Evaporating Black Holes And An Entropic Scale-Hierarchy

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It is argued that a characteristic length may be associated with the entropic state of a spherically symmetric black hole in the cosmological context. This length is much smaller than the Schwarzschild-radius of a black hole and may act as a regulator of arbitrarily high frequencies apparently entering the usual derivation of Hawking's radiation.
7 pages, Latex, (ISTPM) IPM-94-055

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General Relativity and Quantum Cosmology

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http://salesiana.dossiersoluciones.com/handle/123456789/35533

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/gr-qc/9409023
 http://arxiv.org/abs/gr-qc/9409023

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arXiv