Hawking Radiation from General Kerr-(anti)de Sitter Black Holes
نویسندگان
چکیده
We calculate the total flux of Hawking radiation from Kerr-(anti)de Sitter black holes by using gravitational anomaly method developed in [6]. We consider the general Kerr(anti)de Sitter black holes in arbitrary D dimensions with the maximal number [D/2] of independent rotating parameters. We find that the physics near the horizon can be described by an infinite collection of (1 + 1)-dimensional quantum fields coupled to a set of gauge fields with charges proportional to the azimuthal angular momentums mi. With the requirement of anomaly cancellation and regularity at the horizon, the Hawking radiation is determined. Email:[email protected] Email:[email protected]
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