Bianchi Type I Magnetofluid Cosmological Models with Variable Cosmological Constant Revisited

Details Bianchi Type I Magnetofluid Cosmological Models with Variable Cosmological Constant Revisited Bianchi Type I Magnetofluid Cosmological Models with Variable Cosmological Constant Revisited

2003-07-11

arxiv.org/abs/gr-qc/0307058v1

Int.J.Mod.Phys. D13 (2004) 503-516

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

13 pages

Scientific paper

10.1142/S0218271804004736

The behaviour of magnetic field in anisotropic Bianchi type I cosmological model for bulk viscous distribution is investigated. The distribution consists of an electrically neutral viscous fluid with an infinite electrical conductivity. It is assumed that the component $\sigma^{1}_{1}$ of shear tensor $\sigma^{j}_{i}$ is proportional to expansion ($\theta$) and the coefficient of bulk viscosity is assumed to be a power function of mass density. Some physical and geometrical aspects of the models are also discussed in presence and also in absence of the magnetic field.

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