This paper studies the analytic continuation of a divisor function series constrained by a linear equation, revealing its meromorphic structure and applying it to count rational points on a specific algebraic variety.
Contribution
It extends the understanding of divisor function series by providing their meromorphic continuation and applies this to count solutions on a bihomogeneous variety.
Findings
01
Series converges for Re(s)>1-1/k
02
Meromorphic continuation to Re(s)>1-2/(k+1) with specific poles
03
Asymptotic formula with power saving error for rational points on the variety
Abstract
Motivated by arithmetic applications on the number of points in a bihomogeneous variety and on moments of Dirichlet L-functions, we provide analytic continuation for the series Aaā(s):=ān1ā,ā¦,nkāā„1ā(n1āāÆnkā)sd(n1ā)āÆd(nkā)ā with the sum restricted to solutions of a non-trivial linear equation a1ān1ā+āÆ+akānkā=0. The series Aaā(s) converges absolutely for ā(s)>1āk1ā and we show it can be meromorphically continued to ā(s)>1āk+12ā with poles at s=1ākāj1ā only, for 1ā¤j<(kā1)/2. As an application, we obtain an asymptotic formula with power saving error term for the number of points in the variety a1āx1āy1ā+āÆ+akāxkāykā=0 in Pkā1(Q)ĆPkā1(Q).
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Taxonomy
TopicsAnalytic Number Theory Research Ā· Algebraic Geometry and Number Theory Ā· Coding theory and cryptography
Full text
Linear correlations of the divisor function
Sandro Bettin
Abstract
Motivated by arithmetic applications on the number of points in a bihomogeneous variety and on moments of Dirichlet L-functions, we provide analytic continuation for the series Aaā(s):=ān1ā,ā¦,nkāā„1ā(n1āāÆnkā)sd(n1ā)āÆd(nkā)ā with the sum restricted to solutions of a non-trivial linear equation a1ān1ā+āÆ+akānkā=0. The series Aaā(s) converges absolutely for ā(s)>1āk1ā and we show it can be meromorphically continued to ā(s)>1āk+12ā with poles at s=1ākāj1ā only, for 1ā¤j<(kā1)/2.
As an application, we obtain an asymptotic formula with power saving error term for the number of points in the variety a1āx1āy1ā+āÆ+akāxkāykā=0 in Pkā1(Q)ĆPkā1(Q).
1 Introduction
Motivated by some applications which we shall describe below, we consider the Dirichlet series Aaā(s) obtained by adding a linear constraints among the variables of summation when expanding (ζ(s)2)k into a product of k Dirichlet series. More precisely, for kāNā„2ā, a=(a1āā¦,akā)āZī =0kā, and ā(s)>1āk1ā we define Aaā(s) to be
[TABLE]
where d(n) is the number of divisors of n and where haā(n) is defined implicitly by the second identity. Notice we can assume that a1ā,ā¦,akā donāt all have the same sign, since otherwise Aaā(s)=0.
The function Aaā(s) can be regarded as a degree 2 analogue of
[TABLE]
This function is a particular case of the Shintani zeta-function, which was investigated in a series of works by Shintani (see, e.g.Ā [Shi76, Shi78]). In particular, he showed that Saā(s) admits a meromorphic continuation to C and studied its special values displaying a connection with the values at s=1 of Hecke L-function of totally real fields.
The value at s=1 of the function Aaā(s) also has an arithmetic interpretation. Indeed, inĀ [Bet15] it was shown that Aaā(1) appears as the leading constant for the moments of a ācotangent sumā related to the Nyman-Beurling criterion for the Riemann hypothesis. More specifically, it was shown that as qāā
[TABLE]
where c0ā(h/q):=āām=1qāqmācot(qĻmhā). We defer toĀ [Bag, BC13a, BC13b] for more details on c0ā and on its relation with the Nyman-Beurling criterion. Also, we remark that the asymptotic for the moments of c0ā(h/q) was previously computed inĀ [MR16a] with a different expression for the leading constant.
In this paper we are interested in the analytic continuation of Aaā(s).
For k=2 it is very easy to analytically continue Aaā(s) to a meromorphic function on C. Indeed, for a1ā,a2āāN one has has
[TABLE]
by Ramanujanās identity, where Ī·a1ā,a2āā(s) is a certain arithmetic factor which is meromorphic in C with poles all located on the line ā(s)=0.
In the case kā„3 the coefficients haā(n) inĀ (1.1) are no longer multiplicative and the problem of providing meromorphic continuation for Aaā(s) becomes significantly harder, but we are still able to enlarge the domain of holomorphicity of Aaā(s) to ā(s)>1āk+12ā.
Theorem 1**.**
Let kā„3, a=(a1āā¦,akā)āZī =0kā with a1ā,ā¦,akā not all with the same sign. Then, Aaā(s) admits meromorphic continuation to ā(s)>1āk+12ā.
More precisely, there exist cm,jā(a)āR for 2k+2āā¤mā¤k, 1ā¤jā¤m+1 such that
[TABLE]
is holomorphic on ā(s)>1āk+12ā. Moreover, there exists an absolute constant A>0 such that for ā(s)>1āk+12āεā one has \mathcal{F}_{\boldsymbol{a}}(s)\ll_{\varepsilon}\mathopen{}\mathclose{{}\left((\frac{k}{\varepsilon}\max_{m=1}^{k}|a_{m}|)^{A}(1+|s|)^{7}}\right)^{Ak^{2}(1-1/k-\sigma)+k\varepsilon}, where the implicit constant depends on ε only.
Notice that TheoremĀ 1 is uniform in k,a and s. We remark that the uniformity in k of some bounds for Aaā(s) at s=1 was crucial in the worksĀ [Bet15] andĀ [MR16b] and, in general, it is also needed for our applicationĀ [Bet].
The value of the arithmetic factors cm,jā(a) can be computed explicitly starting from equationĀ (3.2) below. In particular, for m=k, j=k+1 one has
[TABLE]
where r is the number of aiā which are positive and Ļ(a) is as defined inĀ (3.5); in particular if GCD(a1ā,ā¦,akā)=1 then 1āŖĻ(a)āŖĪµāā£a1āāÆakāā£Īµ. Also, for 1ā¤jā¤k one has that ck,jā(a) can be written in terms of an arithmetic factor of shape similar to Ļ(a) times an expression depending on Eulerās constant γ, the derivatives of ζ(sā1) and ζ(s) computed at k, and the derivatives of the Ī-function computed at k1ā, krā and 1ākrā (cf. equationĀ (LABEL:dacc2)). To give an explicit numerical example for k=3, a=(ā1,1,1), we have
[TABLE]
An interesting question left open by TheoremĀ 1 is whether Aaā(s) extends meromorphically further to the left, perhaps to a meromorphic function on C with poles at s=1ām1ā for all 1ā¤mā¤k, or whether it has a natural boundary. As an approach to this problem one could try to input a recursive argument into the proof of TheoremĀ 1.
We notice however that the expression for the coefficients cm,jā arising in the proof of TheoremĀ 1 does not visibly extend to a meaningful formula in the case mā¤21ā(4k+1ā+1) for k>3 (m=1 if k=3), thus suggesting these coefficients might change form at some point or perhaps casting doubts on the possibility of a meromorphic continuation of Aaā(s) to C. Finally we mention that numerical computations in the case k=3 suggest there is a pole also at the subsequent expected location s=21ā (i.e. a term of order P(logX)X23ā inĀ (1.4) below), however the computations do not clarify whether the corresponding coefficients have the same shape of the previous coefficients or not.
Our first application of TheoremĀ 1 is given in the following Corollary.
Corollary 1**.**
Let kā„3 and aāZī =0kā. Let Φ(x) be a smooth function with support in [ā1,1] and such that Ļ(j)(x)āŖjBj for some B>0 and all xāR. Then, for 2k+1ā<iā¤k there exist polynomials Pa,iā(x)āR[x] of degree i such that for all Xā„1
[TABLE]
for some absolute constant A>0.
To give two examples, in the cases k=3 and k=4 (with a1ā=ā1) CorollaryĀ 1 gives
[TABLE]
for any a,b,cāN and where Q3,a,bā(x),R3,a,b,cā(x) and R4,a,b,cā(x) are polynomials of degree 3,3 and 4 respectively and A is an absolute constant.
