A procedure to generate new exact solutions to Einstein equations for perfect fluids is applied to LRS Bianchi type I line-element. Starting from some known solutions a class of new perfect fluid solutions of Bianchi type I are presented. The physical and kinematical properties of spatially homogeneous and anisotropic cosmological models are studied.
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Fulling, S.A., Parker, L. and Hu, B.L.: 1974,Phys. Rev. D 10, 3905.
Hajj-Boutrs, J.: 1986,J. Math. Phys. 27, 1592.
Hawking, S.W. and Ellis, G.F.R.: 1973,The Large Scale Structure of Space-Time, Cambridge University Press.
Iyer, B.R. and Vishveshwara, C.V.: 1987,J. Math. Phys. 28, 1377.
Jacobs, K.C.: 1968,Astrophys. J. 153, 661.
Pimentel, Luis O.: 1992,Gen. Rel. Grav. 24, 985.
Shri Ram: 1987,Astrophys. Space Sci. 133, 397.
Shri Ram: 1989,Gen. Rel. Grav. 21, 697.
Thorne, K.S.: 1967,Astrophys. J. 148, 51.
Vajk, J.P. and Eltgroth, P.G.: 1970,J. Math. Phys. 11, 2212.
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Singh, J.K., Ram, S. A class of new Bianchi I perfect fluid space-times. Astrophys Space Sci 225, 57–65 (1995). https://doi.org/10.1007/BF00657843
- Exact Solution
- Cosmological Model
- Einstein Equation
- Perfect Fluid
- Bianchi Type