Towards a microscopic description of de Sitter dynamics
Vladimir Narovlansky

TL;DR
This paper proposes a quantum system based on SYK to model de Sitter space dynamics, successfully reproducing classical gravity correlators and revealing unique chaotic features.
Contribution
It introduces a microscopic quantum model that captures key semiclassical de Sitter properties and exhibits novel chaotic behavior consistent with gravitational scattering.
Findings
Correlators match classical de Sitter gravity limits.
Quantum system reproduces UV behavior of quantum fields.
OTOCs show a Lyapunov exponent twice the chaos bound.
Abstract
Describing dynamics in a gravitational universe with positive cosmological constant, such as de Sitter space, is a conceptually challenging problem. We propose a principle for constructing a quantum system that can potentially be used to study this question. This quantum system describes a heavy object in such a universe interacting with its environment, to which gauge invariant dynamical observables can be anchored. In order to describe gravity with positive cosmological constant, the proposed quantum system needs to agree with all known semiclassical results. We investigate this with a particular microscopic realization constructed using SYK. We first find that correlators match the classical limit of gravity, given by quantum fields in rigid de Sitter space. In particular, the usual UV behavior of quantum fields is surprisingly reproduced by the quantum mechanical system. In order to…
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