mathfrak{p}\in S}\pi_{\mathfrak{p}}^{v_{\mathfrak{p}}}\right),\qquad u\in\mathcal{O}^{\times},\quad v_{\mathfrak{p}}\geq0,

belong to one finite family of ray characters with a common modulus supported on SS; this family is determined by uu and the residues vp(mod6)v_{\mathfrak{p}}\pmod{6}.

Proof. Let ξ6=a\xi^6=a. Since FF contains all sixth roots of unity, all roots of X6−aX^6-a lie in F(ξ)F(\xi), and σ↦σ(ξ)/ξ\sigma\mapsto\sigma(\xi)/\xi embeds its Galois group into μ6\mu_6. The extension is therefore abelian. A prime outside 6a6a is unramified; for example this follows from the discriminant of X6−aX^6-a, which is supported on 6a6a. At such a prime, arithmetic Frobenius is characterized on the residue field by x↦xqpx\mapsto x^{q_{\mathfrak p}}. Consequently its quotient on ξ\xi reduces to a(qp−1)/6a^{(q_{\mathfrak p}-1)/6}. Reduction is injective on μ6\mu_6 outside 66, proving the displayed identity. Multiplicativity of the Artin map gives the assertion for ideals. Artin reciprocity makes this map factor through a ray group with modulus supported on the primes dividing 6a6a; these are the power-residue and ray-group assertions in [22 Chapter VIII, (5.3) and (5.5)]].

For the last statement, an ideal AA outside SS is coprime to every πp\pi_{\mathfrak p} and to every unit. Its symbol therefore has no zero there, and the power of each χA(πp)∈μ6\chi_A(\pi_{\mathfrak p})\in\mu_6 depends only on vpv_{\mathfrak p} (mod 6). There are at most 6∣S∣+16^{|S|+1} possible displayed numerators after this reduction. Apply the first assertion to each and take a common multiple of their ray moduli. Their prime supports are all contained in SS because SS contains the primes above 6.

The word fixed in this lemma is essential: a numerator containing a moving good prime does not thereby enter a ray group fixed independently of ZZ. Its character and its natural zero support remain moving data.

At a base Z>1Z>1, a plain polynomial of real log-length nn is

Sψ(n;W)=Z−n/2∑lψ(l)W(ql/Zn),S_\psi(n;W)=Z^{-n/2}\sum_l\psi(l)W(q_l/Z^n),

and the centrally normalized inverse polynomial of log-length rr is

Mψ(r;W)=Z−r/2∑nμ(n)ψ(n)W(qn/Zr).M_\psi(r;W)=Z^{-r/2}\sum_n\mu(n)\psi(n)W(q_n/Z^r).

Every mask in ψ\psi is retained in both definitions. At base UU, when ψ(n)=ν(n)χn(u)\psi(n)=\nu(n)\chi_n(u), we also denote the latter polynomial by Mu(Ur;W)M_u(U^r;W), or by Mu(D;W)M_u(D;W) when D=UrD=U^r.

An annular test is a smooth function with support in a fixed compact subinterval of (0,∞)(0,\infty). Families of annular or coupled profiles are used only with fixed logarithmic support and uniform bounds for every logarithmic derivative that is invoked. The precise separation norm is given in Lemma 4.5. In a product of two plain factors, both factors have the same row character, including the same fixed finite-ray twist. Conjugating a whole factor inside its absolute value permits the opposite orientation; conjugating only part of its coefficients does not.

We use the following uniformity convention. Log-lengths range over fixed bounded sets, and every estimate allows any specified positive power loss. The exponents of the norm scales depend only on those real parameter ranges, the strict margins, and the specified losses. Write A\mathcal A for this fixed arithmetic datum: the complete zero-extended presentations of the fixed finite characters, their defining moduli and the fixed finite ray group used to present them, the excluded set, and any fixed arithmetic normalization. It is chosen independently of ZZ, the current rows, and the averaged labels, though it may depend on a previously fixed target. Finite seminorm orders, polynomial height orders, implied constants, and lower thresholds may depend on A\mathcal A. They are uniform over the declared moving moduli and outer labels in their stated ranges, even when an outer label is fixed during one row sum.

For a nonzero ideal a\mathfrak a, let dO(a)=#{d:d∣a}d_{\mathcal O}(\mathfrak a)=\#\{\mathfrak d:\mathfrak d\mid\mathfrak a\}, where the count includes all integral ideal divisors, including those meeting SS, and for 0≠f∈O0\ne f\in\mathcal O put dO(f)=dO((f))d_{\mathcal O}(f)=d_{\mathcal O}((f)). A nonnegative multiplicity w(f)w(f) is called divisor-bounded only if

w(f)≤C dO(f)Cw(f)\le C\,d_{\mathcal O}(f)^C

for one fixed C≥1C\ge1, independent of ZZ, the current rows, and the averaged labels. The constant CC may depend on A\mathcal A. This convention does not relax any separate condition that ww depend only on ff. For every δ>0\delta> 0 it implies w(f)≪C,δqfδw(f) \ll_{C,\delta} q_f^\delta uniformly. Indeed, for prime ideals p\mathfrak{p} of sufficiently large norm, (e+1)C≤qpδe(e+1)^C \le q_{\mathfrak{p}}^{\delta e} for every integer e≥0e \ge0, by e+1≤2ee+1 \le2^e for e≥1e \ge1. For each of the finitely many remaining prime ideals, sup⁡e≥0(e+1)Cqp−δe<∞\sup_{e\ge0}(e+1)^Cq_{\mathfrak{p}}^{-\delta e}<\infty; multiplying these bounds over the prime factorization of ff proves the assertion.

Gauss sums and the finite reciprocity phase

We first evaluate the prime Gauss sums. This also fixes the orientation of the cubic symbol in all subsequent formulas.

Lemma 4.2 (Prime Gauss identities). Let pp be the primary generator of a prime ideal outside SS, and put H=χpH=\chi_p and P=qpP=q_p. Then

γ2(p)3=−α(p),γ1(p)γ2(p)=H(4)‾γ3(p)γ2(p)3.\gamma_2(p)^3=-\alpha(p),\qquad\gamma_1(p)\gamma_2(p)=\overline{H(4)}\gamma_3(p)\gamma_2(p)^3.

For j≢0(mod6)j\not\equiv0\pmod6, one has ∣γj(p)∣=1|\gamma_j(p)|=1.

Proof. Let k=O/(p)k=\mathcal O/(p) and let ψ(x)=e(x/p)\psi(x)=e(x/p) be its nontrivial additive character. For a multiplicative character AA of k×k^\times, extended by zero, put

τ(A)=∑x∈kA(x)ψ(x),J(A,B)=∑x∈kA(x)B(1−x).\tau(A)=\sum_{x\in k}A(x)\psi(x),\qquad J(A,B)=\sum_{x\in k}A(x)B(1-x).

If AA is nonprincipal, the change of variables x=tyx=ty gives

∣τ(A)∣2=∑t∈k×A(t)∑y∈k×ψ((t−1)y)=P.|\tau(A)|^2=\sum_{t\in k^\times}A(t)\sum_{y\in k^\times}\psi((t-1)y)=P.

The inner sum is P−1P-1 for t=1t=1 and −1-1 otherwise, and ∑t∈k×A(t)=0\sum_{t\in k^\times}A(t)=0. Conjugation also gives τ(A)τ(A‾)=A(−1)P\tau(A)\tau(\overline A)=A(-1)P. When ABAB is nonprincipal, grouping the product τ(A)τ(B)\tau(A)\tau(B) by x+yx+y gives

τ(A)τ(B)=J(A,B)τ(AB).\tau(A)\tau(B)=J(A,B)\tau(AB).

The group with x+y=0x+y=0 vanishes because ABAB is nonprincipal; for a nonzero sum, division by x+yx+y gives the displayed Jacobi factor. In particular ∣J(A,B)∣=P|J(A,B)|=\sqrt{P} if A,B,ABA,B,AB are all nonprincipal.

The number of solutions of 4x(1−x)=y4x(1-x)=y is 1+H3(1−y)1+H^3(1-y). Summing H(y)H(y) times this identity and using ∑yH(y)=0\sum_yH(y)=0 gives J(H,H3)=H(4)J(H,H)J(H,H^3)=H(4)J(H,H). Write τj=τ(Hj)\tau_j=\tau(H^j). The Gauss–Jacobi identity and τ2τ4=P\tau_2\tau_4=P now give

τ1τ3τ4=H(4)τ12τ2,τ1τ2=H(4)‾τ3τ23P.\frac{\tau_1\tau_3}{\tau_4} =H(4)\frac{\tau_1^2}{\tau_2},\qquad \tau_1\tau_2=\overline{H(4)}\frac{\tau_3\tau_2^3}{P}.

Here H2(−1)=1H^2(-1)=1 because −1-1 is a cube.

It remains to fix the cubic Jacobi sum, including its unit. Put m=(P−1)/3m=(P-1)/3. The definition of H2H^2 gives, in kk,

J(H2,H2)≡∑x∈kxm(1−x)m=0(modp).J(H^2,H^2)\equiv\sum_{x\in k}x^m(1-x)^m=0\pmod p.

Indeed the polynomial has degree 2m<P−12m<P-1, and the sum over kk of each monomial of degree less than P−1P-1 is zero in kk (the constant case is P=0P=0 in kk). The Jacobi sum belongs to O\mathcal O and has absolute value P\sqrt{P}.

For x≠0,1x\ne0,1, choose jx∈{0,1,2}j_x\in\{0,1,2\} such that H2(x(1−x))=ωjxH^2(x(1-x))=\omega^{j_x}. The products of xx and of 1−x1-x over these xx are both −1-1, so ∏x≠0,1x(1−x)=1\prod_{x\ne0,1}x(1-x)=1. Hence ∑x≠0,1jx≡0(mod3)\sum_{x\ne0,1}j_x\equiv0\pmod3. Since

ωj≡1+j(ω−1)(mod(ω−1)2),((ω−1)2)=(3),\omega^j\equiv1+j(\omega-1)\pmod{(\omega-1)^2},\qquad((\omega-1)^2)=(3),

we obtain J(H2,H2)≡P−2≡−1(mod3)J(H^2,H^2) \equiv P-2 \equiv-1 \pmod{3}. Divisibility by pp and equality of norms imply J(H2,H2)=upJ(H^2,H^2)=up for a unit uu. As pp is primary and the six units have distinct residues modulo 33, the congruence forces u=−1u=-1. Finally, τ23=J(H2,H2)τ2τ4=−pP\tau_2^3=J(H^2,H^2)\tau_2\tau_4=-pP. Dividing the two Gauss identities by the appropriate powers of P\sqrt{P} proves the lemma.

The remaining phase is quadratic. Its evaluation below is valid even for odd elements that are not squarefree or primary.

Lemma 4.3 (Quadratic four-term formula). For a nonzero odd c∈Oc \in\mathcal{O}, define

Γ(c)=∣c∣−1∑x mod ce(x2/c).\Gamma(c)=|c|^{-1}\sum_{x\bmod c}e(x^2/c).

Then

Γ(c)=12∑y mod 2Oe(−cy2/4)\Gamma(c)=\frac{1}{2}\sum_{y\bmod2\mathcal{O}}e(-cy^2/4)

For c=a+bωc=a+b\omega the right side is (1+i−b+ia+ib−a)/2(1+i^{-b}+i^a+i^{b-a})/2. In particular Γ\Gamma depends only on c mod 4Oc\bmod4\mathcal{O} and Γ(cv2)=Γ(c)\Gamma(cv^2)=\Gamma(c) for every odd vv. The units modulo 44 have square subgroup {1,ω,ω2}\{1,\omega,\omega^2\} and square-class representatives 1,−1,λ,−λ1,-1,\lambda,-\lambda. The function Γ\Gamma never vanishes on these units, and r(a,b)=Γ(ab)/(Γ(a)Γ(b))\mathfrak r(a,b)=\Gamma(ab)/(\Gamma(a)\Gamma(b)) satisfies

cc11−1-1λ\lambda−λ-\lambda
Γ(c)\Gamma(c)1111ii−i-i
r((−1)eλf,(−1)gλh)=(−1)eh+fg+fh,e,f,g,h∈{0,1}.\mathfrak{r}((-1)^e\lambda^f,(-1)^g\lambda^h)=(-1)^{eh+fg+fh},\qquad e,f,g,h\in\{0,1\}.

Thus ∣Γ(c)∣=1|\Gamma(c)|=1 and r\mathfrak{r} is a symmetric {±1}\{\pm1\}-valued bicharacter of the square-class group.

Proof. Use the Fourier transform with kernel e(−zy)e(-zy) and measure dμd\mu. For ε>0\varepsilon>0 apply Poisson summation on O\mathcal{O} to fε(z)=e(z2/c)e−πε∣z∣2f_\varepsilon(z)=e(z^2/c)e^{-\pi\varepsilon|z|^2}. Direct Gaussian integration gives, with rε=1+3qcε2/16r_\varepsilon=1+3q_c\varepsilon^2/16,

f^ε(y)=∣c∣2rεe−πεqc∣y∣2/(4rε)e(−cy2/(4rε)).\widehat f_\varepsilon(y) =\frac{|c|}{2\sqrt{r_\varepsilon}} e^{-\pi\varepsilon q_c|y|^2/(4r_\varepsilon)} e\bigl(-cy^2/(4r_\varepsilon)\bigr).

To check the normalization, rotate zz by half the argument of cc. The quadratic matrix of the resulting real two-variable Gaussian is

(ε−4i/(3∣c∣)−4i/(3∣c∣)ε),det⁡=16rε3qc.\begin{pmatrix} \varepsilon& -4i/(\sqrt{3}|c|)\\ -4i/(\sqrt{3}|c|) & \varepsilon \end{pmatrix}, \qquad\det=\frac{16r_\varepsilon}{3q_c}.

Its eigenvalues are conjugates with positive real part. The positive square root of the determinant, the factor 2/32/\sqrt{3} in dμd\mu, and completion of the square give the formula above.

Put Iε=∫Ce−πε∣z∣2dμ(z)=2/(3ε)I_\varepsilon=\int_{\mathbb C}e^{-\pi\varepsilon|z|^2}d\mu(z) =2/(\sqrt3\varepsilon). For a fixed ideal (b)(b), a fixed class v mod bv\bmod b, and a>0a>0, Gaussian Poisson summation on bOb\mathcal{O} gives

1Iε∑z∈v+bOe−πaε∣z∣2⟶1aqb(ε↓0).\frac{1}{I_\varepsilon}\sum_{z\in v+b\mathcal{O}}e^{-\pi a\varepsilon|z|^2}\longrightarrow\frac{1}{aq_b}\qquad(\varepsilon\downarrow0).

The zero dual vector gives the limit and every nonzero dual vector is exponentially small. The phase e(z2/c)e(z^2/c) is periodic modulo cc. Consequently the normalized left side of Poisson’s identity tends to Γ(c)/∣c∣\Gamma(c)/|c|.

On the right side one may replace rεr_\varepsilon by 11. For fixed cc, the total error from the phase is at most

Ccε2∑y∈O∣y∣2e−Cc−1ε∣y∣2=Oc(1),C_c\varepsilon^2\sum_{y\in\mathcal{O}}|y|^2e^{-C_c^{-1}\varepsilon|y|^2}=O_c(1),

because the sum is Oc(ε−2)O_c(\varepsilon^{-2}). The amplitude error is Oc(ε)O_c(\varepsilon), as is the damping error, by the same lattice estimate. All three are o(Iε)o(I_\varepsilon). The phase e(−cy2/4)e(-cy^2/4) is periodic modulo 2O2\mathcal O. In the preceding Gaussian mean take b=2b=2 and a=qc/4a=q_c/4; each of its four classes has normalized mean 1/qc1/q_c. The normalized right side therefore tends to (2∣c∣)−1∑y mod 2e(−cy2/4)(2|c|)^{-1}\sum_{y\bmod2}e(-cy^2/4), which proves (4.3).

The representatives 0,1,ω,ω20,1,\omega,\omega^2 modulo 22 give the asserted four-term expression. Multiplication by an odd vv permutes these classes, so the same formula gives Γ(cv2)=Γ(c)\Gamma(cv^2)=\Gamma(c). The group of units modulo 44 has order 1212. Squaring a lift modulo 44 depends only on its class modulo 22, and its three possible squares are 1,ω,ω21,\omega,\omega^2. The four representatives in the statement are distinct modulo this subgroup; also λ2=−3≡1(mod4)\lambda^2=-3\equiv1\pmod4. Evaluating the four-term expression on them gives the table. Evaluating Γ(ab)/(Γ(a)Γ(b))\Gamma(ab)/(\Gamma(a)\Gamma(b)) on the two generators −1,λ-1,\lambda gives the displayed exponent, proving the last claims.

Lemma 4.4 (Sextic reciprocity and the fixed Gauss phase). For coprime primary a,ba,b outside SS,

χb(a)=R(a,b)χa(b),R(a,b)=r(a,b).\chi_b(a)=\mathcal{R}(a,b)\chi_a(b),\qquad\mathcal{R}(a,b)=\mathfrak{r}(a,b).

On all primary pairs outside SS, including noncoprime pairs, define R\mathcal{R} by the bicharacter r\mathfrak{r} of Equation (4.4). Define, on every primary index outside SS,

G(c)=χc(4)‾Γ(c).G(c)=\overline{\chi_c(4)}\Gamma(c).

It has modulus one and factors through a fixed ray group supported at 2,32,3. For all such v,wv,w,

G(vw)=G(v)G(w)R(v,w),G(1)=1.G(vw)=G(v)G(w)\mathcal{R}(v,w),\qquad G(1)=1.

Moreover G(v2)=χv(4)G(v^2)=\chi_v(4), and at good primes

G(p3)=γ3(p),R(p,p)=γ3(p)2=χp(−1).G(p^3)=\gamma_3(p),\qquad\mathcal{R}(p,p)=\gamma_3(p)^2=\chi_p(-1).

On every primary nn outside SS, one has χn(−1)=R(n,n)\chi_n(-1)=\mathcal{R}(n,n). The diagonal t↦R(t,t)t\mapsto\mathcal{R}(t,t) is a character of the fixed ray group. In the square-class notation of Equation (4.4), it is r(−1,n)\mathfrak{r}(-1,n), where −1-1 denotes its residue square class modulo 44, not the ideal ray class of the unit ideal (−1)(-1). For squarefree cc the complete Gauss identities are

γ2(c)3=μ(c)α(c),γ1(c)γ2(c)=μ(c)α(c)G(c),G(c)=χc(4)‾γ3(c),∣G(c)∣=1.\gamma_2(c)^3=\mu(c)\alpha(c),\qquad\gamma_1(c)\gamma_2(c)=\mu(c)\alpha(c)G(c),\qquad G(c)=\overline{\chi_c(4)}\gamma_3(c),\qquad|G(c)|=1.

All occurrences of GG on nonsquarefree indices mean the finite-ray function just defined, not a nonsquarefree Gauss sum.

Proof. At a good prime, counting square roots in the residue field gives

∑x mod pe(x2/p)=∑y mod p(1+χp(y)3)e(y/p)=∑y mod pχp(y)3e(y/p).\sum_{x\bmod p}e(x^2/p)=\sum_{y\bmod p}\left(1+\chi_p(y)^3\right)e(y/p)=\sum_{y\bmod p}\chi_p(y)^3e(y/p).

The additive sum without the character is zero. Hence Γ(p)=γ3(p)\Gamma(p)=\gamma_3(p), and replacing x2/px^2/p by ux2/pux^2/p for a unit uu multiplies the sum by χp(u)3\chi_p(u)^3. For squarefree cc, representing a residue as ∑p∣c(c/p)xp\sum_{p\mid c}(c/p)x_p gives, in both sums,

Γ(c)=∏p∣cχp(c/p)3Γ(p),γ3(c)=∏p∣cχp(c/p)3γ3(p).\Gamma(c)=\prod_{p\mid c}\chi_p(c/p)^3\Gamma(p),\qquad\gamma_3(c)=\prod_{p\mid c}\chi_p(c/p)^3\gamma_3(p).

The cross terms in the square are integral in the additive character. Thus Γ(c)=γ3(c)\Gamma(c)=\gamma_3(c) for squarefree cc. In particular, for distinct good primes p,qp,q,

Γ(pq)Γ(p)Γ(q)=χp(q)3χq(p)3.\frac{\Gamma(pq)}{\Gamma(p)\Gamma(q)}=\chi_p(q)^3\chi_q(p)^3.

We use cubic reciprocity in the following precise form: for coprime primary a,ba,b one has (a/b)3=(b/a)3(a/b)_3=(b/a)_3; see [8 Equation (1.4)]. Thus the quotient χb(a)/χa(b)\chi_b(a)/\chi_a(b) is a sign. At p,qp,q its cube is χq(p)3χp(q)3\chi_q(p)^3\chi_p(q)^3, so this sign equals r(p,q)\mathfrak r(p,q). Multiplicativity in both arguments and the bicharacter property extend the equality to every coprime primary pair. The definition by r\mathfrak r on noncoprime pairs involves no division of zero symbols.

The element −2-2 is primary and −1-1 is a cube. Cubic reciprocity therefore gives

χc(4)=(2/c)3=(−2/c)3=(c/(−2))3.\chi_c(4)=(2/c)_3=(-2/c)_3=(c/(-2))_3.

This is a character of cc mod 2. Together with the dependence of Γ\Gamma on cc mod 4, this proves that GG is a function on a fixed ray group (for example the ray group modulo 12 suffices here). Indeed, if two primary generators represent the same ray class modulo 12, their quotient differs from an element congruent to one modulo 12 by a unit; reduction modulo 3 forces that unit to be one. The generators therefore have the same residue modulo 4. Its multiplicative refinement is the definition of r\mathfrak r. Since Γ(v2)=1\Gamma(v^2)=1 and χv(4)\chi_v(4) has order dividing three, G(v2)=χv(4)‾ 2=χv(4)G(v^2)=\overline{\chi_v(4)}^{\,2}=\chi_v(4).

The table also gives

Γ(p)2=(−1)(qp−1)/2=χp(−1).\Gamma(p)^2=(-1)^{(q_p-1)/2}=\chi_p(-1).

For the last equality use χp(−1)=(−1)(qp−1)/6\chi_p(-1)=(-1)^{(q_p-1)/6} and the equality of these parities. Now Γ(p3)=Γ(p)\Gamma(p^3)=\Gamma(p), and χp(4)‾ 3=1\overline{\chi_p(4)}^{\,3}=1, proving G(p3)=γ3(p)G(p^3)=\gamma_3(p). Finally R(p,p)=1/Γ(p)2=Γ(p)2\mathcal{R}(p,p)=1/\Gamma(p)^2=\Gamma(p)^2, as this square is a sign.

For a symmetric sign-valued bicharacter its diagonal is multiplicative:

R(vw,vw)=R(v,v)R(v,w)2R(w,w)=R(v,v)R(w,w).\mathcal{R}(vw,vw)=\mathcal{R}(v,v)\mathcal{R}(v,w)^2\mathcal{R}(w,w)=\mathcal{R}(v,v)\mathcal{R}(w,w).

The prime identity consequently gives R(n,n)=χn(−1)\mathcal{R}(n,n)=\chi_n(-1) for every primary nn outside SS. On the square class (−1)eλf(-1)^e\lambda^f, the table gives both this diagonal and r(−1,n)\mathfrak r(-1,n) the value (−1)f(-1)^f. This use of −1-1 is in the residue square-class group; the ideal (−1)(-1) is the identity in an ideal ray class group and is not being substituted there.

For coprime squarefree primary a,ba,b outside SS, the Chinese remainder theorem gives

γj(ab)=χa(b)jχb(a)jγj(a)γj(b).\gamma_j(ab)=\chi_a(b)^j\chi_b(a)^j\gamma_j(a)\gamma_j(b).

One obtains this by representing a residue as bx+aybx+ay with xx mod aa and yy mod bb. Cubing the factor for j=2j=2 gives one. The product of the factors for j=1j=1 and j=2j=2 is (χa(b)χb(a))3=R(a,b)(\chi_a(b)\chi_b(a))^3=\mathcal{R}(a,b). The prime identities from Lemma 4.2, followed by (4.5), therefore prove (4.7) by induction on the number of prime factors. □

For later element rows, fix the generators πp\pi_{\mathfrak p} from Lemma 4.1. Every 0≠m∈O0\ne m\in\mathcal{O} has a unique expression

m=umSmgood,mS=∏p∈Sπpvp(m),m=u m_S m_{\mathrm{good}},\qquad m_S=\prod_{\mathfrak p\in S}\pi_{\mathfrak p}^{v_{\mathfrak p}(m)},

where uu is a unit and mgoodm_{\mathrm{good}} is the primary generator of the part of (m)(m) outside SS. On every primary AA outside SS, multiplicativity and sextic reciprocity give the zero-preserving identity

χA(m)=χA(umS)R(A,mgood)∏p∣mgoodχp(A)vp(m).\chi_A(m)=\chi_A(um_S)\mathcal{R}(A,m_{\mathrm{good}})\prod_{p\mid m_{\mathrm{good}}}\chi_p(A)^{v_p(m)}.

For (A,mgood)=1(A,m_{\mathrm{good}})=1 this is the reciprocity formula just proved; if they meet, both sides are zero and R\mathcal{R} is evaluated as its separately defined bicharacter. Once the good part’s fixed ray class and the SS-valuations modulo six are fixed, the first two factors on the right range over a fixed finite family of characters of AA. The product over good primes retains the moving character factors and all their zeros.

Every function on a fixed finite abelian ray group has a finite Fourier expansion in its characters. For example, if ϕ:T→C\phi:T\to\mathbb{C}, then

ϕ(v)=∑θ∈T^aθθ(v),aθ=1∣T∣∑u∈Tϕ(u)θ(u)‾.\phi(v)=\sum_{\theta\in\widehat{T}}a_\theta\theta(v),\qquad a_\theta=\frac{1}{|T|}\sum_{u\in T}\phi(u)\overline{\theta(u)}.

Parseval and Cauchy–Schwarz bound ∑θ∣aθ∣\sum_\theta|a_\theta| by ∣T∣1/2max⁡T∣ϕ∣|T|^{1/2}\max_T|\phi|. Applying the same statement on T×TT\times T separates R(a,b)\mathcal{R}(a,b) as a finite sum of products of characters. These expansions remain valid at noncoprime primary pairs because R\mathcal{R} there is the fixed-ray bicharacter, not a symbolic quotient. For example, for a good prime pp and every primary nn outside SS,

χn(p)χp(n)‾=R(p,n)1(n,p)=1.\chi_n(p)\overline{\chi_p(n)}=\mathcal{R}(p,n)1_{(n,p)=1}.

On coprime pairs this is sextic reciprocity, and on the remaining pairs both sides vanish. Thus cancellation of the moving local characters can leave both a coprimality indicator and a fixed-ray phase; neither may be discarded.

Smooth norm profiles

The following conventions make the smooth dependence in character-polynomial estimates quantitative. They distinguish derivatives of a fixed test from powers of a spectral height. This distinction is needed when a Fourier tail is removed only after the height range has been chosen.

For a profile ww on (0,∞)d(0,\infty)^d with logarithmic support in a fixed compact set Ω⊂Rd\Omega\subset\mathbb{R}^d, put

wlog⁡(u)=w(eu1,…,eud),pj(w)=∑∣α∣≤jsup⁡u∈Rd∣∂αwlog⁡(u)∣.w_{\log}(\boldsymbol u)=w(e^{u_1},\ldots,e^{u_d}),\qquad p_j(w)=\sum_{|\alpha|\le j}\sup_{\boldsymbol u\in\mathbb R^d} |\partial^\alpha w_{\log}(\boldsymbol u)|.

We always understand that wlog⁡w_{\log} is smooth and supported in Ω\Omega. Define

w^(t)=∫Rdwlog⁡(u)e−it⋅u du,∥w∥J,sep=∫Rd∣w^(t)∣(1+∣t∣)J dt.\widehat w(\boldsymbol t)=\int_{\mathbb R^d}w_{\log}(\boldsymbol u) e^{-i\boldsymbol t\cdot\boldsymbol u}\,d\boldsymbol u, \qquad \|w\|_{J,\mathrm{sep}} =\int_{\mathbb R^d}|\widehat w(\boldsymbol t)| (1+|\boldsymbol t|)^J\,d\boldsymbol t.

For a fixed finite tuple w=(w1,…,wr)\boldsymbol{w}=(w_1,\ldots,w_r), possibly of different fixed dimensions, we use pj(w)=1+∑i=1rpj(wi)p_j(\boldsymbol{w})=1+\sum_{i=1}^r p_j(w_i).

Lemma 4.5 (Smooth calculus). For integers J≥0J\ge0,

∥w∥J,sep≪J,d,ΩpJ+d+2(w).\|w\|_{J,\mathrm{sep}}\ll_{J,d,\Omega}p_{J+d+2}(w).

Logarithmic Fourier inversion separates any fixed norm monomial. More precisely, if xj=cj∏ℓ=1ryℓajℓx_j=c_j\prod_{\ell=1}^r y_\ell^{a_{j\ell}} with cj,yℓ>0c_j,y_\ell>0 and fixed real exponents ajℓa_{j\ell}, then

w(x1,…,xd)=1(2π)d∫Rdw^(t)∏jcjitj∏ℓyℓi∑jajℓtj dt.w(x_1,\ldots,x_d)=\frac1{(2\pi)^d}\int_{\mathbb R^d} \widehat w(\boldsymbol t)\prod_j c_j^{it_j} \prod_\ell y_\ell^{i\sum_j a_{j\ell}t_j}\,d\boldsymbol t.

If the coefficient measure in this formula is common to a collection of rows, Minkowski’s inequality passes any separated row ℓ2\ell^2 bound through the integral using ∥w∥J,sep\|w\|_{J,\mathrm{sep}} whenever the separated bound has height growth at most (1+∣t∣)J(1+|\boldsymbol t|)^J.

For a unit box I⊂RdI\subset\mathbb{R}^d and a smooth scalar function FF on I+[−1,1]dI+[-1,1]^d,

sup⁡I∣F∣2≪d∑α∈{0,1}d∫I+[−1,1]d∣∂αF∣2.\sup_I|F|^2\ll_d\sum_{\alpha\in\{0,1\}^d}\int_{I+[-1,1]^d}|\partial^\alpha F|^2.

Consequently, under the corresponding derivative bounds, rowwise choices of scales in a polynomial range cost powers of log⁡Z\log Z, and rowwise choices of norm-twist heights of absolute value at most T1T_1 cost a fixed power of 1+T11+T_1.

For T1≥1T_1 \ge1 and integers J,N≥0J,N \ge0,

∫∣t∣>T1∣w^(t)∣(1+∣t∣)J dt≤T1−N∥w∥J+N,sep.\int_{|\boldsymbol t|>T_1}|\widehat w(\boldsymbol t)| (1+|\boldsymbol t|)^J\,d\boldsymbol t \le T_1^{-N}\|w\|_{J+N,\mathrm{sep}}.

With the Mellin convention MW(s)=∫0∞W(y)ys dy/y\mathcal{M}W(s)=\int_0^\infty W(y)y^s\,dy/y, a pure twist obeys

M[W(y)yiω](s)=MW(s+iω).\mathcal{M}[W(y)y^{i\omega}](s)=\mathcal{M}W(s+i\omega).

Let Dy=y∂yD_y=y\partial_y, let I⊂RI\subset\mathbb{R} be compact, and let N≥0N\ge0 be an integer. Suppose the integrals below are finite and the boundary terms in NN logarithmic integrations by parts vanish. Then, uniformly for σ∈I\sigma\in I and T∈RT\in\mathbb{R},

∣MW(σ+iT)∣≪I,N(1+∣T∣)−N∑j=0N∫0∞yσ∣DyjW(y)∣ dyy.\lvert\mathcal{M}W(\sigma+iT)\rvert\ll_{I,N}(1+\lvert T\rvert)^{-N}\sum_{j=0}^{N}\int_0^\infty y^\sigma\lvert D_y^jW(y)\rvert\,\frac{dy}{y}.

These hypotheses hold for annular WW on every such II. They also hold when WW is smooth at zero and Schwartz at infinity and II is a compact subset of (0,∞)(0,\infty). In particular a horizontal contour join, whose imaginary coordinate is fixed, is estimated by this pointwise bound, not solely by the integrated tail in Equation (4.10).

The following joint version will also be useful. For measurable functions a(v),b(w)a(v),b(w) for which the right side is finite, and integers J,N≥0J,N\ge0,

∫R2e−(T+v)2∣a(v)b(w)∣(1+∣T∣+∣v∣+∣w∣)J dv dw≪J,N(1+∣T∣)−Nsup⁡v(1+∣v∣)J+N∣a(v)∣∫R(1+∣w∣)J∣b(w)∣ dw.\int_{\mathbb{R}^2}e^{-(T+v)^2}\lvert a(v)b(w)\rvert(1+\lvert T\rvert+\lvert v\rvert+\lvert w\rvert)^J\,dv\,dw \ll_{J,N}(1+\lvert T\rvert)^{-N}\sup_v(1+\lvert v\rvert)^{J+N}\lvert a(v)\rvert\int_{\mathbb{R}}(1+\lvert w\rvert)^J\lvert b(w)\rvert\,dw.

Thus the product of a Gaussian in the sum of two heights and rapidly decreasing Mellin transforms in the other two heights has rapid pointwise decay on a fixed-height slice. For integrated tails, the linear map (t1,t2,t3)↦(t1+t2,t2,t3)(t_1,t_2,t_3)\mapsto(t_1+t_2,t_2,t_3) is invertible, so all fixed weighted L1L^1 moments of this product also control complements of boxes in the original heights. Appending finitely many separating frequencies and fixed linear translations of these three arguments gives the same conclusion by a block triangular change of variables.

After translating a pure twist in the Mellin variable, a discarded separated integrand bounded by ZB(1+∣t∣)JZ^B(1+|\boldsymbol t|)^J has absolute tail at most ZBT1−N∥w∥J+N,sepZ^BT_1^{-N}\lVert w\rVert_{J+N,\mathrm{sep}}. Here BB and JJ must be fixed before NN is chosen. Further derivatives of a uniformly smooth separating profile change this last seminorm, not the previously fixed height order. On a join of bounded real length at height comparable to T1T_1, Equation (4.11) with order N+⌈J⌉N+\lceil J\rceil gives ZBT1−NZ^BT_1^{-N} times the corresponding finite weighted derivative norm of the external test, provided the other factors have the stated bound there. This is O(ZBT1−N)O(Z^BT_1^{-N}) when those external norms are uniform.

Proof. For an integer mm with 2m>J+d2m>J+d, integration by parts gives

(1+∣t∣2)mw^(t)=∫Rd(1−Δ)mwlog⁡(u)e−it⋅u du.(1+|\boldsymbol t|^2)^m\widehat w(\boldsymbol t) =\int_{\mathbb R^d}(1-\Delta)^m w_{\log}(\boldsymbol u) e^{-i\boldsymbol t\cdot\boldsymbol u}\,d\boldsymbol u.

Its absolute value is bounded by the volume of Ω\Omega times Cm,dp2m(w)C_{m,d}p_{2m}(w). The weighted integral is finite because 2m>J+d2m>J+d; one can choose 2m≤J+d+22m\le J+d+2. Fourier inversion gives the monomial formula. For row vectors B(t)B(\boldsymbol t) in ℓ2\ell^2, the precise inequality used there is

∥1(2π)d∫w^(t)B(t) dt∥ℓ2≤1(2π)d∫∣w^(t)∣∥B(t)∥ℓ2 dt.\left\|\frac1{(2\pi)^d}\int\widehat w(\boldsymbol t) B(\boldsymbol t)\,d\boldsymbol t\right\|_{\ell^2} \le\frac1{(2\pi)^d}\int|\widehat w(\boldsymbol t)| \|B(\boldsymbol t)\|_{\ell^2}\,d\boldsymbol t.

In one dimension, the fundamental theorem of calculus, averaging a base point over the enlarged interval, and Cauchy–Schwarz give sup⁡I∣F∣2≪∫I+[−1,1](∣F∣2+∣F′∣2)\sup_I\lvert F\rvert^2\ll\int_{I+[-1,1]}(\lvert F\rvert^2+\lvert F'\rvert^2). Applying this successively in each coordinate proves Equation (4.9). It can be summed over rows before the derivative integrals, since all terms are nonnegative. A logarithmic scale range of length O(log⁡Z)O(\log Z) needs O(log⁡Z)O(\log Z) unit intervals; a height range [−T1,T1][-T_1,T_1] needs O(1+T1)O(1+T_1) intervals. Derivatives with respect to a logarithmic scale insert yW′(y)yW'(y), together with the constant derivative of a central normalization. Derivatives of a normalized twist yity^{it} insert powers of log⁡y\log y. These are again annular profiles with finite seminorm bounds. For example, if a fixed-parameter squared row bound is O((1+∣t∣)H)O((1+|t|)^H) and there are dtd_t height parameters, the covering and integration cost at most a fixed multiple of (1+T1)H+dt(1+T_1)^{H+d_t}.

On ∣t∣>T1|\boldsymbol t|>T_1 one has (1+∣t∣)−N≤T1−N(1+|\boldsymbol t|)^{-N}\le T_1^{-N}, proving Equation (4.10). The Mellin shift is immediate from its definition. To prove Equation (4.11), put Fσ(u)=eσuW(eu)F_\sigma(u)=e^{\sigma u}W(e^u). For ∣T∣≥1|T|\ge1, integration by parts gives

MW(σ+iT)=(−iT)−N∫RFσ(N)(u)eiTu du,Fσ(N)(u)=eσu∑j=0N(Nj)σN−jDyjW(eu).\mathcal{M}W(\sigma+iT)=(-iT)^{-N}\int_{\mathbb{R}}F_\sigma^{(N)}(u)e^{iTu}\,du,\qquad F_\sigma^{(N)}(u)=e^{\sigma u}\sum_{j=0}^{N}\binom{N}{j}\sigma^{N-j}D_y^jW(e^u).

Taking absolute values gives the bound on a compact real strip. For ∣T∣<1|T|<1, the absolute integral gives it after increasing the constant. The two stated classes of WW have the required endpoint decay: compact support suffices in the first case, while eσue^{\sigma u} at −∞-\infty and Schwartz decay at +∞+\infty suffice in the second.

For Equation (4.12), use

1+∣T∣≤(1+∣T+v∣)(1+∣v∣),1+∣T∣+∣v∣+∣w∣≤2(1+∣T+v∣)(1+∣v∣)(1+∣w∣).1+|T|\le(1+|T+v|)(1+|v|),\qquad1+|T|+|v|+|w|\le2(1+|T+v|)(1+|v|)(1+|w|).

Move (1+∣T∣)N(1+|T|)^N to the left, bound the weighted a(v)a(v) pointwise, and integrate the remaining polynomial weight against the Gaussian in T+vT+v. The remaining ww integral is the one displayed. This proves the joint bound and also the asserted join estimate. For the integrated assertion, both the map (t1,t2,t3)↦(t1+t2,t2,t3)(t_1,t_2,t_3)\mapsto(t_1+t_2,t_2,t_3) and its inverse have fixed operator norm. A fixed polynomial weight in the original variables is therefore bounded by a fixed polynomial weight in the transformed ones. On a complement of a box one inserts the additional inverse power of that weight and integrates the Gaussian and the two Mellin factors separately. The appended block triangular map has the same property because all of its coefficients and those of its inverse are fixed.

A kernel depending on a common product, such as y1y2y_1y_2, gives the same norm power on both variables in the monomial formula; this preserves an equal-product-scale difference. A nonsmooth arithmetic mask has no such derivative bound and must instead be resolved before this lemma is applied.

Lemma 4.6 (Gaussian annular decomposition). Put

WG(y)=12πexp⁡(−14(log⁡y)2).W_{\mathrm{G}}(y)=\frac{1}{2\sqrt{\pi}}\exp\left(-\frac{1}{4}(\log y)^2\right).

This function is not annular. Choose a fixed χ∈Cc∞(R)\chi\in C_c^\infty(\mathbb R) such that ∑k∈Zχ(u−k)=1\sum_{k\in\mathbb{Z}}\chi(u-k)=1, and define

WG,k(y)=WG(y)χ(log⁡y−k),wk(x)=WG(ekx)χ(log⁡x).W_{\mathrm{G},k}(y)=W_{\mathrm{G}}(y)\chi(\log y-k),\qquad w_k(x)=W_{\mathrm{G}}(e^kx)\chi(\log x).

The profiles wkw_k have one fixed compact logarithmic support and, for every fixed A≥0A\ge0 and integer j≥0j\ge0,

∑k∈ZeA∣k∣pj(wk)<∞.\sum_{k\in\mathbb{Z}}e^{A|k|}p_j(w_k)<\infty.

Consequently Lemma (4.5) may be applied on each annulus after y=ekxy=e^kx, and the resulting weighted separation norms are summable. For fixed κ>0\kappa>0, A,B,C0≥0A,B,C_0\ge0, and M>0M>0 one also has

ZB∑∣k∣>κlog⁡Z−C0eA∣k∣pj(wk)≪Z−M(Z→∞).Z^B\sum_{|k|>\kappa\log Z-C_0}e^{A|k|}p_j(w_k)\ll Z^{-M}\qquad(Z\to\infty).

Directly, MWG(s)=es2\mathcal{M}W_{\mathrm{G}}(s)=e^{s^2}, and the weighted logarithmic derivatives in Equation (4.11) are finite uniformly on every compact real strip.

Proof. Such a partition is obtained by normalizing the integer translates of a nonnegative compactly supported smooth function positive on [−1/2,1/2][-1/2,1/2]. Let supp⁡χ⊂[−C,C]\operatorname{supp}\chi\subset[-C,C]. Each logarithmic derivative of WG(ekx)W_{\mathrm{G}}(e^k x) is a polynomial in k+log⁡xk+\log x times the same Gaussian. The product rule therefore gives

pj(wk)≤Cj(1+∣k∣)jexp⁡(−14((∣k∣−C)+)2).p_j(w_k)\le C_j(1+|k|)^j\exp\left(-\frac{1}{4}((|k|-C)_+)^2\right).

This is summable after multiplication by eA∣k∣e^{A|k|} for every fixed AA. The first assertion follows, and the separation norms follow from Lemma 4.5. In the profile’s logarithmic Fourier transform, rescaling an annulus inserts only the unit phase e−ikte^{-ikt}, so it does not change these norms; any real normalization of a surrounding polynomial remains explicit. On the indicated tail, the logarithm of the last bound after multiplication by ZBeA∣k∣Z^B e^{A|k|} is at most −cκ2(log⁡Z)2+O(log⁡Z)-c\kappa^2(\log Z)^2+O(\log Z) for some fixed c>0c>0; summing the Gaussian tail proves the stated estimate for every MM. Finally, set u=log⁡yu=\log y and complete the square in its Gaussian integral to obtain MWG(s)=es2\mathcal{M}W_{\mathrm{G}}(s)=e^{s^2}. The same Gaussian bounds every eσu(d/du)jWG(eu)e^{\sigma u}(d/du)^jW_{\mathrm{G}}(e^u) in L1(R)L^1(\mathbb{R}), uniformly for σ\sigma in a compact interval.

We record explicit finite-order continuity statements for the two types of kernels that accompany this separation. They make no assertion about an arithmetic transform; that transform must supply the stated kernel and its available real lines.

Lemma 4.7 (Finite seminorms for Fourier and Mellin kernels). For a Schwartz function ff on Rd\mathbb{R}^d, put

sj(f)=∑∣α∣,∣β∣≤j∥xα∂βf(x)∥L1(Rd).s_j(f)=\sum_{|\alpha|,|\beta|\le j}\left\|x^\alpha\partial^\beta f(x)\right\|_{L^1(\mathbb{R}^d)}.

For every A≥0A\ge0 and multi-index β\beta, the ordinary Fourier transform satisfies

sup⁡ξ(1+∣ξ∣)A∣∂βf^(ξ)∣≪A,β,ds⌈A⌉+∣β∣(f).\sup_{\xi}(1+|\xi|)^A|\partial^\beta\widehat{f}(\xi)|\ll_{A,\beta,d}s_{\lceil A\rceil+|\beta|}(f).

The same conclusion, with a fixed change in the constant, holds for any fixed nondegenerate linear Fourier pairing. For a radial transform written as f^(ξ)=F(∣ξ∣2)\widehat{f}(\xi)=F(|\xi|^2), any prescribed bound

sup⁡r≥0(1+r)A∣(r∂r)jF(r)∣\sup_{r\ge0}(1+r)^A|(r\partial_r)^jF(r)|

is therefore controlled by finitely many Schwartz seminorms of ff.

For the Mellin assertion, let m(s)m(s) be holomorphic on a fixed closed vertical strip and suppose, uniformly there, ∣m(σ+it)∣≤C(1+∣t∣)h|m(\sigma+it)|\le C(1+|t|)^h for a fixed h≥0h\ge0. On an available line ℜs=σ\Re s=\sigma in that strip define

KW(x)=12πi∫(σ)MW(−s)m(s)x−s dsK_W(x)=\frac{1}{2\pi i}\int_{(\sigma)}\mathcal{M}W(-s)m(s)x^{-s}\,ds

where WW has the finite weighted logarithmic derivatives needed to make the integral absolutely convergent, with the boundary terms in the logarithmic integrations by parts vanishing. For every integer j≥0j\ge0,

∣(x∂x)jKW(x)∣≪x−σ∫R∣MW(−σ−it)∣(1+∣t∣)h+j dt.|(x\partial_x)^jK_W(x)|\ll x^{-\sigma}\int_{\mathbb{R}}|\mathcal{M}W(-\sigma-it)|(1+|t|)^{h+j}\,dt.

*The integral on the right is bounded by finitely many integrals of y−σ∣(y∂y)kW(y)∣ dy/yy^{-\sigma}|(y\partial_y)^kW(y)|\,dy/y, uniformly for σ\sigma in the fixed strip. For W(y)yiωW(y)y^{i\omega} the same bound costs at most an additional factor (1+∣ω∣)h+j(1+|\omega|)^{h+j}. After multiplication by a fixed annular cutoff, these conclusions also bound every fixed logarithmic seminorm of y↦KW(Ry)y\mapsto K_W(Ry), with the factor R−σR^{-\sigma}.

Proof. Differentiating f^\widehat{f} inserts xβx^{\beta}, and multiplication by a monomial in ξ\xi differentiates xβfx^{\beta}f before Fourier transformation. The L1L^1 bound for the Fourier transform, the product rule, and the bound of (1+∣ξ∣)A(1+|\xi|)^A by a finite sum of monomials of degrees at most ⌈A⌉\lceil A\rceil give the first assertion. For a radial function, r∂rr\partial_r corresponds to (ξ⋅∂ξ)/2(\xi\cdot\partial_\xi)/2. Expanding its jjth power gives finitely many polynomial multiples of Fourier derivatives, so the first assertion gives the radial one. A fixed linear change of coordinates changes only its constants.

For the Mellin assertion, differentiation under the absolutely convergent integral inserts (−s)j(-s)^j. On the fixed strip this is bounded by a constant times (1+∣t∣)j(1+|t|)^j. Write y=euy=e^u and integrate the Fourier transform of e−σuW(eu)e^{-\sigma u}W(e^u) by parts more than h+j+1h+j+1 times. The product rule bounds the resulting L1L^1 derivatives by the stated weighted logarithmic derivatives, because σ\sigma ranges over a fixed set. For a pure twist the Mellin integrand is MW(−σ−it+iω)\mathcal{M}W(-\sigma-it+i\omega). Substitute v=t−ωv=t-\omega and use (1+∣v+ω∣)h+j≤(1+∣v∣)h+j(1+∣ω∣)h+j(1+|v+\omega|)^{h+j}\leq(1+|v|)^{h+j}(1+|\omega|)^{h+j}. Finally the product rule for a fixed annular cutoff and the chain rule for RyRy give the last statement.

Growth and logarithmic control for Hecke functions

The disk estimate will be applied only after zeros have been excluded from that disk. The following elementary growth bound provides the input for the complex-analytic argument and makes clear which constants are uniform in the conductor. When ψ\psi is a Hecke character, L(s,ψ)L(s,\psi) abbreviates LF(s,ψ)L_F(s,\psi). In this subsection Γ(s)\Gamma(s) denotes Euler’s gamma function; the finite quadratic function Γ(c)\Gamma(c) was confined to the arithmetic identities above.

Lemma 4.8 (Hecke strip growth). Let ψ\psi be a primitive nonprincipal finite-order Hecke character of FF, with conductor norm QQ. Then

∣L(σ+it,ψ)∣≪Q3/5(3+∣t∣)2,−1/10≤σ≤11/10.|L(\sigma+it,\psi)|\ll Q^{3/5}(3+|t|)^2,\qquad-1/10\leq\sigma\leq11/10.

For the principal character, the same bound with Q=1Q=1 holds for (s−1)ζF(s)/(s+1)(s-1)\zeta_F(s)/(s+1), with the removable value used at s=1s=1.

Proof. A finite-order character has trivial infinite type, since C×\mathbb{C}^{\times} is connected. The primitive Hecke functional equation in this case is

Λ(s,ψ)=(3Q)s/2(2π)−sΓ(s)L(s,ψ),Λ(s,ψ)=ε(ψ)Λ(1−s,ψ‾),∣ε(ψ)∣=1.\Lambda(s,\psi)=(3Q)^{s/2}(2\pi)^{-s}\Gamma(s)L(s,\psi),\qquad\Lambda(s,\psi)=\varepsilon(\psi)\Lambda(1-s,\overline{\psi}),\qquad|\varepsilon(\psi)|=1.

This is the functional equation for primitive characters of trivial infinite type stated in [11 Equation (1.1)]; a nonprincipal L(s,ψ)L(s,\psi) is entire. Absolute Euler convergence bounds L(11/10+it,ψ)L(11/10+it,\psi) uniformly in Q,tQ,t. Applying the functional equation and Stirling’s formula on ℜs=−1/10\Re s=-1/10 gives

∣L(−1/10+it,ψ)∣≪Q3/5(3+∣t∣)6/5.|L(-1/10+it,\psi)|\ll Q^{3/5}(3+|t|)^{6/5}.

The estimate for bounded tt follows by continuity of the gamma quotient on that line, so the constant is uniform there as well.

For completeness, the growth hypothesis needed to use the strip principle can be obtained directly from a lattice theta integral. Let f=(f)\mathfrak{f}=(f) be the conductor and define the periodic residue character ϕ(a)=ψ((a))\phi(a)=\psi((a)) when (a,f)=1(a,\mathfrak{f})=1, with value zero otherwise. For the principal conductor (1)(1) put ϕ(a)=1\phi(a)=1 for all aa, including a=0a=0. Since the ideal class group is trivial, conductor one has no nonprincipal character. Periodicity modulo f\mathfrak{f} follows from the ray character property; ϕ\phi is trivial on the six units because (u)=(1)(u)=(1) for a unit. Thus, for ℜs>1\Re s>1,

6π−sΓ(s)L(s,ψ)=∫0∞(Θϕ(v)−ϕ(0))vs−1 dv,Θϕ(v)=∑a∈Oϕ(a)e−πvqa.6\pi^{-s}\Gamma(s)L(s,\psi)=\int_0^\infty\bigl(\Theta_\phi(v)-\phi(0)\bigr)v^{s-1}\,dv,\qquad\Theta_\phi(v)=\sum_{a\in\mathcal{O}}\phi(a)e^{-\pi vq_a}.

The factor six counts the generators of each ideal. If ϕ^(h)=Q−1∑a mod fϕ(a)e(−ha/f)\widehat{\phi}(h) = Q^{-1}\sum_{a \bmod f}\phi(a)e(-ha/f), finite Fourier inversion and Gaussian Poisson summation give

Θϕ(v)=23v∑h mod fϕ^(h)∑b∈Oexp⁡(−4π∣b−h/f∣23v).\Theta_\phi(v)=\frac{2}{\sqrt3v} \sum_{h\bmod f}\widehat\phi(h) \sum_{b\in\mathcal O} \exp\left(-\frac{4\pi|b-h/f|^2}{3v}\right).

Changing the generator ff only reindexes the finite sum. For each fixed conductor, the nonzero dual vectors have a positive minimum length. With Aϕ=2ϕ^(0)/3A_{\phi}=2\widehat{\phi}(0)/\sqrt{3}, this proves

Θϕ(v)=Aϕv−1+Oϕ(v−1e−cϕ/v)(0<v≤1),Θϕ(v)=ϕ(0)+Oϕ(e−cϕv)(v≥1)\Theta_{\phi}(v)=A_{\phi}v^{-1}+O_{\phi}(v^{-1}e^{-c_{\phi}/v})\quad(0<v\leq1),\qquad\Theta_{\phi}(v)=\phi(0)+O_{\phi}(e^{-c_{\phi}v})\quad(v\geq1)

for some cϕ>0c_{\phi}>0. Splitting the Mellin integral at one consequently gives

6π−sΓ(s)L(s,ψ)=Aϕs−1−ϕ(0)s+∫01(Θϕ(v)−Aϕ/v)vs−1 dv+∫1∞(Θϕ(v)−ϕ(0))vs−1 dv.\begin{aligned} 6\pi^{-s}\Gamma(s)L(s,\psi) ={}&\frac{A_\phi}{s-1}-\frac{\phi(0)}s +\int_0^1\bigl(\Theta_\phi(v)-A_\phi/v\bigr)v^{s-1}\,dv\\ &+\int_1^\infty\bigl(\Theta_\phi(v)-\phi(0)\bigr)v^{s-1}\,dv. \end{aligned}

Both integrals are entire and bounded in height on each bounded real strip, with constants that may depend on the fixed conductor. Stirling’s formula for 1/Γ(s)1/\Gamma(s) therefore gives at most exponential height growth for L(s,ψ)L(s,\psi) on that strip. In the principal case the same conclusion holds after multiplication by (s−1)/(s+1)(s-1)/(s+1). Only this qualitative growth, for each fixed conductor, is used in the strip principle.

To see explicitly that the fixed-conductor growth constants do not enter the uniform strip bound, put

HQ(s)=Q−3/5L(s,ψ)(s+2)2.H_Q(s)=Q^{-3/5}\frac{L(s,\psi)}{(s+2)^2}.

It is holomorphic in the closed strip and is bounded by one absolute constant CC on both vertical boundary lines, by the bounds already proved. For δ>0\delta>0, apply the maximum principle on the rectangle of height TT to HQ(s)exp⁡(δ(s−1/2)2)H_Q(s)\exp(\delta(s-1/2)^2). On the vertical sides the exponential has modulus at most e9δ/25e^{9\delta/25}, because ∣ℜs−1/2∣≤3/5|\Re s-1/2|\leq3/5. On the horizontal sides its modulus is at most eδ(9/25−T2)e^{\delta(9/25-T^2)}, which tends to zero faster than the qualitative fixed-QQ exponential growth as T→∞T\to\infty. First let T→∞T\to\infty for this fixed Q,δQ,\delta, and then let δ↓0\delta\downarrow0. The result is ∣HQ(s)∣≤C|H_Q(s)|\leq C throughout the strip, with the same constant for every QQ. Multiplication by Q3/5∣s+2∣2Q^{3/5}|s+2|^2 proves Equation (4.14).

For the principal function, the factor (s−1)/(s+1)(s-1)/(s+1) removes its only pole in the strip and is bounded on the boundary. Its functional equation gives the same boundary bounds with Q=1Q=1. This equation also follows from the preceding Poisson formula with ϕ=1\phi=1: after writing v=2t/3v=2t/\sqrt{3}, the theta relation is Θϕ(2t/3)=t−1Θϕ(2/(3t))\Theta_{\phi}(2t/\sqrt{3})=t^{-1}\Theta_{\phi}(2/(\sqrt{3}t)), whose split Mellin integral is invariant under s↦1−ss\mapsto1-s. Apply the same damped-rectangle argument to (s−1)ζF(s)/((s+1)(s+2)2)(s-1)\zeta_F(s)/((s+1)(s+2)^2).

Lemma 4.9 (Logarithmic control). Let ψ\psi be a primitive nonprincipal finite-order Hecke character of conductor norm QQ, and put L(s)=L(s,ψ)\mathcal{L}(s)=L(s,\psi). For the principal character put Q=1Q=1 and L(s)=(s−1)ζF(s)/(s+1)\mathcal{L}(s)=(s-1)\zeta_F(s)/(s+1), with its removable value at one. Fix a∈[1/2,1]a\in[1/2,1] and 0<e<10−30<e<10^{-3}. Suppose L\mathcal{L} has no zero in the open disk of radius 2−a−2e2-a-2e centered at 2+it2+it. Uniformly on the closed concentric disk of radius 2−a−6e2-a-6e,

∣L(s)∣+∣L(s)−1∣≪e,ϵ{2Q(3+∣t∣)2}ϵ.|\mathcal L(s)|+|\mathcal L(s)^{-1}| \ll_{e,\epsilon}\{2Q(3+|t|)^2\}^{\epsilon}.

On the disk of radius 2−a−8e2-a-8e one also has

∣L′(s)/L(s)∣≪elog⁡{2Q(3+∣t∣)2}.|\mathcal L'(s)/\mathcal L(s)|\ll_e\log\{2Q(3+|t|)^2\}.

In particular, for every fixed b≥β∗b\geq\beta_* and v>0v>0, these bounds hold on ℜs≥b+v\Re s\geq b+v, with constants depending on v,ϵv,\epsilon (and with the height of ss in place of tt). In the principal case the reciprocal bound passes to 1/ζF1/\zeta_F; the upper and logarithmic-derivative bounds are for the regularized function L\mathcal{L}.

Proof. Write Rj=2−a−jeR_j=2-a-je and C=2Q(3+∣t∣)2\mathcal C=2Q(3+|t|)^2. All the disks used here lie in ℜs>1/2\Re s>1/2, where the principal regularizer is holomorphic. On the zero-free disk choose a holomorphic logarithm g=log⁡Lg=\log\mathcal{L} whose value near the center is the Euler logarithm, together with the logarithm of the regularizing factor in the principal case. The value g(2+it)g(2+it) is uniformly bounded. Lemma 4.8 and Euler convergence to the right of 11/1011/10 give

ℜg(s)=log⁡∣L(s)∣≪log⁡C(∣s−(2+it)∣≤R3).\Re g(s)=\log|\mathcal L(s)|\ll\log\mathcal C \qquad(|s-(2+it)|\le R_3).

The possible heights differ from tt by at most 3/23/2, which is included in C\mathcal C. Borel–Carathéodory on radii R3,R4R_3,R_4, whose difference is ee, now gives ∣g∣≪elog⁡C|g|\ll_e\log\mathcal C on the disk of radius R4R_4.

On the disk of fixed radius r0=49/100r_0=49/100, one has ℜs≥151/100>1\Re s\ge151/100>1. The absolutely convergent Euler logarithm is uniformly bounded there. For the principal function the logarithm of (s−1)/(s+1)(s-1)/(s+1) is also bounded on this disk, using its branch in ℜs>1\Re s>1. Since r0<R6<R4r_0<R_6<R_4, Hadamard’s three-circles theorem applied to gg gives

max⁡∣s−(2+it)∣≤R6∣g(s)∣≪e(log⁡C)θ,θ=log⁡(R6/r0)log⁡(R4/r0)<1.\max_{|s-(2+it)|\le R_6}|g(s)| \ll_e(\log\mathcal C)^\theta, \qquad \theta=\frac{\log(R_6/r_0)}{\log(R_4/r_0)}<1.

For fixed ee, continuity on the compact interval 1/2≤a≤11/2\le a\le1 makes θ\theta uniformly smaller than one. For every ϵ>0\epsilon>0, exp⁡(Ce(log⁡C)θ)≪e,ϵCϵ\exp(C_e(\log\mathcal C)^\theta)\ll_{e,\epsilon}\mathcal C^\epsilon. Applying this to both ege^g and e−ge^{-g} proves Equation (4.15). Cauchy’s estimate between radii R6R_6 and R8R_8 gives the stated bound for g′=L′/Lg'=\mathcal{L}'/\mathcal{L}.

For the global assertion first suppose β∗≤b≤1\beta_*\le b\le1. Choose 0<e<min⁡(10−3,v/8)0<e<\min(10^{-3},v/8) and put a=ba=b. The disk of radius R2R_2 is contained in ℜs>b+2e>β∗\Re s>b+2e>\beta_*, so it is zero-free by the definition of β∗\beta_* and absolute Euler convergence beyond one. The disk of radius R8R_8 covers the points b+v≤ℜs≤2b+v\le\Re s\le2 at its center’s height; Euler convergence covers ℜs≥2\Re s\ge2. The preceding constants are uniform in bb. If b>1b>1, Euler convergence on ℜs≥1+v\Re s\ge1+v suffices. Finally

1ζF(s)=s−1s+1L(s)−1,∣s−1s+1∣≤1(ℜs≥0),\frac{1}{\zeta_F(s)}=\frac{s-1}{s+1}\mathcal{L}(s)^{-1},\qquad\left|\frac{s-1}{s+1}\right|\le1\qquad(\Re s\ge0),

which proves the principal reciprocal assertion.

Lemma 4.10 (Deleted Euler factors). Let RR be a squarefree ideal and let ∣ap∣≤1|a_p|\le1 for p∣Rp\mid R. Put DR(s)=∏p∣R(1−apqp−s)D_R(s)=\prod_{p\mid R}(1-a_pq_p^{-s}). For fixed σ0>0\sigma_0>0 and every ϵ>0\epsilon>0,

∣DR(s)∣+∣DR(s)−1∣≪σ0,ϵqRϵ(ℜs≥σ0).|D_R(s)|+|D_R(s)^{-1}|\ll_{\sigma_0,\epsilon}q_R^\epsilon\qquad(\Re s\ge\sigma_0).

On a bounded real strip one has, uniformly in the height,

∣DR(s)∣≪ϵqR(−ℜs)++ϵ,∣DR′(s)DR(s)∣≪σ0log⁡(2qR)(ℜs≥σ0).|D_R(s)|\ll_\epsilon q_R^{(-\Re s)_++\epsilon},\qquad\left|\frac{D_R'(s)}{D_R(s)}\right|\ll_{\sigma_0}\log(2q_R)\qquad(\Re s\ge\sigma_0).

In particular a support qR≤ZBq_R\le Z^B with bounded BB costs any prescribed positive power of ZZ on a fixed positive real half-plane. For an imprimitive function L(s,ψ∗)DR(s)L(s,\psi^*)D_R(s), both the primitive conductor and the deletion radical RR must be included when applying logarithmic control.

Proof. Every factor is nonzero on ℜs>0\Re s>0. For ℜs≥σ0\Re s\ge\sigma_0, both its absolute value and the absolute value of its inverse are at most (1−qp−σ0)−1(1-q_p^{-\sigma_0})^{-1}. For sufficiently large qpq_p, depending on σ0,ϵ\sigma_0,\epsilon, −log⁡(1−qp−σ0)≤ϵlog⁡qp-\log(1-q_p^{-\sigma_0})\le\epsilon\log q_p. The finitely many smaller primes contribute a fixed constant. This proves the first estimate. For any real σ\sigma,

∏p∣R(1+qp−σ)≤qR(−σ)+2#{p:p∣R}≪ϵqR(−σ)++ϵ.\prod_{p\mid R}(1+q_p^{-\sigma}) \le q_R^{(-\sigma)_+}2^{\#\{p:p\mid R\}} \ll_\epsilon q_R^{(-\sigma)_++\epsilon}.

The last inequality follows by separating the finitely many primes with qp<21/ϵq_p < 2^{1/\epsilon}. Finally, logarithmic differentiation gives

∣DR′DR(s)∣≤∑p∣Rlog⁡qpqpσ0−1≪σ0log⁡(2qR).\left|\frac{D_R'}{D_R}(s)\right| \le\sum_{p\mid R}\frac{\log q_p}{q_p^{\sigma_0}-1} \ll_{\sigma_0}\log(2q_R).

If qR≤ZBq_R \leq Z^B, choose the exponent in the first estimate smaller than the desired exponent of ZZ divided by the bounded value of BB; the case B=0B=0 is immediate. This proves the stated interpretation for deleted factors.

Completed cubic reflection and unmarked row energy

This section first transforms a completed sum of Gauss coefficients while retaining every zero extension in its character. It then combines that identity with the quadratic large sieve to bound its mean square over arbitrary nonzero element rows. At equal row and completed lengths, the result is the bound Z1+ϵZ^{1+\epsilon} needed in the balanced argument.

The theta function and its Fourier coefficients at three fixed cusps are the unconditional input from Dunn and Radziwiłł [8 Section 5 and Appendix A]]. The original coefficient and cusp calculations are in Patterson [24 Theorem 8.1 and Sections 7–8]]; the formal input here remains the formulas in [8]. The finite transform below derives the masked formula, including its local factors and phase. The later mean-square argument uses this phase only after fixing its finite cusp sectors.

The completed reflection

Write

eˇ(z)=exp⁡(2πi(z+zˉ)),e(z)=eˇ(z/λ)(z∈C).\check e(z)=\exp\bigl(2\pi i(z+\bar z)\bigr), \qquad e(z)=\check e(z/\lambda)\qquad(z\in\mathbb C).

On FF, the exponent in eˇ\check e is 2πiTr⁡F/Qz2\pi i\operatorname{Tr}_{F/\mathbb{Q}}z. For every integer exponent, a power of a residue character is understood to be zero at a nonunit. In particular, χp(x)0=1p∤x\chi_p(x)^0=1_{p\nmid x}.

Proposition 5.1 (Completed cubic reflection). Fix a finite family X\mathcal{X} of finite-ray characters whose conductors are supported on SS. Choose one fixed integral modulus E\mathfrak{E} with prime support exactly SS, divisible by every conductor in this family. On primary elements extend each member of X\mathcal{X} by zero away from the E\mathfrak{E}-units. Choose a single L∈O∖{0}L\in\mathcal{O}\setminus\{0\} with prime support SS, with (18)∣(L)(18)\mid(L) and E∣(L)\mathfrak{E}\mid(L), large enough that, for every Ψ0∈X\Psi_0\in\mathcal{X}, the function on O\mathcal{O}

ϕ(x)={χx(λ)2Ψ0(x),x≡1(mod3), (x,E)=1,0,otherwise,ϕ^(h)=qL−1∑x mod Lϕ(x)e(−hx/L)\phi(x)= \begin{cases} \chi_x(\lambda)^2\Psi_0(x), & x\equiv1\pmod{3},\ (x,\mathfrak{E})=1,\\ 0, & \text{otherwise}, \end{cases} \qquad \widehat{\phi}(h)=q_L^{-1}\sum_{x\bmod L}\phi(x)e(-hx/L)

is LL-periodic. The zero branch is evaluated without evaluating either character. Such a choice of LL exists by the cubic supplementary law and the ray periodicity, as verified below. Both E\mathfrak{E} and LL are fixed for the entire family before any moving prime is chosen. Fix a member Ψ0∈X\Psi_0\in\mathcal{X} and put L=(L)\mathfrak{L}=(L). Let P\mathcal{P} be any finite set of distinct primary primes not dividing LL, choose jp∈{0,1,…,5}j_p\in\{0,1,\ldots,5\} for each p∈Pp\in\mathcal P, and set, on primary elements,

Ψ(n)=Ψ0(n)∏p∈Pχp(n)jp.\Psi(n)=\Psi_0(n)\prod_{p\in\mathcal P}\chi_p(n)^{j_p}.

No coprimality between the two variables in the following product is imposed:

D(s,Ψ)=∑n≡1 (3)(n,E)=1sfγ2(n)α‾(n)Ψ(n)qn−s,D(s,\Psi)=\sum_{\substack{n\equiv1\ (3)\\(n,\mathfrak{E})=1}}^{\mathrm{sf}}\gamma_2(n)\overline{\alpha}(n)\Psi(n)q_n^{-s},
L0(s,Ψ)=∑b≡1 (3)(b,E)=1α‾(b)3Ψ(b)3qb−3s+1/2,T(s,Ψ)=L0(s,Ψ)D(s,Ψ).L_0(s,\Psi)=\sum_{\substack{b\equiv1\ (3)\\(b,\mathfrak{E})=1}}\overline{\alpha}(b)^3\Psi(b)^3q_b^{-3s+1/2},\qquad T(s,\Psi)=L_0(s,\Psi)D(s,\Psi).

Both series and their product converge absolutely for ℜs>1\Re s>1.

Let X>0X>0. Suppose that V∈C∞(0,∞)V\in C^\infty(0,\infty) and that, for every C>0C>0 and every integer j≥0j\geq0, (x∂x)jV(x)(x\partial_x)^jV(x) is OC,j(xC)O_{C,j}(x^C) as x→0x\to0 and OC,j(x−C)O_{C,j}(x^{-C}) as x→∞x\to\infty. Define

V^(t)=∫0∞V(x)xtdxx.\widehat{V}(t)=\int_0^\infty V(x)x^t\frac{dx}{x}.

The smoothed expression to be transformed is the completed sum

12πi∫(a)V^(s−1/2)Xs−1/2T(s,Ψ) ds=∑n sf, bn,b≡1 (3)(nb,E)=1γ2(n)α(nb3)‾Ψ(nb3)qn qbV ⁣(qnqb3X),a>1.\begin{aligned} &\frac1{2\pi i}\int_{(a)}\widehat V(s-1/2)X^{s-1/2}T(s,\Psi)\,ds\\ &\quad=\sum_{\substack{n\ {\rm sf},\ b\\n,b\equiv1\ (3)\\(nb,\mathfrak E)=1}} \frac{\gamma_2(n)\overline{\alpha(nb^3)}\Psi(nb^3)} {\sqrt{q_n}\,q_b} V\!\left(\frac{q_nq_b^3}{X}\right),\qquad a>1. \end{aligned}

This equality follows by absolute convergence and Mellin inversion. The character acts on the whole index nb3nb^3, with its zero values retained; nn and bb may share prime factors.

The reflected test is defined by

K=(2π)427,R(t)=∏±Γ(1+t±1/6)Γ(1−t±1/6),K=\frac{(2\pi)^4}{27},\qquad R(t)=\prod_{\pm}\frac{\Gamma(1+t\pm1/6)}{\Gamma(1-t\pm1/6)},
V♯(x)=12πi∫(σ)V^(−t)R(t)(Kx)−t dt(σ≥0).V^\sharp(x)=\frac{1}{2\pi i}\int_{(\sigma)}\widehat{V}(-t)R(t)(Kx)^{-t}\,dt\qquad(\sigma\geq0).

The integral defining V♯V^\sharp is absolutely convergent and is independent of σ≥0\sigma\geq0.

The product TT has an entire continuation. On every fixed vertical strip it has polynomial growth, with constants allowed to depend on LL, Ψ0\Psi_0, P\mathcal{P}, (jp)(j_p) and the strip. There is one fixed triple of cusp coefficient functions from λ−4O∖{0}\lambda^{-4}\mathcal{O}\setminus\{0\} to C\mathbb{C}, constructed from the theta expansions in the proof. The same triple is used for all choices of the arithmetic data, scale, and test profile. For each fixed arithmetic choice above, there is a finite family of terms, indexed as in (1), independent of XX, VV, and the contour parameter a>1a>1. In each term, dd is selected from this triple and ϑ\vartheta is an additive character of O\mathcal{O} modulo a fixed modulus depending only on LL; their sectorwise dependence is exactly that stated in (3), and the remaining data have properties (1)–(3). For these terms and every a>1a>1, the identity is

12πi∫(a)V^(s−1/2)Xs−1/2T(s,Ψ) ds=∑termsζ∑0≠μ∈λ−4Od(μ)α(μ)ϑ(λ4μ)qμ∏p activeBp(λ4μ)V♯ ⁣(qμXqc2).\begin{aligned} &\frac1{2\pi i}\int_{(a)}\widehat V(s-1/2)X^{s-1/2}T(s,\Psi)\,ds\\ &\quad=\sum_{\text{terms}}\zeta \sum_{0\ne\mu\in\lambda^{-4}\mathcal O} \frac{d(\mu)\alpha(\mu)\vartheta(\lambda^4\mu)}{\sqrt{q_\mu}} \prod_{p\ {\rm active}}B_p(\lambda^4\mu) V^\sharp\!\left(\frac{q_\mu X}{q_c^2}\right). \end{aligned}

Every inner sum is absolutely convergent. The terms have the following precise properties.

  1. A term is specified by h0 mod Lh_0\bmod L mod LL and a subset of active primes. Every pp with jp≠0j_p \ne0 is active, while a prime with jp=0j_p = 0 may be active or inactive. Write r=∏p activepr = \prod_{p\ \mathrm{active}} p. Then c=cFrc = c_F r, where cFc_F is the reduced denominator of λ2h0/L\lambda^2 h_0/L, with a normalizing unit. Thus cFc_F ranges over a fixed finite set and its prime divisors divide LL. There are OL(2∣P∣)O_{\mathfrak L}(2^{|\mathcal P|}) terms, or OL(4∣P∣)O_{\mathfrak L}(4^{|\mathcal P|}) after splitting each Ramanujan factor in the next display into its two summands.

  1. The local column factors are

Bp(x)={χp(x)−jp−2,jp≠0,4,qp−1/2(−1+qp1p∣x),jp=4,qp−1/2χp(x)−2,jp=0 and p is active.B_p(x)= \begin{cases} \chi_p(x)^{-j_p-2}, & j_p \ne0,4,\\ q_p^{-1/2}(-1+q_p1_{p\mid x}), & j_p=4,\\ q_p^{-1/2}\chi_p(x)^{-2}, & j_p=0\ \text{and }p\ \text{is active}. \end{cases}

The function dd is one of three fixed cusp coefficient functions. Writing uu for an Eisenstein unit, their support and size satisfy

supp⁡d⊂{uλknb3:k≥−4, n,b≡1(mod3), n sf},∣d(μ)∣≤27 3k/6∣b∣.\operatorname{supp}d\subset \{u\lambda^k n b^3:k\ge-4,\ n,b\equiv1\pmod3,\ n\ {\rm sf}\}, \qquad |d(\mu)|\le27\,3^{k/6}|b|.

The bound refers to the displayed representation of a supported index. It permits common primes of nn and bb, and it imposes no exclusion at the primes of LL other than the displayed restriction at λ\lambda. The character ϑ\vartheta is an additive character of a quotient of O\mathcal{O} by a fixed modulus depending only on LL.

  1. The scalar ζ\zeta is independent of μ\mu and satisfies ∣ζ∣≤1/81|\zeta|\le1/81. Its moving-prime dependence can be specified exactly. For m≢0(mod6)m\not\equiv0\pmod{6}, put

τp,m±=qp−1/2∑y mod pχp(y)me(±y/p),∣τp,m±∣=1.\tau_{p,m}^{\pm}=q_p^{-1/2}\sum_{y\bmod p}\chi_p(y)^m e(\pm y/p), \qquad |\tau_{p,m}^{\pm}|=1.

For each active pp, define units modulo pp by

σp=λ2c/p,ϵp=−((λ3c/p)σp)−1,\sigma_p=\lambda^2c/p,\qquad\epsilon_p=-((\lambda^3c/p)\sigma_p)^{-1},

and put

ωp,j={τp,j−τp,j+2+χp(ϵp)−j−2,j≠0,4,τp,4−,j=4,−τp,2+χp(ϵp)−2,j=0.\omega_{p,j}=\begin{cases} \tau_{p,j}^{-}\tau_{p,j+2}^{+}\chi_p(\epsilon_p)^{-j-2},&j\ne0,4,\\ \tau_{p,4}^{-},&j=4,\\ -\tau_{p,2}^{+}\chi_p(\epsilon_p)^{-2},&j=0. \end{cases}

The indices of τ\tau are read modulo six. With M=λ12L4M=\lambda^{12}L^4, there is a number κF\kappa_F of absolute value one, depending only on h0h_0 and the class of rr modulo M2M^2, such that

ζ=−i81α‾(c)2ϕ^(h0)κ‾F∏p inactive(1−qp−1)∏p activeχp(σp)−2ωp,jp.\zeta=-\frac{i}{81}\overline{\alpha}(c)^2\widehat{\phi}(h_0)\overline{\kappa}_F \prod_{p\ \mathrm{inactive}}(1-q_p^{-1}) \prod_{p\ \mathrm{active}}\chi_p(\sigma_p)^{-2}\omega_{p,j_p}.

In each of the finitely many classes of h0h_0 and rr mod M2M^2, both dd and ϑ\vartheta are fixed. Consequently these are common column factors within that sector. Apart from the displayed scale qc2q_c^2, all other moving-prime dependence outside the BpB_p is in the scalar ζ\zeta, which may depend on the whole active set.

The branch conventions are simultaneous for all local prime sets with the same LL and Ψ0\Psi_0. In particular, if a good prime pp is added to the local set with exponent zero and is declared inactive, the resulting branch has the same cFc_F, cc, dd, ϑ\vartheta, κF\kappa_F, the same data at every other active prime, and the same kernel as the branch in which pp is absent. Its scalar is multiplied by 1−qp−11-q_p^{-1}. This compatibility includes every h0h_0, not only the unit classes modulo LL.

Bounds for the transformed test. For A≥0A \ge0 and an integer B≥0B \ge0, put

MA,B(V)=sup⁡−A≤η≤1/4∫R(1+∣u∣)B∣V^(η+iu)∣ du.\mathfrak{M}_{A,B}(V)=\sup_{-A\le\eta\le1/4}\int_{\mathbb{R}}(1+|u|)^B|\widehat{V}(\eta+iu)|\,du.

For every integer j≥0j\ge0,

∣(x∂x)jV♯(x)∣≪A,jmin⁡{x1/4,(1+x)−A}MA,⌈4A⌉+j+2(V).|(x\partial_x)^jV^\sharp(x)| \ll_{A,j}\min\{x^{1/4},(1+x)^{-A}\} \mathfrak M_{A,\lceil4A\rceil+j+2}(V).

If χ∈Cc∞(0,∞)\chi\in C_c^\infty(0,\infty) is fixed, Y>0Y>0, and J≥0J\ge0 is an integer, then

∫R(1+∣u∣)J∣∫0∞χ(y)V♯(Yy)y−iudyy∣du≪A,J,χmin⁡{Y1/4,(1+Y)−A}MA,⌈4A⌉+J+4(V).\int_{\mathbb R}(1+|u|)^J \left|\int_0^\infty\chi(y)V^\sharp(Yy)y^{-iu}\frac{dy}{y}\right|du \ll_{A,J,\chi}\min\{Y^{1/4},(1+Y)^{-A}\} \mathfrak M_{A,\lceil4A\rceil+J+4}(V).

These are finite smooth seminorms. More precisely,

MA,B(V)≪A,B∫0∞(1+x−A+x1/4)(∣V(x)∣+∣(x∂x)B+2V(x)∣)dxx.\mathfrak{M}_{A,B}(V)\ll_{A,B}\int_0^\infty(1+x^{-A}+x^{1/4})(|V(x)|+|(x\partial_x)^{B+2}V(x)|)\frac{dx}{x}.

Replacing V(x)V(x) by xiu0V(x)x^{iu_0}V(x) multiplies MA,B\mathfrak{M}_{A,B} by at most (1+∣u0∣)B(1+|u_0|)^B.

Proof. We first express the character masks through finitely many translated theta values. We then transform their rational cusps and compute the resulting automorphy multipliers and local Fourier factors; the final Mellin comparison gives the reflection identity and the bounds for its transformed test.

The fixed theta input. Let Γ=SL⁡2(O)\Gamma=\operatorname{SL}_2(\mathcal{O}), Γ1(3)={g∈Γ:g≡I(mod3)}\Gamma_1(3)=\{g\in\Gamma:g\equiv I\pmod3\}, and Γ2=⟨SL⁡2(Z),Γ1(3)⟩\Gamma_2=\langle\operatorname{SL}_2(\mathbb{Z}),\Gamma_1(3)\rangle. The unconditional formulas of [8 Equations (5.4), (5.7), (5.9), and (5.12)–(5.17)], give a smooth cubic theta function θ\theta on H3=C×R>0\mathbb{H}^3=\mathbb{C}\times\mathbb{R}_{>0} with

θ(gw)=κ(g)θ(w)(g∈Γ2),κ(abcδ′)=(ca)3((abcδ′)∈Γ1(3), c≠0).\theta(gw)=\kappa(g)\theta(w)\quad(g\in\Gamma_2),\qquad \kappa\begin{pmatrix}a&b\\c&\delta'\end{pmatrix}=\left(\frac{c}{a}\right)_3\quad\left(\begin{pmatrix}a&b\\c&\delta'\end{pmatrix}\in\Gamma_1(3),\ c\ne0\right).

Here κ\kappa is one on SL2(Z)\mathrm{SL}_2(\mathbb Z) and is one on an element of Γ1(3)\Gamma_1(3) with lower left entry zero. The subscript 3 denotes the ordinary cubic residue symbol; for a good prime p∉Sp\notin S, one has (x/p)3=χp(x)2(x/p)_3=\chi_p(x)^2. These automorphy and coefficient formulas have no hypothesis about zeros of LL-functions.

Put

L(t)=(10t1),(t0,t1,t2)=(0,ω2,ω),Θb(w)=θ(L(tb)w).\begin{aligned} \mathsf L(t)=\begin{pmatrix}1&0\\t&1\end{pmatrix},\qquad (t_0,t_1,t_2)=(0,\omega^2,\omega),\qquad \Theta_b(w)=\theta(\mathsf L(t_b)w). \end{aligned}

If v∈Z+3Ov\in\mathbb{Z}+3\mathcal{O}, then L(v)\mathsf L(v) is a product of an element of SL⁡2(Z)\operatorname{SL}_2(\mathbb{Z}) and a lower translation in Γ1(3)\Gamma_1(3) with multiplier one. The analogous assertion holds for upper translations. Therefore

θ(L(λ)w)=Θ1(w),θ(L(−λ)w)=Θ2(w),\theta(\mathsf L(\lambda)w)=\Theta_1(w),\qquad \theta(\mathsf L(-\lambda)w)=\Theta_2(w),

because λ−ω2=2+3ω\lambda-\omega^2=2+3\omega and −λ−ω=−1−3ω-\lambda-\omega=-1-3\omega. If u0=s+tωu_0=s+t\omega with 0≤s,t<30\le s,t<3, and E=(0−110)\begin{aligned}E=\bigl(\begin{smallmatrix}0&-1\\1&0\end{smallmatrix}\bigr)\end{aligned}, then

(u0−110)=EL(−u0),−u0−tt∈Z+3O,\begin{aligned} \begin{pmatrix}u_0&-1\\1&0\end{pmatrix}=E\mathsf L(-u_0), \qquad -u_0-t_t\in\mathbb Z+3\mathcal O, \end{aligned}

and hence θ((u0−110)w)=Θt(w)\begin{aligned}\theta\bigl(\bigl(\begin{smallmatrix}u_0&-1\\1&0\end{smallmatrix}\bigr)w\bigr) =\Theta_t(w)\end{aligned}. These are the only cusp representatives needed below.

For any of them, define dHd_H by

θ‾(H(z,v))=CH(v)+∑μ≠0dH(μ)vK1/3(4π∣μ∣v)eˇ(μz).\overline{\theta}(H(z,v))=C_H(v)+\sum_{\mu\ne0}d_H(\mu)vK_{1/3}(4\pi|\mu|v)\check{e}(\mu z).

Here CH(v)C_H(v) is independent of zz. The three functions Θ0,Θ1,Θ2\Theta_0,\Theta_1,\Theta_2 are respectively F1,F19,F10F_1,F_{19},F_{10} in [8]. Its Appendix A, rows 1, 19, 10, expresses their coefficients in terms of τ,τ1,τ2\tau,\tau_1,\tau_2 in its Equations (5.7), (5.13), and (5.14). In their notation the conjugate expansion uses dj(−μ)‾\overline{d_j(-\mu)}, as in their Equation (5.16). Those formulas give the support inclusion in Equation (5.2). For completeness, the two possible magnitudes from τ\tau at μ=uλknb3\mu=u\lambda^k nb^3 are

3k/6+8/3∣b∣and3k/6+3∣b∣,3^{k/6+8/3}|b| \qquad\text{and}\qquad3^{k/6+3}|b|,

and τ1,τ2\tau_1,\tau_2 have magnitude 9∣b∣9|b| and k=−4k=-4. Here the Gauss sums use only the cubic symbol, including at primes in SS. To make their domain explicit, for every primary squarefree nn define, as in [8 Equation (1.7)],

g~3(n)=qn−1/2∑v mod n(vn)3eˇ(v/n),g~3(1)=1.\widetilde g_3(n)=q_n^{-1/2}\sum_{v\bmod n} \left(\frac vn\right)_3\check e(v/n), \qquad \widetilde g_3(1)=1.

The ordinary cubic symbol is defined at every prime other than λ\lambda and is extended by zero on nonunits and multiplicatively in the denominator. Every primary nn is prime to λ\lambda. At each prime divisor of nn the cubic character is nontrivial, and eˇ(v/n)=e(λv/n)\check e(v/n)=e(\lambda v/n) is primitive because λ\lambda is a unit there. The finite-field Gauss identity and the Chinese remainder theorem therefore give ∣g~3(n)∣=1|\widetilde{g}_3(n)|=1 for every such squarefree nn. This includes the primary prime −2-2 of norm 44; no sextic character with that denominator is used. Also, whenever (t,n)=1(t,n)=1, the change of variable y=tvy=tv gives

qn−1/2∑v mod n(vn)3eˇ(tv/n)=(tn)3−1g~3(n).q_n^{-1/2}\sum_{v\bmod n}\left(\frac vn\right)_3\check e(tv/n) =\left(\frac tn\right)_3^{-1}\widetilde g_3(n).

This covers the twists t=λ2,ωλ2,ω2λ2t=\lambda^2,\omega\lambda^2,\omega^2\lambda^2 in the other source coefficient families. Thus the unnormalized Gauss sums occurring in all three cusp families have magnitude ∣n∣|n|. Consequently each coefficient magnitude displayed above is at most 27 3k/6∣b∣27\,3^{k/6}|b|, including k=−4k=-4. The formulas require only that nn be squarefree and that n,bn,b be primary; they do not require (n,b)=1(n,b)=1. Prime valuations of nb3nb^3 also show that its representation by such n,bn,b, when it exists, is unique. In particular the same bound is valid when the variables share primes or contain primes excluded from the primal sums.

At infinity the condition x=λ3μ≡1(mod3)x=\lambda^3\mu\equiv1\pmod3 isolates exactly μ=λ−3nb3\mu=\lambda^{-3}nb^3 with n,bn,b primary and nn squarefree. The infinity support has λ3μ∈O\lambda^3\mu\in\mathcal{O}; every other ramified exponent in Equation (5.7) of [8] makes xx divisible by λ\lambda, and the negative sign in the remaining pair gives x≡−1(mod3)x\equiv-1\pmod3. At the isolated index the coefficient in θˉ\bar{\theta} is

dI(λ−3nb3)=35/2∣b∣g~3(n).d_I(\lambda^{-3}nb^3)=3^{5/2}|b|\widetilde{g}_3(n).

This is the unmasked source formula, valid for every primary squarefree nn and every primary bb, with no coprimality condition between them. Only when (n,S)=1(n,S)=1 may it be expressed in the global sextic notation: substituting y=λvy=\lambda v in γ2(n)\gamma_2(n) gives

g~3(n)=(λn)3−1γ2(n)=χn(λ)−2γ2(n)((n,S)=1).\widetilde{g}_3(n)=\left(\frac{\lambda}{n}\right)_3^{-1}\gamma_2(n)=\chi_n(\lambda)^{-2}\gamma_2(n)\qquad((n,S)=1).

The cubic supplementary laws in [8 Equation (1.5)] make (λ/x)3(\lambda/x)_3 periodic on all primary xx modulo 99. On primary elements prime to SS it equals χx(λ)2\chi_x(\lambda)^2. A character in X\mathcal{X} is periodic on primary elements prime to E\mathfrak E modulo its conductor, and the zero condition (x,E)≠1(x,\mathfrak E)\ne1 is periodic modulo E\mathfrak E. Thus a sufficiently divisible LL with prime support SS works for every member of the fixed finite family. This verifies its choice before the moving local primes are selected.

Finite Fourier inversion with the zero extensions. For j∈{0,…,5}j\in\{0,\ldots,5\} define

Cp,j(h)=qp−1∑x mod pχp(x)je(−hx/p).C_{p,j}(h)=q_p^{-1}\sum_{x\bmod p}\chi_p(x)^j e(-hx/p).

The character pairing furnished by ee is nondegenerate on O/(p)\mathcal{O}/(p). Changing variables in a Gauss sum, and using the orthogonality of a nontrivial multiplicative character, gives

Cp,j(h)={qp−1/2τp,j−χp(h)−j,j≠0, h≠0,0,j≠0, h=0,−qp−1,j=0, h≠0,1−qp−1,j=0, h=0.C_{p,j}(h)= \begin{cases} q_p^{-1/2}\tau_{p,j}^{-}\chi_p(h)^{-j}, & j\ne0,\ h\ne0,\\ 0, & j\ne0,\ h=0,\\ -q_p^{-1}, & j=0,\ h\ne0,\\ 1-q_p^{-1}, & j=0,\ h=0. \end{cases}

Here and below h=0h=0 means h≡0(modp)h\equiv0\pmod p. Each nontrivial power of χp\chi_p is primitive modulo the prime pp, so the usual finite-field Gauss-sum identity gives ∣τp,m±∣=1|\tau_{p,m}^{\pm}|=1.

Fourier inversion on O/(L)\mathcal{O}/(L) and on each O/(p)\mathcal{O}/(p) now gives

ϕ(x)∏pχp(x)jp=∑hC(h)e ⁣(x(h0/L+∑php/p)),C(h)=ϕ^(h0)∏pCp,jp(hp).\phi(x)\prod_p\chi_p(x)^{j_p} =\sum_h C(h)e\!\left(x\left(h_0/L+\sum_p h_p/p\right)\right), \qquad C(h)=\widehat\phi(h_0)\prod_pC_{p,j_p}(h_p).

This uses every additive frequency, including nonunit h0h_0 and zero local frequencies. We do not invoke the twisted formula in [8 Lemma 5.2 and Corollary 5.1], whose unit-Fourier-support hypothesis need not hold for these masks. The theta function with this multiplier on its infinity coefficient x=λ3μ∈Ox=\lambda^3\mu\in\mathcal{O} is the finite sum

F(z,v)=∑hC(h)θˉ(z+zh,v),zh=λ2(h0/L+∑php/p).\mathcal F(z,v)=\sum_hC(h)\bar\theta(z+z_h,v),\qquad z_h=\lambda^2\left(h_0/L+\sum_p h_p/p\right).

For an isolated infinity index x=nb3x=nb^3, the piecewise definition of ϕ\phi first discards every term for which (nb,E)≠1(nb,\mathfrak{E})\ne1. This is a mask on the whole completed index: (nb3,E)=1(nb^3,\mathfrak{E})=1 if and only if both nn and bb are E\mathfrak{E}-units. Only on that remaining domain do we use complete multiplicativity, including χb(λ)6=1\chi_b(\lambda)^6=1, to write

ϕ(nb3)∏pχp(nb3)jp=χn(λ)2Ψ(n)Ψ(b)3((nb,E)=1).\phi(nb^3)\prod_p\chi_p(nb^3)^{j_p} =\chi_n(\lambda)^2\Psi(n)\Psi(b)^3 \qquad((nb,\mathfrak{E})=1).

It remains true when n,bn,b share a moving prime, since the corresponding local powers retain their zero values, including for jp=0j_p=0. For the discarded terms the completed coefficient is defined to be zero directly; no value of χn(λ)\chi_n(\lambda) is evaluated there. Combining Equations (5.9) and (5.10) on the retained domain now identifies the direct Mellin series with the product TT. The dual coefficient functions dHd_H keep the full source support in Equation (5.2); no SS-mask is placed on them.

Fix h0h_0 and declare pp active precisely when hp≠0h_p\ne0. Equation (5.11) forces all primes with jp≠0j_p\ne0 to be active. Choose once for each h0 mod Lh_0\bmod L a representative and a reduced expression λ2h0/L=aF/cF\lambda^2h_0/L=a_F/c_F. Multiplying numerator and denominator by one unit, normalize the numerator to be 1(mod3)1\pmod3 if λ∣cF\lambda\mid c_F and the denominator to be 1(mod3)1\pmod3 otherwise. Since every active prime is primary, this unit depends only on h0h_0. For r=∏p activepr=\prod_{p\ \mathrm{active}}p, Equation (5.12) then gives

zh=ac,c=cFr,a=aFr+λ2cF∑p∣r(r/p)hp.z_h=\frac{a}{c}, \qquad c=c_Fr, \qquad a=a_Fr+\lambda^2c_F\sum_{p\mid r}(r/p)h_p.

At a prime dividing cFc_F, the numerator is congruent to aFra_Fr and is a unit. At p∣rp\mid r, it is congruent to λ2cF(r/p)hp\lambda^2c_F(r/p)h_p and is again a unit. Thus this fraction is reduced, even when h0h_0 is a nonunit modulo LL. The empty product r=1r=1 is allowed. Replacing any lift by another changes zhz_h by an element of λ2O=3O\lambda^2\mathcal{O}=3\mathcal{O}, a period of θ\theta.

Choice of the cusp matrix and its multiplier. The next construction determines the automorphy multiplier and reflected additive phase for each reduced cusp fraction just obtained. Set M=λ12L4M=\lambda^{12}L^4. For every active pp, the Chinese remainder theorem permits the chosen nonzero class hph_p mod pp to be lifted with hp≡0(modM2)h_p\equiv0\pmod{M^2}. Restrict rr to one class modulo M2M^2. Equation (5.13) shows that aa is then fixed modulo McFMc_F; in fact its moving terms are divisible by M2cFM^2c_F, and aFra_F r is fixed modulo M2M^2, which is divisible by McFMc_F because cFc_F divides LL up to a unit. It also shows a≡1(mod3)a\equiv1\pmod3 if λ∣c\lambda\mid c, and c≡1(mod3)c\equiv1\pmod3 otherwise.

Choose δ′\delta' by the following compatible local congruences:

δ′≡a−1(modMcF)at every prime dividing cF,δ′≡0(modM)at every prime dividing M but not cF,δ′≡a−1(modp)(p∣r).\begin{aligned} \delta'&\equiv a^{-1}\pmod{Mc_F} &&\text{at every prime dividing }c_F,\\ \delta'&\equiv0\pmod M &&\text{at every prime dividing }M\text{ but not }c_F,\\ \delta'&\equiv a^{-1}\pmod p &&(p\mid r). \end{aligned}

The first line means the indicated prime-power parts of McFMc_F. All inverses exist because a/ca/c is reduced. Put b=(aδ′−1)/cb=(a\delta'-1)/c and g=(abcδ′)\begin{aligned}g=\bigl(\begin{smallmatrix}a&b\\c&\delta'\end{smallmatrix}\bigr)\end{aligned}. Then g∈Γg\in\Gamma, and division of aδ′−1a\delta'-1 by cc gives

b≡0(modM) at primes of cF,b≡−c−1(modM) at the other primes of M.b\equiv0\pmod M\text{ at primes of }c_F,\qquad b\equiv-c^{-1}\pmod M\text{ at the other primes of }M.

Consequently a,b,c,δ′a,b,c,\delta' have fixed residues at the needed powers of every prime dividing LL, independent of the classes hph_p. Whenever a zero entry would occur in a residue-symbol calculation, one may first translate zhz_h by λ2M2O\lambda^2M^2\mathcal O and then add a multiple of the combined congruence modulus to δ′\delta'. These changes preserve all displayed congruences and avoid the finitely many values making an entry zero. They do not change the translated theta function.

There are three cases, distinguished by vλ(c)v_\lambda(c). If 3∣c3\mid c, put H=IH=I. Then G=g∈Γ1(3)G=g\in\Gamma_1(3), and cubic reciprocity for the primary aa and the primary primes of rr gives

κ(G)=(cFa)3(ar)3.\kappa(G)=\left(\frac{c_F}{a}\right)_3\left(\frac{a}{r}\right)_3.

If vλ(c)=1v_\lambda(c)=1, take the unique u0∈{λ,−λ}u_0\in\{\lambda,-\lambda\} with u0≡c(mod3)u_0\equiv c\pmod3 and put H=L(u0)H=\mathsf L(u_0); these are the two possibilities because O/(λ)≃F3\mathcal O/(\lambda)\simeq\mathbb F_3. The congruences above show that G=gH−1∈Γ1(3)G=gH^{-1}\in\Gamma_1(3). Write A=a−u0bA=a-u_0b. Both AA and aa are primary, and they are coprime: (a,b)=1(a,b)=1 and (a,u0)=1(a,u_0)=1. The determinant equation gives

a(c−u0δ′)=cA−u0,bc≡−1(moda).a(c-u_0\delta')=cA-u_0,\qquad bc\equiv-1\pmod a.

It follows, by cubic reciprocity for a,Aa,A, that

κ(G)=(−u0A)3(aA)3−1=(−u0A)3(c/u0a)3=(−u0A)3(cF/u0a)3(ar)3.\begin{aligned} \kappa(G)&=\left(\frac{-u_0}{A}\right)_3\left(\frac{a}{A}\right)_3^{-1}\\ &=\left(\frac{-u_0}{A}\right)_3\left(\frac{c/u_0}{a}\right)_3 =\left(\frac{-u_0}{A}\right)_3\left(\frac{c_F/u_0}{a}\right)_3\left(\frac{a}{r}\right)_3. \end{aligned}

For the second equality, reduce AA modulo aa and use (A/a)3=(−u0b/a)3=(u0/a)3(c/a)3−1(A/a)_3=(-u_0b/a)_3=(u_0/a)_3(c/a)_3^{-1}; the cubic symbol of −1-1 is one. Finally suppose (λ,c)=1(\lambda,c)=1. Choose u0=s+tω≡a(mod3)u_0=s+t\omega\equiv a\pmod3 with 0≤s,t<30\le s,t<3 and put H=(u0−110)\begin{aligned}H=\bigl(\begin{smallmatrix}u_0&-1\\1&0\end{smallmatrix}\bigr)\end{aligned}. Here c≡1c\equiv1, δ′≡0\delta'\equiv0, and b≡−1(mod3)b\equiv-1\pmod3, so

G=gH−1=(−ba+bu0−δ′c+δ′u0)∈Γ1(3).G=gH^{-1}= \begin{pmatrix} -b&a+bu_0\\ -\delta'&c+\delta'u_0 \end{pmatrix}\in\Gamma_1(3).

Both −b-b and cc are primary. Moreover −bc=1−aδ′≡1(mod9)-bc=1-a\delta'\equiv1\pmod9. Factor δ′=uλkδ0\delta'=u\lambda^k\delta_0 with δ0\delta_0 primary. The supplementary laws make (uλk/(1−aδ′))3=1(u\lambda^k/(1-a\delta'))_3=1; cubic reciprocity makes (δ0/(1−aδ′))3=1(\delta_0/(1-a\delta'))_3=1 because the numerator after reciprocity is 1(modδ0)1\pmod{\delta_0}. Thus

(δ′−bc)3=1,κ(G)=(δ′−b)3=(δ′c)3−1=(ac)3=(acF)3(ar)3.\left(\frac{\delta'}{-bc}\right)_3=1,\qquad \kappa(G)=\left(\frac{\delta'}{-b}\right)_3 =\left(\frac{\delta'}{c}\right)_3^{-1} =\left(\frac{a}{c}\right)_3 =\left(\frac{a}{c_F}\right)_3\left(\frac{a}{r}\right)_3.

The last inverse uses aδ′≡1(modc)a\delta'\equiv1\pmod c.

In all three cases we have proved

κ(G)=κF∏p∣rχp(a)2,∣κF∣=1.\kappa(G)=\kappa_F\prod_{p\mid r}\chi_p(a)^2,\qquad|\kappa_F|=1.

The factor κF\kappa_F is constant as the active hph_p vary in the fixed sector. If 3∣c3\mid c, it is (cF/a)3(c_F/a)_3: the unit and λ\lambda-power factors are determined by a mod 9a\bmod9, and reciprocity determines the remaining fixed-prime factors from the residue of aa at the primes of cFc_F. In the middle case it is (−u0/A)3((cF/u0)/a)3(-u_0/A)_3((c_F/u_0)/a)_3, determined in the same way by the fixed residues of A=a−u0bA=a-u_0b and aa. In the last case it is (a/cF)3(a/c_F)_3, which is determined directly by the fixed denominator cFc_F and a mod cFa\bmod c_F. The displayed congruences for a,b,c,δ′a,b,c,\delta' therefore determine κF\kappa_F using only h0h_0 and r mod M2r\bmod M^2. They also determine the chosen one of the three functions Θb\Theta_b.

The reflected additive phase. Write x=λ4μx=\lambda^4\mu and DF=λ3cFD_F=\lambda^3c_F. At each p∣rp\mid r, Equation (5.13) gives a≡σphp(modp)a\equiv\sigma_ph_p\pmod p. Hence δ′≡σp−1hp−1(modp)\delta'\equiv\sigma_p^{-1}h_p^{-1}\pmod p. Additive Chinese remaindering for the coprime factors of DFrD_Fr gives the exact identity

eˇ(−δ′μ/c)=e(−δ′x/(DFr))=ϑ(x)∏p∣re(ϵphp−1x/p),ϑ(x)=e(−δF′r−1x/DF).\begin{aligned} \check e(-\delta'\mu/c) &=e(-\delta'x/(D_Fr))\\ &=\vartheta(x)\prod_{p\mid r}e(\epsilon_ph_p^{-1}x/p), \qquad \vartheta(x)=e(-\delta'_F r^{-1}x/D_F). \end{aligned}

Here δF′\delta'_F is the class of δ′\delta' modulo DFD_F, and r−1r^{-1} in the formula for ϑ\vartheta is taken modulo DFD_F. For example, the local numerator at pp is −δ′(DFr/p)−1=ϵphp−1-\delta'(D_Fr/p)^{-1}=\epsilon_ph_p^{-1}; this verifies the signs and the powers of λ\lambda. The chosen congruences fix δF′\delta'_F, since DFD_F divides the corresponding local moduli, and the sector fixes r−1 mod DFr^{-1}\bmod D_F. A common multiple of the finitely many DFD_F is therefore a fixed modulus for all the characters ϑ\vartheta.

Conjugating Equation (5.15) contributes κˉF∏p∣rχp(σp)−2χp(hp)−2\bar\kappa_F\prod_{p\mid r}\chi_p(\sigma_p)^{-2}\chi_p(h_p)^{-2}. For j≠0j\ne0, multiplication by Equation (5.11) leaves the local sum

qp−1/2τp,j−∑h≠0χp(h)−j−2e(ϵph−1x/p).q_p^{-1/2}\tau_{p,j}^{-} \sum_{h\ne0}\chi_p(h)^{-j-2}e(\epsilon_ph^{-1}x/p).

Upon putting y=h−1y=h^{-1}, the sum is a Gauss sum of exponent j+2j+2. If j≠4j\ne4, its value is qp1/2τp,j+2+χp(ϵpx)−j−2q_p^{1/2}\tau_{p,j+2}^{+}\chi_p(\epsilon_px)^{-j-2}, also at p∣xp\mid x because both sides then vanish. If j=4j=4, it is the Ramanujan sum

∑y≠0e(ϵpxy/p)=−1+qp1p∣x.\sum_{y\ne0}e(\epsilon_pxy/p)=-1+q_p1_{p\mid x}.

For an active j=0j=0, the same substitution gives

−qp−1∑h≠0χp(h)−2e(ϵph−1x/p)=−qp−1/2τp,2+χp(ϵpx)−2.-q_p^{-1}\sum_{h\ne0}\chi_p(h)^{-2}e(\epsilon_ph^{-1}x/p) =-q_p^{-1/2}\tau_{p,2}^{+}\chi_p(\epsilon_px)^{-2}.

These are exactly ωp,jBp(x)\omega_{p,j}B_p(x); an inactive zero exponent contributes 1−qp−11-q_p^{-1}. This proves every local factor, including its zero extension. The choices of h0h_0 and the active subset give at most qL2#{p:jp=0}q_L2^{\#\{p:j_p=0\}} terms. Splitting the jp=4j_p=4 factors multiplies this by at most 2#{p:jp=4}2^{\#\{p:j_p=4\}}, proving the stated counts.

The denominator and the fixed-sector data constructed before these local sums depend on the local prime set only through h0h_0 and the active radical rr; the remaining active-frequency dependence is exactly the local dependence just summed. We use the same representatives and normalized fractions for each h0h_0, and the same fixed-sector choices of cusp function, fixed additive character, and κF\kappa_F whenever those data recur. An absent prime and an inactive zero-exponent prime have the same active radical; their other active σp,ϵp\sigma_p,\epsilon_p are therefore also identical. The inactive coefficient 1−qp−11-q_p^{-1} is the only change. This proves the simultaneous branch compatibility in the statement.

The marked reflection in Section 14.2 will use the following dependence on pairs of active primes. Since

ϵp=−λ−5(c/p)−2(modp),\epsilon_p=-\lambda^{-5}(c/p)^{-2}\pmod p,

there is a scalar ξp,j\xi_{p,j} of absolute value one, depending on p,jp,j but on no other active prime such that

χp(σp)−2ωp,j=ξp,jχp(c/p)2j+2.\chi_p(\sigma_p)^{-2}\omega_{p,j} =\xi_{p,j}\chi_p(c/p)^{2j+2}.

For j=4j=4 this uses 2j+2≡−2(mod6)2j+2\equiv-2\pmod6; for the other exponents it follows immediately by inserting the expression for ϵp\epsilon_p. Thus the contribution of another active prime to the phase at pp has exponent exactly 2j+22j+2 modulo six. In particular an active exponent j=1j=1 has column coupling χp(x)−3=χp(x)3\chi_p(x)^{-3}=\chi_p(x)^3.

Mellin normalization and continuation. Let

J(s)=∫0∞∂zˉF(z,v)∣z=0v2s−1 dv.J(s)=\int_0^\infty\left.\partial_{\bar z}\mathcal{F}(z,v)\right|_{z=0}v^{2s-1}\,dv.

The Bessel identity used in [8 Lemma 5.3] is

∫0∞K1/3(y)yw−1 dy=2w−2Γ((w−1/3)/2)Γ((w+1/3)/2)(ℜw>1/3).\int_0^\infty K_{1/3}(y)y^{w-1}\,dy =2^{w-2}\Gamma((w-1/3)/2)\Gamma((w+1/3)/2) \qquad(\Re w>1/3).

On ℜs>1\Re s>1 the coefficient sums converge absolutely, so we may differentiate and integrate their expansions term by term. Since ∂zˉeˇ(μz)=2πiμ‾eˇ(μz)\partial_{\bar z}\check e(\mu z)=2\pi i\overline{\mu}\check e(\mu z), the identity with w=2s+1w=2s+1 gives

J(s)=i4(2π)−2sΓ(s+1/3)Γ(s+2/3)∑0≠μ∈λ−3OdI(μ)ϕ(λ3μ)∏pχp(λ3μ)jpαˉ(μ)qμ−s.J(s)=\frac i4(2\pi)^{-2s}\Gamma(s+1/3)\Gamma(s+2/3) \sum_{0\ne\mu\in\lambda^{-3}\mathcal O}d_I(\mu)\phi(\lambda^3\mu) \prod_p\chi_p(\lambda^3\mu)^{j_p} \bar\alpha(\mu)q_\mu^{-s}.

First use the whole-index mask to restrict to (nb,E)=1(nb,\mathfrak{E})=1 as above, then insert Equations (5.9) and (5.10). Using qλ−3=27−1q_{\lambda^{-3}}=27^{-1} and αˉ(λ−3)=−i\bar\alpha(\lambda^{-3})=-i gives

J(s)=35/24(27(2π)2)sΓ(s+1/3)Γ(s+2/3)T(s,Ψ).J(s)=\frac{3^{5/2}}{4}\left(\frac{27}{(2\pi)^2}\right)^s\Gamma(s+1/3)\Gamma(s+2/3)T(s,\Psi).

For one translated term zh=a/cz_h=a/c, use the matrix g=GHg=GH constructed above. The coordinate action of g−1g^{-1} on hyperbolic space, from [8 Equation (5.1)], gives

g−1(z+a/c,v)=(−δ′c−zˉc2(v2+∣z∣2),vqc(v2+∣z∣2)).g^{-1}(z+a/c,v)=\left(-\frac{\delta'}{c}-\frac{\bar z}{c^2(v^2+|z|^2)},\frac{v}{q_c(v^2+|z|^2)}\right).

At z=0z=0, the derivative of its first coordinate with respect to zˉ\bar z is −(cv)−2-(cv)^{-2}; the derivatives of its conjugate coordinate and of its vertical coordinate with respect to zˉ\bar z are zero. The chain rule and θˉ(gw)=κˉ(G)θˉ(Hw)\bar\theta(gw)=\bar\kappa(G)\bar\theta(Hw) therefore give

∂zˉθˉ(z+a/c,v)∣z=0=−κˉ(G)c2v2∂zθˉ(H(z,1/(qcv)))∣z=−δ′/c.\left.\partial_{\bar z}\bar\theta(z+a/c,v)\right|_{z=0} =-\frac{\bar\kappa(G)}{c^2v^2} \left.\partial_z\bar\theta(H(z,1/(q_cv)))\right|_{z=-\delta'/c}.

In particular the derivative removes CH(v)C_H(v) from every cusp expansion in Equation (5.7). Substituting that expansion and then v↦1/(qcv)v\mapsto1/(q_cv) in the integral gives, for ℜs<0\Re s<0, the contribution

−i4(2π)2s−2αˉ(c)2qc1−2sκˉ(G)∏±Γ(3/2−s±1/6)×∑μ≠0dH(μ)α(μ)eˇ(−δ′μ/c)qμ−(1−s).\begin{aligned} -\frac i4(2\pi)^{2s-2}\bar\alpha(c)^2q_c^{1-2s}\bar\kappa(G) \prod_{\pm}\Gamma(3/2-s\pm1/6)\\ {} \times\sum_{\mu\ne0}d_H(\mu)\alpha(\mu) \check e(-\delta'\mu/c)q_\mu^{-(1-s)}. \end{aligned}

To verify the scalar directly, before applying the Bessel integral the factor is −2πic−2qc2−2s-2\pi i c^{-2}q_c^{2-2s} and the remaining integral is ∫0∞u2−2sK1/3(4π∣μ∣u) du\int_0^\infty u^{2-2s}K_{1/3}(4\pi|\mu|u)\,du. The Bessel identity with w=3−2sw=3-2s, together with c−2=αˉ(c)2/qcc^{-2}=\bar\alpha(c)^2/q_c, gives exactly the display.

We justify both the continuation and the contour operations here. The coefficient bound in Equation (5.2) implies absolute convergence of the reflected series when ℜ(1−s)>1\Re(1-s)>1: the separate majorants are

∑nsfqn−(1−ℜs),∑bqb1/2−3(1−ℜs),∑k≥−43k(1/6−(1−ℜs)).\sum_n^{\rm sf}q_n^{-(1-\Re s)},\qquad \sum_b q_b^{1/2-3(1-\Re s)},\qquad \sum_{k\ge-4}3^{k(1/6-(1-\Re s))}.

Each converges in that region. The fixed support has a positive lower bound for ∣μ∣|\mu|. The exponential decay of K1/3K_{1/3} and of all its derivatives, the coefficient bound, and the direct expansion imply exponential decay at v→∞v\to\infty for every logarithmic derivative of each translated derivative. The chain-rule formula just obtained implies exponential decay at v→0v\to0 as well, with constants depending on the fixed translated term. Repeated integration by parts in log⁡v\log v now shows that JJ is entire and decreases faster than every power of ∣ℑs∣|\Im s| on each fixed strip.

Equation (5.18), with reciprocal gamma functions on its right, continues TT to an entire function. Its direct series is bounded on any line to the right of 11. Equation (5.19) and Stirling’s formula give a polynomial bound on any line to the left of 00; the exponential parts of the two gamma products cancel. On a strip between such lines, the rapid bound for JJ and the reciprocal gamma factors first give ∣T(σ+it)∣≪(1+∣t∣)Ceπ∣t∣|T(\sigma+it)|\ll(1+|t|)^C e^{\pi|t|} for some CC. Divide TT by a sufficiently large power of B+sB+s, with BB chosen so that B+sB+s has no zero on the strip, and multiply by eεs2e^{\varepsilon s^2}. The horizontal sides of a growing rectangle tend to zero for each ε>0\varepsilon>0. The maximum principle, followed by ε→0\varepsilon\to0, transfers the polynomial bounds on the two vertical sides to the strip. This proves the stated polynomial strip growth.

Shift the integral on the left of Equation (5.1) from ℜs=a\Re s=a to ℜs=1/2−σ<0\Re s=1/2-\sigma<0 with σ>1/2\sigma>1/2. The entire continuation, polynomial strip bound, and rapid Mellin decay justify the shift: Equation (4.11) applied to the weighted logarithmic derivatives of VV makes the horizontal joins tend to zero. Inserting Equation (5.19) divided by Equation (5.18), and putting t=1/2−st=1/2-s, gives the gamma quotient R(t)R(t) and the factor

−i81αˉ(c)2qμ−1/2(KqμXqc2)−t.-\frac i{81}\bar\alpha(c)^2q_\mu^{-1/2} \left(\frac{Kq_\mu X}{q_c^2}\right)^{-t}.

Indeed (2π)4s−227−s3−5/2=3−4K−t(2\pi)^{4s-2}27^{-s}3^{-5/2} =3^{-4}K^{-t} and qc1−2sqμs−1=qμ−1/2(qμ/qc2)−tq_c^{1-2s}q_\mu^{s-1}=q_\mu^{-1/2}(q_\mu/q_c^2)^{-t}. The reflected coefficient series is absolutely convergent on this line, so it may be interchanged with the integral. Summing its finite local factors using Equation (5.16) and the computed Gauss sums proves Equation (5.1) and Equation (5.3). Since ∣ϕ∣≤1|\phi|\le1, we have ∣ϕ^(h0)∣≤1|\widehat\phi(h_0)|\le1; every other factor in the scalar has absolute value at most one. This proves ∣ζ∣≤1/81|\zeta|\leq1/81.

Uniform estimates for the transformed test. The first negative pole of the numerator of R(t)R(t) is −5/6-5/6. The reciprocal denominator gamma functions are entire. Hence the integrand defining V♯V^{\sharp} is holomorphic for ℜt>−5/6\Re t>-5/6. On −1/4≤σ≤A-1/4\leq\sigma\leq A, Stirling’s formula gives

∣R(σ+iu)∣≪A(1+∣u∣)4σ.|R(\sigma+iu)|\ll_A (1+|u|)^{4\sigma}.

The estimate is uniform also for bounded uu, since this closed strip has no numerator pole. Equation (4.11) makes V^\widehat{V} rapidly decreasing pointwise on every vertical strip. Rectangular contour shifts are therefore valid within −1/4≤ℜt≤A-1/4\leq\Re t\leq A, including between any two nonnegative lines. Applying (x∂x)j(x\partial_x)^j contributes (−t)j(-t)^j. The three lines −1/4,0,A-1/4,0,A bound the resulting integral respectively by constant multiples of

x1/4MA,⌈4A⌉+j+2(V),MA,⌈4A⌉+j+2(V),x−AMA,⌈4A⌉+j+2(V).x^{1/4}\mathfrak M_{A,\lceil4A\rceil+j+2}(V),\quad \mathfrak M_{A,\lceil4A\rceil+j+2}(V),\quad x^{-A}\mathfrak M_{A,\lceil4A\rceil+j+2}(V).

Combining them proves Equation (5.4). The rapid large-xx bound, with AA arbitrarily large, also makes every dual sum in Equation (5.1) absolutely convergent when V♯V^{\sharp} is represented on the zero line. Thus the shift of the kernel contour does not require a termwise shift of a conditionally convergent Dirichlet series.

For Equation (5.5), set fY(v)=χ(ev)V♯(Yev)f_Y(v)=\chi(e^v)V^\sharp(Ye^v). This is supported on a fixed compact interval. Integrating its Fourier transform by parts J+2J+2 times and using the trivial bound for ∣u∣≤1|u|\le1 gives

∫R(1+∣u∣)J∣f^Y(u)∣ du≪J∑j=0J+2∥fY(j)∥L1(R).\int_{\mathbb R}(1+|u|)^J|\widehat f_Y(u)|\,du \ll_J\sum_{j=0}^{J+2}\|f_Y^{(j)}\|_{L^1(\mathbb R)}.

Leibniz’s rule and Equation (5.4) bound each norm by the right side of Equation (5.5), because eve^v stays in a fixed compact subinterval of (0,∞)(0,\infty). Finally, for ∣u∣≥1|u|\ge1, B+2B+2 integrations by parts give

∣V^(η+iu)∣≤∣η+iu∣−B−2∫0∞∣(x∂x)B+2V(x)∣xηdxx.|\widehat{V}(\eta+iu)|\le|\eta+iu|^{-B-2}\int_0^\infty|(x\partial_x)^{B+2}V(x)|x^\eta\frac{dx}{x}.

