A Non-Static Magnetohydrodynamic Universe in General Relativity

Vol-3 | Issue-06 | June 2018 | Published Online: 19 June 2018    PDF ( 208 KB )
Author(s)
Dr. Sunil Kumar 1

1Assistant Teacher Rashtriya Inter School, Daudnagar, Aurangabad (Bihar)

Abstract

In this paper we have discussed Bianchi type-I cosmological model with perfect fluid and electromagnetic, field. Taking a suitable metric we have also calculated various physical and geometrical properties e.g. pressure, density, scalar of expansion and components of shear tensor. We have also discussed behaviour of a test particle and Doppler’s Effect in the model.

Keywords
Model, test particle, Universe pressure, density
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