The Voronoi summation formula

Jordan Bell
September 16, 2015

1 Mellin transform

The Mellin transform of f:(0,∞)→ℂ is defined by

ℳ⁢(f)⁢(s)=∫0∞xs-1⁢f⁢(x)⁢𝑑x.

For example, s↦Γ⁢(s) is the Mellin transform of x↦e-x.

Suppose that f continuous on (0,∞), that there is some α∈ℝ such that f⁢(x)=O⁢(x-α) as x→0, and that for any n≥1, f⁢(x)xn→0 as x→∞. Then [4, p. 107, Proposition 9.7.7] ℳ⁢(f)⁢(s) is holomorphic on ℜ⁡(s)>α, and for σ>α and x>0,

f⁢(x)=12⁢π⁢i⁢∫ℜ⁡(s)=σx-s⁢ℳ⁢(f)⁢(s)⁢𝑑s.

(The Mellin inversion formula.)

2 Generalized Poisson summation formula

Cohen [4, pp. 177–182, §10.2.5] presents a “generalized Poisson summation formula” which yields both the Poisson summation formula and the Voronoi summation formula.

We denote by 𝒮⁢(ℝ) the Fréchet space of Schwartz functions ℝ→ℂ.

Theorem 1.

Let a be arithmetic function and define

L⁢(a,s)=∑n=1∞a⁢(n)⁢n-s,ℜ⁡(s)>1.

Suppose that L⁢(a,s) has an analytic continuation to ℂ whose only possible pole is at s=1. Suppose also that there are A,a1,…,ag>0 such that for

γ⁢(s)=As⁢∏j=1gΓ⁢(aj⁢s),

L⁢(a,s) satisfies the functional equation

γ⁢(s)⁢L⁢(a,s)=γ⁢(1-s)⁢L⁢(a,1-s).

Let f∈𝒮⁢(ℝ) and define for x>0,

K⁢(x)=12⁢π⁢i⁢∫ℜ⁡(s)=32γ⁢(s)γ⁢(1-s)⁢x-s⁢𝑑s,g⁢(x)=∫0∞f⁢(y)⁢K⁢(x⁢y)⁢𝑑y.

Then,

∑n=1∞a⁢(n)⁢f⁢(n)=f⁢(0)⁢L⁢(a,0)+Ress=1⁢ℳ⁢(f)⁢(s)⁢L⁢(a,s)+∑n=1∞a⁢(n)⁢g⁢(n).
Proof.

Since f is a Schwartz function, ℳ⁢(f) is holomorphic on ℜ⁡(s)>0. Futhermore, for ℜ⁡(s)>0, integrating by parts,

ℳ⁢(f)⁢(s)=∫0∞xs-1⁢f⁢(x)⁢𝑑x=f⁢(x)⁢xss|0∞-∫0∞f′⁢(x)⁢xss⁢𝑑x=-1s⁢ℳ⁢(f′)⁢(s+1).

It follows that ℳ⁢(f) has an analytic continuation to ℂ possibly with poles at 0,-1,-2,-3,…. Write F=ℳ⁢(f). By the Mellin inversion formula we get

∑n=1∞a⁢(n)⁢f⁢(n) =∑n=1∞a⁢(n)⁢12⁢π⁢i⁢∫ℜ⁡(s)=32n-s⁢F⁢(s)⁢𝑑s
=12⁢π⁢i⁢∫ℜ⁡(s)=32F⁢(s)⁢∑n=1∞an⁢n-s⁢d⁢s
=12⁢π⁢i⁢∫ℜ⁡(s)=32F⁢(s)⁢L⁢(a,s)⁢𝑑s.

