Hawking radiation and propagation of massive charged scalar field on a three-dimensional Godel black hole

dc.contributor.authorGonzalez, P. A.
dc.contributor.authorOvgun, Ali
dc.contributor.authorSaavedra, Joel
dc.contributor.authorVasquez, Yerko
dc.date.accessioned2026-02-06T18:34:28Z
dc.date.issued2018
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractIn this paper we consider the three-dimensional Godel black hole as a background and we study the vector particle tunneling from this background in order to obtain the Hawking temperature. Then, we study the propagation of a massive charged scalar field and we find the quasinormal modes analytically, which turns out be unstable as a consequence of the existence of closed time-like curves. Also, we consider the flux at the horizon and at infinity, and we compute the reflection and transmission coefficients as well as the absorption cross section. Mainly, we show that massive charged scalar waves can be superradiantly amplified by the three-dimensional Godel black hole and that the coefficients have an oscillatory behavior. Moreover, the absorption cross section is null at the high frequency limit and for certain values of the frequency.
dc.description.sponsorshipComision Nacional de Ciencias y Tecnologia through FONDECYT [3170035, 11140674]; Direccion de Investigacion y Desarrollo de la Universidad de La Serena
dc.description.sponsorshipThis work was partially supported by the Comision Nacional de Ciencias y Tecnologia through FONDECYT Grants Nos. 3170035 (AO) and 11140674 (PAG) and by the Direccion de Investigacion y Desarrollo de la Universidad de La Serena (Y.V.). P. A. G. acknowledges the hospitality of the Universidad de La Serena, National Technical University of Athens and Pontificia Universidad Catolica de Valparaiso where part of this work was undertaken. A. O. is grateful to Prof. Douglas Singleton for hosting him as a research visitor at the California State University, Fresno. In addition A. O. would like to thank Prof. Leonard Susskind and Stanford Institute for Theoretical Physics for hospitality.
dc.identifier.doi10.1007/s10714-018-2389-x
dc.identifier.issn0001-7701
dc.identifier.issn1572-9532
dc.identifier.issue6
dc.identifier.orcid0000-0002-9889-342X
dc.identifier.orcid0000-0002-1430-3008
dc.identifier.scopus2-s2.0-85047212975
dc.identifier.scopusqualityQ2
dc.identifier.urihttps://doi.org/10.1007/s10714-018-2389-x
dc.identifier.urihttps://hdl.handle.net/11129/11794
dc.identifier.volume50
dc.identifier.wosWOS:000432919800003
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherSpringer/Plenum Publishers
dc.relation.ispartofGeneral Relativity and Gravitation
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20260204
dc.subjectGodel black hole
dc.subjectHawking radiation
dc.subjectQuantum tunneling
dc.subjectQuasinormal modes
dc.subjectGreybody factors
dc.titleHawking radiation and propagation of massive charged scalar field on a three-dimensional Godel black hole
dc.typeArticle

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