Dynamics of Bianchi IX universe with massive scalar field
arXiv:gr-qc/9907047
Abstract
The dynamics of the Bianchi IX cosmological model with minimally coupled massive real scalar field is studied. The possibility of non-singular transition from contraction to expansion is shown. A set of initial conditions that lead to non-singular solutions is studied numerically.
15 pages with 2 eps figures and 3 gif figures