Evaporation of charged black holes near extremality

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dc.creatorFabbri, A.
dc.creatorNavarro, D. J.
dc.creatorNavarro-Salas, J.
dc.date2000-12-04
dc.date.accessioned2026-07-07T04:11:04Z
dc.date.available2026-07-07T04:11:04Z
dc.descriptionThe AdS_2\timesS^2 geometry of near-extremal Reissner-Nordstrom black holes can be described by an effective solvable model which allows to follow analytically the evaporation process including the backreaction. We find that an infinite amount of time is required for the black hole to decay to extremality.
dc.descriptionLaTeX file, 3 pages. Talk given at the Ninth Marcel Grossmann Meeting
dc.identifierhttps://arxiv.org/abs/hep-th/0012019
dc.identifierhttp://arxiv.org/abs/hep-th/0012019
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/50437
dc.subjectHigh Energy Physics - Theory
dc.titleEvaporation of charged black holes near extremality
dc.typetext

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