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Majorana neutrinos, neutrino mass spectrum, and the |m|∼10-3eV frontier in neutrinoless double beta decay

PASCOLI S
•
Petkov, Serguey
2008
  • journal article

Periodico
PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY
Abstract
If future neutrino oscillation experiments show that the neutrino mass spectrum is with normal ordering, m(1) < m(2) < m(3), and the searches for neutrinoless double beta [(beta beta)(0 nu)] decay with sensitivity to values of the effective Majorana mass |< m >| greater than or similar to 10(-2) eV give negative results, the next frontier in the quest for (beta beta)(0 nu)-decay will correspond to |< m >| similar to 10(-3) eV. By assuming that massive neutrinos are Majorana particles and their exchange is the dominant mechanism generating (beta beta)(0 nu) - decay, we analyze the conditions under which |< m >|, in the case of three-neutrino mixing and a neutrino mass spectrum with normal ordering, would satisfy |< m >| >= 0.001 eV. We consider the specific cases of (i) a normal hierarchical neutrino mass spectrum, (ii) a relatively small value of the CHOOZ angle theta(13), as well as (iii) the general case of a spectrum with normal ordering, a partial hierarchy, and a value of theta(13) close to the existing upper limit. We study the ranges of the lightest neutrino mass m(1) and/or of sin(2)theta(13) for which |< m >| >= 0.001 eV and discuss the phenomenological implications of such scenarios. We provide also an estimate of |< m >| when the three-neutrino masses and the neutrino mixing originate from a neutrino mass term of the Majorana type for the (left-handed) flavor neutrinos and Sigma(3)(j)m(j)U(ej)(2) = 0, but there does not exist a symmetry which forbids the (beta beta)(0 nu)-decay.
DOI
10.1103/PhysRevD.77.113003
WOS
WOS:000257290300011
Archivio
http://hdl.handle.net/20.500.11767/16878
info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-44949229175
Diritti
closed access
Soggetti
  • Decay

  • Neutrinos

  • Double β

  • Settore FIS/02 - Fisi...

Scopus© citazioni
66
Data di acquisizione
Jun 2, 2022
Vedi dettagli
Web of Science© citazioni
60
Data di acquisizione
Mar 28, 2024
Visualizzazioni
3
Data di acquisizione
Apr 19, 2024
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