The only possible pole of L⁢(a,s) is at s=1. From

ℳ⁢(f)⁢(s)=-1s⁢ℳ⁢(f′)⁢(s+1),

the only possible pole of F⁢(s) in the half-plane ℜ⁡(s)>-1 is at s=0, and the residue of F⁢(s)⁢L⁢(a,s) at s=0 is

-ℳ⁢(f′)⁢(1)=-∫0∞f′⁢(x)⁢𝑑x=-(f⁢(∞)-f⁢(0))=f⁢(0),

so the residue of F⁢(s)⁢L⁢(a,s) at s=0 is

f⁢(0)⁢L⁢(a,0).

Therefore, by the residue theorem, taking as given that F⁢(s)⁢L⁢(a,s)→0 uniformly in -12≤ℜ⁡(s)≤32 as |ℑ⁡(s)|→∞,

∑n=1∞a⁢(n)⁢f⁢(n) =f⁢(0)⁢L⁢(a,0)+Ress=1⁢F⁢(s)⁢L⁢(a,s)+12⁢π⁢i⁢∫ℜ⁡(s)=-12F⁢(s)⁢L⁢(a,s)⁢𝑑s.

Define

G⁢(s)=F⁢(1-s)⁢γ⁢(s)γ⁢(1-s).

Using the functional equation for L⁢(a,s),

12⁢π⁢i⁢∫ℜ⁡(s)=-12F⁢(s)⁢L⁢(a,s)⁢𝑑s =12⁢π⁢i⁢∫ℜ⁡(s)=-12F⁢(s)⁢γ⁢(1-s)γ⁢(s)⁢L⁢(a,1-s)⁢𝑑s
=12⁢π⁢i⁢∫ℜ⁡(s)=32F⁢(1-s)⁢γ⁢(s)γ⁢(1-s)⁢L⁢(a,s)⁢𝑑s
=12⁢π⁢i⁢∫ℜ⁡(s)=32G⁢(s)⁢L⁢(a,s)⁢𝑑s.

Furthermore, define

J⁢(x)=12⁢π⁢i⁢∫ℜ⁡(s)=3211-s⁢γ⁢(s)γ⁢(1-s)⁢x1-s⁢𝑑s,

which satisfies

J′⁢(x)=K⁢(x).

We have

12⁢π⁢i⁢∫ℜ⁡(s)=32x-s⁢G⁢(s)⁢𝑑s =12⁢π⁢i⁢∫ℜ⁡(s)=32x-s⁢F⁢(1-s)⁢γ⁢(s)γ⁢(1-s)⁢𝑑s
=12⁢π⁢i⁢∫ℜ⁡(s)=32x-s⁢(-11-s⁢ℳ⁢(f′)⁢(2-s))⁢γ⁢(s)γ⁢(1-s)⁢𝑑s
=12⁢π⁢i⁢∫ℜ⁡(s)=32x-s⁢(-11-s⁢∫0∞y1-s⁢f′⁢(y)⁢𝑑y)⁢γ⁢(s)γ⁢(1-s)⁢𝑑s
=-1x⁢∫0∞f′⁢(y)⁢12⁢π⁢i⁢∫ℜ⁡(s)=3211-s⁢γ⁢(s)γ⁢(1-s)⁢(x⁢y)1-s⁢𝑑s
=-1x⁢∫0∞f′⁢(y)⁢J⁢(x⁢y)⁢𝑑y
=-1x⁢f⁢(y)⁢J⁢(x⁢y)|0∞+1x⁢∫0∞f⁢(y)⁢J′⁢(x⁢y)⁢x⁢𝑑y
=0+∫0∞f⁢(y)⁢J′⁢(x⁢y)⁢𝑑y
=∫0∞f⁢(y)⁢K⁢(x⁢y)⁢𝑑y
=g⁢(x).

Therefore,

∑n=1∞a⁢(n)⁢g⁢(n) =∑n=1∞a⁢(n)⁢12⁢π⁢i⁢∫ℜ⁡(s)=32n-s⁢G⁢(s)⁢𝑑s
=12⁢π⁢i⁢∫ℜ⁡(s)=32G⁢(s)⁢∑n=1∞a⁢(n)⁢n-s⁢d⁢s
=12⁢π⁢i⁢∫ℜ⁡(s)=32G⁢(s)⁢L⁢(a,s)⁢𝑑s.

