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Harper's beyond square-root conjecture for random matrices

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Abstract

For a Haar unitary matrix UNU_N of size NN, we prove that the first absolute moment of tr⁡(Sym⁡kUN)\operatorname{tr}(\operatorname{Sym}^k U_N) tends to zero as min⁡(N,k)→∞\min(N,k)\to\infty. This settles the random matrix version of Harper's beyond square-root conjecture formulated by Wang and Xu, with no restriction on k/Nk/N. The proof is elementary and self-contained, combining exact weighted trace moments with a Gaussian change of measure. It also connects the result to the critical chaos model studied by Soundararajan and Zaman, also known as holomorphic multiplicative chaos.

Introduction

Background

Harper’s theorem on “better than square-root cancellation” in partial sums of random multiplicative functions [6] marked a major advance in probabilistic number theory, revealing a surprising connection with critical multiplicative chaos. We refer to [8, 9] for surveys of these ideas and their number theoretic significance.

A particularly attractive feature of Harper’s theorem is that it also sheds light on fundamental deterministic problems in number theory. For example, using a derandomization argument, Harper [7] proved that for a prime modulus rr,

1r−1∑χ mod r∣∑n≤xχ(n)∣=o(x)\frac{1}{r-1}\sum_{\chi\bmod r}\left|\sum_{n\le x}\chi(n)\right|=o(\sqrt{x})

whenever min⁡(x,r/x)→∞\min(x,r/x)\to\infty. An analogous result holds for the continuous family nitn^{it}, averaged over ∣t∣≤T|t|\le T, when min⁡(x,T/x)→∞\min(x,T/x)\to\infty. A further application to Möbius cancellation is particularly striking: Harper proved that the same phenomenon holds in the same range after twisting by the Möbius function μ\mu, and he conjectured that this should hold for x≤r100x\le r^{100}. It turns out that this seemingly unimportant summation range x≤r100x\le r^{100} is crucial. Indeed, it is not hard to show that if Harper’s conjecture holds, then Möbius cancellation holds in the form

∑x≤n≤x+yμ(n)=o(y)\sum_{x\le n\le x+y}\mu(n)=o(y)

as long as y≫x/W(x)y\gg\sqrt{x}/W(x) for some W(x)W(x) tending to infinity. In fact, Harper’s conjecture is quantitative, and as a corollary, one can take W(x)=(log⁡log⁡x)cW(x)=(\log\log x)^c for any fixed 0<c<1/40<c<1/4. This would break the famous square-root barrier, which remains out of reach even under the Riemann Hypothesis. See also [7, 9]. In [17], Wang and Xu managed to prove the discrete version of Harper’s conjecture under strong assumptions, namely the Ratios conjecture and the Generalized Riemann Hypothesis.

In this paper, we establish Harper’s conjecture unconditionally in the random matrix setting, which one may also view as a function field analogue. Since Möbius twists occur as coefficients in the Dirichlet series of reciprocals of LL-functions, the relevant random matrix quantities are the coefficients

hk(U)=[zk]det⁡(I−zU)−1=tr⁡(Sym⁡kU),U∈U(N).(1)h_k(U)=[z^k]\det(I-zU)^{-1}=\operatorname{tr}(\operatorname{Sym}^{k}U),\qquad U\in U(N). \tag*{(1)}

Wang and Xu conjectured that the corresponding first absolute moment tends to 0 as k→∞k\to\infty, provided k≤BNk\le BN for a fixed B>0B>0 [17 Conjecture 1.5]. In the arithmetic analogy, kk corresponds to log⁡x\log x and NN to the logarithm of the conductor, so a bounded ratio k/Nk/N corresponds to sums of length at most a fixed power of the conductor. We prove their conjecture in a stronger form, i.e., with no restriction on k/Nk/N.

Main result

We write EU(N)\mathbb{E}_{U(N)} for integration against the normalized Haar measure on U(N)U(N), and E\mathbb{E} for expectation over the auxiliary random variables introduced below.

