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The mean analytic rank of quadratic twists of elliptic curves

OpenAI, 6 October 2026

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Part of family 006: Goldfeld’s conjecture: densities and mean analytic rank. Read it with its family

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Abstract

For every elliptic curve over \Q, we prove that the average analytic rank of its quadratic twists tends to 1/2 when signed squarefree twist parameters are ordered by absolute value. This resolves Goldfeld’s mean analytic-rank conjecture in this counting convention.

1 Introduction

Goldfeld’s mean-rank conjecture predicts that the average central order of vanishing in a quadratic-twist family is 1/2 [5, p. 113, Conjecture (B)]. The issue addressed here is the contribution of rare twists of large analytic rank: knowing the densities of ranks zero and one does not determine the mean without control of this contribution.

Let E/\Q be an elliptic curve. For a nonzero squarefree integer d, write E^{(d)} for its quadratic twist, and put

\mathcal D(Y)=\{d\in\Z:0<|d|\le Y,\ d\text{ squarefree}\}, \qquad a(E^{(d)})=\ord_{s=1}L(E^{(d)},s).

Both signs of d are included. We call a the analytic rank and write r(E^{(d)})=\operatorname{rank}_{\Z}E^{(d)}(\Q) for the algebraic or Mordell–Weil rank. Outside the explicitly algebraic statements below, rank means analytic order of vanishing.

Theorem 1.1. For every elliptic curve E/\Q,

\lim_{Y\to\infty}\frac{1}{\#\mathcal D(Y)} \sum_{d\in\mathcal D(Y)}a(E^{(d)})=\frac12.

Theorem 1.1 resolves positively Goldfeld’s mean analytic-rank conjecture in this signed squarefree counting convention. It applies without restrictions on complex multiplication, rational torsion, rational isogenies, or reduction type.

The analytic density theorem [12, Theorem 1.2] states that, for this same family and every E/\Q,

\frac{\#\{d\in\mathcal D(Y):a(E^{(d)})=j\}}{\#\mathcal D(Y)} \longrightarrow\frac12 \qquad(j=0,1). \tag{1.1}

For the analytic mean theorem, (1.1) is the only input from the companion manuscript identified in the bibliography. A zero-density exceptional family can still contribute to a rank-weighted average. The new assertion needed for the mean is the following tail estimate, whose proof is independent of (1.1).

Theorem 1.2. For every elliptic curve E/\Q, there are constants C_E>0 and an integer R_E\ge1 such that, for every integer R\ge R_E,

\limsup_{Y\to\infty}\frac1Y \sum_{\substack{d\in\mathcal D(Y)\\a(E^{(d)})>R}}a(E^{(d)}) \le \frac{C_E}{R}.

Together, (1.1) and Theorem 1.2 show that

\sum_{\substack{d\in\mathcal D(Y)\\a(E^{(d)})\ge2}}a(E^{(d)})=o_E(Y).

For each fixed sufficiently large integer R, (1.1) makes the complement of ranks zero and one have density zero, so ranks 2 through R contribute o_{E,R}(Y). For the remaining ranks, use the height limsup in Theorem 1.2 and then let R tend to infinity. This order of limits will be made explicit in Section 6.

1.1 Algebraic-rank moments

The same signed squarefree family has the following algebraic-rank moment limits. This consequence uses the companion’s density conclusions and its density-one equality of analytic and algebraic ranks, together with the exponential-moment bound of Koymans and Smith. It does not use the analytic tail estimate of Theorem 1.2.

Corollary 1.3 (Fixed algebraic-rank moments). Fix an elliptic curve E/\Q. For every fixed real t,

\lim_{Y\to\infty}\frac1{\#\mathcal D(Y)} \sum_{d\in\mathcal D(Y)}\exp\!\bigl(t\,r(E^{(d)})\bigr) =\frac{1+e^t}{2}.

For every fixed positive integer m,

\lim_{Y\to\infty}\frac1{\#\mathcal D(Y)} \sum_{d\in\mathcal D(Y)}r(E^{(d)})^m=\frac12.

The proof appears in Section 7.

All parameters t and moment orders m in Corollary 1.3 are fixed before Y\to\infty. The corollary concerns algebraic ranks only: it gives no higher analytic-rank moments, no uniformity for parameters varying with Y, and no moment limit for thin polynomial subfamilies.

1.2 History and significance

Goldfeld’s original question concerns the change of rank when a fixed elliptic curve is viewed over quadratic fields. Under Birch–Swinnerton-Dyer, that change is the central order of the associated quadratic twist. His Conjecture (B) formulates the average directly in terms of this analytic order, using quadratic-field discriminants ordered by absolute value [5, pp. 113–114]. Here the counting parameter is instead the signed squarefree integer d in \mathcal D(Y). The rank-zero/rank-one density prediction describes the smallest orders allowed by the two functional-equation signs. The mean prediction also requires the larger orders, however sparse, to have negligible total contribution.

Conditional analytic estimates illustrate both aspects of the problem. Heath-Brown proved an upper bound 3/2+o(1) for smooth averages over fundamental discriminants coprime to the conductor, separately for each functional-equation sign [7, Theorem 3]. His nonnegative compactly supported weight selects one sign of the discriminant, and his Riemann-hypothesis assumption concerns every quadratic twist, including those not coprime to the conductor. Under the same twistwise Riemann-hypothesis assumption, Miller and Wong bounded higher analytic-rank moments and obtained exponentially decreasing large-rank counting tails [11, Theorem 1.1 and Corollary 1.2]. Their weighted sums run over integer parameters, with possible repeated squareclasses; the weight selects one parameter sign without fixing the functional-equation sign. Their tail estimate fixes the rank threshold before taking the height limit. Fiorilli obtained the exact mean 1/2 over signed squarefree parameters coprime to the conductor, assuming the Riemann hypothesis for elliptic-curve L-functions and an additional averaged cancellation hypothesis for nonreal zeros [4, Theorem 1.1 and Hypothesis M]. Thus this exact conditional mean uses more than the Riemann hypothesis.

A different route to densities comes from Selmer groups. Smith proved that, for every rational elliptic curve, the full 2-power Selmer corank is zero or one with density 1/2 each, using signed integer twist parameters [17, Theorem 1.1]. His analytic density corollary assumes Birch–Swinnerton-Dyer [17, Corollary 1.2]. The companion’s 2-converse supplies the analytic implication needed for (1.1) in the signed squarefree convention. Theorem 1.2 addresses the additional rank-mass question independently of that density argument.

Koymans and Smith prove exponential moment bounds for Mordell–Weil rank in polynomial quadratic-twist families [9, Theorem 1.4]. The specialization in the proof of Corollary 1.3 supplies the needed algebraic tail control. Such bounds do not supply an analytic-rank identity or higher analytic-rank moments.

Hanners claims the full Birch–Swinnerton-Dyer conjecture for every rational elliptic curve [6, Theorems 28.1, 39.4 and 39.5]. We do not use this claim. The unresolved point is how the bridge conditions supported by tests on eighteen curves in Section 39.1 are established for every rational elliptic curve, as required by the transfer in Section 39.2. This is not a refutation of the claimed theorem.

Modularity provides the analytic continuation and functional equation for every curve in the argument [1, Theorem A]. Our estimates use these analytic properties and the local coefficient bounds. The proof invokes neither the Birch–Swinnerton-Dyer conjecture nor the generalized Riemann hypothesis.

Earlier work on a fixed elliptic curve already connected derivative moments to nonvanishing and analytic-rank averages. Perelli and Pomykała proved first-derivative nonvanishing results and bounds for the sum of analytic ranks [13]; Pomykała extended this nonvanishing approach to higher derivatives of fixed order in a congruence-restricted twisting family [14]. In the family of weight-two newforms of varying prime level, Kowalski, Michel, and VanderKam combined high completed derivatives, mollification, and consecutive derivative orders to control both functional-equation signs. Their passage from these nonvanishing counts to rank-weighted tails also uses a separate bound for the second moment of analytic rank [8, Sections 2, 4, and 8]. In the present quadratic-twist argument the derivative order grows with height. This uniformity, together with a pointwise rank bound, controls the rank mass beyond the available counting range without requiring a bounded second analytic-rank moment.

Second moments of the twist L-functions themselves supply the analytic comparison used below. For full-level holomorphic Hecke forms of weight divisible by four, Soundararajan and Young obtained the second-moment asymptotic over positive discriminants 8d, with d odd and squarefree, under GRH for the twists, the Riemann zeta function, and the symmetric-square L-function [19, Theorem 1.2]. Li proved the asymptotic unconditionally in this full-level setting [10, Theorem 1.1]. We adapt the Fourier-cutoff and prime-square inflation mechanism in Li’s proof, establishing the needed logarithmic bounds for our finite family of arbitrary elliptic curves with its conductor and bad-prime factors retained. Neither asymptotic is an input to the argument.

1.3 The analytic argument

The starting point is the exact identity of Lemma 4.1, forced by the vanishing of a derivative of order k of the completed L-function. Its Dirichlet-series weight is obtained by exponentially smoothing a k-th power of a truncated logarithm. Near the square root of the conductor, at lengths of order X for twists of height X, this weight suppresses the late terms. The approximation (1-u)^k\approx e^{-ku} for u=O(1/k) motivates mollification: at u=\log n/\log X, the exponential corresponds to a small positive shift from the center of the L-function. A short approximation to its inverse Euler product then makes the first weighted piece close to a positive main term. We split the weighted series using smooth cutoffs into finite pieces and a terminal series, use progressively shorter mollifiers as the lengths of the finite pieces increase, and estimate the terminal series without mollification.

Two features make the resulting estimates uniform for k as large as a fixed power of \log X. First, a Poisson argument and inflation give unmollified second moments with only powers of logarithms (Propositions 3.1 and 3.2). The inflation mechanism is related to Li’s work on quadratic twists [10, Lemmas 2.7 and 3.1, Proposition 3.2]; we prove the estimate needed here for the entire fixed finite family of curves, including its local factors at bad primes. Second, Proposition 5.9 gives mean-square bounds for the mollified finite pieces in a model that replaces odd-prime character values by independent variables with their complete-residue distributions. The mean-square estimates use the whole probability space, without discarding exceptional outcomes. Proposition 3.7 transfers these bounds to integer averages. Separately, Proposition 5.3 compares the mollifiers with positive reciprocal Euler products on most integer parameters and relates these products to one another. We can then remove the mollifiers and compare every piece with the same positive product: the first piece dominates the later pieces and the terminal series. The resulting nonzero sum contradicts the completed-derivative identity whenever the rank exceeds the derivative order of matching parity. Consecutive orders cover both signs.

For admissible twists of height X, Proposition 6.1 proves a bound O_E(X/k^2) for the number of ranks exceeding k, uniformly up to k=(\log X)^{3/5}. A conductor-uniform Jensen bound (Lemma 6.2) gives the pointwise estimate a(E^{(d)})=O_E(\log X). The count at the largest permissible k then controls the remaining rank mass, and summation of the integer tails proves Theorem 1.2. The numerical exponents used in the length partition leave ample room between the comparison error and the later thresholds; their optimization is not needed.

The sections follow the inputs required by this argument. Section 2 fixes the finite auxiliary family and the integer residue model. Section 3 proves the moments and the comparison with that model. Section 4 constructs the completed-derivative weights and bounds their terminal series. Section 5 constructs the short mollifiers and proves the model estimates. Section 6 combines them into the counting and rank-weighted tail bounds, and uses the companion density theorem only in the final deduction of the mean. Section 7 proves the separate algebraic-rank moment corollary.

1.4 Conventions

Implied constants may depend on the original curve E, on fixed smooth functions, and on a specified fixed order of differentiation. They do not depend on the varying height, derivative order, or scale index unless this is explicitly stated. We write \tau(n) for the divisor function and use the Fourier kernel e^{-2\pi ixy} when applying Poisson summation. All sufficiently large lower thresholds for the integer k are chosen after the fixed analytic exponents and smoothness orders.

2 Twist families and the integer model

We first reduce upper bounds for arbitrary twists to a fixed finite family of curves with coprime twisting parameters. This gives exact conductor formulas while preserving the bounds for nonnegative sums needed later. We then define the probability model for complete integer residue averages.

We use unitary normalization:

L_F(s)=L(F,s+1/2)=\sum_{n\ge1}\lambda_F(n)n^{-s}, \qquad q_F=\operatorname{cond}(F), \qquad C_F=\frac{\sqrt{q_F}}{2\pi}.

The series converges absolutely in \Re s>1. Modularity and the local rules for the Hasse–Weil L-function give real multiplicative coefficients and inverse Euler factors

1-\lambda_F(p)p^{-s}+\xi_{F,p}p^{-2s}, \qquad \xi_{F,p}=\mathbf 1_{p\nmid q_F}. \tag{2.1}

At a good prime the two factor parameters have modulus one by Hasse’s bound [16, Chapter V, Theorem 2.3.1(a)]. At a multiplicative prime there is one parameter, of modulus p^{-1/2}, and at an additive prime the factor is one [2, Definitions 17–18 and Theorem 19]. In particular,

|\lambda_F(n)|\le\tau(n). \tag{2.2}

The completed function

\Lambda_F(s)=C_F^s\Gamma(s+1/2)L_F(s)

is entire of finite order and satisfies

\Lambda_F(s)=\epsilon_F\Lambda_F(1-s),\qquad \epsilon_F\in\{1,-1\}. \tag{2.3}

Analytic continuation and the functional equation follow from modularity [1, Theorem A] and the standard completion [16, Appendix C, Theorems 16.3–16.4]. The standard finite-order bounds follow, for example, from the split Mellin integral of the modular cusp form and its Fricke transform. They also give polynomial growth in every fixed vertical strip for each fixed curve F, independently of the averaged estimates proved below. Indeed, enclose the strip in a\le\Re s\le b, with a\le-1 and b\ge2. Absolute convergence bounds L_F on the right boundary; (2.3) and Stirling’s formula give L_F(a+it)\ll_{F,a}(1+|t|)^{1-2a} on the left boundary. Take A=1-a and an integer N>1-2a, so that L_F(s)/(s+A)^N is bounded on both boundaries. For \varepsilon>0 and 0<\kappa<\pi/(b-a), multiply this quotient by

\exp\left\{-\varepsilon\cos\left(\kappa \left(s-\frac{a+b}{2}\right)\right)\right\}.

The multiplier has modulus at most one on the vertical boundaries and at most \exp(-c\varepsilon\cosh(\kappa\Im s)) on the horizontal sides, for a fixed c>0. This dominates the finite-order growth. The maximum principle on expanding rectangles, followed by \varepsilon\downarrow0, therefore gives L_F(\sigma+it)\ll_{F,a,b}(1+|t|)^N on the strip. These individual bounds justify contour displacements. Their constants may depend on the fixed curve; estimates uniform in the varying twist parameters will be proved separately.

2.1 A finite family closed under reduction

Fix the primes

S=\{p:p\mid 2q_E\},\qquad Q_S=\prod_{p\in S}p.

Let \mathcal F be the finite set, up to \Q-isomorphism, of curves obtained from E by twisting by signed squarefree products of primes in S. The curve E is included. Every F\in\mathcal F has good reduction outside S.

Call a signed squarefree integer d admissible if

d\equiv1\pmod4,\qquad (d,Q_S)=1.

For a dyadic X, put

\mathcal A(X)=\{d:d\text{ admissible},\ X\le|d|<2X\}.

Lemma 2.1. For every F\in\mathcal F and signed squarefree b, there are F'\in\mathcal F and an admissible d such that

F^{(b)}\simeq (F')^{(d)},\qquad |d|\le |b|.

The correspondence can be chosen to have bounded multiplicity, uniformly in b. Every sum of nonnegative functions of these twists can therefore be bounded by a fixed multiple of the corresponding sums over \mathcal F and admissible parameters of no greater height.

