Quantum general relativity and Hawking radiation
arXiv:gr-qc/0208083 · doi:10.1103/PhysRevD.67.024014
Abstract
In a previous paper we have set up the Wheeler-DeWitt equation which describes the quantum general relativistic collapse of a spherical dust cloud. In the present paper we specialize this equation to the case of matter perturbations around a black hole, and show that in the WKB approximation, the wave-functional describes an eternal black hole in equilibrium with a thermal bath at Hawking temperature.
13 pages, minor revisions in: (i) para 5 of Introduction, (ii) para following Eqn. (10). Revised version to appear in Phys. Rev. D
References in corpus (4)
Cited by in corpus (19)
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