On the chiral model of cosmological inflation

Details On the chiral model of cosmological inflation On the chiral model of cosmological inflation

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ruphj..38..539c&link_type=abstract

Russian Physics Journal, Volume 38, Issue 5, pp.539-543

Physics

Scientific paper

The chiral nonlinear sigma model, which interacts with the gravitational field, is considered an effective model for the description of the inflationary stage of the early Universe. Exact solutions are found for the gravitational and chiral fields in the quasi-vacuum state of matter within the framework of the mass sigma model in Friedmann-Robertson-Walker spaces.

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