Proof. Write b=b_S b_0, where b_S>0 is the product of the primes of S dividing b. Then b_0 is odd and prime to Q_S. Choose \varepsilon\in\{1,-1\} so that d=\varepsilon b_0\equiv1\pmod4, and put F'=F^{(\varepsilon b_S)}. Quadratic twisting depends only on the square class and composes by multiplication of square classes. Thus F' is in \mathcal F and (F')^{(d)}\simeq F^{(b)}. Moreover |d|=|b|/b_S\le |b|. There are at most 2^{|S|+1} choices of the signed S-part. Possible coincidences among the finitely many curves only change this fixed multiplicity.

Lemma 2.2. For F\in\mathcal F and admissible d,

L_{F^{(d)}}(s)=\sum_{n\ge1}\lambda_F(n)\chi_d(n)n^{-s}, \qquad q_{F^{(d)}}=q_F|d|^2, \qquad \chi_d(n)=\left(\frac dn\right). \tag{2.4}

Here the symbol is the Kronecker symbol and d=1 has the untwisted convention. For an arbitrary signed squarefree b, the same good-prime twisting rule holds at primes outside S: the local trace is multiplied by (b/p) when p\nmid b, and the local factor is one when p\mid b.

Proof. We compute the inverse local Euler factors using geometric Frobenius on the inertia invariants of the dual of the rational Tate module, and the conductor as the Artin conductor [2, Definitions 17–18 and Theorem 19]. The rational Tate-module representation of a quadratic twist is the original representation tensored with the corresponding quadratic character. This follows from the isomorphism over the twisting extension, whose conjugate differs by the scalar automorphism [-1].

An unramified scalar twist preserves the conductor and multiplies Frobenius eigenvalues on inertia invariants by the character value. Since an admissible d is an odd fundamental discriminant, its character is unramified at every prime of S. At a prime p\mid d, the representation of F is unramified and the quadratic character is tamely ramified. The tensor product has no inertia invariants, Swan conductor zero, and Artin conductor exponent two. At all other primes the scalar twist is unramified. Computing the inertia-invariant Euler factors and the conductor gives (2.4). For an arbitrary squarefree b, these same computations apply at odd primes outside S, regardless of the character’s behavior at two.

The constants in what follows are chosen uniformly over the finite set \mathcal F. The nonincreasing height in Lemma 2.1 is useful in the second-moment induction: a dual squarefree parameter of absolute value at most M/2 remains in a smaller dyadic block after reduction.

2.2 Complete integer averages

Fix c\in\{1,-1\}. For m\in\Z, define a completely multiplicative formal character on positive integers by

z_m(2)=c,\qquad z_m(p)=\left(\frac mp\right) \quad(p\text{ odd}).

Let Z be the completely multiplicative random model with Z(2)=c and independent odd-prime values distributed by

\Prob(Z(p)=0)=\frac1p,\qquad \Prob(Z(p)=1)=\Prob(Z(p)=-1)=\frac{1-1/p}{2}. \tag{2.5}

For every polynomial involving only finitely many prime values, its expectation is the average over a complete residue system for the corresponding odd-prime periods. This follows from the Chinese remainder theorem and the equal numbers of nonzero quadratic residues and nonresidues modulo each odd prime.

We use this model for averages over all integers m. Nonnegative estimates can subsequently be restricted to admissible squarefree d, separated into the two classes \chi_d(2)=c; on either class, z_d(n)=\chi_d(n) for every n.

3 Poisson summation and logarithmic second moments

We retain the finite family \mathcal F, the fixed set S, and the unitary normalization from Lemmas 2.1 and 2.2. In particular, |\lambda_F(n)|\leq\tau(n), all local parameters have modulus at most one, and reduction of a squarefree twisting parameter to an admissible one does not increase its absolute value. All constants in this section are uniform in F\in\mathcal F.

Our first aim is to bound the second moments of the twist functions and their localized Dirichlet polynomials with only logarithmic losses. For a compactly supported smooth function G on (0,\infty), write

P_d(N,t;G)=\sum_{n\geq1} \lambda_F(n)\chi_d(n)n^{-1/2-it}G(n/N).

All dyadic parameters below belong to \{1,2,4,\ldots\}.

Proposition 3.1 (Logarithmic second moments). There are fixed positive integers A,B such that, for every dyadic M\geq1, every F\in\mathcal F, every t\in\mathbb R, and 1/2\leq\sigma\leq2,

\frac1M\sum_{\substack{d\ \mathrm{admissible}\\M\leq|d|<2M}} |L_{F^{(d)}}(\sigma+it)|^2 \ll_{\mathcal F}\log^B(3M)(1+|t|)^A. \tag{3.1}

For arbitrary signed squarefree twisting parameters and H\geq1,

\sum_{\substack{0<|h|\leq H\\h\ \mathrm{squarefree}}} |L_{F^{(h)}}(\sigma+it)|^2 \ll_{\mathcal F}H\log^B(3H)(1+|t|)^A. \tag{3.2}

Proposition 3.2 (Dirichlet-polynomial second moments). With the same fixed integers A,B, every fixed smooth G of compact support in (0,\infty) satisfies

\frac1M\sum_{\substack{d\ \mathrm{admissible}\\M\leq|d|<2M}} |P_d(N,t;G)|^2 \ll_{\mathcal F,G} \log^B(3M)(1+|t|)^A(1+N/M)^A \qquad(N>0). \tag{3.3}

The bound is uniform for fixed uniformly smooth families of weights with common compact support.

We prove these estimates by induction on the twisting height M. Poisson summation turns a polynomial mean square into a sum of products of twist L-functions at dual squarefree parameters. To put those parameters below the current height, we first enlarge the family by replacing d with dp^2, where p\asymp P. The new averaging height is U=MP^2. A weight with compact Fourier support then restricts the dual parameters to size O(N^2/(MP^2)), which is at most M/2 for a sufficiently large P. Recovering the original squarefree average costs O(P\log(2P)). The nonzero-frequency estimate gains P^{-2}, so after recovery its recursive coefficient contains N\log(2P)/(MP). We choose P as a sufficiently large fixed power of \log(3M)(1+N/M)(1+|t|), with a large fixed leading constant, to make this coefficient small. The approximate functional equation and a strip estimate then close the induction for the L-functions themselves. The compact Fourier support construction and prime-square inflation are related to Li’s treatment of quadratic twists [10].

The arithmetic preparation below keeps its arithmetic exponents independent of the number of weight derivatives. Once the induction is closed, we sum all dual frequencies to compare short polynomial averages with the integer model. The polynomial moment bound will also control the unmollified terminal series in Section 4.

3.1 The normalized Gauss sums

Put e(x)=\exp(2\pi i x). For an odd positive integer l, set

\tau_h(l)=\sum_{a\bmod l}\left(\frac a l\right)e(ah/l),\qquad \epsilon_l=\begin{cases}1&l\equiv1\pmod4,\\i&l\equiv3\pmod4,\end{cases} \qquad B_h(l)=\frac{\tau_h(l)}{\epsilon_l\sqrt l}.

We use B_h(1)=1. The square root is positive. These are the normalized quadratic Gauss sums of [18, Section 2.2, Lemma 2.3]: in that notation, B_h(l)=G_h(l)/\sqrt l. We give the formulas and their proof in the present normalization.

Lemma 3.3 (Exact Gauss-sum formulas). For fixed h, the function l\mapsto B_h(l) is multiplicative on odd positive integers, and

B_{-h}(l)=\left(\frac{-1}{l}\right)B_h(l),\qquad \epsilon_l B_h(l)=\frac{1+i}{2}B_h(l)+\frac{1-i}{2}B_{-h}(l). \tag{3.4}

If h\ne0, p is odd, t=v_p(h), and v\geq1, then

B_h(p^v)= \begin{cases} p^{v/2}(1-p^{-1}),&v\text{ even},\ v\leq t,\\ -p^{v/2-1},&v\text{ even},\ v=t+1,\\ p^{(v-1)/2}\left(\dfrac{h/p^{v-1}}p\right), &v\text{ odd},\ v=t+1,\\ 0,&\text{otherwise}. \end{cases} \tag{3.5}

Consequently B_h(p^v)=0 for v>t+1 and |B_h(p^v)|\leq p^{v/2}. If t=0, only v=1 can survive and B_h(p)=(h/p). If t=1, only v=2 can survive and B_h(p^2)=-1.

Proof. For coprime odd l_1,l_2, the Chinese remainder theorem, followed by a change of variable in each Gauss sum, gives

\tau_h(l_1l_2)= \left(\frac{l_1}{l_2}\right)\left(\frac{l_2}{l_1}\right) \tau_h(l_1)\tau_h(l_2).

Quadratic reciprocity says that the displayed product of symbols is \epsilon_{l_1l_2}/(\epsilon_{l_1}\epsilon_{l_2}). This proves multiplicativity. Substituting a\mapsto-a proves the first identity in (3.4); the second follows by considering the two residue classes of l modulo four.

For even v, the Jacobi symbol modulo p^v is the indicator of the units. Thus

\tau_h(p^v)=\sum_{a\bmod p^v}e(ah/p^v) -\sum_{b\bmod p^{v-1}}e(bh/p^{v-1}),

which equals p^v-p^{v-1} when p^v\mid h, equals -p^{v-1} when p^{v-1}\Vert h, and otherwise vanishes. Here \epsilon_{p^v}=1. For odd v, write a=y+pz with y modulo p and z modulo p^{v-1}. The z-sum vanishes unless p^{v-1}\mid h; in that case

\tau_h(p^v)=p^{v-1}\sum_{y\bmod p} \left(\frac yp\right)e\big(y(h/p^{v-1})/p\big).

This is zero if p^v\mid h. Otherwise the quadratic Gauss-sum formula makes it p^{v-1}\epsilon_p\sqrt p\,\bigl(\frac{h/p^{v-1}}p\bigr). Since \epsilon_{p^v}=\epsilon_p for odd v, division by \epsilon_{p^v}p^{v/2} gives (3.5).

For later use, fix once and for all the arithmetic exponent

C_{\rm ar}=256. \tag{3.6}

This exponent will not change when we require more derivatives of a weight or more decay in an imaginary direction.

Lemma 3.4 (Two-variable Euler factorization). Let r be positive and odd, and write h=h_1h_2^2\ne0, where h_1 is signed squarefree and h_2\geq1. For \nu\in\{1,-1\}, the series

\mathcal G_{h,r}^{\nu}(s_1,s_2)= \sum_{\substack{n_1,n_2\geq1\\n_1,n_2\ \mathrm{odd}}} \frac{\lambda_F(n_1)\lambda_F(n_2)B_{\nu h}(rn_1n_2)} {n_1^{s_1}n_2^{s_2}}

initially converges in a right half-plane and continues to \Re s_1,\Re s_2>1/2 as

\mathcal G_{h,r}^{\nu}(s_1,s_2)= L_{F^{(\nu h_1)}}(s_1)L_{F^{(\nu h_1)}}(s_2) \mathcal Q_{h,r}^{\nu}(s_1,s_2). \tag{3.7}

For 0<b\leq1/4 and \Re s_i\geq1/2+b,

|\mathcal Q_{h,r}^{\nu}(s_1,s_2)| \ll_{\mathcal F} b^{-C_{\rm ar}}r^{C_{\rm ar}} \tau(h_2)^{C_{\rm ar}}. \tag{3.8}

The function \mathcal Q is holomorphic in these open half-planes.

Proof. For an odd prime put e_p=v_p(r) and t_p=v_p(h). Multiplicativity expresses the series as the product of the local sums

T_p(s_1,s_2)=\sum_{a,b'\geq0} \lambda_F(p^a)\lambda_F(p^{b'}) B_{\nu h}(p^{e_p+a+b'})p^{-as_1-b's_2}.

The symbol b' here is an integer exponent, distinct from the real shift b. No division by B_{\nu h}(p^{e_p}) is made; that quantity may vanish. Write D_p^*(s) for the inverse local factor of the elliptic curve F^{(\nu h_1)}. The correction factor at p is T_p(s_1,s_2)D_p^*(s_1)D_p^*(s_2). At two it is just D_2^*(s_1)D_2^*(s_2), because the summation indices are odd.

There are three types of odd prime. If p\notin S and p\nmid rh, put \chi=(\nu h/p)=(\nu h_1/p) and x_i=p^{-s_i}. The local formulas give exactly

T_p=1+\lambda_F(p)\chi(x_1+x_2),\qquad D_p^*(s_i)=1-\lambda_F(p)\chi x_i+x_i^2.

Multiplication cancels both terms of total degree one. The sum of the absolute values of all polynomial coefficients before cancellation is at most 5\cdot4\cdot4=80. Therefore the correction is 1+O(80p^{-1-2b}), uniformly in the imaginary parts.

If p\notin S, p\nmid r, and t_p=1, the twisting curve has a trivial local factor at p. By (3.5),

T_p=1-\lambda_F(p^2)(x_1^2+x_2^2)-\lambda_F(p)^2x_1x_2 =1+O(10p^{-1-2b}).

In particular these primes do not produce a cost for every prime factor of the squarefree part h_1.

The remaining odd primes lie in S or divide rh_2. The support in (3.5) gives e_p+a+b'\leq t_p+1 for every nonzero summand, except that B_{\nu h}(1)=1 is already covered when e_p=a=b'=0. Hence

|T_p|\leq p^{e_p/2} \sum_{a+b'\leq t_p+1}(a+1)(b'+1) \leq p^{e_p/2}(t_p+3)^4.

Each inverse local factor has modulus at most (1+p^{-1/2})^2, so the product of the two costs at most 9. Writing u_p=v_p(h_2), we have t_p\leq2u_p+1. If u_p\geq1, the bound 9(2u_p+4)^4\leq(u_p+1)^{17} absorbs this cost into a fixed divisor power, with p^{e_p/2} absorbed by r. If u_p=0 and e_p\geq1, the cost is at most 9\cdot4^4p^{e_p/2}\leq p^{8e_p} for p\geq3. If u_p=e_p=0, this is one of the fixed primes of S, whose cost is a fixed constant. The factor at two is bounded by (1+2^{-1/2})^4.

The nonexceptional product is bounded by

\exp\left(80\sum_p p^{-1-2b}\right) \leq\zeta(1+2b)^{80}\ll b^{-80}.

Combining the estimates proves (3.8) with the stated C_{\rm ar}. The nonexceptional correction product converges normally on compact subsets of \Re s_i>1/2; all exceptional factors are polynomials. Multiplication by the entire twist L-functions therefore gives the claimed continuation. This argument never divides by a global L-value.

3.2 A weighted Poisson estimate

The Euler factorization identifies the twist functions that occur at nonzero frequencies. We now turn it into a weighted comparison formula: the zero frequency gives the integer residue average, and the remaining frequencies are bounded by those twist functions. This is a quadratic Poisson method used in [18, Section 2.4, Lemma 2.6], with the weights and normalization specified below.

Fix a compact interval [a_0,a_1]\subset(0,\infty) for the first two scaled variables. The third variable ranges over \mathbb R. For an integer D\geq0, a convenient finite seminorm is

\|W\|_{D,*}=\max_{\alpha+\beta+\gamma\leq D} \sup_{y_1,y_2,x}(1+|x|)^D \left|\partial_{y_1}^{\alpha}\partial_{y_2}^{\beta} \partial_x^\gamma W(y_1,y_2,x)\right|.

The functions under consideration vanish outside [a_0,a_1]^2 in the first two variables and have the indicated finite decay and smoothness in the third. Requiring a larger fixed D below causes no change to C_{\rm ar}.