Theorem 1.1. Let UNU_N be Haar distributed on U(N)U(N). Then

EU(N)∣tr⁡(Sym⁡kUN)∣⟶0as min⁡(N,k)⟶∞.\mathbb{E}_{U(N)}\left|\operatorname{tr}(\operatorname{Sym}^{k} U_N)\right| \longrightarrow0 \qquad\text{as } \min(N,k) \longrightarrow\infty.

The conclusion also holds with the first moment replaced by any fixed ppth absolute moment, 0<p<20 < p < 2, by Jensen’s inequality and interpolation with the second moment, which equals exactly one by Schur orthogonality. The methods here can likely be adapted to other compact groups, e.g., the symplectic and orthogonal families. See also [5, 18] for related recent arithmetic developments.

Remark 1.2. In view of the arithmetic applications discussed above, Theorem 1.1 should also yield cancellation in Möbius sums over function fields for short intervals below the square-root barrier. Stronger estimates in the large-field setting have already been obtained by Sawin [14], using different methods.

Connections with function fields and multiplicative chaos

The relation with function fields is explicit. For a primitive odd Dirichlet character χ\chi modulo a monic squarefree polynomial Q∈Fq[T]Q \in\mathbb{F}_q[T], with deg⁡Q≥2\deg Q \ge2, write L(u,χ)=det⁡(I−quΘχ)L(u,\chi) = \det(I - \sqrt{q}u\Theta_\chi), where Θχ∈U(deg⁡Q−1)\Theta_\chi\in U(\deg Q - 1). Then

q−k/2∑f monicdeg⁡f=kμ(f)χ(f)=hk(Θχ).q^{-k/2}\sum_{\substack{f\ \mathrm{monic}\\ \deg f=k}}\mu(f)\chi(f)=h_k(\Theta_\chi).

Katz’s equidistribution theorem [10] shows that averages over these characters converge to Haar averages as q→∞q \to\infty at fixed kk and conductor degree. This gives a function field interpretation of our theorem, with the field size tending to infinity first. See also work of Gorodetsky [4].

The relation between random multiplicative functions and critical chaos has been instrumental in many recent works. See [16 Section 1.6] for a recent account. This becomes especially transparent through the multiplicative chaos model studied by Soundararajan and Zaman [15]. Let X(j)X(j) be independent standard complex Gaussian random variables, and define A(k)A(k) by

∑k≥0A(k)zk=exp⁡(∑j≥1X(j)jzj).(2)\sum_{k\ge0} A(k)z^k=\exp\left(\sum_{j\ge1}\frac{X(j)}{\sqrt{j}}z^j\right). \tag*{(2)}

The random power series in (2) is also studied as critical holomorphic multiplicative chaos by Najnudel, Paquette and Simm [12]. These coefficients arise as large-field limits of normalized sums of Steinhaus random multiplicative functions over polynomials of fixed degree [15]. For fixed kk, they also arise as the limits in distribution of hk(UN)h_k(U_N) as N→∞N \to\infty, by the trace limit theorem of Diaconis and Shahshahani [3]. Soundararajan and Zaman proved

E∣A(k)∣2=1,E∣A(k)∣≍(log⁡k)−1/4.\mathbb{E}|A(k)|^2=1,\qquad\mathbb{E}|A(k)|\asymp(\log k)^{-1/4}.

matching the saving in Harper’s theorem under the correspondence of kk with log⁡x\log x. An asymptotic refinement of this estimate was conjectured and supported numerically in [1]. Together with the second moment identity, the fixed kk convergence gives the iterated limit

lim⁡k→∞lim⁡N→∞EU(N)∣hk(UN)∣=0.\lim_{k\to\infty}\lim_{N\to\infty}\mathbb{E}_{U(N)}|h_k(U_N)|=0.

