Stability of Chaplygin gas thin-shell wormholes

dc.creatorEiroa, Ernesto F.
dc.creatorSimeone, Claudio
dc.date2007-04-09
dc.date2007-06-13
dc.date.accessioned2026-07-07T11:20:12Z
dc.date.available2026-07-07T11:20:12Z
dc.descriptionIn this paper we construct spherical thin-shell wormholes supported by a Chaplygin gas. For a rather general class of geometries we introduce a new approach for the stability analysis of static solutions under perturbations preserving the symmetry. We apply this to wormholes constructed from Schwarzschild, Schwarzschild-de Sitter, Schwarzschild-anti de Sitter and Reissner-Nordstrom metrics. In the last two cases, we find that there are values of the parameters for which stable static solutions exist.
dc.description14 pages, 5 figures; v2: minor changes and new references added. Accepted for publication in Physical Review D
dc.identifierhttps://arxiv.org/abs/0704.1136
dc.identifierhttp://arxiv.org/abs/0704.1136
dc.identifierPhys.Rev.D76:024021,2007
dc.identifierdoi:10.1103/PhysRevD.76.024021
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193888
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleStability of Chaplygin gas thin-shell wormholes
dc.typetext

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