International Journal of Mathematics and Mathematical Sciences
VolumeΒ 2009Β (2009), Article IDΒ 626489, 22 pages
doi:10.1155/2009/626489
Research Article

On Rational Approximations to Euler's Constant 𝛾 and to 𝛾 + l o g ( π‘Ž / 𝑏 )

Fachhochschule für die Wirtschaft Hannover, Freundallee 15, 30173 Hannover, Germany

Received 4 December 2008; Accepted 13 April 2009

Academic Editor: StéphaneΒ Louboutin

Copyright Β© 2009 Carsten Elsner. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

Abstract

The author continues to study series transformations for the Euler-Mascheroni constant 𝛾 . Here, we discuss in detail recently published results of A. I. Aptekarev and T. Rivoal who found rational approximations to 𝛾 and 𝛾 + l o g π‘ž ( π‘ž ∈ β„š > 0 ) defined by linear recurrence formulae. The main purpose of this paper is to adapt the concept of linear series transformations with integral coefficients such that rationals are given by explicit formulae which approximate 𝛾 and 𝛾 + l o g π‘ž . It is shown that for every π‘ž ∈ β„š > 0 and every integer 𝑑 β‰₯ 4 2 there are infinitely many rationals π‘Ž π‘š / 𝑏 π‘š for π‘š = 1 , 2 , … such that | 𝛾 + l o g π‘ž βˆ’ π‘Ž π‘š / 𝑏 π‘š | β‰ͺ ( ( 1 βˆ’ 1 / 𝑑 ) 𝑑 / ( 𝑑 βˆ’ 1 ) 4 𝑑 ) π‘š and 𝑏 π‘š ∣ 𝑍 π‘š with l o g 𝑍 π‘š ∼ 1 2 𝑑 2 π‘š 2 for π‘š tending to infinity.

1. Introduction

Let 𝑠 𝑛 ξ‚€ 1 ∢ = 1 + 1 2 + 1 3 1 + β‹― +  βˆ’ 𝑛 βˆ’ 1 l o g 𝑛 ( 𝑛 β‰₯ 2 ) . ( 1 . 1 ) It is well known that the sequence ( 𝑠 𝑛 ) 𝑛 β‰₯ 1 converges to Euler's constant 𝛾 = 0 , 5 7 7 … , where 𝑠 𝑛 ξ‚€ 1 = 𝛾 + π’ͺ 𝑛  ( 𝑛 β‰₯ 1 ) . ( 1 . 2 ) Nothing is known on the algebraic background of such mathematical constants like Euler's constant 𝛾 . So we are interested in better diophantine approximations of these numbers, particularly in rational approximations.

In 1995 the author [1] introduced a linear transformation for the series ( 𝑠 𝑛 ) 𝑛 β‰₯ 1 with integer coefficients which improves the rate of convergence. Let 𝜏 be an additional positive integer parameter.

Proposition 1.1 (see [1]). For any integers 𝑛 β‰₯ 1 and 𝜏 β‰₯ 2 one has | | | | | 𝑛  π‘˜ = 0 ( βˆ’ 1 ) 𝑛 + π‘˜ ξ‚€ 𝑛 𝑛 π‘˜  𝑛 + π‘˜ + 𝜏 βˆ’ 1  ξ‚€ β‹… 𝑠 π‘˜ + 𝜏 | | | | | ≀ βˆ’ 𝛾 ( 𝜏 βˆ’ 1 ) ! . 2 𝑛 ( 𝑛 + 1 ) ( 𝑛 + 2 ) β‹― ( 𝑛 + 𝜏 ) ( 1 . 3 ) Particularly, by choosing 𝜏 = 𝑛 β‰₯ 2 , one gets the following result.

Corollary 1.2. For any integer 𝑛 β‰₯ 2 one has | | | | | 𝑛  π‘˜ = 0 ( βˆ’ 1 ) 𝑛 + π‘˜ ξ‚€ 𝑛 𝑛 π‘˜  2 𝑛 + π‘˜ βˆ’ 1  ξ‚€ β‹… 𝑠 𝑛 + π‘˜ | | | | | ≀ 1 βˆ’ 𝛾 2 𝑛 2 ξ€· 𝑛 2 𝑛 ξ€Έ ≀ 1 𝑛 3 / 2 β‹… 4 𝑛 . ( 1 . 4 )

Some authors have generalized the result of Proposition 1.1 under various aspects. At first one cites a result due to Rivoal [2].

Proposition (see [2]). For 𝑛 tending to infinity, one has | | | | | 1 𝛾 βˆ’ ( βˆ’ 2 ) 𝑛 𝑛  π‘˜ = 0 ( βˆ’ 1 ) π‘˜ ξ‚€ 𝑛 𝑛 π‘˜  𝑠 2 𝑛 + 2 π‘˜  ξ‚€ 2 π‘˜ + 𝑛 + 1 | | | | | ξ‚΅ 1 = π’ͺ 𝑛 2 7 𝑛 / 2 ξ‚Ά . ( 1 . 5 ) Kh. Hessami Pilehrood and T. Hessami Pilehrood have found some approximation formulas for the logarithms of some infinite products including Euler's constant 𝛾 . These results are obtained by using Euler-type integrals, hypergeometric series, and the Laplace method [3].

Proposition ([3]). For 𝑛 tending to infinity the following asymptotic formula holds: | | | | | 𝛾 βˆ’ 𝑛  π‘˜ = 0 ( βˆ’ 1 ) 𝑛 + π‘˜ ξ‚€ 𝑛 𝑛 π‘˜  𝑠 𝑛 + π‘˜  ξ‚€ π‘˜ + 𝑛 + 1 | | | | | = 1 4 𝑛 + π‘œ ( 𝑛 ) . ( 1 . 6 )

Recently the author has found series transformations involving three parameters 𝑛 , 𝜏 1 and 𝜏 2 , [4]. In Propositions 1.5 and 1.6 certain integral representations of the (discrete) series transformations are given, which exhibit important (analytical) tools to estimate the error terms of the transformations.

Proposition 1.5 (see [4]). Let 𝑛 β‰₯ 1 , 𝜏 1 β‰₯ 1 , and 𝜏 2 β‰₯ 1 be integers. Additionally one assumes that 1 + 𝜏 1 ≀ 𝜏 2 . ( 1 . 7 ) Then one has 𝑛  π‘˜ = 0 ( βˆ’ 1 ) 𝑛 + π‘˜ ξ‚€ 𝑛 + 𝜏 1 𝑛 𝑛 π‘˜  + π‘˜  ξ‚€ β‹… 𝑠 π‘˜ + 𝜏 2 βˆ’ 𝛾 = ( βˆ’ 1 ) 𝑛 + 1 ξ€œ 1 0 ξ‚΅ 1 + 1 1 βˆ’ 𝑒 ξ‚Ά 𝑙 π‘œ 𝑔 𝑒 β‹… 𝑒 𝜏 2 βˆ’ 𝜏 1 βˆ’ 1 β‹… πœ• 𝑛 πœ• 𝑒 𝑛 ξ‚΅ 𝑒 𝑛 + 𝜏 1 ( 1 βˆ’ 𝑒 ) 𝑛 ξ‚Ά 𝑛 ! 𝑑 𝑒 . ( 1 . 8 )

Proposition (see [4]). Let 𝑛 β‰₯ 1 , 𝜏 1 β‰₯ 1 and 𝜏 2 β‰₯ 1 be integers. Additionally one assumes that 1 + 𝜏 1 ≀ 𝜏 2 ≀ 1 + 𝑛 + 𝜏 1 . ( 1 . 9 ) Then one has 𝑛  π‘˜ = 0 ( βˆ’ 1 ) 𝑛 + π‘˜ ξ‚€ 𝑛 + 𝜏 1 𝑛 𝑛 π‘˜  + π‘˜  ξ‚€ β‹… 𝑠 π‘˜ + 𝜏 2 βˆ’ 𝛾 = ( βˆ’ 1 ) 𝑛 + 𝜏 2 βˆ’ 𝜏 1 ξ€œ 1 0 ξ€œ 1 0 𝑀 ( 𝑑 ) β‹… ( 1 βˆ’ 𝑒 ) 𝑛 + 𝜏 1 𝑒 𝑛 ( 1 βˆ’ 𝑑 ) 𝜏 2 βˆ’ 𝜏 1 βˆ’ 1 𝑑 𝑛 + 𝜏 1 βˆ’ 𝜏 2 + 1 ( 1 βˆ’ 𝑒 𝑑 ) 𝑛 + 1 𝑑 𝑒 𝑑 𝑑 , ( 1 . 1 0 ) with 1 𝑀 ( 𝑑 ) ∢ = ξ‚€ πœ‹ 𝑑 β‹… 2 + l o g 2 ξ‚€ 1 𝑑 . βˆ’ 1   ( 1 . 1 1 )

Setting 𝑛 = 𝜏 2 = 𝑑 π‘š , 𝜏 1 = ( 𝑑 βˆ’ 1 ) π‘š βˆ’ 1 , ( 𝑑 β‰₯ 2 ) , ( 1 . 1 2 ) one gets an explicit upper bound from Proposition 1.6

Corollary 1.7. For integers π‘š β‰₯ 2 , 𝑑 β‰₯ 3 , one has | | | | | 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ ξ‚€ ( π‘˜  2 𝑑 βˆ’ 1 ) π‘š + π‘˜ βˆ’ 1 𝑑 π‘š  ξ‚€ 𝑑 π‘š β‹… 𝑠 π‘˜ + 𝑑 π‘š | | | | | βˆ’ 𝛾 < 𝐢 𝑑 β‹… ξ‚΅ ( 1 βˆ’ 1 / 𝑑 ) 𝑑 ( 𝑑 βˆ’ 1 ) 4 𝑑 ξ‚Ά π‘š βˆ’ 2 , ( 1 . 1 3 ) where 0 < 𝐢 𝑑 ≀ 1 / 1 6 πœ‹ 2 is some constant depending only on 𝑑 . For 𝑑 = 2 one gets | | | | | 2 π‘š  π‘˜ = 0 ( βˆ’ 1 ) π‘˜ ξ‚€ π‘˜  3 π‘š + π‘˜ βˆ’ 1 2 π‘š  ξ‚€ 2 π‘š β‹… 𝑠 π‘˜ + 2 π‘š | | | | | < ξ‚€ βˆ’ 𝛾 1 6  7 πœ‹ 2 β‹… 1 6 4 π‘š ( π‘š β‰₯ 1 ) . ( 1 . 1 4 ) For an application of Corollary 1.7 let the integers 𝐡 π‘š and 𝐴 π‘š be defined by 𝐡 π‘š 𝐴 ∢ = 𝑙 . 𝑐 . π‘š . ( 1 , 2 , 3 , … , 4 π‘š ) , π‘š ∢ = 𝐡 π‘š 2 π‘š  π‘˜ = 0 ( βˆ’ 1 ) π‘˜ ξ‚΅ π‘˜ ξ‚Ά β‹… ξ‚€ 1 3 π‘š + π‘˜ βˆ’ 1 2 π‘š ξ‚Ά ξ‚΅ 2 π‘š 1 + 2 1 + β‹― +  . π‘˜ + 2 π‘š βˆ’ 1 ( 1 . 1 5 ) Ξ› ( π‘˜ ) denotes the von Mangoldt function. By [5, Theorem  434] one has  πœ“ ( π‘š ) ∢ = π‘˜ ≀ π‘š Ξ› ( π‘˜ ) ∼ π‘š . ( 1 . 1 6 ) Then, for πœ€ ∢ = ( l o g 5 5 ) / 4 βˆ’ 1 > 0 . 0 0 1 8 , there is some integer π‘š 0 such that 𝐡 π‘š = 𝑒 πœ“ ( 4 π‘š ) < 𝑒 4 ( 1 + πœ€ ) π‘š = 5 5 π‘š ξ€· π‘š β‰₯ π‘š 0 ξ€Έ . ( 1 . 1 7 ) Multiplying (1.14) by 𝐡 π‘š , we deduce the following corollary.

