Time-dependent diffusive interactions between dark matter and dark
  energy in the context of $k-$essence cosmology
  We investigated the scenario of time-dependent diffusive interaction between
dark matter and dark energy and showed that such a model can be accommodated
within the observations of luminosity distance - redshift data in Supernova Ia
(SNe Ia) observations. We obtain constrains on different relevant parameters of
this model from the observational data. We consider a homogeneous scalar field
$\phi(t)$ driven by a $k-$essence Lagrangian of the from $L = V(\phi)F(X)$ with
constant potential $V(\phi) = V$, to describe the dynamics of dark energy in
this model. Using the temporal behaviour of the FRW scale factor, the equation
of state and total energy density of the dark fluid, extracted from the
analysis of SNe Ia (JLA) data, we have obtained the time-dependence of the
$k-$essence scalar field and also reconstructed form of the function $F(X)$ in
the $k-$essence Lagrangian.
