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Please use this identifier to cite or link to this item: http://hdl.handle.net/11129/1969

Title: Entropy Conservation of Linear Dilaton Black Holes in Quantum Corrected Hawking Radiation
Authors: Sakallı, İzzet
Paşaoğlu, Hale
Halilsoy, Mustafa
Keywords: general relativity
black holes
hawking radiation
quantum tunneling
Information loss paradox
Entropy conservation
Parikh-Wilczek’s tunneling method
Quantum gravity effect
Linear dilaton black hole
Issue Date: 2011
Publisher: International Journal of Theoretical Physics, Springer
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).
Series/Report no.: ;International Journal of Theoretical Physics 50 (10): 3212-3224, 2011
Abstract: It 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.
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: 10.1007/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.
URI: http://dx.doi.org/10.1007/s10773-011-0824-9
http://hdl.handle.net/11129/1969
ISSN: 1572-9575 (online)
0020-7748 (print)
Appears in Collections:PHY – Journal Articles: Publisher & Author Versions (Post-Print Author Versions) – Physics

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