Lambert series in analytic number theory

Jordan Bell
[email protected]
(February 22, 2023)
Abstract

Tour of 19th and early 20th century analytic number theory.

1 Introduction

Let d⁢(n) denote the number of positive divisors of n. For |z|<1,

∑n=1∞d⁢(n)⁢zn=∑n=1∞zn1-zn.

2 Euler

The first use of the term “Lambert series” was by Euler to describe the roots of an equation.

Euler writes in E25 [28] about the particular value of a Lambert series.

3 Lambert

Bullynck [7, pp. 157–158]: “As he recorded in his scientific diary, the Monatsbuch, Lambert started thinking about the divisors of integers in June 1756. An essay by G.W. Krafft (1701–1754) in the St. Petersburg Novi Commentarii seems to have triggered Lambert’s interest [Bopp 1916, p. 17, 40].”

Bullynck [7, p. 163]:

Lambert did more than deliver the factor table. He also addressed the absence of any coherent theory of prime numbers and divisors. Filling such a lacuna could be important for the discovery of new and more primality criteria and factoring tests. For Lambert the absence of such a theory was also an occasion to apply the principles laid out in his philosophical work. A fragmentary theory, or one with gaps, needed philosophical and mathematical efforts to mature.

To this aim [prime recognition] and others I have looked into the theory of prime numbers, but only found certain isolated pieces, which did not seem possible to make easily into a connected and well formed system. Euclid has few, Fermat some mostly unproven theorems, Euler individual fragments, that anyway are farther away from the first beginnings, and leave gaps between them and the beginnings. [Lambert 1770, p. 20]

Bullynck [7, pp. 164–165]:

In 1770, Lambert presented two sketches of what would be needed for something like a theory of numbers. The first dealt mainly with factoring methods [Lambert 1765-1772, II, pp. 1–41], while the second gave a more axiomatic treatment [Lambert 1770, pp. 20–48]. In the first essay, Lambert explained how, for composite number with small factors, Eratosthenes’ sieve could be used and optimised. For larger factors, Lambert explained that approximation from above, starting by division by numbers that are close to the square root of the tested number p, was more advantageous. For both methods, Lambert advised the use of tables. The second essay had more theoretical bearings. Lambert rephrased Euclid’s theorems for use in factoring, included the greatest common divisor algorithm, and put the idea of relatively prime numbers to good use. He also noted that binary notation, because of the frequent symmetries, could be helpful. Finally,Lambert also recognized Fermat’s little theorem as a good, though not infallible criterion for primality, “but the negative example is very rar” [Lambert 1770, p. 43].

Monatsbuch, September 1764, “Singula haec in Capp. ult. Ontol. occurunt”, and Anm. 5, Anm. 25, 1764, Anm. 12 1765, Anm. 19, 1765 [2].

Lambert [53, pp. 506–511, §875]

Youschkevitch [87]

Lorey [59, p. 23]

Löwenhaupt [60, p. 32]

4 Krafft

Krafft [50, pp. 244–245]

5 Servois

Servois [72] and [73, p. 166]

6 Lacroix

Lacroix [51, pp. 465–466, §1195]

7 Klügel

Klügel [46, pp. 52–53, s.v. “Theiler einer Zahl”, §12]:

Ist N=αm⁢βn⁢γp⁢⋯, wo α,β,γ, Primzahlen sind; so erhellet auch leicht, daßalle Theiler von N, die Einheit und die Zahl selbst mit engeschlossen, durch die Glieder des Products

(1+α+α2+⋯+αm)⁢(1+β+β2+⋯+βn)⁢(1+γ+γ2+⋯+γp)⁢⋯

argestelle werden. Die Anzahl der Glieder dieses Products, d. i. die Anzahl aller Theiler von N, ist offenbar =(m+1)⁢(n+1)⁢(p+1)⁢⋯. Für das obige Beispiel =4⋅3⋅2=24, wo die Einheit mit engeschlossen ist.
In der aus der Entwickelung von

x1-x+x21-x2+x31-x3+⋯+xn1-xn+⋯

entspringenden Reihe:

x+2⁢x2+2⁢x3+3⁢x4+2⁢x5+4⁢x6+2⁢x7+⋯

welche Lambert in seiner Architektonik S. 507. mittheilt, enthalt jeder Coefficient so viele Einheiten, als der Exponent der entsprechendenden Potenz von x Theiler hat.

8 Stern

Stern [77]

9 Clausen

Clausen [21] states that

∑n=1∞xn1-xn=∑n=1∞xn2⁢(1+xn1-xn),

and that the right-hand series converges quickly for small x. Clausen does prove this expansion, and a proof is later given by Scherk [68]. Scherk’s argument uses the fact

1+2⁢t+2⁢t2+2⁢t3+2⁢t4+⋯=(1+t+t2+t3+t4+⋯)+t⁢(1+t+t2+t3+t4+⋯)=1+t1-t.

We write

∑n=1∞xn1-xn=∑n=1∞∑m=1∞xn⁢m.

The series is

x+x2+x3+x4+x5+x6+etc.+x2+x4+x6+x8+x10+x12+etc.+x3+x6+x9x12+x15+x18+etc.+x4+x8+x12+x16+x20+x24+etc.+x5+x10+x15+x20+x25+x30+etc.+x6+x12+x18+x24+x30+x36+etc.+etc.

We sum the terms in the first row and column: the sum of these is

x+2x2+2x3+2x4+etc.=x(1+x1-x).

Then, from what remains we sum the terms in the second row and column: the sum of these is

x4+2x6+2x8+2x10+etc.=x4(1+x21-x2).

Then, from what remains, we sum the terms in the third row and column: the sum of these is

x9+2x12+2x15+2x18+etc.=x9(1+x31-x3),

etc.

10 Eisenstein

Eisenstein [27] states that for |z|<1,

∑n=1∞zn1-zn=1(1-x)⁢(1-x2)⁢(1-x3)⁢⋯⁢∑n=1∞(-1)n+1⁢n⁢zn⁢(n+1)/2(1-x)⁢⋯⁢(1-xn).

For t=1z, Eisenstein states that

z1-z+z21-z2+z31-z3+z41-z4+etc.

is equal to

1t-1-(t-1)2t2-1-t⁢(t-1)2t3-1-t⁢(t2-1)2t4-1-t2⁢(t2-1)2t5-1-t2⁢(t3-1)2t6-1-t3⁢(t3-1)2t7-1-etc.

Expressing Lambert series using continued fractions is relevant to the irrationality of the value of the series. See Borwein [3]. See also Zudilin [90].

11 Möbius

Möbius [62]

12 Jacobi

Jacobi’s Fundamenta nova [44, §40, 66 and p. 185]

Chandrasekharan [20, Chapter X]: using Lambert series to prove the four squares theorem.

13 Dirichlet

Dirichlet [25]

Fischer [29]

14 Cauchy

Cauchy [13] and [14] two memoirs in the same volume.

