Cosmological scaling solutions of minimally coupled scalar fields in three dimensions

Details Cosmological scaling solutions of minimally coupled scalar fields in three dimensions Cosmological scaling solutions of minimally coupled scalar fields in three dimensions

2000-07-17

arxiv.org/abs/gr-qc/0007038v1

Class.Quant.Grav. 17 (2000) 2867-2874

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

LaTeX2e, 11 pages, 4 figures. To be published in Classical and Quantum Gravity

Scientific paper

10.1088/0264-9381/17/15/302

We examine Friedmann-Robertson-Walker models in three spacetime dimensions. The matter content of the models is composed of a perfect fluid, with a $\gamma$-law equation of state, and a homogeneous scalar field minimally coupled to gravity with a self-interacting potential whose energy density red-shifts as $a^{-2 \nu}$, where a denotes the scale factor. Cosmological solutions are presented for different range of values of $\gamma$ and $\nu$. The potential required to agree with the above red-shift for the scalar field energy density is also calculated.

Affiliated with

Also associated with

No associations

Rating

Cosmological scaling solutions of minimally coupled scalar fields in three dimensions 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 Cosmological scaling solutions of minimally coupled scalar fields in three dimensions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cosmological scaling solutions of minimally coupled scalar fields in three dimensions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-685071