We remark that one could use an easier argument to give the leading term in the asymptotic for the left hand side ofĀ (LABEL:mtmcce). In fact the main difficulty of CorollaryĀ 1 lies in unravelling the complicated combinatorics required to obtain the full main term Pa,iā(logX)Xkā1. This difficulties are implicitly treated in TheoremĀ 1, which allows us to go even further than the full main term. Indeed, for kā„4 we are able to identify also some new terms whose order is a power smaller than the main term (cf.Ā (1.5)). This is an example of an arithmetic stratification, where one has other āmain termsā, coming from sub-varieties, of order (typically) different from the main term one expects from the variety under consideration. This phenomenon was discussed by Manin and TschinkelĀ [MT] and explored in the context of the circle method by Vaughan and Wooley in the Appendix ofĀ [VW]. Recently, the arithmetic stratification was also indicated by Wooley as a potential source for the various terms in the Conrey-Keating analyisĀ [CK] of the asymptotic for moments of the Riemann zeta-function. In our case, the lower order contribution could be explained as coming from affine sub-varieties, that is solutions of n1ām1ā+āÆ+nkāmkā=0 which also satisfy one or more other equations r1ān1ām1ā+āÆ+rkānkāmkā=r0ā for some āsmallā r0ā,ā¦,rkāāZ.
A result similar toĀ (1.4), with the significant difference in the different way of counting, was obtained by BrowningĀ [Bro]. He computed the asymptotic with power-saving error term for
[TABLE]
where L1ā,L2ā,L3āāZ[x1ā,x2ā] are linearly independent linear forms. He also consideredĀ (1.6) when the sums are unbalanced, i.e. where the sum is restricted to n1āā¤N1ā, n2āā¤N2ā with N2ā smaller than N1ā. He was able to prove the asymptotic as long as N13/4+εāā¤N2āā¤N1ā (for L1ā(n1ā,n2ā)=n1āān2ā, L1ā(n1ā,n2ā)=n1ā, L3ā(n1ā,n2ā)=n1ā+n2ā), a range that was recently enlarged by BlomerĀ [Blo] who was able to consider the case N11/3+εāā¤N2āā¤N1ā (with a smooth cut-off for n2ā). In a different direction, we also cite the work of Browning and de la BretĆØcheĀ [dlBB], who considered the case k=3 with a quadratic relation among the variables.
For larger values of k, we cite the important work of MatthiesenĀ [Mat] who considered a variation ofĀ (LABEL:mtmcce) as well as the more general case when one has more than one linear constraint. Her work differs from ours in that in her case the variables vary inside a convex set, whereas in our case the variables are essentially summed over the hyperbolic region. Also, her method is based on the Green-Tao transference principleĀ [GT] which can only give the leading term cXkā1(logX)k in the asymptotic formula.
In particular we notice that neither the work of Matthiesen nor those of Browning and Blomer were able to produce terms of order a lower power of X.
Before introducing our second application, we first mention that we shall actually prove a more general version of TheoremĀ 1 where shifts are introduced, i.e. where instead of each divisor function d(n) we have Ļαiā,βiāā(n):=āab=nāaāαiābāβiā with αiā,βiāāC. We defer to TheoremĀ 3 in SectionĀ 2 for the complete statement. The shifts make our result extremely flexible. In particular one can use it to count integer solutions (x1ā,ā¦,xkā,y1ā,ā¦,ykā) in the flag variety
[TABLE]
when ordered according to various possible choices of height. To give a specific example we take the anticanonical height (maxiāā£xiāā£ā maxjāā£yjāā£)kā1, verifying Maninās conjecture in this particular case.
Theorem 2**.**
Let kāNā„3ā. For xāPkā1(Q), let (x1ā,ā¦,xkā) be a representative of x such that x1ā,ā¦,xkāāZ and (x1ā,ā¦,xkā)=1. Let H:Pkā1(Q)āR>0ā be defined by H(x):=(max1ā¤iā¤kāā£xiāā£)kā1 and let a=(a1ā,ā¦,akā)āZī =0kā. Then,
[TABLE]
for some explicitly computable f(a)āR, and
[TABLE]
where ĻXā is the characteristic function of the set X.
We remark that we made no effort to optimize the power saving Ī“kā which could be easily improved by refining our method (in particular focusing more on the shift dependency in TheoremĀ 3).
The varietyĀ (1.7) has already been considered in several papers. In particular, we mention the works of RobbianiĀ [Rob] (for kā„3), SpencerĀ [Spe], BrowningĀ [Bro] (for k=2), and Blomer and BrüdernĀ [BBa] (for more general multihomogeneous diagonal equations) and, previously, by Franke, Manin and TschinzelĀ [FMT] and ThunderĀ [Thu] (with height function ā„xā„kā1ā„yā„kā1)111Here ā„ā ā„ is the Euclidean norm and x=(x1ā,ā¦,xkā), y=(y1ā,ā¦,ykā) in the more general setting of Fano varieties. Among all these works, the only ones where the full main term, with error term O(B1āĪ“), is obtained areĀ [FMT] (see the Corollary after Theorem 5) andĀ [BBa] (inĀ [BBb] the explicit value Ī“=81ā was obtained for k=3). TheoremĀ 2 thus gives an alternative proof of this result as well as providing an explicit power saving for all k. Also, another novelty in our approach is that it shows that also complex analytic methods can be used to tackle these problems.
We notice that TheoremĀ 2 appears very similar to CorollaryĀ 1, which essentially counts points inĀ (1.7) ordering them according to the size of the product of all the variables, ā£x1āāÆxkāā y1āāÆykāā£.222One could easily modify our argument to count points with respect to maxiāā£xiāyiāā£, since our proof starts by introducing partitions of unity which localize each xiāyiā. The different way of counting however changes the problem significantly and the deduction of TheoremĀ 2 from (the generalization of) TheoremĀ 1 is much subtler. In particular, the computation of the full main term for N(B) requires a careful analysis of some complex integrals resulting from integrating over the shifts in TheoremĀ 3. Notice that also in this case the problem becomes much easier if one only computes the leading term in the asymptotic for N(B).
A third application of TheoremĀ 1 comes from the theory of the moments of L-functions. InĀ [Bet] it is considered the moment
[TABLE]
where āā² indicates that the sum is over primitive characters Ļ1ā,ā¦,Ļkā1ā modulo q and L(s,Ļ) is the Dirichlet L-function associated to the character Ļ. It turns out that the ādiagonal termā in Mkā(q) has the shape āϵā{±1}kācϵāā«(2)āAϵā(s)qksH(s)ds for a meromorphic function H(s) and some cϵāāR. Thanks toĀ TheoremĀ 1 we are able to evaluate the diagonal term and thus, evaluating also the off-diagonal term using a similar method, we are able to obtain the following asymptotic formula for Mkā(q) when kā„3 (the case k=2 corresponds to the 4-th moment of Dirichlet L-function and was computed by YoungĀ [You])
[TABLE]
where Ļ(n) is Eulerās Ļ function, ν(n) is the number of different prime factors of n and Ī“kā>0. We also mention that, thanks to the workĀ [Bet16],Ā (1.9) can be interpreted also as the moment of some functions involving continued fractions.
The proof of TheoremĀ 1 is quite simple in spirit but it has to face a number of technical challenges, mainly coming from the identification of the polar structure (equivalently, of the main terms inĀ (LABEL:mtmcce)). Before giving a brief outline of our proof, we mention that one could have chosen to proceed also in different ways, for example using the circle method. The main difficulty however comes from the evaluation of the polar structure and this is not visibly simplified by choosing such different routes. We also remark that the our technique would allow to give analytic continuation also when the constraint is a non-homogeneous linear equation. The only difference with our case is that in LemmaĀ 9 below we would need to use the Deshouillers and IwaniecĀ [DI] bound for sums of Kloosterman sums (cf.Ā [Bet] where this is done for a similar problem). However, for simplicity we content ourself with dealing with the homogenous case only.
We conclude with a rough sketch of the proof of TheoremĀ 1 referring for simplicity to CorollaryĀ 1 which is essentially equivalent to it.
