Search results for "Muon"

showing 10 items of 1376 documents

"Table 14" of "Search for supersymmetry in final states with jets, missing transverse momentum and one isolated lepton in sqrt{s} = 7 TeV pp collisio…

2016

Effective mass in the muon plus three jets W+jets control region.

Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaSUSY7000.0P P --> MU- .GE.3JET MM XJet ProductionNMuon productionInclusiveP P --> MU+ .GE.3JET MM XProton-Proton ScatteringPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentSupersymmetry
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"Table 24" of "Search for supersymmetry in final states with jets, missing transverse momentum and one isolated lepton in sqrt{s} = 7 TeV pp collisio…

2016

Effective mass in the 3-jet loose signal region (muon channel).

Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaSUSY7000.0P P --> MU- .GE.3JET MM XJet ProductionNMuon productionInclusiveP P --> MU+ .GE.3JET MM XProton-Proton ScatteringPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentSupersymmetryComputer Science::Information Theory
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"Table 26" of "Search for supersymmetry in final states with jets, missing transverse momentum and one isolated lepton in sqrt{s} = 7 TeV pp collisio…

2016

Effective mass in the 3-jet tight signal region (muon channel).

Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaSUSY7000.0P P --> MU- .GE.3JET MM XJet ProductionNMuon productionInclusiveP P --> MU+ .GE.3JET MM XProton-Proton ScatteringPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentSupersymmetryComputer Science::Information Theory
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Performance of tracking stations of the underground cosmic-ray detector array EMMA

2018

Abstract The new cosmic-ray experiment EMMA operates at the depth of 75 m (50 GeV cutoff energy for vertical muons; 210 m.w.e.) in the Pyhasalmi mine, Finland. The underground infrastructure consists of a network of eleven stations equipped with multi-layer, position-sensitive detectors. EMMA is designed for cosmic-ray composition studies around the energy range of the knee, i.e., for primary particles with energies between 1 and 10 PeV. In order to yield significant new results EMMA must be able to record data in the full configuration for about three years. The key to the success of the experiment is the performance of its tracking stations. In this paper we describe the layout of EMMA an…

Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenatutkimuslaitteetHigh-energy muonsCosmic rayScintillatorTracking (particle physics)01 natural sciencesOpticscosmic rays0103 physical sciencesAngular resolutiondrift chambersUnderground experimentCosmic rays010303 astronomy & astrophysicsImage resolutionPhysicsMuonDrift chambersta114010308 nuclear & particles physicsbusiness.industryDetectorAstronomy and Astrophysicshigh-energy muonsilmaisimetunderground experimentScintillation counterPlastic scintillation detectorsHigh Energy Physics::Experimentbusinesskosminen säteilyMuon trackingmuon trackingplastic scintillation detectorsAstroparticle Physics
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A method for detection of muon induced electromagnetic showers with the ANTARES detector

2012

The primary aim of ANTARES is neutrino astronomy with upward going muons created in charged current muon neutrino interactions in the detector and its surroundings. Downward going muons are background for neutrino searches. These muons are the decay products of cosmic-ray collisions in the Earths atmosphere far above the detector. This paper presents a method to identify and count electromagnetic showers induced along atmospheric muon tracks with the ANTARES detector. The method is applied to both cosmic muon data and simulations and its applicability to the reconstruction of muon event energies is demonstrated. © 2012 Elsevier B.V. All rights reserved.

Physics::Instrumentation and DetectorsAtmospheric muonsDecay productsNeutrino telescopeElectromagnetic shower identification01 natural sciences7. Clean energyneutrino telescope electromagnetic shower identification high energy muons energy reconstruction; high energy muons; neutrino telescope; electromagnetic shower identification; energy reconstructionMuon neutrinoNEUTRINO TELESCOPE010303 astronomy & astrophysicsInstrumentationEnergy reconstructionPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorAstrophysics::Instrumentation and Methods for AstrophysicsDetectorsHigh energy muonNeutrino detectorMuon colliderNeutrino astronomyFísica nuclearNeutrinoNeutrino telescope; Energy reconstruction; High energy muonsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaFLUXNuclear and High Energy PhysicsParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Charged current[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayMuon neutrinoNuclear physicsElectromagnetism0103 physical sciencesHigh energy physicsneutrino telescope electromagnetic shower identification high energy muons energy reconstructionInstrumentation and Methods for Astrophysics (astro-ph.IM)MuonANTARES010308 nuclear & particles physicsCharged particles[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]FISICA APLICADATEVPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNeutrino astronomyNeutrino telescopesElectro-magnetic showersHigh energy muons
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"Table 1" of "Precision measurement of scaled momentum, charge multiplicity and thrust in nu/mu N and anti-nu/mu N interactions."