For ∣u∣≤1|u|\le1 use the corresponding undifferentiated integral. On −A≤η≤1/4-A\le\eta\le1/4, xη≤1+x−A+x1/4x^\eta\le1+x^{-A}+x^{1/4}, proving Equation (5.6). The identity xiu0V^(η+iu)=V^(η+i(u+u0))\widehat{x^{iu_0}V}(\eta+iu)=\widehat V(\eta+i(u+u_0)) and 1+∣u∣≤(1+∣u+u0∣)(1+∣u0∣)1+|u|\le(1+|u+u_0|)(1+|u_0|) give the asserted norm-twist bound. In particular the Gaussian test V(x)=(2π)−1exp⁡(−(log⁡x)2/4)V(x)=(2\sqrt{\pi})^{-1}\exp(-(\log x)^2/4), whose Mellin transform is et2e^{t^2}, satisfies the hypotheses of this Proposition directly. □

Element rows and fixed sectors

To apply the reflection to a character A↦χA(m)A\mapsto\chi_A(m), we separate the fixed supplementary phases from the good prime divisors of the row. The separation retains the zero at every shared good prime.

Lemma 5.2 (Fixed ray sectors for nonzero rows). Let Ψbase\Psi_{\mathrm{base}} range over a fixed finite family of finite-ray characters with conductors supported on SS, extended by zero off the primary elements prime to SS. Use the fixed generators πl\pi_{\mathfrak l} for l∈S\mathfrak l\in S from Lemma 4.1. For 0≠m∈O0\ne m\in\mathcal{O}, write uniquely

m=umSmgood,mS=∏l∈Sπlvl(m),mgood=∏p∉Spvp(m),m=u m_Sm_{\rm good},\qquad m_S=\prod_{\mathfrak l\in S}\pi_{\mathfrak l}^{v_{\mathfrak l}(m)},\qquad m_{\rm good}=\prod_{p\notin S}p^{v_p(m)},

where the good prime generators are primary and uu is a unit. On every primary element AA prime to SS one has

χA(m)=χA(umS)R(A,mgood)∏p∣mgoodχp(A)vp(m).\chi_A(m)=\chi_A(um_S)\mathcal{R}(A,m_{\mathrm{good}})\prod_{p\mid m_{\mathrm{good}}}\chi_p(A)^{v_p(m)}.

All powers on the right retain their zero values, including when vp(m)≡0(mod6)v_p(m)\equiv0\pmod6. Fix uu, the valuations vl(m)v_{\mathfrak l}(m) modulo six, and the class of mgoodm_{\mathrm{good}} in the fixed ray group through which R\mathcal{R} factors. In such a sector define

Ψ0[m](A)={Ψbase(A)χA(umS)R(A,mgood),A≡1(mod3), (A,S)=1,0,otherwise.\Psi_0^{[m]}(A)= \begin{cases} \Psi_{\mathrm{base}}(A)\chi_A(um_S)\mathcal{R}(A,m_{\mathrm{good}}),&A\equiv1\pmod3,\ (A,S)=1,\\ 0,&\text{otherwise}. \end{cases}

The nonzero branch is a member of a fixed finite family of finite-ray characters with conductors supported on SS. Therefore a single E,L\mathfrak E,L in Proposition 5.1 works for all these sectors. The local prime set contains every p∣mgoodp\mid m_{\mathrm{good}}, with exponent vp(m)v_p(m) modulo six, even when this exponent is zero. No moving good prime is absorbed into LL.

Proof. If (A,mgood)=1(A,m_{\mathrm{good}})=1, multiplicativity and the symmetric reciprocity factor in Lemma 4.4 give Equation (5.20). If a good prime is shared, both sides are zero: the left side is the zero extension of χA(m)\chi_A(m), and its local factor on the right is zero even for a six-divisible exponent. This proves the identity on the entire stated domain.

On this domain χA(umS)\chi_A(um_S) depends only on uu and the SS-valuations modulo six, because every numerator factor is a unit modulo AA. For each of the finitely many representatives d=u∏l∈Sπleld=u\prod_{\mathfrak l\in S}\pi_{\mathfrak l}^{e_{\mathfrak l}}, 0≤el<60\le e_{\mathfrak l}<6, Lemma 4.1 identifies A↦χA(d)A\mapsto\chi_A(d) with a finite-ray character whose conductor is supported at primes over 6d6d, all in SS. Once the good ray class is fixed, A↦R(A,mgood)A\mapsto\mathcal R(A,m_{\rm good}) is one of a fixed finite family of characters supported at the primes over 2,32,3. Their products with the finite family of base characters give the asserted fixed family. Choosing a common multiple of its conductors and the SS-mask gives the common E\mathfrak E and then LL. Additional good local residue-symbol factors in a completed coefficient are placed in P\mathcal{P} and combined at a shared prime with the same zero convention; they do not alter this fixed modulus. The argument requires m≠0m\ne0 and makes no local-prime assertion for the row m=0m=0.

Common profiles and lattice tails

The reflected series has a scale depending on its row. We keep that dependence inside one joint smooth profile until after Fourier inversion; this gives one coefficient measure for the whole row norm.

Lemma 5.3 (Common annular kernel profile). Let VV satisfy the hypotheses of Proposition 5.1. Fix an integer d≥1d\ge1, a compact set Ω⊂Rd\Omega\subset\mathbb{R}^d, and real exponents a1,…,ada_1,\ldots,a_d. Let WW be one smooth profile with logarithmic support in Ω\Omega, common to all rows in a given block, and let Y>0Y>0 be fixed within that block. Put

h(y)=∏i=1dyiai,FY(y)=W(y)V♯(Yh(y)),mA(Y)=min⁡{Y1/4,(1+Y)−A}.h(\boldsymbol y)=\prod_{i=1}^d y_i^{a_i},\qquad F_Y(\boldsymbol y)=W(\boldsymbol y)V^\sharp(Yh(\boldsymbol y)),\qquad \mathfrak m_A(Y)=\min\{Y^{1/4},(1+Y)^{-A}\}.

For A≥0A\ge0 and integers j,J≥0j,J\ge0,

pj(FY)≪A,j,d,Ω,amA(Y)pj(W)MA,⌈4A⌉+j+2(V),p_j(F_Y)\ll_{A,j,d,\Omega,\boldsymbol{a}}\mathfrak m_A(Y)p_j(W)\mathfrak{M}_{A,\lceil4A\rceil+j+2}(V),
∥FY∥J,sep≪A,J,d,Ω,amA(Y)pJ+d+2(W)MA,⌈4A⌉+J+d+4(V).\lVert F_Y\rVert_{J,\mathrm{sep}}\ll_{A,J,d,\Omega,\boldsymbol{a}}\mathfrak m_A(Y)p_{J+d+2}(W)\mathfrak{M}_{A,\lceil4A\rceil+J+d+4}(V).

Here pjp_j is the homogeneous seminorm of a single profile, not the inhomogeneous seminorm of a tuple. The constants are independent of YY and of the actual norm labels within the block.

Proof. On the support of WW, the monomial hh is bounded above and below by positive constants depending only on Ω\Omega and the exponents. Each operator yi∂yiy_i\partial_{y_i} acting on V♯(Yh(y))V^\sharp(Yh(\boldsymbol{y})) is aia_i times the Euler derivative of V♯V^\sharp at Yh(y)Yh(\boldsymbol{y}). It produces no additional power of YY. Leibniz’s rule and (5.4) prove (5.22). Applying Lemma 4.5 with j=J+d+2j=J+d+2 gives (5.23).

Here is the norm consequence, including its order of operations. Let I\mathcal{I} be the original row set, and suppose a row vector U\mathcal U is linear in the whole profile FYF_Y. The profile includes the cutoffs for the full fixed logarithmic boxes of its row and column norm variables. Assume that simultaneous logarithmic Fourier inversion expresses the vector using one density common to every row. After the relevant arithmetic coefficient independences have been verified, write FY=mA(Y)F~YF_Y=\mathfrak m_A(Y)\widetilde F_Y. Minkowski gives

∥U∥ℓ2(I)≤mA(Y)(2π)d∫Rd∣F~Y^(t)∣∥B(t)∥ℓ2(I) dt.\|\mathcal U\|_{\ell^2(\mathcal I)} \le \frac{\mathfrak m_A(Y)}{(2\pi)^d} \int_{\mathbb R^d}|\widehat{\widetilde F_Y}(\boldsymbol t)| \|B(\boldsymbol t)\|_{\ell^2(\mathcal I)}\,d\boldsymbol t.

Here B(t)B(\boldsymbol t) is the separated row vector, whose norm powers all have absolute value one. The identity underlying this inequality is a Bochner integral in ℓ2(I)\ell^2(\mathcal{I}); the finite separation norm above ensures its absolute integrability whenever the separated norm has the stated polynomial height growth. Uniform bounds for densities chosen separately for individual rows would not give this identity. Only inside the nonnegative norm on the right may the row set subsequently be enlarged, using the same separated formula for BB on the added rows. No comparison of the kernel argument with YY is asserted on the added rows. Squaring this inequality gives the factor mA(Y)2\mathfrak m_A(Y)^2. If only the small-argument bound is being used, the same argument permits the weaker scalar min⁡{1,Y1/4}\min\{1,Y^{1/4}\}, whose square is min⁡{1,Y1/2}\min\{1,Y^{1/2}\}. The normalized profile has bounded tuple seminorms; they are not claimed to be small, since the tuple seminorm includes a constant one. A kernel occurring once in an already expanded quadratic expression instead contributes its scalar once, not automatically its square.

The Gaussian test in Proposition 5.1 is directly admissible there and in Lemma 5.3: only the joint factor WW in the latter lemma needs compact logarithmic support. If the compact-support calculus is instead applied to the Gaussian itself, Lemma 4.6 supplies the required absolutely summable annular decomposition.

Lemma 5.4 (Lattice kernel tails). Let Λ\Lambda be either O\mathcal{O} or λ−4O\lambda^{-4}\mathcal{O}. Suppose K:(0,∞)→CK:(0,\infty)\to\mathbb{C} satisfies ∣K(x)∣≤CAx−A|K(x)|\le C_Ax^{-A} for x≥1x\ge1, where A>1A>1. Then, for a>0a>0 and U≥1U\ge1,

∑0≠μ∈Λaqμ>U∣K(aqμ)∣≪ACA(1+a−1)U1−A.\sum_{\substack{0\ne\mu\in\Lambda\\ aq_\mu>U}} |K(aq_\mu)| \ll_A C_A(1+a^{-1})U^{1-A}.

For K=V♯K=V^\sharp one may take CA≪AMA,⌈4A⌉+2(V)C_A\ll_A\mathfrak M_{A,\lceil4A\rceil+2}(V).

Proof. The shell 2jU<aqμ≤2j+1U2^jU<aq_\mu\le2^{j+1}U contains O(1+2jU/a)O(1+2^jU/a) points of either fixed lattice. Its contribution is at most CA(1+2jU/a)(2jU)−AC_A(1+2^jU/a)(2^jU)^{-A}. Summing the two geometric series gives OA(CA(U−A+a−1U1−A))O_A(C_A(U^{-A}+a^{-1}U^{1-A})), which implies the display because U≥1U\ge1. The last assertion follows from Equation (5.4).

A quadratic norm for completed indices

The next estimate bounds the quadratic character left by reflection on a squarefree factor times a cube. We begin with the imported sieve. For squarefree primary ideals outside a fixed set containing the primes over 66, the quadratic kernel χa(b)3\chi_a(b)^3 satisfies

∑a sfqa≤U∣∑b sfqb≤Vcbχa(b)3∣2≪ϵ(UV)ϵ(U+V)∑b∣cb∣2.\sum_{\substack{a\ \mathrm{sf}\\q_a\le U}} \left|\sum_{\substack{b\ \mathrm{sf}\\q_b\le V}} c_b\chi_a(b)^3\right|^2 \ll_\epsilon(UV)^\epsilon(U+V)\sum_b|c_b|^2.

This is Goldmakher–Louvel’s quadratic large sieve [13 Definition 1 and Theorem 1.1]. To verify its family hypotheses, let ϑa((x))\vartheta_a((x)) denote the quadratic residue symbol evaluated at the primary generator of (x)(x). The adjustment of xx to its primary generator contributes ελ(x)e(a)\varepsilon_\lambda(x)^{e(a)}, where ελ\varepsilon_\lambda is the nontrivial character modulo λ\lambda and e(a)=(qa−1)/2 mod 2e(a)=(q_a-1)/2\bmod2. The powers of ω\omega contribute nothing because they are squares. CRT therefore gives exact primitive conductor aλe(a)a\lambda^{e(a)} and trivial infinite type. We use the primitive inducing character: the displayed formula first specifies its restriction to the λ\lambda-units, and the factor at λ\lambda is absent when e(a)=0e(a)=0. This does not change any value on the indices in Equation (5.26). In a fixed primary square class modulo 44, two indices have the same e(a)e(a); for coprime such indices the primitive product has conductor exactly their product. The reciprocity factor is the fixed bicharacter R\mathcal{R} of Equation (4.4). These are precisely the family conditions of the cited theorem. A finite ray partition and transpose duality give Equation (5.26) in the displayed orientation.

A fixed restriction on the row set decreases the positive outer sum. A fixed restriction on the coefficient support is implemented by setting the omitted coefficients to zero. Neither observation permits an arbitrary mask depending simultaneously on a row and a column. The next reduction resolves the collision mask produced by square factors of a completed index.

Lemma 5.5 (Quadratic reduction for completed indices). Let K,N,B≥1K,N,B \ge1. Let I\mathcal{I} be any set of squarefree primary good ideals kk with qk≪Kq_k \ll K. Let nn range over squarefree primary ideals with qn≍Nq_n \asymp N, and let bb range over primary ideals with qb≍Bq_b \asymp B. The ideals n,bn,b may contain primes of SS other than λ\lambda. Let β(n,b)\beta(n,b) be arbitrary complex coefficients independent of kk. Fixed restrictions on I\mathcal{I} and fixed restrictions on the (n,b)(n,b)-support are allowed.

Write uniquely b=gt2b=gt^2 with gg squarefree, and set c=(n,g)c=(n,g), n=cmn=cm, g=chg=ch. Thus c,m,hc,m,h are pairwise coprime and squarefree. Fix one set of dyadic ranges

qc≍C,qg≍G,qt≍T,B≍GT2,q_c \asymp C,\qquad q_g \asymp G,\qquad q_t \asymp T,\qquad B\asymp GT^2,

where all comparison constants are fixed. Let QC,G,T(β)\mathcal Q_{C,G,T}(\beta) be the sum over k∈Ik\in\mathcal{I} of the squared absolute value of the (n,b)(n,b)-sum restricted to this set of ranges, with summand β(n,b)χk(nb)3\beta(n,b)\chi_k(nb)^3. For a squarefree good ideal rr and a fixed tt, let Dr(t)\mathcal{D}_r(t) be the set of triples (c′,m,h)(c',m,h) for which

c=rc′,n=rc′m,b=rc′ht2c=rc',\qquad n=rc'm,\qquad b=rc'ht^2

belongs to the original support and to these ranges, with the stated squarefreeness and pairwise coprimality of c,m,hc,m,h. Then

QC,G,T(β)≪ϵ(KNB)ϵT∑qt≍T ∑r sf, (r,S)=1qr≪min⁡(K,C)(Kqr+NGC2)Cqr∑(c′,m,h)∈Dr(t)∣β(rc′m,rc′ht2)∣2.\begin{aligned} \mathcal Q_{C,G,T}(\beta) \ll_\epsilon{}&(KNB)^\epsilon T \sum_{q_t\asymp T}\ \sum_{\substack{r\ {\rm sf},\ (r,S)=1\\q_r\ll\min(K,C)}} \left(\frac K{q_r}+\frac{NG}{C^2}\right)\frac C{q_r} \sum_{(c',m,h)\in\mathcal D_r(t)} |\beta(rc'm,rc'ht^2)|^2. \end{aligned}

Empty quotient ranges contribute zero; all bounded ranges, including the unit ideal, are included by the fixed comparison constants. Fixed ray sectors and bounded row scalars are permitted. In particular, if ∣β(n,b)∣≤1|\beta(n,b)|\le1, then

∑k∈I∣∑n,bβ(n,b)χk(nb)3∣2≪ϵ(KNB)ϵ(K+NB)NB.\sum_{k\in\mathcal{I}}\left|\sum_{n,b}\beta(n,b)\chi_k(nb)^3\right|^2\ll_\epsilon(KNB)^\epsilon(K+NB)NB.

The constants may depend on the fixed support comparisons and on SS, but are uniform in the coefficients and in the permitted support restrictions.

Proof. The factorization b=gt2b=gt^2 permits gg and tt to share primes. Since nb=c2mht2nb=c^2mht^2, the zero convention gives the exact identity

χk(nb)3=χk(mh)3 1(k,ct)=1.\chi_k(nb)^3=\chi_k(mh)^3\,1_{(k,ct)=1}.

Indeed a square has sixth power under the displayed quadratic character; this is one on units and zero at a collision. The identity therefore also holds when nn or gg shares a prime with tt.

For the chosen ranges there are O(T)O(T) possible tt. Hilbert-space Cauchy gives

∥∑qt≍TFt∥22≪T∑qt≍T∥Ft∥22.\left\|\sum_{q_t\asymp T}F_t\right\|_2^2\ll T\sum_{q_t\asymp T}\|F_t\|_2^2.

Fix tt in the positive sum. The condition (k,t)=1(k,t)=1 is now a fixed row restriction. For the remaining condition use the full identity

1(k,c)=1=∑r∣(k,c)μ(r).1_{(k,c)=1}=\sum_{r\mid(k,c)}\mu(r).

For each kk the number of possible rr is at most dO(k)d_{\mathcal O}(k). Rowwise Cauchy followed by summation over kk costs (KNB)ϵ(KNB)^\epsilon and gives a positive sum over fixed squarefree good rr. Write k=rk′k=rk' and c=rc′c = rc'. Squarefreeness gives the fixed row restriction (k′,r)=1(k',r)=1 and the coefficient restriction (c′,r)=1(c',r)=1; terms with (r,t)>1(r,t)>1 vanish, and otherwise (k′,t)=1(k',t)=1 is another fixed row restriction. There is no remaining (k′,c′)(k',c') condition in an individual rr-summand: the full collision mask was already expanded. A fixed ray sector for kk becomes a fixed sector for k′k' once rr is fixed.

The factor χr(mh)3\chi_r(mh)^3 is a bounded column factor. Split the squarefree parts of m,hm,h supported on SS from their good parts: m=mSmgm=m_Sm_{\rm g} and h=hShgh=h_Sh_{\rm g}. There are only finitely many choices of mS,hSm_S,h_S. Their symbols are bounded row factors, while j=mghgj=m_{\rm g}h_{\rm g} is squarefree and good, of norm O(NG/C2)O(NG/C^2). For fixed r,t,mS,hSr,t,m_S,h_S, group the remaining columns by jj. If CjC_j is the resulting coefficient, the quadratic large sieve gives

∑k′∣∑jCjχk′(j)3∣2≪ϵ(KNB)ϵ(Kqr+NGC2)∑j∣Cj∣2.\sum_{k'}\left|\sum_j C_j\chi_{k'}(j)^3\right|^2 \ll_{\epsilon}(KNB)^\epsilon\left(\frac{K}{q_r}+\frac{NG}{C^2}\right)\sum_j|C_j|^2.

The outer sum may retain all its fixed restrictions. On a nonempty range, both quotient lengths in the last display are bounded below by a fixed positive constant; replacing them by their maxima with one changes only the comparison constant.

For each jj, the number of factorizations into mg,hgm_{\rm g},h_{\rm g} is divisor-bounded. There are O(C/qr)O(C/q_r) possible c′c' in its range. Cauchy over these two choices therefore gives

∑j∣Cj∣2≪ϵ(KNB)ϵCqr∑(c′,m,h)∈Dr(t)∣β(rc′m,rc′ht2)∣2.\sum_j|C_j|^2 \ll_\epsilon (KNB)^\epsilon\frac C{q_r} \sum_{(c',m,h)\in\mathcal D_r(t)} |\beta(rc'm,rc'ht^2)|^2.

The bounded column factor from χr\chi_r has been discarded only in this positive sum. The fixed bad-part symbols were row factors of unit modulus and were removed from the outer modulus before applying the sieve. The ideals m,hm,h here are the original ideals, reconstructed from their fixed SS-parts; the SS-part of c′c' is untouched. Combining the displays proves Equation (5.27).

Suppose now ∣β∣≤1|\beta|\le1. Ideal counting gives

#Dr(t)≪CqrNGC1C.\#\mathcal D_r(t)\ll\frac{C}{q_r}\frac{NG}{C}\frac{1}{C}.

For qr≍r0q_r\asymp r_0, its product with the preceding factor C/qrC/q_r is O(NG/r02)O(NG/r_0^2). There are O(r0)O(r_0) possible rr in this range and O(T)O(T) possible tt. Since B≍GT2B\asymp GT^2, their contribution to Equation (5.27) is at most

(KNB)ϵNBr0(Kr0+NGC2)≪(KNB)ϵNB(K+NB).(KNB)^\epsilon\frac{NB}{r_0}\left(\frac{K}{r_0}+\frac{NG}{C^2}\right) \ll(KNB)^\epsilon NB(K+NB).

Here r0,C,Tr_0,C,T are bounded below on a nonempty range and G≪BG\ll B. The number of dyadic choices for C,G,T,r0C,G,T,r_0 is logarithmic in the norm ranges. Hilbert-space triangle over the C,G,TC,G,T blocks, followed by a rescaling of ϵ\epsilon, proves Equation (5.28).

The unmarked reflected energy

For a fixed finite-ray character ν\nu, extended by zero away from primary elements prime to SS, and for m≠0m\ne0, define the central completed sum

CV(X;m,ν)=∑c sf, nc,n≡1 (3)(cn,S)=1γ2(c)α(cn3)‾ν(cn3)χcn3(m)qc qnV ⁣(qcqn3X).\mathcal C_V(X;m,\nu)= \sum_{\substack{c\ {\rm sf},\ n\\c,n\equiv1\ (3)\\(cn,S)=1}} \frac{\gamma_2(c)\overline{\alpha(cn^3)}\nu(cn^3)\chi_{cn^3}(m)} {\sqrt{q_c}\,q_n} V\!\left(\frac{q_cq_n^3}{X}\right).

Here c,nc,n may share primes. The defining series is absolutely convergent for every X>0X>0 when VV satisfies the hypotheses of Proposition 5.1. Complete multiplicativity, with the zeros retained, gives χcn3(m)=χc(m)χn(m)3\chi_{cn^3}(m)=\chi_c(m)\chi_n(m)^3. Thus for every a>1a>1,

CV(X;m,ν)=12πi∫(a)V^(s−1/2)Xs−1/2T(s,νχ∙(m)) ds.\mathcal C_V(X;m,\nu)=\frac1{2\pi i}\int_{(a)} \widehat V(s-1/2)X^{s-1/2}T(s,\nu\chi_\bullet(m))\,ds.

Indeed, absolute convergence permits termwise Mellin inversion on that line.

We bound the mean square of this completed sum over nonzero element rows. At equal completed and row norm scales, the goal is

∑0<qm≤CmZ∣CV(Z;m,ν)∣2≪Z1+ϵMA,J(V)2\sum_{0<q_m\le C_mZ}|\mathcal C_V(Z;m,\nu)|^2 \ll Z^{1+\epsilon}\mathfrak M_{A,J}(V)^2

for every fixed Cm≥1C_m\ge1 and ϵ>0\epsilon>0, with suitable finite orders A,JA,J. Lemma 5.8 below gives the more general estimate that tracks the repeated prime factors of the row.

The reason for the quadratic sieve is already visible for squarefree rows. Take m=Rm=R primary, squarefree and good, with qR≍Zq_R\asymp Z, and set X=ZX=Z. Fix a row sector, a cusp sector, a dual unit uu, and one integer k≥−4k\ge-4 in the dual support. There are no frozen good local primes in this case. Every prime of RR enters reflection with exponent one, so for μ=uλknb3\mu=u\lambda^k n b^3 its column factor gives

χR(λ4μ)3=χR(uλk+4)3χR(nb)3\chi_R(\lambda^4\mu)^3=\chi_R(u\lambda^{k+4})^3\chi_R(nb)^3

This identity retains all zeros, and n,bn,b may share primes. The first factor depends only on RR; the cusp coefficient and additive character are common throughout the sector. Their coefficient bound leaves the column normalization qn−1/2qb−1q_n^{-1/2}q_b^{-1}, up to a constant depending on the fixed kk. Thus the only arithmetic interaction between the row and the two column indices is the kernel of Lemma 5.5.

On dual dyads qn≍Uq_n\asymp U, qb≍Bq_b\asymp B, the reflected kernel has argument comparable to UB3/ZUB^3/Z. Its rapid decay permits discarding whole blocks with UB3>Z1+τUB^3>Z^{1+\tau} for any fixed τ>0\tau>0; the tail argument below makes this restriction uniform when the ramified exponent and the other parameters vary. On the retained blocks, Lemma 5.3 separates the kernel with one common coefficient measure while retaining the actual row annulus. Write UU,B,k(R)\mathcal U_{U,B,k}(R) for this dyadic piece of the reflected sum. For a retained block, the quadratic norm and the squared column normalization give

∑R∣UU,B,k(R)∣2≪V,k,τ,ϵZϵ(Z+UB)UBUB2=ZϵZ+UBB≪V,k,τ,ϵZ1+τ+ϵ.\sum_R|\mathcal U_{U,B,k}(R)|^2 \ll_{V,k,\tau,\epsilon}Z^\epsilon \frac{(Z+UB)UB}{UB^2} =Z^\epsilon\frac{Z+UB}{B} \ll_{V,k,\tau,\epsilon}Z^{1+\tau+\epsilon}.

Here B≥1B\ge1 and UB3≤Z1+τUB^3\le Z^{1+\tau} give the last inequality. This explains the balanced energy scale. The general argument must also sum the ramified exponents, retain the kernel saving at unequal scales, and treat repeated prime factors of the row. We freeze the prime powers of the row whose exponents are at least two and apply the same quadratic norm to its squarefree residual factor. The next definition records the resulting local terms; the completed-row lemma then sums them.

Definition 5.6 (An unmarked reflected block). Fix Z≥2Z\ge2, X=ZNX=Z^N, one of the fixed characters Ψ0\Psi_0 and its common modulus LL from Proposition 5.1, and put Mref=λ12L4M_{\mathrm{ref}}=\lambda^{12}L^4. For the current norm over RR, freeze a finite set F\mathcal{F} of good primes with exponents jp∈{0,…,5}j_p\in\{0,\ldots,5\}. Let RR range over squarefree primary good ideals coprime to every prime of F\mathcal{F}, in one fixed class modulo Mref2M_{\rm ref}^2 and with any further fixed row restrictions. These restrictions are independent of the dual variables. On primary elements prime to SS set

ΨR(A)=Ψ0(A)∏p∈Fχp(A)jp∏p∣Rχp(A).\Psi_R(A)=\Psi_0(A)\prod_{p\in\mathcal{F}}\chi_p(A)^{j_p}\prod_{p\mid R}\chi_p(A).

Every local power retains its zero. In the reflection for ΨR\Psi_R, fix h0h_0, the active or inactive decision at every jp=0j_p=0 prime of F\mathcal{F}, and one of the two summands of every jp=4j_p=4 Ramanujan factor. All primes of RR are active and have exponent one. Let FactF_{\mathrm{act}} be the product of the active primes in F\mathcal{F}.

For each chosen divisibility summand at jp=4j_p=4, use the exact partition

1p∣n0b03=1p∣n0+1p∤n01p∣b0.1_{p\mid n_0b_0^3}=1_{p\mid n_0}+1_{p\nmid n_0}1_{p\mid b_0}.

Choose one term. Let NFN_F be the product of the primes assigned to the squarefree ideal n0n_0, and let BFB_F be the product assigned to b0b_0 but not n0n_0. Write n0=NFnn_0 = N_F n and b0=BFbb_0 = B_F b. In the first assignment only the occurrence in n0n_0 is extracted, even if b0b_0 contains that prime; in the second exactly one occurrence is extracted from b0b_0. All remaining source restrictions are retained on nn, bb. Let FsmF_{\mathrm{sm}} be the product of the small jp=4j_p = 4 summands and the active jp=0j_p = 0 primes, and put

A0=log⁡ZqFact,S0=log⁡ZqFsm,N0=log⁡ZqNF,B0=log⁡ZqBF.A_0=\log_Zq_{F_{\rm act}},\qquad S_0=\log_Zq_{F_{\rm sm}},\qquad N_0=\log_Zq_{N_F},\qquad B_0=\log_Zq_{B_F}.

Empty products have log-norm zero.

Fix a unit uu, an integer k≥−4k \ge-4, and dual ranges

μ=uλkNFn(BFb)3,qn≍Zv,qb≍Zℓb,qλk=Zeλ.\mu= u\lambda^k N_F n(B_F b)^3, \qquad q_n \asymp Z^v, \qquad q_b \asymp Z^{\ell_b}, \qquad q_{\lambda^k} = Z^{e_\lambda}.

where v,ℓb≥0v,\ell_b \ge0. The squarefree nn and the primary bb retain the full source support of Equation (5.2), including permitted primes of SS and shared primes. Let H≥0H \ge0, and choose a common smooth profile W1(yR,yn,yb)W_1(y_R,y_n,y_b) on a fixed compact logarithmic box, where

yR=qR/ZH,yn=qn/Zv,yb=qb/Zℓb.y_R = q_R/Z^H, \qquad y_n = q_n/Z^v, \qquad y_b = q_b/Z^{\ell_b}.

Choose fixed smooth annular cutoffs χrow,χn,χb\chi_{\mathrm{row}},\chi_n,\chi_b for these three ranges, and put

W0(y)=χrow(yR)χn(yn)χb(yb)W1(y).W_0(\mathbf{y}) = \chi_{\mathrm{row}}(y_R)\chi_n(y_n)\chi_b(y_b)W_1(\mathbf{y}).

The supports and invoked seminorms are fixed uniformly over the block. Denote by Uv,ℓb,eλ(R)\mathcal{U}_{v,\ell_b,e_\lambda}(R) the specified term of the right side of Equation (5.1), restricted to this dual representation and multiplied by W0(yR,yn,yb)W_0(y_R,y_n,y_b). The original row set IH\mathcal{I}_H consists of the allowed RR for which χrow(qR/ZH)≠0\chi_{\mathrm{row}}(q_R/Z^H) \ne0. This definition is made separately for every fixed choice above.

The frozen primes in this definition may vary between invocations; they are not added to the fixed arithmetic modulus LL. The definition fixes them only before taking the current norm over RR.

Lemma 5.7 (Unmarked reflected block). For an unmarked reflected block, set

T0=2H+2A0−N−N0−3B0,ν0=v2+ℓb+eλ3+S0+B02.T_0 = 2H + 2A_0 - N - N_0 - 3B_0, \qquad\nu_0 = \frac{v}{2} + \ell_b + \frac{e_\lambda}{3} + \frac{S_0+B_0}{2}.

Let all these log-lengths range over fixed bounded sets. Put

Y=qλkNFBF3XZvZ3ℓbqcFFact2Z2H,W(y)=yn−1/2yb−1W0(y),FY(y)=W(y)V♯(Yynyb3yR−2).Y=\frac{q_{\lambda^kN_FB_F^3}X Z^vZ^{3\ell_b}} {q_{c_FF_{\rm act}}^2Z^{2H}},\qquad W(\boldsymbol y)=y_n^{-1/2}y_b^{-1}W_0(\boldsymbol y),\qquad F_Y(\boldsymbol y)=W(\boldsymbol y)V^\sharp(Yy_ny_b^3y_R^{-2}).

There are functions ρ(R)\rho(R) and β(n,b)\beta(n,b), with absolute values at most one, such that β\beta is independent of RR and

Uv,ℓb,eλ(R)=13Z−ν0ρ(R)∑n,bβ(n,b)χR(nb)3FY(yR,yn,yb).\mathcal{U}_{v,\ell_b,e_\lambda}(R) = \frac{1}{3}Z^{-\nu_0}\rho(R)\sum_{n,b}\beta(n,b)\chi_R(nb)^3F_Y(y_R,y_n,y_b).

The sum retains all the fixed dual restrictions from the definition. The only arithmetic factor here that depends simultaneously on RR and the dual variables is the displayed zero-extended quadratic symbol. Moreover,

qμXqc2=Yynyb3yR−2,c=cFFactR.\frac{q_\mu X}{q_c^2}=Yy_ny_b^3y_R^{-2},\qquad c=c_FF_{\rm act}R.

This is an exact identity on the original support, including when NFN_F shares primes with bb.

For every ϵ>0\epsilon> 0 and every fixed A≥0A \ge0,

∑R∈IH∣Uv,ℓb,eλ(R)∣2≪ϵ,AZE0+ϵp5(W)2MA,⌈4A⌉+7(V)2,\sum_{R\in\mathcal{I}_H}\left|\mathcal{U}_{v,\ell_b,e_\lambda}(R)\right|^2 \ll_{\epsilon,A} Z^{E_0+\epsilon}p_5(W)^2\mathfrak{M}_{A,\lceil4A\rceil+7}(V)^2,
E0=max⁡(H,v+ℓb)−S0−B0−ℓb−2eλ3−12(T0−v−3ℓb−eλ)+.E_0={}\max(H,v+\ell_b)-S_0-B_0-\ell_b-\frac{2e_\lambda}{3} -\frac12(T_0-v-3\ell_b-e_\lambda)_+.

The constants may depend on the fixed kernel order AA, the fixed arithmetic data, the bounded log-length ranges, and the fixed support box, but not on the moving frozen local set F\mathcal F. Norm twists in W0W_0 have the polynomial cost supplied by its finite seminorms.

Proof. For the fixed h0h_0 and the fixed class of RR modulo Mref2M_{\mathrm{ref}}^2, the class of FactRF_{\mathrm{act}}R is fixed. Proposition 5.1 therefore gives one common dd and one common additive character ϑ\vartheta for the whole row set. Write xF=uλk+4NFBF3x_F=u\lambda^{k+4}N_FB_F^3, so that λ4μ=xFnb3\lambda^4\mu=x_Fnb^3. The residual local factors are exactly

∏p∣RBp(λ4μ)=χR(xF)3χR(nb3)3=χR(xF)3χR(nb)3.\prod_{p\mid R} B_p(\lambda^4\mu)=\chi_R(x_F)^3\chi_R(nb^3)^3=\chi_R(x_F)^3\chi_R(nb)^3.

Both equalities include zeros; no unit symbol has been divided. In particular, any collision with xFx_F is a restriction depending only on RR. Every remaining local factor is fixed and depends only on the dual index. The scalar ζR\zeta_R of the reflection depends on RR but not on μ\mu.

Define on the specified dual support

δ(n,b)=d(μ)α(μ)ϑ(λ4μ)27 3k/6∣BFb∣.\delta(n,b)=\frac{d(\mu)\alpha(\mu)\vartheta(\lambda^4\mu)}{27\,3^{k/6}|B_Fb|}.

The coefficient bound gives ∣δ(n,b)∣≤1|\delta(n,b)|\le1. Its denominator is nonzero, and the definition remains valid when the numerator is zero. Using qμ=3kqNFnqBFb3q_\mu=3^kq_{N_Fn}q_{B_Fb}^3 gives the exact factorization

d(μ)α(μ)ϑ(λ4μ)qμ=27δ(n,b)qλk−1/3qNFn−1/2qBFb−1.\frac{d(\mu)\alpha(\mu)\vartheta(\lambda^4\mu)}{\sqrt{q_\mu}} =27\delta(n,b)q_{\lambda^k}^{-1/3}q_{N_Fn}^{-1/2}q_{B_Fb}^{-1}.

A small Ramanujan factor or an active zero-mask factor contributes qp−1/2q_p^{-1/2}. A divisibility factor contributes qp1/2q_p^{1/2}; for a prime assigned to NFN_F it cancels qp−1/2q_p^{-1/2} from the squarefree denominator, and for a prime assigned to BFB_F it leaves qp−1/2q_p^{-1/2} after extraction. When a prime assigned to NFN_F also divides bb, its entire occurrence in bb remains in qb−1q_b^{-1} and in δ(n,b)\delta(n,b). These facts give exactly the common power Z−ν0yn−1/2yb−1Z^{-\nu_0}y_n^{-1/2}y_b^{-1}.

Absorb δ\delta, the signs of small Ramanujan terms, the bounded fixed local characters, and the fixed dual indicators into β(n,b)\beta(n,b). This function is bounded by one and is independent of RR. Put ρ(R)=81ζRχR(xF)3\rho(R)=81\zeta_R\chi_R(x_F)^3; it is bounded by one because ∣ζR∣≤1/81|\zeta_R|\le1/81. The factor 27/81=1/327/81=1/3 now proves (5.32). Multiplicativity of the norm proves (5.33). It does not use any coprimality between NFN_F and bb.

By the definitions of the log-norms,

Y=qcF−2Zv+3ℓb+eλ−T0.Y=q_{c_F}^{-2}Z^{v+3\ell_b+e_\lambda-T_0}.

The finite set of possible cFc_F depends only on LL. Consequently mA(Y)≪LZ−(T0−v−3ℓb−eλ)+/4\mathfrak m_A(Y)\ll_L Z^{-(T_0-v-3\ell_b-e_\lambda)_+/4}. Apply Lemma 5.3 in dimension three and (5.24) to the structural identity. The single density is common to all RR because WW uses the row and both dual norms as coordinates. At each Fourier mode the norm powers have absolute value one and can be absorbed into the bounded row scalar and the common dual coefficient. Only now enlarge the positive row norm from IH\mathcal{I}_H to squarefree good RR with qR≪ZHq_R\ll Z^H, retaining any fixed restrictions. No kernel estimate is used on the added rows.

Equation (5.28), with K=ZHK=Z^H, Ncol=ZvN_{\mathrm{col}}=Z^v, and Bcol=ZℓbB_{\mathrm{col}}=Z^{\ell_b}, bounds the separated squared norm by

Zϵ+max⁡(H,v+ℓb)+v+ℓb.Z^{\epsilon+\max(H,v+\ell_b)+v+\ell_b}.

The squared common coefficient in the structural identity has exponent −v−2ℓb−2eλ/3−S0−B0-v-2\ell_b-2e_\lambda/3-S_0-B_0. The square of the extracted profile scalar contributes −(T0−v−3ℓb−eλ)+/2-(T_0-v-3\ell_b-e_\lambda)_+/2. Combining these exponents and the dimension-three separation norm proves (5.34). ∎

For later summation, call a dual block retained when

v+3ℓb+eλ≤T0+τref,τref>0.v+3\ell_b+e_\lambda\le T_0+\tau_{\rm ref}, \qquad \tau_{\rm ref}>0.

On the fixed support box, Equation (5.33) places the kernel argument in [Cker−1,Cker][C_{\mathrm{ker}}^{-1},C_{\mathrm{ker}}] times Zv+3ℓb+eλ−T0Z^{v+3\ell_b+e_\lambda-T_0}, for one fixed CkerC_{\mathrm{ker}}. If log⁡Z≥2log⁡Cker/τref\log Z \ge2\log C_{\mathrm{ker}}/\tau_{\mathrm{ref}}, every unretained whole block has actual argument greater than Zτref/2Z^{\tau_{\mathrm{ref}}/2} throughout its support. These blocks can be removed before Fourier inversion with arbitrary power saving when the other log-lengths lie in bounded ranges. Here are the details needed for that uniform assertion.

On the full source support,

∣d(μ)∣qμ≤27qλk−1/3qn0−1/2qb0−1≤27qλ4/3.\frac{|d(\mu)|}{\sqrt{q_\mu}} \le27q_{\lambda^k}^{-1/3}q_{n_0}^{-1/2}q_{b_0}^{-1} \le27q_\lambda^{4/3}.

After its indicator is discarded, each local factor is bounded by qp1/2q_p^{1/2}, uniformly in μ\mu. The product of these bounds has a fixed polynomial size when the active log-norm is bounded. For a fixed row put a=X/qc2a=X/q_c^2. Its factor 1+a−11+a^{-1} also has a fixed polynomial bound on the stated row and conductor ranges. The finite local choices and bounded row counts have a further fixed polynomial cost; call the sum of these norm-scale exponents BtailB_{\mathrm{tail}}. The fixed profile seminorms and their polynomial height costs remain multiplicative factors outside this exponent. It is chosen before the kernel order and does not count discarded dual indices. The remaining dual sum is the unrestricted lattice sum in Lemma 5.4, with U=Zτref/2U=Z^{\tau_{\mathrm{ref}}/2}. For any D>0D>0, choosing

A>1+2(Btail+D)τrefA > 1+\frac{2(B_{\mathrm{tail}}+D)}{\tau_{\mathrm{ref}}}

makes the discarded contribution O(Z−D)O(Z^{-D}) times a finite seminorm of VV and the fixed profile bounds. The assertion holds either for the absolute total or, after increasing BtailB_{\mathrm{tail}} to include the bounded row count, for the row norm. The dyadic cutoffs have bounded overlap, so this lattice estimate controls their whole sum. In particular no bound on the discarded dual lengths has been assumed.

We finish by summing the reflected blocks for an element row. The following norm observation records the actual support that governs this summation. Suppose an element row has an ideal factorization (m)=mpowmsupR(m)=m_{\mathrm{pow}}m_{\mathrm{sup}}R, with integral factors, and the fixed support constants give

qm≤CmZM,qmpow≥ZO/CO,qR≥ZH/CH.q_m \le C_m Z^M,\qquad q_{m_{\mathrm{pow}}} \ge Z^O/C_O,\qquad q_R \ge Z^H/C_H.

Since qmsup≥1q_{m_{\mathrm{sup}}}\ge1, multiplicativity gives

H≤M−O+log⁡Creslog⁡Z,Cres=CHCmCO.H \le M-O+\frac{\log C_{\mathrm{res}}}{\log Z},\qquad C_{\mathrm{res}}=C_HC_mC_O.

This inequality does not require msupm_{\mathrm{sup}} to have bounded norm, and it need not be an equality. We will use it with the three factors on disjoint prime supports and with the unit residual ideal in the bounded H=0H=0 dyad.

Lemma 5.8 (Unmarked completed-row moment). Let ν\nu range over a fixed finite family of multiplicative finite-ray characters with conductors supported on SS, all extended by zero away from the primary elements prime to SS. Fix bounded ranges for M≥0M\ge0 and N∈RN\in\mathbb{R}, a constant Cm≥1C_m\ge1, and fixed dyadic support comparisons. For a nonzero element mm, let

mpow=∏vp(m)≥2pvp(m)m_{\mathrm{pow}}=\prod_{v_{\mathfrak p}(m)\ge2}\mathfrak p^{v_{\mathfrak p}(m)}

be its maximal powerful ideal factor. Use nonnegative centers OO for its dyadic ranges, with center zero for the unit range.

For every ϵ>0\epsilon> 0 there exist a finite A≥0A \ge0 and an integer J≥0J \ge0 such that, for every test VV satisfying Proposition 5.1, every actual OO-dyad, and all sufficiently large ZZ,

∑0<qm≤CmZMqmpow≍ZO∣CV(ZN;m,ν)∣2≪ZO/2+max⁡{M−O, 2M−O−N}+ϵMA,J(V)2.\sum_{\substack{0<q_m\le C_mZ^M\\q_{m_{\rm pow}}\asymp Z^O}} |\mathcal C_V(Z^N;m,\nu)|^2 \ll Z^{O/2+\max\{M-O,\,2M-O-N\}+\epsilon} \mathfrak M_{A,J}(V)^2.

The finite orders, constant, and lower threshold may depend on the fixed arithmetic data, the parameter ranges, CmC_m, the dyadic support comparisons, and ϵ\epsilon. They are uniform in the element rows and in ν\nu in the fixed family. The estimate directly includes the Gaussian test; no annular support assumption is made on VV. Replacing V(x)V(x) by xit0V(x)x^{it_0}V(x) has at most a fixed polynomial cost in 1+∣t0∣1+\lvert t_0\rvert.

Proof. Fix one character ν\nu. Lemma 5.2, with Ψbase=ν\Psi_{\mathrm{base}}=\nu, supplies a fixed finite family of literal characters for the reflection of ν(A)χA(m)\nu(A)\chi_A(m). Choose their common E,L\mathfrak E,L before any good row prime varies. Partition the rows into the finitely many unit, SS-valuation residue, and good-ray sectors from that lemma. This keeps every good local prime, including those whose row valuation is divisible by six.

For a row in the prescribed OO-dyad, split its valuation-one primes into msupm_{\mathrm{sup}} supported on SS and the squarefree good product RR. Thus (m)=mpowmsupR(m)=m_{\mathrm{pow}}m_{\mathrm{sup}}R on disjoint prime supports. Freeze the unit, the actual ideals mpow,msupm_{\mathrm{pow}},m_{\mathrm{sup}}, and then partition RR into actual smooth annuli qR≍ZHq_R\asymp Z^H, with H≥0H\ge0 and the unit in the bounded zero dyad. Keep this row cutoff in each reflected vector. Equation (5.35) gives

H≤M−O+Ofixed(1/log⁡Z).H \le M-O+O_{\mathrm{fixed}}(1/\log Z).

The fixed row restrictions, including coprimality with the frozen factors, are independent of the dual variables.

After the row-sector conversion, take F\mathcal{F} in Definition 5.6 to be the good primes of mpowm_{\mathrm{pow}}, with their valuations reduced modulo six. The primes of RR have exponent one. Fix h0h_0, a class of RR modulo Mref2M_{\mathrm{ref}}^2, and the local active and Ramanujan choices at the frozen primes. Every active frozen good prime divides mpowm_{\mathrm{pow}} to exponent at least two. Consequently

qFact2≤qmpow,2A0≤O+Ofixed(1/log⁡Z).q_{F_{\rm act}}^2\le q_{m_{\rm pow}},\qquad 2A_0\le O+O_{\rm fixed}(1/\log Z).

This uses the actual powerful dyad’s upper comparison. The possible SS-prime factors of mpowm_{\mathrm{pow}} only increase its norm.

Apply Equation (5.1) at X=ZNX=Z^N to the Mellin representation in Equation (5.31). Its dual sum is absolutely convergent. Insert fixed smooth dyadic partitions in the residual squarefree and cube norms, and fix the unit and ramified exponent of the dual index. These operations give the blocks of Definition 5.6 with uniformly bounded seminorms for WW. No partition of the primal test VV is needed: the compact profile here is the product of the dual and row cutoffs with the normalized inverse roots, and V♯V^\sharp remains the kernel.

Fix a small τref>0\tau_{\mathrm{ref}}>0. The row lengths H,OH,O, the active length A0A_0, and NN lie in fixed bounded ranges. The same is true of S0,N0,B0S_0,N_0,B_0, since their prime products divide FactF_{\mathrm{act}}. The tail argument following Lemma 5.7 therefore removes all unretained whole dual blocks with any prescribed power saving, with a finite seminorm of VV. Its polynomial cost includes the row and local counts below but not the discarded dual indices. Choose its kernel order first, and increase A,JA,J in the statement so that MA,J(V)\mathfrak{M}_{A,J}(V) dominates this tail seminorm and the block seminorm. This is possible because increasing AA widens the supremum defining MA,J\mathfrak{M}_{A,J} and increasing JJ increases its weight.

Write e=eλe=e_\lambda. The source restriction k≥−4k\ge-4 gives e≥−4log⁡3/log⁡Ze\ge-4\log3/\log Z. For a retained block,

v+3ℓb+e≤T0+τref.v+3\ell_b+e\le T_0+\tau_{\rm ref}.

Since v,ℓb≥0v,\ell_b \ge0 and T0T_0 is bounded, this also bounds every retained dual length. There are only logarithmically many retained choices for the dual annuli and for kk. Choose a nonnegative ϵZ=Ofixed(1/log⁡Z)\epsilon_Z=O_{\mathrm{fixed}}(1/\log Z) large enough to cover the support offsets in Equations (5.37) and (5.38), and to ensure e≥−ϵZe\ge-\epsilon_Z.

The exponent in Equation (5.34) satisfies

E0≤max⁡{H,T0−S0−B0}+53ϵZ+τref.E_0\le\max\{H,T_0-S_0-B_0\}+\frac{5}{3}\epsilon_Z+\tau_{\mathrm{ref}}.

To see this, use max⁡(H,v+ℓb)−ℓb=max⁡(H−ℓb,v)\max(H,v+\ell_b)-\ell_b=\max(H-\ell_b,v) and discard the nonpositive kernel term. The first branch is at most H+2ϵZ/3H+2\epsilon_Z/3, since ℓb,S0,B0≥0\ell_b,S_0,B_0\ge0. In the second branch, retention gives v≤T0−3ℓb−e+τrefv\le T_0-3\ell_b-e+\tau_{\mathrm{ref}}, so it is at most T0−S0−B0+5ϵZ/3+τrefT_0-S_0-B_0+5\epsilon_Z/3+\tau_{\mathrm{ref}}. Moreover,

T0−S0−B0=2H+2A0−N−N0−S0−4B0≤2M−O−N+O(ϵZ),\begin{aligned} T_0-S_0-B_0&=2H+2A_0-N-N_0-S_0-4B_0\\ &\le2M-O-N+O(\epsilon_Z), \end{aligned}

by Equations (5.37) and (5.38). Thus every retained block, with its frozen row parts fixed, has exponent at most

max⁡{M−O,2M−O−N}+τref+O(ϵZ).\max\{M-O,2M-O-N\}+\tau_{\mathrm{ref}}+O(\epsilon_Z).

It remains to count the frozen parts and the finite expansions. Every powerful ideal is uniquely x2y3x^2y^3 with yy squarefree: at a prime, the exponent of yy is the parity of the powerful exponent, and an odd positive exponent is at least three. Ideal counting and ∑yqy−3/2<∞\sum_yq_y^{-3/2}<\infty therefore give

#{mpow:qmpow≪ZO}≪ZO/2.\#\{m_{\mathrm{pow}}:q_{m_{\mathrm{pow}}}\ll Z^O\}\ll Z^{O/2}.

The squarefree msupm_{\mathrm{sup}} is a divisor of the fixed radical of SS and has only finitely many choices. The local branches at the good primes of mpowm_{\mathrm{pow}} have divisor-bounded multiplicity, as do their Ramanujan assignments. Rowwise divisor Cauchy and then summation of the local choices cost an arbitrarily small power of ZZ. The choices of h0h_0, fixed ray sectors, and units are finite, and the actual row and retained dual annuli cost only powers of log⁡Z\log Z. This counts the powerful contribution O/2O/2 exactly once.

Choose τref\tau_{\mathrm{ref}} and the local small-power losses within the prescribed ϵ\epsilon allowance. Then increase the fixed-data threshold for ZZ so that the O(ϵZ)O(\epsilon_Z) terms lie within that allowance. The block bound, the preceding counts, and the already chosen tail saving prove Equation (5.36). The twist assertion follows from the norm-twist bound for MA,J\mathfrak M_{A,J} in Proposition 5.1. □

For clarity about the test used at equal lengths, put

VG(y)=12πexp⁡(−(log⁡y)24).V_{\mathrm{G}}(y)=\frac{1}{2\sqrt{\pi}}\exp\left(-\frac{(\log y)^2}{4}\right).

It satisfies the hypotheses of Proposition 5.1 directly, has V^G(t)=et2\widehat{V}_{\mathrm{G}}(t)=e^{t^2}, and has finite MA,J\mathfrak M_{A,J} for every finite A,JA,J. Thus the preceding lemma applies to it without an additional annular extension. At X=ZX=Z its exact Mellin form is

CVG(Z;m,ν)=12πi∫(4)Ztet2T(t+1/2,νχ∙(m)) dt.\mathcal C_{V_{\rm G}}(Z;m,\nu)=\frac1{2\pi i}\int_{(4)} Z^t e^{t^2}T(t+1/2,\nu\chi_\bullet(m))\,dt.

In the defining sum the coefficients remain normalized by qc−1/2qn−1q_c^{-1/2}q_n^{-1}; the scale occurs in VG(qcqn3/Z)V_{\mathrm{G}}(q_cq_n^3/Z).

Finally take M=N=1M=N=1. The exponent in an actual OO-dyad is 1−O/2+ϵ1-O/2+\epsilon. The nonnegative OO-dyads are logarithmically many, and their unit dyad is included. Summing them, with a smaller preliminary loss, gives the equal-length conclusion for every admissible VV:

∑0<qm≤CmZ∣CV(Z;m,ν)∣2≪Z1+ϵMA,J(V)2.\sum_{0<q_m\le C_mZ}|\mathcal C_V(Z;m,\nu)|^2 \ll Z^{1+\epsilon}\mathfrak M_{A,J}(V)^2.

The base probe and its balanced low estimate

We now place the completed sums of the preceding section inside one average Iη(X,Y,Z)I_\eta(X,Y,Z). Its original representation separates into an additive polynomial and a completed theta row. At the balanced scales X=Y=Z1/2X=Y=Z^{1/2}, their mean-square estimates give the direct bound Iη≪ηZ1/4+ϵI_\eta\ll_\eta Z^{1/4+\epsilon}. We first define the average for independent positive scales X,Y,ZX,Y,Z; only the final proposition in this section specializes them. The next section applies Poisson summation to this same average and identifies the reciprocal of the target LL-function in its principal row.

Definition and separation of the two factors

Choose a finite ray group TT, independently of the target character, through which the functions R\mathcal{R}, GG, and the fixed primary and supplementary phases supported over 2,32,3 in Lemma 4.4 factor. The target-dependent fixed-numerator characters below need not factor through TT. For a finite-order Hecke character η\eta, write

Θ=⟨η,T^⟩\Theta=\langle\eta,\widehat{T}\rangle

Use one excluded set SS for the finite family {ηθ:θ∈T^}\{\eta\theta:\theta\in\widehat{T}\}. It contains the primes over 66, the prime supports of the defining moduli of the fixed zero-extended presentations of η\eta and the characters in T^\widehat{T}, and every prime of norm at most a fixed P0P_0. These full presentations belong to the fixed arithmetic data. They are fixed before X,Y,ZX,Y,Z and the varying row and prime parameters are chosen. Enlarging SS will not change TT.

The finite transform should exclude frequencies meeting SS, including zero, and should leave coefficients that factor prime by prime. The following character and phase corrections arrange these two properties.

Let b∗b_\ast generate the squarefree product of the primes in SS. Choose a residue character ξ\xi modulo b∗b_\ast whose restriction to each prime factor is nonprincipal and whose order divides six. Such a choice exists: at a prime of odd residue characteristic one may use the quadratic character, and the residue field at the prime over 22 has order four and has a character of order three. The Chinese remainder theorem makes ξ\xi primitive modulo b∗b_\ast. All residue characters below are extended by zero on nonunits. Put

gψ(c,k)=∑d mod cψ(d)e(kd/c),τ=qb∗−1/2gξ(b∗,1),Ξ(a)=ξ(a)χa(b∗),Ψm,s,η(a)=η(a)Ξ(a)−1R(a,s)χa(m)((a,S)=1).\begin{aligned} g_\psi(c,k)&=\sum_{d\bmod c}\psi(d)e(kd/c),\qquad \tau=q_{b_\ast}^{-1/2}g_\xi(b_\ast,1),\qquad \Xi(a)=\xi(a)\chi_a(b_\ast),\\ \Psi_{m,s,\eta}(a)&=\eta(a)\Xi(a)^{-1}\mathcal{R}(a,s)\chi_a(m)\qquad((a,S)=1). \end{aligned}

Finite character orthogonality at each prime gives ∣τ∣=1|\tau|=1. By Lemma 4.1, the fixed-numerator symbol a↦χa(b∗)a\mapsto\chi_a(b_\ast) is a finite ray character whose conductor is supported on SS. Thus Ξ\Xi is a fixed finite character for this target, although it need not factor through TT.

The primitive character ξ\xi at the primes in SS will force the Poisson frequency to be prime to SS. The accompanying normalizations cancel the unit factors introduced by the auxiliary modulus b∗b_\ast. For the completed index A=cn3A=cn^3, the factor R(A,s)\mathcal{R}(A,s) cancels the cross-prime reciprocity phases between AA and ss, while G(A)‾\overline{G(A)} cancels the remaining pair phases within AA. We verify these cancellations coefficientwise in Section 7.2.

Define the corrected row at spectral parameter t+1/2t+1/2 by

Tm,s,η(t)=∑c sfnγ2(c)α(cn3)‾Ψm,s,η(cn3)G(cn3)‾qc−1/2−tqn−1−3t.T_{m,s,\eta}(t)= \sum_{\substack{c\ {\rm sf}\\n}} \gamma_2(c)\overline{\alpha(cn^3)}\Psi_{m,s,\eta}(cn^3) \overline{G(cn^3)}q_c^{-1/2-t}q_n^{-1-3t}.

Here and below the ideal variables avoid SS. In particular every factor in Ξ(a)−1\Xi(a)^{-1} is evaluated on a unit. The value G(cn3)G(cn^3) is the finite-ray extension in (4.5), also when cn3cn^3 is not squarefree.

Fix nonnegative, nonzero functions W0,W1∈Cc∞(0,∞)W_0,W_1 \in C_c^\infty(0,\infty) and put Φ(t)=et2\Phi(t)=e^{t^2}. Define

Iη(X,Y,Z)=1Y∑sW1(qs/Y)χs(b∗)τξ(s)qb∗qsX⋅∑m∈Oξ(m)qs−1/2gχs(s,−m)W0 ⁣(qmqb∗qsX)12πi∫(4)ZtΦ(t)Tm,s,η(t) dt.\begin{aligned} I_\eta(X,Y,Z)={}&\frac1Y\sum_s \frac{W_1(q_s/Y)\chi_s(b_*)} {\tau\xi(s)\sqrt{q_{b_*}q_sX}}\\ &\quad\cdot\sum_{m\in\mathcal O} \xi(m)q_s^{-1/2}g_{\chi_s}(s,-m) W_0\!\left(\frac{q_m}{q_{b_*}q_sX}\right) \frac1{2\pi i}\int_{(4)} Z^t\Phi(t)T_{m,s,\eta}(t)\,dt. \end{aligned}

The masks in this definition remove nonunits at SS. All sums in Equation (6.1) are absolutely convergent on the displayed line; the mm and ss sums are finite because the weights are annular.

The fixed finite Fourier expansion of the correction is

G(A)‾=∑θ∈T^aθθ(A),aθ=1∣T∣∑v∈TG(v)‾ θ(v)‾.\overline{G(A)}=\sum_{\theta\in\widehat T}a_\theta\theta(A), \qquad a_\theta=\frac1{|T|}\sum_{v\in T} \overline{G(v)}\,\overline{\theta(v)}.

Parseval and Cauchy–Schwarz give ∑θ∣aθ∣≤∣T∣1/2\sum_\theta\lvert a_\theta\rvert\leq\lvert T\rvert^{1/2}. For a ray class σ∈T\sigma\in T choose a representative sσs_\sigma and put

νσ(a)=η(a)Ξ(a)−1R(a,sσ)((a,S)=1),\nu_\sigma(a)=\eta(a)\Xi(a)^{-1}\mathcal R(a,s_\sigma) \quad ((a,S)=1),
Bm,σ(Z)=∑θ∈T^aθ12πi∫(4)ZtΦ(t)T(t+1/2,νσθχ∙(m)) dt.B_{m,\sigma}(Z)=\sum_{\theta\in\widehat{T}}a_\theta\frac{1}{2\pi i}\int_{(4)}Z^t\Phi(t)T(t+1/2,\nu_\sigma\theta\chi_\bullet(m))\,dt.

Extend νσ\nu_\sigma by zero away from the primary elements prime to SS, without evaluating Ξ(a)−1\Xi(a)^{-1} there. The function TT here is the completed product in Equation (5.1), with its original zero masks. Since R(A,s)=R(A,sσ)\mathcal R(A,s)=\mathcal R(A,s_\sigma) for s∈σs\in\sigma, the displayed Mellin integral of the corrected row equals Bm,σ(Z)B_{m,\sigma}(Z) throughout that class.

For m≠0m\neq0, the central Mellin identity (5.31) gives the direct specialization

Bm,σ(Z)=∑θ∈T^aθCVG(Z;m,νσθ).B_{m,\sigma}(Z)=\sum_{\theta\in\widehat T}a_\theta \mathcal C_{V_{\rm G}}(Z;m,\nu_\sigma\theta).

The characters νσθ\nu_\sigma\theta form one fixed finite family whose conductor and defining-modulus supports are contained in SS. They need not factor through TT. Their original zero extensions are those in the completed-row moment, so that estimate applies directly to this family of row sums. The triangle inequality in the row Hilbert space costs only the fixed factor ∑θ∣aθ∣\sum_\theta\lvert a_\theta\rvert. The row-sector conversion used by that estimate retains the zeros at shared good primes, including when a row valuation is divisible by six.

Write Q=qb∗XYQ=q_{b_*}XY. Choose a smooth compactly supported function Ω\Omega on (0,∞)(0,\infty) equal to one on every value of qm/Qq_m/Q that can occur on the support of W1(qs/Y)W0(qm/(qb∗qsX))W_1(q_s/Y)W_0(q_m/(q_{b_*}q_sX)). For v∈Rv\in\mathbb{R}, set

Am,σ,v(Y)=1Y∑s∈σW1(qs/Y)χs(b∗)τξ(s)(qs/Y)−1/2+ivqs−1/2gχs(s,−m).A_{m,\sigma,v}(Y)=\frac1Y\sum_{s\in\sigma} \frac{W_1(q_s/Y)\chi_s(b_*)}{\tau\xi(s)} (q_s/Y)^{-1/2+iv}q_s^{-1/2}g_{\chi_s}(s,-m).

Our Mellin convention for W0W_0 is W^0(iv)=∫0∞W0(r)riv dr/r\widehat{W}_0(iv)=\int_0^\infty W_0(r)r^{iv}\,dr/r. Since qm/(qb∗qsX)=(qm/Q)/(qs/Y)q_m/(q_{b_*}q_sX)=(q_m/Q)/(q_s/Y), Mellin inversion gives the exact identity

Iη(X,Y,Z)=Q−1/22π∑σ∈T∫RW^0(iv)∑m≠0Ω(qm/Q)ξ(m)(qm/Q)−ivAm,σ,v(Y)Bm,σ(Z) dv.I_\eta(X,Y,Z)=\frac{Q^{-1/2}}{2\pi}\sum_{\sigma\in T}\int_{\mathbb{R}}\widehat{W}_0(iv)\sum_{m\neq0}\Omega(q_m/Q)\xi(m)(q_m/Q)^{-iv}A_{m,\sigma,v}(Y)B_{m,\sigma}(Z)\,dv.

The omitted m=0m=0 term vanishes by the annular support of W0W_0. The factor (qm/Q)−iv(q_m/Q)^{-iv} has absolute value one. In AA, the arithmetic coefficient is fixed and bounded independently of m,vm,v; all dependence on vv occurs in a norm power of the annular variable.

The Gaussian VGV_{\rm G} has Mellin transform et2e^{t^2} and satisfies the reflection hypotheses directly. Thus Lemma (5.8) applies without an annular decomposition of this test.

The balanced low estimate

For the balanced estimate, the completed-row moment already bounds the mean square of Bm,σ(Z)B_{m,\sigma}(Z). It remains to bound the additive factor Am,σ,v(Y)A_{m,\sigma,v}(Y). Its Gauss expansion gives distinct reduced fractions in C/O\mathbb{C}/\mathcal{O}; their separation and coefficient mass give the required mean square. The planar additive large sieve is classical; compare Huxley’s multivariable and number-field inequality [19] and the Poisson proof in [1 Section 3, Theorem 3]. We include the lattice proof to record the normalization used here.

Lemma 6.1 (Planar additive large sieve). Let 0<δ≤10<\delta\le1, let Q≥1Q\ge1, and let z1,…,zJz_1,\ldots,z_J be a finite set of points in C/O\mathbb{C}/\mathcal{O} satisfying

inf⁡n∈O∣zj−zk−n∣≥δ(j≠k).\inf_{n\in\mathcal{O}} \lvert z_j-z_k-n\rvert\ge\delta\qquad(j\ne k).

Then, for arbitrary complex numbers a1,…,aJa_1,\ldots,a_J,

∑m∈Oqm≤Q∣∑j=1Jaje(mzj)∣2≪(Q+δ−2)∑j=1J∣aj∣2.\sum_{\substack{m\in\mathcal{O}\\ q_m\le Q}}\left\lvert\sum_{j=1}^{J}a_j e(mz_j)\right\rvert^2\ll(Q+\delta^{-2})\sum_{j=1}^{J}\lvert a_j\rvert^2.

The implied constant is absolute for the lattice, additive character, and self-dual measure fixed above. A fixed multiple of QQ in the row ball is allowed by changing this constant.

Proof. The assertion is immediate when J=0J=0. The characters e(mzj)e(mz_j) are well defined on C/O\mathbb{C}/\mathcal{O} by self-duality. Choose representatives in C\mathbb{C} for the other cases. We use the Fourier transforms

F^(y)=∫CF(x)e(−xy) dμ(x),ϕˇ(x)=∫Cϕ(y)e(xy) dμ(y).\widehat{F}(y)=\int_{\mathbb{C}}F(x)e(-xy)\,d\mu(x),\qquad\check{\phi}(x)=\int_{\mathbb{C}}\phi(y)e(xy)\,d\mu(y).

Choose a nonnegative ϕ∈Cc∞(C)\phi\in C_c^\infty(\mathbb C) of integral one, supported in a sufficiently small disk about zero. Since ∣e(xy)−1∣≤(4π/3)∣x∣∣y∣\lvert e(xy)-1\rvert\le(4\pi/\sqrt{3})\lvert x\rvert\lvert y\rvert, its support can be chosen so that

∣ϕˇ(x)−1∣≤12(∣x∣≤1).\lvert\check{\phi}(x)-1\rvert\le\frac{1}{2}\qquad(\lvert x\rvert\le1).

Thus F(x)=4∣ϕˇ(x)∣2F(x)=4\lvert\check{\phi}(x)\rvert^2 is a nonnegative Schwartz function and F(x)≥1F(x)\ge1 on the unit disk. If ϕ~(y)=ϕ(−y)‾\widetilde\phi(y)=\overline{\phi(-y)}, Fourier inversion and the product formula, with convolution taken with respect to dμd\mu, give

F^=4ϕ∗ϕ~.\widehat{F}=4\phi*\widetilde{\phi}.

In particular, F^\widehat{F} is bounded and supported in a disk of some fixed radius LL. This is the bandlimited majorant we need.

Put R=QR=\sqrt{Q}. Positivity of FF first gives

∑qm≤Q∣∑jaje(mzj)∣2≤∑m∈OF(m/R)∣∑jaje(mzj)∣2.\sum_{q_m\le Q}\left|\sum_j a_je(mz_j)\right|^2 \le \sum_{m\in\mathcal O}F(m/R) \left|\sum_j a_je(mz_j)\right|^2.

All sums on the right converge absolutely. For any z∈Cz\in\mathbb{C}, the Fourier transform of x↦F(x/R)e(xz)x\mapsto F(x/R)e(xz) at yy is R2F^(R(y−z))R^2\widehat{F}(R(y-z)). The factor R2R^2 is the Jacobian of the real two-dimensional dilation; no lattice-volume factor occurs because dμd\mu has covolume one on O\mathcal{O}. Poisson summation therefore expands the right side as

R2∑j,kajak‾∑n∈OF^(R(n−zj+zk)).R^2\sum_{j,k}a_j\overline{a_k}\sum_{n\in\mathcal{O}}\widehat{F}\bigl(R(n-z_j+z_k)\bigr).

For each fixed jj, a term in the inner sum can be nonzero only if the lift zk+nz_k+n lies within distance L/RL/R of zjz_j. The set of all lifts {zk+n:1≤k≤J, n∈O}\{z_k+n:1\le k\le J,\ n\in\mathcal{O}\} is δ\delta-separated in C\mathbb{C}. Distinct classes have this property by hypothesis, and two distinct lifts of one class differ by a nonzero Eisenstein integer, whose absolute value is at least one and hence at least δ\delta. The disks of radius δ/3\delta/3 about lifts in a disk of radius L/RL/R are disjoint and lie in the concentric disk of radius L/R+δ/3L/R+\delta/3. Comparing their Euclidean areas bounds the number of these lifts by

(1+3LRδ)2≪1+(Rδ)−2.\left(1+\frac{3L}{R\delta}\right)^2\ll1+(R\delta)^{-2}.

The same bound holds with jj and kk interchanged. Taking absolute values in the Poisson expansion, using the fixed bound for F^\widehat{F}, and then using 2∣ajak∣≤∣aj∣2+∣ak∣22|a_ja_k|\le|a_j|^2+|a_k|^2, we obtain

∑qm≤Q∣∑jaje(mzj)∣2≪R2(1+(Rδ)−2)∑j∣aj∣2.\sum_{q_m\le Q}\left|\sum_j a_j e(mz_j)\right|^2\ll R^2\left(1+(R\delta)^{-2}\right)\sum_j|a_j|^2.

Since R2=QR^2=Q, this is the asserted estimate. Replacing QQ by a fixed multiple proves the final statement.

We apply this estimate to the full residue classes in the Gauss sums. The zero extension of the character is important here: it makes the fractions reduced with respect to the displayed modulus, not merely with respect to an inducing conductor.

Lemma 6.2 (The balanced additive norm). Fix the arithmetic data of the probe, the annular weight W1W_1, a ray class σ∈T\sigma\in T, and a row-ball constant C>0C>0. For Y,Q≥1Y,Q\ge1 and every real vv, the polynomial Am,σ,v(Y)A_{m,\sigma,v}(Y) satisfies

∑m∈Oqm≤CQ∣Am,σ,v(Y)∣2≪A,W1,CQ+Y2Y.\sum_{\substack{m\in\mathcal O\\q_m\le CQ}} |A_{m,\sigma,v}(Y)|^2 \ll_{\mathcal A,W_1,C}\frac{Q+Y^2}{Y}.

The bound is uniform in vv. In particular, when Q=qb∗Y2Q=q_{b_*}Y^2,

∑qm≤CQ∣Am,σ,v(Y)∣2≪A,W1,CQY.\sum_{q_m\le CQ}|A_{m,\sigma,v}(Y)|^2 \ll_{\mathcal A,W_1,C}\frac QY.

Proof. For a primary ss outside SS, put rs=qs/Yr_s=q_s/Y and

cσ(s)=1s∈σχs(b∗)τξ(s).c_\sigma(s)=1_{s\in\sigma}\frac{\chi_s(b_*)}{\tau\xi(s)}.

The inverse is evaluated only on these elements prime to SS. Here ∣τ∣=1|\tau|=1, ∣ξ(s)∣=1|\xi(s)|=1, and ∣χs(b∗)∣=1|\chi_s(b_*)|=1, because b∗b_* is supported on SS. Thus ∣cσ(s)∣≤1|c_\sigma(s)|\le1. The definition of AA and the Gauss expansion give the exact identity

Am,σ,v(Y)=Y−3/2∑scσ(s)W1(rs)rs−1+iv∑d mod sχs(d)e(−md/s).A_{m,\sigma,v}(Y)=Y^{-3/2}\sum_s c_\sigma(s)W_1(r_s)r_s^{-1+iv}\sum_{d\bmod s}\chi_s(d)e(-md/s).

The sum is over primary ideals outside SS. For every such ss, the character χs(d)\chi_s(d) is zero exactly when (d,s)>1(d,s)>1, and has absolute value one otherwise. This includes nonsquarefree ss: a local exponent divisible by six is the indicator of the units at that prime, not the constant function one. For s=1s=1 the single residue class is included and χ1=1\chi_1=1.

We verify that the fractions d/sd/s for the contributing pairs are distinct modulo O\mathcal{O}. Suppose that (d,s)=(d′,s′)=1(d,s)=(d',s')=1 and d/s−d′/s′∈Od/s-d'/s'\in\mathcal{O}. Then ds′−d′sds'-d's is divisible by ss′ss'. Reducing this divisibility modulo ss and using the inverse of dd modulo ss gives s∣s′s \mid s'. The symmetric argument gives s′∣ss' \mid s. The primary generator of an ideal outside SS is unique, so s=s′s=s'; the original congruence then gives d=d′d=d' (mod ss). The same conclusion includes the unit modulus. Changing a residue representative only translates its fraction by an element of O\mathcal{O}.

Let 0<r−<r+0<r_-<r_+ be fixed with supp⁡W1⊂[r−,r+]\operatorname{supp}W_1\subset[r_-,r_+]. For two distinct contributing fractions and every n∈On\in\mathcal{O}, the Eisenstein integer ds′−d′s−nss′ds'-d's-nss' is nonzero. Hence

∣ds−d′s′−n∣=∣ds′−d′s−nss′∣∣ss′∣≥1∣ss′∣≥1r+Y.\left|\frac d s-\frac{d'}{s'}-n\right| =\frac{|ds'-d's-nss'|}{|ss'|} \ge\frac1{|ss'|}\ge\frac1{r_+Y}.

The last inequality uses qs,qs′≤r+Yq_s,q_{s'}\le r_+Y. Thus these fractions are δY\delta_Y-separated in C/O\mathbb{C}/\mathcal{O}, where δY=min⁡(1,r+−1)/Y≤1\delta_Y=\min(1,r_+^{-1})/Y\le1.

Writing the expanded polynomial as ∑s,das,de(−md/s)\sum_{s,d}a_{s,d}e(-md/s), with only the unit residue classes retained, its coefficient square mass is exactly

∑s,d∣as,d∣2=Y−3∑s∣cσ(s)W1(rs)∣2rs−2φO(s),\sum_{s,d}|a_{s,d}|^2=Y^{-3}\sum_s|c_\sigma(s)W_1(r_s)|^2r_s^{-2}\varphi_{\mathcal{O}}(s),
φO(s):=#(O/sO)×,φO(1):=1.\varphi_{\mathcal{O}}(s):=\#(\mathcal{O}/s\mathcal{O})^\times,\qquad\varphi_{\mathcal{O}}(1):=1.

There is no dependence on vv in this expression. Since φO(s)≤qs≤r+Y\varphi_{\mathcal O}(s)\le q_s\le r_+Y, rs≥r−r_s\ge r_- on the support, and there are O(Y)O(Y) ideals with qs≤r+Yq_s\le r_+Y, this mass is O(Y−1)O(Y^{-1}). Lemma 6.1, applied to the points −d/s-d/s with separation δY\delta_Y, now proves the first bound. Finally qb∗≥1q_{b_*}\ge1, so Q=qb∗Y2Q=q_{b_*}Y^2 implies Q+Y2≤2QQ+Y^2\le2Q, proving the second.

The additive norm now has precisely the scale needed to pair with the unmarked completed-row norm. The following proposition performs that pairing for the original probe.

Proposition 6.3 (Balanced low estimate). Fix the arithmetic data and smooth weights used to define IηI_\eta. For every ϵ>0\epsilon>0, as Z→∞Z\to\infty,

∣Iη(Z1/2,Z1/2,Z)∣≪A,ϵZ1/4+ϵ.\bigl|I_\eta(Z^{1/2},Z^{1/2},Z)\bigr| \ll_{\mathcal A,\epsilon} Z^{1/4+\epsilon}.

The exponent is independent of the target character; the implied constant and lower threshold may depend on its fixed arithmetic data.

Proof. Set X=Y=Z1/2X=Y=Z^{1/2} and Q=qb∗XY=qb∗ZQ=q_{b_*}XY=q_{b_*}Z. The function Ω\Omega in Equation (6.2) is bounded and supported in a fixed compact subinterval of (0,∞)(0,\infty). Thus all rows in that identity lie in 0<qm≤CΩQ0<q_m\le C_\Omega Q for a fixed constant CΩC_\Omega.

The specialization M=N=1M=N=1 of Lemma 5.8, followed by the finite ray decomposition defining Bm,σB_{m,\sigma}, gives for every ϵ1>0\epsilon_1>0

∑0<qm≤CΩQ∣Bm,σ(Z)∣2≪A,ϵ1Z1+ϵ1.\sum_{0<q_m\le C_\Omega Q}|B_{m,\sigma}(Z)|^2 \ll_{\mathcal A,\epsilon_1} Z^{1+\epsilon_1}.

Indeed, qb∗q_{b_*} is fixed, so the row ball is a fixed multiple of the M=1M=1 ball. The completed scale is ZZ, which is N=1N=1 in that lemma. The lemma applies directly to the Gaussian profile in the completed integrals defining BB; the fixed finite Fourier sum over ray characters costs only a fixed factor by the triangle inequality in the row Hilbert space. In particular this application retains the original row zero masks.

Apply Cauchy–Schwarz to the row sum in Equation (6.2). The factor (qm/Q)−iv(q_m/Q)^{-iv} has absolute value one, ∣ξ(m)∣≤1|\xi(m)|\le1 with its zero extension, and Ω\Omega is bounded. Lemma 6.2 is uniform in vv, while BB is independent of vv. Since W0W_0 is smooth and annular, ∫R∣W^0(iv)∣ dv<∞\int_{\mathbb{R}}|\widehat{W}_0(iv)|\,dv<\infty. The finite sum over σ∈T\sigma\in T therefore gives

∣Iη(X,Y,Z)∣≪A,ϵ1Q−1/2(QY)1/2Z1/2+ϵ1/2=Z1/4+ϵ1/2.\begin{aligned} |I_\eta(X,Y,Z)| &\ll_{\mathcal A,\epsilon_1} Q^{-1/2}\left(\frac QY\right)^{1/2}Z^{1/2+\epsilon_1/2}\\ &=Z^{1/4+\epsilon_1/2}. \end{aligned}

Taking ϵ1=2ϵ\epsilon_1=2\epsilon proves the proposition. ∎

The Poisson representation and its Euler factors

The direct estimate is now available. To compare the probe with the Mellin signal in Proposition 2.12.1, we return to independent positive scales XX, YY, ZZ and apply Poisson summation in the element variable mm. The resulting rows are indexed by the sixth-power-free part of the frequency. We will factor each row into Hecke LL-functions and a holomorphic Euler product; the row u=1u=1 will contain the reciprocal of the target function.

The exact Poisson series

The correction G(A)‾\overline{G(A)} is independent of mm, and the varying character in the completed row is precisely χA(m)\chi_A(m), including its zeros. Consequently Poisson summation uses the full modulus sb∗As b_* A, even if ss and AA share primes. Expand the ss-Gauss sum and first sum the lifts of a residue modulo b∗Ab_* A. The lifts impose H≡b∗Ad(mods)H \equiv b_* A d \pmod{s} and give the coefficient

F(s,A,H)=∑dmodsH≡b∗Ad(mods)χs(d)gξχA(b∗A,H−b∗Ads).F(s,A,H)=\sum_{\substack{d \bmod s\\ H\equiv b_*Ad\pmod{s}}}\chi_s(d)g_{\xi\chi_A}\left(b_*A,\frac{H-b_*Ad}{s}\right).

Indeed, the finite Fourier transform of ξ(m)χA(m)qs−1/2gχs(s,−m)\xi(m)\chi_A(m)q_s^{-1/2}g_{\chi_s}(s,-m) modulo sb∗As b_* A is qs1/2F(s,A,H)q_s^{1/2}F(s,A,H). The Poisson prefactor for the row scale qb∗qsXq_{b_*}q_sX is X/qAX/q_A. After the outer square-root normalization in Equation (6.1), leaving its separate Y−1Y^{-1} outside, their product is X1/2/(qb∗1/2qA)X^{1/2}/(q_{b_*}^{1/2}q_A). This also verifies all factors of qsq_s in the transformation.

At the primes of b∗b_* the primitive Gauss sum vanishes unless (H,S)=1(H,S)=1. It therefore also removes H=0H=0. Every remaining element has a unique expression H=ua6H=ua^6, where uu is a sixth-power-free element, including its unit factor, and aa is the primary generator of an ideal. Write ∑u(6)\sum_u^{(6)} for the sum over such nonzero uu with (u,S)=1(u,S)=1.

Let W~0(∣y∣2)\widetilde{W}_0(|y|^2) be the planar Fourier transform of W0(∣y∣2)W_0(|y|^2) for the self-dual measure and character fixed in Section 4. The radial Fourier argument after Poisson is XqH/qAXq_H/q_A. Put

M(z)=∫0∞W~0(r)rz−1 dr,W^1(w)=∫0∞W1(r)rw−1 dr.M(z)=\int_0^\infty\widetilde{W}_0(r)r^{z-1}\,dr,\qquad\widehat{W}_1(w)=\int_0^\infty W_1(r)r^{w-1}\,dr.

Smoothness at zero and Schwartz decay show that MM is holomorphic for ℜz>0\Re z>0. On every compact positive real strip it has arbitrary polynomial decay in ℑz\Im z: every derivative of e(ℜz)vW~0(ev)e^{(\Re z)v}\widetilde W_0(e^v) is integrable in vv, uniformly on that strip, so repeated integration by parts applies. The same argument gives arbitrary polynomial decay for W^1\widehat{W}_1 on every fixed real strip.

We will need the strict positivity

M(1/6)>0.M(1/6)>0.

Here is a proof that does not require the Fourier transform itself to be nonnegative. For 0<σ<10<\sigma<1,

∣y∣2σ−2=1Γ(1−σ)∫0∞t−σe−t∣y∣2 dt.|y|^{2\sigma-2}=\frac{1}{\Gamma(1-\sigma)}\int_0^\infty t^{-\sigma}e^{-t|y|^2}\,dt.

The pairing of the left side with W~0(∣y∣2)\widetilde{W}_0(|y|^2) is absolutely integrable. Fubini and Fourier duality express it as

1Γ(1−σ)∫0∞t−σ∫CW0(∣x∣2)2π3texp⁡(−4π2∣x∣23t)dμ(x) dt>0.\frac{1}{\Gamma(1-\sigma)}\int_0^\infty t^{-\sigma}\int_{\mathbb{C}}W_0(|x|^2)\frac{2\pi}{\sqrt{3}t}\exp\left(-\frac{4\pi^2|x|^2}{3t}\right)d\mu(x)\,dt>0.

The inner integral is strictly positive for every t>0t>0, since W0W_0 is nonnegative and nonzero. Absolute integrability follows either from the displayed representation on the Fourier side or from the annular support of W0W_0 on this side. Polar integration identifies the original pairing with (2π/3)M(σ)(2\pi/\sqrt{3})M(\sigma), proving Equation (7.2).

Set x=t+1−zx=t+1-z after Mellin inversion of the two weights. For a nonzero sixth-power-free uu with (u,S)=1(u,S)=1, define

Fη,u(x,w,z)=∑c sfn,s,aKη(c,n,s,a;u)qc−1/2−xqn−1−3xqs−wqa−6z.\mathcal{F}_{\eta,u}(x,w,z)=\sum_{\substack{c\ \mathrm{sf}\\ n,s,a}}K_{\eta}(c,n,s,a;u)q_c^{-1/2-x}q_n^{-1-3x}q_s^{-w}q_a^{-6z}.

where A=cn3A=cn^3 and the coefficient, with all normalizations retained, is

Kη(c,n,s,a;u)=F(s,A,ua6)χs(b∗)qb∗τξ(s)ξ(u)‾γ2(c)α(A)G(A)‾η(A)Ξ(A)−1R(A,s).K_\eta(c,n,s,a;u)= \frac{F(s,A,ua^6)\chi_s(b_*)} {\sqrt{q_{b_*}}\tau\xi(s)\overline{\xi(u)}} \gamma_2(c)\overline{\alpha(A)G(A)} \eta(A)\Xi(A)^{-1}\mathcal R(A,s).

For convenience define the common Mellin weight

W(X,Y,Z;x,w,z)=X1/2−zZx+z−1Yw−1Φ(x+z−1)M(z)W^1(w).\mathcal{W}(X,Y,Z;x,w,z)=X^{1/2-z}Z^{x+z-1}Y^{w-1}\Phi(x+z-1)M(z)\widehat{W}_1(w).

For example, the lines ℜx=3\Re x=3, ℜw=3\Re w=3, ℜz=2\Re z=2 correspond to the original line ℜt=4\Re t=4 and lie in absolute convergence. The complete high identity is

Iη(X,Y,Z)=1(2πi)3∫(3)∫(3)∫(2)W(X,Y,Z;x,w,z)⋅∑u(6)qu−zξ(u)‾Fη,u(x,w,z) dz dw dx.I_{\eta}(X,Y,Z)=\frac{1}{(2\pi i)^3}\int_{(3)}\int_{(3)}\int_{(2)}\mathcal{W}(X,Y,Z;x,w,z) \cdot\sum_u^{(6)}q_u^{-z}\overline{\xi(u)}\mathcal{F}_{\eta,u}(x,w,z)\,dz\,dw\,dx.

One may justify all interchanges on these lines by the elementary bound ∣F(s,A,H)∣≤qsqb∗A|F(s,A,H)|\le q_sq_{b_*A} and by the annular weights. In particular, Equations (6.2) and (7.5) are identities for the same probe, not estimates for separately chosen test expressions.

The scalar Euler identity

We next evaluate the coefficient in Equation (7.4). Our objective is to prove that the high series is a scalar Euler product for the target η\eta. The calculation also records separately the terms with positive valuation of the completed index AA at a given prime. We keep every ray phase until it has been cancelled or assigned to a local factor.

Fix a nonzero sixth-power-free row uu with (u,S)=1(u,S)=1 and a prime p∉Sp\notin S. Set

Q=qp,j=vp(u)∈{0,…,5},ρ=χp(u/pj),ωp=χp(−1),Q=q_p,\qquad j=v_p(u)\in\{0,\ldots,5\},\qquad\rho=\chi_p(u/p^j),\qquad\omega_p=\chi_p(-1),
ap=α(p)‾3η(p)3,bp=α(p)‾2η(p)2χp(4)‾,bp3=ap2,a_p=\overline{\alpha(p)}^3\eta(p)^3,\qquad b_p=\overline{\alpha(p)}^2\eta(p)^2\overline{\chi_p(4)}, \qquad b_p^3=a_p^2,
V=Q−6z,R=ap2Q4−6x−6z,Wloc=ρQ−w.V=Q^{-6z},\qquad R=a_p^2Q^{4-6x-6z},\qquad W_{\mathrm{loc}}=\rho Q^{-w}.

The values ρ\rho, apa_p, bpb_p have absolute value one, and ωp∈{1,−1}\omega_p\in\{1,-1\}. No ray-class restriction on pp is imposed.

The finite scalar and its unit factors. Write Gr=gχpr(p,1)G_r=g_{\chi_p^r}(p,1), with G0=−1G_0=-1, and γr=Q−1/2Gr\gamma_r=Q^{-1/2}G_r for 1≤r≤51\le r\le5. For t≥1t\ge1 and j′≥0j'\ge0, summing the lifts of a residue modulo pp gives

gχpr(pt,pj′)={Qt−1Gr1j′=t−1,6∤r,Qt1j′≥t−Qt−11j′≥t−1,6∣r.g_{\chi_p^r}(p^t,p^{j'})= \begin{cases} Q^{t-1}G_r1_{j'=t-1},&6\nmid r,\\ Q^t1_{j'\ge t}-Q^{t-1}1_{j'\ge t-1},&6\mid r. \end{cases}

The second line is the Ramanujan sum for the principal character extended by zero. Orthogonality also gives G1G−1=ωpQG_1G_{-1}=\omega_pQ.

Let e0=vp(c)∈{0,1}e_0=v_p(c)\in\{0,1\}, l=vp(n)l=v_p(n), t=e0+3lt=e_0+3l, k=vp(s)k=v_p(s), and m=vp(a)m=v_p(a), so vp(H)=j′=j+6mv_p(H)=j'=j+6m. The part of Equation (7.1) at pp, before its unit factors are restored, is

Cp(t,k,j′)=∑dmodpkpj′≡ptd(modpk)χpk(d)gχpt(pt,pj′−ptdpk).C_p(t,k,j')=\sum_{\substack{d\bmod p^k\\ p^{j'}\equiv p^t d\pmod{p^k}}}\chi_p^k(d)g_{\chi_p^t}\left(p^t,\frac{p^{j'}-p^t d}{p^k}\right).

At modulus one both factors in this formula mean one. Its complete evaluation is

Cp(t,k,j′)={1,t=k=0,1j′=0,t=0, k>0,gχpt(pt,pj′),t>0, k=0,ωp−1G1gχpt−1(pt,pj′−1),t>0, k=1, j′≥1,0,otherwise.C_p(t,k,j')= \begin{cases} 1,&t=k=0,\\ 1_{j'=0},&t=0,\ k>0,\\ g_{\chi_p^t}(p^t,p^{j'}),&t>0,\ k=0,\\ \omega_p^{-1}G_1g_{\chi_p^{t-1}}(p^t,p^{j'-1}),&t>0,\ k=1,\ j'\geq1,\\ 0,&\text{otherwise}. \end{cases}

For t=0t=0 and k>0k>0, the congruence fixes d=pj′d=p^{j'} modulo pkp^k, whose zero-extended character is nonzero exactly when j′=0j'=0. For the fourth line the congruence first forces j′≥1j'\geq1. Expanding the inner Gauss sum, the sum over d mod pd\bmod p is

∑d mod pχp(d)e(−vd/p)=ωp−1G1χp(v)−1(p∤v),\sum_{d\bmod p}\chi_p(d)e(-vd/p)=\omega_p^{-1}G_1\chi_p(v)^{-1}\qquad(p\nmid v),

which changes the Gauss character from χpt\chi_p^t to χpt−1\chi_p^{t-1}. If t>0t>0 and k≥2k\geq2, the permitted lifts d=d0+pk−1vd=d_0+p^{k-1}v do not change χpk(d)\chi_p^k(d), but their Gauss phase is e(−yv/p)e(-yv/p) with the Gauss variable yy a unit. Their sum is zero. This proves Equation (7.8), including the cases where the Gauss character is principal and zero-extended.

For the original units write hp=H/pj′h_p=H/p^{j'}, sp=s/pks_p=s/p^k, and Ap∘=A/ptA_p^\circ=A/p^t. Chinese remaindering and the substitution d=hp(b∗Ap∘)−1d′d=h_p(b_*A_p^\circ)^{-1}d' give the additional unit factor

Up=χpk−t(hp)χpt(sp)χpt−k(Ap∘)χpt−k(b∗).U_p=\chi_p^{k-t}(h_p)\chi_p^t(s_p)\chi_p^{t-k}(A_p^\circ)\chi_p^{t-k}(b_*).

More explicitly, the outer residue character gives χpk(hp)χp−k(b∗Ap∘)\chi_p^k(h_p)\chi_p^{-k}(b_*A_p^\circ), while the Chinese remainder factor and the rescaling of the Gauss argument give χpt(b∗Ap∘)χp−t(hp/sp)\chi_p^t(b_*A_p^\circ)\chi_p^{-t}(h_p/s_p). Their product is Equation (7.9). Since hp=(u/pj)(a/pm)6h_p=(u/p^j)(a/p^m)^6, one has χp(hp)=ρ\chi_p(h_p)=\rho.

At the primes of b∗b_*, one has (H−b∗Ad)/s≡H/s(modb∗)(H-b_*Ad)/s\equiv H/s\pmod{b_*}. The local factor in the complete Gauss sum is qb∗τξ(A)ξ(H/s)‾\sqrt{q_{b_*}}\tau\xi(A)\overline{\xi(H/s)}. Here ξ(H/s)‾=ξ(u)‾ξ(s)\overline{\xi(H/s)}=\overline{\xi(u)}\xi(s) because ξ(a)6=1\xi(a)^6=1. This cancels every displayed ξ\xi factor in Equation (7.4). The product of the last factors in Equation (7.9) cancels χs(b∗)χA(b∗)−1\chi_s(b_*)\chi_A(b_*)^{-1}. This cancellation is coefficientwise. For any fixed enlargement of SS, the same calculation uses the same ray group TT.

Cancellation of the remaining pair phases. With tp=vp(A)t_p=v_p(A) and kp=vp(s)k_p=v_p(s), reciprocity at each pair of distinct primes gives

R(A,s)∏pχptp(sp)χp−kp(Ap∘)=∏pR(p,p)tpkp.\mathcal{R}(A,s)\prod_p\chi_p^{t_p}(s_p)\chi_p^{-k_p}(A_p^\circ)=\prod_p\mathcal{R}(p,p)^{t_pk_p}.

Indeed, for p≠rp\ne r the two orientations have opposite symbol exponents, and their quotient is R(p,r)\mathcal{R}(p,r); this cancels the corresponding pair in the bicharacter R(A,s)\mathcal{R}(A,s). Only its diagonal remains. Equation (4.7) gives γ2(c)=μ(c)α(c)G(c)/γ1(c)\gamma_2(c)=\mu(c)\alpha(c)G(c)/\gamma_1(c). The Chinese remainder formula

γ1(c)=∏p∣cγ1(p)∏p<r, p,r∣cχp(r)χr(p)\gamma_1(c)=\prod_{p\mid c}\gamma_1(p) \prod_{p<r,\ p,r\mid c}\chi_p(r)\chi_r(p)

removes the squarefree part of the remaining pair product. If ep=vp(c)e_p=v_p(c) and lp=vp(n)l_p=v_p(n), its exponent at a pair p<rp<r is tptr−eper=3(eplr+erlp+3lplr)t_pt_r-e_pe_r=3(e_pl_r+e_rl_p+3l_pl_r). The cube of χp(r)χr(p)\chi_p(r)\chi_r(p) is R(p,r)\mathcal R(p,r), whose square is one. Thus the pair product left after this division is

∏p<rR(p,r)eplr+erlp+lplr=R(c,n)G(n3)∏pG(p3)‾ lpR(p,p)−eplp−lp(lp−1)/2.\prod_{p<r}\mathcal R(p,r)^{e_pl_r+e_rl_p+l_pl_r} =\mathcal R(c,n)G(n^3) \prod_p\overline{G(p^3)}^{\,l_p} \mathcal R(p,p)^{-e_pl_p-l_p(l_p-1)/2}.

The equality follows by expanding the quadratic refinement Equation (4.5) on the prime factors of n3n^3. The same refinement gives G(c)R(c,n)G(n3)=G(cn3)G(c)\mathcal R(c,n)G(n^3)=G(cn^3), which is cancelled by the inserted G(cn3)‾\overline{G(cn^3)}. Finally Equation (4.6) gives G(p3)=γ3(p)G(p^3)=\gamma_3(p) and R(p,p)=ωp\mathcal R(p,p)=\omega_p. These identities account for all pair phases, with no restriction on the ray class of pp.

The coefficient in Equation (7.4) has therefore separated into prime factors. In absolute convergence, its factor at pp is the series

Pp=∑e0=0,1l,k,m≥0(−1)e0γ1−e0η(p)e0(apγ3‾)lρk−tωptk−e0l−l(l−1)/2Cp(t,k,j+6m)⋅Q−(x+1/2)e0−(1+3x)l−wk−6zm,t=e0+3l.\begin{aligned} P_p={}&\sum_{\substack{e_0=0,1\\l,k,m\ge0}} (-1)^{e_0}\gamma_1^{-e_0}\eta(p)^{e_0} (a_p\overline{\gamma_3})^l\rho^{k-t} \omega_p^{tk-e_0l-l(l-1)/2}C_p(t,k,j+6m)\\ &\hspace{33mm}\cdot Q^{-(x+1/2)e_0-(1+3x)l-wk-6zm},\qquad t=e_0+3l. \end{aligned}

Let Pp∗P_p^* be the same sum restricted to t>0t>0, equivalently to positive valuation of the completed index AA.

Lemma 7.1 (The complete local identity). For every nonzero sixth-power-free uu with (u,S)=1(u,S)=1 and every prime p∉Sp\notin S, the factors just defined are

Pp∗=11−R{R(1−Q−1)−η(p)(Q−1)Q−x−wV1j≤11−V+Jj},P_p^*=\frac1{1-R}\left\{ \frac{R(1-Q^{-1})-\eta(p)(Q-1) Q^{-x-w}V^{1_{j\le1}}}{1-V}+J_j\right\},
Pp=11−V+1j=0Wloc1−Wloc+Pp∗,P_p=\frac1{1-V}+1_{j=0}\frac{W_{\rm loc}}{1-W_{\rm loc}}+P_p^*,

where the six values of JjJ_j are

jjJjJ_j
0−η(p)ρ−1Q−x+WlocR-\eta(p)\rho^{-1}Q^{-x}+W_{\mathrm{loc}}R
1η(p)Q−x−w\eta(p)Q^{-x-w}
2apρ−3Q3/2−3xa_p\rho^{-3}Q^{3/2-3x}
3−η(p)bpρ−2Q2−3x−w+bp2ρ−4Q2−4x-\eta(p)b_p\rho^{-2}Q^{2-3x-w}+b_p^2\rho^{-4}Q^{2-4x}
4−η(p)apρ−3Q5/2−4x−w-\eta(p)a_p\rho^{-3}Q^{5/2-4x-w}
5−ap2Q3−6x-a_p^2Q^{3-6x}

Put W=χp(u)Q−wW=\chi_p(u)Q^{-w} and D=η(p)χp(u)‾Q−xD=\eta(p)\overline{\chi_p(u)}Q^{-x}, with the original zero extension at p∣up\mid u, and define

Hp=Pp(1−V)(1−W)1−D,Hη,u=∏p∉SHp.H_p=P_p\frac{(1-V)(1-W)}{1-D},\qquad \mathcal H_{\eta,u}=\prod_{p\notin S}H_p.

Then the series in Equation (7.3) has the scalar factorization

Fη,u(x,w,z)=ζFS(6z)LS(w,χ∙(u))LS(x,ηχ∙(u)‾)Hη,u(x,w,z).\mathcal F_{\eta,u}(x,w,z)= \frac{\zeta_F^S(6z)L^S(w,\chi_\bullet(u))} {L^S(x,\eta\overline{\chi_\bullet(u)})} \mathcal H_{\eta,u}(x,w,z).

Write xr=ℜxx_r=\Re x, wr=ℜww_r=\Re w, and zr=ℜzz_r=\Re z. For every fixed ϵ0>0\epsilon_0>0, the correction product converges normally on a neighborhood of every point in each of the following regions, and hence defines a holomorphic function there:

xr≥51/100,zr≥17/50,wr≥−1/100,xr+wr≥1+ϵ0; x_r\ge51/100,\quad z_r\ge17/50,\quad w_r\ge-1/100,\quad x_r+w_r\ge1+\epsilon_0;
xr≥7/8,zr≥33/200,wr≥19/20.x_r\geq7/8,\qquad z_r\geq33/200,\qquad w_r\geq19/20.

Uniformly in imaginary parts and unit phases, Hη,u≪ϵquϵ\mathcal H_{\eta,u}\ll_\epsilon q_u^\epsilon, with the constant also depending on ε0\varepsilon_0 in the first region. For u=1u=1 in the second region, Hη,1=1+O(P0−cH)\mathcal H_{\eta,1}=1+O(P_0^{-c_H}) with, for example, cH=4/5c_H=4/5. Equation (7.13) begins in absolute convergence and supplies a meromorphic continuation through these regions.

The first region will contain the buffered contours for nonprincipal rows, including the reflected numerator line. The second contains the principal residue point w=1w=1, z=1/6z=1/6 and the contours used to reach it.

Proof. There are four families with t>0t>0: (e0,l)=(0,2r+2),(1,2r),(0,2r+1),(1,2r+1)(e_0,l)=(0,2r+2),(1,2r),(0,2r+1),(1,2r+1), where r≥0r\geq0. In each family, increasing rr by one and the first permitted mm by one multiplies the summand of Equation (7.10) by RR. In fact the phase ratio is ap2a_p^2: the remaining ratio is one because γ32=ωp\gamma_3^2=\omega_p, ωp2=1\omega_p^2=1, and ρ6=1\rho^6=1. Increasing mm further multiplies a summand by VV.

For transparency, the following table lists every nonzero summand after division by RrR^r. In its first row jj is arbitrary; all other conditions are as displayed. Every omitted case is zero by Equation (7.8).

(e0,l)kcondition on (j,m)R−r times summand(0,2r+2)0m≥r+1R(1−Q−1)Vm−r−1(0,2r+2)0j=5, m=r−ap2Q3−6x(0,2r+2)1j=0, m=r+1WlocR(1,2r)0j=0, m=r−η(p)ρ−1Q−x(1,2r)1j=1, m=rη(p)Q−x−w(1,2r)1m≥r+1j≤1−η(p)(Q−1)Q−x−wVm−r(0,2r+1)0j=2, m=rapρ−3Q3/2−3x(0,2r+1)1j=3, m=r−η(p)bpρ−2Q2−3x−w(1,2r+1)0j=3, m=rbp2ρ−4Q2−4x(1,2r+1)1j=4, m=r−η(p)apρ−3Q5/2−4x−w.\begin{array}{c|c|l|l} (e_0,l)&k&\text{condition on }(j,m)&R^{-r}\text{ times summand}\\\hline (0,2r+2)&0&m\ge r+1&R(1-Q^{-1})V^{m-r-1}\\ (0,2r+2)&0&j=5,\ m=r&-a_p^2Q^{3-6x}\\ (0,2r+2)&1&j=0,\ m=r+1&W_{\rm loc}R\\ (1,2r)&0&j=0,\ m=r&-\eta(p)\rho^{-1}Q^{-x}\\ (1,2r)&1&j=1,\ m=r&\eta(p)Q^{-x-w}\\ (1,2r)&1&m\ge r+1_{j\le1}&-\eta(p)(Q-1)Q^{-x-w}V^{m-r}\\ (0,2r+1)&0&j=2,\ m=r&a_p\rho^{-3}Q^{3/2-3x}\\ (0,2r+1)&1&j=3,\ m=r&-\eta(p)b_p\rho^{-2}Q^{2-3x-w}\\ (1,2r+1)&0&j=3,\ m=r&b_p^2\rho^{-4}Q^{2-4x}\\ (1,2r+1)&1&j=4,\ m=r&-\eta(p)a_p\rho^{-3}Q^{5/2-4x-w}. \end{array}

Here is a direct check of its entries. In the first family t=6r+6t=6r+6. For k=0k=0, the principal Gauss lift is Qt(1−Q−1)Q^t(1-Q^{-1}) for m≥r+1m\geq r+1; its extra boundary value at (j,m)=(5,r)(j,m)=(5,r) is −Qt−1-Q^{t-1}. For k=1k=1, the product ωp−1G1G−1=Q\omega_p^{-1}G_1G_{-1}=Q allows only (j,m)=(0,r+1)(j,m)=(0,r+1). These give the first three rows. In the second family t=6r+1t=6r+1. For k=0k=0 the nonprincipal equality j′=t−1j'=t-1 gives the fourth row. For k=1k=1, the principal Gauss lift has its negative boundary at j′=tj'=t, giving the fifth row, and its value Qt−1(Q−1)Q^{t-1}(Q-1) for j′>tj'>t, giving the sixth row. The latter condition is exactly m≥r+1j≤1m\ge r+1_{j\le1}.

For the two odd families t=6r+3t=6r+3 and t=6r+4t=6r+4. Their k=0k=0 lines require j′=t−1j'=t-1 and their k=1k=1 lines require j′=tj'=t. The phase reductions are

γ1γ2=−α(p)χp(4)‾γ3,γ4γ1=−α(p)‾G(p).\gamma_1\gamma_2 =-\alpha(p)\overline{\chi_p(4)}\gamma_3, \qquad \frac{\gamma_4}{\gamma_1} =-\frac{\overline{\alpha(p)}}{G(p)}.

The first is Equation (4.7) at pp; the second follows from the first and γ2γ4=1\gamma_2\gamma_4=1. Substitution gives the last four rows, including both j=3j=3 terms. Thus the table covers all five ramified valuations as well as j=0j=0.

Summing r≥0r\geq0 gives (1−R)−1(1-R)^{-1}, and the two unbounded mm ranges give (1−V)−1(1-V)^{-1}. These sums are precisely the formula for Pp∗P_p^* in Equation (7.11). If t=0t=0, then e0=l=0e_0=l=0. The k=0k=0 terms give (1−V)−1(1-V)^{-1}, while the k>0k>0 terms require j=m=0j=m=0 and give Wloc/(1−Wloc)W_{\mathrm{loc}}/(1-W_{\mathrm{loc}}). This proves the formula for PpP_p as well.

It remains to justify the analytic assertions, especially where wrw_r is negative. Put Ep=Pp∗+D\mathcal E_p=P_p^*+D. The contribution from t=0t=0 is (1−V)−1+W/(1−W)(1-V)^{-1}+W/(1-W), so an exact simplification gives

Hp−1=D(V+W−VW)−VW+(1−V)(1−W)Ep1−D.H_p-1= \frac{D(V+W-VW)-VW+(1-V)(1-W)\mathcal E_p}{1-D}.

This expression has no 1−W1-W denominator. At p∣up \mid u, where D=W=0D=W=0, it reduces to (1−V)Ep(1-V)\mathcal{E}_p. In both stated regions ∣R∣<1|R|<1, ∣V∣<1|V|<1, and ∣D∣<1|D|<1, uniformly away from one, so these are holomorphic local expressions.

For p∤up\nmid u and ϑ=(−wr)+\vartheta=(-w_r)_+, the j=0j=0 row gives

∣Ep∣≪Q4−6xr−6zr+ϑ+Q1−xr−wr−6zr.|\mathcal{E}_p| \ll Q^{4-6x_r-6z_r+\vartheta}+Q^{1-x_r-w_r-6z_r}.

In the first region 4−6xr−6zr≤−11/104-6x_r-6z_r\le-11/10 and ϑ≤1/100\vartheta\le1/100. The extra factor 1−W1-W in Equation (7.17) therefore leaves this contribution at most Q−27/25Q^{-27/25}. The term DWDW is at most Q−1−ϵ0Q^{-1-\epsilon_0}; the other terms in that equation are smaller. For p∣up\mid u, the strict second-family term has exponent 1−xr−wr≤−ϵ01-x_r-w_r\le-\epsilon_0. The closest other exponents in the table are

3/2−3xr≤−3/100,2−3xr−wr≤−1/50−ϵ0,3/2-3x_r\le-3/100,\qquad2-3x_r-w_r\le-1/50-\epsilon_0,

and all remaining ones are no larger than −3/100-3/100. Consequently, with ϵH=min⁡(ϵ0,1/50)\epsilon_H=\min(\epsilon_0,1/50),

Hp−1=O(Q−1−ϵH)(p∤u),Hp−1=O(Q−ϵH)(p∣u).H_p-1=O(Q^{-1-\epsilon_H})\quad(p\nmid u),\qquad H_p-1=O(Q^{-\epsilon_H})\quad(p\mid u).

In the second region the same comparison gives the stronger bounds

Hp−1=O(Q−363/200)(p∤u),Hp−1=O(Q−33/40)(p∣u).H_p-1=O(Q^{-363/200})\quad(p\nmid u),\qquad H_p-1=O(Q^{-33/40})\quad(p\mid u).

The closest good-prime term here is Q1−xr−wr−6zrQ^{1-x_r-w_r-6z_r}, and the closest ramified term is Q1−xr−wrQ^{1-x_r-w_r}.

The sum over primes not dividing uu converges normally, and the finite product over primes of uu is Oϵ(quϵ)O_\epsilon(q_u^\epsilon) by the divisor-product bound. The estimates are uniform in all imaginary parts and unit phases. When u=1u=1, the good-prime tail above P0P_0 is O(P0−163/200)O(P_0^{-163/200}) by the ideal count, which implies the asserted O(P0−4/5)O(P_0^{-4/5}) estimate for the product. Finally extracting (1−V)−1(1−W)−1(1−D)(1-V)^{-1}(1-W)^{-1}(1-D) at every prime gives Equation (7.13). The normal convergence of the remaining product proves its claimed continuation.

For u=1u=1, Equation (7.13) contains 1/LS(x,η)1/L^S(x,\eta), and its numerator has the two principal factors ζFS(6z)\zeta_F^S(6z) and ζFS(w)\zeta_F^S(w). Their residues will produce the target Mellin signal. For intermediate row norms, the next section assigns one zero-free rectangle to the finite family of twists associated with each row and produces simultaneous polynomial witnesses from a selected zero. The principal and bounded rows, together with the outer norm ranges, are treated in Section 10.

A zero detector with saturated witnesses

The high expansion contains a sum over sixth-power-free rows uu. We associate each nonprincipal row with a buffered zero-free rectangle for the finite family of character presentations that it determines. Whenever the resulting bin lies above a fixed floor, a zero produces an inverse polynomial and a plain polynomial with simultaneous lower bounds. These witnesses can then be counted using different mean estimates. The analytic inputs here are Lemma 4.9, the smooth calculus of Lemma 4.5, and the global growth estimate in Equation (4.14), together with the deleted Euler-factor bounds of Lemma 4.10.

Throughout this section, assume β∗>51/100\beta_* > 51/100, where β∗\beta_* is the global supremum in Equation (2.1). This setting does not select either of the two boundaries in the continuation criterion.

Buffered rectangles and pointwise bounds

Fix the arithmetic data A\mathcal{A} independently of ZZ, as in Section 4. In particular, the finite group

Θ=⟨η,T^⟩\Theta=\langle\eta,\widehat{T}\rangle

contains the target and the fixed ray twists used in the high-row family, and every conductor prime of a member of Θ\Theta belongs to SS. For a sixth-power-free element uu, define the finite collection of presentations

Xu={ψu,ν,ς(n)=ν(n)χn(u)ς:ν∈Θ, ς∈{−1,1}}.\mathcal{X}_u=\left\{\psi_{u,\nu,\varsigma}(n)=\nu(n)\chi_n(u)^{\varsigma}:\nu\in\Theta,\ \varsigma\in\{-1,1\}\right\}.

At a nonunit the value of χn(u)−1\chi_n(u)^{-1}, like every other power of the symbol, is zero. The group property of Θ\Theta shows that Xu\mathcal{X}_u is closed under conjugation. It contains the numerator character χ∙(u)\chi_{\bullet}(u), the denominator character ηχ∙(u)‾\eta\overline{\chi_\bullet(u)}, and every zero-extended presentation obtained by multiplying either orientation of the sextic symbol by a member of Θ\Theta.

Let ψ∗\psi^* be the primitive character inducing a presentation ψ∈Xu\psi\in\mathcal{X}_u, and let QψQ_\psi be its conductor norm. Reciprocity and the fixed conductor primes give

Qψ≪Aqu,Lorig(s,ψ)=L(s,ψ∗)∏p∈Eu(1−ψ∗(p)qp−s),Eu⊂S∪{p:p∣u}.Q_\psi\ll_{\mathcal A}q_u,\qquad L_{\rm orig}(s,\psi) =L(s,\psi^*)\prod_{p\in E_u}(1-\psi^*(p)q_p^{-s}), \qquad E_u\subset S\cup\{p:p\mid u\}.

The radical of the deleted product has norm OS(qu)O_S(q_u). These identities retain the original zero extensions; in particular, they do not replace a row-dependent mask by an independently chosen mask.

If vp(u)=j∈{1,…,5}v_p(u)=j\in\{1,\ldots,5\} at a prime p∉Sp\notin S, the local character of χ∙(u)\chi_{\bullet}(u) on units at pp has order 6/gcd⁡(6,j)>16/\gcd(6,j)>1. A character in Θ\Theta is unramified there, so it cannot cancel this local character. Consequently a presentation in Xu\mathcal{X}_u can induce the principal character only when uu is supported on SS. There are finitely many such sixth-power-free rows, including unit factors. Remove them for the present detector; each application must estimate these bounded physical rows separately.

Fix 0<dmin⁡<dmax⁡<∞0<d_{\min}<d_{\max}<\infty and write U=ZdU=Z^d, where dmin⁡≤d≤dmax⁡d_{\min}\le d\le d_{\max}. The rows in the present dyad satisfy qu≍Uq_u\asymp U, with fixed comparison constants. Let

0<τ≤dmin⁡/100,T1=Zτ>2,0<e<10−3,I=⌈1/e⌉+2.0<\tau\le d_{\min}/100,\qquad T_1=Z^\tau>2,\qquad 0<e<10^{-3},\qquad I=\lceil1/e\rceil+2.

The value of τ\tau will be chosen after the fixed height orders are known. For now it is fixed independently of ZZ. In particular T1≤U1/100T_1\le U^{1/100}.

Lemma 8.1 (Buffered zero-free bins). For every retained row uu, there are an index i∈{1,…,I−1}i\in\{1,\ldots,I-1\} and a grid point

a∈(51/100+eZ≥0)∩[51/100,1]a\in(51/100+e\mathbb Z_{\ge0})\cap[51/100,1]

with the following properties. For j=1,…,Ij=1,\ldots,I, set

Mj(u)=max⁡({51/100}∪{ℜρ: ψ∈Xu, L(ρ,ψ∗)=0, ℜρ≥51/100, ∣ℑρ∣≤3jT1}).M_j(u)=\max\left(\{51/100\}\cup\left\{\Re\rho:\ \psi\in\mathcal{X}_u,\ L(\rho,\psi^*)=0,\ \Re\rho\ge51/100,\ |\Im\rho|\le3jT_1\right\}\right).

Then

a≤Mi(u)<a+e,Mi+1(u)<a+2e.a\le M_i(u)<a+e,\qquad M_{i+1}(u)<a+2e.

If a>51/100a>51/100, some ψ∈Xu\psi\in\mathcal{X}_u has a zero ρ=σ+iγ\rho=\sigma+i\gamma with

a≤σ<a+e,∣γ∣≤3iT1.a\le\sigma<a+e,\qquad |\gamma|\le3iT_1.

For every ϵ1>0\epsilon_1>0, every ψ∈Xu\psi\in\mathcal{X}_u, and sufficiently large ZZ, uniformly in the retained row,

∣Lorig(s,ψ)∣+∣Lorig(s,ψ)−1∣≪A,e,ϵ1Uϵ1(ℜs≥a+6e, ∣ℑs∣≤(3i+2)T1).|L_{\rm orig}(s,\psi)|+|L_{\rm orig}(s,\psi)^{-1}| \ll_{\mathcal A,e,\epsilon_1} U^{\epsilon_1} \quad \left(\Re s\ge a+6e,\ |\Im s|\le(3i+2)T_1\right).

On the reflected line in the same height range,

∣Lorig(1−a−6e+it,ψ)∣≪A,e,ϵ1Ua−1/2+12e+ϵ1(3+T1)C,|L_{\rm orig}(1-a-6e+it,\psi)| \ll_{\mathcal A,e,\epsilon_1} U^{a-1/2+12e+\epsilon_1}(3+T_1)^C,

where CC depends only on the fixed real strip and the field. There are Oe(1)O_e(1) possible pairs (i,a)(i,a), independently of the row and its conductor.

Proof. Each maximum exists: the collection is finite, the zeros of each nonprincipal primitive LL-function are discrete in compact rectangles, and absolute Euler convergence excludes zeros with real part greater than one. The sequence Mj(u)M_j(u) is nondecreasing and lies in [51/100,1][51/100,1]. If every one of its I−1I-1 increments exceeded ee, then

MI(u)−M1(u)>(I−1)e>1,M_I(u)-M_1(u)>(I-1)e>1,

which is impossible. Choose an index with Mi+1(u)−Mi(u)≤eM_{i+1}(u)-M_i(u)\le e, and round Mi(u)M_i(u) down on the stated grid. This gives the two inequalities. When a>51/100a>51/100, the maximum Mi(u)M_i(u) is attained by an actual zero, giving ρ\rho. This reasoning allows a zero on the line one.

For ∣t∣≤(3i+2)T1|t|\le(3i+2)T_1, the closed disk centered at 2+it2+it with radius 2−a−2e2-a-2e has real part at least a+2ea+2e. Its radius is less than 3/2<T13/2<T_1, so every point in it has imaginary part of absolute value less than 3(i+1)T13(i+1)T_1. The bound Mi+1(u)<a+2eM_{i+1}(u)<a+2e therefore excludes every zero of every primitive function in this disk. Lemma 4.9 controls the concentric disk of radius 2−a−6e2-a-6e. Apply it with center 2+iℑs2+i\Im s, and use absolute Euler convergence farther right. Since Qψ≪AUQ_\psi\ll_{\mathcal A}U and (3+∣t∣)2≪eU1/50(3+|t|)^2\ll_e U^{1/50}, the arbitrarily small power in that lemma can be chosen so that its contribution is Uε1/2U^{\varepsilon_1/2}. The estimates for polynomial-size deleted Euler products following that lemma supply the other Uε1/2U^{\varepsilon_1/2}.

For the last assertion, the primitive functional equation recalled in the proof of Lemma 4.8 [11 Equation (1.1)] relates the value at 1−a−6e+it1-a-6e+it to the conjugate primitive function at a+6e−ita+6e-it. The conjugate presentation is in Xu\mathcal{X}_u. The conductor and gamma quotient contribute at most

Qψa−1/2+6e(3+∣t∣)C.Q_\psi^{a-1/2+6e}(3+|t|)^C.

The reflected primitive value has an arbitrarily small UU-power by the preceding disk bound. Finally, 1−a−6e≥−6e1-a-6e\ge-6e, so the upper bound for the deleted product is U6e+ε1U^{6e+\varepsilon_1}, after reducing the preliminary losses. This proves the reflected estimate. The ranges of ii and aa give Oe(1)O_e(1) pairs.

We call (i,a)(i,a) the bin of the row and put

δ=2a−1,1/50≤δ≤1.\delta=2a-1,\qquad1/50\le\delta\le1.

Every primitive character inducing a presentation in Xu\mathcal{X}_u is a finite-order Hecke character. The definition of β∗\beta_*, together with β∗>51/100\beta_*>51/100, therefore gives Mi(u)≤β∗M_i(u)\le\beta_*. In particular, the bin satisfies the exact inequalities

a≤β∗,δ≤2β∗−1.a\le\beta_*,\qquad\delta\le2\beta_*-1.

The bin a=51/100a=51/100 will be bounded by the trivial row count. For a>51/100a>51/100, the zero in Lemma 8.1 produces large polynomials to which the moments can be applied.

