Introduction

Parity is a basic test of whether a shallow circuit can combine information from all of its inputs. For a computational-basis string x=(x1,…,xn)∈{0,1}nx=(x_1,\ldots,x_n)\in\{0,1\}^n, its value is PARITY⁡(x)=x1⊕⋯⊕xn\operatorname{PARITY}(x)=x_1\oplus\cdots\oplus x_n. We study circuits generated by arbitrary one-qubit unitaries and Toffoli gates with any number of controls and one target. Gates in each parallel layer have pairwise disjoint supports. The depth is the number of such layers.

The circuit starts in ∣x⟩⊗∣0⟩⊗(N−n)\lvert x\rangle\otimes\lvert0\rangle^{\otimes(N-n)} on NN total qubits. Its answer is the result of measuring one designated output qubit in the computational basis; the remaining registers may be discarded in arbitrary final states, and the input need not be preserved. For 0<ε≤1/20<\varepsilon\le1/2, computing parity with worst-case advantage ε\varepsilon means giving the correct answer with probability at least 1/2+ε1/2+\varepsilon for every xx. The class QAC0\mathrm{QAC}^{0} uses constant depth and polynomially many total qubits. This also bounds the gate count: a disjoint layer on NN qubits has at most NN nonempty gates. The gates may depend on nn, but not on the input string. We use unitary circuits, with no intermediate measurements, postselection, or primitive unbounded-fanout gate.

Theorem 1 (Parity lower bound). Fix a nonnegative integer dd, a real number c≥1c\ge1, and 0<ε≤1/20<\varepsilon\le1/2. For all sufficiently large nn, no circuit of depth at most dd on nn input qubits and at most ncn^c total qubits, using arbitrary one-qubit unitaries and unbounded-arity Toffoli gates, computes PARITY⁡(x)\operatorname{PARITY}(x) with probability at least 1/2+ε1/2+\varepsilon for every x∈{0,1}nx\in\{0,1\}^n. Gates in each layer have disjoint supports, ancillas start in ∣0⟩\lvert0\rangle, and one output qubit is measured; the other qubits may be discarded.

Taking ε=1/6\varepsilon=1/6 gives the usual success threshold 2/32/3. Thus Theorem 1 resolves positively the conjecture PARITY⁡∉QAC0\operatorname{PARITY}\notin\mathrm{QAC}^{0}, with bounded error, polynomially many ancillas, and only a measured output required.

History and significance

In the classical class AC0\mathrm{AC}^{0}, circuits use unbounded-fan-in AND and OR gates and NOT gates, with unrestricted reuse of wires. The superpolynomial constant-depth lower bounds for parity of Furst, Saxe, and Sipser [8] and, independently, Ajtai [1], were fundamental explicit circuit lower bounds. Yao obtained exponential bounds [26], and Håstad obtained almost optimal exponential bounds through the switching lemma [12]. Quantum circuits introduce a different constraint: the supports of gates in a parallel layer are disjoint, so a wire cannot control arbitrarily many simultaneous gates.

Moore introduced the corresponding quantum circuit classes and related coherent parity to unbounded fanout [17]. The latter is the unitary sending ∣b,y1,…,yk⟩\lvert b,y_1,\ldots,y_k\rangle to ∣b,y1⊕b,…,yk⊕b⟩\lvert b,y_1\oplus b,\ldots,y_k\oplus b\rangle. The coherent parity transformation sends the same input to ∣b⊕PARITY⁡(y),y1,…,yk⟩\lvert b\oplus\operatorname{PARITY}(y),y_1,\ldots,y_k\rangle, where y=(y1,…,yk)y=(y_1,\ldots,y_k). Hadamard conjugation interchanges these two transformations. Moore’s original formulation required ancillary qubits to return to zero; our result also treats the more permissive measured-output model. Green, Homer, Moore, and Pollett developed the associated quantum counting classes and modular-gate equivalences [9]. The constant-depth constructions of Høyer and Špalek demonstrate how much computational power a primitive fanout operation provides [13].

Early lower bounds revealed the importance of the ancillary register. Fang, Fenner, Green, Homer, and Zhang obtained a depth lower bound of order log⁡(n/(a+1))\log(n/(a+1)) for exact, clean parity computation with aa ancillary qubits [6], Corollary 4.6; Bera developed a different lower-bound method in the ancilla-free setting [4]. Padé, Fenner, Grier, and Thierauf ruled out exact clean simulation at entangling depth two [21]. Fenner, Grier, Padé, and Thierauf subsequently removed the final-state cleanliness requirement for exact single-output parity at that depth [7], Theorem 6.1. Here the quoted depth-two results count multiqubit layers, allowing arbitrary one-qubit layers between them; we call this entangling depth. Rosenthal proved lower bounds for approximate parity unitaries and related cat-like states, and gave constant-depth approximation constructions with superpolynomial resources [23]. Approximate unitary implementation and computation of a single measured classical bit have different output requirements, so the distinction matters in comparing lower bounds.

More recent work developed spectral and Fourier methods for QAC0\mathrm{QAC}^{0}. Nadimpalli, Parham, Vasconcelos, and Yuen used the Pauli spectrum to prove ancilla-restricted lower bounds [18]. Anshu, Dong, Ou, and Yao ruled out a fixed positive parity advantage with O~(n1+3−d)\widetilde{O}(n^{1+3^{-d}}) ancillas at every fixed entangling depth d≥1d\ge1 [2], Corollary 4.4 and Theorem 4.6. Dong, Ou, and Yao increased this ancilla range to O~(n1+2−d)\widetilde{O}(n^{1+2^{-d}}) [5], Corollary 3.3. Here O~\widetilde{O} suppresses logarithmic factors. Both results use spectral-norm approximation of conjugated observables.

Joshi, Tal, Vasconcelos, and Wright proved exact parity lower bounds at entangling depth three and bounded parity correlation at entangling depth two by exp⁡(−Ω(n))\exp(-\Omega(\sqrt{n})), without a size restriction [14], Theorem 1.2 and Corollary 5.9. Kintali’s September 2026 preprint reports correlation at most exp⁡(−Ω(n))\exp(-\Omega(n)) at entangling depth three and an exponential multiqubit gate lower bound for exact parity at entangling depth four [15], Theorems 1–2. These results retain a resource restriction or a fixed upper bound on entangling depth. Gretta, Gupta, and Joshi established an equivalence between the general parity lower-bound question and Fourier concentration [10], and Xu and Li extended related fanout reductions to symmetric Boolean functions [25]. Our theorem permits every fixed depth and every fixed polynomial bound on the total number of qubits, with arbitrary discarded garbage and any fixed positive worst-case advantage.

The localization argument

Unbounded gate arity is the first obstacle to a lower bound. A single Toffoli gate can involve every input, so the number of wires in an output’s backward light cone gives no useful restriction. Our argument instead bounds transitions from a fixed product condition to states with many mismatches from that condition. We keep the amplitude lost when imposing a projection, without normalizing the resulting state.

A product projection fixes a chosen one-qubit vector on each qubit of a subset and acts as the identity elsewhere. Fix reference unit vectors viv_i on a subset S⊆{1,…,N}S \subseteq\{1,\ldots,N\}. Their mismatch count is

M=∑i∈S(I−∣vi⟩⟨vi∣)i;M = \sum_{i \in S}(I-\lvert v_i\rangle\langle v_i\rvert)_i;

its eigenvalue counts the factors orthogonal to their reference vectors. Write [M=0][M = 0] and [M≥r][M \ge r] for its zero and high-count spectral projections. Given a shallow circuit UU and a product projection AA, our structural theorem bounds

∥[M≥Nt]UAU†[M=0]∥≤e−Ns(0≤s<t)\left\lVert[M \ge N^t]UAU^\dagger[M = 0]\right\rVert\le e^{-N^s} \qquad(0 \le s < t)

for every fixed depth and all sufficiently large NN. The norm is the operator norm, and the estimate is uniform in UU, AA, MM. In particular, the uncounted register can carry an arbitrary, internally entangled state. Theorem 2 gives the precise statement in a reflection-gate model containing the original circuits.

There are two inductions. The outer induction removes one circuit layer. Every allowed Toffoli is a reflection I−2PI - 2P about a product projection. If AA fixes only kk qubits, at most kk gates in a disjoint layer meet its support. Expanding those reflections on the two sides of AA expresses the conjugate as a sum of products of three projections, each conjugated by a circuit of one smaller depth. Intermediate mismatch cutoffs bound these ordered products. This proves localization for projections supported on few qubits (Section 4).

The reflection expansion has a cost exponential in the support size, so it does not directly control arbitrary product projections. To handle such a projection, write it as [D=0][D = 0] for a second mismatch count DD. A polynomial p(D)p(D) of low degree expands into projections on few qubits. The construction in Section 3 controls both its approximation error on a low-count interval and the sum of its coefficients weighted by the cost of this expansion. It need not be a good approximation at large counts. The second induction controls precisely that remaining error.