Lemma 3.5 (Poisson estimate). Let U>0, let r be odd and positive, and let N_i be bounded below by a fixed positive constant. Fix 0<b\leq1/4. In the expression

\frac1U\sum_{m\in\mathbb Z} \sum_{\substack{n_1,n_2\geq1\\n_1,n_2\ \mathrm{odd}}} \frac{\lambda_F(n_1)\lambda_F(n_2)} {(n_1n_2)^{1/2}n_1^{it_1}n_2^{it_2}} \left(\frac m{rn_1n_2}\right) W(n_1/N_1,n_2/N_2,m/U), \tag{3.9}

Poisson summation gives the zero frequency, namely the complete-residue average integrated in x, together with the nonzero frequencies. For every fixed J_1>0, a sufficiently large fixed seminorm order D bounds the absolute contribution of frequency h=h_1h_2^2\ne0 by

\begin{align*} &C_{J_1,\mathcal F}\|W\|_{D,*} (N_1N_2)^{-1/2+b}b^{-C_{\rm ar}}r^{C_{\rm ar}} \tau(h_2)^{C_{\rm ar}} \left(1+\frac{|h|U}{rN_1N_2}\right)^{-J_1} \\[-2pt] &\hspace{8mm}\cdot \sum_{\nu=\pm1}\int_{\mathbb R^2} \frac{\prod_{i=1}^2 |L_{F^{(\nu h_1)}}(1/2+b+i(t_i+v_i))|} {(1+|v_1|+|v_2|)^{J_1}}\,dv_1\,dv_2. \tag{3.10}\end{align*}

If the Fourier transform of W in x is supported in a fixed interval [-C_W,C_W], all modes with |h|>C_Wa_1^2rN_1N_2/U vanish exactly.

Proof. Our Fourier convention is \widehat W(y_1,y_2,\xi)=\int_{\mathbb R}W(y_1,y_2,x)e(-x\xi)\,dx. Applying Poisson summation in each residue class modulo l=rn_1n_2 gives exactly

\frac1U\sum_m\left(\frac ml\right)W(y_1,y_2,m/U) =\sum_{h\in\mathbb Z}\frac{\tau_h(l)}l \widehat W(y_1,y_2,hU/l).

Thus the normalized frequency factor is

\frac{1}{\sqrt{n_1n_2}}\frac{\tau_h(rn_1n_2)}{rn_1n_2} =\frac{\epsilon_{rn_1n_2}B_h(rn_1n_2)} {\sqrt r\,n_1n_2}.

Use (3.4) to replace the numerator by a fixed linear combination of B_h and B_{-h}.

Put \rho=hU/(rN_1N_2) and

V_h(y_1,y_2)=\widehat W(y_1,y_2,\rho/(y_1y_2)),\qquad \widetilde V_h(z_1,z_2)= \int_0^\infty\!\int_0^\infty V_h(y_1,y_2)y_1^{z_1}y_2^{z_2} \frac{dy_1dy_2}{y_1y_2}.

On any fixed bounded range of real parts, Fourier integration by parts in x, followed by Mellin integration by parts in y_1,y_2, yields

|\widetilde V_h(z_1,z_2)| \ll_{J_1}\|W\|_{D,*}(1+|\rho|)^{-J_1} (1+|\Im z_1|+|\Im z_2|)^{-J_1}. \tag{3.11}

To see why differentiation causes no arithmetic loss, each derivative of \rho/(y_1y_2) contributes a bounded multiple of \rho on the fixed compact support. For any fixed number of such derivatives, take that many additional integrations by parts in x. The powers of \rho are then absorbed by its Fourier decay. All other factors are bounded functions of y_1,y_2.

Mellin inversion first on right lines expresses the \nu part of the mode as

\frac1{\sqrt r(2\pi i)^2} \int\!\int \widetilde V_h(z_1,z_2)N_1^{z_1}N_2^{z_2} \mathcal G_{h,r}^{\nu}(1+it_1+z_1,1+it_2+z_2) \,dz_1\,dz_2.

Move both lines to \Re z_i=-1/2+b. Lemma 3.4 and the entire continuation of the twist functions show that no pole is crossed. Polynomial growth in fixed strips, together with a larger fixed order in (3.11), makes the horizontal segments tend to zero. The scale factor is (N_1N_2)^{-1/2+b}. Applying (3.8) and (3.11), and discarding r^{-1/2}\leq1, proves (3.10). The final assertion follows directly from the support of \widehat W before Mellin inversion.

Whenever unrestricted positive indices occur, write n=2^a n' with n' odd. For z_m(2)=c the factor taken outside an odd-index sum is \lambda_F(2^a)c^a2^{-a(1/2+it)}. Its absolute values have the uniformly convergent majorant

\sum_{a\geq0}(a+1)2^{-a/2}<\infty. \tag{3.12}

The new length is N/2^a; a nonempty localized sum has this length bounded below by a constant depending only on [a_0,a_1].

3.3 Closing a logarithmic second-moment induction

Proof of Propositions 3.1 and 3.2. We give a simultaneous induction for all F\in\mathcal F. The induction hypothesis at smaller dyadic heights is

\frac1{M'}\sum_{\substack{d\ \mathrm{admissible}\\M'\leq|d|<2M'}} |L_{F^{(d)}}(\sigma+it)|^2 \leq K\log^B(3M')(1+|t|)^A \qquad(M'<M). \tag{3.13}

The constant K, common to the finite family, will be selected last. Since the reduction in Lemma 2.1 does not increase height and has bounded multiplicity, this hypothesis implies

\sum_{\substack{0<|h_1|\leq H\\h_1\ \mathrm{squarefree}}} |L_{F^{(\nu h_1)}}(1/2+b+iv)|^2 \leq C_{\mathcal F}KH\log^B(3M)(1+|v|)^A \quad(1\leq H\leq M/2). \tag{3.14}

Indeed all admissible images lie in earlier dyadic blocks, whose lengths have sum at most 2H. If H<1, the sum is empty. In particular the arguments below at M=1 require no induction input.

The polynomial average at inflated height. First we prove a polynomial estimate with a small coefficient in front of K. Put L=\log(3M), T=1+|t|, and let N>0. Choose P sufficiently large, with

P\geq C_{\mathcal F,G}(1+N/M). \tag{3.15}

Let \mathcal P consist of the primes p\in[P,2P] outside S. For a sufficiently large fixed lower threshold on P, the elementary dyadic prime estimate of Erdős [3, §6, equation (10)] gives |\mathcal P|\gg P/\log(2P).

Choose a fixed nonnegative Schwartz function \Phi that is at least one on [-8,8] and has compactly supported Fourier transform. For completeness, take a nonzero even real smooth bump g in frequency space with \int g>0. Its inverse Fourier transform f is real, Schwartz, and nonzero near zero. A sufficiently small dilation makes f(\alpha x) nonzero throughout [-8,8]; a fixed multiple of f(\alpha x)^2 then has the required properties. Its Fourier transform is a compactly supported convolution.

Put U=MP^2. For c=\pm1 use the formal character z_m with z_m(2)=c, and let P_m^c(N',t;G) be the corresponding polynomial. We claim, uniformly for 0<N'\leq N,

\begin{align*} \frac1U\sum_{m\in\mathbb Z}\Phi(m/U)|P_m^c(N',t;G)|^2 &\leq C_G\log^{C_0}(3M+3N) \left(1+C_{A,B,\mathcal F,G}K\frac{N}{MP^2}L^BT^A\right), \tag{3.16}\end{align*}

where we may fix C_0=512, independently of A,B and of the required smoothness orders.

To prove the claim, apply Lemma 3.5 with r=1 to the expansion of the square, first separating powers of two by (3.12). Take b=1/(10\log(3M+3N)). For the zero mode the complete-residue mean vanishes unless the odd part of n_1n_2 is a square, and its absolute value is at most one. Inserting (n_1n_2)^{-b} at the bounded cost (C_GN)^{2b}\ll_G1 majorizes the resulting sum by an Euler product. At an odd prime this product has factor

\sum_{\substack{a,b'\geq0\\a+b'\ \mathrm{even}}} (a+1)(b'+1)p^{-(a+b')(1/2+b)} =1+O(100p^{-1-2b}).

For example this follows by putting z=p^{-1/2-b}\leq3^{-1/2} in \tfrac12((1-z)^{-4}+(1+z)^{-4}) and bounding its terms of degree at least two. The prime two costs a bounded factor by (3.12). The zero mode is therefore O_G(b^{-100}).

For the nonzero modes, denote the two odd lengths by N_1,N_2. The Fourier support restricts the frequencies to

0<|h|\leq H_0=C_\Phi N_1N_2/(MP^2).

Increasing the constant in (3.15) ensures H_0\leq M/2 for every such pair of lengths. For fixed h_2, Cauchy–Schwarz and (3.14) bound the sum over h_1 occurring in (3.10) by

\ll_{\mathcal F}K\frac{H_0}{h_2^2}L^B (1+|t+v_1|)^{A/2}(1+|-t+v_2|)^{A/2}.

This formula is only used when H_0/h_2^2\geq1; otherwise that sum is empty. Choose J_1>A+4. Since 1+|\pm t+v|\leq T(1+|v|), the integral in v_1,v_2 is O_A(T^A). Also

\sum_{h_2\geq1}\frac{\tau(h_2)^{C_{\rm ar}}}{h_2^2}<\infty. \tag{3.17}

One proof of this convergence is its Euler product: its local factor is 1+O_{C_{\rm ar}}(p^{-2}), since \sum_{a\geq1}(a+1)^{C_{\rm ar}}p^{-2a} \ll_{C_{\rm ar}}p^{-2} uniformly for p\geq2. Consequently the nonzero contribution is bounded by

\ll_{A,B,\mathcal F,G}b^{-C_{\rm ar}}KL^BT^A (N_1N_2)^{-1/2+b}H_0 \ll_{A,B,\mathcal F,G} \log^{C_0}(3M+3N)K\frac{N}{MP^2}L^BT^A.

Here (N_1N_2)^b\ll_G1 and \sqrt{N_1N_2}\ll_GN. The sums of the factors from two converge by (3.12). This proves (3.16). If the Fourier support contains no nonzero frequency, the same proof uses only its zero-mode part.

Recovering the squarefree average. Now inflate an admissible parameter by setting m=dp^2. If c=\chi_d(2), multiplicativity gives the exact identity

P_d(N,t;G)=\sum_{a\geq0} \lambda_F(p^a)\chi_d(p)^a p^{-a(1/2+it)} P_{dp^2}^c(N/p^a,t;G). \tag{3.18}

Indeed z_{dp^2}(n) deletes all positive powers of p and agrees with \chi_d(n) on integers prime to p; reinstating their Euler coefficients gives the original sum. If p\mid d, the terms with a\geq1 vanish, so the identity also covers that case.

Equip pairs (d,p), with M\leq|d|<2M, \chi_d(2)=c, and p\in\mathcal P, with squared norm (M|\mathcal P|)^{-1}\sum_{d,p}|\cdot|^2. The map (d,p)\mapsto dp^2 is injective: in the prime factorization of its absolute value the only exponent exceeding one occurs at p, and is either two or three. Moreover |dp^2|<8U. Thus the a=0 term has norm at most

\left(\frac{U}{M|\mathcal P|}\right)^{1/2} \sup_{0<N'\leq N} \left(\frac1U\sum_m\Phi(m/U)|P_m^c(N',t;G)|^2\right)^{1/2} \ll(P\log(2P))^{1/2}\mathcal B^{1/2},

where \mathcal B denotes the right side of (3.16). For a\geq1 fix p before summing in d. The weaker bound \sum_d|P_{dp^2}^c(N/p^a,t;G)|^2\leq U\mathcal B gives pair norm at most (a+1)P^{1-a/2}\mathcal B^{1/2}. Minkowski’s inequality and

\sum_{a\geq1}(a+1)P^{-a/2}\ll P^{-1/2}

show that these terms together have norm O(P^{1/2}\mathcal B^{1/2}). Summing the two choices of c proves

\begin{align*} \frac1M\sum_d|P_d(N,t;G)|^2 &\ll_G\log^{C_0}(3M+3N)P\log(2P) \left(1+C_{A,B,\mathcal F,G}K\frac{N}{MP^2}L^BT^A\right). \tag{3.19}\end{align*}

Here is an explicit noncircular choice of exponents. Set

\begin{split} C_0&=512,\qquad C_1=C_0+32,\qquad C_2=C_0+C_1+4,\\ R&=C_2+4,\qquad C_3=3C_2+10,\qquad A=B=2(C_3+20). \end{split} \tag{3.20}

The letter R in this proof denotes a fixed contour abscissa; it is unrelated to a rank truncation threshold used later in the paper. For any prescribed \varepsilon>0, choose

P=P_0[L(1+N/M)T]^{C_1}. \tag{3.21}

Once A,B and the fixed weight family have been selected, a sufficiently large P_0 ensures (3.15) and gives

\begin{align*} \frac1M\sum_d|P_d(N,t;G)|^2 &\leq C_*[L(1+N/M)T]^{C_2} \\ &\quad+\varepsilon K L^{B-10}T^{A-4}(1+N/M)^{-4}. \tag{3.22}\end{align*}

The constant C_* can depend on P_0 and the chosen fixed data, but not on K,M,N,t. For explicit verification, put q=1+N/M and D_0=LqT. Then \log(3M+3N)\ll Lq and

\frac{\log(2P)}P \leq\frac{\log(2P_0)+C_1}{P_0}D_0^{-C_1+1}.

The recursive coefficient in (3.19) is therefore at most a fixed multiple of

\frac{\log(2P_0)+C_1}{P_0} K L^{B+C_0-C_1+1}T^{A-C_1+1}q^{C_0-C_1+2}.

Our value of C_1 leaves at least the losses 10,4,4 displayed in (3.22). Its prefactor can be made smaller than \varepsilon. The nonrecursive term is bounded by C_*D_0^{C_0+C_1+1} and hence by the stated C_2 power. In particular C_2 was fixed before A,B,\varepsilon,P_0,K.

Reconstructing the central-line values. We next reconstruct L on the central line. Choose a fixed smooth dyadic partition G_0 with common compact support in (0,\infty), so that \sum_{N=1,2,4,\ldots}G_0(n/N)=1 for every integer n\geq1. Let C_d=\sqrt{q_F}|d|/(2\pi) and define

I_d(t)=\frac1{2\pi i}\int_{(R)} L_{F^{(d)}}(1/2+it+w)C_d^w \frac{\Gamma(1+it+w)}{\Gamma(1+it)}\frac{e^{w^2}}w\,dw.

Moving the contour to \Re w=-R crosses only the residue L_{F^{(d)}}(1/2+it), because the completed function is entire. Apply its functional equation on the new line and replace w by -w. One obtains the exact approximate functional equation

L_{F^{(d)}}(1/2+it)=I_d(t)+\omega_d(t)I_d(-t),\qquad \omega_d(t)=\epsilon_d C_d^{-2it} \frac{\Gamma(1-it)}{\Gamma(1+it)}, \quad |\omega_d(t)|=1. \tag{3.23}

The Gaussian makes the contour displacement legitimate. Initially, on \Re w=R, the Dirichlet series is absolutely convergent, so we may insert the dyadic partition.

For 0\leq c\leq R, Stirling’s formula uniformly gives

\left|\frac{\Gamma(1+c+i(t+v))}{\Gamma(1+it)}\right| \ll_R T^c(1+|v|)^{R+1/2}e^{\pi|v|/2}. \tag{3.24}

Indeed the quotient of the exponential factors is at most e^{\pi|v|/2}, and

\frac{(1+|t+v|)^{c+1/2}}{(1+|t|)^{1/2}} \leq T^c(1+|v|)^{c+1/2}.

The same estimates with 1+|t+v| also cover bounded ordinates, including v near -t. Thus the bound is uniform as c tends to zero. For a fixed dyadic piece the polynomial is finite, so its contour can be moved to any 0<c\leq R. Multiplying (3.24) by |e^{(c+iv)^2}| absorbs its v-factors into O_R(e^{-v^2/2}) and yields

|L_{F^{(d)}}(1/2+it)| \ll_{R,\mathcal F}\sum_{\nu=\pm1}\sum_N \int_{\mathbb R}\frac{e^{-v^2/2}}{|c_N+iv|} \left(\frac{MT}N\right)^{c_N} |P_d(N,\nu t+v;G_0(y)y^{-c_N})|\,dv. \tag{3.25}

There is no use of the desired moment to justify this representation: on the initial fixed line R, the elementary bound |P_d(N,t;G)|\ll_G\sqrt N\log(2+N) makes the sum of the long pieces converge, since R>1/2. Finitely many shorter pieces can then be moved separately. The moment estimates below also show convergence after taking the family norm.