First, we split the sum on the right hand side ofĀ (LABEL:mtmcce) introducing partitions of unity to control the size of the niā. When one variable is much larger than the others a simple bound suffices, so we are left with considering the case when the variables have about the same size. In this case we eliminate the larger variable using the linear equation and we separate the remaining variables arithmetically and analytically using, respectively, a slightly modified version of Ramanujanās formula,
[TABLE]
where cāā(m) is the Ramanujan sum and Ļαā(n):=ādā£nādα and a generalized version of the Mellin formula for (1±x)ās as given inĀ [Bet]. We end up with a formula of the shape (for a=(1,ā¦,1))
[TABLE]
for some smooth function f. Applying Voronoiās summation formula to each variable n1ā,ā¦,nkā transform each sum over niā in a main term Miā plus a sum of similar shape but with h replaced by h and thus we obtain
[TABLE]
for some smooth functions fiā. We then treat as main terms the terms where we pick up more Miā than series, and treat the other terms as error terms which we estimate essentially trivially. We then treat and assembly the main terms (which correspond to the poles of Aaā(s)), an operation which constitutes the main difficulty of the paper as we have to deal with several integral transforms in order to take them to their final form (actually, we choose the equivalent root of moving the lines of integration of several complex integrals, collecting the contribution of the residues of some poles). Combining the two cases for the range of the variables one then deduces CorollaryĀ 1.
We notice that the above structure of the proof of TheoremĀ 1 is at first glance very similar to that of the asymptotic for Mkā(q) performed inĀ [Bet]. There are however several important differences at a more detailed level, e.g. in the ways the integrals are manipulated, in the treatment of the error terms and in the combinatorics.
The paper is organized as follow. In SectionĀ 2 we state TheoremĀ 3 which gives the analytic continuation for the shifted version of Aaā(s) and in SectionĀ 3 we easily deduce TheoremĀ 1 from it and we compute the constants given inĀ (1.2). In SectionĀ 4 we prove TheoremĀ 2 by integrating over the shifts introduced in TheoremĀ 3 and evaluating the resulting complex integrals. The rest of the paper is dedicated to the proof of TheoremĀ 3: in SectionĀ 5 we give a uniform bound for the region of absolute convergence, whereas in SectionĀ 6 we set up the proof of TheoremĀ 3 dividing the sum according to the range of the variables. In SectionĀ 7 we estimate the case where the variables have roughly the same size and in SectionĀ 8 we give a trivial bound for the case where thereās a large variable. Finally, in SectionĀ 9 we recompose the various sums reconstructing the polar terms.
Acknowledgments
The author wishes to thank Trevor Wooley and Tim Browning for useful comments.
The work of the author is partially supported by FRA 2015 āTeoria dei Numeriā and by PRIN āNumber Theory and Arithmetic Geometryā.
2 The shifted case
For kā„3, a as above and α=(α1ā,ā¦,αkā), β=(β1ā,ā¦,βkā)āCk we define the Dirichlet series
[TABLE]
where Ļα,βā(n):=ād1ād2ā=nād1āαād2āβā. If ā£ā(αmā)ā£,ā£ā(βmā)ā£ā¤2(kā1)1ā for all m, then it is easy to see (cf. LemmaĀ 4 below) that Aa;α,βā(s) converges absolutely on
[TABLE]
The following Theorem gives the analytic continuation for Aa;α,βā(s) to a larger half-plane, provided that
[TABLE]
is not too large. Before stating the theorem we need to introduce (a slight variation of) the Estermann function, which for α,βāC, hāZ and āāN is defined as
[TABLE]
for ā(s)>1āmin(ā(α),ā(β)) and where \operatorname{e}\mathopen{}\mathclose{{}\left(x}\right):=e^{2\pi ix}. The Estermann function can be continued to a meromorphic function on C satisfying a functional equation (see e.g.Ā [BC13b]).
Lemma 2**.**
Let α,βāC, hāZ and āāN with (h,ā)=1. Then
[TABLE]
can be extended to an entire function of s. Moreover, one has
[TABLE]
where h denotes the inverse of h\leavevmode\nobreak\ \mathopen{}\mathclose{{}\left(\textnormal{mod}\leavevmode\nobreak\ \ell}\right) and
[TABLE]
For α,βā{zāCā£ā£ā(z)ā£<2(kā1)1ā}k we also define
[TABLE]
where āā indicates the the sum is over h which are coprime to ā, and the second sum is over αā=(αiāā)iāIā, βā=(βā)iāIāāCā£I⣠satisfying the above condition. Also, we put sI,αāā:=ārāIāαrāā and
[TABLE]
if neither of the two sums inside the Ī functions are empty sums and Īαā;Iā:=0 otherwise.
Remark 1**.**
EquationĀ (LABEL:dfm) should be interpreted as defining Ma;α,βā(s) as a meromorphic function. Also, the definition of Ma;α,βā(s) can be extended to include the case where αiā=βiā since the limit for αiāāβiā exists (cf. the proof of TheoremĀ 1).
The absolute convergence of the series over ā inĀ (LABEL:dfm) for α,βā{zāCā£ā£ā(z)ā£<2(kā1)1ā}k is ensured by the convexity bound for the Estermann function,
[TABLE]
valid for Ī“>0, ā(α),ā(β)āŖ1, ā£1āsāαā£,ā£1āsāβā£>Ī“, and
[TABLE]
Indeed, usingĀ (2.4) one has that the series over ā converges as long as ā£Iā£>2+ā£Iā£ā£Jā£ā+āiāIā(ā£Iā£kāā(αiāā)āā(βiāā))āājāJāmin(ā(αjā),ā(βjā)). The right hand side is less than 4, so the only problematic case is when ā£Iā£=3. This can happen only for k=3 and k=4, and in the first case the convergence is clear since there is no Estermann function. Finally, the series converges also for k=4, ā£Iā£=3 and ā£Jā£=1 since one can save an extra factor of ā1āε using the convexity bound for āhāāDα,βā(s,āhā)
[TABLE]
for s satisfyingĀ (2.5) and where we used the bound cāā(m)āŖd(ā)(m,ā) for the Ramanujan sum c_{\ell}(m):=\sum_{\ell|a}\operatorname{e}\mathopen{}\mathclose{{}\left(\frac{hm}{\ell}}\right).
We are now ready to state our main theorem.
Theorem 3**.**
Let kā„3, aāZī =0kā. Then, Aa;α,βā(s) admits meromorphic continuation to ā(s)>1āk+12ā2ηα,βāā, α,βā{sāCā£ā£ā(s)ā£<2(kā1)1ā}k. Moreover, if for some ε>0 one has α,βā{sāCā£ā£ā(s)ā£<2(kā1)1āεā}k and 1āk+12ā2ηα,βāāεāā¤ā(s)ā¤1āk1āεā+k+1ηα,βāā, then
[TABLE]
for some absolute constant A>0.
Remark 2**.**
Clearly TheoremĀ 3 provides analytic continuation also for
[TABLE]
since Aa;α,βāā(s)=āϵā{±1}kāAaϵā;α,βā(s), where aϵā=(±1āa1ā,ā¦,±kāa). Moreover, the sum over ϵ in the āpolar termā Ma;α,βāā(s):=āϵā{±1}kāMaϵā;α,βāā(s) for Aa;α,βāā(s) can be executed giving a neater expression for Maϵā;α,βāā(s). Indeed, for āiāIāziā=1 we have
[TABLE]
by the identities for the Ī function (Ī(z)Ī(1āz))ā1=Ļ1āsin(Ļz) and \cos\mathopen{}\mathclose{{}\left(\frac{\pi z}{2}}\right)\Gamma(z)=\frac{\pi^{1/2}2^{z-1}\Gamma(\frac{z}{2})}{\Gamma(\frac{1-z}{2})}. Thus, since āiāIā(āαiāā+ā£Iā£1+sI,αāāā)=1, it follows that
[TABLE]
where Dcos;α,βā(s,āhā):=21ā(Dα,βā(s,āhā)+Dα,βā(s,āāhā)).
Throughout the rest of the paper, by a bold symbol v we indicate the vector (v1ā,ā¦,vkā)āCk. Also, for any set Iā{1,ā¦,k} by vIā we indicate the vector (viā)iāIāāCā£Iā£.
For any cāR, by ā«(c)āā ds we indicate that the integral is taken along the vertical line from cāiā to c+iā. Also, we will often abbreviate ā«(c1ā)āāÆā«(crā)ā with ā«(c1ā,ā¦,crā)ā.
Finally, by ε we indicate a sufficiently small positive real number, and by A a positive absolute constant whose value might be different at each occurrence.
We now show how to derive TheoremĀ 1 from TheoremĀ 3.
