Surrounded Bonnor-Vaidya solution by cosmological fields

buir.contributor.authorHeydarzade, Yaghoub
dc.citation.epage1004-1en_US
dc.citation.issueNumber12en_US
dc.citation.spage1004-27en_US
dc.citation.volumeNumber78en_US
dc.contributor.authorHeydarzade, Yaghouben_US
dc.contributor.authorDarabi, F.en_US
dc.date.accessioned2019-02-21T16:06:40Z
dc.date.available2019-02-21T16:06:40Z
dc.date.issued2018en_US
dc.departmentDepartment of Mathematicsen_US
dc.description.abstractIn the present work, we generalize our previous work (Heydarzade and Darabi in arXiv:1710.04485, 2018 on the surrounded Vaidya solution by cosmological fields to the case of Bonnor-Vaidya charged solution. In this regard, we construct a solution for the classical description of the evaporating-accreting charged Bonnor-Vaidya black holes in the generic dynamical backgrounds. We address some interesting features of these solutions and classify them according to their behaviors under imposing the positive energy condition. Also, we analyze the timelike geodesics associated with the obtained solutions and show that some new correction terms arise in comparison to the case of standard Schwarzschild black hole. Then, we explore all these features for each of the cosmological backgrounds of dust, radiation, quintessence and cosmological constant-like fields in more detail.
dc.description.sponsorshipAcknowledgements This work has been supported financially by Research Institute for Astronomy and Astrophysics of Maragha (RIAAM) under research project no. 1/5237-17.
dc.identifier.doi10.1140/epjc/s10052-018-6465-x
dc.identifier.issn1434-6044
dc.identifier.urihttp://hdl.handle.net/11693/50324
dc.language.isoEnglish
dc.publisherSpringer
dc.relation.isversionofhttps://doi.org/10.1140/epjc/s10052-018-6465-x
dc.relation.projectResearch Institute for Astronomy and Astrophysics of Maragha, RIAAM - Research Institute for Astronomy and Astrophysics of Maragha, RIAAM: 1/5237-17
dc.rightsinfo:eu-repo/semantics/openAccess
dc.source.titleEuropean Physical Journal Cen_US
dc.titleSurrounded Bonnor-Vaidya solution by cosmological fieldsen_US
dc.typeArticleen_US

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