Use

c_N=\frac1{\log(3MT)}\quad(N\leq MT^2),\qquad c_N=R\quad(N>MT^2).

Apply (3.22) uniformly to the fixed smooth family G_0(y)y^{-c}, 0\leq c\leq R, and use Minkowski in (3.25). We spell out the two contributions. For the nonrecursive square-root term and N\leq MT^2,

[L(1+N/M)(1+|\nu t+v|)]^{C_2/2} \ll L^{C_2/2}T^{3C_2/2}(1+|v|)^{C_2/2}.

There are O(\log(3MT^2)) such dyadic pieces, (MT/N)^{c_N}\leq e for N\geq1, and 1/|c_N+iv|\leq\log(3MT). Since both logarithms are O(LT), their squared total cost gives at most C_{**}(LT)^{3C_2+4} in the mean square. For the long pieces put q'=N/M>T^2. Then

\sum_{q'>T^2}\left(\frac T{q'}\right)^R(q')^{C_2/2} \ll_R T^{-R+C_2},

where q' runs over a dyadic progression. Including the outside factor L^{C_2/2}T^{C_2/2} again fits within C_{**}(LT)^{C_3} by (3.20).

For the recursive square-root term, the short dyadic sum satisfies

\sum_{N\leq MT^2}(1+N/M)^{-2}\ll\log(3M)=L.

The Gaussian absorbs (1+|v|)^{(A-4)/2}, so the resulting norm is at most

C_{A,R,\mathcal F}\sqrt{\varepsilon K}\, L^{B/2-5}T^{A/2-2}\,L\log(3MT) \ll C_{A,R,\mathcal F}\sqrt{\varepsilon K}\, L^{B/2}T^{A/2}.

For the long pieces we have the stronger estimate

\sum_{q'>T^2}\left(\frac T{q'}\right)^R(1+q')^{-2} \ll_R T^{-R-4}, \tag{3.26}

which gives the same bound. Squaring the total norm now proves

\frac1M\sum_d|L_{F^{(d)}}(1/2+it)|^2 \leq C_{**}(LT)^{C_3} +C_{\dagger}\varepsilon K L^BT^A. \tag{3.27}

Here C_{\dagger} depends on A,R,\mathcal F but not on P_0,K,M,t; C_{**} may depend on P_0. This independence is essential when choosing the constants.

Closing the induction in the strip. It remains to extend the estimate to the strip without a factor for the number of twists. Form the vector

\mathbf V_F(s)=\big(M^{-1/2}L_{F^{(d)}}(s)\big)_d

in the finite-dimensional Euclidean space indexed by the current admissible block. On \Re s=2 its squared norm is bounded by an absolute constant: each L-value has modulus at most \sum_n\tau(n)n^{-2}=\zeta(2)^2, and the number of parameters is O(M). On \Re s=1/2, (3.27) gives the stated vector norm bound.

For each constant unit vector u apply the scalar strip principle to

f_u(s)=\frac{\langle\mathbf V_F(s),u\rangle}{(1+s)^{A/2}}.

Here A is even by (3.20). On both boundaries |1+s|\asymp1+|\Im s|, with constants independent of the number of twists. The scalar boundary bound is therefore at most

C_A\big(C_{**}L^{C_3}+C_{\dagger}\varepsilon K L^B+1\big)^{1/2}.

For clarity, finite-order growth suffices for the strip principle: multiply f_u(s) by \exp\{-\rho\cos(s-5/4)\}, with \rho>0. Its modulus is at most one on the strip boundaries and it decays faster than every finite-order growth bound on horizontal sides, since \cos(\Re s-5/4)>0 for 1/2\leq\Re s\leq2. Apply the maximum principle on rectangles and then let their heights tend to infinity and \rho decrease to zero. Taking the supremum over unit vectors at the desired point gives

\|\mathbf V_F(\sigma+it)\|_2^2 \leq C_{\rm st} \big(C_{**}L^{C_3}+C_{\dagger}\varepsilon K L^B+1\big)T^A, \qquad 1/2\leq\sigma\leq2. \tag{3.28}

This argument has no dimension-dependent loss.

The choice order is now explicit. Fix the family, the elementary arithmetic exponent, C_0,C_1,C_2,R,C_3,A,B as above, and then all needed fixed kernel orders. Next choose 0<\varepsilon<(4C_{\rm st}C_{\dagger})^{-1}, choose P_0 to obtain (3.22) for the entire weight family, and finally choose K so large that C_{\rm st}(C_{**}L^{C_3}+1)\leq K L^B/2 for every L\geq\log3. This is possible because B>C_3 and C_{**} is independent of K. Equation (3.28) proves (3.13) at height M. At M=1, all dual sums used above are empty, so this also establishes the initial step. The simultaneous induction is complete.

The induction just completed uses the fixed weight family G_0(y)y^{-c}, 0\leq c\leq R. For any other fixed smooth compactly supported G, repeat the polynomial argument through (3.22), using the established L-function bound at smaller heights. The constants P_0 and C_* may now depend on G, while K,A,B remain fixed. Since A,B>C_2, this proves (3.3), with the asserted uniformity for fixed uniformly smooth weight families. Finally use Lemma 2.1, bounded multiplicity, and a sum over admissible dyadic blocks of total length O(H) to obtain (3.2). No analytic-density input has entered the argument.

3.4 Short polynomials and auxiliary multipliers

The second moments are now available at every height. We use them to bound the complete sum of nonzero Poisson frequencies, retaining the zero frequency as an exact independent-model average. The resulting comparison permits a short polynomial multiplier, as required for the mollifiers below.

Fix a nonnegative smooth function \Psi compactly supported in \{x:0<|x|<\infty\}, with \Psi(x)\geq1 when 1\leq|x|\leq2. Fix c\in\{1,-1\}. The formal character z_m and the independent variables Z always have value c at two. At odd primes their model law is

\mathbb P(Z(p)=0)=\frac1p,\qquad \mathbb P(Z(p)=1)=\mathbb P(Z(p)=-1)=\frac{1-1/p}{2}.

They are extended completely multiplicatively. This is a model for complete integer residue averages.

Lemma 3.6 (Summation of all dual frequencies). For fixed B\geq0, J_1>1, and Q>0,

\sum_{T=1,2,4,\ldots}T\log^B(3T)(1+T/Q)^{-J_1} \ll_{B,J_1} \begin{cases} Q^{J_1},&0<Q<1,\\ Q\log^B(3Q),&Q\geq1. \end{cases} \tag{3.29}

In particular the first bound is at most a constant times Q.

Proof. If Q<1, bound (1+T/Q)^{-J_1} by (Q/T)^{J_1}. The remaining series is \sum_{j\geq0}2^{-(J_1-1)j}\log^B(3\cdot2^j)<\infty. For Q\geq1, the part T\leq Q is bounded by \log^B(3Q)\sum_{T\leq Q}T\ll Q\log^B(3Q). For the remaining part choose the first dyadic T_0>Q, so Q<T_0\leq2Q, and write T=2^jT_0. The summand is at most

C_B Q\,2^{-(J_1-1)j} \big(\log^B(3Q)+(j+1)^B\big).

Both resulting geometric series converge. This estimates the infinite frequency tail before any logarithm is replaced by \log X.

Proposition 3.7 (Comparison with the independent model). Let \ell=\log X, where X is sufficiently large, and let

c_1\ell^{-1/10}\leq\Delta\leq\frac12

for a fixed c_1>0. There are fixed constants \eta,c_2>0 for which the following holds. Let

S_V(x)=\sum_{n\geq1}\frac{\lambda_F(n)V(n)}{\sqrt n}\, w_x(\ell^{-1}\log n),\qquad H_V=\sum_{r'\leq R_0}h(r')V(r'),

where V=z_m or Z. Suppose that S_V has length at most X^{1-\Delta}, that

1\leq R_0\leq X^{\eta\Delta},\qquad \sum_{r'\leq R_0}|h(r')|\leq C_H R_0^2, \tag{3.30}

and that w_x and a function A(x) have bounds by a fixed power of \ell for all derivatives up to a sufficiently large fixed order. For w_x these bounds are required after smooth dyadic localization in n, on the scaled variables n/N and x in a fixed neighborhood of \operatorname{supp}\Psi. They may in particular follow from bounds in u=\ell^{-1}\log n\geq0 and x, with a smooth extension at n=1. Then

\begin{align*} &\frac1X\sum_{m\in\mathbb Z}\Psi(m/X) |H_{z_m}S_{z_m}(m/X)-A(m/X)|^2 \\ &\hspace{8mm}= \int_{\mathbb R}\Psi(x)\, \mathbb E|H_ZS_Z(x)-A(x)|^2\,dx +O\big(\exp(-c_2\Delta\ell)\big). \tag{3.31}\end{align*}

The constants and the sufficiently large X threshold are uniform when the stated support, coefficient, and derivative bounds are uniform. They do not depend on \Delta or on an index parametrizing such weights. One may take

C'=C_{\rm ar}+1=257,\qquad \eta=\frac1{4(4+2C')},\qquad c_2=\frac12. \tag{3.32}

Proof. Put L=X^{1-\Delta}. If the length hypothesis specifies only that the integer coefficients vanish for n>L, multiply the interpolating weight by \rho_+(n/L), where \rho_+ is a fixed smooth function equal to one on (-\infty,1] and zero on [2,\infty). This preserves every integer coefficient and gives real support in n\leq2L. On a dyadic scale meeting the transition, N/L is bounded, so derivatives of \rho_+(Ny/L) add only fixed constants to the assumed scaled seminorm bounds. Thus all nonempty localized lengths satisfy N_i\ll L.

Expand the square on the left of (3.31). A term involving two multiplier indices r_1',r_2' has character factor z_m(r_1'r_2'n_1n_2). Its odd multiplier part is an integer r\leq R_0^2. Powers of two contribute only fixed signs. Split powers of two out of n_1,n_2, and insert smooth dyadic partitions in their odd parts. Each resulting term has exactly the form (3.9) with U=X, t_1=t_2=0, and a weight W whose required seminorm is O(\ell^{D_1}) for a fixed D_1. The independent factors coming from the powers of two satisfy (3.12). Cross terms with A(x) are covered by using an index supported just at one: choose a fixed smooth function supported in (1/2,3/2) and equal to one at one. The identity \lambda_F(1)=1 then puts them in the same form. The term |A|^2 is covered by two such indices. Its derivatives obey the same fixed polynomial bounds.

The zero frequency is exactly the model expression. In fact, for an odd prime and v\geq1,

\frac1{p^v}\sum_{a\bmod p^v}\left(\frac a{p^v}\right) =\begin{cases}0&v\text{ odd},\\1-p^{-1}&v\text{ even},\end{cases} =\mathbb E Z(p)^v.

For v=0 both sides are one. Chinese remaindering gives independence at distinct odd primes, and the value at two is already fixed. The integral of the zero-frequency smooth amplitude is thus the corresponding term on the right of (3.31).

It remains to estimate the nonzero frequencies. Fix an odd multiplier r and localized odd lengths N_1,N_2, and set

b=\frac1{10\ell},\qquad Q=\frac{rN_1N_2}{X}.

Only nonempty lengths need be considered, so N_i is bounded below by a fixed positive constant. Also N_i\ll X^{1-\Delta}, whence (N_1N_2)^b\ll1. Proposition 3.1 is available at every height. For a dyadic frequency range T\leq|h|<2T, write h=h_1h_2^2. For fixed h_2, the parameter h_1 lies in 0<|h_1|<2T/h_2^2. Cauchy–Schwarz and (3.2) imply

\begin{align*} &\sum_{\substack{T\leq|h|<2T\\h=h_1h_2^2}} \tau(h_2)^{C_{\rm ar}} \prod_{i=1}^2 |L_{F^{(\nu h_1)}}(1/2+b+iv_i)|\\ &\quad\ll T\log^B(3T)(1+|v_1|)^{A/2}(1+|v_2|)^{A/2} \sum_{h_2\leq\sqrt{2T}}\frac{\tau(h_2)^{C_{\rm ar}}}{h_2^2}\\ &\quad\ll T\log^B(3T) (1+|v_1|)^{A/2}(1+|v_2|)^{A/2}.\end{align*}

This inequality applies separately to each \nu; it includes both signs of h. Choose J_1>A+4 in (3.10), and then fix the corresponding smoothness order. Its vertical integral is convergent. The remaining sum is bounded, by Lemma 3.6, by

\ll \ell^{D_2}r^{C_{\rm ar}}(N_1N_2)^{-1/2} \begin{cases}Q^{J_1}&Q<1,\\Q\log^B(3Q)&Q\geq1. \end{cases}

When Q\geq1 we have Q\ll X using r\leq R_0^2, (3.30), and \eta<1; hence \log(3Q)\ll\ell. When Q<1 use Q^{J_1}\leq Q. In both regimes the error for this localized pair is therefore

\ll\ell^{D_3}r^{C'}\frac{\sqrt{N_1N_2}}X, \qquad C'=C_{\rm ar}+1. \tag{3.33}

The increase from C_{\rm ar} to C' is only the factor r in Q, not a smoothness loss. Notice that this argument controls arbitrarily large dual frequencies as well as the case Q<1.

There are O(\ell) possible nonempty dyadic pieces for each main index. Their cost is a fixed logarithmic power. Summing the coefficients from powers of two by (3.12) costs only a constant. The two multiplier coefficient sums and the bound r\leq R_0^2 cost at most

(1+\textstyle\sum|h(r')|)^2R_0^{2C'}\ll_{C_H}R_0^{4+2C'}.

Since \sqrt{N_1N_2}/X\ll X^{-\Delta}, including the terms with an index at one, the full error is

\ll\ell^{D_4}X^{-\Delta}R_0^{4+2C'} \leq\ell^{D_4}\exp(-3\Delta\ell/4). \tag{3.34}

Our choices in (3.32) give the last inequality. The power D_4 is fixed before choosing X. Because \Delta\ell\geq c_1\ell^{9/10}, for one sufficiently large X the factor \ell^{D_4} is at most \exp(\Delta\ell/4). This proves (3.31) with c_2=1/2.

The endpoint at n=1 in this proposition needs no extension to a fixed negative interval in u. Extend a dyadically localized weight only to, say, n\geq1/2. In the coordinate \log n=\ell u this is a fixed interval, and smooth cutoffs there introduce at most fixed powers of \ell in u derivatives. On a dyadic scale, repeated differentiation of w_x(\log(Ny)/\ell) instead introduces powers of 1/\ell and bounded powers of 1/y. Thus the required finite seminorm bounds are precisely those in the proposition, even at the first piece.

4 Completed derivatives and their weights

A large analytic rank forces a completed derivative to vanish. For the matching functional-equation sign, we express that vanishing as an exact weighted-series identity, partition the series into short pieces, and bound the remaining infinite piece using the second moments of Section 3. The short pieces will be treated by mollification in Section 5.

Fix a curve F in the finite family \mathcal F, write \lambda=\lambda_F, and put C_F=\sqrt{q_F}/(2\pi). The variable x will range over a fixed compact subset \mathcal K of \mathbb R\setminus\{0\}, chosen large enough to contain the support of the averaging weight in Proposition 3.7. Derivative bounds in x are understood on a fixed compact neighborhood of \mathcal K disjoint from zero. All constants below may depend on this compact set and on the fixed finite family.

The order of choices is as follows. First fix the exponents in Proposition 3.2, and all the finite orders of differentiation needed for Proposition 3.7, the Mellin inversion below, and the subsequent Fourier estimates. Next choose a sufficiently large fixed integer k_0. Finally choose one lower bound for X, valid simultaneously for all the integers

\ell=\log X,\qquad k_0\le k\le \lfloor\ell^{3/5}\rfloor . \tag{4.1}

The estimates in this section respect this order. In particular, the number of derivatives is never allowed to increase with k or X.

