Search results for " Oscillation"

showing 10 items of 845 documents

Search for coherent charged pion production in neutrino-carbon interactions

2005

We report the result from a search for charged-current coherent pion production induced by muon neutrinos with a mean energy of 1.3 GeV. The data are collected with a fully active scintillator detector in the K2K long-baseline neutrino oscillation experiment. No evidence for coherent pion production is observed and an upper limit of $0.60 \times 10^{-2}$ is set on the cross section ratio of coherent pion production to the total charged-current interaction at 90% confidence level. This is the first experimental limit for coherent charged pion production in the energy region of a few GeV.

Particle physicsMesonPhysics::Instrumentation and DetectorsNeutrino-nucleus reactionsFOS: Physical sciencesGeneral Physics and Astronomyddc:500.201 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)PionExperiment-HEP0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationNuclear ExperimentNuclear ExperimentCharged currentPhysicsMuonTamura Norio010308 nuclear & particles physicsNeutrino oscillationsFísica田村 詔生Production (computer science)High Energy Physics::ExperimentNeutrinoLepton
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Measurement of the inclusive $\nu_{\mu}$ charged current cross section on iron and hydrocarbon in the T2K on-axis neutrino beam

2014

We report a measurement of the $\nu_\mu$ inclusive charged current cross sections on iron and hydrocarbon in the T2K on-axis neutrino beam. The measured inclusive charged current cross sections on iron and hydrocarbon averaged over the T2K on-axis flux with a mean neutrino energy of 1.51 GeV are $(1.444\pm0.002(stat.)_{-0.157}^{+0.189}(syst.))\times 10^{-38}\mathrm{cm}^2/\mathrm{nucleon}$, and $(1.379\pm0.009(stat.)_{-0.147}^{+0.178}(syst.))\times 10^{-38}\mathrm{cm}^2/\mathrm{nucleon}$, respectively, and their cross section ratio is $1.047\pm0.007(stat.)\pm0.035(syst.)$. These results agree well with the predictions of the neutrino interaction model, and thus we checked the correct treatme…

Particle physicsNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaFluxFOS: Physical sciencesAstronomy & Astrophysics7. Clean energy01 natural sciencesPhysics Particles & FieldsHigh Energy Physics - ExperimentNuclear physicsCross section (physics)Physics and Astronomy (all)High Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsNeutrino oscillationNuclear ExperimentDETECTORCharged currentMathematical Physicschemistry.chemical_classificationPhysicsScience & Technologyhep-ex010308 nuclear & particles physicsPhysicsT2K experimentFísicaHydrocarbonchemistryPhysical SciencesHigh Energy Physics::ExperimentNuclear and High Energy Physics; Mathematical Physics; Physics and Astronomy (all)NeutrinoNucleon
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Impact of CP-violation on neutrino lepton number asymmetries revisited

2017

We revisit the effect of the (Dirac) CP-violating phase on neutrino lepton number asymmetries in both mass- and flavor-basis. We found that, even if there are sizable effects on muon- and tau-neutrino asymmetries, the effect on the asymmetry of electron-neutrinos is at most similar to the upper bound set by BBN for initial neutrino degeneracy parameters smaller than order unity. We also found that, for the asymmetries in mass-basis, the changes caused by CP-violation is of sub-\% level which is unlikely to be accesible neither in the current nor in the forthcoming experiments.

Particle physicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and Detectorsmedia_common.quotation_subjectFOS: Physical sciences01 natural sciencesAsymmetryNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationmedia_commonPhysicsMuon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyLepton numberlcsh:QC1-999Massless particleHigh Energy Physics - PhenomenologyCP violationHigh Energy Physics::ExperimentNeutrinolcsh:PhysicsLeptonAstrophysics - Cosmology and Nongalactic Astrophysics
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Test of Lorentz and CPT violation with short baseline neutrino oscillation excesses

2011

The sidereal time dependence of MiniBooNE ν[subscript e] and ν[over-bar][subscript e] appearance data is analyzed to search for evidence of Lorentz and CPT violation. An unbinned Kolmogorov–Smirnov (K–S) test shows both the ν[subscript e] and ν[over-bar][subscript e] appearance data are compatible with the null sidereal variation hypothesis to more than 5%. Using an unbinned likelihood fit with a Lorentz-violating oscillation model derived from the Standard Model Extension (SME) to describe any excess events over background, we find that the ν[subscript e] appearance data prefer a sidereal time-independent solution, and the ν[over-bar][subscript e] appearance data slightly prefer a sidereal…

Particle physicsNuclear and High Energy PhysicsNeutrino oscillationPhysics::Instrumentation and DetectorsLorentz transformationAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesMiniBooNEPartícules (Física nuclear)High Energy Physics - ExperimentNuclear physicsMiniBooNEsymbols.namesakeHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Violació CP (Física nuclear)Standard-Model ExtensionStatistical analysisNeutrino oscillationPhysicsOscillationNull (mathematics)High Energy Physics::PhenomenologyLorentz violationHigh Energy Physics - PhenomenologySidereal timesymbolsHigh Energy Physics::ExperimentPhysics Letters B
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Absence of a day-night asymmetry in the7Be solar neutrino rate in Borexino

2012

We report on a search for the day-night asymmetry of the Be-7 solar neutrino rate measured by Borexino at the Laboratori Nazionali del Gran Sasso (LNGS), Italy. The measured value, Adn=0.001 +- 0.012 (stat) +- 0.007 (syst), shows the absence of a significant asymmetry. This result alone rejects the so-called LOW solution at more than 8.5 sigma. Combined with the other solar neutrino data, it isolates the Large Mixing Angle (LMA) -- MSW solution at DeltaChi2 > 190 without relying on the assumption of CPT symmetry in the neutrino sector. We also show that including the day-night asymmetry, data from Borexino alone restricts the MSW neutrino oscillations to the LMA solution at 90% confidence l…

