Solution of Deformed Einstein Equations and Quantum Black Holes

Recently, one- and two-parameter deformed Einstein equations have been studied for extremal quantum black holes which have been proposed to obey deformed statistics by Strominger. In this study, we give a deeper insight into the deformed Einstein equations and consider the solutions of these equatio...

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Main Authors: Emre Dil, Erdinç Kolay
Format: Article
Language:English
Published: Wiley 2016-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2016/3973706
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author Emre Dil
Erdinç Kolay
author_facet Emre Dil
Erdinç Kolay
author_sort Emre Dil
collection DOAJ
description Recently, one- and two-parameter deformed Einstein equations have been studied for extremal quantum black holes which have been proposed to obey deformed statistics by Strominger. In this study, we give a deeper insight into the deformed Einstein equations and consider the solutions of these equations for the extremal quantum black holes. We then represent the implications of the solutions, such that the deformation parameters lead the charged black holes to have a smaller mass than the usual Reissner-Nordström black holes. This reduction in mass of a usual black hole can be considered as a transition from classical to quantum black hole regime.
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spelling doaj-art-a0cca4e6d66b463abb92f20ba1987e1d2025-02-03T05:43:43ZengWileyAdvances in High Energy Physics1687-73571687-73652016-01-01201610.1155/2016/39737063973706Solution of Deformed Einstein Equations and Quantum Black HolesEmre Dil0Erdinç Kolay1Department of Physics, Sinop University, Korucuk, 57000 Sinop, TurkeyDepartment of Statistics, Sinop University, Korucuk, 57000 Sinop, TurkeyRecently, one- and two-parameter deformed Einstein equations have been studied for extremal quantum black holes which have been proposed to obey deformed statistics by Strominger. In this study, we give a deeper insight into the deformed Einstein equations and consider the solutions of these equations for the extremal quantum black holes. We then represent the implications of the solutions, such that the deformation parameters lead the charged black holes to have a smaller mass than the usual Reissner-Nordström black holes. This reduction in mass of a usual black hole can be considered as a transition from classical to quantum black hole regime.http://dx.doi.org/10.1155/2016/3973706
spellingShingle Emre Dil
Erdinç Kolay
Solution of Deformed Einstein Equations and Quantum Black Holes
Advances in High Energy Physics
title Solution of Deformed Einstein Equations and Quantum Black Holes
title_full Solution of Deformed Einstein Equations and Quantum Black Holes
title_fullStr Solution of Deformed Einstein Equations and Quantum Black Holes
title_full_unstemmed Solution of Deformed Einstein Equations and Quantum Black Holes
title_short Solution of Deformed Einstein Equations and Quantum Black Holes
title_sort solution of deformed einstein equations and quantum black holes
url http://dx.doi.org/10.1155/2016/3973706
work_keys_str_mv AT emredil solutionofdeformedeinsteinequationsandquantumblackholes
AT erdinckolay solutionofdeformedeinsteinequationsandquantumblackholes