Hawking Radiation via Gravitational Anomalies in Non-spherical Topologies
arXiv:0812.1759 · doi:10.1103/PhysRevD.79.084022
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.
arXiv comment25 pages, no figures, version to be published in Phys. Rev. D
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