UV/IR Mixing and Black Hole Thermodynamics

dc.creatorNozari, Kourosh
dc.creatorFazlpour, Behnaz
dc.date2007-08-09
dc.date.accessioned2026-07-07T11:18:34Z
dc.date.available2026-07-07T11:18:34Z
dc.descriptionThe goal of this paper is to investigate the final stage of black hole evaporation process in the framework of Lorentz violating Modified Dispersion Relations(MDRs). As a consequence of MDRs, the high energy sector of the underlying field theory does not decouple from the low energy sector, the phenomenon which is known as UV/IR mixing. In the absence of exact supersymmetry, we derive a modified dispersion relation which shows UV/IR mixing by a novel energy dependence. Then we investigate the effects of these type of MDRs on the thermodynamics of a radiating noncommutative Schwarzschild black hole. The final stage of black hole evaporation obtained in this framework is compared with existing pictures.
dc.description17 pages, 3 eps figures, accepted for publication in IJMPD
dc.identifierhttps://arxiv.org/abs/0708.1220
dc.identifierhttp://arxiv.org/abs/0708.1220
dc.identifierInt.J.Mod.Phys.D17:55-69,2008
dc.identifierdoi:10.1142/S0218271808011869
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193385
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleUV/IR Mixing and Black Hole Thermodynamics
dc.typetext

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