Relationship between Hawking Radiation and Gravitational Anomalies

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.

5 pages, 1 figure; v2: typo corrected, reference added; v3: comment added, minor editorial changes to agree with published version

Cited by in corpus (231)

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