arXiv · hep-th/0602146
Hawking Radiation from Charged Black Holes via Gauge and Gravitational Anomalies
Abstract
Extending gr-qc/0502074, 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-Nordstrom black hole background must be equal to that of a (1+1) dimensional blackbody at the Hawking temperature with the appropriate chemical potential.
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Satoshi Iso, Hiroshi Umetsu, Frank Wilczek. 2006-06-05. Hawking Radiation from Charged Black Holes via Gauge and Gravitational Anomalies. https://doi.org/10.1103/physrevlett.96.151302
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