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Evaporating Black Holes And An Entropic Scale-Hierarchy

Hadi Salehi
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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.

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Hadi Salehi. 1994-09-12. Evaporating Black Holes And An Entropic Scale-Hierarchy. https://arxiv.org/abs/gr-qc/9409023

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