Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.262..145b&link_type=abstract
Astrophysics and Space Science, v. 262, Issue 2, p. 145-155 (1998).
Astronomy and Astrophysics
Astrophysics
12
Scientific paper
The behaviour of magnetic field in anisotropic Bianchi type I cosmological model for perfect fluid distribution in General Relativity, is investigated. The distribution consists of an electrically neutral perfect fluid with an infinite electrical conductivity. It is assumed that the component sigma^1_1 of shear tensor sigma^jW_i is proportional to the expansion theta which leads to A = (BC)^n. The other physical and geometrical aspects of the model are also discussed, Bali (1986) obtained the cosmological model for n = 1 in presence of magnetic field. We have investigated the model for general values of n and discussed the particular case and general behaviour of the model.
Bali Raj
Chand Jain Vimal
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