Thermodynamics of a collapsing shell in an expanding Universe

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dc.creatorAlberghi, G. L.
dc.creatorCasadio, R.
dc.creatorVenturi, G.
dc.date2004-09-30
dc.date.accessioned2026-07-07T11:42:58Z
dc.date.available2026-07-07T11:42:58Z
dc.descriptionWe describe the quasi-static collapse of a radiating, spherical shell of matter in de Sitter space-time using a thermodynamical formalism. It is found that the specific heat at constant area and other thermodynamical quantities exhibit singularities related to phase transitions during the collapse.
dc.description9 pages, 2 figures, accepted for publication in Phys. Lett. B
dc.identifierhttps://arxiv.org/abs/gr-qc/0409118
dc.identifierhttp://arxiv.org/abs/gr-qc/0409118
dc.identifierPhys.Lett.B602:8-13,2004
dc.identifierdoi:10.1016/j.physletb.2004.09.063
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/201073
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThermodynamics of a collapsing shell in an expanding Universe
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