Non-Einsteinian black holes in generic 3D gravity theories

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buir.contributor.authorGürses, Metin
dc.citation.epage064053-6en_US
dc.citation.issueNumber6en_US
dc.citation.spage064053-1en_US
dc.citation.volumeNumber100en_US
dc.contributor.authorGürses, Metinen_US
dc.contributor.authorŞişman, T. Ç.en_US
dc.contributor.authorTekin, B.en_US
dc.date.accessioned2020-02-11T06:54:31Z
dc.date.available2020-02-11T06:54:31Z
dc.date.issued2019
dc.departmentDepartment of Mathematicsen_US
dc.description.abstractThe Bañados-Teitelboim-Zanelli (BTZ) black hole metric solves the three-dimensional Einstein’s theory with a negative cosmological constant as well as all the generic higher derivative gravity theories based on the metric; as such it is a universal solution. Here, we find, in all generic higher derivative gravity theories, new universal non-Einsteinian solutions obtained as Kerr-Schild type deformations of the BTZ black hole. Among these, the deformed nonextremal BTZ black hole loses its event horizon while the deformed extremal one remains intact as a black hole in any generic gravity theory.en_US
dc.identifier.doi10.1103/PhysRevD.100.064053en_US
dc.identifier.issn2470-0010
dc.identifier.urihttp://hdl.handle.net/11693/53251
dc.language.isoEnglishen_US
dc.publisherAmerican Physical Societyen_US
dc.relation.isversionofhttps://dx.doi.org/10.1103/PhysRevD.100.064053en_US
dc.source.titlePhysical Review Den_US
dc.subjectGravitationen_US
dc.subjectCosmologyen_US
dc.subjectAstrophysicsen_US
dc.subjectAlternative gravity theoriesen_US
dc.subjectGravity in dimensions other than fouren_US
dc.titleNon-Einsteinian black holes in generic 3D gravity theoriesen_US
dc.typeArticleen_US

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