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arXiv · gr-qc/0502074

Relationship between Hawking Radiation and Gravitational Anomalies

Sean P. Robinson·Frank Wilczek
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Abstract

We show that in order to avoid a breakdown of general covariance at the quantum level the total flux in each outgoing partial wave of a quantum field in a black hole background must be equal to that of a (1+1)-dimensional blackbody at the Hawking temperature.

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Sean P. Robinson, Frank Wilczek. 2005-08-23. Relationship between Hawking Radiation and Gravitational Anomalies. https://doi.org/10.1103/physrevlett.95.011303

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