Answers are grounded in this paper and cite their sources.
The dynamics of a spatially homogeneous scalar field, generating a conformally flat Friedman metric, is considered. It is assumed that the scalar field is weakly coupled to ordinary matter and is described by a rather arbitrary potential. The examples of some exact and asymptotic solutions to the non-linear differential equation appearing in the problem, are presented. The possible implications of the solutions for cosmology are briefly pointed out.
No takes yet. Share an insight, caveat, or question.
A. G. Muslimov (1990) studied this question.
Synapse has enriched 5 related papers. Consider them for comparative context: