Bianchi VI0 cosmological model in Saez and Ballester theory

Details Bianchi VI0 cosmological model in Saez and Ballester theory Bianchi VI0 cosmological model in Saez and Ballester theory

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ap%26ss.288..611m&link_type=abstract

Astrophysics and Space Science, v. 288, Issue 4, p. 611-618 (2003).

Astronomy and Astrophysics

Astrophysics

8

Scientific paper

The problem of perfect fluid distribution in spatially homogeneous and anisotropic Bianchi type VI0 space-time is considered in a scalar tensor theory of gravitation proposed by Saez and Ballester (1985). Exact solutions of the field equations are derived when the metric potentials are functions of cosmic time only. Some physical and geometrical properties of the solutions are also discussed.

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