Quantum-Corrected Black Hole Thermodynamics in Extra Dimensions

dc.creatorNozari, Kourosh
dc.creatorMehdipour, S. Hamid
dc.date2005-11-19
dc.date2006-01-24
dc.date.accessioned2026-07-07T11:26:19Z
dc.date.available2026-07-07T11:26:19Z
dc.descriptionBekenstein-Hawking formalism of black hole thermodynamics should be modified to incorporate quantum gravitational effects. Generalized Uncertainty Principle(GUP) provides a suitable framework to perform such modifications. In this paper, we consider a general form of GUP to find black hole thermodynamics in a model universe with large extra dimensions. We will show that black holes radiate mainly in the four-dimensional brane. Existence of black holes remnants as a possible candidate for dark matter is discussed.
dc.description19 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0511110
dc.identifierhttp://arxiv.org/abs/gr-qc/0511110
dc.identifierInt.J.Mod.Phys.A21:4979-4992,2006
dc.identifierdoi:10.1142/S0217751X06031570
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/195788
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleQuantum-Corrected Black Hole Thermodynamics in Extra Dimensions
dc.typetext

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