Bianchi Type-I cosmological model in Einstein–Cartan theory

Abstract

In this paper, we obtain a solution of Bianchi Type-I cosmological model using Einstein–Cartan theory for perfect fluid distribution with the improved stress–energy–momentum tensor of Ray and Smalley. Here, we use a special law of variation for Hubble's parameter proposed by Bermann (Nuovo Cim B 74:182, 1983). Some physical behaviours of the cosmological model are also studied.

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