Are Extremal 2D Black Holes Really Frozen ?

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dc.creatorVagenas, Elias C.
dc.date2000-12-15
dc.date2001-02-23
dc.date.accessioned2026-07-07T12:03:36Z
dc.date.available2026-07-07T12:03:36Z
dc.descriptionIn the standard methodology for evaluating the Hawking radiation emanating from a black hole, the background geometry is fixed. Trying to be more realistic we consider a dynamical geometry for a two-dimensional charged black hole and we evaluate the Hawking radiation as tunneling process. This modification to the geometry gives rise to a nonthermal part in the radiation spectrum. We explore the consequences of this new term for the extremal case.
dc.description7 pages, LaTeX, no figures
dc.identifierhttps://arxiv.org/abs/hep-th/0012134
dc.identifierhttp://arxiv.org/abs/hep-th/0012134
dc.identifierPhys.Lett.B503:399-403,2001
dc.identifierdoi:10.1016/S0370-2693(01)00242-8
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/207843
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleAre Extremal 2D Black Holes Really Frozen ?
dc.typetext

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