Abstract
An algorithm is derived for constructing spatially-homogeneous perfect fluid solutions of Einstein's field equations which are of Bianchi type-I and are locally rotationally-symmetric. Starting from Bayin and Krisch solution a new exact solution is obtained. Some physical and kinematic properties of the cosmological model are discussed.
References
Bayin, S. S. and Krisch, J. P.: 1986,J. Math. Phys. 27, 262.
Collins, C. B. and Wainwright, J.: 1983,Phys. Rev. D27, 262.
Hajj-Boutros, J.: 1984,Lecture Notes in Physics, Gravitation, Geometry, and Relativity Physics 212, 51.
Hajj-Boutros, J.: 1985,J. Math. Phys. 26, 2297.
Hajj-Boutros, J.: 1986,J. Math. Phys. 27, 1592.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Ram, S. The LRS Bianchi type-I perfect fluids space-times. Astrophys Space Sci 133, 397–401 (1987). https://doi.org/10.1007/BF00642498
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00642498