Hawking radiation via Gauss-Bonnet theorem

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dc.contributor.authorOvgun, A.
dc.contributor.authorSakalli, I
dc.date.accessioned2026-02-06T18:36:20Z
dc.date.issued2020
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractIn this paper, we apply the topological method to the various black holes to derive their Hawking temperature. We show that the this method can easily be employed to compute the Hawking temperature of black holes having spherically symmetric topology. Therefore, we conclude that the topological method provides a consistent formula to achieve the Hawking temperature. (C) 2020 Elsevier Inc. All rights reserved.
dc.description.sponsorshipComision Nacional de Ciencias y Tecnologia of Chile through FONDECYT, Chile [3170035]
dc.description.sponsorshipThis work was supported by Comision Nacional de Ciencias y Tecnologia of Chile through FONDECYT, Chile Grant No 3170035 (A. O.).
dc.identifier.doi10.1016/j.aop.2020.168071
dc.identifier.issn0003-4916
dc.identifier.issn1096-035X
dc.identifier.orcid0000-0001-7827-9476
dc.identifier.orcid0000-0002-9889-342X
dc.identifier.scopus2-s2.0-85077653649
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1016/j.aop.2020.168071
dc.identifier.urihttps://hdl.handle.net/11129/12312
dc.identifier.volume413
dc.identifier.wosWOS:000512473400011
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherAcademic Press Inc Elsevier Science
dc.relation.ispartofAnnals of Physics
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20260204
dc.subjectBlack hole
dc.subjectTemperature
dc.subjectHawking radiation
dc.subjectThermodynamics
dc.subjectGauss Bonnet theorem
dc.subjectEuler characteristic
dc.titleHawking radiation via Gauss-Bonnet theorem
dc.typeArticle

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