Here the order of the operators is decisive. Put P=[M=0]P = [M = 0], Q=U[D=0]U†Q = U[D = 0]U^\dagger, and H=[M≥Nt]H = [M \ge N^t]. Squaring the transition norm gives ∥HQP∥2=∥HQPQH∥\lVert HQP\rVert^2 = \lVert HQP QH\rVert. Replacing only the first QQ by p(UDU†)p(UDU^\dagger) leaves an error acting on PQPQ. After conjugation by U†U^\dagger, the high-count part of that error is another localization problem, with the two counts exchanged and a larger mismatch threshold. We prove the universal statement at that larger threshold first. A finite chain of thresholds ends above the maximum possible count NN, where localization is automatic; working backward proves the original statement (Section 5). The same-depth inverse-circuit invocation is therefore part of a finite induction.

Finally, the output-zero probability is the diagonal of the conjugated output projection. Its parity coefficient is the average of matrix entries between complementary Hadamard product states. Those states differ on all nn input qubits. The localization theorem makes every such entry small when NN is polynomial in nn, whereas a fixed worst-case advantage forces their average to stay positive (Section 6). This final step places no restriction on the unmeasured registers.

The polynomial ingredients have a substantial history. The combination of Chebyshev approximation with exact roots at exceptional integer points follows an established approximation-and-interpolation pattern for symmetric predicates [24], Section 3.1. Polynomial localization and concentration for quantum states appear in work of Kuwahara, Arad, Amico, and Vedral [16] and Anshu and Metger [3]. The latter also track the total norm of local terms. For QAC0^{0}, the spectral-norm approximation approach of Anshu, Dong, Ou, and Yao [2] is a particularly relevant predecessor. We prove the required polynomial and coefficient estimates here. The finite inverse-circuit induction supplies the additional scale improvement: localization holds for every fixed exponent pair 0≤s<t0 \le s < t, uniformly in both counts and the entire uncounted register.

The companion article Regular trajectories, pruning and quantum parity [20], Sections 4–7 gives an independent proof through state-dependent propagation, projection insertion, and pruning. Its structural estimates concern regular trajectories; the present operator-norm theorem is proved without a trajectory hypothesis. Both articles prove their own polynomial estimates and their own parity conversion, so neither parity proof invokes the other.

Consequences

Localization and parity also constrain symmetric computation and state preparation. We combine them with reductions of Xu and Li [25] and state constructions of Gretta, Gupta, and Joshi [11]. In particular, strict majority, MAJ⁡n(x)=1{∣x∣>n/2}\operatorname{MAJ}_n(x) = 1\{|x| > n/2\}, where ∣x∣|x| is the Hamming weight, cannot be computed in this circuit model with worst-case advantage 1/(log⁡n)γ1/(\log n)^\gamma for any fixed γ>0\gamma> 0 (Corollary 10). This separates the model from the corresponding one with unbounded threshold gates.

The state-preparation consequences rule out inverse-polynomial measurement probabilities for both a string and its bitwise complement, and sufficiently accurate preparation of uniform superpositions of strings of a fixed Hamming weight kk with nδ≤k≤n/2n^\delta\le k \le n/2 for fixed δ>0\delta> 0 (Corollary 8). For a single measured output, define its expected sign as the probability of zero minus the probability of one. Localization implies that its Fourier coefficients have total squared weight that decays faster than every inverse power of nn on input subsets of size at least nδn^\delta, for every fixed 0<δ≤10 < \delta\le1 (Corollary 9). Finally, majority cannot be computed with average success at least 1−12n−δ1 - \frac{1}{2}n^{-\delta} on uniformly random inputs, for any fixed δ>0\delta> 0 (Corollary 11). The precise quantifiers and proofs appear after the parity proof in Section 7.

Organization. Section 2 states the localization theorem and fixes the circuit model. Section 3 proves the polynomial approximation. Section 4 reduces small-support projections to the preceding depth, and Section 5 completes the finite scale induction. Section 6 derives Theorem 1, and Section 7 proves the consequences just described.

Product projections and localization

The parity proof will use localization for a single output projection. We prove the stronger uniform statement for every product projection, because its induction exchanges the projected and counted registers.

All operators act on HN=(C2)⊗N\mathcal{H}_N = (\mathbb{C}^2)^{\otimes N}, and ∥⋅∥\lVert\cdot\rVert denotes the operator norm. Identities on unmentioned qubits are implicit. Spectral projections are written in brackets; for example, [M≥r][M \ge r] is the projection onto the sum of eigenspaces of a self-adjoint operator MM with eigenvalues at least rr. All logarithms are natural.

A count is an operator

M=∑i∈S(I−∣vi⟩⟨vi∣)i,S⊆{1,…,N},∥vi∥=1.(1)M = \sum_{i \in S} \left(I - \lvert v_i\rangle\langle v_i\rvert\right)_i,\qquad S \subseteq\{1,\ldots,N\},\qquad\lVert v_i\rVert= 1. \tag*{(1)}

The subscript indicates the qubit on which the summand acts. The reference vector vi∈C2v_i \in\mathbb{C}^2 can be chosen separately at each qubit. The summands commute, and the spectrum of MM is contained in {0,…,∣S∣}\{0,\ldots,\lvert S\rvert\}. A product projection is a tensor product of rank-one one-qubit projections on a subset, with identity on the complement. Its support is the selected subset. The empty product is II. These are precisely the projections [M=0][M=0]. In particular, a product projection need not have rank one on HN\mathcal{H}_N.

We use a slightly enlarged gate set of product-state reflections, as in [23], Section 2 and Proposition 2.1. Let Ud(N)\mathcal{U}_d(N) be the set of unitaries

U=(LdRd)⋯(L1R1)L0,U = (L_dR_d)\cdots(L_1R_1)L_0,

where each LjL_j is a product of one-qubit unitaries and each RjR_j is a layer of gates I−2AI-2A with disjoint supports, with AA a product projection on the gate’s qubits. Identity layers are allowed. The class U0(N)\mathcal{U}_0(N) consists of products of one-qubit unitaries.

This model contains the circuits of theorem:1. Indeed, if CC projects onto all controls being 1, a Toffoli gate equals

(I−C)⊗I+C⊗X=I−2C⊗∣−⟩⟨−∣,∣−⟩=∣0⟩−∣1⟩2.(I-C)\otimes I+C\otimes X=I-2C\otimes\lvert-\rangle\langle-\rvert,\qquad\lvert-\rangle=\frac{\lvert0\rangle-\lvert1\rangle}{\sqrt{2}}.

Grouping the local gates in each parallel step gives (2.2) with a number of reflection layers bounded by the original depth. Discarded qubits can be retained as idle wires without changing any later measurement probability. Here dd counts reflection layers in the enlarged model; it is at most the number of physical layers in the original circuit. The arbitrary local layers in (2.2) are included in this definition, rather than charged separately to dd.

We will also use closure under inversion at the same depth. Each RjR_j is self-adjoint, since it is a product of commuting self-adjoint reflections. Thus

U†=L0†R1L1†⋯RdLd†∈Ud(N).(2)U^\dagger=L_0^\dagger R_1L_1^\dagger\cdots R_dL_d^\dagger\in\mathcal{U}_d(N). \tag*{(2)}

This is the same normal form with the layer indices reversed: the new local layers are Ld†,…,L0†L_d^\dagger,\ldots,L_0^\dagger, in temporal order, and the new reflection layers are Rd,…,R1R_d,\ldots,R_1. No factors on overlapping supports have been commuted.

Theorem 2 (Localization of conjugated product projections). Fix a nonnegative integer dd and real numbers 0≤s<t0\le s<t. For all sufficiently large NN, every U∈Ud(N)U\in\mathcal{U}_d(N) and every pair of counts M,DM,D on HN\mathcal{H}_N satisfy

∥[M≥Nt]U[D=0]U†[M=0]∥≤exp⁡(−Ns).(3)\left\lVert[M\ge N^t]U[D=0]U^\dagger[M=0]\right\rVert\le\exp(-N^s). \tag*{(3)}

The sufficient lower bound on NN depends only on d,s,td,s,t, not on the circuit, the counted subsets, or their reference vectors.

Write Bd(s,t)\mathcal{B}_d(s,t) for the assertion of theorem:2 at the specified d,s,td,s,t, including its uniformity. If t>1t>1, it is immediate for N>1N>1, since [M≥Nt]=0[M\ge N^t]=0. We prove the theorem by induction on dd, assuming all fixed exponent pairs at the preceding depth. The counts M,DM,D are allowed to be different because the proof will exchange their roles when applying (2).

The next two sections supply the approximation and depth-reduction estimates. The proof of theorem:2 is completed in Section 5.

A polynomial approximation with controlled coefficients

We will approximate the zero spectral projection of a count by a polynomial. Small approximation error alone is not enough: expanding the kkth power of a count produces up to NkN^k product projections. For a polynomial f(x)=∑kckxkf(x) = \sum_k c_k x^k, define its weighted coefficient norm by

WN(f)=∑k∣ck∣Nk.W_N(f) = \sum_k |c_k|N^k.

