Thermodynamics for radiating shells in anti-de Sitter space-time

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dc.creatorAlberghi, G. L.
dc.creatorCasadio, R.
dc.creatorVenturi, G.
dc.date2003-02-11
dc.date.accessioned2026-07-07T11:46:19Z
dc.date.available2026-07-07T11:46:19Z
dc.descriptionA thermodynamical description for the quasi-static collapse of radiating, self-gravitating spherical shells of matter in anti-de Sitter space-time is obtained. It is shown that the specific heat at constant area and other thermodynamical quantities may diverge before a black hole has eventually formed. This suggests the possibility of a phase transition occurring along the collapse process. The differences with respect to the asymptotically flat case are also highlighted.
dc.description9 pages, 2 figures, PLB style
dc.identifierhttps://arxiv.org/abs/gr-qc/0302038
dc.identifierhttp://arxiv.org/abs/gr-qc/0302038
dc.identifierPhys.Lett.B557:7-11,2003
dc.identifierdoi:10.1016/S0370-2693(03)00185-0
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202186
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleThermodynamics for radiating shells in anti-de Sitter space-time
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