15 Burhenne

Burhenne [8] says the following about Lambert series. For

F⁢(x)=∑n=1∞d⁢(n)⁢xn,

we have

d⁢(n)=F(n)⁢(0)n!.

Define

Fk⁢(x)=xk1-xk,

so that

F⁢(x)=∑k=1∞Fk⁢(x).

It is apparent that if k>n, then

Fk(n)⁢(0)=0,

hence

F(n)⁢(0)=∑k=1nFk(n)⁢(0).

The above suggests finding explicit expressions for Fk(n)⁢(0). Burhenne cites Sohncke [74, pp. 32–33]: for even k,

dn⁢(xpxk-ak)d⁢xn =(-1)n⁢n!k⁢ak-p-1⁢(1(x-a)n+1-(-1)p⁢1(x+a)n+1)
+(-1)n⁢n!12⁢k⁢ak-p-1⁢∑h=112⁢k-1cos⁡(2⁢h⁢(p+1)⁢πk+(n+1)⁢ϕh)(x2-2⁢x⁢a⁢cos⁡2⁢h⁢πn+a2)n+1

and for odd k,

dn⁢(xpxk-ak)d⁢xn =(-1)n⁢n!k⁢ak-p-1⁢1(x-a)n+1
+(-1)n⁢n!12⁢k⁢ak-p-1⁢∑h=1k-12cos⁡(2⁢h⁢(p+1)⁢πk+(n+1)⁢ϕh)(x2-2⁢x⁢a⁢cos⁡2⁢h⁢πn+a2)n+1,

where

cos⁡ϕh=x-a⁢cos⁡2⁢h⁢πkx2-2⁢x⁢a⁢cos⁡2⁢h⁢πk+a2,sin⁡ϕh=a⁢sin⁡2⁢h⁢πkx2-2⁢x⁢a⁢cos⁡2⁢h⁢πk+a2.

For a=1 and x=0,

cos⁡ϕh=-cos⁡2⁢h⁢πk,sin⁡ϕh=sin⁡2⁢h⁢πk,

from which

ϕh=π-2⁢h⁢πk,

and thus

cos⁡(2⁢h⁢(k+1)⁢πk+(n+1)⁢ϕh) =cos⁡(2⁢h⁢(k+1)⁢πk+(n+1)⁢(π-2⁢h⁢πk))
=cos⁡(2⁢h⁢π+2⁢h⁢πk+π-2⁢h⁢πk+n⁢(π-2⁢h⁢πk))
=cos⁡((n+1)⁢π-2⁢n⁢h⁢πk)
=(-1)n+1⁢cos⁡2⁢n⁢h⁢πk.

For even k, taking p=k we have

dn⁢(xk1-xk)d⁢xn=(-1)n+1⁢n!k⁢(1(-1)n+1-1)+(-1)n+1⁢n!12⁢k⁢∑h=112⁢k-1(-1)n+1⁢cos⁡2⁢n⁢h⁢πk,

i.e.,

Fk(n)⁢(0)=n!k⁢(1-(-1)n+1)+2⋅n!k⁢∑h=112⁢k-1cos⁡2⁢n⁢h⁢πk.

For odd k, taking p=k we have

dn⁢(xk1-xk)d⁢xn=(-1)n+1⁢n!k⁢1(-1)n+1+(-1)n+1⁢n!12⁢k⁢∑h=1k-12(-1)n+1⁢cos⁡2⁢n⁢h⁢πk,

i.e.,

Fk(n)⁢(0)=n!k+2⋅n!k⁢∑h=1k-12cos⁡2⁢n⁢h⁢πk.

Using the identity, for h∉2⁢π⁢ℤ,

∑h=1Mcos⁡h⁢θ=-12+sin⁡(M+12)⁢θ2⁢sin⁡θ2=-12+12⁢(sin⁡M⁢θ⁢cot⁡θ2+cos⁡M⁢θ),

we get for even k,

Fk(n)⁢(0) ={n!k⁢cot⁡n⁢πk⁢sin⁡n⁢πk|̸nn!k⁢(1-(-1)n+1)+2⋅n!k⁢(12⁢k-1)k|n
={0k|̸nn!-n!k⁢(1+(-1)n+1)k|n.

For odd k,

Fk(n)⁢(0) ={n!k⁢csc⁡n⁢πk⁢sin⁡n⁢πk|̸nn!k+2⋅n!k⁢k-12k|n.
={0k|̸nn!k|n.

16 Zehfuss

Zehfuss [88]

17 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 periodic Bernoulli functions.

18 Euler-Maclaurin summation formula

Euler E47 and E212, §142, for the summation formula. Euler’s studies the gamma function in E368. In particular, in §12 he gives Stirling’s formula, and in §14 he obtains Γ′⁢(1)=-γ. Euler in §142 of E212 states that

γ=12+∑n=1∞(-1)n+1⁢B2⁢n2⁢n.

Bromwich [6, Chapter XII]

The Euler-Maclaurin summation formula [5, p. 280, Ch. VI, Eq. 35] tells us that for f∈C∞⁢([0,1]),

f⁢(0)=∫01f⁢(t)⁢𝑑t+B1⁢(f⁢(1)-f⁢(0))+∑m=1k1(2⁢m)!⁢B2⁢m⁢(f(2⁢m-1)⁢(1)-f(2⁢m-1)⁢(0))+R2⁢k,

where

R2⁢k=-∫01P2⁢k⁢(1-η)(2⁢k)!⁢f(2⁢k)⁢(η)⁢𝑑η.

Poisson and Jacobi on the Euler-Maclaurin summation formula.

19 Schlömilch

Schlömilch [69] and [71, p. 238], [70]

For m≥1,

∫0∞t2⁢m-1e2⁢π⁢t-1⁢𝑑t=(-1)m+1⁢B2⁢m4⁢m. (1)

For α>0,

∫0∞sin⁡α⁢te2⁢π⁢t-1⁢𝑑t=14+12⁢(1eα-1-1α) (2)

and

∫0∞1-cos⁡α⁢te2⁢π⁢t-1⁢d⁢tt=14⁢α+12⁢(log⁡(1-e-α)-log⁡α). (3)

For ξ>0 and n≥1, using (2) with α=ξ,2⁢ξ,3⁢ξ,…,2⁢n⁢ξ and also using

∑k=1Nsin⁡k⁢θ=12⁢cot⁡θ2-cos⁡(N+12)⁢θ2⁢sin⁡θ2,

we get

∑m=12⁢n(1em⁢ξ-1-1m⁢ξ) =∑m=12⁢n(-12+2⁢∫0∞sin⁡m⁢ξ⁢te2⁢π⁢t-1⁢𝑑t)
=-n+∫0∞1e2⁢π⁢t-1⁢∑m=12⁢n2⁢sin⁡m⁢ξ⁢t⁢d⁢t
=-n+∫0∞1e2⁢π⁢t-1⁢(cot⁡ξ⁢t2-cos⁡(2⁢n+12)⁢ξ⁢tsin⁡ξ⁢t2)⁢𝑑t.

