We study the dynamics of the scalar tensor cosmological model in the presence of tachyon field.In an alternative approach, in two exponential and power law form of the scalar field functions in the model, field equations are solved by simultaneously best fitting the model parameters with the most recent observational data. This approach gives us an observationally verified interpretation of the dynamics of the universe. We then discuss the best fitted of equation of state parameter, the statefinder parameters and the reconstructed scalar field in the model.
We study FRW cosmology for a double scalar - tensor theory of gravity where
two scalar fields are nonminimally coupled to the geometry. In a framework to
study stability and attractor solutions of the model in the phase space, we
constraint the model parameters with the observational data. For an
accelerating universe, the model behaves like quintom dark energy models and
predicts a transition from quintessence era to phantom era.Comment: 10 pages, 6 figures, to appear in Astrophysics and space sci
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