First, we assume ā£Ī±iāā£,ā£Ī²iāā£<2kεā and ā(s)>1. Then, by the residue theorem
[TABLE]
where wIā²ā:=(āwiā²ā)iāIā, sI,wIā²āā=āāiāIāwiā, and the circles are oriented in the positive direction. Thus, letting α,βā0 we obtain
[TABLE]
Now, for wī =0 we have
[TABLE]
as w1ā,ā¦,wkāā0 and so
[TABLE]
Also, if ā£wiāā£<kεā for all iāI with ε small enough, then we have
[TABLE]
for some fI,SāāC. It follows that
[TABLE]
where Ī“iāS1āāŖS2āā=1 if iāS1āāŖS2ā and Ī“iāS1āāŖS2āā=0 otherwise. By analytic continuation this gives an expression for Ma;0,0ā(s) for all sāC and so TheoremĀ 1 follows by TheoremĀ 3.
ā
We conclude the section by computing the value of the constant ck,k+1ā(a).
First we observe that the terms in this sum with I={1,ā¦,k} are
[TABLE]
(we remark that f{1,ā¦,k},S2āā(ā)/Ļ(ā) does not depend on ā). Among these, the term with m=k is
[TABLE]
since f{1,ā¦,k},ā ā=Ļ(ā)Ī(k1ā)kĪ0;{1,ā¦,k}ā. Finally,
[TABLE]
where
[TABLE]
with νpā(a)=r if prā£ā£a. Thus, the expression inĀ (LABEL:fcf) can be rewritten as
[TABLE]
where r={1ā¤iā¤kā£sign(aiā)=1} (and the above expression has to be interpreted as [math] if rā{0,k}).
We remark that for all qā„1 one has, as expected, Ļ(qa1ā,ā¦,qakā)=qĻ(a1ā,ā¦,akā). Finally, we observe that if we assume GCD(a1ā,ā¦,akā)=1 and let Īŗ(a):=āpā£a1āāÆakāāpmpā, where mpā is the second smallest among vpā(a1ā),ā¦,vpā(akā) (the smallest being 1 by hypothesis), then we have
[TABLE]
and so, in particular 1āŖĻ(a)āŖĪµāā£a1āāÆakāā£Īµ.
Indeed, we have
Also the coefficients ckā1,rā with 1ā¤rā¤k can be expressed in terms of the Gamma and zeta functions. Indeed, by Ramanujanās formulaĀ (1.10) if ā(s)>1, ā(s+w)>1, then
[TABLE]
since ānā„1ānsĻaā(n)Ļbā(n)ā=ζ(2sāaāb)ζ(s)ζ(sāa)ζ(sāb)ζ(sāaāb)ā (cf.Ā (1.3.3) inĀ [Tit]) and the same formula holds for ā(s+w)>2, ā(2s+w)>2, ā(w)>1 by analytic continuation. In particular, assuming for simplicity a=(ā1,1,ā¦,1) one computes that the contribution of the terms with ā£Iā£=kā1 toĀ (LABEL:fias) is
[TABLE]
where sāā=sāā(w1ā,ā¦,wkā1ā):=ār=1ākā1āwrā. Proceeding as above one can then compute the coefficients ckā1,rā for 1ā¤rā¤k.
First, we observe that the contribution to N(Bk) coming from the terms where the maximum max{ā£x1āā£,ā¦,ā£xkāā£,ā£y1āā£,ā¦ā£ykāā£} is attained at more than one of the ā£xiāā£, ā£yjā⣠is Oa,εā(Bkā23ā+ε). Indeed, the contribution of the terms with ā£xiāā£,ā£yiāā£ā¤ā£x1āā£=ā£y2ā⣠for all i=1,ā¦,k is
[TABLE]
and one can bound similarly all the other cases. Thus,
[TABLE]
where
[TABLE]
Notice that in the first line we divided by 4 since āx=x in P1(Q) and we multiplied by 2 since we assumed the maximum among the xiā,yjā is attained at one of the xiā.
By symmetry it is sufficient to consider the case i=1. Also, we can assume B is a half-integer.
Using Mƶbius inversion formula we find
[TABLE]
Then, we express the inequalities x1āā£yjāā£<B/d1ād2ā and x2āā¦,xkā,ā£y1āā£,ā¦ā£ykāā£<x1ā analytically via the following formula (see Theorem G inĀ [Ing])
[TABLE]
where Ļ[0,1)ā(x) is the indicator function of the set [0,1) and ā«ā² indicates that the integral is truncated at ā£ā(z)ā£ā¤T. We shall choose the parameter 1ā¤Tā¤B at the end of the argument. Bounding as above the error coming from the cases where x1ā/xiā=1, x1ā/yjā=1 for some i=2,ā¦,k or j=1,ā¦,k, we obtain
[TABLE]
where ā«ā²ā² indicates the integral is truncated at ā£ā(ufā)ā£ā¤2T and the lines of integration are czjāā=1āk1ā+3ε, cwjāā=ε and cufāā=1āk1ā+ε, for some small ε>0. The error term E is Oε,a,kā(Bkā1+3kε/T). Indeed, for example, in the most delicate case one needs to bound sums of the following form (we take a1ā=āÆ=akā=1 for simplicity, but the same proof extends to the general case):
[TABLE]
Now, (logā£x/yā£)ā1āŖā£xāyā£ā£xā£ā if ā£xāyā£<ā£xā£/2 (and thus ā£yā£ā„ā£xā£/2) and (logā£x/yā£)ā1āŖ1 otherwise. Thus, this sum is
[TABLE]
Now, a simple computation shows that for mī =0
[TABLE]
and so, writing r=x1āāy2ā, n=y1ā+x2ā and m=x3āy3ā+āÆ+xkāykā and bounding easily the case m=0, we see that the sum inĀ (LABEL:poet) is bounded by
[TABLE]
The terms with ā£mā£>(ā£x1ānā£+ā£x2ārā£)/4 can be bounded easily by using ā£mā£āk2āāŖā£x1ānā£āk2ā and disregarding the linear equation. For the terms with ā£mā£ā¤(ā£x1ānā£+ā£x2ārā£)/4, we have also ā£x1ānā£ā¤35āā£x2ār⣠and so, since r<ā£x1āā£/2, then ā£nā£<65āā£x2ā⣠and so ā£nāx2āā£1āk1ā+εā«ā£x2āā£1āk1ā+ε. Thus, we obtain that the sum inĀ (LABEL:poet) is
[TABLE]
Then, we write m=ā+x1āg with \ell\equiv-x_{2}r\leavevmode\nobreak\ \mathopen{}\mathclose{{}\left(\textnormal{mod}\leavevmode\nobreak\ |x_{1}|}\right), ā£gā£āŖā£x1āā£ā£x2ārā£ā, ā2ā£x1āā£ā<āā¤2ā£x1āā£ā and (ā,g)ī =(0,0), ā+x1āgī =x2ār. Dividing according to whether gī =0 and g=0 we obtain that the above sum is
[TABLE]
as claimed.
Now, we go back toĀ (4.1) and make the change of variables ufāāufā+zfā for all f=2,ā¦,k. Summing the Dirichlet series, we obtain
[TABLE]
where Aaϵā;z+α,z+βāā(0) is as defined inĀ (2.7), cufāā=ā2ε,
[TABLE]
and ā«ā²ā²ā² indicates the integral is truncated at ā£ā(zfā+ufā)ā£ā¤2T.
Now, we apply TheoremĀ 3 to Aa;z+α,z+βāā(0)=Aa;z+αāξ,z+βāξāā(1āk1ā), where ξ:=(1āk1ā,ā¦,1āk1ā). We keep as main term only the summand inĀ (LABEL:dfmas) with I={1,ā¦,k}, treating the other summands as error terms. Thus, we write
[TABLE]
where
[TABLE]
and Ea;z+α,z+βāāā is holomorphic on a region containing
[TABLE]
where it satisfies
[TABLE]
Assuming ε is small enough with respect to k, we can bound the contribution coming from Eāā by moving the line of integration czkāā to czkāā=2k1āā6kε, obtaining a contribution of O(Bkā1+26kε(T7Bā2k1ā+Tā1)) form the integrals over the new line of integration and on the horizontal segments.
Thus, we obtain
[TABLE]
where
[TABLE]
with
[TABLE]
and where N1,ϵā²ā²ā(B) is defined in the same way, but with the condition (α1āā,β1āā)=(α1ā,w1ā) in the sum replaced by (α1āā,β1āā)=(w1ā,α1ā).