Thus we have

∑n=1∞a⁢(n)⁢f⁢(n)=f⁢(0)⁢L⁢(a,0)+Ress=1⁢F⁢(s)⁢L⁢(a,s)+∑n=1∞a⁢(n)⁢g⁢(n)

∎

Take a⁢(n)=1 for all n. Then,

L⁢(a,s)=∑n=1∞n-s=ζ⁢(s).

The Riemann zeta function satisfies the functional equation

π-s/2⁢Γ⁢(s2)⁢ζ⁢(s)=π-(1-s)/2⁢Γ⁢(1-s2)⁢ζ⁢(1-s).

So with

γ⁢(s)=π-s/2⁢Γ⁢(s2),

we have

γ⁢(s)⁢ζ⁢(s)=γ⁢(1-s)⁢ζ⁢(1-s).

Using

Γ⁢(1-z)⁢Γ⁢(z)=πsin⁡π⁢z

and

Γ⁢(z)⁢Γ⁢(z+12)=21-2⁢z⁢π⁢Γ⁢(2⁢z),

we have

Γ⁢(1-s2) =Γ⁢(1-s+12)
=πsin⁡π⁢(s+1)2⁢Γ⁢(s+12)
=πsin⁡π⁢(s+1)2⁢Γ⁢(s2+12)
=π⁢Γ⁢(s2)sin⁡π⁢(s+1)2⁢21-s⁢π⁢Γ⁢(s),

and so

π-s/2⁢Γ⁢(s2)π-(1-s)/2⁢Γ⁢(1-s2) =π-s+12⁢Γ⁢(s2)⋅sin⁡π⁢(s+1)2⁢21-s⁢π⁢Γ⁢(s)π⁢Γ⁢(s2)
=sin⁡π⁢(s+1)2⋅2⁢(2⁢π)-s⁢Γ⁢(s)
=cos⁡π⁢s2⋅2⁢(2⁢π)-s⁢Γ⁢(s).

Therefore

K⁢(x)=12⁢π⁢i⁢∫ℜ⁡(s)=32γ⁢(s)γ⁢(1-s)⁢x-s⁢𝑑s=12⁢π⁢i⁢∫ℜ⁡(s)=32cos⁡π⁢s2⋅2⁢(2⁢π)-s⁢Γ⁢(s)⁢x-s⁢𝑑s

But, taking as known

∫0∞cos⁡(2⁢π⁢x)⁢xs-1⁢𝑑x=(2⁢π)-s⁢cos⁡π⁢s2⁢Γ⁢(s),

it follows that

K⁢(x)=2⁢cos⁡2⁢π⁢x.

Thus Theorem 1 tells us that for f∈𝒮⁢(ℝ),

∑n=1∞f⁢(n)=f⁢(0)⁢ζ⁢(0)+Ress=1⁢ℳ⁢(f)⁢(s)⁢ζ⁢(s)+2⁢∑n=1∞∫0∞f⁢(y)⁢cos⁡(2⁢π⁢n⁢y)⁢𝑑y,

i.e.,

∑n=1∞f⁢(n)=-12⁢f⁢(0)+∫0∞f⁢(x)⁢𝑑x+2⁢∑n=1∞∫0∞f⁢(y)⁢cos⁡(2⁢π⁢n⁢y)⁢𝑑y.

If f:ℝ→ℂ is even, this is the Poisson summation formula.

Take a⁢(n)=d⁢(n) for all n. Then,

L⁢(d,s)=∑n=1∞d⁢(n)⁢n-s=ζ2⁢(s).

For

γ⁢(s)=π-s⁢Γ⁢(s2)2,

it follows from the functional equation for the Riemann zeta function that L⁢(d,s) satisfies the functional equation

γ⁢(s)⁢L⁢(d,s)=γ⁢(1-s)⁢L⁢(d,1-s).