This bounds the sum of absolute coefficients in the later operator expansion. The construction uses Chebyshev approximation together with exact roots at the first integer points, a classical approximation-and-interpolation pattern; see [24], Section 3.1 and Lemma 3.9. Controlling this sum is in the same general spirit as tracking the total local norm of [3], Definition 2.3 and Lemma 4.5. We supply the exact bounds needed here, including intervals whose endpoint exceeds the maximum count NN.

Lemma 3. Fix real numbers 0<a<b0 < a < b and u>(a+b)/2u > (a + b)/2. For every sufficiently large integer NN, there is a real polynomial pp such that

deg⁡p≤Nu,WN(p)≤exp⁡(Nu),p(0)=1,\deg p \le N^u,\qquad W_N(p) \le\exp(N^u),\qquad p(0) = 1,

and

∣p(x)∣≤exp⁡(−Na)for every integer 1≤x≤⌈Nb⌉.|p(x)| \le\exp(-N^a)\qquad\text{for every integer }1 \le x \le\lceil N^b\rceil.

The threshold for NN depends only on aa, bb, uu. No restriction b≤1b \le1 is imposed.

Proof. Put

r=⌈Na⌉,m=⌈Nb⌉,ℓ=⌈2mrlog⁡m⌉.r = \lceil N^a\rceil,\qquad m = \lceil N^b\rceil,\qquad\ell= \lceil2\sqrt{mr}\log m\rceil.

Since a<ba < b, we have m≥2rm \ge2r once NN is sufficiently large. Define the root polynomial

F(x)=∏j=1r(1−xj).F(x) = \prod_{j=1}^{r}\left(1-\frac{x}{j}\right).

It is one at zero and vanishes at the first rr positive integers. On [r,m][r,m] we only use the crude bound ∣F(x)∣≤mr|F(x)| \le m^r. To overcome this growth, we multiply it by a polynomial that is one at zero and small throughout [r,m][r,m]. To construct that factor, define the Chebyshev polynomials by

T0(x)=1,T1(x)=x,Tj+1(x)=2xTj(x)−Tj−1(x).T_0(x) = 1,\qquad T_1(x) = x,\qquad T_{j+1}(x) = 2xT_j(x) - T_{j-1}(x).

Induction in this recurrence, using the corresponding addition identities, gives

Tj(cos⁡θ)=cos⁡(jθ),Tj(h+h−12)=hj+h−j2(h>0).T_j(\cos\theta) = \cos(j\theta),\qquad T_j\left(\frac{h+h^{-1}}{2}\right) = \frac{h^j+h^{-j}}{2}\quad(h>0).

In particular, ∣Tj(x)∣≤1|T_j(x)| \le1 on [−1,1][-1,1]. Set

p(x)=F(x)Tℓ((m+r−2x)/(m−r))Tℓ((m+r)/(m−r)).p(x) = F(x)\frac{T_\ell((m+r-2x)/(m-r))}{T_\ell((m+r)/(m-r))}.

The denominator is positive, and p(0)=1p(0) = 1.

To bound the denominator, write q=r/mq = \sqrt{r/m} and h=(1+q)/(1−q)h = (1+q)/(1-q). Then 0<q<10 < q < 1 and

h+h−12=m+rm−r,log⁡h=2∫0qdy1−y2≥2q.\frac{h+h^{-1}}{2}=\frac{m+r}{m-r},\qquad\log h=2\int_0^q\frac{dy}{1-y^2}\ge2q.

Consequently

Tℓ(m+rm−r)≥12exp⁡(2ℓr/m)≥12m4r.T_{\ell}\left(\frac{m+r}{m-r}\right)\ge\frac{1}{2}\exp\left(2\ell\sqrt{r/m}\right)\ge\frac{1}{2}m^{4r}.

This denominator is also at least 11, by (hℓ+h−ℓ)/2≥1(h^\ell+h^{-\ell})/2\ge1.

The polynomial vanishes at the integers 1,…,r1,\ldots,r. For r≤x≤mr\le x\le m, the affine Chebyshev argument in (3.3) lies in [−1,1][-1,1], and each factor ∣1−x/j∣|1-x/j| is at most mm. Thus

∣p(x)∣≤2m−3r(r≤x≤m).|p(x)|\le2m^{-3r}\qquad(r\le x\le m).

Since r≥Nar\ge N^a and log⁡m⟶∞\log m\longrightarrow\infty, this is at most exp⁡(−Na)\exp(-N^a) for all sufficiently large NN. Together with the exact roots, this proves (3.2). No estimate is needed at noninteger points between 00 and rr.

It remains to bound the degree and the coefficient cost. The coefficient convolution formula gives WN(fg)≤WN(f)WN(g)W_N(fg)\le W_N(f)W_N(g). Hence the root product has weighted norm at most

∏j=1r(1+N/j)≤(1+N)r.\prod_{j=1}^{r}(1+N/j)\le(1+N)^r.

For z(x)=(m+r−2x)/(m−r)z(x)=(m+r-2x)/(m-r), we have

β:=WN(z)=m+r+2Nm−r≤3+2N.\beta:=W_N(z)=\frac{m+r+2N}{m-r}\le3+2N.

Here m≥2rm\ge2r controls the constant coefficient, while the positive integer m−r≥1m-r\ge1 controls the linear coefficient. This bound remains valid when m>Nm>N.

Let A=2β+1A=2\beta+1. The Chebyshev recurrence and induction give WN(Tj(z))≤AjW_N(T_j(z))\le A^j: the inductive step uses

2βAj+Aj−1≤Aj+1,A2−2βA−1=2β≥0.2\beta A^j+A^{j-1}\le A^{j+1},\qquad A^2-2\beta A-1=2\beta\ge0.

The initial cases follow from WN(T0(z))=1W_N(T_0(z))=1 and WN(T1(z))=β≤AW_N(T_1(z))=\beta\le A. Since A≤7+4N≤11(1+N)A\le7+4N\le11(1+N) and the denominator in (3.3) is at least 11, we obtain

WN(p)≤(1+N)r(11(1+N))ℓ,deg⁡p≤r+ℓ.W_N(p)\le(1+N)^r\bigl(11(1+N)\bigr)^\ell,\qquad\deg p\le r+\ell.

Finally, with γ=(a+b)/2>a\gamma=(a+b)/2>a, the rounded definitions imply

r=O(Na),ℓ=O(Nγlog⁡N),log⁡WN(p)=O(Nγ(log⁡N)2).r=O(N^a),\qquad\ell=O(N^\gamma\log N),\qquad\log W_N(p)=O\left(N^\gamma(\log N)^2\right).

Both r+ℓr+\ell and log⁡WN(p)\log W_N(p) are o(Nu)o(N^u) because u>γu>\gamma. All constants depend only on the fixed exponents, proving (3.1) with the asserted uniform threshold.

Depth reduction for small-support projections

We begin the proof of Theorem 2 at depth zero. We then show that the full localization statement at depth d−1d-1 controls projections of small support at depth dd. All large-NN thresholds in this section depend only on the displayed exponents and the depth, not on the circuits, counts, or product projections.

Lemma 4 (Depth zero). For every fixed 0≤s<t0 \le s < t, the statement B0(s,t)\mathcal{B}_0(s,t) holds.

Proof. If U∈U0(N)U \in\mathcal{U}_0(N), then Q=U[D=0]U†Q = U[D = 0]U^{\dagger} is a product projection. Let SS be the counted subset of MM, let P=[M=0]P = [M = 0], and put I∗=S∩supp⁡QI_* = S \cap\operatorname{supp} Q. Write ∣vi⟩|v_i\rangle for the reference vectors of MM and ∣wi⟩|w_i\rangle for the projected vectors of QQ on I∗I_*. Set

pi=1−∣⟨wi∣vi⟩∣2(i∈I∗).p_i = 1 - |\langle w_i \mid v_i\rangle|^2 \qquad(i \in I_*).

Every vector in the range of PP has the fixed tensor factor ⨂i∈S∣vi⟩\bigotimes_{i \in S}|v_i\rangle on SS. Its factor on the complement of SS is arbitrary and need not be a product state. Applying QQ contributes the squared-amplitude factor ∏i∈I∗(1−pi)\prod_{i \in I_*}(1-p_i) on SS, and a contraction on its complement. If this amplitude is nonzero, the resulting normalized factor on SS is

⨂i∈I∗∣wi⟩⊗⨂i∈S∖I∗∣vi⟩,\bigotimes_{i \in I_*}|w_i\rangle\otimes\bigotimes_{i \in S \setminus I_*}|v_i\rangle,

with factors placed in their original qubit order. In this product vector, the mismatch count has the law of a sum KK of independent Bernoulli variables with parameters pip_i; coordinates in S∖I∗S \setminus I_* never contribute. Keeping the squared-amplitude factor, we obtain, for every r>0r > 0,

∥[M≥r]QP∥2≤∏i∈I∗(1−pi)Pr⁡(K≥r)\left\|[M \ge r]QP\right\|^2 \le\prod_{i \in I_*}(1-p_i)\Pr(K \ge r)
≤2−r∏i∈I∗(1−pi)(1+pi)≤2−r.\le2^{-r}\prod_{i \in I_*}(1-p_i)(1+p_i) \le2^{-r}.

