Abstract
An exact Bianchi type-V cosmological model is obtained in a scalar-tensor theory of gravitation proposed by Saez and Ballester (Phys. Lett. A 113:467, 1986) in case of perfect fluid distribution. Some physical properties of the model are also discussed.
Article PDF
Similar content being viewed by others
Avoid common mistakes on your manuscript.
References
Brans, C.H., Dicke, R.H.: Phys. Rev. 124, 925 (1961)
Einstein, A.: Ann. Phys. 49, 769 (1916)
Krammer, D., et al.: Exact solutions of Einstein’s Field Equations. UEB, Berlin (1980)
Reddy, D.R.K.: Astrophys. Space Sci. 286, 359–363 (2003)
Reddy, D.R.K., Venkateswara Rao, N.: Astrophys. Space Sci. 277, 461 (2001)
Reddy, D.R.K., Naidu, R.L., Rao, V.U.M.: Astrophys. Space Sci. 306, 185 (2006)
Saez, D., Ballester, V.J.: Phys. Lett. A 113, 467 (1986)
Saha, B.: Astrophys. Space Sci. 302, 83 (2006)
Singh, C.P., Shri, R.: Astrophys. Space Sci. 284, 1199 (2003)
Singh, T., Agarwal, A.K.: Astrophys. Space Sci. 182, 289 (1991)
Singh, T., Chaubey, R.: Pramana—J. Phys. 67, 415 (2006)
Shri, R., Tiwari, S.K.: Astrophys. Space Sci. 259, 91 (1998)
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Rao, V.U.M., Vinutha, T. & Vijaya Shanthi, M. An exact Bianchi type-V cosmological model in Saez-Ballester theory of gravitation. Astrophys Space Sci 312, 189–191 (2007). https://doi.org/10.1007/s10509-007-9674-6
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s10509-007-9674-6