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arXiv · 0705.2233

Gravitational anomalies: a recipe for Hawking radiation

Saurya Das·Sean P. Robinson·Elias C. Vagenas
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Abstract

We explore the method of Robinson and Wilczek for deriving the Hawking temperature of a black hole. In this method, the Hawking radiation restores general covariance in an effective theory of near-horizon physics which otherwise exhibits a gravitational anomaly at the quantum level. The method has been shown to work for broad classes of black holes in arbitrary spacetime dimensions. These include static black holes, accreting or evaporating black holes, charged black holes, rotating black holes, and even black rings. In the case of charged and rotating black holes, the expected super-radiant current is also reproduced.

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Saurya Das, Sean P. Robinson, Elias C. Vagenas. 2008-03-27. Gravitational anomalies: a recipe for Hawking radiation. https://doi.org/10.1142/s0218271808012218

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