Quantum Bound States Around Black Holes

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dc.creatorGrain, J.
dc.creatorBarrau, A.
dc.date2007-01-29
dc.date2007-12-19
dc.date.accessioned2026-07-07T11:44:02Z
dc.date.available2026-07-07T11:44:02Z
dc.descriptionQuantum mechanics around black holes has shown to be one of the most fascinating fields of theoretical physics. It involves both general relativity and particle physics, opening new eras to establish the principles of unified theories. In this article, we show that quantum bound states with no classical equivalent -- as it can easily be seen at the dominant monopolar order -- should be formed around black holes for massive scalar particles. We qualitatively investigate some important physical consequences, in particular for the Hawking evaporation mechanism and the associated greybody factors.
dc.description5 pages, 6 figures
dc.identifierhttps://arxiv.org/abs/hep-th/0701265
dc.identifierhttp://arxiv.org/abs/hep-th/0701265
dc.identifierEur.Phys.J.C53:641-648,2008
dc.identifierdoi:10.1140/epjc/s10052-007-0494-1
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/201460
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectQuantum Physics
dc.titleQuantum Bound States Around Black Holes
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