Thermal analysis of black hole in de Rham--Gabadadze--Tolley massive gravity in Barrow entropy framework

Fuente: arXiv
Salvato in:
Dettagli Bibliografici
Autori principali: Yasir, Muhammad, Xia, Tiecheng, Upadhyay, Sudhaker
Natura: Preprint
Pubblicazione: 2024
Soggetti:
Accesso online:
Tags: Aggiungi Tag
Nessun Tag, puoi essere il primo ad aggiungerne!!
_version_ 1866917661327228928
author Yasir, Muhammad
Xia, Tiecheng
Upadhyay, Sudhaker
author_facet Yasir, Muhammad
Xia, Tiecheng
Upadhyay, Sudhaker
contents This study examines a recently hypothesized black hole solution in de Rham--Gabadadze--Tolley massive gravity. Firstly, we consider the negative cosmological constant as a thermodynamic pressure. We extract the thermodynamical properties such as Hawking temperature, heat capacity and Gibbs free energy using the Barrow entropy. We also obtain a new pressure associated to the perfect fluid dark matter and discuss the first-order van der Waals-like phase transition. This black hole's stability is investigated through specific heat and Gibbs free energy. Also, we analyze the thermodynamic curvatures behavior of black hole through geometry methods (Weinhold, Ruppeiner, Hendi-Panahiyah-Eslam-Momennia (HPEM), and geometrothermodynamics (GTD)).
format Preprint
id arxiv_https___arxiv_org_abs_2405_04833
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Thermal analysis of black hole in de Rham--Gabadadze--Tolley massive gravity in Barrow entropy framework
Yasir, Muhammad
Xia, Tiecheng
Upadhyay, Sudhaker
General Relativity and Quantum Cosmology
High Energy Physics - Theory
This study examines a recently hypothesized black hole solution in de Rham--Gabadadze--Tolley massive gravity. Firstly, we consider the negative cosmological constant as a thermodynamic pressure. We extract the thermodynamical properties such as Hawking temperature, heat capacity and Gibbs free energy using the Barrow entropy. We also obtain a new pressure associated to the perfect fluid dark matter and discuss the first-order van der Waals-like phase transition. This black hole's stability is investigated through specific heat and Gibbs free energy. Also, we analyze the thermodynamic curvatures behavior of black hole through geometry methods (Weinhold, Ruppeiner, Hendi-Panahiyah-Eslam-Momennia (HPEM), and geometrothermodynamics (GTD)).
title Thermal analysis of black hole in de Rham--Gabadadze--Tolley massive gravity in Barrow entropy framework
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2405.04833