Sm. Bilenky et al., Constraints from neutrino oscillation experiments on the effective Majorana mass in neutrinoless double beta-decay, PHYS LETT B, 465(1-4), 1999, pp. 193-202
We determine the possible values of the effective Majorana neutrino mass \[
m]\ = \Sigma(j)U(ej)(2)m(j)\ in the different phenomenologically viable thr
ee and four-neutrino scenarios. The quantities U-alpha j (alpha = e,mu,tau,
...) denote the elements of the neutrino mixing matrix and the Majorana neu
trino masses m(j) (j = 1,2,3,...) are ordered as m(1) < m(2) < ... Assuming
m(1) << m(3) in the three-neutrino case and m(1) << m(4) in the four-neutr
ino case, we discuss, in particular, how constraints on \[m]\ depend on the
mixing angle relevant in solar neutrino oscillations and on the three mass
-squared differences obtained from the analyses of the solar, atmospheric a
nd LSND data. If neutrinoless double beta-decay proceeds via the mechanism
involving \[m]\, conclusions about neutrinoless double beta-decay can be dr
awn. If one of the two viable four-neutrino schemes (Scheme A) is realized
in nature, \[m]\ can be as large as 1 eV and neutrinoless double beta-decay
could possibly be discovered in the near future. In this case a Majorana C
P phase of the mixing matrix U could be determined. In the other four-neutr
ino scheme (Scheme B) there is an upper bound on \[m]\ of the order of 10(-
2) eV. In the case of three-neutrino mixing the same is true if the neutrin
o mass spectrum is hierarchical, however, if there exist two quasi-degenera
te neutrinos and the first neutrino has a much smaller mass, values of \[m]
\ as large as similar to 0.1 eV are possible. (C) 1999 Elsevier Science B.V
. All rights reserved.