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Signal of neutrinoless double beta decay, neutrino spectrum and oscillation scenarios
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The lower and upper bounds on the neutrinoless double beta (0nu-2beta) decay rate are obtained, as functions of the parameters of neutrino oscillations and of the lightest neutrino mass. The constraints on these parameters from the search for the 0nu-2beta transition, as well as from the interpretation of solar and atmospheric neutrino data in terms of oscillations, can be conveniently represented in one unitarity triangle. This representation helps to clarify the cases when the 0nu-2beta rate is small; the crucial dependence on the scenarios assumed for solar neutrino oscillations and on the neutrino spectrum is emphasized. We consider hierarchical and non-hierarchical neutrino spectra, and discuss their interest in view of future searches of the 0nu-2beta decay.
Forward citations
Cited by 3 Pith papers
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Towards the meV limit of the effective neutrino mass in neutrinoless double-beta decays
Neutrinoless double-beta decay at 1 meV sensitivity would constrain the lightest neutrino mass to 0.7 to 8 meV and the Majorana phase rho to 130 to 230 degrees.
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