2009/05/21 by G. L. Fogli, Fogli, G. L., E. Lisi +7 · 1 citation
Physics and Astronomy · #Cosmology and Gravitation Theories #FOS: Physical sciences #High Energy Physics - Experiment (hep-ex) #High Energy Physics - Phenomenology (hep-ph) #Neutrino Physics Research #Nuclear Experiment (nucl-ex) #Nuclear Theory (nucl-th) #Particle physics theoretical and experimental studies #hep-ex #hep-ph #nucl-ex #nucl-th
paper · pdf · doi:10.48550/arxiv.0905.3549
9 pages, including 4 figures. Talk presented by G.L. Fogli at NEUTEL 2009, XIII International Workshop on "Neutrino Telescopes" (Venice, Italy, March 10-13, 2009). Note: Title and abstract modified in the current arXiv version
openalex publication_date 2009/05/21 · arxiv created 2009/07/16 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
At the previous Venice meeting NO-VE 2008, we discussed possible hints in favor of a nonzero value for the unknown neutrino mixing angle theta(13), emerging from the combination of solar and long-baseline reactor data, as well as from the combination of atmospheric, CHOOZ and long-baseline accelerator numu->numu data. Recent MINOS 2009 results in the numu->nue appearance channel also seem to support such hints. A combination of all current oscillation data provides, as preferred range, sin2 theta(13) = 0.02 +- 0.01 (1σ). We review several issues raised by such hints in the last year, and comment on their possible near-future improvements and tests.