Bopp-Podolsky black holes and the no-hair theorem

Registro completo de metadados
MetadadosDescriçãoIdioma
Autor(es): dc.contributorUniversidade Estadual Paulista (UNESP)-
Autor(es): dc.creatorCuzinatto, R. R.-
Autor(es): dc.creatorMelo, C. A. M. de-
Autor(es): dc.creatorMedeiros, L. G.-
Autor(es): dc.creatorPimentel, B. M.-
Autor(es): dc.creatorPompeia, P. J.-
Data de aceite: dc.date.accessioned2021-03-10T23:56:53Z-
Data de disponibilização: dc.date.available2021-03-10T23:56:53Z-
Data de envio: dc.date.issued2018-11-26-
Data de envio: dc.date.issued2018-11-26-
Data de envio: dc.date.issued2018-01-19-
Fonte completa do material: dc.identifierhttp://dx.doi.org/10.1140/epjc/s10052-018-5525-6-
Fonte completa do material: dc.identifierhttp://hdl.handle.net/11449/163756-
Fonte: dc.identifier.urihttp://educapes.capes.gov.br/handle/11449/163756-
Descrição: dc.descriptionCoordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)-
Descrição: dc.descriptionConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)-
Descrição: dc.descriptionCAPES: 88881.119228/2016-01-
Descrição: dc.descriptionCNPq: 112861/2015-6-
Descrição: dc.descriptionBopp-Podolsky electrodynamics is generalized to curved space-times. The equations of motion are written for the case of static spherically symmetric black holes and their exterior solutions are analyzed using Bekenstein's method. It is shown that the solutions split up into two parts, namely a non-homogeneous (asymptotically massless) regime and a homogeneous (asymptotically massive) sector which is null outside the event horizon. In addition, in the simplest approach to Bopp-Podolsky black holes, the non-homogeneous solutions are found to be Maxwell's solutions leading to a Reissner-Nordstrom black hole. It is also demonstrated that the only exterior solution consistent with the weak and null energy conditions is the Maxwell one. Thus, in the light of the energy conditions, it is concluded that only Maxwell modes propagate outside the horizon and, therefore, the no-hair theorem is satisfied in the case of Bopp-Podolsky fields in spherically symmetric space-times.-
Formato: dc.format9-
Idioma: dc.languageen-
Publicador: dc.publisherSpringer-
Relação: dc.relationEuropean Physical Journal C-
Relação: dc.relation2,022-
Direitos: dc.rightsopenAccess-
Título: dc.titleBopp-Podolsky black holes and the no-hair theorem-
Tipo de arquivo: dc.typelivro digital-
Aparece nas coleções:Repositório Institucional - Unesp

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