Corollary. There is an integer π‘š 0 such that one has for all integers π‘š β‰₯ π‘š 0 that | | | | | 𝐡 π‘š 2 π‘š  π‘˜ = 0 ( βˆ’ 1 ) π‘˜ ξ‚€ π‘˜  3 π‘š + π‘˜ βˆ’ 1 2 π‘š  ξ‚€ 2 π‘š β‹… l o g ( π‘˜ + 2 π‘š ) + 𝛾 𝐡 π‘š βˆ’ 𝐴 π‘š | | | | | < ξ‚€ 1 6  7 πœ‹ 2 β‹… ξ‚€ 5 5  6 4 π‘š . ( 1 . 1 8 )

2. Results on Rational Approximations to 𝜸

In 2007, Aptekarev and his collaborators [6] found rational approximations to 𝛾 , which are based on a linear third-order recurrence. For the sake of brevity, let 𝐷 ( 𝑛 ) = l . c . m . ( 1 , 2 , … , 𝑛 ) .

Proposition (see [6]). Let ( 𝑝 𝑛 ) 𝑛 β‰₯ 0 and ( π‘ž 𝑛 ) 𝑛 β‰₯ 0 be two solutions of the linear recurrence ( 1 6 𝑛 βˆ’ 1 5 ) ( 𝑛 + 1 ) 𝑒 𝑛 + 1 = ξ€· 1 2 8 𝑛 3 + 4 0 𝑛 2 ξ€Έ 𝑒 βˆ’ 8 2 𝑛 βˆ’ 4 5 𝑛 ξ€· βˆ’ 𝑛 2 5 6 𝑛 3 βˆ’ 2 4 0 𝑛 2 ξ€Έ 𝑒 + 6 4 𝑛 βˆ’ 7 𝑛 βˆ’ 1 + 𝑛 ( 𝑛 βˆ’ 1 ) ( 1 6 𝑛 + 1 ) 𝑒 𝑛 βˆ’ 2 ( 2 . 1 ) with 𝑝 0 = 0 , 𝑝 1 = 2 , 𝑝 2 = 3 1 / 2 and π‘ž 0 = 1 , π‘ž 1 = 3 , π‘ž 2 = 2 5 . Then, one has π‘ž 𝑛 ∈ β„€ , 𝐷 ( 𝑛 ) 𝑝 𝑛 ∈ β„€ , and | | | | 𝑝 𝛾 βˆ’ 𝑛 π‘ž 𝑛 | | | | ∼ 𝑐 0 𝑒 √ βˆ’ 2 2 𝑛 , | | π‘ž 𝑛 | | ∼ 𝑐 1 𝑛 1 / 4 ( 2 𝑛 ) ! 𝑒 𝑛 ! √ 2 𝑛 , ( 2 . 2 ) with two positive constants 𝑐 0 , 𝑐 1 . It seems interesting to replace the fraction 𝑝 𝑛 / π‘ž 𝑛 by 𝐴 𝑛 𝐡 𝑛 ∢ = 𝐷 ( 𝑛 ) 𝑝 𝑛 𝐷 ( 𝑛 ) π‘ž 𝑛 , ( 2 . 3 ) and to estimate the remainder in terms of 𝐡 𝑛 .

Corollary 2.2. Let 0 < πœ€ < 1 . Then there are two positive constants 𝑐 2 , 𝑐 3 , such that for all sufficiently large integers 𝑛 one has 𝑐 2 ξ‚€ √ e x p βˆ’ 2 ( 1 + πœ€ ) 2 √ l o g 𝐡 𝑛 / l o g l o g 𝐡 𝑛  < | | | | 𝐴 𝛾 βˆ’ 𝑛 𝐡 𝑛 | | | | < 𝑐 3 ξ‚€ √ e x p βˆ’ 2 ( 1 βˆ’ πœ€ ) 2 √ l o g 𝐡 𝑛 / l o g l o g 𝐡 𝑛  . ( 2 . 4 )

Recently, Rivoal [7] presented a related approach to the theory of rational approximations to Euler's constant 𝛾 , and, more generally, to rational approximations for values of derivatives of the Gamma function. He studied simultaneous Padé approximants to Euler's functions, from which he constructed a third-order recurrence formula that can be applied to construct a sequence in β„š ( 𝑧 ) that converges subexponentially to l o g ( 𝑧 ) + 𝛾 for any complex number 𝑧 ∈ β„‚ β§΅ ( βˆ’ ∞ , 0 ] . Here, l o g is defined by its principal branch. We cite a corollary from [7].

Proposition 2.3 (see [7]). (i) The recurrence ( 𝑛 + 3 ) 2 ( 8 𝑛 + 1 1 ) ( 8 𝑛 + 1 9 ) π‘ˆ 𝑛 + 3 = ξ€· 2 4 𝑛 2 ξ€Έ + 1 4 5 𝑛 + 2 1 5 ( 8 𝑛 + 1 1 ) π‘ˆ 𝑛 + 2 βˆ’ ξ€· 2 4 𝑛 3 + 1 0 5 𝑛 2 ξ€Έ + 1 2 4 𝑛 + 2 5 ( 8 𝑛 + 2 7 ) π‘ˆ 𝑛 + 1 + ( 𝑛 + 2 ) 2 ( 8 𝑛 + 1 9 ) ( 8 𝑛 + 2 7 ) π‘ˆ 𝑛 , ( 2 . 5 ) provides two sequences of rational numbers ( 𝑝 𝑛 ) 𝑛 β‰₯ 0 and ( π‘ž 𝑛 ) 𝑛 β‰₯ 0 with 𝑝 0 = βˆ’ 1 , 𝑝 1 = 4 , 𝑝 2 = 7 7 / 4 and π‘ž 0 = 1 , π‘ž 1 = 7 , π‘ž 2 = 6 5 / 2 such that ( 𝑝 𝑛 / π‘ž 𝑛 ) 𝑛 β‰₯ 0 converges to 𝛾 .(ii) The recurrence ( 𝑛 + 1 ) ( 𝑛 + 2 ) ( 𝑛 + 3 ) π‘ˆ 𝑛 + 3 = ξ€· 3 𝑛 2 ξ€Έ + 1 9 𝑛 + 2 9 ( 𝑛 + 1 ) π‘ˆ 𝑛 + 2 βˆ’ ξ€· 3 𝑛 3 + 6 𝑛 2 ξ€Έ π‘ˆ βˆ’ 7 𝑛 βˆ’ 1 3 𝑛 + 1 + ( 𝑛 + 2 ) 3 π‘ˆ 𝑛 , ( 2 . 6 ) provides two sequences of rational numbers ( 𝑝 𝑛 ) 𝑛 β‰₯ 0 and ( π‘ž 𝑛 ) 𝑛 β‰₯ 0 with 𝑝 0 = βˆ’ 1 , 𝑝 1 = 1 1 , 𝑝 2 = 7 1 and π‘ž 0 = 0 , π‘ž 1 = 8 , π‘ž 2 = 5 6 such that ( 𝑝 𝑛 / π‘ž 𝑛 ) 𝑛 β‰₯ 0 converges to l o g ( 2 ) + 𝛾 .

The goal of this paper is to construct rational approximations to 𝛾 + l o g ( π‘Ž / 𝑏 ) without using recurrences by a new application of series transformations. The transformed sequences of rationals are constructed as simple as possible, only with few concessions to the rate of convergence (see Theorems 2.4 and 6.2 below).

In the following we denote by 𝐡 2 𝑛 the Bernoulli numbers, that is, 𝐡 2 = 1 / 6 , 𝐡 4 = βˆ’ 1 / 3 0 , 𝐡 6 = 1 / 4 2 , and so on (In Sections 36 the Bernoulli numbers cannot be confused with the integers 𝐡 𝑛 from Corollary 2.2.) In this paper we will prove the following result.

Theorem 2.4. Let π‘Ž β‰₯ 1 , 𝑏 β‰₯ 1 , 𝑑 β‰₯ 4 2 and π‘š β‰₯ 1 be positive integers, and 𝑆 𝑛 ∢ = π‘Ž 𝑛 βˆ’ 1  𝑗 = 1 1 𝑗 βˆ’ 𝑏 𝑛 βˆ’ 1  𝑗 = 1 1 𝑗 + 2 𝑛 βˆ’ 1  𝑗 = 1 1 𝑗 βˆ’ 𝑛 2 βˆ’ 1  𝑗 = 1 1 𝑗 βˆ’ 1 2 𝑛 2 + 𝑑 π‘š  𝑗 = 1 𝐡 2 𝑗 ξ‚΅ 1 2 𝑗 𝑛 2 𝑗 ξ‚΅ 1 π‘Ž 2 𝑗 βˆ’ 1 𝑏 2 𝑗 ξ‚Ά βˆ’ 1 + 1 𝑛 4 𝑗 ξ‚Ά , ( 𝑛 β‰₯ 1 ) . ( 2 . 7 ) Then, | | | | | 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ ξ‚€ ( π‘˜  𝑆 2 𝑑 βˆ’ 1 ) π‘š + π‘˜ βˆ’ 1 𝑑 π‘š  ξ‚€ 𝑑 π‘š π‘˜ + 𝑑 π‘š π‘Ž βˆ’ 𝛾 βˆ’ l o g 𝑏 | | | | | < 𝑐 4 β‹… ξ‚΅ ( 1 βˆ’ 1 / 𝑑 ) 𝑑 ( 𝑑 βˆ’ 1 ) 4 𝑑 ξ‚Ά π‘š , ( 2 . 8 ) where 𝑐 4 is some positive constant depending only on 𝑑 .

3. Proof of Theorem 2.4

Lemma 3.1. One has for positive integers 𝑑 and π‘š ξ‚€ π‘˜  𝑔 ( π‘˜ ) ∢ = ( 2 𝑑 βˆ’ 1 ) π‘š + π‘˜ βˆ’ 1 𝑑 π‘š  ξ‚€ 𝑑 π‘š < 1 6 𝑑 π‘š ( 0 ≀ π‘˜ ≀ 𝑑 π‘š ) . ( 3 . 1 )

Proof. Applying the well known inequality ( 𝑔 β„Ž ) ≀ 2 𝑔 , we get ξ‚€ π‘˜  ( 2 𝑑 βˆ’ 1 ) π‘š + π‘˜ βˆ’ 1 𝑑 π‘š  ξ‚€ 𝑑 π‘š ≀ 2 ( 2 𝑑 βˆ’ 1 ) π‘š + 𝑑 π‘š βˆ’ 1 2 𝑑 π‘š = 2 4 𝑑 π‘š βˆ’ π‘š βˆ’ 1 < 1 6 𝑑 π‘š . ( 3 . 2 ) This proves the lemma.