4.1 The exact completed derivative identity

For k\ge1, x\ne0, and real u, define

W_{k,x}(u)= \int_0^\infty e^{-v} \left(1-u+\frac{\log(C_F|x|v)}{\ell}\right)_+^k\,dv, \qquad y_+=\max(y,0). \tag{4.2}

For every fixed choice of the parameters the integral is finite. The weighted sum below is an infinite, absolutely convergent smoothed Dirichlet series; its individual short pieces will be finite sums.

Lemma 4.1 (Completed derivative identity). Let d be admissible, X\le |d|<2X, and x=d/X. Set

g_d(z)=L_{F^{(d)}}(1/2+z)(C_F|d|)^z\Gamma(1+z), \qquad \epsilon_d=\operatorname{sign}(F^{(d)}).

Then g_d is entire, g_d(-z)=\epsilon_d g_d(z), and

\begin{split} \mathcal S_d &:= \sum_{n\ge1}\frac{\lambda(n)\chi_d(n)}{\sqrt n} W_{k,x}(\ell^{-1}\log n)\\ &=\frac{k!}{\ell^k}\frac{1}{2\pi i} \int_{(2)}g_d(z)\frac{dz}{z^{k+1}}. \end{split} \tag{4.3}

More precisely,

\bigl(1+\epsilon_d(-1)^k\bigr)\mathcal S_d =\ell^{-k}g_d^{(k)}(0). \tag{4.4}

Consequently, if a(F^{(d)})>k and \epsilon_d=(-1)^k, then

\sum_{n\ge1}\frac{\lambda(n)\chi_d(n)}{\sqrt n} W_{k,d/X}(\ell^{-1}\log n)=0. \tag{4.5}

Proof. The completed function is

\Lambda_d(s)=(C_F|d|)^s\Gamma(s+1/2)L_{F^{(d)}}(s).

Thus g_d(z)=(C_F|d|)^{-1/2}\Lambda_d(1/2+z). Its entireness and reflection law follow from those of \Lambda_d.

For T>0, Mellin inversion gives

\frac{1}{2\pi i}\int_{(2)}\frac{T^z}{z^{k+1}}\,dz =\frac{(\log T)_+^k}{k!}.

Insert the absolutely convergent Dirichlet series for L_{F^{(d)}}(1/2+z), and use \Gamma(1+z)=\int_0^\infty e^{-v}v^z\,dv. On this line all exchanges are absolutely convergent: the series is dominated by \sum_n\tau(n)n^{-5/2}, and the other two factors to be integrated are dominated by e^{-v}v^2 and |2+it|^{-k-1}. The result is (4.3), because

\ell^{-1}\log(C_F|d|v/n) =1-\ell^{-1}\log n+\ell^{-1}\log(C_F|x|v).

This argument, or the same computation with absolute coefficient values, also proves absolute convergence of the series.

Let I_+ and I_- denote the integrals of g_d(z)z^{-k-1}/(2\pi i) on the upward oriented lines \operatorname{Re}z=2 and \operatorname{Re}z=-2. Shifting between these lines crosses only the pole at zero, and gives

I_+-I_-=\frac{g_d^{(k)}(0)}{k!}.

The horizontal integrals tend to zero: in this fixed strip the uncompleted L-function has polynomial growth, while the gamma factor has exponential decay on horizontal segments tending to infinity. Apparent gamma poles on the real axis are removable in g_d. Changing z to -z, with orientations included, gives

I_-=(-1)^{k+1}\epsilon_d I_+.

Multiplication by k!/\ell^k proves (4.4). Finally, the completing factor is holomorphic and nonzero at zero. Hence a(F^{(d)})>k implies g_d^{(k)}(0)=0, and the stipulated sign makes the coefficient on the left of (4.4) equal to two.

4.2 Partition and derivative estimates

Fix a C^\infty, nondecreasing function f_*\colon\mathbb R\to[0,1] which is zero on (-\infty,1/4] and one on [1/2,\infty). Define

J=\left\lfloor\frac{\log\ell}{10\log2}\right\rfloor,\qquad \delta_j=2^{-j},\qquad F_j(u)=f_*((1-u)/\delta_j)\quad(0\le j\le J). \tag{4.6}

In particular, for sufficiently large X,

J\ge1,\qquad \ell^{-1/10}\le\delta_J<2\ell^{-1/10},\qquad \frac{k}{\ell\delta_j}\le\ell^{-3/10} \quad(0\le j\le J). \tag{4.7}

Set

\begin{aligned} w_{0,x}(u)&=F_0(u)W_{k,x}(u),\\ w_{j,x}(u)&=(F_j(u)-F_{j-1}(u))W_{k,x}(u) &&(1\le j\le J),\\ w_{*,x}(u)&=(1-F_J(u))W_{k,x}(u). \end{aligned} \tag{4.8}

These weights sum exactly to W_{k,x}. For V=\chi_d,z_m, or Z, write

\begin{aligned} S_{j,V}(x)&=\sum_{n\ge1} \frac{\lambda(n)V(n)}{\sqrt n}w_{j,x}(\ell^{-1}\log n),\\ S_{*,V}(x)&=\sum_{n\ge1} \frac{\lambda(n)V(n)}{\sqrt n}w_{*,x}(\ell^{-1}\log n). \end{aligned} \tag{4.9}

The first definition includes j=0. All the formal character values in these definitions have modulus at most one. The sums through j=J have length at most X^{1-\delta_j/4}, and

\operatorname{supp} w_{j,x} \subset[1-\delta_j,1-\delta_j/4]\quad(1\le j\le J). \tag{4.10}

Indeed F_j-F_{j-1} vanishes when 1-u\le\delta_j/4 or 1-u\ge\delta_j. The terminal weight is supported in u\ge1-\delta_J/2.

Lemma 4.2 (Fixed-order weight bounds). Fix an integer r\ge0, and then take k_0\ge r+2. For a,b\ge0, a+b\le r, uniformly in (4.1), x\in\mathcal K, and the indicated arguments, one has

\begin{align*} |\partial_u^a\partial_x^b w_{j,x}(u)| &\le C_r(k/\delta_j)^r\delta_j^k &&(1\le j\le J,\ u\in\mathbb R), \tag{4.11}\\ |\partial_u^a\partial_x^b w_{0,x}(u)| &\le C_r k^r &&(u\ge-\log2/\ell). \tag{4.12}\end{align*}

There is also c>0, independent of r,k,X, such that, with \delta=\delta_J and n=e^{\ell u}>0,

|\partial_u^a\partial_x^b w_{*,x}(u)| \le C_r(k/\delta)^r\delta^k e^{-cn/X}. \tag{4.13}

Changing the fixed compact neighborhood of \mathcal K changes only the constants.

Proof. It is convenient first to differentiate using D_x=x\partial_x. For

h=1-u+\ell^{-1}\log(C_F|x|v)

and a+b\le r, differentiation under the integral gives

\partial_u^aD_x^b h_+^k =(-1)^a\ell^{-b}(k)_{a+b}h_+^{k-a-b}, \tag{4.14}

where (k)_t=k(k-1)\cdots(k-t+1). The choice k\ge r+2 ensures enough continuous derivatives at h=0; domination for differentiating follows from the estimates below. Ordinary x-derivatives are fixed linear combinations of x^{-b}D_x^i, i\le b, and therefore satisfy the same bounds on our compact set.

Suppose 1-u\le\delta', where \delta'>0. For 0\le t\le r, write m=k-t>0 and a_t=m/(\ell\delta'). The elementary inequality (1+q)_+^m\le e^{mq}, valid for every real q, gives

h_+^m \le(\delta')^m(C_F|x|v)^{a_t}. \tag{4.15}

If \delta'=\delta_j, then 0<a_t\le\ell^{-3/10} by (4.7), so

\int_0^\infty e^{-v}(C_F|x|v)^{a_t}\,dv =(C_F|x|)^{a_t}\Gamma(1+a_t)\le C.

The bound is uniform once X is large enough that a_t\le1. Thus, on 1-u\le\delta_j, a derivative of W_{k,x} involving at most r differentiations is bounded by a constant times k^r\delta_j^{k-r}. The cutoff derivatives of order q cost O_r(\delta_j^{-q}). More precisely, each Leibniz term with t derivatives hitting W and q hitting a cutoff has t+q\le r, and is at most

C_r k^t\delta_j^{k-t-q} \le C_r(k/\delta_j)^r\delta_j^k.

This proves (4.11).

For u\ge-\log2/\ell, use instead \delta'=1+\log2/\ell. Now (\delta')^k\le\exp(k\log2/\ell)\le2 for large X, and a_t\le k/\ell\le\ell^{-2/5}. The same argument and the fixed derivative bounds for F_0 prove (4.12).

On the support of the terminal cutoff, or any nonzero derivative of it, 1-u\le\delta_J/2\le\delta_J. Moreover h>0 implies

v>\frac{n}{C_F|x|X}.

Retain half the exponential in the integral. Uniformly on our compact set,

\begin{split} \int_{\{h>0\}}e^{-v}(C_F|x|v)^{a_t}\,dv &\le e^{-n/(2C_F|x|X)} (C_F|x|)^{a_t} \int_0^\infty e^{-v/2}v^{a_t}\,dv\\ &=e^{-n/(2C_F|x|X)} (C_F|x|)^{a_t}2^{1+a_t}\Gamma(1+a_t) \le C e^{-cn/X}. \end{split} \tag{4.16}

Here a_t=(k-t)/(\ell\delta_J)\le\ell^{-3/10}, so 2^{1+a_t}\Gamma(1+a_t) is bounded independently of k. The same Leibniz calculation now proves (4.13). All integrands used for differentiation are dominated on compact sets by the displayed integrable majorants, which also justifies (4.14) under the integral.

Corollary 4.3 (Comparison interface). For every fixed derivative order r, the short weights satisfy the smoothness assumptions of Proposition 3.7 with derivative bounds \ell^{C_r}, uniformly in j,k,X. They have length X^{1-\Delta_j}, with

\Delta_j=\delta_j/4,\qquad \tfrac14\ell^{-1/10}\le\Delta_j\le\tfrac14 .

The deterministic term

s=k/\ell,\qquad A_x=(C_F|x|)^s\Gamma(1+s) \tag{4.17}

has uniformly bounded derivatives of each fixed order on \mathcal K, and is bounded above and below by positive constants. The endpoint enlargement at n=1 can be made inside the fixed range n\ge1/2.

Proof. The bounds k\le\ell^{3/5} and \delta_j^{-1}\le\ell^{1/10} make (4.11) polynomial in \ell. Choose a fixed smooth function \chi equal to zero on (-\infty,-\log2] and equal to one on [0,\infty). For the comparison alone, replace w_{0,x}(u) on the real line by

\widetilde w_{0,x}(u)=\chi(\ell u)w_{0,x}(u).

It agrees with the original weight at every positive integer n=e^{\ell u}, and its extra derivatives cost only fixed powers of \ell, by (4.12). Its left support is u\ge-\log2/\ell, exactly the enlargement n\ge1/2. For j\ge1, the weights already vanish on a neighborhood of u\le0. After a fixed smooth dyadic localization n=Ny, the operator y\partial_y acts as \ell^{-1}\partial_u, so the same bounds give all the required seminorms in the scaled variables. The endpoint extension has therefore taken place in \log n; no extension to a fixed negative value of u is used.

Finally 0<s\le\ell^{-2/5}, while C_F|x| lies in a fixed positive compact interval. The formula for A_x, its derivatives in x, and the continuity and positivity of \Gamma(1+s) give the assertions concerning A_x.

4.3 The terminal mean square

We use the following consequence of Proposition 3.2. For general X, cover [X,2X) by at most two dyadic blocks whose heights are comparable to X; the normalization and polynomial factors in that proposition then change by fixed constants only. For any fixed smooth compactly supported function G on (0,\infty), there are fixed exponents A,B such that

\frac1X\sum_{\substack{d\ {\rm admissible}\\X\le|d|<2X}} \left|\sum_{n\ge1}\frac{\lambda(n)\chi_d(n)}{\sqrt n}\, n^{-it}G(n/N)\right|^2 \ll_G \ell^B(1+|t|)^A(1+N/X)^A. \tag{4.18}

Its applicability includes the fixed enlarging bump used below.

Proposition 4.4 (Terminal mean square). There is a fixed exponent C_T, chosen before k_0, such that uniformly in (4.1),

\frac1X\sum_{\substack{d\ {\rm admissible}\\X\le|d|<2X}} |S_{*,\chi_d}(d/X)|^2 \ll \ell^{C_T}\delta_J^{2k}. \tag{4.19}

The same estimate holds after restricting the summation to either value of \chi_d(2).

Proof. Choose a smooth dyadic partition with a fixed \rho\in C_c^\infty((1/2,2)) satisfying

\sum_{N\in\{1,2,4,\ldots\}}\rho(n/N)=1\qquad(n\ge1).

For example one may start with a smooth nonincreasing function equal to one on (0,1] and zero on [2,\infty), and take its difference at arguments y and 2y; choosing its transition strictly inside (1,2) gives the asserted compact support. Fix also G\in C_c^\infty((0,\infty)) equal to one on \operatorname{supp}\rho. Put

T_N(y,x)=\rho(y)w_{*,x}(\ell^{-1}\log(Ny)),\qquad \widehat T_N(t,x)=\int_0^\infty T_N(y,x)y^{it}\frac{dy}{y}.

Select once and for all integers r>A/2+2 and D>A/2+2, and then choose k_0\ge r+2. If derivatives required elsewhere are of higher order, increase this fixed r first. By Lemma 4.2, differentiation on the y-scale through order r gives

\left|(y\partial_y)^a T_N(y,x)\right| \ll_r \ell^{C_r}\delta_J^k e^{-c'N/X} \qquad(0\le a\le r),

uniformly in x\in\mathcal K. There is no boundary term when integrating by parts in \log y. Consequently,

\sup_{x\in\mathcal K}|\widehat T_N(t,x)| \ll_{r,D}\ell^{C_r}\delta_J^k (1+N/X)^{-D}(1+|t|)^{-r}. \tag{4.20}

In passing from the exponential to (1+N/X)^{-D}, the constant depends on the fixed D, not on k.

Mellin inversion now expresses the N-piece of the terminal sum as

\frac1{2\pi}\int_{\mathbb R} \widehat T_N(t,d/X)N^{it} P_d(N,t)\,dt,\qquad P_d(N,t)=\sum_{n\ge1}\frac{\lambda(n)\chi_d(n)}{\sqrt n}\, n^{-it}G(n/N).

Indeed G(n/N)T_N(n/N,x)=T_N(n/N,x). Define the normalized family norm by

\|B_d\|_{2,X} =\left(\frac1X\sum_{\substack{d\ {\rm admissible}\\X\le|d|<2X}} |B_d|^2\right)^{1/2}.

We bound the kernel uniformly before applying the family moment. For each fixed t,

\|\widehat T_N(t,d/X)P_d(N,t)\|_{2,X} \le \sup_{x\in\mathcal K}|\widehat T_N(t,x)| \|P_d(N,t)\|_{2,X}.

Minkowski’s inequality, followed by (4.18) and (4.20), therefore yields

\begin{split} \|S_{*,\chi_d}(d/X)\|_{2,X} &\ll \ell^{C_r+B/2}\delta_J^k \sum_{N=1,2,4,\ldots}(1+N/X)^{-D+A/2} \int_{\mathbb R}(1+|t|)^{-r+A/2}\,dt\\ &\ll \ell^{C_r+B/2+1}\delta_J^k. \end{split}

The integral converges by the fixed choice of r. There are O(\ell) dyadic terms with N\le X, and those with N>X form a convergent geometric tail by the choice of D. All sums and integrals can first be truncated; the displayed integrable majorants justify passage to the limit. Squaring proves (4.19), for example with C_T=2C_r+B+2. This exponent depends only on choices made before k_0. Restricting the family can only decrease the nonnegative sum.

