2008/02/29 by M. C. González-García, M. C. Gonzalez-Garcia, Michele Maltoni · 1 citation
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Neutrino Physics Research #Particle physics theoretical and experimental studies #astro-ph #hep-ex #hep-ph
paper · pdf · doi:10.1016/j.physletb.2008.04.041
published as Phys.Lett.B663:405-409,2008 · LaTeX file using elsart style, 10 pages and 2 figures included. Final version
arxiv created 2008/04/15 · openalex publication_date 2008/04/24 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We study the interplay of neutrino oscillation and invisible decay in atmospheric and long-baseline neutrinos experiments. We perform a global analysis of the full atmospheric data from Super-Kamiokande together with long-baseline K2K and MINOS in these scenarios. We find that the admixture of νμ→ντ oscillations with parameters Δm322=2.6×10−3 eV2 and θ23∼34° plus decay of the heavy neutrino, ν3, with lifetime of the order τ3/m3∼2.6×10−12 s/eV provides a reasonable fit to atmospheric neutrinos, although this solution becomes more disfavored (dropping to the 99% CL) once long-baseline data are included. Other than this local minimum, the analysis shows no evidence in favor of a non-vanishing neutrino decay width and an lower bound on the decay lifetime τ3/m3⩾9.3×10−11 s/eV is set at 99% CL. In the framework of Majoron models, this constraint can be translated into a bound on the Majoron coupling to ν3 and an unmixed very light sterile state, |gs3|⩽8.6×10−3(2.2 eV/m3).