Microscopic origin of the entropy of single-sided black holes

Abstract In this paper, we provide a state-counting derivation of the Bekenstein-Hawking entropy formula for single-sided black holes. We firstly articulate the concept of the black hole microstates. Then we construct explicit mircostates of single-sided black holes in (2+1)-dimensional spacetimes w...

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Main Authors: Hao Geng, Yikun Jiang
Format: Article
Language:English
Published: SpringerOpen 2025-04-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP04(2025)133
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author Hao Geng
Yikun Jiang
author_facet Hao Geng
Yikun Jiang
author_sort Hao Geng
collection DOAJ
description Abstract In this paper, we provide a state-counting derivation of the Bekenstein-Hawking entropy formula for single-sided black holes. We firstly articulate the concept of the black hole microstates. Then we construct explicit mircostates of single-sided black holes in (2+1)-dimensional spacetimes with a negative cosmological constant. These microstates are constructed by putting a Karch-Randall brane behind the black hole horizon. Their difference is described by different interior excitations which gravitationally backreact. We show that these microstates have nonperturbatively small overlaps with each other. As a result, we use this fact to give a state-counting derivation of the Bekenstein-Hawking entropy formula for single-sided black holes. At the end, we notice that there are no negative norm states in the resulting Hilbert space of the black hole microstates which in turn ensures unitarity. All calculations in this paper are analytic and can be easily generalized to higher spacetime dimensions.
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spelling doaj-art-ece8c41f81c14cfeb3da4cc6a47f99e32025-08-20T03:09:35ZengSpringerOpenJournal of High Energy Physics1029-84792025-04-012025412910.1007/JHEP04(2025)133Microscopic origin of the entropy of single-sided black holesHao Geng0Yikun Jiang1Center for the Fundamental Laws of Nature, Harvard UniversityDepartment of Physics, Northeastern UniversityAbstract In this paper, we provide a state-counting derivation of the Bekenstein-Hawking entropy formula for single-sided black holes. We firstly articulate the concept of the black hole microstates. Then we construct explicit mircostates of single-sided black holes in (2+1)-dimensional spacetimes with a negative cosmological constant. These microstates are constructed by putting a Karch-Randall brane behind the black hole horizon. Their difference is described by different interior excitations which gravitationally backreact. We show that these microstates have nonperturbatively small overlaps with each other. As a result, we use this fact to give a state-counting derivation of the Bekenstein-Hawking entropy formula for single-sided black holes. At the end, we notice that there are no negative norm states in the resulting Hilbert space of the black hole microstates which in turn ensures unitarity. All calculations in this paper are analytic and can be easily generalized to higher spacetime dimensions.https://doi.org/10.1007/JHEP04(2025)133AdS-CFT CorrespondenceBlack HolesGauge-Gravity Correspondence
spellingShingle Hao Geng
Yikun Jiang
Microscopic origin of the entropy of single-sided black holes
Journal of High Energy Physics
AdS-CFT Correspondence
Black Holes
Gauge-Gravity Correspondence
title Microscopic origin of the entropy of single-sided black holes
title_full Microscopic origin of the entropy of single-sided black holes
title_fullStr Microscopic origin of the entropy of single-sided black holes
title_full_unstemmed Microscopic origin of the entropy of single-sided black holes
title_short Microscopic origin of the entropy of single-sided black holes
title_sort microscopic origin of the entropy of single sided black holes
topic AdS-CFT Correspondence
Black Holes
Gauge-Gravity Correspondence
url https://doi.org/10.1007/JHEP04(2025)133
work_keys_str_mv AT haogeng microscopicoriginoftheentropyofsinglesidedblackholes
AT yikunjiang microscopicoriginoftheentropyofsinglesidedblackholes