Search results for "Muon"

showing 10 items of 1376 documents

Measurement of Atmospheric Neutrino Oscillations with IceCube

2013

We present the first statistically significant detection of neutrino oscillations in the high-energy regime ($>$ 20 GeV) from an analysis of IceCube Neutrino Observatory data collected in 2010-2011. This measurement is made possible by the low energy threshold of the DeepCore detector ($\sim 20$ GeV) and benefits from the use of the IceCube detector as a veto against cosmic ray-induced muon background. The oscillation signal was detected within a low-energy muon neutrino sample (20 -- 100 GeV) extracted from data collected by DeepCore. A high-energy muon neutrino sample (100 GeV -- 10 TeV) was extracted from IceCube data to constrain systematic uncertainties. Disappearance of low-energy upw…

Particle physicsTELESCOPEPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and Astronomyddc:500.201 natural sciencesHigh Energy Physics - ExperimentIceCubeIceCube Neutrino ObservatoryHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesddc:550Muon neutrino010306 general physicsNeutrino oscillationHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMuon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyPERFORMANCESolar neutrino problem3. Good healthPhysics and AstronomyNeutrino detector13. Climate actionHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaSYSTEM
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Improved limits on the lepton-flavor violating decays tau(-) -> l(-)l(+)l(-)

2007

A search for the neutrinoless, lepton-flavor violating decay of the tau lepton into three charged leptons has been performed using 376fb-1 of data collected at an e+e- center-of-mass energy around 10.58 GeV with the BABAR detector at the SLAC PEP-II storage rings. In all six decay modes considered, the numbers of events found in data are compatible with the background expectations. Upper limits on the branching fractions are set in the range (4-8)×10-8 at 90% confidence level. © 2007 The American Physical Society.

Particle physicsVIOLATIONMesonElectron–positron annihilationCharged particleGeneral Physics and AstronomyElectron01 natural sciencesNuclear physicsParticle decaySEARCH; LEPTON; FLAVOR; VIOLATION; BABAR; SLACPositronSEARCH0103 physical sciencesFree energyLEPTON010306 general physicsPhysicsVolume fractionMuon010308 nuclear & particles physicsBranching fractionHigh Energy Physics::PhenomenologyParticle physicsBABAR detectorLepton flavorCharged leptonHEPGermanium compoundBaBarHigh Energy Physics::ExperimentParticle detectorSLACFísica de partículesExperimentsFLAVORLepton
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Hadronic light-by-light contribution to $(g-2)_\mu $ from lattice QCD: a complete calculation

2021

The European physical journal / C 81(7), 651 (2021). doi:10.1140/epjc/s10052-021-09455-4

Particle physicsmagnetic momentPhysics and Astronomy (miscellaneous)High Energy Physics::LatticeHadronNuclear TheoryLattice (group)hep-lat01 natural sciences530pi: massPionHigh Energy Physics - Latticemuon0103 physical sciencesddc:530010306 general physicsEngineering (miscellaneous)latticeParticle Physics - PhenomenologyPhysicsMuon010308 nuclear & particles physicsScattering[PHYS.HLAT]Physics [physics]/High Energy Physics - Lattice [hep-lat]High Energy Physics::Phenomenologylattice field theoryphoton photon: scatteringhep-phParticle Physics - LatticeFunction (mathematics)Lattice QCDtensionQuadrature (mathematics)High Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experimentn-point function: 4statistical
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International Scoping Study (ISS) for a future neutrino factory and Super-Beam facility. Detectors and flux instrumentation for future neutrino facil…

2009

Technical report by The ISS Detector Working Group; This report summarises the conclusions from the detector group of the International Scoping Study of a future Neutrino Factory and Super-Beam neutrino facility. The baseline detector options for each possible neutrino beam are defined as follows: 1. A very massive (Megaton) water Cherenkov detector is the baseline option for a sub-GeV Beta Beam and Super Beam facility. 2. There are a number of possibilities for either a Beta Beam or Super Beam (SB) medium energy facility between 1-5 GeV. These include a totally active scintillating detector (TASD), a liquid argon TPC or a water Cherenkov detector. 3. A 100 kton magnetized iron neutrino det…

Particle physicsneutrino factoryCherenkov detectorPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaBeam-line instrumentation (beam position and profile monitorsddc:500.27. Clean energy01 natural sciencesBunch length monitors)law.inventionNuclear physicsneutrinolaw0103 physical sciencesbeam-intensity monitorsneutrino oscillation[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Detectors and Experimental Techniques010306 general physicsInstrumentationbeam-intensity monitorMathematical PhysicsdetectorsPhysicsMuon010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physicsDetectorFísicaBeam-intensity monitorsFIS/01 - FISICA SPERIMENTALENeutrino detectorLarge detector systems for particle and astroparticle physicBeam-line instrumentation (beam position and profile monitorbunch length monitors)Physics::Accelerator PhysicsNeutrino FactoryHigh Energy Physics::ExperimentCloud chamberNeutrinoBeam (structure)
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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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Study of W Boson Production in Association with Beauty and Charm

2015

The associated production of a W boson with a jet originating from either a light parton or heavy-flavor quark is studied in the forward region using proton-proton collisions. The analysis uses data corresponding to integrated luminosities of 1.0 and 2.0  fb[superscript -1] collected with the LHCb detector at center-of-mass energies of 7 and 8 TeV, respectively. The W bosons are reconstructed using the W → μν decay and muons with a transverse momentum, p[subscript T], larger than 20 GeV in the pseudorapidity range 2.0 20  GeV and 2.2 20  GeV. The fraction of W + jet events that originate from beauty and charm quarks is measured, along with the charge asymmetries of the W + b and W + c produ…

PartonATLAS DETECTOR01 natural sciencesPRODUCTION CROSS-SECTIONSHigh Energy Physics - ExperimentPhysics Particles & FieldsSettore FIS/04 - Fisica Nucleare e SubnucleareHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Charm (quantum number)Nuclear ExperimentBosonPhysicsPhysicsParticle physics14.70.FmPseudorapidityPhysical Sciences13.87.-aLHCParticle Physics - ExperimentQuarkNuclear and High Energy PhysicsParticle physicsCOLLISIONSAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesLHCb - Abteilung HofmannHadronsAstronomy & AstrophysicsCharm quarkStandard ModelNOJets in large-Q2 scatteringNuclear physicsRATIO0103 physical sciencesSDG 7 - Affordable and Clean Energy010306 general physicsLarge Hadron Collider (France and Switzerland)MuonScience & Technology/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyROOT-S=7 TEV010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyGran Col·lisionador d'HadronsHEPLHCbJETSW bosonHigh Energy Physics::ExperimentFísica de partículesExperimentsDECAY
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Importance of Spin-Orbit Interaction for the Electron Spin Relaxation in Organic Semiconductors

2013

Despite the great interest organic spintronics has recently attracted, there is only a partial understanding of the fundamental physics behind electron spin relaxation in organic semiconductors. Mechanisms based on hyperfine interaction have been demonstrated, but the role of the spin-orbit interaction remains elusive. Here, we report muon spin spectroscopy and time-resolved photoluminescence measurements on two series of molecular semiconductors in which the strength of the spin-orbit interaction has been systematically modified with a targeted chemical substitution of different atoms at a particular molecular site. We find that the spin-orbit interaction is a significant source of electro…

PhotoluminescenceMaterials scienceGeneral Physics and Astronomy02 engineering and technology010402 general chemistry01 natural sciencesSpin-Orbit InteractionHyperfine structureComputingMilieux_MISCELLANEOUSCondensed matter physicsSpintronicsbusiness.industryOrganic SemiconductorRelaxation (NMR)Settore FIS/01 - Fisica SperimentaleSpin–orbit interactionMuon spin spectroscopy021001 nanoscience & nanotechnology0104 chemical sciencesOrganic semiconductorSemiconductorElectron Spin RelaxationCondensed Matter::Strongly Correlated Electrons[PHYS.COND.CM-SCE]Physics [physics]/Condensed Matter [cond-mat]/Strongly Correlated Electrons [cond-mat.str-el]0210 nano-technologybusiness
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Measurement of the atmospheric muon flux with a 4 GeV threshold in the ANTARES neutrino telescope

2010

A new method for the measurement of the muon flux in the deep-sea ANTARES neutrino telescope and its dependence on the depth is presented. The method is based on the observation of coincidence signals in adjacent storeys of the detector. This yields an energy threshold of about 4 GeV. The main sources of optical background are the decay of 40K and the bioluminescence in the sea water. The 40K background is used to calibrate the efficiency of the photo-multiplier tubes.

PhotomultiplierPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAtmospheric muonsFOS: Physical sciencesLINECosmic rayPotassium-4001 natural sciencesParticle detectorNuclear physicsPOTASSIUM-40NEUTRINO TELESCOPESatmospheric muons; depth intensity relation; potassium-400103 physical sciencesDepth intensity relation14. Life underwater010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)ATMOSPHERIC MUONSPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsPotassium-40DetectorAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsPERFORMANCEDEPTH INTENSITY RELATIONLIGHTNeutrino detector13. Climate actionddc:540Física nuclearHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]SYSTEMLepton
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Extraction of the Muon Signals Recorded with the Surface Detector of the Pierre Auger Observatory Using Recurrent Neural Networks

2021

The Pierre Auger Observatory, at present the largest cosmic-ray observatory ever built, is instrumented with a ground array of 1600 water-Cherenkov detectors, known as the Surface Detector (SD). The SD samples the secondary particle content (mostly photons, electrons, positrons and muons) of extensive air showers initiated by cosmic rays with energies ranging from $10^{17}~$eV up to more than $10^{20}~$eV. Measuring the independent contribution of the muon component to the total registered signal is crucial to enhance the capability of the Observatory to estimate the mass of the cosmic rays on an event-by-event basis. However, with the current design of the SD, it is difficult to straightfo…

PhotonPhysics::Instrumentation and DetectorsAstronomyElectron01 natural sciencesHigh Energy Physics - ExperimentAugerHigh Energy Physics - Experiment (hep-ex)mass [cosmic radiation]surface [detector]Observatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]photon: cosmic radiationInstrumentationMathematical PhysicsPhysicsAGASAPhysicsSettore FIS/01 - Fisica SperimentaleDetectorcosmic radiation [photon]Astrophysics::Instrumentation and Methods for AstrophysicsMonte Carlo [numerical calculations]electromagnetic [showers]Augerobservatorycosmic radiation [electron]Analysis and statistical methodsnumerical calculations: Monte CarloAnalysis and statistical methodperformancepositron: cosmic radiationatmosphere [showers]Cherenkov detectordata analysis methodAnalysis and statistical methods; Calibration and fitting methods; Cherenkov detectors; Cluster finding; Large detector systems for particle and astroparticle physics; Pattern recognitionCherenkov counter: waterairneural networkAstrophysics::High Energy Astrophysical Phenomena610FOS: Physical sciencesCosmic raycosmic radiation [positron]cosmic radiation: massCalibration and fitting methodNuclear physicsstatistical analysisPattern recognition0103 physical sciencesshowers: electromagneticddc:530ddc:610High Energy Physics010306 general physicsZenithPierre Auger ObservatoryCalibration and fitting methodscosmic radiation [muon]Muonshowers: atmosphere010308 nuclear & particles physicsdetector: surfacehep-exLarge detector systems for particle and astroparticle physicswater [Cherenkov counter]Cherenkov detectorsCluster findingelectron: cosmic radiationRecurrent neural networkmuon: cosmic radiationLarge detector systems for particle and astroparticle physicExperimental High Energy PhysicsHigh Energy Physics::ExperimentRAIOS CÓSMICOSexperimental results
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Transverse extension of partons in the proton probed in the sea-quark range by measuring the DVCS cross section

2019

Physics letters / B B793, 188-194 (2019). doi:10.1016/j.physletb.2019.04.038

Photongeneralized parton distributionmuon: polarizationProtonGeneralized Parton DistributionPartonmeasured [cross section]Proton sizenucl-exmomentum transfer dependence01 natural sciencesCOMPASSSubatomär fysikp: sizeSubatomic Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentMonte CarloQuantum chromodynamicsPhysicsRange (particle radiation)photon: productionGeneralized Parton DistributionsCOMPASS; Deep inelastic scattering; Deeply virtual Compton scattering; Exclusive reactions; Generalized Parton Distributions; Proton size; Quantum chromodynamicsExclusive reactionlcsh:QC1-999transversebeam [muon]Exclusive reactionsslopesize: (transverse)Particle Physics - ExperimentDeep inelastic scatteringQuarkNuclear and High Energy Physicsexclusive reactionslope: (calculated)liquid: target [hydrogen]photon: mediation[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]530Nuclear physicshydrogen: liquid: target0103 physical sciencesddc:530Nuclear Physics - Experiment010306 general physicsbeam: polarizationhep-ex010308 nuclear & particles physicsmuon: beam160 GeV/cmuon p --> muon p photonsize [p]Compton scatteringcross section: measuredCERN SPSDeep inelastic scattering[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::ExperimentDeeply virtual Compton scatteringlcsh:PhysicsQuantum chromodynamicsexperimental results
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