Abstract

We investigate cosmological consequences of nonlinear sigma model coupled with a cosmological fluid which satisfies the continuity equation. The target space action is of de Sitter type and is composed of four scalar fields. The potential which is a function of only one of the scalar fields is also introduced. We perform a general analysis of the ensuing cosmological equations and give various critical points and their properties. Then, we show that the model exhibits exact cosmological solution which yields a transition from matter domination into dark energy and compare it with the ΛΛCDM behavior. Especially, we calculate the age of the Universe and show that it is consistent with the observational value if the equation of the state ωfω_f for the cosmological fluid is within the range of 0.13<ωf<0.22.0.13 < ω_f < 0.22. Some implication of this result is also discussed.

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