On Thermodynamic Stability of Black Holes. Part II: AdS Family of Solutions

Fuente: arXiv
Guardado en:
Detalles Bibliográficos
Autores principales: Avramov, V., Dimov, H., Radomirov, M., Rashkov, R. C., Vetsov, T.
Formato: Preprint
Publicado: 2024
Materias:
Acceso en línea:
Etiquetas: Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
_version_ 1866910762937614336
author Avramov, V.
Dimov, H.
Radomirov, M.
Rashkov, R. C.
Vetsov, T.
author_facet Avramov, V.
Dimov, H.
Radomirov, M.
Rashkov, R. C.
Vetsov, T.
contents This study is aimed at providing a thorough analysis of the classical thermodynamic stability of black holes within the Anti-de Sitter (AdS) family. We utilize the Nambu bracket formalism to calculate local heat capacities and employ Sylvester's criterion in the mass-energy ensemble to determine both local and global thermodynamic stability regions. Emphasizing the crucial role of the cosmological constant, we establish the conditions necessary for the existence of thermodynamically stable black hole configurations. Our work highlights the applicability of classical thermodynamics in understanding black hole physics, while acknowledging the potential deviations that may impact the observables of the system beyond the classical level.
format Preprint
id arxiv_https___arxiv_org_abs_2402_07272
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle On Thermodynamic Stability of Black Holes. Part II: AdS Family of Solutions
Avramov, V.
Dimov, H.
Radomirov, M.
Rashkov, R. C.
Vetsov, T.
General Relativity and Quantum Cosmology
This study is aimed at providing a thorough analysis of the classical thermodynamic stability of black holes within the Anti-de Sitter (AdS) family. We utilize the Nambu bracket formalism to calculate local heat capacities and employ Sylvester's criterion in the mass-energy ensemble to determine both local and global thermodynamic stability regions. Emphasizing the crucial role of the cosmological constant, we establish the conditions necessary for the existence of thermodynamically stable black hole configurations. Our work highlights the applicability of classical thermodynamics in understanding black hole physics, while acknowledging the potential deviations that may impact the observables of the system beyond the classical level.
title On Thermodynamic Stability of Black Holes. Part II: AdS Family of Solutions
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2402.07272