Bogoliubov Coefficients of 2D Charged Black Holes

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dc.creatorChristodoulakis, T.
dc.creatorDiamandis, G. A.
dc.creatorGeorgalas, B. C.
dc.creatorVagenas, E. C.
dc.date2000-10-12
dc.date.accessioned2026-07-07T12:03:36Z
dc.date.available2026-07-07T12:03:36Z
dc.descriptionWe exactly calculate the thermal distribution and temperature of Hawking radiation for a two-dimensional charged dilatonic black hole after it has settled down to an "equilibrium" state. The calculation is carried out using the Bogoliubov coefficients. The background of the process is furnished by a preexisting black hole and not by collapsing matter as considered by Giddings and Nelson for the case of a Schwarzschild black hole. Furthermore, the vanishing of the temperature and/or the Hawking radiation in the extremal case is obtained as a regular limit of the general case.
dc.description9 pages, 1 eps figure
dc.identifierhttps://arxiv.org/abs/hep-th/0010097
dc.identifierhttp://arxiv.org/abs/hep-th/0010097
dc.identifierPhys.Lett.B501:269-276,2001
dc.identifierdoi:10.1016/S0370-2693(01)00118-6
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/207841
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBogoliubov Coefficients of 2D Charged Black Holes
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