The middle inequality is Markov’s inequality applied to 2K2^K. The same bound is immediate if the amplitude vanishes. Taking r=Ntr = N^t gives ∥[M≥Nt]QP∥≤exp⁡(−12(log⁡2)Nt)\left\|[M \ge N^t]QP\right\| \le\exp\left(-\frac{1}{2}(\log2)N^t\right), which is at most exp⁡(−Ns)\exp(-N^s) for all sufficiently large NN. ∎

The depth-zero estimate incorporates both the chance of producing a mismatch and the amplitude lost under projection. We next extend the preceding-depth hypothesis from one mismatch pattern to all patterns below a small threshold. This is the input needed to control successive factors in the layer expansion.

Lemma 5 (Propagation from low counts). Fix d≥1d \ge1 and assume Bd−1(s,t)\mathcal{B}_{d-1}(s,t) for every fixed pair 0≤s<t0 \le s < t. For fixed α,σ≥0\alpha,\sigma\ge0 and β>max⁡{α,σ}\beta> \max\{\alpha,\sigma\}, all sufficiently large NN satisfy

∥[M≥Nβ]B[M<Nα]∥≤exp⁡(−Nσ)(4)\left\|[M \ge N^\beta]B[M < N^\alpha]\right\| \le\exp(-N^\sigma) \tag*{(4)}

uniformly for every count MM and every B=VP∗V†B = VP_*V^\dagger, where V∈Ud−1(N)V \in\mathcal{U}_{d-1}(N) and P∗P_* is a product projection.

Proof. Let SS be the counted subset of MM. For F⊆SF \subseteq S, define MFM^F by replacing the reference vector on each coordinate of FF with an orthogonal unit vector, leaving the other references unchanged. The projection [MF=0][M^F = 0] specifies precisely the mismatch pattern FF for MM, with identity on the complement of SS. Hence

[M<Nα]=∑F⊆S∣F∣<Nα[MF=0].[M < N^\alpha] = \sum_{\substack{F \subseteq S\\ |F| < N^\alpha}} [M^F = 0].

These counts are diagonal in the same product basis, and pointwise in that basis MF≥M−∣F∣IM^F \ge M - |F|I. Choose fixed exponents

max⁡{α,σ}<σ′<β′<β.\max\{\alpha,\sigma\} < \sigma' < \beta' < \beta.

For all sufficiently large NN, uniformly over the indicated FF, Nβ−∣F∣≥Nβ′N^\beta- |F| \ge N^{\beta'}. Thus

∥[M≥Nβ]B[MF=0]∥≤∥[MF≥Nβ′]B[MF=0]∥≤exp⁡(−Nσ′),\left\|[M \ge N^\beta]B[M^F = 0]\right\| \le\left\|[M^F \ge N^{\beta'}]B[M^F = 0]\right\| \le\exp(-N^{\sigma'}),

where the last inequality is Bd−1(σ′,β′)B_{d-1}(\sigma',\beta'). There are at most (1+N)⌈Nα⌉+1(1+N)^{\lceil N^\alpha\rceil+1} patterns. The triangle inequality therefore bounds the left side of (4) by

exp⁡((⌈Nα⌉+1)log⁡(1+N)−Nσ′)≤exp⁡(−Nσ)\exp\left((\lceil N^\alpha\rceil+1)\log(1+N)-N^{\sigma'}\right) \le\exp(-N^\sigma)

for all sufficiently large NN, since σ′>α,σ\sigma' > \alpha,\sigma. □

We can now remove one reflection layer when the tested projection has small support. The expansion produces three ordered factors; the low-count estimate just proved bounds the transitions between them.

Lemma 6 (Small-support depth reduction). Fix d≥1d \ge1 and assume Bd−1(s,t)B_{d-1}(s,t) for every fixed pair 0≤s<t0 \le s < t. For fixed u,w≥0u,w \ge0 and t>max⁡{u,w}t > \max\{u,w\}, all sufficiently large NN satisfy

∥[M≥Nt]UAU†[M=0]∥≤exp⁡(−Nw)(5)\left\|[M \ge N^t]UAU^\dagger[M = 0]\right\| \le\exp(-N^w) \tag*{(5)}

uniformly for every U∈Ud(N)U \in\mathcal{U}_d(N), every count MM, and every product projection AA supported on at most NuN^u qubits.

Proof. The claim is immediate when t>1t > 1, so suppose t≤1t \le1. Write

U=VR1L0,V=(LdRd)⋯(L2R2)L1∈Ud−1(N),U = V R_1L_0,\qquad V = (L_dR_d)\cdots(L_2R_2)L_1 \in\mathcal{U}_{d-1}(N),

where V=L1V = L_1 if d=1d = 1, and put A′=L0AL0†A' = L_0AL_0^\dagger. This is a product projection with the same support as AA, of size k≤Nuk \le N^u. Gates of R1R_1 whose supports avoid supp⁡A′\operatorname{supp} A' commute with A′A' and cancel in R1A′R1R_1A'R_1. Because the gates in R1R_1 have disjoint supports, at most kk gates remain.

Expand each remaining reflection I−2P∗I - 2P_* on both sides of A′A'. Each term is a scalar multiple of PleftA′PrightP_{\mathrm{left}}A'P_{\mathrm{right}}, where the two side factors are product projections: within either side, the selected gate projections have disjoint supports. The sum of the absolute scalar coefficients is at most

(1+2)2k=9k.(1+2)^{2k} = 9^k.

Conjugation by VV turns each such term into a product B1B2B3B_1B_2B_3, with

B1=VPleftV†,B2=VA′V†,B3=VPrightV†.B_1 = VP_{\mathrm{left}}V^\dagger,\qquad B_2 = VA'V^\dagger,\qquad B_3 = VP_{\mathrm{right}}V^\dagger.

Each BjB_j is therefore a contraction to which Lemma 5 applies. No commutation between these three factors is asserted or needed.

Choose fixed exponents

max⁡{w,u}<w′<τ1<τ2<t.\max\{w,u\}<w'<\tau_1<\tau_2<t.

and set

P=[M=0],H=[M≥Nt],E1=[M<Nτ1],E2=[M<Nτ2].P=[M=0],\qquad H=[M\ge N^t],\qquad E_1=[M<N^{\tau_1}],\qquad E_2=[M<N^{\tau_2}].

Insert these cutoffs between the three factors, read from right to left. The resulting terms isolate a jump to the first cutoff, a jump from below the first to the second, and a jump from below the second to the final high-count sector:

HB1B2B3P=HB1B2(I−E1)B3P+HB1(I−E2)B2E1B3P+HB1E2B2E1B3P.\begin{aligned} HB_1B_2B_3P={}&HB_1B_2(I-E_1)B_3P\\ &+HB_1(I-E_2)B_2E_1B_3P\\ &+HB_1E_2B_2E_1B_3P. \end{aligned}

The first term has norm at most exp⁡(−Nw′)\exp(-N^{w'}) by Bd−1(w′,τ1)\mathcal{B}_{d-1}(w',\tau_1), applied to (I−E1)B3P(I-E_1)B_3P. For the second term, Lemma 5 with (α,σ,β)=(τ1,w′,τ2)(\alpha,\sigma,\beta)=(\tau_1,w',\tau_2) bounds (I−E2)B2E1(I-E_2)B_2E_1 by the same quantity. For the third, that lemma with (α,σ,β)=(τ2,w′,t)(\alpha,\sigma,\beta)=(\tau_2,w',t) bounds HB1E2HB_1E_2. All other factors are contractions. Therefore

∥HB1B2B3P∥≤3exp⁡(−Nw′).\lVert HB_1B_2B_3P\rVert\le3\exp(-N^{w'}).

Summing with (4.3) gives

∥HUAU†P∥≤3exp⁡((log⁡9)Nu−Nw′)≤exp⁡(−Nw).\lVert HUAU^\dagger P\rVert\le3\exp\left((\log9)N^u-Nw'\right)\le\exp(-N^w).

for all sufficiently large NN. The strict gaps w′>u,ww'>u,w absorb the entire expansion cost uniformly for k≤Nuk\le N^u.

The finite scale induction

The preceding depth gives localization for projections with small support. We now extend that estimate to arbitrary product projections. The extension uses the inverse circuit at a larger mismatch scale. The main constraint is how far that scale can move: to prove Bd(s,t)\mathcal{B}_d(s,t) from Bd(t,b)\mathcal{B}_d(t,b), we need t<b<2t−st<b<2t-s. This interval leaves room for a polynomial whose approximation error decays faster than e−Nse^{-N^s} while its degree and the logarithm of its weighted coefficient norm remain below the mismatch threshold NtN^t.

Lemma 7 (One backward step). Fix d≥1d\ge1, and assume Bd−1(s,t)\mathcal{B}_{d-1}(s,t) for every fixed 0≤s<t0\le s<t. Let s,t,bs,t,b be fixed real numbers with

0≤s<t<b<2t−s.0\le s<t<b<2t-s.

If Bd(t,b)\mathcal{B}_d(t,b) holds, then Bd(s,t)\mathcal{B}_d(s,t) holds.