1999

Average neutrino energy. Peak postion of distribution on log(1/z) is presented.

Physics::Instrumentation and DetectorsHigh Energy Physics::PhenomenologyNUMU NUCLEON --> MUON HADRON (HADRONS)6.72ExclusiveHigh Energy Physics::ExperimentTHRUSTMuon productionMULT
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Measurement of the anomalous precession frequency of the muon in the Fermilab Muon g−2 Experiment

2021

The Muon g-2 Experiment at Fermi National Accelerator Laboratory (FNAL) has measured the muon anomalous precession frequency $\omega_a$ to an uncertainty of 434 parts per billion (ppb), statistical, and 56 ppb, systematic, with data collected in four storage ring configurations during its first physics run in 2018. When combined with a precision measurement of the magnetic field of the experiment's muon storage ring, the precession frequency measurement determines a muon magnetic anomaly of $a_{\mu}({\rm FNAL}) = 116\,592\,040(54) \times 10^{-11}$ (0.46 ppm). This article describes the multiple techniques employed in the reconstruction, analysis and fitting of the data to measure the preces…

Physics::Instrumentation and DetectorsMeasure (physics)FOS: Physical sciences7. Clean energy01 natural sciencesOmegaHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment; High Energy Physics - Experiment; Nuclear ExperimentHigh Energy Physics - Experiment (hep-ex)muon0103 physical sciencesFermilabNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentLarmor precessionPhysicsMuon010308 nuclear & particles physicsSettore FIS/01 - Fisica Sperimentaleanomalous magnetic moment3. Good healthMagnetic fieldPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentStorage ringFermi Gamma-ray Space TelescopePhysical Review
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"Table 22" of "Search for supersymmetry in final states with jets, missing transverse momentum and one isolated lepton in sqrt{s} = 7 TeV pp collisio…

2016

Effective mass in the muon plus four jets top control region.

Physics::Instrumentation and DetectorsSUSY7000.0Jet ProductionNMuon productionComputer Science::Computers and SocietyInclusiveNonlinear Sciences::Exactly Solvable and Integrable SystemsProton-Proton ScatteringPhysics::Atomic and Molecular ClustersP P --> MU- .GE.4JET MM XHigh Energy Physics::ExperimentSupersymmetryP P --> MU+ .GE.4JET MM X
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"Table 16" of "Search for supersymmetry in final states with jets, missing transverse momentum and one isolated lepton in sqrt{s} = 7 TeV pp collisio…

2016

Effective mass in the muon plus three jets top control region.

Physics::Instrumentation and DetectorsSUSY7000.0P P --> MU- .GE.3JET MM XJet ProductionNMuon productionComputer Science::Computers and SocietyInclusiveP P --> MU+ .GE.3JET MM XNonlinear Sciences::Exactly Solvable and Integrable SystemsProton-Proton ScatteringPhysics::Atomic and Molecular ClustersHigh Energy Physics::ExperimentSupersymmetry
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Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory

2011

Erratum: Phys. Rev. D 85, 029902(E) (2012) [http://dx.doi.org/10.1103/PhysRevD.85.029902]

Physics::Instrumentation and DetectorsSolar neutrinoAstrophysicsUPPER LIMITPHOTON FRACTION01 natural sciences7. Clean energyneutrinoObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsORIGINPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]pionAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryCOSMIC-RAYScosmic ray detectorsand other elementary particle detectorsCosmic neutrino backgroundNEUTRINOSFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaFLUXFERMI-LATNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]TELESCOPEAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayEXTENSIVE AIR-SHOWERSSURFACE DETECTORCosmic RayPionmuon0103 physical sciencesNeutrino010306 general physicsCosmic raysPierre Auger ObservatoryMuon010308 nuclear & particles physicsFísicaand other elementary particlesUltra-high energy cosmic raysPERFORMANCECosmic rayneutrino flavor; air showers; surface detector; observatory; atmosphere; Auger; cosmic radiation; energy spectrum13. Climate actionHigh Energy Physics::Experiment
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