The de Broglie-Bohm Interpretation of Evaporating Black-Holes

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dc.creatorde Barros, J. Acacio
dc.creatorOliveira-Neto, G.
dc.creatorVale, T. B.
dc.date2004-04-16
dc.date.accessioned2026-07-07T03:28:36Z
dc.date.available2026-07-07T03:28:36Z
dc.descriptionIn this work we apply the de Broglie-Bohm interpretation of quantum mechanics to the quantized spherically symmetric black-hole coupled to a massless scalar field. The wave-functional used was first obtained by Tomimatsu using the standard ADM quantization and a gauge that places the observer close to the black-hole horizon. Using the causal interpretation, we compute quantum trajectories determined by the initial conditions. We show that the quantum trajectories for the black-hole mass can either increase or decrease with time. The quantum trajectories that show increasing mass represent the usual black-hole behavior of continuous energy absorption. The mass-decreasing quantum trajectories are a purely quantum mechanical phenomena. They can be physically interpreted as describing a black-hole that evaporates.
dc.descriptionRevtex version, 13 pages, no figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0404073
dc.identifierhttp://arxiv.org/abs/gr-qc/0404073
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34894
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe de Broglie-Bohm Interpretation of Evaporating Black-Holes
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