We remark that if ε is small enough, Qαā,βāā(z,w) is holomorphic on a region containing
[TABLE]
where by Stirlingās formula it satisfies
[TABLE]
Now we move cz1āā to cz1āā=1ā2k3ā+6kε passing through the pole at kā1āāi=1kā(ziā+αiāā)=0. Notice that doing so α1āāāβ1āā stays constant so we donāt cross the pole of ζ(1āα1āā+β1āā). The contribution of the integrals on the new line of integration and on the horizontal segments is trivially Ok,ε,aā(Bkā1+12kε(Bā2k1ā+Tā1)), whereas the contribution of the residue is
[TABLE]
where zā²=(kā1āα1āāāi=2kā(ziā+αiāā),z2ā,ā¦,zkā) and where we used that for z1ā=kā1āα1āāāāi=2kā(ziā+αiāā) one has
[TABLE]
Next, we observe that the terms in the sum over αā,βā for which (αhāā,βhāā)=(whā,uhā) for some hā{2,ā¦,k} are Ok,ε,aā(Bkā1+12kε(TBā2k1ā+Tā1)); indeed one can move cwhāā and cuhāā to cuhāā=ā2k1ā+(6kā2)ε and cwhāā=2k1āā(6kā1)ε and then bound trivially obtaining the claimed bound. Notice that doing so we donāt pass through any poles, since ā(1āα1āā+β1āā)=1+ā(2w1ā+āj=2kāujā+wjā) stays constant, whereas ā(1āαhāā+βhāā)=ā(1āwhāā+uhāā) stays less than one.
Thus, we only have to consider the term with (αjāā,βjāā)=(ujā,wjā) for all j=2,ā¦,k and moving the lines of integration as above for all i=2,ā¦,k one obtains that itās enough to consider the contribution from the residue at wjā=0 for all j=2,ā¦,k. To summarize, we arrive to
[TABLE]
with wā²=(w1ā,0,ā¦,0). Next we move the line of integration cw1āā to cw1āā=ā4k1ā+6kε passing through the pole at w1ā=0 only, so that bounding trivially the contribution of the new line of integration we obtain
N1ā²ā(B)=C1,1ā(T)Bkā1+Ok,ε,aā(Bkā1+12kε(TBā4k1ā+Tā1)),
where
[TABLE]
with uā²=(āāj=2kāujā,u2ā,ā¦,ukā) and zā²=(kā1āα1āāāāi=2kā(ziā+uiā),z2ā,ā¦,zkā)=(kā1āāi=2kāziā,z2ā,ā¦,zkā) and lines of integration cujāā=ā2ε, cziāā=1āk1ā+3ε. Notice thatĀ (4.3) in this case gives
[TABLE]
and thus, using the convexity bound ζ(1+āj=2kāujā)āŖĪµā(1+ā£u2ā+āÆ+ukāā£)(k+1)ε, we obtain
[TABLE]
where C1,1ā²ā is defined as C1,1ā(T) but where we removed the truncations at ā£ā(ziā)ā£ā¤T and ā£ā(ziā+uiā)ā£ā¤2T from the integrals. Thus,
[TABLE]
We can treat N1ā²ā²ā(B) in the same way, the only difference being that in this case ājāzjā=kā1āw1āāāj=2kāαjāā so that we still obtain a non-negligible contribution only from the summand with (αiāā,βiāā)=(uiā,wiā) for all i=2,ā¦,k. We arrive to
[TABLE]
with zā²=(kā1+w1āāāj=2kāujāāāj=2kāzjā,z2ā,ā¦,zkā) and wā²=(w1ā,0,ā¦,0). We move the line of integration cw1āā to cw1āā=4k1āā6kε, passing through a pole at w1ā=ā21āāj=2kāujā. The integral on the new line of integration can be bounded trivially, whereas the contribution of the residue is
[TABLE]
where wā²=(ā21āāj=2kāujā,0,ā¦,0). Next, for each j=3,ā¦,k we move cujāā to cujāā=2k1āā6kε, passing through the pole of ζ(1āujā). The contribution on the new line of integration can be bounded trivially, and we obtain that the above is
[TABLE]
where αā²=(ā21āu2ā,u2ā,0,ā¦,0) and βā²=(ā21āu2ā,0,ā¦,0). Moving cu2āā to cu2āā=2k1āā6kε picking up the pole at u2ā=0, we then obtain
[TABLE]
where
[TABLE]
with z=(kā1āāj=2kāzjā,z2ā,ā¦,zkā). ByĀ (4.3) and the analogous bound for the logarithmic derivative of Qαā²,βā²ā we have
[TABLE]
where C1,2ā²ā and C1,3ā²ā defined as C1,2ā,C1,3ā but without the truncation at ā£ā(ziā)ā£ā¤T in the integrals. Finally, we write C1,2ā²ā as C1,2ā²ā=S(a)Ļiā(a), where
[TABLE]
and
[TABLE]
Summarizing, we proved
[TABLE]
Thus, TheoremĀ 4 follows by taking T=B15kā21ā and applying the following Lemma.
Lemma 3**.**
For kā„3 we have Ļ1ā²ā(a)=Ļ1ā(a)
where Ļ1ā(a) is as inĀ (1.8).
Proof.
We only give a sketch, leaving the problem of justifying the manipulation of certain conditionally convergent integrals to the interested reader.
First, by symmetry, we observe that
[TABLE]
Then, we detect the characteristic function Ļ(0,1)ā using its Mellin transform obtaining
[TABLE]
with cz1āā=k1ā.
Then, we use LemmaĀ 8 below with B=0333The Lemma is stated for B large to avoid issues coming with the conditional convergence of the integrals. To make this rigorous itās enough to take a larger B, and then later in the argument recompose the sum over ν usingĀ (7.22). obtaining
[TABLE]
where G(s) is entire with G(0)=1, āi±ā indicates the sum is restricted to indexes such that ±iāsign(aiā)=±1, with ±1ā1:=āsign(a1ā), and the lines of integrations are cziāā²ā=kā11ā and cziāā=k+11ā for i=2,ā¦,k and cz1āā=cz1āā²ā=k1ā. Then, we notice that we can take instead cziāā=cziāā²ā=k1ā for i=2,ā¦,k and cz1āā=k+11ā,cz1āā²ā=kā11ā. We take the integral over xiā and yiā inside and execute them, obtaining
[TABLE]
By the residue theorem the difference of the integrals in z1ā is equal to minus the residue at z1ā=1āz2āāāÆāzkā and so
[TABLE]
where z1ā:=1āz2āāāÆāzkā. We take the sum over ϵ inside, and evaluate it usingĀ (LABEL:regac) (notice that since the value of ±1ā1 is fixed we have to multiply by 21ā). We obtain
[TABLE]
Making the change of variables ziāā1āziā for all i=2,ā¦,k we obtain Ļ1ā²ā(a).
ā
5 The region of absolute convergence
In this section we prove a bound for Aa;α,βā(s) in the region of absolute convergence. We remark that if we were not concerned with the uniformity in k, then an easier argument would have sufficed.
Lemma 4**.**
Let kā„3, aāZī =0kā and α,βāCk with ā£ā(αiā)ā£,ā£ā(βiā)ā£ā¤2(kā1)1ā for all i=1,ā¦,k. Then Aa;α,βā(s) converges absolutely on ā(s)>1āk1āāk1āāi=1kāmin(ā(αiā),ā(βiā)). Moreover, if
[TABLE]
for some ε>0, then \mathcal{A}_{\boldsymbol{a};\boldsymbol{\alpha},\boldsymbol{\beta}}(s)\ll_{\varepsilon}\mathopen{}\mathclose{{}\left(\frac{Ak}{\varepsilon}}\right)^{4k} where the implicit constant depends on ε only and A is an absolute constant.
Proof.
Clearly, we can assume s,αiā,βiāāR and αiāā¤Ī²iā for all i=1,ā¦,k and that ε<81ā. Also, it is sufficient to establish the claimed bound for s=1āk1āāk1āāi=1kāαiā+k4εā.
We have Ļα,βā(n)ā¤d(n)nmax(āα,āβ) and so
[TABLE]
say, where we wrote siā:=s+αiā. By hypothesis s1āāε>1āk1āākā11āāε>0 and so
[TABLE]
say.