𝑔 ( π‘˜ ) takes its maximum value for π‘˜ = π‘˜ 0 with π‘˜ 0 = √ 5 𝑑 2 βˆ’ 4 𝑑 + 1 βˆ’ 𝑑 + 1 2 π‘š + π’ͺ ( 1 ) , ( 3 . 3 ) which leads to a better bound than 1 6 𝑑 π‘š in Lemma 3.1. But we are satisfied with Lemma 3.1. A main tool in proving Theorem 2.4 is Euler's summation formula in the form 𝑛  𝑖 = 1 ξ€œ 𝑓 ( 𝑖 ) = 𝑛 1 𝑓 ( π‘₯ ) 𝑑 π‘₯ + 𝑓 ( 1 ) + 𝑓 ( 𝑛 ) 2 + π‘Ÿ  𝑗 = 1 𝐡 2 𝑗 ξ€· 𝑓 ( 2 𝑗 ) ! ( 2 𝑗 βˆ’ 1 ) ( 𝑛 ) βˆ’ 𝑓 ( 2 𝑗 βˆ’ 1 ) ξ€Έ ( 1 ) + 𝑅 π‘Ÿ , ( 3 . 4 ) where π‘Ÿ ∈ β„• is a suitable chosen parameter, and the remainder 𝑅 π‘Ÿ is defined by a periodic Bernoulli polynomial 𝑃 2 π‘Ÿ + 1 ( π‘₯ ) , namely 𝑅 π‘Ÿ = 1 ( ξ€œ 2 π‘Ÿ + 1 ) ! 𝑛 1 𝑃 2 π‘Ÿ + 1 ( π‘₯ ) 𝑓 ( 2 π‘Ÿ + 1 ) ( π‘₯ ) 𝑑 π‘₯ , ( 3 . 5 ) with 𝑃 2 π‘Ÿ + 1 ( π‘₯ ) = ( βˆ’ 1 ) π‘Ÿ βˆ’ 1 ( 2 π‘Ÿ + 1 ) ! ∞  𝑗 = 1 2 s i n ( 2 πœ‹ 𝑗 π‘₯ ) ( 2 πœ‹ 𝑗 ) 2 π‘Ÿ + 1 . ( 3 . 6 ) Applying the summation formula to the function 𝑓 ( π‘₯ ) = 1 / π‘₯ , we get (see [8, equation ( 5)] ) 𝑛 βˆ’ 1  𝑖 = 1 1 𝑖 1 = l o g 𝑛 + 2 βˆ’ 1 + 2 𝑛 π‘Ÿ  𝑗 = 1 𝐡 2 𝑗 ξ‚€ 1 2 𝑗 1 βˆ’ 𝑛 2 𝑗  βˆ’ ξ€œ 𝑛 1 𝑃 2 π‘Ÿ + 1 ( π‘₯ ) π‘₯ 2 π‘Ÿ + 2 𝑑 π‘₯ , ( 𝑛 , π‘Ÿ ∈ β„• ) . ( 3 . 7 ) It follows that 𝑛 2 βˆ’ 1  𝑖 = 𝑛 1 𝑖 1 βˆ’ l o g 𝑛 = βˆ’ 1 2 𝑛 2 𝑛 2 + π‘Ÿ  𝑗 = 1 𝐡 2 𝑗 ξ‚€ 1 2 𝑗 𝑛 2 𝑗 βˆ’ 1 𝑛 4 𝑗  βˆ’ ξ€œ 𝑛 2 𝑛 𝑃 2 π‘Ÿ + 1 ( π‘₯ ) π‘₯ 2 π‘Ÿ + 2 𝑑 π‘₯ , ( 𝑛 , π‘Ÿ ∈ β„• ) . ( 3 . 8 ) We prove Theorem 2.4 for π‘Ž β‰₯ 𝑏 . The case π‘Ž < 𝑏 is treated similarly. So we have again by the above summation formula that π‘Ž 𝑛 βˆ’ 1  𝑖 = 𝑏 𝑛 1 𝑖 π‘Ž βˆ’ l o g 𝑏 = ξ‚€ 1 𝑏 βˆ’ 1 π‘Ž  1 + 2 𝑛 π‘Ÿ  𝑗 = 1 𝐡 2 𝑗 2 𝑗 𝑛 2 𝑗 ξ‚΅ 1 𝑏 2 𝑗 βˆ’ 1 π‘Ž 2 𝑗 ξ‚Ά βˆ’ ξ€œ π‘Ž 𝑛 𝑏 𝑛 𝑃 2 π‘Ÿ + 1 ( π‘₯ ) π‘₯ 2 π‘Ÿ + 2 𝑑 π‘₯ , ( 𝑛 , π‘Ÿ ∈ β„• ) . ( 3 . 9 ) First, we estimate the integral on the right-hand side of (3.8). We have | | | | ξ€œ 𝑛 2 𝑛 𝑃 2 π‘Ÿ + 1 ( π‘₯ ) π‘₯ 2 π‘Ÿ + 2 | | | | ≀ ξ€œ 𝑑 π‘₯ 𝑛 2 𝑛 | | 𝑃 2 π‘Ÿ + 1 | | ( π‘₯ ) π‘₯ 2 π‘Ÿ + 2 ξ€œ 𝑑 π‘₯ ≀ ∞ 𝑛 | | 𝑃 2 π‘Ÿ + 1 | | ( π‘₯ ) π‘₯ 2 π‘Ÿ + 2 ξ€œ 𝑑 π‘₯ ≀ 2 ( 2 π‘Ÿ + 1 ) ! ∞ 𝑛 1 π‘₯ ∞ 2 π‘Ÿ + 2  𝑗 = 1 1 ( 2 πœ‹ 𝑗 ) 2 π‘Ÿ + 1 = 𝑑 π‘₯ 2 ( 2 π‘Ÿ + 1 ) ! ( 2 πœ‹ ) 2 π‘Ÿ + 1 ξ‚Έ βˆ’ 1 ( 2 π‘Ÿ + 1 ) π‘₯ 2 π‘Ÿ + 1 ξ‚Ή ∞ ∞ π‘₯ = 𝑛  𝑗 = 1 1 𝑗 2 π‘Ÿ + 1 = 2 ( 2 π‘Ÿ ) ! ( 2 πœ‹ ) 2 π‘Ÿ + 1 𝑛 2 π‘Ÿ + 1 𝜁 ( 2 π‘Ÿ + 1 ) < 3 ( 2 π‘Ÿ ) ! ( 2 πœ‹ ) 2 π‘Ÿ + 1 𝑛 2 π‘Ÿ + 1 , ( 3 . 1 0 ) since 2 𝜁 ( 2 π‘Ÿ + 1 ) ≀ 2 𝜁 ( 3 ) < 3 . Next, we assume that 𝑛 β‰₯ π‘Ž . Hence [ 𝑏 𝑛 , π‘Ž 𝑛 ] βŠ† [ 𝑛 , 𝑛 2 ] , and therefore we estimate the integral on the right-hand side in (3.9) by | | | | ξ€œ π‘Ž 𝑛 𝑏 𝑛 𝑃 2 π‘Ÿ + 1 ( π‘₯ ) π‘₯ 2 π‘Ÿ + 2 | | | | ≀ ξ€œ 𝑑 π‘₯ π‘Ž 𝑛 𝑏 𝑛 | | 𝑃 2 π‘Ÿ + 1 | | ( π‘₯ ) π‘₯ 2 π‘Ÿ + 2 ≀ ξ€œ 𝑑 π‘₯ 𝑛 2 𝑛 | | 𝑃 2 π‘Ÿ + 1 | | ( π‘₯ ) π‘₯ 2 π‘Ÿ + 2 𝑑 π‘₯ ≀ 3 ( 2 π‘Ÿ ) ! ( 2 πœ‹ ) 2 π‘Ÿ + 1 𝑛 2 π‘Ÿ + 1 . ( 3 . 1 1 ) In the sequel we put π‘Ÿ = 𝑑 π‘š . Moreover, in the above formula we now replace 𝑛 by 𝑑 π‘š + π‘˜ with 0 ≀ π‘˜ ≀ 𝑑 π‘š . In order to estimate ( 2 π‘Ÿ ) ! we use Stirling's formula √ ξ‚€ π‘š 2 πœ‹ π‘š 𝑒  π‘š √ < π‘š ! < ξ‚€ π‘š 2 πœ‹ ( π‘š + 1 ) 𝑒  π‘š , ( π‘š > 0 ) . ( 3 . 1 2 ) Then, it follows that | | | | ξ€œ ( 𝑑 π‘š + π‘˜ ) 2 𝑑 π‘š + π‘˜ 𝑃 2 π‘Ÿ + 1 ( π‘₯ ) π‘₯ 2 π‘Ÿ + 2 | | | | ≀ 𝑑 π‘₯ 3 ( 2 π‘Ÿ ) ! ( 2 πœ‹ ) 2 π‘Ÿ + 1 ( 𝑑 π‘š + π‘˜ ) 2 π‘Ÿ + 1 ≀ 3 ( 2 π‘Ÿ ) ! ( 2 πœ‹ ) 2 π‘Ÿ + 1 ( 𝑑 π‘š ) 2 π‘Ÿ + 1 = 3 ( 2 𝑑 π‘š ) ! ( 2 πœ‹ ) 2 𝑑 π‘š + 1 ( 𝑑 π‘š ) 2 𝑑 π‘š + 1 ≀ 3 √ πœ‹ ( 2 𝑑 π‘š + 1 ) ( 2 πœ‹ 𝑑 π‘š ) 2 𝑑 π‘š + 1 β‹… ξ‚€ 2 𝑑 π‘š 𝑒  2 𝑑 π‘š ≀ 3 √ 3 πœ‹ 𝑑 π‘š ( 2 πœ‹ 𝑑 π‘š ) ( πœ‹ 𝑒 ) 2 𝑑 π‘š , ( 3 . 1 3 ) and similarly we have | | | | ξ€œ π‘Ž ( 𝑑 π‘š + π‘˜ ) 𝑏 ( 𝑑 π‘š + π‘˜ ) 𝑃 2 π‘Ÿ + 1 ( π‘₯ ) π‘₯ 2 π‘Ÿ + 2 | | | | ≀ 3 √ 𝑑 π‘₯ 3 πœ‹ 𝑑 π‘š ( 2 πœ‹ 𝑑 π‘š ) ( πœ‹ 𝑒 ) 2 𝑑 π‘š , ( 𝑑 π‘š β‰₯ π‘Ž ) . ( 3 . 1 4 ) By using the definition of 𝑆 𝑛 in Theorem 2.4, the formula (1.1) for 𝑠 𝑛 , and the identities (3.8), (3.9), it follows that 𝑆 𝑛 π‘Ž βˆ’ 𝛾 βˆ’ l o g 𝑏 = ξ€· 𝑠 𝑛 ξ€Έ + ξ€· 𝑠 βˆ’ 𝛾 𝑛 βˆ’ 𝑠 2 𝑛 ξ€Έ + ξ€· 𝑠 π‘Ž 𝑛 βˆ’ 𝑠 𝑏 𝑛 ξ€Έ βˆ’ 1 2 𝑛 2 + π‘Ÿ  𝑗 = 1 𝐡 2 𝑗 ξ‚΅ 1 2 𝑗 𝑛 2 𝑗 ξ‚΅ 1 π‘Ž 2 𝑗 βˆ’ 1 𝑏 2 𝑗 ξ‚Ά βˆ’ 1 + 1 𝑛 4 𝑗 ξ‚Ά = ξ€· 𝑠 𝑛 ξ€Έ + 1 βˆ’ 𝛾 ξ‚€ 1 2 𝑛 𝑏 βˆ’ 1 π‘Ž  + ξ€œ βˆ’ 1 𝑛 2 𝑛 𝑃 2 π‘Ÿ + 1 ( π‘₯ ) π‘₯ 2 π‘Ÿ + 2 ξ€œ 𝑑 π‘₯ βˆ’ π‘Ž 𝑛 𝑏 𝑛 𝑃 2 π‘Ÿ + 1 ( π‘₯ ) π‘₯ 2 π‘Ÿ + 2 𝑑 π‘₯ , ( 3 . 1 5 ) where π‘Ÿ is specified to π‘Ÿ = 𝑑 π‘š and 𝑛 to 𝑛 = 𝑑 π‘š + π‘˜ . Moreover, we know from [4, Lemma  2] that 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) = 1 , ( π‘š β‰₯ 1 ) . ( 3 . 1 6 ) By setting 𝑛 = 𝑑 π‘š + π‘˜ , the above formula for the series transformation of 𝑆 𝑑 π‘š + π‘˜ simplifies to | | | | | 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) 𝑆 𝑑 π‘š + π‘˜ π‘Ž βˆ’ 𝛾 βˆ’ l o g 𝑏 | | | | | = | | | | | 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ ξ€· 𝑠 𝑔 ( π‘˜ ) 𝑑 π‘š + π‘˜ ξ€Έ + 1 βˆ’ 𝛾 2 ξ‚€ 1 𝑏 βˆ’ 1 π‘Ž  βˆ’ 1 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) + 𝑑 π‘š + π‘˜ 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ ξ€œ 𝑔 ( π‘˜ ) ( 𝑑 π‘š + π‘˜ ) 2 𝑑 π‘š + π‘˜ 𝑃 2 π‘Ÿ + 1 ( π‘₯ ) π‘₯ 2 π‘Ÿ + 2 βˆ’ 𝑑 π‘₯ 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ ξ€œ 𝑔 ( π‘˜ ) π‘Ž ( 𝑑 π‘š + π‘˜ ) 𝑏 ( 𝑑 π‘š + π‘˜ ) 𝑃 2 π‘Ÿ + 1 ( π‘₯ ) π‘₯ 2 π‘Ÿ + 2 | | | | | ≀ | | | | | 𝑑 π‘₯ 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ ξ€· 𝑠 𝑔 ( π‘˜ ) 𝑑 π‘š + π‘˜ ξ€Έ | | | | | + βˆ’ 𝛾 𝑑 π‘š  π‘˜ = 0 | | | | ξ€œ 𝑔 ( π‘˜ ) ( 𝑑 π‘š + π‘˜ ) 2 𝑑 π‘š + π‘˜ 𝑃 2 π‘Ÿ + 1 ( π‘₯ ) π‘₯ 2 π‘Ÿ + 2 | | | | + 𝑑 π‘₯ 𝑑 π‘š  π‘˜ = 0 | | | | ξ€œ 𝑔 ( π‘˜ ) π‘Ž ( 𝑑 π‘š + π‘˜ ) 𝑏 ( 𝑑 π‘š + π‘˜ ) 𝑃 2 π‘Ÿ + 1 ( π‘₯ ) π‘₯ 2 π‘Ÿ + 2 | | | | 𝑑 π‘₯ < 𝐢 𝑑 β‹… ξ‚΅ ( 1 βˆ’ 1 / 𝑑 ) 𝑑 ( 𝑑 βˆ’ 1 ) 4 𝑑 ξ‚Ά π‘š βˆ’ 2 + 𝑑 π‘š  π‘˜ = 0 3 √ 𝑔 ( π‘˜ ) 3 πœ‹ 𝑑 π‘š πœ‹ 𝑑 π‘š ( πœ‹ 𝑒 ) 2 𝑑 π‘š , ( 3 . 1 7 ) where 𝑑 π‘š β‰₯ π‘Ž , π‘š β‰₯ 2 , and 𝑑 β‰₯ 3 . Here, we have used the results from Corollary 1.7, (3.13), and (3.14). The sum 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) 𝑑 π‘š + π‘˜ ( 3 . 1 8 ) vanishes, since for every real number π‘₯ > βˆ’ 𝑑 π‘š we have 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ ξ€· ( 2 𝑑 βˆ’ 1 ) π‘š + π‘˜ βˆ’ 1 𝑑 π‘š ξ€Έ ξ€· π‘˜ 𝑑 π‘š ξ€Έ = 𝑑 π‘š + π‘˜ + π‘₯ ( 1 βˆ’ ( 𝑑 βˆ’ 1 ) π‘š + π‘₯ ) β‹― ( π‘š + π‘₯ ) ( 𝑑 π‘š + π‘₯ ) 𝑑 π‘š + 1 , ( 3 . 1 9 ) where on the right-hand side for an integer π‘₯ with βˆ’ π‘š ≀ π‘₯ ≀ ( 𝑑 βˆ’ 1 ) π‘š βˆ’ 1 one term in the numerator equals to zero.

