Non - singular inflationary Universe

Details Non - singular inflationary Universe Non - singular inflationary Universe

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987qpif.book..176z&link_type=abstract

Quantum processes in intensive fields (Russian title: Kvantovyie processy v intensivnyh polyah), Kishinev Izdatel Shtiintsa, Kis

Physics

Cosmology, Inflation, Massless Scalar Field, Self-Action

Scientific paper

An open homogenous isotropic Universe is examined, with De Sitter phase at the yearly stage of its evolution. A spontaneous breackdown of the symmetry of the masless self-acting scalar field is occuring for all realistic values of the self-action constant "lambda". The taking into account of the back action of that spontaneously breacked field on the metric lead to avoiding of the initial singularity in Cosmology for "lambda" = 10^-2, ...10^-12 for z>= 10^29, where Z^3 is the Entropy of the Universe at the present moment to the Entropy of Universe at the beggining of the inflationary phase ratio.
Bibliography: 4

Affiliated with

Also associated with

No associations

Rating

Non - singular inflationary Universe 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 Non - singular inflationary Universe, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Non - singular inflationary Universe will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1777150