Semiclassical Quantization on Black Hole Spacetimes

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dc.creatorCasadio, R.
dc.creatorHarms, B.
dc.creatorLeblanc, Y.
dc.date1997-11-07
dc.date.accessioned2026-07-07T03:31:58Z
dc.date.available2026-07-07T03:31:58Z
dc.descriptionThe thermodynamical description of black holes is reviewed and critiqued. We present an alternative, microcanonical description of black holes and discuss the major differences. In particular the decay rates of black holes are compared in the two different pictures.
dc.description3 pages, mprocl.sty, To appear in the proceedings of the 8th Marcel Grossmann Meeting
dc.identifierhttps://arxiv.org/abs/gr-qc/9711029
dc.identifierhttp://arxiv.org/abs/gr-qc/9711029
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36060
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleSemiclassical Quantization on Black Hole Spacetimes
dc.typetext

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