Evaporating Black Holes And An Entropic Scale-Hierarchy
General Relativity and Quantum Cosmology
2007-05-23 v1
Abstract
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.
Keywords
Cite
@article{arxiv.gr-qc/9409023,
title = {Evaporating Black Holes And An Entropic Scale-Hierarchy},
author = {Hadi Salehi},
journal= {arXiv preprint arXiv:gr-qc/9409023},
year = {2007}
}
Comments
7 pages, Latex, (ISTPM) IPM-94-055