The inequality ξ‚΅ 6 4 ( πœ‹ 𝑒 ) 2 ξ‚Ά 𝑑 < ( 1 βˆ’ 1 / 𝑑 ) 𝑑 2 ( 𝑑 βˆ’ 1 ) ( 3 . 2 0 ) holds for all integers 𝑑 β‰₯ 4 2 . Now, using Lemma 3.1, we estimate the right-hand side in (3.17) for 𝑑 π‘š β‰₯ π‘Ž and 𝑑 β‰₯ 4 2 as follows: | | | | | 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) 𝑆 𝑑 π‘š + π‘˜ π‘Ž βˆ’ 𝛾 βˆ’ l o g 𝑏 | | | | | < 𝐢 𝑑 β‹… ξ‚΅ ( 1 βˆ’ 1 / 𝑑 ) 𝑑 ( 𝑑 βˆ’ 1 ) 4 𝑑 ξ‚Ά π‘š βˆ’ 2 + 𝑑 π‘š  π‘˜ = 0 3 √ 3 πœ‹ 𝑑 π‘š πœ‹ 𝑑 π‘š 1 6 𝑑 π‘š ( πœ‹ 𝑒 ) 2 𝑑 π‘š = 𝐢 𝑑 β‹… ξ‚΅ ( 1 βˆ’ 1 / 𝑑 ) 𝑑 ( 𝑑 βˆ’ 1 ) 4 𝑑 ξ‚Ά π‘š βˆ’ 2 + √ 3 ( 𝑑 π‘š + 1 ) 3 𝑑 π‘š √ 𝑑 π‘š πœ‹ 1 4 𝑑 π‘š ξ‚΅ 6 4 ( πœ‹ 𝑒 ) 2 ξ‚Ά 𝑑 π‘š ( 3 . 2 0 ) < 𝐢 𝑑 β‹… ξ‚΅ ( 1 βˆ’ 1 / 𝑑 ) 𝑑 ( 𝑑 βˆ’ 1 ) 4 𝑑 ξ‚Ά π‘š βˆ’ 2 + √ 3 ( 𝑑 π‘š + 1 ) 3 𝑑 π‘š 𝑑 π‘š 2 π‘š √ πœ‹ ξ‚΅ ( 1 βˆ’ 1 / 𝑑 ) 𝑑 ( 𝑑 βˆ’ 1 ) 4 𝑑 ξ‚Ά π‘š ≀ 𝐢 𝑑 β‹… ξ‚΅ ( 1 βˆ’ 1 / 𝑑 ) 𝑑 ( 𝑑 βˆ’ 1 ) 4 𝑑 ξ‚Ά π‘š βˆ’ 2 + 8 5 ξ‚™ 2 8 3 𝑑 πœ‹ ξ‚΅ ( 1 βˆ’ 1 / 𝑑 ) 𝑑 ( 𝑑 βˆ’ 1 ) 4 𝑑 ξ‚Ά π‘š ≀ 𝑐 4 ξ‚΅ ( 1 βˆ’ 1 / 𝑑 ) 𝑑 ( 𝑑 βˆ’ 1 ) 4 𝑑 ξ‚Ά π‘š . ( 3 . 2 1 ) The last but one estimate holds for all integers π‘š β‰₯ 2 , 𝑑 β‰₯ 4 2 , and 𝑐 4 is a suitable positive real constant depending on 𝑑 . This completes the proof of Theorem 2.4.

4. On the Denominators of 𝐒 𝐧

In this section we will investigate the size of the denominators 𝑏 π‘š of our series transformations π‘Ž π‘š 𝑏 π‘š = 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) 𝑆 π‘˜ + 𝑑 π‘š , ( 4 . 1 ) for π‘š tending to infinity, where π‘Ž π‘š ∈ β„€ and 𝑏 π‘š ∈ β„• are coprime integers.

Theorem 4.1. For every π‘š β‰₯ 1 there is an integer 𝑍 π‘š with 𝑍 π‘š > 0 , 𝑏 π‘š | 𝑍 π‘š , and l o g 𝑍 π‘š ∼ 1 2 𝑑 2 π‘š 2 , ( π‘š ⟢ ∞ ) . ( 4 . 2 )

Proof. We will need some basic facts on the arithmetical functions πœ— ( π‘₯ ) and πœ“ ( π‘₯ ) . Let  πœ— ( π‘₯ ) = 𝑝 ≀ π‘₯  l o g 𝑝 , ( π‘₯ > 1 ) , πœ“ ( π‘₯ ) = 𝑝 ≀ π‘₯ ξ‚Έ l o g π‘₯ ξ‚Ή l o g 𝑝 l o g 𝑝 , ( π‘₯ > 1 ) , ( 4 . 3 ) where 𝑝 is restricted on primes. Moreover, let 𝐷 𝑛 ∢ = l . c . m ( 1 , 2 , … , 𝑛 ) for positive integers 𝑛 . Then, πœ“ ( 𝑛 ) = l o g 𝐷 𝑛 , ( 𝑛 β‰₯ 1 ) , ( 4 . 4 ) πœ“ ( π‘₯ ) ∼ πœ— ( π‘₯ ) ∼ πœ‹ ( π‘₯ ) l o g π‘₯ ∼ π‘₯ , ( π‘₯ ⟢ ∞ ) , ( 4 . 5 ) where (4.5) follows from [5, Theorem  420] and the prime number theorem. By [5, Theorem  118] (von Staudt's theorem) we know how to obtain the prime divisors of the denominators of Bernoulli numbers 𝐡 2 π‘˜ : The denominators of 𝐡 2 π‘˜ are squarefree, and they are divisible exactly by those primes 𝑝 with ( 𝑝 βˆ’ 1 ) ∣ 2 π‘˜ . Hence, 𝐡 2 π‘˜  𝑝 ≀ 2 π‘˜ + 1 𝑝 ∈ β„€ , ( π‘˜ = 1 , 2 , … ) . ( 4 . 6 ) Next, let m a x { π‘Ž , 𝑏 } ≀ 𝑑 π‘š ≀ 𝑛 ≀ 2 𝑑 π‘š ( 𝑛 = π‘˜ + 𝑑 π‘š are the subscripts of 𝑆 π‘˜ + 𝑑 π‘š in Theorem 2.4). First, we consider the following terms from the series transformation in 𝑆 π‘š : π‘Ž 𝑛 βˆ’ 1  𝑗 = 1 1 𝑗 βˆ’ 𝑏 𝑛 βˆ’ 1  𝑗 = 1 1 𝑗 + 2 𝑛 βˆ’ 1  𝑗 = 1 1 𝑗 βˆ’ 𝑛 2 βˆ’ 1  𝑗 = 1 1 𝑗 = ∢ 𝑛 2 βˆ’ 1  𝑗 = 1 𝑒 𝑗 𝑗 , ( 4 . 7 ) with 𝑒 𝑗 ⎧ βŽͺ βŽͺ ⎨ βŽͺ βŽͺ ⎩ ∢ = 1 , i f 1 ≀ 𝑗 ≀ 𝑛 βˆ’ 1 βˆ’ 1 , i f 𝑛 ≀ 𝑗 ≀ 𝑏 𝑛 βˆ’ 1 0 , i f 𝑏 𝑛 ≀ 𝑗 ≀ π‘Ž 𝑛 βˆ’ 1 βˆ’ 1 , i f π‘Ž 𝑛 ≀ 𝑗 ≀ 𝑛 2 βˆ’ 1 ( π‘Ž β‰₯ 𝑏 ) , 𝑒 𝑗 ⎧ βŽͺ βŽͺ ⎨ βŽͺ βŽͺ ⎩ ∢ = 1 , i f 1 ≀ 𝑗 ≀ 𝑛 βˆ’ 1 βˆ’ 1 , i f 𝑛 ≀ 𝑗 ≀ π‘Ž 𝑛 βˆ’ 1 βˆ’ 2 , i f π‘Ž 𝑛 ≀ 𝑗 ≀ 𝑏 𝑛 βˆ’ 1 βˆ’ 1 , i f 𝑏 𝑛 ≀ 𝑗 ≀ 𝑛 2 βˆ’ 1 . ( π‘Ž < 𝑏 ) . ( 4 . 8 ) For every π‘š β‰₯ 1 there is a rational π‘₯ π‘š / 𝑦 π‘š defined by π‘₯ π‘š 𝑦 π‘š = 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) ( π‘˜ + 𝑑 π‘š ) 2 βˆ’ 1  𝑗 = 1 𝑒 𝑗 𝑗 , ( 4 . 9 ) where π‘₯ π‘š ∈ β„€ , 𝑦 π‘š ∈ β„• , ( π‘₯ π‘š , 𝑦 π‘š ) = 1 , and 𝑦 π‘š ∣ π‘Œ π‘š ∢ = 𝐷 4 𝑑 2 π‘š 2 , ( 𝑑 π‘š β‰₯ m a x { π‘Ž , 𝑏 } ) . ( 4 . 1 0 ) Similarly, we define rationals 𝑒 π‘š / 𝑣 π‘š by 𝑒 π‘š 𝑣 π‘š = 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ Γ—  βˆ’ 1 𝑔 ( π‘˜ ) 2 ( π‘˜ + 𝑑 π‘š ) 2 + 𝑑 π‘š  𝑗 = 1 𝐡 2 𝑗 ξ‚΅ 1 2 𝑗 ( π‘˜ + 𝑑 π‘š ) 2 𝑗 ξ‚΅ 1 π‘Ž 2 𝑗 βˆ’ 1 𝑏 2 𝑗 ξ‚Ά βˆ’ 1 + 1 ( π‘˜ + 𝑑 π‘š ) 4 𝑗 ξ‚Ά ξƒͺ , ( 4 . 1 1 ) where 𝑒 π‘š ∈ β„€ , 𝑣 π‘š ∈ β„• and ( 𝑒 π‘š , 𝑣 π‘š ) = 1 . We have ( π‘˜ + 𝑑 π‘š ) 2 𝑗 ∣ ( π‘˜ + 𝑑 π‘š ) 4 𝑑 π‘š , ( 0 ≀ π‘˜ ≀ 𝑑 π‘š , 1 ≀ 𝑗 ≀ 𝑑 π‘š ) . ( 4 . 1 2 ) Therefore, using the conclusion (4.6) from von Staudt's theorem, we get 𝑣 π‘š ∣ 𝑉 π‘š ∢ = 2 ( π‘Ž 𝑏 ) 2 𝑑 π‘š 𝐷 𝑑 π‘š   𝑝 ≀ 2 𝑑 π‘š + 1 𝑝 ξƒͺ ξ€· 𝐷 2 𝑑 π‘š ξ€Έ 4 𝑑 π‘š , ( 𝑑 π‘š β‰₯ m a x { π‘Ž , 𝑏 } ) . ( 4 . 1 3 ) Note that 𝐷 2 𝑑 π‘š = l . c . m . ( 𝑑 π‘š , … , 2 𝑑 π‘š ) , since every integer 𝑛 1 with 1 ≀ 𝑛 1 < 𝑑 π‘š divides at least one integer 𝑛 2 with 𝑑 π‘š ≀ 𝑛 2 ≀ 2 𝑑 π‘š .
From (4.10) and (4.13) we conclude on 𝑏 π‘š ∣ 𝑍 π‘š ∢ = 2 ( π‘Ž 𝑏 ) 2 𝑑 π‘š 𝐷 𝑑 π‘š 𝐷 4 𝑑 2 π‘š 2 ξ€· 𝐷 2 𝑑 π‘š ξ€Έ 4 𝑑 π‘š   𝑝 ≀ 2 𝑑 π‘š + 1 𝑝 ξƒͺ . ( 4 . 1 4 ) Hence we have from (4.4) and (4.5) that l o g 𝑍 π‘š ξ€· = l o g 2 + 2 𝑑 π‘š l o g ( π‘Ž 𝑏 ) + πœ“ ( 𝑑 π‘š ) + πœ“ 4 𝑑 2 π‘š 2 ξ€Έ + 4 𝑑 π‘š πœ“ ( 2 𝑑 π‘š ) + πœ— ( 2 𝑑 π‘š + 1 ) ∼ l o g 2 + 2 𝑑 π‘š l o g ( π‘Ž 𝑏 ) + 𝑑 π‘š + 4 𝑑 2 π‘š 2 + 8 𝑑 2 π‘š 2 + ( 2 𝑑 π‘š + 1 ) = 1 + l o g 2 + ( 3 + 2 l o g ( π‘Ž 𝑏 ) ) 𝑑 π‘š + 1 2 𝑑 2 π‘š 2 ∼ 1 2 𝑑 2 π‘š 2 ( π‘š ⟢ ∞ ) . ( 4 . 1 5 ) The theorem is proved.

