Bianchi Type I Anisotropic Magnetized Cosmological Models with Varying $Λ$

Details Bianchi Type I Anisotropic Magnetized Cosmological Models with Varying $Λ$ Bianchi Type I Anisotropic Magnetized Cosmological Models with Varying $Λ$

2002-12-26

arxiv.org/abs/gr-qc/0212109v2

Int.J.Mod.Phys. D12 (2003) 1299-1314

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

16 pages

Scientific paper

10.1142/S0218271803003761

Bianchi type I magnetized cosmological models in the presence of a bulk viscous fluid are investigated. The source of the magnetic field is due to an electric current produced along x-axis. The distribution consists of an electrically neutral viscous fluid with an infinite electrical conductivity. The coefficient of bulk viscosity is assumed to be a power function of mass density. The cosmological constant $\Lambda$ is found to be positive and is a decreasing function of time which is supported by results from recent supernovae observations. The behaviour of the models in presence and absence of magnetic field are also discussed.

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