6533b7d3fe1ef96bd1260c43

RESEARCH PRODUCT

On the interpretation of the atmospheric neutrino data in terms of flavor changing neutrino interactions

M. Concha Gonzalez-garciaNicolao FornengoJosé W. F. Valle

subject

PhysicsNuclear and High Energy PhysicsParticle physicsMuonOscillationAnomaly (natural sciences)Astrophysics (astro-ph)FlavourFOS: Physical sciencesFísicaAstrophysicsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)BibliographyHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationZenith

description

Flavour changing (FC) neutrino-matter interactions have been proposed as a solution to the atmospheric neutrino anomaly. Here we perform the analysis of the full set of the recent 52 kTy Super-Kamiokande atmospheric neutrino data, including the zenith angle distribution of the contained events as well as the higher energy upward-going stopping and through-going muon events. Our results show that the FC mechanism can describe the full data sample with a chi^2_{min}=44/(33 d.o.f) which is acceptable at the 90% confidence level. The combined analysis confines the amount of FC to be either close to maximal or to the level of about (10-50)%.

https://doi.org/10.1088/1126-6708/2000/07/006