Search results for "KAMIOKANDE"

showing 10 items of 14 documents

Neutral-current atmospheric neutrino flux measurement using neutrino-proton elastic scattering in Super-Kamiokande

2003

Recent results show that atmospheric $\nu_\mu$ oscillate with $\delta m^2 \simeq 3 \times 10^{-3}$ eV$^2$ and $\sin^2{2\theta_{atm}} \simeq 1$, and that conversion into $\nu_e$ is strongly disfavored. The Super-Kamiokande (SK) collaboration, using a combination of three techniques, reports that their data favor $\nu_\mu \to \nu_\tau$ over $\nu_\mu \to \nu_{sterile}$. This distinction is extremely important for both four-neutrino models and cosmology. We propose that neutrino-proton elastic scattering ($\nu + p \to \nu + p$) in water \v{C}erenkov detectors can also distinguish between active and sterile oscillations. This was not previously recognized as a useful channel since only about 2% …

Elastic scatteringPhysicsNuclear and High Energy PhysicsParticle physicsNeutral currentProtonPhysics::Instrumentation and DetectorsHigh Energy Physics::PhenomenologyFOS: Physical sciencesParticle identificationHigh Energy Physics - ExperimentNuclear physicsMiniBooNEHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics::ExperimentNeutrinoNeutrino oscillationSuper-KamiokandePhysical Review D
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Simultaneous measurement of the muon neutrino charged-current cross section on oxygen and carbon without pions in the final state at T2K

2020

Authors: K. Abe,56 N. Akhlaq,45 R. Akutsu,57 A. Ali,32 C. Alt,11 C. Andreopoulos,54,34 L. Anthony,21 M. Antonova,19 S. Aoki,31 A. Ariga,2 T. Arihara,59 Y. Asada,69 Y. Ashida,32 E. T. Atkin,21 Y. Awataguchi,59 S. Ban,32 M. Barbi,46 G. J. Barker,66 G. Barr,42 D. Barrow,42 M. Batkiewicz-Kwasniak,15 A. Beloshapkin,26 F. Bench,34 V. Berardi,22 L. Berns,58 S. Bhadra,70 S. Bienstock,53 S. Bolognesi,6 T. Bonus,68 B. Bourguille,18 S. B. Boyd,66 A. Bravar,13 D. Bravo Berguño,1 C. Bronner,56 S. Bron,13 A. Bubak,51 M. Buizza Avanzini ,10 T. Campbell,7 S. Cao,16 S. L. Cartwright,50 M. G. Catanesi,22 A. Cervera,19 D. Cherdack,17 N. Chikuma,55 G. Christodoulou,12 M. Cicerchia,24,† J. Coleman,34 G. Collazu…

Fermi gasPhysics::Instrumentation and DetectorsMonte Carlo methodmeasured [channel cross section]KAMIOKANDEmuon neutrino01 natural sciencesPhysics Particles & FieldsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)secondary beam [neutrino/mu][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Particle Physics ExperimentsMuon neutrinoQDCharged currentQCPhysicsneutrino: energy spectrumJ-PARC LabPhysicsinteraction [neutrino nucleus]T2K experimentoscillation [neutrino]Monte Carlo [numerical calculations]suppressionNuclear & Particles PhysicskinematicsPhysical Sciences0202 Atomic Molecular Nuclear Particle and Plasma PhysicsGround statenumerical calculations: Monte Carlochannel cross section: measuredParticle Physics - Experiment530 PhysicsFOS: Physical sciencesAstronomy & Astrophysics530Nuclear physicsPionnear detector0103 physical sciencessimultaneous measurement0201 Astronomical and Space SciencesSCATTERINGddc:530010306 general physicsNeutrino oscillation0206 Quantum Physicscross section: charged currentMuonScience & Technologynucleus: ground stateNUCLEI010308 nuclear & particles physicsnucleus: targethep-excarbonenergy spectrum [neutrino]neutrino nucleus: interactionground state [nucleus]neutrino/mu: secondary beamtarget [nucleus]random phase approximationcharged current [cross section]High Energy Physics::Experimentneutrino: oscillationoxygenexperimental resultsPhysical Review D
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Characterization of nuclear effects in muon-neutrino scattering on hydrocarbon with a measurement of final-state kinematics and correlations in charg…

2018

This paper reports measurements of final-state proton multiplicity, muon and proton kinematics, and their correlations in charged-current pionless neutrino interactions, measured by the T2K ND280 near detector in its plastic scintillator (C$_8$H$_8$) target. The data were taken between years 2010 and 2013, corresponding to approximately 6$\times10^{20}$ protons on target. Thanks to their exploration of the proton kinematics and of kinematic imbalances between the proton and muon kinematics, the results offer a novel probe of the nuclear-medium effects most pertinent to the (sub-)GeV neutrino-nucleus interactions that are used in accelerator-based long-baseline neutrino oscillation measureme…

