6533b7d1fe1ef96bd125c498
RESEARCH PRODUCT
Three-neutrino mixing after the first results from K2K and KamLAND
Carlos Pena-garayM. C. Gonzalez-garciaM. C. Gonzalez-garciasubject
Astrofísica nuclearNuclear and High Energy PhysicsParticle physicsSolar neutrinoFOS: Physical sciencesContext (language use)01 natural sciences7. Clean energyPartícules (Física nuclear)Nuclear physicsHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNeutrinsNeutrinos010306 general physicsNeutrino oscillationMixing (physics)Particles (Nuclear physics)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyObservableHigh Energy Physics - Phenomenology13. Climate actionK2K experimentAstronomiaCP violationNuclear astrophysicsHigh Energy Physics::ExperimentNeutrinodescription
We analyze the impact of the data on long baseline \nu_\mu disappearance from the K2K experiment and reactor \bar\nu_e disappearance from the KamLAND experiment on the determination of the leptonic three-generation mixing parameters. Performing an up-to-date global analysis of solar, atmospheric, reactor and long baseline neutrino data in the context of three-neutrino oscillations, we determine the presently allowed ranges of masses and mixing and we consistently derive the allowed magnitude of the elements of the leptonic mixing matrix. We also quantify the maximum allowed contribution of \Delta m^2_{21} oscillations to CP-odd and CP-even observables at future long baseline experiments.
year | journal | country | edition | language |
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2003-06-02 | Physical Review D |