Evaporating Black Holes And An Entropic Scale-Hierarchy

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dc.creatorSalehi, Hadi
dc.date1994-09-12
dc.date.accessioned2026-07-07T03:30:26Z
dc.date.available2026-07-07T03:30:26Z
dc.descriptionIt 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.
dc.description7 pages, Latex, (ISTPM) IPM-94-055
dc.identifierhttps://arxiv.org/abs/gr-qc/9409023
dc.identifierhttp://arxiv.org/abs/gr-qc/9409023
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35533
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleEvaporating Black Holes And An Entropic Scale-Hierarchy
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