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Hawking radiation from charged black holes via gauge and gravitational anomalies
Satoshi Iso ; Hiroshi Umetsu ; Frank Wilczek ;
Date:	21 Apr 2006
Journal:	Phys Rev Lett, 96 (15), 151302
Abstract:	Extending the method of Robinson and Wolczek, we show that in order to avoid a breakdown of general covariance and gauge invariance at the quantum level the total flux of charge and energy in each outgoing partial wave of a charged quantum field in a Reissner-Nordström black hole background must be equal to that of a (1 + 1)-dimensional blackbody at the Hawking temperature with the appropriate chemical potential.
Source:	PubMed, pmid16712145
Other source:	[GID 925677] hep-th/0602146
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