We worked out above that

π-s/2⁢Γ⁢(s2)π-(1-s)/2⁢Γ⁢(1-s2)=cos⁡π⁢s2⋅2⁢(2⁢π)-s⁢Γ⁢(s),

whence

γ⁢(s)γ⁢(1-s) =(2⁢π)-2⁢s⁢4⁢cos2⁡π⁢s2⁢Γ⁢(s)2
=(2⁢π)-2⁢s⁢(2+2⁢cos⁡π⁢s)⁢Γ⁢(s)2.

Taking as given two identities for Bessel functions

∫0∞xs-1⁢K0⁢(4⁢π⁢x1/2)⁢𝑑x=12⁢(2⁢π)-2⁢s⁢Γ⁢(s)2

and

∫0∞xs-1⁢Y0⁢(4⁢π⁢x1/2)⁢𝑑x=-1π⁢(2⁢π)-2⁢s⁢cos⁡π⁢s⁢Γ⁢(s)2,

it follows that

K⁢(x)=4⁢K0⁢(4⁢π⁢x1/2)-2⁢π⁢Y0⁢(4⁢π⁢x1/2).

Thus Theorem 1 tells us that for f∈𝒮⁢(ℝ),

∑n=1∞d⁢(n)⁢f⁢(n) =f⁢(0)⁢ζ2⁢(0)+Ress=1⁢ℳ⁢(f)⁢(s)⁢ζ2⁢(s)
+∑n=1∞d⁢(n)⁢∫0∞f⁢(y)⁢(4⁢K0⁢(4⁢π⁢(n⁢y)1/2)-2⁢π⁢Y0⁢(4⁢π⁢(n⁢y)1/2))⁢𝑑y.

Using

ζ2⁢(s)=1(s-1)2+2⁢γs-1+O⁢(1),s→1,

and

xs-1=1+(s-1)⁢log⁡x+O⁢(|s-1|2),

we have

Ress=1⁢ℳ⁢(f)⁢(s)⁢ζ2⁢(s)=2⁢γ+log⁡x,

and so

∑n=1∞d⁢(n)⁢f⁢(n) =14⁢f⁢(0)+∫0∞f⁢(x)⁢(2⁢γ+log⁡x)⁢𝑑x
+∑n=1∞d⁢(n)⁢∫0∞f⁢(y)⁢(4⁢K0⁢(4⁢π⁢(n⁢y)1/2)-2⁢π⁢Y0⁢(4⁢π⁢(n⁢y)1/2))⁢𝑑y.

3 Bernoulli numbers

The Bernoulli polynomials are defined by

t⁢et⁢xet-1=∑m=0∞Bm⁢(x)⁢tmm!.

The Bernoulli numbers are defined by Bm=Bm⁢(0).

We denote by [x] the greatest integer ≤x, and we define {x}=x-[x], namely, the fractional part of x. We define Pm⁢(x)=Bm⁢({x}), the Bernoulli functions.

4 Wigert

The following result is proved by Wigert [18]. Our proof follows Titchmarsh [13, p. 163, Theorem 7.15]. Cf. Landau [10].

Theorem 2.

For λ<12⁢π and N≥1,

∑n=1∞d⁢(n)⁢e-n⁢z=γz-log⁡zz+14-∑n=0N-1B2⁢n+22(2⁢n+2)!⁢(2⁢n+2)⁢z2⁢n+1+O⁢(|z|2⁢N)

as z→0 in any angle |arg⁡z|≤λ.

Proof.

For σ>1, s=σ+i⁢t,

ζ2⁢(s)=∑n=1∞d⁢(n)ns.

