Cosmic acceleration in non-canonical scalar field model - An interacting
  scenario
  In this paper we have studied the dynamics of accelerating scenario within
the framework of scalar field models possessing a non-canonical kinetic term.
In this toy model, the scalar field is allowed to interact with the dark matter
component through a source term. We have assumed a specific form for the
coupling term and then have studied the dynamics of the scalar field having a
constant equation of state parameter. We have also carried out the dynamical
system study of such interacting non-canonical scalar field models for power
law potentials for some physically relevant specific values of the model
parameters. It has been found that the only for two particular stable fixed
points of the system, an accelerating solution is possible and the universe
will settle down to a $\Lambda$CDM universe in future and thus there is no
future singularity in this model.