Using cos⁡(a+b)=cos⁡a⁢cos⁡b-sin⁡a⁢sin⁡b, this becomes

∑m=12⁢n(1em⁢ξ-1-1m⁢ξ) =-n+∫0∞1e2⁢π⁢t-1⁢(1-cos⁡2⁢n⁢ξ⁢t)⁢cot⁡ξ⁢t2⁢d⁢t (4)
+∫0∞1e2⁢π⁢t-1⁢sin⁡2⁢n⁢ξ⁢t⁢d⁢t.

For α=2⁢n⁢ξ, (3) tells us

∫0∞1-cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢d⁢tt=14⋅2⁢n⁢ξ+12⁢(log⁡(1-e-2⁢n⁢ξ)-log⁡2⁢n⁢ξ).

Rearranging,

log⁡2⁢nξ=n+log⁡(1-e-2⁢n⁢ξ)-log⁡ξξ-2ξ⁢∫0∞1-cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢d⁢tt (5)

Adding (4) and (5) gives

∑m=12⁢n1em⁢ξ-1-1ξ⁢(-log⁡2⁢n+∑m=12⁢n1m)=log⁡(1-e-2⁢n⁢ξ)-log⁡ξξ-∫0∞(2ξ⁢t-cot⁡ξ⁢t2)⁢1-cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢𝑑t+∫0∞1e2⁢π⁢t-1⁢sin⁡2⁢n⁢ξ⁢t⁢d⁢t.

Writing

Cn=-log⁡n+∑m=1n1m

and using (2) this becomes

∑m=12⁢n1em⁢ξ-1-1ξ⁢C2⁢n=log⁡(1-e-2⁢n⁢ξ)-log⁡ξξ-2⁢∫0∞(1ξ⁢t-12⁢cot⁡ξ⁢t2)⁢1-cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢𝑑t+14+12⁢(1e2⁢n⁢ξ-1-12⁢n⁢ξ).

We write

I2⁢n⁢(ξ)=2⁢∫0∞(1ξ⁢t-12⁢cot⁡ξ⁢t2)⁢1-cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢𝑑t,

and we shall obtain an asymptotic formula for I2⁢n⁢(ξ).

We apply the Euler-Maclaurin summation formula. Let h>0, and for f⁢(t)=cos⁡h⁢t we have f′⁢(t)=-h⁢sin⁡h⁢t, and for m≥1 we have f(2⁢m)⁢(t)=(-1)m⁢h2⁢m⁢cos⁡h⁢t and f(2⁢m-1)⁢(t)=(-1)m⁢h2⁢m-1⁢sin⁡h⁢t. Thus the Euler-Maclaurin formula yields

1=∫01cos⁡h⁢t⁢d⁢t-12⁢(cos⁡h-1)+∑m=1k1(2⁢m)!⁢B2⁢m⁢(-1)m⁢h2⁢m-1⁢sin⁡h+R2⁢k.

Using the identity cot⁡θ2=1+cos⁡θsin⁡θ and dividing by sin⁡h, this becomes

12⁢cot⁡h2=1h+∑m=1k1(2⁢m)!⁢B2⁢m⁢(-1)m⁢h2⁢m-1+1sin⁡h⁢R2⁢k. (6)

Because Pm⁢(1-η)=Pm⁢(η) for even m,

R2⁢k =-∫01P2⁢k⁢(η)(2⁢k)!⁢(-1)k⁢h2⁢k⁢cos⁡h⁢η⁢d⁢η
=-B2⁢k⁢∫011(2⁢k)!⁢(-1)k⁢h2⁢k⁢cos⁡h⁢η⁢d⁢η-∫01(P2⁢k⁢(η)-B2⁢k)(2⁢k)!⁢(-1)k⁢h2⁢k⁢cos⁡h⁢η⁢d⁢η
=(-1)k+1⁢B2⁢k⁢h2⁢k(2⁢k)!⁢sin⁡hh+(-1)k+1⁢h2⁢k(2⁢k)!⁢∫01(P2⁢k⁢(η)-B2⁢k)⁢cos⁡h⁢η⁢d⁢η.

Since P2⁢k⁢(η)-B2⁢k does not change sign on (0,1), by the mean-value theorem for integration there is some θ=θ⁢(h,k), 0<θ<1, such that (using ∫01P2⁢k⁢(η)⁢𝑑η=0)

∫01(P2⁢k⁢(η)-B2⁢k)⁢cos⁡h⁢η⁢d⁢η=cos⁡h⁢θ⁢∫01(P2⁢k⁢(η)-B2⁢k)⁢𝑑η=-B2⁢k⁢cos⁡h⁢θ.

Therefore (6) becomes

12⁢cot⁡h2-1h =∑m=1k1(2⁢m)!⁢B2⁢m⁢(-1)m⁢h2⁢m-1
+(-1)k+1⁢B2⁢k⁢h2⁢k-1(2⁢k)!+(-1)k+2⁢h2⁢k(2⁢k)!⁢sin⁡h⁢B2⁢k⁢cos⁡h⁢θ,

i.e.,

12⁢cot⁡h2-1h=∑m=1k-11(2⁢m)!⁢B2⁢m⁢(-1)m⁢h2⁢m-1+(-1)k⁢h2⁢k(2⁢k)!⁢sin⁡h⁢B2⁢k⁢cos⁡h⁢θ.

Write

Ek⁢(h)=(-1)k+1⁢h2⁢k(2⁢k)!⁢sin⁡h⁢B2⁢k⁢cos⁡h⁢θ.

We apply the above to I2⁢n⁢(ξ), and get, for any k≥1,

I2⁢n⁢(ξ) =2⁢∫0∞(Ek⁢(ξ⁢t)-∑m=1k-11(2⁢m)!⁢B2⁢m⁢(-1)m⁢(ξ⁢t)2⁢m-1)⁢1-cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢𝑑t
=-2⁢∑m=1k-11(2⁢m)!⁢B2⁢m⁢(-1)m⁢ξ2⁢m-1⁢∫0∞t2⁢m-1⁢1-cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢𝑑t
+2⁢∫0∞Ek⁢(ξ⁢t)⁢1-cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢𝑑t.

Using (1),

∫0∞t2⁢m-1⁢1-cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢𝑑t =∫0∞t2⁢m-1e2⁢π⁢t-1⁢𝑑t-∫0∞t2⁢m-1⁢cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢𝑑t
=(-1)m+1⁢B2⁢m4⁢m-∫0∞t2⁢m-1⁢cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢𝑑t.

Let

f⁢(x)=1ex-1-1x.

By (2),

f⁢(x)+12=2⁢∫0∞sin⁡x⁢te2⁢π⁢t-1⁢𝑑t.

For m≥1,

f(2⁢m-1)⁢(x)=2⁢∫0∞(-1)m-1⁢t2⁢m-1⁢cos⁡x⁢te2⁢π⁢t-1⁢𝑑t,

which for x=2⁢n⁢ξ becomes

(-1)m-12⁢f(2⁢m-1)⁢(2⁢n⁢ξ)=∫0∞t2⁢m-1⁢cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢𝑑t.

