  We consider the cosmological system with two interacting fluids: dark energy
and dark matter, in a homogeneous and isotropic universe with dissipation. The
modified gravitational equation for dark matter is solved. The analytic
representations for the Little Rip, the Pseudo Rip, and the bounce cosmology
models with dissipation are obtained in terms of the thermodynamic parameters
in the equation of state. We analyze the corrections in the energy density for
dark matter, in view of the dissipative processes and the coupling with dark
energy.