Lemma 8.2 (Pointwise dyadic estimates). Fix bounded nonnegative ranges for rr, mm, and let

Mr=Mψ(r;WM),Sm=Sψ(m;WS)M_r=M_\psi(r;W_M),\qquad S_m=S_\psi(m;W_S)

denote the polynomials of Equations (4.2) and (4.1), now at base UU. Suppose ψ∈Xu\psi\in\mathcal{X}_u, the untwisted profiles have uniformly bounded smooth seminorms on a fixed annulus, and any pure norm twist has height at most (3i+1)T1(3i+1)T_1. All additional Mellin frequencies entering the same LL-argument are required to have total absolute value at most T1/2T_1/2.

For every ε>0\varepsilon>0, there are e0>0e_0>0, depending only on ε\varepsilon and the bounded length ranges, and a finite height order AAA_{\mathcal{A}}, uniform in the moving rows and profiles, such that, when

0<e<e0,(1+T1)AA≤Uϵ/10,0<e<e_0,\qquad (1+T_1)^{A_{\mathcal A}}\le U^{\epsilon/10},

the following estimates hold for sufficiently large ZZ:

∣Mr∣2≪A,ϵUδr+ϵ,|M_r|^2\ll_{\mathcal A,\epsilon}U^{\delta r+\epsilon},
∣Sm∣2≪A,ϵUδmin⁡(m,1−m)+ϵ.|S_m|^2\ll_{\mathcal A,\epsilon} U^{\delta\min(m,1-m)+\epsilon}.

The external tail order may be chosen after the positive number τ\tau. It does not change AAA_{\mathcal A}.

Proof. We spell out the height restriction because a full infinite contour shift would not be justified by the bin. For a fixed annular WW, a bounded real number σ\sigma, and a pure twist yiωy^{i\omega}, Mellin inversion on a line c+σ>1c+\sigma>1 gives

U−r/2∑nμ(n)ψ(n)W(qn/Ur)(qn/Ur)−σ+iω=12πi∫(c)MW(s)Ur(s+σ−iω−1/2)Lorig(s+σ−iω,ψ)−1 ds.U^{-r/2}\sum_n \mu(n)\psi(n)W(q_n/U^r)(q_n/U^r)^{-\sigma+i\omega} = \frac{1}{2\pi i}\int_{(c)}\mathcal{M}W(s)U^{r(s+\sigma-i\omega-1/2)}L_{\mathrm{orig}}(s+\sigma-i\omega,\psi)^{-1}\,ds.

Here MW\mathcal{M}W is the Mellin transform defined in Lemma 4.5. The twist occurs in the LL-argument, not in the transform whose tails are estimated. Shift only the portion with added frequency at most the assigned fraction of T1T_1 to ℜ(s+σ)=a+6e\Re(s+\sigma)=a+6e. The horizontal joins and the shifted portion remain in the zero-free rectangle of Lemma 8.1. Its bound gives U(a−1/2+6e)r+ϵ1U^{(a-1/2+6e)r+\epsilon_1} for the central portion.

Leave the remaining tails on the absolute line, which we may take to be ℜ(s+σ)=2\Re(s+\sigma)=2. There the reciprocal Euler product is absolutely bounded. On the inverse joins the reciprocal remains inside the buffered rectangle. Since the real join interval and the length range are bounded, the remaining arithmetic and scale factors on a join are O(UB(1+∣ℑs∣)J)O(U^B(1+|\Im s|)^J) for fixed B,JB,J chosen before the external tail order. The pointwise Mellin bound in (4.11), applied on that compact real interval with derivative order N+⌈J⌉+1N+\lceil J\rceil+1, bounds each horizontal join by O(UBT1−N)O(U^B T_1^{-N}). The separate vertical tails have the same bound by (4.10). Both estimates apply to the untwisted profile, uniformly in the stated family. Because T1=ZτT_1=Z^\tau, τ>0\tau>0, and all lengths lie in a fixed bounded interval, a sufficiently large fixed NN makes these errors smaller than the claimed bound. Taking ee and ϵ1\epsilon_1 small in the prescribed ϵ\epsilon proves (8.1).

For the plain polynomial the same calculation uses LorigL_{\mathrm{orig}} instead of its reciprocal. Shifting to ℜ(s+σ)=a+6e\Re(s+\sigma)=a+6e gives

∣Sm∣≪U(a−1/2+6e)m+ϵ1+O(UBT1−N).|S_m|\ll U^{(a-1/2+6e)m+\epsilon_1} +O(U^B T_1^{-N}).

Alternatively shift its central portion to ℜ(s+σ)=1−a−6e\Re(s+\sigma)=1-a-6e. The function is entire because the row is nonprincipal. The reflected estimate of Lemma 8.1 gives

∣Sm∣≪Ua−1/2+12e+ϵ1U(1/2−a−6e)m(3+T1)C+O(UBT1−N).|S_m|\ll U^{a-1/2+12e+\epsilon_1} U^{(1/2-a-6e)m}(3+T_1)^C +O(U^B T_1^{-N}).

The joins here need only the global upper strip bound and the negative-strip bound for the deleted product, since no reciprocal is present. These give fixed B,JB,J as above, so the pointwise Mellin estimate bounds the joins and the integrated Fourier estimate bounds the absolute-line tails. Taking the better central bound, choosing NN to dominate also the possibly negative exponent when m>1m>1, and using the displayed height hypothesis proves (8.2). A primitive conductor smaller than UU reduces the reflected conductor factor. The original deleted Euler factors have already been included in Lemma 8.1.

There are only finitely many separated variables in any one LL-argument. Assign each a fixed fraction of the single T1/2T_1/2 allowance; do not assign that allowance anew at successive shifts. The profile windows and the finite height orders used in the row estimates are fixed before NN. Lemma 4.5 differentiates only the untwisted separating profiles when increasing NN, which proves the last assertion.

Simultaneous saturated witnesses

At a selected zero, the truncated-inverse construction below produces a product with squared size at least Uδ(r+m)−ϵU^{\delta(r+m)-\epsilon}. The pointwise estimates bound the same product by Uδ(r+min⁡(m,1−m))+ϵU^{\delta(r+\min(m,1-m))+\epsilon}. Since δ≥1/50\delta\ge1/50, these two bounds force m≤1/2+O(ϵ)m\le1/2+O(\epsilon). Each factor then attains its own pointwise exponent up to the prescribed loss; this is the saturation asserted in the next proposition.

Proposition 8.3 (Two saturated witnesses). Let uu have a bin (i,a)(i,a) with a>51/100a > 51/100, and assume the loss and height hypotheses of Lemma 8.2. For every t∈[1,3/2]t \in[1,3/2], and every prescribed ϵ>0\epsilon> 0, after reducing its preliminary losses, there are ψ∈Xu\psi\in\mathcal X_u, a zero ρ=σ+iγ\rho= \sigma+i\gamma as in Lemma 8.1, dyadic lengths D=UrD = U^r, N=UmN = U^m, and two polynomials Mr,SmM_r,S_m for the common row character ψ\psi such that

r≤t+O(1/log⁡U),r+m≥t−O(1/log⁡U),∣MrSm∣2≫A,ϵUδ(r+m)−ϵ.r\le t+O(1/\log U),\qquad r+m\ge t-O(1/\log U),\qquad |M_rS_m|^2\gg_{\mathcal A,\epsilon} U^{\delta(r+m)-\epsilon}.

Their lengths and individual values also satisfy

t−12−O(ϵ)≤r≤t+O(1/log⁡U),0≤m≤12+O(ϵ),t-\frac{1}{2}-O(\epsilon) \le r \le t+O(1/\log U), \qquad0 \le m \le\frac{1}{2}+O(\epsilon),
∣Mr∣2≫A,ϵUδr−ϵ,∣Sm∣2≫A,ϵUδm−ϵ.|M_r|^2\gg_{\mathcal A,\epsilon}U^{\delta r-\epsilon}, \qquad |S_m|^2\gg_{\mathcal A,\epsilon}U^{\delta m-\epsilon}.

The constants in the O(ϵ)O(\epsilon) terms are absolute on the stated parameter ranges. Both polynomials have the same twist height γ−ν\gamma-\nu, where ∣ν∣≤cT1|\nu| \le cT_1 for a fixed c>0c > 0 chosen within the cumulative frequency allowance. Their untwisted profiles form a uniformly smooth annular family. For each row, both witnesses use one presentation ψu,ϑ,ς\psi_{u,\vartheta,\varsigma}, selected by a label (ϑ,ς)(\vartheta,\varsigma) in the fixed finite set Θ×{−1,1}\Theta\times\{-1,1\}. The presentation itself varies with uu. The dyadic pair can likewise be selected separately for each row from O((log⁡U)2)O((\log U)^2) possibilities.

Proof. The truncated-inverse and Gamma-integral construction is a form of the classical zero detector; compare [21 Appendix C] and [14 Section 13.1]. The buffered row-dependent rectangle and the simultaneous lower bounds needed here are established below. Choose the zero ρ\rho supplied by the bin and set

D∗=Ut,Y∗=U20.D_* = U^t, \qquad Y_* = U^{20}.

Let V≤V_{\le} be a fixed smooth function equal to one on [0,1][0,1] and zero on [2,∞)[2,\infty). Define

Cψ(s)=∑lμ(l)ψ(l)V≤(ql/D∗)ql−s,J=12πi∫(2)Y∗zΓ(z)Lorig(ρ+z,ψ)Cψ(ρ+z) dz.C_\psi(s)=\sum_l\mu(l)\psi(l)V_{\le}(q_l/D_*)q_l^{-s}, \qquad J=\frac1{2\pi i}\int_{(2)} Y_*^z\Gamma(z)L_{\rm orig}(\rho+z,\psi) C_\psi(\rho+z)\,dz.

The row character is nonprincipal, so Lorig⁡L_{\operatorname{orig}} is entire. Moving the line to ℜz=−1/4\Re z=-1/4 crosses only the pole of Γ(z)\Gamma(z) at zero, and its residue vanishes because Lorig⁡(ρ,ψ)=0L_{\operatorname{orig}}(\rho,\psi)=0. The global strip bound in (4.14), together with the deleted Euler factors, bounds the new line by

U−5U2D∗1−σ+1/4+o(1)T12.U^{-5}U^2D_*^{1-\sigma+1/4+o(1)}T_1^2.

Indeed ℜ(ρ−1/4)≥26/100>0\Re(\rho-1/4)\ge26/100>0, so the deleted product has an arbitrarily small UU-power; the deliberately weaker U2U^2 includes the primitive conductor bound. The finite polynomial is bounded by the displayed power of D∗D_* using the ideal count. Finally, the fixed polynomial in the added height is integrable against Γ(−1/4+iv)\Gamma(-1/4+iv), since (1+∣γ+v∣)2≤(1+∣γ∣)2(1+∣v∣)2(1+|\gamma+v|)^2\le(1+|\gamma|)^2(1+|v|)^2. Uniformly for 1≤t≤3/21\le t\le3/2,

−3+t(5/4−σ)≤−3+32(54−51100)=−189100.-3+t(5/4-\sigma)\le-3+\frac{3}{2}\left(\frac{5}{4}-\frac{51}{100}\right)=-\frac{189}{100}.

Thus J=o(1)J=o(1). This Gamma integration uses only global upper bounds and consumes no reciprocal height allowance.

On the original line, absolute convergence and the Mellin formula for the exponential give

J=∑l,kμ(l)ψ(lk)V≤(ql/D∗)(qlqk)−ρe−qlqk/Y∗.J=\sum_{l,k}\mu(l)\psi(lk)V_{\le}(q_l/D_*) (q_lq_k)^{-\rho}e^{-q_lq_k/Y_*}.

For 1<qn≤D∗1<q_n\le D_*, the coefficient of ψ(n)qn−ρ\psi(n)q_n^{-\rho} is ∑l∣nμ(l)=0\sum_{l\mid n}\mu(l)=0. For n=1n=1 it is one. When qn>D∗q_n>D_*, V≤(2qn/D∗)=0V_{\le}(2q_n/D_*)=0. Consequently insertion of 1−V≤(2qlqk/D∗)1-V_{\le}(2q_lq_k/D_*) removes exactly the unit contribution e−1/Y∗=1+o(1)e^{-1/Y_*}=1+o(1). The resulting tail has absolute value 1+o(1)1+o(1). Multiplying it by a fixed smooth terminal cutoff equal to one for qlqk≤U21q_lq_k \le U^{21} and zero for qlqk≥2U21q_lq_k \ge2U^{21} changes it by o(1)o(1); this follows from Y∗=U20Y_* = U^{20}, exponential decay, and the ideal count. Partition ql≍Dq_l \asymp D, qk≍Nq_k \asymp N by a fixed smooth dyadic partition. There are O((log⁡U)2)O((\log U)^2) relevant pairs, and their support satisfies

D≪D∗,DN≫D∗,DN≪U21.D \ll D_*, \qquad DN \gg D_*, \qquad DN \ll U^{21}.

With x=ql/Dx=q_l/D, y=qk/Ny=q_k/N, the profile for a pair is

W1(x)V≤(Dx/D∗)W2(y)HD,N(xy),W_1(x)V_{\leq}(Dx/D_*)W_2(y)H_{D,N}(xy),

where Ω\Omega is a fixed annular cutoff equal to one on the product of the supports of W1,W2W_1,W_2, and

HD,N(s)=Ω(s)[1−V≤(2DNs/D∗)]e−DNs/Y∗Vterm(DNs/U21).H_{D,N}(s)=\Omega(s)[1-V_{\leq}(2DNs/D_*)]e^{-DNs/Y_*}V_{\mathrm{term}}(DNs/U^{21}).

Every fixed logarithmic derivative is bounded uniformly in D,N,UD,N,U. On a cutoff transition its argument is bounded, and a logarithmic derivative of the exponential is a polynomial in its argument times that exponential. Logarithmic Fourier inversion therefore gives

HD,N(xy)=12π∫RH^D,N(ν)xiνyiν dν,H_{D,N}(xy)=\frac{1}{2\pi}\int_{\mathbb{R}}\widehat{H}_{D,N}(\nu)x^{i\nu}y^{i\nu}\,d\nu,
∫∣ν∣>cT1∣H^D,N(ν)∣(1+∣ν∣)J dν≪J,N0,cT1−N0\int_{|\nu|>cT_1}\left|\widehat{H}_{D,N}(\nu)\right|(1+|\nu|)^J\,d\nu\ll_{J,N_0,c}T_1^{-N_0}

for every fixed J,N0J,N_0. The coefficient L1L^1-norm on the full line is also uniformly bounded. Trivial bounds for the two finite polynomials have a fixed UU-power because their lengths are bounded by U21+o(1)U^{21+o(1)}. After τ>0\tau>0 is fixed, choose N0N_0 so that the discarded Fourier tail is o(1)o(1).

The absolute value of the remaining sum of integrals is bounded below by a positive constant. The number of dyadic pairs and the uniform L1L^1-norm show that, for one pair and one ∣ν∣≤cT1|\nu|\leq cT_1, the product of the two unnormalized blocks has absolute value ≫(log⁡U)−2\gg(\log U)^{-2}. Both profiles have the same height γ−ν\gamma-\nu:

WM(x)=W1(x)V≤(Dx/D∗)x−σ−i(γ−ν),W_M(x)=W_1(x)V_{\leq}(Dx/D_*)x^{-\sigma-i(\gamma-\nu)},
WS(y)=W2(y)y−σ−i(γ−ν).W_S(y)=W_2(y)y^{-\sigma-i(\gamma-\nu)}.

The first extra cutoff remains part of the inverse annular profile and creates no second frequency. Removing the factors D1/2−σD^{1/2-\sigma} and N1/2−σN^{1/2-\sigma} by central normalization gives

∣MrSm∣2≫(log⁡U)−4(DN)2σ−1≥Uδ(r+m)−ϵ|M_rS_m|^2\gg(\log U)^{-4}(DN)^{2\sigma-1}\geq U^{\delta(r+m)-\epsilon}

for sufficiently large UU. The support inequalities give the two length bounds in Equation (8.3). Apply Lemma 8.2 to these profiles, choosing its loss smaller than the present ϵ\epsilon. Comparison of the product lower bound with the two upper bounds gives

δ{m−min⁡(m,1−m)}=2δ(m−1/2)+≪ϵ.\delta\{m-\min(m,1-m)\}=2\delta(m-1/2)_+\ll\epsilon.

Since δ≥1/50\delta\geq1/50, this implies m≤1/2+O(ϵ)m\leq1/2+O(\epsilon) with an absolute constant. The support inequality then gives r≥t−1/2−O(ϵ)r\geq t-1/2-O(\epsilon). Dividing the product lower bound in turn by each individual upper bound gives the two individual lower bounds in Equation (8.4). Only the dyadic support errors are O(1/log⁡U)O(1/\log U); all other losses are arbitrarily small fixed powers. Lemma 4.5 permits the stated rowwise choices with a fixed polynomial height factor.

A sextic-sieve row count

The zero detector supplies a large inverse polynomial for each row above the floor bin. We now turn that lower bound into a count of physical rows. We first prove the required squarefree sextic large sieve in the primary convention, using the norm-recursion method of Blomer, Goldmakher, and Louvel [4 Section 3]. We then fix the part of a physical row whose prime valuations are at least two and apply the sieve to its squarefree factor. The size of the fixed part also gives an independent upper bound for the number of rows; the better of the two bounds produces the required exponent.

The sextic large sieve in the primary convention

We continue to use the fixed finite set SS of prime ideals, containing the primes above 6 and all fixed conductor primes. All ideal indices in the next lemma are prime to SS and are represented by their primary generators. In particular, “squarefree” refers to ideals of O=Z[ω]\mathcal{O} = \mathbb{Z}[\omega], not to their rational norms.

Lemma 9.1 (Sextic large sieve). Let K,D≥1K,D \ge1, let ς∈{−1,1}\varsigma\in\{-1,1\}, and let (cn)(c_n) be any sequence of complex numbers indexed by the squarefree ideals outside SS. The sequence is fixed independently of the row kk. For every ϵ>0\epsilon> 0,

∑k sfqk≤K∣∑n sfqn≤Dcnχn(k)ς∣2≪S,ϵ(KD)ϵ{K+D+(KD)2/3}∑n sfqn≤D∣cn∣2.\sum_{\substack{k\ {\rm sf}\\q_k\le K}} \left|\sum_{\substack{n\ {\rm sf}\\q_n\le D}} c_n\chi_n(k)^{\varsigma}\right|^2 \ll_{S,\epsilon}(KD)^\epsilon \bigl\{K+D+(KD)^{2/3}\bigr\} \sum_{\substack{n\ {\rm sf}\\q_n\le D}}|c_n|^2.

Every symbol in this formula has its original zero value on a nonunit. A fixed restriction of the row set is allowed. A fixed restriction of the coefficient support is allowed by extending that coefficient sequence by zero. Such a restriction may depend on an object fixed before the row sum, but the coefficients may not otherwise depend on kk.

Proof. We follow the higher-order large-sieve recursion of Blomer, Goldmakher, and Louvel [4 Section 3], giving the local verification for the present primary normalization. In the finite Fourier calculation the individual residue characters act on elements; their unit-trivial quotient is the character on ideals to which we apply Poisson summation.

For good ideals a,ba,b, represented by their primary generators, put

Fb(a)=χa(b),J={1,2,4}.F_b(a)=\chi_a(b),\qquad J=\{1,2,4\}.

This uses the original zero-extended symbol, also when aa is not squarefree. It is multiplicative in both aa and bb. In every power below, including a multiple of six, a nonunit still has value zero. For M>0M>0 let

IM={a good:M<qa≤2M},AM={a∈IM:a squarefree}.\mathcal I_M=\{a\text{ good}:M<q_a\le2M\},\qquad \mathcal A_M=\{a\in\mathcal I_M:a\text{ squarefree}\}.

For a sequence supported on AN\mathcal{A}_N write ∥λ∥22=∑b∈AN∣λb∣2\|\lambda\|_2^2=\sum_{b\in\mathcal{A}_N}|\lambda_b|^2, and define

Dj(M,N)=sup⁡∥λ∥2=1∑a∈AM∣∑b∈ANλbFb(a)j∣2,D_j(M,N)=\sup_{\|\lambda\|_2=1}\sum_{a\in\mathcal{A}_M}\left|\sum_{b\in\mathcal{A}_N}\lambda_bF_b(a)^j\right|^2,
Ej(M,N)=sup⁡∥λ∥2=1∑a∈IM∣∑b∈ANλbFb(a)j∣2.E_j(M,N)=\sup_{\|\lambda\|_2=1}\sum_{a\in\mathcal{I}_M}\left|\sum_{b\in\mathcal{A}_N}\lambda_bF_b(a)^j\right|^2.

An empty support gives norm zero. These norms include all finite ray classes. We will prove the symmetric bound for D1D_1; the matrix in the lemma is its transpose with the two lengths exchanged.

The squarefree norm DjD_j is our target. We also need EjE_j, since Poisson summation produces arbitrary evaluation ideals. Opening the square in its defining sum and pairing the column characters will replace a row length MM by a dual length of order N2/MN^2/M. A power decomposition then returns the unrestricted row sum to squarefree norms. It selects either the first-power or the second-power factor, so the exponents j∈{1,2,4}j \in\{1,2,4\} are kept together: this set is closed under j↦2j(mod6)j\mapsto2j\pmod6 (mod 6). We will use this cycle to improve a provisional exponent in the bound for DjD_j.

The paired summation formula. Use the fixed finite group

T=ker⁡((O/36O)×⟶(O/3O)×),t(b)=b mod 36O.\mathcal T=\ker\bigl((\mathcal O/36\mathcal O)^\times \longrightarrow(\mathcal O/3\mathcal O)^\times\bigr), \qquad t(b)=b\bmod36\mathcal O.

The primary normalization identifies these with the ray classes modulo 36O36\mathcal{O}: each unit orbit has a unique representative equal to one modulo 3. In particular tt is multiplicative. This subdivision is fixed, since the primes above 2 and 3 belong to SS.

For a global unit uu and a good prime pp, reduction modulo pp gives χp(u)=u(qp−1)/6\chi_p(u)=u^{(q_p-1)/6}. Since qp≡1(mod6)q_p\equiv1\pmod{6}, multiplication over the prime factors of bb gives

χb(u)=u(qb−1)/6.\chi_b(u)=u^{(q_b-1)/6}.

The exponent is read modulo six: expanding a product of integers 1+6h1+6h proves the equality of exponents. Thus equal tt-classes have the same restriction to the six global units. They also have the same residue modulo 4, which controls the reciprocity factor R\mathcal{R} of Lemma 4.4.

Let b,cb,c be coprime squarefree good ideals with t(b)=t(c)t(b)=t(c) and let j∈Jj\in J. The raw character on elements

Θb,c(j)(z)=χb(z)jχc(z)j‾(z mod bc)\Theta_{b,c}^{(j)}(z)=\chi_b(z)^j\overline{\chi_c(z)^j} \quad (z\bmod bc)

is trivial on global units by Equation (9.2). It therefore defines a finite-order ray character on ideals by

Ψb,c(j)((z))=Θb,c(j)(z).\Psi_{b,c}^{(j)}((z))=\Theta_{b,c}^{(j)}(z).

For fractional ideals prime to bcbc, the residue symbols are evaluated on local unit fractions; the same unit cancellation makes this definition independent of the generator. At each good prime the sextic residue character has exact order six, since the residue multiplicative group is cyclic. Hence its powers jj and −j-j are nontrivial. CRT shows that Θb,c(j)\Theta_{b,c}^{(j)} has raw conductor bcbc, and the ray character has the same conductor: omitting a prime would contradict this nontriviality by varying only its residue. It is extended by zero on ideals meeting bcbc. For the pair b=c=1b=c=1 define Ψ1,1(j)\Psi_{1,1}^{(j)} to be principal.

Sextic reciprocity, with its factor fixed by t(b)=t(c)t(b)=t(c), gives for every good ideal aa

Ψb,c(j)(a)=Fb(a)jFc(a)j‾.\Psi_{b,c}^{(j)}(a)=F_b(a)^j\overline{F_c(a)^j}.

For coprime inputs the two reciprocity factors cancel; on the other inputs both sides are zero. With the Gauss sums already defined in the arithmetic preliminaries, CRT using z=cv+bwz=cv+bw gives

Γb,c(j):=qbc−1/2∑z mod bcΘb,c(j)(z)e(z/(bc))=χb(c)jχc(b)j‾γj(b)γ−j(c)=ηt(b),jγj(b)γ−j(c),\begin{aligned} \Gamma_{b,c}^{(j)} &:=q_{bc}^{-1/2}\sum_{z\bmod bc}\Theta_{b,c}^{(j)}(z)e(z/(bc))\\ &=\chi_b(c)^j\overline{\chi_c(b)^j}\gamma_j(b)\gamma_{-j}(c) =\eta_{t(b),j}\gamma_j(b)\gamma_{-j}(c), \end{aligned}

where ηt(b),j=R(b,c)j\eta_{t(b),j}=\mathcal{R}(b,c)^j depends only on the common class. Every γ±j\gamma_{\pm j} here has modulus one by prime Gauss orthogonality and CRT. Formula (9.4) retains γ−j\gamma_{-j} itself, including its factor at −1-1 under conjugation.

Choose once a nonnegative W∈Cc∞((0,∞))W\in C_c^\infty((0,\infty)) with W≥1W \ge1 on [1,2][1,2]. For the Fourier transform and self-dual measure in the arithmetic preliminaries, put w(z)=W(∣z∣2)w(z)=W(|z|^2) and define W\mathscr W by

w^(y)=W(∣y∣2).\widehat w(y)=\mathscr W(|y|^2).

The transform is radial, smooth at zero, and rapidly decreasing. Thus

W(x)≪A(1+x)−A,∫R∣MW(σ+it)∣ dt<∞(σ>0).\mathscr W(x)\ll_A(1+x)^{-A},\qquad \int_{\mathbb R}|\mathcal M\mathscr W(\sigma+it)|\,dt<\infty \quad(\sigma>0).

Here M\mathcal{M} denotes the Mellin transform. The second assertion follows by integration by parts in the Mellin integral; all logarithmic derivatives are bounded at zero and rapidly decreasing at infinity. Scaling the Fourier transform gives MW(M∣y∣2)M\mathscr W(M|y|^2) for z↦W(∣z∣2/M)z\mapsto W(|z|^2/M).

For bc≠1bc\ne1, finite Fourier inversion for the primitive raw character is

∑v mod bcΘb,c(j)(v)e(vy/(bc))=Θb,c(j)(y)‾qbcΓb,c(j).\sum_{v\bmod bc}\Theta_{b,c}^{(j)}(v)e(vy/(bc))=\overline{\Theta_{b,c}^{(j)}(y)}\sqrt{q_{bc}}\Gamma_{b,c}^{(j)}.

For a nonunit yy the left side vanishes because one nontrivial local character is summed against the trivial additive character. For the stated ee and dμd\mu, the trace pairing on the basis (1,ω)(1,\omega) has matrix (011−1)\begin{aligned}\left(\begin{smallmatrix}0&1\\1&-1\end{smallmatrix}\right)\end{aligned}, of determinant −1-1, and the dμd\mu-covolume of O\mathcal{O} is one. Thus the dual of bcObc\mathcal{O} is (bc)−1O(bc)^{-1}\mathcal{O}, while the covolume of bcObc\mathcal{O} is qbcq_{bc}. Coset Poisson summation, followed by division by the six generators of each ideal, therefore gives

∑a≠0W(qa/M)Ψb,c(j)(a)=MΓb,c(j)qbc∑a≠0W(Mqa/qbc)Ψb,c(j)(a)‾.\sum_{\mathfrak a\ne0}W(q_{\mathfrak a}/M)\Psi_{b,c}^{(j)}(\mathfrak a) =\frac{M\Gamma_{b,c}^{(j)}}{\sqrt{q_{bc}}} \sum_{\mathfrak a\ne0}\mathscr W(Mq_{\mathfrak a}/q_{bc}) \overline{\Psi_{b,c}^{(j)}(\mathfrak a)}.

Both sums here are over all nonzero integral ideals. The division by six uses unit-triviality of Θb,c(j)\Theta_{b,c}^{(j)} and radiality of the weight. The zero frequency vanishes since this character is nontrivial. Poisson transformation of the squared norm. For λ\lambda supported on one tt-class in AN\mathcal{A}_N, set

Qj(M,N;λ)=∑b,c∈AN(b,c)=1λbλc‾∑a≠0W(qa/M)Ψb,c(j)(a).Q_j(M,N;\lambda)= \sum_{\substack{b,c\in\mathcal A_N\\(b,c)=1}} \lambda_b\overline{\lambda_c} \sum_{\mathfrak a\ne0}W(q_{\mathfrak a}/M) \Psi_{b,c}^{(j)}(\mathfrak a).

We claim, for every ε>0\varepsilon>0,

∣Qj(M,N;λ)∣≪S,ε(2+MN)ε∥λ∥22×{M+MNmax⁡1≤HH≪S,ε(2+MN)εN2/MEj(H,N)}.|Q_j(M,N;\lambda)|\ll_{S,\varepsilon}(2+MN)^\varepsilon\|\lambda\|_2^2 \times\left\{M+\frac{M}{N}\max_{\substack{1\le H\\H\ll_{S,\varepsilon}(2+MN)^\varepsilon N^2/M}}E_j(H,N)\right\}.

The maximum runs over dyadic shells and is zero if empty. If N≤1N\le1, only the unit good ideal can occur and the annular ideal count proves the MM term. Also Qj=0Q_j=0 when MM is below a fixed positive constant, because WW has a fixed upper support endpoint and nonzero ideals have norm at least one.

Suppose N>1N>1 and normalize ∥λ∥2=1\|\lambda\|_2=1. Then every pair in QjQ_j is nontrivial and qbc≍N2q_{bc}\asymp N^2. Apply Equation (9.6) and take the triangle inequality over the dual ideals. For a small δ>0\delta>0 put Z=(2+MN)δZ=(2+MN)^\delta. Cauchy gives (∑b∣λb∣)2≪N(\sum_b|\lambda_b|)^2\ll N. By Equation (9.5), the part with qa>ZN2/Mq_{\mathfrak a}>ZN^2/M is, for any A>1A>1, at most

M∑qa>ZN2/M(Mqa/N2)−A≪N2Z1−A.M\sum_{q_{\mathfrak a}>ZN^2/M}(Mq_{\mathfrak a}/N^2)^{-A} \ll N^2Z^{1-A}.

The same bound holds if the cutoff is below one. Taking AA large makes this an arbitrary negative power error.

In the remaining sum write a=a0s\mathfrak a=a_0\mathfrak s, with a0a_0 good and s\mathfrak{s} supported on SS, and choose one generator s0s_0 for each fixed s\mathfrak{s}. Equations (9.3) and (9.4) give the separated factors

Ψb,c(j)(a0s)‾=Fb(a0)j‾Fc(a0)jχb(s0)j‾χc(s0)j.\overline{\Psi_{b,c}^{(j)}(a_0\mathfrak s)} =\overline{F_b(a_0)^j}F_c(a_0)^j \overline{\chi_b(s_0)^j}\chi_c(s_0)^j.

All χb(s0)\chi_b(s_0) have modulus one. Split a0a_0 into shells a0∈IHa_0\in\mathcal{I}_H, where H≪ZN2/(Mqs)H\ll ZN^2/(Mq_{\mathfrak{s}}), and insert Mellin inversion for W\mathscr W on ℜw=δ\Re w=\delta. Apart from a bounded factor depending on MM, qa0q_{a_0}, qsq_{\mathfrak{s}}, the two coefficient sequences are

Ab=λbγj(b)χb(s0)j‾qb−1/2+δ+it,Bb=λb‾γ−j(b)χb(s0)jqb−1/2+δ+it.A_b=\lambda_b\gamma_j(b)\overline{\chi_b(s_0)^j} q_b^{-1/2+\delta+it},\qquad B_b=\overline{\lambda_b}\gamma_{-j}(b)\chi_b(s_0)^j q_b^{-1/2+\delta+it}.

They are fixed across the a0a_0 sum and have absolute values ≪N−1/2+δ∣λb∣\ll N^{-1/2+\delta}|\lambda_b|. Detecting (b,c)=1(b,c)=1 by Möbius inversion and applying Cauchy in a0a_0 gives

∑a0∈IH∣∑b,c∈AN(b,c)=1AbBcFb(a0)j‾Fc(a0)j∣≤Ej(H,N)∑d(∑d∣b∣Ab∣2)1/2(∑d∣b∣Bb∣2)1/2≪N−1+3δEj(H,N).\begin{aligned} &\sum_{a_0\in\mathcal I_H} \left|\sum_{\substack{b,c\in\mathcal A_N\\(b,c)=1}} A_bB_c\overline{F_b(a_0)^j}F_c(a_0)^j\right|\\ &\quad\le E_j(H,N)\sum_{\mathfrak d} \left(\sum_{\mathfrak d\mid b}|A_b|^2\right)^{1/2} \left(\sum_{\mathfrak d\mid b}|B_b|^2\right)^{1/2} \ll N^{-1+3\delta}E_j(H,N). \end{aligned}

Here the divisor bound absorbs the sum over d\mathfrak d. Conjugating the entire first polynomial uses the same EjE_j norm. The factors with H<1H<1 have just the unit evaluation ideal and satisfy Ej(H,N)≪NE_j(H,N)\ll N. There are only a fixed power of log⁡(2+ZN2)\log(2+ZN^2) choices of s\mathfrak{s} and of the dyadic shell, because SS is fixed and a nonzero QjQ_j has MM bounded below. Equation (9.5) integrates the tt variable. Choosing δ\delta sufficiently small in terms of ε\varepsilon proves Equation (9.7), including the allowed global loss on its MM term.

We now apply this paired estimate to EjE_j. Partition its inner sum by tt, insert WW, and open the square. Write the two squarefree indices as dbdb, dcdc, where dd is their gcd, (b,c)=1(b,c)=1, and (d,bc)=1(d,bc)=1. Their residual classes agree because tt is multiplicative. Index multiplicativity and Equation (9.3) give on every good aa

Fdb(a)jFdc(a)j‾=1(a,d)=1Ψb,c(j)(a).F_{db}(a)^j\overline{F_{dc}(a)^j} =1_{(a,d)=1}\Psi_{b,c}^{(j)}(a).

Let sS=∏p∈Sp\mathfrak s_S=\prod_{\mathfrak p\in S}\mathfrak p. Möbius inversion for (a,sSd)=1(a,\mathfrak{s}_Sd)=1 writes a=raa=\mathfrak r\mathfrak a with r∣sSd\mathfrak{r}\mid\mathfrak{s}_Sd. Choose one generator r0r_0 of each fixed r\mathfrak{r}. The value of Ψ\Psi at r\mathfrak{r} separates as χb(r0)jχc(r0)j‾\chi_b(r_0)^j\overline{\chi_c(r_0)^j}, so the common residual sequence is

λb′=λdb1(b,d)=1χb(r0)j,∣λb′∣≤∣λdb∣.\lambda'_b=\lambda_{db}1_{(b,d)=1}\chi_b(r_0)^j, \qquad |\lambda'_b|\le|\lambda_{db}|.

It is supported on AN/qd\mathcal A_{N/q_d} in one class. Apply Equation (9.7) with lengths M/qrM/q_{\mathfrak{r}} and N/qdN/q_d. The summed coefficient mass is at most

∑d∑r∣sSd∑b∣λdb∣2≤dO(sS)∑mdO(m)2∣λm∣2≪S,δ(2+N)δ∥λ∥22.\sum_d\sum_{\mathfrak r\mid\mathfrak s_Sd}\sum_b|\lambda_{db}|^2 \le d_{\mathcal O}(\mathfrak s_S) \sum_m d_{\mathcal O}(m)^2|\lambda_m|^2 \ll_{S,\delta}(2+N)^\delta\|\lambda\|_2^2.

Writing Δr=qr\Delta_{\mathrm r}=q_{\mathfrak r} and Δd=qd\Delta_{\mathrm d}=q_d, we have 1≤Δd≤2N1\le\Delta_{\mathrm d}\le2N and 1≤Δr≤qsSΔd1\le\Delta_{\mathrm r}\le q_{\mathfrak s_S}\Delta_{\mathrm d}. We obtain the recursive interface

Ej(M,N)≪S,ε(2+MN)εmax⁡1≤Δd≤2N1≤Δr≤qsSΔd{MΔr+MΔdNΔrmax⁡1≤HH≪S,ε(2+MN)εN2Δr/(MΔd2)Ej(H,N/Δd)}.\begin{aligned} E_j(M,N) &\ll_{S,\varepsilon}(2+MN)^\varepsilon \max_{\substack{1\le\Delta_{\mathrm d}\le2N\\ 1\le\Delta_{\mathrm r}\le q_{\mathfrak s_S}\Delta_{\mathrm d}}} \left\{\frac M{\Delta_{\mathrm r}}\right.\\ &\qquad\left.+ \frac{M\Delta_{\mathrm d}}{N\Delta_{\mathrm r}} \max_{\substack{1\le H\\ H\ll_{S,\varepsilon}(2+MN)^\varepsilon N^2\Delta_{\mathrm r}/(M\Delta_{\mathrm d}^2)}} E_j(H,N/\Delta_{\mathrm d})\right\}. \end{aligned}

The maxima may be restricted to nonempty ranges. This is the combination of the gcd and Poisson steps in [4 Lemmas 3.2–3.3]]; every sequence used here is common within its norm sum, and SS remains fixed.

The initial and power bounds. Row inclusion gives Dj≤EjD_j \le E_j. Hilbert space duality and sextic reciprocity, splitting one matrix variable by its finite tt-class, give

Dj(M,N)≪SDj(N,M).D_j(M,N) \ll_S D_j(N,M).

The phases are unit-valued and the noncoprime entries are zero in both orientations. We also have the initial estimate

Dj(M,N)≪SM2+N(M,N≥1).D_j(M,N) \ll_S M^2+N \qquad(M,N\geq1).

Indeed, for the squarefree row aa, finite Fourier inversion gives on every bb, including nonunits,

χa(b)j=1qaγ−j(a)∑x mod aχa(x)j‾e(xb/a).\chi_a(b)^j=\frac1{\sqrt{q_a}\gamma_{-j}(a)} \sum_{x\bmod a}\overline{\chi_a(x)^j}e(xb/a).

Cauchy costs at most #(O/(a))×/qa≤1\#(\mathcal{O}/(a))^\times/q_a\leq1. The reduced fractions x/ax/a from a∈AMa\in\mathcal{A}_M are distinct modulo O\mathcal{O} and separated by at least 1/(2M)1/(2M): a nonzero numerator of x/a−y/c−hx/a-y/c-h has absolute value at least one, while ∣ac∣≤2M|ac|\leq2M; equality modulo O\mathcal{O} forces the same primary denominator and residue. The dual of Lemma 6.1, with the coefficient generators in the ball qb≤2Nq_b\leq2N, proves Equation (9.10).

We need the following near-monotonicity, also used in the large-sieve recursions of [13 Lemma 4.4 and Remark 5]] and [4 Lemma 3.1]]:

Dj(M1,N)≪SDj(M2,N)if M2≥CM1log⁡(2M1N),M1,M2,N≥1.D_j(M_1,N)\ll_S D_j(M_2,N)\quad\text{if }M_2\geq CM_1\log(2M_1N),\quad M_1,M_2,N\geq1.

Here is a direct verification. The assertion is immediate for a zero norm. Otherwise choose a maximizing unit coefficient vector for Dj(M1,N)D_j(M_1,N), and split the row shell at 3M1/23M_1/2; one part carries at least half its mass. Put L=M2/M1L=M_2/M_1. For the first part use good prime ideals of norms in (L,4L/3](L,4L/3], and for the second use norms in (2L/3,L](2L/3,L]. Then ap∈AM2ap\in\mathcal{A}_{M_2} when p∤ap\nmid a. The fixed-field prime ideal theorem supplies P≫SL/log⁡LP\gg_S L/\log L such primes. An ideal of norm at most 2x2x contains at most dx=log⁡(2x)/log⁡(2L/3)d_x=\log(2x)/\log(2L/3) of them. For Sa(v)=∑bvbFb(a)jS_a(v)=\sum_b v_bF_b(a)^j and p∤ap\nmid a, multiplicativity gives

Sa(λ)=Sap((λbFb(p)j‾)b)+Sa((λb1p∣b)b).S_a(\lambda)=S_{ap}\bigl((\lambda_b\overline{F_b(p)^j})_b\bigr) +S_a\bigl((\lambda_b1_{p\mid b})_b\bigr).

The first coefficient is zero at p∣bp\mid b and cancels the factor at pp otherwise. Squaring and summing over the chosen rows and primes gives

P−dM12Dj(M1,N)≤2PDj(M2,N)+2dNDj(M1,N).\frac{P-d_{M_1}}{2}D_j(M_1,N)\leq2PD_j(M_2,N)+2d_ND_j(M_1,N).

For the stated threshold with CC sufficiently large, dM1+4dN≤P/2d_{M_1}+4d_N\leq P/2, proving Equation (9.11).

We finish with the power decomposition and recursion of [4 Lemmas 3.4–3.5]]. Suppose, simultaneously for j∈Jj\in J, that for every positive loss

Dj(M,N)≪S,ε(MN)ε{Mα+N+(MN)2/3},α>4/3,D_j(M,N)\ll_{S,\varepsilon}(MN)^\varepsilon\{M^\alpha+N+(MN)^{2/3}\},\qquad\alpha>4/3,

for M,N≥1M,N\geq1; the unit shells satisfy the same bound directly. The initial estimate gives this with α=2\alpha=2. Write a good evaluation ideal uniquely as

a=a1a22a33a44a55a66,a=a_1a_2^2a_3^3a_4^4a_5^5a_6^6,

where a1,…,a5a_1,\ldots,a_5 are pairwise coprime and squarefree, and a6a_6 is arbitrary. Insert ai∈IXia_i \in\mathcal{I}_{X_i} and put X=∏iXiX=\prod_i X_i; here Xi≥1/2X_i \ge1/2 and ∏iXii≍M\prod_i X_i^i \asymp M. Choose ℓ∈{1,2}\ell\in\{1,2\} with Xℓ=max⁡(X1,X2)X_\ell=\max(X_1,X_2). After the other factors are fixed, the coefficient

λb′=λb∏i≠ℓFb(ai)ij\lambda'_b=\lambda_b\prod_{i\ne\ell}F_b(a_i)^{ij}

has absolute value at most ∣λb∣|\lambda_b|, and the remaining kernel is exactly that of Djℓ mod 6(Xℓ,N)D_{j\ell\bmod6}(X_\ell,N). Enlarging its fixed positive row restriction gives this norm bound. This includes the zero of the sixth power factor. The set JJ is closed under j↦jℓ mod 6j\mapsto j\ell\bmod6. Counting the fixed ideals and forgetting their coprimalities in positive sums gives

Ej(M,N)≪S,ε(MN)εmax⁡Xmin⁡{M1/3,(M/Xℓ)2/3}Djℓ mod 6(Xℓ,N).E_j(M,N)\ll_{S,\varepsilon}(MN)^\varepsilon \max_{\boldsymbol X} \min\left\{M^{1/3},(M/X_\ell)^{2/3}\right\} D_{j\ell\bmod6}(X_\ell,N).

To verify the factor, the number of fixed choices is O(X/Xℓ)O(X/X_\ell). For ℓ=1\ell=1 it is at most a constant times both (M/X1)1/2≪(M/X1)2/3(M/X_1)^{1/2}\ll(M/X_1)^{2/3} and (MX2/X1)1/3≤M1/3(MX_2/X_1)^{1/3}\le M^{1/3}; for ℓ=2\ell=2 it is at most a constant times (MX12/X22)1/3≤M1/3≪(M/X2)2/3(MX_1^2/X_2^2)^{1/3}\le M^{1/3}\ll(M/X_2)^{2/3}. The number of boxes is a fixed power of log⁡(2+M)\log(2+M).

Substituting Equation (9.12) into Equation (9.13) yields

Ej(M,N)≪S,ε(MN)ε(Mα+M1/3N).E_j(M,N)\ll_{S,\varepsilon}(MN)^\varepsilon(M^\alpha+M^{1/3}N).

The three terms before simplification are bounded by MαM^\alpha, M1/3NM^{1/3}N, and (MN)2/3(MN)^{2/3}; the last is bounded by one of the first two according as N≤MN\le M or N≥MN\ge M. Use this estimate in Equation (9.8). All auxiliary nonempty scales are bounded by fixed powers of 2+MN2+MN: here N/Δd≥1/2N/\Delta_{\mathrm d}\ge1/2 and H(N/Δd)≪S,ε(2+MN)3+εH(N/\Delta_{\mathrm d})\ll_{S,\varepsilon}(2+MN)^{3+\varepsilon}. The unit column shell satisfies the same estimate directly. Thus preliminary losses can be chosen smaller to give any specified final loss. The two scale factors are

Δrα−1Δd1−2α≪SΔd−α≤1,(ΔrΔd)−2/3≤1.\Delta_{\mathrm r}^{\alpha-1}\Delta_{\mathrm d}^{1-2\alpha} \ll_S\Delta_{\mathrm d}^{-\alpha}\le1, \qquad (\Delta_{\mathrm r}\Delta_{\mathrm d})^{-2/3}\le1.

Consequently, for M,N≥1M,N\ge1,

Dj(M,N)≤Ej(M,N)≪S,ε(MN)ε{M+N2α−1M1−α+(MN)2/3}.D_j(M,N)\le E_j(M,N)\ll_{S,\varepsilon}(MN)^\varepsilon\{M+N^{2\alpha-1}M^{1-\alpha}+(MN)^{2/3}\}.

Put h=2−3/(3α−1)=(2α−5/3)/(α−1/3)h=2-3/(3\alpha-1)=(2\alpha-5/3)/(\alpha-1/3) and β=2−2/(3α−1)\beta=2-2/(3\alpha-1). If M≥NhM\ge N^h, the middle term in Equation (9.14) is at most (MN)2/3(MN)^{2/3}. If M<NhM<N^h, apply Equation (9.11) with a fixed multiple of Nhlog⁡(2MN)N^h\log(2MN) in place of MM. Equation (9.14) there gives (MN)εNβ(MN)^\varepsilon N^\beta, since 2(h+1)/3=β2(h+1)/3=\beta and h<βh<\beta. Thus in both cases

Dj(M,N)≪S,ε(MN)ε{M+Nβ+(MN)2/3}.D_j(M,N)\ll_{S,\varepsilon}(MN)^\varepsilon\{M+N^\beta+(MN)^{2/3}\}.

Symmetry gives Equation (9.12) with β\beta in place of α\alpha, simultaneously for every j∈Jj\in J. Starting from 22, the map α↦2−2/(3α−1)\alpha\mapsto2-2/(3\alpha-1) decreases to 4/34/3. For a requested loss take finitely many iterations until the remaining exponent gap is smaller than a fixed fraction of that loss, and absorb it into (MN)ε(MN)^\varepsilon. Combining the bound and its symmetric form, using M4/3≤(MN)2/3M^{4/3}\le(MN)^{2/3} when M≤NM\le N and the analogous inequality when N≤MN\le M, proves

Dj(M,N)≪S,ε(MN)ε{M+N+(MN)2/3}(j∈J).D_j(M,N)\ll_{S,\varepsilon}(MN)^\varepsilon\{M+N+(MN)^{2/3}\}\qquad(j\in J).

Dyadic subdivision of both norm balls, with Cauchy across the column shells, converts Equation (9.15) to the same bound for the ball matrix with entries Fb(a)=χa(b)F_b(a)=\chi_a(b). The logarithmic factors are absorbed by a smaller preliminary loss, and the unit shells are bounded directly. The matrix in Equation (9.1) for ς=1\varsigma=1 is the transpose of this matrix at lengths (D,K)(D,K). A complex matrix and its transpose have the same operator norm, by the adjoint identity followed by whole-vector conjugation. The bound is symmetric in the two lengths, so it gives precisely K+D+(KD)2/3K+D+(KD)^{2/3}. Conjugating the entire inner sum gives ς=−1\varsigma=-1, with unchanged zeros. Finally, a fixed row restriction removes nonnegative terms, and a fixed coefficient restriction is imposed by zero extension. This proves all assertions of the lemma.

Physical rows and their inverse witnesses

With the sieve proved, it remains to apply it to the detector witnesses. We apply the lemma only to a squarefree factor of the physical row. The separation of squarefree and powerful row factors is also used in the proof of Corollary 1.4 of [4]; here we keep the actual norm of the powerful factor because it controls both the moment and the number of rows.

Proposition 9.2 (Sextic-sieve row envelope). Fix the arithmetic data A\mathcal{A}, the bounded physical range dmin⁡≤d≤dmax⁡d_{\min} \le d \le d_{\max}, and the height and loss hypotheses of Lemmas 8.1 and 8.2. Put U=ZdU=Z^d and retain the notation T1T_1 of those lemmas. Let B\mathcal{B} be any set of retained sixth-power-free element rows uu with qu≍Uq_u \asymp U, all in one bin (i,a)(i,a) with a>51/100a > 51/100. Put δ=2a−1\delta= 2a - 1, so 1/50<δ≤11/50 < \delta\le1.

For every ϵ>0\epsilon> 0, after reducing the preliminary losses in Proposition 8.3, for all sufficiently large ZZ,

#B≪A,ϵUR(δ)+ϵ(1+T1)AA,R(δ)=min⁡{1,max⁡(1−δ2,43−δ)}.\#\mathcal{B} \ll_{\mathcal{A},\epsilon} U^{R(\delta)+\epsilon}(1+T_1)^{A_{\mathcal{A}}}, \qquad R(\delta)=\min\left\{1,\max\left(1-\frac{\delta}{2},\frac{4}{3}-\delta\right)\right\}.

The finite order AAA_{\mathcal{A}} is uniform in the physical dyad, the bin, and all moving rows. It may be fixed before the positive exponent in T1=ZτT_1=Z^\tau is chosen. The estimate is valid for each fixed retained tuple of external parameters and for the original row restrictions. The implied constant may depend on the fixed comparison constants and finitely many of the shared profile seminorms. The rowwise profile choices are precisely those permitted by Proposition 8.3 and Lemma 4.5; no arbitrary row-dependent coefficients are allowed.

The floor bin a=51/100a=51/100 is excluded from the witness assertion. For that bin the elementary bound #B≪AU\#\mathcal{B}\ll_{\mathcal{A}} U applies; it agrees with the numerical value R(1/50)=1R(1/50)=1.

Proof. Fix a small preliminary loss ϵ0>0\epsilon_0>0. Apply Proposition 8.3 with t=1t=1 to every row in B\mathcal{B}. Subdivide by its presentation labels in ψu,ν,ς(n)=ν(n)χn(u)ς\psi_{u,\nu,\varsigma}(n)=\nu(n)\chi_n(u)^{\varsigma} and its dyadic pair of polynomial lengths. There are a fixed finite number of presentation labels and OA((log⁡U)2)O_{\mathcal{A}}((\log U)^2) pairs. Within one such subdivision, the inverse length D=UrD=U^r and the pair (ν,ς)(\nu,\varsigma) are fixed. In this subdivision write

Mu(D;W)=D−1/2∑nμ(n)ν(n)χn(u)ςW(qn/D)M_u(D;W)=D^{-1/2}\sum_n \mu(n)\nu(n)\chi_n(u)^{\varsigma}W(q_n/D)

for the inverse polynomial of that presentation. The witness gives

12−O(ϵ0)≤r≤1+O(1/log⁡U),∣Mu(D;Wu)∣2≫A,ϵ0Uδr−ϵ0.\frac{1}{2}-O(\epsilon_0)\le r\le1+O(1/\log U), \qquad|M_u(D;W_u)|^2\gg_{\mathcal{A},\epsilon_0} U^{\delta r-\epsilon_0}.

The notation WuW_u retains the permitted rowwise norm-profile parameters. The polynomial here is the original one for the displayed presentation, not the polynomial of its primitive inducing character. We first bound it when those parameters are fixed, and then handle their rowwise choice.

For each sixth-power-free row, factor its ideal uniquely as

(u)=swk,s=∏p∈Spvp(u),w=∏p∉S2≤vp(u)≤5pvp(u),k=∏p∉Svp(u)=1p.(u)=\mathfrak s\mathfrak w\mathfrak k, \quad \mathfrak s=\prod_{p\in S}p^{v_p(u)},\quad \mathfrak w=\prod_{\substack{p\notin S\\2\le v_p(u)\le5}}p^{v_p(u)}, \quad \mathfrak k=\prod_{\substack{p\notin S\\v_p(u)=1}}p.

Thus k\mathfrak k is squarefree, (k,w)=1(\mathfrak k,\mathfrak w)=1, and w\mathfrak w is powerful, meaning that each of its positive prime valuations is at least two. There are only finitely many possibilities for s\mathfrak{s}, because its valuations lie in {0,…,5}\{0,\ldots,5\} on the fixed set SS. Choose one generator sss_{\mathfrak{s}} for each of these ideals. Writing w,kw,k for the primary generators of w,k\mathfrak w,\mathfrak k, there is a unique unit υ\upsilon such that

u=υsswk.u=\upsilon s_{\mathfrak s}wk.

We fix s\mathfrak{s} and υ\upsilon whenever a row sum is taken.

Insert dyadic ranges qw≍Vq_{\mathfrak{w}} \asymp V, including the unit ideal in the bounded range V=1V=1. Only 1≤V≪AU1\le V\ll_{\mathcal A}U can occur, and there are OA(log⁡U)O_{\mathcal A}(\log U) such ranges. The original annulus qu≍Uq_u \asymp U gives the actual residual annulus

qk=quqsqw≍AUV.q_{\mathfrak k}=\frac{q_u}{q_{\mathfrak s}q_{\mathfrak w}} \asymp_{\mathcal A}\frac UV.

We keep this restriction when forming the sum. It will be enlarged to the ball qk≪AU/Vq_k\ll_{\mathcal A}U/V only when applying a positive row bound. Let UV\mathcal{U}_V denote the rows of the current witness subdivision in this powerful-part dyad, with all original physical restrictions retained.

The number of powerful ideals of norm at most VV is O(V1/2)O(V^{1/2}). Indeed, every powerful ideal has a unique expression v2y3\mathfrak v^2\mathfrak y^3 with y\mathfrak y squarefree; the two factors need not be coprime. The ideal count from the arithmetic preliminaries gives

#{w:qw≤V, w powerful}≪V1/2∑yqy−3/2≪V1/2.\#\{\mathfrak w:q_{\mathfrak w}\le V,\ \mathfrak w\ {\rm powerful}\} \ll V^{1/2}\sum_{\mathfrak y}q_{\mathfrak y}^{-3/2} \ll V^{1/2}.

The last series converges by the same ideal count. For each fixed w\mathfrak{w} in its dyad, the ball containing (9.18) has OA(U/V)O_{\mathcal A}(U/V) ideals. A nonempty annulus has U/VU/V bounded below by a fixed positive constant, which also covers the unit residual ideal. Since the factorization of (u)(u) and its unit are unique, the number of rows in this powerful-part dyad satisfies

#UV≪AUV−1/2.\#\mathcal U_V\ll_{\mathcal A}U V^{-1/2}.

Discarding any of the restrictions defining UV\mathcal{U}_V in this upper count can only add rows.

For fixed w,s,υ\mathfrak w,\mathfrak s,\upsilon, put v=υsswv=\upsilon s_{\mathfrak s}w. Multiplicativity in the numerator gives the exact identity

χn(u)ς=χn(v)ςχn(k)ς.\chi_n(u)^{\varsigma} =\chi_n(v)^{\varsigma}\chi_n(k)^{\varsigma}.

It includes the zero extensions: if nn meets either factor, both sides are zero, and otherwise it is ordinary multiplicativity. In particular, the inverse polynomial for a fixed profile WW is the row sum in Lemma 9.1 with coefficients

cn=D−1/2μ(n)ν(n)χn(v)ςW(qn/D).c_n=D^{-1/2}\mu(n)\nu(n)\chi_n(v)^{\varsigma}W(q_n/D).

The factor μ(n)\mu(n) keeps the columns squarefree. The factor χn(v)ς\chi_n(v)^{\varsigma} retains every original zero at (n,v)>1(n,v)>1 and is fixed across the residual row kk. The only remaining zero depending on both nn and kk is the zero of the displayed sieve kernel itself. The restriction (k,w)=1(k,w)=1, and any restriction inherited from the physical row set for fixed external parameters, is a fixed row restriction in this application. We do not enlarge SS to contain the primes of ww. Consequently the constant in the sieve is independent of ww, even though its fixed coefficient mask may have large norm.

The common annular support and ideal counting give, uniformly for the fixed profile parameters,

∑n∣cn∣2≤D−1∑qn≍D∣W(qn/D)∣2≪A1.\sum_n|c_n|^2 \le D^{-1}\sum_{q_n\asymp D}|W(q_n/D)|^2\ll_{\mathcal A}1.

The same statement holds for each of the finitely many profile derivatives used below, with the corresponding fixed seminorm. Apply Lemma 9.1 after enlarging the positive residual row sum from its actual annulus to qk≪AU/Vq_k\ll_{\mathcal A}U/V. A fixed enlargement makes the row bound at least one on every nonempty quotient range and includes the annular column support. Summing the result over the O(V1/2)O(V^{1/2}) choices of w\mathfrak{w} and the finitely many choices of s,υ\mathfrak s,\upsilon yields

∑u∈UV∣Mu(D;W)∣2≪A,ϵ1(UD)ϵ1V1/2{UV+D+(UDV)2/3}.\sum_{u\in\mathcal U_V}|M_u(D;W)|^2 \ll_{\mathcal A,\epsilon_1}(UD)^{\epsilon_1}V^{1/2} \left\{\frac UV+D+\left(\frac{UD}{V}\right)^{2/3}\right\}.

All coefficient sequences in this derivation are fixed within the row sum to which the sieve is applied. They may differ for different frozen values of w\mathfrak{w}, which are summed only after those positive bounds.

We now restore the rowwise choice of WuW_u in Equation (9.17). Here the detector was used with t=1t=1, so D∗=UD_\ast=U. After the presentation and dyadic pair are fixed, its inverse profiles have the form

Wdyad(x)V≤(Dx/U)x−σ−iω,ω=γ−νF,W_{\mathrm{dyad}}(x)V_{\leq}(Dx/U)x^{-\sigma-i\omega}, \qquad\omega=\gamma-\nu_F,

where WdyadW_{\mathrm{dyad}} is the fixed smooth dyadic cutoff and νF\nu_F is the Fourier frequency from the detector. The factor V≤(Dx/U)V_{\leq}(Dx/U) is common to the row sum; the varying parameters are σ∈[51/100,1]\sigma\in[51/100,1] and ∣ω∣≤(3i+1)T1|\omega|\leq(3i+1)T_1. Differentiating in either parameter inserts a power of log⁡x\log x, which is bounded on the fixed annulus. Cover these two parameter ranges by unit boxes. There are at most a fixed power of 1+T11+T_1 such boxes. The parameter Sobolev inequality in Lemma 4.5 bounds the supremum on a box by a finite sum of integrals of squared profile derivatives. Sum over the rows before these integrals. At each fixed parameter value, differentiation changes only the fixed profile coefficient, inserting the allowed logarithmic weights or profile derivatives. Equation (9.21) therefore applies to every such integral. This proves

∑u∈UV∣Mu(D;Wu)∣2≪A,ϵ1(UD)ϵ1(1+T1)AAV1/2{UV+D+(UDV)2/3}.\sum_{u\in\mathcal U_V}|M_u(D;W_u)|^2 \ll_{\mathcal A,\epsilon_1}(UD)^{\epsilon_1}(1+T_1)^{A_{\mathcal A}} V^{1/2}\left\{\frac UV+D+ \left(\frac{UD}{V}\right)^{2/3}\right\}.

The derivative order and hence AAA_{\mathcal A} are fixed before choosing τ\tau. The height intervals and the total allowance for additional frequencies are exactly those in the shared detector estimates; the Sobolev step does not assign a new frequency allowance or change a contour. It does not permit a coefficient to be selected separately for each kk.

It remains to combine this moment with the independent count Equation (9.19). Write

V=Uo,D=Ur,eo(r)=o2+max⁡{1−o,r,2(1−o+r)3}.V=U^o,\qquad D=U^r,\qquad e_o(r)=\frac{o}{2}+\max\left\{1-o,r,\frac{2(1-o+r)}{3}\right\}.

These are the parameters of the actual dyads. A nonempty dyad has 0≤o≤1+OA(1/log⁡U)0\le o\le1+O_{\mathcal A}(1/\log U); the unit dyad has o=0o=0. Since the witness lengths stay bounded, the arbitrarily small power of UDUD in Equation (9.22) can be written as an arbitrarily small power of UU. Dividing that equation by the spike in Equation (9.17), and also using Equation (9.19), gives for this subdivision

#UV≪Umin⁡{1−o/2,eo(r)−δr}+O(ϵ0)+ϵ1(1+T1)AA,\#\mathcal U_V \ll U^{\min\{1-o/2,e_o(r)-\delta r\}+O(\epsilon_0)+\epsilon_1} (1+T_1)^{A_{\mathcal A}},

after decreasing the sieve loss denoted by ϵ1\epsilon_1 if necessary.

We compute the largest exponent in this expression first on 0≤o≤10\leq o\leq1 and 1/2≤r≤11/2\leq r\leq1. Put x=1−ox=1-o and A=(1+x)/2A=(1+x)/2. Then

eo(r)−δr=max⁡{A−δr,1−x2+(1−δ)r,12+x6+(23−δ)r}.e_o(r)-\delta r=\max\left\{A-\delta r,\frac{1-x}{2}+(1-\delta)r,\frac{1}{2}+\frac{x}{6}+\left(\frac{2}{3}-\delta\right)r\right\}.

The minimum of AA with a maximum of three real numbers is the maximum of its minima with those numbers. The first such minimum is A−δr≤1−δ/2A-\delta r\leq1-\delta/2. For fixed rr, the second is the minimum of an increasing and a decreasing affine function of xx. They cross at x=(1−δ)r∈[0,1]x=(1-\delta)r\in[0,1], so its maximum over xx is

1+(1−δ)r2≤1−δ2.\frac{1+(1-\delta)r}{2}\leq1-\frac{\delta}{2}.

Both functions in the third minimum increase with xx. Its maximum over xx is therefore

min⁡{1,23+(23−δ)r}.\min\left\{1,\frac{2}{3}+\left(\frac{2}{3}-\delta\right)r\right\}.

The affine expression in rr takes the values 1−δ/21-\delta/2 and 4/3−δ4/3-\delta at the two endpoints. It follows, and equality is attained at one of those endpoints, that

max⁡0≤o≤11/2≤r≤1min⁡{1−o/2,eo(r)−δr}=min⁡{1,max⁡(1−δ2,43−δ)}.\max_{\substack{0\leq o\leq1\\1/2\leq r\leq1}}\min\{1-o/2,e_o(r)-\delta r\} =\min\left\{1,\max\left(1-\frac{\delta}{2},\frac{4}{3}-\delta\right)\right\}.

This computation is uniform for 0≤δ≤10 \le\delta\le1.

The functions just used are maxima and minima of affine functions whose slopes are uniformly bounded on a fixed neighborhood of these compact ranges. Replacing the actual oo by its nearest point in [0,1][0,1], and the actual witness rr by its nearest point in [1/2,1][1/2,1], changes the exponent by at most OA(ϵ0+1/log⁡U)O_{\mathcal A}(\epsilon_0+1/\log U), by (9.17) and the actual dyad bounds. Thus this replacement is made only in the final optimization, not in the row sum or its sieve application. Choose ϵ0\epsilon_0 and the preliminary sieve loss small enough in terms of the prescribed ϵ\epsilon. The O((log⁡U)2)O((\log U)^2) witness pairs and O(log⁡U)O(\log U) powerful-part dyads cost only another arbitrarily small power. Summing (9.23) proves (9.16).

Finally, the bin a=51/100a=51/100 need not contain an actual zero, so no use of Proposition 8.3 is made there. Counting all elements in its physical annulus gives OA(U)O_{\mathcal A}(U) rows. Since 1/50<1/31/50<1/3, the displayed formula for RR gives R(1/50)=1R(1/50)=1, as claimed.

For use in the high estimate, the row envelope has the explicit form

R(δ)={1,0≤δ≤1/3,4/3−δ,1/3≤δ≤2/3,1−δ/2,2/3≤δ≤1.R(\delta)= \begin{cases} 1, & 0\le\delta\le1/3,\\ 4/3-\delta, & 1/3\le\delta\le2/3,\\ 1-\delta/2, & 2/3\le\delta\le1. \end{cases}

The argument uses only the inverse witness. No estimate for a product with the plain witness is needed in this row count.

Analytic estimates for the high expansion

The row envelope now enters the Poisson representation of the base probe. For the first-stage application, retain the supposition Δ1=β∗−11/12>0\Delta_1=\beta_* - 11/12>0 and set X=Y=Z1/2X=Y=Z^{1/2}. Write ss for the first Mellin variable called xx in Section 7.2. Equations (7.5) and (7.13) give the actual integral to be estimated:

Iη(Z1/2,Z1/2,Z)=1(2πi)3∫(3)∫(3)∫(2)W(Z1/2,Z1/2,Z;s,w,z)⋅∑u(6)qu−zξ(u)‾ζFS(6z)LS(w,χ∙(u))LS(s,ηχ∙(u)‾)Hη,u(s,w,z) dz dw ds.\begin{aligned} I_\eta(Z^{1/2},Z^{1/2},Z) =\frac1{(2\pi i)^3}\int_{(3)}\int_{(3)}\int_{(2)} &\mathcal W(Z^{1/2},Z^{1/2},Z;s,w,z)\\ &\cdot\sum_u^{(6)}q_u^{-z}\overline{\xi(u)} \frac{\zeta_F^S(6z)L^S(w,\chi_\bullet(u))} {L^S(s,\eta\overline{\chi_\bullet(u)})} \mathcal H_{\eta,u}(s,w,z)\,dz\,dw\,ds. \end{aligned}

Here

W(X,Y,Z;s,w,z)=X1/2−zZs+z−1Yw−1e(s+z−1)2M(z)W^1(w).\mathcal W(X,Y,Z;s,w,z)=X^{1/2-z}Z^{s+z-1}Y^{w-1} e^{(s+z-1)^2}M(z)\widehat W_1(w).

The rows are the nonzero sixth-power-free elements, with their unit factors and the physical restriction (u,S)=1(u,S)=1. Both character presentations retain their original zeros at primes dividing uu. The coefficientwise calibration of the base probe is already included in this identity.

The row u=1u=1 contains the reciprocal of the target function. For the intermediate row norms we will keep one buffered bin fixed, move its integral to

ℜs=a+16e,ℜw=1−a−6e,ℜz=17/50,\Re s=a+16e,\qquad \Re w=1-a-6e,\qquad \Re z=17/50,

and apply the envelope R(2a−1)R(2a-1) there. Apart from small real losses and a fixed height factor, the numerator on this contour costs Ua−1/2U^{a-1/2} for a row norm qu≍Uq_u\asymp U; the row envelope controls how many such terms occur. We first identify the principal signal, then carry out this contour move and its concrete first-stage estimate. Principal residues and direct bounds for the outer row norms complete the comparison.

The principal row and the normalization

We identify the row whose numerator is principal. A physical row with a prime factor outside SS has nonprincipal numerator by the ramification argument in Section 8. Because the physical mask imposes (u,S)=1(u,S)=1, the remaining rows are units. If a unit u≠1u\ne1 had a sixth root in FF, that root would have valuation zero at every prime, hence would be a unit of FF; every unit of FF has sixth power one. Thus F(u1/6)/FF(u^{1/6})/F is nontrivial. It is finite Galois because FF contains the sixth roots of unity. Chebotarev applied to a nonidentity Frobenius class supplies a prime outside the fixed set SS where the associated sextic character is nontrivial [27 Theorem 1.1]. By the Kummer description in Lemma 4.1, this is χ∙(u)\chi_{\bullet}(u). Therefore u=1u=1 is the sole principal numerator row. A denominator attached to a bounded unit row may be principal; its reciprocal has a zero at one and will be kept on a global line below.

Define

Hη(s)=Hη,1(s,1,1/6),cS=W^1(1)M(1/6)(Res⁡v=1ζFS(v))2/6.H_\eta(s)=\mathcal H_{\eta,1}(s,1,1/6),\qquad c_S=\widehat W_1(1)M(1/6) \left(\operatorname*{Res}_{v=1}\zeta_F^S(v)\right)^2/6.

Lemma 7.1 makes HηH_\eta holomorphic on ℜs>7/8\Re s>7/8. Its uniform estimate Hη=1+O(P0−4/5)H_\eta=1+O(P_0^{-4/5}) permits a choice of P0P_0 before the target, because the local bound is uniform in the target unit phases. Fix P0P_0 large enough that

sup⁡ℜs>7/8∣Hη(s)−1∣≤12.\sup_{\Re s>7/8}|H_\eta(s)-1|\le\frac{1}{2}.

Enlarging SS by these primes leaves the fixed ray group TT unchanged, as the calibration in the local identity holds coefficientwise. The excluded set and hence the particular function HηH_\eta may differ between applications, but within one application they are exactly those of the exact high representation being used.

The constant cSc_S is positive. Indeed W^1(1)>0\widehat W_1(1)>0 because W1W_1 is nonnegative and nonzero, and M(1/6)>0M(1/6)>0 by (7.2). The simple pole of ζFS\zeta_F^S has positive residue: deletion multiplies the positive residue of ζF\zeta_F by ∏p∈S(1−qp−1)>0\prod_{p\in S}(1-q_p^{-1})>0.

For the first stage put

CI(s)=s−23,JI,η(Z)=Iη(Z1/2,Z1/2,Z)cS.C_{\mathrm I}(s)=s-\frac23,\qquad J_{\mathrm I,\eta}(Z)=\frac{I_\eta(Z^{1/2},Z^{1/2},Z)}{c_S}.

Let fI,ηf_{\mathrm I,\eta} be the integral in (2.3) with C=CIC=C_{\mathrm I}, S=S\mathcal S=S, and the function HηH_\eta just defined. The two scalar poles at w=1w=1 and z=1/6z=1/6 will give cSfI,ηc_S f_{\mathrm I,\eta}; our remaining objective is a common power saving for every other term, measured relative to ZCI(β∗)Z^{C_{\mathrm I}(\beta_*)}.

The exact identity used in contour moves

The contour proof uses the full holomorphic correction in the displayed integral. To reuse that proof with the compensated probe, we record the identity and bounds that it requires. In the present application the correction is Hη,u\mathcal H_{\eta,u}, independent of ZZ, and the parameters below are lx=ly=h=1/2l_x=l_y=h=1/2 and ℓ=0\ell=0.

The scalar quotient in (7.13) is the part of the high expansion that determines both the contour move and the principal residues. We keep that quotient fixed and state explicitly what may be changed around it. Put

D1(ϵ0)={(s,w,z):ℜs≥51/100,ℜz≥17/50,ℜw≥−1/100,ℜ(s+w)≥1+ϵ0},ϵ0>0,\begin{aligned} \mathcal D_1(\epsilon_0)=\{(s,w,z):{}\Re s\ge51/100,\quad \Re z\ge17/50,\quad \Re w\ge-1/100,\\ \Re(s+w)\ge1+\epsilon_0\},\qquad \epsilon_0>0,\end{aligned}
D2={(s,w,z):ℜs≥7/8,ℜz≥33/200,ℜw≥19/20}.\mathcal D_2=\{(s,w,z):{}\Re s\ge7/8,\quad \Re z\ge33/200,\quad \Re w\ge19/20\}.

These are the two regions in Lemma 7.1. A real box below means a compact rectangular subset of R3\mathbb{R}^3 for (ℜs,ℜw,ℜz)(\Re s,\Re w,\Re z).

Definition 10.1 (Data for an exact high representation). Fix real numbers lx,ly>0l_x,l_y>0 and ℓ≥0\ell\geq0 such that

X=Zlx,Y=Zly,h=1−lx+ℓ>0,C(s)=s+lx2−1+h6=s−56+lx3+ℓ6.X=Z^{l_x},\qquad Y=Z^{l_y},\qquad h=1-l_x+\ell>0,\qquad C(s)=s+\frac{l_x}{2}-1+\frac{h}{6}=s-\frac{5}{6}+\frac{l_x}{3}+\frac{\ell}{6}.

These real numbers are fixed before the target character. For each primitive finite-order target η\eta, fix the data S,ξ,W0,W1S,\xi,W_0,W_1 of Section 6, independently of ZZ. Data for an exact high representation consist of the following objects and assertions.

First, Iη(Z)\mathscr I_\eta(Z) is an independently specified complex-valued quantity for every sufficiently large real ZZ. In each application it is given by a finite linear combination, for that ZZ, of the completed sums in Equation (6.1), allowing specified restrictions on the completed index AA and specified rescalings of its three positive scales. The number of terms and coefficients in this finite combination may depend on ZZ. Any direct estimate for Iη\mathscr I_\eta refers to this expression, not to a separately defined high integral.

Second, for every nonzero sixth-power-free element uu with (u,S)=1(u,S)=1 and every such ZZ, there is a function Hη,u,Z(s,w,z)\mathfrak H_{\eta,u,Z}(s,w,z). It is holomorphic on a neighborhood of each point of D2\mathcal{D}_2 and of every D1(ϵ0)\mathcal{D}_1(\epsilon_0). For every D>0D>0 and every real box K\mathcal{K} contained in one of these regions, there are finite constants Bη,K,DB_{\eta,\mathcal{K},D} and Jη,K,DJ_{\eta,\mathcal{K},D} such that, uniformly for 1≤qu≤ZD1\leq q_u\leq Z^D, all imaginary parts, and real parts in K\mathcal{K},

∣Hη,u,Z(s,w,z)∣≪η,K,DZBη,K,D(1+∣ℑs∣+∣ℑw∣+∣ℑz∣)Jη,K,D.|\mathfrak H_{\eta,u,Z}(s,w,z)| \ll_{\eta,\mathcal K,D} Z^{B_{\eta,\mathcal K,D}} (1+|\Im s|+|\Im w|+|\Im z|)^{J_{\eta,\mathcal K,D}}.

The constants and exponents are independent of ZZ, uu and of any later order of integration by parts. No nonvanishing of H\mathfrak H or of any of its local factors is assumed.

Finally, the following identity is asserted for the independently given Iη(Z)\mathscr I_\eta(Z), with absolute convergence of the sum and integrals on the displayed lines:

Iη(Z)=1(2πi)3∫(3)∫(3)∫(2)W(X,Y,Z;s,w,z)∑u(6)qu−zξ(u)‾⋅ζFS(6z)LS(w,χ∙(u))LS(s,ηχ∙(u)‾)Hη,u,Z(s,w,z) dz dw ds,\begin{aligned} \mathscr I_\eta(Z)=\frac1{(2\pi i)^3} \int_{(3)}\int_{(3)}\int_{(2)} &\mathcal W(X,Y,Z;s,w,z) \sum_u^{(6)}q_u^{-z}\overline{\xi(u)}\\ &\cdot \frac{\zeta_F^S(6z)L^S(w,\chi_\bullet(u))} {L^S(s,\eta\overline{\chi_\bullet(u)})} \mathfrak H_{\eta,u,Z}(s,w,z)\,dz\,dw\,ds, \end{aligned}

where the sum has the physical restrictions of Equation (7.5), and

W(X,Y,Z;s,w,z)=X1/2−zZs+z−1Yw−1e(s+z−1)2M(z)W^1(w).\mathcal W(X,Y,Z;s,w,z) =X^{1/2-z}Z^{s+z-1}Y^{w-1} e^{(s+z-1)^2}M(z)\widehat W_1(w).

Thus Equation (10.5) is a hypothesis to be proved for the physical expression, not its definition.

For the base probe, the physical expression is Iη(Zlx,Zly,Z)I_\eta(Z^{l_x},Z^{l_y},Z), ℓ=0\ell=0, and Hη,u,Z=Hη,u\mathfrak H_{\eta,u,Z}=\mathcal H_{\eta,u}. Equations (7.5) and (7.13) prove the required identity, and Lemma 7.1 gives the holomorphy and Equation (10.4). More generally, the function H\mathfrak H in the definition always means the full correction after the displayed scalar quotient is removed. If that correction is a sum of products of local factors, the products themselves must be holomorphic in the stated regions. Writing a quotient by an individual local factor at its zeros does not establish this condition. The decompositions used only to estimate a retained contour will be stated separately below.

External tails on vertical lines and horizontal joins

The product of our three Mellin tests decays in three independent height directions. The following estimate turns that decay into bounds both off a large box and on the horizontal sides of a contour rectangle.

Lemma 10.2 (External integrated and trace tails). Let m≥2m \ge2, let K\mathcal{K} be a compact set of real contour parameters, and, for r∈K\boldsymbol r\in\mathcal K and Z≥2Z \ge2, let Kr,ZK_{\boldsymbol r,Z} be a nonnegative Borel measurable kernel on Rm\mathbb{R}^{m}. Suppose it is jointly Borel measurable in (r,t)(\boldsymbol r,\boldsymbol t) and, for every integer L≥0L \ge0,

Kr,Z(t)≪L(1+∣t∣)−LK_{\boldsymbol r,Z}(\boldsymbol t) \ll_L(1+|\boldsymbol t|)^{-L}

uniformly in r\boldsymbol r, ZZ, t\boldsymbol t. Let D⊆Rm\mathcal D\subseteq\mathbb R^m be Borel measurable, and suppose a Borel measurable factor FZF_Z satisfies on D\mathcal D

∣FZ(t)∣≤CZB(1+∣t∣)J,|F_Z(\boldsymbol t)|\le C Z^B(1+|\boldsymbol t|)^J,

where B,J,CB,J,C are fixed independently of ZZ and of the integer NN below. Write t^j\widehat{\boldsymbol t}_j for the vector obtained by omitting the jjth coordinate of t\boldsymbol t. Uniformly for T≥1T \ge1 and r∈K\boldsymbol r\in\mathcal K,

∫D∩{max⁡j∣tj∣>T}Kr,Z(t)∣FZ(t)∣ dt≪NZBT−N,\int_{\mathcal D\cap\{\max_j|t_j|>T\}} K_{\boldsymbol r,Z}(\boldsymbol t)|F_Z(\boldsymbol t)|\,d\boldsymbol t \ll_N Z^B T^{-N},
∫D∩{tj=T}Kr,Z(t)∣FZ(t)∣ dt^j≪NZB(1+∣T∣)−N.\int_{\mathcal D\cap\{t_j=T\}} K_{\boldsymbol r,Z}(\boldsymbol t)|F_Z(\boldsymbol t)|\, d\widehat{\boldsymbol t}_j \ll_N Z^B(1+|T|)^{-N}.

The second assertion holds for either sign of TT and every jj, using coordinate Lebesgue measure on tj=Tt_j=T. Both assertions remain valid after integration over a real contour interval of bounded length when the hypotheses are uniform there and the kernels, domain indicators and arithmetic factors are jointly Borel measurable in that real parameter and the remaining coordinates.

Proof. Multiply the kernel bound by (10.6). Integrating (1+∣t∣)J−L(1+|\boldsymbol t|)^{J-L} outside the box proves (10.7) when L>N+J+mL>N+J+m. On tj=Tt_j=T, integration in the other m−1m-1 coordinates gives

∫Rm−1(1+∣T∣+∣t^j∣)J−Ldt^j≪(1+∣T∣)J−L+m−1.\int_{\mathbb R^{m-1}} (1+|T|+|\widehat{\boldsymbol t}_j|)^{J-L} d\widehat{\boldsymbol t}_j \ll(1+|T|)^{J-L+m-1}.

Taking L>N+J+m−1L>N+J+m-1 proves (10.8). Restricting to D\mathcal D decreases these positive integrals, and a bounded real interval contributes only its length.

For our triple integral, take

(y1,y2,y3)=(ℑ(s+z),ℑz,ℑw),Kr,Z(t)=e−y12∣M(rz+iy2)∣ ∣W^1(rw+iy3)∣.(y_1,y_2,y_3)=(\Im(s+z),\Im z,\Im w),\qquad K_{\boldsymbol r,Z}(\boldsymbol t) =e^{-y_1^2}|M(r_z+iy_2)|\,|\widehat W_1(r_w+iy_3)|.

The change of height variables has determinant one. On a fixed real box with rzr_z in a compact subinterval of (0,∞)(0,\infty), the Mellin estimates of Section 7 give arbitrary polynomial decay of MM and W^1\widehat{W}_1. The Gaussian has the same property. Their product is therefore OL((1+∣y∣)−L)O_L((1+|\boldsymbol y|)^{-L}) for every LL, hence also OL((1+∣t∣)−L)O_L((1+|\boldsymbol t|)^{-L}). The omitted factor e(ℜ(s+z)−1)2e^{(\Re(s+z)-1)^2} is bounded on that real box.

After the ww residue only s,zs,z remain. The same proof applies to the kernel

Kr,Z(2)(t)=e−y12∣M(rz+iy2)∣,(y1,y2)=(ℑ(s+z),ℑz).K^{(2)}_{\boldsymbol r,Z}(\boldsymbol t) =e^{-y_1^2}|M(r_z+iy_2)|, \qquad(y_1,y_2)=(\Im(s+z),\Im z).

This supplies the trace bound needed for the subsequent zz-join.

The same kernel test handles additional external separating variables. For m≥3m \ge3, let y=At\boldsymbol y=A\boldsymbol t with a fixed A∈GL⁡m(R)A\in\operatorname{GL}_m(\mathbb{R}), and multiply the three-factor kernel by a Borel density ∣vr,Z(y4,…,ym)∣|v_{\boldsymbol r,Z}(y_4,\ldots,y_m)|, jointly Borel in (r,v)(\boldsymbol r,\boldsymbol v), satisfying

sup⁡r,Z,v(1+∣v∣)L∣vr,Z(v)∣<∞for every integer L≥0.\sup_{\boldsymbol r,Z,\boldsymbol v} (1+|\boldsymbol v|)^L|v_{\boldsymbol r,Z}(\boldsymbol v)|<\infty \quad\text{for every integer }L\ge0.

For m=3m=3 the density is one on the zero-dimensional space. The product is again rapidly decreasing in all mm coordinates, since AA and its inverse are fixed. For the two-factor kernel, the identical argument uses a density on Rm−2\mathbb{R}^{m-2} and m≥2m\ge2, with density one when m=2m=2. Thus both product-kernel forms have the integrated and trace bounds above.

Uniform annular profiles separated by logarithmic Fourier inversion satisfy (10.10) by repeated integration by parts, as in Lemma 4.5. Translate every pure norm twist into its Mellin argument first. The additional height coordinates then append a block triangular matrix with fixed inverse to the three-dimensional change of variables.

An internal coefficient measure known only through a fixed weighted L1L^1 norm is not thereby covered by the pointwise density hypothesis or by its trace conclusion. Such a measure remains integrated at its already fixed moment order inside the factor FZF_Z. Any additional external coordinate on which a trace estimate is used must separately satisfy (10.10).

The domain D\mathcal{D} in the lemma is important. Suppose a reciprocal is bounded only while the imaginary part of its argument γ+∑jajtj\gamma+\sum_j a_jt_j lies in a buffered interval. A coordinate with aj≠0a_j\ne0 may be integrated only over the range that preserves this condition; the lemma does not extend the reciprocal bound beyond it. Coordinates with aj=0a_j=0 may be extended when the other factors satisfy (10.6) there. All factors on an extended axis must use their global or absolute estimates, not an estimate valid only on a retained interval. In particular, an integrated tail alone does not justify a horizontal join: that join uses (10.8).

Increasing NN in this lemma increases only the decay orders of the external smooth tests. It does not differentiate FZF_Z. Thus a fixed moment-profile order or a fixed arithmetic height exponent in FZF_Z is unchanged when NN is chosen later. This is the same order distinction made in Lemma 4.5.

Moving a fixed bin

We first move the full row integral. The row envelope will be applied only after this step, on the retained contour.

Lemma 10.3 (Contour transformation for a fixed bin). Assume Definition 10.1. Fix σ0∈[7/8,1)\sigma_0\in[7/8,1) with β∗>σ0\beta_*> \sigma_0, put z0=17/50z_0=17/50, and let U=ZdU=Z^d with 0<dmin⁡≤d≤dmax⁡<∞0<d_{\min}\le d\le d_{\max}<\infty. Let B\mathcal{B} be a finite set of retained physical rows qu≍Uq_u\asymp U in one bin (i,a)(i,a) of Lemma 8.1, fixed before any Mellin variable is moved. The comparison constants in this annulus are fixed. Take 0<e<10−30<e<10^{-3} and T1=Zτ>2T_1=Z^\tau>2, where 0<τ≤dmin⁡/1000<\tau\le d_{\min}/100. The real ranges and ee are independent of the target.

Fix positive constants cs,cw,cz≤1/2c_s,c_w,c_z\le1/2, independently of ZZ and the rows. Retain the original heights ∣ℑs∣≤csT1|\Im s|\le c_sT_1, ∣ℑw∣≤cwT1|\Im w|\le c_wT_1 and ∣ℑz∣≤czT1|\Im z|\le c_zT_1. The contribution of B\mathcal{B} on the starting lines in (10.5) equals its integral on these retained segments of

ℜs=a+16e,ℜw=1−a−6e,ℜz=z0,\Re s=a+16e,\qquad\Re w=1-a-6e,\qquad\Re z=z_0,

up to Oη,N(ZBηT1−N)O_{\eta,N}(Z^{B_\eta}T_1^{-N}) for every fixed NN. The finite exponent BηB_\eta is fixed before NN. An empty row set contributes zero. The transformation uses the full holomorphic correction; no decomposition of that correction or subdivision depending on a contour point is needed.

Proof. Section 8 gives a≤β∗a\le\beta_*, including the floor bin. Isolate the finite sum over B\mathcal{B} on the absolute lines in (10.5). Move zz from 2 to z0z_0, keep w=3w=3, and move ss from 3 to β∗+20e\beta_*+20e. These moves stay in D1(ϵ0)\mathcal{D}_1(\epsilon_0) for a fixed positive ϵ0\epsilon_0, the two numerator arguments remain to the right of their poles, and the reciprocal stays in ℜs>β∗\Re s>\beta_*. Its global bound follows from Lemmas 4.9 and 4.10, using the conductor and deletion radical bounds in Section 8. The correction obeys (10.4). Lemma 10.2 with T→∞T\to\infty therefore justifies these moves.

Now move ww from 3 to 1−a−6e1-a-6e while ss stays on that global line. Throughout the move,

ℜ(s+w)≥1+(β∗−a)+14e≥1+14e.\Re(s+w)\ge1+(\beta_*-a)+14e\ge1+14e.

The numerator character of every retained row is nonprincipal, so its LL-function is entire. Also ℜw≥−6e>−1/100\Re w\ge-6e>-1/100 and ℜz=z0\Re z=z_0. Thus the correction remains holomorphic in D1(ϵ0)\mathcal{D}_1(\epsilon_0), for example with ϵ0=10e\epsilon_0=10e, and no pole is crossed. On a ww-join the reciprocal is still global. The global upper strip bound for the numerator, the deleted-factor bound and (10.4) give a majorant of the form (10.6) on the axes integrated there. The trace estimate makes the joins tend to zero.

Before moving ss farther, restrict the three original Mellin heights to the stated box. On the discarded part keep ss on ℜs=β∗+20e\Re s=\beta_*+20e. There the global reciprocal bound, the global numerator bound, the deleted factors and the all-height correction bound give ZBηZ^{B_\eta} times a fixed polynomial in the heights: the row range is bounded by qu≪Zdmax⁡q_u\ll Z^{d_{\max}}, and the number of rows is O(U)O(U). The integrated tail in Lemma 10.2 gives Oη,N(ZBηT1−N)O_{\eta,N}(Z^{B_\eta}T_1^{-N}).

Move only the retained ss segment to a+16ea+16e. On this rectangle,

ℜ(s+w)≥1+10e,\Re(s+w)\ge1+10e,

and the other inequalities defining D1(10e)\mathcal D_1(10e) still hold. The real part of the reciprocal argument is at least a+16e>a+6ea+16e>a+6e. The stated height box places both scalar arguments strictly inside ∣ℑv∣≤(3i+2)T1|\Im v|\le(3i+2)T_1 for sufficiently large ZZ. Lemma 8.1 therefore excludes its zeros throughout the retained rectangle. Since 6z0>16z_0>1, the scalar zeta factor has no pole on this move. Thus no pole is crossed.

For an ss-join, its imaginary coordinate is fixed at a constant multiple of T1T_1. The scalar denominator in (10.5) depends only on ss, so its buffered estimate remains valid when the ℑz\Im z and ℑw\Im w integrations are extended to their whole axes. On those extended axes use the global numerator estimate and (10.4). The trace estimate then gives Oη,N(ZBηT1−N)O_{\eta,N}(Z^{B_\eta}T_1^{-N}). No ww- or zz-join in this argument extends an ss-axis that has been moved into a merely buffered region.

The exact high representation is a triple integral with a majorant for its full correction. We can therefore perform this transformation before introducing any auxiliary separating variable. If a central estimate later uses such variables, their retained domains and discarded parts must be justified in that estimate; they are not new coordinates of the contour identity just proved.

Applying the row envelope

For the base correction, Lemma 7.1 verifies the hypotheses of Lemma 10.3. Indeed ∣Hη,u∣≪ϵquϵ|\mathcal{H}_{\eta,u}|\ll_\epsilon q_u^\epsilon uniformly in all three heights in both Euler regions; for qu≤ZDq_u\le Z^D, taking ϵ=1\epsilon=1 gives (10.4) with B=DB=D and height order zero. We now estimate the retained integral, using lx=ly=h=1/2l_x=l_y=h=1/2 and ℓ=0\ell=0 throughout this subsection.

Fix

dmin⁡=163,ζ=11000,dmax⁡=h+ζ=5011000.d_{\min}=\frac{1}{63},\qquad\zeta=\frac{1}{1000},\qquad d_{\max}=h+\zeta=\frac{501}{1000}.

For a dyad U=ZdU=Z^d in this range, fix one dynamic bin (i,a)(i,a) before moving any Mellin variable, and put δ=2a−1\delta=2a-1. Proposition 9.2, with requested loss ϵr>0\epsilon_r>0, gives its cardinality at most UR(δ)+ϵr(1+T1)AηU^{R(\delta)+\epsilon_r}(1+T_1)^{A_\eta} up to a fixed constant. For the floor this is the direct count Oη(U)O_\eta(U), since R(1/50)=1R(1/50)=1; it uses no witness.

The numerator LS(w,χ∙(u))L^S(w,\chi_\bullet(u)) is precisely the original zero-extended presentation with ν=1\nu=1 in Section 8. On the retained line ℜw=1−a−6e\Re w=1-a-6e, Lemma 8.1 bounds it by Uδ/2+12e+ϵn(3+T1)CU^{\delta/2+12e+\epsilon_n}(3+T_1)^C for any ϵn>0\epsilon_n>0. This also holds in the floor bin. The central point lies in D1(10e)\mathcal D_1(10e), so the stronger local estimate in Lemma 7.1 gives ∣Hη,u∣≪e,ϵHUϵH|\mathcal H_{\eta,u}|\ll_{e,\epsilon_H}U^{\epsilon_H} there, for any ϵH>0\epsilon_H>0. Consequently

∑u∈B∣LS(w,χ∙(u))Hη,u(s,w,z)∣≪ηUR(δ)+δ/2+12e+ϵr+ϵn+ϵH(1+T1)Aη′.\sum_{u\in\mathcal B} |L^S(w,\chi_\bullet(u))\mathcal H_{\eta,u}(s,w,z)| \ll_\eta U^{R(\delta)+\delta/2+12e+\epsilon_r+\epsilon_n+\epsilon_H} (1+T_1)^{A'_\eta}.

Here Aη′A'_\eta is finite and is fixed before the final external tail order.

Put εc=12e+ϵr+ϵn+ϵH\varepsilon_c=12e+\epsilon_r+\epsilon_n+\epsilon_H. The buffered reciprocal costs UϵdU^{\epsilon_d} for any ϵd>0\epsilon_d>0, and ζFS(6z0)\zeta_F^S(6z_0) is absolutely bounded. The tests have bounded joint L1L^1 norm in the three independent height coordinates above. The outside powers, including qu−z0q_u^{-z_0}, are

Za/2−3/4+z0/2+13eU−z0.Z^{a/2-3/4+z_0/2+13e}U^{-z_0}.

Multiplying these bounds gives, for every ϵp>0\epsilon_p>0, a retained bin contribution at most

≪ηZ1/4+EI(d)+13e+(1+d)εc+dεd+εp(1+T1)Aη′.\ll_\eta Z^{1/4+E_{\mathrm I}(d)+13e +(1+d)\varepsilon_c+d\varepsilon_d+\varepsilon_p} (1+T_1)^{A'_\eta}.

Here we have harmlessly enlarged the bound by Zϵc+ϵpZ^{\epsilon_c+\epsilon_p} so that the losses use the same form as the later general estimate, and

EI(d)=−34+δ+R(δ)2+(d−12)(R(δ)+δ2−1750).E_{\mathrm I}(d)=-\frac34+\frac{\delta+R(\delta)}2 +\left(d-\frac12\right) \left(R(\delta)+\frac\delta2-\frac{17}{50}\right).

There is no additional Mellin integral in this application. Its scalar buffered arguments have heights ℑs\Im s and ℑw\Im w. The witness frequencies and profile choices in the row count stay within the detector’s existing allowance and do not enter either scalar argument.

At d=h=1/2d=h=1/2, the three pieces of the row envelope give, respectively,

EI(h)={−1/4+δ/2,0≤δ≤1/3,−1/12,1/3≤δ≤2/3,−(1−δ)/4,2/3≤δ≤1.E_{\mathrm I}(h)= \begin{cases} -1/4+\delta/2,&0\le\delta\le1/3,\\ -1/12,&1/3\le\delta\le2/3,\\ -(1-\delta)/4,&2/3\le\delta\le1. \end{cases}

The first two pieces are at most −1/12-1/12. In the third, the exact bin ceiling from Section 8 is

δ≤2β∗−1=56+2Δ1.\delta\leq2\beta_* -1=\frac{5}{6}+2\Delta_1.

It follows in every piece that

EI(h)−Δ1≤−124−Δ12.E_{\mathrm I}(h)-\Delta_1 \le-\frac1{24}-\frac{\Delta_1}{2}.

This is the comparison with CI(β∗)C_{\mathrm I}(\beta_*) required here; EI(h)E_{\mathrm I}(h) itself need not be negative. The frequency slope has the three forms

R(δ)+δ2−1750={33/50+δ/2,0≤δ≤1/3,149/150−δ/2,1/3≤δ≤2/3,33/50,2/3≤δ≤1.R(\delta)+\frac{\delta}{2}-\frac{17}{50}= \begin{cases} 33/50+\delta/2, & 0\leq\delta\leq1/3,\\ 149/150-\delta/2, & 1/3\leq\delta\leq2/3,\\ 33/50, & 2/3\leq\delta\leq1. \end{cases}

It therefore lies in [33/50,62/75][33/50,62/75]. Positivity controls all d≤hd\leq h, and the extension to d≤h+ζd\leq h+\zeta costs at most (62/75)ζ(62/75)\zeta. Thus, before adjustable losses, every central dyad has saving at least

mc=124−6275ζ=102125000m_c=\frac{1}{24}-\frac{62}{75}\zeta=\frac{1021}{25000}

relative to CI(β∗)C_{\mathrm I}(\beta_*).

Central estimates for a correction split into pieces

The preceding calculation multiplied one aggregate absolute row bound by the outside Mellin powers. We record its form when the full correction is estimated by several pieces and the available bound varies between sets of rows. The contour has already been justified for the fixed bin; these sets will be used only to estimate its retained integrand.

Lemma 10.4 (A retained integral and its exponent). Assume the data of Definition 10.1. Fix σ0∈[7/8,1)\sigma_0 \in[7/8,1) with β∗>σ0\beta_* > \sigma_0, and put z0=17/50z_0=17/50. Let 0<dmin⁡<dmax⁡<∞0<d_{\min}<d_{\max}<\infty, U=ZdU=Z^d with dmin⁡≤d≤dmax⁡d_{\min}\le d\le d_{\max}, and let B\mathcal{B} be a finite set of physical rows uu with qu≍Uq_u\asymp U in one retained bin (i,a)(i,a) of Lemma 8.1. The comparison constants in qu≍Uq_u\asymp U are fixed. Put δ=2a−1\delta=2a-1, take 0<e<10−30<e<10^{-3} as in that lemma, and let T1=Zτ>2T_1=Z^\tau>2 with 0<τ≤dmin⁡/1000<\tau\le d_{\min}/100. The real ranges and ee are chosen independently of the target.

The bin B\mathcal{B} is fixed before any Mellin variable is moved. On the retained central contours of Equation (10.11), suppose that there is a decomposition

Hη,u,Z(s,w,z)=∑λ∈ΛHη,u,Z(λ)(s,w,z),\mathfrak H_{\eta,u,Z}(s,w,z) =\sum_{\lambda\in\Lambda} \mathfrak H^{(\lambda)}_{\eta,u,Z}(s,w,z),

where Λ\Lambda is finite, nonempty and fixed before ZZ. This equality is required only on the retained contours; the summands need not be holomorphic away from them. For each λ\lambda and each retained (s,w,z)(s,w,z), suppose B\mathcal{B} is partitioned into at most C(1+log⁡Z)DC(1+\log Z)^D sets Bλ,ν(s,w,z)\mathcal{B}_{\lambda,\nu}(s,w,z), with fixed C,DC,D. For each set at each retained point let R,gR,g be real numbers in a fixed bounded range. Assume that, for fixed ϵc≥0\epsilon_c\ge0 and a finite Aη≥0A_\eta\ge0,

∑u∈Bλ,ν(s,w,z)∣LS(w,χ∙(u))Hη,u,Z(λ)(s,w,z)∣≪ηUR+δ/2+εcZℓ(z0−1/2)+g+εc(1+T1)Aη.\sum_{u\in\mathcal B_{\lambda,\nu}(s,w,z)} \left|L^S(w,\chi_\bullet(u)) \mathfrak H^{(\lambda)}_{\eta,u,Z}(s,w,z)\right| \ll_\eta U^{R+\delta/2+\varepsilon_c} Z^{\ell(z_0-1/2)+g+\varepsilon_c}(1+T_1)^{A_\eta}.

The bound is uniform in the retained point, row set and moving labels. The number ϵc\epsilon_c and the bounded range for R,gR,g are fixed before the target; R,gR,g may depend on d,ad,a, the pointwise set and the global number β∗\beta_*, but not otherwise on η\eta. Let PZ\mathcal P_Z be the set of all pairs (R,g)(R,g) that occur at any retained point in this decomposition.

Here “retained” has the following precise height meaning. List once all external coordinates v1,…,vmv_1,\ldots,v_m that enter a buffered LL-value, reciprocal, or logarithmic derivative in the verification of Equation (10.13), and include all three original Mellin heights, with zero coefficients when they do not occur in an argument. After pure-twist translations, every such argument has imaginary part γj+∑k=1majkvk\gamma_j+\sum_{k=1}^m a_{jk}v_k, where the finite matrix (ajk)(a_{jk}) is fixed and ∣γj∣≤(3i+1)T1|\gamma_j|\le(3i+1)T_1. Restrict

∣vk∣≤ckT1,ck=12m(1+max⁡j∣ajk∣).|v_k|\le c_kT_1,\qquad c_k=\frac{1}{2m(1+\max_j|a_{jk}|)}.

Coordinates with zero coefficients may be restricted by the same rule. Then every added height is at most T1/2T_1/2 in total. Fixed bounded enlargements are included by increasing the lower threshold for ZZ. If extra Mellin integrals are used to establish Equation (10.13), that inequality is required for its full left side after those integrations. Any discarded parts must have been left on their global or absolute lines, bounded by Lemma 10.2 or Lemma 4.5, and included in the displayed bound before the hypothesis is asserted. The allowance T1/2T_1/2 is not renewed at successive estimates.

The common ideal exponent associated with a pair (R,g)(R,g) is

Eσ0(d;R,g)=a−σ0+h(z0−1/6)−aly−ℓ/2+g+d(R+δ/2−z0).E_{\sigma_0}(d;R,g)=a-\sigma_0+h(z_0-1/6)-a l_y-\ell/2+g +d(R+\delta/2-z_0).

If B\mathcal{B} is empty its contribution is zero. Otherwise put

Eσ0,Zmax⁡(d)=sup⁡(R,g)∈PZEσ0(d;R,g).E^{\max}_{\sigma_0,Z}(d) =\sup_{(R,g)\in\mathcal P_Z}E_{\sigma_0}(d;R,g).

For every ϵd,ϵp>0\epsilon_d,\epsilon_p>0, the total contribution of B\mathcal{B} on the central contours is, for sufficiently large ZZ,

≪ηZC(σ0)+Eσ0,Zmax⁡(d)+(16−6ly)e⋅Z(1+d)εc+dεd+εp(1+T1)Aη.\begin{aligned} \ll_\eta{}& Z^{C(\sigma_0)+E^{\max}_{\sigma_0,Z}(d)+(16-6l_y)e}\\ &\cdot Z^{(1+d)\varepsilon_c+d\varepsilon_d+\varepsilon_p} (1+T_1)^{A_\eta}. \end{aligned}

The supremum is finite because the pairs lie in a fixed bounded range. The power εp\varepsilon_p absorbs the pointwise logarithmic multiplicity. No separate integral for a pointwise piece or row set is asserted. All discarded portions and horizontal joins in this contour move are Oη,N(ZBηT1−N)O_{\eta,N}(Z^{B_\eta}T_1^{-N}) for every fixed NN, where BηB_\eta is finite and is fixed before NN.

Proof. Apply Lemma 10.3 to the original triple integral, using for its three box constants the corresponding ckc_k in (10.14). These constants are positive and at most 1/21/2. The full correction and the fixed bin therefore give the retained integral and the asserted errors before any pointwise pieces are introduced. Any auxiliary integrations used for the central bound are subject to the additional hypotheses in the statement.

Now use the central decomposition and form the pointwise sets Bλ,ν\mathcal{B}_{\lambda,\nu}. At each retained point apply the triangle inequality to the original row sum, and then apply (10.13) to the sets present at that point. There are at most a fixed multiple of (1+log⁡Z)D(1+\log Z)^D such sets pointwise. Bound each of their exponents by the supremum over PZ\mathcal{P}_Z and integrate only the original holomorphic row sum. Thus neither measurability of an individual pointwise subdivision nor one common label set across contour points is needed. On the retained contours, Lemma 8.1 bounds the reciprocal by Oη,e,εd(Uεd)O_{\eta,e,\varepsilon_d}(U^{\varepsilon_d}). The tests have a uniformly bounded joint L1L^1 norm, since the transformation (ℑs,ℑz,ℑw)↦(ℑ(s+z),ℑz,ℑw)(\Im s,\Im z,\Im w)\mapsto(\Im(s+z),\Im z,\Im w) is invertible. The scalar factor ζFS(6z0)\zeta_F^S(6z_0) is absolutely bounded. It remains to compute the real power of ZZ.

The outside factor, including qu−z0q_u^{-z_0} and the real displacements in (10.11), contributes

lx(1/2−z0)+a+z0−1−aly−dz0+(16−6ly)e.l_x(1/2-z_0)+a+z_0-1-a l_y-dz_0+(16-6l_y)e.

(10.13) adds d(R+δ/2+εc)+ℓ(z0−1/2)+g+εcd(R+\delta/2+\varepsilon_c)+\ell(z_0-1/2)+g+\varepsilon_c. The reciprocal adds dεdd\varepsilon_d. Subtracting C(σ0)=σ0+lx/2−1+h/6C(\sigma_0)=\sigma_0+l_x/2-1+h/6 and using h=1−lx+ℓh=1-l_x+\ell gives (10.15) and the remaining terms in (10.16). The pointwise logarithmic multiplicity is bounded by ZεpZ^{\varepsilon_p} for sufficiently large ZZ. This proves the claim. □

The lemma separates two uses of the correction. Its holomorphy and all-height majorant justify the contour move before the rows are subdivided by their pointwise sizes. The pieces in (10.13) are used only after the move; they may be defined using local divisions whose nonvanishing has been proved on that retained region. Such a division supplies no continuation or tail bound outside that region. For the base correction there is only one piece, and Lemma 8.1 supplies the reflected numerator factor Uδ/2+12e+ϵU^{\delta/2+12e+\epsilon} appearing in the central hypothesis.

Extracting the principal signal

The intermediate-row estimate leaves the principal row and the two outer norm ranges. We first cross the two scalar poles in the principal row. The following formulation also records the precise condition under which a different correction has the same target signal.

Lemma 10.5 (Extraction of the principal signal). Assume Definition 10.1 and (10.2). Fix σ0∈[7/8,1)\sigma_0\in[7/8,1) with β∗>σ0\beta_*>\sigma_0 and 0<e<10−30<e<10^{-3}. Suppose that for every ε>0\varepsilon>0, uniformly in all imaginary parts on

ℜs=β∗+e,19/20≤ℜw≤1+e,33/200≤ℜz≤1/6+e,\Re s=\beta_*+e,\qquad 19/20\le\Re w\le1+e, \qquad 33/200\le\Re z\le1/6+e,

one has

∣Hη,1,Z(s,w,z)∣≪η,e,ϵZℓℜz+ϵ(1+∣ℑs∣+∣ℑw∣+∣ℑz∣)Jη,e,ϵ,|\mathfrak H_{\eta,1,Z}(s,w,z)| \ll_{\eta,e,\epsilon} Z^{\ell\Re z+\epsilon} (1+|\Im s|+|\Im w|+|\Im z|)^{J_{\eta,e,\epsilon}},

with finite Jη,e,ϵJ_{\eta,e,\epsilon} fixed before any external tail order. Suppose also that Aη(Z)≠0A_\eta(Z)\ne0 for every sufficiently large real ZZ, that ∣Aη(Z)∣−1≪η,εZε|A_\eta(Z)|^{-1}\ll_{\eta,\varepsilon} Z^\varepsilon for every ε>0\varepsilon>0, and that on ℜs=β∗+e\Re s=\beta_*+e, uniformly in ℑs\Im s,

Hη,1,Z(s,1,1/6)=Hη(s)Zℓ/6Aη(Z)(1+Rη,Z(s)).\mathfrak H_{\eta,1,Z}(s,1,1/6) =H_\eta(s)Z^{\ell/6}A_\eta(Z)(1+\mathcal R_{\eta,Z}(s)).

Here either Rη,Z\mathcal R_{\eta,Z} is identically zero, or there is a number μ>0\mu> 0, chosen independently of η\eta, such that ∣Rη,Z(s)∣≪ηZ−μ|\mathcal R_{\eta,Z}(s)|\ll_\eta Z^{-\mu} on that entire line.

Let Pη(Z)\mathscr P_\eta(Z) be the u=1u=1 term of (10.5), and define

fη(Z)=12πi∫(2)ZC(s)e(s−5/6)2Hη(s)LFS(s,η) ds.f_{\eta}(Z)=\frac{1}{2\pi i}\int_{(2)} Z^{C(s)}e^{(s-5/6)^2}\frac{H_{\eta}(s)}{L_F^S(s,\eta)}\,ds.

Then cS>0c_S>0, and, for every ϵ>0\epsilon>0,

Pη(Z)cSAη(Z)−fη(Z)≪η,e,ϵZC(β∗)+(1+h)e−ly/20+ϵ+ZC(β∗)+e−h/600+ϵ+ZC(β∗)+e−μ+ϵ.\begin{aligned} \frac{\mathscr P_\eta(Z)}{c_SA_\eta(Z)}-f_\eta(Z) \ll_{\eta,e,\epsilon}{}& Z^{C(\beta_*)+(1+h)e-l_y/20+\epsilon} +Z^{C(\beta_*)+e-h/600+\epsilon}\\ &+Z^{C(\beta_*)+e-\mu+\epsilon}. \end{aligned}

The last term is omitted when Rη,Z\mathcal R_{\eta,Z} is identically zero. The implied constants and lower thresholds may depend on the target, but the displayed real exponents do not.

Proof. For u=1u=1, the scalar factor in the high identity is

ζFS(6z)ζFS(w)LFS(s,η).\frac{\zeta_F^S(6z)\zeta_F^S(w)}{L_F^S(s,\eta)}.

Isolate this term on the absolute contours. Move to ℜs=β∗+e\Re s=\beta_*+e, ℜw=1+e\Re w=1+e and ℜz=1/6+e\Re z=1/6+e. The reciprocal stays in ℜs>β∗\Re s>\beta_*, and both zeta arguments stay to the right of one. The paths lie in D2\mathcal D_2, so the correction is holomorphic. The all-height majorant and Lemma 10.2 justify the horizontal limits.

Move ww to 19/2019/20, crossing its simple pole at w=1w=1. In that residue move zz to 33/200=1/6−1/60033/200=1/6-1/600, crossing its simple pole at z=1/6z=1/6. The unresidued ww integral keeps ℜz=1/6+e\Re z=1/6+e. All these paths lie in D2\mathcal D_2, and M(z)M(z) is holomorphic for ℜz>0\Re z>0. Thus the two stated scalar poles are the only poles crossed. The reciprocal remains on its global line throughout, even when η\eta is principal. Every extended vertical ww- or zz-axis used to bound a tail lies strictly on one side of its scalar pole; w=1w=1 and z=1/6z=1/6 occur only as residues, and the horizontal joins have large nonzero height. On those axes the zeta functions have fixed polynomial bounds. Consequently the integrated and trace estimates of Lemma 10.2 apply without an unremoved pole in their majorants. After the ww residue, its Mellin factor has become the constant W^1(1)\widehat{W}_1(1). The remaining heights use the two-dimensional kernel in (10.9), with (y1,y2)=(ℑ(s+z),ℑz)(y_1,y_2)=(\Im(s+z),\Im z); its trace estimate justifies the subsequent zz-join.

On the principal contours, (10.17) and the outside powers give the raw exponent

lx2+ℜs−1+hℜz+ly(ℜw−1).\frac{l_x}{2}+\Re s-1+h\Re z+l_y(\Re w-1).

For the unresidued ww integral this is C(β∗)+(1+h)e−ly/20C(\beta_*)+(1+h)e-l_y/20; for the leftover zz integral in the ww residue it is C(β∗)+e−h/600C(\beta_*)+e-h/600. The reciprocal on ℜs=β∗+e\Re s=\beta_*+e has an arbitrarily small power of its fixed target conductor and a fixed polynomial in height by Lemmas 4.9 and 4.10. The tests integrate those height powers. Requesting the small powers in the correction and in Aη−1A_{\eta}^{-1} to be sufficiently small gives the first two terms of (10.19).

The product of the scalar residues is cSc_S: the residue of ζFS(6z)\zeta_F^S(6z) at 1/61/6 is one sixth of the residue of ζFS(v)\zeta_F^S(v) at one. Positivity of cSc_S was proved when the normalization was defined.

At the double residue the outside power is

X1/3Zs−5/6Zℓ/6=ZC(s),Φ(s+1/6−1)=e(s−5/6)2.X^{1/3}Z^{s-5/6}Z^{\ell/6}=Z^{C(s)}, \qquad \Phi(s+1/6-1)=e^{(s-5/6)^2}.

(10.18) therefore makes the normalized double residue

12πi∫(β∗+e)ZC(s)e(s−5/6)2Hη(s)LFS(s,η)(1+Rη,Z(s)) ds.\frac1{2\pi i}\int_{(\beta_*+e)} Z^{C(s)}e^{(s-5/6)^2}\frac{H_\eta(s)}{L_F^S(s,\eta)} (1+\mathcal R_{\eta,Z}(s))\,ds.

When present, the error factor is estimated on this line; the global reciprocal bound and Gaussian give Oη,e,ϵ(ZC(β∗)+e−μ+ϵ)O_{\eta,e,\epsilon}(Z^{C(\beta_*)+e-\mu+\epsilon}). No continuation of that error factor is required.

Move only the main integral right to ℜs=2\Re s = 2. The reciprocal is holomorphic for ℜs>β∗\Re s > \beta_* by the definition of β∗\beta_* and absolute Euler convergence beyond one. At a principal pole its reciprocal has a zero, so that case adds no residue. The function HηH_\eta is holomorphic there by Lemma 7.1, and is bounded there by (10.2). The global reciprocal estimate is polynomial in height uniformly on the fixed real strip, while the Gaussian is O(e−(ℑs)2)O(e^{-(\Im s)^2}). Rectangular contours therefore have vanishing horizontal sides, and the shifted integral is exactly fη(Z)f_\eta(Z). This also covers β∗=1\beta_* = 1. The three remainders give the asserted bound.

The function HηH_\eta in this lemma is the correction of the unmodified scalar Euler product at the double residue. A different full correction is permitted only when it verifies (10.18) with a nonzero normalizer. For the base correction that equation holds with Aη=1A_\eta= 1 and Rη,Z=0\mathcal R_{\eta,Z}=0. The normalized physical quantity in any application is Iη/(cSAη)\mathscr I_\eta/(c_SA_\eta); the same normalizer must be used for its direct estimate and for this principal comparison. The raw central and outer-row bounds acquire only an arbitrarily small additional power after this division, by the hypothesis on Aη−1A_\eta^{-1}.

The base correction. Take lx=ly=h=1/2l_x = l_y = h = 1/2 and ℓ=0\ell= 0. On the principal rectangle of Lemma 10.5, the local correction is bounded uniformly in every height because that rectangle lies in D2\mathcal D_2. Thus Equation (10.17) holds with ℓ=0\ell= 0 and height order zero. At the double residue it satisfies exactly

Hη,1,Z(s,1,1/6)=Hη(s)=Hη(s)Zℓ/6⋅1⋅(1+0).\mathfrak H_{\eta,1,Z}(s,1,1/6)=H_\eta(s) =H_\eta(s)Z^{\ell/6}\cdot1\cdot(1+0).

Hence Aη=1A_\eta= 1 and the residue error is identically zero. In the row u=1u = 1, the outside factor qu−zξ(u)‾q_u^{-z}\overline{\xi(u)} is one; the sole factor 1/61/6 is already in cSc_S from the residue of ζFS(6z)\zeta_F^S(6z). Lemma 10.5 therefore has just its two remainder terms. Their savings before losses are

mw=ly20=140,mz=h600=11200.m_w=\frac{l_y}{20}=\frac{1}{40},\qquad m_z=\frac{h}{600}=\frac{1}{1200}.

Small and large row norms

The buffered bin estimate is needed only on a bounded interval of positive row exponents. The following direct bounds cover its two complements. They ask for explicit absolute estimates on the full correction and do not use its central decomposition.

Lemma 10.6 (Outer row norms). Assume Definition 10.1. Fix σ0∈[7/8,1)\sigma_0 \in[7/8,1) with β∗>σ0\beta_* > \sigma_0, 0<e<10−30 < e < 10^{-3}, z0=17/50z_0 = 17/50, and dmin⁡>0d_{\min} > 0. For a dyadic number U≥1U \ge1, let Rη(U;Z)\mathscr R_\eta(U;Z) denote the contribution in Equation (10.5) of physical rows U≤qu<2UU \le q_u < 2U, omitting u=1u = 1.

Suppose that for every ϵ>0\epsilon> 0, for all such rows with qu≤2Zdmin⁡q_u \le2Z^{d_{\min}}, and uniformly in all imaginary parts on (ℜs,ℜw,ℜz)=(β∗+e,1/2,z0)(\Re s,\Re w,\Re z)=(\beta_*+e,1/2,z_0),

∣Hη,u,Z(s,w,z)∣≪η,e,ϵZℓz0+ϵquϵ(1+∣ℑs∣+∣ℑw∣+∣ℑz∣)Jη,e,ϵ.|\mathfrak H_{\eta,u,Z}(s,w,z)| \ll_{\eta,e,\epsilon} Z^{\ell z_0+\epsilon}q_u^\epsilon (1+|\Im s|+|\Im w|+|\Im z|)^{J_{\eta,e,\epsilon}}.

Then, for every ϵ>0\epsilon> 0 and 1≤U≤Zdmin⁡1\le U\le Z^{d_{\min}},

∣Rη(U;Z)∣≪η,e,ϵZC(β∗)+h(z0−1/6)−ly/2+e+ϵU63/50+ϵ.|\mathscr R_\eta(U;Z)| \ll_{\eta,e,\epsilon} Z^{C(\beta_*)+h(z_0-1/6)-l_y/2+e+\epsilon} U^{63/50+\epsilon}.

In particular the sum of these dyads is

≪η,e,ϵZC(β∗)+h(z0−1/6)−ly/2+e+(63/50)dmin⁡+ϵ.\ll_{\eta,e,\epsilon} Z^{C(\beta_*)+h(z_0-1/6)-l_y/2+e+(63/50)d_{\min}+\epsilon}.

For the other end, suppose that for every fixed v>2v>2 and ϵ>0\epsilon>0, for every physical row, uniformly in all imaginary parts on (ℜs,ℜw,ℜz)=(2,2,v)(\Re s,\Re w,\Re z)=(2,2,v),

∣Hη,u,Z(s,w,z)∣≪η,v,ϵZℓv+ϵquϵ(1+∣ℑs∣+∣ℑw∣+∣ℑz∣)Jη,v,ϵ.|\mathfrak H_{\eta,u,Z}(s,w,z)| \ll_{\eta,v,\epsilon} Z^{\ell v+\epsilon}q_u^\epsilon (1+|\Im s|+|\Im w|+|\Im z|)^{J_{\eta,v,\epsilon}}.

Write B0=lx/2+1+lyB_0 = l_x/2 + 1 + l_y. Then, for every dyad UU,

∣Rη(U;Z)∣≪η,v,ϵZB0+hv+ϵU1+ϵ−v.|\mathscr R_\eta(U;Z)| \ll_{\eta,v,\epsilon}Z^{B_0+hv+\epsilon}U^{1+\epsilon-v}.

