Explicit black hole thermodynamics in natural variables

Abstract We consider the general thermal asymptotically flat Kerr-Newman black holes in 4d Einstein-Maxwell theory. Even though their thermodynamics has been understood for decades, the Gibbs free energy and on-shell action are only known implicitly as functions of the standard chemical potentials....

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Main Author: Kiril Hristov
Format: Article
Language:English
Published: SpringerOpen 2023-08-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP08(2023)003
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author Kiril Hristov
author_facet Kiril Hristov
author_sort Kiril Hristov
collection DOAJ
description Abstract We consider the general thermal asymptotically flat Kerr-Newman black holes in 4d Einstein-Maxwell theory. Even though their thermodynamics has been understood for decades, the Gibbs free energy and on-shell action are only known implicitly as functions of the standard chemical potentials. Using the so-called left and right moving (or holomorphic and anti-holomorphic) variables related to the chemical potentials on both the outer and the inner horizons, we are able to present explicit and very simple expressions for all quantities. We discuss various limits in the parameter space, remarkably finding a smooth BPS limit allowing direct access to the extremal surface. In the BPS limit the anti-holomorphic part of the on-shell action vanishes identically, leading automatically to the holomorphic expression expected microscopically. This gives us confidence that the newly defined thermal partition function in terms of these variables is the natural candidate for a full microscopic description.
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spelling doaj.art-13578ee2c91d4040ae46ee558262a8e62023-10-29T12:12:23ZengSpringerOpenJournal of High Energy Physics1029-84792023-08-012023811210.1007/JHEP08(2023)003Explicit black hole thermodynamics in natural variablesKiril Hristov0Faculty of Physics, Sofia UniversityAbstract We consider the general thermal asymptotically flat Kerr-Newman black holes in 4d Einstein-Maxwell theory. Even though their thermodynamics has been understood for decades, the Gibbs free energy and on-shell action are only known implicitly as functions of the standard chemical potentials. Using the so-called left and right moving (or holomorphic and anti-holomorphic) variables related to the chemical potentials on both the outer and the inner horizons, we are able to present explicit and very simple expressions for all quantities. We discuss various limits in the parameter space, remarkably finding a smooth BPS limit allowing direct access to the extremal surface. In the BPS limit the anti-holomorphic part of the on-shell action vanishes identically, leading automatically to the holomorphic expression expected microscopically. This gives us confidence that the newly defined thermal partition function in terms of these variables is the natural candidate for a full microscopic description.https://doi.org/10.1007/JHEP08(2023)003Black HolesBlack Holes in String TheoryClassical Theories of Gravity
spellingShingle Kiril Hristov
Explicit black hole thermodynamics in natural variables
Journal of High Energy Physics
Black Holes
Black Holes in String Theory
Classical Theories of Gravity
title Explicit black hole thermodynamics in natural variables
title_full Explicit black hole thermodynamics in natural variables
title_fullStr Explicit black hole thermodynamics in natural variables
title_full_unstemmed Explicit black hole thermodynamics in natural variables
title_short Explicit black hole thermodynamics in natural variables
title_sort explicit black hole thermodynamics in natural variables
topic Black Holes
Black Holes in String Theory
Classical Theories of Gravity
url https://doi.org/10.1007/JHEP08(2023)003
work_keys_str_mv AT kirilhristov explicitblackholethermodynamicsinnaturalvariables