e n n e n ln x ln en n 2 P1(x a)dx = 2 P1(x a)dx, (2.44) Z1 x − en Zη − for some η with 1 η e . Therefore, we obtain ≤ ≤ n n en ln x nn en 1 nn 2 P1(x a)dx = n n P1(x a)dx n n . (2.45) Z1 x − 2 e Zη − ≤ 6 2 e
Here we have used the standard Fourier series for P1(x) [36] (p. 151) or [1] (p. 805),
∞ sin(2nπx) P (x)= , (2.46) 1 − nπ nX=1 giving c 1 ∞ cos[2nπ(x a)] c P1(x a)dx = − , (2.47) b − 2 n2π2 Z n=1 b X so that c 2 1 P1(x a)dx 2 ζ(2) = . (2.48) Zb − ≤ 2π 6
Similarly, we have
∞ n n ξ ln x ln en 2 P1(x a)dx = 2 P1(x a)dx, (2.49) Zen x − en Zen − 20 for some ξ with e ξ < . This gives n ≤ ∞ ∞ lnn x nn ξ 1 nn 2 P1(x a)dx = n n P1(x a)dx n n . (2.50) Zen x − 2 e Zen − ≤ 6 2 e
Combining the 4 integral contributions of (2.43) yields the Proposition, as
1 (n 1)n−1n nn enn Cn(a) − + . (2.51) | | ≤ 3 " 2n−1en−1 2nen # ≤ 2nen
Remarks. Zhang and Williams previously found the better bound
[3 + ( 1)n](2n)! C (a) − . (2.52) | n | ≤ nn+1(2π)n
However, our presentation shows possibility for improvement. If, for instance, a better bound is found for the integrals c P (x a)dx, then we may expect a tighter b 1 − R estimation.
Let us note also that the use of (2.40) for ζ(j)(pk +1, a) together with the expres- sions of Proposition 2 provides many other opportunities for the estimation of γ (a) | k | and C (a) . | k | Proposition 8. We apply the formula of Klusch [22] (2.5),
∞ (s) L(x, s, a + ξ)= ( 1)k k L(x, s + k, a)ξk. (2.53) − k! kX=0 This formula may be obtained by Taylor expansion, expansion of an integral repre- sentation, or by binomial expansion in (1.15). We take n derivatives of (2.53) using the product rule. We evaluate at s = 1 using Lemma 1 and the defining relation
(1.17) of ℓn. Separating the k = 0 term yields the Proposition and then Corollary 3.
21 Remark. As very special cases, we have
1 1 1+ a a ℓ0 , a = ψ ψ , 2 2 2 − 2 1 1 a 1+ a 1+ a a ℓ1 , a = ln 2 ψ ψ + γ1 γ1 , 2 2 2 − 2 2 − 2 and
1 1 2 1+ a a a a +1 ℓ2 , a = ln 2 ψ ψ + 2 ln 2 γ1 γ1 2 4 2 − 2 2 − 2 a a +1 +γ2 γ2 . (2.54) 2 − 2 As another example, from
1 ∞ in a a +2 a +1 a +3 L ,s,a = =4−s ζ s, ζ s, + i ζ s, ζ s, , 4 (n + a)s 4 − 4 4 − 4 nX=0 (2.55) by taking the real and imaginary parts of derivatives evaluated at s = 1, we obtain expressions for γ (a/4) γ [(a + 2)/4] and γ [(a + 1)/4] γ [(a + 3)/4]. Evidently k − k k − k for x a rational number such relations always exist.