Therefore

2⁢∫0∞t2⁢m-1⁢1-cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢𝑑t=(-1)m+1⁢B2⁢m2⁢m+(-1)m⁢f(2⁢m-1)⁢(2⁢n⁢ξ).

Thus I2⁢n⁢(ξ) is

I2⁢n⁢(ξ) =-∑m=1k-11(2⁢m)!⁢B2⁢m⁢(-1)m⁢ξ2⁢m-1⁢((-1)m+1⁢B2⁢m2⁢m+(-1)m⁢f(2⁢m-1)⁢(2⁢n⁢ξ))
+2⁢∫0∞Ek⁢(ξ⁢t)⁢1-cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢𝑑t
=∑m=1k-1B2⁢m2(2⁢m)!⁢2⁢m⁢ξ2⁢m-1-∑m=1k-1B2⁢m(2⁢m)!⁢ξ2⁢m-1⁢f(2⁢m-1)⁢(2⁢n⁢ξ)
+2⁢∫0∞Ek⁢(ξ⁢t)⁢1-cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢𝑑t.

But

|∫0∞Ek⁢(ξ⁢t)⁢1-cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢𝑑t| =|∫0∞(-1)k+1⁢(ξ⁢t)2⁢k(2⁢k)!⁢sin⁡ξ⁢t⁢B2⁢k⁢cos⁡ξ⁢t⁢θ⁢1-cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢d⁢t|
≤|B2⁢k|(2⁢k)!⁢∫0∞(ξ⁢t)2⁢k|sin⁡ξ⁢t|⁢1-cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢𝑑t.

It is a fact that for all u∈ℝ,

1-cos⁡2⁢n⁢u|sin⁡u|≤π2⁢1-cos⁡2⁢n⁢uu,

we obtain

|∫0∞Ek⁢(ξ⁢t)⁢1-cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢𝑑t|≤π2⁢|B2⁢k|(2⁢k)!⁢∫0∞(ξ⁢t)2⁢k-1⁢1-cos⁡2⁢n⁢ξ⁢te2⁢π⁢t-1⁢𝑑t=π2⁢|B2⁢k|(2⁢k)!⁢ξ2⁢k-1⋅12⁢((-1)k+1⁢B2⁢k2⁢k+(-1)k⁢f(2⁢k-1)⁢(2⁢n⁢ξ)).

Hence

I2⁢n⁢(ξ) =∑m=1k-1B2⁢m2(2⁢m)!⁢2⁢m⁢ξ2⁢m-1-∑m=1k-1B2⁢m(2⁢m)!⁢ξ2⁢m-1⁢f(2⁢m-1)⁢(2⁢n⁢ξ)
+O⁢(B2⁢k2(2⁢k)!⁢2⁢k⁢ξ2⁢k-1)+O⁢(|B2⁢k|(2⁢k)!⁢ξ2⁢k-1⁢f(2⁢k-1)⁢(2⁢n⁢ξ)).

Therefore we have

∑m=12⁢n1em⁢ξ-1-1ξ⁢C2⁢n=log⁡(1-e-2⁢n⁢ξ)-log⁡ξξ+14+12⁢(1e2⁢n⁢ξ-1-12⁢n⁢ξ)-I2⁢n⁢(ξ)=log⁡(1-e-2⁢n⁢ξ)-log⁡ξξ+14+12⁢(1e2⁢n⁢ξ-1-12⁢n⁢ξ)-∑m=1k-1B2⁢m2(2⁢m)!⁢2⁢m⁢ξ2⁢m-1+∑m=1k-1B2⁢m(2⁢m)!⁢ξ2⁢m-1⁢f(2⁢m-1)⁢(2⁢n⁢ξ)+O⁢(B2⁢k2(2⁢k)!⁢2⁢k⁢ξ2⁢k-1)+O⁢(|B2⁢k|(2⁢k)!⁢ξ2⁢k-1⁢f(2⁢k-1)⁢(2⁢n⁢ξ)).

Taking n→∞,

∑m=1∞1em⁢ξ-1-γξ=-log⁡ξξ+14-∑m=1k-1B2⁢m2(2⁢m)!⁢2⁢m⁢ξ2⁢m-1+O⁢(B2⁢k2(2⁢k)!⁢2⁢k⁢ξ2⁢k-1).

20 Voronoi summation formula

The Voronoi summation formula [22, p. 182] states that if f:ℝ→ℂ is a Schwartz function, then

∑n=1∞d⁢(n)⁢f⁢(n) =∫0∞f⁢(t)⁢(log⁡t+2⁢γ)⁢𝑑t+f⁢(0)4
+∑n=1∞d⁢(n)⁢∫0∞f⁢(t)⁢(4⁢K0⁢(4⁢π⁢(n⁢t)1/2)-2⁢π⁢Y0⁢(4⁢π⁢(n⁢t)1/2))⁢𝑑t,

where K0 and Y0 are Bessel functions.

Let 0<x<1. For f⁢(t)=e-t⁢x, we compute

∫0∞f⁢(t)⁢(4⁢K0⁢(4⁢π⁢(n⁢t)1/2)-2⁢π⁢Y0⁢(4⁢π⁢(n⁢t)1/2))⁢𝑑t=-2x⁢exp⁡(4⁢π2⁢nx)⁢Ei⁢(-4⁢π2⁢nx)-2x⁢exp⁡(-4⁢π2⁢nx)⁢Ei⁢(4⁢π2⁢nx),

where

Ei⁢(x)=-∫-x∞e-tt⁢𝑑t,x≠0,

the exponential integral. Then the Voronoi summation formula yields

∑n=1∞d⁢(n)⁢e-n⁢x=γx-log⁡xx+14+∑n=1∞d⁢(n)⁢(-2x⁢exp⁡(4⁢π2⁢nx)⁢Ei⁢(-4⁢π2⁢nx)-2x⁢exp⁡(-4⁢π2⁢nx)⁢Ei⁢(4⁢π2⁢nx)).

Egger and Steiner [26] give a proof of the Voronoi summation formula involving Lambert series.

Kluyver [47] and [48]

Guinand [36]

21 Curtze

Curtze [23]

22 Laguerre

Laguerre [52]

23 V. A. Lebesgue

V. A. Lebesgue [56]:

24 Bouniakowsky

Bouniakowsky [4]

25 Chebyshev

Chebyshev [80]

26 Catalan

Catalan [9]

Catalan [10, p. 89]

Catalan [11, p. 119, §CXXIV] and [12, pp. 38–39, §CCXXVI]

27 Pincherle

Pincherle [63]

28 Glaisher

Glaisher [34, p. 163]

29 Günther

Günther [37, p. 83] and [38, p. 178]

30 Stieltjes

Stieltjes [78]

cf. Zhang [89]

31 Rogel

Rogel [65] and [66]

32 Cesàro

Cesàro [15]

Cesàro [16]

Cesàro [17] and [18, pp. 181–184]

Bromwich [6, p. 201, Chapter VIII, Example B, 35]

33 de la Vallée-Poussin

de la Vallée-Poussin [24]

34 Torelli

Torelli [83]

35 Fibonacci numbers

Landau [54]

36 Knopp

Knopp [49]

37 Generating functions

Hardy and Wright [40, p. 258, Theorem 307]:

Theorem 1.

