Search results for "Muons."

showing 10 items of 46 documents

Drift Time Measurement in the ATLAS Liquid Argon Electromagnetic Calorimeter using Cosmic Muons

2010

The ionization signals in the liquid argon of the ATLAS electromagnetic calorimeter are studied in detail using cosmic muons. In particular, the drift time of the ionization electrons is measured and used to assess the intrinsic uniformity of the calorimeter gaps and estimate its impact on the constant term of the energy resolution. The drift times of electrons in the cells of the second layer of the calorimeter are uniform at the level of 1.3% in the barrel and 2.8% in the endcaps. This leads to an estimated contribution to the constant term of (0.29-0.04+0.05)% in the barrel and (0.54-0.04+0.06)% in the endcaps. The same data are used to measure the drift velocity of ionization electrons …

Drift velocityPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsInstrumentationFOS: Physical sciencesddc:500.2ElectronAstrophysics::Cosmology and Extragalactic AstrophysicsElectromagnetic CalorimeterATLAS; Drift Time Measurement; Cosmic Muons5307. Clean energy01 natural sciencesPartícules (Física nuclear)High Energy Physics - Experiment010305 fluids & plasmasNuclear physicsHigh Energy Physics - Experiment (hep-ex)Atlas (anatomy)Ionization0103 physical sciencesmedicineFysikddc:530High Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Cosmic MuonsDetectors and Experimental Techniques010306 general physicsEngineering (miscellaneous)Ciencias ExactasDetectors de radiacióPhysicsCalorimeter (particle physics)010308 nuclear & particles physicsAcceleradors de partículesResolution (electron density)Instrumentation and Detectors (physics.ins-det)ATLASliquid argonElectromagnetic calorimetermedicine.anatomical_structureExperimental High Energy PhysicsDrift Time MeasurementPhysical SciencesComputingMethodologies_DOCUMENTANDTEXTPROCESSINGHigh Energy Physics::ExperimentLHC
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Muon multiplicities measured using an underground cosmic-ray array

2016

EMMA (Experiment with Multi-Muon Array) is an underground detector array designed for cosmic-ray composition studies around the knee energy (or similar to 1 - 10 PeV). It operates at the shallow depth in the Pyhasalmi mine, Finland. The array consists of eleven independent detector stations similar to 15 m(2) each. Currently seven stations are connected to the DAQ and the rest will be connected within the next few months. EMMA will determine the multiplicity, the lateral density distribution and the arrival direction of high-energy muons event by event. The preliminary estimates concerning its performance together with an example of measured muon multiplicities are presented.

HistoryPhysics::Instrumentation and Detectorsmuonscosmic-raysCosmic rayEXTENSIVE AIR-SHOWERS01 natural sciencesEducationunderground detectorsNuclear physicsEVENTSData acquisition0103 physical sciencesDetector array010303 astronomy & astrophysicsDETECTORPhysicsMuon010308 nuclear & particles physicsDetectorMultiplicity (mathematics)LEPComputer Science ApplicationsDensity distributionKASCADE-GRANDEHigh Energy Physics::ExperimentEvent (particle physics)EMMA (Experiment with Multi-Muon Array)
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Performance of the First ANTARES Detector Line

2009

In this paper we report on the data recorded with the first Antares detector line. The line was deployed on the 14th of February 2006 and was connected to the readout two weeks later. Environmental data for one and a half years of running are shown. Measurements of atmospheric muons from data taken from selected runs during the first six months of operation are presented. Performance figures in terms of time residuals and angular resolution are given. Finally the angular distribution of atmospheric muons is presented and from this the depth profile of the muon intensity is derived.

MODULEPhysics::Instrumentation and DetectorsFOS: Physical sciencesAstrophysics01 natural sciencesNuclear physicsNEUTRINO TELESCOPESAngular distributionantares; deep-sea; first line; neutrino0103 physical sciencesNeutrino[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]WATERAngular resolutionNEUTRINO TELESCOPE010306 general physicsATMOSPHERIC MUONSAstroparticle physicsPhysicsMuonANTARES010308 nuclear & particles physicsAstrophysics (astro-ph)DetectorDeep-seaAstronomy and AstrophysicsTime resolutionGeodesyMUON FLUXFirst lineSINGLEFísica nuclearUNDERWATER DETECTORLine (text file)NeutrinoSYSTEM
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Direct measurement of the muonic content of extensive air showers between 2× 1017 and 2×1018 eV at the Pierre Auger Observatory

2020

The hybrid design of the Pierre Auger Observatory allows for the measurement of the properties of extensive air showers initiated by ultra-high energy cosmic rays with unprecedented precision. By using an array of prototype underground muon detectors, we have performed the first direct measurement, by the Auger Collaboration, of the muon content of air showers between 2 × 10 17 and 2 × 10 18 eV. We have studied the energy evolution of the attenuation-corrected muon density, and compared it to predictions from air shower simulations. The observed densities are found to be larger than those predicted by models. We quantify this discrepancy by combining the measurements from the muon detector …

Muon detector ultra-high energy cosmic raysmuonsUHE Cosmic Rays
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Implementation and performance of the third level muon trigger of the ATLAS experiment at LHC

2006

The trigger system of the ATLAS experiment at the LHC aims at a high selectivity in order to keep the full physics potential while reducing the 40 MHz initial event rate imposed by the LHC bunch crossing down to /spl sim/100 Hz, as required by the data acquisition system. Algorithms working in the final stage of the trigger environment (Event Filter) are implemented to run both in a "wrapped" mode (reconstructing tracks in the entire Muon Spectrometer) and in a "seeded" mode (according to a dedicated strategy that performs pattern recognition only in regions of the detector where trigger hypotheses have been produced at earlier stages). The working principles of the offline muon reconstruct…

