6533b85afe1ef96bd12b96c5
RESEARCH PRODUCT
Status of global fits to neutrino oscillations
Mariam TórtolaMichele MaltoniT. SchwetzJose W.f. Vallesubject
Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoPhysics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and AstronomyFluxAstrophysics01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationNuclear ExperimentPhysicsStandard solar modelDegree (graph theory)010308 nuclear & particles physicsOscillationAnomaly (natural sciences)Astrophysics (astro-ph)High Energy Physics::PhenomenologyFísicaSolar neutrino problemAtomic and Molecular Physics and Opticsddc:High Energy Physics - Phenomenology13. Climate actionMeasurements of neutrino speedHigh Energy Physics::ExperimentAtmospheric neutrinoNeutrinodescription
We review the present status of global analyses of neutrino oscillations, taking into account the most recent neutrino data including the latest KamLAND and K2K updates presented at Neutrino2004, as well as state-of-the-art solar and atmospheric neutrino flux calculations. We give the two-neutrino solar + KamLAND results, as well as two-neutrino atmospheric + K2K oscillation regions, discussing in each case the robustness of the oscillation interpretation against departures from the Standard Solar Model and the possible existence of non-standard neutrino physics. Furthermore, we give the best fit values and allowed ranges of the three-flavour oscillation parameters from the current worlds' global neutrino data sample and discuss in detail the status of the small parameters $\alpha \equiv \Dms/\Dma$ as well as $\sin^2\theta_{13}$, which characterize the strength of CP violating effects in neutrino oscillations. We also update the degree of rejection of four-neutrino interpretations of the LSND anomaly in view of the most recent developments.
year | journal | country | edition | language |
---|---|---|---|---|
2004-05-18 |