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Bibliographic Details
Main Author: Wang, Zhi
Format: Preprint
Published: 2025
Subjects:
Online Access:https://arxiv.org/abs/2506.03058
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author Wang, Zhi
author_facet Wang, Zhi
contents We construct an infinite family of semiclassical de Sitter (dS) microstates, realized as backreacted geometries of dS spacetime with a constant tension thin-shell brane located outside the dS event horizon. We further show that wormhole contributions to the semiclassical Euclidean gravitational path integral lead to universal nonperturbative overlaps between these microstates. By evaluating the nonperturbative overlaps, we count the dimension of the Hilbert space spanned by the semiclassical dS microstates and find that it precisely equals the exponential of the Gibbons-Hawking entropy of dS spacetime. Our construction thus provides a state-counting derivation for Gibbons-Hawking entropy of dS spacetime.
format Preprint
id arxiv_https___arxiv_org_abs_2506_03058
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Microscopic origin of the entropy of de Sitter spacetime
Wang, Zhi
High Energy Physics - Theory
We construct an infinite family of semiclassical de Sitter (dS) microstates, realized as backreacted geometries of dS spacetime with a constant tension thin-shell brane located outside the dS event horizon. We further show that wormhole contributions to the semiclassical Euclidean gravitational path integral lead to universal nonperturbative overlaps between these microstates. By evaluating the nonperturbative overlaps, we count the dimension of the Hilbert space spanned by the semiclassical dS microstates and find that it precisely equals the exponential of the Gibbons-Hawking entropy of dS spacetime. Our construction thus provides a state-counting derivation for Gibbons-Hawking entropy of dS spacetime.
title Microscopic origin of the entropy of de Sitter spacetime
topic High Energy Physics - Theory
url https://arxiv.org/abs/2506.03058