Observables sensitive to absolute neutrino masses. II

Details Observables sensitive to absolute neutrino masses. II Observables sensitive to absolute neutrino masses. II

2008-05-16

arxiv.org/abs/0805.2517v3

Phys.Rev.D78:033010,2008

Physics

High Energy Physics

High Energy Physics - Phenomenology

Final version for PRD. Includes one more cosmological dataset (CMB+LSS) in Table II and in Fig. 3. Title slightly changed in j

Scientific paper

10.1103/PhysRevD.78.033010

In this followup to Phys. Rev. D 75, 053001 (2007) [arXiv:hep-ph/0608060] 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 0nu2beta decay results in 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 0nu2beta limits in 130-Te recently set by Cuoricino, and on prospective limits or signals from the KATRIN experiment.

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