Exact solutions of a flat cosmological model in BSTT

Details Exact solutions of a flat cosmological model in BSTT Exact solutions of a flat cosmological model in BSTT

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap.....37..189s&link_type=abstract

Astrophysics, Volume 37, Issue 2, pp.189-195

Astronomy and Astrophysics

Astrophysics

Scientific paper

We solve the cosmological equations for the bimetric scalar—tensor theory of gravitation (BSTT) for a flat model of the Friedmann type with the equation of state p = aɛ. In the initial stage of expansion, the energy density of the scalar field dominates over the energy density of matter. As a result, the behavior of the solution in this limit does not depend on a. For later stages of expansion of the Universe, the solution obtained goes to a special solution having the form of a power law function of time. In this case, the relative change in the gravitational scalar is proportional to the Hubble parameter. In the limit of large values for the parameter of the theory, only a simple solution with zero value of the constant of integration goes to the corresponding Friedmann solution of general relativity theory.

Affiliated with

Also associated with

No associations

Rating

Exact solutions of a flat cosmological model in BSTT 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 Exact solutions of a flat cosmological model in BSTT, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Exact solutions of a flat cosmological model in BSTT will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1255463