Search results for " Detectors"

showing 10 items of 2027 documents

Measurement of the intrinsic electron neutrino component in the T2K neutrino beam with the ND280 detector

2014

The T2K experiment has reported the first observation of the appearance of electron neutrinos in a muon neutrino beam. The main and irreducible background to the appearance signal comes from the presence in the neutrino beam of a small intrinsic component of electron neutrinos originating from muon and kaon decays. In T2K, this component is expected to represent 1.2% of the total neutrino flux. A measurement of this component using the near detector (ND280), located 280 m from the target, is presented. The charged current interactions of electron neutrinos are selected by combining the particle identification capabilities of both the time projection chambers and electromagnetic calorimeters…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences01 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyT2K experimentFísicaSolar neutrino problem3. Good healthCosmic neutrino backgroundNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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Light sterile neutrino sensitivity at the nuSTORM facility

2014

A facility that can deliver beams of electron and muon neutrinos from the decay of a stored muon beam has the potential to unambiguously resolve the issue of the evidence for light sterile neutrinos that arises in short-baseline neutrino oscillation experiments and from estimates of the effective number of neutrino flavors from fits to cosmological data. In this paper, we show that the nuSTORM facility, with stored muons of 3.8 GeV/c $\pm$ 10%, will be able to carry out a conclusive muon neutrino appearance search for sterile neutrinos and test the LSND and MiniBooNE experimental signals with 10$\sigma$ sensitivity, even assuming conservative estimates for the systematic uncertainties. This…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy & AstrophysicsComputer Science::Digital LibrariesPartícules (Física nuclear)High Energy Physics - ExperimentMiniBooNENuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0201 Astronomical and Space SciencesTOOLKITNeutrino oscillationDETECTOR0206 Quantum PhysicsPhysicsGALLEXScience & Technologyhep-exPhysicsPHYSICS PARTICLES & FIELDSHigh Energy Physics::Phenomenologyhep-phSolar neutrino problemNuclear & Particles PhysicsCosmic neutrino backgroundHigh Energy Physics - PhenomenologyNeutrino detectorPhysical Sciences0202 Atomic Molecular Nuclear Particle and Plasma PhysicsComputer Science::Mathematical SoftwareMeasurements of neutrino speedPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNeutrinoParticle Physics - Experiment
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Measurement of the atmospheric neutrino energy spectrum from 100 GeV to 400 TeV with IceCube

2010

A measurement of the atmospheric muon neutrino energy spectrum from 100 GeV to 400 TeV was performed using a data sample of about 18,000 up-going atmospheric muon neutrino events in IceCube. Boosted decision trees were used for event selection to reject mis-reconstructed atmospheric muons and obtain a sample of up-going muon neutrino events. Background contamination in the final event sample is less than one percent. This is the first measurement of atmospheric neutrinos up to 400 TeV, and is fundamental to understanding the impact of this neutrino background on astrophysical neutrino observations with IceCube. The measured spectrum is consistent with predictions for the atmospheric muon ne…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesDeep IceSouth-PoleHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)ddc:530Muon neutrinoNeutrino oscillationPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)FluxHigh Energy Physics::PhenomenologyOptical-PropertiesDetectorSolar neutrino problemHigh Energy Physics - PhenomenologyNeutrino detectorMeasurements of neutrino speedPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical PhenomenaTelescopesPhys.Rev.D
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T2K neutrino flux prediction

2013

The Tokai-to-Kamioka (T2K) experiment studies neutrino oscillations using an off-axismuon neutrino beam with a peak energy of about 0.6 GeV that originates at the Japan Proton Accelerator Research Complex accelerator facility. Interactions of the neutrinos are observed at near detectors placed at 280 m from the production target and at the far detector-Super-Kamiokande-located 295 km away. The flux prediction is an essential part of the successful prediction of neutrino interaction rates at the T2K detectors and is an important input to T2K neutrino oscillation and cross section measurements. A FLUKA and GEANT3-based simulation models the physical processes involved in the neutrino producti…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical Phenomenaddc:500.2Antiprotons01 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsPions0103 physical sciencesMomentum rangeMuon neutrino010306 general physicsNeutrino oscillationNuclear ExperimentQCPhysicsGev-c010308 nuclear & particles physicsParticle-productionHigh Energy Physics::PhenomenologyT2K experimentFísicaDetectorMonitorSolar neutrino problemNucleiNeutrino detector13. Climate actionMeasurements of neutrino speedPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNeutrinoProtonsAbsorption cross-sectionsParticle Physics - Experiment
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Status of the CPT violating interpretations of the LSND signal

