Appendix A Elements of Classical Analysis
A.1 Exotic Constants
He who understands Archimedes and Apollonius will admire less the achievements of the foremost men of later times. Gottfried Wilhelm Leibniz (1646Ð1716)
The Euler–Mascheroni constant, γ, is the special constant defined by 1 1 γ = lim 1 + + ···+ − lnn = 0.57721 56649 01532 86060.... n→∞ 2 n
In other words γ measures the amount by which the partial sum of the harmonic series differs from the logarithmic term lnn. The connection between 1 + 1/2 + 1/3 + ···+ 1/n and lnn was first established in 1735 by Euler [41], who used the notation C for it and stated that was worthy of serious consideration. It is worth mentioning that it was the Italian geometer Lorenzo Mascheroni (1750Ð1800) who actually introduced the symbol γ for the constant (although there is controversy about this claim) and also computed, though with error, the first 32 digits [36]. Unsurprisingly, establishing the existence of γ has attracted many proofs [65, pp. 69Ð73], [133, p. 235] to mention a few. However, a short and elegant proof is based on showing that the sequence (1 + 1/2 + 1/3 + ···+ 1/n − lnn)n≥1 is strictly decreasing and bounded below by 0. The EulerÐMascheroni constant, γ, considered to be the third important mathe- matical constant next to π and e, has appeared in a variety of mathematical formulae involving series, products, and integrals [43, pp. 28Ð32], [65, p. 109], [122, pp. 4Ð6], [123, pp. 13Ð22]. For an interesting survey paper on γ, as well as other reference material, the reader is referred to [34]. We mention that it is still an open problem to determine whether γ is a rational or an irrational number.
O. Furdui, Limits, Series, and Fractional Part Integrals: Problems in Mathematical 253 Analysis, Problem Books in Mathematics, DOI 10.1007/978-1-4614-6762-5, © Springer Science+Business Media New York 2013 254 A Elements of Classical Analysis
The nth harmonic number, Hn, is defined for n ≥ 1by
1 1 H = 1 + + ···+ . n 2 n In other texts, it is also defined as the partial sum of the harmonic series ∞ 1 n 1 ∑ = lim ∑ = ∞. n→∞ k=1 k k=1 k
The nth harmonic number verifies the recurrence formula Hn = Hn−1 + 1/n for n ≥ 2 with H1 = 1 which can be used to establish the generating function ( − ) ∞ −ln 1 x = n, − ≤ < . − ∑ Hnx 1 x 1 1 x n=1
Significantly, one of the most important properties on the nth harmonic number refers to its divergence. The first proof of the divergence of the harmonic series is attributed, surprisingly, to Nicholas Oresme (1323Ð1382), one of the greatest philosophers of the Middle Ages, and similar proofs were discovered in later centuries by the Bernoulli brothers. Even Euler proved this result by evaluating an improper integral in two different ways [65, p. 23]. Another curious property is that Hn is nonintegral. This means that even though Hn increases without bound, it avoids all integers, apart from n = 1. The nth harmonic number has been involved in a variety of mathematical results: from summation formulae involving the binomial coefficients to a nice formula that expresses the nth harmonic number in terms of the unsigned Stirling numbers of the first kind [13]. A detailed history on the nth harmonic number as well as its connection to γ can be found in Havil’s book [65]. The Glaisher–Kinkelin constant, A, is defined by the limit
n 2 2 A = lim n−n /2−n/2−1/12en /4 ∏ kk = 1.28242 71291 00622 63687.... n→∞ k=1
Equivalently, n n2 n 1 n2 lnA = lim ∑ k lnk − + + lnn + . n→∞ k=1 2 2 12 4
Another remarkable formula, involving factorials, in which A appears is the following: 1 1! · 2!···(n − 1)! e 12 lim = . →∞ − 3 n2 1 n 1 n2− 1 n e 4 (2π) 2 n 2 12 A These formulae are due to Kinkelin [72], Jeffery [71], and Glaisher [59Ð61]. A.1 Exotic Constants 255 √ The constant A, which plays the same role as 2π plays in Stirling’s formula, has the following closed-form expression [43, p. 135]:
1 ζ (2) ln(2π)+γ A = exp − ζ (−1) = exp − + , 12 2π2 12 where ζ denotes the derivative of the Riemann zeta function and γ is the EulerÐ Mascheroni constant. Many beautiful formulae including A exist in the literature, from infinite products and definite integrals [43, pp. 135Ð136] to the evaluation of infinite series involving Riemann zeta function [122]. Other formulae involving infinite series and products, believed to be new in the literature, in which A appears, are recorded as problems in this book. The Stieltjes constants, γn, are the special constants defined by m (lnk)n (lnm)n+1 γn = lim ∑ − , m→∞ + k=1 k n 1 and, in particular, γ0 = γ, the EulerÐMascheroni constant. They occur in the Laurent expansion of the Riemann zeta function in a neighborhood of its simple pole at z = 1(see[98, Entry 25.2.4, p. 602]):
∞ (− )n ζ( )= 1 + 1 γ ( − )n, ℜ( ) > . s − ∑ n s 1 s 0 s 1 n=0 n!
Interesting properties related to the sign of the Stieltjes constants as well as an open problem involving their magnitudes are recorded in [43, pp. 166Ð167]. The logarithmic constants, δn, are defined by m m n n 1 n n (n) δn = lim ∑ ln k − ln xdx − ln m =(−1) (ζ (0)+n!). m→∞ k=1 1 2
In particular δ0 = 1/2, δ1 = 1/2ln(2π) − 1. Sitaramachandrarao [118] proved that they appear in the Laurent expansion of the Riemann zeta function at the origin rather than at unity
∞ (− )n ζ( )= 1 + 1 δ n. z − ∑ nz z 1 n=0 n!
We called these constants logarithmic for simplicity and because of the logarith- mic terms involved in their definition. The constants, which are also discussed in [43, p. 168], have been used in Problem 3.98 in order to evaluate a double logarithmic series. 256 A Elements of Classical Analysis
A.2 Special Functions
Euler’s integral appears everywhere and is inextricably bound to a host of special functions. Its frequency and simplicity make it fundamental. Philip J. Davis
Euler’s Gamma function, which extends factorials to the set of complex numbers, is a function of a complex variable defined by