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

Abstract

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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