Upper Bound of Barrow Entropy Index from Black Hole Fragmentation

Fuente: arXiv
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Autori principali: Xia, Jiayi, Ong, Yen Chin
Natura: Preprint
Pubblicazione: 2024
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author Xia, Jiayi
Ong, Yen Chin
author_facet Xia, Jiayi
Ong, Yen Chin
contents Both classical and quantum arguments suggest that if Barrow entropy is correct, its index $δ$ must be energy dependent, which would affect the very early universe. Based on thermodynamic stability that sufficiently large black holes should not fragment, we argue that Barrow entropy correction must be small except possibly at the Planckian regime. Furthermore, the fact that a solar mass black hole does not fragment implies an upper bound $δ\lesssim O(10^{-3})$, which surprisingly lies in the same range as the bound obtained from some cosmological considerations assuming fixed $δ$. This indicates that allowing $δ$ to run does not raise its allowed value. We briefly comment on the case of Kaniadakis entropy.
format Preprint
id arxiv_https___arxiv_org_abs_2404_09278
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Upper Bound of Barrow Entropy Index from Black Hole Fragmentation
Xia, Jiayi
Ong, Yen Chin
General Relativity and Quantum Cosmology
High Energy Physics - Theory
Both classical and quantum arguments suggest that if Barrow entropy is correct, its index $δ$ must be energy dependent, which would affect the very early universe. Based on thermodynamic stability that sufficiently large black holes should not fragment, we argue that Barrow entropy correction must be small except possibly at the Planckian regime. Furthermore, the fact that a solar mass black hole does not fragment implies an upper bound $δ\lesssim O(10^{-3})$, which surprisingly lies in the same range as the bound obtained from some cosmological considerations assuming fixed $δ$. This indicates that allowing $δ$ to run does not raise its allowed value. We briefly comment on the case of Kaniadakis entropy.
title Upper Bound of Barrow Entropy Index from Black Hole Fragmentation
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2404.09278