Abstract
Bianchi Type I magnetized Cosmological model for perfect fluid distribution is investigated. The magnetic field is due to an electric current produced along x-axis. The distribution consists of an electrically neutral perfect fluid with an infinite electrical conductivity. To get a determinate solution, a supplementary conditionA = BC between metric potentials is used. The behaviour of the model in presence and absence of magnetic field is also discussed.
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References
Bali, R. and Jain, Vimal Chand: 1999, Astrophys. Space Sci. 262, 145.
Collins, C.B.: 1972, Comm. Math. Phys. 27, 37.
Ellis, G.F.R.: 1971, in: R.K. Sachs (ed.), General Relativity and Cosmology, p. 117.
Jacobs, K.C.: 1968, Astrophys. J. 153, 661.
Jacobs, K.C.: 1969, Astrophys. J. 155, 379.
Lichnerowicz, A.: 1967, Relativistic Hydrodynamics & Magnetohydrodynamics, Benjamin, New York, p. 13.
Robertson, H.P. and Walker, A.G.: 1936, Proc. London Math. Soc. 42, 90.
Roy, S.R. and Prakash, S.: 1978, Ind. J. Phys. 52B (1), 47.
Roy, S.R. and Singh, J.P. and Narayan, S.: 1985, Astrophys. Space Sci. 111, 389.
Thorne, K.S.: 1967, Astrophys. J. 148, 55.
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Bali, R., Gokhroo, A. Bianchi Type I Anisotropic Magnetized Cosmological Model in General Relativity. Astrophysics and Space Science 278, 283–293 (2001). https://doi.org/10.1023/A:1013147215707
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DOI: https://doi.org/10.1023/A:1013147215707