de Sitter JT gravity from double-scaled SYK

Fuente: arXiv
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Main Author: Okuyama, Kazumi
Format: Preprint
Published: 2025
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author Okuyama, Kazumi
author_facet Okuyama, Kazumi
contents It is known that the double-scaled SYK model (DSSYK) reduces to JT gravity with a negative cosmological constant by zooming in on the lower edge $E=-E_0$ of the spectrum. We find that the de Sitter JT gravity (i.e. JT gravity with a positive cosmological constant) is reproduced from DSSYK by taking a scaling limit around the upper edge $E=E_0$ of the spectrum. We also argue that the appearance of de Sitter JT gravity is consistent with the behavior of the classical solution of the sine dilaton gravity.
format Preprint
id arxiv_https___arxiv_org_abs_2505_08116
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle de Sitter JT gravity from double-scaled SYK
Okuyama, Kazumi
High Energy Physics - Theory
It is known that the double-scaled SYK model (DSSYK) reduces to JT gravity with a negative cosmological constant by zooming in on the lower edge $E=-E_0$ of the spectrum. We find that the de Sitter JT gravity (i.e. JT gravity with a positive cosmological constant) is reproduced from DSSYK by taking a scaling limit around the upper edge $E=E_0$ of the spectrum. We also argue that the appearance of de Sitter JT gravity is consistent with the behavior of the classical solution of the sine dilaton gravity.
title de Sitter JT gravity from double-scaled SYK
topic High Energy Physics - Theory
url https://arxiv.org/abs/2505.08116