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arxiv: 1203.6520 · v3 · pith:BICHU2H6new · submitted 2012-03-29 · 🌀 gr-qc · astro-ph.CO· hep-th

Exact solution and exotic fluid in cosmology

classification 🌀 gr-qc astro-ph.COhep-th
keywords cosmologicalfluidequationexactfieldsmodelomegascalar
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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 $\Lambda$CDM 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 $\omega_f$ for the cosmological fluid is within the range of $0.13 < \omega_f < 0.22.$ Some implication of this result is also discussed.

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