Vacuum shell in the Schwarzschild-de Sitter world

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dc.creatorChernov, S. V.
dc.creatorDokuchaev, V. I.
dc.date2007-09-05
dc.date.accessioned2026-07-07T11:19:06Z
dc.date.available2026-07-07T11:19:06Z
dc.descriptionWe construct the classification scheme for all possible evolution scenarios and find the corresponding global geometries for dynamics of a thin spherical vacuum shell in the Schwarzschild-de Sitter metric. This configuration is suitable for the modelling of vacuum bubbles arising during cosmological phase transitions in the early Universe. The distinctive final types of evolution from the local point of view of a rather distant observer are either the unlimited expansion of the shell or its contraction with a formation of black hole (with a central singularity) or wormhole (with a baby universe in interior).
dc.description15 pages, 8 figures
dc.identifierhttps://arxiv.org/abs/0709.0616
dc.identifierhttp://arxiv.org/abs/0709.0616
dc.identifierClass.Quant.Grav.25:015004,2008
dc.identifierdoi:10.1088/0264-9381/25/1/015004
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193570
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleVacuum shell in the Schwarzschild-de Sitter world
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