Published August 1, 2008 | Version v1
Journal article

Observables sensitive to absolute neutrino masses. II

  • 1. Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Bari, Via Orabona 4, 70126 Bari (Italy)
  • 2. Dipartimento di Fisica, Universita di Bari, Via Amendola 173, 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)

Description

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 0ν2β decay results in 76Ge 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 0ν2β limits in 130Te recently set by Cuoricino and on prospective limits or signals from the Karlsruhe tritium neutrino experiment.

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
78
Journal Issue
3
Journal Page Range
p. 033010-033010.5
ISSN
0556-2821
CODEN
PRVDAQ

Optional Information

Notes
(c) 2008 The American Physical Society