Search results for "muon: atmosphere"

showing 3 items of 3 documents

EV-Scale Sterile Neutrino Search Using Eight Years of Atmospheric Muon Neutrino Data from the IceCube Neutrino Observatory

2020

Physical review letters 125(14), 141801 (1-11) (2020). doi:10.1103/PhysRevLett.125.141801

Sterile neutrinoPhysics::Instrumentation and DetectorsGeneral Physics and Astronomysterile [neutrino]01 natural sciencesCosmologyIceCubeHigh Energy Physics - ExperimentSubatomär fysikHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Astronomi astrofysik och kosmologiSubatomic PhysicsTOOLAstronomy Astrophysics and Cosmologyatmosphere [muon]Muon neutrinoPhysicsPhysicsoscillation [neutrino]Astrophysics::Instrumentation and Methods for Astrophysicshep-phneutrino: sterilemass difference [neutrino]ddc:muon: atmosphereobservatoryHigh Energy Physics - PhenomenologyPhysique des particules élémentairessignatureParticle physicsdata analysis methodScale (ratio)Astrophysics::High Energy Astrophysical Phenomenaneutrino: mass differenceFOS: Physical sciences530IceCube Neutrino Observatorystatistical analysis0103 physical sciencesOSCILLATIONSddc:530010306 general physicshep-exICEHigh Energy Physics::Phenomenologyneutrino: mixing angleCONVERSIONPhysics and AstronomyCOSMOLOGYHigh Energy Physics::Experimentneutrino: oscillationBAYESIAN-INFERENCEmixing angle [neutrino]experimental results
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Calibration of the underground muon detector of the Pierre Auger Observatory

2021

To obtain direct measurements of the muon content of extensive air showers with energy above $10^{16.5}$ eV, the Pierre Auger Observatory is currently being equipped with an underground muon detector (UMD), consisting of 219 10 $\mathrm{m^2}$-modules, each segmented into 64 scintillators coupled to silicon photomultipliers (SiPMs). Direct access to the shower muon content allows for the study of both of the composition of primary cosmic rays and of high-energy hadronic interactions in the forward direction. As the muon density can vary between tens of muons per m$^2$ close to the intersection of the shower axis with the ground to much less than one per m$^2$ when far away, the necessary bro…

muon: showersdata acquisitionPhysics::Instrumentation and DetectorsAstronomyDetector alignment and calibration methods (lasers sources particle-beams)primary [cosmic radiation]Particle detectors7. Clean energy01 natural sciencesEtc)030218 nuclear medicine & medical imaging0302 clinical medicinecalibration [detector]ObservatoryAPDsdetector: calibrationatmosphere [muon]InstrumentationPhoton detectors for UVshowers [muon]Mathematical PhysicsPhoton detectors for UV visible and IR photons (solid-state) (PIN diodes APDsSi-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc)Particle-beams)Physicsenergy: highdetector [muon]EBCCDsPhysicselectronicsSettore FIS/01 - Fisica SperimentalePhoton detectors for UV visible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc)Astrophysics::Instrumentation and Methods for AstrophysicsSourcesSi-PMTsdetector: alignmentAugermuon: atmosphereobservatorydensity [muon]G-APDshigh [energy]Particle detectorAstrophysics - Instrumentation and Methods for Astrophysicsatmosphere [showers]Detector alignment and calibration methods (lasers sourcesparticle-beams)FOS: Physical sciencesCosmic rayScintillatorParticle detectorVisible and IR photons (solid-state) (PIN diodes03 medical and health sciencesOpticsSilicon photomultipliermuon: density0103 physical sciencesCalibrationddc:530photomultiplier: silicon[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ddc:610High Energy PhysicsCMOS imagersInstrumentation and Methods for Astrophysics (astro-ph.IM)scintillation counterParticle detectors; Detector alignment and calibration methods (lasers sources particle-beams); Photon detectors for UV visible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc); Performance of High Energy Physics DetectorsPierre Auger ObservatoryMuonshowers: atmosphere010308 nuclear & particles physicsbusiness.industrymuon: detectorCCDscosmic radiation: primaryDetector alignment and calibration methods (lasersEMCCDsanalog-to-digital converterAPDs; CCDs; CMOS imagers; Detector alignment and calibration methods (lasers; EBCCDs; EMCCDs; Etc); G-APDs; Particle detectors; Particle-beams); Performance of High Energy Physics Detectors; Photon detectors for UV; Si-PMTs; Sources; Visible and IR photons (solid-state) (PIN diodesExperimental High Energy Physicssilicon [photomultiplier]Performance of High Energy Physics DetectorsHigh Energy Physics::Experimentphoton: detectorbusinessalignment [detector]RAIOS CÓSMICOSdetector [photon]astro-ph.IM
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Studies on the response of a water-Cherenkov detector of the Pierre Auger Observatory to atmospheric muons using an RPC hodoscope

2020

Extensive air showers, originating from ultra-high energy cosmic rays, have been successfully measured through the use of arrays of water-Cherenkov detectors (WCDs). Sophisticated analyses exploiting WCD data have made it possible to demonstrate that shower simulations, based on different hadronic-interaction models, cannot reproduce the observed number of muons at the ground. The accurate knowledge of the WCD response to muons is paramount in establishing the exact level of this discrepancy. In this work, we report on a study of the response of a WCD of the Pierre Auger Observatory to atmospheric muons performed with a hodoscope made of resistive plate chambers (RPCs), enabling us to selec…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsAstronomy01 natural sciences030218 nuclear medicine & medical imaginglaw.invention0302 clinical medicinelawObservatoryatmosphere [muon]Instrumentationphysics.ins-detMathematical PhysicsLarge detector-systems performancePhysicsInstrumentation et méthodes en physiquePerformance of high energy physics detectorsData reduction methods; Large detector systems for particle and astroparticle physics; Large detector-systems performance; Performance of high energy physics detectorsDetectorSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsresistive plate chamberInstrumentation and Detectors (physics.ins-det)trajectory [muon]Augerobservatorymuon: atmosphereAstrophysics - Instrumentation and Methods for AstrophysicsData reduction methodsatmosphere [showers]Cherenkov detectorairCherenkov counter: waterAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencesCosmic raymuon: trajectoryNuclear physics03 medical and health sciencesHodoscopeData reduction method0103 physical sciencesCalibrationHigh Energy Physicsddc:610cosmic radiation: UHE[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Instrumentation and Methods for Astrophysics (astro-ph.IM)ZenithCiencias ExactasPierre Auger Observatoryshowers: atmosphere010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physicswater [Cherenkov counter]hodoscopeFísicaAutres mathématiquesstabilitycalibrationData reduction methods Large detector systems for particle and astroparticle physics Large detector-systems performance Performance of High Energy Physics DetectorsExperimental High Energy PhysicsLarge detector systems for particle and astroparticle physicHigh Energy Physics::ExperimentRAIOS CÓSMICOSastro-ph.IM
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