Quantum tunneling from rotating black holes with scalar hair in three dimensions

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dc.contributor.authorSakalli, I.
dc.contributor.authorGursel, H.
dc.date.accessioned2026-02-06T18:51:18Z
dc.date.issued2016
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractWe study the Hawking radiation of scalar and Dirac particles (fermions) emitted from a rotating scalar hair black hole (RSHBH) within the context of three dimensional (3D) Einstein gravity using non-minimally coupled scalar field theory. Amalgamating the quantum tunneling approach with the Wentzel-Kramers-Brillouin approximation, we obtain the tunneling rates of the outgoing particles across the event horizon. Inserting the resultant tunneling rates into the Boltzmann formula, we then obtain the Hawking temperature (T-H) of the 3D RSHBH.
dc.description.sponsorshipSCOAP3
dc.description.sponsorshipFunded by SCOAP3.
dc.identifier.doi10.1140/epjc/s10052-016-4158-x
dc.identifier.issn1434-6044
dc.identifier.issn1434-6052
dc.identifier.issue6
dc.identifier.orcid0000-0001-7827-9476
dc.identifier.orcid0000-0002-6531-5156
dc.identifier.scopus2-s2.0-84976406340
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1140/epjc/s10052-016-4158-x
dc.identifier.urihttps://hdl.handle.net/11129/15276
dc.identifier.volume76
dc.identifier.wosWOS:000383793300001
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherSpringer
dc.relation.ispartofEuropean Physical Journal C
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20260204
dc.subjectGravity
dc.subjectScattering
dc.subjectAmplitudes
dc.titleQuantum tunneling from rotating black holes with scalar hair in three dimensions
dc.typeArticle

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