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Ehrhart theory of cosmological polytopes

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arxiv 2412.01602 v2 pith:CA6MUELT submitted 2024-12-02 math.CO

classification math.CO
keywords cosmologicalpolynomialpolytopepolytopesresultsassociatedboundcomputed
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abstract

The cosmological polytope of a graph $G$ was recently introduced to give a geometric approach to the computation of wavefunctions for cosmological models with associated Feynman diagram $G$. Basic results in the theory of positive geometries dictate that this wavefunction may be computed as a sum of rational functions associated to the facets in a triangulation of the cosmological polytope. The normalized volume of the polytope then provides a complexity estimate for these computations. In this paper, we examine the (Ehrhart) $h^\ast$-polynomial of cosmological polytopes. We derive recursive formulas for computing the $h^\ast$-polynomial of disjoint unions and $1$-sums of graphs. The degree of the $h^\ast$-polynomial for any $G$ is computed and a characterization of palindromicity is given. Using these observations, a tight lower bound on the $h^\ast$-polynomial for any $G$ is identified and explicit formulas for the $h^\ast$-polynomials of multitrees and multicycles are derived. The results generalize the existing results on normalized volumes of cosmological polytopes. A tight upper bound and a combinatorial formula for the $h^\ast$-polynomial of any cosmological polytope are conjectured.

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  1. Ternary relations and their polytopes

    math.CO 2025-09 conditional novelty 6.0 of 10

    Cosmological polytopes and Graev polytopes are unified through ternary relations on 2-dimensional simplicial posets, yielding new facet families for some root-system polytopes.

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