Abstract
Spatially-homogenous and anisotropic Bianchi type-II and III cosmological models are obtained in Barber's second self-creation theory of gravitation both in vacuum and in the presence of perfect fluid with pressure equal to energy density. Some properties of the models are discussed.
Article PDF
Similar content being viewed by others
Avoid common mistakes on your manuscript.
References
Barber, G. A.: 1982,Gen. Rel. Grav. 14, 117.
Brans, C.: 1987,Gen. Rel. Grav. 19, 949.
Brans, C. and Dicke, R. H.: 1961,Phys. Rev. 124, 925.
Lorenz, D.: 1980,Phys. Letters A79, 19.
Reddy, D. R. K. and Venkateswarlu, r.: 1989,Astrophys. Space Sci. 155, 135.
Soleng, H. H.: 1987,Astrophys. Space Sci. 139, 13.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Shanthi, K., Rao, V.U.M. Bianchi type-II and III models in self-creation cosmology. Astrophys Space Sci 179, 147–153 (1991). https://doi.org/10.1007/BF00642359
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00642359