Abstract
Totally anisotropic Bianchi type-II cosmological solutions are presented in Barber's second self-creation theory of gravitation both in vacuum and in the presence of stiff-matter. The corresponding cosmological models have no finite singularity. The stiff-matter model gives essentially an empty universe for large time. Some physical and kinematical properties of the models are discussed.
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References
Barber, G.A.: 1982, Gen. Relativ. Gravitation 14, 117.
Brans, C.: 1987, Gen. Relativ. Gravitation 19, 949.
Brans, C. and Dicke, R.H.: 1961, Phys. Rev. 124, 925.
Guzman, E.: 1991, Astrophy. Space Sci. 179, 331.
Pimentel, L.O.: 1985, Astrophys. Space Sci. 116, 395.
Reddy, D.R.K. and Venkateswarlu, R.: 1989, Astrophys. Space Sci. 155, 135.
Shanthi, K. and Rao, V.V.M.: 1991, Astrophys. Space Sci. 179, 147.
Soleng, H.H.: 1987, Astrophys. Space Sci. 139, 13.
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Ram, S., Singh, C. Anisotropic Bianchi Type-II Cosmological Models in Self-Creation Cosmology. Astrophysics and Space Science 257, 287–292 (1997). https://doi.org/10.1023/A:1001146029530
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DOI: https://doi.org/10.1023/A:1001146029530