Dynamics of a magnetized Bianchi VI 0 universe with anisotropic fluid

Details Dynamics of a magnetized Bianchi VI 0 universe with anisotropic fluid Dynamics of a magnetized Bianchi VI 0 universe with anisotropic fluid

May 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ap%26ss.339...45s&link_type=abstract

Astrophysics and Space Science, Volume 339, Issue 1, pp.45-51

Astronomy and Astrophysics

Astrophysics

Scientific paper

We discuss spatially homogeneous and anisotropic Bianchi type VI 0 cosmological model with anisotropic fluid and magnetic field. The energy-momentum tensor consists of anisotropic fluid with anisotropic EoS and a uniform magnetic field of energy density ρ B . Exact solution of the field equations is obtained by using the condition that expansion is proportional to the shear scalar. We focus on the future evolution of the model both in the presence and absence of magnetic field. In particular, we address the question whether these models approach to isotropy.

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