Exact scalar quasibound states solutions of f(R) theory's static spherically symmetric black hole

dc.contributor.authorSenjaya D.
dc.contributor.correspondenceSenjaya D.
dc.contributor.otherMahidol University
dc.date.accessioned2024-02-21T18:11:13Z
dc.date.available2024-02-21T18:11:13Z
dc.date.issued2024-03-01
dc.description.abstractFollowing the recent developments in black holes' quasibound states exact solutions by Senjaya (2023b,c), in this letter, we present a novel exact solution of quasibound states of a scalar around a static spherically symmetric black hole solution of f(R) theory of gravity. We start with the relativistic scalar field wave equation, i.e. the Klein-Gordon equation, isolating the radial equation and finally successfully obtain the exact radial wave solutions in terms of General Heun functions. Having the exact solutions in hand, the energy levels expression is obtained from the radial wave polynomial conditions. In the last part of this letter, the Hawking radiation is investigated via the Damour-Ruffini method and the Hawking temperature is obtained from radiation distribution function.
dc.identifier.citationJournal of High Energy Astrophysics Vol.41 (2024) , 61-66
dc.identifier.doi10.1016/j.jheap.2024.01.004
dc.identifier.issn22144048
dc.identifier.scopus2-s2.0-85184906799
dc.identifier.urihttps://repository.li.mahidol.ac.th/handle/20.500.14594/97293
dc.rights.holderSCOPUS
dc.subjectPhysics and Astronomy
dc.titleExact scalar quasibound states solutions of f(R) theory's static spherically symmetric black hole
dc.typeArticle
mu.datasource.scopushttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85184906799&origin=inward
oaire.citation.endPage66
oaire.citation.startPage61
oaire.citation.titleJournal of High Energy Astrophysics
oaire.citation.volume41
oairecerif.author.affiliationMahidol University

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