Using this, for ℜ⁡z>0 we have

12⁢π⁢i⁢∫2-i⁢∞2+i⁢∞Γ⁢(s)⁢ζ2⁢(s)⁢z-s⁢𝑑s =∑n=1∞d⁢(n)⁢12⁢π⁢i⁢∫2-i⁢∞2+i⁢∞Γ⁢(s)⁢(n⁢z)-s⁢𝑑s
=∑n=1∞d⁢(n)⁢e-n⁢z. (1)

Define F⁢(s)=Γ⁢(s)⁢ζs⁢(s)⁢z-s. F has poles at 1,0, and the negative odd integers. (At each negative even integer, Γ has a first order pole but ζ2 has a second order zero.) First we determine the residue of F at 1. We use the asymptotic formula

ζ⁢(s)=1s-1+γ+O⁢(|s-1|),s→1,

the asymptotic formula

Γ⁢(s)=1-γ⁢(s-1)+O⁢(|s-1|2),s→1,

and the asymptotic formula

z-s=1z-log⁡zz⁢(s-1)+O⁢(|s-1|2),s→1,

to obtain

Γ⁢(s)⁢ζs⁢(s)⁢z-s =(1-γ⁢(s-1)+O⁢(|s-1|2))⋅(1(s-1)2+2⁢γs-1+O⁢(|s-1|2))
⋅(1z-log⁡zz⁢(s-1)+O⁢(|s-1|2))
=1z⁢(s-1)2-γz⁢(s-1)+2⁢γz⁢(s-1)-log⁡zz⁢(s-1)+O⁢(1)
=1z⁢(s-1)2+γz⁢(s-1)-log⁡zz⁢(s-1)+O⁢(1).

Hence the residue of F at 1 is

γz-log⁡zz.

Now we determine the residue of F at 0. The residue of Γ at 0 is 1, and hence the residue of F at 0 is

1⋅ζ2⁢(0)⋅z0=ζ2⁢(0)=(-12)2=14.

Finally, for n≥0 we determine the residue of F at -(2⁢n+1). The residue of Γ at -(2⁢n+1) is (-1)2⁢n+1(2⁢n+1)!, hence the residue of F at -(2⁢n+1) is

(-1)2⁢n+1(2⁢n+1)!⋅ζ2⁢(2⁢n+1)⋅z2⁢n+1=-B2⁢n+22(2⁢n+2)!⁢(2⁢n+2)⁢z2⁢n+1

using

ζ⁢(-m)=-Bm+1m+1,m≥1.

Let M>0, and let C be the rectangular path starting at 2-i⁢M, then going to 2+i⁢M, then going to -2⁢N+i⁢M, then going to -2⁢N-i⁢M, and then ending at 2-i⁢M. By the residue theorem,

∫CF⁢(s)⁢𝑑s=2⁢π⁢i⁢(γz-log⁡zz+14+∑n=0N-1-B2⁢n+22(2⁢n+2)!⁢(2⁢n+2)⁢z2⁢n+1). (2)

Denote the right-hand sideof (2) by 2⁢π⁢i⁢R. We have

∫CF⁢(s)⁢𝑑s=∫2-i⁢M2+i⁢MF⁢(s)⁢𝑑s+∫2+i⁢M-2⁢N+i⁢MF⁢(s)⁢𝑑s+∫-2⁢N+i⁢M-2⁢N-i⁢MF⁢(s)⁢𝑑s+∫-2⁢N-i⁢M2-i⁢MF⁢(s)⁢𝑑s.

We shall show that the second and fourth integrals tend to 0 as M→∞. For s=σ+i⁢t with -2⁢N≤σ≤2, Stirling’s formula [14, p. 151] tells us that

|Γ⁢(s)|∼2⁢π⁢e-π2⁢|t|⁢|t|σ-12,|t|→∞.

As well [13, p. 95], there is some K>0 such that in the half-plane σ≥-2⁢N,

ζ⁢(s)=O⁢(|t|K).

Also,

z-s =e-s⁢log⁡z
=e-(σ+i⁢t)⁢(log⁡|z|+i⁢arg⁡z)
=e-σ⁢log⁡|z|+t⁢arg⁡z-i⁢(σ⁢arg⁡z+t⁢log⁡|z|),

and so for |arg⁡z|≤λ,

|z-s|=e-σ⁢log⁡|z|+t⁢arg⁡z≤e-σ⁢log⁡|z|+λ⁢|t|=|z|-σ⁢eλ⁢|t|.

