Gravitational anomalies: a recipe for Hawking radiation
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Date
2016-01-07
Authors
Das, Saurya
Robinson, Sean P.
Vagenas, Elias C.
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Abstract
We explore the method of Robinson andWilczek 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 cases of charged and rotating black holes, the expected
super-radiant current is also reproduced.
Description
Sherpa Romeo yellow journal. Preprint of an article published in International Journal of Modern Physics D © World Scientific Publishing Company https://www.worldscientific.com/worldscinet/ijmpd
Keywords
Hawking temperature , Gravitational anomaly , Black holes , Hawking radiation
Citation
Das, S., Robinson, S. P., & Vagenas, E. C. (2008). Gravitational anaomalies: A recipe for Hawking radiation. International Journal of Modern Physics D, 17(03-04), 533-539. https://doi.org/10.1142/S0218271808012218