Remark 4.2. On the one side we have shown that l o g π‘Œ π‘š ∼ 4 𝑑 2 π‘š 2 and l o g 𝑉 π‘š ∼ 8 𝑑 2 π‘š 2 . On the other side, every prime 𝑝 dividing 𝑉 π‘š satisfies 𝑝 ≀ m a x { π‘Ž , 𝑏 , 𝑑 π‘š , 2 𝑑 π‘š + 1 , 2 𝑑 π‘š } = 2 𝑑 π‘š + 1 and therefore 𝑝 divides π‘Œ π‘š = 𝐷 4 𝑑 2 π‘š 2 . Conversely, all primes 𝑝 with 2 𝑑 π‘š + 1 < 𝑝 < 4 𝑑 2 π‘š 2 divide π‘Œ π‘š , but not 𝑉 π‘š . That means: 𝑉 π‘š is much bigger than π‘Œ π‘š , but 𝑉 π‘š is formed by powers of small primes, whereas π‘Œ π‘š is divisible by many big primes.

5. Simplification of the Transformed Series

Let 𝑅 𝑛 1 ∢ = βˆ’ 2 𝑛 2 + 𝑑 π‘š  𝑗 = 1 𝐡 2 𝑗 ξ‚΅ 1 2 𝑗 𝑛 2 𝑗 ξ‚΅ 1 π‘Ž 2 𝑗 βˆ’ 1 𝑏 2 𝑗 ξ‚Ά βˆ’ 1 + 1 𝑛 4 𝑗 ξ‚Ά , ( 5 . 1 ) such that 𝑆 𝑛 = π‘Ž 𝑛 βˆ’ 1  𝑗 = 1 1 𝑗 βˆ’ 𝑏 𝑛 βˆ’ 1  𝑗 = 1 1 𝑗 + 2 𝑛 βˆ’ 1  𝑗 = 1 1 𝑗 βˆ’ 𝑛 2 βˆ’ 1  𝑗 = 1 1 𝑗 + 𝑅 𝑛 . ( 5 . 2 ) In Theorem 2.4 the sequence 𝑆 𝑛 is transformed. In view of a simplified process we now investigate the transformation of the series 𝑆 𝑛 βˆ’ 𝑅 𝑛 . Therefore we have to estimate the contribution of 𝑅 π‘˜ + 𝑑 π‘š to the series transformation in Theorem 2.4. For this purpose, we define 𝐸 π‘š ∢ = 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ ξ‚€ π‘˜  𝑅 ( 2 𝑑 βˆ’ 1 ) π‘š + π‘˜ βˆ’ 1 𝑑 π‘š  ξ‚€ 𝑑 π‘š π‘˜ + 𝑑 π‘š 1 = βˆ’ 2 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) ( 𝑑 π‘š + π‘˜ ) 2 + 𝑑 π‘š  𝑗 = 1 𝐡 2 𝑗  ξ‚΅ 1 2 𝑗 π‘Ž 2 𝑗 βˆ’ 1 𝑏 2 𝑗 ξ‚Ά + 1 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) ( 𝑑 π‘š + π‘˜ ) 2 𝑗 βˆ’ 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) ( 𝑑 π‘š + π‘˜ ) 4 𝑗 ξƒͺ . ( 5 . 3 ) A major step in estimating 𝐸 π‘š is to expressthe sums on the right-hand side by integrals.

Lemma 5.1. For positive integers 𝑑 , 𝑗 and π‘š one has 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) ( 𝑑 π‘š + π‘˜ ) 2 𝑗 = βˆ’ ( βˆ’ 1 ) 𝑑 π‘š ξ€œ ( 𝑑 π‘š ) ! ( 2 𝑗 βˆ’ 1 ) ! 1 0 𝑒 π‘š ( l o g 𝑒 ) 2 𝑗 βˆ’ 1 πœ• 𝑑 π‘š πœ• 𝑒 𝑑 π‘š ξ€· 𝑒 ( 2 𝑑 βˆ’ 1 ) π‘š βˆ’ 1 ( 1 βˆ’ 𝑒 ) 𝑑 π‘š ξ€Έ 𝑑 𝑒 . ( 5 . 4 )

Proof. For integers π‘˜ , π‘Ÿ and a real number 𝜌 with π‘˜ + 𝜌 > 0 the identity 1 ( π‘˜ + 𝜌 ) π‘Ÿ = 1 ξ€œ ( π‘Ÿ βˆ’ 1 ) ! ∞ 0 𝑒 βˆ’ ( π‘˜ + 𝜌 ) 𝑑 𝑑 π‘Ÿ βˆ’ 1 𝑑 𝑑 ( 5 . 5 ) holds, which we apply with π‘Ÿ = 2 𝑗 and 𝜌 = 𝑑 π‘š to substitute the fraction 1 / ( 𝑑 π‘š + π‘˜ ) 2 𝑗 . Introducing the new variable 𝑒 ∢ = 𝑒 βˆ’ 𝑑 , we then get 2 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) ( π‘˜ + 𝑑 π‘š ) 2 𝑗 = βˆ’ ( βˆ’ 1 ) 𝑑 π‘š ( 2 𝑗 βˆ’ 1 ) ! 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) π‘˜ ξ€œ 𝑔 ( π‘˜ ) 1 0 𝑒 π‘˜ + 𝑑 π‘š βˆ’ 1 ( l o g 𝑒 ) 2 𝑗 βˆ’ 1 𝑑 𝑒 = βˆ’ ( βˆ’ 1 ) 𝑑 π‘š ξ€œ ( 2 𝑗 βˆ’ 1 ) ! 1 0  𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) π‘˜ 𝑔 ( π‘˜ ) 𝑒 π‘˜ + ( 𝑑 βˆ’ 1 ) π‘š βˆ’ 1 ξƒͺ 𝑒 π‘š ( l o g 𝑒 ) 2 𝑗 βˆ’ 1 𝑑 𝑒 . ( 5 . 6 ) The sum inside the brackets of the integrand can be expressed by using the equation 𝑛  π‘˜ = 0 ( βˆ’ 1 ) π‘˜ ξ‚€ 𝑛 𝑛 π‘˜  𝑒 𝑛 + 𝜏 + π‘˜  ξ‚€ 𝜏 + π‘˜ = πœ• 𝑛 πœ• 𝑒 𝑛 ξ‚΅ 𝑒 𝑛 + 𝜏 ( 1 βˆ’ 𝑒 ) 𝑛 ξ‚Ά 𝑛 ! , ( 𝑛 , 𝜏 ∈ β„• βˆͺ { 0 } ) , ( 5 . 7 ) in which we put 𝑛 = 𝑑 π‘š and 𝜏 = ( 𝑑 βˆ’ 1 ) π‘š βˆ’ 1 . This gives the identity stated in the lemma.

The following result deals with the case 𝑗 = 1 , in which we express the finite sum by a double integral on a rational function.

Corollary. For every positive integer π‘š one has 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) ( 𝑑 π‘š + π‘˜ ) 2 = ( βˆ’ 1 ) ( 𝑑 βˆ’ 1 ) π‘š ξ€œ 1 0 ξ€œ 1 0 ( 1 βˆ’ 𝑒 ) 𝑑 π‘š ( 1 βˆ’ 𝑀 ) π‘š 𝑒 ( 2 𝑑 βˆ’ 1 ) π‘š βˆ’ 1 𝑀 ( 𝑑 βˆ’ 1 ) π‘š βˆ’ 1 ( 1 βˆ’ ( 1 βˆ’ 𝑒 ) 𝑀 ) 𝑑 π‘š + 1 𝑑 𝑒 𝑑 𝑀 . ( 5 . 8 )