Proof. Choose fixed auxiliary exponents

s<a<2t−b,a+b2<u<w<t.s<a<2t-b,\qquad\frac{a+b}{2}<u<w<t.

These choices are possible because b<2t−sb<2t-s. Since b>t>ab>t>a, they give exactly the inequalities required by the polynomial and small-support estimates:

0≤s<a<u<w<t<b,u>a+b2.0\le s<a<u<w<t<b,\qquad u>\frac{a+b}{2}.

Fix U∈Ud(N)U \in\mathcal{U}_d(N) and counts MM, DD, and put

P=[M=0],H=[M≥Nt],C=UDU†,Q=[C=0]=U[D=0]U†.P = [M = 0], \qquad H = [M \ge N^t], \qquad C = UDU^\dagger, \qquad Q = [C = 0] = U[D = 0]U^\dagger.

Let p(x)=∑kckxkp(x) = \sum_k c_k x^k be the polynomial in Lemma 3 for a,b,ua,b,u. We will first control Hp(C)PHp(C)P by small-support localization. Squaring the desired norm will then place the remaining high-CC error on PQPQ, where the larger-scale hypothesis applies after inversion.

Each count summand is a rank-one projection on one qubit. Expanding DkD^k gives at most NkN^k ordered monomials, each a product projection on at most kk qubits: repeated indices collapse by idempotence, while different indices commute. For k≤deg⁡p≤Nuk \le\deg p \le N^u, Lemma 6 applies to every such monomial with the same fixed exponents uu, ww, tt. Since p(C)=Up(D)U†p(C) = Up(D)U^\dagger, its coefficient bound gives

∥Hp(C)P∥≤e−Nw∑k∣ck∣Nk≤eNu−Nw.(6)\lVert Hp(C)P\rVert\le e^{-N^w}\sum_k |c_k|N^k \le e^{N^u-N^w}. \tag*{(6)}

The constant term causes no difficulty: it is a multiple of II, and HP=0HP = 0. Also, ∥C∥≤N\lVert C\rVert\le N gives

∥p(C)∥≤∑k∣ck∣Nk≤eNu.(7)\lVert p(C)\rVert\le\sum_k |c_k|N^k \le e^{N^u}. \tag*{(7)}

The polynomial need not approximate QQ on all of HN\mathcal{H}_N. Squaring the desired norm makes the approximation error occur as (Q−p(C))PQ(Q-p(C))PQ, rather than (Q−p(C))P(Q-p(C))P:

∥HQP∥2=∥HQPQH∥≤∥Hp(C)PQH∥+∥H(Q−p(C))PQH∥≤∥Hp(C)P∥+∥(Q−p(C))PQ∥.(8)\begin{aligned} \lVert HQP\rVert^2 &= \lVert HQPQH\rVert\\ &\le\lVert Hp(C)PQH\rVert+ \lVert H(Q-p(C))PQH\rVert\\ &\le\lVert Hp(C)P\rVert+ \lVert(Q-p(C))PQ\rVert. \tag*{(8)} \end{aligned}

Only the leftmost QQ was replaced in this decomposition. No commutation of PP with CC or QQ is involved.

Split the last error at the spectral threshold NbN^b of CC. The spectral projections of CC commute with QQ and p(C)p(C). On [C<Nb][C < N^b], the error is zero at eigenvalue 00, since p(0)=1p(0) = 1, and at most e−Nae^{-N^a} at every positive eigenvalue, since these eigenvalues are integers. Hence

∥(Q−p(C))PQ∥≤e−Na+(1+eNu)∥[C≥Nb]PQ∥.(9)\lVert(Q-p(C))PQ\rVert\le e^{-N^a} + (1+e^{N^u})\lVert[C \ge N^b]PQ\rVert. \tag*{(9)}

The remaining factor is exactly the transition controlled by the inverse circuit. Unitary conjugation gives

∥[C≥Nb]PQ∥=∥[D≥Nb]U†[M=0]U[D=0]∥≤e−Nt.(10)\begin{aligned} \lVert[C \ge N^b]PQ\rVert &= \lVert[D \ge N^b]U^\dagger[M=0]U[D=0]\rVert\\ &\le e^{-N^t}. \tag*{(10)} \end{aligned}

Here Bd(t,b)\mathcal{B}_d(t,b) applies with circuit U†U^\dagger, mismatch count DD, and projected count MM. Inverse closure (2) and the universal quantifiers in Bd(t,b)\mathcal{B}_d(t,b) are both used.

Combining (6), (8), (9), and (10) yields

∥HQP∥2≤eNu−Nw+e−Na+(1+eNu)e−Nt.(11)\lVert HQP\rVert^2 \le e^{N^u-N^w} + e^{-N^a} + (1+e^{N^u})e^{-N^t}. \tag*{(11)}

By (5.1), each term is eventually at most 13e−2Ns\frac{1}{3}e^{-2N^s}. Indeed w>uw>u, t>ut>u, and a,w,t>sa,w,t>s. This remains true for s=0s=0, when the comparison quantity is a fixed positive constant. Taking the square root proves Bd(s,t)\mathcal{B}_d(s,t). All sufficient lower bounds on NN depend only on the fixed parameters and dd, so the conclusion is uniform. ∎

We now choose a finite chain of scales within this interval. Each step will advance the mismatch exponent by almost the current gap t−st-s. Keeping at least half of the initial gap for O(1/(t−s))O(1/(t-s)) steps will carry that exponent above one, where the tail projection vanishes. A slack of order (t−s)2(t-s)^2 per step is small enough to preserve the gap.

Proof of Theorem 2. The case d=0d=0 is Lemma 4. Fix d≥1d \ge1, and assume the theorem at depth d−1d-1 for every fixed exponent pair. It remains to prove Bd(s,t)\mathcal{B}_d(s,t) for fixed 0≤s<t≤10 \le s < t \le1; the case t>1t>1 is immediate. Put

g=t−s,η=g2100,s0=s,t0=t,g=t-s,\qquad\eta=\frac{g^2}{100},\qquad s_0=s,\qquad t_0=t,

and define

si+1=ti,ti+1=2ti−si−3η.s_{i+1}=t_i,\qquad t_{i+1}=2t_i-s_i-3\eta.

Writing gi=ti−sig_i=t_i-s_i, we have

gi=g−3iη,ti+1−ti=gi+1.g_i=g-3i\eta,\qquad t_{i+1}-t_i=g_{i+1}.

Let K=⌈2/g⌉K=\lceil2/g\rceil. Since 0<g≤10<g\le1,

3Kη≤3(2/g+1)g2100≤0.09g<g2.3K\eta\le\frac{3(2/g+1)g^2}{100}\le0.09g<\frac{g}{2}.

Thus gi>g/2g_i>g/2 for i≤Ki\le K, and

tK=t+∑i=1Kgi>t+Kg/2≥t+1>1.t_K=t+\sum_{i=1}^{K}g_i>t+Kg/2\ge t+1>1.

Let J≤KJ\le K be the first index for which tJ>1t_J>1. This index and every exponent in the chain are independent of NN. The assertion Bd(sJ,tJ)\mathcal{B}_d(s_J,t_J) is trivial.

Suppose now that Bd(si+1,ti+1)\mathcal{B}_d(s_{i+1},t_{i+1}) has been proved, where i<Ji<J. The recurrence and the positive next gap give

ti<ti+1=2ti−si−3η<2ti−si.t_i<t_{i+1}=2t_i-s_i-3\eta<2t_i-s_i.

Thus Lemma 7 applies with b=ti+1b=t_{i+1}. Its assumed assertion is precisely Bd(ti,ti+1)=Bd(si+1,ti+1)\mathcal{B}_d(t_i,t_{i+1})=\mathcal{B}_d(s_{i+1},t_{i+1}), so it proves Bd(si,ti)\mathcal{B}_d(s_i,t_i). Working backward reaches the target pair, as in Figure 1.

Same-depth induction along a finite chain

Figure 1. The same-depth induction runs from right to left along a finite chain; JJ is the first index with tJ>1t_J>1. Each implication is Lemma 7 and also uses the already established localization theorem at depth d−1d-1. The inverse circuit is substituted only into the universal statement at the next pair, after that statement has been proved.

There are only finitely many steps for each fixed d,s,td,s,t. Taking the maximum of their sufficient lower bounds on NN preserves uniformity over every circuit and pair of counts. Each step uses only finitely many fixed exponent tuples from depth d−1d-1; the number of monomials and their varying supports are paid for by the explicit coefficient estimates, not by further asymptotic thresholds. Thus the induction does not require a threshold uniform over all real exponent pairs. This completes the depth induction.

From localization to parity

We finish by relating the output probability to transitions between product states. All localization estimates have already been proved; no assumption about coherent or clean computation is needed here. For the broader Fourier-concentration setting, see [10]; the character-orthogonality identity needed here is proved directly.

Proof of Theorem 1. Suppose that a circuit as in the theorem exists on nn input qubits and N−nN-n initially zero ancillas, with n≤N≤ncn \le N \le n^c. Retain any discarded qubits as idle wires and write WW for the resulting unitary. By Section 2, W∈Ud(N)W \in\mathcal{U}_d(N) after padding with identity layers. Let OO project the output qubit onto ∣0⟩|0\rangle, and put

B=W†OW,p0(x)=⟨x,0∣B∣x,0⟩.B = W^\dagger O W,\qquad p_0(x) = \langle x,0|B|x,0\rangle.

