Geodesic
Hawking radiation as tunneling with back-reaction for the Kerr–anti-de Sitter black hole
Teoretičeskaâ i matematičeskaâ fizika, Tome 161 (2009) no. 1, pp. 136-144 Cet article a éte moissonné depuis la source Math-Net.Ru

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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.
Keywords: covariant result, energy conservation, angular momentum conservation, back-reaction. 
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     journal = {Teoreti\v{c}eska\^a i matemati\v{c}eska\^a fizika},
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Hui-Ling Li; Rong Lin; Teng-Jiao Zhou; Tao Huang. Hawking radiation as tunneling with back-reaction for the Kerr–anti-de Sitter black hole. Teoretičeskaâ i matematičeskaâ fizika, Tome 161 (2009) no. 1, pp. 136-144. http://geodesic.mathdoc.fr/item/TMF_2009_161_1_a11/

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