Abstract
A spatially-homogeneous and anisotropic magnetized cosmological model in Lyra's manifold is obtained when the source of the gravitational field is a perfect fluid distribution. The magnetic field is due to an electric current produced along thex-axis. The physical behaviour of the model is discussed.
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References
Bali, R.: 1986,Int. J. Theor. Phys. 25, 755.
Collins, C. B.: 1972,Comm. Math. Phys. 27, 37.
Jacobs, K. C.: 1968,Astrophys. J. 153, 661.
Jacobs, K. C.: 1969,Astrophys. J. 155, 379.
Lyra, G.: 1951,Math. Z. 54, 52.
Roy, S. R. and Prakash, S.: 1978,Indian J. Phys. 52B(1),47.
Sen, D. K.: 1957,Z. Phys. 149, 311.
Thorne, K. S.: 1967,Astrophys. J. 148, 51.
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Reddy, D.R.K., Venkateswarlu, R. Magnetized cosmological model in Lyra manifold. Astrophys Space Sci 149, 287–291 (1988). https://doi.org/10.1007/BF00639797
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DOI: https://doi.org/10.1007/BF00639797