Cosmological dynamics of Scalar--Tensor Gravity

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

25 pages, 4 figures, 12 tables, submitted to CQG

Scientific paper

10.1088/0264-9381/25/3/035008

We study the phase--space of FLRW models derived from Scalar--Tensor Gravity where the non--minimal coupling is $F(\phi)=\xi\phi^2$ and the effective potential is $V(\phi)=\lambda \phi^n$. Our analysis allows to unfold many feature of the cosmology of this class of theories. For example, the evolution mechanism towards states indistinguishable from GR is recovered and proved to depend critically on the form of the potential $V(\phi)$. Also, transient almost--Friedmann phases evolving towards accelerated expansion and unstable inflationary phases evolving towards stable ones are found. Some of our results are shown to hold also for the String-Dilaton action.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Cosmological dynamics of Scalar--Tensor Gravity 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 dynamics of Scalar--Tensor Gravity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cosmological dynamics of Scalar--Tensor Gravity will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-293959

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.