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Title: Observables sensitive to absolute neutrino masses. II

Journal Article · · Physical Review. D, Particles Fields
; ;  [1];  [2];  [3];  [4];  [5];  [6];  [7]
  1. Dipartimento di Fisica, Universita di Bari, Via Amendola 173, 70126, Bari (Italy)
  2. Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Bari, Via Orabona 4, 70126 Bari (Italy)
  3. Dipartimento di Fisica and Sezione INFN, Universita degli Studi di Roma 'La Sapienza', P.le Aldo Moro 5, 00185 Rome (Italy)
  4. AHEP Group, Institut de Fisica Corpuscular, CSIC/Universitat de Valencia, Edifici Instituts d'Investigacio, Apartado 22085, 46071 Valencia (Spain)
  5. Department of Physics and Astronomy, University of California, Irvine, California 92697-4575 (United States)
  6. Astrophysics, Denys Wilkinson Building, Keble Road, Oxford, OX1 3RH (United Kingdom)
  7. 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