Abstract
The question of cosmological homogeneity was earlier studied from the physical point of view, the consideration being limited to the case where the velocity vector is orthogonal to the pressure constant hypersurfaces. The present paper extends the investigation where this condition may not hold true. However the proof of homogeneity requires the introduction of some additional assumptions.
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References
Raychaudhuri A K and Modak B 1985Phys. Rev. D31 1807
Eisenhart L P 1945Riemannian geometry (Princeton: University Press)
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Modak, B. Physical approach to cosmological homogeneity II. Pramana - J. Phys. 26, 499–504 (1986). https://doi.org/10.1007/BF02880909
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DOI: https://doi.org/10.1007/BF02880909