Plane Symmetric Inhomogeneous Cosmological Models with a Perfect Fluid in General Relativity

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dc.creatorPradhan, Anirudh
dc.creatorPandey, Purnima
dc.creatorSingh, Sunil Kumar
dc.date2006-10-26
dc.date2007-08-20
dc.date.accessioned2026-07-07T10:41:05Z
dc.date.available2026-07-07T10:41:05Z
dc.descriptionIn this paper we investigate a class of solutions of Einstein equations for the plane-symmetric perfect fluid case with shear and vanishing acceleration. If these solutions have shear, they must necessarily be non-static. We examine the integrable cases of the field equations systematically. Among the cases with shear we find three classes of solutions.
dc.description12 pages, no figures, corrected minor typos
dc.identifierhttps://arxiv.org/abs/gr-qc/0610125
dc.identifierhttp://arxiv.org/abs/gr-qc/0610125
dc.identifierInt.J.Theor.Phys.46:1584-1595,2007
dc.identifierdoi:10.1007/s10773-006-9294-x
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181522
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titlePlane Symmetric Inhomogeneous Cosmological Models with a Perfect Fluid in General Relativity
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