Radiation via Tunneling in the Charged BTZ Black Hole

Details Radiation via Tunneling in the Charged BTZ Black Hole Radiation via Tunneling in the Charged BTZ Black Hole

2001-10-30

arxiv.org/abs/hep-th/0110289v4

Class.Quant.Grav. 19 (2002) 589-598

Physics

High Energy Physics

High Energy Physics - Theory

16 pages, Latex; references added and clarity added to some equations and some discussion

Scientific paper

10.1088/0264-9381/19/3/313

It is often convenient to view Hawking (black hole) radiation as a process of quantum tunneling. Within this framework, Kraus and Wilczek (KW) have initiated an analytical treatment of black hole emission. Notably, their methodology incorporates the effects of a dynamical black hole geometry. In the current paper, the KW formalism is applied to the case of a charged BTZ black hole. In the context of this interesting model, we are able to demonstrate a non-thermal spectrum, with the usual Hawking result being reproduced at zeroth order in frequency. Considerable attention is then given to the examination of near-extremal thermodynamics.

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