  The present paper deals with cylindrically symmetric metric in the form of
Marder (1958) with Saez-Ballester theory of gravitation in the presence of
perfect fluid and dark energy. In order to obtain the deterministic solution of
the field equations we have assumed that the expansion scalar in the model is
proportional to the Eigen value of the shear tensor. We have also assumed that
the two sources, here the perfect fluid and dark energy interact minimally with
separate conservative parts of their energy momentum tensors together with the
constant EoS parameter of the perfect fluid. The role of the dark energy in the
present model with variable equation of state parameter is studied more in
detail. Some physical properties of model are also discussed.