We write
[TABLE]
where ξrā is any real number in the interval (1,2) such that ā£crāā£>2kεā (notice that since ā£Ī±rāā£ā¤2(kā1)1ā we also have crā>āε+ξrākεā>ā81ā). Now,
[TABLE]
by the residue theorem, where I is the set of rā{3,ā¦,k} for which crā<0 and ĻIā is the characteristic function of the set I. We replace the condition nrāā¤n2ā for all r=3,ā¦,k by this formula and obtain
[TABLE]
since siā>1+kεā for all iāI, and where L:={3,ā¦,k}āJ. (Here and below the exchanges in the orders of sums and integrals are justified by the absolute convergence).
Exchanging the order of summation and integration and summing the Dirichlet series we obtain
[TABLE]
The real part of the argument of the last ζ in the above equation is
[TABLE]
by the definition of sāā and since ξāāā¤2 and s=1āk1āāk1āāi=1kāαiā+k4εā. Since ā£Ī±iāā£ā¤2(kā1)1ā for all i=1,ā¦,k, then the above expression is
[TABLE]
where m:=kā2āā£L⣠(so that 0ā¤mā¤kā2). Thus, if m<k/2 then ā(s1ā+s2āāεāāāāLāwāā)ā„1+k4āε, and the same holds if mā„k/2 since in this case we have
[TABLE]
for kā„3 and ε<81ā.
It follows that
[TABLE]
since by our choice we have sāā+cāā=1+ξāākεā>1 for all āāL.
Finally, since ā£cāāā£>2kεā and cāā>ā21ā we have
[TABLE]
and so, since srā>1+ξrākεā for all rāI and sāā+cāā>kεā for all r=3,ā¦,k, we have
[TABLE]
for some fixed A>0. The same bound clearly holds for Zi,jā for all i,j and so the Lemma follows.
ā
Then, we notice that instead ofĀ (LABEL:bdmt), it is enough to prove
[TABLE]
for ā(s)ā„1āk+12ā2ηα,βāāεā. Indeed, we can apply the Phragmen-Lindelƶf principle on the region 1āk+12ā2ηα,βāāεāā¤ā(s)ā¤1āk1āεā+k+1ηα,βāā usingĀ (6.2) on the left boundary line and the bound for Aa;α,βā(s) given in LemmaĀ 4 with a trivial bound for Ma;α,βā(s) on the line ā(s)=1āk1āεā+k+1ηα,βāā. Also, inĀ (LABEL:bdmt) we can take (1+ā£sā£)7 rather than (1+ā£sā£)A since for s=Ļ+it one has Aa;α,βā(s)=Aa;α+tā²,β+tā²ā(Ļ) where tā²:=(t,ā¦,t).
Furthermore, we notice it is sufficient to prove TheoremĀ 3 in the case ā£Ī±iāāβiāā£>kεā for i=1,ā¦,k. Indeed, assume we have proved TheoremĀ 3 in this restricted case and let
[TABLE]
where αā²(ξ)=(α1ā²ā,ā¦,αkā²ā):=(α1ā+ξ,α2ā,ā¦,αkā). Then, Fa;α,βā(s) defines a holomorphic function in (s,α,β) in the domain
We localize the variables of summation by introducing partitions of unity
[TABLE]
such that āā Xā1ā¤Nā¤Xā1āŖlogX and with P(x) supported on 1ā¤xā¤2 and satisfying P(j)(x)āŖjAj for some A>0. Notice that under these conditions, the Mellin transform of P(x),
[TABLE]
is entire and satisfies
[TABLE]
for some C>0.
Thus, for s satisfyingĀ (5.1) we can write
[TABLE]
where
[TABLE]
and, here and in the following, we omit to indicate the dependence on a and N1ā,ā¦,Nkā to save notation. The main step in the proof consists in the following lemma which we shall prove in SectionĀ 7.
Since both Aα,βā(s) and the main term on the right side ofĀ (6.6) are symmetric in N1ā,ā¦,Nkā and with respect to the change aāāa (cf. RemarkĀ 9 at the end of SubsectionĀ 7.5), we can and shall assume that N1ā is the maximum among the Niā and that a1ā<0.
7.1 Separating the variables
The condition āa1ān1ā=a2ān2ā+āÆ+akānkā can be used to eliminate the variable n1ā in the definitionĀ (6.5) of Aα,βā(s), by adding the conditions
[TABLE]
and replacing each occurrences of n1ā by (a2ān2ā+āÆ+akānkā)/ā£a1āā£. This poses the problem of expressing Ļα1ā,β1āā(n1ā)=n1āαāĻαāβā(n1ā) in a more flexible way, which we achieve by the following modification of Ramanujanās identityĀ (1.10) which also allows us to remove the above congruence condition.
Lemma 7**.**
Let a,māN and γāC. Then we have
[TABLE]
where Ī“aā£nā=1 if aā£n and Ī“aā£nā=0 otherwise, c_{\ell}(n):=\operatornamewithlimits{\sum\nolimits^{*}}_{h\leavevmode\nobreak\ \mathopen{}\mathclose{{}\left(\textnormal{mod}\leavevmode\nobreak\ n}\right)}\operatorname{e}\mathopen{}\mathclose{{}\left(\frac{hn}{\ell}}\right) is the Ramanujan sum and for any cwā>ā£ā(γ)ā£
[TABLE]
where G(w) is any even entire function which decays faster than any polynomial in vertical strips and is such that G(0)=1.
Proof.
We start by observing that for ā(s)>1 we have
[TABLE]
Indeed, by the orthogonality of additive characters, the left hand side is
[TABLE]
as claimed. By Ramanujanās identityĀ (1.10), one has thatĀ (7.2) gives
[TABLE]
for ā(s)>1.
Now, by the residue theorem for any cwā>ā£ā(γ)⣠we have
[TABLE]
since Ļγ+wā(m)=mγ+wĻāγāwā(m) and G(āw)=G(w), and so the lemma then follows byĀ (7.3).
ā
Remark 5**.**
It will be convenient to take G(w) with a zero which cancels the pole of the zeta-function in the definitionĀ (7.1) of Ļ . Thus we take
[TABLE]
where ξ(s):=21ās(sā1)ĻāĻ/2Ī(21āw)ζ(w) is the Riemann ξ-function. Notice that G(0)=1 and that by the functional equation we have Gα1ā,β1āā(w)=Gα1ā,β1āā(āw). Also, by Stirlingās formula we have
[TABLE]
for any rā„0.
Applying this lemma we obtain
[TABLE]
where the sum is over αā=(α1āā,ā¦,αkāā), βā=(β1āā,ā¦,βkāā) and
[TABLE]
Next, we express P and Ļ using their Mellin transforms so that, after making the change of variables uiāāuiāās for all iā{1,ā¦,k}, we obtain
[TABLE]
with lines of integrations
[TABLE]
Next, we separate the variables in the expression (a2ān2ā+āÆ+akānkā)21ā+α1ā+u1āā2wā using the following lemma which we quote from SectionĀ 10 ofĀ [Bet] in a slightly adapted form.
Lemma 8**.**
Let Īŗā„2 and x1ā,ā¦xĪŗā>0. Let ϵ=(±1ā,āÆ,±κā1)ā{±1}Īŗ, with ±1ā1=ā1. Let BāZā„0ā be such that 2Īŗā+21ā<ā(v1ā)<B+1. Moreover, let cv2āā,ā¦,cvĪŗāā,cv2āā²ā,ā¦,cvĪŗāā²ā>0 be such that
[TABLE]
Then
[TABLE]
where
[TABLE]
and G(s) is any entire function such that G(0)=1 and G(Ļ+it)āŖeāC1āā£tā£(1+ā£Ļā£)C2āā£Ļ⣠for some fixed C1ā,C2ā>0. Moreover, writing siā=Ļiā+itiā for i=1,ā¦,Īŗ, we have
[TABLE]
for some A>0, provided that the siā are located at a distance greater than Ī“>0 from the poles of Ψϵ,Bā.
Remark 6**.**
If ϵ=(ā1,ā¦,ā1), then Ψϵ,Bā has to be interpreted as being identically zero.
Remark 7**.**
The function Ψϵ,Bā(s1ā,ā¦,sĪŗā) has poles at siāāZā¤0ā and at s1ā+āÆ+skā=B+1.
Remark 8**.**
As a function G in this case we take G(s):=ξ(21ā+s)/ξ(21ā).
We apply LemmaĀ 8 toĀ (7.5) with ϵ:=(signa1ā,ā¦,signakā), v1ā=1āα1āāu1ā+2wā and B=4k, so that by our choice for the lines of integrationĀ (7.6), we have ā(v1ā)=1+4kāε.
