On the Degree of Generality of Inflation in Friedmann Cosmological Models with a Massive Scalar Field

Details On the Degree of Generality of Inflation in Friedmann Cosmological Models with a Massive Scalar Field On the Degree of Generality of Inflation in Friedmann Cosmological Models with a Massive Scalar Field

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pthph..79..676b&link_type=abstract

Progress of Theoretical Physics, Vol. 79, No. 3, pp. 676-684

Physics

28

Scientific paper

Friedmann cosmological models with a massive minimally coupled scalar field are investigated by numerical methods. It is indicated that the majority of the solutions undergo the inflationary stage in flat and open models. In a closed model the ratio of the number of solutions without adequate inflation to the number of the total solutions are obtained numerically.

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