Abstract
We show the way of dark matter and dark energy presentation via ansatzs on the kinetic energies of the fields in the two-component chiral cosmological model. To connect a kinetic interaction of dark matter and dark energy with observational data the reconstruction procedure for the chiral metric component and the potential of (self)interaction has been developed. The reconstruction of and for the early and later inflation have been performed. The proposed model is confronted to model as well.
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