Notice that thanks toĀ (7.7) we donāt have problems of convergence of the integrals.
We obtain,
[TABLE]
where, after opening the Ramanujan sum and summing over n2ā,ā¦,nkā,
[TABLE]
with cv2āā,ā¦,cvkāā=kεā, and where Rν;α,βā²ā(s) is defined in the same way, but with lines of integrations cviāā²ā=1/2+εāmin(ā(αiā),ā(βiā)) for i=2,ā¦,k.
We notice that by our choices for the lines of integration we have that the sum of the arguments of the function Ψϵ,4kā in Rν;α,βā(s) has real part 4k+1ākεā and so is less than 4k+1 as needed for the application of LemmaĀ 8
(whereas for Rν;α,βā(s) one has that such real part is (much) larger than 4k+1).
Now, Rν;α,βā²ā can be bounded trivially by moving the line of integrations cuiāā to cuiāā=21ā+νiā for i=2,ā¦,k, cwā to cwā=1+ā£ā(α1āāβ1ā)ā£+2ε, and cu1āā to cu1āā=1ā6kāā(α1ā)+2cwāā without passing through any pole (cf. RemarkĀ 7).
We obtain that Rν;α,βā²ā(s) is bounded by
[TABLE]
byĀ (6.4) andĀ (7.7) with Xs,k,a,εā as inĀ (6.1), and where for the last bound we used that
N1ā is the largest of the Niā and ν2ā+āÆ+νkā=4k. Thus, summarizing this section we proved
7.2 Picking up the poles of the Estermann functions
Next, after moving cwā and cu1āā to ensure the convergence of the sum over ā, we move the line of integration cuiāā to cuiāā=āmax(ā(αiā),ā(βiā))ā2kεā+νiā for each i=2,ā¦,k , passing through the poles (cf. LemmaĀ 2) of the Estermann functions. We obtain:
[TABLE]
where after changing the order of sums and integrals (as can by done by the absolute convergence of the sum and integrals)
[TABLE]
and the lines of integrations can be taken to be
[TABLE]
Notice that with this choice the sum over ā converges absolutely by the convexity boundĀ (2.4) for the Estermann function.
We will treat SI;ν;α,βā differently depending on whether ā£Iā£ā¤ā£J⣠or ā£Iā£>ā£Jā£.
7.3 The case ā£Iā£ā¤ā£Jā£
If ā£Iā£ā¤ā£J⣠(or, equivalently, ā£Jā£ā„2kā1ā), then we use the following lemma, whose proof we postpone until the end of this subsection.
Lemma 9**.**
Let aāZī =0Īŗā and γ,Ī“āCĪŗ.
Let S be the meromorphic function defined by
[TABLE]
Then
[TABLE]
where Sā(z) is holomorphic on ā(z)ā¤āmaxi=1Īŗāmax(ā(γiā),ā(Ī“iā)) and Sāā(z)=0 if Īŗ=1 and otherwise Sāā(z) is holomorphic on ā(z)ā¤Īŗ1āāκεāāĪŗ1āāi=1Īŗāmax(ā(γiā),ā(Ī“iā)). Furthermore, if ā£ā(γiā)ā£,ā£ā(Ī“iā)ā£ā¤21ā and
[TABLE]
then
[TABLE]
Moreover, if ā£ā(γiā)ā£,ā£ā(Ī“iā)ā£ā¤2(Īŗā1)1ā and
[TABLE]
then
[TABLE]
We apply this Lemma with Īŗ=ā£Jā£, splitting SI;ν;α,βā(s) into
[TABLE]
in the way suggested by the notation, with Sāā=0 if ā£Jā£=1. For Sā we useĀ (7.13) with
[TABLE]
(since Dα,βā(w,khā)=Dα+w,β+wā(0,khā)). We move the line of integration cwā to
[TABLE]
keeping the other ones as inĀ (LABEL:cloi). Notice that we stay in the region of holomorphicity of Sā and that we can applyĀ (7.13) since āmax(ā(γiā),ā(Ī“iā))=kεāā„3ā£Jā£Īµā whereas, using the trivial bound (ajā,ā)ā¤ā£ajāā£, the condition on u in the Lemma becomes
[TABLE]
which is verified with our choice of lines of integration. Thus, we have thatĀ (7.13) gives
[TABLE]
UsingĀ (6.4) (with r=5 and r=5k),Ā (7.4) (with r=5k) andĀ (7.7), we obtain
Now, since ā£Jā£=kā1āā£Iā£, the above bound implies
[TABLE]
since ν2ā+āÆ+νkā=4k and Niāā¤N1ā for all i=2,ā¦,k.
If ā£Iā£<ā£J⣠we can bound Sāā in the same way, usingĀ (7.14) instead ofĀ (7.13), with the difference that now we move the line of integrations to
[TABLE]
(Notice that, with respect to the case of Sā, we have essentially moved cujāā to the right by ā£Jā£1ā, cwā to the left by 1 and thus cu1āā to the right by 21ā). Thus, we obtain
[TABLE]
Also, we have
[TABLE]
since ā£Iā£=kā1āā£Jā£, and the maximum value of the expression on the right is obtained for ā£Jā£=kā1 since N1kāā„N1āāÆNkā. Thus,
[TABLE]
If ā£Iā£=ā£Jā£, then we cannot move the line of integration cwā as inĀ (LABEL:dsdss) without passing through the pole at w=0. Thus, we move cwā to cwā=āi=1kāā£ā(αjā+βjā)ā£+2ε and leave the other lines of integrations as inĀ (LABEL:dsdss). Bounding trivially we obtain
[TABLE]
Now we have ā£Jā£1āāĻā¤0 for Ļā„21ā (we can take ā£Jā£>1 since otherwise Sāā=0) and N1āā„Niā for all i=2,ā¦,k and so for 21āā¤Ļā¤1 we have
[TABLE]
since in this case ā£Iā£=2kā1ā.
Thus, summarizing, in this subsection we proved that if ā£Jā£ā„ā£I⣠and 21āā¤Ļā¤1, then
[TABLE]
We conclude the subsection with the proof of LemmaĀ 9.
First, we write ājā=ā/(ajā,ā) and ajā²ā=ajā/(ajā,ā), so that
[TABLE]
We apply the functional equationĀ (2.2) to each of the Estermann functions, obtaining
[TABLE]
where hajā²āā is the inverse of ha_{j}\leavevmode\nobreak\ \mathopen{}\mathclose{{}\left(\textnormal{mod}\leavevmode\nobreak\ \ell_{j}}\right). Now we assume ā(z)<āmaxi=1kāmax(ā(γiā),ā(Ī“iā)) and we expand the Estermann functions into their Dirichlet series and execute the sum over h. We obtain
[TABLE]
where
[TABLE]
Then we divide S(z) into S(z)=Sā(z)+Sāā(z) according to whether Ļī =0 or Ļ=0 (notice that Sāā(z)=0 if Īŗ=1). For the terms with Ļ=0, we observe that by LemmaĀ 4 we have
[TABLE]
for
[TABLE]
Thus from Stirlingās formula in the crude form
[TABLE]
and since ājāā¤ā, for ā(γjā),ā(Ī“jā)āŖ1 and ā£ā(γiā)ā£,ā£ā(Ī“iā)ā£ā¤21ā we have
In order to prove (7.13) it is sufficient to show that for all fixed ε>0 we have
[TABLE]
for ā(z)ā¤ā3κεāāmaxiā(max(γiā,Ī“iā))uā²ā„1+ε.
Moreover, we observe that we can assume z,γiā,Ī“iā are real and we can also assume z=ā3κεāāmaxiā(max(γiā,Ī“iā)).
Since ā£cāā(Ļ)ā£ā¤ādā£(Ļ,ā)ādāŖĪµā(Ļ,ā)1+ε, we have
[TABLE]
(Notice that Ļ depends on ā.) Now, we write
[TABLE]
for diā=(aiā,ā), so that
[TABLE]
where Ļαā(n):=ādā£nādα, since for all cāN, u>1 we have
[TABLE]
Thus, for uā„1+ε
[TABLE]
We divide the sum into a sum of k sums, according to which of the miā is the largest. For the contribution where m1āā„maxi=2Īŗā(miā) we observe that, for z1ā:=1āzāmax(γ1ā,Ī“1ā)>1 we have
[TABLE]
by the Cauchy-Schwarz inequality. Then, since ā£Ļā²ā£ā¤Īŗm1āā£a1āāÆaĪŗā⣠we have that the above sum is
[TABLE]
since z1āā¤2 and ānā„1āān2sd(n)2ā=ζ(4s)ζ(2s)4ā.
