  The rapid oscillating scalar field is considered as the quintessence in the
framework of nonminimal kinetic coupling model. The scalar field behaves like a
perfect fluid with a variable equation of state parameter which can be
expressed as a function of the Hubble parameter. This feature enables us to
study its evolution via continuity equation.
  The scalar field may behave as dark energy in the present epoch, while it
behaves like dark matter in the future. This characteristic allows the
occurrence of a decelerated expansion after the present acceleration, without
invoking any interaction. The model is also studied in the presence of an
interaction between dark sectors alleviating the coincidence problem. The
stability of the model is investigated and the stable attractor solutions are
studied.
