Apparaît dans la collection : Combinatorics and Arithmetic for Physics : Special Days
We report on further investigations of combinatorial sequences in form of integral
ratios of factorials. We conceive these integers as Hausdorff power moments for
weights W (x), concentrated on the support x ∈ (0, R), and we solve this mo-
ment problem by furnishing the exact expressions for W (x)’s. In many instances
we can formally prove that the sequences are positive definite. We considered
a large set of families of such sequences including: formulas of Tutte et al. for
enumerations of planar maps, several generalizations of Catalan numbers such
as Fuss-Catalan and Raney numbers, the constellation numbers, and the ratios
of multiple factorials, such as the iconic Kontsevich ($\frac{(6n)!n !}{(3n)![(2n)!]²}$
And Chebyshev ($\frac{(30n)!n !}{(6n)!(10n)!(15n) !}$ ) sequences. Furthermore, we provide the exact solutions for all
three parametrized families of Bober ratios (2009) of factorials, as well as for the
”sporadic” ratios, for all of which the ordinary generating functions (ogf) are alge-
braic. Finally, in the same spirit, we studied the sequences recently constructed by
Rodriquez Villegas (2019-2022), including $\frac{(63n)!(8n)!(2n)!}{
n!(4n)!(16n)!(21n)!(31n)!}$ . In all the cases
listed above we have identified a precisely defined and persistent pattern relating
the Meijer G-encodings of appropriate ogf G(z) and of W (x). In fact, it appears
that in the language of Meijer G-functions, the solutions W (x) are practically
automatically obtained by reshuffling of data characterizing the ogf G(z) only,
i.e. the parameter lists and its radius of convergence R^{−1}. We attempt to cate-
gorize these observations and try to find the criteria for moments which would
allow for such an automatisation. It is also intriguing that the counterexamples
can be found, which clearly point to the limits of this procedure. Finding the pre-
cise criteria for moments which would permit for such a speedy method, is still a
challenging open problem.
⋆ Collaboration at various stages of this work with:
N. Behr, G. H. E. Duchamp, K. Górska, M. Kontsevich, and G. Koshevoy.