Proof. Set 𝑗 = 1 in Lemma 5.1, and note that ξ€œ l o g 𝑒 = βˆ’ ( 1 βˆ’ 𝑒 ) 1 0 𝑑 𝑀 . 1 βˆ’ ( 1 βˆ’ 𝑒 ) 𝑀 ( 5 . 9 ) Hence, 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) ( 𝑑 π‘š + π‘˜ ) 2 = βˆ’ ( βˆ’ 1 ) 𝑑 π‘š ξ€œ ( 𝑑 π‘š ) ! 1 0 𝑒 π‘š πœ• l o g 𝑒 𝑑 π‘š πœ• 𝑒 𝑑 π‘š ξ€· 𝑒 ( 2 𝑑 βˆ’ 1 ) π‘š βˆ’ 1 ( 1 βˆ’ 𝑒 ) 𝑑 π‘š ξ€Έ = 𝑑 𝑒 ( βˆ’ 1 ) 𝑑 π‘š ξ€œ ( 𝑑 π‘š ) ! 1 0 ξ€œ 1 0 ( 1 βˆ’ 𝑒 ) 𝑒 π‘š πœ• 1 βˆ’ ( 1 βˆ’ 𝑒 ) 𝑀 𝑑 π‘š πœ• 𝑒 𝑑 π‘š ξ€· 𝑒 ( 2 𝑑 βˆ’ 1 ) π‘š βˆ’ 1 ( 1 βˆ’ 𝑒 ) 𝑑 π‘š ξ€Έ 𝑑 𝑒 𝑑 𝑀 . ( 5 . 1 0 ) Let 𝑠 be any positive integer. Then we have the following decomposition of a rational function, in which 𝑒 is considered as variable and 𝑀 as parameter: 𝑒 𝑠 = 1 βˆ’ ( 1 βˆ’ 𝑒 ) 𝑀 𝑠 βˆ’ 1  𝜈 = 0 ( 𝑀 βˆ’ 1 ) 𝜈 𝑀 𝜈 + 1 𝑒 𝑠 βˆ’ 𝜈 βˆ’ 1 + ξ‚€ 𝑀 βˆ’ 1 𝑀  𝑠 1 . 1 βˆ’ ( 1 βˆ’ 𝑒 ) 𝑀 ( 5 . 1 1 ) We additionally assume that 𝑠 βˆ’ 1 < 𝑑 π‘š . Then, differentiating this identity 𝑑 π‘š -times with respect to 𝑒 , the polynomial in 𝑒 on the right-hand side vanishes identically: πœ• 𝑑 π‘š πœ• 𝑒 𝑑 π‘š ξ‚΅ 𝑒 𝑠 ξ‚Ά = ξ‚€ 1 βˆ’ ( 1 βˆ’ 𝑒 ) 𝑀 𝑀 βˆ’ 1 𝑀  𝑠 ( βˆ’ 1 ) 𝑑 π‘š ( 𝑑 π‘š ) ! 𝑀 𝑑 π‘š ( 1 βˆ’ ( 1 βˆ’ 𝑒 ) 𝑀 ) 𝑑 π‘š + 1 . ( 5 . 1 2 ) Therefore, we get from (5.10) by iterated integrations by parts: 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) ( 𝑑 π‘š + π‘˜ ) 2 = 1 ξ€œ ( 𝑑 π‘š ) ! 1 0 ξ€œ 1 0 𝑒 ( 2 𝑑 βˆ’ 1 ) π‘š βˆ’ 1 ( 1 βˆ’ 𝑒 ) 𝑑 π‘š πœ• 𝑑 π‘š πœ• 𝑒 𝑑 π‘š ξ‚΅ 𝑒 π‘š βˆ’ 𝑒 π‘š + 1 ξ‚Ά = 1 1 βˆ’ ( 1 βˆ’ 𝑒 ) 𝑀 𝑑 𝑒 𝑑 𝑀 ξ€œ ( 𝑑 π‘š ) ! 1 0 ξ€œ 1 0 𝑒 ( 2 𝑑 βˆ’ 1 ) π‘š βˆ’ 1 ( 1 βˆ’ 𝑒 ) 𝑑 π‘š ξ‚΅ ξ‚€ 𝑀 βˆ’ 1 𝑀  π‘š βˆ’ ξ‚€ 𝑀 βˆ’ 1 𝑀  π‘š + 1 ξ‚Ά Γ— ( βˆ’ 1 ) 𝑑 π‘š ( 𝑑 π‘š ) ! 𝑀 𝑑 π‘š 𝑑 𝑒 𝑑 𝑀 ( 1 βˆ’ ( 1 βˆ’ 𝑒 ) 𝑀 ) 𝑑 π‘š + 1 . ( 5 . 1 3 ) The corollary is proved by noting that ξ‚€ 𝑀 βˆ’ 1 𝑀  π‘š βˆ’ ξ‚€ 𝑀 βˆ’ 1 𝑀  π‘š + 1 = ( βˆ’ 1 ) π‘š ( 1 βˆ’ 𝑀 ) π‘š 𝑀 π‘š + 1 . ( 5 . 1 4 )

6. Estimating 𝐄 𝐦

In this section we estimate 𝐸 π‘š defined in (5.3). Substituting 1 βˆ’ 𝑒 for 𝑒 into the integral in Lemma 5.1 and applying iterated integration by parts, we get 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) ( 𝑑 π‘š + π‘˜ ) 2 𝑗 = βˆ’ ( βˆ’ 1 ) 𝑑 π‘š ξ€œ ( 𝑑 π‘š ) ! ( 2 𝑗 βˆ’ 1 ) ! 1 0 πœ• 𝑑 π‘š πœ• 𝑒 𝑑 π‘š ξ€· ( 1 βˆ’ 𝑒 ) π‘š ( l o g ( 1 βˆ’ 𝑒 ) ) 2 𝑗 βˆ’ 1 ξ€Έ ξ€· ( 1 βˆ’ 𝑒 ) ( 2 𝑑 βˆ’ 1 ) π‘š βˆ’ 1 𝑒 𝑑 π‘š ξ€Έ 𝑑 𝑒 . ( 6 . 1 ) Set 𝑓 ( 𝑒 ) ∢ = ( 1 βˆ’ 𝑒 ) π‘š ( l o g ( 1 βˆ’ 𝑒 ) ) 2 𝑗 βˆ’ 1 , ( 6 . 2 ) where π‘š and 𝑗 are kept fixed. We have 𝑓 ( 0 ) = 0 . For an integer π‘˜ > 0 we use Cauchy's formula 𝑓 ( π‘˜ ) ( π‘Ž ) = π‘˜ ! ξ€œ 2 πœ‹ 𝑖 𝐢 𝑓 ( 𝑧 ) ( 𝑧 βˆ’ π‘Ž ) π‘˜ + 1 𝑑 𝑧 ( 6 . 3 ) to estimate | 𝑓 ( π‘˜ ) ( 0 ) | . Let 𝐢 denote the circle in the complex plane centered around 0 with radius 𝑅 ∢ = 1 βˆ’ 1 / 2 π‘˜ . With π‘Ž = 0 and 𝑓 ( 𝑧 ) defined above, Cauchy's formula yields the identity 𝑓 ( π‘˜ ) ( 0 ) = π‘˜ ! 2 πœ‹ 𝑅 π‘˜ ξ€œ πœ‹ βˆ’ πœ‹ 𝑒 βˆ’ 𝑖 π‘˜ πœ™ ξ€· 1 βˆ’ 𝑅 𝑒 𝑖 πœ™ ξ€Έ π‘š l o g 2 𝑗 βˆ’ 1 ξ€· 1 βˆ’ 𝑅 𝑒 𝑖 πœ™ ξ€Έ 𝑑 πœ™ . ( 6 . 4 ) For the complex l o g arithm function occurring in (6.4) we cut the complex plane along the negative real axis and exclude the origin by a small circle. All arguments πœ™ of a complex number 𝑧 βˆ‰ ( βˆ’ ∞ , 0 ] are taken from the interval ( βˆ’ πœ‹ , πœ‹ ) . Therefore, using 1 βˆ’ 𝑅 𝑒 𝑖 πœ™ = 1 βˆ’ 𝑅 c o s πœ™ βˆ’ 𝑖 𝑅 s i n πœ™ , we get | | 1 βˆ’ 𝑅 𝑒 𝑖 πœ™ | | =  1 + 𝑅 2 √ βˆ’ 2 𝑅 c o s πœ™ = ∢ ξ€· 𝐴 ( 𝑅 , πœ™ ) , a r g 1 βˆ’ 𝑅 𝑒 𝑖 πœ™ ξ€Έ ξ‚΅ = βˆ’ a r c t a n 𝑅 s i n πœ™ ξ‚Ά . 1 βˆ’ 𝑅 c o s πœ™ ( 6 . 5 ) Hence, ξ€· l o g 1 βˆ’ 𝑅 𝑒 𝑖 πœ™ ξ€Έ  = l n 1 + 𝑅 2 ξ‚΅ βˆ’ 2 𝑅 c o s πœ™ βˆ’ 𝑖 a r c t a n 𝑅 s i n πœ™ ξ‚Ά = 1 1 βˆ’ 𝑅 c o s πœ™ 2 l n ξ‚΅ ( 𝐴 ( 𝑅 , πœ™ ) ) βˆ’ 𝑖 a r c t a n 𝑅 s i n πœ™ ξ‚Ά . 1 βˆ’ 𝑅 c o s πœ™ ( 6 . 6 ) Thus, it follows from (6.4) that

| | 𝑓 ( π‘˜ ) | | ≀ ( 0 ) π‘˜ ! 2 πœ‹ 𝑅 π‘˜ ξ€œ πœ‹ βˆ’ πœ‹ | | 1 βˆ’ 𝑅 𝑒 𝑖 πœ™ | | π‘š β‹… | | l o g ξ€· 1 βˆ’ 𝑅 𝑒 𝑖 πœ™ ξ€Έ | | 2 𝑗 βˆ’ 1 = 𝑑 πœ™ π‘˜ ! 2 πœ‹ 𝑅 π‘˜ ξ€œ πœ‹ βˆ’ πœ‹ ( 𝐴 ( 𝑅 , πœ™ ) ) π‘š / 2 ξ‚΅ 1 4 l n 2 ( 𝐴 ( 𝑅 , πœ™ ) ) + a r c t a n 2 ξ‚΅ 𝑅 s i n πœ™ 1 βˆ’ 𝑅 c o s πœ™ ξ‚Ά ξ‚Ά ( 2 𝑗 βˆ’ 1 ) / 2 = 𝑑 πœ™ π‘˜ ! πœ‹ 𝑅 π‘˜ ξ€œ πœ‹ 0 ( 𝐴 ( 𝑅 , πœ™ ) ) π‘š / 2 ξ‚΅ 1 4 l n 2 ( 𝐴 ( 𝑅 , πœ™ ) ) + a r c t a n 2 ξ‚΅ 𝑅 s i n πœ™ 1 βˆ’ 𝑅 c o s πœ™ ξ‚Ά ξ‚Ά ( 2 𝑗 βˆ’ 1 ) / 2 𝑑 πœ™ . ( 6 . 7 ) From 0 < 𝑅 < 1 we conclude on 0 < ( 1 βˆ’ 𝑅 ) 2 = 1 + 𝑅 2 βˆ’ 2 𝑅 ≀ 1 + 𝑅 2 βˆ’ 2 𝑅 c o s πœ™ = 𝐴 ( 𝑅 , πœ™ ) < 4 , ( 0 ≀ πœ™ ≀ πœ‹ ) , 0 ≀ 𝑅 s i n πœ™ ≀ 1 βˆ’ 𝑅 c o s πœ™ s i n πœ™ , 1 βˆ’ c o s πœ™ ( 0 < πœ™ ≀ πœ‹ ) . ( 6 . 8 ) Since a r c t a n is a strictly increasing function, we get ξ‚΅ a r c t a n 𝑅 s i n πœ™ ξ‚Ά ξ‚΅ 1 βˆ’ 𝑅 c o s πœ™ ≀ a r c t a n s i n πœ™ ξ‚Ά = 1 βˆ’ c o s πœ™ a r c t a n c o t ξ‚΅ πœ™ 2 ξ‚Ά ξ‚΅ ξ‚΅ = a r c t a n t a n πœ‹ βˆ’ πœ™ 2 = ξ‚Ά ξ‚Ά πœ‹ βˆ’ πœ™ 2 , ( 0 < πœ™ ≀ πœ‹ ) . ( 6 . 9 ) For 0 < 𝑅 < 1 , this upper bound also holds for πœ™ = 0 . Finally, we note that 𝑅 π‘˜ = ( 1 βˆ’ 1 / 2 π‘˜ ) π‘˜ β‰₯ 1 / 2 . Altogether, we conclude from (6.7) on | | 𝑓 ( π‘˜ ) | | ≀ ( 0 ) π‘˜ ! πœ‹ 𝑅 π‘˜ ξ€œ πœ‹ 0 4 π‘š / 2 ξ‚΅ l n 2 4 4 + a r c t a n 2 ξ‚΅ s i n πœ™ 1 βˆ’ c o s πœ™ ξ‚Ά ξ‚Ά ( 2 𝑗 βˆ’ 1 ) / 2 ≀ 2 𝑑 πœ™ π‘š + 1 π‘˜ ! πœ‹ ξ€œ πœ‹ 0  l n 2 ξ‚΅ 2 + πœ‹ βˆ’ πœ™ 2 ξ‚Ά 2 ξƒͺ ( 2 𝑗 βˆ’ 1 ) / 2 ≀ 2 𝑑 πœ™ π‘š + 1 π‘˜ ! πœ‹ ξ€œ πœ‹ 0 ξ‚΅ l n 2 πœ‹ 2 + 2 4 ξ‚Ά 𝑗 βˆ’ 1 / 2 ≀ 2 𝑑 πœ™ π‘š + 1 π‘˜ ! πœ‹ ξ€œ πœ‹ 0 3 𝑗 βˆ’ 1 / 2 𝑑 πœ™ ≀ 2 π‘š + 1 3 𝑗 π‘˜ ! . ( 6 . 1 0 ) It follows that the Taylor series expansion of 𝑓 ( 𝑒 ) , 𝑓 ( 𝑒 ) = ∞  π‘˜ = 0 𝑓 ( π‘˜ ) ( 0 ) 𝑒 π‘˜ ! π‘˜ , ( 6 . 1 1 ) converges at least for βˆ’ 1 < 𝑒 < 1 . Then, 𝑓 ( 𝑑 π‘š ) ( 𝑒 ) = ∞  π‘˜ = 𝑑 π‘š 𝑓 ( π‘˜ ) ( 0 ) 𝑒 ( π‘˜ βˆ’ 𝑑 π‘š ) ! π‘˜ βˆ’ 𝑑 π‘š = ∞  π‘˜ = 0 𝑓 ( π‘˜ + 𝑑 π‘š ) ( 0 ) 𝑒 π‘˜ ! π‘˜ , ( 6 . 1 2 ) and the estimate given by (6.10) implies for 0 < 𝑒 < 1 that | | 𝑓 ( 𝑑 π‘š ) ( | | ≀ 𝑒 ) ∞  π‘˜ = 0 | | 𝑓 ( π‘˜ + 𝑑 π‘š ) ( | | 0 ) 𝑒 π‘˜ ! π‘˜ ≀ 2 π‘š + 1 3 𝑗 ∞  π‘˜ = 0 ( π‘˜ + 𝑑 π‘š ) ! 𝑒 π‘˜ ! π‘˜ = 2 π‘š + 1 3 𝑗 ( 𝑑 π‘š ) ! ∞  π‘˜ = 0 ξ‚€ π‘˜  𝑒 π‘˜ + 𝑑 π‘š π‘˜ = 2 π‘š + 1 3 𝑗 ( 𝑑 π‘š ) ! ( 1 βˆ’ 𝑒 ) 𝑑 π‘š + 1 . ( 6 . 1 3 ) Combining (6.13) with the result from (6.1), we get for π‘š > 1 | | | | | 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) ( 𝑑 π‘š + π‘˜ ) 2 𝑗 | | | | | ≀ 2 π‘š + 1 3 𝑗 ξ€œ ( 2 𝑗 βˆ’ 1 ) ! 1 0 ( 1 βˆ’ 𝑒 ) ( 𝑑 βˆ’ 1 ) π‘š βˆ’ 2 𝑒 𝑑 π‘š = 2 𝑑 𝑒 π‘š + 1 3 𝑗 ( 2 𝑗 βˆ’ 1 ) ! Ξ“ ( 𝑑 π‘š + 1 ) Ξ“ ( ( 𝑑 βˆ’ 1 ) π‘š βˆ’ 1 ) = Ξ“ ( ( 2 𝑑 βˆ’ 1 ) π‘š ) 2 𝑑 βˆ’ 1 β‹… 2 𝑑 βˆ’ 1 π‘š + 1 3 𝑗 β‹… 1 ( 2 𝑗 βˆ’ 1 ) ! ( ( 𝑑 βˆ’ 1 ) π‘š βˆ’ 1 ) ξ€· ( 2 𝑑 βˆ’ 1 ) π‘š 𝑑 π‘š ξ€Έ . ( 6 . 1 4 )

