Remarks on Hawking radiation as tunneling from the BTZ black holes | Zendy

ShuangQing Wu | Zendy; Qing-Quan Jiang | Zendy

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Remarks on Hawking radiation as tunneling from the BTZ black holes

Author(s) -

ShuangQing Wu,

Qing-Quan Jiang

Publication year - 2006

Publication title -

journal of high energy physics

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 0.998

H-Index - 261

eISSN - 1126-6708

pISSN - 1029-8479

DOI - 10.1088/1126-6708/2006/03/079

Subject(s) - hawking radiation , physics , btz black hole , event horizon , micro black hole , semiclassical physics , black hole thermodynamics , black hole (networking) , black hole information paradox , quantum tunnelling , angular momentum , hawking , entropy (arrow of time) , quantum mechanics , quantum electrodynamics , classical mechanics , quantum , event (particle physics) , de sitter–schwarzschild metric , computer network , routing protocol , routing (electronic design automation) , computer science , link state routing protocol

Hawking radiation viewed as a semiclassical tunneling process from the eventhorizon of the (2 + 1)-dimensional rotating BTZ black hole is carefullyreexamined by taking into account not only the energy conservation but also theconservation of angular momentum when the effect of the emitted particle'sself-gravitation is incorporated. In contrast to previous analysis of thisissue in the literature, our result obtained here fits well to theKraus-Parikh-Wilczek's universal conclusion without any modification to theBekenstein-Hawking area-entropy formulae of the BTZ black hole.Comment: 12pages, no figure, use JHEP3.cls. Version better than published one in JHE

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