Thermodynamics of the three-dimensional black hole with torsion

Abstract The stationary black hole solution of a Chern-Simons model based on the semi-simple extension of the Poincaré gauge group is studied. The solution resembles the metric properties of the BTZ geometry but contains, in addition, non-vanishing torsion. The global structure of spacetime is chara...

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Main Authors: Luis Avilés, Diego Hidalgo, Omar Valdivia
Format: Article
Language:English
Published: SpringerOpen 2023-09-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP09(2023)185
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author Luis Avilés
Diego Hidalgo
Omar Valdivia
author_facet Luis Avilés
Diego Hidalgo
Omar Valdivia
author_sort Luis Avilés
collection DOAJ
description Abstract The stationary black hole solution of a Chern-Simons model based on the semi-simple extension of the Poincaré gauge group is studied. The solution resembles the metric properties of the BTZ geometry but contains, in addition, non-vanishing torsion. The global structure of spacetime is characterized by three conserved charges: two associated with the mass and angular momentum and one extra constant triggered by spacetime torsion. Consequently, we show that the entropy deviates from the standard Bekenstein-Hawking value and discuss the implications of torsional charges in the context of black hole thermodynamics.
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spelling doaj.art-0a1fe4b0100e49d9a287b677b5e531892023-12-31T12:08:15ZengSpringerOpenJournal of High Energy Physics1029-84792023-09-012023911910.1007/JHEP09(2023)185Thermodynamics of the three-dimensional black hole with torsionLuis Avilés0Diego Hidalgo1Omar Valdivia2Instituto de Ciencias Exactas y Naturales (ICEN), Universidad Arturo PratScience Institute, University of IcelandInstituto de Ciencias Exactas y Naturales (ICEN), Universidad Arturo PratAbstract The stationary black hole solution of a Chern-Simons model based on the semi-simple extension of the Poincaré gauge group is studied. The solution resembles the metric properties of the BTZ geometry but contains, in addition, non-vanishing torsion. The global structure of spacetime is characterized by three conserved charges: two associated with the mass and angular momentum and one extra constant triggered by spacetime torsion. Consequently, we show that the entropy deviates from the standard Bekenstein-Hawking value and discuss the implications of torsional charges in the context of black hole thermodynamics.https://doi.org/10.1007/JHEP09(2023)185Black HolesChern-Simons TheoriesClassical Theories of GravitySpace-Time Symmetries
spellingShingle Luis Avilés
Diego Hidalgo
Omar Valdivia
Thermodynamics of the three-dimensional black hole with torsion
Journal of High Energy Physics
Black Holes
Chern-Simons Theories
Classical Theories of Gravity
Space-Time Symmetries
title Thermodynamics of the three-dimensional black hole with torsion
title_full Thermodynamics of the three-dimensional black hole with torsion
title_fullStr Thermodynamics of the three-dimensional black hole with torsion
title_full_unstemmed Thermodynamics of the three-dimensional black hole with torsion
title_short Thermodynamics of the three-dimensional black hole with torsion
title_sort thermodynamics of the three dimensional black hole with torsion
topic Black Holes
Chern-Simons Theories
Classical Theories of Gravity
Space-Time Symmetries
url https://doi.org/10.1007/JHEP09(2023)185
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AT diegohidalgo thermodynamicsofthethreedimensionalblackholewithtorsion
AT omarvaldivia thermodynamicsofthethreedimensionalblackholewithtorsion