For every fixed ζ>0\zeta> 0, if ϵ<v−1\epsilon< v-1, its sum over U>Zh+ζU > Z^{h+\zeta} is

≪η,v,ϵZB0+(h+ζ)(1+ϵ)−ζv+ϵ.\ll_{\eta,v,\epsilon} Z^{B_0+(h+\zeta)(1+\epsilon)-\zeta v+\epsilon}.

Thus a fixed sufficiently large vv makes this last contribution smaller than any prescribed power of ZZ.

Proof. Every row under consideration has nonprincipal numerator by the classification preceding Lemma 10.5. The denominator may be principal for a bounded unit row; its reciprocal is nevertheless holomorphic and bounded on ℜs=β∗+e\Re s = \beta_* + e by the principal specialization of Lemma 4.9.

For all rows, the conductor and deletion radical bounds in Section 8, together with Lemma 4.10, give an arbitrarily small power of quq_u and a fixed height polynomial for that reciprocal.

For a small dyad move its finite sum to (ℜs,ℜw,ℜz)=(β∗+e,1/2,z0)(\Re s,\Re w,\Re z) = (\beta_* + e,1/2,z_0). The reciprocal stays global. The numerator is entire, and the scalar zeta argument stays to the right of one. These paths may be taken in D1(3/8)\mathcal{D}_1(3/8): at the final point ℜ(s+w)=β∗+e+1/2>1+3/8\Re(s+w) = \beta_* + e + 1/2 > 1 + 3/8, and the other inequalities are immediate. The all-height correction bound and Lemma 10.2 justify the moves. On the final lines, Equation (4.14) and the deletion bound give U3/5+ϵU^{3/5+\epsilon} times a fixed height polynomial for the nonprincipal numerator. There are O(U)O(U) element rows in the dyad, including unit factors, and qu−z0≪U−z0q_u^{-z_0} \ll U^{-z_0}. The correction is bounded by Equation (10.20). The tests integrate all fixed height powers. The resulting exponent outside the row power, relative to C(β∗)C(\beta_*), is

h(z0−1/6)−ly/2+e,h(z_0 - 1/6) - l_y/2 + e,

and the row power is 1+3/5−z0=63/501 + 3/5 - z_0 = 63/50. Requesting the component small powers to sum to the displayed ϵ\epsilon proves Equation (10.21). The row exponent is positive, so dyadic summation up to Zdmin⁡Z^{d_{\min}} gives Equation (10.22), after decreasing the preliminary losses.

For each fixed ZZ and large dyad, move its finite row sum to the absolute lines (2,2,v)(2,2,v). The path from (3,3,2)(3,3,2) remains in ℜs,ℜw≥2\Re s,\Re w \ge2 and ℜz≥2\Re z \ge2, so the scalar factors are holomorphic there. For this fixed dyad choose DD large enough to contain its rows in qu≤ZDq_u \le Z^D; Equation (10.4) and the external trace bound make its horizontal limits vanish. Constants used only to justify this equality may depend on the fixed dyad. The estimate on the final lines is uniform in the dyad by Equation (10.23). The scalar LL-factors are absolutely bounded there, as is ζFS(6z)\zeta_F^S(6z), and Equation (10.23) applies. The outside power, including the correction but not the row count, is

lx(1/2−v)+1+v+ly+ℓv=B0+hv.l_x(1/2-v) + 1 + v + l_y + \ell v = B_0 + hv.

The O(U)O(U) rows and qu−vq_u^{-v} give U1−vU^{1-v}; the tests integrate the fixed height polynomial. This proves Equation (10.24). Because 1+ϵ−v<01+\epsilon-v<0, summing its geometric dyadic tail gives Equation (10.25). For fixed ζ>0\zeta> 0, the coefficient of vv in that exponent is −ζ-\zeta, proving the last assertion. The original row series is absolutely convergent on its starting lines, and the displayed bounds give an absolutely summable final tail, so the individual dyadic contour identities may be summed. The number vv and the finite test orders it requires are fixed before ZZ tends to infinity. □

The first-stage outer ranges. Use lx=ly=h=1/2l_x=l_y=h=1/2, ℓ=0\ell=0, dmin⁡=1/63d_{\min}=1/63 and ζ=1/1000\zeta=1/1000, as in the intermediate-row estimate. For the small rows, the line (β∗+e,1/2,z0)(\beta_*+e,1/2,z_0) lies in D1(3/8)\mathcal{D}_1(3/8), since β∗>11/12\beta_* > 11/12. The local bound Hη,u≪ϵquϵ\mathcal H_{\eta,u}\ll_\epsilon q_u^\epsilon, uniform in all heights, verifies Equation (10.20) for all the prescribed rows, with height order zero. Equation (10.22) then has the following relative exponent before its losses:

h(z0−1/6)−ly2+6350dmin⁡=13150−14+150=−43300.h(z_0-1/6)-\frac{l_y}{2}+\frac{63}{50}d_{\min} =\frac{13}{150}-\frac14+\frac{1}{50} =-\frac{43}{300}.

For the large rows, (2,2,v)(2,2,v) with v>2v>2 lies in D2\mathcal D_2. The same all-height local bound verifies Equation (10.23) for every physical row. Here B0=lx/2+1+ly=7/4B_0=l_x/2+1+l_y=7/4, so Equation (10.25) has exponent

74+5011000(1+ϵ)−v1000+ϵ.\frac{7}{4}+\frac{501}{1000}(1+\epsilon)-\frac{v}{1000}+\epsilon.

It tends to −∞-\infty as the fixed number vv increases. For example, v=4000v=4000 makes it less than −1-1 when ϵ≤10−6\epsilon\leq10^{-6}, whereas CI(β∗)≥1/4C_{\mathrm I}(\beta_*)\ge1/4. This more than supplies the saving needed below. The three ranges U≤Zdmin⁡U\leq Z^{d_{\min}}, Zdmin⁡<U≤Zh+ζZ^{d_{\min}}<U\leq Z^{h+\zeta}, and U>Zh+ζU>Z^{h+\zeta} cover every physical dyad. The row u=1u=1 was already assigned to the principal term.

The 11/12 conclusion

For the normalized base probe the central estimate, principal extraction, and outer-row estimates now give the following margins before adjustable losses:

contributionsaving relative to CI(β∗)C_{\mathrm I}(\beta_*)
intermediate rows1021/250001021/25000
unresidued principal ww integral1/401/40
remaining principal zz integral1/12001/1200
small rows43/30043/300
large rows (v=4000v=4000)>1>1

The smallest margin comes from the principal zz remainder. We retain a common positive margin after all real losses, then choose the analysis height for each target. The physical sum and the signal do not depend on that height.

Choosing the final height

The preceding estimates separate real powers from finite powers of the analysis height T1T_1. The following elementary step records the order of choices needed to obtain one power saving for every target.

Lemma 11.1 (Late choice of height and external order). Fix σ0∈(1/2,1)\sigma_0\in(1/2,1) with Δ0=β∗−σ0>0\Delta_0=\beta_*-\sigma_0>0 and an affine function C(s)=s+cC(s)=s+c. Suppose that all real parameters and finite structural choices in an application have been fixed independently of η\eta. Suppose there are common numbers m>0m>0 and 0<ω<Δ00<\omega<\Delta_0 such that, for every primitive finite-order target, functions JηJ_\eta, fηf_\eta independent of T1T_1 satisfy

∣Jη(Z)∣≪ηZC(σ0)+ω.|J_\eta(Z)|\ll_\eta Z^{C(\sigma_0)+\omega}.

Assume that after a finite sum of estimates, for every integer N≥0N\geq0,

∣Jη(Z)−fη(Z)∣≪η,NZC(β∗)−m(1+T1)Aη+ZBηT1−N.|J_\eta(Z)-f_\eta(Z)|\ll_{\eta,N} Z^{C(\beta_*)-m}(1+T_1)^{A_\eta}+Z^{B_\eta}T_1^{-N}.

where Aη≥0A_\eta\geq0 and BηB_\eta are finite and independent of NN. Suppose there is a number τ0,η>0\tau_{0,\eta}>0, fixed after the real choices and the finite profile orders for the target but before NN and ZZ, such that the estimate is valid for sufficiently large ZZ whenever T1=ZτT_1=Z^\tau and 0<τ≤min⁡{dmin⁡/100,τ0,η}0<\tau\leq\min\{d_{\min}/100,\tau_{0,\eta}\}, with a fixed dmin⁡>0d_{\min}>0. This additional ceiling may encode a height condition in a preceding estimate, such as the one in Lemma (8.2). The lower threshold may depend on η,N,τ\eta,N,\tau. Increasing NN is assumed to change only external test seminorms, not AηA_\eta or the already fixed real powers in Equation (11.1).

Then τ\tau and NN can be chosen after η\eta so that

∣Jη(Z)−fη(Z)∣≪ηZC(β∗)−m/2.|J_\eta(Z)-f_\eta(Z)|\ll_\eta Z^{C(\beta_*)-m/2}.

In particular the common saving σ=m/2\sigma=m/2, together with the displayed low estimate, has the target quantifier required by Proposition (2.1).

Proof. For the fixed target choose

0<τη≤min⁡{dmin⁡100,τ0,η,m4(Aη+1)},T1=Zτη.0 < \tau_\eta\le\min\left\{\frac{d_{\min}}{100},\tau_{0,\eta},\frac{m}{4(A_\eta+1)}\right\}, \qquad T_1 = Z^{\tau_\eta}.

Then (1+T1)Aη≪ηZm/4(1+T_1)^{A_\eta} \ll_\eta Z^{m/4}, so the first term in Equation (11.1) is Oη(ZC(β∗)−3m/4)O_\eta(Z^{C(\beta_*)-3m/4}). Next choose a fixed integer NN such that

Bη−Nτη<C(β∗)−m/2.B_\eta-N\tau_\eta<C(\beta_*)-m/2.

This is possible because τη>0\tau_\eta>0 and BηB_\eta is finite. The second term is then bounded by the required power. Increase the lower threshold for ZZ after these choices. Both mm and ω\omega were fixed before the target, whereas τη\tau_\eta, NN and the threshold may depend on it. Since JηJ_\eta and fηf_\eta do not contain T1T_1, this proves the asserted family-wide exponent without changing either function. □

Proposition 11.2 (Balanced high estimate). Under the supposition Δ1>0\Delta_1>0, for every primitive finite-order target η\eta and all sufficiently large ZZ,

∣JI,η(Z)−fI,η(Z)∣≪ηZCI(β∗)−1/4800.|J_{\mathrm I,\eta}(Z)-f_{\mathrm I,\eta}(Z)| \ll_\eta Z^{C_{\mathrm I}(\beta_*)-1/4800}.

The displayed saving is independent of the target; the implied constant and lower threshold may depend on it.

Proof. Use lx=ly=h=1/2l_x=l_y=h=1/2, ℓ=0\ell=0 and C=CIC=C_{\mathrm I}. The exact identity and local correction were verified at the start of Section 10; Equation (10.12) estimates its intermediate rows, and the principal and outer specializations there give the margins listed above. It remains to choose their losses.

Order of choices. We give a common loss budget. Put

m0=11200,ϵ∗=10−6,m=12400,ω=Δ12.m_0=\frac{1}{1200},\qquad\epsilon_* = 10^{-6},\qquad m=\frac{1}{2400},\qquad\omega=\frac{\Delta_1}{2}.

The error-free central, small, principal, and large savings just proved are all at least m0m_0. Fix the displayed geometry, row ranges, and v=4000v=4000 before the target. Request loss ϵ∗\epsilon_* in the row count, numerator, local correction, buffered reciprocal, central multiplicity, and each principal or outer estimate. Reserve a further loss ϵ∗\epsilon_* for the O(log⁡Z)O(\log Z) physical dyads. The witness-pair and powerful-part logarithms are already included in the requested row-count loss; the Oe(1)O_e(1) bins and fixed presentation choices cost constants.

To obtain the requested row-count loss, first choose its preliminary witness, dyadic, and sieve losses sufficiently small in terms of ϵ∗\epsilon_*. These choices are independent of the target. Indeed the witness length error has an absolute coefficient, and the affine slopes in the optimization of Proposition 9.2 are uniformly bounded. The target-dependent constants in the actual dyadic endpoints multiply only 1/log⁡U1/\log U, which changes a fixed constant or lower threshold. Apply Lemma 8.2 on the enclosing pre-saturation ranges 0≤r,m≤220\le r,m\le22: the detector’s terminal product cutoff is O(U21)O(U^{21}) before it proves the shorter witness lengths. Its number e0e_0 depends only on the requested dyadic loss and these bounded ranges. We may thus fix, still before the target,

0<e<min⁡{10−3,ϵ∗,e0}.0<e<\min\{10^{-3},\epsilon_*,e_0\}.

With ϵr=ϵn=ϵH=ϵ∗\epsilon_r=\epsilon_n=\epsilon_H=\epsilon_*, this gives ϵc≤15ϵ∗\epsilon_c\le15\epsilon_*. Since d≤501/1000<1d\le501/1000<1, the explicit central losses in Equation (10.12), together with the reserved physical-dyad loss, are at most

13ϵ∗+2(15ϵ∗)+ϵ∗+ϵ∗+ϵ∗=46ϵ∗<14800=m04.13\epsilon_*+2(15\epsilon_*)+\epsilon_*+\epsilon_*+\epsilon_*=46\epsilon_*<\frac{1}{4800}=\frac{m_0}{4}.

The two principal losses are at most (3/2+1)ϵ∗(3/2+1)\epsilon_* and 2ϵ∗2\epsilon_*; the small-row loss is at most 2ϵ∗2\epsilon_*. Each is less than m0/4m_0/4. The displayed large-row estimate already uses its requested loss. Therefore all these terms, after division by the fixed cSc_S, retain at least 3m0/4=1/16003m_0/4 = 1/1600 before the height factor. We use only m=1/2400m = 1/2400, leaving a further power 1/48001/4800 available below.

It remains to check when the height hypotheses hold. Let ϵdet>0\epsilon_{\rm det}>0 be the fixed dyadic loss chosen above, and, after fixing a target, let Adet,ηA_{{\rm det},\eta} dominate the finitely many orders in its uses of Lemma 8.2. Set

τ0,η=dmin⁡ϵdet20(Adet,η+1)>0.\tau_{0,\eta} =\frac{d_{\min}\epsilon_{\rm det}} {20(A_{{\rm det},\eta}+1)}>0.

For 0<τ≤τ0,η0 < \tau\le\tau_{0,\eta} and sufficiently large ZZ,

(1+Zτ)Adet,η≤Zdmin⁡ϵdet/10≤Uϵdet/10(d≥dmin⁡).(1+Z^\tau)^{A_{{\rm det},\eta}} \le Z^{d_{\min}\epsilon_{\rm det}/10} \le U^{\epsilon_{\rm det}/10} \qquad(d\ge d_{\min}).

This verifies the detector height condition uniformly over the physical range. The fixed factor from 1+Zτ≤2Zτ1+Z^\tau\le2Z^\tau is absorbed by the lower threshold. We also impose τ≤dmin⁡/100\tau\le d_{\min}/100 as required by the bins. The internal tail orders used to establish the witnesses are chosen after this τ\tau and are separate from the final external order NN below. Their increase does not change the retained profile or height orders. Any fixed constants introduced by those internal choices are absorbed into the unused power 1/48001/4800 by increasing the lower threshold, which may depend on η\eta and τ\tau.

For every final integer N≥0N \ge0, Lemma 10.3 bounds the discarded high portions and joins by Oη,N(ZBηT1−N)O_{\eta,N}(Z^{B_\eta}T_1^{-N}), with BηB_\eta fixed before NN. The bounded real and row ranges and the finite set of bins permit one such BηB_\eta for all the central dyads. Summing the O(log⁡Z)O(\log Z) dyads can be absorbed by increasing BηB_\eta by one, again before NN. Combining the preceding estimates gives

∣JI,η(Z)−fI,η(Z)∣≪η,NZCI(β∗)−m(1+T1)Aη+ZBηT1−N|J_{\mathrm I,\eta}(Z)-f_{\mathrm I,\eta}(Z)| \ll_{\eta,N}Z^{C_{\mathrm I}(\beta_*)-m}(1+T_1)^{A_\eta} +Z^{B_\eta}T_1^{-N}

for some finite Aη,BηA_\eta,B_\eta, whenever 0<τ≤min⁡{dmin⁡/100,τ0,η}0 < \tau\le\min\{d_{\min}/100,\tau_{0,\eta}\} and ZZ is sufficiently large. Both functions are independent of T1T_1. Proposition 6.3, applied with loss ω\omega and divided by the same fixed cSc_S, supplies

∣JI,η(Z)∣≪ηZ1/4+ω=ZCI(11/12)+ω,0<ω<Δ1.|J_{\mathrm I,\eta}(Z)|\ll_\eta Z^{1/4+\omega}=Z^{C_{\mathrm I}(11/12)+\omega}, \qquad 0<\omega<\Delta_1.

All hypotheses of Lemma 11.1 are now verified. It gives the saving m/2=1/4800m/2 = 1/4800 asserted in the proposition.

Transfer to Dirichlet LL-functions

The continuation criterion concerns the Hecke family over FF. We prove once that a strict zero-free half-plane for that family has the corresponding Dirichlet consequence.

Proposition 11.3 (Quadratic transfer). Let σ0∈[1/2,1)\sigma_0 \in[1/2,1). Suppose every primitive finite-order Hecke LL-function over F=Q(−3)F = \mathbb{Q}(\sqrt{-3}) is zero-free on ℜs>σ0\Re s > \sigma_0, with its principal pole at one allowed. Then every finite-order Hecke LL-function over FF and every Dirichlet LL-function is zero-free on that same strict half-plane, again allowing the principal pole at one.

Proof. Passing from a primitive Hecke character to one that it induces changes only finitely many factors 1−η(p)Np−s1-\eta(\mathfrak p)N\mathfrak p^{-s}. They are nonzero for ℜs>0\Re s > 0, so the Hecke assertion extends to all finite-order characters. The same observation for factors 1−χ(p)p−s1-\chi(p)p^{-s} reduces the Dirichlet assertion to a primitive Dirichlet character χ\chi of conductor qq.

Let χ−3\chi_{-3} be the quadratic character of conductor three, and let η\eta be the finite-order Hecke character given by a↦χ(Na)\mathfrak a \mapsto\chi(N\mathfrak a) on ideals coprime to 3q3q. It is a ray character: if α≡1(modqO)\alpha\equiv1 \pmod{q\mathcal O}, then Nα≡1(modq)N\alpha\equiv1 \pmod q, so the norm character is trivial on the corresponding principal ray subgroup. Let SQS_{\mathbb Q} be the rational primes dividing 3q3q, and let SQ\mathcal S_{\mathbb Q} be the primes of FF above them. Superscripts by these sets denote deletion of those Euler factors.

For p∉SQp \notin S_{\mathbb Q}, the local factors agree as follows. If pp splits in FF, then χ−3(p)=1\chi_{-3}(p)=1, the two prime ideals have norm pp, and the Hecke factor is (1−χ(p)p−s)−2(1-\chi(p)p^{-s})^{-2}. This is the product of the Dirichlet factors for χ\chi and χχ−3\chi\chi_{-3}. If pp is inert, then χ−3(p)=−1\chi_{-3}(p)=-1, the unique prime ideal has norm p2p^2, and its factor is

(1−χ(p)2p−2s)−1=(1−χ(p)p−s)−1(1+χ(p)p−s)−1.(1-\chi(p)^2p^{-2s})^{-1}=(1-\chi(p)p^{-s})^{-1}(1+\chi(p)p^{-s})^{-1}.

These exhaust the primes outside SQS_{\mathbb{Q}}. Absolute Euler convergence for ℜs>1\Re s>1, followed by uniqueness of meromorphic continuation, gives

LFSQ(s,η)=LSQ(s,χ)LSQ(s,χχ−3).L_F^{\mathcal S_{\mathbb Q}}(s,\eta) =L^{S_{\mathbb Q}}(s,\chi) L^{S_{\mathbb Q}}(s,\chi\chi_{-3}).

The product character on the right may be imprimitive; deletion of SQS_{\mathbb{Q}} makes the identity independent of that choice. Every deleted factor is nonzero for ℜs>0\Re s>0.

Both Dirichlet factors are holomorphic in 0<ℜs<10<\Re s<1. A zero of L(s,χ)L(s,\chi) there would therefore give a zero of the Hecke factor, with no cancellation by a pole, and the assumed Hecke half-plane excludes it when ℜs>σ0\Re s>\sigma_0. Absolute Euler convergence handles ℜs>1\Re s>1. On s=1+its=1+it with t≠0t\ne0, neither Dirichlet factor has a pole, so the same product argument applies.

At s=1s=1, a pole-zero cancellation could occur only if one primitive inducing character among χ\chi and χχ−3\chi\chi_{-3} were principal. The other would then be χ−3\chi_{-3}. Its Dirichlet series converges at one by bounded partial sums of the nonprincipal periodic character, and grouping consecutive terms gives

L(1,χ−3)=∑n≥0(13n+1−13n+2)=∫011−x1−x3 dx=∫01dx1+x+x2=π33>0.L(1,\chi_{-3})=\sum_{n\ge0}\left(\frac{1}{3n+1}-\frac{1}{3n+2}\right) =\int_0^1\frac{1-x}{1-x^3}\,dx =\int_0^1\frac{dx}{1+x+x^2} =\frac{\pi}{3\sqrt{3}}>0.

The first integral follows by monotone convergence of the nonnegative paired integrands. Thus there is no zero in this last case either; a principal pole is allowed. This proves the strict half-plane assertion with no claim on its boundary.

Proof of Theorem 3.1. Suppose that β∗>11/12\beta_* > 11/12. Lemma 7.1 and (10.2) give the required holomorphic, nonzero HηH_\eta on ℜs>11/12\Re s>11/12 for every primitive target. The low and high bounds established in Proposition 11.2 and its proof verify Proposition 2.1 with

σ0=1112,C=CI,ω=Δ12,σ=14800.\sigma_0=\frac{11}{12},\qquad C=C_{\mathrm I},\qquad \omega=\frac{\Delta_1}{2},\qquad \sigma=\frac1{4800}.

These two positive losses are independent of the target, while the allowed constants, excluded sets, and thresholds may depend on it. The continuation criterion contradicts the supposition. Therefore β∗≤11/12\beta_* \le11/12. By its definition and absolute Euler convergence in ℜs>1\Re s>1, every primitive finite-order Hecke LL-function over FF is zero-free in the strict half-plane ℜs>11/12\Re s>11/12, with the principal pole allowed.

Proposition 11.3, applied at the same boundary, extends this assertion to all finite-order Hecke characters and all Dirichlet LL-functions, including ζ(s)\zeta(s). It preserves the strict half-plane and the allowed principal pole. This proves the theorem.

II The seven-eighths zero-free half-plane

The compensated probe

Theorem 3.1 applies to every primitive character entering the supremum in Equation (2.1), and therefore gives β∗≤11/12\beta_* \le11/12. Suppose for contradiction throughout Part II that β∗>7/8\beta_*>7/8, and put

Δ:=β∗−78,0<Δ≤124,κ:=2β∗−1=34+2Δ≤56.\Delta:=\beta_*-\frac{7}{8},\qquad0<\Delta\le\frac{1}{24},\qquad\kappa:=2\beta_*-1=\frac{3}{4}+2\Delta\le\frac{5}{6}.

The exact bin ceiling in Section 8 applies, since β∗>7/8>51/100\beta_\ast> 7/8 > 51/100. For every retained nonprincipal row and its bin (i,a)(i,a) it gives

a≤β∗,δ=2a−1≤κ≤56.a \le\beta_\ast,\qquad\delta= 2a-1 \le\kappa\le\frac{5}{6}.

Indeed, the finite set defining Mi(u)M_i(u) consists of the floor 51/10051/100 and real parts of actual zeros, all at most β∗\beta_\ast. This uses only the definition of the supremum, not its attainment. The boundary case δ=5/6\delta= 5/6 remains part of the argument.

For the second application of Proposition 2.1, write throughout Part II

C(s)=CII(s):=s−1116,C(7/8)=316.C(s)=C_{\mathrm{II}}(s):=s-\frac{11}{16},\qquad C(7/8)=\frac{3}{16}.

Our task is to construct a normalized probe JII,ηJ_{\mathrm{II},\eta} from the finite expression below. It is distinct from the balanced probe JI,ηJ_{\mathrm{I},\eta}. Its low-side target is ∣JII,η(Z)∣≪ηZ3/16+ω|J_{\mathrm{II},\eta}(Z)|\ll_\eta Z^{3/16+\omega} for a common 0<ω<Δ0<\omega<\Delta; its high side must satisfy the signal estimate in (2.5) with this CC. The nonzero scalar normalization will be specified after the principal term is evaluated.

For each primitive target η\eta, use an admissible fixed instance of the data TT, SS, b∗b_*, ξ\xi, τ\tau, Ξ\Xi, W0W_0, W1W_1 from Section 6. The permitted choice of P0P_0 will be made in the parameter order below. These data may differ from those used in Part I, but within this application they are independent of ZZ and are the same in the physical probe and its high representation.

We first define the two-term modification on the original probe, before moving any contour. The subsequent low and high estimates will concern this same finite expression.

Use the fixed geometry

b=18,h=1316,ℓ=16,b=\frac{1}{8},\qquad h=\frac{13}{16},\qquad\ell=\frac{1}{6},
lx=1+ℓ−h=1748,ly=lx+b=2348,l_x=1+\ell-h=\frac{17}{48},\qquad l_y=l_x+b=\frac{23}{48},
X=Zlx,Y=Zly,M=lx+ly=56,M+ℓ=1.X=Z^{l_x},\qquad Y=Z^{l_y},\qquad M=l_x+l_y=\frac56,\qquad M+\ell=1.

Fix positive slot lengths ℓ1,…,ℓK\ell_1,\ldots,\ell_K of total length ℓ\ell, and put Pi=ZℓiP_i=Z^{\ell_i}. Each physical slot has a nonnegative, nonzero smooth annular weight Wi(qp/Pi)W_i(q_p/P_i). Its allowed prime set is

Pi(Z)={p prime:p∉S, p∈1T, qp/Pi∈supp⁡Wi}.\mathcal{P}_i(Z)=\{p\ \text{prime}:p\notin S,\ p\in1_T,\ q_p/P_i\in\operatorname{supp}W_i\}.

The underlying window sets {p prime:qp/Pi∈supp⁡Wi}\{p\ \text{prime}:q_p/P_i\in\operatorname{supp}W_i\} for distinct slots are required to be disjoint before imposing the ray and SS restrictions. In particular, the sets Pi(Z)\mathcal{P}_i(Z) are disjoint, and every tuple in ∏iPi(Z)\prod_i\mathcal{P}_i(Z) consists of distinct primes. The number and lengths of the slots will be chosen later, but they are fixed independently of ZZ. A sum over p∈1Tp\in1_T for slot ii below always retains this same exclusion and annular support.

For a squarefree product DD of slot primes, let Iη;D(X,Y,Z)I_{\eta;D}(X,Y,Z) denote Equation (6.1) with the indicator 1D∣cn31_{D\mid cn^3} inserted in its completed row. Thus Iη;1=IηI_{\eta;1}=I_\eta. For a tuple (p1,…,pK)∈∏iPi(Z)(p_1,\ldots,p_K)\in\prod_i\mathcal{P}_i(Z) and J⊆{1,…,K}J\subseteq\{1,\ldots,K\} write pJ=∏i∈Jpip_J=\prod_{i\in J}p_i, with p∅=1p_\varnothing=1. The subset JJ indexes the rescaled slots and JcJ^c the marked slots; this subset notation is distinct from the normalized probe JII,ηJ_{\mathrm{II},\eta}. Define the modified probe by the finite identity

Iη,modified(Z)=∑(pi)∈∏iPi(Z)∏i=1KWi(qpi/Pi)∑J⊆{1,…,K}(−1)∣J∣qpJ−3/2η(pJc)‾⋅Iη;pJc(X/qpJ,Y/qpJ,ZqpJc).\begin{aligned} I_{\eta,\mathrm{modified}}(Z) =\sum_{(p_i)\in\prod_i\mathcal P_i(Z)}\prod_{i=1}^K W_i(q_{p_i}/P_i) \sum_{J\subseteq\{1,\ldots,K\}}&(-1)^{|J|}q_{p_J}^{-3/2} \overline{\eta(p_{J^c})}\\ &\cdot I_{\eta;p_{J^c}} (X/q_{p_J},Y/q_{p_J},Zq_{p_{J^c}}). \end{aligned}

Equivalently, at each prime pp the operation is the marked term η(p)‾Iη;p(X,Y,Zqp)\overline{\eta(p)}I_{\eta;p}(X,Y,Zq_p) minus the rescaled term qp−3/2Iη(X/qp,Y/qp,Z)q_p^{-3/2}I_\eta(X/q_p,Y/q_p,Z). Formula (12.5) specifies their composition: every slot window stays at its original scale PiP_i, including when another slot changes the completed scale. On 1T1_T one has θ(p)=1\theta(p)=1 for every θ∈T^\theta\in\widehat{T}. Thus marking commutes with the Fourier decomposition of G‾\overline G and preserves the same excluded set and zero masks in every summand. The subtraction is designed to cancel the scalar prime contribution on the high side, leaving the sextic-character prime factor used by the moment estimates. Section 16 proves the exact identity and bounds the remaining local errors.

Coefficient conventions and finite correlations

We record the additional coefficient conventions for the prime factors, then prove a fixed-ray prime normalizer and the full finite Fourier correlations needed below. The latter retain shared prime powers and will be used in the additive Gram bound as well as the fourth moment. The residue-symbol and fixed-data conventions of Part I remain in force.

Additional coefficient conditions

We use the plain and inverse polynomials, annular profiles, and fixed arithmetic datum A\mathcal{A} from Section 4. The following conditions specify the extra prime factors and moving zero supports used in this part.

A prime slot of log-length ziz_i is

Qψ,i=Z−zi/2∑p primeψ(p)νi(p)Wi(qp/Zzi).Q_{\psi,i}=Z^{-z_i/2}\sum_{p\ \mathrm{prime}}\psi(p)\nu_i(p)W_i\left(q_p/Z^{z_i}\right).

Here νi\nu_i is a fixed finite-ray character or a fixed finite linear combination of such characters. It is independent of the row and of the other selected primes. Distinct slots have disjoint underlying prime supports before any common mask or row zero extension is imposed. For the fourth moment of Section 18, a fixed finite group Θ\Theta of ray characters is part of the data, and every character component with nonzero coefficient in every positive-length slot must belong to Θ\Theta. The inverse moment of Section 17 also allows a bounded coefficient ai(p)a_i(p) chosen independently for each slot and independently of the row and all other columns; the coefficient of a prime tuple is then the product of its individual slot coefficients. The Θ\Theta restriction does not apply to these separate inverse-moment weights.

For an auxiliary fourth moment the rows are elements 0<qk≪Zm0<q_k\ll Z^m, and

ψk(n)=τ(n)χn(k),M=m+q.\psi_k(n)=\tau(n)\chi_n(k),\qquad M=m+q.

The twist τ\tau is common to the row sum after its outer labels are fixed, and its displayed factorization into fixed finite-ray and moving residue-symbol factors is part of the data. Let DmovD_{\mathrm{mov}} be the squarefree product of all good primes at which at least one displayed moving factor has its natural zero on nonunits. This includes a prime even when that factor has exponent divisible by six, including exponent zero, or when local characters cancel after multiplication. We require qDmov≤Zqq_{D_{\mathrm{mov}}}\le Z^q, counting an overlapping prime once.

An additional puncture is an indicator 1(n,R)=11_{(n,R)=1} with RR squarefree, qR≤ZBq_R\le Z^B, and BB in a prescribed bounded range. It must be common to the current row sum and to every plain and prime factor in that sum; it may depend on previously frozen outer labels. A prime may be removed from DmovD_{\mathrm{mov}} and put in RR only through an exact factorization of its displayed local factor into that coprimality indicator and the local or fixed-ray character phases that remain. Those phases must be retained, the refactored zero must be removed from the displayed moving factor, and the common puncture is deleted before the natural reflection in Section 18. No zero prime may be omitted from both supports. If a moving character still ramified at that prime remains, the prime stays in DmovD_{\mathrm{mov}}; only a redundant zero may be transferred to RR. A fixed finite-ray character here has its complete zero-extended presentation and ray group fixed in the preceding sense; a character with moving conductor cannot be relabeled as fixed. A locally frozen moving twist factor or redundant zero mask retains the stated moving-support and puncture requirements. In particular a ZZ-varying redundant mask cannot be included in the fixed arithmetic datum. The zero extension of χn(k)\chi_n(k) is allowed to vary naturally with kk, but cancellation between that varying row factor and a fixed twist may not be recast as a separately chosen puncture for each row. Externally chosen row-dependent punctures and row-dependent column coefficients are not part of this class. This full-support convention governs every fourth-moment invocation in Section 18.

The common uniformity convention has the following additional clauses for these coefficient classes. Any required slot mesh depends only on the fixed real log-length ranges, the strict margins, and the specified positive power losses. Finite seminorm orders, polynomial height orders, implied constants, and lower thresholds may also depend on a specified fixed number of slots. They are uniform over the moving moduli, the radicals included in MM, the admissible punctures, and the outer labels in their stated ranges, even when an outer label is fixed during one row sum. The constant CC in the definition of a divisor-bounded multiplicity may also depend on this fixed slot count. The independence of CC from ZZ, the current rows, and the averaged labels, and any separate requirement that the multiplicity depend only on ff, remain as in Section 4. The slot count is a separate fixed parameter, and moving labels remain outside A\mathcal{A}.

Prime counting in a fixed ray class

Lemma 13.1 (Fixed-ray prime normalizer). Let TT be a fixed quotient of a ray class group of FF, and write p∈1Tp\in1_T when the image of an unramified prime ideal is the identity. For a fixed nonnegative, nonzero smooth annular weight WW,

∑p∈1TW(qp/P)qp−5/6∼P1/6∣T∣log⁡P∫0∞W(y)y−5/6 dy.\sum_{p\in1_T}W(q_p/P)q_p^{-5/6} \sim\frac{P^{1/6}}{|T|\log P} \int_0^\infty W(y)y^{-5/6}\,dy.

Deleting any further fixed finite set of primes does not change this asymptotic. Its lower threshold may depend on all the fixed data.

Proof. For the fixed abelian extension of FF corresponding to TT, the prime ideal theorem in a fixed Frobenius class gives

π1T(x):=#{p∈1T:qp≤x}∼Li⁡(x)∣T∣.\pi_{1_T}(x):=\#\{p\in1_T:q_p\le x\} \sim\frac{\operatorname{Li}(x)}{|T|}.

This is the fixed-extension consequence of Chebotarev in [27 Theorem 1.1]; the extension and its conductor are fixed as x→∞x\to\infty. If supp⁡W⊂[a,b]⊂(0,∞)\operatorname{supp} W\subset[a,b]\subset(0,\infty), the error o(x/log⁡x)o(x/\log x) is uniform for aP≤x≤bPaP\le x\le bP as P→∞P\to\infty. Stieltjes integration by parts therefore changes the left side of Equation (13.3) by o(P1/6/log⁡P)o(P^{1/6}/\log P) when dπ1T(x)d\pi_{1_T}(x) is replaced by dx/(∣T∣log⁡x)dx/(|T|\log x). The resulting integral is

P1/6∣T∣log⁡P∫abW(y)y−5/6log⁡Plog⁡(Py) dy.\frac{P^{1/6}}{|T|\log P}\int_a^b W(y)y^{-5/6}\frac{\log P}{\log(Py)}\,dy.

The last ratio tends uniformly to one. This proves the formula and its positivity. A fixed finite set is eventually outside the annular window. No error exponent uniform in the ray conductor is used. □\square

Full finite Fourier correlations

We now allow arbitrary prime powers in a modulus. The two-argument notation G(a,k)G(a,k) below is a finite Fourier sum; it is distinct from the one-argument finite-ray function G(a)G(a) of Lemma 4.4. Define

G(a,k)=qa−1/2∑x mod aχa(x)e(kx/a),G(1,k)=1.G(a,k)=q_a^{-1/2}\sum_{x\bmod a}\chi_a(x)e(kx/a),\qquad G(1,k)=1.

All characters in this subsection have the zero extensions specified in Section 4, and we put vp(0)=+∞v_p(0)=+\infty.

Lemma 13.2 (Prime-power Fourier sums). For P=qpP=q_p and every integer a≥1a\ge1,

∣G(pa,k)∣=P(a−1)/21vp(k)=a−1,6∤a,|G(p^a,k)|=P^{(a-1)/2}1_{v_p(k)=a-1},6\nmid a,
G(pa,k)=Pa/21pa∣k−Pa/2−11pa−1∣k,6∣a.G(p^a,k)=P^{a/2}1_{p^a\mid k} -P^{a/2-1}1_{p^{a-1}\mid k},6\mid a.

Proof. Write a residue modulo pap^a as x0+pyx_0+py, with x0 mod px_0\bmod p and y mod pa−1y\bmod p^{a-1}. The sum over yy is zero unless pa−1∣kp^{a-1}\mid k, and equals Pa−1P^{a-1} otherwise. In the latter case write k=pa−1k0k=p^{a-1}k_0. The remaining normalized sum is

Pa/2−1∑x0 mod pχp(x0)ae(k0x0/p).P^{a/2-1}\sum_{x_0\bmod p}\chi_p(x_0)^a e(k_0x_0/p).

If 6∤a6\nmid a, its inner sum vanishes when p∣k0p\mid k_0 and otherwise has absolute value P\sqrt{P}. If 6∣a6\mid a, the inner sum is the sum of the additive character over the units, namely P1p∣k0−1P1_{p\mid k_0}-1. These are exactly the two cases in the statement.

Lemma 13.3 (Full correlation and common factors). For primary moduli u,vu,v outside SS and j∈Oj\in\mathcal{O}, put

F(u,v;j)=∑xmodu, ymodvvx−uy≡j(moduv)χu(x)χv(y)‾.F(u,v;j)=\sum_{\substack{x\bmod u,\ y\bmod v\\ vx-uy\equiv j\pmod{uv}}}\chi_u(x)\overline{\chi_v(y)}.

Then

F(u,v;j)=1quqv∑h mod uvG(u,h)G(v,h)‾e(−jh/(uv)).F(u,v;j)=\frac{1}{\sqrt{q_uq_v}}\sum_{h\bmod uv}G(u,h)\overline{G(v,h)}e(-jh/(uv)).

At zero frequency, F(u,v;0)=0F(u,v;0)=0 unless u=vu=v, and F(u,u;0)=φ(u)F(u,u;0)=\varphi(u), where φ(u)\varphi(u) is the number of units modulo uu.

Let C=(u,v)C=(u,v) and write u=Cn1u=Cn_1, v=Cn2v=Cn_2, where (n1,n2)=1(n_1,n_2)=1. Then F(u,v;j)=0F(u,v;j)=0 unless C∣jC\mid j. For j=Ckj=Ck,

F(Cn1,Cn2;Ck)=χn1(k)χn2(−k)‾R(n1,n2)LC(n1,n2;k),F(Cn_1,Cn_2;Ck) =\chi_{n_1}(k)\overline{\chi_{n_2}(-k)} \mathcal R(n_1,n_2)L_C(n_1,n_2;k),
LC(n1,n2;k)=∑x,ymodCn2x−n1y≡k(modC)χC(x)χC(y)‾=∏pc∥CLpc.L_C(n_1,n_2;k)=\sum_{\substack{x,y\bmod C\\ n_2x-n_1y\equiv k\pmod C}}\chi_C(x)\overline{\chi_C(y)} =\prod_{p^c\parallel C}L_{p^c}.

For P=qpP=q_p and p∤n1n2p\nmid n_1n_2, the local factor is

Lpc=Pc−1χp(n1/n2)c{P−1,p∣k,−1,p∤k, 6∤c,P−2,p∤k, 6∣c.L_{p^c}=P^{c-1}\chi_p(n_1/n_2)^c \begin{cases} P-1, & p\mid k,\\ -1, & p\nmid k,\ 6\nmid c,\\ P-2, & p\nmid k,\ 6\mid c. \end{cases}

If pp divides exactly one of n1,n2n_1,n_2, the local factor is Pc−1(P−1)16∣c1p∤kP^{c-1}(P-1)1_{6\mid c}1_{p\nmid k}. On the genuine residual locus (n1,n2)=1(n_1,n_2)=1, LCL_C means the congruence sum in Equation (13.7). When LCL_C is used on all residual pairs, it instead denotes the artificial product extension of these local formulas, with the local value defined to be zero if p∣(n1,n2)p\mid(n_1,n_2). Outside the genuine residual locus this is not the original congruence sum. The genuine function and this artificial extension both satisfy ∣LC∣≤qC|L_C|\le q_C, and the extension is periodic modulo rad⁡C\operatorname{rad} C in each residual column.

Proof. Expanding both Gauss sums in the displayed Fourier transform leaves

1quqv∑x mod u,y mod vχu(x)χv(y)‾∑h mod uve(h(vx−uy−j)/(uv)).\frac1{q_uq_v}\sum_{x\bmod u,y\bmod v}\chi_u(x)\overline{\chi_v(y)} \sum_{h\bmod uv}e\bigl(h(vx-uy-j)/(uv)\bigr).

Additive orthogonality makes the inner sum quqvq_uq_v when the congruence holds and zero otherwise. If j=0j=0 and a summand is nonzero, xx and yy are units modulo uu and vv. Reducing the congruence modulo uu gives u∣vu\mid v, and reducing modulo vv gives v∣uv\mid u. Since the generators are primary, u=vu=v. The congruence then says x=y mod ux=y\bmod u and gives φ(u)\varphi(u). This argument uses the zero masks also when a local character power is principal.

The divisibility by CC is immediate. After division by CC, the congruence for j=Ckj=Ck is

n2x−n1y≡k(modCn1n2).n_2x-n_1y\equiv k\pmod{Cn_1n_2}.

Reduction modulo n1n_1 and n2n_2 gives, with zero values retained,

χn1(x)=χn1(k)χn1(n2)‾,χn2(y)‾=χn2(−k)‾χn2(n1).\chi_{n_1}(x)=\chi_{n_1}(k)\overline{\chi_{n_1}(n_2)},\qquad \overline{\chi_{n_2}(y)}=\overline{\chi_{n_2}(-k)}\chi_{n_2}(n_1).

The product of the two unit factors is R(n1,n2)\mathcal{R}(n_1,n_2). It remains to identify the multiplicity of lifts of the congruence modulo CC. This can be checked at each prime. If c=vp(C)c=v_p(C) and neither residual modulus contains pp, there is no additional lift. If, say, d=vp(n1)>0d=v_p(n_1)>0 and p∤n2p\nmid n_2, then y mod pcy\bmod p^{c} is free and the congruence uniquely determines x mod pc+dx\bmod p^{c+d} from it. Reduction modulo pcp^c is exactly the common congruence in Equation (13.7). The case p∣n2p\mid n_2 is symmetric, and this argument includes c=0c=0. The Chinese remainder theorem thus gives a bijection with the common solutions used in LCL_C, even when CC meets one residual modulus.

For the local calculation put kp=O/(p)k_p=\mathcal{O}/(p) and A=χpcA=\chi_p^c, a character of kp×k_p^\times extended by zero. Since at least one of n1,n2n_1,n_2 is a unit at pp, each solution modulo pp has Pc−1P^{c-1} lifts modulo pcp^c. If both are units and p∣kp\mid k, the unit variables are proportional and the field sum is A(n1/n2)(P−1)A(n_1/n_2)(P-1). If p∤n1n2kp\nmid n_1n_2k, put y=(k/n1)ty=(k/n_1)t and x=(k/n2)(1+t)x=(k/n_2)(1+t). The field sum becomes

A(n1/n2)∑t≠0,−1A((1+t)/t)=A(n1/n2)∑z∈kp×∖{1}A(z).A(n_1/n_2)\sum_{t\ne0,-1}A((1+t)/t) =A(n_1/n_2)\sum_{z\in k_p^\times\setminus\{1\}}A(z).

It is −A(n1/n2)-A(n_1/n_2) for nonprincipal AA and (P−2)A(n1/n2)(P-2)A(n_1/n_2) for principal AA. If p∣n1p\mid n_1 and p∤n2p\nmid n_2, the field equation forces x=k/n2x=k/n_2. For p∣kp\mid k its character is zero. For p∤kp\nmid k the remaining sum over yy is zero unless AA is principal, in which case it is P−1P-1. The other case is symmetric. This proves all local formulas on the genuine residual locus. Extending them by the stipulated zero when both residuals meet pp gives functions of the residual columns modulo pp, each of absolute value at most PcP^c. Their product proves the final assertions for the artificial extension as well; no congruence-sum identity is asserted at a newly added pair.

For some applications it is preferable to remove all primes common to the two full moduli, with their entire multiplicities. The next form leaves one common row character on each remaining product.

Lemma 13.4 (Complete-common-support correlation). Suppose u=Dau=Da, v=Ebv=Eb are primary and outside SS, with (a,b)=1(a,b)=1 and (ab,DE)=1(ab,DE)=1. Then, for every j∈Oj\in\mathcal{O},

F(Da,Eb;j)=F(D,E;j)R(a,E)R(b,D)‾R(a,b)⋅χa(j)χb(−j)‾.\begin{aligned} F(Da,Eb;j)={}&F(D,E;j)\mathcal R(a,E) \overline{\mathcal R(b,D)}\mathcal R(a,b)\\ &\hspace{8mm}\cdot\chi_a(j)\overline{\chi_b(-j)}. \end{aligned}

The moduli D,ED,E may contain any prime powers, including shared auxiliary prime factors.

Proof. At primes of aa and bb, solving the congruence in Equation (13.6) gives respectively χa(j)χa(Eb)‾\chi_a(j)\overline{\chi_a(Eb)} and χb(−j)‾χb(Da)\overline{\chi_b(-j)}\chi_b(Da). These statements remain valid when a character of jj is zero; only the displayed unit factors are inverted. At primes of DEDE change variables x′=bx mod Dx'=bx\bmod D, y′=ay mod Ey'=ay\bmod E. The congruence becomes Ex′−Dy′≡j(modDE)Ex'-Dy'\equiv j\pmod{DE} and its character factor changes by χD(b)‾χE(a)\overline{\chi_D(b)}\chi_E(a). The remaining unit factor is

χE(a)χa(E)χb(D)χD(b)χb(a)χa(b)=R(a,E)R(b,D)‾R(a,b).\frac{\chi_E(a)}{\chi_a(E)} \frac{\chi_b(D)}{\chi_D(b)} \frac{\chi_b(a)}{\chi_a(b)} =\mathcal R(a,E)\overline{\mathcal R(b,D)}\mathcal R(a,b).

All denominators here are symbols of units by the hypotheses. The Chinese remainder theorem and the definition of F(D,E;j)F(D,E;j) complete the proof.

The hypotheses of (13.9) are not removed by extending R\mathcal{R} as a bicharacter. To state exactly the extension used with Möbius inversion, fix D,E,jD,E,j and define F~D,E(a,b;j)\widetilde{F}_{D,E}(a,b;j) to be the right side of that equation for all primary a,ba,b outside SS with (ab,DE)=1(ab,DE)=1, retaining its zero symbols even when (a,b)>1(a,b)>1. For any finite coefficient array c(a,b)c(a,b) on this locus,

∑(a,b)=1c(a,b)F(Da,Eb;j)=∑a,bc(a,b)F~D,E(a,b;j)∑t∣a, t∣bμ(t).\sum_{(a,b)=1}c(a,b)F(Da,Eb;j) =\sum_{a,b}c(a,b)\widetilde F_{D,E}(a,b;j) \sum_{t\mid a,\ t\mid b}\mu(t).

Indeed the full inner divisor sum is 1(a,b)=11_{(a,b)=1}, and the two correlation expressions agree on that locus. The value of F~D,E\widetilde{F}_{D,E} elsewhere is artificial, not a formula for F(Da,Eb;j)F(Da,Eb;j). In particular the full divisor sum must be inserted before a factorwise estimate separates the two residual columns; extra common primes introduced by an individual divisor term do not become primes of the genuine D,ED,E correlation.

Marked completion and reflected row energy

The compensated low estimate and the inverse moment use the same marked completion. We establish its reflected mean square here. The low estimate will use the case with no additional squarefree label or puncture; the more general form allows the labels and masks introduced by the inverse moment’s Poisson transformations.

We retain the notation of Section 4. In particular, ideal variables have their multiplicative primary generators, the fixed excluded set SS contains the primes over 6, and every power of a residue symbol is zero on nonunits, even when its exponent is divisible by six. Element rows need not be squarefree or prime to SS.

Completed sums and product-form marks

Fix a finite index set II and pairwise disjoint lists Pi\mathcal{P}_i of primes outside SS, with qp≍Zziq_p\asymp Z^{z_i} for p∈Pip\in\mathcal{P}_i. The lists and their bounded individual coefficients ai(p)a_i(p) are independent of the current row and squarefree label. Their nominal lengths ziz_i lie in fixed bounded ranges.

Here and below a fixed puncture means a function

ρ(n)=1(n,rρ)=1,\rho(n)=1_{(n,\mathfrak r_\rho)=1},

where rρ\mathfrak r_\rho is squarefree and is required to be fixed only within the indicated current row and label sums. A bounded product of such functions has this form with rρ\mathfrak r_\rho equal to the radical of the product of their moduli. The norm of this radical will be bounded explicitly. It may depend on previously fixed outer ideals, but not on either current averaging variable.

Let ff be a squarefree ideal outside SS, with qf≍ZVq_f\asymp Z^V for a nonnegative VV in a fixed bounded range, and let k∈Ok\in\mathcal{O}. For a fixed multiplicative finite ray character ν\nu whose full zero-extended defining modulus has prime support in SS, define a(n)a(n) only for squarefree primary nn outside SS, and define Ψk(n)\Psi_k(n) for every primary nn outside SS by

a(n)=αˉ(n)γ2(n)ν(n)ρ(n),Ψk(n)=ν(n)ρ(n)χn(k)χn(f)4.a(n)=\bar\alpha(n)\gamma_2(n)\nu(n)\rho(n),\qquad \Psi_k(n)=\nu(n)\rho(n)\chi_n(k)\chi_n(f)^4.

The finite character, puncture, and all slot lists are independent of kk, ff. A fixed function on a finite ray group is always expanded into genuine group characters before this definition is used; thus ν\nu is multiplicative even when an earlier step produced a finite linear combination of characters.

For a subcollection I′⊂II' \subset I of disjoint prime lists with bounded coefficients, define its mark by

dI′(A)=∑(pi)∈∏i∈I′Pi∏i∈I′ai(pi)1pi∣A.\mathfrak d_{I'}(A)= \sum_{(p_i)\in\prod_{i\in I'}\mathcal P_i} \prod_{i\in I'}a_i(p_i)1_{p_i\mid A}.

We omit I′I' from the notation when it is understood. Because the lists are disjoint, a tuple has a squarefree product. For every fixed ϵ>0\epsilon>0, the number of tuples dividing AA is Oϵ(qAϵ)O_\epsilon(q_A^\epsilon). The coefficient in Equation (14.1) is a product of functions of the individual primes; this property, not merely the pointwise divisor bound, will be used when some slots are assigned to an extracted factor.

For a smooth annular WW, put V∗(y)=y1/2W(y)V_*(y)=y^{1/2}W(y) and define the completed marked sum

Td(X;k)=∑n sfbαˉ(n)γ2(n)Ψk(n) αˉ(b)3Ψk(b)3qn qbd(nb3)V∗(qnqb3/X).\mathcal T_{\mathfrak d}(X;k)= \sum_{\substack{n\ {\rm sf}\\b}} \frac{\bar\alpha(n)\gamma_2(n)\Psi_k(n)\, \bar\alpha(b)^3\Psi_k(b)^3}{\sqrt{q_n}\,q_b} \mathfrak d(nb^3)V_*(q_nq_b^3/X).

Both primal ideals avoid SS; they may share primes. The mark belongs to the whole index nb3nb^3. With d=1\mathfrak d=1, this is the Mellin completion on the left of Equation (5.1). The Gaussian Mellin test from that Equation is also permitted when only the completed estimate is used.

For the reflection formula we use Lemma 5.2, only for a nonzero row. Write k=ukSkgoodk=u k_S k_{\mathrm{good}} as in that Lemma. After fixing the unit, the SS-valuations modulo six, and the good row ray class, its literal sector character is

Ψ0[k](A)={ν(A)χA(ukS)R(A,kgood),A≡1(mod3), (A,S)=1,0,otherwise.\Psi_0^{[k]}(A)= \begin{cases} \nu(A)\chi_A(uk_S)\mathcal{R}(A,k_{\mathrm{good}}), & A\equiv1\pmod3,\ (A,S)=1,\\ 0, & \text{otherwise}. \end{cases}

The zero branch is evaluated before either character. The Lemma supplies one finite family and hence one common LL, with prime support SS, before the good primes vary. Write Mref=λ12L4M_{\mathrm{ref}}=\lambda^{12}L^4; the full reflection sector modulus is Mref2M_{\mathrm{ref}}^2. All good primes of kk, ff, rρ\mathfrak r_\rho remain in the local prime set, with their exponents combined modulo six and every zero retained. The fourth power at ff has no extra reciprocity sign, since R(A,f)4=1\mathcal{R}(A,f)^4=1. The puncture is the product of the local zero powers at its good primes. Thus the local presentation gives exactly Ψk(n)Ψk(b)3\Psi_k(n)\Psi_k(b)^3 on the stated primal support, including at shared good primes; no moving good prime enters LL.

Whole-index marked reflection

The next corollary adds the product-form marks to the exact reflection in Part I. Its branch data are important: an inactive marked prime is absent from the conductor, so the marked transform is not obtained by multiplying one fixed-conductor dual sum by independent local factors.

Corollary 14.1 (Completed reflection with whole-index marks). Fix an invocation of Proposition 5.1, with base local prime set P0\mathcal P_0, powers jpj_p, fixed multiplier ϕ\phi, and test VV. Put Mref=λ12L4M_{\mathrm{ref}}=\lambda^{12}L^4 for this invocation. Let Q\mathcal Q be a finite set of distinct good primes disjoint from P0\mathcal P_0. In the direct completed coefficient sum, insert the factor ∏q∈Q1q∣nb3\prod_{q\in\mathcal Q}1_{q\mid nb^3}; denote this sum by TQ(X;Ψ,V)\mathcal T_{\mathcal Q}(X;\Psi,V). It has the same normalization as Equation (14.2), with Ψk,V∗\Psi_k,V_* replaced by Ψ,V\Psi,V. The primal squarefree and cube ideals may share primes.

There is an exact finite expansion

TQ(X;Ψ,V)=∑BζQ∑0≠μ∈λ−4Od(μ)α(μ)ϑ(λ4μ)qμ∏p∈A0Bp(λ4μ)⋅∏q∈AQqq−1/2χq(λ4μ)−2V♯ ⁣(qμXqc2).\begin{aligned} \mathcal T_{\mathcal Q}(X;\Psi,V) =\sum_{\mathcal B}\zeta_{\mathcal Q} \sum_{0\ne\mu\in\lambda^{-4}\mathcal O} &\frac{d(\mu)\alpha(\mu)\vartheta(\lambda^4\mu)}{\sqrt{q_\mu}} \prod_{p\in\mathcal A_0}B_p(\lambda^4\mu)\\ &\cdot\prod_{q\in\mathcal A_{\mathcal Q}} q_q^{-1/2}\chi_q(\lambda^4\mu)^{-2} V^\sharp\!\left(\frac{q_\mu X}{q_c^2}\right). \end{aligned}

Here a branch B\mathcal{B} specifies h0 mod Lh_0\bmod L mod LL, the base active and inactive sets A0\mathcal{A}_0, I0\mathcal{I}_0, and a partition Q=AQ⊔IQ\mathcal Q=\mathcal A_{\mathcal Q}\sqcup\mathcal I_{\mathcal Q}. All base primes with jp≠0j_p\ne0 are active. Put

r=∏p∈A0∪AQp,c=cF(h0)r.r=\prod_{p\in\mathcal A_0\cup\mathcal A_{\mathcal Q}}p, \qquad c=c_F(h_0)r.

The base factors BpB_p and the canonical functions d,ϑd,\vartheta are those of Proposition 5.1 for this active radical. With every σp,ϵp,ωp,j\sigma_p,\epsilon_p,\omega_{p,j} computed using this branch’s whole cc, the scalar is

ζQ=−i81αˉ(c)2ϕ^(h0)κˉF∏p∈I0(1−qp−1)∏q∈IQqq−1⋅∏p∈A0χp(σp)−2ωp,jp∏q∈AQχq(σq)−2(−ωq,0).\begin{aligned} \zeta_{\mathcal Q}={}&-\frac{i}{81}\bar\alpha(c)^2 \widehat\phi(h_0)\bar\kappa_F \prod_{p\in\mathcal I_0}(1-q_p^{-1}) \prod_{q\in\mathcal I_{\mathcal Q}}q_q^{-1}\\ &\cdot\prod_{p\in\mathcal A_0}\chi_p(\sigma_p)^{-2}\omega_{p,j_p} \prod_{q\in\mathcal A_{\mathcal Q}} \chi_q(\sigma_q)^{-2}(-\omega_{q,0}). \end{aligned}

In particular ∣ζQ∣≤1/81|\zeta_{\mathcal Q}|\le1/81. The functions d,ϑd,\vartheta and the scalar κF\kappa_F have the canonical dependence on h0h_0 and rr mod r mod Mref2r\bmod M_{\rm ref}^2 from Part I. Every dual sum is absolutely convergent and has the same full source support as there. If a marked prime instead belongs to the base local set, the corresponding primal term is identically zero and is removed before this formula is used.

Proof. For every good prime and every A∈OA\in\mathcal{O}, the zero convention gives the pointwise identity 1q∣A=1−χq(A)01_{q\mid A}=1-\chi_q(A)^0. Expand its product over Q\mathcal Q, and apply Proposition 5.1 to each of the resulting finitely many completed sums. For a fixed h0h_0 and active radical, the Proposition uses the same cF,c,d,ϑ,κFc_F,c,d,\vartheta,\kappa_F, other local phases, and kernel whether an absent prime is omitted from the local set or included with exponent zero in its inactive branch. Thus the two inactive contributions at qq combine with coefficient 1−(1−qq−1)=qq−11-(1-q_q^{-1})=q_q^{-1}. The active contribution comes only from the subtracted zero-mask transform and has local factor qq−1/2χq(λ4μ)−2q_q^{-1/2}\chi_q(\lambda^4\mu)^{-2} and scalar −ωq,0=τq,2+χq(ϵq)−2-\omega_{q,0}=\tau_{q,2}^{+}\chi_q(\epsilon_q)^{-2}. Collecting these choices at all marked primes proves (14.3) and (14.4). The inactive prime is absent from rr, hence from that branch’s conductor and kernel scale. This is finite inclusion-exclusion between compatible branches, not a new theta identity.

If a marked prime is a base local prime, the mark forces it to divide nb3nb^3, while the zero-extended base factor at that prime then vanishes, including for exponent zero. This proves the last assertion without any division of a zero symbol. It also covers the case where the primal squarefree and cube ideals share the marked prime. □

For the row norm, the phase consequence of this corollary must be stated with its exact scope. For distinct active good primes p,qp,q, Equation (5.17) and cubic reciprocity give

χp(q)2jp+2χq(p)2jq+2=(qp)3jp+jq+2.\chi_p(q)^{2j_p+2}\chi_q(p)^{2j_q+2}=\left(\frac{q}{p}\right)_3^{j_p+j_q+2}.

For an active mark the exponent is jq=0j_q=0; its changed sign occurs only in its one-prime scalar. A residual row prime with jp=1j_p=1 and a marked prime therefore have pair factor (q/p)33=1(q/p)_3^3=1. A jp=1j_p=1 row prime and a moving jq=4j_q=4 prime would instead leave (q/p)3(q/p)_3, which need not be one. All nonresidual base primes, especially every j=4j=4 prime, are therefore fixed before the inner row norm.

Write RR for the product of the residual j=1j=1 row primes and PP for the product of active marked primes. Primal row-mark collisions are removed first by the last assertion of the corollary, and are subsequently represented by 1(P,R)=11_{(P,R)=1}. If the frozen active base product is FactF_{\mathrm{act}}, then r=FactRPr=F_{\mathrm{act}}RP. Fix separate classes of RR and PP modulo the full Mref2M_{\mathrm{ref}}^2, not merely their product and not merely their smaller reciprocity classes. This fixes the cusp data without adding a pair-dependent restriction. Row-row phases are row scalars, mark-mark phases are tuple scalars, and their interactions with frozen primes depend on only one of those sets. The angular conductor scalar factors in the same way.

After fixing the dual unit, its λ\lambda-valuation, and extracted frozen factors, write the remaining dual part as nb3nb^{3}. The moving columns are exactly

χR(nb3)3=χR(nb)3,χP(nb3)−2=χP(n)−21(P,b)=1.\chi_{R}(nb^{3})^{3}=\chi_{R}(nb)^{3},\qquad\chi_{P}(nb^{3})^{-2}=\chi_{P}(n)^{-2}1_{(P,b)=1}.

These identities include every zero. A zero caused by a row or a tuple meeting an extracted frozen factor is a fixed restriction on that row or tuple. The source coefficient, fixed additive factor, and all frozen local column factors are functions of the full extracted dual index alone. Hence, after common smooth separation, the tuple coefficient may be a general bounded function of the tuple independent of R,n,bR,n,b, while the dual coefficient is independent of R,PR,P. The earlier product form of the marks remains required when slots are assigned to extracted factors.

A quadratic–cubic norm estimate

Part I established the required orientation of Goldmakher–Louvel’s quadratic large sieve and proved the zero-preserving completed reduction in Lemma 5.5. We add Heath–Brown’s cubic large sieve:

∑a≡1 (3)qa≤U∗∣∑b≡1 (3)qb≤V∗cb(ba)3∣2≪ϵ(UV)ϵ{U+V+(UV)2/3}∑b∗∣cb∣2,\sum_{\substack{a\equiv1\ (3)\\q_a\le U}}^{*} \left|\sum_{\substack{b\equiv1\ (3)\\q_b\le V}}^{*} c_b\left(\frac ba\right)_3\right|^2 \ll_\epsilon (UV)^\epsilon \{U+V+(UV)^{2/3}\}\sum_b^{*}|c_b|^2,

where both stars mean squarefree in O\mathcal{O}, and the coefficients are arbitrary complex numbers [17 Theorem 2]. The indices need not have squarefree rational norm, and there is no exclusion of rational prime factors. Conjugation and cubic reciprocity allow the opposite orientation. In this sieve and (5.26), a fixed restriction on the row set decreases the positive outer sum. A fixed restriction on the coefficient support is instead implemented by setting the omitted coefficients to zero and applying the same theorem; no column-support monotonicity is claimed. This observation does not allow an arbitrary pair-dependent mask; the next lemma resolves the two such masks that it uses.

Lemma 14.2 (A quadratic–cubic norm bound). Let K,N,B,L≥1K,N,B,L\ge1. Let k,n,Pk,n,P be squarefree primary ideals with qk≪Kq_k\ll K, qn≍Nq_n\asymp N, and qP≍Lq_P\asymp L; let bb be any primary ideal with qb≍Bq_b\asymp B. The ideals k,Pk,P avoid the current excluded set SS; additional fixed exclusions are allowed. The source ideals n,bn,b may contain primes of SS other than λ\lambda. Let a(P)a(P) and β(n,b)\beta(n,b) satisfy

∣a(P)∣≤1,∣β(n,b)∣≤1.|a(P)|\le1,\qquad|\beta(n,b)|\le1.

Here aa is independent of k,n,bk,n,b, and β\beta is independent of k,Pk,P. Then

∑k∣∑Pa(P)qP1(P,k)=1∑n,bβ(n,b)χk(nb)3χP(n)−21(P,b)=1∣2≪ε(KNBL)ε(K+NB)B{N+L+(NL)2/3}.\sum_k\left|\sum_P\frac{a(P)}{\sqrt{q_P}}1_{(P,k)=1}\sum_{n,b}\beta(n,b)\chi_k(nb)^3\chi_P(n)^{-2}1_{(P,b)=1}\right|^2 \ll_{\varepsilon}(KNBL)^{\varepsilon}(K+NB)B\{N+L+(NL)^{2/3}\}.

Fixed restrictions on the kk-set and fixed restrictions on the (n,b)(n,b)- or PP-supports are allowed, as are fixed ray sectors. All such restrictions must preserve the two coefficient-independence conditions above. Divisor-bounded multiplicities may be included if they preserve those conditions; otherwise they must first be removed by the divisor Cauchy inequalities in the proof.

Proof. Write H\mathcal{H} for the left side of (14.7). First remove the complete moving row-mark mask:

1(P,k)=1=∑D∣(P,k)μ(D).1_{(P,k)=1}=\sum_{D\mid(P,k)}\mu(D).

For each row the number of such divisors is at most dO(k)d_{\mathcal O}(k). Rowwise divisor Cauchy, followed by the positive sum over rows, therefore costs a permitted factor (KNBL)ε(KNBL)^{\varepsilon}. In a fixed DD-summand write P=DP′P=DP' and k=Dk′k=Dk'. Squarefreeness gives the fixed restrictions (D,P′)=(D,k′)=1(D,P')=(D,k')=1. Define

aD(P′)=a(DP′)1(D,P′)=1,a_D(P')=a(DP')1_{(D,P')=1},
βD(n,b)=β(n,b)χD(nb)3χD(n)−21(D,b)=1.\beta_D(n,b)=\beta(n,b)\chi_D(nb)^3\chi_D(n)^{-2}1_{(D,b)=1}.

All these factors retain their zeros and ∣βD∣≤1|\beta_D|\le1. Factoring qP−1/2=qD−1/2qP′−1/2q_P^{-1/2}=q_D^{-1/2}q_{P'}^{-1/2} gives

H≪(KNBL)ε∑D1qD∑k′∣∑n,bβD(n,b)χk′(nb)3∑P′aD(P′)qP′χP′(n)−21(P′,b)=1∣2.\mathcal{H}\ll(KNBL)^{\varepsilon}\sum_D\frac{1}{q_D}\sum_{k'}\left|\sum_{n,b}\beta_D(n,b)\chi_{k'}(nb)^3\sum_{P'}\frac{a_D(P')}{\sqrt{q_{P'}}}\chi_{P'}(n)^{-2}1_{(P',b)=1}\right|^2.

Here qk′≪K/qDq_{k'}\ll K/q_D, qP′≍L/qDq_{P'}\asymp L/q_D, and all inherited fixed restrictions are retained. The outer DD’s are the squarefree good divisors allowed by the split, so qD≪min⁡(K,L)q_D\ll\min(K,L). In particular, no (P′,k′)(P',k') mask is reinstated inside an individual DD-summand. Its cancellation belongs to the complete Möbius sum already bounded by rowwise Cauchy.

For fixed DD, the product of βD(n,b)\beta_D(n,b) and the inner P′P'-sum is an arbitrary complex coefficient independent of k′k'. Apply Equation (5.27) with row length K/qDK/q_D. Use its notation

b=gt2,c=(n,g),n=cm,g=ch,qc≍C,qg≍G,qt≍T,b=gt^2,\qquad c=(n,g),\qquad n=cm,\qquad g=ch,\qquad q_c\asymp C,\qquad q_g\asymp G,\qquad q_t\asymp T,

so B≍GT2B\asymp GT^2, and write c=rc′c=rc' for its complete cc-mask divisor. The ideals c,m,hc,m,h are pairwise coprime and squarefree; no coprimality between gg and tt is imposed. The cited reduction already includes the natural k′k'-tt restriction and the complete Möbius expansion of the k′k'-cc mask. It does not reinstate a mask between the remaining row and c′c'.

For one C,G,TC,G,T block its positive output, inserted in Equation (14.8), is at most

(KNBL)ϵ∑D1qDT∑qt≍T∑r sf, (r,S)=1qr≪min⁡(K/qD,C){KqDqr+NGC2}Cqr∑c′,m,h∣βD(rc′m,rc′ht2)∣2(KNBL)^\epsilon\sum_D\frac1{q_D}T\sum_{q_t\asymp T} \sum_{\substack{r\ {\rm sf},\ (r,S)=1\\q_r\ll\min(K/q_D,C)}} \left\{\frac K{q_Dq_r}+\frac{NG}{C^2}\right\}\frac C{q_r} \sum_{c',m,h}|\beta_D(rc'm,rc'ht^2)|^2
⋅∣∑P′aD,r(P′)qP′χP′(c′m)−21(P′,ht)=1∣2,\quad\cdot\left| \sum_{P'}\frac{a_{D,r}(P')}{\sqrt{q_{P'}}} \chi_{P'}(c'm)^{-2}1_{(P',ht)=1} \right|^2,

where the positive c′,m,hc',m,h-sum keeps the original support and

aD,r(P′)=aD(P′)χP′(r)−2.a_{D,r}(P')=a_D(P')\chi_{P'}(r)^{-2}.

The factorization used here is, including all zeros,

χP′(rc′m)−21(P′,rc′ht2)=1=χP′(r)−2χP′(c′m)−21(P′,ht)=1.\chi_{P'}(rc'm)^{-2}1_{(P',rc'ht^2)=1}=\chi_{P'}(r)^{-2}\chi_{P'}(c'm)^{-2}1_{(P',ht)=1}.

The character already supplies the missing zeros at rr, c′c', and mm. Thus the rr-factor is tuple-only, including its zero when (P′,r)≠1(P',r)\ne1. The fixed DD-phases remain inside βD\beta_D until this positive bound. The quadratic reduction has already separated the finitely many squarefree SS-parts of m,hm,h before sieving their good product; m,hm,h in Equation (14.9) are the original ideals.

We may now discard ∣βD∣2≤1|\beta_D|^2\le1. For fixed h,t,D,rh,t,D,r, the P′P'-coefficients are independent of j=c′mj=c'm, and ideal counting gives

∑P′∣aD,r(P′)∣21(P′,ht)=1qP′≪ε(KNBL)ε.\sum_{P'}\frac{|a_{D,r}(P')|^2 1_{(P',ht)=1}}{q_{P'}}\ll_{\varepsilon}(KNBL)^{\varepsilon}.

The product j=c′m=n/rj=c'm=n/r is squarefree primary and has norm O(N/qr)O(N/q_r). It may contain a permitted prime of SS other than λ\lambda, since only the quadratic column was stripped of its fixed SS-part. Grouping c′,mc',m by jj costs at most a divisor factor. Enlarge only this positive squarefree jj-range. Cubic reciprocity, conjugation, and Equation (14.6), followed by the O(G/C)O(G/C) choices of hh, give, on qD≍D0q_D \asymp D_0, qr≍r0q_r \asymp r_0,

(KNBL)εGC{Nr0+LD0+(NLr0D0)2/3}.(KNBL)^{\varepsilon}\frac{G}{C}\left\{\frac{N}{r_0}+\frac{L}{D_0}+\left(\frac{NL}{r_0D_0}\right)^{2/3}\right\}.

The fixed mask at htht is a coefficient restriction in this cubic sieve, not a row-dependent mask. The reduction supplies T∑tT\sum_t, with O(T)O(T) possible tt, and the factor C/qrC/q_r. Together with the hh-count, these contribute

T2(C/r0)(G/C)≍B/r0.T^2(C/r_0)(G/C)\asymp B/r_0.

There are O(r0)O(r_0) possible rr in its dyad, while the sum of qD−1q_D^{-1} over its dyad is O(1)O(1), up to a permitted small power. Both sieve factors increase when D0,r0D_0,r_0 are replaced by 1, and NG/C2≪NBNG/C^2\ll NB. Summing the logarithmically many dyads proves Equation (14.7). Subunit quotient ranges are empty, and bounded ranges are included by changing the fixed annular constants. This argument has introduced neither a (g,t)=1(g,t)=1 condition nor a new pair-dependent mask.

The reflected energy bound

We next quantify the reflection of Equation (14.2). The following description also specifies the dyadic contribution used in the statement.

Reflected block data. Fix f,ρf,\rho and put Q=log⁡ZqrρQ=\log_Zq_{\mathfrak r_\rho}. For an element row 0<qk≪ZM0<q_k\ll Z^M, define the maximal powerful part of its ideal by

kpow=∏vp(k)≥2pvp(k).k_{\mathrm{pow}}=\prod_{v_p(k)\ge2}p^{v_p(k)}.

Split the valuation-one primes into the squarefree product ksupk_{\mathrm{sup}} supported on S∪supp⁡(frρ)S\cup\operatorname{supp}(f\mathfrak r_\rho) and the squarefree product kresk_{\mathrm{res}} outside that set. These three prime supports are pairwise disjoint, and their product is the ideal of kk. A powerful ideal here means that every positive prime valuation is at least two. Fix the unit of kk. Insert smooth dyadic partitions in

qkpow≍ZO,qkres≍ZH.q_{k_{\mathrm{pow}}}\asymp Z^O,\qquad q_{k_{\mathrm{res}}}\asymp Z^H.

Choose these ideal centers nonnegative, with center zero for the unit dyad. In particular, an actual annular factor χrow(qkres/ZH)\chi_{\mathrm{row}}(q_{k_{\mathrm{res}}}/Z^H) is kept in the row sum. The bounded dyad includes kres=1k_{\mathrm{res}}=1. Choose fixed constants Ck,CO,CH≥1C_k,C_O,C_H\ge1, from these supports, such that

qk≤CkZM,qkpow≥ZO/CO,qkres≥ZH/CH.q_k\le C_kZ^M,\qquad q_{k_{\mathrm{pow}}}\ge Z^O/C_O,\qquad q_{k_{\mathrm{res}}}\ge Z^H/C_H.

Since qksup≥1q_{k_{\mathrm{sup}}}\ge1, the general norm inequality Equation (5.35) gives here

H≤M−O+log⁡Creslog⁡Z,Cres=CHCkCO.H\le M-O+\frac{\log C_{\mathrm{res}}}{\log Z},\qquad C_{\mathrm{res}}=C_HC_kC_O.

The inequality need not be an equality, because ksupk_{\mathrm{sup}} may have positive norm length. Freeze the actual ideals kpow,ksupk_{\mathrm{pow}},k_{\mathrm{sup}}. At every prime outside SS, combine the local exponents of ρ(n)χn(k)χn(f)4\rho(n)\chi_n(k)\chi_n(f)^4 modulo six, always retaining the zero extension. The primes of kresk_{\mathrm{res}} have exponent j=1j=1. All other such primes, including every non-slot prime of exponent j=4j=4, are now fixed. In the reflection formula call a prime active when it occurs in cc. For a fixed choice of the active zero-exponent primes and a fixed splitting of each j=4j=4 Ramanujan factor, let: A0A_0 be the log-norm of all active non-slot primes outside kresk_{\mathrm{res}}, S0S_0 be the log-norm of the small Ramanujan terms and active zero-mask terms among them, N0N_0 be the log-norm of the j=4j=4 divisibility terms assigned to the squarefree dual ideal, B0B_0 be the log-norm of the j=4j=4 divisibility terms assigned to the cube ideal but not the squarefree ideal.

Here a log-norm is log⁡Z\log_Z of the norm of the indicated product. The assignment uses 1p∣nb3=1p∣n+1p∤n1p∣b1_{p\mid nb^3}=1_{p\mid n}+1_{p\nmid n}1_{p\mid b}. Let za=∑i activeziz_a=\sum_{i\ {\rm active}}z_i be the sum of their nominal slot lengths. The product of the active primes has norm divided by ZzaZ^{z_a} in a fixed compact interval, including for zero nominal lengths or the empty list. After extracting the forced squarefree and cube primes, restrict the remaining dual ideals to

qn≍Zv,qb≍Zℓb,qλhλ=Zeλ.q_n\asymp Z^v,\qquad q_b\asymp Z^{\ell_b},\qquad q_{\lambda^{h_\lambda}}=Z^{e_\lambda}.

Choose the ideal centers v,ℓbv,\ell_b nonnegative. These are source dual ideals: they retain every prime of SS permitted by Equation (5.2); no extra SS-mask is placed on them. Only the displayed λ\lambda-valuation support is imposed. The unit and the integer hλ≥−4h_\lambda\geq-4 are fixed in this dyad. For these choices, denote by Uv,ℓb,eλ(kres)\mathcal U_{v,\ell_b,e_\lambda}(k_{\rm res}) the right side of Equation (14.3), summed with the product-form tuple coefficients, with the specified local choices and dual restrictions, and the actual factor χrow(qkres/ZH)\chi_{\mathrm{row}}(q_{k_{\mathrm{res}}}/Z^H). Active slot tuples are still summed in this definition. This definition is made separately for each fixed powerful and supported row part and each sector obtained by fixing separate classes of the residual row product and active slot product modulo the full reflection modulus Mref2M_{\mathrm{ref}}^2.

Lemma 14.3 (Reflected energy). Retain the reflected block data above. Let Z≥2Z\geq2, and suppose their log-lengths range over fixed bounded sets. In the completed sum of Equation (14.2), the fixed character, puncture, and slot coefficients are independent of kk, ff, the slot supports are disjoint, and the slot coefficients are products as in Equation (14.1). The fixed row restrictions after freezing kpow,ksupk_{\mathrm{pow}},k_{\mathrm{sup}} must be independent of the active slots and dual variables, apart from the explicit zero mask 1(P,kres)=11_{(P,k_{\rm res})=1}. Fix a small τref>0\tau_{\mathrm{ref}}>0, put X=ZN∗X=Z^{N_*}. Define TdT_d and call a dyad retained by the following formula:

Td=2H+2A0+2za−N∗−N0−3B0,T_d=2H+2A_0+2z_a-N_*-N_0-3B_0,
v+3ℓb+eλ≤Td+τreffor a retained dyad.v+3\ell_b+e_\lambda\le T_d+\tau_{\rm ref} \quad\text{for a retained dyad}.

Terms with

v+3ℓb+eλ>Td+τrefv+3\ell_b+e_\lambda>T_d+\tau_{\mathrm{ref}}

have arbitrarily small total size, with a fixed polynomial height cost, after a sufficiently far kernel contour shift and a threshold for ZZ depending only on the fixed support intervals and τref\tau_{\mathrm{ref}}. Every retained dyad has coefficient exponent, per active tuple,

−v/2−ℓb−eλ/3−(S0+B0+za)/2.-v/2-\ell_b-e_\lambda/3-(S_0+B_0+z_a)/2.

Define

u=min⁡{v,za,(v+za)/3}.u=\min\{v,z_a,(v+z_a)/3\}.

and

Eref=O/2+max⁡(H,v+ℓb)−S0−B0+za−u−ℓb−2eλ/3−12(Td−v−3ℓb−eλ)+.\begin{aligned} E_{\rm ref}={}&O/2+\max(H,v+\ell_b)-S_0-B_0+z_a-u-\ell_b -2e_\lambda/3\\ &-\tfrac12(T_d-v-3\ell_b-e_\lambda)_+. \end{aligned}

For every ϵ>0\epsilon>0, the contribution with fixed kpow,ksupk_{\mathrm{pow}},k_{\mathrm{sup}} satisfies

∑kres sf∣Uv,ℓb,eλ(kres)∣2≪ZEref−O/2+ϵ.\sum_{k_{\rm res}\ {\rm sf}} |\mathcal U_{v,\ell_b,e_\lambda}(k_{\rm res})|^2 \ll Z^{E_{\rm ref}-O/2+\epsilon}.

Summing the fixed parts in their OO-dyad and the local choices changes this to O(ZEref+ϵ)O(Z^{E_{\mathrm{ref}}+\epsilon}). The bounds are uniform in the moving ideals and punctures in the stated ranges, with finitely many smooth seminorms and a fixed polynomial cost for norm-twist heights. The negative value of eλe_{\lambda}, when present, is O(1/log⁡Z)O(1/\log Z). In particular, the formula is used only on actual residual-row dyads satisfying Equation (5.35).

Proof. First remove the inactive slots by triangle inequality in the row Hilbert space. At such a slot the absolute coefficient mass is

∑p∈Piqp−1≪ϵZϵ,\sum_{p\in\mathcal{P}_i}q_p^{-1}\ll_{\epsilon} Z^{\epsilon},

uniformly under any fixed restriction, including for a bounded or zero-length list. It therefore suffices to prove a uniform bound with those primes fixed. Each such branch has its own conductor, cusp sector, and kernel scale, with the inactive prime absent from the conductor. Its earlier collision exclusion is now a fixed row restriction.

Fix ff, ρ\rho, kpowk_{\mathrm{pow}}, ksupk_{\mathrm{sup}}, the non-slot local choices, h0h_0, and separate classes of the residual row product and active slot product modulo the full Mref2M_{\mathrm{ref}}^2. Also fix the unit and ramified exponent of the dual index. No non-slot j=4j=4 label remains averaged. We use only the algebraic frozen-base extraction in Equation (5.32), inside the original sum over active tuples. Corollary 14.1 and the subsequent phase separation make that extraction simultaneous across the tuples: the base coefficient is common to the residual rows and tuples after their separate sectors are fixed, while the remaining scalar separates into a row factor and a tuple factor. We do not apply the numerical unmarked estimate separately to each tuple.

The structural extraction gives the common central coefficient

Z−v/2−ℓb−eλ/3−(S0+B0)/2Z^{-v/2-\ell_b-e_{\lambda}/3-(S_0+B_0)/2}

times normalized inverse-root factors and bounded coefficients. Its N0N_0-assignment extracts a forced j=4j=4 prime only from the squarefree dual ideal, even if the cube ideal shares it; the entire shared cube part remains in its residual norm and coefficient. Its B0B_0-assignment extracts one occurrence from the cube ideal and leaves the factor qp−1/2q_p^{-1/2}. These are statements about the full source support, including the permitted primes of SS. Every active marked column in Equation (14.3) contributes qp−1/2q_p^{-1/2}. Since qP/Zzaq_P/Z^{z_a} lies in a fixed compact interval, this proves the per-tuple coefficient exponent in Equation (14.12).

We now record the precise marked instance of the common profile. Let FactF_{\mathrm{act}}, NFN_F, BFB_F be the actual frozen products with log-norms A0A_0, N0N_0, B0B_0. Put R=kresR=k_{\mathrm{res}}, P=∏i activepiP=\prod_{i\ \mathrm{active}}p_i. The branch denominator and a supported dual index are

c=cFFactRP,μ=uλhλNFn(BFb)3.c=c_FF_{\rm act}RP,\qquad \mu=u\lambda^{h_\lambda}N_Fn(B_Fb)^3.

With the fixed block centers, define

yR=qR/ZH,yn=qn/Zv,yb=qb/Zℓb,yi=qpi/Zzi,y_R=q_R/Z^H,\qquad y_n=q_n/Z^v,\qquad y_b=q_b/Z^{\ell_b},\qquad y_i=q_{p_i}/Z^{z_i},
Y=qλhλNFBF3XZvZ3ℓbqcFFact2Z2H∏i activeZ2zi=qcF−2Zv+3ℓb+eλ−Td.Y=\frac{q_{\lambda^{h_\lambda}N_FB_F^3}X Z^vZ^{3\ell_b}} {q_{c_FF_{\rm act}}^2Z^{2H}\prod_{i\ {\rm active}}Z^{2z_i}} =q_{c_F}^{-2}Z^{v+3\ell_b+e_\lambda-T_d}.

Multiplicativity gives the exact identity

qμXqc2=Yynyb3yR−2∏i activeyi−2.\frac{q_{\mu}X}{q_c^2}=Yy_ny_b^3y_R^{-2}\prod_{i\ \mathrm{active}}y_i^{-2}.

It remains true if NFN_F shares primes with bb. All frozen factors in YY are their actual products, and every moving norm remains a coordinate. The actual row cutoff and the individual dual and slot cutoffs therefore place the kernel argument in

[Cker−1,Cker]Zv+3ℓb+eλ−Td[C_{\mathrm{ker}}^{-1},C_{\mathrm{ker}}]Z^{v+3\ell_b+e_{\lambda}-T_d}

for one Cker≥1C_{\mathrm{ker}} \ge1 depending only on the fixed support intervals and the common fixed modulus. In particular this comparison has not used any shorter row added by positivity.

Put Dker=Td−v−3ℓb−eλD_{\mathrm{ker}}=T_d-v-3\ell_b-e_\lambda. On this full product of actual annuli, Lemma 5.3 permits

mker=Z−(Dker)+/4m_{\mathrm{ker}}=Z^{-(D_{\mathrm{ker}})_+/4}

to be factored from the entire homogeneous linear row vector, at a factor at most Cker1/4C_{\mathrm{ker}}^{1/4} in its fixed seminorm constants. The normalized profile has bounded fixed Euler seminorms; no inhomogeneous tuple seminorm is claimed to become small. The profile includes the normalized inverse roots from the structural extraction and every other common smooth norm window.

The tail is removed on the genuine, unseparated sums. If log⁡Z≥2log⁡Cker/τref\log Z \ge2\log C_{\mathrm{ker}}/\tau_{\mathrm{ref}}, every whole dyad with center excess greater than τref\tau_{\mathrm{ref}} has actual kernel argument greater than Zτref/2Z^{\tau_{\mathrm{ref}}/2}. Apply Lemma 5.4 with lattice λ−4O\lambda^{-4}\mathcal{O}, a=X/qc2a=X/q_c^2, and U=Zτref/2U=Z^{\tau_{\mathrm{ref}}/2}. On the full source support, the coefficient bound used in Part I gives

∣d(μ)∣/qμ≤27qλ4/3.\lvert d(\mu)\rvert/\sqrt{q_\mu}\le27q_\lambda^{4/3}.

Each base or marked local factor is at most qp1/2q_p^{1/2} after its indicator is discarded. The bounded row, tuple, and local log-length ranges, the local branch counts, and 1+a−11+a^{-1} have a fixed polynomial cost ZBtailZ^{B_{\mathrm{tail}}}, with BtailB_{\mathrm{tail}} chosen independently of the kernel order. For any desired saving D>0D>0, the choice

A>1+2(Btail+D)τrefA>1+\frac{2(B_{\mathrm{tail}}+D)}{\tau_{\mathrm{ref}}}

in that shell lemma makes the absolute total of these whole dyads O(Z−D)O(Z^{-D}) times a finite test seminorm. Norm twists have the fixed polynomial height cost of that seminorm. The shell sum counts all discarded dual indices, so no count at a retained dual length is used for this tail. It is removed before Fourier absolutization.

For a retained dyad, apply the common-profile lemma and Equation (5.24) to the one joint profile in Equation (14.15). Its density is common to the entire current row Hilbert space, including the active-tuple sum: the actual row, dual, and individual slot norms are its coordinates, not parameters of separately chosen measures. The full fixed support boxes govern every invoked weighted Fourier norm and height cost. At a separated mode the norm powers have absolute value one and preserve the row, tuple, and dual coefficient independences. Only inside this separated nonnegative row norm may the row set be enlarged from the original annulus to qR≪ZHq_R\ll Z^H, using the same separated formula on the added rows. The kernel is never evaluated there.

After extracting the common coefficient but before using mker2m_{\mathrm{ker}}^2, the separated squared norm is bounded by

Z−v−2ℓb−2eλ/3−S0−B0+εN,Z^{-v-2\ell_b-2e_\lambda/3-S_0-B_0+\varepsilon}\mathcal{N},

where

N=∑kres sfqkres≪ZH∣∑pa(p)qP1(P,kres)=1∑n sfbβ(n,b)χkres(nb)3χP(n)−21(P,b)=1∣2,\mathcal N={} \sum_{\substack{k_{\rm res}\ {\rm sf}\\q_{k_{\rm res}}\ll Z^H}} \left| \sum_{\boldsymbol p} \frac{a(\boldsymbol p)}{\sqrt{q_P}}1_{(P,k_{\rm res})=1} \sum_{\substack{n\ {\rm sf}\\b}} \beta(n,b)\chi_{k_{\rm res}}(nb)^3 \chi_P(n)^{-2}1_{(P,b)=1} \right|^2,
P=∏i activepi,qP≍Zza.P=\prod_{i\ {\rm active}}p_i,\qquad q_P\asymp Z^{z_a}.

The ideals n,bn,b retain their stated dyadic norms and fixed coefficient restrictions. After extracting common bounds, ∣a(p)∣,∣β(n,b)∣≤1|a(\boldsymbol p)|,|\beta(n,b)|\le1.

We verify the two independence hypotheses before invoking the norm bound. Every residual prime has exponent j=1j=1, every active slot is a whole-index j=0j=0 mark, and all other active primes are frozen. The separate full Mref2M_{\mathrm{ref}}^2 classes fix the cusp coefficient and additive factor. Equation (14.5) cancels every row-slot phase, while the preceding marked-reflection discussion assigns all row-row, slot-slot, and frozen interactions to a row scalar or a tuple scalar. The angular conductor scalar separates in the same fashion. The remaining source and frozen local columns depend only on the full extracted dual index; their zeros at a frozen factor give fixed row, tuple, or dual restrictions. Finally the exact zero-preserving column identities leave only 1(P,kres)=11_{(P,k_{\rm res})=1} and 1(P,b)=11_{(P,b)=1} in addition to the character zeros. Hence aa is independent of kres,n,bk_{\mathrm{res}},n,b, and β\beta is independent of kres,pk_{\mathrm{res}},\mathbf{p}, exactly as required in (14.16). The function aa need not retain product form at this norm step.

Apply Lemma 14.2 with

K=ZH,N=Zv,B=Zℓb,L=Zza.K=Z^H,\qquad N=Z^v,\qquad B=Z^{\ell_b},\qquad L=Z^{z_a}.

Aggregating tuples with the same PP costs only a divisor factor. Since

v+za−u=max⁡{v,za,2(v+za)/3},v+z_a-u=\max\{v,z_a,2(v+z_a)/3\},

the hybrid bound and the outside coefficient give exponent

max⁡(H,v+ℓb)−S0−B0+za−u−ℓb−2eλ/3.\max(H,v+\ell_b)-S_0-B_0+z_a-u-\ell_b-2e_\lambda/3.

Only now does the squared scalar mker2m_{\mathrm{ker}}^2 supply the last term in (14.14). This proves the fixed-part assertion.

Every powerful ideal is uniquely x2y3x^2y^3 with yy squarefree. Ideal counting and ∑yqy−3/2<∞\sum_y q_y^{-3/2}<\infty give O(ZO/2)O(Z^{O/2}) such ideals in the OO-dyad. The supported squarefree part divides the radical of SfrρS f\mathfrak r_\rho, so it has O(Zϵ)O(Z^{\epsilon}) choices in the stated ranges; the local choices have the same divisor bound. Rowwise divisor Cauchy on the local expansion followed by the positive sum over these fixed parts therefore adds O/2+ϵO/2+\epsilon once. The active tuples were already inside the hybrid norm and are not counted again. This proves the aggregate assertion.

The dependence on the original row length can be bounded without identifying HH with M−OM-O. At one active non-slot prime the contribution to 2A0−N0−S0−4B02A_0-N_0-S_0-4B_0 is as follows:

local choicecoefficient of its log-norm
jj odd, or j=2j=222
j=0j=0 active11
j=4j=4 small or assigned to nn11
j=4j=4 assigned to bb−2-2
j=0j=0 inactive00

A residual row prime contributes two through 2H2H. Prime by prime, these coefficients are bounded by the valuations in

(qk2/qkpow) qfqrρ.(q_k^2/q_{k_{\rm pow}})\,q_fq_{\mathfrak r_\rho}.

Indeed, a powerful prime of row valuation e≥2e\ge2 has valuation ee in the first factor, a squarefree row prime has valuation two, and a prime belonging only to the squarefree ff or to rρ\mathfrak r_\rho has valuation one. Intersections only increase the valuation of this upper bound. Fixed excluded primes contribute only a fixed factor CS≥1C_S\ge1. Equivalently, summing over primes gives the actual norm inequality

qkres2Z2A0−N0−S0−4B0≤CSqk2qkpow qfqrρ.q_{k_{\rm res}}^2 Z^{2A_0-N_0-S_0-4B_0} \le C_S\frac{q_k^2}{q_{k_{\rm pow}}}\,q_fq_{\mathfrak r_\rho}.

Choose a fixed Cf≥1C_f\ge1 with qf≤CfZVq_f\le C_f Z^V, and put Cwidth=CH2CSCk2COCfC_{\mathrm{width}}=C_H^2C_SC_k^2C_OC_f. The preceding inequality and the definition of TdT_d imply

Td−S0−B0≤2M−O+Q+V−N∗+2za+log⁡Cwidthlog⁡Z.T_d-S_0-B_0\le2M-O+Q+V-N_*+2z_a+\frac{\log C_{\mathrm{width}}}{\log Z}.

For empty slot lists, za=u=0z_a=u=0. Choose η>0\eta>0 and then take ZZ so large that the two displayed constant errors are at most η\eta and eλ≥−ηe_\lambda\geq-\eta; the latter follows from log⁡Z≥4log⁡qλ/η\log Z\geq4\log q_\lambda/\eta.

On a retained dyad, Equation (14.14) and v+3ℓb+eλ≤Td+τrefv+3\ell_b+e_\lambda\leq T_d+\tau_{\mathrm{ref}} give

Eref≤O/2+max⁡{H,Td−S0−B0}+53η+τref.E_{\mathrm{ref}}\leq O/2+\max\{H,T_d-S_0-B_0\}+\frac{5}{3}\eta+\tau_{\mathrm{ref}}.

For the first branch, drop the nonpositive terms after using the lower bound for eλe_\lambda; for the second, use v≤Td−3ℓb−eλ+τrefv\leq T_d-3\ell_b-e_\lambda+\tau_{\mathrm{ref}}. The maximum is increasing in each argument. We may therefore use Equation (5.35) for its first argument and Equation (14.17) for its second, then sum the logarithmically many actual HH-dyads. Taking η\eta, τref\tau_{\mathrm{ref}} and the local small-power losses sufficiently small in terms of ϵ\epsilon proves

∑0<qk≪ZM′∣T1(ZN∗;k)∣2≪ZO/2+max⁡{M−O, 2M−O+Q+V−N∗}+ϵ.\sum_{0<q_k\ll Z^M}'|\mathcal T_1(Z^{N_*};k)|^2 \ll Z^{O/2+\max\{M-O,\,2M-O+Q+V-N_*\}+\epsilon}.

The prime on the sum restricts the powerful part to its OO-dyad. A bounded dual range is included in the first term; an empty range is negligible. No equality H=M−OH=M-O has been used.

The compensated low estimate

We now bound the finite compensated probe defined in Equation (12.5). Its exact low separation has two factors. We first bound the completed row after summing the marked slots by applying Lemma 14.3 directly. We then prove a quantitative Gram bound for the additive polynomial from Section 6. Cauchy–Schwarz will combine these estimates to give the exponent 3/163/16.

The marked completed row

For a fixed rescaled subset JJ, with marked subset JcJ^c, put

d=∑i∈Jℓi,X′=X/qpJ≍XZ−d,Y′=Y/qpJ≍YZ−d,d=\sum_{i\in J}\ell_i,\qquad X'=X/q_{p_J}\asymp XZ^{-d},\qquad Y'=Y/q_{p_J}\asymp YZ^{-d},
M′=M−2d,ℓ′=ℓ−d,0≤d≤ℓ=1/6.M'=M-2d,\qquad\ell'=\ell-d,\qquad0\leq d\leq\ell=1/6.

For a squarefree product DD of slot primes, define the marked completed series

TD(s0,ψ)=∑c sfnγ2(c)α(cn3)‾ψ(cn3)1D∣cn3qc−s0qn−3s0+1/2.T_D(s_0,\psi)=\sum_{\substack{c\ {\rm sf}\\n}} \gamma_2(c)\overline{\alpha(cn^3)}\psi(cn^3) 1_{D\mid cn^3}q_c^{-s_0}q_n^{-3s_0+1/2}.

The ideals c,nc,n are the original ideals prime to SS, represented by their primary generators, with cc squarefree; they may share primes. All character powers retain their original zero extensions. For the empty product D=1D=1 this is the completed T(s0,ψ)T(s_0,\psi). For this fixed JJ, let

Bm,σJ(Z)=∑pi∈Pi(Z), i∉J∏i∉Jη(pi)‾Wi(qpi/Pi)∑θ∈T^aθ12πi∫(4)(ZqpJc)tΦ(t)⋅TpJc(t+1/2,νσθχ∙(m)) dt.\begin{aligned} B^J_{m,\sigma}(Z)= \sum_{p_i\in\mathcal P_i(Z),\ i\notin J} \prod_{i\notin J}\overline{\eta(p_i)}W_i(q_{p_i}/P_i) \sum_{\theta\in\widehat T}a_\theta\frac1{2\pi i} \int_{(4)} &(Zq_{p_{J^c}})^t\Phi(t)\\ &\cdot T_{p_{J^c}}(t+1/2, \nu_\sigma\theta\chi_\bullet(m))\,dt. \end{aligned}

Thus BJB^J is exactly the completed-row factor for the JJ summand of Equation (12.5) after the marked slots have been summed. The fixed tuple pJp_J affects only X′,Y′X',Y' in its low separation.

Lemma 15.1 (The compensated completed-row norm). For every ϵ>0\epsilon>0, every fixed rescaled subset JJ, and every σ∈T\sigma\in T, with Q=qb∗X′Y′≍ZM′Q=q_{b_*}X'Y'\asymp Z^{M'},

∑0<qm≪Q∣Bm,σJ(Z)∣2≪ZM′+((d−1/6)/4)++ϵ=ZM′+ϵ.\sum_{0<q_m\ll Q}|B^J_{m,\sigma}(Z)|^2 \ll Z^{M'+((d-1/6)/4)_++\epsilon} =Z^{M'+\epsilon}.

The bound is uniform in the fixed rescaled tuple and has no loss depending on the mesh of the surviving slots.

Proof. Put A=cn3A = cn^{3} and ϱi=qpi/Pi\varrho_i = q_{p_i}/P_i for i∉Ji \notin J. Since qA=qcqn3q_A = q_cq_n^{3} even when c,nc,n share primes, and qpJc=Zℓ′∏i∉Jϱiq_{p_{J^c}}=Z^{\ell'}\prod_{i\notin J}\varrho_i, Mellin inversion of the displayed integral defining BJB^J gives the physical smooth factor

V ⁣(qAZqpJc)=WG ⁣(r∏i∉Jϱi),r=qAZ1+ℓ′.\begin{gathered} V\!\left(\frac{q_A}{Zq_{p_{J^c}}}\right) =W_{\mathrm G}\!\left(\frac{r}{\prod_{i\notin J}\varrho_i}\right),\\ r=\frac{q_A}{Z^{1+\ell'}}. \end{gathered}

Here V=WGV=W_{\mathrm G} is the Gaussian of Lemma 4.6. Empty products are one.

Use the fixed translate partition χ\chi from that lemma on rr. On the annulus r=ekxr = e^k x, retain the single joint profile

wk,J(x,ϱ)=χ(log⁡x)WG ⁣(ekx∏i∉Jϱi)∏i∉JWi(ϱi).w_{k,J}(x,\boldsymbol\varrho) =\chi(\log x)W_{\mathrm G}\!\left( \frac{e^kx}{\prod_{i\notin J}\varrho_i}\right) \prod_{i\notin J}W_i(\varrho_i).

The logarithms of xx and of all the ϱi\varrho_i lie in fixed compact sets on this support. Thus the logarithm of the Gaussian argument is k+Ofixed(1)k + O_{\mathrm{fixed}}(1). The derivative estimate in Lemma 4.6, with this bounded shift and the fixed slot windows, gives for every fixed κG>0\kappa_{\mathrm G}>0, Acnt,Bcnt,Cann≥0A_{\mathrm{cnt}}, B_{\mathrm{cnt}}, C_{\mathrm{ann}} \ge0, Dtail>0D_{\mathrm{tail}} > 0, and fixed seminorm order jj,

∑k∈ZeAcnt∣k∣pj(wk,J)<∞,\sum_{k\in\mathbb{Z}}e^{A_{\mathrm{cnt}}|k|}p_j(w_{k,J}) < \infty,
ZBcnt∑∣k∣>κGlog⁡Z−CanneAcnt∣k∣pj(wk,J)≪Z−Dtail.Z^{B_{\rm cnt}} \sum_{|k|>\kappa_{\mathrm G}\log Z-C_{\rm ann}} e^{A_{\rm cnt}|k|}p_j(w_{k,J}) \ll Z^{-D_{\rm tail}}.

The constants may depend on the fixed slot system, but not on its moving prime labels. On an annulus log⁡r=k+O(1)\log r = k + O(1), an absolute bound for the row ℓ2\ell^2 norm is at most ZBcnteAcnt∣k∣pj(wk,J)Z^{B_{\mathrm{cnt}}}e^{A_{\mathrm{cnt}}|k|}p_j(w_{k,J}) for some fixed exponents, by the elementary row, slot, and ideal counts. Choose CannC_{\mathrm{ann}} larger than the fixed logarithmic radius of χ\chi and discard only whole annuli with ∣k∣>κGlog⁡Z+Cann|k|>\kappa_{\mathrm G}\log Z+C_{\rm ann}. Summing their norm bounds and then squaring gives less than any prescribed power of Z−1Z^{-1}. Every annulus meeting ∣log⁡Zr∣≤κG|\log_Z r|\le\kappa_{\mathrm G} is retained.

For each remaining annulus, keep fixed individual annular cutoffs equal to one on the support of wk,Jw_{k,J} and apply Lemma 4.5 to this whole profile. Its logarithmic Fourier inversion uses one coefficient density common to every row and every surviving slot tuple. The normalized slot ratios remain variables of the joint profile until separation; they do not index separately chosen densities. For fixed Fourier variables, each resulting slot coefficient is a product of the original arithmetic coefficient η(pi)‾\overline{\eta(p_i)} and an individual annular cutoff and norm power. It remains bounded and independent of the row and of every other slot. The completed factor is an annular test at length

N∗=1+ℓ′+θN,θN=klog⁡Z,∣θN∣≤κG+Ofixed(1/log⁡Z).N_*=1+\ell'+\theta_N,\qquad \theta_N=\frac{k}{\log Z},\qquad |\theta_N|\le\kappa_{\mathrm G}+O_{\rm fixed}(1/\log Z).

These retained lengths lie in a fixed bounded range. The weighted Fourier norms have a summable total by the displayed Gaussian estimate; the small annular weight stays in this homogeneous single-profile Fourier norm, not in an inhomogeneous tuple seminorm. Minkowski’s inequality passes the separated row norm through this common density. The existing qc−1/2qn−1q_c^{-1/2}q_n^{-1} normalization stays unchanged when the test scale is recentered, so no additional power of eke^k is introduced. Choose κG\kappa_{\mathrm G} within the final ε\varepsilon allowance. For each fixed θ\theta, Lemma 5.2 supplies the row-sector reduction of νσθχ∙(m)\nu_\sigma\theta\chi_\bullet(m) with every original zero mask. It covers all nonzero element rows, including those meeting SS; no factor ξ(m)\xi(m) is used in this row norm. The row ball depends only on the fixed rescaled tuple pJp_J, through Q=qb∗X′Y′Q=q_{b_*}X'Y', and is independent of the surviving marked slots and dual variables. The physical slot sets remain disjoint and their separated coefficients are product-form. Finite triangle over θ\theta and Lemma 14.3 therefore give the exponent in (14.14) at this actual N∗N_*, taking the retention parameter τref\tau_{\mathrm{ref}} and the independently prescribed output and separation losses all at most a small ϵ0>0\epsilon_0 > 0. We use the exponent ErefE_{\rm ref} after the fixed row parts are summed; their count is already included in Eref+ϵ0E_{\rm ref}+\epsilon_0, with principal exponent O/2O/2, and is not counted again.

Here f=1f=1 and the puncture is ρ=1\rho=1, so the only moving non-slot primes are those of the row. After the finite unit and reflection-sector splits in Lemma 14.3, freeze its powerful part of norm length OO and its valuation-one part supported on SS, and split its residual squarefree good product into actual dyads of norm ≍ZH\asymp Z^H. Let ϵZ=Ofixed(1/log⁡Z)\epsilon_Z=O_{\mathrm{fixed}}(1/\log Z) be nonnegative and large enough to contain all fixed annular and fixed-conductor logarithmic offsets in this calculation. Then

H≤M′−O+ϵZ,ΔH=M′−O−H≥−ϵZ,O≥−ϵZ.H \le M' - O + \epsilon_Z,\qquad\Delta_H = M' - O - H \ge-\epsilon_Z,\qquad O \ge-\epsilon_Z.

The actual row and dual annular cutoffs are kept in one joint profile while its common Fourier density is separated. The small kernel amplitude is extracted from that homogeneous density before the row norm is squared, and only then may the positive sieve sum be enlarged, as in Equation (5.24). In particular the kernel saving in Equation (14.14) uses this HH; it is not reevaluated on any shorter rows added by the positive enlargement.

In the notation of that energy estimate, every moving non-slot prime counted in A0A_0 divides the powerful row part to exponent at least two. The comparison of its exact norm with the powerful dyad, and any fixed-conductor contribution, therefore gives

2A0≤O+ϵZ,N0≤A0,za≤ℓ′.2A_0 \le O+\epsilon_Z,\qquad N_0 \le A_0,\qquad z_a \le\ell'.

The available dual length at the actual completed scale is

Td=2H+2A0+2za−1−ℓ′−θN−N0−3B0.T_d = 2H + 2A_0 + 2z_a - 1 - \ell' - \theta_N - N_0 - 3B_0.

Since M′+ℓ′−1=−3dM' + \ell' - 1 = -3d, direct subtraction gives

Td−(H−3d)=H−M′+2A0+2(za−ℓ′)−N0−3B0−θN≤2ϵZ+∣θN∣.T_d - (H-3d) = H - M' + 2A_0 + 2(z_a-\ell') - N_0 - 3B_0 - \theta_N \le2\epsilon_Z + \lvert\theta_N\rvert.

As in the proof of the reflected energy, dual ranges below a fixed negative length are negligible after a positive Mellin shift, and the bounded boundary range costs an arbitrarily small power. The source dual ideals n,bn,b in these dyads retain the support of Equation (5.2): they may share primes and may contain the permitted primes of SS; no additional SS-mask or coprimality condition between nn and bb is imposed. On each remaining dual dyad, put y=v+3ℓb+eλy=v+3\ell_b+e_\lambda. Retention gives y≤Td+ϵ0y\le T_d+\epsilon_0, while the nonzero unit ranges give v,ℓb,eλ≥−ϵZv,\ell_b,e_\lambda\ge-\epsilon_Z after increasing its fixed constant. It follows that

max⁡(H,v+ℓb)=H+O(ϵ0+κG+ϵZ).\max(H,v+\ell_b)=H+O(\epsilon_0+\kappa_{\mathrm G}+\epsilon_Z).

Write shyb=min⁡{v,za,(v+za)/3}s_{\mathrm{hyb}}=\min\{v,z_a,(v+z_a)/3\} for the quantity called uu in Equation (14.13). If shyb=zas_{\mathrm{hyb}}=z_a, then −S0−B0+za−shyb≤0-S_0-B_0+z_a-s_{\mathrm{hyb}}\le0, the kernel term is nonpositive, and

−ℓb−2eλ3≤53ϵZ.-\ell_b-\frac{2e_\lambda}{3}\le\frac{5}{3}\epsilon_Z.

Here the standalone OO is the powerful-row logarithmic length. It follows that

Eref≤O/2+H+O(ϵ0+κG+ϵZ)=M′−O/2−ΔH+O(ϵ0+κG+ϵZ).\begin{aligned} E_{\rm ref}&\le O/2+H+O(\epsilon_0+\kappa_{\mathrm G}+\epsilon_Z)\\ &=M'-O/2-\Delta_H+O(\epsilon_0+\kappa_{\mathrm G}+\epsilon_Z). \end{aligned}

Otherwise shyb≥v/2−O(ϵZ)s_{\mathrm{hyb}}\ge v/2-O(\epsilon_Z), and the bounded unit ranges imply

shyb+ℓb+2eλ3+(Td−y)+2≥y4+(Td−y)+2−O(ϵZ)≥Td4−O(ϵZ).s_{\mathrm{hyb}}+\ell_b+\frac{2e_\lambda}{3}+\frac{(T_d-y)_+}{2} \ge\frac{y}{4}+\frac{(T_d-y)_+}{2}-O(\epsilon_Z)\ge\frac{T_d}{4}-O(\epsilon_Z).

The last inequality holds separately for y≤Tdy \le T_d and y≥Tdy \ge T_d. Here the squared kernel saving is obtained by first extracting min⁡{1,Z(y−Td)/4}\min\{1,Z^{(y-T_d)/4}\} from the common Fourier density and only then squaring the row norm. Relative to M′M', the saving before the remaining +za+z_a is exactly

O/2+ΔH+S0+B0+Td/4=2M′+2za−1−ℓ′+2ΔH−θN4+2A0−N0+B0+4S04.\begin{aligned} O/2+\Delta_H+S_0+B_0+T_d/4 ={}&\frac{2M'+2z_a-1-\ell'+2\Delta_H-\theta_N}{4}\\ &+\frac{2A_0-N_0+B_0+4S_0}{4}. \end{aligned}

The second numerator is nonnegative. Since za≤ℓ′z_a\le\ell', the energy in this branch is at most

M′+1+3ℓ′−2M′−2ΔH+θN4+O(ϵ0+κG+ϵZ)=M′+d−1/6−2ΔH+θN4+O(ϵ0+κG+ϵZ).\begin{aligned} &M'+\frac{1+3\ell'-2M'-2\Delta_H+\theta_N}{4} +O(\epsilon_0+\kappa_{\mathrm G}+\epsilon_Z)\\ &\qquad=M'+\frac{d-1/6-2\Delta_H+\theta_N}{4} +O(\epsilon_0+\kappa_{\mathrm G}+\epsilon_Z). \end{aligned}

After using O≥−ϵZO\ge-\epsilon_Z and absorbing θN\theta_N, the two upper bounds are

M′−ΔH+O(ϵ0+κG+ϵZ),M'-\Delta_H+O(\epsilon_0+\kappa_{\mathrm G}+\epsilon_Z),
M′+d−1/6−2ΔH4+O(ϵ0+κG+ϵZ).M'+\frac{d-1/6-2\Delta_H}{4} +O(\epsilon_0+\kappa_{\mathrm G}+\epsilon_Z).

They are nonincreasing in ΔH\Delta_H. Since ΔH≥−ϵZ\Delta_H\ge-\epsilon_Z, their formal ΔH=0\Delta_H=0 values bound every actual dyad up to O(ϵZ)O(\epsilon_Z), whether or not an endpoint dyad occurs. Their maximum is therefore at most M′+((d−1/6)/4)++O(ϵ0+κG+ϵZ)M'+((d-1/6)/4)_++O(\epsilon_0+\kappa_{\mathrm G}+\epsilon_Z). At d=1/6d=1/6 one has ℓ′=za=0\ell'=z_a=0 and the clipped unit range falls in the first branch; bounded negative unit dyads change only ϵZ\epsilon_Z. Choose ϵ0\epsilon_0 and κG\kappa_{\mathrm G} within the prescribed ϵ\epsilon allowance, and then increase the fixed-data lower threshold so that ϵZ\epsilon_Z also lies within it. Summing the logarithmically many row and dual dyads proves the lemma.

The additive Gram bound

We next estimate the additive factor in the range Y′2/Q≥1Y'^{2}/Q\ge1. The full correlation of Lemma 13.3 retains the collision zeros that determine both its cancellation and its exceptional frequencies.

Proposition 15.2 (A quantitative additive Gram bound). Fix the arithmetic data S,T,b∗,ξS,T,b_*,\xi, the annular weight W1W_1, and a ray class σ∈T\sigma\in T. Let Q,Y′≥1Q,Y'\ge1 be in fixed polynomial ranges in ZZ, and suppose

Pa=Y′2/Q≥1.P_a=Y'^{2}/Q\ge1.

For a real height ν\nu, put Am=Am,σ,ν(Y′)A_m=A_{m,\sigma,\nu}(Y') as defined in Section 6. For every fixed row ball qm≪Qq_m\ll Q and every ϵ>0\epsilon>0, one has

∑qm≪Q∣Am∣2≪(1+∣ν∣)JGrQY′(1+Pa1/6+Pa2Y′)Zϵ.\sum_{q_m\ll Q}|A_m|^2\ll(1+|\nu|)^{J_{\mathrm{Gr}}}\frac{Q}{Y'}\left(1+P_a^{1/6}+\frac{P_a^2}{Y'}\right)Z^\epsilon.

Here JGrJ_{\mathrm{Gr}} is a fixed seminorm order, independent of the moving scales and of ν\nu. The same assertion holds for any fixed finite linear combination of the ray coefficients 1s∈σχs(b∗)/ξ(s)1_{s\in\sigma}\chi_s(b_*)/\xi(s). No arbitrary row-dependent arithmetic coefficient is asserted.

Proof. Majorize the row ball by a fixed nonnegative radial Schwartz function. Put rs=qs/Y′r_s=q_s/Y' and, on the primary elements prime to SS, cσ(s)=1s∈σχs(b∗)/(τξ(s))c_\sigma(s)=1_{s\in\sigma}\chi_s(b_*)/(\tau\xi(s)), extended by zero elsewhere before the inverse character is evaluated. The exact annular rewriting of the polynomial is

Am=Y′−3/2∑scσ(s)W1(rs)rs−1+iνgχs(s,−m).A_m=Y'^{-3/2}\sum_s c_\sigma(s)W_1(r_s)r_s^{-1+i\nu}g_{\chi_s}(s,-m).

Thus the expanded square has the common normalization Y′−3Y'^{-3} and the joint annular profile contains the factors W1(rs1)rs1−1+iνW1(rs2)rs2−1−iνW_1(r_{s_1})r_{s_1}^{-1+i\nu}W_1(r_{s_2})r_{s_2}^{-1-i\nu}. Write s1=Cn1s_1=Cn_1, s2=Cn2s_2=Cn_2, with (n1,n2)=1(n_1,n_2)=1. Poisson in the row variable has factor Q/(qs1qs2)Q/(q_{s_1}q_{s_2}), whereas the complete transform of the two unnormalized Gauss sums is qs1qs2F(s1,s2;j)q_{s_1}q_{s_2}F(s_1,s_2;j). It therefore gives the exact prefactor Q/Y′3Q/Y'^{3} and the correlation F(Cn1,Cn2;Ck)F(Cn_1,Cn_2;Ck) of (13.7). Here FF again denotes the full correlation of (13.6), not the local coefficient of (7.1). The first Fourier kernel has argument comparable to qCqk/Paq_Cq_k/P_a.

On coprime residuals the factor LCL_C in that correlation has ∣LC∣≤qC\lvert L_C\rvert\le q_C. For the subsequent signed extension use its specified bounded extension, periodic modulo rad⁡C\operatorname{rad} C in both columns, including when CC shares primes with a column. Its value is defined to be zero when a prime of CC divides both columns; this is a definition of the extension, not a claim about the genuine correlation there. Before any factorwise estimate, insert the complete Möbius identity

1(n1,n2)=1=∑d∣n1, d∣n2μ(d)1_{(n_1,n_2)=1}=\sum_{d\mid n_1,\ d\mid n_2}\mu(d)

and write ni=dmin_i=dm_i. No coprimality condition on m1,m2m_1,m_2 is then imposed. Nonzero terms have (d,Ck)=1(d,Ck)=1. Throughout this step use the fixed ray extension of R(n1,n2)\mathcal{R}(n_1,n_2); a quotient of zero residue symbols would not be defined.

We specify a common fixed modulus for that coefficient. For k≠0k\ne0 write k=ζkSkgoodk=\zeta k_Sk_{\mathrm{good}} using the unit convention and the fixed SS-prime generators of Lemma 4.1, with kS=∏p∈Sπpepk_S=\prod_{\mathfrak p\in S}\pi_{\mathfrak p}^{e_{\mathfrak p}} and kgood=∏p∉Spepk_{\mathrm{good}}=\prod_{p\notin S}p^{e_p}. For a primary residual ideal mm outside SS, reciprocity gives

χm(k)=κζ,e(m)R(kgood,m)∏p∣kgoodχp(m)ep,\chi_m(k)=\kappa_{\zeta,\boldsymbol e}(m) \mathcal R(k_{\mathrm{good}},m) \prod_{p\mid k_{\mathrm{good}}}\chi_p(m)^{e_p},
κζ,e(m)=χm(ζ)∏p∈Sχm(πp)ep mod 6.\kappa_{\zeta,\boldsymbol e}(m) =\chi_m(\zeta)\prod_{\mathfrak p\in S} \chi_m(\pi_{\mathfrak p})^{e_{\mathfrak p}\bmod6}.

Every displayed good local power retains its zero on a shared prime, including when 6∣ep6\mid e_p. Lemma 4.1 places the finitely many κζ,e\kappa_{\zeta,\boldsymbol e} in a fixed ray group supported on SS. Also R(kgood,m)\mathcal{R}(k_{\mathrm{good}},m) belongs to a fixed finite family in mm.

