Abstract

We present accurate predictions of the effective Majorana mass $|m_{\beta\beta}|$ in neutrinoless double-$\beta$ decay in the standard case of $3\nu$ mixing and in the case of 3+1 neutrino mixing indicated by the reactor, Gallium and LSND anomalies. We have taken into account the uncertainties of the neutrino mixing parameters determined by oscillation experiments. It is shown that the predictions for $|m_{\beta\beta}|$ in the cases of $3\nu$ and 3+1 mixing are quite different, in agreement with previous discussions in the literature, and that future measurements of neutrinoless double-$\beta$ decay and of the effective light neutrino mass in $\beta$ decay or the total mass of the three lightest neutrinos in cosmological experiments may distinguish the $3\nu$ and 3+1 cases if the mass ordering is determined by oscillation experiments. We also present a relatively simple method to determine the minimum value of $|m_{\beta\beta}|$ in the general case of $N$-neutrino mixing.

Highlights

  • Three-neutrino mixingIn the standard three-neutrino (3ν) mixing framework, the effective Majorana mass in neutrinoless double-beta decay is given by

  • A fundamental questions that remains open is: are neutrinos Dirac or Majorana particles? This question cannot be investigated in neutrino oscillation experiments, where the total lepton number is conserved and there is no difference between Dirac neutrinos with a conserved total lepton number and truly neutral Majorana neutrinos, which do not have a conserved total lepton number

  • We present accurate predictions of the effective Majorana mass |mββ| in neutrinoless double-β decay in the standard case of 3ν mixing and in the case of 3+1 neutrino mixing indicated by the reactor, Gallium and LSND anomalies

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Summary

Three-neutrino mixing

In the standard three-neutrino (3ν) mixing framework, the effective Majorana mass in neutrinoless double-beta decay is given by. The results for the neutrino squared-mass differences are expressed in terms of the solar and atmospheric squared mass differences, which are defined by. Given this assignment of the squared mass differences, it is currently unknown if the ordering of the neutrino masses is normal (NO), such that m1 < m2 < m3 or inverted (IO), such that m3 < m1 < m2. We discuss these two cases separately in the following subsections

Normal ordering
Inverted ordering
Conclusions
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