Dynamics of Bianchi IX universe with massive scalar field
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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
15 pages with 2 eps figures and 3 gif figures