Some Cosmological Models in Scalar-Tensor Theory of Gravitation

Details Some Cosmological Models in Scalar-Tensor Theory of Gravitation Some Cosmological Models in Scalar-Tensor Theory of Gravitation

Jul 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ap%26ss.277..461r&link_type=abstract

Astrophysics and Space Science, Volume 277, Issue 3, pp.461-472

Astronomy and Astrophysics

Astrophysics

29

Scientific paper

Field equations in a scalar-tensor theory of gravitation proposed by Saezand Ballester (1985) are obtained with the aid of (i) Friedmann-type metric (ii) a non static plane symmetric metric and (iii) spatially homogeneous Bianchi type - III metric. Some cosmological models corresponding to perfect fluid and bulk viscous fluid are presented. Physical and kinematical properties of the models are also discussed.

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