Abstract
A plane-symmetric inhomogeneous cosmological model of perfect fluid distribution with electromagnetic field, is obtained.F 12 is the non-vanishing component of the electromagnetic field tensor. To get a determinate solution, we assume the free gravitational field is Petrov type-II non-degenerate. In general, the model represents an expanding, shearing, non-rotating universe in which the flow vector is geodetic. The behaviour of the electromagnetic field tensor together with some geometrical and physical aspect of the model are also discussed.
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References
Bali, R. and Tyagi, A.: 1989,Gen. Rel. Grav. 21, 1989.
Collins, C. B. and Szafran, D. A.: 1979,J. Math. Phys. 20, 2347.
Hawking, S. W. and Ellis, G. F. R. (1973),The Large-scale Structure of Space Time, Cambridge University Press, Cambridge, p. 94.
Lichnerowicz, A.: 1967,Relativistic Hydrodynamics and Magneto-hydrodynamics, W. A. Benjamin Inc., New York, p. 93.
Roy, S. R. and Narayan, S.: 1979,Ind. J. Pure Appl. Math. 10, 763.
Roy, S. R. and narayan, S.: 1981,Int. J. Theor. Phys. 20 709
Roy, S. R. and Singh, J. P.: 1982,Ind. J. Pure Appl. Math. 13 (11), 1285.
Synge, J. L.: 1960,Relativity: The General Theory, North-Holland Publ. Co., Amsterdam, p. 356.
Szafran, D. A. and Collins, C. B.: 1979,J. Math. Phys. 20, 2354.
Szekeres, P.: 1975,Comm. Math. Phys. 41, 55.
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Bali, R., Tyagi, A. A plane-symmetric inhomogeneous cosmological model of perfect fluid distribution with electromagnetic field. Astrophys Space Sci 173, 233–240 (1990). https://doi.org/10.1007/BF00643932
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DOI: https://doi.org/10.1007/BF00643932