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Observables sensitive to absolute neutrino masses. II

2008/05/31 by G. L. Fogli, E. Lisi, A. Marrone +8 · 180 citations
Physics and Astronomy · #CMB cold spot #Dark Matter and Cosmic Phenomena #Limit (mathematics) #MINOS #Measurements of neutrino speed #Mixing (physics) #Neutrino #Neutrino Physics Research #Neutrino oscillation #Nuclear physics #Observable #Particle physics #Particle physics theoretical and experimental studies #Physics #Pontecorvo–Maki–Nakagawa–Sakata matrix #Quantum mechanics #Solar neutrino #Solar neutrino problem #astro-ph #hep-ex #hep-ph #nucl-ex

paper · pdf · doi:10.1103/physrevd.78.033010

published in Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields 78(3) (American Physical Society) · Final version for PRD. Includes one more cosmological dataset (CMB+LSS) in Table II and in Fig. 3. Title slightly changed in journal

arxiv created 2008/08/18 · openalex publication_date 2008/08/18 · arxiv updated 2010/05/12 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

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\ensuremathν2\ensuremathβ 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 0\ensuremathν2\ensuremathβ limits in 130Te recently set by Cuoricino and on prospective limits or signals from the Karlsruhe tritium neutrino experiment.

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