Nuclear and High Energy PhysicsParticle physicsHLTPhysics::Instrumentation and DetectorsMuonReal-time computingevent filter01 natural sciencesData acquisitionAtlas (anatomy)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]medicineElectrical and Electronic EngineeringDiscrete event simulationDetectors and Experimental TechniquesPhysicsMuonsLarge Hadron Collider010308 nuclear & particles physicsEvent (computing)DetectorATLAS experimentMuons.ATLASTriggermedicine.anatomical_structureNuclear Energy and EngineeringFilter (video)Event Filter
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The neutron background of the XENON100 dark matter search experiment

2013

TheXENON100 experiment, installed underground at the LaboratoriNazionali del Gran Sasso, aims to directly detect dark matter in the form of weakly interacting massive particles (WIMPs) via their elastic scattering off xenon nuclei. This paper presents a study on the nuclear recoil background of the experiment, taking into account neutron backgrounds from (alpha, n) reactions and spontaneous fission due to natural radioactivity in the detector and shield materials, as well as muon-induced neutrons. Based on MonteCarlo simulations and using measured radioactive contaminations of all detector components, we predict the nuclear recoil backgrounds for the WIMP search results published by theXENO…

Nuclear and High Energy PhysicsParticle physicsLarge Underground Xenon experimentPhysics::Instrumentation and DetectorsDark matterGeant4Astrophysics::Cosmology and Extragalactic AstrophysicsWIMP Argon Programme01 natural sciencesNuclear physicsWIMPNuclear and High Energy Physics Neutron Background Dark Matter Search XENON TPC0103 physical sciencesNeutron[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNuclear ExperimentGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)ComputingMilieux_MISCELLANEOUSSpontaneous fissionPhysicsElastic scatteringFluxMuons010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsDetectorsWeakly interacting massive particlesHigh Energy Physics::ExperimentSimulation
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A fast algorithm for muon track reconstruction and its application to the ANTARES neutrino telescope.

2011

An algorithm is presented, that provides a fast and robust reconstruction of neutrino induced upward-going muons and a discrimination of these events from downward-going atmospheric muon background in data collected by the ANTARES neutrino telescope. The algorithm consists of a hit merging and hit selection procedure followed by fitting steps for a track hypothesis and a point-like light source. It is particularly well-suited for real time applications such as online monitoring and fast triggering of optical follow-up observations for multi-messenger studies. The performance of the algorithm is evaluated with Monte Carlo simulations and various distributions are compared with that obtained …

Optical telescopesAMANDASelection proceduresRobust reconstructionMonte Carlo methodAtmospheric muonsReal-time applicationNeutrino telescope01 natural sciencesHigh Energy Physics - ExperimentFast algorithmsHigh Energy Physics - Experiment (hep-ex)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsDetectorMonte Carlo SimulationMonte Carlo methodsComputer simulationLIGHTddc:540Física nuclearNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAlgorithmAlgorithmsFLUXOnline monitoring[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeFOS: Physical sciencesTrack reconstructionOptical telescopeNuclear physicsMuon tracks0103 physical sciencesAngular resolutionLight sources010306 general physicsOptical follow-upDETECTORInstrumentation and Methods for Astrophysics (astro-ph.IM)MuonANTARESneutrino telescope; track reconstruction010308 nuclear & particles physicsCharged particlesTrack (disk drive)track reconstructionAstronomy and Astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics - Data Analysis Statistics and ProbabilityFISICA APLICADAATMOSPHERIC NEUTRINOSNeutrino telescopesSYSTEMData Analysis Statistics and Probability (physics.data-an)
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"Table 1.3" of "Production of muons from heavy-flavour hadron decays at high transverse momentum in Pb-Pb collisions at $\sqrt{s_{\rm NN}}=5.02$ and …

2021

$p_{\rm T}$-differential yield of muons from heavy-flavour hadron decays at forward rapidity ($2.5 < y < 4$) for central (0--10%) Pb--Pb collisions at $\sqrt{s_{\rm NN}}=2.76$ TeV.

PB PB --> MUON X1/NEV DN/DPT/DY OF HEAVY FLAVOUR DECAY MUONS2760High Energy Physics::PhenomenologyHigh Energy Physics::ExperimentNuclear Experiment
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"Table 1.2" of "Production of muons from heavy-flavour hadron decays at high transverse momentum in Pb-Pb collisions at $\sqrt{s_{\rm NN}}=5.02$ and …

2021

$p_{\rm T}$-differential yield of muons from heavy-flavour hadron decays at forward rapidity ($2.5 < y < 4$) for peripheral (60--80%) Pb--Pb collisions at $\sqrt{s_{\rm NN}}=5.02$ TeV.

PB PB --> MUON X1/NEV DN/DPT/DY OF HEAVY FLAVOUR DECAY MUONSHigh Energy Physics::Phenomenology5020High Energy Physics::ExperimentNuclear Experiment
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"Table 1.1" of "Production of muons from heavy-flavour hadron decays at high transverse momentum in Pb-Pb collisions at $\sqrt{s_{\rm NN}}=5.02$ and …

2021

$p_{\rm T}$-differential yield of muons from heavy-flavour hadron decays at forward rapidity ($2.5 < y < 4$) for central (0--10%) and semi-central (20--40%) Pb--Pb collisions at $\sqrt{s_{\rm NN}}=5.02$ TeV.

PB PB --> MUON X1/NEV DN/DPT/DY OF HEAVY FLAVOUR DECAY MUONSHigh Energy Physics::Phenomenology5020High Energy Physics::ExperimentNuclear Experiment
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