0000000000235275

AUTHOR

Shigetaka Moriyama

showing 7 related works from this author

Evidence for Muon Neutrino Oscillation in an Accelerator-Based Experiment

2005

We present results for muon neutrino oscillation in the KEK to Kamioka (K2K) long-baseline neutrino oscillation experiment. K2K uses an accelerator-produced muon neutrino beam with a mean energy of 1.3 GeV directed at the Super-Kamiokande detector. We observed the energy dependent disappearance of muon neutrino, which we presume have oscillated to tau neutrino. The probability that we would observe these results if there is no neutrino oscillation is 0.0050% (4.0 sigma).

Particle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciencesddc:500.201 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesMuon neutrino010306 general physicsNeutrino oscillationPhysicsTamura Norio010308 nuclear & particles physicsOscillationDetectorHigh Energy Physics::PhenomenologySigmaFísicaSolar neutrino problemK2K experimentPhysics::Accelerator Physics田村 詔生High Energy Physics::ExperimentBeam (structure)
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Search for Coherent Elastic Scattering of Solar B8 Neutrinos in the XENON1T Dark Matter Experiment

2021

We report on a search for nuclear recoil signals from solar $^8$B neutrinos elastically scattering off xenon nuclei in XENON1T data, lowering the energy threshold from 2.6 keV to 1.6 keV. We develop a variety of novel techniques to limit the resulting increase in backgrounds near the threshold. No significant $^8$B neutrino-like excess is found in an exposure of 0.6 t $\times$ y. For the first time, we use the non-detection of solar neutrinos to constrain the light yield from 1-2 keV nuclear recoils in liquid xenon, as well as non-standard neutrino-quark interactions. Finally, we improve upon world-leading constraints on dark matter-nucleus interactions for dark matter masses between 3 GeV/…

Elastic scatteringPhysicsPhysics::Instrumentation and DetectorsScatteringAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoDark matterGeneral Physics and Astronomychemistry.chemical_element01 natural sciences7. Clean energyNuclear physicsXenonRecoilchemistry0103 physical sciencesHigh Energy Physics::ExperimentNeutrinoNuclear Experiment010306 general physicsOrder of magnitudePhysical Review Letters
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Measurement of neutrino oscillation by the K2K experiment

2006

We present measurements of nu_mu disappearance in K2K, the KEK to Kamioka long-baseline neutrino oscillation experiment. One hundred and twelve beam-originated neutrino events are observed in the fiducial volume of Super-Kamiokande with an expectation of 158.1^{+9.2}_{-8.6} events without oscillation. A distortion of the energy spectrum is also seen in 58 single-ring muon-like events with reconstructed energies. The probability that the observations are explained by the expectation for no neutrino oscillation is 0.0015% (4.3sigma). In a two flavor oscillation scenario, the allowed Delta m^2 region at sin^2(2theta) is between 1.9 and 3.5 x 10^{-3} eV^2 at the 90% C.L. with a best-fit value o…

PhysicsNuclear and High Energy PhysicsParticle physicsTamura Norio010308 nuclear & particles physicsOscillationT2K experimentFOS: Physical sciencesFísicaElementary particle7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsMassless particleHigh Energy Physics - Experiment (hep-ex)K2K experiment0103 physical sciences田村 詔生Neutrino010306 general physicsNeutrino oscillationLeptonPhysical Review D
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$^{222}$Rn emanation measurements for the XENON1T experiment

2021

The selection of low-radioactive construction materials is of utmost importance for the success of low-energy rare event search experiments. Besides radioactive contaminants in the bulk, the emanation of radioactive radon atoms from material surfaces attains increasing relevance in the effort to further reduce the background of such experiments. In this work, we present the $^{222}$Rn emanation measurements performed for the XENON1T dark matter experiment. Together with the bulk impurity screening campaign, the results enabled us to select the radio-purest construction materials, targeting a $^{222}$Rn activity concentration of 10 $\mu$Bq/kg in 3.2 t of xenon. The knowledge of the distribut…

Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Radon emanationFOS: Physical scienceschemistry.chemical_element01 natural sciencesNOHigh Energy Physics - Experimentradon: nuclideHigh Energy Physics - Experiment (hep-ex)XENONXenon222 RnPE2_2PE2_10103 physical sciencesActivity concentration[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Dark Matter[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsEngineering (miscellaneous)background: radioactivityPhysicsradon: admixture010308 nuclear & particles physicsdetector: surfacescreeningInstrumentation and Detectors (physics.ins-det)chemistryXenon Dark matter 222 Rn radioactivityDark Matter Radon emanation XENON Direct Dark MatterDirect Dark MatterradioactivityAtomic physics
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Projected WIMP sensitivity of the XENONnT dark matter experiment

2020

XENONnT is a dark matter direct detection experiment, utilizing 5.9 t of instrumented liquid xenon, located at the INFN Laboratori Nazionali del Gran Sasso. In this work, we predict the experimental background and project the sensitivity of XENONnT to the detection of weakly interacting massive particles (WIMPs). The expected average differential background rate in the energy region of interest, corresponding to (1, 13) keV and (4, 50) keV for electronic and nuclear recoils, amounts to 12.3 ± 0.6 (keV t y)-1 and (2.2± 0.5)× 10−3 (keV t y)-1, respectively, in a 4 t fiducial mass. We compute unified confidence intervals using the profile construction method, in order to ensure proper coverage…

WIMP nucleon: scatteringdata analysis methodCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsHadronDark matterFOS: Physical sciencesElementary particledark matter: direct detection01 natural sciencesWIMP: dark matterHigh Energy Physics - ExperimentNONuclear physicsHigh Energy Physics - Experiment (hep-ex)XENONPE2_2WIMPPE2_1electron: recoil0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutron[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsPE2_4Dark matter experimentComputingMilieux_MISCELLANEOUSactivity reportnucleus: recoilPhysicsxenon: liquid010308 nuclear & particles physicsbackgroundAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)Dark matter experiments dark matter simulationssensitivityBaryonDark matter experimentsDark matter simulationsWeakly interacting massive particlesDark matter experiments; Dark matter simulationsNucleon[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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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 inclusive pi(0) production in the charged-current interactions of neutrinos in a 1.3-GeV wide band beam

2010

In this paper we report on the measurement of the rate of inclusive $\pi^0$ production induced by charged-current neutrino interactions in a C$_8$H$_8$ target at a mean energy of 1.3 GeV in the K2K near detector. Out of a sample of 11,606 charged current neutrino interactions, we select 479 $\pi^0$ events with two reconstructed photons. We find that the cross section for the inclusive $\pi^0$ production relative to the charged-current quasi-elastic cross section is $$\frac{\sigma_{CC\pi^0}}{\sigma_{CCQE}}=0.426\pm0.032(stat.)\pm0.035(syst.)$$ The energy dependent cross section ratio is also measured. The results are consistent with previous experiments for exclusive channels on different ta…

PhysicsNuclear and High Energy PhysicsParticle physicsMuonMesonPhysics::Instrumentation and Detectors010308 nuclear & particles physicsFísica01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsPionGargamelle0103 physical sciencesMuon neutrinoHigh Energy Physics::ExperimentNeutrino010306 general physicsCharged currentLepton
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