Answers are grounded in this paper and cite their sources.
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. 1. Introduction Inflationary cosmological model has been studied from various aspects.
No takes yet. Share an insight, caveat, or question.
Belinsky et al. (1988) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: