Search results for "ddc:500"

showing 10 items of 255 documents

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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Search for stable hadronising squarks and gluinos with the ATLAS experiment at the LHC

2011

Hitherto unobserved long-lived massive particles with electric and/or colour charge are predicted by a range of theories which extend the Standard Model. In this Letter a search is performed at the ATLAS experiment for slow-moving charged particles produced in proton–proton collisions at 7 TeV centre-of-mass energy at the LHC, using a data-set corresponding to an integrated luminosity of 34 pb[superscript −1]. No deviations from Standard Model expectations are found. This result is interpreted in a framework of supersymmetry models in which coloured sparticles can hadronise into long-lived bound hadronic states, termed R-hadrons, and 95% CL limits are set on the production cross-sections of…

Nuclear and High Energy PhysicsParticle physicsR-hadronCiências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]HadronATLAS experimentFOS: Physical sciencesddc:500.253001 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Supersymmetry; Long-lived particle; R-hadron; LimitMASSIVE CHARGED PARTICLES0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Fysikddc:530High Energy Physics010306 general physicsPhysicsGluinoLarge Hadron ColliderScience & Technology010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleATLAS experimentHigh Energy Physics::PhenomenologyFísicaSuperpartnerSupersymmetryATLASLong-lived particleCharged particleR-hadronPhysical SciencesExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearHigh Energy Physics::ExperimentLHCSupersymmetryLimitlimit; supersymmetry; long-lived particle; r-hadronParticle Physics - Experiment
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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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Observation of Exclusive Dijet Production at the Fermilab Tevatron p-pbar Collider

2007

We present the first observation and cross section measurement of exclusive dijet production in pbar-p interactions, pbar + p --> pbar + dijet + p. Using a data sample of 310 pb-1 collected by the Run II Collider Detector at Fermilab at sqrt{s}=1.96 TeV, exclusive cross sections for events with two jets of transverse energy ET >= 10 GeV have been measured as a function of minimum ET(jet). The exclusive signal is extracted from fits to data distributions based on Monte Carlo simulations of expected dijet signal and background shapes. The simulated background distribution shapes are checked in a study of a largely independent data sample of 200 pb-1 of b-tagged jet events, where exclusi…

Nuclear and High Energy PhysicsParticle physicsTevatronFOS: Physical sciencesddc:500.201 natural scienceslaw.inventionHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Particle decaylaw0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsColliderPhysicsLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::Phenomenology13.87.Ce 12.38.Qk 12.40.NnHiggs boson_Production (computer science)High Energy Physics::ExperimentCollider Detector at FermilabEnergy (signal processing)
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Measurement of atmospheric neutrino oscillations with the ANTARES neutrino telescope

2012

The data taken with the ANTARES neutrino telescope from 2007 to 2010, a total live time of 863 days, are used to measure the oscillation parameters of atmospheric neutrinos. Muon tracks are reconstructed with energies as low as 20 GeV. Neutrino oscillations will cause a suppression of vertical upgoing muon neutrinos of such energies crossing the Earth. The parameters determining the oscillation of atmospheric neutrinos are extracted by fitting the event rate as a function of the ratio of the estimated neutrino energy and reconstructed flight path through the Earth. Measurement contours of the oscillation parameters in a two-flavour approximation are derived. Assuming maximal mixing, a mass …

Nuclear and High Energy PhysicsParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2Neutrino telescope01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Experiment0103 physical sciencesNeutrinsHigh Energy PhysicsNeutrinos010306 general physicsNeutrino oscillationPhysicsMuonANTARES:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsNeutrino oscillations[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]High Energy Physics::PhenomenologySolar neutrino problemNeutrino astrophysicsCosmic neutrino backgroundNeutrino detectorFISICA APLICADAMeasurements of neutrino speedFísica nuclearHigh Energy Physics::ExperimentNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Physics Letters B
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Measurements of the T2K neutrino beam properties using the INGRID on-axis near detector

2012

Precise measurement of neutrino beam direction and intensity was achieved based on a new concept with modularized neutrino detectors. INGRID (Interactive Neutrino GRID) is an on-axis near detector for the T2K long baseline neutrino oscillation experiment. INGRID consists of 16 identical modules arranged in horizontal and vertical arrays around the beam center. The module has a sandwich structure of iron target plates and scintillator trackers. INGRID directly monitors the muon neutrino beam profile center and intensity using the number of observed neutrino events in each module. The neutrino beam direction is measured with accuracy better than 0.4 mrad from the measured profile center. The …

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsNeutrino oscillationPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical Phenomenaon-axis near detectorFOS: Physical sciencesddc:500.201 natural sciences7. Clean energyNeutrino oscillation; on-axis near detectorneutrino oscillation; neutrino detector; wavelength shifting fiber; t2k; extruded scintillator; neutrino beamNeutrino detectorNuclear physicsNeutrino beamneutrino beam0103 physical sciencesExtruded scintillatorMuon neutrinoneutrino oscillation[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationInstrumentationT2KPhysicst2k010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyNeutrino oscillation; T2K; Neutrino beam; Neutrino detector; Extruded scintillator; Wavelength shifting fiberT2K experimentextruded scintillatorFísicaInstrumentation and Detectors (physics.ins-det)Neutrino detectorneutrino detectorWavelength shiftingfiberMeasurements of neutrino speedPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNeutrinoBeam (structure)Leptonwavelength shifting fiber
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Measurement of South Pole ice transparency with the IceCube LED calibration system

2013

The IceCube Neutrino Observatory, approximately 1 km^3 in size, is now complete with 86 strings deployed in the Antarctic ice. IceCube detects the Cherenkov radiation emitted by charged particles passing through or created in the ice. To realize the full potential of the detector, the properties of light propagation in the ice in and around the detector must be well understood. This report presents a new method of fitting the model of light propagation in the ice to a data set of in-situ light source events collected with IceCube. The resulting set of derived parameters, namely the measured values of scattering and absorption coefficients vs. depth, is presented and a comparison of IceCube …

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsSouth Pole icePhoton progagationAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsddc:500.201 natural sciencesHigh Energy Physics - ExperimentIceCube Neutrino ObservatoryIceCubePhysics::GeophysicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesCalibrationddc:53014. Life underwater010306 general physicsAbsorption (electromagnetic radiation)InstrumentationInstrumentation and Methods for Astrophysics (astro-ph.IM)Cherenkov radiationRemote sensingPhysicsOptical properties010308 nuclear & particles physicsScatteringDetectorAstrophysics::Instrumentation and Methods for AstrophysicsIceCube; Optical properties; Photon propagation; South Pole iceSouth PoleiceInstrumentation and Detectors (physics.ins-det)Charged particleData setPhoton propagationAstrophysics - Instrumentation and Methods for AstrophysicsNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Comparison of large-angle production of charged pions with incident protons on cylindrical long and short targets

2009

The HARP Collaboration has presented measurements of the double-differential pi(+/-) production cross section in the range of momentum 100 MeV/c <= p <= 800 MeV/c and angle 0.35 rad <=theta <= 2.15 rad with proton beams hitting thin nuclear targets. In many applications the extrapolation to long targets is necessary. In this article the analysis of data taken with long (one interaction length) solid cylindrical targets made of carbon, tantalum, and lead is presented. The data were taken with the large-acceptance HARP detector in the T9 beam line of the CERN proton synchrotron. The secondary pions were produced by beams of protons with momenta of 5, 8, and 12GeV/c. The tracking and identific…

Nuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsNuclear TheoryFOS: Physical sciencesddc:500.27. Clean energy01 natural sciencesBildungHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Basic research0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsNuclear ExperimentPhysics010308 nuclear & particles physicsFísicaSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)Calculation methodsResearch councilPhysics::Accelerator PhysicsAngular dependenceHumanitiesParticle Physics - Experiment
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Forward production of charged pions with incident protons on nuclear targets at the CERN Proton Synchrotron

2009

et al.

Nuclear and High Energy PhysicsProtonHadronchemistry.chemical_elementProton Synchrotronddc:500.201 natural sciences7. Clean energyNuclear physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear interaction lengthNuclear Experiment010306 general physicsHARPPhysicsLarge Hadron Collider010308 nuclear & particles physicsFísicaSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)chemistryBeamlinePhysics::Accelerator PhysicsHigh Energy Physics::ExperimentBerylliumAtomic physicsParticle Physics - Experiment
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Search for Galactic PeV gamma rays with the IceCube Neutrino Observatory

2013

Gamma-ray induced air showers are notable for their lack of muons, compared to hadronic showers. Hence, air shower arrays with large underground muon detectors can select a sample greatly enriched in photon showers by rejecting showers containing muons. IceCube is sensitive to muons with energies above ~500 GeV at the surface, which provides an efficient veto system for hadronic air showers with energies above 1 PeV. One year of data from the 40-string IceCube configuration was used to perform a search for point sources and a Galactic diffuse signal. No sources were found, resulting in a 90% C.L. upper limit on the ratio of gamma rays to cosmic rays of 1.2 x 10^(-3)for the flux coming from …

Nuclear and High Energy PhysicsTELESCOPEPoint sourcePhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysicsddc:500.201 natural sciences7. Clean energyIceCube Neutrino ObservatoryIceCubeHESS0103 physical sciencesddc:530MILAGRO010306 general physics010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMuonGamma rayAstrophysics::Instrumentation and Methods for AstrophysicsPLANEGalactic planeAir showerPhysics and Astronomy13. Climate actionDISCOVERYMilagroMOLECULAR CLOUDSTEVRADIATIONHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaEMISSION
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