Abstract
Some cylindrically symmetric inhomogeneous cosmological models for perfect fluid distributions with electromagnetic field are obtained. To get a determinate solution, a supplementary condition between metric potentials is used. Various physical and geometrical properties of the models with some special cases are also discussed.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
References
Bali, R.: 1986, Int. J. Theor. Phys. 25, 7, 755.
Bali, Raj and Singh, Ghanshyam: 1987, Astrophys. Space Sci. 134, 47.
Collins, C.B. and Sza Frau, D.A.: 1979, J. Math. Phys. 20, 2347.
Collins, C.B. and Sza Frau, D.A.: 1979, J. Math. Phys. 20, 2362.
Lorentz, D.: 1980, Phys. Lett. 79A, 79.
Lorentz, D.: 1980, Lettor Nuorocim 29, 238.
Lorentz, D.: 1982, Astrophys. Space Sci. 85, 59.
Roy, S.R. and Tiwari, O.P.: 1983, Int. J. Pure and Appl. Math. 14, 2, 233.
Roy, S.R. and Singh, P.N.: 1986, J. Phys. A. Mathematical and General 9 (2), 255.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Singh, G., Mehta, P. & Gupta, S. Some Inhomogeneous Perfect Fluid Cosmological Models in the Presence of Electromagnetic Field. Astrophysics and Space Science 281, 677–688 (2002). https://doi.org/10.1023/A:1016388031818
Issue Date:
DOI: https://doi.org/10.1023/A:1016388031818