It does not, however, provide the uniformity needed when kk grows with NN.

For the ordinary characteristic polynomial, whose coefficient of zkz^k is (−1)ktr⁡(∧kUN)(-1)^k\operatorname{tr}(\wedge^k U_N), with ∧k\wedge^k denoting the kkth exterior power, Najnudel, Paquette and Simm [12, Theorem 1.2] proved convergence to zero in distribution as k→∞k \to\infty with k≤N/2k \le N/2. Since the second moment equals one, the first absolute moment also tends to zero. Our theorem concerns the symmetric powers arising from the reciprocal characteristic polynomial and allows arbitrary relative growth of kk and NN. These coefficient problems are also related to the harmonic analysis of Gaussian multiplicative chaos measures (see [13]). A further connection between our proof and critical chaos is explained in § 3.3.

Notation and preliminaries

Partitions and symmetric functions

A partition is a finite nonincreasing sequence λ=(λ1,…,λℓ)\lambda=(\lambda_1,\ldots,\lambda_\ell) of positive integers. Write ℓ(λ)=ℓ\ell(\lambda)=\ell for its length, ∣λ∣=∑iλi|\lambda|=\sum_i\lambda_i for its size and mj(λ)=#{i:λi=j}m_j(\lambda)=\#\{i:\lambda_i=j\} for the number of parts equal to jj. We write λ⊢n\lambda\vdash n if ∣λ∣=n|\lambda|=n and include the empty partition for n=0n=0. Put

zλ=∏j≥1jmj(λ)mj(λ)!.z_\lambda=\prod_{j\geq1}j^{m_j(\lambda)}m_j(\lambda)!.

For variables x1,…,xNx_1,\ldots,x_N, consider the power sums pjp_j and the complete homogeneous symmetric polynomials hnh_n, defined by

pj(x)=∑i=1Nxijandhn(x)=∑1≤i1≤⋯≤in≤Nxi1⋯xin.p_j(x)=\sum_{i=1}^{N}x_i^j \qquad\text{and}\qquad h_n(x)=\sum_{1\leq i_1\leq\cdots\leq i_n\leq N}x_{i_1}\cdots x_{i_n}.

Set h0=1h_0=1 and hn=0h_n=0 for n<0n<0. Their generating function identity is

∑n≥0hn(x)zn=∏i=1N(1−xiz)−1=exp⁡(∑j≥1pj(x)zjj).(3)\sum_{n\geq0}h_n(x)z^n=\prod_{i=1}^{N}(1-x_i z)^{-1}=\exp\left(\sum_{j\geq1}\frac{p_j(x)z^j}{j}\right). \tag*{(3)}

For algebraic calculations, regard the pjp_j as indeterminates with weighted degree jj. Expanding the exponential and grouping terms by the multiplicities of the parts gives

hn=∑λ⊢npλzλ,pλ=∏j≥1pjmj(λ).h_n=\sum_{\lambda\vdash n}\frac{p_\lambda}{z_\lambda}, \qquad p_\lambda=\prod_{j\geq1}p_j^{m_j(\lambda)}.

If the xix_i are the eigenvalues of U∈U(N)U\in U(N), then pj(U)=tr⁡Ujp_j(U)=\operatorname{tr}U^j and hn(U)=tr⁡(Sym⁡nU)h_n(U)=\operatorname{tr}(\operatorname{Sym}^n U) as in (1.1).

A Gaussian inner product

Recall that the X(j)X(j) are independent standard complex Gaussians. For g=(jX(j))j≥1\mathbf{g}=(\sqrt{j}X(j))_{j\geq1}, write P(g)P(\mathbf{g}) for the specialization pj=jX(j)p_j=\sqrt{j}X(j). In particular,

hn(g)=A(n)=∑λ⊢n∏j≥1X(j)mj(λ)jmj(λ)/2mj(λ)!.h_n(\mathbf{g})=A(n)=\sum_{\lambda\vdash n}\prod_{j\geq1}\frac{X(j)^{m_j(\lambda)}}{j^{m_j(\lambda)/2}m_j(\lambda)!}.

