Gravitational field of the Early Universe: standard and chiral inflationary models.

Details Gravitational field of the Early Universe: standard and chiral inflationary models. Gravitational field of the Early Universe: standard and chiral inflationary models.

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.177c&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

We consider two sources of the gravitational field of the Early Universe: a self-interacting scalar field and a chiral field (non-linear sigma model). Both of this sources permit an inflationary stage. New exact solutions in standard inflationary model and theirs relation to approximate ones (slow rolling solutions) are considered. Chiral inflationary model based on non-linear sigma model are considered as well. The method of generation new exact solutions from standard inflation are developed. The differences for cosmological perturbations for standard and chiral inflationary model are investigated. It is shown that internal target space influences for perturbations.

Affiliated with

Also associated with

No associations

Rating

Gravitational field of the Early Universe: standard and chiral inflationary models. 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 Gravitational field of the Early Universe: standard and chiral inflationary models., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gravitational field of the Early Universe: standard and chiral inflationary models. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-767891