Spectroscopy of Rindler Modified Schwarzschild Black Hole

dc.contributor.authorSakallı, İzzet
dc.contributor.authorMirekhtiary, Seyedeh Fatemeh
dc.date.accessioned2016-01-11T12:48:17Z
dc.date.available2016-01-11T12:48:17Z
dc.date.issued2014
dc.descriptionThe 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 (with DOI: 10.1007/s10509-013-1776-8) 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.abstractWe study quasinormal modes (QNMs) of uncharged Grumiller black hole (GBH). This massive BH has a Rindler acceleration a, and hence it is also called Rindler modified Schwarzschild BH. After reducing the radial equation of the massless Klein-Gordon equation to the Zerilli equation, we compute the complex frequencies of the QNMs of the GBH. To this end, an approximation method which considers small perturbation around its horizon is used. Considering the highly damped QNMs in the process proposed by Maggiore, the quantum entropy and area spectra of these BHs are found. Although the QNM frequencies are tuned by the Rindler term, we show in detail that the spacing does not depend on it. Here, dimensionless constant {\epsilon} of the area spectrum is found to be double of its Schwarzschild value. The latter result is also discussed.en_US
dc.description.versionPost-Print Author Version (Final Author Manuscript, accepted for publication, after peer-review process).
dc.identifier.citation"Spectroscopy of Rindler Modified Schwarzschild Black Hole", " Izzet Sakalli and Seyedeh Fatemeh Mirekhtiary, Astrophys. Space Sci. 350, 727 (2014).en_US
dc.identifier.doi10.1007/s10509-013-1776-8
dc.identifier.issn1572-946X (online)
dc.identifier.issn0004-640X (print)
dc.identifier.otherDOI: 10.1007/s10509-013-1776-8
dc.identifier.scopus2-s2.0-84896717152
dc.identifier.scopusqualityQ3
dc.identifier.urihttp://dx.doi.org/10.1007/s10509-013-1776-8
dc.identifier.urihttps://hdl.handle.net/11129/1962
dc.identifier.wosWOS:000332664500035
dc.identifier.wosqualityQ3
dc.indekslendigikaynakScopus
dc.indekslendigikaynakWeb of Science
dc.language.isoen
dc.publisherAstrophysics and Space Science, Springeren_US
dc.relation.ispartofseriesSpringer;Astrophys. Space Sci. 350 (2), 727-731 (2014)
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.subjectgeneral relativityen_US
dc.subjectblack holesen_US
dc.subjectSpectroscopyen_US
dc.subjectquasinormal modesen_US
dc.titleSpectroscopy of Rindler Modified Schwarzschild Black Holeen_US
dc.typeArticle

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