Bianchi type-I cosmological effective stiff fluid model in Saez and Ballester theory

Details Bianchi type-I cosmological effective stiff fluid model in Saez and Ballester theory Bianchi type-I cosmological effective stiff fluid model in Saez and Ballester theory

Apr 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap%26ss.291...75m&link_type=abstract

Astrophysics and Space Science, v. 291, Issue 1, p. 75-83 (2004).

Astronomy and Astrophysics

Astrophysics

9

Scientific paper

The problem of viscous fluid distribution in Bianchi type I space-time is considered here in a new scalar tensor theory of gravitation proposed by Saez and Ballester (1986). Particular solutions of the field equations are derived assuming the viscous coefficient to be the power functions of energy density. Some physical and geometrical properties of the solutions are also discussed.

Affiliated with

Also associated with

No associations

Rating

Bianchi type-I cosmological effective stiff fluid model in Saez and Ballester theory does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Bianchi type-I cosmological effective stiff fluid model in Saez and Ballester theory, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Bianchi type-I cosmological effective stiff fluid model in Saez and Ballester theory will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1386532