Physical effects involved in the measurements of neutrino masses with future cosmological data

Future Cosmic Microwave Background experiments together with upcoming galaxy and 21-cm surveys will provide extremely accurate measurements of different cosmological observables located at different epochs of the cosmic history. The new data will be able to constrain the neutrino mass sum with the best precision ever. In order to exploit the complementarity of the different redshift probes, a deep understanding of the physical effects driving the impact of massive neutrinos on CMB and large scale structures is required. The goal of this work is to describe these effects, assuming a summed neutrino mass close to its minimum allowed value. We find that parameter degeneracies can be removed by appropriate combinations, leading to robust and model independent constraints. A joint forecast of the sensitivity of Euclid and DESI surveys together with a CORE-like CMB experiment leads to a 1 sigma uncertainty of 14meV on the summed neutrino mass. Finally the degeneracy between M-nu and the optical depth at reionization tau(reio), originating in the combination of CMB and low redshift galaxy probes, might be broken by future 21-cm surveys, thus further decreasing the uncertainty on M-nu. For instance, an independent determination of the optical depth with an accuracy of sigma(tau(reio)) = 0.001 ( which might be achievable, although this is subject to astrophysical uncertainties) would decrease the uncertainty down to sigma(M-nu) = 12 meV.