Furthermore, Euler proved from the properties of the Bernoulli numbers, for given by the generating function
and the classical Euler, Bernoulli relation (see, [1], p. 166), that
The Riemann zeta function, , is defined as
and the Dirichlet eta function, , is defined by
where defines the real part of The harmonic numbers of integer order p are defined as
where and are the sets of complex numbers and positive integers, respectively.
The term represents the familiar Euler–Mascheroni constant (see, e.g., [1], Section 1.2), and denotes the digamma (or psi) function defined by
where is the familiar Gamma function (see, e.g., [1], Section 1.1). Following the notation of Flajolet and Salvy [2], we define classes of linear Euler harmonic sums of the type
for and with the integer designated as the weight. We define
In this paper, we shall obtain linear combinations of (1) in closed form in terms of special functions, such as
where the Dirichlet lambda function is defined as the term-wise arithmetic mean of the Dirichlet eta function and the Riemann zeta function:
For the case where , we recall the following known results
due to Euler [3]. For the alternating case, for odd weight , Sitaramachandrarao [4] published
and recently Alzer and Choi [5] obtained the following nice result, for
and
There are many interesting and significant results associated with Euler harmonic sum identities, some of which may be seen in the works of [6,7,8,9,10,11,12,13,14]. Linear Euler harmonic sums play an important role in the evaluation of integral equations in many areas of science research such as combinatorics and statistical plasma physics, especially in the context of the Sommerfeld temperature expansion of electronic entropy; see [15,16]. The majority of the published works dealing with Euler harmonic sums of the type (6) deal with the case where
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