Uniqueness of the non-singular family and characterisation of cosmological models

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We prove that for an orthogonal spacetime metric separable in space and time in comoving coordinates, the requirements of perfect fluid and non-singularity single out the unique family of singularity free cosmological models. Further homogeneous models could only be Bianchi I or FLRW while inhomogeneous ones can be with or without a singularity.
TeX pages 13, IUCAA-14/94

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