Choose lfixed\mathfrak{l}_{\mathrm{fixed}} once to contain the primary-class modulus and the SS zero masks, the moduli of every fixed ray coefficient in AmA_m, a period for R\mathcal{R} in each variable, and the conductors of all the preceding κζ,e\kappa_{\zeta,\boldsymbol e} characters. The extended coefficient is zero off the primary class or at a fixed nonunit before any inverse character is evaluated. This modulus is independent of C,d,kC,d,k, and may have higher powers at SS than rad⁡(k)\operatorname{rad}(k). After reciprocity the joint arithmetic coefficient in m1,m2m_1,m_2 is periodic modulo

r=lcm⁡(lfixed,rad⁡C,rad⁡(k)),qr≪fixedqCqk.\mathfrak{r}=\operatorname{lcm}(\mathfrak{l}_{\mathrm{fixed}},\operatorname{rad} C,\operatorname{rad}(k)),\qquad q_{\mathfrak{r}}\ll_{\mathrm{fixed}} q_Cq_k.

If kk has a valuation epe_p not divisible by six at a prime outside CC and lfixed\mathfrak{l}_{\mathrm{fixed}}, call kk nonexceptional. At that prime the first residual column has the nonprincipal zero-extended factor χp(m1)ep\chi_p(m_1)^{e_p} up to a unit scalar. The lift, the fixed phases, and the other prime factors are independent of m1m_1 modulo pp. Its complete mean, and hence the complete joint mean by the Chinese remainder theorem, is zero. The substitution by dd does not change this conclusion because (d,k)=1(d,k)=1. Principal zero masks at valuations divisible by six remain present in the exceptional case.

The frequency k=0k=0 contributes only the diagonal: the correlation forces n1=n2=1n_1=n_2=1 and equals φ(C)\varphi(C). There are O(Y′)O(Y') possible CC of norm comparable to Y′Y', each with φ(C)≤qC≪Y′\varphi(C)\le q_C\ll Y'. Its contribution is therefore O(Q/Y′)O(Q/Y').

For k≠0k\ne0, split the Fourier argument into dyadic shells qCqk/Pa≍Rq_Cq_k/P_a\asymp R, with R=1,2,4,…R=1,2,4,\ldots and the first shell including all arguments at most two. Choose dyadic centers C0,D0∈{1,2,4,…}C_0,D_0\in\{1,2,4,\ldots\} for qC≍C0q_C\asymp C_0 and qd≍D0q_d\asymp D_0, with the first dyads containing the bounded unit ranges. Use the nominal positive residual scale

N=Y′/(C0D0),Q=qr≪fixedRPa.N=Y'/(C_0D_0),\qquad \mathcal Q=q_{\mathfrak r}\ll_{\rm fixed}RP_a.

The actual residual norms lie in fixed multiples of NN; the nominal value NN is allowed to be below one. Fix arbitrary A>2A>2 and B>2B>2. For each fixed C,d,kC,d,k, the one joint annular profile WRW_R for the two columns has the finitely many homogeneous single-profile seminorms used below bounded by OB,JGr((1+∣ν∣)JGrR−B)O_{B,J_{\mathrm{Gr}}}((1+|\nu|)^{J_{\mathrm{Gr}}}R^{-B}), with one fixed JGrJ_{\mathrm{Gr}} chosen after these derivative orders and A,BA,B. This follows by differentiating the first Fourier kernel, whose Schwartz decay absorbs every resulting power of RR; derivatives of the norm powers cost a fixed power of 1+∣ν∣1+|\nu|. This factor R−BR^{-B} remains in the single-profile Fourier estimate and occurs once in the linear lattice sum below; no small inhomogeneous tuple seminorm is used.

Let aC,d,ka_{C,d,k} be this periodic arithmetic coefficient. For a nonexceptional frequency its normalized complete Fourier transform, with normalization Q−2\mathcal Q^{-2} on the two residue variables, has absolute value at most qCq_C and vanishes at (0,0)(0,0). Since every ideal of O\mathcal{O} is principal, the period lattice has linear scale Q1/2\mathcal Q^{1/2}. Four-dimensional lattice Poisson therefore gives, for this AA,

∣∑m∈O2aC,d,k(m)WR(m/N)∣≪(1+∣ν∣)JGrR−BqCN2min⁡{1,(Q/N)A}.\left|\sum_{\mathbf m\in\mathcal O^2} a_{C,d,k}(\mathbf m)W_R(\mathbf m/\sqrt N)\right| \ll (1+|\nu|)^{J_{\mathrm{Gr}}} R^{-B}q_C N^2 \min\{1,(\mathcal Q/N)^A\}.

For N≥QN\ge\mathcal Q, the zero frequency vanishes and the other dual vectors have linear scale (N/Q)1/2(N/\mathcal Q)^{1/2}. Fourier decay of order 2A>42A>4 bounds their sum by (Q/N)A(\mathcal Q/N)^A. For N<QN<\mathcal Q, use the point count in the two annuli. A nonempty subunit annulus has NN bounded below by a fixed positive constant, so it still contains O(N)O(N) lattice points; below that constant it is empty. This proves Equation (15.5) without any primitivity or tensor-product assumption on aC,d,ka_{C,d,k}.

Put KR=RPa/C0K_R=RP_a/C_0. The fixed shell comparison constants give qk≤CshKRq_k\le C_{\mathrm{sh}}K_R for a fixed Csh>0C_{\mathrm{sh}}>0. Hence the nonzero frequency range is empty when KR<Csh−1K_R<C_{\mathrm{sh}}^{-1}. On a nonempty range, elementary lattice counting gives

#{k:0<qk≤CshKR}≪fixedKR+KR+1≪fixedKR.\#\{k:0<q_k\le C_{\mathrm{sh}}K_R\}\ll_{\mathrm{fixed}} K_R+\sqrt{K_R}+1\ll_{\mathrm{fixed}}K_R.

There are therefore O(C0D0KR)O(C_0D_0K_R) choices of C,d,kC,d,k on these dyads. Multiplying Equation (15.5) by this count and by the common prefactor gives at most

(1+∣ν∣)JGrR−BQY′RPaC0D0min⁡{1,(RPaC0D0Y′)A}.(1+|\nu|)^{J_{\mathrm{Gr}}}R^{-B}\frac{Q}{Y'}\frac{RP_a}{C_0D_0}\min\left\{1,\left(\frac{RP_aC_0D_0}{Y'}\right)^A\right\}.

For Λ=Y′/(RPa)\Lambda=Y'/(RP_a) the required positive dyadic sum is

∑i,j≥02−i−jmin⁡{1,(2i+j/Λ)A}=∑n≥0(n+1)2−nmin⁡{1,(2n/Λ)A}≪A1+log⁡(2+Λ)Λ.\sum_{i,j\ge0}2^{-i-j}\min\{1,(2^{i+j}/\Lambda)^A\} =\sum_{n\ge0}(n+1)2^{-n}\min\{1,(2^n/\Lambda)^A\} \ll_A\frac{1+\log(2+\Lambda)}{\Lambda}.

For Λ≥1\Lambda\ge1, split the two geometric tails at 2n≍Λ2^n\asymp\Lambda; for Λ<1\Lambda<1, the left side is bounded and the displayed right side is larger than a positive constant. Thus the nonexceptional frequencies contribute

≪(1+∣ν∣)JGrQY′Pa2Y′Zε\ll(1+|\nu|)^{J_{\mathrm{Gr}}}\frac{Q}{Y'}\frac{P_a^2}{Y'}Z^\varepsilon

after the RR sum, on choosing a fixed B>2B>2.

It remains to count the exceptional nonzero frequencies. They have (k)=a16e(k)=a_1^6e, where ee is sixth-power-free and supported on the primes of CC and the fixed support. There are at most 6ω(C)+OS(1)≪ϵqCϵ6^{\omega(C)+O_S(1)}\ll_\epsilon q_C^\epsilon possible ee. For each of them the shell bound qk≤CshKRq_k\le C_{\mathrm{sh}}K_R permits only qa1≤(CshKR/qe)1/6q_{a_1}\le(C_{\rm sh}K_R/q_e)^{1/6}. If this range is nonempty, its upper bound is at least one, and the ideal count gives Ofixed(KR1/6)O_{\mathrm{fixed}}(K_R^{1/6}) choices; if qe>CshKRq_e>C_{\mathrm{sh}}K_R it is empty. Unit factors cost only a fixed factor. Hence there are Oε(KR1/6qCε)O_\varepsilon(K_R^{1/6}q_C^\varepsilon) such elements kk, including the bounded subunit range of KRK_R.

Use KR=RPa/C0K_R=RP_a/C_0, ∣LC∣≤qC|L_C|\le q_C, and the trivial two-column point count. Before multiplication by Q/Y′3Q/Y'^3, the contribution on these dyads is

≪(1+∣ν∣)JGrR−BZϵY′2(RPa)1/6C0−1/6D0−1.\ll (1+|\nu|)^{J_{\mathrm{Gr}}} R^{-B}Z^\epsilon Y'^2(RP_a)^{1/6}C_0^{-1/6}D_0^{-1}.

The sums over C0,D0C_0,D_0 converge after reducing the arbitrary small power, and the RR sum converges for the same fixed B>2B>2. This gives the term (Q/Y′)Pa1/6Zϵ(Q/Y')P_a^{1/6}Z^\epsilon. Adding the diagonal and nonexceptional terms proves the proposition.

Completion of the low bound

The two preceding estimates now apply to the two factors of the same rescaled summand in the exact low separation.

Proposition 15.3 (The compensated low estimate). For the probe in (12.5), the geometry in (12.4), and every ϵ>0\epsilon>0,

∣Iη,modified(Z)∣≪Zlx/2+b/12+ϵ=Z3/16+ϵ.|I_{\eta,\mathrm{modified}}(Z)| \ll Z^{l_x/2+b/12+\epsilon}=Z^{3/16+\epsilon}.

The exponent is independent of the target and the slot mesh; the constant and lower threshold may depend on the fixed arithmetic data, slot system, and smooth tests.

Proof. For a fixed rescaled subset and tuple, put Q=qb∗X′Y′Q=q_{b_*}X'Y'. Its separation is (6.2) with Am,σ,v(Y′)A_{m,\sigma,v}(Y') and Bm,σJ(Z)B^J_{m,\sigma}(Z). Put rJ=qpJ/Zdr_J=q_{p_J}/Z^d; the fixed annular supports give 0<cJ≤rJ≤CJ<∞0<c_J\le r_J\le C_J<\infty uniformly in the tuple. Exactly,

X′=Zlx−d/rJ,Y′=Zly−d/rJ,X'=Z^{l_x-d}/r_J,\qquad Y'=Z^{l_y-d}/r_J,
Q=qb∗ZM′/rJ2,Pa=Y′2/Q=qb∗−1Z1/8.Q=q_{b_*}Z^{M'}/r_J^2,\qquad P_a=Y'^2/Q=q_{b_*}^{-1}Z^{1/8}.

In particular Pa≥1P_a\ge1 for Z≥qb∗8Z\ge q_{b_*}^{8}. Enlarge the allowed fixed-data lower threshold so that Q,Y′≥1Q,Y'\ge1 uniformly over the tuple ratios as well; this is possible because M′≥1/2M'\ge1/2 and ly−d≥5/16l_y-d\ge5/16. The remaining length inequalities are

lx−d≥3/16,ly−d≥5/16,ly−d−11b/6≥1/12.l_x-d\ge3/16,\qquad l_y-d\ge5/16, \qquad l_y-d-11b/6\ge1/12.

The last one gives

Y′Pa11/6=qb∗11/6rJ−1Zly−d−11b/6≫fixedZ1/12,\frac{Y'}{P_a^{11/6}}=q_{b_*}^{11/6}r_J^{-1}Z^{l_y-d-11b/6}\gg_{\mathrm{fixed}} Z^{1/12},

and hence Pa2/Y′≪Pa1/6P_a^2/Y'\ll P_a^{1/6}. Proposition (15.2) therefore gives

∑qm≪Q∣Am,σ,v(Y′)∣2≪(1+∣v∣)JGr(Q/Y′)Pa1/6Zϵ.\sum_{q_m\ll Q}|A_{m,\sigma,v}(Y')|^2\ll(1+|v|)^{J_{\mathrm{Gr}}}(Q/Y')P_a^{1/6}Z^\epsilon.

Cauchy–Schwarz in the row sum, Lemma 15.1, and the integrability of (1+∣v∣)JGr/2∣W^0(iv)∣(1+|v|)^{J_{\mathrm{Gr}}/2}|\widehat W_0(iv)| now bound this tuple’s unscaled separation by ZϵZ^\epsilon times

Q−1/2[(Q/Y′)Pa1/6]1/2[ZM′]1/2=[ZM′/Y′]1/2Pa1/12=rJ(X′)1/2Pa1/12.\begin{aligned} Q^{-1/2}\bigl[(Q/Y')P_a^{1/6}\bigr]^{1/2} \bigl[Z^{M'}\bigr]^{1/2} &=\bigl[Z^{M'}/Y'\bigr]^{1/2}P_a^{1/12}\\ &=r_J(X')^{1/2}P_a^{1/12}. \end{aligned}

Since rJr_J is bounded, this is O((X′)1/2Pa1/12Zϵ)O((X')^{1/2}P_a^{1/12}Z^\epsilon).

For d=∑i∈Jℓid=\sum_{i\in J}\ell_i there are at most Zd+ϵZ^{d+\epsilon} rescaled tuples, the coefficient is O(Z−3d/2)O(Z^{-3d/2}), and (X′)1/2≍X1/2Z−d/2(X')^{1/2}\asymp X^{1/2}Z^{-d/2}. The total additional exponent is consequently

f(d)=d−3d/2−d/2=−d≤0.f(d)=d-3d/2-d/2=-d\le0.

Choose the small powers in the component estimates so that their sum lies within the prescribed ϵ\epsilon. Summing the finitely many subsets proves (15.6). For the already defined C=CIIC=C_{\mathrm{II}} of (12.3), the normalization used for the principal signal satisfies

CII(s)=lx/2+s−1+h/6=s−11/16,C_{\mathrm{II}}(s)=l_x/2+s-1+h/6=s-11/16,
CII(7/8)=3/16=lx/2+b/12.C_{\mathrm{II}}(7/8)=3/16=l_x/2+b/12.

Thus, under the contradiction assumed in Part II, this low bound is smaller than ZCII(β∗)Z^{C_{\mathrm{II}}(\beta_*)} by the exact power Δ=β∗−7/8\Delta=\beta_*-7/8, apart from the arbitrarily prescribed ϵ\epsilon.

The local compensation and its errors

The physical modification in Section 12 has already been estimated from its separated low representation. We now identify its full Euler correction and bound the local errors left by the two-term operation. Throughout, the local notation PpP_p, Pp∗P_p^*, HpH_p, VV, WW, DD, RR is that of Lemma 7.1; in the shared analytic estimates its variable xx is called ss. Fix a nonzero sixth-power-free physical row uu with (u,S)=1(u,S)=1. All slot primes belong to the sets Pi(Z)\mathcal{P}_i(Z) of Section 12; for each such prime put Q=qpQ=q_p. As in Lemma 7.1, write xr=ℜxx_r=\Re x, wr=ℜww_r=\Re w, and zr=ℜzz_r=\Re z. The factor Wloc=ρQ−wW_{\mathrm{loc}}=\rho Q^{-w} inside Pp∗P_p^* is distinct from W=χp(u)Q−wW=\chi_p(u)Q^{-w}: at p∣up\mid u, the latter and DD vanish, while the former retains its unit phase.

The full holomorphic correction

For a fixed slot prime pp, restricting the completed index to p∣Ap\mid A replaces PpP_p by Pp∗P_p^* in the high series. Changing ZZ to ZQZQ multiplies its Mellin weight by Qx+z−1Q^{x+z-1}. The marked term of Equation (12.5) therefore has, at points where PpP_p is defined and nonzero, multiplier η(p)‾Qx+z−1Pp∗/Pp\overline{\eta(p)}Q^{x+z-1}P_p^*/P_p. The rescaled term has multiplier

Q−3/2Q−(1/2−z)Q−(w−1)=Qz−w−1.Q^{-3/2}Q^{-(1/2-z)}Q^{-(w-1)}=Q^{z-w-1}.

Thus, on the same locus, the exact local multiplier of the two-term operation is

Qz−1Bp,Bp=η(p)‾QxPp∗/Pp−Q−w.Q^{z-1}\mathcal B_p,\qquad \mathcal B_p=\overline{\eta(p)}Q^xP_p^*/P_p-Q^{-w}.

Define the combined local replacement by

Gp=(η(p)‾Qx−Q−w)(1−V)(1−W)Pp∗−Q−w(1−VW)1−D.G_p=\frac{\left(\overline{\eta(p)}Q^x-Q^{-w}\right)(1-V)(1-W)P_p^*-Q^{-w}(1-VW)}{1-D}.

At points in the Euler regions where the raw quotient in Equation (16.1) is defined, one has Gp=HpBpG_p=H_p\mathcal B_p. The displayed formula defines GpG_p also where that quotient is not defined. There is neither a PpP_p nor a 1−W1-W denominator on the right. The bounds ∣R∣,∣V∣,∣D∣<1|R|,|V|,|D|<1 in Lemma 7.1, together with its formula for Pp∗P_p^*, show that GpG_p is holomorphic in both stated Euler regions, including at zeros of PpP_p or HpH_p.

At points in the Euler regions where the selected quotients are defined, write the full slot multiplier

Bi(u;x,w,z)=∑p∈Pi(Z)Wi(qp/Pi)qpz−1Bp.\mathcal B_i(u;x,w,z)=\sum_{p\in\mathcal P_i(Z)} W_i(q_p/P_i)q_p^{z-1}\mathcal B_p.

The correction used for contour moves is defined without these quotients:

Hη,u,Z(x,w,z)=∑(pi)∈∏iPi(Z)∏i=1K[Wi(qpi/Pi)qpiz−1Gpi]∏p∉Sp∉{p1,…,pK}Hp.\mathfrak H_{\eta,u,Z}(x,w,z)= \sum_{(p_i)\in\prod_i\mathcal P_i(Z)} \prod_{i=1}^K\bigl[W_i(q_{p_i}/P_i)q_{p_i}^{z-1}G_{p_i}\bigr] \prod_{\substack{p\notin S\\p\notin\{p_1,\ldots,p_K\}}}H_p.

This is the full correction after the scalar quotient in Equation (7.13) has been extracted. To verify this assertion, fix an allowed tuple and put P={p1,…,pK}\mathcal{P}=\{p_1,\ldots,p_K\}. On the absolute starting lines the selected operation replaces PpP_p by

η(p)‾Qx+z−1Pp∗−Qz−w−1Pp=1−D(1−V)(1−W)Qz−1Gp.\overline{\eta(p)}Q^{x+z-1}P_p^*-Q^{z-w-1}P_p =\frac{1-D}{(1-V)(1-W)}Q^{z-1}G_p.

The equality follows by substituting Pp−Pp∗=(1−V)−1+W/(1−W)P_p-P_p^*=(1-V)^{-1}+W/(1-W) into Equation (16.2). It extracts the same scalar local factor (1−V)−1(1−W)−1(1−D)(1-V)^{-1}(1-W)^{-1}(1-D) as at an unselected prime. Each selected prime occurs exactly once, because the slot supports are disjoint. The complete factor for this tuple is therefore the scalar quotient in Equation (7.13) times its summand in Equation (16.3). This reasoning involves no division by PpP_p or HpH_p. At points in the Euler regions where all raw selected quotients are defined, the same finite sum also factors as Hη,u∏iBi\mathcal H_{\eta,u}\prod_i\mathcal B_i.

The unselected product in each summand converges normally in both Euler regions. More quantitatively, in any fixed subregion of Equation (7.14), put ϵH=min⁡(ϵ0,1/50)>0\epsilon_H=\min(\epsilon_0,1/50)>0. The primewise defect bounds in Lemma (7.1) give, uniformly in the selected tuple,

∏p∉Sp∉P∣Hp∣≤∏p∉Sp∤u(1+Cqp−1−ϵH)∏p∣u(1+Cqp−ϵH)≪ϵquϵ.\prod_{\substack{p\notin S\\p\notin\mathcal{P}}}|H_p| \leq \prod_{\substack{p\notin S\\p\nmid u}}(1+Cq_p^{-1-\epsilon_H}) \prod_{p\mid u}(1+Cq_p^{-\epsilon_H}) \ll_{\epsilon}q_u^{\epsilon}.

The first positive product converges by the ideal count, and the second satisfies the divisor-product bound. Omitting selected factors only removes factors from these positive majorants. In the second Euler region the same argument uses the respective defect exponents −363/200-363/200 and −33/40-33/40. Thus Equation (16.5) holds there as well, with the corresponding positive majorants. No non-vanishing of HpH_p is asserted by these upper bounds.

For each fixed ZZ, Equation (16.3) is a finite sum of products of holomorphic selected factors and normally convergent unselected products. It is therefore holomorphic on a neighborhood of every point in both Euler regions. It also satisfies the all-height requirement in Definition 10.1. Indeed, on a fixed real box in either region, the formula for Pp∗P_p^* and the denominators bounded away from zero give ∣Gp∣≪QB|G_p|\ll Q^B for some fixed BB, uniformly in all imaginary parts and unit phases. There are O(Pi)O(P_i) ideals in a slot and qp≍Piq_p\asymp P_i there. The finite tuple sum and Equation (16.5) consequently give

∣Hη,u,Z(x,w,z)∣≪ϵquϵ∏iPizr+B≪ϵquϵZB′.|\mathfrak H_{\eta,u,Z}(x,w,z)| \ll_\epsilon q_u^\epsilon\prod_iP_i^{z_r+B} \ll_\epsilon q_u^\epsilon Z^{B'}.

for a fixed B′B' on that box. For qu≤ZDq_u\leq Z^D this is Equation (10.4), even with height exponent zero. All constants here are fixed before any later order of integration by parts.

Combining the exact finite operation with Equations (7.5) and (7.13) now gives

Iη,modified(Z)=1(2πi)3∫(3)∫(3)∫(2)W(X,Y,Z;x,w,z)⋅∑u(6)qu−zξ(u)‾ζFS(6z)LS(w,χ∙(u))LS(x,ηχ∙(u)‾)Hη,u,Z(x,w,z) dz dw dx.\begin{aligned} I_{\eta,\mathrm{modified}}(Z) ={}&\frac1{(2\pi i)^3}\int_{(3)}\int_{(3)}\int_{(2)} \mathcal W(X,Y,Z;x,w,z)\\ &\quad\cdot\sum_u^{(6)}q_u^{-z}\overline{\xi(u)} \frac{\zeta_F^S(6z)L^S(w,\chi_\bullet(u))} {L^S(x,\eta\overline{\chi_\bullet(u)})} \mathfrak H_{\eta,u,Z}(x,w,z)\,dz\,dw\,dx. \end{aligned}

This identity is absolutely convergent on the displayed lines, because for fixed ZZ it is obtained from finitely many absolutely convergent rescaled base-probe identities. It has no additional outside Euler factor. It verifies the exact high representation of Definition 10.1 for the physical expression Iη,modifiedI_{\eta,\mathrm{modified}}, with the geometry in Equation (12.4). In particular, lx/2−1+h/6=17/96−1+13/96=−11/16l_x/2-1+h/6=17/96-1+13/96=-11/16, as required by Equation (12.3). It is an identity for the very probe bounded in Proposition (15.3). Every continuation uses the full correction in Equation (16.3), not a globally defined product of individual quotients.

Dynamic local errors

At an identity-ray prime every fixed phase from TT is one, although η(p)\eta(p) may be any unit. Suppose first that p∤up\nmid u and put v=χp(u)v=\chi_p(u). Then D=η(p)v−1Q−xD=\eta(p)v^{-1}Q^{-x}, and η(p)‾QxD=v−1\overline{\eta(p)}Q^xD=v^{-1}. Using v−1W=Q−wv^{-1}W=Q^{-w} and Ep=Pp∗+D\mathcal{E}_p=P_p^*+D gives the exact normalized cancellation

Gp+v−1Hp=(1−V)(1−W)1−D[(v−1−Q−w){V/(1−V)−D}+(η(p)‾Qx+v−1−Q−w)Ep].\begin{aligned} G_p+v^{-1}H_p={}& \frac{(1-V)(1-W)}{1-D} \Bigl[(v^{-1}-Q^{-w})\{V/(1-V)-D\}\\ &\hspace{17mm}+(\overline{\eta(p)}Q^x+v^{-1}-Q^{-w}) \mathcal E_p\Bigr]. \end{aligned}

This is an identity of holomorphic local expressions in the Euler regions. Within these regions, on the raw quotient locus its left side is Hp(Bp+v−1)H_p(\mathcal B_p+v^{-1}). To see the cancellation directly on that locus, substitute Pp∗=−D+EpP_p^*=-D+\mathcal E_p and Pp=(1−V)−1+W/(1−W)+Pp∗P_p=(1-V)^{-1}+W/(1-W)+P_p^* into the left side before normalization. The constants v−1−Q−wv^{-1}-Q^{-w}, and (v−1−Q−w)W/(1−W)=Q−w(v^{-1}-Q^{-w})W/(1-W)=Q^{-w} sum to zero. The resulting rational identity has only the denominators 1−R1-R, 1−V1-V, and 1−D1-D, which are nonzero in the Euler regions; hence it gives the displayed holomorphic identity there. For p∣up\mid u, the main term is zero by the original zero extension, and Equation (16.2) instead becomes

Gp=η(p)‾Qx(1−V)Ep−Q−wHp.G_p= \overline{\eta(p)}Q^x(1-V)\mathcal E_p-Q^{-w}H_p.

We now give the bound on the remaining error slots. Its analytic input is stated explicitly: the reflected primitive numerator must be small at the retained height. Instantiate Section 8 with the current fixed data and Θ=⟨η,T^⟩\Theta=\langle\eta,\widehat{T}\rangle, using its zero-extended presentations ν(n)χn(u)ς\nu(n)\chi_n(u)^\varsigma for ν∈Θ\nu\in\Theta and ς∈{−1,1}\varsigma\in\{-1,1\}. The numerator χ∙(u)\chi_\bullet(u) and its conjugate belong to Xu\mathcal{X}_u with fixed multiplier 1∈Θ1\in\Theta, while the denominator ηχ∙(u)‾\eta\overline{\chi_\bullet(u)} belongs to Xu\mathcal{X}_u with fixed multiplier η∈Θ\eta\in\Theta. The buffered estimates there, together with the inverse deleted-factor bound of Lemma 4.10, therefore supply the reflected-numerator hypothesis below at the retained heights: for the points used below, ℜ(1−w)=a+6e\Re(1-w)=a+6e and ∣ℑ(1−w)∣≤T1|\Im(1-w)|\le T_1, within the buffered rectangle. The identity-ray restriction makes every fixed TT phase equal to one at a slot prime, without changing the physical row or any nonunit zero.

Proposition 16.1 (Dynamic local errors and conductor allocation). Let 51/100≤a≤151/100\le a\le1, 0<e≤10−30<e\le10^{-3}, and take

xr=a+16e,wr=1−a−6e,zr=17/50.x_r=a+16e,\qquad w_r=1-a-6e,\qquad z_r=17/50.

Choose P0P_0 sufficiently large in terms of ee and the fixed data. For U,T1≥1U,T_1\ge1 and a sixth-power-free row uu with (u,S)=1(u,S)=1 and qu≍Uq_u\asymp U, let ψu∗\psi_u^* be the primitive character inducing χ∙(u)\chi_\bullet(u). Let Wu\mathcal{W}_u be any subset of {w:ℜw=wr, ∣ℑw∣≤T1}\{w:\Re w=w_r,\ |\Im w|\le T_1\}. Suppose ψu∗\psi_u^* is nonprincipal and, uniformly for w∈Wuw\in\mathcal{W}_u,

∣L(1−w,ψu∗‾)∣≪Uϵ|L(1-w,\overline{\psi_u^*})|\ll U^\epsilon

with any prescribed small power. For this row on the displayed dynamic region, define Bi\mathcal{B}_i by its preceding slot sum, interpreting each Bp\mathcal B_p as Gp/HpG_p/H_p, with GpG_p from Equation (16.2). The stated choice of P0P_0 makes Hp≠0H_p\ne0 there for every slot prime, as proved at the start of the proof. This statement asserts individual continuation only on this dynamic region. Define the main and error parts of a slot by

Qi(u;z)=−∑p∈Pi(Z)Wi(qp/Pi)qpz−1χp(u)‾,Di(u)=Bi(u;x,w,z)−Qi(u;z).\mathcal Q_i(u;z)= -\sum_{p\in\mathcal P_i(Z)}W_i(q_p/P_i)q_p^{z-1}\overline{\chi_p(u)}, \qquad \mathcal D_i(u)=\mathcal B_i(u;x,w,z)-\mathcal Q_i(u;z).

Then, for every subset II of the slots and the same points w∈Wuw\in\mathcal{W}_u,

∣LS(w,χ∙(u))∏i∈IDi(u)∣≪Ua−1/2+O(e)+ϵ(3+T1)C∏i∈IPizr−1/2+O(e)+ϵ.\left|L^S(w,\chi_\bullet(u))\prod_{i\in I}\mathcal D_i(u)\right| \ll U^{a-1/2+O(e)+\epsilon}(3+T_1)^C \prod_{i\in I}P_i^{z_r-1/2+O(e)+\epsilon}.

The main parts retain the physical row, all zero masks, and the fixed identity-ray restriction. In particular, their central normalization is

Qi(u;z)=−Piz−1/2(Pi−1/2∑p∈Pi(Z)χp(u)‾Wi(qp/Pi)(qp/Pi)z−1).\mathcal Q_i(u;z)=-P_i^{z-1/2} \left(P_i^{-1/2}\sum_{p\in\mathcal P_i(Z)} \overline{\chi_p(u)}W_i(q_p/P_i)(q_p/P_i)^{z-1}\right).

At the same points w∈Wuw\in\mathcal{W}_u, and on this dynamic region only, the full correction has the finite decomposition

Hη,u,Z=Hη,u∏i=1K(Qi+Di)=Hη,u∑I⊆{1,…,K}∏i∈IDi∏i∉IQi.\mathfrak H_{\eta,u,Z} =\mathcal H_{\eta,u}\prod_{i=1}^K(\mathcal Q_i+\mathcal D_i) =\mathcal H_{\eta,u} \sum_{I\subseteq\{1,\ldots,K\}} \prod_{i\in I}\mathcal D_i\prod_{i\notin I}\mathcal Q_i.

Proof. In this region ϑ=(−wr)+≤6e\vartheta=(-w_r)_+\le6e. The estimates in the proof of Lemma 7.1 sharpen to Hp−1=O(Q−1−10e)H_p-1=O(Q^{-1-10e}) for p∤up\nmid u and Hp−1=O(Q−10e)H_p-1=O(Q^{-10e}) for p∣up\mid u. Increase the fixed P0P_0 so that ∣Hp−1∣<1/2\lvert H_p-1\rvert<1/2 for all these primes. The holomorphic factor GpG_p in (16.2), divided by HpH_p, now defines Bp\mathcal B_p throughout this region. It is HpH_p, not the possibly singular raw factor PpP_p, that is bounded away from zero when wr<0w_r<0.

Consequently the tuple sum in (16.3) factors as Hη,u∏iBi\mathcal H_{\eta,u}\prod_i\mathcal B_i on this dynamic region. Substituting Bi=Qi+Di\mathcal B_i=\mathcal Q_i+\mathcal D_i proves (16.10). This factorization is not used to continue the correction outside the present region.

For p∤up\nmid u, (16.8) and the estimate for Ep\mathcal E_p give

∣Hp(Bp+χp(u)‾)∣≪Q−xr+2ϑ+Q−6zr+2ϑ+Q4−5xr−6zr+2ϑ+Q1−wr−6zr+ϑ≪Q−51/100.|H_p(\mathcal B_p+\overline{\chi_p(u)})| \ll Q^{-x_r+2\vartheta}+Q^{-6z_r+2\vartheta} +Q^{4-5x_r-6z_r+2\vartheta} +Q^{1-w_r-6z_r+\vartheta} \ll Q^{-51/100}.

The four exponents are bounded respectively by −a−4e-a-4e, −51/25+12e-51/25+12e, 49/25−5a−68e49/25-5a-68e, and a−51/25+12ea-51/25+12e. Division by the bounded HpH_p preserves this estimate. The number of primes in a slot is O(Pi)O(P_i) by the ideal count; hence its total contribution from p∤up\nmid u, including Qz−1Q^{z-1}, is O(Pizr−51/100+ϵ)O(P_i^{z_r-51/100+\epsilon}).

For p∣up\mid u there are only divisor-many possible labels. A monomial in Ep\mathcal E_p is multiplied by Qz−1+xQ^{z-1+x} in Qz−1BpQ^{z-1}\mathcal B_p, so after separating QzQ^z its exponent is xr−1x_r-1 plus the exponent of that monomial. For the non-tail boundary terms of the six-valuation table, these exponents at e=0e=0 are

jj12345
a−2a-21/2−2a1/2-2a−a, 1−3a-a,\ 1-3a1/2−2a1/2-2a2−5a2-5a

At positive ee their changes are respectively +6e+6e, −32e-32e, (−26e,−48e)(-26e,-48e), −42e-42e, −80e-80e. They are all strictly below −1/2-1/2 in the stated range. The common RR term is smaller still: its exponent after separating QzQ^z is at most 49/25−1−5a−80e<−1/249/25-1-5a-80e<-1/2. Additional valuation pairs and mm values have ratios ∣R∣≤Q−11/10\lvert R\rvert\le Q^{-11/10} and ∣V∣=Q−51/25\lvert V\rvert=Q^{-51/25}, so their geometric sums preserve these bounds. The strict second-family term with an additional VV is also smaller than Q−1/2Q^{-1/2} after this normalization.

The sole remaining term is the strict (e0,l,k,m)=(1,0,1,0)(e_0,l,k,m)=(1,0,1,0) term, which occurs for j≥2j\ge2 and is −η(p)(Q−1)Q−x−w-\eta(p)(Q-1)Q^{-x-w}. Its exponent after separating QzQ^z is −wr-w_r. The explicit rescaling term −Q−w-Q^{-w} has exponent after separating QzQ^z −1−wr<−1/2-1-w_r<-1/2, so it needs no further estimate.

Let fu\mathfrak f_u be the conductor of ψu∗\psi_u^*. Write u=ϵu∏p∣upjpu=\epsilon_u\prod_{p\mid u}p^{j_p}, with ϵu\epsilon_u a unit. For primary nn coprime to uSuS, reciprocity gives

χn(u)=ϵu(qn−1)/6∏p∣uR(p,n)jpχp(n)jp.\chi_n(u)=\epsilon_u^{(q_n-1)/6}\prod_{p\mid u}\mathcal{R}(p,n)^{j_p}\chi_p(n)^{j_p}.

The unit exponent is read modulo six. The prime formula extends to composite nn: when A≡B≡1(mod6)A\equiv B\equiv1\pmod6,

AB−16≡A−16+B−16(mod6).\frac{AB-1}{6}\equiv\frac{A-1}{6}+\frac{B-1}{6}\pmod6.

Thus the unit factor depends only on qnq_n modulo 36, and the R\mathcal{R} product depends only on nn modulo 4. Together with the multiplicativity of R\mathcal{R} and the local symbols, the displayed norm congruence makes the right side multiplicative on integral ideals prime to 6u6u; extend it to their fractional ideal group. A generator congruent to one modulo (36)rad⁡(u)(36)\operatorname{rad}(u) is already primary and makes every displayed factor one. This character therefore has a ray presentation with that fixed 2,32,3 modulus times rad⁡(u)\operatorname{rad}(u). It agrees with the Kummer character χ∙(u)\chi_\bullet(u) of Lemma 4.1 on ideals avoiding SS. These characters induce the same primitive character: in the principal ideal ring O\mathcal{O}, the Chinese remainder theorem supplies a representative avoiding the additional finite set SS in every ray class of a common modulus. At a good prime p∣up\mid u, hold the fixed class and all other good residues at one and vary the residue modulo pp by the Chinese remainder theorem. The remaining local character χpjp\chi_p^{j_p} has exact order 6/gcd⁡(6,jp)>16/\gcd(6,j_p)>1. Its conductor exponent at pp is therefore exactly one: the displayed ray modulus has only the first power of pp, and the character cannot descend to a modulus omitting pp. This is a local assertion; the ideal character may still need the fixed normalization modulus at 2, 3.

It follows that, for any set J0J_0 of distinct selected ramified labels,

qfu≪Sqrad⁡(u)≤qu∏p∈J0qp−(jp−1).q_{\mathfrak f_u}\ll_S q_{\operatorname{rad}(u)} \le q_u\prod_{p\in J_0}q_p^{-(j_p-1)}.

The functional equation for the primitive numerator [11 Equation (1.1)], the assumed reflected bound, and Stirling give a cost qfuA∗Uϵ(3+T1)Cq_{\mathfrak f_u}^{A_*}U^\epsilon(3+T_1)^C, where

A∗=1/2−wr=a−1/2+6e>0.A_*=1/2-w_r=a-1/2+6e>0.

At a selected p∣up\mid u the primitive character already has value zero, so restoring the original local factor there multiplies by exactly one. The remaining deleted Euler factors have radical OS(U)O_S(U) and cost at most U6e+ϵU^{6e+\epsilon}, because wr≥−6ew_r\ge-6e.

Expand a product of error slots into their coprime-prime terms, their already bounded ramified terms, and their strict ramified terms. For each fixed tuple in this triangle expansion, let J0J_0 be precisely its strict ramified labels. They are distinct because the slot supports are disjoint. Apply the single inequality (16.11) to this entire J0J_0 before summing the labels. The numerator together with these local factors, including qpz−1q_p^{z-1} at each selected prime, is then bounded by

UA∗+6e+ϵ(3+T1)C∏p∈J0qpzr−wr−(jp−1)A∗≤Ua−1/2+12e+ϵ(3+T1)C∏p∈J0qpzr−1/2,U^{A_*+6e+\epsilon}(3+T_1)^C \prod_{p\in J_0}q_p^{z_r-w_r-(j_p-1)A_*} \le U^{a-1/2+12e+\epsilon}(3+T_1)^C \prod_{p\in J_0}q_p^{z_r-1/2},

because jp≥2j_p\ge2 and −wr−A∗=−1/2-w_r-A_*=-1/2. Thus different selected labels use different factors of the conductor deficit, and the bounds hold simultaneously. Summing the divisor-many ramified labels costs UϵU^\epsilon, while the coprime labels have the stronger exponent zr−51/100z_r-51/100. This proves (16.9).

This argument uses triangle only on error labels. It never changes the physical row or the coefficients and masks in any main slot. The tuple-independent factor Hη,u\mathcal{H}_{\eta,u} separately costs UϵU^\epsilon by Lemma 7.1. Relative to the central scale Pizr−1/2P_i^{z_r-1/2} of a main slot, an error slot thus has no positive amplitude exponent in the later row count.

The principal local factor. In the second Euler region of Lemma 7.1, take u=1u=1 and p∈1Tp\in1_T. Then v=1v=1 in (16.8), and HpH_p is bounded away from zero after the same fixed enlargement of P0P_0. For this principal row on this region, define Bp=Gp/Hp\mathcal B_p=G_p/H_p and define Bi\mathcal B_i by the same slot sum as above. The lower bound and the disjoint supports give the separate principal factorization

Hη,1,Z(x,w,z)=Hη,1(x,w,z)∏i=1KBi(1;x,w,z)in the second Euler region.\mathfrak H_{\eta,1,Z}(x,w,z) =\mathcal H_{\eta,1}(x,w,z)\prod_{i=1}^K\mathcal B_i(1;x,w,z) \qquad\text{in the second Euler region}.

in the second Euler region.

This does not extend the central main/error decomposition beyond its stated dynamic region. The four error exponents are now

−xr,−6zr,4−5xr−6zr,1−wr−6zr.-x_r,\qquad-6z_r,\qquad4-5x_r-6z_r,\qquad1-w_r-6z_r.

Each is at most −7/8-7/8 in that region. Hence the principal multiplier satisfies

Bp=−1+O(Q−7/8),\mathcal{B}_p=-1+O(Q^{-7/8}),

uniformly in the imaginary parts and the target unit phase. This is the local estimate used to normalize the principal residue.

It also gives the absolute principal correction required by the shared residue estimate. Indeed Gp=HpBp=O(1)G_p=H_p\mathcal B_p=O(1) here, and the unselected product has a bounded positive majorant by the second-region version of (16.5). Ideal counting in each annular slot therefore gives, on every fixed real box in the second Euler region and uniformly in all imaginary parts,

∣Hη,1,Z(x,w,z)∣≤∑(pi)∈∏iPi(Z)∏i[∣Wi(qpi/Pi)∣qpizr−1∣Gpi∣]∏p∉Sp∉{p1,…,pK}∣Hp∣≪∏iPizr=Zℓzr.\left|\mathfrak{H}_{\eta,1,Z}(x,w,z)\right| \le\sum_{(p_i)\in\prod_i\mathcal{P}_i(Z)}\prod_i\left[\left|W_i(q_{p_i}/P_i)\right|q_{p_i}^{z_r-1}|G_{p_i}|\right]\prod_{\substack{p\notin S\\p\notin\{p_1,\ldots,p_K\}}}|H_p| \ll\prod_i P_i^{z_r}=Z^{\ell z_r}.

This uses the separate principal-row lower bound only to obtain the local approximation; it asserts no nonvanishing of a general HpH_p.

Absolute bounds for the remaining contour lines

The dynamic decomposition is not available on every contour used by the shared analytic estimates. The following bounds instead retain each selected factor GpG_p before taking absolute values.

Lemma 16.2 (Absolute local tuple bounds). Let Z≥2Z\ge2, and let uu be a nonzero sixth-power-free row with (u,S)=1(u,S)=1 and qu≍U≥1q_u\asymp U\ge1, with fixed comparison constants. Retain the fixed physical slot system of Section 12. The following bounds are uniform in all imaginary parts and unit phases.

  1. On

xr=β∗+e,wr=1/2,zr=17/50,0<e≤10−3,x_r=\beta_*+e,\qquad w_r=1/2,\qquad z_r=17/50,\qquad0<e\le10^{-3},

one has Gp=O(1)G_p=O(1) at selected primes p∤up\nmid u and Gp≪Q1/2G_p\ll Q^{1/2} at selected primes p∣up\mid u.

  1. For every fixed z∞>2z_\infty>2, on

xr=wr=2,zr=z∞,x_r=w_r=2,\qquad z_r=z_\infty,

one has Gp=Oz∞(1)G_p=O_{z_\infty}(1) at every selected prime.

In either case the positive sum over the full selected tuples satisfies

∑(pi)∈∏iPi(Z)∏i[∣Wi(qpi/Pi)∣qpizr−1∣Gpi∣]∏p∉Sp∉{p1,…,pK}∣Hp∣≪εUε∏iPizr.\sum_{(p_i)\in\prod_i\mathcal{P}_i(Z)}\prod_i\left[\left|W_i(q_{p_i}/P_i)\right|q_{p_i}^{z_r-1}|G_{p_i}|\right]\prod_{\substack{p\notin S\\p\notin\{p_1,\ldots,p_K\}}}|H_p|\ll_\varepsilon U^\varepsilon\prod_iP_i^{z_r}.

The constants may depend on the fixed data, ee, and, in the second case, z∞z_\infty, but not on ZZ, uu or the imaginary parts. These estimates remain valid at zeros of PpP_p or HpH_p.

Proof. Both sets of lines lie in the first Euler region with ϵ0=3/8\epsilon_0=3/8. Its primewise defect estimates give Hp=O(1)H_p=O(1), while (16.5) bounds the positive product of all unselected factors by Oε(Uε)O_\varepsilon(U^\varepsilon).

Consider first xr=β∗+ex_r=\beta_*+e, wr=1/2w_r=1/2, and zr=17/50z_r=17/50. For a selected p∤up\nmid u, (16.8) gives

∣Gp+χp(u)‾Hp∣≪Q−xr+Q−6zr+Q4−5xr−6zr+Q1−wr−6zr.|G_p+\overline{\chi_p(u)}H_p| \ll Q^{-x_r}+Q^{-6z_r} +Q^{4-5x_r-6z_r}+Q^{1-w_r-6z_r}.

The four exponents are at most −7/8−e-7/8-e, −51/25-51/25, −483/200−5e-483/200-5e, −77/50-77/50, respectively. Consequently Gp=O(1)G_p=O(1) off uu, without division by HpH_p.

For a selected p∣up\mid u, one has W=D=0W=D=0 and Ep=Pp∗\mathcal E_p=P_p^*. Equation (16.2) becomes

Gp=η(p)‾Qx(1−V)Ep−Q−wHp.G_p=\overline{\eta(p)}Q^x(1-V)\mathcal E_p-Q^{-w}H_p.

After multiplication by QxrQ^{x_r}, the strict term of the local table has exponent at most 1−wr=1/21-w_r=1/2; for j=1j=1 it also contains the factor VV. The exponents of the boundary terms JjJ_j, in order j=1,…,5j=1,\ldots,5, are

−12,32−2xr,(32−2xr,2−3xr),2−3xr,3−5xr.-\frac{1}{2},\quad\frac{3}{2}-2x_r,\quad\left(\frac{3}{2}-2x_r,2-3x_r\right),\quad2-3x_r,\quad3-5x_r.

They are bounded above by −1/2-1/2, −1/4−2e-1/4-2e, (−1/4−2e,−5/8−3e)(-1/4-2e,-5/8-3e), −5/8−3e-5/8-3e, −11/8−5e-11/8-5e, respectively. The common RR term has exponent 4−5xr−6zr≤−483/200−5e4-5x_r-6z_r\le-483/200-5e. All further terms in the geometric families decrease these powers, since ∣R∣≤Q−329/100−6e|R|\le Q^{-329/100-6e} and ∣V∣=Q−51/25\lvert V\rvert=Q^{-51/25}. Finally Q−wHp=O(Q−1/2)Q^{-w}H_p=O(Q^{-1/2}). Hence Gp≪Q1/2G_p\ll Q^{1/2} on uu, also at a zero of HpH_p.

The labels dividing uu are divisor-many, while a slot contains O(Pi)O(P_i) ideals. Its positive sum is therefore

∑p∈Pi(Z)∣Wi(qp/Pi)∣qpzr−1∣Gp∣≪Pizr+UϵPizr−1/2≪UϵPizr.\sum_{p\in\mathcal P_i(Z)} |W_i(q_p/P_i)|q_p^{z_r-1}|G_p| \ll P_i^{z_r}+U^\epsilon P_i^{z_r-1/2} \ll U^\epsilon P_i^{z_r}.

Using the positive majorant for the unselected product and distributing the requested ϵ\epsilon among the fixed number of slots proves Equation (16.15) on the first lines.

Now fix xr=wr=2x_r=w_r=2 and zr=z∞>2z_r=z_\infty>2. For a selected prime off uu, the four exponents in Equation (16.8) are −2-2, −6z∞-6z_\infty, −6−6z∞-6-6z_\infty, −1−6z∞-1-6z_\infty, so Gp=Oz∞(1)G_p=O_{z_\infty}(1). On uu, the strict term after multiplication by QxrQ^{x_r} has exponent at most 1−wr=−11-w_r=-1. The boundary exponents are −2-2, −5/2-5/2, (−4,−4)(-4,-4), −11/2-11/2, −7-7, the common RR exponent is −6−6z∞-6-6z_\infty, and ∣R∣=Q−8−6z∞\lvert R\rvert=Q^{-8-6z_\infty}, ∣V∣=Q−6z∞\lvert V\rvert=Q^{-6z_\infty}. The rescaling term is O(Q−2)O(Q^{-2}). Thus Gp=Oz∞(1)G_p=O_{z_\infty}(1) on uu as well. A positive slot sum is consequently Oz∞(Piz∞)O_{z_\infty}(P_i^{z_\infty}). Together with Equation (16.5), this proves Equation (16.15) on the second lines.

Equation (16.7) supplies the full high representation of the physical function just bounded on the low side. Proposition 16.1 controls the error factors jointly with the numerator, and Lemma 16.2 supplies the bounds on the remaining contour lines. The main factors are the prime polynomials displayed in Proposition 16.1. To count rows on which those factors and a detector witness are large, we next prove the inverse and fourth-moment estimates used in Section 19.

The inverse moment with prime factors

We now bound an inverse Dirichlet polynomial multiplied by independently weighted prime sums. The estimate applies to the inverse witness in Section 8 together with selected main factors from the local compensation. Its proof uses the completed row energy of Section 14. A final amplification gives an unmarked estimate on sixth-power-free rows at longer column lengths.

Statement of the marked estimate

Let ν\nu be a fixed finite-order ray character whose full zero-extended defining modulus has prime support in SS. This entire presentation belongs to the fixed arithmetic datum; a locally frozen moving zero support is instead retained as a puncture whose radical is included in the explicit norm bound below. Fix one sign εχ∈{1,−1}\varepsilon_\chi\in\{1,-1\}, and set

ψu(n)=ν(n)χn(u)εχ.\psi_u(n)=\nu(n)\chi_n(u)^{\varepsilon_\chi}.

The only masks in this definition are the fixed exclusions and the zero extension of χn(u)\chi_n(u). For a smooth annular function WW, define

Mu(Zr;W)=Z−r/2∑nμ(n)ψu(n)W(qn/Zr).M_u(Z^r;W)=Z^{-r/2}\sum_n\mu(n)\psi_u(n)W(q_n/Z^r).

For a fixed finite set II of slots, let Pi\mathcal{P}_i be disjoint sets of primes outside SS, with qp≍Zziq_p \asymp Z^{z_i} for p∈Pip \in\mathcal{P}_i. The sets and the coefficients ai(p)a_i(p) are independent of uu, and ∣ai(p)∣≤1|a_i(p)| \le1. Given fixed smooth annular functions WiW_i, put

Qu=∏i∈IZ−zi/2∑p∈Piai(p)ψu(p)Wi(qp/Zzi),z=∑i∈Izi.Q_u=\prod_{i\in I}Z^{-z_i/2}\sum_{p\in\mathcal{P}_i}a_i(p)\psi_u(p)W_i(q_p/Z^{z_i}),\qquad z=\sum_{i\in I}z_i.

The empty product is one. A fixed finite sum of whole products MuQuM_uQ_u is also allowed by triangle inequality, provided each summand uses one common ν\nu in its inverse and all of its slots.

Lemma 17.1 (Marked inverse moment). Fix bounded ranges for the nonnegative parameters m,r,zim,r,z_i, a bound for ∣I∣|I|, and positive constants c1,c2c_1,c_2. Suppose

r+2z≤m−c1,2r+8z≤3m−c2.r+2z\le m-c_1,\qquad2r+8z\le3m-c_2.

Then, for every ϵ>0\epsilon>0,

∑u∈O0<qu≪Zm∣Mu(Zr;W)Qu∣2≪Zm+ϵ.\sum_{\substack{u\in\mathcal O\\0<q_u\ll Z^m}} |M_u(Z^r;W)Q_u|^2\ll Z^{m+\epsilon}.

The implied constant may depend on the fixed arithmetic data, c1,c2c_1,c_2, the bounded parameter ranges, and finitely many smooth seminorms of the tests, but is uniform in the prime supports and their bounded coefficients. The assertion holds for either common sign εχ\varepsilon_\chi, and for every subcollection of the slots. Norm twists of the tests have a fixed polynomial cost in their heights. There is no lower bound on the individual slot lengths other than the existence of their stated prime supports, and no mesh condition on those lengths.

The proof passes through the canonical family defined next, in which a fourth-power residue symbol is averaged over an additional squarefree ideal. Lemma 17.2 is proved by a terminal application of Lemma 14.3 and a recursive step using two masked Poisson transformations. After the principal contributions and tails have been handled, the retained part is bounded in terms of new admissible sums of that family with a shorter row range. A separate initialization using one masked Poisson transformation then deduces Lemma 17.1, and the final subsection gives its longer unmarked consequence for sixth-power-free rows.

The canonical estimate

Use the fixed puncture, squarefree coefficient, row character, and product-form mark defined in Section 14. The additional squarefree label is now averaged, with a divisor-bounded weight depending on that label alone.

The following is the statement closed by the two Poisson transformations. Its puncture bound is part of the hypothesis, because a frozen moving modulus cannot be treated as part of the fixed arithmetic data. For the recursive Poisson large-sieve framework, compare [16 Section 2], [17 Section 4], and [13 Sections 4–7]; the present marked recursion is proved below.

Lemma 17.2 (Canonical marked estimate). *Fix bounded nonnegative ranges for M,N,V,z0M,N,V,z_0, a bound for the number of slots, and c∗>0c_*>0. Let ff range over squarefree ideals outside SS with qf≍ZVq_f\asymp Z^V. Let ww be a nonnegative function of ff alone satisfying w(f)≤CdO(f)Cw(f)\le C d_{\mathcal O}(f)^C for one fixed C≥1C\ge1. Neither CC nor the choice of ww depends on ZZ, the current rows, or any other averaged variable. The implied constant below may depend on CC, but is uniform over all ww satisfying this fixed bound. Let ν\nu be a fixed multiplicative finite ray character whose full zero-extended defining modulus has prime support in SS, and let ρ(n)=1(n,rρ)=1\rho(n)=1_{(n,\mathfrak r_\rho)=1} be a fixed puncture. Both are independent of k,fk,f. Let d\mathfrak d have the product form in (14.1), with disjoint fixed prime lists of total length at most z0z_0 and bounded coefficients independent of k,fk,f. No other row-dependent column coefficient or puncture is allowed. There is no additional residual coefficient b(n)b(n), even one independent of kk, ff: arbitrary bounded weights are permitted only as the stated product of individual prime-slot coefficients.

Put F0=N+VF_0=N+V. Suppose

qrρ≤ZF0−M−z0−c∗,3M+6z0+c∗≤4F0.\begin{gathered} q_{\mathfrak r_\rho}\le Z^{F_0-M-z_0-c_*},\\ 3M+6z_0+c_*\le4F_0. \end{gathered}

For every smooth annular WW and every ϵ>0\epsilon>0, define

E=Z−V∑fw(f)∑k∈O0<qk≪ZM∣Z−N/2∑n sfαˉ(n)γ2(n)ν(n)ρ(n)×χn(k)χn(f)4d(n)W(qn/ZN)∣2.\begin{aligned} \mathcal E={}&Z^{-V}\sum_f w(f) \sum_{\substack{k\in\mathcal O\\0<q_k\ll Z^M}} \Biggl|Z^{-N/2}\sum_{n\ {\rm sf}} \bar\alpha(n)\gamma_2(n)\nu(n)\rho(n)\\ &\hspace{24mm}\times \chi_n(k)\chi_n(f)^4\mathfrak d(n)W(q_n/Z^N)\Biggr|^2. \end{aligned}

Then E≪ZF0+ϵ\mathcal{E}\ll Z^{F_0+\epsilon}. The constant is uniform in the moving moduli and the frozen outer ideals within the stated ranges. It depends on finitely many smooth seminorms and has a fixed polynomial dependence on separated norm-twist heights. The same conclusion holds for all subcollections of the slots with the original cap z0z_0, including the empty collection.

The reflected energy in Section 14 supplies the terminal estimate for this family. The remaining ranges will be reduced to the same family with shorter rows. Before the two Poisson transformations, we give the common analytic rule for propagating smooth seminorm and height orders through the finite induction.

Finite propagation of seminorm and height orders

We use the following abstract statement about a finite sequence of estimates. It does not assert that any particular arithmetic reduction has its hypotheses. Its purpose is to state exactly which uniform bounds on transformed profiles and Fourier coefficient measures suffice to choose all internal derivative orders before an external height cutoff.

Write ⟨t⟩=1+∣t∣\langle\boldsymbol t\rangle=1+|\boldsymbol t|. Let a finite rooted directed graph have no directed cycles, and let every directed path have at most DD edges. At each vertex vv let Nv(Z,w,t)\mathcal N_v(Z,\boldsymbol w,\boldsymbol t) be a nonnegative quantity, where Z≥1Z\ge1, w\boldsymbol w is a fixed finite tuple of annular profiles, and t\boldsymbol t is a finite-dimensional height vector. The profile dimensions, supports, and height dimensions may depend on vv, but are fixed throughout the graph. Additional labels are allowed in these quantities; every bound below is required uniformly in those labels.

Lemma 17.3 (Finite seminorm propagation). Suppose that at each vertex there is a terminal bound

Tv(Z,w,t)≤CvZavpjv(w)bv⟨t⟩hv\mathcal T_v(Z,\boldsymbol w,\boldsymbol t) \le C_v Z^{a_v}p_{j_v}(\boldsymbol w)^{b_v} \langle\boldsymbol t\rangle^{h_v}

with fixed real ava_v and finite nonnegative jv,bv,hvj_v,b_v,h_v. Suppose also that

Nv(Z,w,t)≤Tv(Z,w,t)+∑e:v→v′Zae∫Rde∣Ke(Z,w,t;ξ)∣Nv′(Z,We,Aet+Beξ) dξ,\begin{aligned} \mathcal N_v(Z,\boldsymbol w,\boldsymbol t) \le{}&\mathcal T_v(Z,\boldsymbol w,\boldsymbol t)\\ &+\sum_{e:v\to v'}Z^{a_e}\int_{\mathbb R^{d_e}} |K_e(Z,\boldsymbol w,\boldsymbol t;\boldsymbol\xi)| \mathcal N_{v'}\bigl(Z,\boldsymbol W_e, A_e\boldsymbol t+B_e\boldsymbol\xi\bigr)\,d\boldsymbol\xi, \end{aligned}

where Ae,BeA_e,B_e are fixed bounded linear maps and We=We(Z,w,t,ξ)\boldsymbol W_e=\boldsymbol W_e(Z,\boldsymbol w,\boldsymbol t, \boldsymbol\xi) is the child profile tuple. Empty edge sums are allowed. Assume the following two bounds for each edge. For every fixed jj there are finite nonnegative numbers me(j),be′(j),ce′(j)m_e(j),b'_e(j),c'_e(j) and a constant Ce,jC_{e,j} such that

pj(We)≤Ce,jpme(j)(w)be′(j)⟨t⟩ce′(j)⟨ξ⟩ce′(j).p_j(\boldsymbol W_e) \le C_{e,j}p_{m_e(j)}(\boldsymbol w)^{b'_e(j)} \langle\boldsymbol t\rangle^{c'_e(j)} \langle\boldsymbol\xi\rangle^{c'_e(j)}.

For every fixed H≥0H \ge0 there are finite nonnegative numbers ℓe(H)\ell_e(H), be(H)b_e(H), ce(H)c_e(H) and a constant Ce,HC_{e,H} such that

∫Rde∣Ke(Z,w,t;ξ)∣⟨ξ⟩H dξ≤Ce,Hpℓe(H)(w)be(H)⟨t⟩ce(H).\int_{\mathbb R^{d_e}}|K_e(Z,\boldsymbol w,\boldsymbol t; \boldsymbol\xi)|\langle\boldsymbol\xi\rangle^H \,d\boldsymbol\xi \le C_{e,H}p_{\ell_e(H)}(\boldsymbol w)^{b_e(H)} \langle\boldsymbol t\rangle^{c_e(H)}.

The seminorm indices may be rounded up to integers. All these constants and indices are uniform in ZZ and the additional labels; the exponents av,aea_v,a_e are fixed real numbers independent of the requested seminorm and height orders.

Then there are finite JJ, BB, HH and CC such that, at the root v0v_0,

Nv0(Z,w,t)≤CZEpJ(w)B⟨t⟩H,E=max⁡v0→⋯→v(av+∑e on the pathae).\mathcal N_{v_0}(Z,\boldsymbol w,\boldsymbol t) \le C Z^E p_J(\boldsymbol w)^B\langle\boldsymbol t\rangle^H, \qquad E=\max_{v_0\to\cdots\to v} \left(a_v+\sum_{e\text{ on the path}}a_e\right).

The indices JJ, BB, HH can be selected backward through the at most DD stages. In particular they are fixed before any restriction ∣t∣≤T1=Zτ|\boldsymbol t|\le T_1=Z^\tau is imposed.

The same conclusion holds for a finite product of children in an integral. Precisely, an edge term may instead have the form

Zae∫Rde∣Ke∣∏r=1reNve,r(Z,We,r,Ae,rt+Be,rξ)θe,r dξ,Z^{a_e}\int_{\mathbb R^{d_e}}|K_e| \prod_{r=1}^{r_e} \mathcal N_{v_{e,r}}\bigl(Z,\boldsymbol W_{e,r}, A_{e,r}\boldsymbol t+B_{e,r}\boldsymbol\xi\bigr)^{\theta_{e,r}} \,d\boldsymbol\xi,

where re≥1r_e\ge1 is a fixed integer and θe,r≥0\theta_{e,r}\ge0 are fixed, all children have smaller remaining depth, and each child profile satisfies its own version of the stated profile bound. The joint coefficient measure satisfies the same weighted bound. In this case define the norm exponent recursively by

Ev=max⁡{av,max⁡e(ae+∑r=1reθe,rEve,r)}.E_v=\max\left\{a_v,\max_e\left(a_e+\sum_{r=1}^{r_e}\theta_{e,r}E_{v_{e,r}}\right)\right\}.

The conclusion holds with E=Ev0E=E_{v_0}. This form includes the square roots of two nonnegative child estimates arising from Cauchy–Schwarz.

Proof. At a terminal vertex the assertion is its stated bound. Suppose a child has already been bounded by CZE′pJ′(We)B′⟨Aet+Beξ⟩H′C Z^{E'}p_{J'}(\boldsymbol W_e)^{B'} \langle A_e\boldsymbol t+B_e\boldsymbol\xi\rangle^{H'}. Since the linear maps are bounded,

⟨Aet+Beξ⟩H′≪e⟨t⟩H′⟨ξ⟩H′.\langle A_e\boldsymbol t+B_e\boldsymbol\xi\rangle^{H'} \ll_e\langle\boldsymbol t\rangle^{H'} \langle\boldsymbol\xi\rangle^{H'}.

The child-profile bound adds the power B′ce′(J′)B'c'_e(J') to each of these two height exponents and replaces its profile factor by pme(J′)(w)B′be′(J′)p_{m_e(J')}(\boldsymbol w)^{B'b'_e(J')}. Use the coefficient-measure bound with He=H′+B′ce′(J′)H_e=H'+B'c'_e(J'). The contribution of this edge is at most

CeZae+E′pmax⁡{me(J′),ℓe(He)}(w)B′be′(J′)+be(He)⟨t⟩He+ce(He).C_e Z^{a_e+E'} p_{\max\{m_e(J'),\ell_e(H_e)\}}(\boldsymbol w)^{B'b'_e(J')+b_e(H_e)} \langle\boldsymbol t\rangle^{H_e+c_e(H_e)}.

Every displayed index is finite. Take the maximum of these indices and of the terminal indices over the finitely many outgoing edges, increasing the profile exponent when necessary because pj(w)≥1p_j(\boldsymbol w)\ge1. This proves the parent bound with exponent equal to the maximum path exponent through that vertex. Reverse induction on the acyclic graph completes the proof. None of these choices mentions an external cutoff or a late derivative order.

For the product form, insert the already proved bound of each child and raise it to θe,r\theta_{e,r}. The total power of ⟨ξ⟩\langle\boldsymbol\xi\rangle that the coefficient measure must integrate is

He=∑r=1reθe,r(Hr+Brce,r′(Jr)).H_e=\sum_{r=1}^{r_e}\theta_{e,r} \bigl(H_r+B_r c'_{e,r}(J_r)\bigr).

The powers of the parent profile and of ⟨t⟩\langle\boldsymbol t\rangle are the corresponding finite sums, followed by the single coefficient-measure bound at HeH_e. The powers of ZZ add as in the displayed recurrence for EvE_v. Taking maxima over the finitely many terms proves this extension by the same reverse induction. ∴

Corollary 17.4 (Indexed finite propagation). In Lemma 17.3, let ℓ\boldsymbol\ell denote any admissible length and outer labels at a vertex vv, and let Φv(ℓ)\Phi_v(\boldsymbol\ell) be its desired norm exponent. Suppose the terminal bound, after division by ZΦv(ℓ)Z^{\Phi_v(\boldsymbol\ell)}, has the form in that lemma with a fixed exponent δv\delta_v. An edge may be indexed by a ZZ-dependent family Γe\Gamma_e with a nonnegative measure νe\nu_e, and may have the form

∫Γe∫RdeZae(ℓ,γ)∣Ke,γ∣∏r=1reNve,r(Z,ℓe,r,We,r,Ae,rt+Be,rξ)θe,r dξ dνe(γ),\int_{\Gamma_e}\int_{\mathbb R^{d_e}} Z^{a_e(\boldsymbol\ell,\gamma)}|K_{e,\gamma}| \prod_{r=1}^{r_e}\mathcal N_{v_{e,r}} \bigl(Z,\boldsymbol\ell_{e,r},\boldsymbol W_{e,r}, A_{e,r}\boldsymbol t+B_{e,r}\boldsymbol\xi\bigr)^{\theta_{e,r}} \,d\boldsymbol\xi\,d\nu_e(\gamma),

where the child labels ℓe,r\boldsymbol\ell_{e,r} may depend on ℓ,γ\boldsymbol\ell,\gamma. Assume uniformly in those labels that

ae(ℓ,γ)+∑rθe,rΦve,r(ℓe,r)−Φv(ℓ)≤δe,a_e(\boldsymbol\ell,\gamma) +\sum_r\theta_{e,r}\Phi_{v_{e,r}}(\boldsymbol\ell_{e,r}) -\Phi_v(\boldsymbol\ell)\le\delta_e,

with fixed δe\delta_e, and that the child-profile bounds of the lemma hold. Assume also that for every fixed H≥0H\geq0,

∫Γe∫Rde∣Ke,γ∣⟨ξ⟩H dξ dνe(γ)≤Ce,HZδemasspℓe(H)(w)be(H)⟨t⟩ce(H),\int_{\Gamma_e}\int_{\mathbb R^{d_e}}|K_{e,\gamma}| \langle\boldsymbol\xi\rangle^H\,d\boldsymbol\xi\,d\nu_e(\gamma) \le C_{e,H}Z^{\delta_e^{\mathrm{mass}}} p_{\ell_e(H)}(\boldsymbol w)^{b_e(H)} \langle\boldsymbol t\rangle^{c_e(H)},

where δemass\delta_e^{\mathrm{mass}} is fixed independently of HH. When the quantities are squared Hilbert-space row norms obtained by separating a profile, this hypothesis must use the coefficient measure common to those rows. There need only be finitely many edge types at each of the finitely many depths; the cardinalities of the Γe\Gamma_e may vary with ZZ.

Then Nv/ZΦv(ℓ)\mathcal N_v/Z^{\Phi_v(\boldsymbol\ell)} has the conclusion of Lemma 17.3, uniformly in ℓ\boldsymbol\ell, with terminal exponents δv\delta_v and edge exponents δe+δemass\delta_e+\delta_e^{\mathrm{mass}}. In particular all required seminorm and height orders are finite and independent of an external cutoff.

Proof. Set N‾v=Z−Φv(ℓ)Nv\overline{\mathcal N}_v=Z^{-\Phi_v(\boldsymbol\ell)}\mathcal N_v. Substitution in an edge and (17.4) bound its norm power by ZδeZ^{\delta_e} times the product of the normalized children. Insert their inductive bounds. As in the product proof of Lemma 17.3, the required coefficient moment is

He=∑rθe,r(Hr+Brce,r′(Jr)).H_e=\sum_r\theta_{e,r}\bigl(H_r+B_{r}c'_{e,r}(J_r)\bigr).

which is finite and independent of γ\gamma. (17.5) at this order contributes ZδemassZ^{\delta_e^{\mathrm{mass}}} and only finite profile and height orders. Backward induction over the finite edge types therefore gives exactly the stated normalized recurrence. A label averaged inside a child remains inside that child throughout this argument; it is not a second integration variable of νe\nu_e. □\square

We make explicit how discrete labels are normalized in this corollary. After the relevant weighted Cauchy inequality, suppose a nonnegative outer measure satisfies ∑γ∈Γwγ≤CZc+ϵ\sum_{\gamma\in\Gamma}w_\gamma\leq CZ^{c+\epsilon}, with fixed cc and ϵ\epsilon selected before the height orders. For a per-label prefactor ZarawZ^{a_{\mathrm{raw}}} common on the block, put

dνΓ(γ)=Z−c∑γ∈Γwγδγ,νΓ(Γ)≤CZϵ.d\nu_\Gamma(\gamma)=Z^{-c}\sum_{\gamma\in\Gamma}w_\gamma\delta_\gamma,\qquad\nu_\Gamma(\Gamma)\leq CZ^\epsilon.

Here δγ\delta_\gamma denotes unit point mass. For nonnegative BγB_\gamma for which the displayed integrals are finite, the exact identity is

Zaraw∑γ∈Γwγ∫∣Kγ(ξ)∣Bγ(ξ) dξ=Zaraw+c∫Γ∫∣Kγ(ξ)∣Bγ(ξ) dξ dνΓ(γ).\begin{aligned} &Z^{a_{\mathrm{raw}}}\sum_{\gamma\in\Gamma}w_\gamma \int |K_\gamma(\boldsymbol\xi)|B_\gamma(\boldsymbol\xi) \,d\boldsymbol\xi\\ &\qquad=Z^{a_{\mathrm{raw}}+c} \int_\Gamma\int |K_\gamma(\boldsymbol\xi)|B_\gamma(\boldsymbol\xi) \,d\boldsymbol\xi\,d\nu_\Gamma(\gamma). \end{aligned}

Uniform weighted moments of KγK_\gamma now give (17.5) with only the remaining ZϵZ^\epsilon mass. Thus a displayed exponent that already includes the count cc must use this normalized measure; retaining the unnormalized sum would count the same labels twice. The rule concerns weighted mass, not cardinality in addition to that mass. It is applied only after any row-dependent eligibility remains within the child or has been removed by a nonnegative inequality. Labels still averaged in a child norm are not included in Γ\Gamma.

There is a separate normalization for a small kernel amplitude. The single-profile seminorm pj(w)p_j(w) is homogeneous, whereas pj(w)=1+∑pj(wi)p_j(\boldsymbol w)=1+\sum p_j(w_i) is not. Suppose a joint annular profile on a fixed block satisfies, for a scalar 0<mR≤10<m_R\le1,

pj(FR)≤mRCjpℓ(j)(w)b(j)⟨t⟩h(j)(j≥0).p_j(F_R)\le m_R C_j p_{\ell(j)}(\boldsymbol w)^{b(j)} \langle\boldsymbol t\rangle^{h(j)} \qquad(j\ge0).

One may keep FRF_R in the Fourier coefficient measure, whose weighted L1L^1 norm then contains the factor mRm_R. Alternatively, write FR=mRF~RF_R=m_R\widetilde{F}_R and put mRm_R outside that measure. If a polynomial or row vector P(FR)\mathcal{P}(F_R) is linear in this whole profile, then

P(FR)=mRP(F~R),∥P(FR)∥22=mR2∥P(F~R)∥22.\mathcal{P}(F_R)=m_R\mathcal{P}(\widetilde{F}_R),\qquad\|\mathcal{P}(F_R)\|_2^2=m_R^2\|\mathcal{P}(\widetilde{F}_R)\|_2^2.

The tuple containing F~R\widetilde{F}_R has bounded, not small, seminorms. A scalar may be removed from a centered difference only when it multiplies the whole difference. A kernel occurring once in an already expanded quadratic expression contributes one factor mRm_R, not automatically its square. These conventions use either the small measure or the outside scalar, never both. If the positive row range will later be enlarged, the scalar and the common profile are first fixed on the actual annuli, and the norm inequality containing that scalar is obtained before the enlargement.

Here are sufficient analytic ways to verify the two edge hypotheses. Let m(y)m(\boldsymbol y) be a fixed norm monomial and let χ\chi be a smooth cutoff with compact logarithmic support in a product of fixed annuli. Suppose a normalized kernel has Euler bounds

∣(r∂r)jK(r)∣≤CA,jSm(A,j)min⁡(1,r−A),|(r\partial_r)^jK(r)|\le C_{A,j}\mathfrak{S}_{m(A,j)}\min(1,r^{-A}),

where Sk\mathfrak{S}_k is an increasing family of specified finite input seminorm and polynomial height bounds, and m(A,j)m(A,j) is taken nondecreasing in jj. The product and chain rules give, uniformly for R>0R>0,

pj(χ(y)K(Rm(y)))≤CA,j′Sm(A,j)min⁡(1,R−A).p_j\bigl(\chi(\boldsymbol y)K(Rm(\boldsymbol y))\bigr) \le C'_{A,j}\mathfrak S_{m(A,j)}\min(1,R^{-A}).

Indeed yi∂yiy_i\partial_{y_i} acting on the kernel is the fixed exponent of yiy_i in mm times r∂rr\partial_r, and mm is bounded above and below on the cutoff support. There is no extra factor RR from differentiation. The same argument preserves a bound with min⁡(R1/4,1,R−A)\min(R^{1/4},1,R^{-A}), when those three kernel estimates are available. The decay order AA is the same at every requested jj; only the input order and its finite height degree increase. For an old window w(cm(y))w(c m(\boldsymbol y)) with c>0c>0, Euler derivatives are bounded by the global logarithmic seminorms of ww and introduce no power of cc depending on the derivative order. Normalized real powers such as y−1/2y^{-1/2} obey the same rule. Pure twists of normalized norms insert only fixed powers of their heights.

Ordinary radial Fourier seminorms must be used only after the radial scale has been normalized. For a fixed annular ww in two real dimensions, fR(x)=w(R∣x∣2)f_R(x)=w(R|x|^2) satisfies

∥∂jfR∥1=Rj/2−1∥∂jf1∥1.\|\partial^j f_R\|_1=R^{j/2-1}\|\partial^j f_1\|_1.

for any fixed directional derivative of order jj, by x↦Rxx\mapsto\sqrt{R}x. Thus an unnormalized shrinking radial test could introduce a scale power depending on jj. Sufficient hypotheses are a fixed-shape radial Schwartz test at its stated row scale, or a radial Cc∞C_c^\infty test constant near zero at that scale. After normalization, Lemma 4.7 applies to its fixed transform, and moving scale ratios enter only as in Equation (17.7). For example qu−1/2=U0−1/2y−1/2q_u^{-1/2}=U_0^{-1/2}y^{-1/2} on qu=U0yq_u=U_0y; the central power belongs to the norm exponent, and the annular factor has order-independent scale bounds. Likewise quit=U0ityitq_u^{it}=U_0^{it}y^{it}, and the central unit phase is factored as a scalar before differentiating the normalized profile.

Logarithmic Fourier separation uses a joint cutoff in a coordinate list containing every normalized norm occurring in a coupled smooth factor. Derived nonsmooth row and label masks remain outside that factor and need no coordinate. A nonzero norm used as such a coordinate and initially ranging in a ball down to norm one must first be partitioned into common whole annuli fixed for the current sector; the zero frequency is separate. In bounded logarithmic ranges there are O((1+log⁡Z)d)O((1+\log Z)^d) such blocks for a fixed number dd of variables, so their count costs a preselected small power. The cutoff and its full support depend only on the block centers and fixed data, not on the individual values of the labels inside a row norm. Provided the coupled smooth factor is this one joint function with no further dependence on the individual labels, its Fourier density is common to those rows, as required by Lemma 4.5; separate uniform bounds for row-dependent densities would not imply the same Hilbert-space inequality. Nonsmooth masks are retained or resolved by exact arithmetic identities, never differentiated or incorporated as label-dependent sharp Fourier selectors.

Finally, suppose an internal dyadic ratio R>ZξR>Z^\xi, with fixed ξ>0\xi>0, has absolute arithmetic count at most ZBRbZ^B R^b. A coefficient bound with the factor R−AR^{-A} gives, for A>bA>b,

∑R dyadicR>ZξZBRb−A≪ZB−ξ(A−b).\sum_{\substack{R\ \mathrm{dyadic}\\ R>Z^\xi}} Z^B R^{b-A} \ll Z^{B-\xi(A-b)}.

Choose AA from the fixed BB, bb, ξ\xi and the desired internal saving. The actual bound may also have finite input seminorm and polynomial height factors; these enter the finite propagation graph. This tail estimate is not a height-free assertion uniform in all heights. Parameter Sobolev adds only a fixed number of profile derivatives and height dimensions, and all these internal orders are chosen before an external cutoff.

Finally suppose the graph and all of its kernel and annular orders have been fixed, giving height degree HH. Suppose an additional, external separation uses annular profiles with pjp_j bounded uniformly in ZZ for every fixed jj, or nonannular profiles with the weighted Mellin or annular norms in the preceding lemmas uniformly bounded at every fixed order, and its discarded integrand has bound ZB0⟨t⟩J0Z^{B_0}\langle\boldsymbol t\rangle^{J_0} with fixed B0,J0B_0,J_0. The external truncation is required to remain outside the graph: it does not replace a profile w\boldsymbol w or a kernel KeK_e by a cutoff-dependent profile. Given a retained-height allowance δ>0\delta>0, first choose 0<τ<δ/(1+H)0<\tau<\delta/(1+H). Then (1+T1)H≤2HZδ(1+T_1)^H\leq2^H Z^\delta for T1=ZτT_1=Z^\tau. After this choice, (4.10) with weight J0J_0 and any fixed integer N>(B0+M)/τN>(B_0+M)/\tau makes an integrated external tail O(Z−M)O(Z^{-M}) for any prescribed M>0M>0. For a horizontal join use (4.11) with the additional fixed height weight, or (4.12) for a joint Gaussian slice. When other coordinates on such a slice are extended to the whole real line, the accompanying arithmetic factors must have global bounds on those coordinates; a coordinate entering a denominator controlled only in a buffered region must remain restricted to that region. The external constants may depend on NN and on the fixed data. This late choice does not alter any internal profile or the internal orders J,HJ,H, which is the asserted order of dependence.

Finite Poisson summation with a mask

We now prove Lemma 17.1, using the arithmetic conventions of Section 4 and Lemma 14.3 for the terminal case. The recursive reduction uses two applications of the following form of Poisson summation, and the initialization uses one. Its explicit divisor variable retains every zero extension.

Lemma 17.5 (Masked primitive Poisson). Let ψ\psi be a primitive finite character modulo an ideal mm, extended by zero on nonunits, and let RR be any ideal. Let Φ(qz)\Phi(q_z) be a radial Schwartz function on C\mathbb{C}, and let FΦ(qy)\mathcal{F}\Phi(q_y) denote its Fourier transform for the self-dual measure and the kernel e(−zy)e(-zy). For K>0K>0,

∑k∈Oψ(k)1(k,R)=1Φ(qk/K)=Kγ(ψ;m)qm∑d∣rad⁡Rμ(d)ψ(d)qd∑h∈Oψ‾(h)FΦ(Kqhqdqm)\sum_{k\in\mathcal{O}} \psi(k)1_{(k,R)=1}\Phi(q_k/K) = \frac{K\gamma(\psi;m)}{\sqrt{q_m}}\sum_{d\mid\operatorname{rad} R}\frac{\mu(d)\psi(d)}{q_d}\sum_{h\in\mathcal{O}}\overline{\psi}(h)\mathcal{F}\Phi\left(\frac{Kq_h}{q_dq_m}\right)

where γ(ψ;m)=qm−1/2∑x mod mψ(x)e(x/m)\gamma(\psi;m)=q_m^{-1/2}\sum_{x\bmod m}\psi(x)e(x/m). For a nonprincipal primitive character, ∣γ(ψ;m)∣=1|\gamma(\psi;m)|=1 and the h=0h=0 term is zero. For the primitive principal character the conventions are m=1m=1, γ(1;1)=1\gamma(1;1)=1, ψ(h)=1\psi(h)=1, including at h=0h=0.

Proof. Expand the mask as ∑d∣rad⁡R, d∣kμ(d)\sum_{d\mid\operatorname{rad} R,\ d\mid k}\mu(d) and write k=dk′k=dk'. The scale becomes K/qdK/q_d and the character contributes ψ(d)\psi(d). Poisson summation in residue classes modulo mm has prefactor K/(qdqm)K/(q_dq_m). Its finite transform is

∑x mod mψ(x)e(hx/m)=qmγ(ψ;m)ψ‾(h).\sum_{x\bmod m}\psi(x)e(hx/m)=\sqrt{q_m}\gamma(\psi;m)\overline{\psi}(h).

For unit hh this follows by changing variables. For nonunit hh the transform is zero by primitivity; for m=1m=1 the stated principal convention applies. This proves (17.8). For a nonprincipal primitive character, finite Parseval gives ∑h∣∑xψ(x)e(hx/m)∣2=qm∑x∣ψ(x)∣2\sum_h\left|\sum_x\psi(x)e(hx/m)\right|^2=q_m\sum_x|\psi(x)|^2. Writing ϕ(m)=∣(O/m)×∣\phi(m)=|(\mathcal{O}/m)^\times|, there are ϕ(m)\phi(m) unit hh's, all with magnitude qm∣γ(ψ;m)∣\sqrt{q_m}|\gamma(\psi;m)|, and ∑x∣ψ(x)∣2=ϕ(m)\sum_x|\psi(x)|^2=\phi(m). Thus ∣γ(ψ;m)∣=1|\gamma(\psi;m)|=1.

A fixed ray restriction can first be expanded into finitely many characters. Each is then replaced by its primitive inducing character, with the removed local zero extensions kept in RR; the same formula applies term by term. For the principal modulus the absolute sum of the nonzero frequencies is OΦ(dO(rad⁡R))O_\Phi(d_{\mathcal O}(\operatorname{rad} R)). Indeed, for all A>0A>0,

A∑h≠0∣FΦ(Aqh)∣≪Φ1.A\sum_{h\ne0}|\mathcal{F}\Phi(Aq_h)|\ll_\Phi1.

Lattice counting proves this when A≤1A\le1, and Schwartz decay proves it when A≥1A\ge1. Sum this bound with A=K/qdA=K/q_d over dd. At every use below the relevant nonempty row scale has K≥1K\ge1, so this is also O(KZε)O(KZ^\varepsilon). When principal nonzero frequencies are added or removed while separating a nonprincipal sum, they will carry the same outer row mask as that sum; their absolute contribution is no larger than this full principal bound.

The canonical reduction and its induction

We now prove Lemma 17.2. The reflected energy handles the short completion; the remaining blocks undergo two Poisson transformations to produce admissible canonical sums with shorter rows.

Proof of Lemma 17.2. The order of the analytic choices is organized by Corollary 17.4 in Section 17.3. Its indexed conclusion will be used on each positive Cauchy-side sum separately; the proof below verifies the required common coefficient measures, fixed norm losses, and finite depth.

At each node, every joint (f,k)(f,k) Hilbert space uses the current label measure w(f)w(f), and that factor is retained exactly once in every parent ff-sum until (17.32) removes the old label.

At each node keep the parameters N,V,MN,V,M fixed, and write

F=N+V,Q=log⁡Zqrρ.F=N+V,\qquad Q=\log_Zq_{\mathfrak r_\rho}.

Here FF is the real length sum N+VN+V, so F=F0F=F_0 at the starting node. The two hypotheses at a node with margin cnodec_{\mathrm{node}} are exactly

F−M−Q−z0≥cnode,4F−3M−6z0≥cnode.F-M-Q-z_0 \ge c_{\mathrm{node}}, \qquad4F-3M-6z_0 \ge c_{\mathrm{node}}.

In particular M+z0+cnode≤FM+z_0+c_{\mathrm{node}}\le F. The number QQ is the actual logarithmic norm of the already fixed puncture radical, not a dyadic center. The parameter MM is the fixed logarithmic row length; the first Poisson test has scale ZMZ^M.

Let Mmax⁡M_{\max} bound the starting row lengths. Choose 0<d≤c∗/2000<d\le c_*/200 and put

D=⌈Mmax⁡+2d⌉+1.D=\left\lceil\frac{M_{\max}+2}{d}\right\rceil+1.

We use positive parameters η\eta, τ\tau, π\pi, τref\tau_{\mathrm{ref}}, πref\pi_{\mathrm{ref}}, chosen in the quantified order at the end of the proof. Here η\eta is a localization tolerance bounding only the logarithms of fixed annular ratios, τ\tau is the common tolerance in the two Poisson tail comparisons, and π\pi bounds the aggregate freely chosen local small-power losses. At depth hh set

ch=c∗−7hη,cnode=ch,c_h=c_*-7h\eta,\qquad c_{\mathrm{node}}=c_h,

and impose the row cap M≤Mmax⁡−hdM\le M_{\max}-hd. We prove the estimate by backwards induction on h≤Dh\le D. Every retained row parameter below is nonnegative. We shall show that a nonterminal passage decreases it by at least dd, loses at most 7η7\eta in either required margin, and increases the energy exponent by at most 40η+τ+π40\eta+\tau+\pi. No invariant will be transferred from the fixed F=N+VF=N+V to an actual column norm.

The short completion. Möbius inversion of the cube factor in Equation (14.2) gives the exact identity

Z−N/2∑n sfa(n)χn(k)χn(f)4d(n)W(qn/ZN)=∑hμ(h)αˉ(h)3Ψk(h)3qhTdh(ZN/qh3;k),dh(A)=d(h3A).\begin{aligned} &Z^{-N/2}\sum_{n\ {\rm sf}}a(n)\chi_n(k)\chi_n(f)^4 \mathfrak d(n)W(q_n/Z^N)\\ &\quad= \sum_h\frac{\mu(h)\bar\alpha(h)^3\Psi_k(h)^3}{q_h} \mathcal T_{\mathfrak d_h}(Z^N/q_h^3;k), \qquad \mathfrak d_h(A)=\mathfrak d(h^3A). \end{aligned}

To check both the mark and the normalization, expand the right side and put c=hbc=hb. The factor V∗(y)=y1/2W(y)V_*(y)=y^{1/2}W(y) changes the absolute coefficient to

Z−N/2α‾(c)3Ψk(c)3qc1/2∑h∣cμ(h).Z^{-N/2}\overline{\alpha}(c)^3\Psi_k(c)^3q_c^{1/2}\sum_{h\mid c}\mu(h).

The mark is d(nc3)\mathfrak d(nc^3), independent of the divisor hh. The divisor sum vanishes unless c=1c=1, proving the identity. Multiplicativity of Ψk\Psi_k, including its punctures, is used here.

Use one fixed smooth dyadic partition with nonnegative ideal centers, the unit dyad having center zero. Suppose V<dV<d and that the center ℓ1\ell_1 of the hh-dyad is less than dd. Freeze hh, assign to it the slots it divides, and retain the others on the completed index. A surviving slot then has the individual coefficient ai(p)1p∤ha_i(p)1_{p\nmid h}. Since hh is fixed, this is a bounded coefficient independent of the current kk, ff, on the same nominal annulus and with the same cap. It is not the unrestricted original coefficient; the recursive branch below restores its original slot lists separately by the child zeros. For an active subcollection define zaz_a to be the sum of its nominal slot lengths. Assignments only delete slots, so 0≤za≤z00\le z_a\le z_0 exactly; an actual tuple norm is never used as this cap. Triangle inequality in the joint (f,k)(f,k) Hilbert space uses ∑qh≍Zℓ1qh−1≪1\sum_{q_h\asymp Z^{\ell_1}}q_h^{-1}\ll1 for the fixed annulus, apart from the separately chosen divisor loss for assignments. The bounded factor Ψk(h)3\Psi_k(h)^3 is a contraction in that space.

Write h^=log⁡Zqh\widehat{h}=\log_Z q_h. The completion is at the actual scale N∗=N−3h^N_* = N-3\widehat{h}. Its fixed support gives h^≤ℓ1+η<d+η\widehat{h}\leq\ell_1+\eta<d+\eta once the fixed annular threshold specified below is imposed. In Lemma 14.3, keep the actual residual-row dyad and choose the same threshold so that

H≤M−O+η,Td−S0−B0≤2M−O+Q+V−N∗+2za+η.H\leq M-O+\eta,\qquad T_d-S_0-B_0\leq2M-O+Q+V-N_*+2z_a+\eta.

These are Equations (5.35) and ((14.17)), not estimates for an enlarged row range. Substituting N∗=N−3h^N_*=N-3\widehat{h} and the first inequality in Equation (17.9) gives

Td−S0−B0≤M−O+2za−z0−cnode+5d+4η.T_d-S_0-B_0\leq M-O+2z_a-z_0-c_{\mathrm{node}}+5d+4\eta.

Indeed, the additional terms are 2V+3h^+η<5d+4η2V+3\widehat{h}+\eta<5d+4\eta.

Take the threshold also to ensure eλ≥−ηe_\lambda\geq-\eta, and discard the whole reflected tail dyads as in Lemma 14.3. Thus every retained dyad satisfies v+3ℓb+eλ≤Td+τrefv+3\ell_b+e_\lambda\leq T_d+\tau_{\mathrm{ref}}. The row branch of Equation (14.14), after dropping its nonpositive terms, obeys

Eref≤M+za+53η≤F−cnode+53η.E_{\mathrm{ref}}\leq M+z_a+\frac{5}{3}\eta\leq F-c_{\mathrm{node}}+\frac{5}{3}\eta.

For the column branch with u=zau=z_a, the retained dual bound first gives Eref≤O/2+(Td−S0−B0)+5η/3+τrefE_{\mathrm{ref}}\leq O/2+(T_d-S_0-B_0)+5\eta/3+\tau_{\mathrm{ref}}. Equation (17.12) and the first invariant then give

Eref≤F−2cnode+5d+173η+τref.E_{\mathrm{ref}}\leq F-2c_{\mathrm{node}}+5d+\frac{17}{3}\eta+\tau_{\mathrm{ref}}.

If u≠zau\ne z_a, its definition implies u≥v/2u\geq v/2. The retained dual bound now first gives

Eref≤O/2+(Td−S0−B0)/2+za+76η+12τref.E_{\mathrm{ref}}\leq O/2+(T_d-S_0-B_0)/2+z_a+\frac{7}{6}\eta+\frac{1}{2}\tau_{\mathrm{ref}}.

Using Equation (17.12), za≤z0z_a\leq z_0, and then the second invariant yields

Eref≤F−M/4−3cnode/4+(5/2)d+196η+12τref.E_{\mathrm{ref}}\leq F-M/4-3c_{\mathrm{node}}/4+(5/2)d+\frac{19}{6}\eta+\frac{1}{2}\tau_{\mathrm{ref}}.

Use the reflected estimate with aggregate local loss πref\pi_{\mathrm{ref}}, including its freely chosen exponent, the label divisor bound, and the finitely many logarithmic sums. If

cnode≥c∗/2,d≤c∗/200,η,τref,πref≤c∗/1000,c_{\mathrm{node}}\geq c_*/2,\qquad d\leq c_*/200,\qquad\eta,\tau_{\mathrm{ref}},\pi_{\mathrm{ref}}\leq c_*/1000,

all three bounds, after adding πref\pi_{\mathrm{ref}}, are strictly below FF. In the last bound M≥0M\geq0. For z0=0z_0=0 only u=za=0u=z_a=0 occurs. The reflected estimate was applied for each fixed ff; the weighted mass bound ∑fw(f)≪ZV+πref\sum_f w(f)\ll Z^{V+\pi_{\mathrm{ref}}} shows that summing its squared bounds over ff costs at most this amount, already included in the aggregate loss, and cancels the outside Z−VZ^{-V}. Thus no moving fourth-power label entered the hybrid norm, and these terminal terms satisfy the canonical estimate.

The remaining terms and their marks. At every factorization, assign a slot first to an extracted factor which its prime divides, and otherwise retain it on the residual column. The basic identity for the completion is

1p∣nb3=1p∣b+1p∤b1p∣n.1_{p\mid nb^3}=1_{p\mid b}+1_{p\nmid b}1_{p\mid n}.

More generally, for an ordered list of extracted factors D1,…,DhD_1,\ldots,D_h, the exact priority identity is

1p∣D1⋯Dhn=∑j=1h1p∣Dj∏a<j1p∤Da+1p∣n∏a≤h1p∤Da.1_{p\mid D_1\cdots D_h n} = \sum_{j=1}^{h}1_{p\mid D_j}\prod_{a<j}1_{p\nmid D_a} + 1_{p\mid n}\prod_{a\leq h}1_{p\nmid D_a}.

It holds even when extracted factors share primes. Applying it to each slot and each copy of a square gives a disjoint partition for each tuple of primes; the two copies of one slot have independent prime choices. There are at most 2∣I∣2^{|I|} choices at one single-factor assignment, and at most (h+1)∣I∣(h+1)^{|I|} for the displayed ordered list. The assigned slots have divisor-bounded coefficients on the extracted factor. Because the original coefficient is ∏iai(pi)\prod_i a_i(p_i), removing assigned slots leaves exactly a subcollection with its original product coefficients. An ideal which will remain an averaging variable is not fixed merely because a slot was assigned to it.

If V<dV<d and ℓ1≥d\ell_1\ge d, reopen the completion on the right of Equation (17.10). If its cube ideal is h′h', first isolate its dyad with center ℓ2≥0\ell_2\ge0 and the hh-dyad by triangle inequality in the joint Hilbert space, before squaring. Put b=hh′b=hh' and define the fixed centers

ℓ=ℓ1+ℓ2,r=N−3ℓ.\ell=\ell_1+\ell_2,\qquad r=N-3\ell.

Both copies b1,b2b_1,b_2 in the resulting square have this same nominal center ℓ\ell; their actual norms need not agree. The mark is d(nb3)\mathfrak d(nb^3), independent of the choice of the divisor hh of bb. Multiplicativity gives a factor χb(k)3\chi_b(k)^3; the fourth power in Ψk(b)3\Psi_k(b)^3 is exactly the mask 1(b,f)=11_{(b,f)=1}. The remaining sum over divisors hh of bb has absolute value at most a divisor function. After dyadic decomposition and separation of qnqb3/ZNq_nq_b^3/Z^N, each squared block is bounded by a small power times

Z−r−2ℓ−V∑fw(f)∑k∈OΦ(qk/ZM)∣∑qb≍Zℓβ(b,f)χb(k)3×∑n sfa(n)χn(k)χn(f)4d(nb3)W(qn/Zr)∣2.(A)\tag{A} \begin{aligned} &Z^{-r-2\ell-V}\sum_f w(f)\sum_{k\in\mathcal O}\Phi(q_k/Z^M) \Biggl|\sum_{q_b\asymp Z^\ell}\beta(b,f)\chi_b(k)^3\\ &\hspace{26mm}\times \sum_{n\ {\rm sf}}a(n)\chi_n(k)\chi_n(f)^4 \mathfrak d(nb^3)W(q_n/Z^r)\Biggr|^2 . \end{aligned}

Here Φ\Phi is a fixed nonnegative radial Schwartz function majorizing the original row ball, and ∣β(b,f)∣≪Zϵ|\beta(b,f)|\ll Z^\epsilon independently of k,nk,n. Its ff-dependence includes the original mask 1(b,f)=11_{(b,f)=1}; all other original cube masks are retained. There is no condition (b,n)=1(b,n)=1. The exponent in front is correct because the original normalization is Z−N/2qb1/2≍Z−r/2−ℓZ^{-N/2}q_b^{1/2}\asymp Z^{-r/2-\ell}. If V≥dV\ge d, use the same block with ℓ=0\ell=0, b=1b=1, r=Nr=N. Thus every remaining block has exactly V+ℓ≥dV+\ell\ge d, by the center classification and ℓ2≥0\ell_2\ge0. The added row k=0k=0 can only contribute in the principal cases counted below.

The two-transform reduction. We prove the following conditional estimate for every remaining block in Equation (A). Let ϵchild≥0\epsilon_{\mathrm{child}}\ge0. Suppose every energy E′\mathcal{E}' of the form (17.3), with all coefficient and support hypotheses of Lemma 17.2, the same fixed slot cap, parameters

0≤M′≤M−d,0≤N′,V′,F′=N′+V′≤F+11η,0\le M'\le M-d,\qquad0\le N',V',\qquad F'=N'+V'\le F+11\eta,

and both margins at least cnode−7ηc_{\mathrm{node}}-7\eta, satisfies E′≪ZF′+ϵchild\mathcal{E}'\ll Z^{F'+\epsilon_{\mathrm{child}}}. The hypothesis is uniform over the bounded ranges used in this induction, with finite-seminorm and fixed polynomial-height dependence as in that lemma. For η≤d/16\eta\le d/16, the remaining block satisfies

block in Equation (A)≪ZF+40η+τ+π+ϵchild,\text{block in Equation (A)} \ll Z^{F+40\eta+\tau+\pi+\epsilon_{\rm child}},

with the same kind of uniform dependence. The freely chosen local losses sum to π\pi; the principal terms and discarded tails are included in this estimate. Thus the reduction supplies exactly the implication needed for backwards induction. Its proof occupies the two transformations below: the first produces a positive inverse-polynomial norm, and the second constructs the smaller canonical energies to which the hypothesis applies.

We next specify the support and localization conventions used in both transformations. For an actual ideal or nonzero element aa, write a^=log⁡Zqa\widehat a=\log_Z q_a. For a named scalar center, aa hat will denote the actual logarithmic norm of its indicated ideal. All ideal centers introduced below are nonnegative centers from the fixed dyadic partition. The already fixed puncture and the ideal q0q_0 introduced below are used at their actual logarithmic norms, without independently rounded centers.

Every individual dyad introduced in the two transformations has a fixed compact normalized support. If aa is its ideal and acena_{\rm cen} its named logarithmic center, we use

∣log⁡Zqa−acen∣≤η.\left|\log_Z q_a-a_{\rm cen}\right|\leq\eta.

This convention applies to the original nin_i, bib_i, ff windows and to each extracted-ideal dyad when it is introduced. Errors for products and quotients are the sums of these individual errors; the fresh residual windows below have the explicitly stated bounds 4η4\eta, 6η6\eta and 4η4\eta. These estimates concern fixed compact normalized-ratio intervals, not annuli of ratio ZηZ^\eta.

For clarity, the intervals are fixed uniformly through the whole finite depth as follows. At each factorization choose fresh individual smooth cutoffs equal to one on the quotient supports, and include the full supports of these cutoffs, of the larger cutoffs used in Fourier separation, and of the enlarged label windows. Include also the bounded clipping families used below. Products and quotients of endpoints locate the initial quotient supports, such as those of b=hh′b=hh', the residual nn, and the child column and label. Iterating this construction through DD levels gives a finite collection ID\mathcal I_D of compact normalized-ratio intervals. If LwinL_{\rm win} is the maximum absolute logarithm of their endpoints, the threshold log⁡Z≥Lwin/η\log Z\geq L_{\rm win}/\eta implies (17.18) and all the fresh-support bounds specified below. After a positive sum is enlarged, its newly added columns or labels need not satisfy an old parent product identity. Their norm bounds at this and the next node come directly from the full independent fresh windows in ID\mathcal I_D. Separated norm powers do not change these supports.

We use the following specialization of the common joint Fourier calculus in Lemma 4.5. Every normalized norm occurring in a coupled smooth factor to be separated from the columns is a coordinate y1,…,ydy_1,\ldots,y_d of one ambient profile. A derived outer mask or label cutoff retained in the weight remains outside and needs no profile coordinate. Keep the current individual dyad cutoffs and fresh column cutoffs outside the inversion, until the weighted Cauchy inequality where they are used. Multiply the coupled profile by larger individual cutoffs Ωj\Omega_j equal to one on the full supports of those retained cutoffs. For the resulting compact profile H\mathfrak H, define before summing any current row or label

H^(t)=∫RdH(eu1,…,eud)e−it⋅u du,H(y)=(2π)−d∫RdH^(t)∏j=1dyjitj dt.\begin{aligned} \widehat{\mathfrak H}(\boldsymbol t) &=\int_{\mathbb R^d}\mathfrak H(e^{u_1},\ldots,e^{u_d}) e^{-i\boldsymbol t\cdot\boldsymbol u}\,d\boldsymbol u,\\ \mathfrak H(\boldsymbol y) &=(2\pi)^{-d}\int_{\mathbb R^d}\widehat{\mathfrak H}(\boldsymbol t) \prod_{j=1}^dy_j^{it_j}\,d\boldsymbol t. \end{aligned}

Arithmetic relations among the norms restrict evaluation points of this identity, not its density. Outer modes stay in the outer weight; for two column coordinates the first test receives y1it1y_1^{it_1} and the second receives y2−it2y_2^{-it_2}, whose conjugate supplies y2it2y_2^{it_2}. All normalized real inverse-root powers are included in the coupled profile, so the final column tests contain no second copy.

This convention also makes the uniformity quantitative. Write Dj=yj∂yjD_j=y_j\partial_{y_j}. On a fixed log rectangle, integration by parts with (1−Δ)m0(1-\Delta)^{m_0}, for 2m0>J+d2m_0>J+d, gives

∫Rd∣H^(t)∣(1+∣t∣)J dt≪J,d,boxmax⁡∣a∣≤2m0∥DaH∥∞.\int_{\mathbb R^d}|\widehat{\mathfrak H}(\boldsymbol t)| (1+|\boldsymbol t|)^J\,d\boldsymbol t \ll_{J,d,\mathrm{box}}\max_{|\boldsymbol a|\le2m_0} \|D^{\boldsymbol a}\mathfrak H\|_\infty.

For a fixed radial Schwartz Fourier kernel KK, every sup⁡x≥0∣(x∂x)jK(x)∣\sup_{x\geq0}|(x\partial_x)^jK(x)| is finite, and

DaK ⁣(A∏jyjej)=(∏jejaj)(x∂x)∣a∣K(x)∣x=A∏jyjej.D^{\boldsymbol a}K\!\left(A\prod_jy_j^{e_j}\right) =\left(\prod_je_j^{a_j}\right) (x\partial_x)^{|\boldsymbol a|}K(x) \big|_{x=A\prod_jy_j^{e_j}}.

Thus the separating seminorms are uniform for every scalar A>0A > 0, with no derivative-order power of ZZ. Normalized real powers have bounded Euler derivatives on the fixed boxes, and inherited norm twists have only a fixed polynomial height cost. No sharp cutoff in a column-dependent kernel ratio is put inside such a profile. For the radial Fourier kernels in the Poisson steps, these are the normalized-kernel bounds of Lemma 4.7 and (17.7).

The raw tail estimate we shall use is, for Y≥1Y \ge1 and A>1A > 1,

∑h≠0: aqh>Y∣K(aqh)∣≪A(1+a−1)Y1−A(a>0).\sum_{h\ne0:\,a q_h>Y}|K(aq_h)| \ll_A(1+a^{-1})Y^{1-A}\qquad(a>0).

Indeed, the shell 2jY<aqh≤2j+1Y2^jY < aq_h \le2^{j+1}Y contains O(1+2jY/a)O(1+2^jY/a) lattice points and the kernel is OA((2jY)−A)O_A((2^jY)^{-A}) there. Summing the two geometric series proves the display; the same argument applies to the fixed lattice λ−4O\lambda^{-4}\mathcal{O}. The proof uses only the large-argument bound ∣K(x)∣≪Ax−A\lvert K(x)\rvert\ll_A x^{-A} for x≥1x \ge1, so it also applies to the reflected kernel on such a tail. Below an actual-ratio inequality is used only to show that the complement of a sector-fixed outer row ball is contained in this tail for each supported raw column pair. That complement is removed before off-coprime extension and before Fourier absolutization. The full smooth kernel is retained inside the ball, whose nonsmooth mask is kept outside Fourier inversion until the relevant weighted Cauchy inequality. The tail orders and the crude raw counts are fixed at the end.

The first Poisson transformation. Expand the square in (A). Put

B=rad⁡(b1b2),ni=AiCui(i=1,2),\mathfrak{B}=\operatorname{rad}(b_1b_2), \qquad n_i=\mathfrak{A}_i C u_i \quad(i=1,2),

where Ai=(ni,B)\mathfrak{A}_i=(n_i,\mathfrak{B}), and CC is the gcd of n1/A1n_1/\mathfrak{A}_1 and n2/A2n_2/\mathfrak{A}_2. Then Ai∣B\mathfrak{A}_i\mid\mathfrak{B}, while u1,u2u_1,u_2 are squarefree, coprime to one another, and prime to CBC\mathfrak{B}. Let Ai,BA_i,B be the fixed centers of Ai,C\mathfrak{A}_i,C, and write A^i=log⁡ZqAi\widehat A_i=\log_Zq_{\mathfrak A_i}, B^=log⁡ZqC\widehat B=\log_Zq_C. For p∣Bp\mid\mathfrak{B}, define

aip=1p∣Ai,πp=vp(b1b2) mod 2,tp=a1p−a2p+3πp mod 6,a_{ip}=1_{p\mid\mathfrak{A}_i}, \qquad\pi_p=v_p(b_1b_2)\bmod2, \qquad t_p=a_{1p}-a_{2p}+3\pi_p\bmod6,

and put R1=∏tp≠0pR_1=\prod_{t_p\ne0}p. Its center is RR, and R^=log⁡ZqR1\widehat R=\log_Zq_{R_1}. The row character and its remaining zero mask are exactly

ψ1=χu1χ‾u2∏tp≠0χptp,m1=u1u2R1,Rmask=CB/R1.\psi_1=\chi_{u_1}\overline{\chi}_{u_2}\prod_{t_p\ne0}\chi_p^{t_p}, \qquad m_1=u_1u_2R_1, \qquad R_{\mathrm{mask}}=C\mathfrak{B}/R_1.

Indeed, the exponents at u1,u2u_1,u_2 are 1,−11,-1; the common off-B\mathfrak{B} factor CC has exponent zero but retains its mask; and the exponent at p∣Bp\mid\mathfrak{B} is tpt_p. Each nonzero local power is nonprincipal and primitive modulo pp, with disjoint supports. Thus ψ1\psi_1 is primitive unless m1=1m_1=1. Every original column mask and the two factors β(b1,f)β(b2,f)‾\beta(b_1,f)\overline{\beta(b_2,f)} remain in the expression.

Apply Lemma 17.5 with K=ZMK=Z^M, and denote its divisor by dk∣CB/R1d_k\mid C\mathfrak{B}/R_1, with center δ\delta and δ^=log⁡Zqdk\widehat\delta=\log_Zq_{d_k}. On this genuine coprime expression, the actual conductor length is

L^1=n^1+n^2−A^1−A^2−2B^+R^.\widehat{L}_1=\widehat{n}_1+\widehat{n}_2-\widehat{A}_1-\widehat{A}_2-2\widehat{B}+\widehat{R}.

The actual kernel argument is ZMqh/(qdkqm1)Z^M q_h/(q_{d_k}q_{m_1}), and the Poisson prefactor has exponent M−δ^−L^1/2M-\widehat{\delta}-\widehat{L}_1/2. We have not yet truncated or Fourier-separated this kernel.

If m1=1m_1=1, then u1=u2=1u_1=u_2=1 and tp=0t_p=0 for every p∣Bp\mid\mathfrak{B}. The latter condition forces πp=0\pi_p=0 and a1p=a2pa_{1p}=a_{2p}. Hence n1=n2n_1=n_2 and b1b2b_1b_2 is a square. Even counting all O(Z2ℓ+ϵ)O(Z^{2\ell+\epsilon}) pairs b1,b2b_1,b_2, all O(Zr+ϵ)O(Z^{r+\epsilon}) equal columns, all O(ZV+ϵ)O(Z^{V+\epsilon}) labels, and O(ZM)O(Z^M) rows, the normalization in (A) gives O(ZM+ϵ)O(Z^{M+\epsilon}). If r<0r<0 but its fixed annular column window is nonempty, then Z−rZ^{-r} is bounded by its fixed upper endpoint, so its ideal count is still O(Zr)O(Z^r) with a fixed constant. Marks and the retained masks do not increase this bound beyond a small power. When the nonzero principal terms are restored below, they will carry the same outer ball mask as the nonprincipal terms; the last part of Lemma 17.5 bounds them at this same cost.

We next identify its column coefficients. For coprime squarefree primary a,ba,b, CRT and reciprocity give

γ2(ab)=γ2(a)γ2(b)χa(b)2χb(a)2=γ2(a)γ2(b)χb(a)4.\gamma_2(ab)=\gamma_2(a)\gamma_2(b)\chi_a(b)^2\chi_b(a)^2=\gamma_2(a)\gamma_2(b)\chi_b(a)^4.

In the first Poisson root, the factors involving u1u_1, including the divisor and frequency, are

γ1(u1)χu1(h)‾χu1(dkR1)∏tp≠0χu1(ptp),\gamma_1(u_1)\overline{\chi_{u_1}(h)} \chi_{u_1}(d_kR_1)\prod_{t_p\ne0}\chi_{u_1}(p^{t_p}),

up to a fixed-ray factor. This follows by writing the CRT factors between u1u_1 and pp as χu1(p)χp(u1)tp\chi_{u_1}(p)\chi_p(u_1)^{t_p} and using reciprocity. On the conjugated second side tpt_p is replaced by −tp-t_p. The cross factor between u1,u2u_1,u_2 is the reciprocity factor R(u1,u2)\mathcal{R}(u_1,u_2), not a quotient of zero-extended symbols.

Put PT=∏tp≠0ptpP_T=\prod_{t_p\ne0}p^{t_p}, regarded in the fixed ray group. Equation (4.7) and Equation (4.5) show that the remaining two-column ray factor is

G(u1u2−1)R(u1u2−1,PT).G(u_1u_2^{-1})\mathcal{R}(u_1u_2^{-1},P_T).

For example, before placing factors inside the conjugated second polynomial, the raw second Gauss-signal factor is μ(u2)χu2(−1)G(u2)‾\mu(u_2)\chi_{u_2}(-1)\overline{G(u_2)}. Its corresponding factor written inside that polynomial is μ(u2)χu2(−1)G(u2)\mu(u_2)\chi_{u_2}(-1)G(u_2). Also G(u2−1)=χu2(−1)G(u2)‾G(u_2^{-1})=\chi_{u_2}(-1)\overline{G(u_2)}. These identities give the displayed quotient. Fix the ray class of PTP_T and Fourier-expand the displayed function on the finite ray group. Its factors on each side are genuine multiplicative ray characters, denoted by νi\nu_i. Their number and coefficient norm depend only on the fixed ray group.

Define

E=∏πp=1pa1p+a2p,h~=hf2E.E=\prod_{\pi_p=1}p^{a_{1p}+a_{2p}},\qquad\widetilde{h}=hf^2E.

The original fourth power at ff equals χui(f2)‾\overline{\chi_{u_i}(f^2)}, including zeros. Assign the slots first to bi,Ai,Cb_i,\mathfrak A_i,C. The remaining local factor at p∣Bp\mid\mathfrak B on side ii has exponent

4aip+1tp≠0(1±tp)+πp(a1p+a2p)(mod6).4a_{ip}+1_{t_p\ne0}(1\mathbin{\pm}t_p) +\pi_p(a_{1p}+a_{2p})\pmod6.

The plus sign belongs to side one. Direct reduction gives the same answer on both sides:

πp\pi_pa1pa_{1p}a2pa_{2p}tpt_pexponent on both sides
00000
01010
00150
01104
10034
11044
10124
11134

Define ξ(n)\xi(n) as the product over p∣Bp\mid\mathfrak B of χn(p)\chi_n(p) raised to the corresponding exponent in the last column. An exponent zero still denotes the puncture at pp. The calculation proves that ξ\xi is common to both sides and independent of hh, ff, CC. The nonprincipal coefficient on side ii, after these assignments, is

μ(ui)νi(ui)ρ(ui)χui(h~)‾χui(C)4χui(dk)ξ(ui)di(ui).(C)\tag{C} \mu(u_i)\nu_i(u_i)\rho(u_i) \overline{\chi_{u_i}(\widetilde h)} \chi_{u_i}(C)^4\chi_{u_i}(d_k)\xi(u_i)\mathfrak d_i(u_i).

It also shows that every character involving the moving bi,Aib_i,\mathfrak A_i is in either ξ\xi or h~\widetilde{h}; their other factors are outer coefficients.

The first transform has produced the inverse-type column coefficient in Equation (C). We next collect its fourth-power factors into one squarefree label before forming the positive row norm for the second transform.

Retaining the fourth-power label from the cubes. Write uniquely b1b2=q2sb_1b_2=q^2s with ss squarefree, and define

J2=∏πp=0a1p=a2p=1p,J=sJ2,q=J2q0.J_2=\prod_{\substack{\pi_{p}=0\\a_{1p}=a_{2p}=1}}p,\qquad J=sJ_2,\qquad q=J_2q_0.

Every prime of J2J_2 has positive even valuation in b1b2b_1b_2, so J2∣qJ_2\mid q. The ideals ss, J2J_2 are coprime and squarefree; hence JJ is squarefree. Let j≥0j\ge0 be the center of JJ, and put

s^=log⁡Zqs,j^2=log⁡ZqJ2,j^=log⁡ZqJ=s^+j^2,ℓ^pair=(b^1+b^2)/2.\widehat{s}=\log_Z q_s,\qquad\widehat{j}_2=\log_Z q_{J_2},\qquad\widehat{j}=\log_Z q_J=\widehat{s}+\widehat{j}_2,\qquad\widehat{\ell}_{\mathrm{pair}}=(\widehat{b}_1+\widehat{b}_2)/2.

The ideal identity b1b2=q02J22sb_1b_2=q_0^2J_2^2s gives exactly

c^:=log⁡Zqq0=ℓ^pair−s^/2−j^2≥0,4ℓ^pair−2s^+j^2=4c^+5j^2≥0.\widehat{c}:=\log_Z q_{q_0}=\widehat{\ell}_{\mathrm{pair}}-\widehat{s}/2-\widehat{j}_2\ge0,\qquad4\widehat{\ell}_{\mathrm{pair}}-2\widehat{s}+\widehat{j}_2=4\widehat{c}+5\widehat{j}_2\ge0.

The table above now proves the exact zero-extended identity

ξ(n)=χn(J)41(n,rad⁡q0)=1.\xi(n)=\chi_n(J)^4 1_{(n,\operatorname{rad}q_0)=1}.

Indeed, the primes with exponent four are exactly those of sJ2sJ_2; every other prime of B\mathfrak{B} divides q0q_0. A prime in both JJ and q0q_0 only repeats the zero already supplied by χn(J)4\chi_n(J)^4. We will fix q0q_0 but keep JJ in a later average. The modulus q0q_0 contributes a puncture and is not part of the fixed ray group. For fixed J,q0J,q_0, the choices of ss, J2J_2, the factorizations b1b2=q02J22sb_1b_2=q_0^2J_2^2s, and the ideals Ai\mathfrak{A}_i have only divisor multiplicity.

We now localize the genuine first Poisson expression, before extending its coprime support or taking absolute Fourier integrals. The local table gives the exact actual-norm identity

R^−A^1−A^2+E^=s^−2j^2.\widehat{R}-\widehat{A}_1-\widehat{A}_2+\widehat{E}=\widehat{s}-2\widehat{j}_2.

For y=hf2Ey=hf^2E, the implication ZMqh/(qdkqm1)≤ZτZ^M q_h/(q_{d_k}q_{m_1})\le Z^\tau and (17.23) give

y^≤n^1+n^2−2B^−M+s^−2j^2+δ^+2f^+τ≤n^1+n^2−2B^−M+4ℓ^pair−j^+δ^+2f^+τ.\begin{aligned} \widehat{y}\le\widehat{n}_1+\widehat{n}_2-2\widehat{B}-M+\widehat{s}-2\widehat{j}_2+\widehat{\delta}+2\widehat{f}+\tau\\ &\le\widehat{n}_1+\widehat{n}_2-2\widehat{B}-M+4\widehat{\ell}_{\mathrm{pair}}-\widehat{j}+\widehat{\delta}+2\widehat{f}+\tau. \end{aligned}

The second inequality is Equation (17.24). Define the formal center and the enclosing outer row scale by

Hc=2r−2B−M+4ℓ+2V+δ−j,Huse=Hc+12η+τ.H_c=2r-2B-M+4\ell+2V+\delta-j,\qquad H_{\mathrm{use}}=H_c+12\eta+\tau.

Relative to HcH_c, the last actual upper bound has error

(n^1−r)+(n^2−r)−2(B^−B)+2(b^1−ℓ)+2(b^2−ℓ)−(j^−j)+(δ^−δ)+2(f^−V),(\widehat{n}_1-r)+(\widehat{n}_2-r)-2(\widehat{B}-B)+2(\widehat{b}_1-\ell)+2(\widehat{b}_2-\ell)-(\widehat{j}-j)+(\widehat{\delta}-\delta)+2(\widehat{f}-V),

whose positive maximum under Equation (17.18) is 12η12\eta. Thus the actual-ratio inequality implies qy≤ZHuseq_y\le Z^{H_{\mathrm{use}}} for every supported raw column pair.

On that raw expression insert only the outer mask

B1(h)=10<qhf2E≤ZHuse.\mathcal B_1(h)=1_{0<q_{hf^2E}\le Z^{H_{\rm use}}}.

For each supported pair, its complement is contained in the actual kernel tail ZMqh/(qdkqm1)>ZτZ^Mq_h/(q_{d_k}q_{m_1})>Z^\tau; apply Equation (17.21) to discard that complement, with the raw counts and order fixed below. No indicator of the ratio inequality is inserted. Inside B1=1\mathcal{B}_1=1 retain the full smooth kernel, including pairs whose ratio is larger than ZτZ^\tau. The mask depends on hh, ff, EE and the fixed sector, but, after the indicated extraction, not on u1,u2u_1,u_2. If Huse<0H_{\mathrm{use}}<0, its nonzero ball is empty and the same tail comparison discards every nonzero frequency. Any principal nonzero terms now restored to unify the formula carry this identical mask. Their absolute contribution is bounded by the full principal restoration already estimated.

Remove the condition (u1,u2)=1(u_1,u_2)=1 by

1(u1,u2)=1=∑t′∣(u1,u2)μ(t′),ui=t′xi,t^=log⁡Zqt′.1_{(u_1,u_2)=1}=\sum_{t'\mid(u_1,u_2)}\mu(t'),\qquad u_i=t'x_i, \qquad \widehat t=\log_Zq_{t'}.