For f⁢(s)=∑n=1∞an⁢n-s and g⁢(s)=∑n=1∞bn⁢n-s,

∑n=1∞an⁢xn1-xn=∑n=1∞bn⁢xn,|x|<1,

if and only if there is some σ such that

ζ⁢(s)⁢f⁢(s)=g⁢(s),Re⁢(s)>σ.

For f⁢(s)=∑n=1∞μ⁢(n)⁢n-s and g⁢(s)=1, using [40, p. 250, Theorem 287]

1ζ⁢(s)=∑n=1∞μ⁢(n)⁢n-s,Re⁢(s)>1,

we get

∑n=1∞μ⁢(n)⁢xn1-xn=x. (7)

For f⁢(s)=∑n=1∞ϕ⁢(n)⁢n-s and

g⁢(s)=ζ⁢(s-1)=∑n=1∞n-s+1=∑n=1∞n⁢n-s,

using [40, p. 250, Theorem 288]

ζ⁢(s-1)ζ⁢(s)=∑n=1∞ϕ⁢(n)⁢n-s,Re⁢(s)>2,

we get

∑n=1∞ϕ⁢(n)⁢xn1-xn=∑n=1∞n⁢xn=x(1-x)2.

For n=p1a1⁢⋯⁢prar, define Ω⁢(n)=a1+⋯+an and

λ⁢(n)=(-1)Ω⁢(n).

For f⁢(s)=∑n=1∞λ⁢(n)⁢n-s and

g⁢(s)=ζ⁢(2⁢s)=∑n=1∞n-2⁢s=∑n=1∞(n2)-s,

using [40, p. 255, Theorem 300]

ζ⁢(2⁢s)ζ⁢(s)=∑n=1∞λ⁢(n)⁢n-s,Re⁢(s)>1,

we get

∑n=1∞λ⁢(n)⁢xn1-xn=∑n=1∞xn2.

We define the von Mangoldt function Λ:ℕ→ℝ by Λ⁢(n)=log⁡p if n is some positive integer power of a prime p, and Λ⁢(n)=0 otherwise. For example, Λ⁢(1)=0, Λ⁢(12)=0, Λ⁢(125)=log⁡5. It is a fact [40, p. 254, Theorem 296] that for any n, the von Mangoldt function satisfies

∑m|nΛ⁢(m)=log⁡n. (8)

For f⁢(s)=∑n=1∞Λ⁢(n)⁢n-s and

g⁢(s)=-ζ′⁢(s)=∑n=1∞log⁡n⁢n-s,

using [40, p. 253, Theorem 294]

-ζ′⁢(s)ζ⁢(s)=∑n=1∞Λ⁢(n)⁢n-s,

we obtain

∑n=1∞Λ⁢(n)⁢xn1-xn=∑n=1∞log⁡n⁢xn.

38 Mertens

For Re⁢s>1, we define

P⁢(s)=∑p1ps.

We also define

H=∑m=2∞∑p1m⁢pm.

Mertens [61] proves the following.

Theorem 2.

As ϱ→0,

P⁢(1+ρ)=log⁡(1ρ)-H+o⁢(1).
Proof.

As ϱ→0,

ζ⁢(1+ϱ)=1ϱ+γ+O⁢(ϱ)=1ϱ⁢(1+γ⁢ϱ+O⁢(ϱ2)).

Taking the logarithm,

log⁡ζ⁢(1+ϱ)=log⁡(1ϱ)+log⁡(1+γ⁢ϱ+O⁢(ϱ2))=log⁡(1ϱ)+γ⁢ϱ+O⁢(ϱ2). (9)

On the other hand, for ϱ>0,

ζ⁢(1+ϱ)=∏p11-1p1+ϱ,

and taking the logarithm,

log⁡ζ⁢(1+ϱ) =-∑plog⁡(1-1p1+ϱ)
=∑p∑m=1∞1m⁢pm⁢(1+ϱ)
=P⁢(1+ρ)+∑m=2∞∑p1m⁢pm⁢(1+ϱ).

Then as ϱ→0,

log⁡ζ⁢(1+ϱ)=P⁢(1+ϱ)+H+o⁢(1).

Combining this with (9) we get that as ϱ→0,

P⁢(1+ρ)=log⁡(1ρ)-H+o⁢(1).

∎

Mertens [61] also proves that for any x there is some

|δ|<4log⁡(x+1)+2x⁢log⁡x

such that

∑p≤x1p=log⁡log⁡x+γ-H+δ.

Thus,

∑p≤x1p=log⁡log⁡x+γ-H+O⁢(1log⁡x).

Mertens shows that

H=-∑n=2∞μ⁢(n)⁢log⁡ζ⁢(n)n.

This can be derived using (7), and we do this now; see [58].

Lemma 3.

For Re⁢s>1,

1s⁢log⁡ζ⁢(s)=∫2∞π⁢(t)⁢d⁢tt⁢(ts-1).
Proof.

For p prime and Re⁢s>0,

∫p∞d⁢tt⁢(ts-1) =∫p∞t-s-1⁢11-t-s⁢𝑑t
=∫p∞t-s-1⁢∑n=0∞(t-s)n⁢d⁢t
=∑n=0∞∫p∞t-n⁢s-s-1⁢𝑑t
=∑n=0∞t-n⁢s-s-n⁢s-s|p∞
=1s⁢∑n=1∞p-n⁢sn
=-1s⁢log⁡(1-p-s),

hence

log⁡(11-p-s)=s⁢∫p∞d⁢tt⁢(ts-1).

On the one hand,

∑p∫p∞d⁢tt⁢(ts-1)=∫2∞π⁢(t)⁢d⁢tt⁢(ts-1).

On the other hand, for Re⁢s>1 we have

∑plog⁡(11-p-s)=log⁢∏p(11-p-s)=log⁡ζ⁢(s).

Combining these, for Re⁢s>1,

1s⁢log⁡ζ⁢(s)=∫2∞π⁢(t)⁢d⁢tt⁢(ts-1).

∎

Theorem 4.
H=-∑n=2∞μ⁢(n)⁢log⁡ζ⁢(n)n.
Proof.

For any prime p and for m≥1,

∫p∞t-m-1⁢𝑑t=t-m-m|p∞=1m⁢pm,

and using this we have

H =∑m=2∞∑p1m⁢pm
=∑m=2∞∑p∫p∞t-m-1⁢𝑑t
=∑m=2∞∫2∞π⁢(t)⁢t-m-1⁢𝑑t
=∫2∞π⁢(t)⁢(∑m=2∞t-m-1)⁢𝑑t
=∫2∞π⁢(t)⁢1t2⁢(t-1)⁢𝑑t

Rearranging (7),

x21-x=-∑n=2∞μ⁢(n)⁢xn1-xn.

