Scalar Perturbations in Inflationary Models Based on the Non-Linear Sigma Model

Details Scalar Perturbations in Inflationary Models Based on the Non-Linear Sigma Model Scalar Perturbations in Inflationary Models Based on the Non-Linear Sigma Model

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004gregr..36.1625k&link_type=abstract

General Relativity and Gravitation, v. 36, Issue 7, p. 1625-1640 (2004).

Computer Science

Scientific paper

The inflationary models based on the non-linear sigma model with the
self-coupling potential are considered. The slow-roll solutions for
long-wavelength inhomogeneities in general two-component chiral models
and diagonal three-component chiral model of a special case are
obtained. Scalar perturbations are calculated for two examples.

Affiliated with

Also associated with

No associations

Rating

Scalar Perturbations in Inflationary Models Based on the Non-Linear Sigma Model 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 Scalar Perturbations in Inflationary Models Based on the Non-Linear Sigma Model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Scalar Perturbations in Inflationary Models Based on the Non-Linear Sigma Model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1010920