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Neutrino oscillations and the seesaw origin of neutrino mass

2016/02/29 by O. G. Miranda, J. W. F. Valle
Chemistry · Physics and Astronomy · #Astrophysics and Cosmic Phenomena #CP violation #Chemistry #Electron #Lepton #Measurements of neutrino speed #Mixing (physics) #Neutrino #Neutrino Physics Research #Neutrino oscillation #Nuclear physics #Oscillation (cell signaling) #Particle physics #Particle physics theoretical and experimental studies #Physics #Physics beyond the Standard Model #Pontecorvo–Maki–Nakagawa–Sakata matrix #Quantum mechanics #Seesaw mechanism #Seesaw molecular geometry #Solar neutrino #Solar neutrino problem #Sterile neutrino #Unitarity #hep-ex #hep-ph

paper · pdf · doi:10.1016/j.nuclphysb.2016.03.027

17 pages, 9 figures. Improved text and figures. To appear in the Nuclear Physics B special issue on Neutrino Oscillations celebrating the Nobel Prize in Physics 2015

openalex publication_date 2016/03/26 · arxiv created 2016/04/12 · arxiv updated 2016/06/22 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

The historical discovery of neutrino oscillations using solar and atmospheric neutrinos, and subsequent accelerator and reactor studies, has brought neutrino physics to the precision era. We note that CP effects in oscillation phenomena could be difficult to extract in the presence of unitarity violation. As a result upcoming dedicated leptonic CP violation studies should take into account the non-unitarity of the lepton mixing matrix. Restricting non-unitarity will shed light on the seesaw scale, and thereby guide us towards the new physics responsible for neutrino mass generation.

Citations