Quasinormal modes of charged dilaton black holes and their entropy spectra

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dc.contributor.author Sakallı, İzzet
dc.date.accessioned 2016-01-12T15:37:09Z
dc.date.available 2016-01-12T15:37:09Z
dc.date.issued 2013
dc.identifier.citation “Quasinormal Modes of Charged Dilaton Black Holes and Their Entropy Spectra”, Izzet Sakalli, Mod. Phys. Lett. A 28, 1350109 (2013). en_US
dc.identifier.issn 0217-7323
dc.identifier.other DOI: 10.1142/S0217732313501095
dc.identifier.uri http://dx.doi.org/10.1142/S0217732313501095
dc.identifier.uri http://hdl.handle.net/11129/1965
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 (with DOI: 10.1142/S0217732313501095) 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 In this study, we employ the scalar perturbations of the charged dilaton black hole (CDBH) found by Chan, Horne and Mann (CHM), and described with an action which emerges in the low-energy limit of the string theory. A CDBH is neither asymptotically flat (AF) nor non-asymptotically flat (NAF) spacetime. Depending on the value of its dilaton parameter "a", it has both Schwarzschild and linear dilaton black hole (LDBH) limits. We compute the complex frequencies of the quasinormal modes (QNMs) of the CDBH by considering small perturbations around its horizon. By using the highly damped QNMs in the process prescribed by Maggiore, we obtain the quantum entropy and area spectra of these BHs. Although the QNM frequencies are tuned by "a", we show that the quantum spectra do not depend on "a", and they are equally spaced. On the other hand, the obtained value of undetermined dimensionless constant {\epsilon} is the double of Bekenstein's result. The possible reason of this discrepancy is also discussed. en_US
dc.language.iso en_US en_US
dc.publisher Modern Physics Letters A, World Scientific Publishing en_US
dc.relation.ispartofseries World Scientific;Modern Physics Letters A, 2013, vol. 28, issue 27, p 1,
dc.subject general relativity en_US
dc.subject black holes en_US
dc.subject entropy spectra en_US
dc.subject Quasinormal modes en_US
dc.subject General Relativity and Quantum Cosmology en_US
dc.title Quasinormal modes of charged dilaton black holes and their entropy spectra en_US
dc.type Article en_US
dc.description.version Post-Print Author Version; (Final Author Manuscript, accepted for publication, after peer-review process).


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