Proposition 9. From the classical theta function-based representation of the Rie- mann zeta function [6] (2) we have
πs/2 ∞ s ∞ 1 s Γ(s/2)ζ(s)= + n−sΓ , πn2 + πs−1/2 ns−1Γ − , πn2 . (2.56) s(s 1) 2 2 − nX=1 nX=1 We expand both sides of this equation in powers of s 1, and equate the coeffi- − cients of (s 1)0 and (s 1)1 on both sides to obtain parts (i) and (ii), respec- − − tively. The coefficient of (s 1)n−1 for n 0 of the term πs/2/[s(s 1)] is given by − ≥ − π1/2( 1)n n ( 1)j lnj π/2j, and the simple polar term from the left side of (2.56) is − j=0 − P 22 cancelled by the n = 0 term. We use the special function relations Γ(0, z)= Ei( z) − − and Γ(1/2, z) = √π[1 erf(√z)]. The incomplete Gamma function [16] is given for − Re x> 0 by
2 ∞ 2xαe−x ∞ t1−2αe−t Γ(α, x)= e−ttα−1dt = dt, (2.57) x Γ(1 α) 0 t2 + x Z − Z where the latter form holds for Re α < 1. It is convenient in finding derivatives of this function to use the relation
xα Γ(α, x)=Γ(α) F (α; α + 1; x), α / N, (2.58) − α 1 1 − − ∈
where 1F1 is the confluent hypergeometric function [1, 16]. It follows that
d 1 F (α; α + 1; x)= [ F (α; α + 1; x) F (α,α; α +1,α + 1; x)] , (2.59) dα 1 1 − α 1 1 − − 2 2 − and
d xα Γ(α, x)=Γ(α)ψ(α)+ [ α ln x F (α; α + 1; x)+ F (α,α; α +1,α + 1; x)] . dα α2 − 1 1 − 2 2 − (2.60)
When α 0 in (2.60), the singular terms 1/α2 cancel. In fact, we have the expansions → 1 γ2 π2 Γ′(α)=Γ(α)ψ(α)= + + + O(α), (2.61) −α2 2 12
and
xα (α) (α) ( x)j (1 j ln x) j α ln x + j − = − ( x)j + O(α), α 0. α2 (α + 1) "− (α + 1) # j! j3(j 1)! − → j j − (2.62)
23 Summing the latter relation on j as α 0 then gives → ∞ (1 j ln x) − ( x)j = x F (1, 1, 1;2, 2, 2; x) + [γ + Γ(0, x) + ln x] ln x. (2.63) j3(j 1)! − − 3 3 − jX=1 − We apply these relations at α =0 and 1/2 and the Proposition follows.
Remarks. By making a change of variable in the theta function-based represen-
tation [6] (2) we may include a parameter in the series representation (2.56), and so
in Proposition 9 too. Beyond this, we may include a parameter b > 0 and a set of polynomials pj(s) with zeros lying only on the critical line in representing the Rie- mann zeta and xi functions [12] (Proposition 3). Thereby, we obtain a generalization of Proposition 9.
In equation (1.20), the sum terms provide a small correction 0.0230957 to ≃ produce the value γ/2 0.288607. Although there are infinite sum corrections in ≃ Proposition 9, the expressions such as (1.20) and (1.21) may have some attraction for computation. This is owing to the very fast decrease of the summands with n. For
(1.20), using known asymptotic forms, the summand terms have exponential decrease
−n2π 2 1 e 2 + O 4 . Similarly for (1.21), the summand has exponential decrease ∼ πn n h i in n. Therefore, high order approximations for the constants may be obtained with
relatively few terms.
We note an integral representation for the term ∞ Ei( πn2) in Proposition − n=1 − 9 in the following. P
∞ n2 Lemma 3. Put the function θ3(y)=1+2 n=1 y . Then we have P ∞ 1 2 1 π/(x−1) dx Ei( πn )= θ3 e 1 − − −2 0 − x 1 nX=1 Z h i − 24 ∞ 1 −πu du = [1 θ3(e )] . (2.64) −2 Z1 − u α Proof. Let Ln be the Laguerre polynomial of degree n and parameter α. We use the relation (e.g., [16], p. 1038)
∞ Lα(x) Γ(α, x)= xαe−x k , α> 1, (2.65) k +1 − kX=0 at α = 0. We then have
∞ ∞ ∞ 2 2 L (πn ) Ei( πn2)= e−πn k − − k +1 nX=1 nX=1 kX=0 ∞ ∞ 1 ∞ −πn2 k 2 = e x dx Lk(πn ) 0 nX=1 kX=0 Z kX=0 ∞ xπn2/(x−1) 2 1 e = e−πn dx, (2.66) − 0 x 1 nX=1 Z − where we used the generating function of the Laguerre polynomials (e.g., [16], p.
