4.4 Article

2020 global reassessment of the neutrino oscillation picture

Journal

JOURNAL OF HIGH ENERGY PHYSICS
Volume -, Issue 2, Pages -

Publisher

SPRINGER
DOI: 10.1007/JHEP02(2021)071

Keywords

Beyond Standard Model; Neutrino Physics

Funding

  1. Spanish grant (AEI/FEDER, UE) [FPA2017-85216-P, FPA2017-85985-P]
  2. Spanish grant (Generalitat Valenciana) [PROMETEO/2018/165, PROMETEO/2019/083]
  3. Red Consolider MultiDark [FPA2017-90566-REDC]
  4. Vetenskapsradet (Swedish Research Council) [638-2013-8993]
  5. Oskar Klein Centre for Cosmoparticle Physics
  6. UdeM [48, 1117]
  7. Juan de la Cierva-Incorporacion program of the Spanish MINECO [IJC2018-036458-I]
  8. European Union's Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant [754496]
  9. FPU grant [FPU18/04571]
  10. European Union Horizon 2020 research and innovation program [690575, 67489]
  11. FPI grant [BES-2015-073593]
  12. research grant The Dark Universe: A Synergic Multimessenger Approach under the program PRIN 2017 - Ministero dell'Istruzione, Universita e della Ricerca (MIUR) [2017X7X85K]
  13. MINECO through the Ramon y Cajal contract [RYC-2013-12438]

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The latest global fit analysis of neutrino oscillation data provides more accurate measurements of theta(13), theta(12), Delta m212, and Delta m312 and suggests a preference for the second octant in the atmospheric angle theta(23) with statistical significance. Cosmological measurements show a clear preference for the normal neutrino mass ordering.
We present an updated global fit of neutrino oscillation data in the simplest three-neutrino framework. In the present study we include up-to-date analyses from a number of experiments. Concerning the atmospheric and solar sectors, besides the data considered previously, we give updated analyses of IceCube DeepCore and Sudbury Neutrino Observatory data, respectively. We have also included the latest electron antineutrino data collected by the Daya Bay and RENO reactor experiments, and the long-baseline T2K and NO nu A measurements, as reported in the Neutrino 2020 conference. All in all, these new analyses result in more accurate measurements of theta (13), theta (12), Delta m212 and Delta m312. The best fit value for the atmospheric angle theta (23) lies in the second octant, but first octant solutions remain allowed at similar to 2.4 sigma. Regarding CP violation measurements, the preferred value of delta we obtain is 1.08 pi (1.58 pi) for normal (inverted) neutrino mass ordering. The global analysis still prefers normal neutrino mass ordering with 2.5 sigma statistical significance. This preference is milder than the one found in previous global analyses. These new results should be regarded as robust due to the agreement found between our Bayesian and frequentist approaches. Taking into account only oscillation data, there is a weak/moderate preference for the normal neutrino mass ordering of 2.00 sigma. While adding neutrinoless double beta decay from the latest Gerda, CUORE and KamLAND-Zen results barely modifies this picture, cosmological measurements raise the preference to 2.68 sigma within a conservative approach. A more aggressive data set combination of cosmological observations leads to a similar preference for normal with respect to inverted mass ordering, namely 2.70 sigma. This very same cosmological data set provides 2 sigma upper limits on the total neutrino mass corresponding to Sigma m(nu)< 0.12 (0.15) eV in the normal (inverted) neutrino mass ordering scenario. The bounds on the neutrino mixing parameters and masses presented in this up-to-date global fit analysis include all currently available neutrino physics inputs.

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