A six-parameter viscous interacting dark energy model is fitted to Union 2.1 supernovae, yielding h0=0.68, omega_de=-1.07, eta=0.05, but the underlying evolution equations for the interacting case are not presented.
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Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario
A six-parameter viscous interacting dark energy model is fitted to Union 2.1 supernovae, yielding h0=0.68, omega_de=-1.07, eta=0.05, but the underlying evolution equations for the interacting case are not presented.