1038). The interchange of summation and integration is justified by the absolute convergence of the integral. Using the definition of θ3 completes the Lemma.
Discussion: Generalization of Proposition 9
We may generalize Proposition 9 to the context of generalized Stieltjes constants coming from the evaluation of Dirichlet L series derivatives at s = 1. For this we require a number of definitions. We use [20] (Ch. 1, Section 4.2).
Let χ be a primitive character modulo k. We need two theta functions,
∞ 2 θ(τ, χ)= χ(n)e−πτn /k, n=−∞ X
25 for χ an even character,
∞ −πτn2/k θ1(τ, χ)= nχ(n)e , n=−∞ X for χ an odd character, and the Gauss sum
k g(χ)= χ(j)e2πij/k. jX=1 We let δ = 0 or 1 depending upon whether χ( 1)=1 or 1, respectively. We put − − s + δ ξ(s, χ)=(πk−1)−(s+1)/2Γ L(s, χ). 2 !
Then by [20] (p. 15) we find for χ an even character,
∞ √k ∞ 2ξ(s, χ)= τ s/2−1θ(s, χ)dτ + τ −(s+1)/2θ(τ, χ¯)dτ Z1 g(¯χ) Z1 ∞ s n2 = π−s/2−1ks/2+1 χ(n)n−s−2Γ +1, π n=−∞ 2 k ! X √k ∞ 1 s n2 + π(s−1)/2k(1−s)/2 χ¯(n)ns−1Γ − , π , g(¯χ) n=−∞ 2 k ! X and for χ an odd character,
∞ ∞ (s−1)/2 i√k −s/2 2ξ(s, χ)= τ θ1(s, χ)dτ + τ θ1(τ, χ¯)dτ Z1 g(¯χ) Z1 ∞ s +1 n2 = π−(s+1)/2k(s+1)/2 nχ(n)n−(s+1)Γ +1, π n=−∞ 2 k ! X i√k ∞ s n2 + πs/2−1k1−s/2 nχ¯(n)ns−2Γ 1 , π . g(¯χ) n=−∞ − 2 k ! X Then one may multiply the expressions for ξ(s, χ) by (πk−1)(s+1)/2 and proceed as in the proof of Proposition 9 in developing both sides in powers of s 1. − 26 In the case of the Hurwitz zeta function we employ the theta function
2 θ(τ, a)= e−πτ(n+a) , nX=06 with its functional equation
2 θ(1/τ,a)= √τe−πa /τ θ(τ, ia/τ). −
Proposition 10. We make use of expressions in the fine paper of Fine [15]. In particular, see his expressions for the function H(a, s) (pp. 362-363). We have
∞ ∞ 1 s 2 π(s−1)/2Γ − [ζ(1 s, a)+ ζ(1 s, 1 a)]=2 cos(2πna) e−πn tts/2−1dt 2 − − − 0 nX=1 Z s ∞ cos(2πna) =2π−s/2Γ 2 ns nX=1 −s/2 s 2πia −2πia = π Γ [Lis(e ) + Lis(e )]. (2.67) 2 Initially, the left side of this equation is valid for Re s< 0. With analytic continuation, the function is H(a, s)+2/s is entire in s. Therefore, we may expand both sides of the representation (2.64) about s = 0. As it must, the singular term 2/s effectively − cancels from both sides of (2.67). Part (i) of the Proposition results from the constant term s0 on both sides of (2.67), and using the reflection formula for the digamma function ψ(1 a) = ψ(a)+ π cot πa. Similarly, part (ii) results from the term s1 on − both sides of (2.60).