The Born rule identifies p0(x)p_0(x) with the probability of output zero, irrespective of the final states of the other qubits. Here and below the last zero denotes all initially zero ancillas.

For h∈{0,1}nh \in\{0,1\}^n, define

∣ξh⟩=⨂j=1n∣0⟩+(−1)hj∣1⟩2,hˉ=(1−h1,…,1−hn).|\xi_h\rangle= \bigotimes_{j=1}^{n} \frac{|0\rangle+ (-1)^{h_j}|1\rangle}{\sqrt{2}},\qquad\bar{h} = (1-h_1,\ldots,1-h_n).

Let MhM_h be the count on the input qubits whose reference vectors are the factors of ξh\xi_h. The vectors ∣ξh,0⟩|\xi_h,0\rangle and ∣ξhˉ,0⟩|\xi_{\bar{h}},0\rangle have exact counts zero and nn, respectively. Choose fixed 0<s<t<1/c0 < s < t < 1/c. For all sufficiently large nn, Nt≤nct<nN^t \le n^{ct} < n. Since OO is a product projection and W†∈Ud(N)W^\dagger\in\mathcal{U}_d(N), (13) gives

∣⟨ξhˉ,0∣B∣ξh,0⟩∣≤e−Nsfor every h.(12)|\langle\xi_{\bar{h}},0|B|\xi_h,0\rangle| \le e^{-N^s}\qquad\text{for every }h. \tag*{(12)}

Its uniformity in the count makes the same lower bound on NN valid for all hh.

Averaging these complementary matrix entries gives the parity Fourier coefficient of p0p_0, namely 2−n∑x(−1)∣x∣p0(x)2^{-n}\sum_x(-1)^{|x|}p_0(x), where ∣x∣=∑jxj|x|=\sum_j x_j. To see this, note that ⟨x∣ξh⟩=2−n/2(−1)h⋅x\langle x|\xi_h\rangle=2^{-n/2}(-1)^{h\cdot x}, where the dot product is taken modulo two. Also, (−1)hˉ⋅x=(−1)∣x∣+h⋅x(-1)^{\bar{h}\cdot x}=(-1)^{|x|+h\cdot x}. Character orthogonality therefore gives

Eh⟨ξhˉ,0∣B∣ξh,0⟩=2−n∑x,y(−1)∣x∣Eh(−1)h⋅(x+y)⟨x,0∣B∣y,0⟩=2−n∑x(−1)∣x∣p0(x).(13)\mathbb{E}_h\langle\xi_{\bar{h}},0|B|\xi_h,0\rangle =2^{-n}\sum_{x,y}(-1)^{|x|}\mathbb{E}_h(-1)^{h\cdot(x+y)}\langle x,0|B|y,0\rangle =2^{-n}\sum_x(-1)^{|x|}p_0(x). \tag*{(13)}

The addition in x+yx+y in the character is modulo two. For even xx, the success guarantee gives p0(x)≥1/2+εp_0(x)\ge1/2+\varepsilon; for odd xx, it gives p0(x)≤1/2−εp_0(x)\le1/2-\varepsilon. The even and odd classes have equal size, so the final expression in (13) is at least ε\varepsilon. But (12) bounds its absolute value by e−Nse^{-N^s}, which tends to zero because N≥nN\ge n. This contradiction proves the theorem.

The role of a polynomial qubit bound is solely the choice of 0<s<t<1/c0<s<t<1/c. The localization theorem itself is uniform on NN qubits and does not assume any relation between NN and an input length. The proof gives no claim of the same lower bound when the ancillary register is allowed to be superpolynomial.

Consequences of localization and parity

The direct parity proof is complete. Localization next bounds complementary-output probabilities, and a construction of Gretta, Gupta, and Joshi [11] gives a Dicke-state obstruction. We also derive scalar-output Fourier concentration directly from localization. This concentration rules out high average accuracy for majority, while Xu and Li’s reductions [25] give worst-case obstructions for symmetric functions. Throughout, discarded registers remain unrestricted.

State preparation

Gretta, Gupta, and Joshi [11] connect complementary-output probabilities and Dicke-state preparation to parity. Here localization bounds the complementary probabilities directly; their block construction then gives the Dicke-state consequence. For an nn-qubit density operator ρ\rho, write

py=⟨y∣ρ∣y⟩,Fn(ρ)=2∑y∈{0,1}npypyˉ.p_y = \langle y \mid\rho\mid y \rangle,\qquad\mathcal{F}_n(\rho) = 2\sum_{y\in\{0,1\}^n} p_y p_{\bar{y}}.

where yˉ\bar{y} is the bitwise complement of yy. This is the felinity of ρ\rho [11], Definition 2.1]. Also write

∣Dkn⟩=(nk)−1/2∑∣y∣=k∣y⟩,TD⁡(ρ,σ)=12∥ρ−σ∥1\lvert D_k^n\rangle= \binom{n}{k}^{-1/2}\sum_{\lvert y\rvert=k}\lvert y\rangle,\qquad\operatorname{TD}(\rho,\sigma)=\frac{1}{2}\lVert\rho-\sigma\rVert_1

for the weight-kk Dicke state and trace distance, respectively.

Corollary 8 (State-preparation obstructions). Fix a nonnegative integer dd, c≥1c \ge1, a>0a > 0, and 0<δ<10 < \delta< 1. For all sufficiently large nn, every nn-qubit reduced state ρ\rho prepared from zero inputs by an allowed depth-at-most-dd circuit on at most ncn^c total qubits satisfies

Fn(ρ)<n−a.\mathcal{F}_n(\rho) < n^{-a}.

Moreover, for every integer kk with nδ≤k≤n/2n^\delta\le k \le n/2,

TD⁡(ρ,∣Dkn⟩⟨Dkn∣)>180k.\operatorname{TD}\left(\rho,\lvert D_k^n\rangle\langle D_k^n\rvert\right) > \frac{1}{80k}.

The remaining qubits may be discarded in arbitrary final states.

Proof. Retain all NN preparation qubits, including those eventually discarded, and write ∣ψ⟩=U∣0N⟩\lvert\psi\rangle= U\lvert0^N\rangle and Q=∣ψ⟩⟨ψ∣Q = \lvert\psi\rangle\langle\psi\rvert. Thus QQ is the conjugate by U∈Ud(N)U \in\mathcal{U}_d(N) of a product projection. For an output string yy, let PyP_y fix the nn output qubits to yy and act identically on the remaining register, and let MyM_y count mismatches from yy on the outputs. Then Py=[My=0]P_y = [M_y = 0] and ∥Pyψ∥2=py\lVert P_y\psi\rVert^2 = p_y. Fix 0<s<t<1/c0 < s < t < 1/c. For sufficiently large nn, Nt<nN^t < n, so the complementary-string projection satisfies Py‾≤[My≥Nt]\overline{P_y} \le[M_y \ge N^t]. Localization gives

pypyˉ=∥PyˉQPy∥≤e−Nsfor every y.\sqrt{p_y p_{\bar{y}}} = \lVert P_{\bar{y}} Q P_y\rVert\le e^{-N^s}\qquad\text{for every }y.

The threshold is uniform in yy. Cauchy–Schwarz gives ∑ypypyˉ≤1\sum_y \sqrt{p_y p_{\bar{y}}} \le1, and hence

Fn(ρ)≤2e−Ns∑ypypyˉ≤2e−Ns<n−a\mathcal{F}_n(\rho) \le2e^{-N^s}\sum_y\sqrt{p_y p_{\bar{y}}} \le2e^{-N^s} < n^{-a}

eventually. This argument uses the pure state on the complete register, so it applies to every reduced output state ρ\rho.

For the second assertion, we give the block construction underlying [10], including the estimates needed at the stated trace distance. Put

ℓ=⌊klog⁡k⌋,p=kn,∣v⟩=1−p∣0⟩+p∣1⟩.\ell= \left\lfloor\frac{k}{\log k} \right\rfloor,\qquad p = \frac{k}{n},\qquad|v\rangle= \sqrt{1-p}|0\rangle+ \sqrt{p}|1\rangle.

Partition the nn sites into ℓ\ell blocks BjB_j whose sizes bjb_j differ by at most one. Append one zero qubit tjt_j per block, and on BjtjB_jt_j apply

(I−Aj)⊗I+Aj⊗X,Aj=(∣v⟩⟨v∣)⊗bj.(I-A_j)\otimes I + A_j\otimes X,\qquad A_j = (|v\rangle\langle v|)^{\otimes b_j}.

Each gate equals I−2Aj⊗∣−⟩⟨−∣I-2A_j\otimes|-\rangle\langle-|, so all these gates form one disjoint product-reflection layer, implemented by parallel one-qubit basis changes, one Toffoli layer, and the inverse basis changes. Let σ∗\sigma_* be the resulting state of the ℓ\ell new qubits when the input is ∣Dkn⟩|D_k^n\rangle. Its all-one probability is

r1=∣⟨v⊗n∣Dkn⟩∣2=(nk)pk(1−p)n−k.r_1 = |\langle v^{\otimes n}|D_k^n\rangle|^2 = \binom{n}{k}p^k(1-p)^{n-k}.

