Search results for "Oscillation"

showing 10 items of 1257 documents

Limit on νe→ντ oscillations from the NOMAD experiment

2000

Abstract In the context of a two-flavour approximation we reinterpret the published NOMAD limit on ν μ → ν τ oscillations in terms of ν e → ν τ oscillations. At 90% C.L. we obtain sin 2 2θ eτ 5.2×10 −2 for large Δm 2 , while for sin 2 2 θ eτ =1 the confidence region includes Δm 2 2 / c 4 .

Nuclear physicsPhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physics0103 physical sciencesContext (language use)Limit (mathematics)Neutrino beam010306 general physicsNeutrino oscillation01 natural sciencesCharged currentPhysics Letters B
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A more sensitive search for νμ→ντ oscillations in NOMAD

1999

With additional data and improved algorithms, we have enhanced the sensitivity of our appearance search for $\numunutau$ oscillations in the NOMAD detector in the CERN-SPS wide-band neutrino beam. The search uses kinematic criteria to identify $\nutau$ charged current interactions followed by decay of the $\tau^-$ to one of several decay modes. Our ``blind'' analyses of deep-inelastic scattering data taken in 1996 and 1997, combined with consistent reanalyses of previously reported 1995 data, yield no oscillation signal. For the two-family oscillation scenario, we present the contour outlining a 90\% C.L. confidence region in the $\sin^22\theta_{\mu \tau} - \Delta m^2$ plane. At large $\Del…

Nuclear physicsPhysicsNuclear and High Energy PhysicsParticle physicsOscillationScatteringHigh Energy Physics::ExperimentSensitivity (control systems)NeutrinoNeutrino beamNeutrino oscillationCharged currentConfidence regionPhysics Letters B
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Search for Electron Antineutrino Appearance at theΔm2∼1  eV2Scale

2009

The MiniBooNE Collaboration reports initial results from a search for nu{sub m}u->nu{sub e} oscillations. A signal-blind analysis was performed using a data sample corresponding to 3.39x10{sup 20} protons on target. The data are consistent with background prediction across the full range of neutrino energy reconstructed assuming quasielastic scattering, 200<E{sub n}u{sup QE}<3000 MeV: 144 electronlike events have been observed in this energy range, compared to an expectation of 139.2+-17.6 events. No significant excess of events has been observed, both at low energy, 200-475 MeV, and at high energy, 475-1250 MeV. The data are inconclusive with respect to antineutrino oscillations suggested …

Nuclear physicsPhysicsNuclear reactionMiniBooNEParticle physicsLiquid Scintillator Neutrino DetectorQuasielastic scatteringGeneral Physics and AstronomyNeutrinoNuclear ExperimentNeutrino oscillationElectron neutrinoLeptonPhysical Review Letters
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Analysis of the Lepton Mixing Matrix from Neutrino Oscillation Experiments

1988

An analysis of experimental results in the framework of simultaneous oscillations of three neutrino flavours is used, in a combined fit, to constrain the elements of the 3×3 unitary lepton mixing matrix and to obtain limits on the three lepton mixing angles αeμ αeτ and αμτ. No evidence for mixing is found.

Nuclear physicsPhysicsParticle physicsHigh Energy Physics::PhenomenologyPontecorvo–Maki–Nakagawa–Sakata matrixHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationLepton numberMixing (physics)Lepton
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Present Knowledge of the Lepton Mixing Matrix from Neutrino Oscillation Experiments

1986

An analysis of experimental results in the framework of simultaneous oscillations of three neutrino flavours is used, in a combined fit, to constrain the elements of the 3 × 3 unitary lepton mixing matrix and to obtain limits on the three lepton mixing angles αeμ, αe τ and αμτ.

Nuclear physicsPhysicsParticle physicsSolar neutrinoHigh Energy Physics::PhenomenologyPontecorvo–Maki–Nakagawa–Sakata matrixMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoSolar neutrino problemNeutrino oscillationMixing (physics)Lepton
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10.2 Discrete Symmetries

2008

1. The asymmetry of the zenith angle distribution of νμ of Super-Kamiokande is the direct evidence of νμ oscillations. 2. The first oscillation minimum was observed in the L/E distribution using the high resolution L/E sample of Super-Kamiokande. It confirms that the distortion of the zenith angle distribution is really due to neutrino oscillations and excludes other hypotheses such as neutrino decay and decoherence model. 3. A search for charged current (CC) interaction of ντ shows a 2.4σ excess of signal and the observed number of events is consistent with the expectation. 4. No indication of νe oscillation is observed so far in atmospheric neutrinos.

