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In the present letter, we consider homogeneous and isotropic noncommutativecosmological models induced by a symplectic formalism coupled to phantomperfect fluids and a cosmological constant. After computing the fieldequations, we solve them to find the scalar factor dynamics. We restrict ourattention to expansive solutions, that may represent the present expansion ofour Universe. Those solutions generate {\it big rip} singularities. We studyhow the parameters, of those models, modify the time it takes to the scalarfactor expands from zero till infinity, at the {\it big rip}.

Noncommutative cosmological models induced by a symplectic formalism coupled to phantom fluids