For a binomial random variable BB with parameters n,pn,p, the integer kk is a mode and Var⁡(B)≤k\operatorname{Var}(B)\le k. Chebyshev’s inequality gives

(4k+1)r1≥Pr⁡(∣B−k∣<2k)≥34,r1≥(316−o(1))k−1/2,(4\sqrt{k}+1)r_1 \ge\Pr(|B-k|<2\sqrt{k})\ge\frac{3}{4},\qquad r_1\ge\left(\frac{3}{16}-o(1)\right)k^{-1/2},

since the displayed interval contains at most 4k+14\sqrt{k}+1 integers. This estimate is uniform in n≥2kn\ge2k. The all-zero probability is r0=∥Π∣Dkn⟩∥2r_0=\|\Pi|D_k^n\rangle\|^2, where Π=∏j(I−Aj)\Pi=\prod_j(I-A_j). To bound it, use the unit vector

∣ν⟩=(1−p∣0⟩−p∣1⟩)⊗n.| \nu\rangle= (\sqrt{1-p}|0\rangle-\sqrt{p}|1\rangle)^{\otimes n}.

Since bj≥n/ℓ−1b_j\ge n/\ell-1, p≤1/2p\le1/2, and k/ℓ≥log⁡kk/\ell\ge\log k,

⟨ν∣Aj∣ν⟩=(1−2p)2bj≤e−4pbj≤e2k−4.\langle\nu|A_j|\nu\rangle=(1-2p)^{2b_j}\le e^{-4pb_j}\le e^2k^{-4}.

The commuting projections satisfy I−Π≤∑jAjI-\Pi\le\sum_j A_j, so ∥(I−Π)ν∥≤ek−3/2\|(I-\Pi)\nu\|\le ek^{-3/2}. Moreover, ∣⟨ν∣Dkn⟩∣=r1|\langle\nu|D_k^n\rangle|=\sqrt{r_1}, because every term of the Dicke state has weight kk. Therefore

r0≥r1−ek−3/2,Fℓ(σ∗)≥4r0r1≥9/64−o(1)k>18k.\sqrt{r_0}\ge\sqrt{r_1}-ek^{-3/2},\qquad\mathcal{F}_{\ell}(\sigma_*)\ge4r_0r_1\ge\frac{9/64-o(1)}{k}>\frac{1}{8k}.

All errors here are uniform for k≤n/2k\le n/2 as k→∞k\to\infty. The factor four counts both complementary strings in the definition of felinity.

Apply the same block circuit to ρ\rho, and call its new-qubit state σ\sigma. Trace distance contracts under a unitary and partial trace. Also, for any two states τ,τ′\tau,\tau' with computational-basis probabilities q,q′q,q', the definition gives

∣Fℓ(τ)−Fℓ(τ′)∣≤4∑y∣qy−qy′∣≤8TD⁡(τ,τ′).|\mathcal{F}_{\ell}(\tau)-\mathcal{F}_{\ell}(\tau')|\le4\sum_y|q_y-q'_y|\le8\operatorname{TD}(\tau,\tau').

Thus TD⁡(ρ,∣Dkn⟩⟨Dkn∣)≤1/(80k)\operatorname{TD}(\rho,|D_k^n\rangle\langle D_k^n|)\le1/(80k) would imply

Fℓ(σ)>18k−880k=140k.\mathcal{F}_{\ell}(\sigma)>\frac{1}{8k}-\frac{8}{80k}=\frac{1}{40k}.

For large kk, ℓ≥k\ell\ge\sqrt{k}, while k≥nδk\ge n^\delta gives n≤ℓ2/δn\le\ell^{2/\delta}. The preparation of σ\sigma therefore has fixed depth and polynomially many total qubits as a function of ℓ\ell. But ℓ2/k→∞\ell^2/k\to\infty, so its felinity exceeds ℓ−2\ell^{-2} eventually, contrary to the first assertion applied with target size ℓ\ell and exponent a=2a=2. Since k≥nδ→∞k\ge n^\delta\to\infty, all thresholds can be chosen uniformly over the allowed kk. ∎

In particular, no such family can assign inverse-polynomial probabilities to both a string and its complement: their two terms contribute 4pypyˉ4p_y p_{\bar{y}} to Fn(ρ)\mathcal{F}_n(\rho).

The polynomial bound in Corollary 8 is measured in the number nn of target qubits. Gretta, Gupta, and Joshi [11], Theorem 1.1 show that every nn-qubit pure state can be prepared exactly at constant depth with 2O(n)2^{O(n)} ancillas, all returned to zero.

Scalar-output Fourier concentration

Gretta, Gupta, and Joshi [10], Conjecture 1 and Corollary 1.2 formulate a qualitative Quantum-LMN statement and establish its equivalence with the parity lower-bound question. Our localization theorem gives this Fourier-concentration statement directly. For an nn-input circuit CC on NN total qubits with output qubit tt, define its expected measured sign and uniform-input Fourier coefficients by

fC(x)=⟨x,0N−n∣C†ZtC∣x,0N−n⟩∈[−1,1],f_C(x) = \langle x,0^{N-n}|C^\dagger Z_t C|x,0^{N-n}\rangle\in[-1,1],
fC^(S)=2−n∑x∈{0,1}nfC(x)(−1)∑i∈Sxi.\widehat{f_C}(S) = 2^{-n} \sum_{x\in\{0,1\}^n} f_C(x)(-1)^{\sum_{i\in S}x_i}.

Write W≥k[fC]=∑∣S∣≥k∣fC^(S)∣2W_{\geq k}[f_C] = \sum_{|S|\geq k}|\widehat{f_C}(S)|^2. This is the absolute squared Fourier tail, not a fraction of the total weight ExfC(x)2≤1\mathbb{E}_x f_C(x)^2 \leq1.

Corollary 9 (Qualitative scalar-output Quantum-LMN). For every fixed nonnegative integer dd, there is a positive function γd\gamma_d on the positive integers, depending only on dd, such that γd(k)/kA→∞\gamma_d(k)/k^A \to\infty for every fixed A>0A>0, and every allowed depth-at-most-dd circuit CC on nn inputs and NN total qubits, every designated output tt, and every integer 1≤k≤n1 \leq k \leq n satisfy

W≥k[fC]≤Nγd(k).W_{\geq k}[f_C] \leq\frac{N}{\gamma_d(k)}.

In particular, fix c≥1c \geq1, 0<δ≤10 < \delta\leq1, and B>0B > 0. For all sufficiently large nn, uniformly over these circuits with N≤ncN \leq n^c,

W≥⌈nδ⌉[fC]≤n−B.W_{\geq\lceil n^\delta\rceil}[f_C] \leq n^{-B}.

The sufficient threshold depends only on dd, cc, δ\delta, BB.

Proof. Fix a circuit CC and let Q=C†O0CQ = C^\dagger O_0 C, where O0O_0 projects its output qubit onto ∣0⟩|0\rangle. For h∈{0,1}nh \in\{0,1\}^n, let ξh\xi_h be the Hadamard product vector from the proof of Theorem 1, and let MhM_h count mismatches from its factors on the nn input qubits. For S⊆[n]S \subseteq[n], write 1S\mathbf{1}_S for its indicator string. The character calculation in (6.2), with hˉ\bar{h} replaced by h⊕1Sh \oplus\mathbf{1}_S, gives

fC^(S)=2Eh⟨ξh⊕1S,0∣Q∣ξh,0⟩(S≠∅),\widehat{f_C}(S) = 2\mathbb{E}_h\langle\xi_{h\oplus\mathbf{1}_S},0|Q|\xi_h,0\rangle\qquad(S\ne\varnothing),

since fC(x)=2⟨x,0∣Q∣x,0⟩−1f_C(x) = 2\langle x,0|Q|x,0\rangle- 1. For fixed hh, the vectors ∣ξh⊕1S,0⟩|\xi_{h\oplus\mathbf{1}_S},0\rangle are orthonormal as SS varies, and their MhM_h counts are exactly ∣S∣|S|. Jensen’s and Bessel’s inequalities therefore yield

W≥k[fC]≤4Eh∑∣S∣≥k∣⟨ξh⊕1S,0∣Q∣ξh,0⟩∣2≤4sup⁡h∥[Mh≥k]Q[Mh=0]∥2.(14)\begin{aligned} W_{\geq k}[f_C] &\leq4\mathbb{E}_h \sum_{|S|\geq k} \left|\langle\xi_{h\oplus\mathbf{1}_S},0|Q|\xi_h,0\rangle\right|^2 \\ &\leq4\sup_h \left\|[M_h\geq k]Q[M_h=0]\right\|^2. \tag*{(14)} \end{aligned}

For any fixed 0<σ<τ0 < \sigma< \tau, Theorem 2 bounds this by 4e−2Nσ4e^{-2N^\sigma} whenever NN is sufficiently large and k≥Nτk \ge N^\tau. The threshold depends only on d,σ,τd,\sigma,\tau.

