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

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Abstract
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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