With x=t-1,

1t⁢(t-1)=-∑n=2∞μ⁢(n)tn-1,

so

1t2⁢(t-1)=-∑n=2∞μ⁢(n)t⁢(tn-1).

Thus we have

H=-∫2∞π⁢(t)⁢(∑n=2∞μ⁢(n)t⁢(tn-1))⁢𝑑t=-∑n=2∞μ⁢(n)⁢∫2∞π⁢(t)⁢d⁢tt⁢(tn-1)⁢𝑑t.

Using Lemma 3 for s=2,3,4,…,

H=-∑n=2∞μ⁢(n)⋅1n⁢log⁡ζ⁢(n),

completing the proof. ∎

39 Preliminaries on prime numbers

We define

ϑ⁢(x)=∑p≤xlog⁡p=log⁢∏p≤xp

and

ψ⁢(x)=∑pm≤xlog⁡p=∑n≤xΛ⁢(n).

One sees that

ψ⁢(x)=∑p≤x[logp⁡x]⁢log⁡p=∑p≤x[log⁡xlog⁡p]⁢log⁡p.

As well,

ψ⁢(x)=∑m=1∞∑p≤x1/mlog⁡p=∑m=1∞ϑ⁢(x1/m); (10)

there are only finitely many terms on the right-hand side, as ϑ⁢(x1/m)=0 if x<2m.

Theorem 5.
ψ⁢(x)=ϑ⁢(x)+O⁢(x1/2⁢(log⁡x)2).
Proof.

For x≥2, ϑ⁢(x)<x⁢log⁡x, giving

∑2≤m≤log⁡xlog⁡2ϑ⁢(x1/m) <∑2≤m≤log⁡xlog⁡2x1/m⁢1m⁢log⁡x
≤x1/2⁢log⁡x⁢∑2≤m≤log⁡xlog⁡21m
=O⁢(x1/2⁢(log⁡x)2).

Thus, using (10) we have

ψ⁢(x)=ϑ⁢(x)+∑2≤m≤log⁡xlog⁡2ϑ⁢(x1/m)=ϑ⁢(x)+O⁢(x1/2⁢(log⁡x)2).

∎

We prove that if limx→∞⁡ϑ⁢(x)x=1 then π⁢(x)x/log⁡x=1.

Theorem 6.
lim infx→∞⁡π⁢(x)x/log⁡x=lim infx→∞⁡ϑ⁢(x)x

and

lim supx→∞⁡π⁢(x)x/log⁡x=lim supx→∞⁡ϑ⁢(x)x.
Proof.

From (10), ϑ⁢(x)≤ψ⁢(x). And,

ψ⁢(x)=∑p≤x[log⁡xlog⁡p]⁢log⁡p≤∑p≤xlog⁡xlog⁡p⁢log⁡p=log⁡x⁢∑p≤x.

Hence

ϑ⁢(x)x≤π⁢(x)⁢log⁡xx,

whence

lim infx→∞⁡ϑ⁢(x)x≤lim infx→∞⁡π⁢(x)x/log⁡x

and

lim supx→∞⁡ϑ⁢(x)x≤lim supx→∞⁡π⁢(x)x/log⁡x.

Let 0<α<1. For x>1,

ϑ⁢(x)=∑p≤xlog⁡p≥∑xα<p≤xlog⁡p>∑xα<p≤xlog⁡xα=α⁢log⁡x⁢(π⁢(x)-π⁢(xα)).

As π⁢(xα)<xα,

ϑ⁢(x)>α⁢π⁢(x)⁢log⁡x-α⁢xα⁢log⁡x,

i.e.,

ϑ⁢(x)x>α⁢π⁢(x)⁢log⁡xx-α⁢log⁡xx1-α.

This yields

lim infx→∞⁡ϑ⁢(x)x≥α⁢lim infx→∞⁡π⁢(x)⁢log⁡xx-α⁢lim infx→∞⁡log⁡xx1-α=α⁢lim infx→∞⁡π⁢(x)⁢log⁡xx

and

lim supx→∞⁡ϑ⁢(x)x≥α⁢lim supx→∞⁡π⁢(x)⁢log⁡xx-α⁢lim supx→∞⁡log⁡xx1-α=α⁢lim supx→∞⁡π⁢(x)⁢log⁡xx.

Since these are true for all 0<α<1, we obtain respectively

lim infx→∞⁡ϑ⁢(x)x≥lim infx→∞⁡π⁢(x)⁢log⁡xx

and

lim supx→∞⁡ϑ⁢(x)x≥lim supx→∞⁡π⁢(x)⁢log⁡xx.

∎

40 Wiener’s tauberian theorem

Wiener [85, Chapter III].

Wiener-Ikehara [19]

Rudin [67, p. 229, Theorem 9.7]

We say that a function s:(0,∞)→ℝ is slowly decreasing if

lim inf⁡(s⁢(ρ⁢v)-s⁢(v))≥0,v→∞,ρ→1+.

Widder [84, p. 211, Theorem 10b]: Wiener’s tauberian theorem tells us that if a∈L∞⁢(0,∞) and is slowly decreasing and if g∈L1⁢(0,∞) satisfies

∫0∞ti⁢x⁢g⁢(t)⁢𝑑t≠0,x∈ℝ,

then

limx→∞⁡1x⁢∫0∞g⁢(tx)⁢a⁢(t)⁢𝑑t=A⁢∫0∞g⁢(t)⁢𝑑t

implies that

limv→∞⁡a⁢(v)=A.

It is straightforward to check the following by rearranging summation.

Lemma 7.

If ∑n=1∞an⁢zn has radius of convergence ≥1, then for |z|<1,

∑n=1∞an⁢zn1-zn=∑n=1∞(∑m|nam)⁢zn.

Using Lemma 7 with an=Λ⁢(n) and z=e-x and applying (8), we get

∑n=1∞Λ⁢(n)⁢zn1-zn=∑n=1∞log⁡(n)⁢zn. (11)

From (11), and Lemma 7 with an=1, we have

∑n=1∞(Λ⁢(n)-1)⁢e-n⁢x1-e-n⁢x=∑n=1∞(log⁡n-d⁢(n))⁢e-n⁢x.

We follow Widder [84, p. 231, Theorem 16.6].

Theorem 8.

As x→0+,

∑n=1∞(log⁡n-d⁢(n))⁢e-n⁢x=-2⁢γx+O⁢(x-1/2).
Proof.

Generally,

(1-z)⁢∑n=1∞zn⁢∑m=1nam =(1-z)⁢∑m=1∞am⁢∑n=m∞zn
=(1-z)⁢∑m=1∞am⁢zm1-z
=∑m=1∞am⁢zm.

Using this with am=log⁡m-d⁢(m) and z=e-x gives

∑n=1∞(log⁡n-d⁢(n))⁢e-n⁢x =(1-e-x)⁢∑n=1∞e-n⁢x⁢(∑m=1nlog⁡m-∑m=1nd⁢(m))
=(1-e-x)⁢∑n=1∞e-n⁢x⁢(log⁡(n!)-∑m=1nd⁢(m)).

Using

log⁡(n!)=n⁢log⁡n-n+O⁢(log⁡n)

and

∑m=1nd⁢(m)=n⁢log⁡n+(2⁢γ-1)⁢n+O⁢(n1/2),

we get

log⁡(n!)-∑m=1nd⁢(m)=-2⁢γ⁢n+O⁢(n1/2).

Therefore,

∑n=1∞(log⁡n-d⁢(n))⁢e-n⁢x=(1-e-x)⁢∑n=1∞e-n⁢x⁢(-2⁢γ⁢n+O⁢(n1/2)).

One proves that there is some K such that for all 0≤y<1,

(1-y)⁢(log⁡1y)1/2⁢∑n=1∞n1/2⁢yn≤K,

whence, with y=e-x,

∑n=1∞n1/2⁢e-n⁢x≤K⁢x-1/21-e-x.

Also,

∑n=1∞n⁢e-n⁢x=e-x(1-e-x)2,

and thus we have

∑n=1∞(log⁡n-d⁢(n))⁢e-n⁢x =-2⁢γ⁢e-x1-e-x+O⁢(x-1/2)
=-2⁢γ⁢1ex-1+O⁢(x-1/2).

But

1ex-1=1x-12+O⁢(x),

so

∑n=1∞(log⁡n-d⁢(n))⁢e-n⁢x=-2⁢γx+O⁢(x-1/2).

∎

Define

f⁢(x)=∑n=1∞(Λ⁢(n)-1)⁢e-n⁢x1-e-n⁢x,

and

h⁢(x)=∑n≤xΛ⁢(n)-1n,

and

g⁢(t)=dd⁢t⁢(t⁢e-t1-e-t).

First we show that h is slowly decreasing.

Lemma 9.

h⁢(x) is slowly decreasing.

Proof.

Using

∑1≤n≤x1n=log⁡x+γ+O⁢(n-1),x→∞,

we have, for 0<x<∞ and ρ>1,

h⁢(ρ⁢x)-h⁢(x) =∑x<n≤ρ⁢xΛ⁢(n)-1n
≥-∑x<n≤ρ⁢x1n
=-∑1≤n≤ρ⁢x1n+∑1≤n≤x1n
=-log⁡(ρ⁢x)+log⁡x+O⁢((ρ⁢x)-1)+O⁢(x-1)
=-log⁡ρ+O⁢((ρ⁢x)-1)+O⁢(x-1).

Hence as x→∞ and ρ→1+,

h⁢(ρ⁢x)-h⁢(x)→0,

which shows that h is slowly decreasing. ∎

The following is from Widder [84, pp. 231–232].

Lemma 10.

As x→∞,

1x⁢∫0∞g⁢(tx)⁢h⁢(t)⁢𝑑t=2⁢γ+O⁢(x-1/2).
Proof.

Let I⁢(t)=0 for t<0 and I⁢(t)=1 for t≥0. Writing

h⁢(x)=∑n=1∞I⁢(x-n)⁢Λ⁢(n)-1n,

we check that for x>0,

∫0∞t⁢e-x⁢t1-e-x⁢t⁢𝑑h⁢(t) =∑n=1∞∫0∞t⁢e-x⁢t1-e-x⁢t⁢Λ⁢(n)-1n⁢d⁢(I⁢(t-n))
=∑n=1∞∫0∞t⁢e-x⁢t1-e-x⁢t⁢Λ⁢(n)-1n⁢𝑑δn⁢(t)
=∑n=1∞n⁢e-n⁢x1-e-n⁢x⁢Λ⁢(n)-1n
=f⁢(x).

On the other hand, integrating by parts,

f⁢(x) =∫0∞t⁢e-x⁢t1-e-x⁢t⁢𝑑h⁢(t)
=∫0∞1x⁢x⁢t⁢e-x⁢t1-ex⁢t⁢𝑑h⁢(t)
=∫0∞1x⁢x⁢t⁢e-x⁢t1-e-x⁢t⁢𝑑h⁢(t)
=∫0∞1x⁢t⁢e-t1-e-t⁢𝑑h⁢(tx)
=1x⁢t⁢e-t1-e-t⁢h⁢(tx)|0∞-∫0∞1x⁢g⁢(t)⁢h⁢(tx)⁢𝑑t
=-∫0∞1x⁢g⁢(t)⁢h⁢(tx)⁢𝑑t
=-∫0∞g⁢(x⁢t)⁢h⁢(t)⁢𝑑t.

By Theorem 8, as x→0+,

f⁢(x)=-2⁢γx+O⁢(x-1/2),

i.e., as x→0+,

∫0∞g⁢(x⁢t)⁢h⁢(t)⁢𝑑t=2⁢γx+O⁢(x-1/2).

Thus, as x→∞,

∫0∞g⁢(tx)⁢h⁢(t)⁢𝑑t=2⁢γ⁢x+O⁢(x1/2).

∎

The following is from Widder [84, p. 232].

Lemma 11.
∫0∞t-i⁢x⁢g⁢(t)⁢𝑑t={-1x=0i⁢x⁢ζ⁢(1-i⁢x)⁢Γ⁢(1-i⁢x)x≠0.
Proof.
∫0∞t-i⁢x⁢g⁢(t)⁢𝑑t =∫0∞t-i⁢x⁢dd⁢t⁢(t⁢e-t1-e-t)⁢𝑑t
=limδ→0⁡∫0∞t-i⁢x+δ⁢dd⁢t⁢(t⁢e-t1-e-t)⁢𝑑t
=limδ→0⁡(t-i⁢x+δ⁢t⁢e-t1-e-t|0∞+(i⁢x-δ)⁢∫0∞t-i⁢x+δ-1⁢t⁢e-t1-e-t⁢𝑑t)
=limδ→0⁡(i⁢x-δ)⁢∫0∞t-i⁢x+δ-1⁢t⁢e-t1-e-t⁢𝑑t
=limδ→0⁡(i⁢x-δ)⁢∫0∞t(-i⁢x+δ+1)-1⁢e-t1-e-t⁢𝑑t.

Using

∫0∞ts-1et-1⁢𝑑t=ζ⁢(s)⁢Γ⁢(s),Re⁢(s)>1,

this becomes

∫0∞t-i⁢x⁢g⁢(t)⁢𝑑t=limδ→0+⁡(i⁢x-δ)⁢ζ⁢(1+δ-i⁢x)⁢Γ⁢(1+δ-i⁢x).

If x=0, then using

ζ⁢(s)=1s-1+γ+O⁢(|s-1|),s→1,

we get

limδ→0+⁡(-δ)⁢ζ⁢(1+δ)⁢Γ⁢(1+δ)=-1.

If x>0, then

limδ→0+⁡(i⁢x-δ)⁢ζ⁢(1+δ-i⁢x)⁢Γ⁢(1+δ-i⁢x)=i⁢x⁢ζ⁢(1-i⁢x)⁢Γ⁢(1-i⁢x).

∎

By Wiener’s tauberian theorem, it follows that

∑n=1∞Λ⁢(n)-1n=-2⁢γ.
Lemma 12.
h⁢(x)=∫12xd⁢(ψ⁢(t)-[t])t.
Proof.

Let I⁢(t)=0 for t<0 and I⁢(t)=1 for t≥0. Writing

ψ⁢(x)=∑n=1∞I⁢(x-n)⁢Λ⁢(n),[x]=∑n=1∞I⁢(x-n),

we have

∫12xd⁢(ψ⁢(t)-[t])t =∫12x1t⁢d⁢(∑n=1∞I⁢(t-n)⁢(Λ⁢(n)-1))
=∫12x1t⁢∑n=1∞(Λ⁢(n)-1)⁢d⁢δn⁢(t)
=∑1≤n≤xΛ⁢(n)-1n
=h⁢(x).

∎

Thus, we have established that

∫12∞d⁢(ψ⁢(t)-[t])t=-2⁢γ.

41 Hermite

Hermite [42]

Hermite [43]

42 Gerhardt

Gerhardt [33, p. 196] refers to Lambert’s Architectonic.

43 Levi-Civita

Levi-Civita [57]

44 Franel

Franel [32] and [31]

The next theorem shows that the set of points on the unit circle that are singularities of ∑n=1∞zn1-zn is dense in the unit circle. Titchmarsh [82, pp. 160–161, §4.71].

Theorem 13.

For |z|<1, define

f⁢(z)=∑n=1∞zn1-zn.

Suppose that p>0,q>1 are relatively prime integers. As r→1-,

(1-r)⁢f⁢(r⁢e2⁢π⁢i/q)→∞.
Proof.

Set z=r⁢e2⁢π⁢i⁢p/q and write

∑n=1∞zn1-zn=∑n≡0(modq)zn1-zn+∑n≢0(modq)zn1-zn.

On the one hand,

(1-r)⁢∑n≡0(modq)zn1-zn =(1-r)⁢∑m=1∞zm⁢q1-zm⁢q
=(1-r)⁢∑m=1∞(r⁢e2⁢π⁢i⁢p/q)m⁢q1-(r⁢e2⁢π⁢i⁢p/q)m⁢q
=(1-r)⁢∑m=1∞rm⁢q1-rm⁢q
=1-r1-rq⁢∑m=1∞rm⁢q1+rq+⋯+r(m-1)⁢q
=11+r+⋯+rq-1⁢∑m=1∞rm⁢q1+rq+⋯+r(m-1)⁢q
≥1q⁢∑m=1∞rm⁢qm
=-1q⁢log⁡(1-rq)
→∞

as r→1.

On the other hand, for n≢0(modq) we have

|1-zn|2 =|1-rn⁢e2⁢π⁢i⁢p⁢n/q|2
=(1-rn⁢e2⁢π⁢i⁢p⁢n/q)⁢(1-rn⁢e-2⁢π⁢i⁢p⁢n/q)
=1-rn⁢(e2⁢π⁢i⁢p⁢n/q+e-2⁢π⁢i⁢p⁢n/q)+r2⁢n
=1-2⁢rn⁢cos⁡2⁢π⁢p⁢n/q+r2⁢n
=1-2⁢rn+4⁢rn⁢sin2⁡π⁢p⁢nq+r2⁢n
=(1-rn)2+4⁢rn⁢sin2⁡π⁢p⁢nq.

So far we have not used the hypothesis that n≡0(modq). We use it to obtain

sin⁡π⁢p⁢nq≥sin⁡πq.

With this we have

|1-zn|2≥4⁢rn⁢sin2⁡πq,

and therefore, as r<1,

(1-r)⁢|∑n≢0(modq)zn1-zn| ≤(1-r)⁢∑n≢0(modq)|z|n|1-zn|
≤(1-r)⁢∑n≢0(modq)rn2⁢rn/2⁢sin⁡πq
≤1-r2⁢sin⁡πq⁢∑n=0∞rn/2
=1-r2⁢sin⁡πq⋅11-r
=1+r2⁢sin⁡πq
<1sin⁡πq.

∎

45 Wigert

The following result is proved by Wigert [86]. Our proof follows Titchmarsh [81, p. 163, Theorem 7.15]. Cf. Landau [55].

Theorem 14.

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 Re⁢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. (12)

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). (13)

Denote the right-hand sideof (13) 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 [82, p. 151] tells us that

|Γ⁢(s)|∼2⁢π⁢e-π2⁢|t|⁢|t|σ-12,|t|→∞.

As well [81, 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 (12) and (13), 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).

46 Steffensen

Steffensen [75]

47 Szegő

Szegő [79]

48 Pólya and Szegő

Pólya and Szegő [64]

49 Partition function

Let

F⁢(x)=∑n=0∞p⁢(n)⁢xn=∏n=1∞11-xn.

Taking the logarithm,

log⁡F⁢(x)=∑n=1∞log⁡11-xn=-∑n=1∞log⁡(1-xn)=-∑n=1∞∑m=1∞-(xn)mm,

and switching the order of summation gives

log⁡F⁢(x)=∑m=1∞1m⁢∑n=1∞(xm)n=∑m=1∞1m⁢xm1-xm.

On the one hand, for 0<x<1 we have m⁢xm-1⁢(1-x)<1-xm and using this,

∑m=1∞1m⁢xm1-xm<∑m=1∞1m⁢xmm⁢xm-1⁢(1-x)=x1-x⁢∑m=1∞1m2=π26⁢x1-x.

On the other hand, for -1<x<1 we have 1-xm<m⁢(1-x), and using this, for 0<x<1 we have

∑m=1∞1m⁢xm1-xm>∑m=1∞1m⁢xmm⁢(1-x)=11-x⁢∑m=1∞xmm2.

Thus, for 0<x<1,

∑m=1∞xmm2<(1-x)⁢log⁡F⁢(x)<π26⁢x.

Taking x→1- gives

π26≤limx→1-⁡(1-x)⁢log⁡F⁢(x)≤π26,

i.e.,

log⁡F⁢(x)∼π26⁢11-x,x→1-.

See Stein and Shakarchi [76, p. 311].

50 Hansen

Hansen [39]

51 Kiseljak

Kiseljak [45]

52 Unsorted

In 1892, in volume VII, no. 23, p. 296 of the weekly Naturwissenschaftliche Rundschau, it is stated that for the year 1893, one of the six prize questions for the Belgian Academy of Sciences in Brussels is to determine the sum of the Lambert series

x1-x+x21-x2+x31-x3+⋯,

or if one cannot do this, to find a differential equation that determines the function.

Gram [35] on distribution of prime numbers.

Hardy [41]

Bohr and Cramer [1, p. 820]

Flajolet, Gourdon and Dumas [30]

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