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 (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 (130)Te recently set by Cuoricino and on prospective limits or signals from the Karlsruhe tritium neutrino experiment.
Observables sensitive to absolute neutrino masses. II / G. L., F., E., L., A., M., Melchiorri, A., A., P., A. M., R., P., S., J., S., A., S.. - In: PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. - ISSN 1550-7998. - 78:3(2008), pp. 033010-033015. [10.1103/physrevd.78.033010]
Observables sensitive to absolute neutrino masses. II
MELCHIORRI, Alessandro;
2008
Abstract
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 (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 (130)Te recently set by Cuoricino and on prospective limits or signals from the Karlsruhe tritium neutrino experiment.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