Since E[X(j)aX(j)‾b]=1a=ba!\mathbb{E}[X(j)^a\overline{X(j)}^b]=\mathbf{1}_{a=b}a!, independence gives E[pλ(g)pρ(g)‾]=1λ=ρzλ\mathbb{E}[p_\lambda(\mathbf{g})\overline{p_\rho(\mathbf{g})}]=\mathbf{1}_{\lambda=\rho}z_\lambda. Thus ⟨P,Q⟩=E[P(g)Q(g)‾]\langle P,Q\rangle=\mathbb{E}[P(\mathbf{g})\overline{Q(\mathbf{g})}] is the Hermitian extension of the Hall inner product to complex symmetric functions.

Schur polynomials

We use three classical facts about symmetric polynomials, recalled here in the forms needed below. See, e.g., [11 Chapter I].

For a partition λ\lambda of length ℓ\ell, define its Schur function by the determinant

sλ=det⁡(hλi−i+j)1≤i,j≤ℓ.s_\lambda=\det\left(h_{\lambda_i-i+j}\right)_{1\leq i,j\leq\ell}.

In particular s(k)=hks_{(k)}=h_k for k≥1k\geq1, with s∅=h0=1s_{\varnothing}=h_0=1. For each nn, the sλs_\lambda with λ⊢n\lambda\vdash n form a basis of the homogeneous polynomials of weighted degree nn in the pjp_j and are orthonormal for the Hall inner product. In NN variables sλs_\lambda vanishes if ℓ(λ)>N\ell(\lambda)>N. For ℓ(λ)≤N\ell(\lambda)\leq N, sλ(U)s_\lambda(U) is an irreducible character of U(N)U(N), so the specializations of these Schur functions are also orthonormal under Haar probability.

The Young diagram of λ\lambda has λi\lambda_i boxes in row ii. Pieri’s rule states that

hksλ=∑ρ: ρ/λ is a horizontal k-stripsρ.(4)h_k s_\lambda=\sum_{\substack{\rho:\ \rho/\lambda\ \text{is a horizontal }k\text{-strip}}}s_\rho. \tag*{(4)}

A horizontal kk-strip means that ρ\rho is obtained from λ\lambda by adding kk boxes, with no two added boxes in the same column. Equivalently,

ρ1≥λ1≥ρ2≥λ2≥⋯ ,∣ρ∣−∣λ∣=k.\rho_1 \ge\lambda_1 \ge\rho_2 \ge\lambda_2 \ge\cdots,\qquad|\rho|-|\lambda|=k.

The essential consequence is ℓ(ρ)≤ℓ(λ)+1\ell(\rho) \le\ell(\lambda)+1. Indeed, two new nonempty rows would both require an added box in column one. This bound is independent of the number kk of boxes added.

Proof of thm:main

Exact moment comparison

We first state a lemma which allows us to transfer weighted moments. The identity follows from a classical moment formula for complete symmetric functions, for instance as in [4 Section 3]. It can also be deduced by coefficient extraction from the unitary ratios formula of Conrey, Farmer, and Zirnbauer [2]. We include a short proof for completeness.

Lemma 3.1. Let P,QP,Q be polynomials in the power sums of weighted degree at most DD. For every k≥0k \ge0 and N≥D+1N \ge D+1,

EU(N)[∣hk(U)∣2P(p(U))Q(p(U))‾]=E[∣A(k)∣2P(g)Q(g)‾].\mathbb{E}_{U(N)}\left[|h_k(U)|^2P(p(U))\overline{Q(p(U))}\right]=\mathbb{E}\left[|A(k)|^2P(g)\overline{Q(g)}\right].

In this statement, p(U)p(U) stands for (pj(U))j≥1(p_j(U))_{j\ge1}.