It remains to obtain one function of kk valid for every circuit size. For each positive integer kk, define

bd(k)=sup⁡W≥k[fC]N,b_d(k) = \sup\frac{W_{\geq k}[f_C]}{N},

where the supremum ranges over all allowed depth-at-most-dd circuits, all designated outputs, and all input and total sizes k≤n≤Nk \leq n \leq N. Parseval’s identity gives W≥k[fC]≤ExfC(x)2≤1W_{\geq k}[f_C] \leq\mathbb{E}_x f_C(x)^2 \leq1, so 0≤bd(k)≤1/k0 \leq b_d(k) \leq1/k. Fix A≥1A \geq1. If N≥kAN \geq k^A, then W≥k[fC]/N≤k−AW_{\geq k}[f_C]/N \leq k^{-A}. For the remaining sizes k≤N<kAk \leq N < k^A, choose fixed 0<σ<τ<1/A0 < \sigma< \tau< 1/A. For sufficiently large kk, we have Nτ<kN^\tau< k, so (14) gives

W≥k[fC]N≤4e−2kσk.\frac{W_{\geq k}[f_C]}{N} \leq\frac{4e^{-2k^\sigma}}{k}.

These two bounds are uniform over the supremum. Since AA is arbitrary, bd(k)=o(k−B)b_d(k) = o(k^{-B}) for every fixed B>0B > 0. Thus the positive function

γd(k)=1bd(k)+e−k\gamma_d(k) = \frac{1}{b_d(k) + e^{-k}}

satisfies γd(k)/kB→∞\gamma_d(k)/k^B \to\infty for every B>0B > 0, and the definition of bdb_d gives W≥k[fC]≤N/γd(k)W_{\geq k}[f_C] \leq N/\gamma_d(k). Finally, choose B′>(c+B)/δB' > (c+B)/\delta in this superpolynomial growth property to obtain the asserted cutoff consequence.

Majority and symmetric functions

The reductions of [25] turn the parity lower bound into a worst-case lower bound for majority and broader symmetric families. For a symmetric fn:{0,1}n→{0,1}f_n : \{0,1\}^n \to\{0,1\}, let fn,if_{n,i} be its value on inputs of Hamming weight ii, and define its transition radius by

ρ(fn)=max⁡0≤i<nfn,i≠fn,i+1min⁡{i+1,n−i},\rho(f_n) = \max_{\substack{0 \leq i < n \\ f_{n,i} \ne f_{n,i+1}}} \min\{i+1,n-i\},

with ρ(fn)=0\rho(f_n) = 0 for a constant function. Write deg⁡~1/3(fn)\widetilde{\deg}_{1/3}(f_n) for the least total degree of a real polynomial approximating fnf_n pointwise within 1/31/3. For nonconstant symmetric functions, Paturi’s characterization [22] gives

deg⁡~1/3(fn)=Θ(nρ(fn)).\widetilde{\deg}_{1/3}(f_n) = \Theta\left(\sqrt{n\rho(f_n)}\right).

Thus the approximate-degree hypothesis below also forces a polynomially large transition radius.

Corollary 10 (Majority and symmetric functions). Let (fn)(f_n) be a symmetric Boolean family satisfying either ρ(fn)≥nδ\rho(f_n) \geq n^\delta for some fixed δ>0\delta> 0, or deg⁡~1/3(fn)=Ω(n1/2+η)\widetilde{\deg}_{1/3}(f_n) = \Omega(n^{1/2+\eta}) for some fixed η>0\eta> 0, for all sufficiently large nn. For every fixed γ>0\gamma> 0, no nonuniform family in the circuit model of Theorem 1, with fixed depth and polynomially many total qubits, computes fnf_n with probability at least 1/2+1/(log⁡n)γ1/2 + 1/(\log n)^\gamma on every input for all sufficiently large nn. In particular, this excludes strict majority MAJn(x)=1{∣x∣>n/2}\mathrm{MAJ}_n(x) = 1\{|x| > n/2\}, whose transition radius is ⌈n/2⌉\lceil n/2\rceil.

Proof. Xu and Li’s Theorem 16 and Corollaries 2–3 [25] turn a family satisfying either hypothesis and the stated success bound into an exact, clean implementation of fanout on nn targets, with constant entangling depth and polynomially many ancillas. Their circuit convention [25] requires the measured output to be an initially zero ancilla; appending one fresh zero qubit and a CNOT from our designated output preserves its measurement distribution, even with arbitrary garbage. Their entangling depth DD uses at most 2D+12D+1 of our layers. Thus the reduction stays within fixed depth and polynomial total qubits. Hadamard conjugation on the fanout data wires gives the exact parity unitary; a zero target and its final measurement contradict Theorem 1. Finite exceptional input lengths do not affect this circuit-family contradiction.

There is consequently a strict separation between the Boolean families computed with worst-case success at least 2/3 in our model and in the matched model obtained by adjoining unit-cost reversible unbounded-arity threshold gates

∣x,b⟩⟼∣x,b⊕1{∣x∣≥t}⟩,t∈{0,…,n},|x,b\rangle\longmapsto|x,b \oplus1_{\{|x| \ge t\}}\rangle,\qquad t \in\{0,\ldots,n\},

while retaining the same depth, disjoint-support, qubit, ancilla, and output conventions. The enlarged model contains the original one and computes strict majority exactly with one such gate at t=⌊n/2⌋+1t=\lfloor n/2\rfloor+1, whereas Corollary 10 excludes even worst-case success 2/3 for majority in the original model.

High average accuracy for majority

The preceding obstruction assumes an advantage on every input. The high-average-accuracy consequence of Gretta, Gupta, and Joshi [10], Corollary 4.6 also follows directly from our Fourier-concentration bound: majority retains a polynomial Fourier tail at a polynomially growing cutoff.

Corollary 11 (High-average-accuracy majority obstruction). For every fixed δ>0\delta>0, no nonuniform family (Cn)(C_n) in the circuit model of Theorem 1, with fixed depth and polynomially many total qubits, satisfies

2−n∑x∈{0,1}nfCn(x)(−1)MAJ⁡n(x)≥1−n−δ2^{-n}\sum_{x\in\{0,1\}^{n}} f_{C_n}(x)(-1)^{\operatorname{MAJ}_n(x)} \ge1-n^{-\delta}

for all sufficiently large nn. Here fCn(x)∈[−1,1]f_{C_n}(x)\in[-1,1] is the expected measured sign: the probability of output zero minus the probability of output one. Equivalently, no such family computes strict majority with average success at least 1−12n−δ1-\frac{1}{2}n^{-\delta}, where the average is over uniform inputs and the output measurement.

Proof. Suppose such a family exists, restrict to odd nn, and put gn(x)=(−1)MAJ⁡n(x)g_n(x)=(-1)^{\operatorname{MAJ}_n(x)} and δ0=min⁡{δ,1/4}\delta_0=\min\{\delta,1/4\}. Since ∣fCn∣≤1|f_{C_n}|\le1 and gn2=1g_n^2=1, the asserted correlation gives

∥fCn−gn∥22≤2(1−ExfCn(x)gn(x))≤2n−δ0,\lVert f_{C_n}-g_n\rVert_2^2 \le2\left(1-\mathbb{E}_x f_{C_n}(x)g_n(x)\right)\le2n^{-\delta_0},

where the norm uses the uniform probability measure.

We use the following finite-size majority tail estimate: for ε≥n−1/3\varepsilon\ge n^{-1/3} and sufficiently large odd nn,

W≥k[gn]>εwhenever k is odd and 1≤k≤116ε2.W_{\ge k}[g_n]>\varepsilon\qquad\text{whenever }k\text{ is odd and }1\le k\le\frac{1}{16\varepsilon^2}.

This is [19], Theorem 3.5.6, p. 50. Set ε=4n−δ0\varepsilon=4n^{-\delta_0} and let knk_n be the largest odd integer at most n2δ0/112n^{2\delta_0}/112. These parameters satisfy the estimate’s hypotheses for all sufficiently large odd $n.

Parseval’s identity and the triangle inequality for the Fourier coefficients at degrees at least knk_n now give

W≥kn[fCn]≥W≥kn[gn]−∥fCn−gn∥2>(2−2)n−δ0/2.\sqrt{W_{\geq k_n}[f_{C_n}]} \geq\sqrt{W_{\geq k_n}[g_n]}-\lVert f_{C_n}-g_n\rVert_2 > (2-\sqrt{2})n^{-\delta_0/2}.

On the other hand, kn≥⌈nδ0⌉k_n \geq\lceil n^{\delta_0}\rceil eventually. Applying Corollary 9 at the latter cutoff, with B=δ0+1B=\delta_0+1, yields W≥kn[fCn]≤n−(δ0+1)W_{\geq k_n}[f_{C_n}] \leq n^{-(\delta_0+1)}, a contradiction. □\square

This conclusion does not assert a constant average-case gap or exclude 1−1/polylog⁡n1-1/\operatorname{polylog} n correlation.

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