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Hawking radiation as tunneling with back-reaction for the Kerr-anti-de Sitter black hole. (English. Russian original) Zbl 1180.83059

Theor. Math. Phys. 161, No. 1, 1438-1444 (2009); translation from Teor. Mat. Fiz. 161, No. 1, 136-144 (2009).
Summary: Medved and Vagenas demonstrated how the Angheben-Nadalini-Vanzo-Zerbini analysis can be adapted in describing the effects of the gravitational back-reaction for the generic spherically symmetric black hole. We extend the Medved-Vagenas quantum tunneling method to the case of the stationary axisymmetric Kerr black hole in anti-de Sitter space-times. We find a correction to the Hawking radiation by considering the effects of the gravitational back-reaction and also energy conservation and angular momentum conservation.

MSC:

83C57 Black holes
83C47 Methods of quantum field theory in general relativity and gravitational theory
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