2000
DOI: 10.1103/physrevd.61.036002
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Neutrinoless double-β decay with three or four neutrino mixing

Abstract: Considering the scheme with mixing of three neutrinos and a mass hierarchy that can accommodate the results of solar and atmospheric neutrino experiments, it is shown that the results of solar neutrino experiments imply a lower bound for the effective Majorana mass in neutrinoless double-β decay, under the natural assumptions that massive neutrinos are Majorana particles and there are no unlikely fine-tuned cancellations among the contributions of the different neutrino masses. Considering the four-neutrino sc… Show more

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Cited by 22 publications
(9 citation statements)
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“…Therefore, strong cancellations between the contributions of 2 and 3 are possible (albeit not likely [53]), whereas the range in Eq. (35) disfavors strong cancellations between the contributions of 2 and 3 and the contribution of 4 .…”
Section: Predictions For Beta-decay and Neutrinoless Double-beta-mentioning
confidence: 93%
“…Therefore, strong cancellations between the contributions of 2 and 3 are possible (albeit not likely [53]), whereas the range in Eq. (35) disfavors strong cancellations between the contributions of 2 and 3 and the contribution of 4 .…”
Section: Predictions For Beta-decay and Neutrinoless Double-beta-mentioning
confidence: 93%
“…For values of this parameter larger than ∆m atm , we get two different realizations of the degenerate case. In the following, it will vary between 10 −7 eV and 1eV: going below this range requires huge right-handed masses, typically above GUT or even Planck scale; going above does not help to increase the asymmetry, and generally violates neutrino-less double beta decay experiments [34,35] (see however [36] for a study of possible cancellations using Majorana phases).…”
Section: Parameterisation and Experimental Inputsmentioning
confidence: 99%
“…It links the mass eigenstates ν 1,2,3,4,5 having masses m 1,2,3,4,5 with the three active flavor states ν e,µ,τ and the two new sterile states ν s 1 and ν s 2 . In what follows we denote the mostly active neutrinos with ν 1,2,3 .…”
Section: Neutrino Mixingmentioning
confidence: 99%
“…Here α 2,3,4,5 are the four possible and unknown 4 Majorana phases (we can choose α 1 = 0). Applying nuclear matrix element uncertainties on the current 90% C.L.…”
Section: Neutrino Massesmentioning
confidence: 99%
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