Mixing Case

Assuming three-neutrino mixing and massive Majorana neutrinos, we study the implications of the neutrino oscillation solutions of the solar and atmospheric neutrino problems and of the results of the CHOOZ experiment for the predictions of the effective Majorana mass in neutrinoless double beta ((ββ) 0ν-)decay, |< m >|. The general case of CP-nonconservation is investigated. The predicted values of |< m >| , which determines the magnitude of the (ββ) 0ν-decay rate, depend strongly on the type of the neutrino mass spectrum, on the solution of the solar neutrino problem, as well as on the values of the two Majorana CP-violating phases, present in the lepton mixing matrix. We find that i) |< m >| ∼ < 0.02 eV for a hierarchical neutrino mass spectrum, ii) |< m >| ∼ < 0.09 eV if the spectrum is of the inverted hierarchy type, and iii) |< m >| ≤ m in the case of three quasi-degenerate neutrinos, m > 0 being the common neutrino mass scale which is limited by the bounds from the 3 H β−decay experiments, m < 2.5 eV. The indicated maximal values of |< m >| are reached in the cases i), ii) and iii) respectively, for the large mixing angle (LMA) MSW solution, the small mixing angle (SMA) MSW, and for all current solutions, of the solar neutrino problem. If CP-invariance holds, |< m >| is very sensitive to the values of the relative CP-parities of the massive Majorana neutrinos. The cases of neutrino mass spectra which interpolate between the hierarchical or inverted hierarchy type and the quasi-degenerate one are also studied. The observation of the (ββ) 0ν-decay with a rate corresponding to |< m >| ∼ > 0.02 eV can provide unique information on the neutrino mass spectrum and on the CP-violation in the lepton sector, and if CP-invariance holds-on the relative CP-parities of the massive Majorana neutrinos.