Observables sensitive to absolute neutrino masses. II
Journal Article
·
· Physical Review. D, Particles Fields
- Dipartimento di Fisica, Universita di Bari, Via Amendola 173, 70126, Bari (Italy)
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Bari, Via Orabona 4, 70126 Bari (Italy)
- Dipartimento di Fisica and Sezione INFN, Universita degli Studi di Roma 'La Sapienza', P.le Aldo Moro 5, 00185 Rome (Italy)
- AHEP Group, Institut de Fisica Corpuscular, CSIC/Universitat de Valencia, Edifici Instituts d'Investigacio, Apartado 22085, 46071 Valencia (Spain)
- Department of Physics and Astronomy, University of California, Irvine, California 92697-4575 (United States)
- Astrophysics, Denys Wilkinson Building, Keble Road, Oxford, OX1 3RH (United Kingdom)
- Berkeley Center for Cosmological Physics, Physics Department, University of California, Berkeley, California 94720 (United States)
In this followup to Phys. Rev. D 75, 053001 (2007) , we report updated constraints on neutrino mass-mixing parameters, in light of recent neutrino oscillation data (KamLAND, SNO, and MINOS) and cosmological observations (WMAP 5-year and other data). We discuss their interplay with the final 0{nu}2{beta} decay results in {sup 76}Ge claimed by part of the Heidelberg-Moscow Collaboration, using recent evaluations of the corresponding nuclear matrix elements, and their uncertainties. We also comment on the 0{nu}2{beta} limits in {sup 130}Te recently set by Cuoricino and on prospective limits or signals from the Karlsruhe tritium neutrino experiment.
- OSTI ID:
- 21250600
- Journal Information:
- Physical Review. D, Particles Fields, Vol. 78, Issue 3; Other Information: DOI: 10.1103/PhysRevD.78.033010; (c) 2008 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2821
- Country of Publication:
- United States
- Language:
- English
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