Hawking radiation of linear dilaton black holes

Simple item page
dc.creatorClement, G.
dc.creatorFabris, J. C.
dc.creatorMarques, G. T.
dc.date2007-04-03
dc.date.accessioned2026-07-07T10:35:25Z
dc.date.available2026-07-07T10:35:25Z
dc.descriptionWe compute exactly the semi-classical radiation spectrum for a class of non-asymptotically flat charged dilaton black holes, the so-called linear dilaton black holes. In the high frequency regime, the temperature for these black holes generically agrees with the surface gravity result. In the special case where the black hole is massless, we show that, although the surface gravity remains finite, there is no radiation, in agreement with the fact that massless objects cannot radiate.
dc.description9 pages
dc.identifierhttps://arxiv.org/abs/0704.0399
dc.identifierhttp://arxiv.org/abs/0704.0399
dc.identifierPhys.Lett.B651:54-57,2007
dc.identifierdoi:10.1016/j.physletb.2007.05.052
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179748
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleHawking radiation of linear dilaton black holes
dc.typetext

Files

Collections

arXiv