  The work deals with homogeneous and isotropic, flat FRW model of the universe
which is filled up with non-interacting dark matter and dark energy to
compatible with recent observational evidences. By choosing the dark energy in
the form of a dilatonic scalar field, the evolution equations are reduced to an
autonomous system. A phase space analysis is done around the critical points
and stability criteria is examined. Finally, cosmological implications of the
nature of the critical points are discussed.
