Hawking Radiation via Gravitational Anomalies in Non-spherical Topologies

Abstract

We study the method of calculating the Hawking radiation via gravitational anomalies in gravitational backgrounds of constant negative curvature. We apply the method to topological black holes and also to topological black holes conformally coupled to a scalar field.

25 pages, no figures, version to be published in Phys. Rev. D

References in corpus (10)

• Anomalies, Hawking Radiations and Regularity in Rotating Black Holes
• Hawking Radiation from Charged Black Holes via Gauge and Gravitational Anomalies
• Hawking Radiation from Rotating Black Holes and Gravitational Anomalies
• Hawking Radiation and Covariant Anomalies
• Hawking Radiation, Effective Actions and Covariant Boundary Conditions
• Periodic boundary conditions on the pseudosphere
• Hawking Radiation, Covariant Boundary Conditions and Vacuum States
• Thermodynamical properties of hairy black holes in n spacetimes dimensions
• Covariant Anomalies, Horizons and Hawking Radiation
• Some results on dynamical black holes

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• Anomaly analysis of Hawking radiation from 2+1 dimensional spinning black hole
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