Abstract
We investigate a class of solutions of Einstein equations for the plane symmetric perfect fluid case. If these solutions have shear, they must necessarily be non-static. Some physical and geometric properties of the models are also discussed.
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Pradhan, A., Rai, A. Plane symmetric inhomogeneous cosmological models with a perfect fluid in General Relativity II. Astrophys Space Sci 314, 225–229 (2008). https://doi.org/10.1007/s10509-008-9763-1
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DOI: https://doi.org/10.1007/s10509-008-9763-1