Singularities in separable metrics with spherical, plane, and hyperbolic symmetry.

Physics

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General Relativity

Scientific paper

We obtain all possible solutions to the Einstein equations for a perfect fluid with a metric of the form ds^2 = - w^2 (x)v^2 (t)dt^2 + g^2 (t)S^2 (x)dx^2 + A^2 (t)B^2 (x)[d which obey the weak and strong energy conditions and do not contain scalar polynomial singularities on surfacesx = const. We show that the only nonstatic solutions satisfying these conditions are the Robertson-Walker spacetimes, spacetimes withw = S = B = 1, and a class of plane symmetric solutions.

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