Therefore

|∫2+i⁢M-2⁢N+i⁢MF⁢(s)⁢𝑑s|≤(2+2⁢N)⁢sup-2⁢N≤σ≤2⁡|F⁢(σ+i⁢M)|=O⁢(e-π2⁢M⁢Mσ-12⁢M2⁢K⁢|z|-σ⁢eλ⁢M),

and because λ<π2 this tends to 0 as M→∞. Likewise,

|∫-2⁢N-i⁢M2-i⁢MF⁢(s)⁢𝑑s|→0

as M→∞. It follows that

∫2-i⁢∞2+i⁢∞F⁢(s)⁢𝑑s+∫-2⁢N+i⁢∞-2⁢N-i⁢∞F⁢(s)⁢𝑑s=2⁢π⁢i⁢R.

Hence,

∫2-i⁢∞2+i⁢∞F⁢(s)⁢𝑑s=2⁢π⁢i⁢R+∫-2⁢N-i⁢∞-2⁢N+i⁢∞F⁢(s)⁢𝑑s.

We bound the integral on the right-hand side. We have

∫-2⁢N-i⁢∞-2⁢N+i⁢∞F⁢(s)⁢𝑑s=∫σ=-2⁢N,|t|≤1F⁢(s)⁢𝑑s+∫σ=-2⁢N,|t|>1F⁢(s)⁢𝑑s.

The first integral satisfies

|∫σ=-2⁢N,|t|≤1F⁢(s)⁢𝑑s|≤∫σ=-2⁢N,|t|≤1|Γ⁢(s)⁢ζ2⁢(s)|⁢|z|-σ⁢eλ⁢|t|⁢𝑑s=|z|2⁢N⋅O⁢(1)=O⁢(|z|2⁢N),

because Γ⁢(s)⁢ζ2⁢(s) is continuous on the path of integration. The second integral satisfies

|∫σ=-2⁢N,|t|>1F⁢(s)⁢𝑑s| ≤∫σ=-2⁢N,|t|>1e-π2⁢|t|⁢|t|σ-12⁢|t|K⁢|z|-σ⁢eλ⁢|t|⁢𝑑s
=|z|2⁢N⁢∫σ=-2⁢N,|t|>1e-π2⁢|t|⁢|t|-2⁢N-12⁢|t|K⁢eλ⁢|t|⁢𝑑t
=|z|2⁢N⋅O⁢(1)
=O⁢(|z|2⁢N),

because λ<π2. This establishes

12⁢π⁢i⁢∫2-i⁢∞2+i⁢∞F⁢(s)⁢𝑑s=R+O⁢(|z|2⁢N).

Using (1) and (2), this becomes

∑n=1∞d⁢(n)⁢e-n⁢z=γz-log⁡zz+14-∑n=0N-1B2⁢n+22(2⁢n+2)!⁢(2⁢n+2)⁢z2⁢n+1+O⁢(|z|-2⁢N),

completing the proof. ∎

For example, as B2=16,B4=-130,B6=142, the above theorem tells us that

∑n=1∞d⁢(n)⁢e-n⁢z=γz-log⁡zz+14-z144-z386400-z57620480+O⁢(|z|6).

5 Other works on the Voronoi summation formula

Voronoi’s papers on the Voronoi summation formula are [15] and [17] and [16].

Iwaniec and Kowalski [9, Chaper 4]

Stein and Shakarchi [12, p. 392, Theorem 8.11].

Ivic [8, pp. 83ff., Chapter 3] and [7]

Miller and Schmid [11]

Hejhal [6]

Flajolet, Gourdon and Dumas [5]

Bettin and Conrey [1]

Chandrasekharan and Narasimhan [2]

Chandrasekharan [3, Chapter VIII]

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