Lemma 4.5 (Uniform absorption of the terminal loss). After increasing the fixed k_0, one sufficiently large lower bound on X makes

\frac1X\sum_{\substack{d\ {\rm admissible}\\X\le|d|<2X}} |S_{*,\chi_d}(d/X)|^2 \ll 2^{-3Jk/2} \tag{4.21}

simultaneously for all k in (4.1). Moreover, for any fixed c,L>0, the comparison errors obey

e^{-c\Delta_j\ell} \le k^{-L}2^{-Ljk}\qquad(0\le j\le J) \tag{4.22}

for one sufficiently large lower bound on X.

Proof. The ratio of the right side of (4.19) to 2^{-3Jk/2}, apart from its fixed implied constant, is

\ell^{C_T}2^{-Jk/2}.

For J\ge1 this decreases with k, so throughout the permitted range it is at most its value at the fixed integer k_0. The floor in the definition of J gives

\ell^{C_T}2^{-Jk/2} \le \ell^{C_T}2^{-Jk_0/2} \le 2^{k_0/2}\ell^{C_T-k_0/20}.

Choose k_0>20C_T after C_T is fixed. The last expression then tends to zero with X. In particular the choice of a single X-threshold works for the entire k-range.

For the second assertion, \Delta_j\ell\ge\ell^{9/10}/4, whereas uniformly in the same range

L\log k+Ljk\log2 =O_L(\ell^{3/5}\log\ell)=o(\ell^{9/10}).

Taking logarithms proves (4.22).

5 Block mollifiers and independent-model mean squares

We seek polynomial multipliers that make the first short piece close to the positive quantity A_x from (4.17), while keeping the later pieces small. The construction has two separate tasks: control the multipliers on most integers, and prove mean-square bounds on the entire independent model. Their combination will allow the first piece to dominate the weighted-series identity.

Fix a member F of the finite family \mathcal F and a value c\in\{-1,1\} at the prime 2, and write \lambda=\lambda_F and \xi_p=\xi_{F,p}. The constants in this section are uniform in these two choices. We use the integer characters z_m and the independent variables Z defined above; in particular, at an odd prime

\mathbb P(Z(p)=0)=p^{-1},\qquad \mathbb P(Z(p)=1)=\mathbb P(Z(p)=-1)=(1-p^{-1})/2, \qquad Z(2)=c.

All model norms below are norms on this entire probability space. We use the parameters and weights of Section 4:

\ell=\log X,\qquad k_0\le k\le\ell^{3/5},\qquad J=\left\lfloor\frac{\log\ell}{10\log2}\right\rfloor, \qquad \delta_j=2^{-j},\qquad s=k/\ell.

Here k is an integer. We always take X sufficiently large that J\ge1 and 0<s\le1. The scaled variable x ranges over a fixed compact subset \mathcal X of \mathbb R\setminus\{0\} containing the support of the averaging weight. Constants may depend on this compact set, the fixed cutoff f_*, and \mathcal F.

The shift s comes from the weight of the first piece. Replacing the truncated power in (4.2) by its exponential reference gives the exact integral

\int_0^\infty e^{-v} \exp\bigl(-ku+s\log(C_F|x|v)\bigr)\,dv =A_xe^{-ku}.

At u=\log n/\ell, the reference weight is therefore A_xn^{-s}. This suggests a multiplier approximating the inverse Euler product at the real shift s. Lemma 5.8 and the final Fourier argument will quantify the replacement in the required norm; the reference calculation alone does not replace the weighted series.

5.1 Elementary prime estimates and local factors

We shall repeatedly use the elementary estimate \pi(y)\ll y/\log(2y). One proof starts with

\sum_{n<p\le2n}\log p\le\log\binom{2n}{n}\le2n\log2.

Summing on dyadic intervals gives \sum_{p\le y}\log p\ll y; separating p\le\sqrt y then proves the asserted estimate for \pi(y). Partial summation gives the following consequences, with absolute constants:

\begin{align*} \sum_{p\le y}\frac1p&\ll1+\log\log(3y),\\ \sum_{a<p\le b}\frac1p&\ll 1+\log\frac{\log b}{\log a}\quad(2\le a\le b), \tag{5.1}\\ \sum_{p>Y}p^{-1-2a} &\ll\int_{2a\log Y}^{\infty}\frac{e^{-v}}v\,dv \ll 1+\log^+\frac1{a\log Y}\qquad(0<a\le1,\ Y\ge2). \tag{5.2}\end{align*}

Here \log^+t=\max(0,\log t). If a\log Y\ge1/2, we also have

\int_{2a\log Y}^{\infty}\frac{e^{-v}}v\,dv \ll\frac{e^{-2a\log Y}}{a\log Y}.

For clarity, the first bound in (5.2) follows by integrating t^{-1-2a} against d\pi(t), discarding the nonpositive boundary term at Y, and using 1+2a\le3. We also need, for 0<a\le1 and h\ge a,

\sum_p\frac{\min(1,h\log p)}p p^{-2a} \ll 1+\log(1+h/a). \tag{5.3}

Here is a direct verification. If h\le1, primes with \log p\le1/h contribute at most

h\sum_{p\le e^{1/h}}\frac{\log p}{p}\ll1.

Between 1/h and 1/a the reciprocal-prime mass is O(1+\log(h/a)) by (5.1); primes beyond e^{1/a} contribute O(1) by (5.2). Empty ranges are omitted. If h>1, discard the minimum and use the same estimates to obtain O(1+\log(1/a)), which is bounded by the right side of (5.3).

For any real character value V(p)\in\{-1,0,1\} define

D_p(b,V)=1-\lambda(p)V(p)p^{-1/2-b} +\xi_p V(p)^2p^{-1-2b},\qquad \Re b\ge0. \tag{5.4}

The local parameter bound gives a factorization D_p(b,V)=\prod_{\nu=1}^2(1-\alpha_{p,\nu}V(p)p^{-1/2-b}), where |\alpha_{p,\nu}|\le1 and zero parameters are permitted. Consequently

(1-p^{-1/2})^2\le |D_p(b,V)|\le(1+p^{-1/2})^2. \tag{5.5}

For real b\ge0, the value of D_p(b,V) is positive: at a good prime its two factors are complex conjugates (or both positive real), and at a bad prime its nontrivial factor is positive. These facts apply equally to V=Z and V=z_m.

5.2 Construction, length, and the simultaneous product event

Radziwiłł and Soundararajan use disjoint prime blocks, truncated exponential polynomials, and relative truncation estimates in their study of central values of quadratic twists [15, Sections 3, 8, and 9]. Here we truncate products of inverse local Euler factors by total degree and estimate shifted norms over the full integer model defined in Section 2.

Put

Y_j=X^{\delta_j^2/\sqrt k},\qquad P_j^{\mathrm{eu}}(V)=\prod_{p\le Y_j}D_p(s,V)^{-1} \quad(0\le j\le J).

Since s\log Y_0=\sqrt k, the prime-tail estimate (5.2) makes \sum_{p>Y_0}p^{-1-2s} exponentially small. This sum will control the residual Euler product in mean square. For the later pieces, the available multiplier length decreases as their lengths approach X. The smaller cutoffs Y_j will keep the truncated products within the comparison allowance X^{\eta\delta_j/4}. In the estimates for these later pieces, the weight factor \delta_j^k will absorb fixed polynomial losses in k and 2^j. In the stated range \log Y_J\ge\ell^{1/2}, so every Y_j exceeds 2 for a single sufficiently large X threshold. For i\ge0 let

I_{ji}=\{p:Y_j^{2^{-i-1}}<p\le Y_j^{2^{-i}}\},\qquad m_{ji}=\lceil k^{1/4}+j+i\rceil.

We omit empty blocks. They form a disjoint partition of the primes at most Y_j, and (5.1) gives

\sum_{p\in I_{ji}}p^{-1}\le C \tag{5.6}

uniformly in j,i,k,X. Indeed, when the lower endpoint is at least 2, the ratio of the logarithms of the endpoints is 2; otherwise a nonempty block has upper endpoint less than 4. Set

\begin{align*} K_{ji}(V,z)&=\prod_{p\in I_{ji}} \left(1-\lambda(p)V(p)p^{-1/2-s}z +\xi_pV(p)^2p^{-1-2s}z^2\right), \\ T_{ji}(V)&=\sum_{b=0}^{m_{ji}}[z^b]K_{ji}(V,z), &H_j(V)&=\prod_i T_{ji}(V). \tag{5.7}\end{align*}

The coefficient extraction in this definition is followed by evaluation at z=1.

Lemma 5.1 (Length and coefficients). The polynomial H_j has an expansion

H_j(V)=\sum_{r\le R_j}h_j(r)V(r),\qquad |h_j(r)|\le\tau(r)r^{-1/2},\qquad \sum_r|h_j(r)|\ll R_j^2,

where, for a fixed constant C_{\rm len}>0, one may take

R_j=\exp\left(C_{\rm len}(k^{1/4}+j+1) \ell\delta_j^2/\sqrt k\right). \tag{5.8}

For every fixed \eta>0, a sufficiently large fixed k_0 ensures R_j\le X^{\eta\delta_j/4} for all 0\le j\le J and all k in the stated range. Thus H_j satisfies the multiplier hypotheses of Proposition 3.7, with \Delta=\delta_j/4.

Proof. In a block, a chosen monomial has prime exponents e_p\in\{0,1,2\} whose sum is at most m_{ji}. Its integer index is therefore at most \exp(m_{ji}2^{-i}\log Y_j). Since

\sum_{i\ge0}m_{ji}2^{-i} \le\sum_{i\ge0}(k^{1/4}+j+i+1)2^{-i} =2k^{1/4}+2j+4,

we obtain (5.8). Unique factorization shows that each index occurs in exactly one prime-exponent pattern. The truncations only delete patterns. A surviving coefficient is a product of local coefficients 1, -\lambda(p)p^{-1/2-s}, or \xi_pp^{-1-2s}, and hence is bounded by \tau(r)r^{-1/2-s}\le\tau(r)r^{-1/2}. For example,

\sum_{r\le R}\tau(r)r^{-1/2} =\sum_{ab\le R}(ab)^{-1/2} \le2\sqrt R\sum_{a\le R}\frac1a \ll\sqrt R\log(2R)\ll R^2\qquad(R\ge1).

Finally,

\frac{\log R_j}{\ell\delta_j/4} \le4C_{\rm len}\bigl(k^{-1/4}+(j+1)2^{-j}k^{-1/2}\bigr) \le8C_{\rm len}k^{-1/4}.

Here (j+1)2^{-j}\le1. Thus the fixed choice k_0\ge(8C_{\rm len}/\eta)^4 suffices simultaneously for all j. The coefficient estimate and this length bound verify both multiplier conditions of Proposition 3.7.

Lemma 5.2 (Prime-sum moments for the integer model). Let \mathcal I be any set of primes at most Y_0, and put

B_{\mathcal I}(V)=\sum_{p\in\mathcal I} \lambda(p)V(p)p^{-1/2-s}.

If k_0 is a sufficiently large absolute constant, then

\frac1X\sum_{X\le|m|<2X}|B_{\mathcal I}(z_m)|^{64} \ll\left(1+\sum_{p\in\mathcal I}\frac1p\right)^{32} \tag{5.9}

uniformly in \mathcal I,k,X.

Proof. First omit the deterministic prime 2 and write a_p=\lambda(p)p^{-1/2-s}. On expanding the model moment, any odd prime that occurs just once has zero expectation. Group the remaining terms by their partition of the 64 positions into q\le32 parts of sizes at least two. Since |a_p|\le2, for every part of size r\ge2 we have |a_p|^r\le2^{r-2}|a_p|^2. Summing the distinct-prime choices and then discarding distinctness bounds the moment by

C\sum_{q=1}^{32}\left(\sum_{p\in\mathcal I}|a_p|^2\right)^q \ll\left(1+\sum_{p\in\mathcal I}\frac1p\right)^{32}.

Restoring the prime 2 changes only the constant, by |u+v|^{64}\le2^{63}(|u|^{64}+|v|^{64}) and |a_2c|\le\sqrt2.

For completeness the passage to integers needs no estimate for primes in progressions. For each ordered 64-tuple of primes, the product of its character values is periodic modulo the product of its odd primes, which is at most Y_0^{64}. Its absolute value is at most one. The arithmetic mean over the two integer intervals X\le|m|<2X differs from its complete-residue mean by O(Y_0^{64}/X). The complete-residue mean is exactly the independent-model mean, by the Chinese remainder theorem and the counts of 0,1,-1 for the Legendre symbol. There are at most Y_0^{64} tuples and each coefficient has absolute value at most 2^{64}. Thus the discrepancy between that arithmetic mean and the model moment is

O(Y_0^{128}/X)=O(X^{-1+128/\sqrt k})=O(X^{-1/2})

after requiring \sqrt{k_0}\ge256. Since the number of integers in these intervals is O(X), this proves (5.9) with its normalization by X. If endpoints are not integers, the same period-counting argument changes only its absolute constant.

Proposition 5.3 (Simultaneous product event). Except for O(Xk^{-2}) integers in X\le|m|<2X, the following inequalities hold simultaneously:

\begin{align*} \frac12\le H_j(z_m)P_j^{\mathrm{eu}}(z_m)&\le2 &&(0\le j\le J), \tag{5.10}\\ \frac{P_0^{\mathrm{eu}}(z_m)}{P_j^{\mathrm{eu}}(z_m)} &\ge2^{-jk/8} &&(1\le j\le J), \tag{5.11}\\ P_0^{\mathrm{eu}}(z_m)&\ge2^{-Jk/8}. \tag{5.12}\end{align*}

The implied constant and the lower threshold k_0 do not depend on k,j,X.

Proof. For a block I=I_{ji} write B=B_I(z_m). The elementary expansion \log(1+w)=w+O(|w|^2) at all sufficiently large primes, together with (5.6), gives

\sup_{|z|=2}|K_{ji}(z_m,z)|\le e^{2|B|+C}, \qquad K_{ji}(z_m,1)\ge e^{-|B|-C}. \tag{5.13}

The finitely many smaller primes are included using (5.5) at z=1 and the direct upper bound \prod_{\nu}(1+2p^{-1/2}) on |z|=2; they change C by an absolute amount. Thus no nonvanishing assertion on the radius-two circle is required. Cauchy’s coefficient estimate now gives, with m=m_{ji},

\frac{|T_{ji}(z_m)-K_{ji}(z_m,1)|}{K_{ji}(z_m,1)} \le C2^{-m}e^{3|B|}.

If every block satisfies |B_{I_{ji}}(z_m)|\le m_{ji}/100, the last quantity is at most Ce^{-c m_{ji}} for a fixed c>0. The sum over i is O(e^{-c(k^{1/4}+j)}). By enlarging k_0, the product over blocks of the ratios T_{ji}(z_m)/K_{ji}(z_m,1) lies between 1/2 and 2. Since \prod_iK_{ji}(z_m,1)=(P_j^{\mathrm{eu}}(z_m))^{-1}, this proves (5.10) on the specified event. The number excluded, divided by X, is at most

C\sum_{j=0}^J\sum_{i\ge0}(k^{1/4}+j+i)^{-64} \ll (k^{1/4})^{-62}=k^{-31/2}\ll k^{-2},

by Lemma 5.2 and (5.6). The sum may be extended to all i because only nonempty blocks impose an event.

The real logarithm is available by positivity, and the same local expansion, including the finitely many small primes separately, gives for every prime set \mathcal I

\log\prod_{p\in\mathcal I}D_p(s,z_m)^{-1} =B_{\mathcal I}(z_m)+O\left(\sum_{p\in\mathcal I}p^{-1}\right). \tag{5.14}

For Y_j<p\le Y_0, (5.1) bounds this reciprocal mass by C(1+j), since \log Y_0/\log Y_j=4^j. For p\le Y_0 it is at most C(1+J): indeed \log\log Y_0\le\log\ell, and \log\ell<10(J+1)\log2. Require that the corresponding prime sums have absolute values at most (\log2)jk/16 and (\log2)Jk/16, respectively. Once k_0 dominates the fixed drift constants in (5.14), these requirements imply (5.11) and (5.12). Their total exceptional proportion is at most

C\sum_{j=1}^J\frac{(1+j)^{32}}{(jk)^{64}} +C\frac{(1+J)^{32}}{(Jk)^{64}} \ll k^{-64}.

