On the quest for a holographic interpretation of the black hole evaporation process

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dc.creatorCasadio, Roberto
dc.creatorGermani, Cristiano
dc.date2004-03-25
dc.date2004-07-21
dc.date.accessioned2026-07-07T04:16:46Z
dc.date.available2026-07-07T04:16:46Z
dc.descriptionThis paper has been withdrawn by the authors because the Hawking radiation outside the core was just obtained for a specific (and somewhat unphysical) model of the tail. Interested readers should instead look at the more recent hep-th/0407191 where more general results are given for the formation and evolution of black-holes on the brane.
dc.descriptionWithdrawn by authors and replaced by more recent hep-th/0407191
dc.identifierhttps://arxiv.org/abs/hep-th/0403258
dc.identifierhttp://arxiv.org/abs/hep-th/0403258
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/52493
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleOn the quest for a holographic interpretation of the black hole evaporation process
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