Magnetized Cosmological Model

Physics

Scientific paper

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Scientific paper

The object of this paper is to investigate the behavior of the magnetic field in a cosmological model for perfect fluid distribution. The magnetic field is due to an electric current produced along the x axis. It is assumed that expansion ( θ) in the model is proportional to σ {1/1}, the eigenvalue of the shear tensor σ {i/j}. The behavior of the model when the magnetic field tends to zero and other physical properties are also discussed.

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