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We have embedded the texture of the neutrino mass matrix with three familiesinto the MaVaNs scenario. We take the power-law potential of the acceleronfield and a typical texture of active neutrinos, which is derived by the D_4symmetry and predicts the maximal mixing of the atmospheric neutrino and thevanishing U_{e3}. The effect of couplings among the dark fermion and activeneutrinos are studied by putting the current cosmological data and theterrestrial neutrino experimental data. It is found that the neutrino flavormixings evolve as well as the neutrino masses. Especially, U_{e3} develops intothe non-vanishing one and \theta_{atm} deviates from the maximal mixing due tocouplings among the dark fermion and active neutrinos.Comment: Sections 3 and 4 are changed and one table is added. 16pages and 2  figure

Embedding the texture of the neutrino mass matrix into the MaVaNs scenario