Cosmohedra
Nima Arkani-Hamed, Carolina Figueiredo, Francisco Vazão
TL;DR
Cosmohedra introduce a new geometric object that unifies the combinatorics of the cosmological wavefunction for $\mathrm{Tr}(\phi^3)$ theory by blowing up associahedra into cosmohedra and organizing contributions via graph associahedra. The framework provides a canonical-form-based route to compute the wavefunction at tree level and extends to loop orders through loop cosmohedra and loop graph associahedra, with permuto-cosmohedra offering a simple, though larger, simple-polytope realization for extraction. It also connects to cosmological correlahedra, proposing a higher-dimensional geometry that captures full correlators by sandwiching cosmohedra and associahedra. The work outlines explicit 5–7 point and loop examples, characterizes facet factorization, and suggests directions toward a stringy formulation of cosmology and deeper relations to kinematic flow and surface-based pictures. Overall, cosmohedra provide a promising, self-contained geometric language for cosmological observables and their diagrammatic structure, with rich avenues for future exploration.
Abstract
It has been a long-standing challenge to find a geometric object underlying the cosmological wavefunction for Tr($φ^3$) theory, generalizing associahedra and surfacehedra for scattering amplitudes. In this note we describe a new class of polytopes -- "cosmohedra" -- that provide a natural solution to this problem. Cosmohedra are intimately related to associahedra, obtained by "blowing up" faces of the associahedron in a simple way, and we provide an explicit realization in terms of facet inequalities that further "shave" the facet inequalities of the associahedron. We also discuss a novel way for computing the wavefunction from cosmohedron geometry that extends the usual connection with polytope canonical forms. We illustrate cosmohedra with examples at tree-level and one loop; the close connection to surfacehedra suggests the generalization to all loop orders. We also briefly describe "cosmological correlahedra" for full correlators. We speculate on how the existence of cosmohedra might suggest a "stringy" formulation for the cosmological wavefunction/correlators, generalizing the way in which the Minkowski sum decomposition of associahedra naturally extend particle to string amplitudes.
