Black Hole Evaporation in 1+1 Dimensions

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dc.creatorRusso, J.
dc.creatorSusskind, L.
dc.creatorThorlacius, L.
dc.date1992-01-29
dc.date.accessioned2026-07-07T11:48:06Z
dc.date.available2026-07-07T11:48:06Z
dc.descriptionThe formation and quantum mechanical evaporation of black holes in two spacetime dimensions can be studied using effective classical field equations, recently introduced by Callan {\it et al.} We find that gravitational collapse always leads to a curvature singularity, according to these equations, and that the region where the quantum corrections introduced by Callan {\it et al.} could be expected to dominate is on the unphysical side of the singularity. The model can be successfully applied to study the back-reaction of Hawking radiation on the geometry of large mass black holes, but the description breaks down before the evaporation is complete.
dc.description10 pages
dc.identifierhttps://arxiv.org/abs/hep-th/9201074
dc.identifierhttp://arxiv.org/abs/hep-th/9201074
dc.identifierPhys.Lett.B292:13-18,1992
dc.identifierdoi:10.1016/0370-2693(92)90601-Y
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202803
dc.subjectHigh Energy Physics - Theory
dc.titleBlack Hole Evaporation in 1+1 Dimensions
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