Two-fluid cosmological models in a Bianchi type I space-times

Details Two-fluid cosmological models in a Bianchi type I space-times Two-fluid cosmological models in a Bianchi type I space-times

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ap%26ss.314...95o&link_type=abstract

Astrophysics and Space Science, Volume 314, Issue 1-3, pp. 95-103

Astronomy and Astrophysics

Astrophysics

Scientific paper

In this paper we present anisotropic, homogeneous two-fluid cosmological models in a Bianchi I space-time. These classes of cosmological models picture two different scenarios of cosmic history; viz., when the radiation and matter content of the universe are in interactive phase and another when the two are non-interacting. The universe is highly anisotropic in the initial stages, however, anisotropy tapers out to insignificance in due course of cosmic evolution. In every model the anisotropy of the space-time is determined by the density parameter Ω0 at the present epoch. For Ω0=1, the anisotropy is washed out before long. An interesting class of models, having an inflationary epoch in finite future, is discovered.

Affiliated with

Also associated with

No associations

Rating

Two-fluid cosmological models in a Bianchi type I space-times 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 Two-fluid cosmological models in a Bianchi type I space-times, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Two-fluid cosmological models in a Bianchi type I space-times will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1421892