6533b837fe1ef96bd12a340a
RESEARCH PRODUCT
Updated global analysis of neutrino oscillations in the presence of eV-scale sterile neutrinos
Ivan Martinez-solerPedro A. N. MachadoMichele MaltoniJoachim KoppJoachim KoppÁLvaro Hernández-cabezudoThomas SchwetzMona Dentlersubject
Nuclear and High Energy PhysicsSterile neutrinoParticle physicsFOS: Physical sciences01 natural sciences7. Clean energySpectral lineHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNeutrino Physicslcsh:Nuclear and particle physics. Atomic energy. Radioactivityddc:530010306 general physicsNeutrino oscillationMixing (physics)Particle Physics - PhenomenologyPhysicshep-ex010308 nuclear & particles physicsOscillationPhysicsHigh Energy Physics::Phenomenologyhep-ph3. Good healthHigh Energy Physics - PhenomenologyMINOSBeyond Standard Modellcsh:QC770-798High Energy Physics::ExperimentAnomaly (physics)NeutrinoParticle Physics - Experimentdescription
We discuss the possibility to explain the anomalies in short-baseline neutrino oscillation experiments in terms of sterile neutrinos. We work in a 3+1 framework and pay special attention to recent new data from reactor experiments, IceCube and MINOS+. We find that results from the DANSS and NEOS reactor experiments support the sterile neutrino explanation of the reactor anomaly, based on an analysis that relies solely on the relative comparison of measured reactor spectra. Global data from the $\nu_e$ disappearance channel favour sterile neutrino oscillations at the $3\sigma$ level with $\Delta m^2_{41} \approx 1.3$ eV$^2$ and $|U_{e4}| \approx 0.1$, even without any assumptions on predicted reactor fluxes. In contrast, the anomalies in the $\nu_e$ appearance channel (dominated by LSND) are in strong tension with improved bounds on $\nu_\mu$ disappearance, mostly driven by MINOS+ and IceCube. Under the sterile neutrino oscillation hypothesis, the p-value for those data sets being consistent is less than $2.6\times 10^{-6}$. Therefore, an explanation of the LSND anomaly in terms of sterile neutrino oscillations in the 3+1 scenario is excluded at the $4.7\sigma$ level. This result is robust with respect to variations in the analysis and used data, in particular it depends neither on the theoretically predicted reactor neutrino fluxes, nor on constraints from any single experiment. Irrespective of the anomalies, we provide updated constraints on the allowed mixing strengths $|U_{\alpha 4}|$ ($\alpha = e,\mu,\tau$) of active neutrinos with a fourth neutrino mass state in the eV range.
year | journal | country | edition | language |
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2018-03-28 | Journal of High Energy Physics |