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

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In 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.
12 pages, no figures, corrected minor typos

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General Relativity and Quantum Cosmology

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http://salesiana.dossiersoluciones.com/handle/123456789/181522

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/gr-qc/0610125
 http://arxiv.org/abs/gr-qc/0610125
 Int.J.Theor.Phys.46:1584-1595,2007
 doi:10.1007/s10773-006-9294-x

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arXiv