Higher dimensional effective stiff fluid cosmological models in scalar tensor theory

Details Higher dimensional effective stiff fluid cosmological models in scalar tensor theory Higher dimensional effective stiff fluid cosmological models in scalar tensor theory

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ap%26ss.317..169m&link_type=abstract

Astrophysics and Space Science, Volume 317, Issue 3-4, pp. 169-173

Astronomy and Astrophysics

Astrophysics

Five Dimensions, Viscous Fluid, Scalar Tensor Theory

Scientific paper

Five dimensional LRS Bianchi type-I effective stiff fluid cosmological
models in scalar tensor theory of gravitation proposed by Saez and
Ballester (Phys. Lett. A 113:467, 1986) are constructed. Further, some
physical and geometrical features of these models are discussed.

Affiliated with

Also associated with

No associations

Rating

Higher dimensional effective stiff fluid cosmological models in scalar tensor 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 Higher dimensional effective stiff fluid cosmological models in scalar tensor theory, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Higher dimensional effective stiff fluid cosmological models in scalar tensor theory will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1665113