2003

We study the status of the CPT violating neutrino mass spectrum which has been proposed to simultaneously accommodate the oscillation data from LSND, KamLAND, atmospheric and solar neutrino experiments, as well as the non-observation of anti-neutrino disappearance in short-baseline reactor experiments. We perform a three-generation analysis of the global data with the aim of elucidating the viability of this solution. We find no compatibility between the results of the oscillation analysis of LSND and all-but-LSND data sets below 3$\sigma$ CL. Furthermore, the global data without LSND show no evidence for CPT violation: the best fit point of the all-but-LSND analysis occurs very close to a …

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoFOS: Physical sciences7. Clean energy01 natural sciencesPartícules (Física nuclear)Nuclear physicsHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesBibliographyNeutrinsNeutrinos010306 general physicsNeutrino oscillationParticles (Nuclear physics)PhysicsLiquid Scintillator Neutrino DetectorViolació càrrega-paritat (Física nuclear)010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemHigh Energy Physics - PhenomenologyCP violationMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoCP violation (Nuclear physics)
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Global status of neutrino oscillation parameters after Neutrino-2012

2012

Here we update the global fit of neutrino oscillations in arXiv:1103.0734 and arXiv:1108.1376 including the recent measurements of reactor antineutrino disappearance reported by the Double Chooz, Daya Bay and RENO experiments, together with latest MINOS and T2K appearance and disappearance results, as presented at the Neutrino-2012 conference. We find that the preferred global fit value of $\theta_{13}$ is quite large: $\sin^2\theta_{13} \simeq 0.025$ for normal and inverted neutrino mass ordering, with $\theta_{13} = 0$ now excluded at more than 10$\sigma$. The impact of the new $\theta_{13}$ measurements over the other neutrino oscillation parameters is discussed as well as the role of th…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoFOS: Physical sciencesCHOOZ01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationPhysicsNOνA010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaSolar neutrino problemHigh Energy Physics - PhenomenologyMINOSMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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Mass Varying Neutrinos in the Sun

2005

In this work we study the phenomenological consequences of the dependence of mass varying neutrinos on the neutrino density in the Sun, which we precisely compute in each point along the neutrino trajectory. We find that a generic characteristic of these scenarios is that they establish a connection between the effective Delta m^2 in the Sun and the absolute neutrino mass scale. This does not lead to any new allowed region in the oscillation parameter space. On the contrary, due to this effect, the description of solar neutrino data worsens for large absolute mass. As a consequence a lower bound on the level of degeneracy can be derived from the combined analysis of the solar and KamLAND da…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoFOS: Physical sciencesParameter spaceAstrophysics01 natural sciences7. Clean energyUpper and lower boundsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationPhysicsStandard solar model010308 nuclear & particles physicsAstrophysics (astro-ph)FísicaSolar neutrino problemHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Measurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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Status of global fits to neutrino oscillations

2004

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' …

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 neutrinoNeutrino
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Updating neutrino magnetic moment constraints

2016

20 pages.- 4 figures.- Addendum on the limit from the Borexino data

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoPhysics beyond the Standard ModelFOS: Physical sciencesElectromagnetic properties01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationMajorana neutrinosBorexinoPhysicsMagnetic moment010308 nuclear & particles physicslcsh:QC1-999High Energy Physics - PhenomenologyNucleus coherent scatteringMeasurements of neutrino speedCP violationBorexinoNeutrinolcsh:Physics
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Study of energy response and resolution of the ATLAS barrel calorimeter to hadrons of energies from 20 to 350 GeV

2010

A fully instrumented slice of the ATLAS detector was exposed to test beams from the SPS (Super Proton Synchrotron) at CERN in 2004. In this paper, the results of the measurements of the response of the barrel calorimeter to hadrons with energies in the range 20 to 350 GeV and beam impact points and angles corresponding to pseudorapidity values in the range 0.2-0.65 are reported. The results are compared to the predictions of a simulation program using the Geant 4 toolkit.

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsTest-beamHadronCalorimetry01 natural sciencesNuclear physicsAtlas (anatomy)0103 physical sciencesmedicine[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNuclear ExperimentInstrumentationPhysicsRange (particle radiation)Large Hadron ColliderCalorimeter (particle physics)010308 nuclear & particles physicsATLASSuper Proton Synchrotronmedicine.anatomical_structurePseudorapidityCalibrationPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentBeam (structure)Simulation
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