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Bianchi Type-VI0 Inhomogeneous Cosmological Model for Stiff Perfect Fluid Distribution in General Relativity

Atul Tyagi, Barkha R. Tripathi


In this paper, we have investigated an inhomogeneous Bianchi type VI0 cosmological model for stiff perfect fluid distribution in general relativity. To obtain the deterministic solution of Einstein’s field equations, we assume that the isotropic pressure is equal to rest density i.e. p = ρ. Some physical and geometric aspects of the models are also discussed.

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