Let tt be its fixed nonnegative center. This inversion is made after the cross phases have been replaced by the fixed ray functions above. Those functions, the unchanged outer mask B1\mathcal{B}_1, all remaining zero-extended local factors, and the formal product qu1qu2qR1q_{u_1}q_{u_2}q_{R_1} in the smooth kernel define an expression also for noncoprime u1,u2u_1,u_2. It agrees with Poisson summation on the coprime support; the displayed divisor identity then recovers exactly that support. No primitive Poisson formula is asserted for the newly introduced noncoprime pairs. Squarefreeness retains the puncture (xi,t′)=1(x_i,t')=1. Assigned slots at t′t' are outer coefficients, while the other slots form the mark on xix_i.

Insert dyads of qhq_h from one fixed partition common to all f,Ef,E, not partitions recentered for those labels. The mask B1\mathcal{B}_1 implies qh≤qhf2E≤ZHuseq_h\le q_{hf^2E}\le Z^{H_{\rm use}}, so there are only logarithmically many such dyads in the bounded retained scale range. Keep B1\mathcal{B}_1 outside every Fourier inversion. Define

si=r−Ai−B−t,κi=M−2r−2ℓ−V−δ+Ai+B−R/2.s_i=r-A_i-B-t,\qquad\kappa_i=M-2r-2\ell-V-\delta+A_i+B-R/2.

The identity ni=AiCt′xin_i=\mathfrak A_iCt'x_i on the factorized expression gives ∣x^i−si∣≤4η|\widehat{x}_i-s_i|\leq4\eta. The full fresh xix_i-support is included in ID\mathcal I_D, so this same bound holds directly on that support after separation, not only on the original product support. The reconstructed formal products used in the current prefactor are also included there.

Separating the first transformed product. We record the actual prefactor before applying Cauchy. It splits exactly over the two column sides as

Z−r−2ℓ−VZM−δ^−L^1/2=Zκ^1/2Zκ^2/2,κ^i=M−r−2ℓ−V−δ^−n^i+A^i+B^−R^/2.Z^{-r-2\ell-V}Z^{M-\widehat{\delta}-\widehat{L}_1/2}=Z^{\widehat{\kappa}_1/2}Z^{\widehat{\kappa}_2/2},\qquad\widehat{\kappa}_i=M-r-2\ell-V-\widehat{\delta}-\widehat{n}_i+\widehat{A}_i+\widehat{B}-\widehat{R}/2.

Equation (17.18) gives on each side

κ^i≤κi+92η.\widehat{\kappa}_i\leq\kappa_i+\frac{9}{2}\eta.

The five error weights are 1,1,1,1,1/21,1,1,1,1/2. We now implement this normalization with all real inverse roots in one joint profile. Fix a first dyadic, ray, and slot pattern σ\sigma, and let h1h_1 be the center of its bare-hh dyad. Use the nine independent normalized coordinates

y=(yA1,yA2,yC,yd,yR,yt,yh,yx1,yx2)=(qA1ZA1,qA2ZA2,qCZB,qdkZδ,qR1ZR,qt′Zt,qhZh1,qx1Zs1,qx2Zs2).\boldsymbol y=(y_{A_1},y_{A_2},y_C,y_d,y_R,y_t,y_h,y_{x_1},y_{x_2}) =\left(\frac{q_{\mathfrak A_1}}{Z^{A_1}}, \frac{q_{\mathfrak A_2}}{Z^{A_2}},\frac{q_C}{Z^B}, \frac{q_{d_k}}{Z^\delta},\frac{q_{R_1}}{Z^R},\frac{q_{t'}}{Z^t}, \frac{q_h}{Z^{h_1}},\frac{q_{x_1}}{Z^{s_1}},\frac{q_{x_2}}{Z^{s_2}}\right).

The exact full root and kernel argument on the formal ua=t′xau_a=t'x_a expression are

Z−r−2ℓ−VZMqdkqR1qt′qx1qx2=Z(κ1+κ2)/2yd−1yR−1/2yt−1(yx1yx2)−1/2,\frac{Z^{-r-2\ell-V}Z^M} {q_{d_k}\sqrt{q_{R_1}}q_{t'}\sqrt{q_{x_1}q_{x_2}}} =Z^{(\kappa_1+\kappa_2)/2} y_d^{-1}y_R^{-1/2}y_t^{-1}(y_{x_1}y_{x_2})^{-1/2},
ZMqhqdkqR1qt′2qx1qx2=Aker,1yhydyRyt2yx1yx2,Aker,1=ZM+h1−δ−R−2t−s1−s2.\begin{aligned} \frac{Z^Mq_h}{q_{d_k}q_{R_1}q_{t'}^2q_{x_1}q_{x_2}} =A_{{\rm ker},1}\frac{y_h}{y_dy_Ry_t^2y_{x_1}y_{x_2}},\\ A_{{\rm ker},1}=Z^{M+h_1-\delta-R-2t-s_1-s_2}. \end{aligned}

Choose fresh cutoffs ωx,a\omega_{x,a} equal to one on the old WW-support divided by the individual Aa,C,t′\mathfrak A_a,C,t' supports, and retain them in the columns. Retain every current outer dyad cutoff outside inversion. Let Ω1,α\Omega_{1,\alpha} be larger cutoffs equal to one on the full supports of these retained cutoffs. With K1=FΦ\mathcal{K}_1=\mathcal{F}\Phi, define the single compact profile

H1,σ(y)=Z−9η/2∏αΩ1,α(yα)yd−1yR−1/2yt−1(yx1yx2)−1/2\mathfrak H_{1,\sigma}(\boldsymbol y)={}Z^{-9\eta/2} \prod_\alpha\Omega_{1,\alpha}(y_\alpha) y_d^{-1}y_R^{-1/2}y_t^{-1}(y_{x_1}y_{x_2})^{-1/2}
×W(yA1yCytyx1)W(yA2yCytyx2)‾K1 ⁣(Aker,1yhydyRyt2yx1yx2).\times W(y_{A_1}y_Cy_ty_{x_1}) \overline{W(y_{A_2}y_Cy_ty_{x_2})} \mathcal K_1\!\left(A_{{\rm ker},1} \frac{y_h}{y_dy_Ry_t^2y_{x_1}y_{x_2}}\right).

The scalar outside this profile is exactly ∏a=12Z(κa+9η/2)/2\prod_{a=1}^{2} Z^{(\kappa_a+9\eta/2)/2}. In particular, the profile contains each real root once, also when the actual column norms differ. Its transform is defined by Equation (17.19) on the ambient nine-dimensional box before any actual f,hf,h or outer ideal is summed. The norms of bab_a, ff, JJ, EE, q0q_0 occur only in outer coefficients, characters, masks or individual cutoffs after Equation (C); they require no additional coupled-profile coordinate.

To expose the arithmetic extraction at t′t', put y=hf2Ey=hf^2E and

B1,a(t′;y)=μ(t′)νa(t′)ρ(t′)χt′(y)‾χt′(CJ)4χt′(dk)1(t′,rad⁡q0)=1.B_{1,a}(t';y)=\mu(t')\nu_a(t')\rho(t')\overline{\chi_{t'}(y)}\chi_{t'}(CJ)^4\chi_{t'}(d_k)1_{(t',\operatorname{rad}q_0)=1}.

Let ε1=1\varepsilon_1=1 and ε2=−1\varepsilon_2=-1. For a fixed first Fourier mode t\boldsymbol t, the remaining polynomials are exactly

Pa(y)=∑x sfμ(x)νa(x)ρ(x)χx(y)‾χx(CJ)4χx(dk)1(x,rad⁡q0t′)=1×dIa(x)ωx,a(qx/Zsa)(qx/Zsa)εaitxa.\begin{aligned} P_a(y)={}&\sum_{x\ {\rm sf}}\mu(x)\nu_a(x)\rho(x) \overline{\chi_x(y)}\chi_x(CJ)^4\chi_x(d_k) 1_{(x,\operatorname{rad}q_0t')=1}\\ &\qquad\times\mathfrak d_{I_a}(x)\omega_{x,a}(q_x/Z^{s_a}) (q_x/Z^{s_a})^{\varepsilon_a it_{x_a}}. \end{aligned}

Multiplicativity is used on squarefree coprime factors, then through the displayed zero extensions; no character is divided at a zero. The one additional μ(t′)\mu(t') from the mutual-gcd inversion is outer. Apply Equation (17.16) with the ordered list (ba,Aa,C,t′;x)(b_a,\mathfrak{A}_a,C,t';x). A surviving prime dividing xx is already prime to ba,Aa,C,t′b_a,\mathfrak{A}_a,C,t': every prime of B\mathfrak{B} is in Jrad⁡q0J\operatorname{rad}q_0, and the displayed fourth powers and punctures supply these zeros. Thus dIa\mathfrak d_{I_a} has the original individual coefficients and lists, while assigned prime identities and priority masks stay outer.

Here is the full structure of the first separated component. Let Ωσ\Omega_\sigma consist of b1,b2,A1,A2,C,dk,t′,f,hb_1,b_2,\mathfrak{A}_1,\mathfrak{A}_2,C,d_k,t',f,h and the assigned slot primes, subject to their reconstruction relations and individual supports. In particular Aa∣B\mathfrak{A}_a\mid\mathfrak{B}, (C,B)=1(C,\mathfrak{B})=1, and dk∣CB/R1d_k\mid C\mathfrak{B}/R_1, while R1,E,J,q0R_1,E,J,q_0 are derived, not free indices. Let A1,σ\mathcal A_{1,\sigma} be the product of the assigned original coefficients and priority masks, with conjugation on side two, and let ψ1,σout\psi_{1,\sigma}^{\rm out} be the product of all retained outer dyad cutoffs. Let eσe_\sigma be the product obtained in the preceding quotient-free CRT extraction of the old multiplicity w(f)w(f), the two original β\beta factors, their cube masks including (ba,f)=1(b_a,f)=1, the extracted zero masks, and the finite Gauss, unit, reciprocity, and first-ray factors at the old outer ideals, excluding the displayed μ(dk)\mu(d_k) and B1,aB_{1,a}. It is independent of x1,x2x_1,x_2; its definition is by that product, not by division by Equation (17.30). Writing O1={A1,A2,C,d,R,t,h}\mathcal{O}_1=\{A_1,A_2,C,d,R,t,h\}, set

w1,σ(ω;t)=eσ(ω)μ(dk)μ(t′)B1,1(t′;y)B1,2(t′;y)‾B1(h)A1,σ(ω)ψ1,σout(ω)∏α∈O1yαitα.w_{1,\sigma}(\omega;\boldsymbol t) =e_\sigma(\omega)\mu(d_k)\mu(t')B_{1,1}(t';y) \overline{B_{1,2}(t';y)}\mathcal B_1(h) \mathcal A_{1,\sigma}(\omega)\psi_{1,\sigma}^{\rm out}(\omega) \prod_{\alpha\in\mathcal O_1}y_\alpha^{it_\alpha}.

For the masked, principal-restored formal first component, Fourier inversion gives the exact identity

T1,σ=(2π)−9∫R9H^1,σ(t)∑ω∈Ωσw1,σ(ω;t)×Z(κ1+9η/2)/2P1(y)Z(κ2+9η/2)/2P2(y)‾ dt.\begin{aligned} \mathcal T_{1,\sigma}=(2\pi)^{-9}\int_{\mathbb R^9} &\widehat{\mathfrak H}_{1,\sigma}(\boldsymbol t) \sum_{\omega\in\Omega_\sigma}w_{1,\sigma}(\omega;\boldsymbol t)\\ &\times Z^{(\kappa_1+9\eta/2)/2}P_1(y) \overline{Z^{(\kappa_2+9\eta/2)/2}P_2(y)}\,d\boldsymbol t. \end{aligned}

Expanding the two polynomials restores the two column modes; the seven outer modes restore the other coordinates of Equation (17.29). Its larger cutoffs are one on the retained supports, and the fresh cutoffs are one wherever the old windows are nonzero. This verifies the identity term by term. The original β\beta factors and every outer mask are still in the complete sum.

The first positive majorant. For any finite or absolutely convergent weighted sum we use

∣∑ωwωU1(ω)U2(ω)‾∣≤∏i=12(∑ω∣wω∣∣Ui(ω)∣2)1/2.(D)\tag{D} \left|\sum_\omega w_\omega U_1(\omega)\overline{U_2(\omega)}\right| \le\prod_{i=1}^2 \left(\sum_\omega|w_\omega||U_i(\omega)|^2\right)^{1/2}.

Apply this first with Ui=Z(κi+9η/2)/2PiU_i=Z^{(\kappa_i+9\eta/2)/2}P_i on the whole Ωσ\Omega_\sigma, for each fixed mode. Only now bound the outer factors absolutely. Their pure arithmetic magnitudes are at most a separately allocated ZπβZ^{\pi_\beta} times the old multiplicity and the absolute assigned-slot product; the retained support gives B1(h)1(C,J)=1\mathcal B_1(h)1_{(C,J)=1}. In particular no factorization of β(b,f)\beta(b,f) has been assumed.

For each fixed old outer reconstruction and nonzero y=h~y=\widetilde{h}, the relation y=hf2Ey=hf^2E implies f2E∣(y)f^2E\mid(y). If its multiplicity is at most C0dO(f)C0C_0d_{\mathcal O}(f)^{C_0}, then

∑f2E∣(y)w(f)≤C0dO((y))C0+1≤CπoldZπold(0<qy≤ZHuse).\sum_{f^2E\mid(y)}w(f) \le C_0d_{\mathcal O}((y))^{C_0+1} \le C_{\pi_{\rm old}}Z^{\pi_{\rm old}} \qquad(0<q_y\le Z^{H_{\rm use}}).

The last bound is uniform because HuseH_{\mathrm{use}} stays in a bounded range; h=y/(f2E)h=y/(f^2E) is then uniquely determined as an element. This is an old-label fibre bound, not a multiplicity depending on a later new label. The polynomial Pi(y)P_i(y) has no remaining dependence on ff or on the individual bi,Aib_i,\mathfrak A_i beyond JJ, q0q_0, the fixed dyadic length AiA_i, and the fixed ray sector: this is precisely Equations (C) and (17.25), with the norm profiles separated. After the first weighted Cauchy inequality, B1\mathcal{B}_1 is simply 10<qy≤ZHuse1_{0<q_y\le Z^{H_{\rm use}}}. At this positive-sum stage, and only now, majorize it by a fixed nonnegative radial Schwartz function Φ+(qy/ZHuse)\Phi_+(q_y/Z^{H_{\mathrm{use}}}) which is at least one for arguments at most one. A nonempty ball has Huse≥0H_{\mathrm{use}}\ge0, so the second Poisson scale is exactly ZHuse≥1Z^{H_{\mathrm{use}}}\ge1. The majorant is not substituted as an equality in the original signed expression. More precisely, let Oσ\mathfrak O_\sigma consist of

o=(b1,b2,A1,A2,C,dk,t′;old assigned slot primes),o=(b_1,b_2,\mathfrak A_1,\mathfrak A_2,C,d_k,t'; \text{old assigned slot primes}),

retaining their full individual supports, the source reconstruction relations independent of f,h,xf,h,x, the assigned priority masks, and (C,J)=1(C,J)=1. Let wo+w_o^+ be the product of the absolute original coefficients of its assigned primes, and zero off this set. It is nonnegative and independent of yy. Each first positive side is at most CZπβ+πoldC Z^{\pi_\beta+\pi_{\rm old}}, times its scalar Zκi+9η/2Z^{\kappa_i+9\eta/2}, times the explicit positive majorant

Si,σ,t=∑o∈Oσwo+∑y∈OΦ+(qy/ZHuse)∣Pi(y)∣2.\mathcal S_{i,\sigma,\boldsymbol t} =\sum_{o\in\mathfrak O_\sigma}w_o^+ \sum_{y\in\mathcal O}\Phi_+(q_y/Z^{H_{\rm use}})|P_i(y)|^2.

At this positive step the old hh cutoff and mode, and the zeros of B1,aB_{1,a} depending on yy, may be removed by their upper bounds. The first weighted Cauchy inequality and the old-label fibre bound have therefore removed the old f,hf,h from this positive majorant and every later outer set; their original −V-V normalization remains in κi\kappa_i. After the following count, we apply the second Poisson transformation to its yy-sum.

Let r^diff≥0\widehat{r}_{\mathrm{diff}}\ge0 be the actual log-norm of the even-parity primes with a1p≠a2pa_{1p}\ne a_{2p}. The table gives R^=s^+r^diff\widehat{R}=\widehat{s}+\widehat{r}_{\mathrm{diff}}, so

c^=ℓ^pair+R^/2−j^−r^diff/2≤ℓ+R/2−j+52η.\widehat{c}=\widehat{\ell}_{\mathrm{pair}}+\widehat{R}/2-\widehat{j}-\widehat{r}_{\mathrm{diff}}/2\le\ell+R/2-j+\frac{5}{2}\eta.

Ideal counting with this actual upper bound counts the fixed q0q_0 while retaining JJ. For a diagonal bound which also counts JJ, its full window has exponent at most j+ηj+\eta, giving the combined upper count Zℓ+R/2+7η/2+ϵZ^{\ell+R/2+7\eta/2+\epsilon}. The choices of the Ai\mathfrak A_i and of dk∣CB/R1d_k\mid C\mathfrak B/R_1 add only divisor factors once b1,b2,Cb_1,b_2,C are specified.

Combining (17.31), weighted Cauchy, and the old-label fibre bound gives the explicit output of the first transformation:

∣T1,σ∣≪Zπβ+πold∫R9∣H^1,σ(t)∣×∏i=12(Zκi+9η/2Si,σ,t)1/2 dt.\begin{aligned} |\mathcal T_{1,\sigma}|\ll{}&Z^{\pi_\beta+\pi_{\rm old}} \int_{\mathbb R^9}|\widehat{\mathfrak H}_{1,\sigma}(\boldsymbol t)|\\ &\quad\times\prod_{i=1}^2 \left(Z^{\kappa_i+9\eta/2}\mathcal S_{i,\sigma,\boldsymbol t}\right)^{1/2} \,d\boldsymbol t. \end{aligned}

Each Si,σ,t\mathcal S_{i,\sigma,\boldsymbol t} is the positive sum in (17.33): its row polynomial has the Möbius coefficient in (17.30), the cube-derived label JJ is retained, and the old f,hf,h no longer occur among the averaged indices. The following transformation is applied to these positive row norms.

The second Poisson transformation. Fix one of the two positive sums obtained from the first Cauchy inequality. Its polynomial has the form

Pi(y)=∑xci(x)χx(y)‾.P_i(y)=\sum_x c_i(x)\overline{\chi_x(y)}.

The coefficient ci(x)c_i(x) consists of the other factors of Equation (C), with ui=t′xu_i=t'x, the puncture at t′t', and the separated weight. It is independent of yy. In particular xx is squarefree and

ci(x)=0unless(x,CJ)=1,(x,rad⁡q0t′)=1.c_i(x)=0\quad\text{unless}\quad (x,CJ)=1,\quad (x,\operatorname{rad}q_0t')=1.

The puncture ρ\rho and the zero of χx(dk)\chi_x(d_k) are retained as well. The yy-sum uses the fixed-shape smooth positive ball at scale ZHuseZ^{H_{\mathrm{use}}}.

In its expanded square put

g′=(x1,x2),xj=g′zj,g^=log⁡Zqg′.g'=(x_1,x_2),\qquad x_j=g'z_j,\qquad \widehat g=\log_Zq_{g'}.

Let g≥0g\geq0 be its fixed center. Then z1,z2z_1,z_2 are squarefree and coprime, and each is prime to g′g'. The row data for Lemma 17.5 are

K=ZHuse,ψ2=χ‾z1χz2,m2=z1z2,Rmask=g′.K=Z^{H_{\mathrm{use}}},\qquad\psi_2=\overline{\chi}_{z_1}\chi_{z_2},\qquad m_2=z_1z_2,\qquad R_{\mathrm{mask}}=g'.

The common factor χ‾g′(y)χg′(y)\overline{\chi}_{g'}(y)\chi_{g'}(y) is exactly this mask. The character is primitive away from m2=1m_2=1, because its two nonzero local powers have disjoint supports. For d2∣g′d_2\mid g', let θ≥0\theta\geq0 be its center and write θ^=log⁡Zqd2\widehat\theta=\log_Zq_{d_2}. The actual conductor length is

L^2=x^1+x^2−2g^,∣L^2−2(si−g)∣≤10η.\widehat{L}_2=\widehat{x}_1+\widehat{x}_2-2\widehat{g},\qquad\left|\widehat{L}_2-2(s_i-g)\right|\leq10\eta.

The last inequality uses the full fresh xx-support bound ∣x^a−si∣≤4η|\widehat{x}_a-s_i|\leq4\eta for each copy and ∣g^−g∣≤η|\widehat{g}-g|\leq\eta. For knew=dkd2k′′k_{\mathrm{new}}=d_kd_2k'', the implication ZHuseqk′′/(qd2qm2)≤ZτZ^{H_{\mathrm{use}}}q_{k''}/(q_{d_2}q_{m_2})\leq Z^\tau gives

knew^≤2(si−g)−Huse+δ+2θ+13η+τ=Mc+η,\begin{aligned} \widehat{k_{\rm new}} &\le2(s_i-g)-H_{\rm use}+\delta+2\theta+13\eta+\tau\\ &=M_c+\eta, \end{aligned}

where

Mc=2(si−g)−Hc+δ+2θ=M−4ℓ−2Ai−2t−2g+2θ−2V+j,Mch=Mc+η.M_c=2(s_i-g)-H_c+\delta+2\theta = M-4\ell-2A_i-2t-2g+2\theta-2V+j,\qquad M_{\mathrm{ch}}=M_c+\eta.

The 13η13\eta consists of 10η10\eta from the conductor, one from dkd_k, and two from d2d_2. Subtracting Huse=Hc+12η+τH_{\mathrm{use}}=H_c+12\eta+\tau cancels the same tolerance τ\tau used in this second Poisson comparison. Thus no separate row clipping or unrecorded boundary error is needed.

Separate the original principal contribution for the direct count below. Before any off-coprime extension or Fourier absolutization, keep on the genuine nonprincipal second Poisson expression only the outer mask

B2(k′′)=10<qdkd2k′′≤ZMch.\mathcal B_2(k'')=1_{0<q_{d_kd_2k''}\le Z^{M_{\rm ch}}}.

For each supported pair its complement is contained in the actual ratio tail just considered, so Equation (17.21) discards it with the order fixed below. Inside the mask retain the full smooth kernel. The mask depends on dk,d2,k′′d_k,d_2,k'' and the fixed sector, not on the residual z1,z2z_1,z_2. If Mch<0M_{\mathrm{ch}}<0, the nonzero ball is empty and the same tail comparison discards every nonzero frequency. In a retained nonempty passage Mch≥0M_{\mathrm{ch}}\geq0.

The actual second prefactor has the exact side split

ZHuse−θ^−L^2/2=Zλ^1/2Zλ^2/2,λ^a=Huse−θ^−x^a+g^.Z^{H_{\mathrm{use}}-\widehat{\theta}-\widehat{L}_2/2} =Z^{\widehat{\lambda}_1/2}Z^{\widehat{\lambda}_2/2},\qquad \widehat{\lambda}_a=H_{\mathrm{use}}-\widehat{\theta}-\widehat{x}_a+\widehat{g}.

For λc=Hc−θ−(si−g)\lambda_c = H_c - \theta- (s_i - g), the same support bounds give

λ^a≤λc+18η+τ.\widehat{\lambda}_a \le\lambda_c + 18\eta+ \tau.

Here 18=12+1+4+118 = 12 + 1 + 4 + 1. As in the first split, all normalized real inverse roots will remain in the joint smooth profile until Fourier inversion; they are not also appended to the final child tests. All original coefficient masks remain. In particular

(g′,CJ)=1,(zj,g′CJ)=1(g',CJ) = 1,\qquad(z_j,g'CJ) = 1

on their nonzero support.

The principal case is z1=z2=1z_1 = z_2 = 1, equivalently x1=x2x_1 = x_2. The nominal identity for its count is

κi+Hc+si+B+t+ℓ+R/2=F−B−j,F=N+V=r+3ℓ+V.\kappa_i + H_c + s_i + B + t + \ell+ R/2 = F - B - j,\qquad F = N + V = r + 3\ell+ V.

The actual upper count adds 9η/29\eta/2 from the first prefactor, 12η+τ12\eta+ \tau from the row scale HuseH_{\mathrm{use}}, 4η4\eta from the diagonal xx-window, η\eta each from CC, t′t', and 7η/27\eta/2 from the combined q0q_0, JJ count. Their sum is 26η+τ26\eta+ \tau. With the aggregate local loss π\pi, this principal contribution is therefore at most ZF−B−j+26η+τ+π≤ZF+26η+τ+πZ^{F-B-j+26\eta+\tau+\pi} \le Z^{F+26\eta+\tau+\pi}. Any nonzero principal frequencies restored to the formal expression carry the same B2\mathcal B_2 mask; their absolute sum is bounded by the full principal restoration in Lemma 17.5, since ZHuse≥1Z^{H_{\mathrm{use}}} \ge1.

For the nonprincipal terms, we now identify the new coefficient class. For squarefree zz, complex conjugation of a primitive Gauss sum and Equation (4.7) give

γ−1(z)=χz(−1)γ1(z)‾,μ(z)γ−1(z)=αˉ(z)γ2(z)χz(−1)G(z)‾.\gamma_{-1}(z)=\chi_z(-1)\overline{\gamma_1(z)},\qquad \mu(z)\gamma_{-1}(z) =\bar\alpha(z)\gamma_2(z)\chi_z(-1)\overline{G(z)}.

The raw second factor is μ(z)γ1(z)=αˉ(z)γ2(z)‾G(z)\mu(z)\gamma_1(z)=\overline{\bar\alpha(z)\gamma_2(z)}G(z); the corresponding factor written inside the conjugated second polynomial has ray factor G(z)‾\overline{G(z)}. The CRT cross factor of the two primitive roots is R(z1,z2)\mathcal{R}(z_1,z_2). Thus their combined ray factor is

G(a,b)=χa(−1)G(a)‾G(b)R(a,b)=G(ba−1).\mathfrak{G}(a,b) = \chi_a(-1)\overline{G(a)}G(b)\mathcal{R}(a,b) = G(ba^{-1}).

The last equality follows from Equation (4.5) and R(a,a)=χa(−1)\mathcal{R}(a,a) = \chi_a(-1), first on primes by Equation (4.6) and then multiplicatively. All quotients in this display are in the fixed finite ray group. In particular,

G(v′n1,v′n2)=G(n1,n2).\mathfrak{G}(v'n_1,v'n_2) = \mathfrak{G}(n_1,n_2).

The common multiplicative character νi(v′)\nu_i(v') also cancels between the two sides.

Insert dyads of qk′′q_{k''} from one partition common to all dk,d2d_k,d_2. The mask B2\mathcal B_2 implies qk′′≤ZMchq_{k''}\le Z^{M_{\rm ch}}, so their number is logarithmic in the bounded retained range. Let h2h_2 be the center of one such bare-frequency dyad. We now record the exact component to be separated. Fix the first mode and selected side ii, write

Ho=CJ,r0=rad⁡q0t′,d0=dk,a0(z)=αˉ(z)γ2(z),K2=FΦ+,H_o=CJ,\qquad r_0=\operatorname{rad}q_0t',\qquad d_0=d_k, \qquad a_0(z)=\bar\alpha(z)\gamma_2(z),\qquad \mathcal K_2=\mathcal F\Phi_+,

and retain K=ZHuseK = Z^{H_{\mathrm{use}}} from Equation (17.36). For squarefree arguments put

Bo(g′)=μ(g′)νi(g′)ρ(g′)1(g′,r0)=1χg′(Ho)4χg′(d0),B_o(g') = \mu(g')\nu_i(g')\rho(g')1_{(g',r_0)=1}\chi_{g'}(H_o)^4\chi_{g'}(d_0),
Lo,d2,k′′(z)=a0(z)νi(z)ρ(z)1(z,r0)=1χz(Ho)4χz(d0)χz(d2)‾χz(k′′).L_{o,d_2,k''}(z)=a_0(z)\nu_i(z)\rho(z)1_{(z,r_0)=1} \chi_z(H_o)^4\chi_z(d_0)\overline{\chi_z(d_2)}\chi_z(k'').

The old separated test in PiP_i is denoted by WiW_i, so Wi(x)=ωx,i(x)xεiitxiW_i(x)=\omega_{x,i}(x)x^{\varepsilon_iit_{x_i}}. Let ψg,ψd2,ψk′′\psi_g,\psi_{d_2},\psi_{k''} denote the retained individual cutoffs on the fixed g′,d2,k′′g',d_2,k'' dyads, evaluated at their normalized norms. For this preliminary pattern σ0\sigma_0, the masked principal-restored nonzero component of Equation (17.33) is exactly

T2,σ0,i=∑o∈Oσ, g′ sfd2∣g′, k′′≠0wo+ψgψd2ψk′′μ(d2)B2(k′′)∣Bo(g′)∣2×∑z1,z2 sf(z1z2,g′)=11(z1,z2)=1Lo,d2,k′′(z1)Lo,d2,k′′(z2)‾G([z2][z1]−1)×dIi(g′z1)dIi(g′z2)‾Wi(qg′qz1/Zsi)Wi(qg′qz2/Zsi)‾×Kqd2qz1qz2K2 ⁣(Kqk′′qd2qz1qz2).\begin{aligned} \mathcal T_{2,\sigma_0,i}={}& \sum_{\substack{o\in\mathfrak O_\sigma,\ g'\ {\rm sf}\\d_2\mid g',\ k''\ne0}} w_o^+\psi_g\psi_{d_2}\psi_{k''}\mu(d_2)\mathcal B_2(k'')|B_o(g')|^2\\ &\times\sum_{\substack{z_1,z_2\ {\rm sf}\\(z_1z_2,g')=1}} 1_{(z_1,z_2)=1}L_{o,d_2,k''}(z_1)\overline{L_{o,d_2,k''}(z_2)} G([z_2][z_1]^{-1})\\ &\times\mathfrak d_{I_i}(g'z_1)\overline{\mathfrak d_{I_i}(g'z_2)} W_i(q_{g'}q_{z_1}/Z^{s_i}) \overline{W_i(q_{g'}q_{z_2}/Z^{s_i})}\\ &\times\frac{K}{q_{d_2}\sqrt{q_{z_1}q_{z_2}}} \mathcal K_2\!\left(\frac{Kq_{k''}}{q_{d_2}q_{z_1}q_{z_2}}\right). \end{aligned}

Here brackets denote classes in the fixed finite ray group. Indeed the arithmetic part of ci(g′z)c_i(g'z) factors into Bo(g′)B_o(g') and its residual μ(z)\mu(z) coefficient on (g′,z)=1(g',z)=1. The common row factor is the mask at g′g', whose Poisson expansion gives the one divisor d2d_2, while the signal calculation above gives the displayed two LL factors and ray quotient. The restored principal pair z1=z2=1z_1=z_2=1 agrees by G(1)=1G(1)=1. Its separate cost, and the raw complement removed before this formula, have already been bounded. Thus this is an equality for the specified component of the positive majorant, not for the original signed block.

Define the summand of Equation (17.41) on all individually admissible squarefree z1,z2z_1,z_2 by its displayed quotient-free LL factors, fixed-ray quotient, formal product norms, full kernel, and unchanged B2\mathcal{B}_2. It agrees with the genuine formula on coprime pairs. Insert the complete identity

1(z1,z2)=1=∑v′∣(z1,z2)μ(v′),za=v′na,1_{(z_1,z_2)=1}=\sum_{v'\mid(z_1,z_2)}\mu(v'),\qquad z_a=v'n_a,

before any factorwise estimate. Let v≥0v\ge0 be the center of the squarefree v′v'-dyad and v^=log⁡Zqv′\widehat v=\log_Z q_{v'}. The nan_a are squarefree, with (v′,na)=1(v',n_a)=1; they need not be mutually coprime. No primitive Poisson formula is used on this extension. For squarefree v′v' put

Do(v′;d2,k′′)=a0(v′)νi(v′)ρ(v′)1(v′,r0)=1χv′(Ho)4χv′(d0)χv′(d2)‾χv′(k′′).D_o(v';d_2,k'')=a_0(v')\nu_i(v')\rho(v')1_{(v',r_0)=1} \chi_{v'}(H_o)^4\chi_{v'}(d_0)\overline{\chi_{v'}(d_2)}\chi_{v'}(k'').

On squarefree coprime v′,nv',n, the exact extraction is

Lo,d2,k′′(v′n)=Do(v′;d2,k′′)a0(n)νi(n)ρ(n)1(n,r0)=1×χn(Ho)4χn(d0)χn(d2)‾χn(k′′)χn(v′)4.\begin{aligned} L_{o,d_2,k''}(v'n)={}&D_o(v';d_2,k'')a_0(n)\nu_i(n)\rho(n)1_{(n,r_0)=1}\\ &\times\chi_n(H_o)^4\chi_n(d_0)\overline{\chi_n(d_2)} \chi_n(k'')\chi_n(v')^4. \end{aligned}

This uses a0(v′n)=a0(v′)a0(n)χn(v′)4a_0(v'n)=a_0(v')a_0(n)\chi_n(v')^4. On an overlap the right side defines the extension to be zero by χn(v′)4\chi_n(v')^4, without evaluating a nonsquarefree Gauss sum. The two common factors give ∣Do(v′;d2,k′′)∣2\lvert D_o(v';d_2,k'')\rvert^2, including the zero (v′,k′′)=1(v',k'')=1 and its fixed-puncture, d0d_0, and label zeros. They remain in the outer weight through Cauchy. The old gcd also leaves 1(v′,g′)=11_{(v',g')=1}. Since DoD_o vanishes on (v′,CJ)>1(v',CJ)>1, we retain equivalently the explicit outer factor 1(v′,g′CJ)=11_{(v',g'CJ)=1}, which repeats that label zero.

Set rg=g′/d2r_g=g'/d_2, knew=dkd2k′′k_{\mathrm{new}}=d_kd_2k'' and fnew=JCd2v′f_{\mathrm{new}}=JCd_2v'. All moving factors on nn satisfy the complete zero-extended identity

χn(dk)χn(k′′)χn(d2)‾χn(CJ)4χn(v′)4=χn(knew)χn(fnew)4.\chi_n(d_k)\chi_n(k'')\overline{\chi_n(d_2)}\chi_n(CJ)^4\chi_n(v')^4=\chi_n(k_{\mathrm{new}})\chi_n(f_{\mathrm{new}})^4.

It uses χn(d2)‾=χn(d2)χn(d2)4\overline{\chi_n(d_2)}=\chi_n(d_2)\chi_n(d_2)^4, also on nonunits. The residual gcd with g′=d2rgg'=d_2r_g splits into the repeated zero at d2d_2 and the fixed puncture at rgr_g. The old punctures at q0,t′q_0,t' remain. If Cray\mathcal C_{\rm ray} denotes the fixed group through which GG factors, put

G^(ϑ)=∣Cray∣−1∑c∈CrayG(c)ϑ(c)‾.\widehat G(\vartheta)=|\mathcal C_{\rm ray}|^{-1} \sum_{c\in\mathcal C_{\rm ray}}G(c)\overline{\vartheta(c)}.

Then

G([n2][n1]−1)=∑ϑ∈C^rayG^(ϑ)ϑ(n1)‾ϑ(n2).G([n_2][n_1]^{-1})=\sum_{\vartheta\in\widehat{\mathcal C}_{\rm ray}} \widehat G(\vartheta)\overline{\vartheta(n_1)}\vartheta(n_2).

Thus both new polynomials in a fixed ray summand use the same νiϑ‾\nu_i\overline{\vartheta}, and its one bounded coefficient G^(ϑ)\widehat{G}(\vartheta) remains outer.

The new canonical data and their admissibility. The second transformation has returned the moving characters to canonical form. We now identify which data will be fixed and which will remain averaged. This distinction also determines the puncture of the child. Put νa′=νiϑ‾\nu_a'=\nu_i\overline\vartheta for both sides and define

γ=(q0,t′,rg),rg=g′/d2,\gamma=(q_0,t',r_g),\qquad r_g=g'/d_2,
knew=dkd2k′′,fnew=JCd2v′,k_{\mathrm{new}}=d_kd_2k'',\qquad f_{\mathrm{new}}=JCd_2v',
ρ′(n)=ργ(n)=ρ(n)1(n,rad⁡q0t′rg)=1.\rho'(n)=\rho_\gamma(n)=\rho(n)1_{(n,\operatorname{rad}q_0t'r_g)=1}.

On the nonzero coefficient support, J,C,d2,v′J,C,d_2,v' are squarefree and pairwise coprime: (C,J)=1(C,J)=1 belongs to Oσ\mathfrak O_\sigma, ∣Bo(g′)∣2|B_o(g')|^2 forces (g′,CJ)=1(g',CJ)=1, d2∣g′d_2\mid g', and the retained zero of DoD_o, together with the old gcd restriction, gives (v′,g′CJ)=1(v',g'CJ)=1. Thus fnewf_{\mathrm{new}} is squarefree on that support. These common factors remain in the outer weight through Cauchy.

The triple γ\gamma will be fixed before the child row and label sums. Its puncture ργ\rho_\gamma is therefore independent of those two averaging variables. The ideals J,C,d2,v′J,C,d_2,v' remain in the new averaged label; they are not counted as additional fixed labels.

Apply (17.16) on each selected-side copy with the ordered list (d2,rg,v′;na)(d_2,r_g,v';n_a). Let Ia′I_a' be the subcollection of the selected side’s slots retained on nan_a in copy aa. Assigned primes and their priority masks remain outer. A surviving prime dividing nn is already prime to JCd2v′JCd_2v' by the fourth-power zero and to rad⁡q0,t′,rg\operatorname{rad}q_0,t',r_g by the fixed puncture. These also supply every earlier survival exclusion because supp⁡B⊂supp⁡(Jq0)\operatorname{supp}\mathfrak B\subset\operatorname{supp}(Jq_0). The surviving mark is therefore an original product-form subcollection. An old slot described as assigned to JJ is only a regrouping of an old ba,Aab_a,\mathfrak A_a assignment by this derived support, not a new independent prime choice.

Keep B2\mathcal B_2 outside the Fourier separation of the full kernel and old windows. Let Ig,Id,Iv,IkI_g,I_d,I_v,I_k be the full supports of the current individual dyad cutoffs ψg,ψd2,ψv,ψk′′\psi_g,\psi_{d_2},\psi_v,\psi_{k''}. Choose fresh cutoffs ωn,a\omega_{n,a} equal to one on the support of WiW_i divided by IgIvI_gI_v, with fixed full supports in an interval [a,b][a,b], where b≥1b\ge1. Choose a nonnegative ωf\omega_f equal to one on IJICIdIvI_JI_CI_dI_v, with fixed full support IfI_f. Include these full supports, and the reconstructed formal product g′v′ng'v'n on them, in the finite window family ID\mathcal I_D specified above. These full fresh child windows give the formal centers and support bounds

Nc=r−Ai−B−t−g−v,Vc=B+θ+v+j,Fc=Nc+Vc,N_c=r-A_i-B-t-g-v,\qquad V_c=B+\theta+v+j,\qquad F_c=N_c+V_c,
∣n^child−Nc∣≤6η,∣f^new−Vc∣≤4η.|\widehat{n}_{\mathrm{child}}-N_c|\le6\eta,\qquad|\widehat{f}_{\mathrm{new}}-V_c|\le4\eta.

On the factorized expression the bounds follow from the exact products ni=AiCt′g′v′nchildn_i=\mathfrak A_iCt'g'v'n_{\rm child} and fnew=JCd2v′f_{\mathrm{new}}=JCd_2v'. The full fresh child cutoff and the full enlarged label window are included in ID\mathcal I_D, so the same bounds hold directly on their supports when independent terms are later added by positivity. Those added terms are not asserted to arise from a parent factorization. During the current separation, the reconstructed formal product x=g′v′nx=g'v'n on the full fresh cutoff is also included in ID\mathcal I_D; thus the 4η4\eta bound used in the second prefactor holds on the whole separated side.

Keep the nonnegative label center VcV_c without rounding it upward. Proceed to a child only if the retained row component is nonzero; then the outer ball has Mch≥0M_{\mathrm{ch}}\ge0. This gate is separate from any structural outer index set, which may contain zero-weight tuples even when B2\mathcal B_2 is identically zero. Similarly, if a full fresh child column window contains no squarefree ideal, its polynomial is zero and that component is omitted. If Nc<0N_c < 0 and a child column exists, its norm is at least one, and Equation (17.45) gives −6η≤Nc<0-6\eta\le N_c < 0. For a retained nonempty child define

Nch=max⁡(0,Nc),δN=Nch−Nc∈[0,6η],Fch=Nch+Vc=Fc+δN.N_{\mathrm{ch}}=\max(0,N_c),\qquad\delta_N=N_{\mathrm{ch}}-N_c\in[0,6\eta],\qquad F_{\mathrm{ch}}=N_{\mathrm{ch}}+V_c=F_c+\delta_N.

This is a bounded change of the test, not a ZηZ^{\eta}-wide support enlargement. Use the fixed enclosing support interval [a,b][a,b] chosen above. If Nc<0N_c<0, nonemptiness gives ZδN≤bZ^{\delta_N}\le b; if Nc≥0N_c\ge0, then δN=0\delta_N=0 and the same bound follows from b≥1b\ge1. Thus 1≤ZδN≤b1\le Z^{\delta_N}\le b in both cases. The fresh annular cutoffs ωn,a(ZδNy)\omega_{n,a}(Z^{\delta_N}y) have support in [a/b,b][a/b,b] and uniformly bounded Euler seminorms. Their scale depends only on the fixed sector centers, not on a current row or label. The full union of these clipping supports is included in ID\mathcal I_D.

Fix a refinement σ\sigma of σ0\sigma_0 by its v′v'-dyad, second ray summand and slot branches. Let Ξσ\Xi_\sigma consist of

ξ=(o,g′ sf,d2∣g′,v′ sf,k′′≠0;new assigned slot primes)\xi=(o,g'\ {\rm sf},d_2\mid g',v'\ {\rm sf},k''\ne0; \text{new assigned slot primes})

with the retained individual supports and slot branches. It contains neither the old f,hf,h nor the current column indices n1,n2n_1,n_2. The identities defining R1,E,J,q0R_1,E,J,q_0 are inherited from oo, and γ,knew,fnew\gamma,k_{\mathrm{new}},f_{\mathrm{new}} are the displayed functions of ξ\xi. The set may be taken before imposing B2\mathcal B_2 and (v′,g′CJ)=1(v',g'CJ)=1, retaining those masks in the signed outer weight. Let A2,σ(ξ)\mathcal A_{2,\sigma}(\xi) be the product of all newly assigned original slot coefficients and their priority masks, conjugated on side two.

Let Xσsrc\mathfrak X_\sigma^{\rm src} be the structural outer set of this transformed component, before adding any independent child rows or labels. It retains o∈Oσo\in\mathfrak O_\sigma, in particular the exact reconstruction b1b2=q02J22sb_1b_2=q_0^2J_2^2s, the derived J=sJ2,q0J=sJ_2,q_0, and the full fixed b1,b2,t′b_1,b_2,t' dyad supports; it also retains the fixed g′,d2g',d_2 supports, d2∣g′d_2\mid g', and its other outer arithmetic and slot conditions. Zero-weight tuples may be retained, and unit Fourier phases are ignored in defining this structural set. Define the set of distinct triples, with no witness multiplicity, by

Γσ={(q0,t′,rg=g′/d2):ξ∈Xσsrc}.\Gamma_\sigma= \{(q_0,t',r_g=g'/d_2):\xi\in\mathfrak X_\sigma^{\rm src}\}.

This projection is taken once over all possible current rows and labels, before fixing any knew,fnewk_{\mathrm{new}},f_{\mathrm{new}} or Fourier mode. Every nonzero transformed term maps into it. Every member has a source witness, which gives c^≤ℓ+η\widehat c\le\ell+\eta, t^≤t+η\widehat t\le t+\eta, and log⁡Zqrg≤g−θ+2η\log_Zq_{r_g}\le g-\theta+2\eta. The first of these bounds will be needed for the child puncture; the containing norm balls used for counting do not imply it. The nonempty row and child-column gates stated above remain separate from this structural projection.

Put

Dc=ℓ+Ai+t+g−θ+V.D_c=\ell+A_i+t+g-\theta+V.

Since r=N−3ℓr=N-3\ell is an exact definition tied to the fixed parent, substitution in Equations (17.45) and (17.37) gives the exact formal identities

Fc=F−Dc−2ℓ+j,Mc=M−2Dc−2ℓ+j,Fc−Mc=F−M+Dc,4Fc−3Mc=4F−3M+2(Ai+t+g−θ+V)+j.\begin{aligned} F_c&=F-D_c-2\ell+j,\qquad&M_c&=M-2D_c-2\ell+j,\\ F_c-M_c&=F-M+D_c,\\ 4F_c-3M_c&=4F-3M+2(A_i+t+g-\theta+V)+j. \end{aligned}

These identities involve the same fixed F=N+VF=N+V as Equation (17.9), not an actual parent norm.

For every γ∈Γσ\gamma\in\Gamma_\sigma, choose any source witness. Its actual divisibility d2∣g′d_2\mid g' and Equation (17.24) give

θ^≤g^,j^≤2ℓ^pair,c^≤ℓ^pair.\widehat\theta\le\widehat g,\qquad \widehat j\le2\widehat\ell_{\rm pair},\qquad \widehat c\le\widehat\ell_{\rm pair}.

Consequently the only actual-to-center inequalities needed here are

g−θ≥−2η,j≤2ℓ+3η,c^≤ℓ+η.g-\theta\ge-2\eta,\qquad j\le2\ell+3\eta,\qquad\widehat c\le\ell+\eta.

The first two are not asserted with zero error. In particular the third inequality holds for every fixed triple because of its source witness, even though it need not hold throughout the containing count ball. The new radical in (17.44) has actual logarithmic norm Qnew=QγQ_{\mathrm{new}}=Q_\gamma, satisfying

Qnew≤Q+c^+t^+g^−θ^≤Q+ℓ+t+g−θ+4η≤Q+Dc+4η.\begin{aligned} Q_{\mathrm{new}} &\le Q+\widehat{c}+\widehat{t}+\widehat{g}-\widehat{\theta}\\ &\le Q+\ell+t+g-\theta+4\eta\le Q+D_c+4\eta. \end{aligned}

This also holds when its factors share primes with the old puncture, because taking the radical only decreases the norm. The last inequality uses Ai,V≥0A_i,V\ge0. Use Fch=Fc+δNF_{\mathrm{ch}}=F_c+\delta_N, Mch=Mc+ηM_{\mathrm{ch}}=M_c+\eta, and 2(Ai+t+g−θ+V)+j≥−4η2(A_i+t+g-\theta+V)+j\ge-4\eta in (17.48). The two child margins satisfy

Fch−Mch−Qnew−z0≥cnode+δN−5η≥cnode−5η,4Fch−3Mch−6z0≥cnode+4δN−7η≥cnode−7η.\begin{aligned} F_{\mathrm{ch}}-M_{\mathrm{ch}}-Q_{\mathrm{new}}-z_0&\ge c_{\mathrm{node}}+\delta_N-5\eta\ge c_{\mathrm{node}}-5\eta,\\ 4F_{\mathrm{ch}}-3M_{\mathrm{ch}}-6z_0&\ge c_{\mathrm{node}}+4\delta_N-7\eta\ge c_{\mathrm{node}}-7\eta. \end{aligned}

The nominal cap z0z_0 is unchanged because the surviving mark is a subcollection. Moreover Dc≥ℓ+V−2ηD_c\ge\ell+V-2\eta and 2ℓ−j≥−3η2\ell-j\ge-3\eta, whence

M−Mch=2Dc+2ℓ−j−η≥2(ℓ+V)−8η≥2d−8η.M-M_{\mathrm{ch}}=2D_c+2\ell-j-\eta\ge2(\ell+V)-8\eta\ge2d-8\eta.

For η≤d/16\eta\le d/16 this is at least 3d/23d/2, hence at least dd. The same identities give Fc≤F−ℓ−V+5ηF_c\le F-\ell-V+5\eta, so Fch≤F+11ηF_{\mathrm{ch}}\le F+11\eta. Because its two summands are nonnegative, this bounds the child Nch,VcN_{\mathrm{ch}},V_c through the finite depth.

The arithmetic construction has thus produced admissible child ranges with a smaller row length. We next express the transformed sum in their canonical polynomials. The required Fourier density is common to all triples γ\gamma, rows and labels; only after that identity will we apply Cauchy and dominate the reconstruction multiplicities.

A common density for the second transformed sum. Before any actual outer ideal is summed, use the six independent coordinates

(yg,yd,yv,yk,y1,y2)=(qg′Zg,qd2Zθ,qv′Zv,qk′′Zh2,qn1ZNc,qn2ZNc).(y_g,y_d,y_v,y_k,y_1,y_2) =\left(\frac{q_{g'}}{Z^g},\frac{q_{d_2}}{Z^\theta}, \frac{q_{v'}}{Z^v},\frac{q_{k''}}{Z^{h_2}}, \frac{q_{n_1}}{Z^{N_c}},\frac{q_{n_2}}{Z^{N_c}}\right).

Use the fresh cutoffs ωn,a,ωf\omega_{n,a},\omega_f already chosen. Retain the four current dyad cutoffs and ωf\omega_f outside inversion, and ωn,a\omega_{n,a} in the two columns. Let Ω2,α\Omega_{2,\alpha} be larger cutoffs equal to one on the full supports of the corresponding four dyad and two column cutoffs. These full supports, IfI_f, and the formal products g′v′ng'v'n on them are the windows already included in ID\mathcal I_D.

The exact second root and kernel argument are

Kqd2qv′qn1qn2=Zλc+12η+τyd−1yv−1(y1y2)−1/2,\frac{K}{q_{d_2}q_{v'}\sqrt{q_{n_1}q_{n_2}}} =Z^{\lambda_c+12\eta+\tau}y_d^{-1}y_v^{-1}(y_1y_2)^{-1/2},
Kqk′′qd2qv′2qn1qn2=Aker,2ykydyv2y1y2,\frac{Kq_{k''}}{q_{d_2}q_{v'}^2q_{n_1}q_{n_2}} =A_{{\rm ker},2}\frac{y_k}{y_dy_v^2y_1y_2},
Aker,2=ZHuse+h2−θ−2v−2Nc.A_{\mathrm{ker},2}=Z^{H_{\mathrm{use}}+h_2-\theta-2v-2N_c}.

Indeed Nc=si−g−vN_c=s_i-g-v and λc=Hc−θ−(si−g)\lambda_c=H_c-\theta-(s_i-g). Define the one ambient profile

H2,σ,t(y)=Z−6η∏αΩ2,α(yα)yd−1yv−1(y1y2)−1/2×Wi(ygyvy1)Wi(ygyvy2)‾K2 ⁣(Aker,2ykydyv2y1y2).\begin{aligned} \mathfrak H_{2,\sigma,\boldsymbol t}(\boldsymbol y)={}&Z^{-6\eta} \prod_\alpha\Omega_{2,\alpha}(y_\alpha) y_d^{-1}y_v^{-1}(y_1y_2)^{-1/2}\\ &\times W_i(y_gy_vy_1)\overline{W_i(y_gy_vy_2)} \mathcal K_2\!\left(A_{{\rm ker},2}\frac{y_k}{y_dy_v^2y_1y_2}\right). \end{aligned}

The scalar outside it is exactly Zλc+18η+τZ^{\lambda_c+18\eta+\tau}. The full qd2q_{d_2} denominator and both normalized real column roots are in this profile, and no such root is appended to the final tests.

For ζ=(ζg,ζd,ζv,ζk,ζ1,ζ2)\boldsymbol\zeta=(\zeta_g,\zeta_d,\zeta_v,\zeta_k, \zeta_1,\zeta_2), put zn=qn/ZNchz_n=q_n/Z^{N_{\mathrm{ch}}} and define

Wa′(z)=ωn,a(ZδNz)zεaiζa,νa′=νiϑ‾,da′=dIa′.W_a'(z)=\omega_{n,a}(Z^{\delta_N}z)z^{\varepsilon_a i\zeta_a}, \qquad \nu_a'=\nu_i\overline\vartheta,\qquad \mathfrak d_a'=\mathfrak d_{I_a'}.

The polynomial on either new Cauchy side is then exactly

Qa,γ,ζ(knew,fnew)=∑n sfαˉ(n)γ2(n)νa′(n)ρ′(n)χn(knew)×χn(fnew)4da′(n)Wa′(qn/ZNch).\begin{aligned} Q_{a,\gamma,\boldsymbol\zeta}(k_{\rm new},f_{\rm new})={}& \sum_{n\ {\rm sf}}\bar\alpha(n)\gamma_2(n)\nu_a'(n)\rho'(n) \chi_n(k_{\rm new})\\ &\times\chi_n(f_{\rm new})^4 \mathfrak d_a'(n)W_a'(q_n/Z^{N_{\rm ch}}). \end{aligned}

After q0q_0, t′t', g′/d2g'/d_2 and the finite ray sector are fixed, νa′\nu_a' and ρ′\rho' are independent of J,C,d2,v′J,C,d_2,v' and the new row. The only new characters on nn are the explicitly displayed row and fourth-power factors; all other phases involving the old bib_i, Ai\mathfrak A_i were placed in Equation (17.25) or in the old row h~\widetilde h. The separated annular weight Wa′W_a' is also independent of the new row and label. The complete remaining outer weight is

Vσ(ξ;ζ)=wo+μ(d2)μ(v′)G^(ϑ)∣Bo(g′)∣2∣Do(v′;d2,k′′)∣21(v′,g′CJ)=1B2(k′′)×A2,σ(ξ)ψg(yg)ψd2(yd)ψv(yv)ψk′′(yk)ωf(qfnew/ZVc)×ygiζgydiζdyviζvykiζkZiδN(ζ1+ζ2).\begin{aligned} V_\sigma(\xi;\boldsymbol\zeta)={}&w_o^+\mu(d_2)\mu(v')\widehat G(\vartheta) |B_o(g')|^2|D_o(v';d_2,k'')|^2 1_{(v',g'CJ)=1}\mathcal B_2(k'')\\ &\times\mathcal A_{2,\sigma}(\xi) \psi_g(y_g)\psi_{d_2}(y_d)\psi_v(y_v)\psi_{k''}(y_k) \omega_f(q_{f_{\rm new}}/Z^{V_c})\\ &\times y_g^{i\zeta_g}y_d^{i\zeta_d}y_v^{i\zeta_v}y_k^{i\zeta_k} Z^{i\delta_N(\zeta_1+\zeta_2)}. \end{aligned}

All old pure arithmetic and priority masks are retained in Oσ\mathfrak O_\sigma, with their nonnegative old coefficient weight wo+w_o^+. The displayed two common magnitudes retain every other common coefficient zero, including the one depending on k′′k''. There is one μ(d2)\mu(d_2), one μ(v′)\mu(v'), and one ray coefficient. The label cutoff is inserted as an equality on the original product supports and remains outer.

Let Tσ,i\mathcal T_{\sigma,i} be the fixed v′v'-dyad, ray, and slot summand obtained from Equation (17.41) by the complete Möbius and slot expansions above. The exact identity needed for the child is

Tσ,i=Zλc+18η+τ(2π)−6∫R6H^2,σ,t(ζ)×∑ξ∈ΞσVσ(ξ;ζ)Q1,γ,ζ(knew,fnew)Q2,γ,ζ(knew,fnew)‾ dζ.\begin{aligned} \mathcal T_{\sigma,i}={}&Z^{\lambda_c+18\eta+\tau}(2\pi)^{-6} \int_{\mathbb R^6}\widehat{\mathfrak H}_{2,\sigma,\boldsymbol t} (\boldsymbol\zeta)\\ &\quad\times\sum_{\xi\in\Xi_\sigma}V_\sigma(\xi;\boldsymbol\zeta) Q_{1,\gamma,\boldsymbol\zeta}(k_{\rm new},f_{\rm new}) \overline{Q_{2,\gamma,\boldsymbol\zeta}(k_{\rm new},f_{\rm new})} \,d\boldsymbol\zeta. \end{aligned}

To check it, expand the two QQ’s. Since ya=ZδNznay_a=Z^{\delta_N}z_{n_a}, their modes together with the last factor of Equation (17.56) are exactly y1iζ1y2iζ2y_1^{i\zeta_1}y_2^{i\zeta_2}. The other four modes are outer. Equation (17.19) restores the full profile, whose larger cutoffs are one on the retained supports. The fresh column cutoffs are one wherever the old WiW_i factors are nonzero, and ωf=1\omega_f=1 on every original label product. The scalar and profile therefore restore the full root, full kernel, and old windows. Equations (17.42), (17.43), and (17.16) restore the arithmetic factors term by term. The fixed-box sums are finite and Equation (17.20) justifies the integral. Extra combinations in the full fresh windows cancel through the old windows in this complex Fourier identity before Cauchy; only later are they kept independently in a positive sum.

The density in Equation (17.57) depends on the fixed sector, ZZ, the fixed tests and t\boldsymbol t, not on actual γ,knew,fnew\gamma,k_{\mathrm{new}},f_{\mathrm{new}}. The coupled kernel uses the bare k′′k'' coordinate, not the derived row; the latter appears only in characters and B2\mathcal{B}_2. The derived label appears only in characters and its outer cutoff. Relations such as g′=d2rgg'=d_2r_g restrict evaluation points, not the transform. For every fixed Bht,Jht≥0B_{\mathrm{ht}},J_{\mathrm{ht}}\ge0, the Euler calculation in Equation (17.20) gives some fixed bb with

∫R9∫R6∣H^1,σ(t)∣∣H^2,σ,t(ζ)∣(1+∣t∣)Bht(1+∣ζ∣)Jht dζ dt≪pb(W)2.\int_{\mathbb R^9}\int_{\mathbb R^6} |\widehat{\mathfrak H}_{1,\sigma}(\boldsymbol t)| |\widehat{\mathfrak H}_{2,\sigma,\boldsymbol t}(\boldsymbol\zeta)| (1+|\boldsymbol t|)^{B_{\rm ht}}(1+|\boldsymbol\zeta|)^{J_{\rm ht}} \,d\boldsymbol\zeta\,d\boldsymbol t\ll p_b(W)^2.

Indeed the inner weighted integral is polynomial in t\boldsymbol t, because WiW_i is a fixed cutoff times a unit norm mode; apply the first transform’s bound at that polynomial order plus BhtB_{\mathrm{ht}}. The constants are uniform in every actual ideal and every positive kernel scalar, with no height-order power of ZZ.

The second Cauchy inequality and the outer counts. Apply Equation (D) to the second transformed sum with Ua=Z(λc+18η+τ)/2Qa,γ,ζU_a=Z^{(\lambda_c+18\eta+\tau)/2}Q_{a,\gamma,\boldsymbol\zeta} on the complete set Ξσ\Xi_\sigma, for each fixed Fourier mode. In particular B2\mathcal B_2, ∣Bo∣2|B_o|^2, ∣Do∣2|D_o|^2, and 1(v′,g′CJ)=11_{(v',g'CJ)=1} are still in its weight. They retain the squarefreeness of fnewf_{\mathrm{new}} proved above. All other factors in the weight are bounded by a fixed constant, including the bounded number of original assigned slot coefficients, the fixed ray coefficient, the individual cutoffs, and the unit modes. Consequently, only after Cauchy, the absolute weights obey

∣Vσ(ξ;ζ)∣≪B2(k′′)μ2(fnew).|V_\sigma(\xi;\boldsymbol\zeta)| \ll \mathcal B_2(k'')\mu^2(f_{\rm new}).

This is the step which permits the new averaged ideal to remain in the squarefree class.

We first record the exact reconstruction needed to dominate a fibre.

dk∣CB/R1⟹dk∣fnewrad⁡q0.d_k\mid C\mathfrak B/R_1 \quad\Longrightarrow\quad d_k\mid f_{\rm new}\operatorname{rad}q_0.

To prove this, a prime of B/R1\mathfrak{B}/R_1 has tp=0t_p=0. The local table shows that it has even parity and equal aipa_{ip}. If both are one it is in J2J_2, and if both are zero it is in rad⁡q0\operatorname{rad}q_0. Primes of CC are already in fnewf_{\mathrm{new}}. This proves the implication. Thus dkd_k also has divisor multiplicity after fnew,q0f_{\mathrm{new}},q_0 are specified. Once these factors are fixed, k′′k'' is uniquely determined by the element knew=dkd2k′′k_{\mathrm{new}}=d_kd_2k''.

Let KslotK_{\mathrm{slot}} bound the original number of slots. At fixed γ=(q0,t′,rg)\gamma=(q_0,t',r_g), squarefree f=fnewf=f_{\mathrm{new}}, and element k=knewk=k_{\mathrm{new}}, the number of possible ξ∈Ξσ\xi\in\Xi_\sigma with nonzero weight is at most a fixed constant times DKslot(f)CKslot(γ)D_{K_{\mathrm{slot}}}(f)C_{K_{\mathrm{slot}}}(\gamma), where

DKslot(f)=dO(f)9+4Kslot,D_{K_{\rm slot}}(f)=d_{\mathcal O}(f)^{9+4K_{\rm slot}},
CKslot(γ)=dO(q0)5+2KslotdO(t′)2KslotdO(rg)2Kslot,C_{K_{\rm slot}}(\gamma)= d_{\mathcal O}(q_0)^{5+2K_{\rm slot}} d_{\mathcal O}(t')^{2K_{\rm slot}} d_{\mathcal O}(r_g)^{2K_{\rm slot}},

Here and below dOd_{\mathcal O} denotes the ideal divisor count. For completeness, the ordered allocation of ff into J,C,d2,v′J,C,d_2,v' costs 4ω(f)=dO(f)24^{\omega(f)}=d_{\mathcal O}(f)^2, and splitting J=sJ2J=sJ_2 costs at most dO(f)d_{\mathcal O}(f). The choices of b1,b2b_1,b_2 with b1b2=q02J22sb_1b_2=q_0^2J_2^2s cost at most dO(q0)2dO(f)3d_{\mathcal O}(q_0)^2d_{\mathcal O}(f)^3; the two choices Aa∣rad⁡(b1b2)\mathfrak{A}_a\mid\operatorname{rad}(b_1b_2) cost at most dO(q0)2dO(f)2d_{\mathcal O}(q_0)^2d_{\mathcal O}(f)^2. These estimates use dO(IJ)≤dO(I)dO(J)d_{\mathcal O}(IJ)\le d_{\mathcal O}(I)d_{\mathcal O}(J) and dO(I2)≤dO(I)2d_{\mathcal O}(I^2)\le d_{\mathcal O}(I)^2. Equation (17.59) costs at most dO(q0)dO(f)d_{\mathcal O}(q_0)d_{\mathcal O}(f) choices for dkd_k. Then g′=d2rgg'=d_2r_g is fixed, and k′′=k/(dkd2)k''=k/(d_kd_2) is the unique element if it is integral. The at most 2Kslot2K_{\mathrm{slot}} old assigned primes divide q0ft′q_0ft', so their choices cost at most [dO(q0)dO(f)dO(t′)]2Kslot[d_{\mathcal O}(q_0)d_{\mathcal O}(f)d_{\mathcal O}(t')]^{2K_{\rm slot}}. The at most 2Kslot2K_{\mathrm{slot}} new assigned primes divide frgfr_g, and cost at most [dO(f)dO(rg)]2Kslot[d_{\mathcal O}(f)d_{\mathcal O}(r_g)]^{2K_{\rm slot}}. The other first side’s surviving slots disappeared on selecting the first positive side; the selected surviving slots occur twice in its new square, exactly as counted here. Thus the displayed product dominates the fibre even if its actual size depends on kk. There is no count of the old f,hf,h, no independent count of J,C,d2,v′J,C,d_2,v', and no second frequency count.

Equation (17.34) and the same source witnesses place Γσ\Gamma_\sigma inside the product of the three norm balls

qq0≤Zℓ+R/2−j+5η/2,qt′≤Zt+η,qrg≤Zg−θ+2η.q_{q_0}\le Z^{\ell+R/2-j+5\eta/2},\qquad q_{t'}\le Z^{t+\eta},\qquad q_{r_g}\le Z^{g-\theta+2\eta}.

We use these balls only to bound the number of distinct triples, not as a replacement domain for the child estimate. Ideal counting gives

#Γσ≤CZCc+11η/2+πcount,Cc=ℓ+R/2−j+t+g−θ.\#\Gamma_\sigma\le CZ^{C_c+11\eta/2+\pi_{\mathrm{count}}}, \qquad C_c=\ell+R/2-j+t+g-\theta.

Here πcount\pi_{\mathrm{count}} is part of the separately chosen aggregate π\pi. In a nonempty sector each upper exponent of these three balls is nonnegative, since it bounds the norm of an existing ideal; the constant term in ideal counting therefore adds no boundary power. In particular JJ is not counted here. The ranges of all three ideals are bounded, so the adjustable divisor bound gives CKslot(γ)≪ZπfibC_{K_{\mathrm{slot}}}(\gamma)\ll Z^{\pi_{\mathrm{fib}}} uniformly on the containing balls. Put cσ=Cc+11η/2c_\sigma=C_c+11\eta/2 and introduce the genuinely row- and label-independent measure

dνσ(γ)=Z−cσ∑γ∈ΓσCKslot(γ)δγ,∥νσ∥≪Zπcount+πfib.d\nu_\sigma(\gamma)=Z^{-c_\sigma} \sum_{\gamma\in\Gamma_\sigma}C_{K_{\rm slot}}(\gamma)\delta_\gamma, \qquad \|\nu_\sigma\|\ll Z^{\pi_{\rm count}+\pi_{\rm fib}}.

The positive canonical children. For a fixed Fourier mode define the positive child sums

Ha,γ=∑f sfqf/ZVc∈IfDKslot(f)∑k∈O0<qk≤ZMch∣Qa,γ,ζ(k,f)∣2=ZFchEa,γ.\mathcal H_{a,\gamma}={} \sum_{\substack{f\ {\rm sf}\\q_f/Z^{V_c}\in I_f}} D_{K_{\rm slot}}(f) \sum_{\substack{k\in\mathcal O\\0<q_k\le Z^{M_{\rm ch}}}} |Q_{a,\gamma,\boldsymbol\zeta}(k,f)|^2 =Z^{F_{\rm ch}}\mathcal E_{a,\gamma}.

The equality is the normalization of (17.3) with this same row ball, the label weight DKslotD_{K_{\mathrm{slot}}}, and the test and puncture in Equations (17.55) and (17.44); if a larger fixed row ball is used there, this equality is instead an inequality in the needed upper-bound direction. The weight depends on ff alone. After reindexing, B2\mathcal B_2 is exactly the displayed row ball. Only the now positive outer row and label sums have been enlarged to their full fixed windows. The columns use their full fixed fresh windows, but their puncture, mark, and test have not been deleted or changed. The actual fibre domination just proved gives

∣∑ξ∈ΞσVσQ1Q2‾∣≤∏a=12(∑ξ∈Ξσ∣Vσ∣∣Qa∣2)1/2≪Zcσ∏a=12(∫ΓσHa,γ dνσ(γ))1/2.\begin{aligned} \left|\sum_{\xi\in\Xi_\sigma}V_\sigma Q_1\overline{Q_2}\right| &\le\prod_{a=1}^2 \left(\sum_{\xi\in\Xi_\sigma}|V_\sigma||Q_a|^2\right)^{1/2}\\ &\ll Z^{c_\sigma}\prod_{a=1}^2 \left(\int_{\Gamma_\sigma}\mathcal H_{a,\gamma} \,d\nu_\sigma(\gamma)\right)^{1/2}. \end{aligned}

Here Qa=Qa,γ,ζ(knew,fnew)Q_a=Q_{a,\gamma,\boldsymbol\zeta}(k_{\rm new},f_{\rm new}). The two square roots each supply Zcσ/2Z^{c_\sigma/2}, hence there is one fixed-count factor. A uniform child bound supplies one total mass ∥νσ∥\|\nu_\sigma\|, not its square. The child bound will be used only for γ∈Γσ\gamma\in\Gamma_\sigma, using the hypotheses already verified in Equation (17.51).

The energy exponent. The formal centers satisfy the exact identity

κi+λc+Cc+2Fc=F.\kappa_i+\lambda_c+C_c+2F_c=F.

This follows by substituting their definitions and Hc=2r−2B−M+4ℓ+2V+δ−jH_c=2r-2B-M+4\ell+2V+\delta-j; all extracted lengths cancel and the result is r+3ℓ+V=N+Vr+3\ell+V=N+V.

We now use the child estimate only for γ∈Γσ\gamma\in\Gamma_\sigma, for which the preceding margins and row decrease have been proved. If it gives Ea,γ≪C(t,ζ)ZFch+ϵchild\mathcal E_{a,\gamma}\ll C(\boldsymbol t,\boldsymbol\zeta) Z^{F_{\rm ch}+\epsilon_{\rm child}} uniformly there, with its fixed polynomial height dependence, then Equation (17.63) and the final weighted Cauchy bound above give

∣∑ξ∈ΞσVσQ1Q2‾∣≪C(t,ζ)Zcσ+2Fch+ϵchild∥νσ∥.\left|\sum_{\xi\in\Xi_\sigma}V_\sigma Q_1\overline{Q_2}\right| \ll C(\boldsymbol t,\boldsymbol\zeta) Z^{c_\sigma+2F_{\rm ch}+\epsilon_{\rm child}}\|\nu_\sigma\|.

The normalized mass is the one in Equation (17.62); witness multiplicity is already in its fibre weights. The common Fourier density is then integrated once using Equation (17.58). It is not part of the discrete measure and is not chosen afresh for any row or label. Thus both the genuine outer count and its normalized mass occur once. The averaged J,C,d2,v′J,C,d_2,v' stay inside the positive child sum and are not also counted.

If a child is bounded by ZFch+ϵchildZ^{F_{\mathrm{ch}}+\epsilon_{\mathrm{child}}}, the first prefactor error, the second prefactor error, the fixed count, and the restored normalization give on each positive second-Cauchy side

κi+λc+Cc+2Fch+(92+18+112)η+τ+π+ϵchild=F+28η+2δN+τ+π+ϵchild≤F+40η+τ+π+ϵchild.\begin{aligned} \kappa_i+\lambda_c+C_c+2F_{\mathrm{ch}}+\left(\frac{9}{2}+18+\frac{11}{2}\right)\eta+\tau+\pi+\epsilon_{\mathrm{child}} &=F+28\eta+2\delta_N+\tau+\pi+\epsilon_{\mathrm{child}}\\ &\le F+40\eta+\tau+\pi+\epsilon_{\mathrm{child}}. \end{aligned}

Both copies of δN\delta_N are present: one restores the child column normalization and the other occurs in its asserted exponent. Each of the two weighted Cauchy inequalities takes a geometric mean of its positive sides, so it does not double this loss. The first principal bound is ZM+πZ^{M+\pi}, and the second principal bound above is at most ZF+26η+τ+πZ^{F+26\eta+\tau+\pi}; both fit the same allowance.

The parameter π\pi has an independent quantifier. Let JstepJ_{\mathrm{step}} be the maximum number of uses of a free divisor or sieve exponent and of logarithmic dyadic-count factors in one fixed two-Poisson, two-Cauchy factorization tree, maximized over the finitely many assignments with at most the fixed slot bound. Once LpowL_{\mathrm{pow}} bounds the log-length of every scale product in such a use, choose each free input exponent at most π/(2Jstepmax⁡(1,Lpow))\pi/(2J_{\mathrm{step}}\max(1,L_{\mathrm{pow}})). For sufficiently large ZZ, the product of the at most JstepJ_{\mathrm{step}} logarithmic factors is at most Zπ/2Z^{\pi/2}. These choices make all non-center, non-frequency local losses at most CZπCZ^\pi. They include the retained common frequency dyads and the reconstruction divisor bounds. In particular the distinct allocations πβ,πold,πcount,πfib\pi_\beta,\pi_{\mathrm{old}},\pi_{\mathrm{count}},\pi_{\mathrm{fib}} and the finite-union dyadic allocation are parts of this single aggregate, not repeated allowances of size π\pi. Fixed ray sums and fixed seminorm constants are constants. The same convention defines the aggregate terminal loss πref\pi_{\mathrm{ref}}. In particular π\pi hides no multiple of η\eta or τ\tau.

This proves the conditional reduction estimate (17.17), including its common-measure and finite-order uniformity once the choices below are made. It remains to fix those choices uniformly and apply the reduction through the finite depth.

Order of choices and termination. For the requested canonical exponent ϵc=ϵ\epsilon_c=\epsilon, first fix the starting ranges, tests, slot bound, c∗c_*, and then d,Dd,D as at the beginning of the proof. Choose

η≤min⁡{d/16,c∗/(14D),ϵc/(160D),c∗/1000,1/100},τ≤min⁡{ϵc/(4D),c∗/1000,1/100},π≤ϵc/(4D),τref,πref≤c∗/1000.\eta\le\min\{d/16,c_*/(14D),\epsilon_c/(160D),c_*/1000,1/100\}, \qquad \tau\le\min\{\epsilon_c/(4D),c_*/1000,1/100\}, \qquad \pi\le\epsilon_c/(4D), \qquad \tau_{\mathrm{ref}},\pi_{\mathrm{ref}} \le c_*/1000.

Use this same τ\tau in both Poisson comparisons. At this point π\pi is a target aggregate loss; its subsidiary input exponents are chosen only after the bounded scale range is known.

Choose the individual cutoffs through depth DD, including every full larger or fresh support and the bounded clipping families described above, and form ID,Lwin\mathcal{I}_D,L_{\mathrm{win}}. Include the product intervals for the active slots and the terminal constants Cres,Cwidth,CkerC_{\mathrm{res}},C_{\mathrm{width}},C_{\mathrm{ker}}, maximized through the depth. This is finite because there are finitely many factorization types per passage and finitely many passages. Put

Fmax⁡=Nmax⁡+Vmax⁡+11Dη,Lall=100(1+Mmax⁡+Fmax⁡+z0,max⁡+c∗).F_{\max}=N_{\max}+V_{\max}+11D\eta,\qquad L_{\mathrm{all}}=100(1+M_{\max}+F_{\max}+z_{0,\max}+c_*).

These bound all retained scale lengths. Indeed, Equation (17.52) and the bound following it give M≤Mmax⁡M\le M_{\max} and N,V≤Fmax⁡N,V\le F_{\max}. A nonempty column window has r≥−ηr\ge-\eta, so ℓ≤(Fmax⁡+η)/3\ell\le(F_{\max}+\eta)/3. The displayed parent products bound every extracted divisor length by 2Fmax⁡+6η2F_{\max}+6\eta. For example dk∣Crad⁡(b1b2)d_k\mid C\operatorname{rad}(b_1b_2) gives δ≤r+2ℓ+4η\delta\le r+2\ell+4\eta, and Equation (17.26) then gives Huse≤7Fmax⁡+18η+τH_{\mathrm{use}}\le7F_{\max}+18\eta+\tau. The terminal active conductor is supported on the row, ff, the puncture, and slots; their total lengths are at most Mmax⁡+2Fmax⁡+z0,max⁡M_{\max}+2F_{\max}+z_{0,\max} plus the already displayed ratio allowances. Equations (17.11) and (14.11) bound the retained terminal dual lengths by 4Mmax⁡+4Fmax⁡+2z0,max⁡+3d+12η+τref4M_{\max}+4F_{\max}+2z_{0,\max}+3d+12\eta+\tau_{\mathrm{ref}}. Under Equation (17.66), all these bounds and the exact conductor product lengths are below LallL_{\mathrm{all}}. We may now take Lpow=LallL_{\mathrm{pow}}=L_{\mathrm{all}} and choose the subsidiary small exponents that realize π\pi and πref\pi_{\mathrm{ref}}.

Define BcrudeB_{\mathrm{crude}} to be the maximum exponent obtained by replacing every bounded nonfrequency ideal or element sum in either raw Poisson expansion, including both column sums, by its lattice count at length LallL_{\mathrm{all}}, and every explicit norm factor, including 1+a−11+a^{-1} in (17.21), by its absolute upper bound. Replace divisor-bounded coefficients and marks by their trivial polynomial norm bounds as well. Exclude only the frequency kernel itself. The expansions contain a fixed finite number of factors, so this defines a finite uniform number.

For the reflected tail define BrefB_{\mathrm{ref}} analogously using its bounded row, local, and active-product counts and 1+a−11+a^{-1} with a=X/qc2a=X/q_c^2. Do not count discarded dual indices at a retained length. Instead, (5.2) gives on its support

∣d(μ)∣qμ≤27qλ−k/3qn−1/2qb−1≤27qλ4/3(k≥−4).\frac{|d(\mu)|}{\sqrt{q_\mu}}\le27q_\lambda^{-k/3}q_n^{-1/2}q_b^{-1}\le27q_\lambda^{4/3}\qquad(k\ge-4).

Every other local factor is bounded by the product of qp1/2q_p^{1/2} over the bounded active primes, independently of μ\mu after its indicators are dropped. Thus BrefB_{\mathrm{ref}} covers all non-kernel coefficients and bounded counts, while the remaining μ\mu-sum is an unrestricted lattice sum on λ−4O\lambda^{-4}\mathcal{O}.

Fix a tail saving T>1+Bcrude+BrefT > 1 + B_{\mathrm{crude}} + B_{\mathrm{ref}}. For each Poisson tail, choose a Schwartz order

A>1+(Bcrude+T)/τ.A > 1 + (B_{\mathrm{crude}} + T)/\tau.

Equation (17.21) with Y=ZτY = Z^\tau then makes the discarded raw outer-ball complement O(Z−T)O(Z^{-T}), up to finitely many input seminorms and a fixed polynomial in any twist heights. For the reflected whole-dyad tail the actual argument is at least Zτref/2Z^{\tau_{\mathrm{ref}}/2}; use the same lattice-shell bound on λ−4O\lambda^{-4}\mathcal{O} and choose

Aref>1+2(Bref+T)/τref.A_{\mathrm{ref}} > 1 + 2(B_{\mathrm{ref}} + T)/\tau_{\mathrm{ref}}.

This proves the discarded-tail assertion without presuming any bound on the discarded dual lengths.

Next choose the finitely many Fourier-height and smooth-seminorm orders backwards through depth DD, above the chosen tail orders and the terminal input orders. Normalized inverse roots are fixed real powers on annuli, and Euler differentiation of a full kernel at a norm monomial introduces no scale power. Equations (17.58) and (17.62) supply the common coefficient measure for each positive indexed Cauchy-side sum. Apply Corollary 17.4 separately to those sums, using the child-profile bounds just proved from Lemma 4.5, and then take the displayed geometric means. The two square roots retain one normalized discrete mass, as already shown, so genuine outer labels are counted only once. Any external height cutoff in a later application is chosen after this internal finite propagation, not inserted into it.

Finally choose ZZ large enough for log⁡Z≥Lwin/η\log Z \ge L_{\mathrm{win}}/\eta, the thresholds for Cres,CwidthC_{\mathrm{res}}, C_{\mathrm{width}} in Equation (17.11), log⁡Z≥2log⁡Cker/τref\log Z \ge2\log C_{\mathrm{ker}}/\tau_{\mathrm{ref}}, log⁡Z≥4log⁡qλ/η\log Z \ge4\log q_\lambda/\eta, and the fixed hh-annulus threshold used in the short completion. Impose also the logarithmic bounds defining the aggregate local losses and the thresholds of the input lemmas. All choices precede this final threshold and depend only on the fixed data. Bounded smaller ZZ are handled by increasing the final constant.

Now ch=c∗−7hη≥c∗/2c_h = c_* - 7h\eta\ge c_*/2 for h≤Dh \le D. Equations (17.51) and (17.52) send every retained nonterminal child to the next depth and its row cap. At depth DD that cap is negative, whereas every retained row parameter is nonnegative. The terminal bounds are at most ZFZ^F; principals and recursive terms cost at most Lstep=40η+τ+πL_{\mathrm{step}} = 40\eta+ \tau+ \pi in exponent. Backward induction gives ZF+(D−h)LstepZ^{F+(D-h)L_{\mathrm{step}}} at depth hh, and

DLstep≤ϵc/4+ϵc/4+ϵc/4<ϵc.DL_{\mathrm{step}} \le\epsilon_c/4 + \epsilon_c/4 + \epsilon_c/4 < \epsilon_c.

This proves E≪ZF0+ϵ\mathcal{E} \ll Z^{F_0+\epsilon}, with the claimed uniform finite-seminorm and polynomial-height dependence.

Initialization of the marked moment

We now convert the inverse polynomial in Lemma 17.1 to the canonical family. Only one Poisson transformation is required.

Proof of Lemma 17.1. In the product Mu(Zr;W)QuM_u(Z^r;W)Q_u, let PP be the product of its slot primes and put j=(n,P)j=(n,P). Both nn and PP are squarefree. Fix the subset of slots occurring in jj, and write

n=jn0,P=jP0,(n0,P0)=1.n = jn_0,\qquad P = jP_0,\qquad(n_0,P_0)=1.

The product c=n0P0c=n_0P_0 is squarefree. The identities

μ(n0)=μ(c)μ(P0),ψu(n)ψu(P)=ψu(j)2ψu(c)\mu(n_0)=\mu(c)\mu(P_0),\qquad\psi_u(n)\psi_u(P)=\psi_u(j)^2\psi_u(c)

hold with all zero extensions. The sign μ(P0)\mu(P_0) is a product of signs on the surviving slots and can be incorporated into their bounded coefficients. The coefficients thus remain of the form in Equation (14.1).

For this fixed assigned subset define GG from its nominal slot centers:

G=∑i assignedzi,z0=z−G,D′=r+z−2G.G=\sum_{i\ {\rm assigned}}z_i,\qquad z_0=z-G,\qquad D'=r+z-2G.

Then G,z0≥0G,z_0\ge0, and z0z_0 is exactly the surviving nominal cap. The normalization satisfies

Z−(r+z)/2=Z−GZ−D′/2.Z^{-(r+z)/2}=Z^{-G}Z^{-D'/2}.

The actual jj is the product of the assigned primes, so qj/ZGq_j/Z^G lies in a fixed product interval. Ideal counting gives at most CZGCZ^G choices, apart from the separately chosen divisor loss for assignments. Triangle inequality in the row Hilbert space uses Z−GZ^{-G} to cancel this count. The whole factor ψu(j)2\psi_u(j)^2 is a bounded row scalar, including its zeros, and is a contraction in that space. The residual column is prime to jj, giving the fixed puncture 1(c,j)=11_{(c,j)=1}.

Here is the exact identity underlying this overlap reduction. Let I0I_0 be the surviving subset and put yj=qj/ZGy_j=q_j/Z^G, yc=qc/ZD′y_c=q_c/Z^{D'}, and yi=qpi/Zziy_i=q_{p_i}/Z^{z_i} for every slot. On the original support,

qnZr=yjyc∏i∈I0yi.\frac{q_n}{Z^r}=\frac{y_jy_c}{\prod_{i\in I_0}y_i}.

For a fixed assigned tuple, its contribution Uu,j\mathcal U_{u,j} to Mu(Zr;W)QuM_u(Z^r;W)Q_u is exactly

Uu,j=μ(j)∏i∉I0ai(pi)Wi(yi) Z−Gψu(j)2Z−D′/2∑c sf(c,j)=1μ(c)ψu(c)×∑(pi)∈∏i∈I0PiP0∣cμ(P0)∏i∈I0ai(pi)Wi(yi)W ⁣(yjyc∏i∈I0yi).\begin{aligned} \mathcal U_{u,j}={}&\mu(j) \prod_{i\notin I_0}a_i(p_i)W_i(y_i)\, Z^{-G}\psi_u(j)^2 Z^{-D'/2} \sum_{\substack{c\ {\rm sf}\\(c,j)=1}}\mu(c)\psi_u(c)\\ &\quad\times \sum_{\substack{(p_i)\in\prod_{i\in I_0}\mathcal P_i\\P_0\mid c}} \mu(P_0)\prod_{i\in I_0}a_i(p_i)W_i(y_i) W\!\left(\frac{y_jy_c}{\prod_{i\in I_0}y_i}\right). \end{aligned}

Indeed a squarefree cc prime to jj, together with a surviving tuple with P0∣cP_0\mid c, reconstructs uniquely n=j(c/P0)n=j(c/P_0) and the prescribed overlap. Squarefreeness of cc already gives (c/P0,P0)=1(c/P_0,P_0)=1, so no further condition was lost. The sign μ(P0)\mu(P_0) is a product of the individual prime signs. This also shows that the jj on both sides of every subsequent square is one fixed ideal: the preceding triangle inequality was taken before that square.

The identity c=nP/j2c=nP/j^2 puts ycy_c in a fixed compact interval. This remains meaningful if D′D' is slightly negative in a bounded nonempty window; D′D' is not yet a canonical parameter. Choose a fresh individual cutoff ωc\omega_c equal to one on this full quotient support. For fixed jj, let Ωc\Omega_c be one on the full support of ωc\omega_c, and let Ωi\Omega_i be one on each full surviving individual slot support. The single joint profile

Hov,j(yc,(yi)i∈I0)=Ωc(yc)∏i∈I0Ωi(yi)W ⁣(yjyc∏i∈I0yi)\mathfrak H_{{\rm ov},j}(y_c,(y_i)_{i\in I_0}) =\Omega_c(y_c)\prod_{i\in I_0}\Omega_i(y_i) W\!\left(\frac{y_jy_c}{\prod_{i\in I_0}y_i}\right)

is compactly supported in these independent coordinates. The current cutoff ωc\omega_c and the individual factors Wi(yi)W_i(y_i) stay outside its transform. Equation (17.19), in dimension 1+∣I0∣1+|I_0|, therefore expresses Equation (17.67) exactly as the same assigned scalar and Z−Gψu(j)2Z^{-G}\psi_u(j)^2, times

(2π)−1−∣I0∣∫R1+∣I0∣H^ov,j(υ)Z−D′/2∑c sfμ(c)ψu(c)1(c,j)=1dυ(c)ωc(yc)yciυc dυ,(2\pi)^{-1-|I_0|}\int_{\mathbb R^{1+|I_0|}} \widehat{\mathfrak H}_{{\rm ov},j}(\boldsymbol\upsilon) Z^{-D'/2}\sum_{c\ {\rm sf}}\mu(c)\psi_u(c)1_{(c,j)=1} \mathfrak d_{\boldsymbol\upsilon}(c) \omega_c(y_c)y_c^{i\upsilon_c}\,d\boldsymbol\upsilon,

where dυ\mathfrak d_{\boldsymbol\upsilon} has the original surviving lists and individual coefficients μ(p)ai(p)Wi(yi)yiiυi\mu(p)a_i(p)W_i(y_i)y_i^{i\upsilon_i}. Expanding the mark and inverting the joint transform proves this equality term by term. No measure is chosen for an actual surviving tuple. The measure may depend on the already fixed jj, but Equation (17.20) is uniform for its yjy_j in the fixed product interval. Minkowski’s inequality is used in the whole row Hilbert space for this one measure. Include the full support of ωc\omega_c, its larger cutoffs, the surviving slot supports, and the jj-product interval in the finite collection ID\mathcal{I}_{D} before the final threshold is chosen. With the same η\eta convention as the canonical proof, we then have

∣c^−D′∣≤η,∣j^−G∣≤η|\widehat{c}-D'| \le\eta,\qquad|\widehat{j}-G| \le\eta

on the full supports actually used below, where c^=log⁡Zqc\widehat{c}=\log_Z q_c. For the sign εχ=1\varepsilon_\chi=1, conjugate the whole residual polynomial, including its finite character, mark, and test; its row norm is unchanged. For the other sign leave it unchanged. It therefore suffices to estimate one polynomial of the exact form

R0(u)=Z−D′/2∑c sfμ(c)ν0(c)1(c,j)=1χc(u)‾d0(c)W0(qc/ZD′).\mathcal R_0(u)=Z^{-D'/2}\sum_{c\ {\rm sf}} \mu(c)\nu_0(c)1_{(c,j)=1}\overline{\chi_c(u)} \mathfrak d_0(c)W_0(q_c/Z^{D'}).

Here ν0\nu_0 is a fixed finite ray character, d0\mathfrak d_0 is the product mark of cap z0z_0 with those individual coefficients or their conjugates, and W0W_0 is ωc(y)yiυc\omega_c(y)y^{i\upsilon_c} or its conjugate. All are independent of the row.

Majorize the original row ball by a fixed nonnegative radial Schwartz function Φinit\Phi_{\mathrm{init}} at scale ZmZ^m, and expand its square. Let CC be the gcd of the two columns and write ci=Czic_i=Cz_i, with z1,z2z_1,z_2 squarefree and coprime. Put c^i=log⁡Zqci\widehat c_i=\log_Zq_{c_i}, so the preceding support bound applies to each i=1,2i=1,2. Let B≥0B\ge0 be the center of CC, and write B^=log⁡ZqC\widehat{B}=\log_Z q_C. The row character has primitive modulus z1z2z_1z_2 and remaining zero mask CC. Apply Lemma 17.5, with d′∣Cd'\mid C. Let θ≥0\theta\ge0 be its center and θ^=log⁡Zqd′\widehat{\theta}=\log_Z q_{d'}. Set

P1=B−θ≥−2η,P_1=B-\theta\ge-2\eta,

where the inequality follows from θ^≤B^\widehat{\theta}\le\widehat{B} and the two η\eta-ratio bounds. The actual conductor length is

L^init=c^1+c^2−2B^,∣L^init−2(D′−B)∣≤4η.\widehat L_{\rm init}=\widehat c_1+\widehat c_2-2\widehat B, \qquad |\widehat L_{\rm init}-2(D'-B)|\le4\eta.

For a positive tolerance τinit\tau_{\mathrm{init}}, the implication Zmqh′/(qd′qz1z2)≤ZτinitZ^m q_{h'}/(q_{d'}q_{z_1z_2})\le Z^{\tau_{\mathrm{init}}} gives

d′h′^≤2D′−m−2P1+6η+τinit.\widehat{d'h'}\le2D'-m-2P_1+6\eta+\tau_{\mathrm{init}}.

Define the fixed formal and enclosing row scales

Mcinit=2D′−m−2P1,Minit=Mcinit+6η+τinit.M_c^{\mathrm{init}}=2D'-m-2P_1,\qquad M_{\mathrm{init}}=M_c^{\mathrm{init}}+6\eta+\tau_{\mathrm{init}}.

The 6η6\eta is 4η4\eta from the conductor and 2η2\eta from the two copies of d′d' in the new row bound.

Separate the original principal contribution for the direct count below. On the genuine nonprincipal coprime Poisson expression, before any off-coprime extension or Fourier absolutization, keep only the outer mask

Binit(h′)=10<qd′h′≤ZMinit.\mathcal B_{\rm init}(h')=1_{0<q_{d'h'}\le Z^{M_{\rm init}}}.

Its complement is contained in the actual ratio tail above for every supported pair. Equation (17.21), with the separate initial raw count and order specified below, discards precisely that complement. Retain the full smooth kernel inside the mask, with no column-dependent ratio selector. The mask depends on d′,h′d',h', the fixed overlap and sector, but not on the residual columns. If Minit<0M_{\mathrm{init}}<0, its nonzero ball is empty and the same tail comparison discards every nonzero frequency; otherwise the retained row parameter is nonnegative.

The actual normalization and Poisson prefactor split over the two sides as

Z−D′Zm−θ^−L^init/2=Zκ^1init/2Zκ^2init/2,κ^iinit=m−D′−θ^−c^i+B^.Z^{-D'}Z^{m-\widehat\theta-\widehat L_{\rm init}/2} =Z^{\widehat\kappa_1^{\rm init}/2} Z^{\widehat\kappa_2^{\rm init}/2}, \quad \widehat\kappa_i^{\rm init}=m-D'-\widehat\theta-\widehat c_i+\widehat B.

Thus the actual side exponents obey

κ^iinit≤κcinit+3η,κcinit=m−2D′+P1.\widehat\kappa_i^{\rm init}\le\kappa_c^{\rm init}+3\eta, \qquad \kappa_c^{\rm init}=m-2D'+P_1.

All normalized real inverse roots will be kept in the single joint profile below, not also in the final child tests. Principal columns have the direct diagonal bound O(Zm+ϵ)O(Z^{m+\epsilon}), also for a bounded nonempty negative D′D'-window. Any principal nonzero frequencies restored to the formal formula carry the same Binit\mathcal{B}_{\mathrm{init}} mask and are bounded by the full principal restoration in Lemma 17.5, since Zm≥1Z^m \ge1.

Insert frequency dyads of qh′q_{h'} from one partition common to all d′d', not a label-recentered partition. The outer mask implies qh′≤ZMinitq_{h'} \le Z^{M_{\mathrm{init}}}, so there are only logarithmically many dyads in the bounded retained range. Let HH be the center of one such bare-frequency dyad, and let ψC,ψd′,ψh′\psi_C,\psi_{d'},\psi_{h'} be the retained individual cutoffs on the current C,d′,h′C,d',h' dyads, evaluated at their normalized norms.

The orientation in (17.68) is now fixed. The calculation in the second canonical Poisson transformation replaces μ(z)γ−1(z)\mu(z)\gamma_{-1}(z) by αˉ(z)γ2(z)χz(−1)G(z)‾\bar\alpha(z)\gamma_2(z)\chi_z(-1)\overline{G(z)}. On the second side the factor inside conjugation has ray factor G(z)‾\overline{G(z)}; together with the CRT cross phase the relative ray factor is G([z2][z1]−1)G([z_2][z_1]^{-1}). Expand it by the fixed group formula above, and in a fixed ray summand put

ν∗=ν0ϑ‾,A∗(z)=αˉ(z)γ2(z)ν∗(z),Kinit=FΦinit.\nu_*=\nu_0\overline\vartheta,\qquad A_*(z)=\bar\alpha(z)\gamma_2(z)\nu_*(z),\qquad \mathcal K_{\rm init}=\mathcal F\Phi_{\rm init}.

For a preliminary pattern Σ0\Sigma_0 fixing the overlap, these dyads and the ray summand, and with the earlier mode held fixed, the masked principal-restored nonzero component is exactly

TΣ0init=∑C sf, d′∣Ch′≠0ψCψd′ψh′μ(d′)G^(ϑ)Binit(h′)1(C,j)=1×∑z1,z2 sf(z1z2,Cj)=11(z1,z2)=1A∗(z1)A∗(z2)‾χz1(d′)‾χz1(h′)χz2(d′)χz2(h′)‾×d0(Cz1)d0(Cz2)‾W0(qCqz1/ZD′)W0(qCqz2/ZD′)‾×Z−D′Zmqd′qz1qz2Kinit ⁣(Zmqh′qd′qz1qz2).\begin{aligned} \mathcal T^{\rm init}_{\Sigma_0}={}& \sum_{\substack{C\ {\rm sf},\ d'\mid C\\h'\ne0}} \psi_C\psi_{d'}\psi_{h'}\mu(d')\widehat G(\vartheta) \mathcal B_{\rm init}(h')1_{(C,j)=1}\\ &\times\sum_{\substack{z_1,z_2\ {\rm sf}\\(z_1z_2,Cj)=1}} 1_{(z_1,z_2)=1} A_*(z_1)\overline{A_*(z_2)} \overline{\chi_{z_1}(d')}\chi_{z_1}(h') \chi_{z_2}(d')\overline{\chi_{z_2}(h')}\\ &\times\mathfrak d_0(Cz_1)\overline{\mathfrak d_0(Cz_2)} W_0(q_Cq_{z_1}/Z^{D'})\overline{W_0(q_Cq_{z_2}/Z^{D'})}\\ &\times\frac{Z^{-D'}Z^m}{q_{d'}\sqrt{q_{z_1}q_{z_2}}} \mathcal K_{\rm init}\!\left( \frac{Z^mq_{h'}}{q_{d'}q_{z_1}q_{z_2}}\right). \end{aligned}

Indeed ∣μ(C)ν0(C)∣2=1|\mu(C)\nu_0(C)|^2=1 for the squarefree CC outside SS, the common row factor is exactly 1(u,C)=11_{(u,C)=1}, and its Poisson expansion contributes the one μ(d′)\mu(d'). The displayed two numerator factors are those of the primitive character χz1‾χz2\overline{\chi_{z_1}}\chi_{z_2} and its Fourier transform. The finite ray sum restores the principal pair by G(1)=1G(1)=1. The cost of that restoration and the raw complement removed before this equality were bounded separately above.

Define the summand in (17.71) on all individually squarefree z1,z2z_1,z_2 prime to CjCj by the displayed separate A∗A_* factors, characters, formal product norms, full kernel, and unchanged outer ball. It agrees on the coprime domain. Insert the complete identity

1(z1,z2)=1=∑s∣(z1,z2)μ(s),za=sna,1_{(z_1,z_2)=1}=\sum_{s\mid(z_1,z_2)}\mu(s),\qquad z_a=sn_a,

before any factorwise bound. Let v≥0v\ge0 be the center of a squarefree ss-dyad, v^=log⁡Zqs\widehat v=\log_Zq_s, and ψs\psi_s its retained individual cutoff. The nan_a are squarefree and prime to ss, but need not be mutually coprime. This formal extension does not apply Poisson summation to a noncoprime conductor. For squarefree coprime s,ns,n, CRT and the zero-preserving identity χn(d′)‾=χn(d′)χn(d′)4\overline{\chi_n(d')}=\chi_n(d')\chi_n(d')^4 give exactly

A∗(sn)χsn(d′)‾χsn(h′)=A∗(s)χs(d′)‾χs(h′)×A∗(n)χn(d′h′)χn(d′s)4.\begin{aligned} A_*(sn)\overline{\chi_{sn}(d')}\chi_{sn}(h') ={}&A_*(s)\overline{\chi_s(d')}\chi_s(h')\\ &\times A_*(n)\chi_n(d'h')\chi_n(d's)^4. \end{aligned}

The fourth power includes the CRT factor χn(s)4\chi_n(s)^4. On an overlap it defines the residual coefficient to be zero, without evaluating γ2\gamma_2 on a nonsquarefree ideal. Since ∣A∗(s)∣=1|A_*(s)|=1 outside SS, the two extracted scalars give

∣A∗(s)χs(d′)‾χs(h′)∣2=1(s,d′h′)=1=1(s,h′)=1when d′∣C, (s,C)=1.|A_*(s)\overline{\chi_s(d')}\chi_s(h')|^2=1_{(s,d'h')=1}=1_{(s,h')=1}\quad\text{when }d'\mid C,\ (s,C)=1.

The original residual and overlap exclusions also give 1(C,j)=11(s,Cj)=11_{(C,j)=1}1_{(s,Cj)=1}. Thus, apart from the assigned coefficients, individual cutoffs, and unit phases, the outer arithmetic weight is precisely

μ(d′)μ(s)G^(ϑ)Binit(h′)1(C,j)=11(s,Cj)=11(s,h′)=1.\mu(d')\mu(s)\widehat G(\vartheta)\mathcal B_{\rm init}(h') 1_{(C,j)=1}1_{(s,Cj)=1}1_{(s,h')=1}.

All these factors remain through weighted Cauchy. Set

t=C/d′,k=d′h′,f=d′s,ρt,j(n)=1(n,rad⁡(tj))=1.t=C/d',\qquad k=d'h',\qquad f=d's,\qquad\rho_{t,j}(n)=1_{(n,\operatorname{rad}(tj))=1}.

The factors on nn in Equation (17.72), together with ρt,j\rho_{t,j}, supply exactly the original exclusions at C,s,jC,s,j and the numerator zeros at d′,h′d',h'. On the nonzero support t,d′,s,nt,d',s,n are pairwise coprime. Apply Equation (17.16) to each mark with this ordered list. Assigned primes and their priority masks stay outer. A surviving prime is already prime to d′sd's by χn(f)4\chi_n(f)^4 and to tjtj by ρt,j\rho_{t,j}, so its original individual list and coefficient can be retained. Its mark is an original subcollection of z0z_0, not a row- or label-dependent residual coefficient.

The substitutions k=d′h′k=d'h', f=d′sf=d's, and the puncture ρt,j\rho_{t,j} have therefore supplied the canonical character and coefficient class. We still need a common separated profile, the outer multiplicity bound, and admissibility of the resulting ranges.

Keep Binit\mathcal{B}_{\mathrm{init}} outside the common Fourier separation of the full kernel and the old windows. The exact formal child centers and the full fresh-support bounds are

Ncinit=D′−B−v,Vcinit=θ+v,Fcinit=D′−P1,N_c^{\mathrm{init}}=D'-B-v,\qquad V_c^{\mathrm{init}}=\theta+v,\qquad F_c^{\mathrm{init}}=D'-P_1,
∣n^−Ncinit∣≤3η,∣f^−Vcinit∣≤2η.|\widehat{n}-N_c^{\mathrm{init}}|\le3\eta,\qquad|\widehat{f}-V_c^{\mathrm{init}}|\le2\eta.

On factorized terms these bounds follow from c=Csnc=Csn and f=d′sf=d's. The full fresh column cutoff and enlarged label window are also included in ID\mathcal I_D, so the same bounds hold directly for independent terms later added by positivity. The reconstructed formal product c=Csnc=Csn on the fresh cutoff is included there as well, so the initial prefactor bound holds on its entire separated side.

Fix a refinement Σ\Sigma by the ss-dyad and the slot branches, with the earlier mode υ\boldsymbol\upsilon held fixed. Before summing any actual outer ideal, use the six independent coordinates

(xC,xd,xs,xh,x1,x2)=(qCZB,qd′Zθ,qsZv,qh′ZH,qn1ZNcinit,qn2ZNcinit).(x_C,x_d,x_s,x_h,x_1,x_2) =\left(\frac{q_C}{Z^B},\frac{q_{d'}}{Z^\theta}, \frac{q_s}{Z^v},\frac{q_{h'}}{Z^H}, \frac{q_{n_1}}{Z^{N_c^{\rm init}}}, \frac{q_{n_2}}{Z^{N_c^{\rm init}}}\right).

Let IC,Id,Is,IhI_C,I_d,I_s,I_h be the full supports of the four current individual cutoffs. Choose ωn,a\omega_{n,a} equal to one on the support of W0W_0 divided by ICIsI_CI_s, with fixed full supports in an enclosing interval [a,b][a,b] whose upper endpoint satisfies b≥1b\ge1. Choose a nonnegative ωf\omega_f equal to one on IdIsI_dI_s, with fixed full support IfI_f. The current four dyad cutoffs and ωf\omega_f remain outside inversion, and ωn,a\omega_{n,a} remain in the columns. Let Ωinit,α\Omega_{\mathrm{init},\alpha} be larger cutoffs equal to one on the full supports of the corresponding four current and two fresh cutoffs. These full supports, IfI_f, and the formal products CsnCsn on them are the windows already included in ID\mathcal I_D. None of these supports depends on a current outer tuple or on a Fourier mode.

Keep Vcinit≥0V_c^{\mathrm{init}}\ge0. Proceed to a child only if the retained row component is nonzero, which implies Minit≥0M_{\mathrm{init}}\ge0. This is a separate gate from the structural outer set below, which may include zero-weight tuples even when the row ball is empty. Independently, if a full fresh child column window contains no squarefree ideal, its polynomial is zero and that component is omitted. For a retained nonempty child define

Ninit=max⁡(0,Ncinit),δinit=Ninit−Ncinit∈[0,3η],Finit=Ninit+Vcinit=Fcinit+δinit.N_{\mathrm{init}}=\max(0,N_c^{\mathrm{init}}),\qquad\delta_{\mathrm{init}}=N_{\mathrm{init}}-N_c^{\mathrm{init}}\in[0,3\eta],\qquad F_{\mathrm{init}}=N_{\mathrm{init}}+V_c^{\mathrm{init}}=F_c^{\mathrm{init}}+\delta_{\mathrm{init}}.

For a nonempty negative-center window, qn≥1q_n \ge1 and Equation (17.74) give δinit≤3η\delta_{\mathrm{init}} \le3\eta, while its upper support endpoint gives Zδinit≤bZ^{\delta_{\mathrm{init}}} \le b. If Ncinit≥0N_c^{\mathrm{init}} \ge0, then δinit=0\delta_{\mathrm{init}}=0 and the latter inequality follows from b≥1b \ge1. Thus 1≤Zδinit≤b1 \le Z^{\delta_{\mathrm{init}}} \le b in every retained case. The cutoff ωn,a(Zδinity)\omega_{n,a}(Z^{\delta_{\mathrm{init}}}y) is supported in [a/b,b][a/b,b] and has uniformly bounded Euler seminorms. Its rescaling depends only on fixed centers, not on a current row or label, and its full clipping family is included in ID\mathcal{I}_D.

On the formal factorization za=snaz_a=sn_a, the complete root and kernel argument are exactly

Z−D′Zmqd′qsqn1qn2=Zκcinitxd−1xs−1(x1x2)−1/2,Zmqh′qd′qs2qn1qn2=Aker,initxhxdxs2x1x2,Aker,init=Zm+H−θ−2(D′−B).\begin{aligned} \frac{Z^{-D'}Z^m}{q_{d'}q_s\sqrt{q_{n_1}q_{n_2}}} &=Z^{\kappa_c^{\rm init}}x_d^{-1}x_s^{-1}(x_1x_2)^{-1/2},\\ \frac{Z^mq_{h'}}{q_{d'}q_s^2q_{n_1}q_{n_2}} &=A_{{\rm ker},{\rm init}}\frac{x_h}{x_dx_s^2x_1x_2},\\ A_{{\rm ker},{\rm init}}&=Z^{m+H-\theta-2(D'-B)}. \end{aligned}

For the first equality use Ncinit=D′−B−vN_c^{\rm init}=D'-B-v and κcinit=m−2D′+B−θ\kappa_c^{\mathrm{init}}=m-2D'+B-\theta. Equivalently its root is xd−1xC(xc1xc2)−1/2x_d^{-1}x_C(x_{c_1}x_{c_2})^{-1/2} with xca=xCxsxax_{c_a}=x_Cx_sx_a. Define the one joint profile

Hinit,Σ,υ(x)=Z−3η∏αΩinit,α(xα)xd−1xs−1(x1x2)−1/2×W0(xCxsx1)W0(xCxsx2)‾Kinit ⁣(Aker,initxhxdxs2x1x2).\begin{aligned} \mathfrak H_{{\rm init},\Sigma,\boldsymbol\upsilon}(\boldsymbol x) ={}&Z^{-3\eta}\prod_\alpha\Omega_{{\rm init},\alpha}(x_\alpha) x_d^{-1}x_s^{-1}(x_1x_2)^{-1/2}\\ &\times W_0(x_Cx_sx_1)\overline{W_0(x_Cx_sx_2)} \mathcal K_{\rm init}\!\left( A_{{\rm ker},{\rm init}}\frac{x_h}{x_dx_s^2x_1x_2}\right). \end{aligned}

Its outside scalar is exactly Zκcinit+3ηZ^{\kappa_c^{\mathrm{init}}+3\eta}. The old cc-windows are coupled and therefore are in this profile, as are all normalized real inverse roots and the full kernel. No real root is also put in a child test.

For ξ=(ξC,ξd,ξs,ξh,ξ1,ξ2)\boldsymbol{\xi}=(\xi_C,\xi_d,\xi_s,\xi_h,\xi_1,\xi_2), put zn=qn/ZNinitz_n=q_n/Z^{N_{\rm init}}, set again ε1=1,ε2=−1\varepsilon_1=1,\varepsilon_2=-1, and define

Wainit(z)=ωn,a(Zδinitz)zεaiξa.W_a^{\mathrm{init}}(z)=\omega_{n,a}(Z^{\delta_{\mathrm{init}}}z)z^{\varepsilon_a i\xi_a}.

If da′\mathfrak d_a' is the surviving subcollection on side aa, the precise unnormalized child polynomial is

Qa,t,j,ξinit(k,f)=∑n sfA∗(n)ρt,j(n)χn(k)χn(f)4da′(n)Wainit(qn/ZNinit).Q^{\rm init}_{a,t,j,\boldsymbol\xi}(k,f) =\sum_{n\ {\rm sf}}A_*(n)\rho_{t,j}(n) \chi_n(k)\chi_n(f)^4\mathfrak d_a'(n) W_a^{\rm init}(q_n/Z^{N_{\rm init}}).

Its fixed finite character, puncture, product mark, and test are independent of k,fk,f. The two sides can have different tests and subcollections, but both have the same canonical coefficient class.

Let ΩΣ\Omega_\Sigma consist of

ω=(C sf,d′∣C,s sf,h′≠0; assigned slot primes).\omega=(C\ \mathrm{sf},d'\mid C,s\ \mathrm{sf},h'\ne0;\text{ assigned slot primes}).

with the retained individual supports and slot branches. It has no current column index. The functions t,k,ft,k,f are the products defined above; the set may be taken before imposing the displayed outer zero masks, which will be in the weight. Let AΣinit(ω)\mathcal A_\Sigma^{\rm init}(\omega) be the product of all assigned coefficients of d0\mathfrak d_0 and their priority masks, conjugated on side two. The complete remaining outer weight is

VΣinit(ω;ξ)=μ(d′)μ(s)G^(ϑ)Binit(h′)1(C,j)=11(s,Cj)=11(s,h′)=1AΣinit(ω)×ψC(xC)ψd′(xd)ψs(xs)ψh′(xh)ωf(qf/ZVcinit)×xCiξCxdiξdxsiξsxhiξhZiδinit(ξ1+ξ2).\begin{aligned} V_\Sigma^{\rm init}(\omega;\boldsymbol\xi)={}& \mu(d')\mu(s)\widehat G(\vartheta)\mathcal B_{\rm init}(h') 1_{(C,j)=1}1_{(s,Cj)=1}1_{(s,h')=1} \mathcal A_\Sigma^{\rm init}(\omega)\\ &\times\psi_C(x_C)\psi_{d'}(x_d)\psi_s(x_s)\psi_{h'}(x_h) \omega_f(q_f/Z^{V_c^{\rm init}})\\ &\times x_C^{i\xi_C}x_d^{i\xi_d}x_s^{i\xi_s}x_h^{i\xi_h} Z^{i\delta_{\rm init}(\xi_1+\xi_2)}. \end{aligned}

The cutoff ωf\omega_f is one on every original label product, so its insertion is an equality before separation. There is one copy of each Möbius factor and one ray coefficient. In particular the common zero at (s,h′)(s,h') is still present.

Let TΣinit\mathcal{T}_{\Sigma}^{\mathrm{init}} be the fixed ss-dyad and slot summand obtained from Equation (17.71) by the complete Möbius and priority expansions. Its exact separated identity is

TΣinit=Zκcinit+3η(2π)−6∫R6H^init,Σ,υ(ξ)×∑ω∈ΩΣVΣinit(ω;ξ)Q1,t,j,ξinit(k,f)Q2,t,j,ξinit(k,f)‾ dξ.\begin{aligned} \mathcal T_\Sigma^{\rm init}={}& Z^{\kappa_c^{\rm init}+3\eta}(2\pi)^{-6} \int_{\mathbb R^6} \widehat{\mathfrak H}_{{\rm init},\Sigma,\boldsymbol\upsilon} (\boldsymbol\xi)\\ &\quad\times\sum_{\omega\in\Omega_\Sigma} V_\Sigma^{\rm init}(\omega;\boldsymbol\xi) Q^{\rm init}_{1,t,j,\boldsymbol\xi}(k,f) \overline{Q^{\rm init}_{2,t,j,\boldsymbol\xi}(k,f)} \,d\boldsymbol\xi. \end{aligned}

Indeed xa=Zδinitznax_a=Z^{\delta_{\mathrm{init}}}z_{n_a}. The two column modes, with the last factor of Equation (17.78), are exactly x1iξ1x2iξ2x_1^{i\xi_1}x_2^{i\xi_2}, and the other four modes are outer. Fourier inversion restores the full profile; its larger cutoffs are one on the retained supports, and the fresh column cutoffs are one wherever the old W0W_0 windows are nonzero. Equation (17.75) restores the full prefactor and kernel. Equation (17.72) and the priority expansion restore every arithmetic factor term by term. Extra combinations in the full fresh windows cancel through the old windows in this complex identity before Cauchy.

The transform in Equation (17.79) is chosen from the fixed ambient profile before any actual C,d′,s,h′C,d',s,h', and hence before any t,k,ft,k,f, is evaluated. It depends on Σ,Z\Sigma,Z, the fixed tests, and the earlier mode υ\boldsymbol\upsilon, and may depend on the already frozen jj, but not on any current outer ideal or reindexed row or label. The bare h′h' norm is a coordinate; the derived row and label occur only in the outer masks or in the displayed characters. The relation C=td′C=td' only restricts evaluation points. By Equation (17.20), for each fixed JJ there are fixed L,b0L,b_0 such that

∫R6∣H^init,Σ,υ(ξ)∣(1+∣ξ∣)J dξ≪(1+∣υ∣)L,∫R1+∣I0∣∣H^ov,j(υ)∣(1+∣υ∣)L dυ≪pb0(W).\int_{\mathbb R^6} |\widehat{\mathfrak H}_{{\rm init},\Sigma,\boldsymbol\upsilon} (\boldsymbol\xi)|(1+|\boldsymbol\xi|)^J\,d\boldsymbol\xi \ll (1+|\boldsymbol\upsilon|)^L,\qquad \int_{\mathbb R^{1+|I_0|}}|\widehat{\mathfrak H}_{{\rm ov},j}(\boldsymbol\upsilon)| (1+|\boldsymbol\upsilon|)^L\,d\boldsymbol\upsilon \ll p_{b_0}(W).

The first bound uses the fixed normalized roots and the uniform Euler bounds of the full kernel for every positive Aker,initA_{{\rm ker},{\rm init}}; W0W_0 has only polynomial υ\boldsymbol\upsilon-dependence. The second is uniform over the fixed jj-product interval. Taking larger LL if needed also controls the earlier row-space Minkowski inequality. No derivative order introduces a power of ZZ.

Equation (17.79) now expresses the component in polynomials of canonical shape with one common Fourier density chosen before the current outer ideals are evaluated. It remains to bound the positive fibres and source measure, verify child admissibility from source witnesses, and restore the normalization in Lemma 17.1.

Apply Equation (D) on the whole ΩΣ\Omega_{\Sigma}, including all quotients tt, before fixing one for the child. Only afterward take absolute weights. The retained (s,C)=1(s,C)=1 and d′∣Cd'\mid C make f=d′sf=d's squarefree, and all other factors of the weight are bounded by a fixed constant. Thus

∣VΣinit(ω;ξ)∣≪Binit(h′)μ2(f).|V_\Sigma^{\rm init}(\omega;\boldsymbol\xi)| \ll\mathcal B_{\rm init}(h')\mu^2(f).

For fixed t,f,kt,f,k, the identities

d′∣f,s=f/d′,C=td′,h′=k/d′if this quotient is an elementd'\mid f,\qquad s=f/d',\qquad C=td',\qquad h'=k/d' \quad\text{if this quotient is an element}

if this quotient is an element show that the reconstruction has at most dO(f)d_{\mathcal O}(f) choices before slots. Here KslotK_{\mathrm{slot}} again denotes the fixed bound for the original number of slots. The at most 2Kslot2K_{\mathrm{slot}} assigned residual primes divide tftf. Their choices cost at most [dO(t)dO(f)]2Kslot[d_{\mathcal O}(t)d_{\mathcal O}(f)]^{2K_{\rm slot}}. The earlier overlap primes were already frozen and counted in the overlap triangle. Hence the fibre, even if its actual size depends on kk, is bounded by

Dinit(f)Cinit(t),Dinit(f)=dO(f)1+2Kslot,Cinit(t)=dO(t)2Kslot.D_{\rm init}(f)C_{\rm init}(t),\qquad D_{\rm init}(f)=d_{\mathcal O}(f)^{1+2K_{\rm slot}},\qquad C_{\rm init}(t)=d_{\mathcal O}(t)^{2K_{\rm slot}}.

There is no independent d′d', ss count and no second frequency count.

Let ΩΣsrc\Omega_{\Sigma}^{\mathrm{src}} be the structural outer set just used, before independent positive row or label additions and ignoring unit Fourier phases, and define the set of distinct source quotients

TΣ={t=C/d′:ω∈ΩΣsrc}.\mathfrak T_\Sigma=\{t=C/d':\omega\in\Omega_\Sigma^{\rm src}\}.

It is projected once over all current rows and labels, not redefined for a fixed k,fk,f. Every member has a source witness on the C,d′C,d' dyads, and therefore log⁡Zqt=B^−θ^≤P1+2η\log_Z q_t=\widehat{B}-\widehat{\theta}\le P_1+2\eta. The containing norm ball bounds its cardinality by #TΣ≪ZP1+2η+πcount,init\#\mathfrak T_\Sigma\ll Z^{P_1+2\eta+\pi_{{\rm count},{\rm init}}}; it is not used as a replacement child domain. In a nonempty sector P1+2η≥0P_1+2\eta\ge0, since it bounds the norm of an existing ideal. The divisor bound on this bounded range gives the normalized measure

dνΣinit(t)=Z−P1−2η∑t∈TΣCinit(t)δt,∥νΣinit∥≪Zπcount,init+πfib,init.d\nu_\Sigma^{\rm init}(t) =Z^{-P_1-2\eta}\sum_{t\in\mathfrak T_\Sigma}C_{\rm init}(t)\delta_t, \qquad \|\nu_\Sigma^{\rm init}\| \ll Z^{\pi_{{\rm count},{\rm init}}+\pi_{{\rm fib},{\rm init}}}.

