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Theoretical aspects of neutrino oscillations

2001/09/17 by André de Gouvêa, Andre de Gouvea · 1 citation
Physics and Astronomy · #Anomaly (physics) #Astrophysics and Cosmic Phenomena #Measurements of neutrino speed #Mixing (physics) #Neutrino #Neutrino Physics Research #Neutrino oscillation #Particle physics #Particle physics theoretical and experimental studies #Physics #Solar neutrino #Solar neutrino problem #hep-ph

paper · pdf · doi:10.1016/s0168-9002(03)00634-x

published as Nucl.Instrum.Meth. A503 (2001) 4-12 · Invited Plenary Talk at the NUFACT'01 Conference, 14 pages, 2 figures

arxiv created 2001/09/17 · openalex publication_date 2003/05/01 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

I review some aspects concerning the physics of neutrino mixing and oscillations. I discuss in some detail the physical neutrino oscillations parameter space in the case of two and three family mixing, and briefly describe the current knowledge of neutrino mixing parameters according to the present solar, atmospheric, and reactor neutrino data. I also briefly comment on the possibility of solving the LNSD anomaly together with the solar and atmospheric ones. I conclude by emphasising that that even though in five to ten years time a lot will be learnt from the next round of neutrino experiments, a great deal about neutrino masses and neutrino mixing will remain unknown.

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