We estimate the binomial coefficient by Stirling's formula (3.12). For this purpose we additionally assume that π‘š β‰₯ 2 𝑑 βˆ’ 1 : ξ‚€  β‰₯ ξƒŽ ( 2 𝑑 βˆ’ 1 ) π‘š 𝑑 π‘š ( 2 𝑑 βˆ’ 1 ) π‘š ξ‚΅ 2 πœ‹ ( 𝑑 π‘š + 1 ) ( ( 𝑑 βˆ’ 1 ) π‘š + 1 ) ( 2 𝑑 βˆ’ 1 ) 2 𝑑 βˆ’ 1 𝑑 𝑑 ( 𝑑 βˆ’ 1 ) 𝑑 βˆ’ 1 ξ‚Ά π‘š β‰₯ ξ‚™ 2 𝑑 βˆ’ 1 2 πœ‹ 𝑑 2 π‘š ξ‚΅ ( 2 𝑑 βˆ’ 1 ) 2 𝑑 βˆ’ 1 𝑑 𝑑 ( 𝑑 βˆ’ 1 ) 𝑑 βˆ’ 1 ξ‚Ά π‘š . ( 6 . 1 5 ) We now assume π‘š β‰₯ 2 𝑑 βˆ’ 1 and substitute the above inequality into (6.14): | | | | | 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) ( 𝑑 π‘š + π‘˜ ) 2 𝑗 | | | | | ≀ 𝑑 ( 2 𝑑 βˆ’ 1 ) 2 π‘š + 1 3 𝑗 √ 2 πœ‹ π‘š √ ( 2 𝑗 βˆ’ 1 ) ! ( 𝑑 βˆ’ 1 ) ( ( 𝑑 βˆ’ 1 ) π‘š βˆ’ 1 ) ξ‚΅ 𝑑 2 𝑑 βˆ’ 1 𝑑 ( 𝑑 βˆ’ 1 ) 𝑑 βˆ’ 1 ( 2 𝑑 βˆ’ 1 ) 2 𝑑 βˆ’ 1 ξ‚Ά π‘š . ( 6 . 1 6 ) For all integers π‘š β‰₯ 1 and 𝑑 β‰₯ 1 we have √ ( 2 𝑑 βˆ’ 1 ) 2 πœ‹ π‘š √ √ 2 𝑑 βˆ’ 1 < 2 πœ‹ 𝑑 π‘š , ( 𝑑 βˆ’ 1 ) ( ( 𝑑 βˆ’ 1 ) π‘š βˆ’ 1 ) β‰₯ ( 𝑑 βˆ’ 1 ) ( 𝑑 βˆ’ 2 ) π‘š . ( 6 . 1 7 ) Thus we have proven the following result.

Lemma 6.1. For all integers 𝑑 , π‘š with 𝑑 β‰₯ 3 and π‘š β‰₯ 2 𝑑 βˆ’ 1 one has | | | | | 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) ( 𝑑 π‘š + π‘˜ ) 2 𝑗 | | | | | < 2 π‘š + 2 3 𝑗 √ πœ‹ 𝑑 3 √ ( 2 𝑗 βˆ’ 1 ) ! ( 𝑑 βˆ’ 1 ) ( 𝑑 βˆ’ 2 ) π‘š ξ‚΅ 𝑑 𝑑 ( 𝑑 βˆ’ 1 ) 𝑑 βˆ’ 1 ( 2 𝑑 βˆ’ 1 ) 2 𝑑 βˆ’ 1 ξ‚Ά π‘š . ( 6 . 1 8 )

Next, we need an upper bound for the Bernoulli numbers 𝐡 2 𝑗 (cf. [9, 23.1.15] ): | | 𝐡 2 𝑗 | | ≀ 2 ( 2 𝑗 ) ! ( 2 πœ‹ ) 2 𝑗 ξ€· 1 βˆ’ 2 1 βˆ’ 2 𝑗 ξ€Έ ≀ 4 ( 2 𝑗 ) ! ( 2 πœ‹ ) 2 𝑗 , ( 𝑗 β‰₯ 1 ) . ( 6 . 1 9 ) Let 𝑑 β‰₯ 3 and π‘š β‰₯ m a x { 2 𝑑 βˆ’ 1 , π‘Ž / 2 } . Using this and Lemma 6.1, we estimate 𝐸 π‘š in (5.3): | | 𝐸 π‘š | | < 3 2 √ πœ‹ 𝑑 3 2 π‘š + 2 √ ( 𝑑 βˆ’ 1 ) ( 𝑑 βˆ’ 2 ) π‘š ξ‚΅ 𝑑 𝑑 ( 𝑑 βˆ’ 1 ) 𝑑 βˆ’ 1 ( 2 𝑑 βˆ’ 1 ) 2 𝑑 βˆ’ 1 ξ‚Ά π‘š + √ πœ‹ 𝑑 3 2 π‘š + 2 √ ( 𝑑 βˆ’ 1 ) ( 𝑑 βˆ’ 2 ) π‘š ξ‚΅ 𝑑 𝑑 ( 𝑑 βˆ’ 1 ) 𝑑 βˆ’ 1 ( 2 𝑑 βˆ’ 1 ) 2 𝑑 βˆ’ 1 ξ‚Ά π‘š Γ— 𝑑 π‘š  𝑗 = 1 𝐡 2 𝑗 ξ‚΅ | | | 1 2 𝑗 π‘Ž 2 𝑗 βˆ’ 1 𝑏 2 𝑗 | | | 3 + 1 𝑗 + 3 ( 2 𝑗 βˆ’ 1 ) ! 2 𝑗 ξ‚Ά ≀ √ ( 4 𝑗 βˆ’ 1 ) ! πœ‹ 𝑑 3 2 π‘š + 2 √ ( 𝑑 βˆ’ 1 ) ( 𝑑 βˆ’ 2 ) π‘š ξ‚΅ 𝑑 𝑑 ( 𝑑 βˆ’ 1 ) 𝑑 βˆ’ 1 ( 2 𝑑 βˆ’ 1 ) 2 𝑑 βˆ’ 1 ξ‚Ά π‘š Γ—  3 2 + 𝑑 π‘š  𝑗 = 1 4 ( 2 𝑗 βˆ’ 1 ) ! ( 2 πœ‹ ) 2 𝑗 ξ‚΅ 2 β‹… 3 𝑗 ( + 3 2 𝑗 βˆ’ 1 ) ! 2 𝑗 ( ξ‚Ά ξƒͺ < 4 √ 4 𝑗 βˆ’ 1 ) ! πœ‹ 𝑑 3 √ ( 𝑑 βˆ’ 1 ) ( 𝑑 βˆ’ 2 ) π‘š ξ‚΅ 2 𝑑 𝑑 ( 𝑑 βˆ’ 1 ) 𝑑 βˆ’ 1 ( 2 𝑑 βˆ’ 1 ) 2 𝑑 βˆ’ 1 ξ‚Ά π‘š βŽ› ⎜ ⎜ ⎝ 3 2 + 8 ∞  𝑗 = 1 βŽ› ⎜ ⎜ ⎝  √ 3 ξƒͺ 2 πœ‹ 2 𝑗 + ξ‚€ 3  2 πœ‹ 2 𝑗 ⎞ ⎟ ⎟ ⎠ ⎞ ⎟ ⎟ ⎠ < √ 1 9 πœ‹ 𝑑 3 √ ( 𝑑 βˆ’ 1 ) ( 𝑑 βˆ’ 2 ) π‘š ξ‚΅ 2 𝑑 𝑑 ( 𝑑 βˆ’ 1 ) 𝑑 βˆ’ 1 ( 2 𝑑 βˆ’ 1 ) 2 𝑑 βˆ’ 1 ξ‚Ά π‘š . ( 6 . 2 0 ) Now, let 𝑇 𝑛 ∢ = π‘Ž 𝑛 βˆ’ 1  𝑗 = 1 1 𝑗 βˆ’ 𝑏 𝑛 βˆ’ 1  𝑗 = 1 1 𝑗 + 2 𝑛 βˆ’ 1  𝑗 = 1 1 𝑗 βˆ’ 𝑛 2 βˆ’ 1  𝑗 = 1 1 𝑗 = 𝑛 2 βˆ’ 1  𝑗 = 1 𝑒 𝑗 𝑗 , ( 𝑛 > 1 ) , ( 6 . 2 1 ) with the numbers 𝑒 𝑗 introduced in the proof of Theorem 4.1. By definition of 𝑅 𝑛 and 𝑆 𝑛 we then have 𝑇 𝑛 = 𝑆 𝑛 βˆ’ 𝑅 𝑛 , and therefore we can estimate the series transformation of 𝑇 𝑛 by applying the results from Theorem 2.4 and (6.20). Again, let π‘š β‰₯ m a x { 2 𝑑 βˆ’ 1 , π‘Ž / 2 } and 𝑑 β‰₯ 4 2 . | | | | | 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ ξ‚€ ( π‘˜  𝑇 2 𝑑 βˆ’ 1 ) π‘š + π‘˜ βˆ’ 1 𝑑 π‘š  ξ‚€ 𝑑 π‘š π‘˜ + 𝑑 π‘š βˆ’ 𝛾 βˆ’ l o g π‘Ž 𝑏 | | | | | ≀ | | | | | 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) 𝑆 π‘˜ + 𝑑 π‘š βˆ’ 𝛾 βˆ’ l o g π‘Ž 𝑏 | | | | | + | | | | | 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) 𝑅 π‘˜ + 𝑑 π‘š | | | | | = | | | | | 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) 𝑆 π‘˜ + 𝑑 π‘š βˆ’ 𝛾 βˆ’ l o g π‘Ž 𝑏 | | | | | + | | 𝐸 π‘š | | < 𝑐 4 β‹… ξ‚΅ ( 1 βˆ’ 1 / 𝑑 ) 𝑑 ( 𝑑 βˆ’ 1 ) 4 𝑑 ξ‚Ά π‘š + √ 1 9 πœ‹ 𝑑 3 √ ( 𝑑 βˆ’ 1 ) ( 𝑑 βˆ’ 2 ) π‘š ξ‚΅ 2 𝑑 𝑑 ( 𝑑 βˆ’ 1 ) 𝑑 βˆ’ 1 ( 2 𝑑 βˆ’ 1 ) 2 𝑑 βˆ’ 1 ξ‚Ά π‘š . ( 6 . 2 2 ) By similar arguments we get the same bound when 𝑏 > π‘Ž . For 𝑑 β‰₯ 3 it can easily be seen that 2 𝑑 𝑑 ( 𝑑 βˆ’ 1 ) 𝑑 βˆ’ 1 ( 2 𝑑 βˆ’ 1 ) 2 𝑑 βˆ’ 1 = 2 ( 2 𝑑 βˆ’ 1 ) β‹… 𝑑 βˆ’ 1 ( 1 βˆ’ 1 / 𝑑 ) 𝑑 ( 1 βˆ’ 1 / 2 𝑑 ) 2 𝑑 β‹… 1 4 𝑑 < 1 8 4 𝑑 + 1 . ( 6 . 2 3 ) Thus, we finally have proven the following theorem.

