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dc.contributor.authorRuiz, Ospa
dc.contributor.authorMolina, Uspa
dc.contributor.authorViloria, Pspa
dc.date.accessioned2020-04-12T18:35:25Z
dc.date.available2020-04-12T18:35:25Z
dc.date.issued2019
dc.identifier.issn1742-6588spa
dc.identifier.issn1742-6596spa
dc.identifier.urihttps://hdl.handle.net/11323/6160spa
dc.description.abstractIn this paper we calculate the Hawking temperature of a black hole described by the Kerr-Newman metric, starting from the surface gravity, the area of the event horizon and the angular velocity of the black hole. To do this we apply the laws of black hole thermodynamics: we first set the energy conservation through a relationship between the mass M, the charge Q and the angular momentum J, then we implement the Hawking's theorem of areas by setting an upper bound to the energy and we get finally the surface gravity of the black hole. In addition, we study the relationship between the black hole parameters (mass M, angular momentum J, electric charge Q) and the Hawking temperature.spa
dc.language.isoeng
dc.publisherJournal of Physics: Conference Seriesspa
dc.rightsCC0 1.0 Universalspa
dc.rights.urihttp://creativecommons.org/publicdomain/zero/1.0/spa
dc.subjectHawking temperaturespa
dc.subjectKerr-Newmanspa
dc.subjectThermodynamic analysisspa
dc.titleThermodynamic analysis of Kerr-Newman black holesspa
dc.typeArtículo de revistaspa
dc.rights.accessrightsinfo:eu-repo/semantics/openAccessspa
dc.identifier.doidoi:10.1088/1742-6596/1219/1/012016spa
dc.identifier.instnameCorporación Universidad de la Costaspa
dc.identifier.reponameREDICUC - Repositorio CUCspa
dc.identifier.repourlhttps://repositorio.cuc.edu.co/spa
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dc.relation.references[2] Hawking S W 1975 Particle Creation by Black Holes Comm. Math. Phys. 43 199spa
dc.relation.references[3] Pankovic V 2009 Black Holes - A Simplified Theory for Quantum Gravity Non-Specialists, arXiv:0911.1026v1 [physics.gen-ph]spa
dc.relation.references[4] Belgiorno F, Caciatori S L, Clerici M, Gorini V, Ortenzi G, Rizzi L, Rubino V G and Faccion D 2010 Hawking Radiation from Ultrashort Laser Pulse Filaments Phys. Rev. Lett. 105 203901spa
dc.relation.references[5] Miranda C, Molina U and Viloria P 2014 Retardo temporal en las lentes por galaxias en el contexto de Reissner - Nordstrom Revista Mexicana de Física 60(3) 190spa
dc.relation.references[6] Newman E, Couch R, Chinnapared K, Exton A, Prakash A and Torrence R 1965 Metric of a rotating charged mass J. Math. Phys. 6 918spa
dc.relation.references[7] Hawking S W 1971 Gravitational radiation from colliding black holes Phys. Rev. Lett. 26 1344spa
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dc.relation.references[11] Misner C, Thorne K and Wheeler J 1973 Gravitation (San Francisco: W.H. Freeman & Co)spa
dc.relation.references[12] Bardeen J M, Carter B and Hawking S W 1973, The Four laws of black hole mechanics Commun. Math. Phys. 31 161spa
dc.relation.references[13] Bekenstein J 1972 Black holes and the second law Lett. Nuo. Cim. 4 737spa
dc.relation.references[14] Bekenstein J 1974 Generalized Second Law of Thermodynamics in Black Hole Physics Phys. Rev. D. 9 3292spa
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dc.type.coarhttp://purl.org/coar/resource_type/c_6501spa
dc.type.contentTextspa
dc.type.driverinfo:eu-repo/semantics/articlespa
dc.type.redcolhttp://purl.org/redcol/resource_type/ARTspa
dc.type.versioninfo:eu-repo/semantics/acceptedVersionspa
dc.type.coarversionhttp://purl.org/coar/version/c_ab4af688f83e57aaspa
dc.rights.coarhttp://purl.org/coar/access_right/c_abf2spa


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