Proof. Expand PP and QQ in the Schur basis. Only partitions of size at most DD occur, and these have length at most DD. By Pieri’s rule (4), every Schur function occurring in hkPh_kP or hkQh_kQ therefore has length at most D+1≤ND+1 \le N. These Schur functions are orthonormal for the Hall inner product and, after evaluation at the eigenvalues of UU, for the Haar inner product too. Consequently

EU(N)[(hkP)(U)(hkQ)(U)]=E[(hkP)(g)(hkQ)(g)].\mathbb{E}_{U(N)}\left[(h_kP)(U)(h_kQ)(U)\right]=\mathbb{E}\left[(h_kP)(g)(h_kQ)(g)\right].

Since hk(g)=A(k)h_k(g)=A(k), this is the desired identity. □

The case P=Q=1P=Q=1 gives E∣A(k)∣2=EU(N)∣hk∣2=1\mathbb{E}|A(k)|^2=\mathbb{E}_{U(N)}|h_k|^2=1. At k=0k=0 the comparison reduces to the classical trace moment identity [3]. Higher moments depend on kk. To control the first moment, we instead apply the method of moments to suitable weighted measures.

Let μN\mu_N be Haar probability and let νN,k\nu_{N,k} be the probability measure defined by dνN,k=∣hk∣2dμNd\nu_{N,k}=|h_k|^2d\mu_N. Fix mm and write

Tm(U)=(pj(U)j)1≤j≤m,Xm=(X(j))j=1m,Wm=(X(j)+eijΘj)1≤j≤m,T_m(U)=\left(\frac{p_j(U)}{\sqrt{j}}\right)_{1\le j\le m},\qquad X_m=(X(j))_{j=1}^m,\qquad W_m=\left(X(j)+\frac{e^{ij\Theta}}{\sqrt{j}}\right)_{1\le j\le m},

where Θ\Theta is independent and uniform on [0,2π)[0,2\pi).

Lemma 3.2. Let P(z,z‾)P(z,\overline{z}) be a polynomial in z1,…,zmz_1,\ldots,z_m and their conjugates such that every monomial zαz‾βz^\alpha\overline{z}^\beta occurring in PP satisfies

∑j=1mjαj≤D,∑j=1mjβj≤D.\sum_{j=1}^{m}j\alpha_j\le D,\qquad\sum_{j=1}^{m}j\beta_j\le D.

For N≥D+1N\ge D+1 and k≥Dk\ge D,

EνN,kP(Tm,Tm‾)=EP(Wm,Wm‾).\mathbb{E}_{\nu_{N,k}}P(T_m,\overline{T_m})=\mathbb{E}P(W_m,\overline{W_m}).

Proof. Using (2) and the complex Gaussian identity EeaX(j)+bX(j)‾=eab\mathbb{E}e^{aX(j)+b\overline{X(j)}}=e^{ab}, we obtain the following identity of formal power series:

∑a,b≥0xaybE[A(a)A(b)‾exp⁡(∑j≤m(tjX(j)+sjX(j)‾))]=exp⁡(∑j≤mtjsj)1−xyexp⁡(∑j≤mtjyj+sjxjj).(5)\sum_{a,b\ge0}x^ay^b\mathbb{E}\left[A(a)\overline{A(b)}\exp\left(\sum_{j\le m}\left(t_jX(j)+s_j\overline{X(j)}\right)\right)\right] = \frac{\exp\left(\sum_{j\le m}t_js_j\right)}{1-xy}\exp\left(\sum_{j\le m}\frac{t_jy^j+s_jx^j}{\sqrt{j}}\right). \tag*{(5)}

Fix a monomial tαsβt^\alpha s^\beta with ∑jjαj,∑jjβj≤D\sum_j j\alpha_j,\sum_j j\beta_j\le D. Every term xaybx^a y^b from the last exponential that contributes to this coefficient has a,b≤Da,b\le D. For k≥Dk\ge D, we therefore have

[xkyk]xayb1−xy=1a=b.[x^k y^k]\frac{x^a y^b}{1-xy}=\mathbf{1}_{a=b}.