Theorem 6.2. Let 𝑇 𝑛 ∢ = π‘Ž 𝑛 βˆ’ 1  𝑗 = 1 1 𝑗 βˆ’ 𝑏 𝑛 βˆ’ 1  𝑗 = 1 1 𝑗 + 2 𝑛 βˆ’ 1  𝑗 = 1 1 𝑗 βˆ’ 𝑛 2 βˆ’ 1  𝑗 = 1 1 𝑗 , ( 𝑛 > 1 ) , ( 6 . 2 4 ) where π‘Ž , 𝑏 are positive integers. Let 𝑑 β‰₯ 4 2 be an integer. Then, there is a positive constant 𝑐 5 depending at most on π‘Ž , 𝑏 and 𝑑 such that | | | | | 𝑑 π‘š  π‘˜ = 0 ( βˆ’ 1 ) π‘˜ ξ‚€ ( π‘˜  𝑇 2 𝑑 βˆ’ 1 ) π‘š + π‘˜ βˆ’ 1 𝑑 π‘š  ξ‚€ 𝑑 π‘š π‘˜ + 𝑑 π‘š π‘Ž βˆ’ 𝛾 βˆ’ l o g 𝑏 | | | | | < 𝑐 5 √ π‘š ξ‚΅ 1 8 4 𝑑 + 1 ξ‚Ά π‘š , ( π‘š β‰₯ 1 ) . ( 6 . 2 5 )

7. Concluding Remarks

It seems that in Theorem 6.2 a smaller bound holds.

Conjecture. Let a , b be positive integers. Let 𝑑 β‰₯ 2 be an integer. Then there is a positive constant 𝑐 6 depending at most on π‘Ž , 𝑏 and 𝑑 such that for all integers π‘š β‰₯ 1 one has | | | | | 𝑑 π‘š  π‘˜ = 0 0 π‘₯ 0 2 0 0 𝑑 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ ξ‚€ ( π‘˜  𝑇 2 𝑑 βˆ’ 1 ) π‘š + π‘˜ βˆ’ 1 𝑑 π‘š  ξ‚€ 𝑑 π‘š π‘˜ + 𝑑 π‘š βˆ’ 𝛾 βˆ’ l o g π‘Ž 𝑏 | | | | | < 𝑐 6 β‹… ξ‚΅ ( 1 βˆ’ 1 / 𝑑 ) 𝑑 ( 𝑑 βˆ’ 1 ) 4 𝑑 ξ‚Ά π‘š . ( 7 . 1 )

A proof of this conjecture would be implied by suitable bounds for the integral stated in Lemma 5.1. For 𝑗 = 1 such a bound follows from the double integral given in Corollary 5.2: | | | | | 𝑑 π‘š  π‘˜ = 0 0 π‘₯ 0 2 0 0 𝑑 ( βˆ’ 1 ) 𝑑 π‘š + π‘˜ 𝑔 ( π‘˜ ) ( 𝑑 π‘š + π‘˜ ) 2 | | | | | = ξ€œ 1 0 ξ€œ 1 0 ( 1 βˆ’ 𝑒 ) 𝑑 π‘š ( 1 βˆ’ 𝑀 ) π‘š 𝑒 ( 2 𝑑 βˆ’ 1 ) π‘š βˆ’ 1 𝑀 ( 𝑑 βˆ’ 1 ) π‘š βˆ’ 1 ( 1 βˆ’ ( 1 βˆ’ 𝑒 ) 𝑀 ) 𝑑 π‘š + 1 = ξ€œ 𝑑 𝑒 𝑑 𝑀 1 0 ξ€œ 1 0 ( 1 βˆ’ 𝑒 ) 2 ( 1 βˆ’ 𝑀 ) 𝑒 2 1 βˆ’ ( 1 βˆ’ 𝑒 ) 𝑀 3 ξ‚΅ ( 1 βˆ’ 𝑒 ) 𝑒 2 𝑀 ξ‚Ά 1 βˆ’ ( 1 βˆ’ 𝑒 ) 𝑀 𝑑 βˆ’ 2 Γ— ξ‚΅ ( 1 βˆ’ 𝑒 ) 𝑑 ( 1 βˆ’ 𝑀 ) 𝑒 2 𝑑 βˆ’ 1 𝑀 𝑑 βˆ’ 1 ( 1 βˆ’ ( 1 βˆ’ 𝑒 ) 𝑀 ) 𝑑 ξ‚Ά π‘š βˆ’ 1 ≀ 1 𝑑 𝑒 𝑑 𝑀 4 𝑑 βˆ’ 2 ξ‚΅ ( 1 βˆ’ 1 / 𝑑 ) 𝑑 ( 𝑑 βˆ’ 1 ) 4 𝑑 ξ‚Ά π‘š βˆ’ 1 ξ€œ 1 0 ξ€œ 1 0 ( 1 βˆ’ 𝑒 ) 2 ( 1 βˆ’ 𝑀 ) 𝑒 2 1 βˆ’ ( 1 βˆ’ 𝑒 ) 𝑀 3 = 𝑑 𝑒 𝑑 𝑀 2 ( 𝑑 βˆ’ 1 ) 3 ( 1 βˆ’ 1 / 𝑑 ) 𝑑 β‹… ξ‚΅ ( 1 βˆ’ 1 / 𝑑 ) 𝑑 ( 𝑑 βˆ’ 1 ) 4 𝑑 ξ‚Ά π‘š , ( π‘š β‰₯ 1 ) , ( 7 . 2 ) where the double integral in the last but one line equals to 1 / 2 4 .

Note that the rational functions ( 1 βˆ’ 𝑒 ) 𝑒 2 𝑀 , 1 βˆ’ ( 1 βˆ’ 𝑒 ) 𝑀 ( 1 βˆ’ 𝑒 ) 𝑑 ( 1 βˆ’ 𝑀 ) 𝑒 2 𝑑 βˆ’ 1 𝑀 𝑑 βˆ’ 1 ( 1 βˆ’ ( 1 βˆ’ 𝑒 ) 𝑀 ) 𝑑 , ( 7 . 3 ) take their maximum values 4 2 βˆ’ 𝑑 and ( 1 βˆ’ 1 / 𝑑 ) 𝑑 / ( ( 𝑑 βˆ’ 1 ) 4 𝑑 ) inside the unit square [ 0 , 1 ] Γ— [ 0 , 1 ] at ( 𝑒 , 𝑀 ) = ( 1 / 2 , 1 ) and ( 𝑒 , 𝑀 ) = ( 1 / 2 , ( 2 𝑑 βˆ’ 2 ) / ( 2 𝑑 βˆ’ 1 ) ) , respectively. Finally, we compare the bound for the series transformation given by Theorem 2.4 with the bound proven for Theorem 6.2. In Theorem 2.4 the bound is 𝑇 1 ( 𝑑 , π‘š ) ∢ = 𝑐 4 β‹… ξ‚΅ ( 1 βˆ’ 1 / 𝑑 ) 𝑑 ( 𝑑 βˆ’ 1 ) 4 𝑑 ξ‚Ά π‘š , ( 𝑑 β‰₯ 4 2 , π‘š β‰₯ 1 ) , ( 7 . 4 ) whereas we have in Theorem 6.2 that 𝑇 2 𝑐 ( 𝑑 , π‘š ) ∢ = 5 √ π‘š ξ‚΅ 1 8 4 𝑑 + 1 ξ‚Ά π‘š , ( 𝑑 β‰₯ 4 2 , π‘š β‰₯ 1 ) . ( 7 . 5 ) For fixed 𝑑 β‰₯ 4 2 and sufficiently large π‘š it is clear on the one hand that 𝑇 1 ( 𝑑 , π‘š ) < 𝑇 2 ( 𝑑 , π‘š ) , but on the other hand we have l i m π‘š β†’ ∞ l i m 𝑑 β†’ ∞ l o g 𝑇 1 ( 𝑑 , π‘š ) l o g 𝑇 2 ( 𝑑 , π‘š ) = 1 = l i m 𝑑 β†’ ∞ l i m π‘š β†’ ∞ l o g 𝑇 1 ( 𝑑 , π‘š ) l o g 𝑇 2 . ( 𝑑 , π‘š ) ( 7 . 6 ) Conversely, for 𝑑 tending to infinity, one gets βˆ’ l o g | | 𝑇 1 | | | | 𝑇 ( 𝑑 , π‘š ) ≫ 𝑑 π‘š l o g 4 , βˆ’ l o g 2 | | ( 𝑑 , π‘š ) ≫ 𝑑 π‘š l o g 4 , ( 7 . 7 ) with implicit constants depending at most on π‘š . For the denominators 𝑏 π‘š of the transformed series 𝑆 π‘˜ + 𝑑 π‘š in Theorem 2.4 we have the bound l o g 𝑏 π‘š β‰ͺ 𝑑 2 π‘š 2 from Theorem 4.1, and a similar inequality holds for the denominators of the transformed series 𝑇 π‘˜ + 𝑑 π‘š in Theorem 6.2.

References

  1. C. Elsner, β€œOn a sequence transformation with integral coefficients for Euler's constant,” Proceedings of the American Mathematical Society, vol. 123, no. 5, pp. 1537–1541, 1995. View at Publisher Β· View at Google Scholar Β· View at Zentralblatt MATH Β· View at MathSciNet
  2. T. Rivoal, β€œPolynômes de type Legendre et approximations de la constante d'Euler,” notes, 2005, http://www-fourier.ujf-grenoble.fr/~rivoal/articles/euler.pdf.
  3. K. H. Pilehrood and T. H. Pilehrood, β€œArithmetical properties of some series with logarithmic coefficients,” Mathematische Zeitschrift, vol. 255, no. 1, pp. 117–131, 2007. View at Publisher Β· View at Google Scholar Β· View at MathSciNet
  4. C. Elsner, β€œOn a sequence transformation with integral coefficients for Euler's constant. II,” Journal of Number Theory, vol. 124, no. 2, pp. 442–453, 2007. View at Publisher Β· View at Google Scholar Β· View at MathSciNet
  5. G. H. Hardy and E. M. Wright, An Introduction to the Theory of Numbers, Clarendon Press, Oxford, UK, 1984.
  6. A. I. Aptekarev, Ed., Rational Approximation of Euler's Constant and Recurrence Relations, A. I. Aptekarev, Ed., Sovremennye Problemy Matematiki, Vol. 9, MIAN (Steklov Institute), Moscow, Russia, 2007. View at Zentralblatt MATH
  7. T. Rivoal, β€œRational approximations for values of derivatives of the Gamma function,” http://www-fourier.ujf-grenoble.fr/~rivoal/articles/eulerconstant.pdf.
  8. D. E. Knuth, β€œEuler's constant to 1271 places,” Mathematics of Computation, vol. 16, no. 79, pp. 275–281, 1962. View at Publisher Β· View at Google Scholar Β· View at Zentralblatt MATH Β· View at MathSciNet
  9. M. Abramowitz and I. Stegun, Handbook of Mathematical Functions, Dover, New York, NY, USA, 1970.