Quasi-Homogeneous Black Hole Thermodynamics in Non-Commutative Geometry

We study the thermodynamic properties of a black hole that takes into account the effects of non-commutative geometry. To emphasize the role of new effects, we have chosen a specific modified Schwarzschild black hole inspired by non-commutative geometry. We show that, in order to apply the laws of q...

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Bibliographic Details
Main Authors: Hernando Quevedo, María N. Quevedo
Format: Article
Language:English
Published: MDPI AG 2025-02-01
Series:Universe
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Online Access:https://www.mdpi.com/2218-1997/11/3/79
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Summary:We study the thermodynamic properties of a black hole that takes into account the effects of non-commutative geometry. To emphasize the role of new effects, we have chosen a specific modified Schwarzschild black hole inspired by non-commutative geometry. We show that, in order to apply the laws of quasi-homogeneous thermodynamics using the formalism of geometrothermodynamics, it is necessary to consider the non-commutative parameter as an independent thermodynamic variable. As a result, the properties of the black hole change drastically, leading to phase transitions that are directly related to the value of the non-commutative parameter. We also prove that an unstable commutative black hole can become stable in non-commutative geometry for particular values of the non-commutative parameter.
ISSN:2218-1997