Black hole radiation of massive spin-2 particles in (3+1) dimensions


Show simple item record Sakallı, İzzet Övgün, Ali 2016-06-07T13:06:52Z 2016-06-07T13:06:52Z 2016-06-03
dc.identifier.issn 2190-5444
dc.description The file in this item is the post-print version of the article (author’s copy; author’s final manuscript, accepted for publication after peer-review process). Due to copyright restrictions, the access to the publisher version (published version) of this article is only available via subscription. You may click URI and have access to the Publisher Version of this article through the publisher web site or online databases, if your Library or institution has subscription to the related journal or publication. en_US
dc.description.abstract This paper is devoted to the study of radiation of massive spin-2 boson (graviton with a nonzero mass) through the event horizon of a generic static and spherically symmetric black hole in (3+1) dimensions. To this end, we consider the problem in the framework of quantum tunneling phenomenon. We evaluate the tunneling rate of the massive gravitons by applying the semiclassical WKB approximation to the Fierz-Pauli equation. The temperature of the radiation is obtained with the aid of the Boltzmann expression. Our findings are in good agreement with the existing Hawking radiation studies in the current literature. en_US
dc.language.iso eng en_US
dc.publisher Springer en_US
dc.relation.isversionof 10.1140/epjp/i2016-16184-5 en_US
dc.rights info:eu-repo/semantics/openAccess en_US
dc.subject gravitation, general relativity ,hawking radiation, Black Holes, spin-2 particles, graviton, quantum tunneling en_US
dc.title Black hole radiation of massive spin-2 particles in (3+1) dimensions en_US
dc.type article en_US
dc.relation.journal The European Physical Journal Plus en_US
dc.contributor.department Eastern Mediterranean University, Faculty of Arts and Sciences, Physics Department en_US
dc.identifier.volume 131 en_US
dc.identifier.startpage 184 en_US

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