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

Anirudh Pradhan·Om Prakash Pandey
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Abstract

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 $Λ$ 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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Anirudh Pradhan, Om Prakash Pandey. 2002-12-28. Bianchi Type I Anisotropic Magnetized Cosmological Models with Varying $Λ$. https://doi.org/10.1142/s0218271803003761

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