Bianchi type VI0 magnetized bulk viscous massive string cosmological model in General Relativity

Details Bianchi type VI0 magnetized bulk viscous massive string cosmological model in General Relativity Bianchi type VI0 magnetized bulk viscous massive string cosmological model in General Relativity

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ap%26ss.317...21b&link_type=abstract

Astrophysics and Space Science, Volume 317, Issue 1-2, pp. 21-26

Astronomy and Astrophysics

Astrophysics

4

Scientific paper

The paper consists of some exact solutions for a homogeneous Bianchi type VI0 universe. The material distribution is taken to be a magnetized bulk viscous fluid in presence of massive cosmological string. We assume that current is flowing along x-direction. Therefore, the magnetic field is in yz-plane. For deterministic model of the universe, we assume that shear ( σ) is proportional to the expansion ( θ) and ζ θ=constant= ξ where ζ the coefficient of bulk viscosity and θ the expansion in the model. The physical and kinematical parameters of the models thus formed are discussed.

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