Records from the S-Matrix Marathon: Observables in Expanding Universes
Paolo Benincasa, Mathieu Giroux, Holmfridur S. Hannesdottir, Sebastian, Mizera, Celina Pasiecznik, Francisco Vaz\~ao

TL;DR
This paper reviews recent advances in understanding observables in expanding universes, focusing on their mathematical structure, the Bunch--Davies wavefunctional, and the combinatorics of cosmological polytopes and nestohedra, with implications for infrared divergences.
Contribution
It introduces a new integral representation for the Bunch--Davies wavefunctional and explores the combinatorial structures underlying cosmological observables.
Findings
Integral representation free of spurious poles
Connection between cosmological polytopes and nestohedra
Insights into infrared divergences in expanding backgrounds
Abstract
Observables in expanding universes are crucial to understand the physics of the early universe. In these lectures, we review some recent progress in understanding their mathematical structure and extract the physics encoded in them. After discussing the most salient features of an expanding background and their consequences for defining an observable, we focus on the so-called Bunch--Davies wavefunctional. We analyze its analytic properties on general grounds and introduce an integral representation for it in perturbation theory for a special class of scalar toy models. We discuss both the diagrammatics associated to the usual Feynman rules and combinatorial rules on the graphs, which generate a representation free of spurious poles. Such combinatorial rules find their origin in the combinatorics of the cosmological polytopes of which we provide a gentle introduction to its definition…
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