Abstract
In this paper cylindrically symmetric, inhomogeneous cosmological models with heat flux, viscous fluid and electromagnetic field are obtained. Various physical and geometrical properties of the models are also discussed.
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Bali, R. and Jain, D.R.: 1988,Astrophys. Space Sci. 141, 207.
Bali, R. and Singh, G.: 1988,Astrophys. Space Sci. 143, 377.
Bali, R. and Tyagi, A.: 1987,Astrophys. Space Sci. 138, 173.
Bali, R. and Tyagi, A.: 1988,Int. J. Phys. 27, 5, 627.
Bali, R. and Tyagi, A.: 1989,Gen. Rel. Grav. 21, 797.
Lichnerowicz, A.: 1967,Relativistic Hydroynamics and Magnetohydrodynamics, W.A. Benjamin Inc., New York, p. 93.
Marder, L.: 1958,Proc. Roy. Soc. A. 246, 133.
Narain, S.: 1988,Gen. Rel. Grav. 20, 15.
Roy, S.R. and Bali, R.: 1984,J. Math. Phys. 25, 1456.
Singh, K.P., Radhakrishnan, L. and Sharan, R.: 1965,Ann. Phys. (USA)32, 46.
Singh, K.P. and Roy, S.R.: 1972,Ind. J. Pure Appl. Math. 3, 532.
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Kilinç, C.B. Cylindrically symmetric and inhomogeneous cosmological models with viscous fluid, heat flux and electromagnetic field. Astrophys Space Sci 222, 171–179 (1994). https://doi.org/10.1007/BF00627091
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DOI: https://doi.org/10.1007/BF00627091