1,823 research outputs found

    Multiple harmonic sums and Wolstenholme's theorem

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    We give a family of congruences for the binomial coefficients (kpβˆ’1pβˆ’1){kp-1\choose p-1} in terms of multiple harmonic sums, a generalization of the harmonic numbers. Each congruence in this family (which depends on an additional parameter nn) involves a linear combination of nn multiple harmonic sums, and holds mod  p2n+3\mod{p^{2n+3}}. The coefficients in these congruences are integers depending on nn and kk, but independent of pp. More generally, we construct a family of congruences for (kpβˆ’1pβˆ’1)mod  p2n+3{kp-1\choose p-1} \mod{p^{2n+3}}, whose members contain a variable number of terms, and show that in this family there is a unique "optimized" congruence involving the fewest terms. The special case k=2k=2 and n=0n=0 recovers Wolstenholme's theorem (2pβˆ’1pβˆ’1)≑1mod  p3{2p-1\choose p-1}\equiv 1\mod{p^3}, valid for all primes pβ‰₯5p\geq 5. We also characterize those triples (n,k,p)(n, k, p) for which the optimized congruence holds modulo an extra power of pp: they are precisely those with either pp dividing the numerator of the Bernoulli number Bpβˆ’2nβˆ’kB_{p-2n-k}, or k≑0,1mod  pk \equiv 0, 1 \mod p.Comment: 22 page

    Families of weighted sum formulas for multiple zeta values

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    Euler's sum formula and its multi-variable and weighted generalizations form a large class of the identities of multiple zeta values. In this paper we prove a family of identities involving Bernoulli numbers and apply them to obtain infinitely many weighted sum formulas for double zeta values and triple zeta values where the weight coefficients are given by symmetric polynomials. We give a general conjecture in arbitrary depth at the end of the paper.Comment: The conjecture at the end is reformulate

    On Multiple Zeta Values of Even Arguments

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    For k <= n, let E(2n,k) be the sum of all multiple zeta values with even arguments whose weight is 2n and whose depth is k. Of course E(2n,1) is the value of the Riemann zeta function at 2n, and it is well known that E(2n,2) = (3/4)E(2n,1). Recently Z. Shen and T. Cai gave formulas for E(2n,3) and E(2n,4). We give two formulas form E(2n,k), both valid for arbitrary k <=n, one of which generalizes the Shen-Cai results; by comparing the two we obtain a Bernoulli-number identity. We also give explicit generating functions for the numbers E(2n,k) and for the analogous numbers E*(2n,k) defined using multiple zeta-star values of even arguments.Comment: DESY number added; misprints fixed; reference added. Second revision (2016): New result on multiple zeta-star values adde
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