Abstract

We consider cosmological models with dynamical dark energy (dDE) coupled to cold dark matter (CDM), while simultaneously allowing neutrinos to be massive. Using a MCMC approach, we compare these models with a wide range of cosmological data sets. We find a strong correlation between this coupling strength and the neutrino mass. This correlation persists when BAO data are included in the analysis. We add then priors on ν mass from particle experiments. The claimed detection of ν mass from the Heidelberg–Moscow neutrinoless double-β decay experiment would imply a 7–8σ detection of CDM–DE coupling. Similarly, the detection of ν mass from coming KATRIN tritium β decay experiment will imply a safe detection of a coupling in the dark sector. Previous attempts to accommodate cosmic phenomenology with such possible ν mass data made recourse to a w<-1 eoS. We compare such an option with the coupling option and find that the latter allows a drastic improvement.

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