Nuclear physicsPhysicsParticle physicsSterile neutrinoNeutrino detectorSolar neutrinoMeasurements of neutrino speedHigh Energy Physics::ExperimentSolar neutrino problemNeutrinoNeutrino oscillationZenith
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Transient analysis of "2 inch Direct Vessel Injection line break" in SPES-2 facility by using TRACE code

2015

In the past few decades a lot of theoretical and experimental researches have been done to understand the physical phenomena characterizing nuclear accidents. In particular, after the Three Miles Island accident, several reactors have been designed to handle successfully LOCA events. This paper presents a comparison between experimental and numerical results obtained for the “2 inch Direct Vessel Injection line break” in SPES-2. This facility is an integral test facility built in Piacenza at the SIET laboratories and simulating the primary circuit, the relevant parts of the secondary circuits and the passive safety systems typical of the AP600 nuclear power plant. The numerical analysis her…

Nuclear power plants -- Design and constructionHistoryEngineeringMathematical modelsbusiness.industryNumerical analysisNuclear engineeringSystem safetyComputer Science ApplicationsEducationlaw.inventionlawNuclear power plantCode (cryptography)Nuclear power plants -- Safety measuresTransient (oscillation)businessSimulationElectronic circuitTRACE (psycholinguistics)Line BreakNumerical analysis
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Low-energy (anti)neutrino physics with Borexino: Neutrinos from the primary proton-proton fusion process in the Sun

2014

The Sun is fueled by a series of nuclear reactions that produce the energy that makes it shine. The primary reaction is the fusion of two protons into a deuteron, a positron and a neutrino. These neutrinos constitute the vast majority of neutrinos reaching Earth, providing us with key information about what goes on at the core of our star. Several experiments have now confirmed the observation of neutrino oscillations by detecting neutrinos from secondary nuclear processes in the Sun; this is the first direct spectral measurement of the neutrinos from the keystone proton-proton fusion. This observation is a crucial step towards the completion of the spectroscopy of pp-chain neutrinos, as we…

Nuclear reactionPhysics - Instrumentation and DetectorsProtonneutrino: solarPhysics::Instrumentation and Detectors01 natural sciences7. Clean energynuclear reactionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)PositronstarPrimary (astronomy)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear Experiment (nucl-ex)[ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear ExperimentNuclear Experiment[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]BorexinoPhysicsSPECTROSCOPYInstrumentation and Detectors (physics.ins-det)SOLAR NEUTRINOSAstrophysics - Solar and Stellar AstrophysicsBorexinoNeutrinomodel: solardeuteronGRAN SASSOParticle physicsNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]talk: Conca Specchiulla 2014/09/07[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationDETECTORSolar and Stellar Astrophysics (astro-ph.SR)neutrino: modelp p: fusion010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyDeuterium13. Climate actionspectralHigh Energy Physics::Experimentneutrino: oscillationexperimental results
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Inclusive charged-current neutrino-nucleus reactions

2011

We present a model for weak CC induced nuclear reactions at energies of interest for current and future neutrino oscillation experiments. This model is a natural extension of the work of Refs.[1,2], where the QE contribution to the inclusive electron and neutrino scattering on nuclei was analyzed. The model is based on a systematic many body expansion of the gauge boson absorption modes that includes one, two and even three body mechanisms, as well as the excitation of Delta isobars. The whole scheme has no free parameters, besides those previously adjusted to the weak pion production off the nucleon cross sections in the deuteron, since all nuclear effects were set up in previous studies o…

Nuclear reactionPhysicsNuclear and High Energy PhysicsParticle physicsGauge bosonNuclear Theory010308 nuclear & particles physicsNuclear TheoryFOS: Physical sciences7. Clean energy01 natural sciencesNuclear Theory (nucl-th)MiniBooNENuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Pion0103 physical sciencesNeutrino010306 general physicsNucleonNeutrino oscillationNuclear ExperimentLepton
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Inclusive quasielastic charged-current neutrino-nucleus reactions

2004

The Quasi-Elastic (QE) contribution of the nuclear inclusive electron scattering model developed in Nucl. Phys. A627 (1997) 543 is extended to the study of electroweak Charged Current (CC) induced nuclear reactions, at intermediate energies of interest for future neutrino oscillation experiments. The model accounts for, among other nuclear effects, long range nuclear (RPA) correlations, Final State Interaction (FSI) and Coulomb corrections. Predictions for the inclusive muon capture in $^{12}$C and the reaction $^{12}$C $(\nu_\mu,\mu^-)X$ near threshold are also given. RPA correlations are shown to play a crucial role and their inclusion leads to one of the best existing simultaneous descri…

Nuclear reactionPhysicsNuclear and High Energy PhysicsParticle physicsNuclear TheoryElectroweak interactionNuclear TheoryFOS: Physical sciencesFísicaMuon captureNuclear Theory (nucl-th)Nuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)CoulombHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationNuclear ExperimentElectron scatteringCharged current
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