For the chosen coefficient, extracting the coefficient of xkykx^k y^k consequently has the same effect as retaining the factor exp⁡(∑j≤mtjsj)\exp(\sum_{j\le m}t_js_j) and averaging the last exponential with x=e−iθx=e^{-i\theta} and y=eiθy=e^{i\theta}. By Fourier orthogonality, the resulting coefficient is that of tαsβt^\alpha s^\beta in

exp⁡(∑j≤mtjsj)∫02πexp⁡(∑j≤mtjeijθ+sje−ijθj)dθ2π.\exp\left(\sum_{j\le m}t_js_j\right)\int_0^{2\pi}\exp\left(\sum_{j\le m}\frac{t_je^{ij\theta}+s_je^{-ij\theta}}{\sqrt{j}}\right)\frac{d\theta}{2\pi}.

Conditioning on Θ\Theta and applying the Gaussian identity again identifies this expression with

Eexp⁡(∑j≤m(tjWm,j+sjW‾m,j)).\mathbb{E}\exp\left(\sum_{j\le m}(t_jW_{m,j}+s_j\overline{W}_{m,j})\right).

Comparing coefficients and multiplying by α!β!\alpha!\beta! gives E[∣A(k)∣2XmαX‾mβ]=E[WmαW‾mβ]\mathbb{E}[|A^{(k)}|^2X_m^\alpha\overline{X}_m^\beta]=\mathbb{E}[W_m^\alpha\overline{W}_m^\beta]. Applying Theorem 3.1 with the polynomials ∏j≤m(pj/j)αj\prod_{j\le m}(p_j/\sqrt{j})^{\alpha_j} and ∏j≤m(pj/j)βj\prod_{j\le m}(p_j/\sqrt{j})^{\beta_j} proves the identity for monomials, and hence for PP by linearity. □

Completion of the proof of Theorem 1.1

Let γm\gamma_m be the law of XmX_m and write Hm=∑j≤mj−1H_m=\sum_{j\le m}j^{-1}. The density of a fixed translate Xm+vX_m+v relative to γm\gamma_m is exp⁡(2ℜ∑jzj‾vj−∑j∣vj∣2)\exp(2\Re\sum_j\overline{z_j}v_j-\sum_j|v_j|^2). Averaging this identity over vj=eijΘ/jv_j=e^{ij\Theta}/\sqrt{j} and changing θ\theta to −θ-\theta in the integral shows that WmW_m has density MmM_m relative to γm\gamma_m, where

Mm(z)=e−Hm∫02πexp⁡(2ℜ∑j≤mzjeijθj)dθ2π.(6)M_m(z)=e^{-H_m}\int_0^{2\pi}\exp\left(2\Re\sum_{j\le m}\frac{z_je^{ij\theta}}{\sqrt{j}}\right)\frac{d\theta}{2\pi}. \tag*{(6)}

In particular, MmM_m is positive and continuous, and EMm(Xm)=1\mathbb{E}M_m(X_m)=1.

For fixed mm, Theorem 3.1 with k=0k=0 shows that every fixed mixed moment of TmT_m under μN\mu_N agrees with the corresponding moment of XmX_m for all sufficiently large NN. By Theorem 3.2, every fixed mixed moment under νN,k\nu_{N,k} agrees with the corresponding moment of WmW_m for all sufficiently large NN and kk. The second moments imply tightness, while higher even moments imply uniform integrability of every fixed polynomial. Consequently, every subsequential limit has the moments of XmX_m or WmW_m, respectively. These laws are determined by their moments, since their real and imaginary coordinates have joint moment generating functions in a neighbourhood of the origin. Thus, for every bounded continuous f:Cm→Cf:\mathbb{C}^m\to\mathbb{C}, as min⁡(N,k)→∞\min(N,k)\to\infty,

