Non-extensive and quasi-homogeneous geometrothermodynamics

Fuente: arXiv
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Autori principali: Quevedo, Hernando, Quevedo, María N.
Natura: Preprint
Pubblicazione: 2025
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author Quevedo, Hernando
Quevedo, María N.
author_facet Quevedo, Hernando
Quevedo, María N.
contents We study the thermodynamic properties of black holes, taking into account the non-extensive character of their entropy at the thermodynamic and statistical level. To this end, we assume that the Rényi entropy determines the fundamental thermodynamic equation of black holes and is represented by a quasi-homogeneous function. As a consequence, the Rényi parameter turns out to be an independent thermodynamic variable, which must be treated in the framework of extended thermodynamics. As a particular example, we use the formalism of geometrothermodynamics to show that the Schwarzschild black hole can become stable for certain values of the Rényi parameter.
format Preprint
id arxiv_https___arxiv_org_abs_2506_21342
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Non-extensive and quasi-homogeneous geometrothermodynamics
Quevedo, Hernando
Quevedo, María N.
General Relativity and Quantum Cosmology
We study the thermodynamic properties of black holes, taking into account the non-extensive character of their entropy at the thermodynamic and statistical level. To this end, we assume that the Rényi entropy determines the fundamental thermodynamic equation of black holes and is represented by a quasi-homogeneous function. As a consequence, the Rényi parameter turns out to be an independent thermodynamic variable, which must be treated in the framework of extended thermodynamics. As a particular example, we use the formalism of geometrothermodynamics to show that the Schwarzschild black hole can become stable for certain values of the Rényi parameter.
title Non-extensive and quasi-homogeneous geometrothermodynamics
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2506.21342