Hawking Radiation of Mass Generating Particles From Dyonic Reissner Nordström Black Hole

EMU I-REP

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dc.contributor.author Sakallı, İzzet
dc.contributor.author Övgün, Ali
dc.date.accessioned 2016-10-25T19:06:26Z
dc.date.available 2016-10-25T19:06:26Z
dc.date.issued 2016-08-20
dc.identifier.issn 0250-6335 (print)
dc.identifier.issn 0973-7758 (online)
dc.identifier.uri http://dx.doi.org/10.1007/s12036-016-9397-6
dc.identifier.uri http://hdl.handle.net/11129/3048
dc.description The file in this item is the publisher version (published version) of the article. en_US
dc.description.abstract The Hawking radiation is considered as a quantum tunneling process, which can be studied in the framework of the Hamilton–Jacobi method. In this study, we present the wave equation for a mass generating massive and charged scalar particle (boson). In sequel, we analyse the quantum tunneling of these bosons from a generic 4-dimensional spherically symmetric black hole. We apply the Hamilton–Jacobi formalism to derive the radial integral solution for the classically forbidden action which leads to the tunneling probability. To support our arguments, we take the dyonic Reissner–Nordström black hole as a test background. Comparing the tunneling probability obtained with the Boltzmann formula, we succeed in reading the standard Hawking temperature of the dyonic Reissner–Nordström black hole. en_US
dc.language.iso eng en_US
dc.publisher Springer en_US
dc.relation.isversionof 10.1007/s12036-016-9397-6 en_US
dc.rights info:eu-repo/semantics/openAccess en_US
dc.subject Hawking radiation en_US
dc.subject quantum tunneling en_US
dc.subject dyonic black holes en_US
dc.subject mass generation en_US
dc.title Hawking Radiation of Mass Generating Particles From Dyonic Reissner Nordström Black Hole en_US
dc.type article en_US
dc.relation.journal Journal of Astrophysics and Astronomy en_US
dc.contributor.department Eastern Mediterranean University, Faculty of Arts and Sciences, Department of Physics and Chemistry en_US
dc.identifier.volume 37 en_US
dc.identifier.issue 21 en_US


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