Fermi gasProtoninteraction: modelPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsKinematicsKAMIOKANDE7. Clean energy01 natural sciencesPhysics Particles & Fieldscharged currentHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Particle Physics ExperimentsMuon neutrinoneutrino oscillationAXISNuclear ExperimentHigh Energy Physics - Experiment; High Energy Physics - Experiment; Physics and Astronomy (miscellaneous)Charged currentneutrino: interactionPhysicsCHALLENGESPhysicsJ-PARC Labp: final state3. Good healthtransversekinematicsPhysical SciencesNeutrinospectral representationFOS: Physical sciencesddc:500.2Astronomy & AstrophysicsREGIONNuclear physicsphase spacenear detectormuon0103 physical sciencesEXCITATIONddc:530010306 general physicsNeutrino oscillationDETECTORnuclear matter effectscintillation counterp: multiplicityMuonScience & Technology010308 nuclear & particles physicshep-exnucleusscatteringnuclear matter: effectneutrino nucleus: interactionfinal-state interactionneutrino/mu: secondary beamPhase spacecorrelationPhysics::Accelerator Physicsneutrino nucleus interactionneutrino: oscillationexperimental results
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Zenith angle distributions at Super-Kamiokande and SNO and the solution of the solar neutrino problem

2000

We have performed a detailed study of the zenith angle dependence of the regeneration factor and distributions of events at SNO and SK for different solutions of the solar neutrino problem. In particular, we discuss oscillatory behaviour and the synchronization effect in the distribution for the LMA solution, the parametric peak for the LOW solution, etc.. Physical interpretation of the effects is given. We suggest a new binning of events which emphasizes distinctive features of zenith angle distributions for the different solutions. We also find the correlations between the integrated day-night asymmetry and the rates of events in different zenith angle bins. Study of these correlations st…

Nuclear and High Energy PhysicsAstrofísica nuclearmedia_common.quotation_subjectSolar neutrinoSolar neutrinosFOS: Physical sciencesAstrophysicsAstrophysicsAsymmetryPartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Neutrins solarsNeutrino oscillationZenithParametric statisticsmedia_commonParticles (Nuclear physics)PhysicsSistema solarAstrophysics (astro-ph)FísicaSolar neutrino problemHigh Energy Physics - PhenomenologyDistribution (mathematics)High Energy Physics::ExperimentNuclear astrophysicsSuper-KamiokandeSolar system
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Measurement of the neutrino-oxygen neutral-current interaction cross section by observing nuclear deexcitation gamma rays

2014

We report the first measurement of the neutrino-oxygen neutral-current quasielastic (NCQE) cross section. It is obtained by observing nuclear deexcitation $\gamma$-rays which follow neutrino-oxygen interactions at the Super-Kamiokande water Cherenkov detector. We use T2K data corresponding to $3.01 \times 10^{20}$ protons on target. By selecting only events during the T2K beam window and with well-reconstructed vertices in the fiducial volume, the large background rate from natural radioactivity is dramatically reduced. We observe 43 events in the $4-30$ MeV reconstructed energy window, compared with an expectation of 51.0, which includes an estimated 16.2 background events. The background …

Nuclear and High Energy PhysicsCherenkov detectorPhysics::Instrumentation and DetectorsC-12FOS: Physical sciencesAstronomy & Astrophysicslaw.inventionHigh Energy Physics - ExperimentPhysics Particles & FieldsNuclear physicsSUPER-KAMIOKANDE DETECTORCross section (physics)High Energy Physics - Experiment (hep-ex)lawEXCITATIONABSORPTION[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]SCATTERINGO-16Nuclear ExperimentPhysicsCALIBRATIONScience & TechnologyNeutral currenthep-exPhysicsGamma rayT2K experimentFísica3. Good healthPhysical SciencesNeutrinoWEAKFiducial markerBeam (structure)
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The T2K Experiment

2011

The T2K experiment is a long-baseline neutrino oscillation experiment. Its main goal is to measure the last unknown lepton sector mixing angle {\theta}_{13} by observing {\nu}_e appearance in a {\nu}_{\mu} beam. It also aims to make a precision measurement of the known oscillation parameters, {\Delta}m^{2}_{23} and sin^{2} 2{\theta}_{23}, via {\nu}_{\mu} disappearance studies. Other goals of the experiment include various neutrino cross section measurements and sterile neutrino searches. The experiment uses an intense proton beam generated by the J-PARC accelerator in Tokai, Japan, and is composed of a neutrino beamline, a near detector complex (ND280), and a far detector (Super-Kamiokande)…

Nuclear and High Energy PhysicsParticle physicsSterile neutrinoPhysics - Instrumentation and DetectorsNeutrino oscillationPhysics::Instrumentation and Detectorsddc:500.27. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Long baseline[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrinos010306 general physicsNeutrino oscillationphysics.ins-detInstrumentationQCPhysicsT2Khep-ex010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyT2K experimentNeutrinos; Neutrino oscillation; Long baseline; T2K; J-PARC; Super-KamiokandeFísicaNeutrino detectorJ-PARCHigh Energy Physics::ExperimentJ-PARCSuper-KamiokandeNeutrinoSuper-KamiokandeLepton
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First measurement of the muon neutrino charged current single pion production cross section on water with the T2K near detector

