Entropy Conservation of Linear Dilaton Black Holes in Quantum Corrected Hawking Radiation

dc.contributor.authorSakallı, İzzet
dc.contributor.authorPaşaoğlu, Hale
dc.contributor.authorHalilsoy, Mustafa
dc.date.accessioned2016-01-13T12:54:47Z
dc.date.available2016-01-13T12:54:47Z
dc.date.issued2011
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/s10773-011-0824-9) 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.abstractIt has been shown recently that information is lost in the Hawking radiation of the linear dilaton black holes in various theories when applying the tunneling formulism without considering quantum gravity effects. In this Letter, we recalculate the emission probability by taking into account of the log-area correction to the Bekenstein-Hawking entropy and the statistical correlation between quanta emitted. The crucial role of the black hole remnant on the entropy conservation is highlighted. We model the remnant as a higher dimensional linear dilaton vacuum in order to show that such a remnant model cannot radiate and its temperature would be zero. In addition to this, the entropy conservation in the higher dimensional linear dilaton black holes is also discussed. In summary, we show in detail that the information can also leak out from the linear dilaton black holes together with preserving unitarity in quantum mechanics.en_US
dc.description.versionPost-Print Author Version (Final Author Manuscript, accepted for publication, after peer-review process).
dc.identifier.citation“Entropy Conservation of Linear Dilaton Black Holes in Quantum Corrected Hawking Radiation”, Izzet Sakalli, Mustafa Halilsoy, and Hale Pasaoglu, Int. J. Theo. Phys. 50, 3212 (2011).en_US
dc.identifier.doi10.1007/s10773-011-0824-9
dc.identifier.issn1572-9575 (online)
dc.identifier.issn0020-7748 (print)
dc.identifier.otherDOI: 10.1007/s10773-011-0824-9
dc.identifier.scopus2-s2.0-80052272466
dc.identifier.scopusqualityQ1
dc.identifier.urihttp://dx.doi.org/10.1007/s10773-011-0824-9
dc.identifier.urihttps://hdl.handle.net/11129/1969
dc.identifier.wosWOS:000294500900026
dc.identifier.wosqualityQ3
dc.indekslendigikaynakScopus
dc.indekslendigikaynakWeb of Science
dc.language.isoen
dc.publisherInternational Journal of Theoretical Physics, Springeren_US
dc.relation.ispartofseries;International Journal of Theoretical Physics 50 (10): 3212-3224, 2011
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.subjectgeneral relativityen_US
dc.subjectblack holesen_US
dc.subjecthawking radiationen_US
dc.subjectquantum tunnelingen_US
dc.subjectInformation loss paradoxen_US
dc.subjectEntropy conservationen_US
dc.subjectParikh-Wilczek’s tunneling methoden_US
dc.subjectQuantum gravity effecten_US
dc.subjectLinear dilaton black holeen_US
dc.titleEntropy Conservation of Linear Dilaton Black Holes in Quantum Corrected Hawking Radiationen_US
dc.typeArticle

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