This set and measure ignore the unit Fourier phases and are common to the whole current row and label sum. The nonempty gates remain separate from this structural projection.

For a fixed mode let

Ha,tinit=∑f sfqf/ZVcinit∈IfDinit(f)∑k∈O0<qk≤ZMinit∣Qa,t,j,ξinit(k,f)∣2=ZFinitEa,tinit.\mathcal H_{a,t}^{\rm init} =\sum_{\substack{f\ {\rm sf}\\q_f/Z^{V_c^{\rm init}}\in I_f}} D_{\rm init}(f)\sum_{\substack{k\in\mathcal O\\0<q_k\le Z^{M_{\rm init}}}} |Q^{\rm init}_{a,t,j,\boldsymbol\xi}(k,f)|^2 =Z^{F_{\rm init}}\mathcal E_{a,t}^{\rm init}.

This is Equation (17.3) with the same row ball; with a larger fixed canonical ball the equality is replaced by the corresponding upper bound. The fibre estimate and weighted Cauchy give

∣∑ω∈ΩΣVΣinitQ1Q2‾∣≪ZP1+2η∏a=12(∫TΣHa,tinit dνΣinit(t))1/2.\left|\sum_{\omega\in\Omega_\Sigma}V_\Sigma^{\rm init}Q_1\overline{Q_2}\right| \ll Z^{P_1+2\eta} \prod_{a=1}^2 \left(\int_{\mathfrak T_\Sigma}\mathcal H_{a,t}^{\rm init} \,d\nu_\Sigma^{\rm init}(t)\right)^{1/2}.

Here Qa=Qa,t,j,ξinit(k,f)Q_a=Q^{\rm init}_{a,t,j,\boldsymbol\xi}(k,f). Only the positive outer f,kf,k sums were enlarged to their full fixed windows; the inner ρt,j\rho_{t,j}, mark, and fresh test are unchanged. The weight DinitD_{\mathrm{init}} depends on ff alone. The new outer ball is exactly 10<qk≤ZMinit1_{0<q_k\le Z^{M_{\mathrm{init}}}}. Thus use of the uniform child bound introduces the displayed quotient-count exponent once and the normalized mass once.

The fixed puncture is exactly at rad⁡(tj)\operatorname{rad}(tj). For each t∈TΣt\in\mathfrak T_\Sigma, its source bound and the fixed overlap bound give

Qinit:=log⁡Zqrρ≤B^−θ^+j^≤P1+G+3η.Q_{\rm init}:=\log_Zq_{\mathfrak r_\rho} \le\widehat B-\widehat\theta+\widehat j\le P_1+G+3\eta.

Shared puncture primes only decrease this bound. It continues to hold when positive new labels or rows are added, because those additions do not change t,jt,j or delete their inner puncture.

The fixed formal centers satisfy

Fcinit−Mcinit−(P1+G)−z0=m−r−2z+2G,F_c^{\mathrm{init}}-M_c^{\mathrm{init}}-(P_1+G)-z_0=m-r-2z+2G,
4Fcinit−3Mcinit−6z0=3m−2r−8z+10G+2P1.4F_c^{\mathrm{init}}-3M_c^{\mathrm{init}}-6z_0=3m-2r-8z+10G+2P_1.

Use the marked premises, G≥0G\ge0, P1≥−2ηP_1\ge-2\eta, Equations (17.69) and (17.84), and the favorable clipping signs. The actual canonical margins are

Finit−Minit−Qinit−z0≥c1+δinit−9η−τinit≥c1−9η−τinit,4Finit−3Minit−6z0≥c2+4δinit−22η−3τinit≥c2−22η−3τinit.\begin{aligned} F_{\mathrm{init}}-M_{\mathrm{init}}-Q_{\mathrm{init}}-z_0&\ge c_1+\delta_{\mathrm{init}}-9\eta-\tau_{\mathrm{init}}\ge c_1-9\eta-\tau_{\mathrm{init}},\\ 4F_{\mathrm{init}}-3M_{\mathrm{init}}-6z_0&\ge c_2+4\delta_{\mathrm{init}}-22\eta-3\tau_{\mathrm{init}}\ge c_2-22\eta-3\tau_{\mathrm{init}}. \end{aligned}

The 22η22\eta is 4η4\eta from the possible negative 2P12P_1 and 18η18\eta from three copies of the row enclosure.

There is also an explicit energy calculation. Apply the canonical bound only for t∈TΣt\in\mathfrak T_\Sigma, where the preceding puncture and margin checks hold. Equations (17.82) and (17.83) then bound the unscaled signed outer sum by

C(υ,ξ)ZP1+2η+2Finit+ϵc∥νΣinit∥.C(\boldsymbol\upsilon,\boldsymbol\xi) Z^{P_1+2\eta+2F_{\rm init}+\epsilon_c} \|\nu_\Sigma^{\rm init}\|.

The one mass is that of Equation (17.81); the label d′sd'ss remains inside the child average. The common Fourier density is integrated separately, once, with the uniform weighted bounds above.

This counts the distinct frozen quotient once, with its witness multiplicity already in the fibre weights. The formal identity

κcinit+P1+2Fcinit=m\kappa_c^{\mathrm{init}} + P_1 + 2F_c^{\mathrm{init}} = m

then gives, after restoring the child normalization and applying the canonical bound with loss ϵc\epsilon_c, the per-side exponent

m+3η+2η+2δinit+πinit+ϵc≤m+11η+πinit+ϵc.m + 3\eta+ 2\eta+ 2\delta_{\mathrm{init}} + \pi_{\mathrm{init}} + \epsilon_c \le m + 11\eta+ \pi_{\mathrm{init}} + \epsilon_c.

Here πinit\pi_{\mathrm{init}} is the aggregate freely chosen local divisor, dyadic, and separation loss, including the assigned-overlap divisor loss and the distinct allocations πcount,init\pi_{{\rm count},{\rm init}}, πfib,init\pi_{{\rm fib},{\rm init}}. These are parts of one aggregate, not repeated allowances. The two clipping copies come from the restored normalization and the child exponent. There is no τinit\tau_{\mathrm{init}} energy factor: the row enlargement occurs inside the canonical child and was accounted for in its margin test. The initial weighted Cauchy takes a geometric mean, and the overlap triangle was already canceled by Z−GZ^{-G}.

We give the parameter and tail order explicitly. Let rmax⁡r_{\max}, zmax⁡z_{\max}, mmax⁡m_{\max} bound the marked ranges, let sslots_{\mathrm{slot}} bound the number of slots, and put Dmax⁡=rmax⁡+zmax⁡D_{\max}=r_{\max}+z_{\max}. Set cˉ=min⁡(c1,c2)\bar{c}=\min(c_1,c_2) and choose the canonical margin c∗=cˉ/2c_*=\bar{c}/2. For η,τinit≤1/100\eta,\tau_{\mathrm{init}}\le1/100, valid a priori starting bounds for that application are

Mmax⁡=2Dmax⁡+1,Nmax⁡=Vmax⁡=Dmax⁡+1.M_{\max}=2D_{\max}+1,\qquad N_{\max}=V_{\max}=D_{\max}+1.

Indeed, P1≥−2ηP_1\ge-2\eta gives Minit≤2Dmax⁡+10η+τinitM_{\mathrm{init}}\le2D_{\max}+10\eta+\tau_{\mathrm{init}}, and Finit≤Dmax⁡+5ηF_{\mathrm{init}}\le D_{\max}+5\eta bounds both nonnegative child parameters. Make the choices in Equation (17.66) with ϵc=ϵ/2\epsilon_c=\epsilon/2, imposing in addition

η,τinit≤cˉ/100,η≤ϵ/88,πinit≤ϵ/8.\eta,\tau_{\mathrm{init}}\le\bar{c}/100,\qquad\eta\le\epsilon/88,\qquad\pi_{\mathrm{init}}\le\epsilon/8.

One may take τinit=τ\tau_{\mathrm{init}}=\tau after imposing both sets of bounds. Equation (17.85) then gives both margins at least 3cˉ/4>c∗3\bar{c}/4>c_*, so Lemma 17.2 applies. Equation (17.86) adds at most ϵ/4\epsilon/4 to its ϵc=ϵ/2\epsilon_c=\epsilon/2 loss.

With these bounded initial ranges fixed, choose the subsidiary input exponents realizing the target πinit\pi_{\mathrm{init}}, before choosing the initial tail and Fourier-height orders.

For the separate initial raw tail, the supported columns satisfy qci≤CZDmax⁡q_{c_i}\le CZ^{D_{\max}}, while D′∈[−zmax⁡,Dmax⁡]D'\in[-z_{\max},D_{\max}]. On the genuine initial expansion put a=Zm/(qd′qz1z2)a=Z^m/(q_{d'}q_{z_1z_2}). Since m≥0m\ge0, d′∣Cd'\mid C, and ci=Czic_i=Cz_i,

a−1≤qd′qz1z2≤qc1qc2/qC≤CZ2Dmax⁡.a^{-1}\le q_{d'}q_{z_1z_2} \le q_{c_1}q_{c_2}/q_C\le C Z^{2D_{\max}}.

The explicit crude exponent

Bcrude,init=10{1+mmax⁡+(sslot+1)(Dmax⁡+1)}B_{\rm crude,init}=10\{1+m_{\max}+(s_{\rm slot}+1)(D_{\max}+1)\}

bounds all raw nonfrequency factors even without cancellation. To verify this, the normalization costs at most zmax⁡z_{\max}, the two column counts cost 2Dmax⁡2D_{\max}, the d′d'-divisor count at most Dmax⁡D_{\max}, and 1+a−11+a^{-1} at most 2Dmax⁡2D_{\max}. The two residual marks cost at most 2sslotDmax⁡2s_{\mathrm{slot}}D_{\max}, using dO(c)sslot≤qcsslotd_{\mathcal O}(c)^{s_{\rm slot}}\le q_c^{s_{\rm slot}}. Even counting overlap pairs and their assigned coefficients without their canceling weights costs at most 2zmax⁡+2sslotzmax⁡2z_{\max}+2s_{\mathrm{slot}}z_{\max}. The Poisson prefactor costs at most mmax⁡m_{\max}. The sum is at most mmax⁡+(8+4sslot)Dmax⁡<Bcrude,initm_{\max}+(8+4s_{\rm slot})D_{\max}<B_{\rm crude,init}.

Choose Tinit>1+Bcrude,initT_{\rm init}>1+B_{\rm crude,init} and then

Ainit>1+(Bcrude,init+Tinit)/τinit.A_{\rm init}>1+(B_{\rm crude,init}+T_{\rm init})/\tau_{\rm init}.

Equation (17.21) makes the raw Binit=0\mathcal{B}_{\mathrm{init}}=0 complement O(Z−Tinit)O(Z^{-T_{\mathrm{init}}}), with fixed seminorm and polynomial-height factors. This order is chosen after the marked ranges and τinit\tau_{\mathrm{init}}, but before the initial Fourier-height orders and before the final ZZ threshold. If τinit=τ\tau_{\mathrm{init}}=\tau, take the maximum of the orders required by this separate crude bound and the canonical tails. The full kernel retained inside the outer ball has the uniform Euler bounds already used in the canonical separation. The final threshold also enforces the full initial support ratios in ID\mathcal I_D. The principal count has exponent mm, and every nonprincipal term has now been bounded by Zm+ϵZ^{m+\epsilon}. The argument keeps all element rows and every original mask, applies to subcollections and either common orientation, and preserves arbitrary bounded row-independent prime coefficients. The common separated measures give the stated finite-seminorm and polynomial-height uniformity. This proves Equation (17.1).

Amplification on sixth-power-free rows

We first extract an unmarked consequence on all element rows. In Lemma 17.1, take Z=HZ=H, m=1m=1, no slots, and r=log⁡HDr=\log_H D. If H≥D1+cH\geq D^{1+c} for a fixed c>0c>0, then 1−r≥c/(1+c)1-r\geq c/(1+c); the second required margin is also positive. For D≤Hϵ/4D\leq H^{\epsilon/4}, the direct bound ∣Mu(D;W)∣2≪D|M_u(D;W)|^2\ll D suffices. Otherwise the starting lengths are in a fixed bounded range away from zero. Bounded H,DH,D are handled directly. We obtain, for H,D≥1H,D\geq1,

∑u∈O0<qu≤H∣D−1/2∑nμ(n)ν(n)χn(u)εχW(qn/D)∣2≪c,ϵ,WH(HD)ϵ,H≥D1+c.\sum_{\substack{u\in\mathcal O\\0<q_u\le H}} \left|D^{-1/2}\sum_n\mu(n)\nu(n)\chi_n(u)^{\varepsilon_\chi} W(q_n/D)\right|^2 \ll_{c,\epsilon,W} H(HD)^\epsilon,\qquad H\ge D^{1+c}.

The fixed arithmetic data and the stated seminorms are included in the dependence of the constant.

Lemma 17.6 (Sixth-power amplification). Let ν\nu, WW, ϵχ\epsilon_\chi and the zero extensions be as in Lemma 17.1, with no prime slots. Let U,D≥1U,D\geq1, and sum over elements uu with qu≍Uq_u\asymp U such that every prime valuation of the ideal (u)(u) is at most five. For every fixed c>0c>0 and ϵ>0\epsilon>0, put

H=max⁡(2U,D1+c),P=(H/U)1/6.H=\max(2U,D^{1+c}),\qquad P=(H/U)^{1/6}.

Then

∑u∣Mu(D;W)∣2≪HP(UD)ϵ≪max⁡{U,U1/6D5(1+c)/6}(UD)ϵ.\sum_u|M_u(D;W)|^2\ll\frac{H}{P}(UD)^\epsilon\ll\max\{U,U^{1/6}D^{5(1+c)/6}\}(UD)^\epsilon.

The implied constant depends only on c,ϵc,\epsilon, the fixed arithmetic data, and finitely many seminorms of WW. In particular, for D=UrD=U^r with rr in a fixed bounded nonnegative range, for every ϵ>0\epsilon>0 the exponent may be written

∑u∣Mu(Ur;W)∣2≪Ue(r)+ϵ,e(r)=max⁡{1,(1+5r)/6}.\sum_u|M_u(U^r;W)|^2\ll U^{e(r)+\epsilon},\qquad e(r)=\max\{1,(1+5r)/6\}.

Both assertions permit a separate test Wσu,tu(y)=W(y)y−σu+ituW_{\sigma_u,t_u}(y)=W(y)y^{-\sigma_u+it_u} in each row, with σu\sigma_u in a fixed compact interval and ∣tu∣≤T1|t_u|\leq T_1, at a cost (1+T1)A(1+T_1)^A for a fixed AA.

Proof. First, Equation (17.87) and Lemma 4.5 imply the rowwise scale bound

∑v∈O0<qv≤CHsup⁡0<D′≤D∣Mv(D′;W)∣2≪H(HD)ϵ,H≥max⁡(2,D1+c).\sum_{\substack{v\in\mathcal O\\0<q_v\leq CH}}\sup_{0<D'\leq D}|M_v(D';W)|^2\ll H(HD)^\epsilon,\qquad H\geq\max(2,D^{1+c}).

Indeed, sufficiently small scales have no ideals in the annular support. Differentiation with respect to log⁡D′\log D' replaces W(y)W(y) by −W(y)/2−yW′(y)-W(y)/2-yW'(y). The one-dimensional Sobolev inequality in Lemma 4.5, followed by Equation (17.87) for these two tests, controls the supremum on a unit logarithmic interval. There are O(log⁡(2+D))O(\log(2+D)) such intervals. A fixed enlargement of HH handles their endpoints, and the direct small-scale bound handles the initial intervals. This proves Equation (17.89).

Ideal counting outside the fixed set SS gives at least cSPc_S P primary ideals aa with qa≤Pq_a \le P, for a fixed cS>0c_S > 0. For bounded PP this follows after reducing cSc_S, since the unit ideal is available; for large PP it follows from the positive-density ideal count with finitely many primes removed.

For squarefree nn, separate the primes dividing aa by n=dmn = dm, where d∣rad⁡ad \mid\operatorname{rad} a and (m,a)=1(m,a) = 1. With the zero extensions,

ψua6(m)=ψu(m)1(m,a)=1.\psi_{ua^6}(m)=\psi_u(m)1_{(m,a)=1}.

This is true also when u,au,a share primes: both sides vanish at a prime dividing mm and either uu or aa, and otherwise the sixth power is one. The separated column therefore gives the exact identity

Mu(D;W)=∑d∣rad⁡aμ(d)ψu(d)qd−1/2Mua6(D/qd;W).M_u(D;W) = \sum_{d\mid\operatorname{rad} a}\mu(d)\psi_u(d)q_d^{-1/2}M_{ua^6}(D/q_d;W).

The coefficient mass is at most dO(a)≪δPδd_{\mathcal O}(a)\ll_\delta P^\delta. It follows that

∣Mu(D;W)∣2≪δP2δsup⁡0<D′≤D∣Mua6(D′;W)∣2.|M_u(D;W)|^2 \ll_\delta P^{2\delta}\sup_{0<D'\le D}|M_{ua^6}(D';W)|^2.

Average this bound over the aa's and sum over uu. The map (u,a)↦ua6(u,a)\mapsto ua^6 is injective on these pairs. In fact, at each prime the valuation modulo six recovers the valuation of the sixth-power-free ideal (u)(u), and its quotient by six recovers the valuation of aa. The primary generator of aa then fixes the element uu, including its unit. This argument does not require (u,a)=1(u,a)=1. Also qua6≪UP6≪Hq_{ua^6}\ll UP^6\ll H. Thus Equation (17.89) gives

∑u∣Mu(D;W)∣2≪HP(UD)ϵ=U1/6H5/6(UD)ϵ,\sum_u |M_u(D;W)|^2 \ll\frac{H}{P}(UD)^\epsilon= U^{1/6}H^{5/6}(UD)^\epsilon,

after choosing the preliminary δ\delta and power losses small enough. Since H=max⁡(2U,D1+c)H=\max(2U,D^{1+c}), this is Equation (17.88). For bounded rr, choose c>0c>0 sufficiently small in terms of rr's bound and the desired power loss; the stated formula for e(r)e(r) follows.

Finally, on the fixed annular support, derivatives in σ,t\sigma,t of Wσ,tW_{\sigma,t} insert bounded powers of log⁡y\log y. Apply the parameter Sobolev inequality in Lemma 4.5 on a bounded cover in σ\sigma and O(1+T1)O(1+T_1) unit intervals in tt, summing the row moments before integrating the derivatives. The finite-seminorm bound already proved has fixed polynomial height order. The cover and these derivatives therefore give a factor (1+T1)A(1+T_1)^A for a fixed AA, uniformly for a separate (σu,tu)(\sigma_u,t_u) in every row. The same reasoning applies to the marked estimate with any fixed finite number of test parameters, while its prime coefficients remain fixed across rows.

In the later application, the positive exponent in T1=ZτηT_1=Z^{\tau_\eta} is chosen after the fixed order AA. It may therefore be chosen small enough to fit the reserved power loss. This use of rowwise test parameters does not permit arbitrary row-dependent prime coefficients.

Fourth moments with short prime factors

The refined row count requires a fourth-moment estimate for two plain character polynomials and a product of short prime polynomials. We prove that estimate here. The two plain polynomials have no length restriction when no prime polynomial is present; otherwise the permitted lengths lie in an affine region. Two finite Fourier transforms return products of the same kind at a smaller effective width. Some transformed rows, however, induce characters in a fixed finite family. Their plain products can have volume-sized main terms. For the longer inputs we therefore subtract a comparison product with the same product of scales. Preserving its common character, mask, and norm power through the transforms makes those main terms cancel. The estimate itself concerns the original, uncentered product.

We use the notation of Section 4 and the coefficient conventions of Section 13. In particular, the rows are elements k∈Ok \in\mathcal{O} with 0<qk≪Zm0 < q_k \ll Z^m, and

ψk(n)=τ(n)χn(k),M=m+q.\psi_k(n) = \tau(n)\chi_n(k), \qquad M = m + q.

The character τ\tau is fixed within a row sum. The union of the prime supports of all its displayed moving residue-symbol factors, before canceling factors or reducing exponents modulo six, has norm at most ZqZ^q. Every displayed factor retains its zero extension, including a canceled or six-divisible factor. A redundant zero may instead be represented by an additional puncture mask only when an exact factorization retains every surviving local and fixed-ray phase. This mask is the indicator of coprimality to one squarefree ideal of norm at most ZBZ^B, for a bounded BB, fixed within the current row sum; the same mask is used in both plain factors and in every prime factor. It may depend on previously frozen labels, but not on the varying row. All ideals in the polynomials are outside the fixed set S\mathcal S.

Fix a finite group Θ\Theta of finite-order ray characters whose conductor primes belong to S\mathcal S. It contains the fixed twists and all characters used to separate the fixed reciprocity phases. Thus it also contains the supplementary character n↦χn(−1)n \mapsto\chi_n(-1): by (4.6) and the fixed bicharacter table, this character is the diagonal character n↦R(n,n)n \mapsto\mathcal{R}(n,n). Membership of an inducing character in Θ\Theta means equality with the primitive inducing character of some member of Θ\Theta, not equality of the chosen zero-extended presentations. All zeros of those presentations remain in the polynomials. Let R0\mathcal{R}_0 be the rows for which ψk\psi_k induces a nonprincipal character. For z>0z > 0, let Rz\mathcal{R}_z be the rows for which the inducing character of ψk\psi_k does not belong to Θ\Theta. Write

A=n1+n2+z.A = n_1 + n_2 + z.

Lemma 18.1 (Fourth moment with short prime factors). Let 3/4≤κ≤13/4 \le\kappa\le1. Let n1,n2≥0n_1,n_2 \ge0, and let Q=∏i∈IQψk,iQ=\prod_{i\in\mathcal I}Q_{\psi_k,i} be a finite product of the prime polynomials in Equation (13.1), of lengths zi≥0z_i \ge0 and total length z=∑i∈Iziz=\sum_{i\in\mathcal I}z_i. Their underlying prime supports are pairwise disjoint before common masks and row zero extensions are imposed. Their coefficients are fixed finite linear combinations of finite-ray characters. For every positive-length slot the expansion has the form

νi(n)=∑j=1Jicijϑij(n),ϑij∈Θ,\nu_i(n) = \sum_{j=1}^{J_i} c_{ij}\vartheta_{ij}(n), \qquad\vartheta_{ij} \in\Theta,

where the finite list and its coefficients are fixed independently of ZZ and of the row. The row and mask hypotheses are those just stated.

For every ϵ>0\epsilon> 0, there is a slot mesh η>0\eta> 0 such that, if zi≤ηz_i \le\eta for every ii, then

∑k∈Rz∣Sψk(n1;W1)Sψk(n2;W2)Q∣2≪ZM+ϵ\sum_{k\in\mathcal{R}_z} \left|S_{\psi_k}(n_1;W_1)S_{\psi_k}(n_2;W_2)Q\right|^2 \ll Z^{M+\epsilon}

in either of the following cases:

  1. z=0z = 0. There is no restriction on the bounded nonnegative lengths n1,n2n_1,n_2, and no lower bound on the conductor.

  1. z>0z > 0 and

n1+n2+6κz=A+(6κ−1)z≤M.n_1+n_2+6\kappa z = A + (6\kappa-1)z \le M.

If κ<1\kappa< 1, assume in addition that β∗≤(1+κ)/2\beta_* \le(1+\kappa)/2. If κ=1\kappa= 1, no zero-free hypothesis is required.

For an empty slot list, Q=1Q = 1. If z=0z = 0 and the list contains zero-length slots, their scales are bounded and absolute counting absorbs them into the constant; the zero-slot assertion therefore has the same strength. All real length parameters range over prescribed bounded sets. The mesh depends only on those sets and ϵ\epsilon, uniformly for κ∈[3/4,1]\kappa\in[3/4,1]. For each fixed ZZ-independent arithmetic datum A\mathcal A and fixed slot count, the bound uses finitely many smooth seminorms and a fixed polynomial in the separated norm-twist heights. Their orders, and the bound itself, are uniform over all moving moduli, admissible masks, and frozen outer labels in the stated ranges.

The application to the 7/87/8 bound sets κ=2β∗−1\kappa= 2\beta_* - 1, so its zero-free hypothesis in this lemma holds by equality. We retain this dynamic value rather than replace it by the value 5/65/6 supplied by the 11/1211/12 bound, since the refined row count uses the resulting affine capacity. The proof below uses the finite Gauss identities of Section 13.3, Lemma 4.5, and Lemma 4.9. Absorb any zero-length slots by absolute counting at their bounded scales; henceforth z=0z = 0 means that no live slot remains. We first make two reductions that preserve the row family.

The later induction is on the effective width M=m+qM = m + q, with all zero-slot bands completed before the positive-slot bands. Within each band the range A≤5M/6A \le5M/6 is proved first. This threshold comes from the transformed rows whose inducing characters lie in Θ\Theta: counting their sixth-power form and bounding their plain products by volume leaves an excess A−5M/6A - 5M/6, before the common-support savings. Reflection handles some longer inputs; the others are reduced to an equal-product-scale difference, whose cancellation removes that excess.

Fixed masks and reflection

Call a character natural when its zeros consist exactly of its primitive conductor primes, its redundant row and declared moving radical primes, and the fixed primes in S\mathcal S. Here a redundant prime is one at which the inducing character is unramified but the displayed zero-extended product still vanishes. A displayed six-divisible power still vanishes on nonunits. If a redundant factor of the fixed twist is not included in the declared moving radical, first factor it exactly into its remaining phase and a coprimality indicator, and put that indicator in a squarefree ideal R\mathfrak R, with qR≤ZBq_{\mathfrak R} \le Z^B, fixed throughout the row sum. In particular, a cancellation between the fixed twist and the varying factor χn(k)\chi_n(k) is not reclassified as a separately chosen extra puncture for each row.

Let ψk0\psi_k^0 be the natural character obtained by deleting these additional punctures, and let Tk(X)T_k(X) denote its centrally normalized plain sum at scale XX. Write Sk,R(X)S_{k,\mathfrak R}(X) for the sum with the extra mask. Multiplicativity, including zero extensions, gives the exact identities

Sk,R(X)=∑d∣Rμ(d)ψk0(d)qd−1/2Tk(X/qd),S_{k,\mathfrak R}(X) = \sum_{d\mid\mathfrak R} \mu(d)\psi_k^0(d)q_d^{-1/2}T_k(X/q_d),
Qk,i,R=Qk,i 0−Pi−1/2∑p∣Rp primeψk0(p)νi(p)Wislot(qp/Pi),Pi=Zzi.Q_{k,i,\mathfrak R} =Q_{k,i}^{\,0} -P_i^{-1/2}\sum_{\substack{p\mid\mathfrak R\\p\ {\rm prime}}} \psi_k^0(p)\nu_i(p)W_i^{\rm slot}(q_p/P_i), \qquad P_i=Z^{z_i}.

For example, the first identity follows by inserting ∑d∣(n,R)μ(d)\sum_{d\mid(n,\mathfrak R)}\mu(d) and writing n=dln = dl. The quotient ll is unrestricted at primes of dd; the original natural zero extension remains on it.

Apply these identities simultaneously to both plain factors and all slots. If the frozen slots form J⊆IJ\subseteq\mathcal I, and the plain divisors are d1,d2d_1,d_2, the scalar depending on the row has modulus at most one. The remaining coefficient has absolute value at most a fixed profile constant times

qd1d2−1/2∏i∈JPi−1/2.q_{d_1d_2}^{-1/2}\prod_{i\in J}P_i^{-1/2}.

The resulting natural product has lengths

A′=A−log⁡Zqd1d2−∑i∈Jzi,z′=z−∑i∈Jzi.A' = A - \log_Z q_{d_1d_2} - \sum_{i\in J}z_i, \qquad z' = z - \sum_{i\in J}z_i.

Its inducing character is unchanged. If z′>0z' > 0, the left side of Equation (18.3) has decreased; if z′=0z' = 0, the zero-slot assertion has no length restriction and Rz⊆R0\mathcal{R}_z \subseteq\mathcal{R}_0.

For every fixed ϵ1>0\epsilon_1 > 0,

∑d∣Rqd−1/2≤∏p∣R(1−qp−1/2)−1≪ϵ1,BZϵ1.\sum_{d \mid\mathfrak{R}} q_d^{-1/2} \le\prod_{p \mid\mathfrak{R}} (1-q_p^{-1/2})^{-1} \ll_{\epsilon_1,B} Z^{\epsilon_1}.

This follows from Lemma 4.10. The corresponding mass for a frozen slot is also Zϵ1Z^{\epsilon_1}: on its annular support, Pi−1/2≪qp−1/2P_i^{-1/2} \ll q_p^{-1/2}, and the same product bounds the sum over p∣Rp \mid\mathfrak{R}. The number of slots is fixed. Minkowski’s inequality therefore reduces Equation (18.2) to the natural assertion at the same width, with an arbitrarily small power loss. A nonempty annular scale below one is bounded below by a positive profile-dependent constant and may be rescaled to one. After this rescaling its new nonnegative length is max⁡{ni−log⁡Zqdi,0}≤ni\max\{n_i-\log_Z q_{d_i},0\} \le n_i, so the asserted nonincrease of the affine expression remains valid.

We next record precisely the reflection used for natural characters. Let ψk∗\psi_k^* be the primitive character inducing ψk0\psi_k^0, and let R0,k\mathfrak{R}_{0,k} be its redundant natural radical. The primes of R0,k\mathfrak{R}_{0,k} are disjoint from the primitive conductor. If QkQ_k is that conductor norm, set Ck=3Qk/(2π)2C_k=3Q_k/(2\pi)^2, the conductor scale in the functional equation. Tameness at primes outside S\mathcal{S} gives

CkqR0,k≪S,τfixedZM.C_k q_{\mathfrak{R}_{0,k}} \ll_{\mathcal{S},\tau_{\mathrm{fixed}}} Z^M.

Indeed, each good prime contributes at most once, either to the primitive conductor or to the redundant radical. Their union is contained in the union of the row radical and the declared moving radical, whose norm is at most qkZqq_k Z^q. By Lemma 4.1, the unit and S\mathcal{S}-supported parts of a row, with valuations reduced modulo six when evaluated on primary elements prime to S\mathcal{S}, range over a fixed finite ray family. Thus all primes in S\mathcal{S} contribute only a fixed factor.

Apply the primitive Hecke functional equation recorded in the proof of Lemma 4.8 to ψk∗\psi_k^*, using the entireness of L(s,ψk∗)L(s,\psi_k^*) stated there. Let ϵk\epsilon_k be its root number, so ∣ϵk∣=1|\epsilon_k|=1. Mellin inversion and a contour shift show that the normalized plain sum of ψk∗\psi_k^* at XX equals the root number times the conjugate character sum at Ck/XC_k/X, with transformed profile W♯W^\sharp defined by

MW♯(s)=MW(1−s)Γ(s)Γ(1−s).\mathcal{M}W^\sharp(s)=\mathcal{M}W(1-s)\frac{\Gamma(s)}{\Gamma(1-s)}.

The Mellin transform convention is the one in Lemma 4.5. The quotient of gamma functions has poles only at the nonpositive integers and zeros at the positive integers. Shifting the inverse Mellin contour to the left gives an expansion in nonnegative integral powers at zero; shifting it to the right gives arbitrary decay at infinity. Thus W♯W^\sharp and its Euler derivatives are bounded at zero and rapidly decreasing at infinity. The height assertion is also quantitative. For Wω(y)=W(y)yiωW_\omega(y)=W(y)y^{i\omega}, the exact identity MWω(s)=MW(s+iω)\mathcal{M}W_\omega(s)=\mathcal{M}W(s+i\omega) puts all height dependence in a translate of the rapidly decreasing Mellin transform. On each fixed vertical line the gamma quotient and each fixed number of Euler derivatives have polynomial growth in the integration height. Integrating the translated Mellin decay therefore gives a fixed polynomial in 1+∣ω∣1+|\omega|, with its degree depending only on the fixed contour and derivative orders. The pointwise Mellin integration-by-parts estimate on a compact real strip in Lemma 4.5 justifies the horizontal joins in these shifts; an integrated Fourier tail is not used to bound a fixed horizontal trace. This proves the required finite-seminorm and polynomial-height bounds for reflection.

Deleting the redundant Euler factors before reflection and restoring them geometrically afterward gives

Tk(X;W)=ϵk∑d0∣R0,krad⁡(h0)∣R0,kμ(d0)ψk∗(d0)ψk∗(h0)‾qd0qh0Tψk0‾(Ckqd0Xqh0;W♯),∣ϵk∣=1.T_k(X;W)=\epsilon_k\sum_{\substack{d_0\mid\mathfrak{R}_{0,k}\\ \operatorname{rad}(h_0)\mid\mathfrak{R}_{0,k}}} \frac{\mu(d_0)\psi_k^*(d_0)\overline{\psi_k^*(h_0)}}{\sqrt{q_{d_0}q_{h_0}}} T_{\overline{\psi_k^0}}\left(\frac{C_kq_{d_0}}{Xq_{h_0}};W^\sharp\right), \qquad|\epsilon_k|=1.

The geometric series is absolutely bounded by ∏p∣R0,k(1−qp−1/2)−1\prod_{p\mid\mathfrak{R}_{0,k}}(1-q_p^{-1/2})^{-1}. Consequently its total coefficient mass, together with the d0d_0 sum, is Zϵ1Z^{\epsilon_1}. The scales are

Y=Ckqd0Xqh0,d0∣R0,k,rad⁡(h0)∣R0,k.Y=\frac{C_kq_{d_0}}{Xq_{h_0}},\qquad d_0\mid\mathfrak{R}_{0,k},\quad\operatorname{rad}(h_0)\mid\mathfrak{R}_{0,k}.

By Equation (18.7), there is a fixed CA≥1C_{\mathcal A}\ge1 such that

CkqR0,k≤CAZM,Y≤CAZM−log⁡ZX.C_kq_{\mathfrak R_{0,k}}\le C_{\mathcal A}Z^M,\qquad Y\le C_{\mathcal A}Z^{M-\log_ZX}.

The profile W♯W^\sharp can be partitioned into smooth annuli. Below its main scale, central normalization gives summable coefficients O(2−j/2)O(2^{-j/2}) on the annuli of relative scale 2−j2^{-j}. Above that scale, rapid decay gives an arbitrary summable power. Fix a small length tolerance ξ>0\xi> 0. Truncate the upper annuli after an enlargement Zξ/2Z^{\xi/2}; sufficiently many fixed derivatives make the omitted part negligible by absolute counting. A main scale below Z−ξZ^{-\xi} is likewise negligible. If a retained annular profile has fixed upper support endpoint BB, a scale SS that can contain a nonzero integral ideal satisfies SB≥1SB \ge1. On such a scale,

max⁡(S,1)≤max⁡(1,B)S.\max(S,1) \le\max(1,B)S.

Thus replacing a retained subunit scale by scale one costs this fixed multiplicative factor. All these assertions are uniform in the moving labels.

The row-dependent choices d0,h0d_0,h_0 are handled by their coefficient mass followed by a rowwise supremum in the resulting scales. Lemma 4.5 bounds a supremum over two polynomial-range scales using O((log⁡Z)2)O((\log Z)^2) unit boxes and derivatives of the profiles. The row character and its natural zeros remain unchanged: after reflection, conjugating that whole factor inside its absolute value replaces the conjugate character by the original character and conjugates its profile. This operation is valid because the absolute value of a product is unchanged by conjugating one factor.

Let Cref≥1C_{\mathrm{ref}} \ge1 include CAC_{\mathcal A}, the fixed annular endpoint multipliers, the logarithmic box multipliers for a reflected factor and any paired unreflected factor, and max⁡(1,B)\max(1,B) for the retained profile types. This constant is fixed after the data and profile types, independently of ZZ and the moving labels. For n=log⁡ZXn=\log_Z X, every retained scale satisfying the preceding support test, after the permitted clipping and box enlargement, has declared nonnegative length

nref≤M−n+ξ2+log⁡Creflog⁡Z≤M−n+ξ(log⁡Creflog⁡Z≤ξ2).n_{\mathrm{ref}} \le M-n+\frac{\xi}{2}+\frac{\log C_{\mathrm{ref}}}{\log Z} \le M-n+\xi \qquad \left(\frac{\log C_{\mathrm{ref}}}{\log Z}\le\frac{\xi}{2}\right).

This is a linear bound also when M−nM-n is slightly negative; if its right side is negative, no such retained scale exists. The smaller upper-annulus range changes only the fixed decay, seminorm, and height orders used for the discarded tail.

For z=0z=0, reflect each original factor whose length exceeds M/2M/2 once, and leave the other factor unchanged. Equation (18.9) bounds every retained reflected factor; the fixed box multiplier for an unreflected factor is included in CrefC_{\mathrm{ref}}. After the preceding annular truncation and scale-box enlargement, the resulting lengths satisfy

ni∗≤M/2+ξ,A∗=n1∗+n2∗≤M+2ξ≤M+δ,n_i^* \le M/2+\xi,\qquad A^*=n_1^*+n_2^* \le M+2\xi\le M+\delta,

provided 2ξ≤δ2\xi\le\delta. We call this the padded zero-slot core. Here δ\delta is the positive padding parameter chosen below after the width floor and step. There is no repeated reflection at the boundary M/2M/2. Reflection and scale suprema are taken before centering; on a later centered term whose primitive inducing character lies outside Θ\Theta, one first applies the triangle inequality to its two rectangles. No such supremum is applied to a centered difference whose primitive inducing character belongs to Θ\Theta.

Prime estimates and the induction order

For κ<1\kappa< 1, put sκ=(1+κ)/2s_\kappa=(1+\kappa)/2. Under the hypothesis sκ≥β∗s_\kappa\ge\beta_*, the global part of Lemma 4.9 gives, for every fixed e>0e>0,

L′L(sκ+e+it,ψ)≪elog⁡ ⁣(2Qψ(3+∣t∣)2)\frac{L'}{L}(s_\kappa+e+it,\psi) \ll_e \log\!\bigl(2Q_\psi(3+|t|)^2\bigr)

for a primitive nonprincipal inducing character ψ\psi. To estimate a prime annulus of scale PP, apply Mellin inversion to a smooth von Mangoldt sum and move its contour to ℜs=sκ+e\Re s=s_\kappa+e. There are no poles in the region of the shift, and the Mellin transform has arbitrary decay, so (18.11) bounds the new integral by Psκ+eP^{s_\kappa+e} times a logarithm of the conductor and a fixed polynomial in the height. Prime powers of exponent at least two contribute O(P1/2+ϵ1)O(P^{1/2+\epsilon_1}). For large PP, dividing the annular weight by log⁡(Py)\log(Py) replaces the von Mangoldt weight by the prime weight; its smooth seminorms are bounded on the annulus. Bounded PP are estimated by absolute counting. Expand each positive-length coefficient in the characters ϑij\vartheta_{ij} from the statement. If the primitive inducing row character ψ∉Θ\psi\notin\Theta made ψϑij\psi\vartheta_{ij} principal, then ψ=ϑij−1∈Θ\psi=\vartheta_{ij}^{-1}\in\Theta, a contradiction. Thus every resulting slot character is nonprincipal on Rz\mathcal{R}_z.

After extra-mask erasure, fix a positive slot list and put W=(Wislot)i∈I\boldsymbol W=(W_i^{\rm slot})_{i\in\mathcal I}. For normalized twist heights ω=(ωi)i∈I\boldsymbol\omega=(\omega_i)_{i\in\mathcal I}, define

Qω=∏i∈I{Pi−1/2∑p primeψk0(p)νi(p)Wislot(qp/Pi)(qp/Pi)iωi}.Q_{\boldsymbol\omega} =\prod_{i\in\mathcal I}\left\{P_i^{-1/2} \sum_{p\ {\rm prime}}\psi_k^0(p)\nu_i(p)W_i^{\rm slot}(q_p/P_i) (q_p/P_i)^{i\omega_i}\right\}.

For every ϵ1>0\epsilon_1>0, central normalization and multiplication over this fixed list, with ee and all subsidiary losses sufficiently small, give finite j,b,h≥0j,b,h\geq0 and a constant CC such that

∣Qω∣2≤CZκz+ϵ1pj(W)b(1+∣ω∣)h(k∈Rz, z>0).|Q_{\boldsymbol\omega}|^2 \le C Z^{\kappa z+\epsilon_1}p_j(\boldsymbol W)^b (1+|\boldsymbol\omega|)^h \qquad(k\in\mathcal R_z,\ z>0).

Here jj may be rounded up to an integer and 2sκ−1=κ2s_{\kappa}-1=\kappa. The orders and CC may depend on the fixed data, slot count, loss, and any fixed requested internal logarithmic or normalized-twist derivatives, but not on ZZ, moving labels, rows, or the numerical heights. The exponent κz+ϵ1\kappa z+\epsilon_1 is independent of these derivative and height orders. Indeed, translate each pure twist in its Mellin variable before integration by parts. The weighted integral of the untwisted Mellin transform then contributes a finite seminorm and a fixed polynomial in ω\boldsymbol{\omega}, while the contour displacement contributes exactly 2ez2ez to the squared exponent. Logarithmic derivatives remain annular, and normalized-twist derivatives insert only powers of the logarithmic profile variable. The redundant natural radical contains only O(log⁡Z)O(\log Z) primes, so deleting it changes a normalized slot by O(Pi−1/2log⁡Z)O(P_i^{-1/2}\log Z) times its fixed profile factor; this is within the stated power loss because Pi≥1P_i\geq1. For κ=1\kappa=1, absolute prime counting gives (18.12) without a zero-free assumption and with h=0h=0 for undifferentiated pure twists, whose modulus is one. For κ<1\kappa<1 the hypothesis remains β∗≤(1+κ)/2\beta_*\leq(1+\kappa)/2. The choice of losses is uniform in κ∈[3/4,1]\kappa\in[3/4,1], since the length ranges are bounded. In every later use of (18.12), its fixed seminorm and height factor is retained in the weighted Fourier estimates; it is not included in the exponent of ZZ.

We now specify the induction, including the estimates at its smallest widths. Choose a width floor ρ>0\rho>0, a width step σ>0\sigma>0, and then δ>0\delta>0, all small in terms of the final ϵ\epsilon, with δ≪min⁡(ρ,σ)\delta\ll\min(\rho,\sigma). Precise loss choices will be made after the depth is bounded. Divide the bounded range of MM into consecutive bands of length σ/4\sigma/4. Prove all zero-slot bands first, in increasing order of width, and then all positive-slot bands. Within a zero-slot band, first prove the uncentered assertion for A≤5M/6A\leq5M/6, and then the padded core in (18.10). Reflection then supplies all zero-slot lengths in that band. Within a positive-slot band, first prove the uncentered assertion for A≤5M/6A\leq5M/6 subject to (18.3), and then the remaining part of that region by centering. A completed earlier band therefore includes the unrestricted zero-slot assertion. Let Mmax⁡M_{\max} bound the initial width range, and define

D=2+⌈2Mmax⁡/σ⌉.D=2+\left\lceil 2M_{\max}/\sigma\right\rceil.

The strict width decrease proved below will show that at most D−2D-2 nonterminal calls occur on a branch.

At M≤ρM\leq\rho, the padded zero-slot core follows from absolute counting: there are O(Zm)O(Z^m) rows and the squared product is O(ZA+ϵ1)O(Z^{A+\epsilon_1}). Its exponent above MM is at most A−q≤ρ+δA-q\leq\rho+\delta. For positive slots, combine the completed zero-slot estimate with (18.12). In the region of (18.3), A≥zA \ge z, whence

z≤M6κ≤2M9,κz≤M6.z \le\frac{M}{6\kappa} \le\frac{2M}{9}, \qquad\kappa z \le\frac{M}{6}.

Thus the extra terminal exponent for positive slots is at most ρ/6\rho/6. These terminal exponents can be made smaller than the reserved final loss by choosing ρ\rho, δ\delta sufficiently small.

For a width above the floor, the two-transform estimate below will first prove the uncentered range A≤5M/6A \le5M/6. We explain now why the remaining inputs can be compared with that range. Set

L=M/4.L = M/4.

For A>5M/6A > 5M/6, the comparison lengths LL, A−z−LA-z-L are both at least LL. In the positive-slot case, (6κ−1)z≤M−A<M/6(6\kappa-1)z \le M-A < M/6, and 6κ−1≥7/26\kappa-1 \ge7/2; hence z<M/21<M/20z < M/21 < M/20. This also shows A−z>2LA-z > 2L.

If one original plain length is b<Lb < L, reflect the other factor. If both are at least LL, introduce the comparison with lengths LL, A−z−LA-z-L and the same two profiles; reflect its longer factor only when estimating the comparison separately. In both cases the total length after that reflection is at most

b+{M−(A−z−b)}+z+ξ≤3M/2−A+2z+ξ,b+\{M-(A-z-b)\}+z+\xi\le3M/2-A+2z+\xi,

where b≤Lb \le L. (18.9) includes the clipped reflected scale and the paired unreflected box multiplier in this same ξ\xi; the discarded tails have the stated fixed-order bounds. Thus

Acomp≤3M/2−A+2z+ξ.A_{\mathrm{comp}} \le3M/2-A+2z+\xi.

For z=0z=0, this gives 5M/6−Acomp≥M/6−ξ5M/6-A_{\mathrm{comp}} \ge M/6-\xi. For z>0z>0, use (6κ−1)z≤M−A(6\kappa-1)z \le M-A, A>5M/6A>5M/6, and z<M/20z<M/20 to get

Acomp≤2330M+ξ,A_{\mathrm{comp}} \le\frac{23}{30}M+\xi,
Acomp+(6κ−1)z≤52M−2A+2z+ξ≤1415M+ξ.A_{\mathrm{comp}}+(6\kappa-1)z \le\frac{5}{2}M-2A+2z+\xi\le\frac{14}{15}M+\xi.

Each required boundary has a margin of at least M/15M/15 before the ξ\xi term. Choose ξ≤ρ/30\xi\le\rho/30. After the threshold in (18.9), the unit-box multipliers are already included in ξ\xi, so every retained reflected comparison calls the previously proved uncentered assertion at this same width. This also completes the original case with a factor shorter than LL.

In the remaining case put Xi=ZniX_i=Z^{n_i}, Y1=ZLY_1=Z^L, and Y2=X1X2/Y1Y_2=X_1X_2/Y_1. Then X1X2=Y1Y2X_1X_2=Y_1Y_2, and all four plain lengths are at least LL. Subtract the unreflected comparison from the original product, leaving the common product QQ of slots; call the result Δk\Delta_k. Multiplicativity and the equal product normalization give the explicit formula

Δk=QX1X2∑l1,l2ψk(l1l2){W1(ql1/X1)W2(ql2/X2)−W1(ql1/Y1)W2(ql2/Y2)}.\begin{aligned} \Delta_k =\frac{Q}{\sqrt{X_1X_2}}\sum_{l_1,l_2}\psi_k(l_1l_2) \bigl\{ &W_1(q_{l_1}/X_1)W_2(q_{l_2}/X_2)\\ -{}&W_1(q_{l_1}/Y_1)W_2(q_{l_2}/Y_2) \bigr\}. \end{aligned}

The comparison is bounded on the original permissible rows. The squared norm of the whole Δk\Delta_k is nonnegative, so it can then be enlarged to all rows in the smooth row ball. In the uncentered case, enlarge the squared norm of the original product instead. The Poisson transforms below are therefore never applied to an indicator selecting exceptional or nonexceptional rows.

The centered coefficient and its support

We keep the subtraction as one coefficient while transforming its row norm. For fixed ideals b=(b1,b2)\mathbf b=(\mathfrak b_1,\mathfrak b_2), define

Db(l1,l2)=∏i=12Wi(qbiqli/Xi)−∏i=12Wi(qbiqli/Yi),X1X2=Y1Y2.D_{\mathbf b}(l_1,l_2) = \prod_{i=1}^2W_i(q_{\mathfrak b_i}q_{l_i}/X_i) - \prod_{i=1}^2W_i(q_{\mathfrak b_i}q_{l_i}/Y_i), \qquad X_1X_2=Y_1Y_2.

An allocation b\mathbf{b} records prime powers already extracted from the two plain variables. If its conditions are impossible for one rectangle, that rectangle’s profile is zero on the corresponding sum; the formal difference in Equation (18.17) is nevertheless retained.

The reason for retaining these common data is already visible in the exceptional case. For a fixed ϑ∈Θ\vartheta\in\Theta, a common mask R∗\mathfrak{R}_*, and a common norm power qlitq_l^{it}, the lattice estimate proved below has leading term

∑lϑ(l)1(l,R∗)=1qlitWi(ql/T)=cϑ,R∗T1+itIi(t)+error,\sum_l \vartheta(l)1_{(l,\mathfrak{R}_*)=1}q_l^{it}W_i(q_l/T)=c_{\vartheta,\mathfrak{R}_*}T^{1+it}I_i(t)+\text{error},

where cϑ,R∗c_{\vartheta,\mathfrak{R}_*} does not depend on TT or tt. Here Ii(t)I_i(t) is a fixed measure constant times ∫0∞Wi(y)yit dy\int_0^\infty W_i(y)y^{it}\,dy. The product main term is therefore cϑ,R∗2T11+itT21+itI1(t)I2(t)c_{\vartheta,\mathfrak{R}_*}^2T_1^{1+it}T_2^{1+it}I_1(t)I_2(t), which agrees for the two rectangles when T1T2T_1T_2 agrees. Lemma 18.3 will quantify the remaining error. This cancellation is used only on the transformed rows inducing characters in Θ\Theta; the common coefficient below is retained on all rows until that later division into cases.

For a remaining slot set I′\mathcal I', write Π=∏i∈I′pi\Pi=\prod_{i\in\mathcal I'}p_i. A coefficient with a common character and mask means a coefficient of the form

(∏i∈I′νi(pi)Wislot(qpi/Pi))Db(l1,l2) τ1(u)quit1(u,R)=11s∣u,u=Πl1l2.\begin{aligned} &\left(\prod_{i\in\mathcal I'} \nu_i(p_i)W_i^{\rm slot}(q_{p_i}/P_i)\right) D_{\mathbf b}(l_1,l_2)\, \tau_1(u)q_u^{it} 1_{(u,\mathfrak R)=1}1_{s\mid u},\\ &\hspace{40mm}u=\Pi l_1l_2. \end{aligned}

Here τ1\tau_1 is one zero-extended product of a fixed finite-ray character and moving residue-symbol factors; R\mathfrak{R} is a fixed squarefree extra mask; ss is a fixed squarefree ideal; and t∈Rt\in\mathbb{R}. The condition s∣us\mid u is omitted when s=1s=1. The slots retain their original disjoint underlying supports. They may share primes with either plain variable.

These common data factor multiplicatively on the full product. For any ideals v1,…,vrv_1,\ldots,v_r, even with common primes,

χ∏vi(h)=∏iχvi(h),q∏viit=∏iqviit,1(∏vi,R)=1=∏i1(vi,R)=1.\chi_{\prod v_i}(h)=\prod_i\chi_{v_i}(h),\qquad q_{\prod v_i}^{it}=\prod_iq_{v_i}^{it},\qquad1_{(\prod v_i,\mathfrak{R})=1}=\prod_i1_{(v_i,\mathfrak{R})=1}.

The first identity includes all zeros: a present prime whose total exponent is divisible by six gives the zero-extended principal factor, not the constant one. The same multiplicativity holds for τ1\tau_1. A fixed-ray character evaluated on a full product also factors with the same character on every variable.

We fix a support convention that will also control the slot-mesh quantifier. Let NN be the original fixed number of slots, and choose fixed intervals [ai,bi][a_i,b_i] containing the support of each WislotW_i^{\mathrm{slot}}. Put hi=max⁡{∣log⁡ai∣,∣log⁡bi∣}h_i=\max\{|\log a_i|,|\log b_i|\}. Choose a fixed number HNH_N at least ∑ihi\sum_i h_i, enlarged to include the two plain profile windows, log⁡Cref\log C_{\mathrm{ref}}, fixed arithmetic normalizations, the relative dyadic boxes, and the finitely many support enlargements through the DD operation stages. The number HNH_N may depend on all the fixed data and on NN, but not on ZZ or any moving label. For every subset II of live or frozen slots,

∣log⁡∏i∈IqpiPi∣≤∑i∈Ihi≤HN,θN:=HNlog⁡Z.\left|\log\prod_{i\in I}\frac{q_{p_i}}{P_i}\right|\leq\sum_{i\in I}h_i\leq H_N,\qquad\theta_N:=\frac{H_N}{\log Z}.

Every residual full product divided by its nominal product scale lies in exp⁡([−HN,HN])\exp([-H_N,H_N]), after increasing HNH_N once for the fixed list of operations. Both rectangles use that same box. Extracted plain prime powers use their exact norms, and a frozen slot contributes its ratio qp/Piq_p/P_i just once. If a nonempty plain scale below one is clipped to one, its error is at most the logarithm of that plain window’s fixed endpoint divided by log⁡Z\log Z, once for that plain. Thus a whole subset of slots or a whole divisor extraction contributes one aggregate O(θN)O(\theta_N) boundary error, not one copy of a preselected tolerance for each slot or prime.

The first Poisson transform and its target bound

We now estimate either the uncentered product or the centered difference selected above. Put H=ZmH=Z^m and X=ZAX=Z^A. Choose a fixed nonnegative smooth radial function that majorizes the row ball. The full index product in either rectangle has norm in a fixed multiple of XX. All comparisons of exponents in this subsection are first made on fixed dyadic norm intervals. Their bounded relative widths change a logarithmic length by O(1/log⁡Z)O(1/\log Z); the final loss discussion includes these changes.

We use the following common localization for both Poisson formulas. Fix a nonnegative smooth dyadic partition ∑λωλ(q/Tλ)=1\sum_\lambda\omega_\lambda(q/T_\lambda)=1 for q>0q>0, with each weight supported in Cd−1≤q/Tλ≤1C_d^{-1}\le q/T_\lambda\le1 for one fixed CdC_d. A sector fixes dyadic boxes for the finite list of aggregate outer norms, not a separate box for each slot. Let TsecT_{\mathrm{sec}} be the supremum in that sector of the nominal frequency scale. Its ratio to the scale at any one set of outer labels is at most a fixed CsecC_{\mathrm{sec}}. Retain exactly the whole weights whose support meets

0<q≤TsecZξ/2.0<q\le T_{\mathrm{sec}}Z^{\xi/2}.

Their union is contained in q≤CdTsecZξ/2q\le C_dT_{\mathrm{sec}}Z^{\xi/2}; every discarded weight is supported above TsecZξ/2T_{\mathrm{sec}}Z^{\xi/2}. The selection depends only on the sector, never on a live column. After NN and the support data are fixed, take ZZ large enough that

2θN+log⁡(CdCsec)log⁡Z<ξ4.2\theta_N+\frac{\log(C_dC_{\mathrm{sec}})}{\log Z}<\frac{\xi}{4}.

One fixed enlargement of CsecC_{\mathrm{sec}} covers all the finitely many sector endpoint factors.

Here is a direct tail bound that justifies this operation on the genuine sums. In both applications the kernel argument is at least q/(e2HNTsec)q/(e^{2H_N}T_{\mathrm{sec}}). On every discarded weight it is therefore at least Zξ/4Z^{\xi/4}, by Equation (18.20). Lemma 4.7 gives arbitrary decay (1+argument)−B(1+\text{argument})^{-B}. For the first formula use ∣G(a,h)∣≤qa1/2|G(a,h)|\le q_a^{1/2}, and for the second use the finite definition ∣F(u,v;j)∣≤quqv|F(u,v;j)|\le q_uq_v. Absolute ideal counting and the divisor bounds for the fixed number of factors bound all raw columns and prefactors in a sector by CNZB0C_NZ^{B_0} times a fixed polynomial in the retained heights, where B0B_0 depends only on the bounded total lengths and chosen subsidiary power shares. A lattice norm dyad of scale TT has O(1+T)O(1+T) frequencies. Summing the radial decay over discarded dyads consequently gives CN,BZB1−Bξ/4C_{N,B}Z^{B_1-B\xi/4} times that height polynomial, for a bounded B1B_1 independent of BB and NN, and a convergent geometric sum when B>1B>1. Choose BB sufficiently large to obtain any prescribed power saving, including the polynomial number of frozen outer labels. This is an absolute bound for the original terms, before any off-coprime extension or Fourier absolutization. It uses neither the later ss-radical saving nor a factorized off-coprime identity. On the retained weights the full smooth kernel is kept; no sharp condition comparing a row norm with the two live column norms is inserted. A retained range below the first nonzero lattice norm is empty, apart from a bounded boundary dyad covered by the clipping convention below.

At zero frequency in the first row Poisson formula, a character mean can be nonzero only if its exponent at every prime is zero modulo six. In particular, no prime occurs to total multiplicity one in the product of the two full index products. This product is therefore a powerful ideal. There are Oε(X1+ε)O_\varepsilon(X^{1+\varepsilon}) such products of norm O(X2)O(X^2): each powerful ideal is a square times a cube of a squarefree ideal, and summing over the latter gives the usual O(Y1/2+ϵ)O(Y^{1/2+\epsilon}) bound up to norm YY. Allocations to the fixed number of factors are divisor-bounded. The central factor is X−1X^{-1}, and the row mean has size at most HH. Thus the zero frequency is O(Zm+ϵ1)O(Z^{m+\epsilon_1}).

For the nonzero frequencies write the two full products as CaC a, DbD b, where C,DC,D contain their complete common prime support and

(a,b)=1,(ab,CD)=1.(a,b)=1,\qquad(ab,CD)=1.

At each common prime, fix its exact valuation in each plain variable and whether it is supplied by a slot. Dividing out these valuations adds that prime to the mask of every remaining factor on the side. A slot that supplied the prime is frozen and removed. This description is valid even when a slot and one or both plain variables supplied that prime. The allocation is made once for the coefficient, so the same ideals bi\mathfrak b_i occur in the two terms of DbD_{\mathbf b}. An impossible allocation is a zero term. In particular, a scalar forced to vanish by an old moving zero or a common mask is not replaced by its absolute upper bound before these support conditions have been imposed.

Let c,dc,d be the logarithmic norms of C,DC,D, and let pp be the logarithmic norm of their common radical. Let r\mathfrak r be the product of common primes whose net exponents are nonzero modulo six; its logarithmic norm is RR. The corresponding character ξr\xi_{\mathfrak r} is primitive modulo r\mathfrak r. In the Möbius expansion of the complementary common row mask, write e\mathfrak e for the selected divisor and EE for its logarithmic norm. In particular

R≤p,E≤p−R.R\le p,\qquad E\le p-R.

Let AC(a)A_C(a) and AD(b)A_D(b) be the allocated convolution coefficients, with the common character τ\tau omitted. They include all profiles, live slot coefficients, and fixed masks; in the centered case each contains the entire allocated difference. Set

τC(a)=τ(a)χa(er)ξr(a),τD(b)=τ(b)χb(er)ξr(b)‾.\tau_C(a)=\tau(a)\chi_a(\mathfrak e\mathfrak r) \xi_{\mathfrak r}(a),\qquad \tau_D(b)=\tau(b)\chi_b(\mathfrak e\mathfrak r) \overline{\xi_{\mathfrak r}(b)}.

Residue-class Poisson, with the self-dual lattice measure from Section 4, gives for this allocation the following nonzero-frequency expression, up to a scalar of bounded modulus in the frozen labels:

HXqeqr∑h≠0Gξr(r,h)∑(a,b)=1AC(a)AD(b)‾qaqb τC(a)τD(b)‾R(a,b)‾ G(a,h)G(b,−h)‾⋅Φ^1(Hqhqeqrqaqb).\begin{aligned} \frac{H}{Xq_{\mathfrak e}\sqrt{q_{\mathfrak r}}} \sum_{h\ne0}G_{\xi_{\mathfrak r}}(\mathfrak r,h) \sum_{(a,b)=1} &\frac{A_C(a)\overline{A_D(b)}}{\sqrt{q_aq_b}}\, \tau_C(a)\overline{\tau_D(b)} \overline{\mathcal R(a,b)}\, G(a,h)\overline{G(b,-h)} \\ &\quad\cdot \widehat\Phi_1\left( \frac{Hq_h}{q_{\mathfrak e}q_{\mathfrak r}q_aq_b} \right). \end{aligned}

Here GξrG_{\xi_{\mathfrak r}} is the normalized primitive Gauss sum and has modulus at most one. To check the normalization, the substitution k=ek′k=\mathfrak e k' and Poisson modulo rab\mathfrak r ab give H/(qeqrqaqb)H/(q_{\mathfrak e}q_{\mathfrak r}q_aq_b). The three unnormalized Gauss sums restore qrqaqb\sqrt{q_{\mathfrak r}q_aq_b}. The global squared central normalization is X−1X^{-1}. For the phase, CRT for the pairwise coprime moduli a,b,ra,b,\mathfrak r supplies

χa(br)χb(ar)‾ξr(ab).\chi_a(b\mathfrak r)\overline{\chi_b(a\mathfrak r)} \xi_{\mathfrak r}(ab).

The substitution k=ek′k=\mathfrak e k' supplies χa(e)χb(e)‾\chi_a(\mathfrak e)\overline{\chi_b(\mathfrak e)}, up to a scalar in the frozen labels. Reciprocity changes χa(b)χb(a)‾\chi_a(b)\overline{\chi_b(a)} into R(a,b)‾\overline{\mathcal R(a,b)}; the remaining factors are precisely τC(a)τD(b)‾\tau_C(a)\overline{\tau_D(b)}. This proves Equation (18.21). Each new character acts on its whole residual product. Its new moving primes belong to the extracted support and puncture every residual factor. Their full displayed union is counted even if the factors at r\mathfrak r cancel on units.

The new full displayed moving support has logarithmic norm at most q~=q+R+E\widetilde q=q+R+E, including any canceled factors at r\mathfrak r. Its nominal frequency scale is exactly

T1(C,D,e,r)=qeqrX2HqCqD=ZK0,K0=2A−c−d+R+E−m.T_1(C,D,\mathfrak e,\mathfrak r) =\frac{q_{\mathfrak e}q_{\mathfrak r}X^2} {Hq_Cq_D}=Z^{K_0}, \qquad K_0=2A-c-d+R+E-m.

The product support convention gives qa/(X/qC),qb/(X/qD)∈exp⁡([−HN,HN])q_a/(X/q_C),q_b/(X/q_D)\in\exp([-H_N,H_N]), so the argument in Equation (18.21) is at least qh/(e2HNTsec)q_h/(e^{2H_N}T_{\mathrm{sec}}) for the supremum of T1T_1 in the outer sector. Apply the preceding whole-dyad localization to this genuine coprime bridge. If K=log⁡ZTλK=\log_Z T_\lambda is the upper length of a retained dyad, then

q~=q+R+E,K≤K0+δfr,1,0≤δfr,1:=ξ2+log⁡(CdCsec)log⁡Z<ξ.\widetilde{q}=q+R+E,\qquad K\leq K_0+\delta_{\mathrm{fr},1},\qquad0\leq\delta_{\mathrm{fr},1}:=\frac{\xi}{2}+\frac{\log(C_dC_{\mathrm{sec}})}{\log Z}<\xi.

The zero frequency already estimated above was the zero term of the original common smooth row ball; it is not restored on a truncated row domain. The later ledgers retain the possible inequality K0−K≥−δfr,1K_0-K\geq-\delta_{\mathrm{fr},1}.

For each retained dyad and genuine common-support allocation, define C1(a,b;h)\mathcal C_1(a,b;h) to be the full bridge summand also on noncoprime residual pairs individually disjoint from CDCD and allowed by the old masks. Use the fixed bicharacter R(a,b)\mathcal{R}(a,b), the full zero-extended G(a,h),G(b,−h)G(a,h),G(b,-h), the displayed whole-product characters, and the same dyad weight, kernel, inverse roots, and formal product norms. CRT identifies this definition with the genuine summand only on (a,b)=1(a,b)=1. On each finite column shell the exact identity is

∑(a,b)=1C1(a,b;h)=∑a,bC1(a,b;h)∑s∣a,bμ(s).\sum_{(a,b)=1}\mathcal C_1(a,b;h) =\sum_{a,b}\mathcal C_1(a,b;h)\sum_{s\mid a,b}\mu(s).

The full squarefree Möbius sum annihilates the artificial noncoprime pairs. Insert it before estimating independent factors, and put s0=log⁡Zqss_0=\log_Zq_s. Separate the fixed-ray phases and all smooth factors in the normalized row norm and the two whole-product norms. In these variables the kernel is Φ^1(Rscx/(y1y2))\widehat\Phi_1(R_{\rm sc}x/(y_1y_2)) on fixed logarithmic boxes. If its aggregate scale ratio RscR_{\mathrm{sc}} varies over the sector, include that single normalized outer ratio as another coordinate. The cutoffs are chosen on the common product annulus of Equation (18.19), before fixing live slot labels. Thus one Fourier coefficient measure is common to the rows and all live labels. It supplies a row phase and only one norm power on each whole column, together with phases in frozen outer norms. It introduces no separate powers on the two plain variables or the two rectangles. The full kernel and inverse roots are kept until this separation; taking their absolute supremum inside DbD_{\mathbf b} would not preserve the coefficient. Apply Cauchy–Schwarz in hh only after this separation, and only then use ∣Gξr∣≤1|G_{\xi_{\mathfrak r}}|\le1. The resulting positive norm on the CC side is

NC=∑h≠0ωK(qh/ZK)∣Z−(A−c)/2∑s∣aAC(a)τC′(a)qaitG(a,h)∣2,ωK≥0,\mathcal N_C= \sum_{h\ne0}\omega_K(q_h/Z^K) \left|Z^{-(A-c)/2} \sum_{s\mid a}A_C(a)\tau_C'(a)q_a^{it}G(a,h)\right|^2, \qquad \omega_K\ge0,

and there is an analogous DD norm. Here τC′\tau_C' includes one separated fixed-ray character. All fixed masks in ACA_C remain present. Complete extraction and multiplicativity therefore leave the coefficient in Equation (18.18), now multiplied by G(a,h)G(a,h). In particular the two rectangles retain the same allocated plain powers, character, puncture, and norm power.

The factors outside these two norms have exponent m−A−R/2−Em-A-R/2-E. The absolute number of common-support labels and Möbius labels has exponent p+s0+ϵ1p+s_0+\epsilon_1. To justify the common-support count uniformly, first count its radical, giving O(Zp+ϵ1)O(Z^{p+\epsilon_1}). For a fixed radical c\mathfrak c of polynomial norm and any fixed TT, Rankin’s bound gives

#{v:rad⁡(v)∣c, qv≤ZT}≤ZaT∏r∣cr prime(1−qr−a)−1≪ZaT+ϵ1\#\{v:\operatorname{rad}(v)\mid\mathfrak c,\ q_v\le Z^T\} \le Z^{aT}\prod_{\substack{r\mid\mathfrak c\\r\ {\rm prime}}} (1-q_r^{-a})^{-1} \ll Z^{aT+\epsilon_1}

for every fixed a>0a>0. Choose aa small and use the polynomial-size Euler-product estimate. This bounds the choices of the powers in C,DC,D by an arbitrarily small power. Their allocations and the choice of e\mathfrak e have divisor-bounded multiplicity. Finally there are O(Zs0+ϵ1)O(Z^{s_0+\epsilon_1}) possible ss.

The allowance ϵG\epsilon_G below denotes the error envelope for the current induction depth, together with its local small-power shares. These envelopes will be chosen compatibly when the finite induction is completed, using the same slot mesh throughout. We will prove the following sufficient bound for the squared CC norm:

NC≪ZA−c+q~+Bc−s0+ϵG,Bc=max⁡{0,(3c−5d−R)/6}.\mathcal N_C\ll Z^{A-c+\widetilde q+\mathcal B_c-s_0+\epsilon_G}, \qquad \mathcal B_c=\max\{0,(3c-5d-R)/6\}.

The analogous quantity is Bd=max⁡{0,(3d−5c−R)/6}\mathcal B_d=\max\{0,(3d-5c-R)/6\}. The complete exponent ledger for this implication is

(m−A−R/2−E)+(p+s0)+12{A−c+q~+Bc−s0+A−d+q~+Bd−s0}=M+12{Bc+Bd−(c+d−2p−R)}.\begin{aligned} &(m-A-R/2-E)+(p+s_0)\\ &\quad+\tfrac12\{A-c+\widetilde q+\mathcal B_c-s_0 +A-d+\widetilde q+\mathcal B_d-s_0\}\\ &=M+\tfrac12\{\mathcal B_c+\mathcal B_d-(c+d-2p-R)\}. \end{aligned}

The last brace is nonpositive:

Bc+Bd≤c+d−2p−R.\mathcal B_c+\mathcal B_d\le c+d-2p-R.

Indeed, at a common prime of multiplicities i≥j≥1i\ge j\ge1, put r=16∤i−jr=1_{6\nmid i-j}. Only the ii side can have a positive local numerator. Its contribution is at most (3i−5j−r)+/6(3i-5j-r)_+/6, whereas the right side contributes i+j−2−ri+j-2-r. The latter is nonnegative. If the former is positive, six times their difference is 3i+11j−12−5r3i+11j-12-5r, which is nonnegative: for r=0r=0 it is at least 2, and for r=1r=1 one has i≥j+1i\ge j+1, giving at least 0. The positive part of a sum is at most the sum of positive parts. Multiplication by each prime’s logarithmic norm and summation proves Equation (18.24). Thus it remains to establish Equation (18.23).

Enlarging the Gauss-row norm

This subsection describes three possible positive norms to which the second transform will be applied. Let ww denote a length removed from the CC column, and let wo≤ww_o\le w be the additional moving-radical length created by that removal. Put a0=A−c−wa_0=A-c-w. When a squared extraction coefficient of size Z−woZ^{-w_o} has been removed, Equation (18.23) allows the unweighted remaining norm the exponent

Λc=a0+q~+wo+w+Bc−s0+ϵG.\Lambda_c= a_0+\widetilde q+w_o+w+\mathcal B_c-s_0+\epsilon_G.

This is just A−c+q~+Bc−s0+ϵG+woA-c+\widetilde q+\mathcal B_c-s_0+\epsilon_G+w_o.

For the initial norm, with w=wo=0w=w_o=0 and a0=A−ca_0=A-c, the first transform gives the following conditional summand after fixing Π\Pi and omitting its outer scalar:

Z−a0/2∑l1,l2Db(l1,l2)τ1(l1l2)ql1l2it1(Πl1l2,R)=11s∣Πl1l2G(Πl1l2,h).Z^{-a_0/2}\sum_{l_1,l_2} D_{\mathbf b}(l_1,l_2)\tau_1(l_1l_2)q_{l_1l_2}^{it} 1_{(\Pi l_1l_2,\mathfrak R)=1}1_{s\mid\Pi l_1l_2} G(\Pi l_1l_2,h).

The slot sums are restored before this polynomial is squared. The same statement with the second rectangle omitted applies to uncentered products. The local calculations below will show that the extracted terms retain this form at their shortened length a0=A−c−wa_0=A-c-w.

Define

J=d−c+(K0−K)−2w+wo,J+=max⁡(J,0).J=d-c+(K_0-K)-2w+w_o,\qquad J_+=\max(J,0).

In the zero-slot proof take w=wo=0w=w_o=0, and set

ℓ=0,g=J++σ.\ell=0,\qquad g=J_++\sigma.

The positive norm NC\mathcal{N}_C is at most the corresponding norm over a smooth ball of length K+gK+g. There is no multiplication of rows in this case.

For positive slots, start with w=wo=0w=w_o=0. Set ℓ∗=σ/3\ell_*=\sigma/3, choose the slot mesh η<σ/6\eta<\sigma/6, and take the fixed pool

P={p:Zℓ∗/2<qp≤Zℓ∗, p∉S}.\mathcal P=\{p: Z^{\ell_*}/2<q_p\le Z^{\ell_*},\ p\notin\mathcal S\}.

The prime ideal theorem in the fixed field, equivalently its fixed ray-class form [27 Theorem 1.1], gives ∣P∣=Zℓ∗+o(1)|\mathcal{P}| = Z^{\ell_*+o(1)}. Because the live slot lengths are at most η\eta and their relative annular supports are fixed, the single inequality Zℓ∗−η>2max⁡ibiZ^{\ell_*-\eta} > 2\max_i b_i makes this pool disjoint from every live slot window. Its exponent gap is at least σ/6\sigma/6, independently of NN; only the threshold depends on the fixed windows. For a row h≠0h \ne0, omit pool primes dividing hh, ss, or any frozen support. Each such integer or ideal has polynomial norm, so O(log⁡Z)O(\log Z) primes are omitted. The remaining set Ph\mathcal{P}_h has size comparable to ∣P∣|\mathcal{P}|, uniformly in the row and frozen labels.

To compare the rows hh and hp6hp^6, write a full modulus as piup^i u with (p,u)=1(p,u)=1. CRT and reciprocity give the exact formula

G(piu,h)=R(p,u)iχp(u)2iG(pi,h)G(u,h).G(p^i u,h)=\mathcal{R}(p,u)^i\chi_p(u)^{2i}G(p^i,h)G(u,h).

Also G(u,hp6)=G(u,h)G(u,hp^6)=G(u,h), since pp is a unit modulo uu and χu(p6)=1\chi_u(p^6)=1. For p∤hp\nmid h, (13.5) shows that replacing hh by hp6hp^6 changes only i=1,6,7i=1,6,7. The factors G(pi,h)G(p^i,h) that occur are a scalar in the row and pp; the displayed remaining factor is one fixed-ray character times one residue character on the whole uu. Since pp is outside every live slot window, pip^i is allocated only to the two plain variables. The residual product is punctured at pp, and the same allocation updates DbD_{\mathbf b} in both rectangles. Because p∤sp\nmid s, the condition s∣us\mid u remains.

Here is the precise averaging argument. Write the normalized polynomial in NC\mathcal N_C as H(h)\mathcal{H}(h). For each eligible pp, local Gauss evaluation gives H(h)=H(hp6)\mathcal{H}(h)=\mathcal{H}(hp^6) plus the extracted terms with pp-adic column valuations 1,6,71,6,7. There are only boundedly many allocations of each of these valuations to the two plain variables. Jensen’s inequality, first in pp and then for this fixed finite sum, gives

∣H(h)∣2≪1∣Ph∣∑p∈Ph{∣H(hp6)∣2+∑i=1,6,7∑allocations∣cp,i(h)∣2∣Hp,i(h)∣2}.|\mathcal H(h)|^2\ll \frac1{|\mathcal P_h|}\sum_{p\in\mathcal P_h} \left\{|\mathcal H(hp^6)|^2+ \sum_{i=1,6,7}\sum_{\rm allocations} |c_{p,i}(h)|^2|\mathcal H_{p,i}(h)|^2\right\}.

The Hp,i\mathcal{H}_{p,i} are normalized at their shortened column scales. The local identity and allocation just described are applied to the whole centered coefficient, so each error retains (18.18).

On the support of the original row weight, the new row hp6hp^6 has norm O(ZK+6ℓ∗)O(Z^{K+6\ell_*}). A fixed output row has only boundedly many representations as hp6hp^6 with p∈Php\in\mathcal{P}_h: every such pp divides that row, and all such primes have norm at least Zℓ∗/2Z^{\ell_*}/2, while the output norm has bounded logarithmic length. Summing the first term over hh therefore gives the factor ∣P∣−1=Z−ℓ∗+o(1)|\mathcal{P}|^{-1}=Z^{-\ell_*+o(1)} times a positive norm on the new rows. For this main term set

ℓ=ℓ∗,g=J++2σ.\ell=\ell_*,\qquad g=J_++2\sigma.

Since 6ℓ∗=2σ6\ell_*=2\sigma, a smooth ball of length K+gK+g contains all the new rows.

For the extracted terms put P=qpP=q_p. When p∤hp\nmid h, Equation (13.5) gives the following central coefficients. At valuation one, the old Gauss sum has modulus one and the new one is zero, so extraction gives squared coefficient P−1P^{-1}. At valuation six, the new Gauss sum is P3(1−P−1)P^3(1-P^{-1}); its central factor is P−3P^{-3}, giving (1−P−1)2(1-P^{-1})^2. At valuation seven, the new Gauss sum has modulus P3P^3, and the central factor P−7/2P^{-7/2} gives P−1P^{-1}. The row phase is χp(h)‾\overline{\chi_p(h)} for valuations one and seven, and is one for valuation six. It multiplies both rectangles.

Let ℓp=log⁡ZP\ell_p=\log_Z P. For sufficiently large ZZ, ℓ∗/2≤ℓp≤ℓ∗\ell_*/2\leq\ell_p\leq\ell_*. The removal and new moving-radical lengths for the three terms are

(w,wo)=(iℓp,eiℓp),i=1,6,7,e1=e7=1,e6=0.(w,w_o)=(i\ell_p,e_i\ell_p),\qquad i=1,6,7,\quad e_1=e_7=1,\quad e_6=0.

The two squared factors P−1P^{-1} give exactly Z−woZ^{-w_o}. For the valuation-six term, the exact factor χp(u)12=1(u,p)=1\chi_p(u)^{12}=1_{(u,p)=1} is represented by the already common fixed puncture at pp, with its fixed-ray phase R(p,u)6\mathcal{R}(p,u)^6 retained. At valuations one and seven the displayed local factor remains, and its prime is counted in the moving radical. In each error, freeze pp, retain its common column puncture, and discard its row eligibility restriction only after taking the positive norm. The average remains ∣P∣−1∑p∈P|\mathcal{P}|^{-1}\sum_{p\in\mathcal{P}}, so a bound uniform in the frozen pp introduces no prime-count factor. For each error set

ℓ=0,g=J++σ\ell=0,\qquad g=J_++\sigma

and enlarge its original rows directly to a smooth ball of length K+gK+g. Errors are not amplified again. All three types of norm satisfy

0≤wo≤w≤7σ/3.0\le w_o\le w\le7\sigma/3.

The row zero is added only at the final smooth ball. Put Ycol=eHNZa0=Za0+θNY_{\mathrm{col}}=e^{H_N}Z^{a_0}=Z^{a_0+\theta_N}. A nonempty column shell satisfies Ycol≥1Y_{\mathrm{col}}\ge1, and hence a0≥−θNa_0\ge-\theta_N. By Equation (13.5), G(u,0)=0G(u,0)=0 unless uu is a sixth power, and ∣G(u,0)∣≤qu1/2≤Ycol1/2|G(u,0)|\le q_u^{1/2}\le Y_{\mathrm{col}}^{1/2}. There are O(Ycol1/6)O(Y_{\mathrm{col}}^{1/6}) sixth powers on this support. If s∣us\mid u, then qs6≤qu≤Ycolq_s^6\le q_u\le Y_{\rm col}, so s0≤(a0+θN)/6s_0\le(a_0+\theta_N)/6. Including the assigned divisor-bounded convolution loss, the squared contribution after central normalization is

≪Z−a0(Ycol1/6Ycol1/2)2Zε1=Za0/3+4θN/3+ε1≤Za0−s0+2θN+ε1.\ll Z^{-a_0}\left(Y_{\mathrm{col}}^{1/6}Y_{\mathrm{col}}^{1/2}\right)^2Z^{\varepsilon_1} =Z^{a_0/3+4\theta_N/3+\varepsilon_1} \le Z^{a_0-s_0+2\theta_N+\varepsilon_1}.

The last inequality follows from a0≥−θNa_0\ge-\theta_N and the displayed bound for s0s_0. Thus Equation (18.25) bounds this added row with the numerical 2θN2\theta_N correction included in the C∗ξC_*\xi stage allowance. Here C∗≥1C_*\ge1 denotes the common constant for aggregate support errors in one stage, chosen independently of the slot count NN. The estimates below establish that one such choice covers all operations in a stage. Zero is never multiplied by a pool prime.

The second transform and smaller-width products

Restore all live slot sums before expanding the square. Let B(u)B(u) denote the full allocated convolution coefficient in one of the preceding Gauss polynomials, including its fixed mask and ss-divisibility condition. It contains the whole difference when centering is used. Its moduli satisfy qu/Za0∈exp⁡([−HN,HN])q_u/Z^{a_0}\in\exp([-H_N,H_N]). Let Φ2\Phi_2 be the nonnegative smooth radial function defining the final row ball. Apart from the Zo(1)Z^{o(1)} loss in the prime density, the norm to be bounded is

Z−ℓ∑hΦ2(qh/ZK+g)∣Z−a0/2∑uB(u)τ1(u)quitG(u,h)∣2.Z^{-\ell}\sum_h\Phi_2\left(q_h/Z^{K+g}\right)\left|Z^{-a_0/2}\sum_uB(u)\tau_1(u)q_u^{it}G(u,h)\right|^2.

The Fourier identity in Lemma 13.3 gives its exact expansion

ZK+g−ℓ−a0∑u,vB(u)B(v)‾τ1(u)τ1(v)‾quitqv−itquqv∑jF(u,v;j)Φ^2(ZK+gqjquqv).Z^{K+g-\ell-a_0}\sum_{u,v}\frac{B(u)\overline{B(v)}\tau_1(u)\overline{\tau_1(v)}q_u^{it}q_v^{-it}}{\sqrt{q_uq_v}}\sum_jF(u,v;j)\widehat{\Phi}_2\left(\frac{Z^{K+g}q_j}{q_uq_v}\right).

The kernel that occurs here is

Φ^2(ZK+gqjquqv).\widehat{\Phi}_2\left(\frac{Z^{K+g}q_j}{q_uq_v}\right).

Both the displayed inverse square roots and this kernel are retained as functions of full u,vu,v until their whole-product separation below. In particular the formula includes every live prime and every shared-prime multiplicity.

At j=0j=0, Lemma 13.3 leaves only u=vu=v, with F(u,u;0)=φ(u)≤quF(u,u;0)=\varphi(u)\le q_u. The number of supported moduli divisible by ss, on a nonempty shell, is at most

CYcolqs=CZa0−s0+θN,C\frac{Y_{\mathrm{col}}}{q_s}=CZ^{a_0-s_0+\theta_N},

because writing u=svu=sv gives Ycol/qs≥1Y_{\mathrm{col}}/q_s\ge1 on that shell. The divisor-bounded coefficients use their separate ε1\varepsilon_1 share. Thus the diagonal exponent is K+g−ℓ−s0+θNK+g-\ell-s_0+\theta_N, including when a0−s0a_0-s_0 is slightly negative. Subtracting the allowance in (18.25) from its nominal part, without ϵG\epsilon_G, gives

(K+g−ℓ−s0)−(a0+q~+wo+w+Bc−s0)=(A−M)−d−(K0−K)−wo−Bc+g−ℓ≤A−M+5σ/3+δfr,1.\begin{aligned} &(K+g-\ell-s_0) -(a_0+\widetilde q+w_o+w+\mathcal B_c-s_0)\\ &\quad=(A-M)-d-(K_0-K)-w_o-\mathcal B_c+g-\ell\\ &\quad\le A-M+5\sigma/3+\delta_{{\rm fr},1}. \end{aligned}

For the inequality, put D0=d+K0−KD_0=d+K_0-K. The contribution −D0−wo+J+-D_0-w_o+J_+ is at most δfr,1\delta_{\mathrm{fr},1}: it is at most −c−2w-c-2w when J≥0J\ge0, and when J<0J<0 use D0≥−δfr,1D_0\ge-\delta_{\mathrm{fr},1}. The largest remaining increment is 2σ−ℓ∗=5σ/32\sigma-\ell_* = 5\sigma/3 in the amplified main norm; the other norms have increment σ\sigma. Thus the diagonal requires only the displayed terminal loss 5σ/35\sigma/3, plus the already reserved frequency perturbation δfr,1\delta_{\mathrm{fr},1} and numerical support correction θN\theta_N, when A≤MA\le M, and an additional δ\delta in the padded zero-slot core. The θN\theta_N correction is included in the C∗ξC_*\xi stage allowance.

For j≠0j\ne0, first perform the whole-dyad localization on this genuine full (u,v,j)(u,v,j) sum, before extracting any common support. The nominal scale is T2=Z2a0−K−gT_2=Z^{2a_0-K-g}, and the kernel argument is at least qj/(e2HNTsec)q_j/(e^{2H_N}T_{\mathrm{sec}}) for its supremum in the current Gauss sector. The tail estimate above applies using ∣F(u,v;j)∣≤quqv|F(u,v;j)|\le q_uq_v, with the literal conditions s∣u,vs\mid u,v still present. Write

Ωret(qj):=∑λ retainedωλ(qj/Tλ).\Omega_{\mathrm{ret}}(q_j):=\sum_{\lambda\ \mathrm{retained}}\omega_\lambda(q_j/T_\lambda).

This common row weight satisfies 0≤Ωret≤10\le\Omega_{\mathrm{ret}}\le1. The full kernel in (18.30) remains on every retained term. All subsequent signed Fourier separations are performed one retained λ\lambda at a time, so the normalized row variable stays on a fixed log box; Ωret\Omega_{\mathrm{ret}} records their sum and common domain. There are O(log⁡Z)O(\log Z) relevant retained dyads in the bounded polynomial ranges. The preceding j=0j=0 term is exactly the diagonal of the same final Φ2\Phi_2 ball, including the previously added Gauss row zero; neither zero term is restored on a different domain.

Now write u=D2au=D_2a, v=E2bv=E_2b, extracting the genuine complete common support, so that (a,b)=1(a,b)=1 and (ab,D2E2)=1(ab,D_2E_2)=1. Allocate all extracted powers to the plain variables and slots as at the first transform. Lemma 13.4 applies on this genuine locus and gives

F(D2a,E2b;j)=F(D2,E2;j)R(a,E2)R(b,D2)‾R(a,b)χa(j)χb(−j)‾.F(D_2a,E_2b;j)=F(D_2,E_2;j)\mathcal R(a,E_2) \overline{\mathcal R(b,D_2)}\mathcal R(a,b) \chi_a(j)\overline{\chi_b(-j)}.

It permits arbitrary prime powers in all four moduli and leaves a row scalar at the common primes. Every extracted prime punctures all remaining factors on its side, and every slot supplying that prime is frozen.

This also explains explicitly the cases where a slot shares a prime with a plain variable. If pp occurs only on one side, with full multiplicity ii, its residual factor is χp(j)i\chi_p(j)^i. Splitting ii among the two plain variables and the possible slot gives precisely the same factor by multiplicativity, including when 6∣i6\mid i and p∣jp\mid j. For example, a plain p5p^5 and a slot pp give the zero-extended factor χp(j)6\chi_p(j)^6. If pp occurs on both sides, its full powers are removed. In the unequal case i>j0≥1i>j_0\ge1, the local correlation is zero unless 6∣j06\mid j_0 and the frequency is pj0kp^{j_0}k with p∤kp\nmid k; when it is nonzero it equals

Pj0−1(P−1)χp(k)i−j0,P=qp.P^{j_0-1}(P-1)\chi_p(k)^{i-j_0},\qquad P=q_p.

This is a row scalar, even if the excess valuation on the first side came partly from a live slot. For instance i=7i=7, j0=6j_0=6 with a plain p6p^6 and slot pp leaves the scalar P5(P−1)χp(k)P^5(P-1)\chi_p(k), freezes that slot, and punctures both remaining plain variables at pp. Equal multiplicities have the scalar factors in Equation (13.8) and the same puncture conclusion. Complete rather than gcd-only extraction is what makes these local factors independent of the residual variables.

Define

c2=log⁡ZqD2,d2=log⁡ZqE2,b2=(c2+d2)/2.c_2=\log_Z q_{D_2},\qquad d_2=\log_Z q_{E_2},\qquad b_2=(c_2+d_2)/2.

Let p2p_2 be the logarithmic norm of their common radical, let Gc=(D2,E2)G_c=(D_2,E_2), and put g2=log⁡ZqGcg_2=\log_Z q_{G_c}. The correlation vanishes unless Gc∣jG_c\mid j. At a common prime with equal multiplicity i≢0(mod6)i\not\equiv0\pmod6, call the divided frequency j/Gcj/G_c a unit or nonunit according as that prime does not or does divide it. Let t2t_2 be the total radical length of these unit primes. Let VidV_{\mathrm{id}} be the product of these nonunit primes and put V=log⁡ZqVidV=\log_Zq_{V_{\rm id}}.

Equation (13.8) gives the following absolute local bounds:

common multiplicities and divided frequencyabsolute correlation bound
i=i, 6∤i, uniti=i,\ 6\nmid i,\ \text{unit}Pi−1P^{i-1}
i=i, 6∤i, nonuniti=i,\ 6\nmid i,\ \text{nonunit}PiP^i
i=i, 6∣i, eitheri=i,\ 6\mid i,\ \text{either}PiP^i
i>j0, 6∣j0, uniti>j_0,\ 6\mid j_0,\ \text{unit}Pj0P^{j_0}

Every unequal case not in the last line is zero. Fix the indicated unit/nonunit partition and write j=GcVidh′j=G_cV_{\mathrm{id}}h'. The partitioned scalar

1part(h′)F(D2,E2;GcVidh′)Zg2−t21_{\rm part}(h') \frac{F(D_2,E_2;G_cV_{\rm id}h')}{Z^{g_2-t_2}}

is defined to be zero off that partition and has modulus at most one everywhere with this definition. We do not assert the unit bound for the unpartitioned correlation on other rows. Every frozen allocation forced to be zero by the old masks is still discarded before this absolute bound is used.

The complete-support identity leaves the row factor χn(GcVidh′)\chi_n(G_cV_{\mathrm{id}}h') on each whole residual column. To count its fixed moving support, put v=GcVidv=G_cV_{\mathrm{id}} and ep=vp(v) mod 6e_p=v_p(v)\bmod 6. Products of the canonical primary generators of these good ideals are primary, so the exact all-input identity is

χn(v)=∏p∣vep≠0χn(p)ep∏p∣vep=01(n,p)=1,\chi_n(v)= \prod_{\substack{p\mid v\\e_p\ne0}}\chi_n(p)^{e_p} \prod_{\substack{p\mid v\\e_p=0}}1_{(n,p)=1},

with any unit of the original row retained in h′h'. All primes in this identity already puncture every residual factor, because they are in the genuine extracted support. The active ep≠0e_p\ne0 primes are contained in the unit set counted by t2t_2 and the nonunit set counted by VV. Equal six-divisible and unequal-minimum-six-divisible primes have ep=0e_p=0 and are represented solely by the common puncture in this fixed factor. A nonunit prime can also have ep=0e_p=0, in which case counting it in VV only enlarges the bound. This factors only χn(v)\chi_n(v): the natural row factor χn(h′)\chi_n(h'), with all its zeros, and all fixed-ray reciprocity phases remain. It does not reclassify a cancellation with the varying row as an extra puncture. Thus the full new moving support has length at most q~+wo+t2+V\widetilde q+w_o+t_2+V.

Define the nominal row and total widths by

m′=2a0−K−g−g2−V,q′=q~+wo+t2+V,M′=m′+q′=M+J−g−g2+t2≤M−σ.\begin{aligned} m'&=2a_0-K-g-g_2-V,& q'&=\widetilde q+w_o+t_2+V,\\ M'&=m'+q' =M+J-g-g_2+t_2 \le M-\sigma. \end{aligned}

Here g2≥t2g_2\ge t_2, and the definitions of gg give g−J≥σg-J\ge\sigma. The identities follow by substituting a0=A−c−wa_0=A-c-w and the definition of K0K_0 preceding Equation (18.22). Put

0≤δfr,2:=ξ2+log⁡(CdCsec)log⁡Z<ξ.0\le\delta_{\mathrm{fr},2}:=\frac{\xi}{2}+\frac{\log(C_dC_{\mathrm{sec}})}{\log Z}<\xi.

The sector constants here are those for the second transform. The retained row weight pulls back exactly to Ωret(qGcVidqh′)\Omega_{\rm ret}(q_{G_cV_{\rm id}}q_{h'}). On its support,

qh′≤CdTsecZξ/2qGcVid≤CdCsecZ2a0−K−g+ξ/2qGcVid=Zm′+δfr,2.q_{h'}\le \frac{C_dT_{\rm sec}Z^{\xi/2}}{q_{G_cV_{\rm id}}} \le\frac{C_dC_{\rm sec}Z^{2a_0-K-g+\xi/2}} {q_{G_cV_{\rm id}}} =Z^{m'+\delta_{{\rm fr},2}}.

Thus it lies in that common enclosing row ball. On a nonempty retained range define the declared nonnegative row length mact′=max⁡{0,m′+δfr,2}m'_{\mathrm{act}}=\max\{0,m'+\delta_{\mathrm{fr},2}\} and Mact′=mact′+q′M'_{\mathrm{act}}=m'_{\mathrm{act}}+q'. Nonemptiness implies m′+δfr,2≥0m' + \delta_{\mathrm{fr},2} \ge0, so 0≤Mact′−M′≤δfr,20 \le M'_{\mathrm{act}} - M' \le\delta_{\mathrm{fr},2}. Regard the pulled-back weight as zero on the rest of this enclosing ball throughout the signed calculation, and do the same for the partitioned scalar. This is an exact extension by zero. They will be replaced by their absolute bounds only after a nonnegative child norm or an exceptional absolute product has been formed. Complete extraction only shortens a plain variable or freezes an entire slot, so the surviving slot length satisfies z′≤zz' \le z.

We record every other exponent in this second transformation. The condition s∣u,vs \mid u,v has not been dropped: it implies that every prime of ss is in the second complete common radical. Thus after the complete extraction there is no remaining ss-divisibility condition on the residual columns. The number of possible radicals of length p2p_2, for this fixed ss, is O(Zp2−s0+ϵ1)O(Z^{p_2-s_0+\epsilon_1}): write that radical as sr2s\mathfrak r_2 with (s,r2)=1(s,\mathfrak r_2)=1, and count the squarefree r2\mathfrak r_2 of the remaining norm. If p2<s0p_2 < s_0 outside the fixed shell boundary, there are none. The same Rankin argument used for C,DC,D bounds their power and allocation multiplicities. Choosing the unit/nonunit partition costs at most 2ω(rad⁡(D2E2))2^{\omega(\operatorname{rad}(D_2E_2))}, another divisor-bounded factor included in ϵ1\epsilon_1. The exponents are

factorexponent
squared central normalization−a0-a_0
row Poisson factor and normalized inverse rootsK+g−a0K+g-a_0
prime density, when present−ℓ-\ell
common-support count with fixed ssp2−s0p_2-s_0
common correlationg2−t2g_2-t_2
conversion to normalized residual productsa0−b2a_0-b_2

The last line is {(a0−c2)+(a0−d2)}/2\{(a_0-c_2)+(a_0-d_2)\}/2. Their sum is

K+g−ℓ−a0+p2−s0+g2−t2−b2.K+g-\ell-a_0+p_2-s_0+g_2-t_2-b_2.

Subtracting this sum from the allowance Equation (18.25) leaves the exponent permitted for the inner plain products. This is the bound to be supplied either by smaller-width moments or by the exceptional-row estimate:

M′+Δchild,Δchild=b2−p2+w+Bc+ℓ≥w+ℓ.M'+\Delta_{\rm child},\qquad \Delta_{\rm child}=b_2-p_2+w+\mathcal B_c+\ell \ge w+\ell.

The inequality uses b2≥p2b_2 \ge p_2, since both multiplicities at each common prime are at least one. We now remove the residual coprimality before forming independent children. For the fixed genuine D2,E2D_2,E_2, define

F~D2,E2(a,b;j):=F(D2,E2;j)R(a,E2)R(b,D2)‾R(a,b)χa(j)χb(−j)‾\widetilde F_{D_2,E_2}(a,b;j) :=F(D_2,E_2;j)\mathcal R(a,E_2) \overline{\mathcal R(b,D_2)}\mathcal R(a,b) \chi_a(j)\overline{\chi_b(-j)}

on all residual pairs individually coprime to D2E2D_2E_2 and allowed by the old masks. It equals the genuine correlation only when (a,b)=1(a,b)=1. Define the remaining C2(a,b;j)\mathcal C_2(a,b;j) on all individually allowed residual pairs by the allocated convolution formulas and the old common masks, including (ab,D2E2)=1(ab,D_2E_2)=1. Keep the formal full-product norms qD2qa,qE2qbq_{D_2}q_a,q_{E_2}q_b, both inverse roots, the full smooth kernel, and the same pulled-back row weight extended by zero on its enclosing ball. For each retained row the exact identity is

∑(a,b)=1C2(a,b;j)F(D2a,E2b;j)=∑t squarefreeμ(t)∑t∣a,bC2(a,b;j)F~D2,E2(a,b;j).\sum_{(a,b)=1}\mathcal C_2(a,b;j)F(D_2a,E_2b;j) =\sum_{\mathfrak t\ {\rm squarefree}}\mu(\mathfrak t) \sum_{\mathfrak t\mid a,b}\mathcal C_2(a,b;j) \widetilde F_{D_2,E_2}(a,b;j).

This is the full Möbius indicator, not a truncation. The individual column shells and the retained row ball are finite. Its equality therefore follows by interchanging finite sums and using the genuine correlation identity only when (a,b)=1(a,b)=1. Extra common primes of t\mathfrak t are not part of the genuine D2,E2D_2,E_2 support or of its frequency restrictions. Since the residual masks already exclude that support, every nonzero t\mathfrak t is disjoint from it and from ss.

On each retained dyad, separate the full kernel and inverse roots in the normalized h′h' norm and the two whole-product norms, as for the first transform. The frozen factor GcVidG_cV_{\mathrm{id}} contributes only an outer phase to the row Fourier power. The fixed support boxes are chosen before the current live labels, so the resulting coefficient measure is common to them, to both rectangles, and to the row. Then fix t\mathfrak t. For each of its primes pp, use the exact factor-allocation identity

1p∣∏ini=∑∅≠J(−1)∣J∣+1∏i∈J1p∣ni,1_{p\mid\prod_i n_i} =\sum_{\varnothing\ne J}(-1)^{|J|+1} \prod_{i\in J}1_{p\mid n_i},

where the factors nin_i are the two plain variables and the live slots. For a selected plain variable write ni=plin_i=pl_i, with no restriction on lil_i. This extracts only a row scalar and qpitq_p^{it}, and replaces both Xi,YiX_i,Y_i by Xi/qp,Yi/qpX_i/q_p,Y_i/q_p. It introduces no one-variable puncture. A selected slot is frozen. If two distinct divisor primes select the same prime slot, the term is zero. The quotients and unselected factors may still contain pp, and may overlap the opposite side; no new coprimality is imposed. Old common masks remain common, and the product of the two new plain scales is equal in the two rectangles. The extracted row scalars, including zero scalars, are retained in the signed identity.

Only now, for a fixed retained dyad and fixed Fourier parameters, is each separated summand a product of two independent residual convolutions, where J\mathbf J records the factor allocations. Their row characters are

τ1(n)ρ(n)χn(GcVidh′),τ1(n)ρ′(n)χn(−GcVidh′),ρ,ρ′∈Θ.\tau_1(n)\rho(n)\chi_n(G_cV_{\mathrm{id}}h'),\qquad\tau_1(n)\rho'(n)\chi_n(-G_cV_{\mathrm{id}}h'),\qquad\rho,\rho'\in\Theta.

They are understood with the fixed-factor support representation above. In particular their inducing-character ratio belongs to Θ\Theta, including the supplementary factor n↦χn(−1)n\mapsto\chi_n(-1); this assertion takes no quotient at a zero. Their natural row zeros are retained. Extracting the selected factors contributes row scalars, not new factors of the residual character and not new support in q′q'. These scalars, including zeros, remain in the signed identity.

Lemma 18.2 (Common coefficient under complete extraction). For a centered input, the two transforms and the intervening Gauss-row enlargement just constructed preserve the following coefficient data. Each Gauss polynomial and each amplifier error retains (18.18), multiplied by G(u,h)G(u,h), apart from bounded frozen scalars and row scalars of modulus at most one. For an uncentered input, omit the second rectangle throughout. After the second transform and the full Möbius factor allocation, each separated child side has that coefficient form without GG and without s∣us\mid u. Every surviving slot has the child’s one whole-product character and its original coefficient νi\nu_i, with no Gauss coefficient. Within a side the plain variables have the same character, puncture mask, and norm power in both rectangles. The two sides of one squared Gauss norm may have different norm powers; their inducing characters differ by a member of Θ\Theta.

If the new inducing character belongs to Θ\Theta, fixing the live slot labels leaves the plain coefficient

ϑ(l1)ϑ(l2)1(l1l2,R∗)=1ql1l2itDb(l1,l2)\vartheta(l_1)\vartheta(l_2) 1_{(l_1l_2,\mathfrak R_*)=1}q_{l_1l_2}^{it}D_{\mathbf b}(l_1,l_2)

for one ϑ∈Θ\vartheta\in\Theta, one squarefree mask R∗\mathfrak{R}_* of polynomial norm, and one real tt. The mask may depend on the frozen row, but is common to both variables and both rectangles. All coefficients are understood with their retained frozen scalars, including zeros, and the exact normalizations recorded below.

Proof. The first-transform calculation proved the Gauss coefficient form; the local pp-power calculation proved it for each amplifier error. The genuine complete-support identity and the full Möbius allocation above proved the child form, preserving one character and norm power on each whole residual product. Thus “common” concerns one separated side; the displayed character ratio is the relation between the two sides. When the inducing character belongs to Θ\Theta, it equals some ϑ∈Θ\vartheta\in\Theta on units. Its redundant natural zeros and the fixed punctures combine into one R∗\mathfrak{R}_* of polynomial norm. For each fixed Π\Pi, multiplicativity factors its value, mask, and norm power on Πl1l2\Pi l_1 l_2 into a scalar in Π\Pi times the three factors stated in the conclusion. This proves the exceptional assertion. □

We next record the exact normalization of the two residual convolutions. Put

α1=a0−c2,α2=a0−d2,α1+α22=a0−b2.\alpha_1=a_0-c_2,\qquad\alpha_2=a_0-d_2,\qquad\frac{\alpha_1+\alpha_2}{2}=a_0-b_2.

At the entrance to the current two-transform stage, let Iin\mathcal{I}_{\mathrm{in}} be its live slot set and let X1,X2X_1,X_2 be the formal scales of its first rectangle. Their exact convention is X1X2∏i∈IinPi=ZAX_1X_2\prod_{i\in\mathcal{I}_{\mathrm{in}}}P_i=Z^A. For side j∈{1,2}j\in\{1,2\}, let Fj\mathcal{F}_j be the slots from this entrance set frozen by the first and second genuine common-support extractions, let Ij\mathcal{I}_j be the slots still live before the final t-allocation, and let Qplain,jQ_{\mathrm{plain},j} be the product of the exact norms of the plain powers extracted at those steps and at the amplifier. Slots removed in an ancestor stage are not included in Fj\mathcal{F}_j. Let TjT_j be the common formal pre-t product of the two plain scales in its rectangles; for an uncentered input use its one formal plain product. Before using slot ratios, discard a frozen-slot profile-zero term, which is identically zero by its frozen data independently of the row and live labels. Complete extraction gives the exact identities

ZA−αj=Qplain,j∏i∈Fjqpi,Z^{A-\alpha_j}=Q_{\mathrm{plain},j}\prod_{i\in\mathcal{F}_j}q_{p_i},
Tj∏i∈IjPi=ZAQplain,j∏i∈FjPi=Zαj+ej,T_j\prod_{i\in\mathcal{I}_j}P_i=\frac{Z^A}{Q_{\mathrm{plain},j}\prod_{i\in\mathcal{F}_j}P_i}=Z^{\alpha_j+e_j},
ej=∑i∈Fjlog⁡Z(qpi/Pi),∣ej∣≤θN.e_j=\sum_{i\in\mathcal F_j}\log_Z(q_{p_i}/P_i), \qquad |e_j|\le\theta_N.

The amplifier contributes only exact plain powers to this calculation. Each earlier frozen slot occurs once, even if it shared its prime with a plain. The already separated inverse roots, kernel, and fixed normalization constants remain outside eje_j.

For side jj, let dj,id_{j,i} be the product of final t-primes selected in plain ii, and let Jj⊆Ij\mathcal{J}_j\subseteq\mathcal{I}_j be the newly frozen slots. Put

aj,i=log⁡Zqdj,i,r~j=aj,1+aj,2+∑i∈Jjzi≥0,ωj=∑i∈Jjlog⁡Z(qpi/Pi).a_{j,i}=\log_Z q_{d_{j,i}},\qquad\widetilde r_j=a_{j,1}+a_{j,2}+\sum_{i\in\mathcal{J}_j}z_i\geq0,\qquad\omega_j=\sum_{i\in\mathcal{J}_j}\log_Z(q_{p_i}/P_i).

The corresponding formal scale is divided by qdj,iq_{d_{j,i}} in both rectangles. An assignment selecting one prime slot at two distinct t-primes, or a newly frozen slot with zero profile value, is identically zero from the frozen data and is discarded before these ratio bounds are used. All other extracted zeros remain until the nonnegative or absolute estimate described below.

Use lower-endpoint divisor dyads T≤qt<2TT\le q_{\mathfrak t}<2T, T≥1T\geq1, and put t−:=log⁡ZTt_-:=\log_Z T. Each dyad contains O(Zt−)O(Z^{t_-}) ideals. The actual selected product on side jj is divisible by t\mathfrak t, so

r~j+ωj=log⁡Z(qdj,1dj,2∏i∈Jjqpi)≥log⁡Zqt≥t−,\widetilde r_j+\omega_j =\log_Z\left(q_{d_{j,1}d_{j,2}} \prod_{i\in\mathcal J_j}q_{p_i}\right) \ge\log_Zq_{\mathfrak t}\ge t_-,
∣ωj∣≤θN,∣ej+ωj∣≤θN(j=1,2).|\omega_j|\le\theta_N,\qquad |e_j+\omega_j|\le\theta_N \quad(j=1,2).

The last inequality uses the disjoint subsets Fj\mathcal{F}_j and Jj\mathcal{J}_j of the current stage entrance slots. It does not include ancestor slots or fixed separation constants.

Writing Tj′=Tj/qdj,1dj,2T'_j=T_j/q_{d_{j,1}d_{j,2}}, the post formal factor product and the nominal raw child scale are

Tj′∏i∈Ij∖JjPi=Zαj+ej−r~j,Npost,j=Zαj−r~j.T'_j\prod_{i\in\mathcal{I}_j\setminus\mathcal{J}_j}P_i=Z^{\alpha_j+e_j-\widetilde r_j},\qquad N_{\mathrm{post},j}=Z^{\alpha_j-\widetilde r_j}.

Define PC,t,J(h′)P_{C,\mathfrak t,\mathbf J}(h') and PD,t,J(h′)P_{D,\mathfrak t,\mathbf J}(h') to be their residual convolutions multiplied by Npost,j−1/2N_{\mathrm{post},j}^{-1/2}. Relative to the nominal pre-normalizer Z−αj/2Z^{-\alpha_j/2}, the exact extraction coefficient on side jj is Z−r~j/2Z^{-\widetilde r_j/2}, apart from the frozen slot amplitudes, retained extracted row scalars, and already separated outer factors. These raw children retain the formal signed rectangles and are not moment-lemma invocations; their formal logarithmic lengths may be negative. No clipping has occurred.

The factor assignments are divisor-bounded for fixed NN; their total is bounded using CNω(t)≪N,aqtaC_N^{\omega(\mathfrak t)} \ll_{N,a}q_{\mathfrak t}^a for any fixed a>0a>0, not by spending a fixed exponent at each prime. The O(log⁡Z)O(\log Z) divisor dyads in the bounded column range use their existing logarithmic share. These discrete losses are separate from the numerical θN\theta_N terms.

For precision, the other common row scalar after extracting Zg2−t2Z^{g_2-t_2} is

vpart,λ(h′)=ωλ(qGcVidqh′/Tλ)1part(h′)F(D2,E2;GcVidh′)Zg2−t2ζ(h′),∣ζ(h′)∣≤1,v_{{\rm part},\lambda}(h')= \omega_\lambda(q_{G_cV_{\rm id}}q_{h'}/T_\lambda) 1_{\rm part}(h') \frac{F(D_2,E_2;G_cV_{\rm id}h')}{Z^{g_2-t_2}}\zeta(h'), \qquad |\zeta(h')|\le1,

where ζ\zeta contains the separated row phases for this dyad and these Fourier parameters. It is zero off the retained partition and enclosing ball, and ∣vpart,λ∣≤1|v_{\mathrm{part},\lambda}|\leq1. The subsequent estimates are made dyad by dyad and then summed with the already allowed O(log⁡Z)O(\log Z) mass. Split the already factorized row sum according to membership of the inducing character in Θ\Theta. On rows outside Θ\Theta, Cauchy–Schwarz yields two nonnegative child norms; on rows in Θ\Theta, take a pointwise absolute product. Only at these steps may the absolute values of the common row weight, partition scalar, or extracted row scalars be bounded by one and the rows enlarged to the common mact′m'_{\mathrm{act}} ball. This can admit extra exceptional rows that violate a former unit restriction, but the character-only count below includes them. Both sides use the same eligibility class and compare with (18.33).

Consider first rows whose child inducing character is outside Θ\Theta. The two sides have the same eligibility condition because their characters differ by a member of Θ\Theta. On such rows, first bound a centered child norm by the sum of the norms of its two rectangles; for an uncentered child there is one rectangle. For one fixed side jj and rectangle ϱ\varrho, write its pre and post formal plain scales as Sϱ,iS_{\varrho,i} and Sϱ,i′=Sϱ,i/qdj,iS'_{\varrho,i}=S_{\varrho,i}/q_{d_{j,i}}. Choose a fixed upper support endpoint BiB_i for each current plain profile type before the current row, divisor, and live labels. Omit a rectangle only when Sϱ,i′Bi<1S'_{\varrho,i}B_i<1 for some ii; then that plain factor is zero on every nonzero integral ideal. Retain equality and every other profile, mask, row-scalar, or arithmetic zero. This test is independent of the row and live labels.

For a retained rectangle put xi=log⁡ZSϱ,ix_i=\log_ZS_{\varrho,i} and yi=xi−aj,iy_i=x_i-a_{j,i}. The fixed endpoint test and aj,i≥0a_{j,i}\geq0, with HNH_N enlarged to contain the two positive parts of the upper endpoint logs, give the exact clipped identities

π0,j,ϱ=∑i=12(−xi)+,πj,ϱ=∑i=12(−yi)+,0≤π0,j,ϱ≤πj,ϱ≤θN,\pi_{0,j,\varrho}=\sum_{i=1}^{2}(-x_i)_+,\qquad \pi_{j,\varrho}=\sum_{i=1}^{2}(-y_i)_+,\qquad 0\leq\pi_{0,j,\varrho}\leq\pi_{j,\varrho}\leq\theta_N,
rclip,j,ϱ=∑i∈Jjzi+∑i=12((xi)+−(yi)+)=r~j−(πj,ϱ−π0,j,ϱ)≥0,r_{{\rm clip},j,\varrho} =\sum_{i\in\mathcal J_j}z_i+ \sum_{i=1}^2\bigl((x_i)_+-(y_i)_+\bigr) =\widetilde r_j-(\pi_{j,\varrho}-\pi_{0,j,\varrho})\ge0,
Aclip,j,ϱ=∑i=12(yi)++∑i∈Ij∖Jjzi=αj+ej−r~j+πj,ϱ=αj+ej+π0,j,ϱ−rclip,j,ϱ.\begin{aligned} A_{{\rm clip},j,\varrho} =\sum_{i=1}^2(y_i)_++\sum_{i\in\mathcal I_j\setminus\mathcal J_j}z_i =\alpha_j+e_j-\widetilde r_j+\pi_{j,\varrho}\\ =\alpha_j+e_j+\pi_{0,j,\varrho}-r_{{\rm clip},j,\varrho}. \end{aligned}

In particular the clipped total decreases by rclip,j,ϱr_{\mathrm{clip},j,\varrho} from its own pre-clipped total αj+ej+π0,j,ϱ\alpha_j+e_j+\pi_{0,j,\varrho}. Different rectangles can have different clipped totals. A retained subunit scale lies in the fixed interval [1/Bi,1][1/B_i,1], so its dilation to scale one preserves finite seminorm bounds. The row character, common mask, and surviving slot weights are unchanged. The exact coefficient from the pre-normalizer Z−αj/2Z^{-\alpha_j/2} to this standard clipped product is

Z(Aclip,j,ϱ−αj)/2=Z(−rclip,j,ϱ+ej+π0,j,ϱ)/2.Z^{(A_{\mathrm{clip},j,\varrho}-\alpha_j)/2}=Z^{(-r_{\mathrm{clip},j,\varrho}+e_j+\pi_{0,j,\varrho})/2}.

For a fixed pair of retained rectangles, suppress their rectangle indices. Equation (18.34) then bounds the paired divisor count and these coefficients by

t−−rclip,1+rclip,22+e1+π0,1+e2+π0,22≤(e1+ω1)+π1+(e2+ω2)+π22t_- -\frac{r_{{\rm clip},1}+r_{{\rm clip},2}}2 +\frac{e_1+\pi_{0,1}+e_2+\pi_{0,2}}2 \le\frac{(e_1+\omega_1)+\pi_1+(e_2+\omega_2)+\pi_2}{2}
≤2θN.\le2\theta_N.

There are at most two rectangles per side, hence at most four such pairs; their triangle factor is fixed. No common clipped reduction is used for the signed difference.

On the c2c_2 side, before the last coprimality extraction, the nominal total length is A′=α1=A−c−w−c2A'=\alpha_1=A-c-w-c_2. For the positive-slot parameters,

(A′−M′)−(A−M)=g+w−d−c2−(K0−K)−wo+g2−t2(A'-M')-(A-M)=g+w-d-c_2-(K_0-K)-w_o+g_2-t_2
≤6(w+ℓ)+δfr,1.\le6(w+\ell)+\delta_{\mathrm{fr},1}.

To prove the inequality, first use g2−t2≤c2g_2-t_2\le c_2. In the amplified main norm, w=wo=0w=w_o=0 and

g=J++2σ≤d+(K0−K)+6ℓ+δfr,1.g=J_++2\sigma\le d+(K_0-K)+6\ell+\delta_{\mathrm{fr},1}.

For an error, g≤d+(K0−K)+σ+δfr,1g\le d+(K_0-K)+\sigma+\delta_{\mathrm{fr},1}, so the excess is at most w−wo+σ+δfr,1w-w_o+\sigma+\delta_{\mathrm{fr},1}. These inequalities use d+K0−K≥−δfr,1d+K_0-K\ge-\delta_{\mathrm{fr},1} and the 1-Lipschitz property of the positive part. The three choices in Equation (18.28), together with ℓp≥σ/6\ell_p\ge\sigma/6, give w−wo+σ≤6ww-w_o+\sigma\le6w. This proves Equation (18.38).

For each retained clipped rectangle, if no slot survives, apply the completed unrestricted zero-slot assertion at the declared width Mact′M'_{\mathrm{act}}. If slots survive, first apply the algebraic mask deletion in Equations (18.4)–(18.6). It expresses this standard clipped product as natural products and only decreases its nonnegative affine expression. For each actual product, after both frequency enclosures, the t\mathfrak t-allocation, and mask deletion, let Aact,zactA_{\mathrm{act}},z_{\mathrm{act}} be its declared total and slot lengths and put

Fact=(Aact−Mact′+(6κ−1)zact)+.F_{\mathrm{act}}=\left(A_{\mathrm{act}}-M'_{\mathrm{act}}+(6\kappa-1)z_{\mathrm{act}}\right)_+.

The parent satisfies Equation (18.3). Before this mask deletion, let z′≤zz'\le z be the surviving slot length of the clipped rectangle. Equations (18.38) and (18.36), together with Mact′≥M′M'_{\mathrm{act}}\ge M', give

Aclip,j,ϱ−Mact′+(6κ−1)z′≤αj−M′+(6κ−1)z+ej+πj,ϱ−r~j−(Mact′−M′)A_{\mathrm{clip},j,\varrho}-M'_{\mathrm{act}}+(6\kappa-1)z' \le\alpha_j-M'+(6\kappa-1)z+e_j+\pi_{j,\varrho}-\widetilde r_j-(M'_{\mathrm{act}}-M')
≤6(w+ℓ)+δfr,1+ej+πj,ϱ.\le6(w+\ell)+\delta_{\mathrm{fr},1}+e_j+\pi_{j,\varrho}.

The same calculation holds on the other side with c2,d2c_2,d_2 exchanged. Taking the positive part and then deleting the fixed mask therefore gives

Fact≤6(w+ℓ)+δfr,1+(ej+πj,ϱ)+≤6(w+ℓ)+δfr,1+2θN.F_{\mathrm{act}}\le6(w+\ell)+\delta_{\mathrm{fr},1}+(e_j+\pi_{j,\varrho})_+\le6(w+\ell)+\delta_{\mathrm{fr},1}+2\theta_N.

Here zact≤z′≤zz_{\mathrm{act}}\le z'\le z. All the displayed ledgers use the fixed list of aggregate lengths

A,z,c,d,p,R,E,s0,K,w,wo,g,ℓ,c2,d2,p2,g2,t2,V.A,z,c,d,p,R,E,s_0,K,w,w_o,g,\ell,c_2,d_2,p_2,g_2,t_2,V.

Their affine coefficients and positive-part Lipschitz constants are numerical and independent of NN. The displayed frequency, raw normalization, and rectangle-clipping bounds are therefore included in C∗ξC_*\xi, for a fixed C∗≥1C_*\ge1 independent of NN, once the aggregate threshold has been imposed. The existence of this fixed error bound uses the single θN=HN/log⁡Z\theta_N=H_N/\log Z before comparing lengths, not NN separate copies of ξ\xi. We enlarge C∗C_* below to cover the fixed number of operations in a stage.

