Solution of Deformed Einstein Equations and Quantum Black Holes

dc.authoridkolay, erdinc/0000-0001-7436-3152
dc.authoridDil, Emre/0000-0002-9042-7694
dc.contributor.authorDil, Emre
dc.contributor.authorKolay, Erdinc
dc.date.accessioned2025-03-23T19:30:52Z
dc.date.available2025-03-23T19:30:52Z
dc.date.issued2016
dc.departmentSinop Üniversitesi
dc.description.abstractRecently, 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-Nordstr om black holes. This reduction in mass of a usual black hole can be considered as a transition from classical to quantum black hole regime.
dc.identifier.doi10.1155/2016/3973706
dc.identifier.issn1687-7357
dc.identifier.issn1687-7365
dc.identifier.scopus2-s2.0-84982795813
dc.identifier.scopusqualityQ2
dc.identifier.urihttps://doi.org/10.1155/2016/3973706
dc.identifier.urihttps://hdl.handle.net/11486/5183
dc.identifier.volume2016
dc.identifier.wosWOS:000380725400001
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherHindawi Ltd
dc.relation.ispartofAdvances in High Energy Physics
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WOS_20250323
dc.subjectEntropic Force
dc.subjectFriedmann Equation
dc.subjectStatistics
dc.subjectThermostatistics
dc.subjectThermodynamics
dc.subjectBehavior
dc.subjectModel
dc.subjectGas
dc.titleSolution of Deformed Einstein Equations and Quantum Black Holes
dc.typeArticle

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