Abstract
Two linear forms, \(\sigma _n \zeta (5)+\tau _n \zeta (3)+\varphi _n\) and \(\sigma _n\zeta (2)+\tau _n/2\), with suitable rational coefficients \(\sigma _n,\tau _n,\varphi _n\), are presented. As a byproduct, we obtain an identity between simple and double binomial sums, where the simple sum is the value of a terminating well-poised Saalschützian \({}_4 F_3\) series. This complements a recent note of the author on two linear forms: \(\alpha _n \widetilde{\zeta }(4)+\beta _n \widetilde{\zeta }(2)+\gamma _n\), based on an identity of Paule–Schneider, and \(\alpha _n\zeta (2)+\beta _n\), coming from the Apéry–Beukers construction.
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1 Main binomial and binomial-harmonic identities
Very well-poised hypergeometric series provide a clue in the study of diophantine properties of the values of the Riemann zeta function \(\zeta (s)\) at positive integers, see e.g. [4, 7, 8], to quote only a few papers dealing with this important topic. Further references can be found in the bibliography of [4].
In the recent paper [5], we observed that the linear forms
and
have two common coefficients, namely
Here and in the sequel, if \(m>0\) is an integer, and \((x)_0=1\). We denote by \(\zeta (s)\) and \(\widetilde{\zeta }(s)\) the following:
The equality \(A_n=\alpha _n\) was noted earlier by Paule and Schneider [6], and is a special case of [4, Proposition 1].
In the present paper we adapt the methods of [5] to the linear forms
and
It seems reasonable to expect that one can solve [9, Problem 1] by similar methods. We assume that the reader is familiar with the background contained in [4, Section 2]. In particular, we have
Throughout this paper,
and the notation for the derivative \(\mathrm{d}/\mathrm{d} j\) is taken from [4, (7.2)].
The main result of the present paper is the following:
Theorem 1.1
We have
Despite the analogy between the equalities \(\tau _n=2T_n\) in (6) and \(\beta _n=B_n\) in the paper [5] quoted above, we currently miss a unified proof. However, both (5) and (6), and similar observations in [5], are implicitely connected to the period structure of some multiple integrals (see [3, Section 9.5]). In particular, the linear forms \(\mathrm{\Lambda }_n\) (respectively, \(\mathrm{\Theta }_n\)) in Sect. 2, and even more general linear forms, are equal to suitable 3-fold (respectively, 5-fold) multiple integrals over (respectively, over ), and similar remarks hold for the linear forms in 1 and \(\zeta (2)\) and in \(1,\zeta (2)\) and \(\zeta (4)\) in [5]. All the integrals alluded to above are period integrals on moduli spaces (see [3, Section 1.3]).
In Sect. 2 we provide more details on the above linear forms and coefficients, and in Sects. 3–4 we prove Theorem 1.1.
By combining (5) with another special case of [4, Proposition 1], we have
Theorem 1.2
We give an independent proof of (7) in the last section of the present paper.
2 Linear forms in \(1,\zeta (2)\) and in \(1,\zeta (3)\) and \(\zeta (5)\)
The following series is a linear form in 1 and \(\zeta (2)\) with rational coefficients:
It is worth noticing that \(\mathrm{\Lambda }_n\) is a Saalschützian \({}_4 F_3\) well-poised hypergeometric series
Throughout the present paper we use identities between values of the function \({}_{q+1} F_q\) with the argument \(z=1\), which is customary omitted.
We have
whence \(S_n\) is the right-hand side of (3) and, similarly, \(T_n\) is given as the right-hand side of (4).
The next series is a linear form in \(1,\zeta (3)\) and \(\zeta (5)\) with rational coefficients:
where
By exchanging j with \(n-j\), i.e. by inverting the order of summation, we have
Therefore \(\sigma _n\) equals the left-hand side of (1), and similarly \(\tau _n\) is given by one of the two equivalent sums in (2).
3 Application of Whipple’s transformation
We apply the following transformation formula, due to Whipple (see [2, 4.3 (4)]):
The coefficient \(\sigma _n\) can be written as
By applying (8), we obtain
Since
we have
Therefore (5) is proved.
Let \(a,b,c,d,\alpha ,\beta ,\gamma ,\delta \) be eight complex parameters to be chosen later. We consider the following functions of \(\varepsilon \):
We have
and similar expressions for the second and third order derivatives of \(f_{n,j}(\varepsilon )\) at \(\varepsilon =0\). With the choice \(a=\beta =1+i\), \(b=\alpha =1-i\), \(c=d=\gamma =\delta =1\), where \(i=\sqrt{-1}\), we have
Therefore,
Application of (8) yields
Using (9) again,
Taking
and computing its first and second derivatives at \(z=0\), after a few simplifications we obtain
4 End of the proof of Theorem 1.1
In this section we denote by \(a,b,\alpha ,\beta \) four real parameters to be chosen later. Let \(h_n(\varepsilon ,\omega )\) be defined by
By applying (see [2, 7.2 (1)])
valid for \(u+v+w=x+y+z-n+1\), with
and
we have
Here we used \((\xi )_n = (-1)^n (1-n-\xi )_n\) with \(\xi =v-z\) and \(\xi =w-z\). By choosing \(a=-1\), \(b=-2\), \(\alpha =1\), \(\beta =-1\) and comparing the two expressions of
we find out that
By using
with \(k=0\) and \(k=n\), the above sum simplifies to
hence
Since
we have
and (6) is proved.
5 Application of Sheppard’s transformation
In this section we give a direct proof of (7). A similar argument was applied in [4, Section 7] to the double binomial sum in the middle of [4, (7.1)].
We start with the double sum in (7), and rewrite it in the form
Let us apply Sheppard’s transformation (see [1, Corollary 3.3.4] and [2, Section 3.9]):
We obtain
Hence the sum (10) is equal to
Exchanging the order of summation and using
the last double sum becomes
The inner sum \({}_2 F_1\) can be evaluated by the Chu–Vandermonde convolution formula (see e.g. [2, Section 1.3]):
Therefore (7) is established.
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Acknowledgements
The author is indebted to the referee for helpful comments and suggestions, and for pointing out to him the reference [3].
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Marcovecchio, R. On hypergeometric identities related to zeta values. European Journal of Mathematics 3, 43–52 (2017). https://doi.org/10.1007/s40879-016-0126-0
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DOI: https://doi.org/10.1007/s40879-016-0126-0