  The variation of the dark energy field is found under the assumption that the
dark energy is parametric and interacts with the cold dark matter. Considering
that the variation of the field could not exceed the Planck mass, we obtain
bounds on the coupling and adiabatic coefficients. Three parameterizations of
the adiabatic coefficients are considered and two coupling terms where the
energy flows from dark energy to dark matter, or the other way around.

Cosmology and Nongalactic Astrophysics