Remarks. Proposition 10 and (2.67) properly reduce as they should for a =1/2.
n In this case, we have the alternating zeta function ∞ (−1) = (21−s 1)ζ(s). Then n=1 ns − both sides of part (i) of Proposition 10 yield γ lnPπ + 2 ln 2. − 27 Proposition 11. By using the definition (1.24) we have
1 y Pn+1(y)= x(1 x)n−1 dx n! Z0 − 1 n−1 y = ( 1)n+k−1s(n 1,k) x(1 x)kdx n! − − 0 − kX=0 Z ( 1)n n−1 s(n 1,k) = − ( 1)k−1 − [(ky + y + 1)(1 y)k(y 1) + 1], (2.68) n! − (k + 2)(k + 1) − − kX=0 whence part (i) follows. Of the many ways to perform the elementary integral here,
it may be evaluated as a special case of the incomplete Beta function (e.g., [16], p.
950)
x p p−1 q−1 x Bx(p, q)= t (1 t) dt = 2F1(p, 1 q; p + 1; x), Re p> 0, Re q > 0. Z0 − p − (2.69)
For part (ii) we again use a generating function relation for s(n, k), writing
y n+1 n y 1 ( 1) k Pn+1(y)= ( x)n dx = − s(n, k) x dx. (2.70) −n! 0 − n! 0 Z kX=0 Z
The second line of (1.26) simply follows from the values s(n, 0) = δn0 and s(n, n) = 1.
The identity of part (iii) follows simply from putting y = 1 in parts (i) and (ii).
For part (iv), we have the well known expression
N k ln m 1 k+1 γk = lim ln N , (2.71) N→∞ m − k +1 ! mX=1 (k) so that limn→∞ rn = 0. We form
n k m+1 k (k) ln m ln x Dn = dx m − m x ! mX=1 Z
28 n 1 lnk m lnk(x + m) = dx. (2.72) 0 " m − x + m # mX=1 Z Therefore, we have
∞ 1 k k (k) ln m ln (x + m) rn = dx. (2.73) 0 " m − x + m # m=Xn+1 Z We now use [10] (5.7)
lnn y lnn(x + y) ∞ xk 1 n−1 n! = ( 1)k lnn y + s(k +1, j + 2) lnn−j−1 y . y − x + y yk+1 − k! (n j 1)! kX=1 jX=0 − − (2.74)
Performing the integration of (2.73) gives part (iv).
Discussion related to Proposition 11
By defining the function f (x, m)=(x + m) lnk m m lnk(x + m), it is possible k − (k) to further decompose the remainders rn of (1.29) by writing
∞ 1 1 ∞ (k) 1 1 fk(x, m) rn = fk(x, m) dx + dx. 0 "m(x + m) − m(m + 1)# 0 m(m + 1) m=Xn+1 Z Z m=Xn+1 (2.75)
The representation (2.74) can then be used three times in this equation. This process of adding and subtracting terms can be continued, building an integral term with denominator m(m + 1) (m + j)(m + x). For k = 0, there is drastic reduction to ··· the original construction of Ser [29].