Particle physicsNuclear and High Energy PhysicsNeutrino oscillationPhysics::Instrumentation and Detectorsmedia_common.quotation_subjectSolar neutrino01 natural sciencesAsymmetrySolar neutrinoNuclear physicsDay-night effect0103 physical sciences010306 general physicsNeutrino oscillationNuclear Experimentday–night effectBorexinomedia_commonPhysicsneutrino oscillations010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaSolar neutrino problemNeutrino detectorsolar neutrinosMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoCPT violation
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Single photon events from neutral current interactions at MiniBooNE

2014

The MiniBooNE experiment has reported results from the analysis of $\nu _e$ and $\bar \nu _e$ appearance searches, which show an excess of signal-like events at low reconstructed neutrino energies, with respect to the expected background. A significant component of this background comes from photon emission induced by (anti)neutrino neutral current interactions with nucleons and nuclei. With an improved microscopic model for these reactions, we predict the number and distributions of photon events at the MiniBooNE detector. Our results are compared to the MiniBooNE in situ estimate and to other theoretical approaches. We find that, according to our model, neutral current photon emission fro…

Particle physicsNuclear and High Energy PhysicsPhotonNuclear TheoryFOS: Physical sciences01 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsMiniBooNENuclear Theory (nucl-th)High Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationPhysicsNeutral current010308 nuclear & particles physicsFísicaSolar neutrino problemlcsh:QC1-999High Energy Physics - PhenomenologyPhoton emissionHigh Energy Physics::ExperimentNeutrinoNucleonlcsh:Physics
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Sensitivities to neutrino electromagnetic properties at the TEXONO experiment

2015

18 pages.- 4 figures.- 1 table

Particle physicsNuclear and High Energy PhysicsQuenching factorCoherent elastic neutrino-nucleus scatteringReactor neutrinosPhysics beyond the Standard ModelFOS: Physical sciencesWeak interactionNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)Charge radiusNeutrino oscillationPhysicsNeutral currentScatteringFísicalcsh:QC1-999Neutrino magnetic momentHigh Energy Physics - PhenomenologyCoherent elastic neutrino–nucleus scattering (CENNS)Neutrino charge radiusNeutrinoRandom phase approximationWeak mixing anglelcsh:PhysicsPhysics Letters B
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Bilinear R-parity violation with flavor symmetry

2012

Bilinear R-parity violation (BRPV) provides the simplest intrinsically supersymmetric neutrino mass generation scheme. While neutrino mixing parameters can be probed in high energy accelerators, they are unfortunately not predicted by the theory. Here we propose a model based on the discrete flavor symmetry Lambda(4) with a single R-parity violating parameter, leading to (i) correct Cabbibo mixing given by the Gatto-Sartori-Tonin formula, and a successful unification-like b-tau mass relation, and (ii) a correlation between the lepton mixing angles theta(13) and theta(23) in agreement with recent neutrino oscillation data, as well as a (nearly) massless neutrino, leading to absence of neutri…

Particle physicsNuclear and High Energy PhysicsSupersymmetric Standard ModelFOS: Physical sciences01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)R-parityDouble beta decay0103 physical sciencesDiscrete and Finite SymmetriesNeutrino Physics010306 general physicsNeutrino oscillationMixing (physics)Physics010308 nuclear & particles physicsComputer Science::Information RetrievalMass generationHigh Energy Physics::PhenomenologyFísicaMassless particleHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Beyond Standard ModelHigh Energy Physics::ExperimentNeutrinoLepton
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Measurement of the $\nu_{\mu}$ charged current quasi-elastic cross-section on carbon with the T2K on-axis neutrino beam

2015

17 pages.- 21 figures

Particle physicsNuclear and High Energy Physicschemistry.chemical_elementPion productionAstronomy & AstrophysicsMASSNeutrino beamPION-PRODUCTION7. Clean energy01 natural sciencesPhysics Particles & FieldsHigh Energy Physics - ExperimentNuclear physicsScatteringCross section (physics)0202 Atomic Molecular Nuclear Particle And Plasma Physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutron010306 general physicsNeutrino oscillationNuclear Experiment0206 Quantum PhysicsCharged currentPhysicsScience & Technologyhep-ex010308 nuclear & particles physicsScatteringPhysicsDetectorNuclear & Particles PhysicsMODEL0201 Astronomical And Space ScienceschemistryPhysical SciencesHigh Energy Physics::ExperimentNeutrinoCarbonNuclear targets
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Conditions for statistical determination of the neutrino mass spectrum in radiative emission of neutrino pairs in atoms

2016

The photon spectrum in macrocoherent atomic de-excitation via radiative emission of neutrino pairs (RENP) has been proposed as a sensitive probe of the neutrino mass spectrum, capable of competing with conventional neutrino experiments. In this paper we revisit this intriguing technique in order to quantify the requirements for statistical determination of some of the properties of the neutrino spectrum, in particular the neutrino mass scale and the mass ordering. Our results are sobering. We find that, even under ideal conditions, the determination of neutrino parameters needs experimental live times of the order of days to years for several laser frequencies, assuming a target of volume o…

Particle physicsPhotonNeutrino theory of lightPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences01 natural sciences7. Clean energyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesRadiative transferNeutrinsNeutrinos010306 general physicsNeutrino oscillationPhysicsPhotons010308 nuclear & particles physicsSolar neutrino problem3. Good healthFotonsHigh Energy Physics - PhenomenologyMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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