6533b824fe1ef96bd12800f3
RESEARCH PRODUCT
Observables sensitive to absolute neutrino masses. II
Paolo SerraA. M. RotunnoA. M. RotunnoEligio LisiAntonio MarroneAntonio MarroneG. L. FogliG. L. FogliAlessandro MelchiorriAnze SlosarAntonio PalazzoJoseph Silksubject
PhysicsMass numberNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics (astro-ph)Cosmic background radiationFOS: Physical sciencesAstrophysicsCMB cold spotHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)MINOSDouble beta decayHigh Energy Physics::ExperimentSensitivity (control systems)Nuclear Experiment (nucl-ex)NeutrinoNeutrino oscillationNuclear Experimentdescription
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.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2008-05-16 | Physical Review D |