Proposition 11 (iv) can be easily extended to expressions for r(k)(a) = γ (a) n k − (k) Dn (a). As pointed out by Ser, it is possible to write many summations and generating
29 function relations with the polynomials Pn. As simple examples, we have
∞ ∞ ′ n n y n y Pn+1(y)z = ( 1) z =1 (1 z) , (2.76) − − n! − − nX=1 nX=1 and ∞ ′ ∞ n Pn+1(y) ( 1) y = − = ψ(y +1)+ γ = Hy. (2.77) n − n n! nX=1 nX=1 With the form (1.27) we easily verify a generating function:
∞ ∞ ( 1)n+1 n s(n, k) p zn−1 = − zn−1 n+1 n! k +1 nX=1 nX=1 kX=1 1 ∞ 1 ∞ s(n, k) 1 ∞ 1 = ( z)n = lnk(1 z) −z k +1 n! − −z (k + 1)! − kX=1 nX=k kX=1 1 1 = + . (2.78) z ln(1 z) − ′ ∞ Pn+1(y) n One may also write a great many hypergeometric series of the form n=1 nj z , that we omit. P
In contrast to an expression of Ser [29], we have
∞ 1 1 1 p (1 ez)n−1 = + n+1 − z 1 ez − 2 nX=2 − 1 1 z = coth z − 2 2 ∞ B = 2k z2k−1, z < 2π, (2.79) (2k)! | | kX=1 where the latter series may be found from [16] (p. 35). This relation serves to connect
the numbers pn+1 with the values ζ(2k). Equivalently, using an integral representation
for ζ(2k), we have
∞ ∞ z n−1 dv pn+1(1 e ) =2 sinh(zv) . (2.80) − 0 e2πv 1 nX=2 Z − 30 As well, we have many extensions including
∞ 1 etz 1 p (1 ez)n−1e−tz(n−1) = + . (2.81) n+1 − ln[1 + ez(1−t) e−tz] 1 ez − 2 nX=2 − − We may inquire as to the asymptotic form of p as n . Using only the n+1 → ∞ leading term of the result of [34], we have
1 n ( 1)k lnk−1 n 1 p − , n . (2.82) n+1 ∼ −n (k + 1) (k 1)! ∼ n ln2 n →∞ kX=1 − There are corrections to this result which overall decrease it. Therefore, one may wonder if it can be proved that the expression on the right serves as an upper bound for all n 2. ≥ Motivated by [1] (p. 824), we conjectured that
1 p , n , (2.83) n+1 ∼ n(ln n + γ)2 →∞ is an improved asymptotic form and upper bound. This asymptotic form has been verified by Knessl [24]. In fact, he has obtained a full asymptotic series for pn+1 in
the form 1 ∞ A p 1+ j , (2.84) n+1 ∼ n ln2 n lnj n jX=1 where Aj are constants that may be explicitly determined from certain logarithmic- exponential integrals. We have A = 2γ and A = 3γ2 π2/2. Knessl develops 1 − 2 − (2.84) from the exact representation
∞ 1 du p = , n 1. (2.85) n+1 n 2 2 Z0 (1 + u) (ln u + π ) ≥
31 From (2.85) we have the following
Corollary 6. We have the integral representation
∞ −z z ln(1 + e ) γ = e 2 2 dz. (2.86) Z−∞ z + π
Proof. We have [16] (p. 943)
1 1 1 1 1 1 γ = ψ(1) = + du = + dv − 0 ln u 1 u 0 ln(1 v) v ! Z − Z − 1 ∞ ∞ n−1 pn+1 = pn+1v dv = , (2.87) 0 n Z nX=1 nX=1 where we used (2.78). Now we use Knessl’s representation (2.85), giving
∞ 1 ∞ 1 du γ = 2 n 0 (1 + u)n (ln u + π2) nX=1 Z ∞ u du = ln 2 2 − Z0 1+ u (ln u + π ) ∞ z e z = 2 2 [z ln(1 + e )]dz − Z−∞ (z + π ) − ∞ z e −z = 2 2 ln(1 + e )dz. (2.87) Z−∞ (z + π )
Summary and very brief discussion
Our methods apply to a wide range of functions of interest to special function theory and analytic number theory, including but not limited to, the Lerch zeta function and Dirichlet L functions. Two dimensional extensions would be to Epstein
and double zeta functions. Our results include an addition formula for the Stieltjes
coefficients, as well as expressions for their derivatives. The series representations for
32 γk(a) have very rapidly convergent forms, making them applicable for multiprecision computation. Byproducts of our results include some summation relations for the
Stieltjes coefficients. We have given a means for estimating the magnitude of these coefficients, although this remains an outstanding problem.
Acknowledgement
I thank R. Smith for useful correspondence. I thank C. Knessl for reading the manuscript and for access to his results on the constants pn+1.
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