Session III of NOW 2008 ("Dodecahedron") has been devoted to a theoretical and experimental review of neutrino oscillation physics at energy scales of O (1)  GeV. Historically, this scale provided the first strong proof of the existence of the oscillation phenomenon through the celebrated zenith angle distributions of atmospheric neutrino events observed in Super-Kamiokande. Nowadays, it is also the scale exploited in long-baseline experiments and will likely play a leading role in the next generation facilities designed to precisely measure the neutrino mixing matrix and study CP violation in the leptonic sector. © 2009 Elsevier B.V. All rights reserved.
Maltoni, M., Terranova, F. (2009). Neutrino physics at and above GeV energies. NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS, 188(C), 383-387 [10.1016/j.nuclphysbps.2009.02.089].
Neutrino physics at and above GeV energies
Terranova, Francesco
2009
Abstract
Session III of NOW 2008 ("Dodecahedron") has been devoted to a theoretical and experimental review of neutrino oscillation physics at energy scales of O (1)  GeV. Historically, this scale provided the first strong proof of the existence of the oscillation phenomenon through the celebrated zenith angle distributions of atmospheric neutrino events observed in Super-Kamiokande. Nowadays, it is also the scale exploited in long-baseline experiments and will likely play a leading role in the next generation facilities designed to precisely measure the neutrino mixing matrix and study CP violation in the leptonic sector. © 2009 Elsevier B.V. All rights reserved.
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