Combining the exceptional sets proves the proposition.

5.3 Euler-product norms on the full model

The preceding proposition controls the multipliers on most integers. We now prove the model norms needed for arithmetic comparison, including the contribution of every event. We first estimate exact Euler products, and then replace each complete block by its degree truncation with a summable relative error.

To avoid any limiting interchange, fix for now a finite real cutoff Q\ge Y_0 and put

\mathcal L_Q(b)=\prod_{p\le Q}D_p(b,Z)^{-1},\qquad \Re b>0. \tag{5.15}

All bounds in this subsection are independent of Q. At fixed Q the product has the absolutely convergent expansion

\mathcal L_Q(b)= \sum_{\substack{n\ge1\\p\mid n\Rightarrow p\le Q}} \lambda(n)Z(n)n^{-1/2-b}. \tag{5.16}

Absolute convergence follows by multiplying the finitely many local geometric series; their absolute sums are bounded by \prod_{p\le Q}(1-p^{-1/2-\Re b})^{-2}.

Lemma 5.4 (Exact shifted products). Let 0<s,\alpha\le1, b=\alpha+it, and Y_j\ge2. If h=\alpha+s+|t| and a=\min(\alpha,s), then

\|(P_j^{\mathrm{eu}})^{-1}\mathcal L_Q(b)\|_2 \ll (1+h/a)^C \left(1+\frac1{\alpha\log Y_j}\right)^C. \tag{5.17}

At the real point b=s, with j=0 and the parameters of this section,

\|(P_0^{\mathrm{eu}})^{-1}\mathcal L_Q(s)-1\|_2^2 \ll \frac{e^{-2\sqrt k}}{\sqrt k}. \tag{5.18}

Proof. We first give the local cancellation with its dependence on b. Write r=p^{-1/2}, u=p^{-s}, v=p^{-b}, and M=\min(1,h\log p). The mean-value formula for the exponential and the trivial bound imply

|u-v|\ll M(u+|v|). \tag{5.19}

By (5.5), uniformly for every prime,

D_p(b,Z)^{-1}-1=O(r|v|).

Subtract the two inverse polynomials and use this last estimate to obtain

\frac{D_p(s,Z)}{D_p(b,Z)} =1+\lambda(p)Z(p)r(v-u) +O\big(r^2|v-u|(u+|v|)\big). \tag{5.20}

For odd p, the displayed linear term has expectation zero. Expanding the squared absolute value, and using M^2\le M and (u+|v|)^2\le2(u^2+|v|^2), therefore gives

\mathbb E\left|\frac{D_p(s,Z)}{D_p(b,Z)}\right|^2 \le \exp\left\{\frac Cp\min(1,h\log p) (p^{-2s}+p^{-2\alpha})\right\}. \tag{5.21}

The constants in the error in (5.20) are uniform even at the small primes, because (1-2^{-1/2})^2 is a common positive lower bound for the denominator. At the deterministic prime 2 the local ratio has a fixed upper bound by (5.5).

For odd primes outside the mollifier, the expansion

D_p(b,Z)^{-1}=1+\lambda(p)Z(p)p^{-1/2-b} +O(p^{-1-2\alpha})

and centering give

\mathbb E|D_p(b,Z)^{-1}|^2 \le \exp(Cp^{-1-2\alpha}). \tag{5.22}

Independence multiplies the local second moments exactly. Sum (5.21) by (5.3), using both a=s and a=\alpha there, and sum (5.22) by (5.2). Taking a square root proves (5.17).

For the distance estimate there is exact cancellation below Y_0. Set

U=(P_0^{\mathrm{eu}})^{-1}\mathcal L_Q(s) =\prod_{Y_0<p\le Q}D_p(s,Z)^{-1},\qquad \Xi=\sum_{p>Y_0}p^{-1-2s}.

This is a positive real random variable. The same expansion gives

\mathbb E D_p(s,Z)^{-1}=1+O(p^{-1-2s}),\qquad \mathbb E D_p(s,Z)^{-2}=1+O(p^{-1-2s}).

The first error may have either sign. Nevertheless, the elementary product bound |\prod(1+e_p)-1|\le\exp(\sum|e_p|)-1 and independence show that

\mathbb EU=1+O(\Xi),\qquad \mathbb EU^2=1+O(\Xi). \tag{5.23}

Indeed (5.2) and s\log Y_0=\sqrt k give

\Xi\ll\int_{2\sqrt k}^{\infty}e^{-v}\frac{dv}v \ll e^{-2\sqrt k}/\sqrt k,

so \Xi is uniformly small after choosing k_0. Finally,

\|U-1\|_2^2=\mathbb EU^2-2\mathbb EU+1\ll\Xi.

This uses both moment estimates in (5.23) and proves (5.18).

Lemma 5.5 (Relative truncation in mean square). For every b with \Re b>0, uniformly in Q\ge Y_0,

\|(H_j-(P_j^{\mathrm{eu}})^{-1})\mathcal L_Q(b)\|_2 \le \left(\exp\left(C\sum_i2^{-m_{ji}}\right)-1\right) \|(P_j^{\mathrm{eu}})^{-1}\mathcal L_Q(b)\|_2. \tag{5.24}

In particular the relative factor is O(2^{-k^{1/4}-j}).

Proof. For a block I=I_{ji} let \mathcal L_I(b)=\prod_{p\in I}D_p(b,Z)^{-1}. We claim there are fixed positive constants c_*,C_* such that

\|K_{ji}(Z,1)\mathcal L_I(b)\|_2\ge c_*,\qquad \sup_{|z|=2}\|K_{ji}(Z,z)\mathcal L_I(b)\|_2\le C_*. \tag{5.25}

For the first assertion, at a large odd prime the exact local ratio is

\frac{D_p(s,Z)}{D_p(b,Z)} =1+\lambda(p)Z(p)p^{-1/2}(p^{-b}-p^{-s})+O(p^{-1}).

The centered linear term shows that its local second moment is 1+O(p^{-1}); for all sufficiently large primes it is at least 1-C/p\ge1/2. Their product is bounded below by \exp(-2C\sum_{p\in I}1/p), which is a fixed positive constant by (5.6). At each of the finitely many smaller primes, including 2, (5.5) gives the pointwise lower bound

\left|\frac{D_p(s,Z)}{D_p(b,Z)}\right| \ge\frac{(1-p^{-1/2})^2}{(1+p^{-1/2})^2}>0.

Their finite product is also bounded below. This proves the first assertion of (5.25).

For the second, on |z|=2 the local quotient is

\frac{1-\lambda(p)Z(p)p^{-1/2-s}z +\xi_p Z(p)^2p^{-1-2s}z^2}{D_p(b,Z)} =1+\lambda(p)Z(p)p^{-1/2}(p^{-b}-zp^{-s})+O(p^{-1})

at large odd primes, uniformly in z and b. Its second moment is 1+O(p^{-1}), and therefore its product is bounded above, again by (5.6). At small primes use the direct numerator upper bound and (5.5). The numerator is permitted to vanish; only an upper bound has been used on this circle.

Apply Cauchy’s coefficient formula to the polynomial z\mapsto K_{ji}(Z,z)\mathcal L_I(b) with values in L^2. For m=m_{ji}, Minkowski’s inequality and (5.25) give

\|(T_{ji}(Z)-K_{ji}(Z,1))\mathcal L_I(b)\|_2 \le C_*\sum_{h>m}2^{-h}\le C_*2^{-m}.

Dividing by the positive lower bound in (5.25) makes this a relative error \varepsilon_i=C2^{-m_{ji}}.

To see explicitly how relative errors combine, put A_i=K_{ji}(Z,1)\mathcal L_I(b) and B_i=T_{ji}(Z)\mathcal L_I(b). Then \|B_i-A_i\|_2\le\varepsilon_i\|A_i\|_2 and \|B_i\|_2\le(1+\varepsilon_i)\|A_i\|_2. Variables belonging to distinct blocks and to the residual primes Y_j<p\le Q are independent. In the telescoping identity for \prod B_i-\prod A_i, the norm of each product of factors on distinct blocks is the product of their norms. Thus its relative norm, also including the independent residual product, is at most

\sum_i\varepsilon_i\prod_{h<i}(1+\varepsilon_h) =\prod_i(1+\varepsilon_i)-1 \le\exp\left(\sum_i\varepsilon_i\right)-1.

This proves (5.24), without a factor equal to the number of blocks. Finally \sum_i2^{-m_{ji}}\le2^{1-k^{1/4}-j}.

Proposition 5.6 (The shifted norms). There are fixed C,c_0>0 such that, uniformly for every real \theta and every cutoff Q\ge Y_0,

\begin{align*} \|H_0(Z)\mathcal L_Q(s/2+i\theta s)\|_2 &\ll(1+|\theta|)^C, \tag{5.26}\\ \|H_0(Z)\mathcal L_Q(s)-1\|_2 &\ll e^{-c_0 k^{1/4}}, \tag{5.27}\\ \|H_j(Z)\mathcal L_Q((1+i\theta)/\ell)\|_2 &\ll (1+|\theta|)^C(k2^j)^C \qquad(0\le j\le J). \tag{5.28}\end{align*}

Proof. In (5.17), first take \alpha=s/2, t=\theta s, and j=0. Then h/\min(\alpha,s)=3+2|\theta| and \alpha\log Y_0=\sqrt k/2. This proves (5.26) with the exact multiplier; use Lemma 5.5 to replace it by H_0. For (5.28), take \alpha=1/\ell and t=\theta/\ell. Since k\ge1,

h/\min(\alpha,s)=1+k+|\theta|, \qquad \alpha\log Y_j=\delta_j^2/\sqrt k.

The bound follows from (5.17) after increasing the fixed exponent C, and then from relative truncation. Finally, (5.18) bounds the distance from one for the exact multiplier and also bounds its norm. The triangle inequality and (5.24) give

\|H_0\mathcal L_Q(s)-1\|_2 \ll 2^{-k^{1/4}}+e^{-\sqrt k}k^{-1/4} \ll e^{-c_0k^{1/4}}.

5.4 Fourier representations and the first weight

We have obtained bounds for the mollified finite Euler products at the three shifts needed below. Fourier inversion now converts these bounds into estimates for the actual weights. For the first piece, the main term is A_x. Its estimate combines the power-to-exponential comparison with the cutoff tail and the exponentially small mollifier error.

We use the Fourier convention

\widehat g(\theta)=\int_{\mathbb R}g(y)e^{i\theta y}\,dy, \qquad g(y)=\frac1{2\pi}\int_{\mathbb R}\widehat g(\theta)e^{-i\theta y} \,d\theta.

The following elementary bound includes negative real arguments, which occur inside the gamma integral.

Lemma 5.7 (Global approximation of the truncated power). For each fixed nonnegative integer r, if k\ge2r+4, then for every z\in\mathbb R,

\left|\frac{d^r}{dz^r} \left((1-z/k)_+^k-e^{-z}\right)\right| \le\frac{C_r}{k}(1+|z|)^2e^{-z}. \tag{5.29}

Proof. For z<k the derivative of the power is

(-1)^r\frac{(k)_r}{k^r}(1-z/k)^{k-r},\qquad (k)_r=k(k-1)\cdots(k-r+1),

and it is zero for z\ge k. The formula is continuous through z=k in the derivative orders under consideration. For z<k, the logarithm of its ratio in absolute value to e^{-z} is

\log((k)_r/k^r)+z+(k-r)\log(1-z/k).

The last two terms have derivative (r-z)/(k-z), so their maximum over z<k is at z=r. It follows at once that the absolute ratio is at most e^r. For |z|\ge\sqrt k this bound and k^{-1}(1+|z|)^2\ge1 prove (5.29). For |z|<\sqrt k we have |z/k|\le1/2. Taylor’s formula for \log(1-z/k) and \log((k)_r/k^r)=O_r(k^{-1}) bound the displayed logarithm by

O_r\big(k^{-1}(1+|z|)^2\big).

This quantity is bounded in this range; applying |e^w-1|\le |w|e^{|w|} proves the result there too. All estimates hold for negative z as well as positive z.

Lemma 5.8 (Fourier error for the first piece). Define

A_x=(C_F|x|)^s\Gamma(1+s),\qquad E_x(y)=w_{0,x}(y/k)-A_xe^{-y}\quad(y\ge0).

For every required fixed integer r, there is an extension g_x of e^{y/2}E_x(y) from y\ge0 to \mathbb R such that

|\widehat g_x(\theta)|\ll_r k^{-1}(1+|\theta|)^{-r}. \tag{5.30}

The constants are uniform in x,k,X after choosing k_0 depending on r. The quantities A_x are bounded above and below by positive fixed constants.

Proof. Write q=C_F|x|, which lies in a fixed compact subinterval of (0,\infty). The exact weight definition gives

W_{k,x}(y/k)=\int_0^\infty e^{-v} \left(1-\frac{y-s\log(qv)}k\right)_+^k\,dv,

whereas

\int_0^\infty e^{-v}e^{-y+s\log(qv)}\,dv=A_xe^{-y}.

For every fixed M, the logarithmic moments

\int_0^\infty e^{-v}(qv)^s (1+|s\log(qv)|)^M\,dv\le C_M \tag{5.31}

are uniform for 0<s\le1: on 0<v\le1, bound v^s\le1 and s|\log v|\le|\log v|; on v\ge1, use v^s\le v and the exponential decay. Lemma 5.7 and differentiation under this dominated integral now imply, for 0\le h\le r and y\ge-2,

\left|\frac{d^h}{dy^h} \left(W_{k,x}(y/k)-A_xe^{-y}\right)\right| \ll_r k^{-1}(1+y^2)e^{-y}. \tag{5.32}

In particular the proof uses (5.29) when y-s\log(qv) is negative and arbitrarily large in absolute value.

The cutoff F_0(y/k) is one for y\le k/2, zero for y\ge3k/4, and its hth derivative in y is O_h(k^{-h}). Write

E_x(y)=F_0(y/k)\big(W_{k,x}(y/k)-A_xe^{-y}\big) +(F_0(y/k)-1)A_xe^{-y}

also for y\ge-2. By (5.32), after multiplication by e^{y/2} the first term and its first r derivatives have L^1([-2,\infty)) norm O_r(k^{-1}). The second term is supported in y\ge k/2 and has these norms O_r(e^{-k/4}). Choose a fixed smooth function \rho equal to zero for y\le-2 and one for y\ge-1, and extend by

g_x(y)=\rho(y)e^{y/2}E_x(y),

with zero value to the left of -2. All derivatives through order r have L^1(\mathbb R) norm O_r(k^{-1}). Integration by parts r times and the bound without integration by parts give (5.30). Lastly, continuity and positivity of q^s\Gamma(1+s) on the compact parameter set q\in[q_-,q_+], 0\le s\le1, give the two bounds for A_x.

Proposition 5.9 (Independent-model estimates for the weight pieces). With the weights and sums S_{j,Z}(x) defined in Section 4, there is a fixed exponent C_5 such that

\begin{align*} \|H_0(Z)S_{0,Z}(x)-A_x\|_2&\ll k^{-1}, \tag{5.33}\\ \|H_j(Z)S_{j,Z}(x)\|_2&\ll(k2^j)^{C_5}\delta_j^k \qquad(1\le j\le J). \tag{5.34}\end{align*}

These bounds are uniform in x\in\mathcal X and over the entire range k_0\le k\le\ell^{3/5}, with one fixed k_0 and one sufficiently large X threshold.