EμNf(Tm)⟶Ef(Xm),\mathbb{E}_{\mu_N}f(T_m)\longrightarrow\mathbb{E}f(X_m),
EνN,kf(Tm)⟶E[Mm(Xm)f(Xm)].(7)\mathbb{E}_{\nu_{N,k}}f(T_m)\longrightarrow\mathbb{E}[M_m(X_m)f(X_m)]. \tag*{(7)}

We next establish the qualitative estimate needed to complete the proof.

Lemma 3.3. As m→∞m\to\infty,

EMm(Xm)1+Mm(Xm)⟶0.\mathbb{E}\frac{M_m(X_m)}{1+M_m(X_m)}\longrightarrow0.

Proof. Realize all the vectors WmW_m using the same Gaussian sequence and the same independent uniform variable Θ\Theta, and put Rm=Mm(Wm)−1R_m=M_m(W_m)^{-1}. Since WmW_m has density MmM_m relative to γm\gamma_m, for n≥mn\ge m and every bounded measurable f:Cm→Cf:\mathbb{C}^m\to\mathbb{C},

E[f(Wm)Rn]=Ef(Xm)=E[f(Wm)Rm].\mathbb{E}[f(W_m)R_n]=\mathbb{E}f(X_m)=\mathbb{E}[f(W_m)R_m].

Thus (Rm)(R_m) is a nonnegative martingale of mean one for the filtration (σ(Wm))m≥1(\sigma(W_m))_{m\ge1}, and consequently converges almost surely to a finite limit.

We claim that lim sup⁡mMm(Wm)=∞\limsup_m M_m(W_m)=\infty almost surely. By rotation invariance, the sequence (Mm(Wm))m≥1(M_m(W_m))_{m\ge1} has the same law as

(Mm((X(j)+j−1/2)j≤m))m≥1.\left(M_m\left((X(j)+j^{-1/2})_{j\le m}\right)\right)_{m\ge1}.

Set

aj,m=sin⁡(j/m)j/m,Gm=2ℜ∑j≤maj,mX(j)j.a_{j,m}=\frac{\sin(j/m)}{j/m}, \qquad G_m=2\Re\sum_{j\le m}\frac{a_{j,m}X(j)}{\sqrt{j}}.

Using periodicity, restricting the integral in (6) to [−1/m,1/m][-1/m,1/m] and applying Jensen’s inequality gives

Mm((X(j)+j−1/2)j≤m)≥1πme−Hm+2∑j≤maj,mj+Gm≥ceGmM_m\left((X(j)+j^{-1/2})_{j\le m}\right)\ge\frac{1}{\pi m}e^{-H_m+2\sum_{j\le m}\frac{a_{j,m}}{j}+G_m}\ge ce^{G_m}

for an absolute constant c>0c>0. Here we used aj,m=1+O((j/m)2)a_{j,m}=1+O((j/m)^2) and Hm=log⁡m+O(1)H_m=\log m+O(1). The variable GmG_m is a centered Gaussian with

Var⁡(Gm)=2∑j≤maj,m2j=2log⁡m+O(1).\operatorname{Var}(G_m)=2\sum_{j\le m}\frac{a_{j,m}^2}{j}=2\log m+O(1).

Hence, for each real AA, P(Gm>A)→1/2\mathbb{P}(G_m>A)\to1/2, which implies P(sup⁡mGm=∞)≥1/2\mathbb{P}(\sup_m G_m=\infty)\ge1/2. Changing finitely many of the variables X(j)X(j) changes the sequence (Gm)(G_m) by an amount bounded uniformly in mm. Thus {sup⁡mGm=∞}\{\sup_m G_m=\infty\} is a tail event, and Kolmogorov’s zero-one law gives it probability one. This proves the claim.

