Thermodynamics of an Evaporating Schwarzschild Black Hole in Noncommutative Space

Simple item page
dc.creatorNozari, Kourosh
dc.creatorFazlpour, Behnaz
dc.date2006-05-11
dc.date2007-01-14
dc.date.accessioned2026-07-07T11:27:28Z
dc.date.available2026-07-07T11:27:28Z
dc.descriptionWe investigate the effects of space noncommutativity and the generalized uncertainty principle on the thermodynamics of a radiating Schwarzschild black hole. We show that evaporation process is in such a way that black hole reaches to a maximum temperature before its final stage of evolution and then cools down to a nonsingular remnant with zero temperature and entropy. We compare our results with more reliable results of string theory. This comparison Shows that GUP and space noncommutativity are similar concepts at least from view point of black hole thermodynamics.
dc.description15 Pages, 2 Figures, revised and refernces added
dc.identifierhttps://arxiv.org/abs/hep-th/0605109
dc.identifierhttp://arxiv.org/abs/hep-th/0605109
dc.identifierMod.Phys.Lett.A22:2917-2930,2007
dc.identifierdoi:10.1142/S0217732307023602
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196158
dc.subjectHigh Energy Physics - Theory
dc.titleThermodynamics of an Evaporating Schwarzschild Black Hole in Noncommutative Space
dc.typetext

Files

Collections

arXiv