Proof. Choose a finite cutoff Q exceeding Y_0 and the lengths of all the short polynomials S_{j,Z}, 0\le j\le J. This is the only requirement on Q; Proposition 5.6 is uniform in its choice. For j\ge1, set g_{j,x}(u)=e^u w_{j,x}(u). The support is contained in [1-\delta_j,1-\delta_j/4]\subset[1/2,1]. The fixed-order derivative bounds in Lemma 4.2 and integration by parts give, for each required fixed r,

|\widehat g_{j,x}(\theta)| \ll_r (k/\delta_j)^{C_r}\delta_j^k(1+|\theta|)^{-r}. \tag{5.35}

Fourier inversion and (5.16) give the exact identity

S_{j,Z}(x)=\frac1{2\pi}\int_{\mathbb R} \widehat g_{j,x}(\theta) \mathcal L_Q((1+i\theta)/\ell)\,d\theta. \tag{5.36}

Indeed every nonzero weight coefficient has index below the chosen cutoff and hence occurs in (5.16); all other indices contribute zero after inversion. At this fixed finite Q, absolute convergence of the Dirichlet expansion and the integrable kernel justify interchanging the sum and integral. Multiply by H_j and use Minkowski’s inequality, (5.28), and (5.35), taking r>C+2. Their integral is O((k/\delta_j)^{C_r}(k2^j)^C\delta_j^k), which proves (5.34) after fixing C_5.

For the first piece, Lemma 5.8 and the same finite-product expansion give

S_{0,Z}(x)-A_x\mathcal L_Q(s) =\frac1{2\pi}\int_{\mathbb R}\widehat g_x(\theta) \mathcal L_Q(s/2+i\theta s)\,d\theta. \tag{5.37}

To check the scaling, at an integer index n put y=k\log n/\ell=s\log n\ge0. Fourier inversion for g_x then reads

w_{0,x}(\log n/\ell)-A_x n^{-s} =\frac1{2\pi}\int\widehat g_x(\theta) n^{-s/2-i\theta s}\,d\theta,

which is exactly the coefficient identity needed in (5.37). Use (5.26) and (5.30) with r>C+2 to bound the norm of (5.37) after multiplication by H_0 by O(k^{-1}). By (5.27),

\|H_0S_{0,Z}-A_x\|_2 \le \|H_0(S_{0,Z}-A_x\mathcal L_Q(s))\|_2 +A_x\|H_0\mathcal L_Q(s)-1\|_2 \ll k^{-1}+e^{-c_0k^{1/4}}\ll k^{-1}.

This proves (5.33).

All smoothness orders used here are fixed after the absolute exponent in Proposition 5.6, and before choosing k_0. The derivative estimates for the weights, the inequality s\le\ell^{-2/5}, and the lower bound \delta_J\ge\ell^{-1/10} then give a single X threshold for the whole parameter range. We have not used the event of Proposition 5.3 anywhere in these model norm arguments. Nor is a passage to an infinite Euler cutoff required: the coefficient identities hold for every sufficiently large finite Q, and all norm estimates are uniform in that cutoff.

6 Nonvanishing and the rank-weighted tail

We now combine the transferred model estimates, the integer product event, and the terminal mean square to count large orders of vanishing. A separate bound for each individual rank then converts this count into the rank-weighted tail. The companion density theorem enters only in the final subsection, after the tail theorem is proved. The constants and the fixed lower threshold k_0 are increased finitely many times in this section. All choices depend only on the fixed family and the already fixed smoothness orders.

6.1 Counting large orders of vanishing

Proposition 6.1. There are k_0, X_0, and C, depending on E, such that for every F\in\mathcal F, every dyadic X\ge X_0, and every integer

k_0+1\le k\le(\log X)^{3/5},

one has

\#\{d\in\mathcal A(X):a(F^{(d)})>k\}\le C Xk^{-2}.

Proof. Write \ell=\log X, and first consider the functional-equation sign (-1)^k, with k_0\le k\le\ell^{3/5}. Fix c=\pm1, and use the weights and partition of Section 4. We write P_j^{\rm eu} for the positive Euler products of Section 5.

Corollary 4.3 and Lemma 5.1 permit Proposition 3.7 to be applied to H_jS_j, for 0\le j\le J, with \Delta=\delta_j/4. By the first assertion of Proposition 5.9, outside O(X/k^2) integers in X\le|m|<2X,

|H_0(z_m)S_{0,z_m}(m/X)-A_{m/X}|<\frac12 A_{m/X}. \tag{6.1}

Indeed A_x=(C_F|x|)^s\Gamma(1+s) is bounded above and below by positive constants on the fixed x-range, uniformly for s=k/\ell\le\ell^{-2/5}. Chebyshev’s inequality applies to the transferred O(k^{-2}) mean-square error. The exponentially small comparison error is absorbed uniformly.

For 1\le j\le J, the second model estimate gives

\frac1X\sum_m\Psi(m/X)|H_j(z_m)S_{j,z_m}(m/X)|^2 \ll (k2^j)^{2C_5}2^{-2jk}+e^{-c\delta_j\ell} \ll 2^{-3jk/2}.

The last inequality follows first by increasing fixed k_0 to absorb the polynomial factor. For the comparison error, use

\delta_j\ell\ge\ell^{9/10},\qquad jk\ll\ell^{3/5}\log\ell,

and then increase one X_0 for all the permitted k,j. The terminal estimate of Lemma 4.5 gives

\frac1X\sum_{d\in\mathcal A(X)} |S_{*,\chi_d}(d/X)|^2\ll 2^{-3Jk/2}.

Chebyshev and summation of the resulting geometric probabilities imply, outside O(X/k^2) further admissible parameters,

|H_j(\chi_d)S_{j,\chi_d}(d/X)|\le2^{-jk/2}\quad(1\le j\le J), \qquad |S_{*,\chi_d}(d/X)|\le2^{-Jk/2}. \tag{6.2}

Here \sum_{j\ge1}2^{-jk/2}\ll k^{-2} after fixing k_0, and J\ge1 for sufficiently large X.

Intersect these events with the event in Proposition 5.3. Its additional exceptional set is also O(X/k^2). On the intersection,

\frac12\le H_jP_j^{\rm eu}\le2,\qquad P_j^{\rm eu}\le 2^{jk/8}P_0^{\rm eu},\qquad 1\le 2^{Jk/8}P_0^{\rm eu}.

Choose a fixed a_*>0 with A_x\ge a_* for all the parameters. Equation (6.1) yields

|S_{0,\chi_d}(d/X)|\ge\frac{a_*}{4}P_0^{\rm eu}.

Equation (6.2) yields

\sum_{j=1}^J|S_{j,\chi_d}(d/X)|+|S_{*,\chi_d}(d/X)| \le P_0^{\rm eu} \left(2\sum_{j=1}^J2^{-3jk/8}+2^{-3Jk/8}\right).

For a sufficiently large fixed k_0, the last parenthesis is less than a_*/4. The entire weighted sum is therefore nonzero. Lemma 4.1 excludes the simultaneous conditions a(F^{(d)})>k and \epsilon_{F^{(d)}}=(-1)^k. Including both values of c, we have proved

\#\{d\in\mathcal A(X): a(F^{(d)})>k,\ \epsilon_{F^{(d)}}=(-1)^k\} \ll Xk^{-2}. \tag{6.3}

For the other functional-equation sign, apply (6.3) at k-1. A rank exceeding k also exceeds k-1, and (k-1)^{-2}\ll k^{-2}. This proves the proposition.

6.2 A uniform bound for an individual rank

Lemma 6.2. Uniformly for F\in\mathcal F and d\in\mathcal A(X),

a(F^{(d)})\ll_E\log(3X).

Proof. Put L=L_{F^{(d)}} and C_d=C_F|d|. On \Re s=5, absolute convergence and (2.2) give a uniform bound. On \Re s=-1, the functional equation is

L(s)=\epsilon_{F^{(d)}} C_d^{\,1-2s} \frac{\Gamma(3/2-s)}{\Gamma(1/2+s)}L(1-s).

At s=-1+it, the modulus of the gamma quotient equals

|(-1/2+it)(1/2+it)(3/2+it)|.

Since L(2-it) is uniformly bounded,

|L(-1+it)|\ll_E X^3(1+|t|)^3.

Apply the strip principle to L(s)/(s+2)^4 on -1\le\Re s\le5. To see that the possibly conductor-dependent finite-order growth in the strip introduces no new constant, first multiply by

\exp\!\left(-\varepsilon \cos\frac{\pi(s-2)}{12}\right),\qquad \varepsilon>0.

Its modulus is at most one on this strip and decays faster than any finite-order growth as |\Im s|\to\infty. The maximum principle on expanding rectangles gives the bound from the two vertical sides. Letting \varepsilon decrease to zero shows that L(s)/(s+2)^4\ll_E X^3 throughout the strip. In particular, the maximum of |L| on the closed disk |s-2|\le5/2 is O_E(X^3).

At the center, the Euler factors and their parameter bounds give

|L(2)|\ge \prod_p(1+p^{-2})^{-2} =\left(\frac{\zeta(4)}{\zeta(2)}\right)^2>0.

Jensen’s formula, with inner radius 2 and outer radius 5/2, therefore bounds the number of zeros in the inner disk, counted with multiplicity, by O_E(\log(3X)). The point 1/2 lies in that inner disk. This proves the result.

6.3 Summing the integer tails

Proof of Theorem 1.2. We first work in \mathcal A(X) for a fixed F\in\mathcal F. Let

T_{F,X}(k)=\#\{d\in\mathcal A(X):a(F^{(d)})>k\}, \qquad K=\lfloor(\log X)^{3/5}\rfloor.

For an integer R\ge k_0+1 and X large enough that K>R, the elementary integer-tail bound gives

\begin{align*} \sum_{\substack{d\in\mathcal A(X)\\a(F^{(d)})>R}}a(F^{(d)}) &\le R T_{F,X}(R) +\sum_{k=R}^{K-1}T_{F,X}(k) +C_E\log X\,T_{F,X}(K) \\ &\ll_E \frac X R+X(\log X)^{-1/5}. \tag{6.4}\end{align*}

For ranks between R+1 and K, the first two terms count the rank exactly. For ranks exceeding K, the last term bounds the remaining mass by Lemma 6.2. Proposition 6.1 supplies every counting estimate used here. In particular the last term is O_E(X\log X/K^2)=O_E(X(\log X)^{-1/5}). The constant in (6.4) is independent of R.

For completeness, fix R and cover 0<|d|\le Y by dyadic blocks. Enlarge the last partial block to a full block, using nonnegativity. The sum of their left endpoints is less than 2Y. The finitely many blocks below the threshold for (6.4) contribute a finite number B_{E,R}. For the error term in the remaining blocks, split at X=\sqrt Y. The smaller blocks contribute O_E(\sqrt Y), and in the larger ones \log X\ge\frac12\log Y. Consequently

\sum_{\substack{d\ {\rm admissible}\\0<|d|\le Y\\a(F^{(d)})>R}} a(F^{(d)}) \le B_{E,R}+\frac{C_EY}{R} +O_E\bigl(\sqrt Y+Y(\log Y)^{-1/5}\bigr).

After division by Y and passage to the limsup, the desired C_E/R bound holds for each F\in\mathcal F. Lemma 2.1, its bounded multiplicity, and the finite maximum of these constants prove the same bound for every original signed squarefree parameter of E.

6.4 The mean

Proof of Theorem 1.1. Write N(Y)=\#\mathcal D(Y) and let N_j(Y) count the parameters of analytic rank j. The elementary squarefree sieve gives

N(Y)=2\sum_{n\le Y}\mu(n)^2 =\frac{2Y}{\zeta(2)}+O(\sqrt Y).

Indeed, expand \mu(n)^2=\sum_{r^2\mid n}\mu(r), interchange the finite sums, and bound the omitted tail of \sum_r\mu(r)/r^2=1/\zeta(2).

By the analytic density theorem (1.1), N_0(Y)/N(Y)\to1/2 and N_1(Y)/N(Y)\to1/2. Thus N(Y)-N_0(Y)-N_1(Y)=o(Y). For every fixed integer R\ge R_E,

\sum_{\substack{d\in\mathcal D(Y)\\2\le a(E^{(d)})\le R}} a(E^{(d)}) \le R\bigl(N(Y)-N_0(Y)-N_1(Y)\bigr)=o_{E,R}(Y).

Theorem 1.2 now implies

\limsup_{Y\to\infty}\frac1Y \sum_{\substack{d\in\mathcal D(Y)\\a(E^{(d)})\ge2}}a(E^{(d)}) \le\frac{C_E}{R}.

Let R\to\infty. The left side is zero by nonnegativity. The total rank sum is consequently N_1(Y)+o_E(Y). Dividing by N(Y) proves the limit 1/2.

7 Algebraic-rank moments

We now prove Corollary 1.3. The inputs are the companion density and rank-equality theorem and the exponential-moment estimate of Koymans and Smith. The latter bounds the contribution of the density-zero exceptional set for every fixed exponential parameter or moment order; the analytic tail theorem is not needed.

Proof of Corollary 1.3. Put N(Y)=\#\mathcal D(Y), r_d=r(E^{(d)}), and let N_j^{\mathrm{alg}}(Y) count the parameters with r_d=j. The rank-equality conclusion of the companion density theorem [12, Theorem 1.2], together with its analytic rank-zero and rank-one densities, gives

\frac{N_j^{\mathrm{alg}}(Y)}{N(Y)}\longrightarrow\frac12 \qquad(j=0,1).

Indeed, analytic and algebraic ranks agree outside a density-zero set, so their rank-j counts differ by o(N(Y)). Consequently

\mathcal B(Y)=\{d\in\mathcal D(Y):r_d\ge2\} \quad\text{satisfies}\quad \#\mathcal B(Y)=o(N(Y)).

For the next bound, E^{(v)} for any nonzero integer v denotes the twist determined by its squareclass, so the integer sum may repeat squareclasses. Theorem 1.4 of Koymans and Smith [9], specialized to F=\Q, A=E, one variable, and P(u)=u, gives a constant C_E>0 such that for every fixed \kappa>0,

\frac1{2Y}\sum_{\substack{v\in\Z\\0<|v|\le Y}} \exp\!\bigl(\kappa\,\operatorname{rank}_{\Z}E^{(v)}(\Q)\bigr) \le \exp\!\bigl(\exp(C_E\kappa)\bigr)

for all sufficiently large Y, with the threshold allowed to depend on \kappa. Their integer box already includes both signs, and P(v)\ne0 excludes exactly v=0. Restricting this nonnegative sum to \mathcal D(Y), and using N(Y)\sim2Y/\zeta(2), gives for each fixed \kappa>0

\limsup_{Y\to\infty}\frac1{N(Y)} \sum_{d\in\mathcal D(Y)}e^{\kappa r_d} \le \zeta(2)\exp\!\bigl(\exp(C_E\kappa)\bigr)<\infty. \tag{7.1}

For fixed t>0, Cauchy–Schwarz and (7.1) at \kappa=2t give

\frac1{N(Y)}\sum_{d\in\mathcal B(Y)}e^{t r_d} \le \left(\frac{\#\mathcal B(Y)}{N(Y)}\right)^{1/2} \left(\frac1{N(Y)} \sum_{d\in\mathcal D(Y)}e^{2t r_d}\right)^{1/2} \longrightarrow0.

For fixed t<0, the same exceptional average is at most \#\mathcal B(Y)/N(Y), since r_d\ge0; for t=0 the full average is identically one. The contributions from ranks zero and one are N_0^{\mathrm{alg}}(Y)/N(Y) and e^tN_1^{\mathrm{alg}}(Y)/N(Y), proving the exponential limit.

Finally, for each fixed positive integer m, one has x^{2m}\ll_m e^x for x\ge0. A second Cauchy–Schwarz application and (7.1) at \kappa=1 therefore give

\frac1{N(Y)}\sum_{d\in\mathcal B(Y)}r_d^m \le \left(\frac{\#\mathcal B(Y)}{N(Y)}\right)^{1/2} \left(\frac1{N(Y)}\sum_{d\in\mathcal D(Y)}r_d^{2m}\right)^{1/2} \longrightarrow0.

The rank-zero contribution is zero and the rank-one contribution is N_1^{\mathrm{alg}}(Y)/N(Y), proving the power-moment limit without differentiating a limiting exponential-moment formula.

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