2017

The T2K off-axis near detector, ND280, is used to make the first differential cross section measurements of muon neutrino charged current single positive pion production on a water target at energies ∼0.8  GeV. The differential measurements are presented as a function of the muon and pion kinematics, in the restricted phase space defined by pπ+>200  MeV/c, pμ>200  MeV/c, cos(θπ+)>0.3 and cos(θμ)>0.3. The total flux integrated νμ charged current single positive pion production cross section on water in the restricted phase space is measured to be ⟨σ⟩ϕ=4.25±0.48(stat)±1.56(syst)×10-40  cm2/nucleon. The total cross section is consistent with the NEUT prediction (5.03×10-40  cm2/nucleon) and 2σ…

Particle physicssingle production [pi]Physics and Astronomy (miscellaneous)Physics::Instrumentation and Detectorswaterneutrinoproduction [pi]FOS: Physical sciencesFluxKAMIOKANDE01 natural sciencesHigh Energy Physics - Experimentcharged currentNuclear physicsHigh Energy Physics - Experiment (hep-ex)phase spacePionnear detectormeasured [differential cross section]secondary beam [neutrino/mu]0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Muon neutrinoddc:530High Energy Physicsmeasured [total cross section]010306 general physicsNuclear Experimentneutrino nucleusCharged currentPhysicsMuon010308 nuclear & particles physicsGenerator (category theory)hep-exJ-PARC Labinteraction [neutrino nucleus]flux [neutrino]Monte Carlo [numerical calculations]3. Good healthkinematicsProduction (computer science)High Energy Physics::ExperimentNucleonParticle Physics - Experimentexperimental results
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Search for Lorentz and CPT violation using sidereal time dependence of neutrino flavor transitions over a short baseline

2017

A class of extensions of the Standard Model allows Lorentz and CPT violations, which can be identified by the observation of sidereal modulations in the neutrino interaction rate. A search for such modulations was performed using the T2K on-axis near detector. Two complementary methods were used in this study, both of which resulted in no evidence of a signal. Limits on associated Lorentz and CPT-violating terms from the Standard Model extension have been derived by taking into account their correlations in this model for the first time. These results imply such symmetry violations are suppressed by a factor of more than 1020 at the GeV scale.

Physics and Astronomy (miscellaneous)CPT symmetryAstrophysicsKAMIOKANDE01 natural scienceshigh energy physicsPhysics Particles & FieldsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Standard-Model Extension[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]neutrino: interactionPhysicssymmetry: violationPhysicsJ-PARC LabCPT symmetrysuppressionLorentz symmetryviolation: LorentzmodulationSidereal timePhysical Sciencesneutrino: flavorsymbolsNeutrinoupper limitParticle physicsdata analysis method530 PhysicsLorentz transformationFOS: Physical sciencesCPT: violationAstronomy & AstrophysicsStandard Modelsymbols.namesakenear detectorstatistical analysis0103 physical sciences010306 general physicsNeutrino oscillationneutrino oscillationsScience & Technology010308 nuclear & particles physicshep-exHigh Energy Physics::PhenomenologySymmetry (physics)neutrino/mu: secondary beamcorrelationtime dependenceHigh Energy Physics::Experimentneutrino: oscillationexperimental results
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Probing the neutrino mass hierarchy with Super-Kamiokande

2012

We show that for recently discovered large values of theta(13), a superbeam with an average neutrino energy of ~ 5 GeV, such as those being proposed at CERN, if pointing to Super-Kamiokande (L = 8770 km), could reveal the neutrino mass hierarchy at 5 sigma in less than two years irrespective of the true hierarchy and CP phase. The measurement relies on the near resonant matter effect in the numu to nue oscillation channel, and can be done counting the total number of appearance events with just a neutrino beam.

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderHierarchy (mathematics)010308 nuclear & particles physicsOscillationPhase (waves)FísicaFOS: Physical sciencesSigma01 natural sciences7. Clean energyHigh Energy Physics - ExperimentHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsSuper-KamiokandeMass hierarchyJournal of High Energy Physics
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Rejection Power of A Horizontal Rpc Telescope For Left and Right Coming Cosmic Muons

1993

Abstract The possibility of performing neutrino astronomy by means of a detector above the ground depends critically on the feasibility of a rejection power on the order of 10 11 required to discriminate the enormous background of cosmic downward going muons from the signal of upward going muons produced by neutrinos. In order to check whether and how this rejection is obtainable, we have built in the Physics Department of the University of Bari a horizontal cosmic muon telescope (MINI) instrumented with resistive plate counters. By performing time-of-flight measurements, we have estimated the rejection power of our telescope for left and right coming cosmic muons. The rejection dependence …

PhysicsNuclear and High Energy PhysicsResistive touchscreenCOSMIC cancer databaseMuonPhysics::Instrumentation and DetectorsSURFACE NEUTRINO DETECTORAstrophysics::High Energy Astrophysical PhenomenaTrack (disk drive)DetectorAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyKAMIOKANDE-II DETECTORlaw.inventionTelescopeNEUTRINOSlawHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyInstrumentation
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