It follows that lim inf⁡mRm=0\liminf_m R_m=0 almost surely. Since (Rm)(R_m) converges, we have Rm→0R_m\to0 almost surely. Finally, the density identity and bounded convergence give

EMm(Xm)1+Mm(Xm)=E11+Mm(Wm)=ERm1+Rm→0,\mathbb{E}\frac{M_m(X_m)}{1+M_m(X_m)} =\mathbb{E}\frac{1}{1+M_m(W_m)} =\mathbb{E}\frac{R_m}{1+R_m}\to0,

as desired. □

Set gm=(1+Mm)−1g_m=(1+M_m)^{-1} and g=gm(Tm)g=g_m(T_m). The Cauchy–Schwarz inequality gives

EU(N)∣hk∣=EU(N)(∣hk∣g)+EU(N)(∣hk∣(1−g))≤EνN,kg+EU(N)(1−g).\mathbb{E}_{U(N)}|h_k|=\mathbb{E}_{U(N)}(|h_k|g)+\mathbb{E}_{U(N)}(|h_k|(1-g))\le\sqrt{\mathbb{E}_{\nu_{N,k}}g}+\sqrt{\mathbb{E}_{U(N)}(1-g)}.

Here we used that μN\mu_N and νN,k\nu_{N,k} are probability measures, and 0≤g≤10\le g\le1. By (7), both expectations on the right tend to E[Mm(Xm)/(1+Mm(Xm))]\mathbb{E}[M_m(X_m)/(1+M_m(X_m))]. Therefore

lim sup⁡min⁡(N,k)→∞EU(N)∣hk(UN)∣≤2(EMm(Xm)1+Mm(Xm))1/2.\limsup_{\min(N,k)\to\infty}\mathbb{E}_{U(N)}|h_k(U_N)| \le2\left(\mathbb{E}\frac{M_m(X_m)}{1+M_m(X_m)}\right)^{1/2}.

Now let m→∞m\to\infty. The right side tends to zero by Theorem 3.3, proving Theorem 1.1.

Connection with critical chaos

The random variable Mm(Xm)M_m(X_m) is the mean one total mass of the Fourier approximation to critical Gaussian multiplicative chaos on the circle. This gives the connection with the critical chaos model discussed in the introduction.

One can also deduce Theorem 3.3 directly from the low moment estimates for the total mass of the chaos, established by Soundararajan and Zaman. Indeed, as in [15], write Fm(z)=exp⁡(∑j≤mX(j)zjj)F_m(z)=\exp\left(\sum_{j\le m}\frac{X(j)z^j}{\sqrt{j}}\right). By (6),

Mm(Xm)=e−Hm2π∫02π∣Fm(eiθ)∣2 dθ.M_m(X_m)=\frac{e^{-H_m}}{2\pi}\int_0^{2\pi}|F_m(e^{i\theta})|^2\,d\theta.

The low moment estimates of [15 Proposition 3.2], with K=mK=m, r=1r=1 and q=1/2q=1/2, gives

EMm(Xm)≪(log⁡m)−1/4→0,\mathbb{E}\sqrt{M_m(X_m)}\ll(\log m)^{-1/4}\to0,

since Hm=log⁡m+O(1)H_m = \log m + O(1). The inequality x/(1+x)≤xx/(1+x) \le\sqrt{x} then implies the desired result.

Acknowledgments. This work was initiated during the first author’s visit to Tsinghua University, whose hospitality he gratefully acknowledges. We thank Victor Wang for helpful discussions and for pointing out the connection between Theorem 3.1 and the theorem of Conrey, Farmer, and Zirnbauer.

References

Department of Mathematics, University of Toronto, Toronto, ON, Canada

Email address: [email protected]

Yau Mathematical Sciences Center, Tsinghua University, Beijing, 100084, China

Beijing Institute of Mathematical Sciences and Applications, Beijing, 101408, China

Email address: [email protected], [email protected]

References

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