If Fact>0F_{\mathrm{act}}>0, remove whole slots from this product until the remaining product satisfies Equation (18.3) or until no slot remains. Removal here means applying the pointwise bound Equation (18.12) to the entire selected prime polynomial; no prime label is frozen. A removed slot of length dd decreases Aact+(6κ−1)zactA_{\mathrm{act}}+(6\kappa-1)z_{\mathrm{act}} by 6κd6\kappa d and contributes κd\kappa d to the squared ZZ-exponent, with the fixed seminorm and height factor retained separately. Since each slot has length at most η\eta, order the positive live lengths and take the first prefix reaching Fact/(6κ)F_{\mathrm{act}}/(6\kappa). Its preceding prefix is smaller than that threshold and its final slot has length at most η\eta. If no prefix reaches the threshold, remove all slots, whose total is smaller. Thus exactly one slot can cause an overshoot, and the total removed length dzd_z satisfies

dz≤min⁡{zact,Fact6κ+η},κdz≤Fact6+κη≤Δchild+δfr,16+θN3+η.\begin{aligned} d_z &\le\min\left\{z_{\mathrm{act}},\frac{F_{\mathrm{act}}}{6\kappa}+\eta\right\},\\ \kappa d_z &\le\frac{F_{\mathrm{act}}}{6}+\kappa\eta\le\Delta_{\mathrm{child}}+\frac{\delta_{\mathrm{fr},1}}{6}+\frac{\theta_N}{3}+\eta. \end{aligned}

If the slots disappear before the affine boundary is reached, the remaining plain lengths may be arbitrary; this is exactly why the completed smaller-width zero-slot assertion includes all lengths. Otherwise apply the positive-slot induction to the remaining product. Its slots still have their original coefficient class, and its inducing rows remain outside Θ\Theta. Cauchy–Schwarz averages the errors of the two separately clipped children, so their possibly different rectangles and slot sets do not double η\eta. Combining Equation (18.39) with the paired coefficient bound in Equation (18.37) and Mact′−M′≤δfr,2M'_{\mathrm{act}}-M'\le\delta_{\mathrm{fr},2}, the strict-edge scale cost beyond the child envelope is at most

δfr,2+δfr,16+η+7θN3.\delta_{\mathrm{fr},2}+\frac{\delta_{\mathrm{fr},1}}{6}+\eta+\frac{7\theta_N}{3}.

If no slot survives, the same bound holds without needing a greedy cost. The numerical θN\theta_N terms and the two frequency corrections give the single O(ξ+η)O(\xi+\eta) edge loss in the ϵG\epsilon_G reserve inherited from Equation (18.25) when using Equation (18.33); the existing local small-power and fixed analytic factors remain separate. The pointwise estimate is requested once for the entire removed product; its internal small-power shares may depend on NN. This one greedy operation occurs only after all boundary defects of the actual child have been included in FactF_{\mathrm{act}}. The argument for the d2d_2 side is the same with c2,d2c_2,d_2 exchanged.

We have now bounded all child rows whose inducing characters lie outside Θ\Theta using only smaller widths. For the remaining rows, the next count and volume bound handle the uncentered range; the centered range uses the subtraction retained in the coefficient lemma.

Rows with inducing characters in Θ\Theta

For this subsection, call a child row exceptional when its inducing character belongs to Θ\Theta. By the coefficient lemma, either both separated sides are exceptional or neither is. Every prime in the existing full displayed moving support is a common column zero, as is every extra common puncture. This is true initially, remains true for e,r\mathfrak e,\mathfrak r in the first transform, and remains true for an amplifier prime. For a nonzero genuine second allocation, the factors τ1(D2),τ1(E2)\tau_1(D_2),\tau_1(E_2) and the old common masks therefore force its complete radical to be disjoint from all those supports. This conclusion is made before replacing any frozen scalar by an upper bound. The artificial residual extension keeps D2,E2D_2,E_2 and those masks fixed and cannot revive an impossible allocation.

We make explicit the finite-ray reduction for row factors at the fixed primes. As in Equation (4.8), write a nonzero row as h′=εhShgoodh'=\varepsilon h_{\mathcal S}h_{\rm good}, with ϵ\epsilon a unit and the two other factors supported on S\mathcal S and its complement. For a primary element nn prime to S\mathcal S, reciprocity gives, with every zero retained,

χn(h′)=χn(εhS)R(n,hgood)∏p∣hgoodχp(n)vp(h′).\chi_n(h')=\chi_n(\varepsilon h_{\mathcal S}) \mathcal R(n,h_{\rm good}) \prod_{p\mid h_{\rm good}}\chi_p(n)^{v_p(h')}.

By Lemma 4.1, the first factor belongs to a finite family of ray characters supported on S\mathcal S after the unit and the S\mathcal S-valuations modulo six are fixed. The second belongs to the fixed reciprocity family after fixing the good ray sector. We do not absorb any moving good prime into this fixed family. The family supplied by the first factor need not be contained in Θ\Theta; there are simply finitely many such choices. Every remaining displayed good-prime factor has its actual local sextic exponent, with nontrivial exponents ramified at that prime.

Let v1v_1 be the radical length of the primes counted in VV whose equal multiplicity is one, and put f=2v1f=2v_1. At such a prime the fixed factor GcVidG_cV_{\mathrm{id}} in the row has valuation two. There is no existing moving character at that prime, and every character of Θ\Theta is unramified there. Sextic reciprocity therefore shows that exceptional induction requires

vp(h′)+2≡0(mod6),that is,vp(h′)≡4(mod6).v_p(h')+2\equiv0 \pmod{6},\qquad\text{that is,}\qquad v_p(h')\equiv4 \pmod{6}.

More generally, at every prime outside S\mathcal S, exceptional induction prescribes a single residue class modulo six for vp(h′)v_p(h'), determined by the frozen moving character and GcVidG_cV_{\mathrm{id}}. Outside their supports that residue is zero. For each of the finitely many choices at S\mathcal S and of unit and fixed-ray data, the ideal of h′h' consequently has a unique form

(h′)=h0v6,(h')=\mathfrak h_0\mathfrak v^6,

where h0\mathfrak h_0 is fixed and sixth-power-free. The displayed valuation-four conditions give qh0≥Z4v1=Z2fq_{\mathfrak h_0}\ge Z^{4v_1}=Z^{2f}. Ideal counting up to qh′≪Zmact′q_{h'}\ll Z^{m'_{\mathrm{act}}} now gives the stronger bound O(Z(mact′−2f)/6+ϵ1)O(Z^{(m'_{\mathrm{act}}-2f)/6+\epsilon_1}) on every nonempty range, with the usual bounded-scale convention. We use only the weaker bound

#{h′:qh′≪Zmact′, exceptional}≪Z(mact′−f)/6+ϵ1≤Z(m′−f)/6+δfr,2/6+ϵ1.\#\{h':q_{h'}\ll Z^{m'_{\rm act}},\ \text{exceptional}\} \ll Z^{(m'_{\rm act}-f)/6+\epsilon_1} \le Z^{(m'-f)/6+\delta_{{\rm fr},2}/6+\epsilon_1}.

If the exponent would describe a scale below one, the forced ideal h0\mathfrak h_0 makes the range empty except at the same bounded-scale boundary. This argument includes the principal character and every other member of Θ\Theta. Additional conditions at old moving primes can only reduce the count. It also covers rows admitted when the partition scalar was bounded after positivity. At a unit prime, such an added row can be exceptional even though it was absent from the original partition; no extra forcing saving from the unit set t2t_2 is used.

On exceptional rows take the absolute product for each already allocated pair of children and multiply by Equation (18.41). Let ct,J(h′)c_{\mathfrak t,\mathbf J}(h') denote its central extraction coefficient and bounded extracted scalars. For an allocation with raw reductions r~1,r~2\widetilde r_1,\widetilde r_2, ∣ct,J(h′)∣≪NZ−(r~1+r~2)/2|c_{\mathfrak t,\mathbf J}(h')|\ll_N Z^{-(\widetilde r_1+\widetilde r_2)/2} after taking absolute values. Using absolute volume rather than cancellation, the unnormalized plain difference on side jj is O(Tj′)O(T'_j) at every positive formal scale, including subunit scales, and the unnormalized live slots contribute ON(∏i∈Ij∖JjPi)O_N(\prod_{i\in\mathcal I_j\setminus\mathcal J_j}P_i). Equation (18.35) therefore gives the raw normalized volume

∣Pj,t,J(h′)∣≪NNpost,j−1/2Tj′∏i∈Ij∖JjPi=Z(αj−r~j)/2+ej|P_{j,\mathfrak t,\mathbf J}(h')| \ll_N N_{{\rm post},j}^{-1/2}T'_j \prod_{i\in\mathcal I_j\setminus\mathcal J_j}P_i =Z^{(\alpha_j-\widetilde r_j)/2+e_j}

up to the fixed seminorm and height factors, where jj denotes its CC or DD side. Thus the exponent for an allocated pair and one lower-endpoint divisor dyad, including its count, is

a0−b2+e1+e2+t−−r~1−r~2≤a0−b2+e1+(e2+ω2)≤a0−b2+2θN.a_0-b_2+e_1+e_2+t_- -\widetilde r_1-\widetilde r_2\le a_0-b_2+e_1+(e_2+\omega_2)\le a_0-b_2+2\theta_N.

Here Equation (18.34) gives t−−r~2≤ω2t_- -\widetilde r_2\le\omega_2, and r~1≥0\widetilde r_1\ge0. Consequently

∑t,J∣ct,J(h′)∣∣PC,t,J(h′)PD,t,J(h′)∣≪Za0−b2+2θN+ϵ1.\sum_{\mathfrak t,\mathbf J} |c_{\mathfrak t,\mathbf J}(h')| |P_{C,\mathfrak t,\mathbf J}(h') P_{D,\mathfrak t,\mathbf J}(h')| \ll Z^{a_0-b_2+2\theta_N+\epsilon_1}.

The displayed sum is over a fixed lower-endpoint divisor dyad; its allocations have already been included in ϵ1\epsilon_1. It does not assert an independent product before Möbius allocation. Subtracting the inner allowance from the reference volume and the nominal exceptional count gives the exact algebraic identity

m′−f6+a0−b2−(M′+Δchild)=A−56M−F1−F2,\frac{m'-f}{6}+a_0-b_2-(M'+\Delta_{\mathrm{child}})=A-\frac{5}{6}M-F_1-F_2,

where

F1=c/6+5{d+(K0−K)}/6+w/3+q~/6+wo+Bc−5g/6+ℓ,F_1=c/6+5\{d+(K_0-K)\}/6+w/3+\widetilde q/6 +w_o+\mathcal B_c-5g/6+\ell,
F2=2b2−56g2−p2+t2+V/6+f/6.F_2=2b_2-\tfrac56g_2-p_2+t_2+V/6+f/6.

The actual excess is bounded by the nominal expression in Equation (18.42) plus δfr,2/6+2θN+ϵ1\delta_{\mathrm{fr},2}/6+2\theta_N+\epsilon_1. For an explicit check, the left side of Equation (18.42) first equals

a0−2b2+p2−w−Bc−ℓ−56m′−q′−f/6.a_0-2b_2+p_2-w-\mathcal B_c-\ell -\tfrac56m'-q'-f/6.

Substitution of Equation (18.32) and K=2A−c−d+R+E−m−(K0−K)K=2A-c-d+R+E-m-(K_0-K) gives Equations (18.42)–(18.43).

The following lower bounds are the reason complete common supports do not consume the available exponent:

F1≥23(c+w)−3σ−56δfr,1,F2≥23b2.F_1\geq\frac{2}{3}(c+w)-3\sigma-\frac{5}{6}\delta_{\mathrm{fr},1},\qquad F_2\geq\frac{2}{3}b_2.

To prove the first, put D0=d+K0−KD_0=d+K_0-K, initially set g=J+g=J_+ and ℓ=0\ell=0, and recall J=D0−c−2w+woJ=D_0-c-2w+w_o. When J≥0J\geq0, direct simplification gives

F1=c+2w+q~/6+wo/6+Bc≥c+2w.F_1=c+2w+\widetilde q/6+w_o/6+\mathcal B_c \ge c+2w.

When J<0J<0, use q~≥R\widetilde{q}\geq R and

Bc+q~/6≥(3c−5D0)+/6−56δfr,1.\mathcal B_c+\widetilde q/6 \ge (3c-5D_0)_+/6-\tfrac56\delta_{{\rm fr},1}.

Indeed, the left side is at least {(3c−5d−R)++R}/6\{(3c-5d-R)_++R\}/6, which is at least (3c−5d)+/6(3c-5d)_+/6, while D0≥d−δfr,1D_0\geq d-\delta_{\mathrm{fr},1}. The positive part is 1-Lipschitz, giving the displayed correction. It follows that

F1≥c+5D0+(3c−5D0)+6+w3−56δfr,1≥23(c+w)−w3−56δfr,1.F_1\geq\frac{c+5D_0+(3c-5D_0)_+}{6}+\frac{w}{3}-\frac{5}{6}\delta_{\mathrm{fr},1}\geq\frac{2}{3}(c+w)-\frac{w}{3}-\frac{5}{6}\delta_{\mathrm{fr},1}.

The actual choices have g≤J++2σg\leq J_++2\sigma and ℓ≥0\ell\geq0. Equation (18.29) therefore bounds the additional loss from 2(c+w)/32(c+w)/3 by

w/3+5σ/3+56δfr,1≤22σ/9+56δfr,1<3σ+56δfr,1.w/3+5\sigma/3+\frac{5}{6}\delta_{\mathrm{fr},1}\leq22\sigma/9+\frac{5}{6}\delta_{\mathrm{fr},1}<3\sigma+\frac{5}{6}\delta_{\mathrm{fr},1}.

For the second inequality in Equation (18.44), compute prime by prime from the definition of F2F_2. In units of the prime’s logarithmic norm, the contributions are

common caseF2F_2b2b_2
i=ii=i, 6∤i6\nmid i, unit7i/67i/6ii
i=ii=i, 6∤i6\nmid i, nonunit(7i−5)/6+131i=1(7i-5)/6+\frac{1}{3}\mathbf{1}_{i=1}ii
i=ii=i, 6∣i6\mid i, either7i/6−17i/6-1ii
i>j0i>j_0, 6∣j06\mid j_0, uniti+j0/6−1i+j_0/6-1(i+j0)/2(i+j_0)/2

The extra 1/31/3 in the second line is f/6f/6. The first line exceeds 2b2/32b_2/3. In the second line equality holds at i=1i=1, and for i≥2i\geq2 the difference is (3i−5)/6≥0(3i-5)/6\geq0. In the third line the difference is (i−2)/2≥0(i-2)/2\geq0, because i≥6i\geq6. In the last line it is (4i−j0−6)/6≥0(4i-j_0-6)/6\geq0, because j0≥6j_0\geq6 and i≥j0+1i\geq j_0+1. Summing proves the claim.

For the uncentered range A≤5M/6A\leq5M/6, Equations (18.42)–(18.44) bound the nominal exceptional excess by 3σ+5δfr,1/63\sigma+5\delta_{\mathrm{fr},1}/6. The actual-count and aggregate support corrections recorded above are further O(ξ)O(\xi) terms in the fixed stage allowance. Together with the diagonal estimate and the smaller-width estimates, this proves the uncentered stage at the current width with the reserved terminal loss. The comparisons constructed earlier may consequently use that stage. It remains to estimate the centered exceptional terms when A>5M/6A>5M/6.

For one separated side of a fixed exceptional row, fix the live slot labels. Lemma (18.2) then gives the same character, puncture, and norm power in the two plain variables and in both rectangle terms. The next lemma shows that the coefficient of X1+itX^{1+it} in each plain sum is independent of XX, so the two product main terms agree at equal products of scales.

Lemma 18.3 (Masked rectangle cancellation). Let ϑ\vartheta range over a fixed finite set of finite-order ray characters with conductor primes in S\mathcal S. Let R∗\mathfrak{R}_* be squarefree with qR∗≤ZB∗q_{\mathfrak{R}_*} \le Z^{B_*} for a fixed B∗B_*, and let W1,W2W_1,W_2 be smooth profiles on fixed annuli. For X>0X > 0 and t∈Rt \in\mathbb{R}, define

Li(X,t):=∑lϑ(l)1(l,R∗)=1qlitWi(ql/X).\mathcal{L}_i(X,t) := \sum_l \vartheta(l)1_{(l,\mathfrak{R}_*)=1}q_l^{it}W_i(q_l/X).

Then

Li(X,t)=cϑ,R∗X1+itIi(t)+O(Zϵ1(1+∣t∣)J),\mathcal L_i(X,t) =c_{\vartheta,\mathfrak R_*}X^{1+it}I_i(t) +O\left(Z^{\epsilon_1}(1+|t|)^J\right),
∣Li(X,t)∣≪X.|\mathcal{L}_i(X,t)| \ll X.

Here JJ is fixed, the constants use finitely many seminorms, cϑ,R∗c_{\vartheta,\mathfrak{R}_*} is independent of X,tX,t, and Ii(t)I_i(t) is a fixed measure constant times ∫0∞Wi(y)yit dy\int_0^\infty W_i(y)y^{it}\,dy. Both estimates are uniform for X>0X > 0, for the stated masks, and for the finite character set.

Let DbD_{\mathbf b} be as in Equation (18.17), and put

Ui=Xi/qbi,Vi=Yi/qbi,T=U1U2=V1V2.U_i=X_i/q_{\mathfrak b_i},\qquad V_i=Y_i/q_{\mathfrak b_i},\qquad T=U_1U_2=V_1V_2.

If Ui,Vi≥ZrU_i,V_i \ge Z^r for i=1,2i=1,2 and some r≥0r \ge0, then

T−1/2∣∑l1,l2ϑ(l1)ϑ(l2)1(l1l2,R∗)=1ql1l2itDb(l1,l2)∣≪Zϵ1(1+∣t∣)2JT1/2Z−r.T^{-1/2}\left| \sum_{l_1,l_2} \vartheta(l_1)\vartheta(l_2) 1_{(l_1l_2,\mathfrak R_*)=1} q_{l_1l_2}^{it}D_{\mathbf b}(l_1,l_2) \right| \ll Z^{\epsilon_1}(1+|t|)^{2J}T^{1/2}Z^{-r}.

Without a nonnegative lower length, the same expression is O(T1/2)O(T^{1/2}).

Proof. First omit the mask. The primary generators representing ideals outside S\mathcal S, with the fixed character weight ϑ\vartheta, are a finite weighted collection of residue classes in a fixed lattice. Apply Poisson on that lattice to

fX,t(z)=qzitWi(qz/X)=Xitft(z/X),ft(z)=qzitWi(qz).f_{X,t}(z) = q_z^{it}W_i(q_z/X) = X^{it}f_t(z/\sqrt{X}), \qquad f_t(z) = q_z^{it}W_i(q_z).

The Fourier transform is X1+itf^t(X ξ)X^{1+it}\widehat f_t(\sqrt X\,\xi). Because ftf_t is supported on a fixed annulus, integration by parts for any fixed J0>2J_0 > 2 gives

∣f^t(ξ)∣≪J0(1+∣t∣)J0(1+∣ξ∣)−J0,|\widehat f_t(\xi)| \ll_{J_0} (1+|t|)^{J_0}(1+|\xi|)^{-J_0},

using finitely many seminorms of WiW_i. For X≥1X \ge1, the sum over nonzero points of the fixed dual lattice is therefore

≪(1+∣t∣)J0X∑ξ≠0(1+X∣ξ∣)−J0≪(1+∣t∣)J0\ll(1+|t|)^{J_0}X\sum_{\xi\ne0}(1+\sqrt{X}|\xi|)^{-J_0} \ll(1+|t|)^{J_0}

after increasing J0J_0 if necessary. For 0<X<10 < X < 1, both the lattice sum and its zero-frequency main term are O(1)O(1) by absolute counting on the fixed annulus. The zero frequency is cϑX1+itIi(t)c_\vartheta X^{1+it}I_i(t), where cϑc_\vartheta is the fixed weighted mean of the residue classes. This proves the unmasked version of Equation (18.45).

Now insert the mask by inclusion–exclusion. First remove from R∗\mathfrak{R}_* its primes in S\mathcal S, since every summation ideal already avoids them. Thus all divisors used below are outside S\mathcal S. With Li0\mathcal{L}_i^0 denoting the unmasked sum, multiplicativity gives

Li(X,t)=∑d∣R∗μ(d)ϑ(d)qditLi0(X/qd,t).\mathcal{L}_i(X,t) = \sum_{d\mid\mathfrak{R}_*}\mu(d)\vartheta(d)q_d^{it}\mathcal{L}_i^0(X/q_d,t).

The main coefficient is

cϑ,R∗=cϑ∑d∣R∗μ(d)ϑ(d)qd.c_{\vartheta,\mathfrak{R}_*} = c_\vartheta\sum_{d\mid\mathfrak{R}_*}\frac{\mu(d)\vartheta(d)}{q_d}.

The qditq_d^{it} from extraction has canceled the qd−itq_d^{-it} in the main term at X/qdX/q_d. This proves that the coefficient is independent of both XX and tt. The errors are multiplied by at most the number of divisors #{d:d∣R∗}≪ϵ1,B∗Zϵ1\#\{d:d\mid\mathfrak{R}_*\}\ll_{\epsilon_1,B_*} Z^{\epsilon_1}. The coefficient itself is also Zϵ1Z^{\epsilon_1}-bounded by the polynomial-size Euler-product estimate. This proves (18.45).

For (18.46), take absolute values in the original sum. It is empty below a fixed positive scale; whenever it is nonempty, ideal counting on the fixed annulus gives O(X)O(X) points. This is uniform in tt and in the mask.

The masked sum in (18.47) is exactly

L1(U1,t)L2(U2,t)−L1(V1,t)L2(V2,t).\mathcal{L}_1(U_1,t)\mathcal{L}_2(U_2,t)-\mathcal{L}_1(V_1,t)\mathcal{L}_2(V_2,t).

The two product main terms in (18.45) are both cϑ,R∗2T1+itI1(t)I2(t)c_{\vartheta,\mathfrak{R}_*}^2T^{1+it}I_1(t)I_2(t). They cancel. Each cross term with one error is bounded by Zϵ1(1+∣t∣)2JZ^{\epsilon_1}(1+|t|)^{2J} times one of U1,U2,V1,V2U_1,U_2,V_1,V_2, and the product of errors has the same bound after reducing the subsidiary power loss. If all four scales are at least ZrZ^r, each is at most TZ−rTZ^{-r}, and 1≤TZ−r1\le TZ^{-r} because T≥Z2rT\ge Z^{2r}. The difference is therefore O(Zϵ1(1+∣t∣)2JTZ−r)O(Z^{\epsilon_1}(1+|t|)^{2J}TZ^{-r}). Division by T1/2T^{1/2} proves (18.47). When no nonnegative lower length is available, (18.46) bounds each product by O(T)O(T), giving the last assertion. □

Apply this lemma to each already allocated exceptional child. The hypotheses on its coefficient and common mask follow from Lemma 18.2; in particular the main terms cancel for the same row, mask, and whole-product norm power before any absolute value. Initially all four plain lengths are at least LL. Before the selected t\mathfrak t-factors are removed, the c2c_2 side has lower plain length at least L−c−w−c2L-c-w-c_2 and nominal total length α1=a0−c2\alpha_1=a_0-c_2: no one plain loses more than the total c+w+c2c+w+c_2 extracted by the two genuine common supports and the amplifier. The other side has the analogous bounds with d2d_2. Put

r=(L−c−w−min⁡(c2,d2))+,r=(L-c-w-\min(c_2,d_2))_+,

and call the side with this reference saving the first side, relabeling its associated raw data together. If r~1<r\widetilde r_1<r, each selected plain length satisfies a1,i≤r~1a_{1,i}\le\widetilde r_1, so all four formal post plain scales have logarithmic length at least r−a1,i≥r−r~1>0r-a_{1,i}\ge r-\widetilde r_1>0. Apply (18.47) on these exact equal-product formal scales. If r~1≥r\widetilde r_1\ge r, including equality, or if r=0r=0, use the all-scale absolute-volume fallback in the same lemma. No formal centered scale is clipped in this branch, and an identically zero rectangle remains in the formal difference. The resulting saving is (r−r~1)+(r-\widetilde r_1)_+. With absolute volume on the other side, this gives the aggregate bound on each lower-endpoint divisor dyad,

∑t,J∣ct,J(h′)∣∣PC,t,J(h′)PD,t,J(h′)∣≪Za0−b2−r+2θN+ϵ1.\begin{aligned} &\sum_{\mathfrak t,\mathbf J} |c_{\mathfrak t,\mathbf J}(h')| |P_{C,\mathfrak t,\mathbf J}(h') P_{D,\mathfrak t,\mathbf J}(h')|\\ &\hspace{15mm}\ll Z^{a_0-b_2-r+2\theta_N+\epsilon_1}. \end{aligned}

Here and below a fixed polynomial in the separated heights is understood. To check the bound, the raw coefficients and volumes give the reference exponent a0−b2+e1+e2a_0-b_2+e_1+e_2 and reduction −r~1−r~2-\widetilde r_1-\widetilde r_2, while the divisor count gives t−t_-. Equation (18.34) gives the one-line inequality

t−−r~1−r~2−(r−r~1)+=(t−−r~2)−max⁡(r,r~1)≤ω2−r.t_- - \widetilde r_1-\widetilde r_2-(r-\widetilde r_1)_+ =(t_- - \widetilde r_2)-\max(r,\widetilde r_1) \le\omega_2-r.

Adding e1+e2e_1+e_2 leaves at most e1+(e2+ω2)−r≤2θN−re_1+(e_2+\omega_2)-r\le2\theta_N-r. The divisor-bounded allocations contribute only ϵ1\epsilon_1, proving Equation (18.48). This applies to the artificial terms even when quotients retain t\mathfrak t-primes, because the coefficient lemma preserves the common mask, equal product scales, and one norm power within each rectangle difference.

The live slots are summed only after the finite transform has removed their Gauss coefficients. Their unnormalized absolute sums contribute ON(∏i livePi)O_N(\prod_{i\ \mathrm{live}}P_i). Combining this with the nominal raw normalizer gives the full eje_j volume factor in Equation (18.35), as included above; it is not replaced by a factor-product normalizer. The Fourier measure was fixed before their labels, so conditioning on those labels changes neither the common mask nor the centered saving. A zero conditional slot scalar is discarded only in the present absolute bound.

Set v=c+w+min⁡(c2,d2)v=c+w+\min(c_2,d_2). By Equation (18.44), F1+F2F_1+F_2 is at least 2v/3−3σ−5δfr,1/62v/3-3\sigma-5\delta_{\mathrm{fr},1}/6, since b2≥min⁡(c2,d2)b_2\ge\min(c_2,d_2). The centered saving in Equation (18.48) now bounds the exceptional deficit, apart from 3σ3\sigma and the recorded frequency and aggregate support perturbations, by

A−56M−23v−(L−v)+≤(A−M)+.A-\frac{5}{6}M-\frac{2}{3}v-(L-v)_+\le(A-M)_+.

Indeed, for 0≤v≤L0\le v\le L the left side is A−5M/6−L+v/3A-5M/6-L+v/3, which increases with vv; for v≥Lv\ge L it is A−5M/6−2v/3A-5M/6-2v/3, which decreases. Its maximum is attained at v=L=M/4v=L=M/4 and equals A−MA-M. For positive slots, Equation (18.3) implies A≤MA\le M. For the zero-slot core, Equation (18.10) gives A−M≤δA-M\le\delta. Thus the centered exceptional terms require only the terminal loss 3σ3\sigma, or δ+3σ\delta+3\sigma in the padded core. The additional δfr,1\delta_{\mathrm{fr},1}, δfr,2\delta_{\mathrm{fr},2}, and θN\theta_N terms are included in the same C∗ξC_*\xi stage allowance. Together with Equation (18.31), this completes the centered stage at the current width.

Completion of the finite induction

We finish by verifying the quantifier order and the finite induction. Every nonterminal call is to a child with nominal width M′M' in Equation (18.32), at least σ\sigma below its parent. The declared row width is Mact′M'_{\mathrm{act}}, and all nonexceptional moment-input lengths are taken after the specified support and clipping operations. Exceptional raw scales remain formal and are not clipped. The two frequency enclosures, the aggregate support errors, and these clippings alter the width comparison by at most C∗ξC_*\xi. Choose this below σ/2\sigma/2. Every nonempty child then has nonnegative width and leaves its band of length σ/4\sigma/4. An empty nonzero-frequency range is discarded; a nonempty formal range just below scale one has already been included by its enclosing length and clipping error.

At each smaller width, Equations (18.4)–(18.6) delete the fixed extra masks before the natural positive-slot estimate. The unrestricted zero-slot assertion follows once from the padded core by reflecting at most its two plains. A centered comparison calls only the earlier uncentered stage in its band, using its strict margin. Each Gauss norm has at most one amplification, whose errors go directly to the second transform. Equation (18.39) is invoked once for each actual natural child, after all its boundary defects have been included in FactF_{\mathrm{act}}. Thus there is no same-band cycle. The integer DD defined above bounds the strict calls by D−2D-2, because each drops the width by at least σ/2\sigma/2 from an initial width at most Mmax⁡M_{\max}.

Here is why C∗C_* and the mesh can be chosen independently of the fixed slot count. Equation (18.19) bounds the entire logarithmic error of any slot subset by θN=HN/log⁡Z\theta_N=H_N/\log Z. Each extracted plain power is measured exactly, and each of the two possible plain clippings in one nonexceptional rectangle, after triangle inequality, has one fixed endpoint error. The exceptional calculation uses raw reductions and the disjoint-subset bounds without clipping. The first and second frequency enclosures use only their one aggregate outer scale and one common row dyad. All the local ledgers are affine or positive parts of affine expressions in the fixed list of aggregate lengths displayed above. Their numerical Lipschitz constants do not depend on NN; the local F2F_2 inequalities and the radical counts use exact prime norms. In particular the change in the positive-slot affine expression is at most

∣ΔM∣+∣ΔA∣+5∣Δz∣.|\Delta M|+|\Delta A|+5|\Delta z|.

because 0≤6κ−1≤50\le6\kappa-1\le5. The total change of zz is aggregated before this inequality is used. These observations give one numerical C∗C_*, enlarged for the fixed number of operations per stage, that covers all frequency, normalization, and boundary errors by C∗ξC_*\xi. The single greedy prefix contributes at most η\eta, not one η\eta per removed slot.

The analytic separations introduce no derivative-order multiple of ξ\xi. On a fixed full-product logarithmic box a radial kernel is Φ^i(Rscexp⁡(L(x)))\widehat\Phi_i(R_{\rm sc}\exp(L(\mathbf x))), where LL is a fixed linear form in the row and whole-column log norms. Every derivative is a fixed combination of Euler derivatives of Φ^i\widehat{\Phi}_i. Lemma 4.7 bounds these uniformly for all Rsc>0R_{\mathrm{sc}}>0, with any prescribed radial decay and derivative orders. One does not use the weaker bound RscJR_{\mathrm{sc}}^J for Rsc≤ZξR_{\mathrm{sc}}\le Z^\xi. After its displayed central power has been extracted, an inverse root is (qu/Za0)−1/2(q_u/Z^{a_0})^{-1/2} on the fixed box; its derivatives cost only fixed constants depending on HNH_N and their order. Lemma 4.5 uses the full weighted Fourier integral, not a supremum over heights below ZξZ^\xi. A required height degree JJ, which may depend on NN, raises an input seminorm order and a fixed constant, not a ZJξZ^{J\xi} exponent. Reflection similarly acts on at most two plains with fixed gamma shape; larger derivative orders raise finite seminorm and height orders, while the upper-annulus subshare ξ/2\xi/2 remains fixed. The fixed polynomial height factor in Equation (18.12) is integrated by these weighted Fourier measures at its required finite order, without changing the previously chosen exponent of ZZ.

The discrete label counts are also used only once. After extracting the displayed exponent for a family of common supports, divisors, or allocations, divide its absolute weighted counting measure by that total mass before applying a separated tuple seminorm. This leaves a measure of mass at most one; its already extracted exponent is not counted again in the smooth norm. Each Fourier measure is common to the live labels by the whole-product construction.

Choices before specifying the slot count. Choose the parameters in the following order. First, from the bounded real ranges and ϵ\epsilon, choose ρ,σ,δ>0\rho,\sigma,\delta>0, with δ\delta small compared to ρ,σ\rho,\sigma, so that

Tterm:=ρ+δ+ρ/6+3σ+5σ/3<ϵ/4.T_{\mathrm{term}} := \rho+\delta+\rho/6+3\sigma+5\sigma/3 < \epsilon/4.

This bounds a terminal width-floor, diagonal, or exceptional loss; the displayed frequency and numerical support corrections belong instead to the per-stage ξ\xi allowance. With DD and C∗≥1C_*\ge1 as above, choose, still before specifying NN or its fixed profiles,

ξ<min⁡{δ2,ρ30,σ4C∗,ϵ16C∗D},\xi< \min\left\{\frac{\delta}{2},\frac{\rho}{30},\frac{\sigma}{4C_*},\frac{\epsilon}{16C_*D}\right\},
η<min⁡{σ6,ϵ16C∗D},ϵ0<ϵ16C∗D.\eta< \min\left\{\frac{\sigma}{6},\frac{\epsilon}{16C_*D}\right\},\qquad \epsilon_0 < \frac{\epsilon}{16C_*D}.

These choices make the strict drop at least σ/2\sigma/2, preserve the comparison margins and padded core, and are uniform for κ∈[3/4,1]\kappa\in[3/4,1].

Choices for a fixed slot system. Now fix any ZZ-independent NN, arithmetic data, and profile windows. Form HNH_N and the finite full support boxes through depth DD. Their fixed factors exp⁡(O(HN))\exp(O(H_N)) belong to the constants. After imposing an eventual threshold log⁡Z≥CHN/ξ\log Z\ge CH_N/\xi, the threshold in Equation (18.9), and Equation (18.20), all occurring column, radical, and mask norms have bounded logarithmic ranges independent of moving labels. In those ranges choose every arbitrarily small power estimate with local shares whose sum in a stage is at most ϵ0\epsilon_0. These shares may depend on NN. For example, the two divisor masses and the at most NN frozen-slot masses in mask deletion may each use a share ϵ0/(10(N+2))\epsilon_0/(10(N+2)). In the prime estimate, the principal squared exponent is exactly κz\kappa z, and the contour displacement cost is 2ez2e z, with bounded total zz, not NηN\eta. Choose ee for its assigned share; the fixed character expansions and powers of log⁡Z\log Z are absorbed after an NN-dependent threshold. The same reasoning applies as individual ziz_i approach zero, since Pi≥1P_i\ge1. For divisor allocations use the global bounds τN+2(v)C≪N,C,aqva\tau_{N+2}(v)^C\ll_{N,C,a}q_v^a and CNω(v)≪N,aqvaC_N^{\omega(v)}\ll_{N,a}q_v^a with a sufficiently small a>0a>0, not a fixed loss at every prime. Rankin’s fixed-radical bound is treated with the same local shares. The one normalized pool average has only its single density loss in a stage.

The induction is simultaneous for every surviving subset of these original NN slots, with the same mesh. To make this precise, for 0≤d≤D−20 \le d \le D-2, let

Ed:=Tterm+(d+1)C∗(η+ξ+ϵ0)\mathcal{E}_d := T_{\mathrm{term}} + (d+1)C_* (\eta+\xi+\epsilon_0)

be the permitted error when at most dd strict calls remain. A terminal group, including its bounded reflection or comparison preprocessing, has error at most E0\mathcal{E}_0. A strict edge and its fixed number of same-band operations use the child envelope Ed−1\mathcal{E}_{d-1} plus at most C∗(η+ξ+ϵ0)C_*(\eta+\xi+\epsilon_0), giving Ed\mathcal{E}_d. The Gauss allowance ϵG\epsilon_G in (18.23) denotes this appropriate envelope and the current local shares; it is not a request to reapply the moment lemma with an NN-dependent loss and a new mesh. Triangle inequalities take the maximum error up to the already counted mass, and Cauchy–Schwarz averages the errors of the two children. Consequently one terminal loss occurs along a branch, not at every ancestor. The largest path error is at most Tterm+C∗D(η+ξ+ϵ0)<ϵT_{\mathrm{term}}+C_*D(\eta+\xi+\epsilon_0)<\epsilon by (18.52).

Finally choose the required finite kernel, reflection, prime, and terminal seminorm and polynomial-height orders backwards through these DD stages. The full weighted Fourier estimates and uniform Euler-kernel estimates above make every such choice finite. Choose one final lower threshold for the aggregate support inequalities, pool separation and density, the raw frequency tails, and all fixed logarithmic losses. The orders, constants, and threshold may grow with NN and the fixed data, but η\eta, ξ\xi, DD, C∗C_* in the exponent comparison do not.

Each new extra mask is supported on frozen columns or a frozen amplifier prime, and its logarithmic norm increases by a bounded total length at a stage. It is fixed within every child row sum. The only row-dependent zeros there are the natural zeros of the row; the declared moving zeros remain in the fixed twist and remain counted. Over depth DD the masks remain of polynomial norm. On an exceptional row, the redundant part of the full moving union and the row radical, together with these extra masks, forms the common polynomial-size R∗\mathfrak{R}_*; the lattice cancellation is uniform for it. The fixed-numerator ray lemma controls the finite choices at S\mathcal{S}, without absorbing a moving good prime into a fixed modulus.

When this estimate and the inverse moment are applied together, all internal orders in both arguments, including the reflection-kernel orders, are fixed first. The later external Fourier-tail order in Lemma 4.5 lies outside this internal propagation: it raises only the external input seminorm and does not change a previously fixed internal height order. This proves the asserted finite-order uniformity. The finite induction proves the natural assertion, and the initial mask deletion proves Lemma 18.1 in its full stated form.

For the later physical application, q=0q=0 and the row uu is sixth-power-free. If a prime outside S\mathcal{S} has valuation 1,…,51,\ldots,5 in uu, its local character has order 6/gcd⁡(6,vp(u))>16/\gcd(6,v_p(u))>1, so the inducing character cannot belong to Θ\Theta. The exceptional physical rows are therefore supported on S\mathcal{S}; sixth-power-freeness makes this a finite set, up to the finite unit group. With abstract moving twists, additional exceptional rows can arise by cancellation. They were included in (18.41) and the fixed-character volume argument.

Prime amplitudes and refined row counts

We use the current Part II arithmetic data and the physical slots of (12.5). Instantiate the shared zero detector of Section 8 with these same fixed data. The main and error factors below belong to the retained dynamic decomposition in (16.10); no individual local quotient is asserted outside that region. Every retained external coordinate obeys the single height allocation in (10.14).

Prime amplitudes

For a main physical slot of scale Pi=ZℓiP_i = Z^{\ell_i}, write its central factor as

Qi(u;z)=Pi−1/2∑p∈1Tχp(u)‾Wi(qp/Pi)(qp/Pi)z−1.Q_i(u;z)=P_i^{-1/2}\sum_{p\in1_T} \overline{\chi_p(u)}W_i(q_p/P_i)(q_p/P_i)^{z-1}.

The main part Qi\mathcal Q_i in Proposition 16.1 is exactly

Qi(u;z)=−∑p∈1Tχp(u)‾qpz−1Wi(qp/Pi)=−Piz−1/2Qi(u;z).\mathcal Q_i(u;z)=-\sum_{p\in1_T}\overline{\chi_p(u)}q_p^{z-1}W_i(q_p/P_i) =-P_i^{z-1/2}Q_i(u;z).

As in Section 12, each sum over p∈1Tp\in1_T retains the same allowed set Pi(Z)\mathcal{P}_i(Z), including its exclusion of SS. The original zero extension is retained, so a prime dividing uu does not contribute to this main slot. The real part of zz is in a fixed bounded range and its imaginary part is one of the external frequencies restricted by the common height allowance.

Lemma 19.1 (Prime bound in a bin). Under the hypotheses of Lemma 8.2, with the prime-annulus Mellin frequency included in its cumulative allowance, for every ϵ1>0\epsilon_1>0

∣Qi(u;z)∣≪A,e,ϵ1Uϵ1Pia−1/2+O(e).|Q_i(u;z)|\ll_{\mathcal A,e,\epsilon_1} U^{\epsilon_1}P_i^{a-1/2+O(e)}.

The implied O(e)O(e) is uniform for 51/100≤a≤151/100\leq a\leq1 and the fixed real ranges. It holds for every main slot in the row.

Proof. Expand 1p∈1T=∣T∣−1∑θ∈T^θ(p)1_{p\in1_T}=|T|^{-1}\sum_{\theta\in\widehat T}\theta(p). Every resulting prime character belongs to Xu\mathcal{X}_u. Lemma 4.9, applied to the buffered disks, bounds its logarithmic derivative on ℜs=a+8e\Re s=a+8e by OA,e(log⁡U)O_{\mathcal A,e}(\log U); the logarithmic derivative of the deleted product has the same bound. Mellin inversion of the corresponding smooth von Mangoldt annulus, shifted only in the retained central range, gives Uϵ1Pia−1/2+O(e)U^{\epsilon_1}P_i^{a-1/2+O(e)} after normalization. The pure twist (qp/Pi)iℑz(q_p/P_i)^{i\Im z} is translated into the logarithmic-derivative argument before the added Mellin frequency is truncated. The joins have bounded real length. On them the logarithmic derivative is OA,e(log⁡U)O_{\mathcal A,e}(\log U) inside its allocated buffer, while on the starting line ℜs=2\Re s=2 it is absolutely bounded. Apply the pointwise estimate in (4.11) to the untwisted transform for the joins, and (4.10) for the absolute-line tails. Choosing the external order after their fixed polynomial scale and height bounds gives the asserted estimate.

To pass from von Mangoldt coefficients to primes, divide the annular weight by log⁡(Piy)\log(P_i y). On the fixed annulus,

(y∂y)j1log⁡(Piy)=(−1)jj!{log⁡(Piy)}j+1,(y\partial_y)^j\frac{1}{\log(P_i y)}=\frac{(-1)^j j!}{\{\log(P_i y)\}^{j+1}},

so this preserves every fixed smooth seminorm for sufficiently large PiP_i, without introducing a power of PiP_i depending on the derivative order. Bounded PiP_i are handled by absolute counting. Prime powers contribute Pio(1)P_i^{o(1)} after central normalization, since their number in a norm annulus is O(Pi1/2+o(1))O(P_i^{1/2+o(1)}). The polynomial-size punctures and their zero extensions are already included in the logarithmic derivative. This proves the bound. □

Here is a precise amplitude subdivision. Choose a fixed bin width ϑ>0\vartheta>0. First reduce ee and ϵ1\epsilon_1, after the slot lengths have been fixed, so that the preceding bound is at most Piδ/2+ϑP_i^{\delta/2+\vartheta} for all sufficiently large ZZ. This is possible because log⁡U/log⁡Pi=d/ℓi\log U/\log P_i=d/\ell_i stays in a fixed bounded range for each fixed mesh. For a main slot with Qi≠0Q_i\ne0, put

gi=min⁡{δ2,max⁡(0,ϑ⌊log⁡∣Qi∣ϑlog⁡Pi⌋)}.g_i=\min\left\{\frac{\delta}{2}, \max\left(0,\vartheta \left\lfloor\frac{\log|Q_i|}{\vartheta\log P_i}\right\rfloor \right)\right\}.

Put gi=0g_i=0 if Qi=0Q_i=0, and also put gi=0g_i=0 for an error slot from (16.9). Then, for a main slot,

∣Qi∣≤Pigi+ϑ,gi>0⟹∣Qi∣≥Pigi.|Q_i| \le P_i^{g_i+\vartheta}, \qquad g_i>0 \Longrightarrow|Q_i| \ge P_i^{g_i}.

No lower bound is asserted for a slot with gi=0g_i=0. The finitely many possible vectors (gi)(g_i), with the possible endpoint value δ/2\delta/2, partition the rows into amplitude bins. Define their length-weighted mean by

q=∑iℓigiℓ,0≤q≤δ/2,ℓ=∑iℓi.q=\frac{\sum_i \ell_i g_i}{\ell}, \qquad0\le q\le\delta/2,\qquad\ell=\sum_i \ell_i.

This qq records prime amplitude; it is not the conductor exponent denoted qq in the auxiliary fourth moment.

Selected prime slots and the row counts

Use Δ\Delta and κ\kappa from (12.1):

0<Δ≤124,κ=2β∗−1=34+2Δ∈(3/4,5/6],α:=56.0<\Delta\le\frac{1}{24},\qquad\kappa=2\beta_* -1=\frac{3}{4}+2\Delta\in(3/4,5/6],\qquad\alpha:=\frac{5}{6}.

The parameter κ\kappa remains dynamic; α\alpha is the fixed slope from sixth-power amplification. Since κ<1\kappa<1 and β∗=(1+κ)/2\beta_*=(1+\kappa)/2, the positive-slot hypothesis of Lemma (18.1) is satisfied by equality. Equation (12.2) gives δ≤κ≤α\delta\le\kappa\le\alpha for the current Part II bins, including the possible endpoint δ=α\delta=\alpha.

Fix a dynamic and amplitude bin and fix the external physical Mellin parameters. Write zphysz_{\mathrm{phys}} for the fixed third Mellin parameter, so the physical slots are Qi(u;zphys)Q_i(u;z_{\mathrm{phys}}). All gig_i, and hence qq, are now fixed within its row sum. At base UU, the length of slot ii is wi=ℓi/dw_i=\ell_i/d, and the total available length is ℓ/d\ell/d. For a requested length 0≤z≤ℓ/d0\le z\le\ell/d, order the positive gig_i decreasingly and fill zz fractionally in that order. The gained exponent is at least qzqz: if positive slots suffice to fill zz, their initial weighted average is at least the average qq of all slots; otherwise retaining them all gives gain qℓ/d≥qzq\ell/d\ge qz. Removing the one possibly fractional slot loses at most (max⁡iwi)δ/2(\max_i w_i)\delta/2. Thus a fixed subcollection of whole positive slots of length at most zz satisfies

∣∏i selectedQi∣2≥U2qz−δmax⁡iwi.\left|\prod_{i\ \mathrm{selected}} Q_i\right|^2\ge U^{2qz-\delta\max_i w_i}.

When a strict moment inequality is needed, we first replace zz by z−ν0z-\nu_0 for a fixed small ν0>0\nu_0>0, or select no slot if z≤ν0z\le\nu_0. The resulting loss in this display is at most 2qν0+δmax⁡iwi2q\nu_0+\delta\max_i w_i, except in the stated zero-capacity neighborhood, where an unweighted moment will be used. Both losses can be made smaller than any prescribed positive power.

The selected factors have exactly the coefficient class required by the moments. Conjugate both witness factors, including their profiles, if necessary and write their row character as ψ(n)=ν(n)χn(u)‾\psi(n)=\nu(n)\overline{\chi_n(u)}, ν∈Θ\nu\in\Theta. Relative to this row, a physical prime has coefficient

ν(p)‾1p∈1T=1∣T∣∑θ∈T^(ν‾θ)(p).\overline{\nu(p)}1_{p\in1_T} =\frac1{|T|}\sum_{\theta\in\widehat T} (\overline{\nu}\theta)(p).

This is a fixed finite combination of members of Θ\Theta; it is independent of the moving row in the fixed row sum. There is no requirement that η(p)=1\eta(p)=1. The factor (qp/Pi)zphys−1(q_p/P_i)^{z_{\mathrm{phys}}-1} is part of its smooth profile. Underlying prime supports remain disjoint before masks. The marked moment permits this negative common row orientation. To apply Lemma (18.1), whose row character has positive orientation, conjugate the whole product of both plain witness factors and all selected prime factors. Its absolute square is unchanged, and its common row character becomes ψ(n)‾=ν(n)‾χn(u)\overline{\psi(n)}=\overline{\nu(n)}\chi_n(u). Both witness profiles and every selected slot profile are conjugated, and each selected slot coefficient becomes ν(p)1p∈1T\nu(p)1_{p\in1_T}, again a fixed finite combination of members of Θ\Theta. Conjugation retains all zero extensions and underlying prime supports. It also preserves whether the inducing character belongs to Θ\Theta, since Θ\Theta is a group. The witness and physical heights need not be equal. Apply Lemma 4.5 to the rowwise witness parameters after fixing the physical parameters and selected indices. Derivatives in those parameters insert only logarithmic profile weights. The cost is a fixed power of 1+T11+T_1, uniform over moving rows and outer labels. Every retained large row induces outside Θ\Theta, because it ramifies at a prime outside SS. Thus the z>0z>0 family condition of Lemma 18.1 holds.

For an actual plain length m≤1/2m\le1/2, its largest zero-loss capacity from Lemma 18.1, at effective row width one, is

zP(m)=1−2m6κ=1−2m9/2+12Δ.z_P(m)=\frac{1-2m}{6\kappa}=\frac{1-2m}{9/2+12\Delta}.

Indeed the moment is applied to two copies of the plain witness, so its condition is 2m+6κz≤12m+6\kappa z\le1. For an inverse witness of length r<1r<1, put zM(r)=(1−r)/2z_M(r)=(1-r)/2. We use this capacity only where the second strict inequality in Lemma 17.1 also has a fixed margin.

Proposition 19.2 (Row counts from the witnesses). Let B\mathcal{B} be a fixed dynamic and amplitude bin of retained sixth-power-free physical rows qu≍U=Zdq_u\asymp U=Z^d, with a>51/100a>51/100, 0<δ=2a−1≤α0<\delta=2a-1\le\alpha, and mean amplitude q∈[0,δ/2]q\in[0,\delta/2]. Put x=q/δx=q/\delta, so 0≤x≤1/20\le x\le1/2, and define

Dx=3−17x9,Px=(2−8x9)(1−x).D_x=3-\frac{17x}{9},\qquad P_x=\left(2-\frac{8x}{9}\right)(1-x).

Assume the total available prime length exceeds 7/377/37 by a fixed positive amount. For every t∈[1,3/2]t\in[1,3/2] and every ϵ>0\epsilon>0, the capacity decrements and slot mesh can be chosen using only ϵ\epsilon, Δ\Delta and the bounded real ranges so that

#B≪A,ϵUmax⁡{Rshort(t),L(t)}+Δ/4+ϵ(1+T1)AA,\#\mathcal B\ll_{\mathcal A,\epsilon} U^{\max\{R_{\rm short}(t),L(t)\}+\Delta/4+\epsilon} (1+T_1)^{A_{\mathcal A}},

where AA<∞A_{\mathcal A}<\infty is uniform over moving rows and

Rshort(t)=1−δ+δPxDx(3/2−t),L(t)=1−δ+(α−δ)(t−1).R_{\mathrm{short}}(t)=1-\delta+\frac{\delta P_x}{D_x}(3/2-t),\qquad L(t)=1-\delta+(\alpha-\delta)(t-1).

The estimate is valid for the rowwise witnesses of Proposition 8.3, with its height condition. If no prime slots are selected, then t=1t=1 instead gives

#B≪A,ϵU1−2δ/3+ϵ(1+T1)AA,\#\mathcal B\ll_{\mathcal A,\epsilon} U^{1-2\delta/3+\epsilon}(1+T_1)^{A_{\mathcal A}},

without a prime-supply hypothesis. At zero inverse capacity use Lemma 17.6; at zero plain capacity use the zero-slot case of Lemma 18.1.

Proof. Subdivide by the witness presentation and dyadic pair. The number of choices is OA((log⁡U)2)O_{\mathcal A}((\log U)^2); the remaining rowwise smooth parameters are handled by the preceding Sobolev argument. Work in one subdivision, denoting it again by B\mathcal{B}, and let r,mr,m be the actual lengths from Proposition 8.3. Whenever the selected slots satisfy the corresponding moment hypotheses and have total requested capacity zz, their spike and the individual witness spikes imply, after reducing preliminary losses,

#B≪U1−δr−2qz+ϵ(1+T1)AA,from Lemma 17.1,\#\mathcal B\ll U^{1-\delta r-2qz+\epsilon}(1+T_1)^{A_\mathcal A},\qquad\text{from Lemma 17.1,}
#B≪U1−2δm−2qz+ϵ(1+T1)AA,from Lemma 18.1.\#\mathcal B\ll U^{1-2\delta m-2qz+\epsilon}(1+T_1)^{A_\mathcal A},\qquad\text{from Lemma 18.1.}

In the second line use two copies of SmS_m, so the denominator is ∣Sm∣4\lvert S_m\rvert^4, not ∣Sm∣2\lvert S_m\rvert^2. The effective width is one because the twist ν\nu is fixed within the row sum and has no moving conductor radical. Each formula includes the arbitrarily small capacity, rounding, moment, and witness losses.

Inverse witnesses without selected primes. Whenever no inverse slot is selected, use instead the sixth-power amplification of Lemma 17.6. It applies to these physical rows because their ideal valuations are at most five and their original zero extensions are unchanged. After the present subdivision, U,t,D,D∗U,t,D,D_\ast are common, and the inverse base profile is

Wbase(y)=W1(y)V≤(Dy/D∗).W_{\mathrm{base}}(y)=W_1(y)V_{\leq}(Dy/D_\ast).

Its fixed logarithmic seminorms are uniformly bounded: a derivative of the second factor is supported where its scaled argument lies in a fixed compact interval. The remaining rowwise parameters are σ\sigma in a fixed compact interval and the pure twist −(γ−ν)-(\gamma-\nu), of absolute value at most (3I+1)T1(3I+1)T_1. The rowwise assertion of Lemma 17.6 therefore applies with that height range. Replacing its factor (1+(3I+1)T1)A(1+(3I+1)T_1)^A by (3I+2)A(1+T1)A(3I+2)^A(1+T_1)^A changes only a fixed constant.

For clarity, this use is uniform even when rr approaches one with UU. If 0≤r≤R00\leq r\leq R_0, (17.88) with preliminary loss ϵ0\epsilon_0 has exponent

max⁡{1,1+5(1+c)r6}+(1+r)ϵ0≤e(r)+5cR06+(1+R0)ϵ0,e(r)=max⁡{1,1+5r6}.\max\left\{1,\frac{1+5(1+c)r}{6}\right\}+(1+r)\epsilon_0 \leq e(r)+\frac{5cR_0}{6}+(1+R_0)\epsilon_0,\qquad e(r)=\max\left\{1,\frac{1+5r}{6}\right\}.

For a requested loss ϵm>0\epsilon_m>0, take, for example, c=3ϵm/(10max⁡{R0,1})c=3\epsilon_m/(10\max\{R_0,1\}) and ϵ0=ϵm/(4(1+R0))\epsilon_0=\epsilon_m/(4(1+R_0)). These are fixed before UU, and the two extra terms are at most ϵm/2\epsilon_m/2. Thus division by the inverse witness spike gives

#B≪Ue(r)−δr+ϵ(1+T1)AA,\#\mathcal B\ll U^{e(r)-\delta r+\epsilon}(1+T_1)^{A_{\mathcal A}},
e(r)−δr={1−δr,0≤r≤1,1−α+(α−δ)r,r≥1.e(r)-\delta r= \begin{cases} 1-\delta r,&0\leq r\leq1,\\ 1-\alpha+(\alpha-\delta)r,&r\geq1. \end{cases}

In particular this is not an application of the strict marked moment with the shrinking margin 1−r1-r.

Cases requiring no selected primes. We first dispose of the cases in which a witness already gives the required count without selecting primes. For r≥1r\geq1, (19.3) uses effective moment exponent (1+5r)/6=1−α+αr(1+5r)/6=1-\alpha+\alpha r. Division by the inverse spike gives 1−α+(α−δ)r1-\alpha+(\alpha-\delta)r. Because δ≤α\delta\leq\alpha and r≤t+O(ϵ)r\leq t+O(\epsilon), this is at most

L(t)=1−α+(α−δ)t=1−δ+(α−δ)(t−1)L(t)=1-\alpha+(\alpha-\delta)t=1-\delta+(\alpha-\delta)(t-1)

up to O(ϵ)O(\epsilon). This includes r=1r=1, where the two branches in (19.3) agree. If m≥1/2m\geq1/2, the zero-slot case of Lemma 18.1 gives count exponent 1−2δm≤1−δ1-2\delta m\leq1-\delta. Since Rshort(t)≥1−δR_{\mathrm{short}}(t)\geq1-\delta, this also satisfies the stated bound. We may therefore assume for the remaining argument that

r<1,m<1/2.r<1,\qquad m<1/2.

Both capacities zM(r)z_M(r) and zP(m)z_P(m) are then positive; when either is too small for the fixed decrement, we will use its unweighted estimate below.

Comparing the positive capacities. For the inverse capacity zM(r)z_M(r), the resulting ideal exponent is AI(r)A_I(r) below. To compare the plain exponent first replace zP(m)z_P(m) by its value at Δ=0\Delta=0, namely 2(1−2m)/92(1-2m)/9. Since the actual mm is at least t−r−O(ϵ)t-r-O(\epsilon), the resulting ideal comparison exponent is

AI(r)=1−δ{x+(1−x)r},A_I(r)=1-\delta\{x+(1-x)r\},
St(r)=1−δ{4x9+(2−8x9)(t−r)}.S_t(r)=1-\delta\left\{\frac{4x}{9}+\left(2-\frac{8x}{9}\right)(t-r)\right\}.

Both the actual plain exponent 1−2δm−2q(1−2m)/(9/2+12Δ)1-2\delta m-2q(1-2m)/(9/2+12\Delta) and its baseline version decrease with mm: their derivatives are respectively

−2δ+4q9/2+12Δ<0,−2δ+8q9<0.-2\delta+\frac{4q}{9/2+12\Delta}<0,\qquad-2\delta+\frac{8q}{9}<0.

The O(ϵ)O(\epsilon) replacement of mm is therefore legitimate.

The two affine expressions in Equation (19.5) cross at

r∗(t)=(2−8x/9)t−5x/9Dx.r_*(t)= \frac{(2-8x/9)t-5x/9}{D_x}.

Here Dx≥37/18>0D_x\ge37/18>0. Directly,

r∗(3/2)=1,r∗(1)=2−13x/93−17x/9≥2337,r_*(3/2)=1,\qquad r_*(1)=\frac{2-13x/9}{3-17x/9}\ge\frac{23}{37},

and

t−r∗(t)=(1−x)t+5x/9Dx.t-r_*(t)=\frac{(1-x)t+5x/9}{D_x}.

The last expression is increasing in tt, equals 1/21/2 at t=3/2t=3/2, and at t=1t=1 is (1−4x/9)/(3−17x/9)≥1/3(1-4x/9)/(3-17x/9)\ge1/3. Thus, throughout the stated ranges,

r∗(t)≥2337,13≤t−r∗(t)≤12,r∗(t)≤1.r_*(t)\ge\frac{23}{37},\qquad \frac13\le t-r_*(t)\le\frac12,\qquad r_*(t)\le1.

Use the plain count when r≤r∗(t)r\le r_*(t), and the inverse count when r∗(t)≤r<1r_*(t)\le r<1, except within the fixed small zero-capacity neighborhoods. On the inverse side r≥23/37r\ge23/37. After decreasing zM(r)z_M(r) by ν0\nu_0,

1−r−2z≥2ν0>0,3−2r−8z=4(1−r−2z)+(2r−1)>0.1-r-2z\ge2\nu_0>0,\qquad3-2r-8z=4(1-r-2z)+(2r-1)>0.

The second inequality has a margin at least 9/379/37 before its positive first term. These are precisely the two strict width conditions of Lemma 17.1 at row width one. The inverse capacity is at most (1−23/37)/2=7/37(1-23/37)/2=7/37. On the plain side, m≥1/3−O(ϵ)m\ge1/3-O(\epsilon), so its capacity is at most 2/27+O(ϵ)2/27+O(\epsilon). At d=hd=h the available length is

ℓh=839,839−737=231443>0.\frac{\ell}{h}=\frac8{39},\qquad \frac8{39}-\frac7{37}=\frac{23}{1443}>0.

The assumed positive supply margin and a sufficiently fine mesh therefore permit every selection just made.

On the plain side, replacing the baseline capacity by the actual capacity in Equation (19.2) raises the count exponent by

2q(1−2m)(29−19/2+12Δ)=24q(1−2m)Δ(9/2)(9/2+12Δ)≤Δ4+O(ϵ).2q(1-2m)\left(\frac{2}{9}-\frac{1}{9/2+12\Delta}\right)=\frac{24q(1-2m)\Delta}{(9/2)(9/2+12\Delta)} \le\frac{\Delta}{4}+O(\epsilon).

For the inequality use m≥1/3−O(ϵ)m\ge1/3-O(\epsilon), 2q≤12q\le1, and the lower bound four for each denominator. The constants in the O(ϵ)O(\epsilon) term are uniform.

The weighted average

Rshort(t)=(2−8x/9)AI(r)+(1−x)St(r)Dx=1−δ+δPxDx(3/2−t).\begin{aligned} R_{\mathrm{short}}(t)=\frac{(2-8x/9)A_I(r)+(1-x)S_t(r)}{D_x} \\ &=1-\delta+\frac{\delta P_x}{D_x}(3/2-t). \end{aligned}

is independent of rr: the rr-coefficients cancel, and the weights sum to DxD_x. It is the common value at r∗(t)r_*(t). Since StS_t is increasing in rr and AIA_I is decreasing, the chosen short count is at most Rshort(t)+Δ/4+O(ϵ)R_{\mathrm{short}}(t)+\Delta/4+O(\epsilon).

Small capacities and the conclusion. If r<1r < 1 but zM(r)≤ν0z_M(r) \le\nu_0, the same no-slot estimate, using e(r)=1e(r) = 1, gives

1−δr≤1−δ+2δν0.1-\delta r \le1-\delta+2\delta\nu_0.

If zP(m)≤ν0z_P(m) \le\nu_0, then 1−2m≤6κν0≤6ν01-2m \le6\kappa\nu_0 \le6\nu_0, and its count is at most 1−δ+6δν01-\delta+6\delta\nu_0. Since Rshort(t)≥1−δR_{\mathrm{short}}(t) \ge1-\delta, choosing ν0\nu_0 within the prescribed ϵ\epsilon preserves the short bound. Finally, r=1/2−O(ϵ)r = 1/2-O(\epsilon) and t≥1t \ge1 force m≥1/2−O(ϵ)m \ge1/2-O(\epsilon), so the same unweighted plain estimate applies. No negative capacity is requested. Together with the cases requiring no selected primes, this proves the stated selected count after adding the finitely many subdivisions.

Finally, use no prime slots and take t=1t = 1. For the inverse side use (19.3), including e(r)=1e(r) = 1 for every r≤1r \le1; for the plain side use the zero-slot case of Lemma 18.1. The same short calculation with selection gain zero, that is, with x=0x = 0 in the two comparison lines, gives Rshort(1)=1−2δ/3R_{\mathrm{short}}(1) = 1-2\delta/3; the long bound is L(1)=1−δL(1) = 1-\delta. Neither input has a prime-supply hypothesis, proving the final assertion.

Remark 19.3 (Unselected inverse witnesses beyond the Part II bin ceiling). The derivation of (19.3) uses only the inverse spike from Proposition 8.3 and Lemma 17.6. It can therefore be repeated for any instance of the shared detector satisfying those hypotheses, independently of the current Part II bin ceiling. Consequently, for each fixed t∈[1,3/2]t \in[1,3/2], the bound in (19.3) holds on each fixed presentation/dyadic subdivision of a fixed dynamic bin of retained rows with actual witnesses from that proposition whenever

a>51/100,1/50<δ=2a−1≤1,a > 51/100,\qquad1/50 < \delta= 2a-1 \le1,

and rr lies in the prescribed bounded nonnegative range. It uses the common inverse profile WbaseW_{\mathrm{base}}, rowwise parameter bounds, and witness loss and height hypotheses used in the preceding proof, but requires neither δ≤α\delta\le\alpha nor a prime-supply hypothesis. This conclusion does not include all rows in the floor bin a=51/100a = 51/100, which need not have an actual witness.

The formulas in Proposition 19.2 describe the only row exponents needed below. The cardinality factor (1+T1)AA(1+T_1)^{A_{\mathcal A}} is kept explicit here. We verify the additional target-dependent height ceiling required by Lemma 11.1. Let ϵht>0\epsilon_{\mathrm{ht}} > 0 be the minimum of the finitely many detector height allowances already chosen with the real losses. For the fixed target, after the internal profile orders are fixed, let Aht,η≥0A_{\mathrm{ht},\eta} \ge0 dominate their finitely many height orders. Set

τ0,η:=dmin⁡ϵht20(Aht,η+1)>0.\tau_{0,\eta} := \frac{d_{\min}\epsilon_{\mathrm{ht}}}{20(A_{\mathrm{ht},\eta}+1)} > 0.

For 0<τ≤τ0,η0 < \tau\le\tau_{0,\eta}, T1=ZτT_1 = Z^\tau, and sufficiently large ZZ, the inequality U≥Zdmin⁡U \ge Z^{d_{\min}} gives

(1+T1)Aht,η≤2Aht,ηZdmin⁡ϵht/20≤Uϵht/10.(1+T_1)^{A_{\mathrm{ht},\eta}} \le2^{A_{\mathrm{ht},\eta}} Z^{d_{\min}\epsilon_{\mathrm{ht}}/20} \le U^{\epsilon_{\mathrm{ht}}/10}.

Thus this ceiling enforces all the preceding detector height hypotheses. It is fixed before the external tail order and ZZ; increasing that order changes only external test seminorms, not these internal height orders. Lemma 11.1 then makes the final height choice without changing the positive real margins or the slot mesh.

The seven-eighths bound

We complete the contradiction assumed in Part II. Recall from Equations (12.1) and (12.2) that

0<Δ=β∗−78≤124,κ=34+2Δ≤56,δ=2a−1≤κ0 < \Delta= \beta_*-\frac{7}{8} \le\frac{1}{24},\qquad\kappa= \frac{3}{4}+2\Delta\le\frac{5}{6},\qquad\delta= 2a-1 \le\kappa

for every retained bin. The compensated low estimate is Proposition 15.3. For the same physical probe, we first normalize the principal term of its high expansion, then bound the remaining rows and verify the target-independent margins required by Proposition 2.1.

The geometry and Mellin exponent are

h=1316,ℓ=16,lx=1748,ly=2348,h=1−lx+ℓ,h=\frac{13}{16},\qquad \ell=\frac16,\qquad l_x=\frac{17}{48},\qquad l_y=\frac{23}{48},\qquad h=1-l_x+\ell,
C(s)=CII(s)=s−1116,C(7/8)=316.C(s)=C_{\mathrm{II}}(s)=s-\frac{11}{16},\qquad C(7/8)=\frac{3}{16}.

These are the values in Equations (12.4) and (12.3). Write ss for the local variable called xx in Section 16; the amplitude ratio x=q/δx=q/\delta below is a different real number.

Use Definition 10.1 with

Iη(Z)=Iη,modified(Z),Hη,u,Z(s,w,z) as in Equation (16.3).\mathscr I_\eta(Z)=I_{\eta,\mathrm{modified}}(Z),\qquad\mathfrak H_{\eta,u,Z}(s,w,z)\ \text{as in Equation (16.3)}.

In the shared analytic lemmas take σ0=7/8\sigma_0=7/8. Section 16 verifies every part of these data: Equation (16.7) is the absolutely convergent high identity for the independently defined finite expression in Equation (12.5), and the full correction is holomorphic in the two required Euler regions and satisfies Equation (10.4). The excluded set, physical row masks, and calibration are unchanged. In particular there is no additional Euler factor outside this full correction. Its scalar denominator is LFS(s,ηχ∙(u)‾)L_F^S(s,\eta\overline{\chi_\bullet(u)}), and its Gaussian is Φ(s+z−1)\Phi(s+z-1).

In the estimates below, 0<e<10−30<e<10^{-3} is an admissible detector width. Its final choice, together with the remaining real losses, is made in the concluding order of choices.

The principal normalizer

We verify the two correction hypotheses of Lemma 10.5. First, Equation (16.14) gives

∣Hη,1,Z(s,w,z)∣≪Zℓℜz|\mathfrak H_{\eta,1,Z}(s,w,z)|\ll Z^{\ell\Re z}

uniformly in all imaginary parts on every fixed real box in the second Euler region. In particular this holds on the entire rectangle in Equation (10.17), with height degree zero. This is a bound for the full tuple correction.

For the residue value, define

Si(Z)=∑p∈Pi(Z)Wi(qp/Pi)qp−5/6,Pi=Zℓi.S_i(Z)=\sum_{p\in\mathcal{P}_i(Z)}W_i(q_p/P_i)q_p^{-5/6},\qquad P_i=Z^{\ell_i}.

Lemma 13.1, including its assertion about deletion of a fixed finite set, gives

Si(Z)∼Pi1/6∣T∣log⁡Pi∫0∞Wi(y)y−5/6 dy.S_i(Z)\sim\frac{P_i^{1/6}}{|T|\log P_i}\int_0^\infty W_i(y)y^{-5/6}\,dy.

Each leading constant is positive. Since the slot count is fixed, all Si(Z)S_i(Z) are positive for every sufficiently large ZZ, with a common lower threshold allowed to depend on the fixed data. Set

AT(Z)=(−1)KZ−ℓ/6∏i=1KSi(Z).A_T(Z)=(-1)^K Z^{-\ell/6}\prod_{i=1}^{K}S_i(Z).

Using log⁡Pi=ℓilog⁡Z\log P_i=\ell_i\log Z and ∑iℓi=ℓ\sum_i\ell_i=\ell, we obtain

AT(Z)∼(−1)K∣T∣K(log⁡Z)K∏i=1K{1ℓi∫0∞Wi(y)y−5/6 dy}.A_T(Z)\sim\frac{(-1)^K}{|T|^K(\log Z)^K}\prod_{i=1}^{K}\left\{\frac{1}{\ell_i}\int_0^\infty W_i(y)y^{-5/6}\,dy\right\}.

Consequently AT(Z)≠0A_T(Z)\ne0 on that range and

∣AT(Z)∣≍T,K,(ℓi,Wi)(log⁡Z)−K,∣AT(Z)∣−1≪ϵZϵ|A_T(Z)|\asymp_{T,K,(\ell_i,W_i)}(\log Z)^{-K}, \qquad |A_T(Z)|^{-1}\ll_\epsilon Z^\epsilon

for every ϵ>0\epsilon> 0. The lower threshold may depend on the target’s finite excluded set; no uniform prime asymptotic in a moving ray conductor is being used.

On the principal second Euler region, Section 16 defines Bp=Gp/Hp\mathcal B_p=G_p/H_p with Hp≠0H_p \ne0, and (16.13) gives Bp=−1+O(qp−7/8)\mathcal B_p=-1+O(q_p^{-7/8}), uniformly in all imaginary parts and target unit phases. Apply the principal factorization in (16.12) at w=1w = 1, z=1/6z = 1/6, where it remains valid even if the original quotient by PpP_p was undefined. It gives

Hη,1,Z(s,1,1/6)=Hη(s)∏i=1K(∑p∈Pi(Z)Wi(qp/Pi)qp−5/6Bp),\mathfrak H_{\eta,1,Z}(s,1,1/6) =H_\eta(s)\prod_{i=1}^K \left(\sum_{p\in\mathcal P_i(Z)} W_i(q_p/P_i)q_p^{-5/6}\mathcal B_p\right),

where HηH_\eta is the function in (10.1) for this same excluded set SS. By nonnegativity of WiW_i, its iith slot equals

−Si(Z){1+ρi(s)},∣ρi(s)∣≪Pi−7/8(ℜs=β∗+e, ℑs∈R).-S_i(Z)\{1+\rho_i(s)\},\qquad|\rho_i(s)|\ll P_i^{-7/8}\quad(\Re s=\beta_*+e,\ \Im s\in\mathbb{R}).

Indeed the sum of the absolute local errors is at most a fixed multiple of Pi−7/8Si(Z)P_i^{-7/8}S_i(Z). Choose any pretarget number

0<κP<78min⁡iℓi.0<\kappa_P<\frac{7}{8}\min_i\ell_i.

Since KK is fixed, Rη,Z(s):=∏i(1+ρi(s))−1\mathcal{R}_{\eta,Z}(s):=\prod_i(1+\rho_i(s))-1 satisfies ∣Rη,Z(s)∣≪Z−κP|\mathcal{R}_{\eta,Z}(s)|\ll Z^{-\kappa_P} on that entire line. Thus the exact residue correction is

Hη,1,Z(s,1,1/6)=Hη(s)Zℓ/6AT(Z){1+Rη,Z(s)},\mathfrak{H}_{\eta,1,Z}(s,1,1/6)=H_\eta(s)Z^{\ell/6}A_T(Z)\{1+\mathcal{R}_{\eta,Z}(s)\},

which is (10.18) with Aη=ATA_\eta=A_T and μ=κP\mu=\kappa_P. This factorization is asserted only at the principal residue; it is not the correction used for general contour moves.

Let cS>0c_S>0 be the scalar in (10.1), whose positivity is part of Lemma 10.5. For sufficiently large ZZ, define the normalized physical probe

JII,η(Z)=Iη,modified(Z)cSAT(Z).J_{\mathrm{II},\eta}(Z)=\frac{I_{\eta,\mathrm{modified}}(Z)}{c_SA_T(Z)}.

This is distinct from JI,ηJ_{\mathrm{I},\eta}, and both its numerator and normalizer are independent of the analysis height T1T_1. Proposition 15.3 and the subpower bound for AT−1A_T^{-1} give, for every ϵ>0\epsilon>0,

∣JII,η(Z)∣≪η,ϵZC(7/8)+ϵ.|J_{\mathrm{II},\eta}(Z)|\ll_{\eta,\epsilon} Z^{C(7/8)+\epsilon}.

The same scalar is used for the high comparison.

Choose the fixed cutoff as required for (10.2). The associated HηH_\eta is holomorphic on ℜs>7/8\Re s>7/8, satisfies the contraction there, and uses this same SS. Let PII,η\mathscr P_{\mathrm{II},\eta} denote the u=1u=1 term of (16.7), and set

fII,η(Z)=12πi∫(2)ZC(s)e(s−5/6)2Hη(s)LFS(s,η) ds.f_{\mathrm{II},\eta}(Z)=\frac{1}{2\pi i}\int_{(2)}Z^{C(s)}e^{(s-5/6)^2}\frac{H_\eta(s)}{L_F^S(s,\eta)}\,ds.

All hypotheses of Lemma 10.5 have now been verified with σ0=7/8\sigma_0=7/8. Its remainder estimate is

∣PII,η(Z)cSAT(Z)−fII,η(Z)∣≪ZC(β∗)+(1+h)e−mw+ϵ+ZC(β∗)+e−mz+ϵ+ZC(β∗)+e−κP+ϵ,\begin{aligned} \left|\frac{\mathscr P_{\mathrm{II},\eta}(Z)}{c_S A_T(Z)} -f_{\mathrm{II},\eta}(Z)\right| \ll{}& Z^{C(\beta_*)+(1+h)e-m_w+\epsilon} +Z^{C(\beta_*)+e-m_z+\epsilon}\\ &+Z^{C(\beta_*)+e-\kappa_P+\epsilon}, \end{aligned}

where the two geometric margins are

mw:=ly20=23960,mz:=h600=139600.m_w:=\frac{l_y}{20}=\frac{23}{960},\qquad m_z:=\frac h{600}=\frac{13}{9600}.

Lemma 10.5 includes the residue paths, the scalar Jacobian, and the rightward shift of the main integral. In particular the last term is the error estimated on its original global line; it is not part of fII,ηf_{\mathrm{II},\eta}. Both this signal and the physical probe are independent of T1T_1.

The compensated high exponent

The low estimate and the principal-row comparison now concern the functions JII,ηJ_{\mathrm{II},\eta} and fII,ηf_{\mathrm{II},\eta} required by the continuation criterion. It remains to prove, for a common σ>0\sigma> 0,

∣Iη,modified(Z)−PII,η(Z)cSAT(Z)∣≪ηZC(β∗)−σ.\left|\frac{I_{\eta,\mathrm{modified}}(Z) -\mathscr P_{\mathrm{II},\eta}(Z)}{c_S A_T(Z)}\right| \ll_\eta Z^{C(\beta_*)-\sigma}.

We estimate these nonprincipal contributions first relative to the raw scale ZC(7/8)Z^{C(7/8)}. Division by cSAT(Z)c_S A_T(Z) costs an arbitrarily small power, reserved once in the final choice of margins.

Lemma 20.1 (A high exponent for one row bin). Let 0<dmin⁡<dmax⁡<∞0 < d_{\min} < d_{\max} < \infty, let U=ZdU = Z^d with dmin⁡≤d≤dmax⁡d_{\min} \le d \le d_{\max}, and let B\mathcal{B} be the finite set of retained nonprincipal physical rows qu≍Uq_u \asymp U in one fixed dynamic bin (i,a)(i,a). Put δ=2a−1\delta= 2a - 1. Assume the bin and height hypotheses of Lemmas 8.18.1, 8.28.2, and 19.119.1, with 0<e<10−30 < e < 10^{-3}, T1=Zτ>2T_1 = Z^\tau> 2, 0<τ≤dmin⁡/1000 < \tau\le d_{\min}/100, and the cumulative allocation in (10.14). The bounded real ranges, the positive losses ee, ϑ\vartheta, ϵ\epsilon, and the slot system are fixed before the target.

For each retained tuple of external parameters and each subset of error slots, partition B\mathcal{B} pointwise into the amplitude sets of Section 19.1, and into the witness subdivisions of Section 19.2 when a witness count is used. Suppose each such set C\mathcal{C} has main-slot mean q∈[0,δ/2]q \in[0,\delta/2], as in (19.1), and

#C≪A,ϵUR+ϵ(1+T1)AA,\#\mathcal C\ll_{\mathcal A,\epsilon} U^{R+\epsilon}(1+T_1)^{A_{\mathcal A}},

uniformly in the retained tuple and moving labels. The occurring R,qR,q range over a fixed bounded set and may depend on the pointwise set, dd, aa, and β∗\beta_*, but not otherwise on the target. For each occurring pair define

E(d)=a−78+h(1750−16)−aly−(1−a)ℓ−(δ/2−q)ℓ+d(R+δ2−1750)=C0+23δ+q6−h(1−R)+(d−h)(R+δ2−1750),C0=−148.\begin{aligned} E(d) &= a-\frac{7}{8}+h\left(\frac{17}{50}-\frac{1}{6}\right)-a l_y-(1-a)\ell-(\delta/2-q)\ell+d\left(R+\frac{\delta}{2}-\frac{17}{50}\right) \\ &= C_0+\frac{2}{3}\delta+\frac{q}{6}-h(1-R)+(d-h)\left(R+\frac{\delta}{2}-\frac{17}{50}\right), \qquad C_0=-\frac{1}{48}. \end{aligned}

If B≠∅\mathcal{B}\ne\varnothing, let Emax⁡,Z(d)E_{\max,Z}(d) be the supremum of these values over all pointwise sets at all retained tuples.

On the central contours

ℜs=a+16e,ℜw=1−a−6e,ℜz=1750,\Re s=a+16e,\qquad\Re w=1-a-6e,\qquad\Re z=\frac{17}{50},

the contribution of the original fixed dynamic-bin sum is bounded by

ZC(7/8)+Emax⁡,Z(d)+O(e+ϑ+ϵ)(1+T1)AA′,Z^{C(7/8)+E_{\max,Z}(d)+O(e+\vartheta+\epsilon)} (1+T_1)^{A'_{\mathcal A}},

where ϑ\vartheta is the amplitude-bin width and AA′<∞A'_{\mathcal A}<\infty is uniform in moving labels. An empty bin contributes zero. The constant in the O(e+ϑ+ϵ)O(e+\vartheta+\epsilon) term depends only on the bounded real ranges and the fixed slot system, not on the target. No separate integral of an individual pointwise set is asserted. After fixing τ>0\tau>0, all discarded external pieces and joins are OA,N(ZBT1−N)O_{\mathcal A,N}(Z^B T_1^{-N}), for a fixed BB and every fixed NN.

Proof. We verify the central hypothesis of Lemma 10.4, which supplies the contour move and its tails for the full correction just specified. Its bin ceiling holds by (12.2). The physical ℑz\Im z coordinate is included in its height allocation because it enters the prime profiles. The other witness, dyadic, and prime-annulus coordinates are the fixed finite list used in the estimates of Section 19.2. Their complete pointwise bounds include the discarded auxiliary integrals on global or absolute lines. Thus the single cumulative allocation in (10.14) applies, without renewing an allowance at a later estimate. Only on the retained contours, Proposition 16.1 gives the decomposition in (16.10). For I⊆{1,…,K}I \subseteq\{1,\ldots,K\}, its summand is

Hη,u,Z(I)=Hη,u(s,w,z)∏i∈IDi(u)∏i∉IQi(u;z).\mathfrak H_{\eta,u,Z}^{(I)} =\mathcal H_{\eta,u}(s,w,z) \prod_{i\in I}\mathcal D_i(u) \prod_{i\notin I}\mathcal Q_i(u;z).

The required reflected primitive numerator bound follows from the buffered estimate for the numerator presentation and its conjugate, together with Lemma 4.10, as verified before Proposition 16.1. The retained ww heights lie in its allowed set. Every retained numerator is nonprincipal. Fix one amplitude set at one retained tuple. For a main slot, Qi=−Piz−1/2Qi\mathcal{Q}_i=-P_i^{z-1/2}Q_i and ∣Qi∣≤Pigi+ϑ\lvert Q_i\rvert\le P_i^{g_i+\vartheta}. Assign gi=0g_i=0 to an error slot. Equation (16.9) bounds all error slots in II jointly with the numerator; its proof uses the actual conductor deficit in Equation (16.11) simultaneously for the distinct strict ramified labels. It is not a separate numerator allowance for each slot. Since Hη,u≪ϵUϵ\mathcal{H}_{\eta,u}\ll_\epsilon U^\epsilon, multiplication of these estimates gives, after choosing the preliminary powers,

∣LS(w,χ∙(u))Hη,u,Z(I)(s,w,z)∣≪Uδ/2+O(e)+ϵ(1+T1)A1⋅Zℓ(17/50−1/2)+qℓ+O(e+ϑ+ϵ).\begin{aligned} \left|L^S(w,\chi_\bullet(u)) \mathfrak H_{\eta,u,Z}^{(I)}(s,w,z)\right| \ll{}&U^{\delta/2+O(e)+\epsilon}(1+T_1)^{A_1}\\ &\cdot Z^{\ell(17/50-1/2)+q\ell+O(e+\vartheta+\epsilon)}. \end{aligned}

Here A1<∞A_1<\infty is a fixed height order for the target and slot system, and ∑iℓigi=qℓ\sum_i\ell_i g_i=q\ell, including the assigned zeros for the errors. No lower bound on an error slot has been used.

Multiplying by the assumed cardinality proves Equation (10.13) with g=qℓg=q\ell, after taking ϵc\epsilon_c to be a fixed sufficiently large multiple of e+ϑ+ϵe+\vartheta+\epsilon. This multiple depends only on the fixed slot system and the bounded real ranges. There are 2K2^K error subsets. The number of amplitude vectors is fixed, and the witness dyadic choices contribute only a fixed power of 1+log⁡Z1+\log Z. Thus the required pointwise multiplicity bound holds. These sets are formed only after Lemma 10.4 has moved the original dynamic-bin sum using H\mathfrak H. They are not used for continuation and are not integrated separately.

Apply Lemma 10.4 with σ0=7/8\sigma_0=7/8 and g=qℓg=q\ell. Its exponent in Equation (10.15) is

a−78+h(1750−16)−aly−ℓ2+qℓ+d(R+δ2−1750).a-\frac78+h\left(\frac{17}{50}-\frac16\right)-a l_y-\frac{\ell}{2} +q\ell+d\left(R+\frac\delta2-\frac{17}{50}\right).

Because −(1−a)ℓ−(δ/2−q)ℓ=−ℓ/2+qℓ-(1-a)\ell-(\delta/2-q)\ell=-\ell/2+q\ell, this is the first line of Equation (20.4). Substituting the geometry and a=(1+δ)/2a=(1+\delta)/2 gives its second line. In particular qℓ=q/6q\ell=q/6 is a base-ZZ exponent, not dq/6dq/6. The explicit errors in Equation (10.16) are O(e+ϑ+ϵ)O(e+\vartheta+\epsilon) on the bounded dd-range after the remaining preliminary powers are chosen. Its supremum is exactly the one in the statement. Lemma 10.4 also gives the stated external tails with a scale degree fixed before NN.

The floor bin a=51/100a=51/100 has δ0=1/50\delta_0=1/50 and requires no zero witness. The ideal count R=1R=1, together with q≤δ0/2q\le\delta_0/2, gives

E(h)≤C0+34δ0=−71200<0.E(h)\le C_0+\frac{3}{4}\delta_0=-\frac{7}{1200}<0.

Its frequency slope R+δ0/2−17/50R+\delta_0/2-17/50 is positive, so this bounds every d≤hd\le h. A small extension above hh will be controlled below.

Small and large row norms

Set dmin⁡=1/100d_{\min}=1/100. Lemma 16.2 bounds the positive sum of the full selected tuples, with every GpG_p retained before taking absolute values. On the small-row lines

ℜs=β∗+e,ℜw=1/2,ℜz=17/50\Re s=\beta_*+e,\qquad\Re w=1/2,\qquad\Re z=17/50

Equation (16.15) gives

∣Hη,u,Z(s,w,z)∣≪εUε∏iPi17/50=UεZ17ℓ/50.|\mathfrak{H}_{\eta,u,Z}(s,w,z)| \ll_{\varepsilon} U^{\varepsilon}\prod_i P_i^{17/50}=U^{\varepsilon}Z^{17\ell/50}.

uniformly in all imaginary parts. This is Equation (10.20), with height degree zero. It remains valid at zeros of individual local factors. The data for Lemma 10.6 were already verified above, so it applies to every physical row u≠1u \ne1 in these dyads. Its classification includes nontrivial unit numerators and permits a principal denominator; no detector witness or selected moment is used here.

The dd-independent part of the relative exponent is

h(1750−16)−ly2=−79800.h\left(\frac{17}{50}-\frac{1}{6}\right)-\frac{l_y}{2}=-\frac{79}{800}.

The row exponent in Equation (10.21) is 63/50<263/50 < 2. Thus the small dyadic sum in Equation (10.22), measured relative to C(β∗)C(\beta_\ast), has exponent at most

−79800+2dmin⁡+O(e+ε)=−63800+O(e+ε).-\frac{79}{800}+2d_{\min}+O(e+\varepsilon)=-\frac{63}{800}+O(e+\varepsilon).

It is negative after the adjustable real losses are made sufficiently small. Write msmall:=63/800m_{\mathrm{small}}:=63/800 for this fixed error-free saving.

For the large rows, fix z∞>2z_\infty>2. On (ℜs,ℜw,ℜz)=(2,2,z∞)(\Re s,\Re w,\Re z)=(2,2,z_\infty), the same Equation (16.15) gives

∣Hη,u,Z(s,w,z)∣≪εUεZℓz∞|\mathfrak{H}_{\eta,u,Z}(s,w,z)|\ll_{\varepsilon} U^{\varepsilon}Z^{\ell z_\infty}

for every physical row and all imaginary parts. This verifies Equation (10.23). Lemma 10.6 therefore gives, with B0=lx/2+1+ly=53/32B_0=l_x/2+1+l_y=53/32,

∣Rη(U;Z)∣≪ZB0+hz∞+ϵU1+ϵ−z∞,|\mathscr R_\eta(U;Z)| \ll Z^{B_0+hz_\infty+\epsilon}U^{1+\epsilon-z_\infty},

and, for every fixed ζ>0\zeta>0 after choosing 0<ε<z∞−10<\varepsilon<z_\infty-1,

∑U>Zh+ζ∣Rη(U;Z)∣≪ZB0+(h+ζ)(1+ϵ)−ζz∞+ϵ.\sum_{U>Z^{h+\zeta}}|\mathscr R_\eta(U;Z)| \ll Z^{B_0+(h+\zeta)(1+\epsilon)-\zeta z_\infty+\epsilon}.

Here Rη\mathscr R_\eta is the row contribution of Lemma 10.6 for the present physical expression. A fixed sufficiently large z∞z_\infty makes the last exponent as negative as required. It is chosen after ζ\zeta but before the target. These invocations use the quotient-free tuple bounds in Section 16, not the central main/error factorization.

The endpoint inequality

We next bound E(h)E(h), first without adjustable losses or height factors. They will be restored with a quantified order of choices. Recall

κ=34+2Δ,α=56.\kappa=\frac{3}{4}+2\Delta,\qquad\alpha=\frac{5}{6}.

At the live upper endpoint δ=α\delta=\alpha, take t=3/2t=3/2 in Proposition 8.3. Then r≥1−O(ε)r\ge1-O(\varepsilon). Apply the no-slot amplified estimate in Equation (19.3) on both sides of r=1r=1. For r≥1r\ge1, its exponent is

1−α+(α−δ)r=1−δ.1-\alpha+(\alpha-\delta)r=1-\delta.

For r<1r<1 in the stated O(ε)O(\varepsilon) neighborhood, the same estimate uses e(r)=1e(r)=1, so its exponent is 1−δr≤1−δ+O(ε)1-\delta r\le1-\delta+O(\varepsilon). The fixed amplification margin is independent of this neighborhood.

Thus no selected primes are needed and the ideal row exponent is R=1−δR=1-\delta. Using q≤δ/2q\le\delta/2 in (20.4) gives

E(h)≤C0+(34−h)δ+O(ϵ)=−148−δ16+O(ϵ)<0.E(h)\le C_0+\left(\frac{3}{4}-h\right)\delta+O(\epsilon)=-\frac{1}{48}-\frac{\delta}{16}+O(\epsilon)<0.

Now assume 1/50<δ<α1/50<\delta<\alpha. Put x=q/δ∈[0,1/2]x=q/\delta\in[0,1/2], and use Dx,Px,Rshort,LD_x,P_x,R_{\mathrm{short}},L from Proposition 19.2. The parameter κ\kappa remains the dynamic value 3/4+2Δ3/4+2\Delta, not the upper bound 5/65/6. Thus the actual plain capacity used in that Proposition is

zP(m)=1−2m6κ=1−2m9/2+12Δ,z_P(m)=\frac{1-2m}{6\kappa}=\frac{1-2m}{9/2+12\Delta},

as in (19.2). The comparison in (19.6) is for this exact capacity and raises the row exponent by at most Δ/4\Delta/4, apart from requested small losses. Define

J=(α−δ)Dx+δPx,t=1+δPx2J,R∗=L(t).\mathcal{J}=(\alpha-\delta)D_x+\delta P_x,\qquad t=1+\frac{\delta P_x}{2\mathcal{J}},\qquad R_\ast=L(t).

The denominator is positive. Indeed

3718≤Dx≤3,79≤Px≤2,Dx−Px=1+x−8x29>0,\frac{37}{18}\le D_x\le3,\qquad\frac{7}{9}\le P_x\le2,\qquad D_x-P_x=1+x-\frac{8x^2}{9}>0,

and consequently

3554≤J≤52.\frac{35}{54}\le\mathcal{J}\le\frac{5}{2}.

Because 0<δ<α0<\delta<\alpha, one has J>δPx>0\mathcal{J}>\delta P_x>0, so 1<t<3/21<t<3/2. Furthermore,

Dx{Rshort(t)−L(t)}=δPx(3/2−t)−(α−δ)Dx(t−1)=δPx2−J(t−1)=0.D_x\{R_{\mathrm{short}}(t)-L(t)\}=\delta P_x(3/2-t)-(\alpha-\delta)D_x(t-1)=\frac{\delta P_x}{2}-\mathcal{J}(t-1)=0.

Thus R∗=Rshort(t)=L(t)R_\ast=R_{\mathrm{short}}(t)=L(t) and this tt balances the two counts. The formulas also have the stated closed-endpoint values: at δ=α\delta=\alpha, one has J=αPx\mathcal{J}=\alpha P_x, t=3/2t=3/2, and R∗=Rshort(3/2)=L(3/2)=1−δR_\ast=R_{\mathrm{short}}(3/2)=L(3/2)=1-\delta. The corresponding crossing has r∗(3/2)=1r_\ast(3/2)=1, so its inverse capacity is zero. The preceding equality argument uses (19.3) at that boundary, not a marked estimate with a vanishing margin.

Lemma 20.2 (Compensated endpoint certificate). For 0≤δ≤5/60\le\delta\le5/6 and 0≤x≤1/20\le x\le1/2, define J,t,R∗\mathcal{J},t,R_\ast by (20.8) where J>0\mathcal{J}>0, and let E∗E_\ast be E(h)E(h) with q=xδq=x\delta and R=R∗R=R_\ast. Then

−E∗≥49440640>110000.-E_\ast\ge\frac{49}{440640}>\frac{1}{10000}.

In particular the bound is uniform on the range 1/50<δ≤5/61/50<\delta\le5/6, including the closed endpoint.

Proof. Set y=1/2−x∈[0,1/2]y=1/2-x\in[0,1/2] and v=51+41yv=51+41y. To verify the calculation, write

py=7+18y+8y2,jy=185+170y+(−138+12y+96y2)δ.p_y=7+18y+8y^2,\qquad j_y=185+170y+(-138+12y+96y^2)\delta.

Then

Dx=37+34y18,Px=py9,J=jy108.D_x=\frac{37+34y}{18},\qquad P_x=\frac{p_y}{9},\qquad\mathcal{J}=\frac{j_y}{108}.

From R∗=1−δ+(α−δ)δPx/(2J)R_\ast=1-\delta+(\alpha-\delta)\delta P_x/(2\mathcal{J}) and (20.4),

−E∗=1+(3+8y)δ48−1332(5/6−δ)δPxJ.-E_\ast=\frac{1+(3+8y)\delta}{48}-\frac{13}{32}\frac{(5/6-\delta)\delta P_x}{\mathcal{J}}.

Multiplying out gives the explicit quadratic

10368J(−E∗)=2jy[1+(3+8y)δ]−468(5/6−δ)δpy=10(37+34y)−8(237+377y+26y2)δ+48(51+131y+94y2+32y3)δ2.10368\mathcal{J}(-E_*) = 2j_y[1 + (3 + 8y)\delta] - 468(5/6 - \delta)\delta p_y = 10(37 + 34y) - 8(237 + 377y + 26y^2)\delta + 48(51 + 131y + 94y^2 + 32y^3)\delta^2.

Multiplication by vv and completion of the square yields

10368vJ(−E∗)=(3+5y){(4vδ−79)2+49}+4y{4vδ[(1+3y)(15+32y)δ+9−13y]+265+3485y}.\begin{aligned} 10368v\mathcal J(-E_*) ={}&(3+5y)\bigl\{(4v\delta-79)^2+49\bigr\}\\ &+4y\bigl\{ 4v\delta[(1+3y)(15+32y)\delta+9-13y] +265+3485y\bigr\}. \end{aligned}

This identity can also be checked by coefficients: expansion of its right side as a polynomial in δ\delta gives respectively

10v(37+34y),10v(37 + 34y),
−8v(237+377y+26y2),-8v(237 + 377y + 26y^2),
48v(51+131y+94y2+32y3),48v(51 + 131y + 94y^2 + 32y^3),

which are the constant, linear, and quadratic coefficients in the preceding display multiplied by vv.

Every term on the right of Equation (20.9) is nonnegative: y,δ≥0y,\delta\ge0 and 9−13y≥5/29 - 13y \ge5/2. The first line is at least 49(3+5y)49(3 + 5y), while v=51+41y≤17(3+5y)v = 51 + 41y \le17(3 + 5y). Hence

−E∗≥49176256J≥49440640>110000,-E_*\ge\frac{49}{176256\mathcal J} \ge\frac{49}{440640}>\frac1{10000},

using J≤5/2\mathcal{J} \le5/2.

The lower bounds for DxD_x and J\mathcal{J} bound all derivatives of the crossing and cutoff on the compact parameter ranges. The saturation losses are uniform because δ≥1/50\delta\ge1/50, and the inverse selection has the explicit supply and width margins proved in Proposition 19.2. At a zero capacity its unweighted bound differs from 1−δ1-\delta by at most a constant times the chosen capacity decrement. Since R∗≥1−δR_* \ge1-\delta, these cases obey the same comparison. Thus all detector, bin, and rounding errors have a total O(ϵ)O(\epsilon) with a target-independent constant once their individual requested losses are at most ϵ\epsilon. Let Eactual(h)E_{\mathrm{actual}}(h) denote the scale exponent relative to C(7/8)C(7/8) after the observed row bound R≤R∗+Δ/4+ϵrowR \le R_* + \Delta/4 + \epsilon_{\mathrm{row}} is inserted. For now the explicit height factors remain outside this exponent. The coefficient of RR in Equation (20.4) is dd, so at d=hd=h the capacity replacement contributes hΔ/4h\Delta/4. Denote by ϵtotal\epsilon_{\mathrm{total}} the sum of hϵrowh\epsilon_{\mathrm{row}} and all other adjustable real losses; the preceding uniformity makes it arbitrarily small with a target-independent coefficient. The certificate gives the comparison actually needed:

Eactual(h)−Δ≤−49440640−(1−h4)Δ+ϵtotal=−49440640−5164Δ+ϵtotal.\begin{aligned} E_{\rm actual}(h)-\Delta &\le-\frac{49}{440640}-\left(1-\frac h4\right)\Delta +\epsilon_{\rm total}\\ &=-\frac{49}{440640}-\frac{51}{64}\Delta +\epsilon_{\rm total}. \end{aligned}

The subtraction of Δ=C(β∗)−C(7/8)\Delta= C(\beta_*) - C(7/8) is essential: the certificate is not a claim that Eactual(h)<0E_{\mathrm{actual}}(h) < 0 for every Δ\Delta. When the height factors are converted to a reserved exponent allowance below, that allowance is added to ϵtotal\epsilon_{\mathrm{total}}.

Frequency ranges

For 1/2≤d≤h1/2 \le d \le h, the available length is

ℓd≥839>15>737.\frac{\ell}{d} \ge\frac{8}{39} > \frac{1}{5} > \frac{7}{37}.

Passing from base ZZ to base UU changes a slot length from ℓi\ell_i to ℓi/d≤2ℓi\ell_i/d \le2\ell_i, so one mesh chosen with this factor of two satisfies the moment requirement throughout the interval. If

0<ζ<5ℓ−h=148,0 < \zeta< 5\ell-h=\frac{1}{48},

then for h<d≤h+ζh<d\le h+\zeta the supply remains greater than 1/51/5, whose margin above 7/377/37 is 2/1852/185.

For 1/50<δ<α1/50<\delta<\alpha, use the ideal row upper exponent R=R∗+Δ/4R=R_*+\Delta/4. For δ=α\delta=\alpha, use R=1−δR=1-\delta. Both are at least 1−δ1-\delta, so

R+δ/2−1750≥3350−δ2≥425>0.R+\delta/2-\frac{17}{50}\ge\frac{33}{50}-\frac{\delta}{2}\ge\frac{4}{25}>0.

The floor has a positive slope as well. Thus d=hd=h bounds all these exponents for d≤hd\le h. The cost of extending to h+ζh+\zeta is at most 2ζ2\zeta: indeed

R∗≤1−δ+α−δ2≤1712,R∗+Δ/4≤13996,R_*\le1-\delta+\frac{\alpha-\delta}{2}\le\frac{17}{12},\qquad R_*+\Delta/4\le\frac{139}{96},

and 139/96+1/2−17/50<2139/96+1/2-17/50<2. The slopes at δ=α\delta=\alpha and floor cases are smaller than two.

For dmin⁡≤d≤1/2d_{\min}\le d\le1/2 and δ≤α\delta\le\alpha, choose t=1t=1 and use no selected primes. Proposition 19.2 gives the ideal exponent 1−2δ/31-2\delta/3 outside the floor. Use the slightly larger common exponent

R=7675−23δ.R=\frac{76}{75}-\frac{2}{3}\delta.

At δ=1/50\delta=1/50 it equals one, so it also covers the floor. Its slope is 101/150−δ/6>0101/150-\delta/6>0 on this range. Using q≤δ/2q\le\delta/2 in (20.4) yields

E(d)≤E(1/2)+O(ϵ)≤−5292400+2596δ+O(ϵ)≤−4914400+O(ϵ)<0.E(d)\le E(1/2)+O(\epsilon)\le-\frac{529}{2400}+\frac{25}{96}\delta+O(\epsilon)\le-\frac{49}{14400}+O(\epsilon)<0.

The middle expression follows by substituting d=1/2d=1/2, R=76/75−2δ/3R=76/75-2\delta/3, and q=δ/2q=\delta/2; the last inequality uses δ≤5/6\delta\le5/6. At δ=α\delta=\alpha, the count used in (20.7) and its positive slope already control every d≤hd\le h. Together with Section 20.3, these cases cover every physical row norm. Only d≥1/2d\ge1/2 uses selected physical prime factors in a row moment; every physical slot remains in the high correction in all ranges.

To compare with C(β∗)C(\beta_*), subtract C(β∗)−C(7/8)=ΔC(\beta_*)-C(7/8)=\Delta from each ideal exponent. In the adaptive range this is precisely the comparison in (20.10); its only positive capacity allowance is hΔ/4h\Delta/4. The other endpoint ranges have nonpositive ideal exponents before subtracting Δ\Delta. Thus all of them retain the target-independent main high margin

mhi:=(1−h4)Δ=5164Δ.m_{\mathrm{hi}}:=\left(1-\frac{h}{4}\right)\Delta=\frac{51}{64}\Delta.

The low exponent has margin mlo:=Δm_{\mathrm{lo}}:=\Delta. The principal contour and approximation margins were established in Section 20.1; we now choose all losses together.

Order of choices and conclusion

We finish by separating the target-independent real choices from the target-dependent height and external test orders. The numerical choices remain part of this application; the final height selection is supplied by Lemma 11.1.

Proposition 20.3 (Order of choices). Under the contradiction in (12.1), there are numbers

0<ω<Δ,σ>00<\omega<\Delta,\qquad\sigma>0

and a fixed geometry, moment losses, capacity decrements, slot system, amplitude width, bin width e>0e>0, and extension 0<ζ<1/480 < \zeta< 1/48, all chosen before the target character, with the following property. For every primitive finite-order target η\eta, one can then choose its fixed arithmetic data, a positive height exponent τη\tau_\eta, a finite external tail order NηN_\eta, and a lower threshold Z0,ηZ_{0,\eta} such that, for Z≥Z0,ηZ \ge Z_{0,\eta},

∣JII,η(Z)∣≪ηZC(7/8)+ω,∣JII,η(Z)−fII,η(Z)∣≪ηZC(β∗)−σ.|J_{\mathrm{II},\eta}(Z)|\ll_\eta Z^{C(7/8)+\omega},\qquad |J_{\mathrm{II},\eta}(Z)-f_{\mathrm{II},\eta}(Z)| \ll_\eta Z^{C(\beta_*)-\sigma}.

The exponents ω,σ\omega,\sigma do not depend on η\eta. The cutoff T1=ZτηT_1=Z^{\tau_\eta} occurs only in the estimates, not in either function.

Proof. The ideal margins are

mlo=Δ,mhi=5164Δ,mhigh:=min⁡{mhi,msmall}>0.m_{\mathrm{lo}}=\Delta,\qquad m_{\mathrm{hi}}=\frac{51}{64}\Delta,\qquad m_{\mathrm{high}}:=\min\{m_{\mathrm{hi}},m_{\mathrm{small}}\}>0.

The principal contour margins are mw,mzm_w,m_z in Equation (20.3). Reserve one half of each of mlo,mhigh,mw,mzm_{\mathrm{lo}},m_{\mathrm{high}},m_w,m_z. On the compact real parameter ranges, the coefficients multiplying all requested detector, moment, capacity, and rounding losses are bounded independently of the target. Indeed, δ≥1/50\delta\ge1/50, Dx≥37/18D_x \ge37/18, and J≥35/54\mathcal{J} \ge35/54; the dyadic lengths are bounded, and Proposition 19.2 gives fixed inverse width and supply margins. The equality δ=α\delta=\alpha uses the separate no-slot bound above. Choose the moment losses and capacity decrement so that their total cost in the high exponent is less than mhigh/8m_{\mathrm{high}}/8.

Let ηmesh>0\eta_{\mathrm{mesh}}>0 be the mesh supplied by Lemma 18.1 for these losses and bounded real ranges. Its uniform assertion on [3/4,1][3/4,1] applies in particular to the compact closure κ∈[3/4,5/6]\kappa\in[3/4,5/6] used here, and the mesh is independent of the number of slots. Only the eventual seminorm and height orders may depend on a fixed slot count. Let bround>0b_{\mathrm{round}}>0 be small enough that a squared-spike rounding loss below broundb_{\mathrm{round}}, after the bounded changes of exponent base, costs less than mhigh/8m_{\mathrm{high}}/8. Choose a fixed even integer KK with

2ℓK<min⁡{ηmesh,bround,1185},ℓi=ℓK(1≤i≤K).\frac{2\ell}{K}<\min\left\{\eta_{\mathrm{mesh}},b_{\mathrm{round}},\frac{1}{185}\right\},\qquad\ell_i=\frac{\ell}{K}\quad(1\le i\le K).

These positive lengths sum to ℓ\ell and are independent of the target and ZZ. Put Pi=P=Zℓ/KP_i=P=Z^{\ell/K}. For 1≤i≤K1\le i\le K, set

Ii=(1+2i−12K+1,1+2i2K+1)⊂(1,2)I_i=\left(1+\frac{2i-1}{2K+1},1+\frac{2i}{2K+1}\right)\subset(1,2)

and choose a nonnegative, nonzero Wi∈Cc∞(Ii)W_i\in C_c^\infty(I_i). The intervals have positive gaps. Hence their underlying prime windows are disjoint for every ZZ, before the ray, excluded-set, or row masks are imposed. Equation (12.5) keeps each window at its original scale in every summand.

For each selected row range, U=ZdU=Z^d has d≥1/2d\ge1/2, so

wi=ℓid≤2ℓK<ηmesh,δmax⁡iwi≤2ℓK<bround.w_i=\frac{\ell_i}{d}\le\frac{2\ell}{K}<\eta_{\rm mesh}, \qquad \delta\max_iw_i\le\frac{2\ell}{K}<b_{\rm round}.

The second inequality uses δ≤5/6<1\delta\le5/6<1. The total available length remains ℓ/d\ell/d. For d≤hd\le h it is at least 8/398/39, exceeding 7/377/37 by 23/144323/1443. For h<d≤h+ζh<d\le h+\zeta with ζ<1/48\zeta<1/48, it exceeds 1/51/5, whose excess over 7/377/37 is 2/1852/185. Thus every selected inverse capacity and the smaller plain capacity are supplied. The extra bound 2ℓ/K<1/1852\ell/K<1/185 is below half the latter gap. A zero-capacity neighborhood, including the equality endpoint, uses the no-slot moment. Actual annular ratios change nominal lengths by OK(1/log⁡U)O_K(1/\log U), absorbed by the fixed strict margins at a sufficiently large threshold.

The internal centered amplifier also stays separated from these windows. Write σwidth\sigma_{\mathrm{width}} for the width decrement denoted σ\sigma in the proof of Lemma 18.1. That proof uses the pool exponent ℓ∗=σwidth/3\ell_* = \sigma_{\mathrm{width}}/3 and a mesh below σwidth/6\sigma_{\mathrm{width}}/6. At base UU, every live physical slot has norm at most 2Uηmesh2U^{\eta_{\mathrm{mesh}}}, whereas the pool begins at Uℓ∗/2U^{\ell_*}/2. Their fixed exponent gap makes these sets disjoint for all sufficiently large UU, uniformly in the selected dd-range. The marked inverse moment has no mesh condition.

The normalizer in (20.1) is nonzero for this actual choice. Put ci=∫0∞Wi(y)y−5/6 dy>0c_i=\int_0^\infty W_i(y)y^{-5/6}\,dy>0. The asymptotic already proved in Section 20.1 specializes to

Si(Z)∼P1/6ci∣T∣log⁡P>0,AT(Z)∼(K∣T∣ℓ)K(∏ici)(log⁡Z)−K>0.S_i(Z) \sim\frac{P^{1/6}c_i}{\lvert T\rvert\log P} > 0,\qquad A_T(Z) \sim\left(\frac{K}{\lvert T\rvert\ell}\right)^K\left(\prod_i c_i\right)(\log Z)^{-K} > 0.

The sign uses even KK. Any later fixed excluded set affects only the common lower threshold, since its primes eventually leave all these windows. Choose

κP=716ℓK=796K,0<κP<78min⁡iℓi=748K,mP:=κP.\kappa_P=\frac7{16}\frac{\ell}{K}=\frac7{96K}, \qquad 0<\kappa_P<\frac78\min_i\ell_i=\frac7{48K}, \qquad m_P:=\kappa_P.

Thus the principal approximation has a positive margin chosen before the target. The number of subsets, the seminorms of the narrow windows, and their finite height orders may depend on this fixed KK.

Choose the amplitude width, the remaining power losses, and ee so that their total high cost is less than mhigh/8m_{\mathrm{high}}/8, and so that

(1+h)e+ϵpr<mw/4,e+ϵpr<mz/4,e+ϵpr<mP/4.(1+h)e+\epsilon_{\mathrm{pr}} < m_w/4,\qquad e+\epsilon_{\mathrm{pr}} < m_z/4,\qquad e+\epsilon_{\mathrm{pr}} < m_P/4.

Here ϵpr>0\epsilon_{\mathrm{pr}}>0 includes the chosen small powers in the principal remainder estimate. Also require e<10−3e < 10^{-3} and the bounds e0e_0 in Lemma 8.2. The slot lengths have already been fixed, so the small powers needed in the amplitude subdivision can be chosen in terms of their positive minimum. All these choices depend only on Δ\Delta and the pretarget slot system.

Choose

0<ζ<min⁡{1/48,mhigh/16}.0 < \zeta< \min\{1/48,m_{\mathrm{high}}/16\}.

The frequency extension then costs at most 2ζ<mhigh/82\zeta< m_{\mathrm{high}}/8. Now choose the absolute line z∞>2z_\infty> 2 in Section 20.3 sufficiently far right that its large-row sum has a saving larger than mhighm_{\mathrm{high}} relative to C(β∗)C(\beta_*). Its exponent depends only on these real choices, so z∞z_\infty also precedes the target. Choose the pretarget cutoff needed for (10.2). Any additional fixed excluded primes required by Proposition 16.1 after the target is fixed may be added to SS: the same positive product-tail majorant preserves the shared contraction, and neither TT nor the slot windows change.

For clarity, the nonprincipal real comparison is uniform over all pointwise pairs in Lemma 20.1. Let ϵreal(d)≥0\epsilon_{\mathrm{real}}(d) \ge0 collect the allocated real, mesh, and moment losses for the relevant range. The endpoint inequality, the intermediate inequality, and the positive slopes give

E(d)+ϵreal(d)≤(β∗−7/8)−ϵhi,ϵhi>0,E(d)+\epsilon_{\mathrm{real}}(d) \le(\beta_* - 7/8)-\epsilon_{\mathrm{hi}},\qquad\epsilon_{\mathrm{hi}}>0,

for every occurring (R,q)(R,q) and every moderate dd, with a fixed fraction of mhighm_{\mathrm{high}} still reserved. Therefore the same inequality holds for Emax⁡,Z(d)E_{\max,Z}(d), uniformly in ZZ. The small and large bounds have their stated separate savings. Apply the subpower normalizer estimate once to the nonprincipal and outer-row contributions, and absorb the remaining finite dyadic multiplicities using a power below mhigh/8m_{\mathrm{high}}/8. Lemma 10.5 already includes its own normalizer allowance ϵpr\epsilon_{\mathrm{pr}}. The four high real allocations above cost less than mhigh/2m_{\mathrm{high}}/2; this last allowance leaves more than 3mhigh/83m_{\mathrm{high}}/8. The principal inequalities leave more than 3/43/4 of each of mw,mz,mPm_w,m_z,m_P. Thus one may fix, before the target,

m=14min⁡{mhigh,mw,mz,mP}>0m = \frac{1}{4}\min\{m_{\mathrm{high}},m_w,m_z,m_P\} > 0

as a common remaining high saving before retained height factors. For the low estimate, apply (20.2) with the pretarget loss Δ/2\Delta/2, and set ω=Δ/2\omega= \Delta/2. Let ϵht>0\epsilon_{\mathrm{ht}} > 0 be the minimum of the finitely many detector height allowances already chosen with these real losses.

Now fix a primitive target η\eta. Choose its admissible fixed arithmetic data and the final excluded set SS, including its conductor, the common cutoff, and the further fixed exclusions just described. The physical expression, HηH_\eta, cSc_S, and the signal all use this same data. The group TT and the slot system remain independent of the target. Fix all internal moment, seminorm, and Sobolev orders supplied by the preceding results for this datum. Their uniformity over moving moduli, common masks, and frozen labels gives a finite AηA_\eta dominating the product of all retained high factors, including the dyadic, prime, numerator-reflection, and row-count height factors. It is independent of any later external test order. The all-height correction bounds and the direct global or absolute bounds in the shared analytic lemmas likewise give a finite scale degree BηB_\eta for all discarded physical pieces, independent of the later order NN. Normalizing those pieces and summing their finitely many types only enlarges this fixed BηB_\eta.

We use the height ceiling verified at the end of Section 19.2. Let Aht,η≤AηA_{\mathrm{ht},\eta} \le A_\eta dominate the finitely many detector height orders, enlarging AηA_\eta if necessary, and put

τ0,η:=dmin⁡ϵht20(1+Aht,η)>0.\tau_{0,\eta} := \frac{d_{\min}\epsilon_{\mathrm{ht}}}{20(1+A_{\mathrm{ht},\eta})} > 0.

This number is fixed after the retained orders for the target, but before NN and ZZ. If 0<τ≤min⁡{dmin⁡/100,τ0,η}0 < \tau\le\min\{d_{\min}/100,\tau_{0,\eta}\} and T1=ZτT_1=Z^\tau, then, for U≥Zdmin⁡U \ge Z^{d_{\min}} and sufficiently large ZZ,

T1≤U1/100,(1+T1)Aht,η≤2Aht,ηZdmin⁡ϵht/20≤Uϵht/10.T_1 \le U^{1/100}, \qquad(1+T_1)^{A_{\mathrm{ht},\eta}} \le2^{A_{\mathrm{ht},\eta}}Z^{d_{\min}\epsilon_{\mathrm{ht}}/20} \le U^{\epsilon_{\mathrm{ht}}/10}.

By the definition of ϵht\epsilon_{\mathrm{ht}}, this proves every literal condition (1+T1)AA≤Uϵ/10(1+T_1)^{A_{\mathcal A}}\le U^{\epsilon/10} in Lemma 8.2 throughout the moderate range. The first bound also makes the detector’s crude error U−189/100+o(1)T12≤U−187/100+o(1)U^{-189/100+o(1)}T_1^2 \le U^{-187/100+o(1)} tend to zero. Every buffered moderate range has d≤h+ζ<1d \le h+\zeta< 1; small and absolute large rows use no buffered cutoff.

The fixed finite list of external coordinates, including the physical ℑz\Im z coordinate, uses the single allocation in Equation (10.14). Its matrix is fixed by the slot system and the finite retained estimates, and is independent of the external derivative order. For each such τ\tau, the dyadic, witness, and prime estimates may choose their auxiliary external orders after τ\tau, as their statements permit, so that their complete pointwise bounds hold. Choose a strict power gap when absorbing their discarded parts; the resulting external seminorm constants are then absorbed by the τ\tau-dependent lower threshold. For any requested remaining order NN, these auxiliary orders may be increased further; this changes only external seminorm constants and the lower threshold, not AηA_\eta, BηB_\eta, or τ0,η\tau_{0,\eta}. No internal moment is reapplied to an externally differentiated profile.

Combining Lemma 20.1, all the row ranges, and the principal remainder estimate therefore gives, for every fixed NN and sufficiently large ZZ in this ceiling range,

∣JII,η(Z)−fII,η(Z)∣≪η,NZC(β∗)−m(1+T1)Aη+ZBηT1−N.|J_{\mathrm{II},\eta}(Z)-f_{\mathrm{II},\eta}(Z)| \ll_{\eta,N} Z^{C(\beta_*)-m}(1+T_1)^{A_\eta} +Z^{B_\eta}T_1^{-N}.

The lower threshold is allowed to depend on τ,N,η\tau,N,\eta. This is Equation (11.1). Its low hypothesis is Equation (20.2) with ω=Δ/2\omega=\Delta/2, and the two functions do not contain T1T_1. Apply Lemma 11.1 with σ0=7/8\sigma_0=7/8, C=CIIC=C_{\mathrm{II}}, this mm, and the verified ceiling τ0,η\tau_{0,\eta}. It chooses τη\tau_\eta, then a common dominating external order NηN_\eta, and finally the threshold. It gives the asserted high estimate with σ=m/2>0\sigma=m/2>0. Both ω\omega and σ\sigma were fixed before the target.

Proposition 20.3 and Equation (10.2) verify the hypotheses of Proposition 2.1 with σ0=7/8\sigma_0=7/8, Jη=JII,ηJ_\eta=J_{\mathrm{II},\eta}, and fη=fII,ηf_\eta=f_{\mathrm{II},\eta}. This contradicts β∗>7/8\beta_*>7/8; hence β∗≤7/8\beta_*\le7/8. Proposition 11.3 at σ0=7/8\sigma_0=7/8 extends the primitive Hecke conclusion to all finite-order Hecke and Dirichlet LL-functions, with the principal pole allowed, and proves Theorem 1.1.

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