Thus,Ā (7.18) can be bounded by
Here we treat SI;ν;α,βā(s), which was defined inĀ (LABEL:dfso), in the case ā£Iā£>ā£Jā£. First, we move the lines of integration cwā and cu1āā inĀ (LABEL:dfso) to
[TABLE]
Bounding as before (in this case one could also simply use the convexity bound for the Estermann functions) one obtains
[TABLE]
In particular, if νjā>0 for some jāJ, then the above bound implies
[TABLE]
For the terms with νjā=0 for all jāJ, we take jāāJ and move the lines of integrations cujāāā and cvjāāā to the left and to the right by 1 respectively, picking up the residue from the simple pole of Ψϵ,4kā at vjāā=0. In the contribution coming from the integrals of the new lines of integration we move cu1āā to the right by 1 (as we can now do without passing through other poles of Ψϵ,4kā) so that bounding trivially we obtain a contribution which is
[TABLE]
We repeat this for all jāJ obtaining
[TABLE]
where TI;ν;α,βā(s) is obtained by SI;ν;α,βā(s) by taking the residue in at vjā=0 for all jāJ, that is
[TABLE]
with I1ā:=IāŖ{1}, vIā:=(viā)iāI1āā, where we put v1ā:=1āα1āāu1ā+2wā and
[TABLE]
Notice that in the integral defining TI;ν;α,βā(s) we have a fast decaying function for each of the variables of integration and so we donāt have to worry anymore about the convergence of the integrals.
Next, we move the line of integrations to
[TABLE]
moving also cu1āā so that we still have cu1āā=ā4kāā(α1ā)+2cwāā+ε. We pass through a simple pole at w=0 only, since the pole of ζ(1āα1ā+β1ā+w) is canceled by the zero of Gα1ā,β1āā(w) (cf. RemarkĀ 5).
Notice that on the new line of integrations the convexity boundĀ (2.4) gives
[TABLE]
which suffices for the convergence of the sum over ā. Thus the integral on the new lines of integrations gives a contribution bounded by
[TABLE]
Thus, since ā£Iā£>ā£J⣠with ā£Iā£+ā£Jā£=kā1ā„2 implies ā£Iā£ā„2, then byĀ (7.19) we have
[TABLE]
where YI;ν;α,βā(s) is the contribution from the residue at w=0.
Now, we move the line of integration cu1āā to cu1āā=1āā(α1ā)+kεā and we make the change of variables viāāviā+νiā for all iāI moving the lines of integration cviāā so that we still have cviāā=kεā for all iāI. Since B=āiāIāνiā (as we only have to consider the terms with νjā=0 for all jāJāŖ{1}) we have that the only factor depending on ν is the function ĪØI1ā,ϵā²ā(viā+ν), where ν=(0,ν2ā,ā¦,νkā). Thus, summing over ν we are left with
[TABLE]
where I1±ā:={iāIā£Ā±iā1=±1}. The identity B(s1ā+1,s2ā)+B(s1ā,s2ā+1)=B(s1ā,s2ā) for the Beta function B(s1ā,s2ā):=Ī(s1ā)Ī(s2ā)Ī(s1ā+s2ā)ā1 generalizes to
[TABLE]
for m,rā„1, s1ā,ā¦,smāāC, and so we have
[TABLE]
Thus, after the change of variables ujāāujā+s for all jāJāŖ{1} and 1āαiāāviāāsāuiā for iāI, we obtain
[TABLE]
where for any set I with ā£Iā£>2k+1ā we define
[TABLE]
where vIā²ā=(viā²ā)iāIā=(1āαiāāuiāās)iāIā, J:={1,ā¦,k}āI and where we can take the lines of integrations to be
[TABLE]
Notice that for any iāI if we move cuiāāā to āαiāāāĻ+ε we obtain the bound
[TABLE]
Also, for all jāāJ (notice we can assume kā„4 since for k=3 we have ā£Iā£>2 and so J=ā ) we have
[TABLE]
as can be seen by moving the lines of integrations to
[TABLE]
(Notice that since ā£Iā£ā„[2k+3ā], with this choice the sum over ā is absolutely convergent by the convexity boundĀ (2.4).)
To summarize, byĀ (7.21) andĀ (7.23) in this section we proved that for ā£Iā£>ā£Jā£
[TABLE]
where E4ā(s) satisfies
[TABLE]
and ZI1ā;α,βā(s) satisfiesĀ (7.25) andĀ (7.26).
Notice that the main term on the right ofĀ (7.28) is symmetric in N1ā,ā¦,Nkā and, by the definitionĀ (7.20) of ĪØI,ϵā, with respect to aāāa (i.e. ϵāāϵ).
As in the proof of LemmaĀ 5 we assume N1ā is the maximum among N1ā,ā¦,Nkā.
Writing the partitions of unity in terms of their Mellin transform, we obtain
[TABLE]
where sā²:=1+sāĻ+kεāāηα,βā²ā with ηα,βā²ā:=k1āāi=1kāmin(ā(αiā),ā(βiā)), αā²:=(ā1+αiā+uiāākεā+Ļ+ηα,βā²ā)iā{1,ā¦,k}ā and βā²:=(ā1+βiā+uiāākεā+Ļ+ηα,βā²ā)iā{1,ā¦,k}ā. We move the lines of integration to
[TABLE]
so that on the new lines of integration we have ā£ā(αiā²ā)ā£,ā£ā(βiā²ā)ā£ā¤2(kā1)1ā for i=2,ā¦,k and
[TABLE]
We cannot apply directly LemmaĀ 4 since we would need also ā£ā(α1ā²ā)ā£,ā£ā(β1ā²ā)ā£ā¤2(kā1)1ā, whereas we have ā(α1ā²ā)=ā1+ā(α1ā), ā(β1ā²ā)=ā1+ā(β1ā). However, we observe that
[TABLE]
since (maxj=2kānjā)ā¤n1āā¤k(maxj=2kānjā)(maxi=2kāā£aiāā£) and where siā²ā=1+kεāāηα,βā²ā+min(ā(αiā),ā(βiā)) for i=2,ā¦,k and s1ā²ā=kεāāηα,βā²ā+min(ā(α1ā),ā(β1ā)). Then, we can proceed exactly as in the proof of LemmaĀ 4 obtaining
since kηα,βā²āā¤Ī·Ī±,βā and the Lemma follows since byĀ (7.25) andĀ (7.26) the main term on the right hand side ofĀ (6.8) also satisfies the boundĀ (6.9).
Finally, byĀ (9.3) one has that for Ļā„1āmax1ā¤iā¤kāmax(ā(αiā),ā(βiā))ākεā TheoremĀ 3 is a consequence of LemmaĀ 4 and so the proof of TheoremĀ 3 is complete.
The reference list from the paper itself. Each links out to its DOI / PubMed record.
1[Bag] Bagchi, B. Nyman, Beurling and Baez-Duarteās Hilbert space reformulation of the Riemann hypothesis . Proc. Indian Acad. Sci. Math. Sci. 116 (2006), no. 2, 137ā146; arxiv math.NT/0607733
2[Bet 15] Bettin, S. On the distribution of a cotangent sum . Internat. Math. Res. Research Notices (2015) no. 21, 11419ā11432.
3[Bet 16] Bettin, S.; On the reciprocity law for the twisted second moment of Dirichlet L-functions . Trans. Amer. Math. Soc. 368 (2016), 6887ā6914.
4[Bet] Bettin, S. High moments of the Estermann function , preprint.
5[BC 13a] Bettin, S.; Conrey, J.B. A reciprocity formula for a cotangent sum . Internat. Math. Res. Research Notices, 2013 no. 24, 5709ā5726.
6[BC 13b] Bettin, S.; Conrey, J.B. Period functions and cotangent sums . Algebra Number Theory 7 (2013), no. 1, 215ā242.
7[Blo] Blomer, V. On triple correlations of divisor functions , to appear in Bull. Lond. Math. So.
8[B Ba] Blomer, V.; Brüdern, J. Counting in hyperbolic spikes: the diophantine analysis of multihomogeneous diagonal equations , to appear in J. reine angew. Math., arxiv math.NT/1402.1122