Search results for "methods"

showing 10 items of 4526 documents

Magnetic field uniformity in neutron electric dipole moment experiments

2019

© 2019 American Physical Society. Magnetic-field uniformity is of the utmost importance in experiments to measure the electric dipole moment of the neutron. A general parametrization of the magnetic field in terms of harmonic polynomial modes is proposed, going beyond the linear-gradients approximation. We review the main undesirable effects of nonuniformities: depolarization of ultracold neutrons and Larmor frequency shifts of neutrons and mercury atoms. The theoretical predictions for these effects were verified by dedicated measurements with the single-chamber neutron electric-dipole-moment apparatus installed at the Paul Scherrer Institute. ispartof: Physical Review A vol:99 issue:4 sta…

Physics - Instrumentation and DetectorsNeutron electric dipole momentmercury: atommeasurement methodsFOS: Physical sciencesHarmonic polynomial01 natural sciences7. Clean energyHigh Energy Physics - Experiment010305 fluids & plasmasHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]NeutronPhysics::Atomic Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNuclear ExperimentFundamental conceptsQCPhysicsLarmor precessionMeasurement methodn: electric momentn: depolarizationmathematical methodsInstrumentation and Detectors (physics.ins-det)Magnetic fieldComputational physicsElectric dipole momentmagnetic field: parametrizationUltracold neutrons
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Enhanced effects of variation of the fundamental constants in laser interferometers and application to dark matter detection

2015

We outline new laser interferometer measurements to search for variation of the electromagnetic fine-structure constant $\alpha$ and particle masses (including a non-zero photon mass). We propose a strontium optical lattice clock -- silicon single-crystal cavity interferometer as a novel small-scale platform for these new measurements. Multiple passages of a light beam inside an interferometer enhance the effects due to variation of the fundamental constants by the mean number of passages ($N_{\textrm{eff}} \sim 10^2$ for a large-scale gravitational-wave detector, such as LIGO, Virgo, GEO600 or TAMA300, while $N_{\textrm{eff}} \sim 10^5$ for a strontium clock -- silicon cavity interferomete…

Physics - Instrumentation and DetectorsPhotonField (physics)Atomic Physics (physics.atom-ph)Dark matterPhysics::OpticsFOS: Physical sciences01 natural sciencesPhysics - Atomic Physicslaw.inventionOpticsHigh Energy Physics - Phenomenology (hep-ph)law0103 physical sciencesAstronomical interferometer010306 general physicsPhysics010308 nuclear & particles physicsbusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)LaserGEO600LIGOHigh Energy Physics - PhenomenologyInterferometrybusinessPhysics - OpticsOptics (physics.optics)
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Material radioassay and selection for the XENON1T dark matter experiment

2017

The XENON1T dark matter experiment aims to detect weakly interacting massive particles (WIMPs) through low-energy interactions with xenon atoms. To detect such a rare event necessitates the use of radiopure materials to minimize the number of background events within the expected WIMP signal region. In this paper we report the results of an extensive material radioassay campaign for the XENON1T experiment. Using gamma-ray spectroscopy and mass spectrometry techniques, systematic measurements of trace radioactive impurities in over one hundred samples within a wide range of materials were performed. The measured activities allowed for stringent selection and placement of materials during the…

Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsDark matterMonte Carlo methodmeasurement methodsFOS: Physical scienceschemistry.chemical_elementRadiopuritylcsh:AstrophysicsWIMP: detectorSciences de l'ingénieur01 natural sciencesgamma ray: energy spectrumNuclear physicsmass spectrumXENONXenonWIMPlcsh:QB460-4660103 physical sciencesDark Matterlcsh:Nuclear and particle physics. Atomic energy. Radioactivity[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsSpectroscopy[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Engineering (miscellaneous)background: radioactivityPhysicsRange (particle radiation)Physique010308 nuclear & particles physicsDetectorInstrumentation and Detectors (physics.ins-det)AstronomiesensitivitychemistryWeakly interacting massive particleslcsh:QC770-798TPCnumerical calculations: Monte Carlo
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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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Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory

2021

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargue. We are very grateful to the following agencies and organizations for financial support: Argentina -Comision Nacional de Energia Atomica; Agencia Nacional de Promocion Cientifica y Tecnologica (ANPCyT); Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET); Gobierno de la Provincia de Mendoza; Municipalidad de Malargue; NDM Holdings and Valle Las Lenas; in gratitude for their continuing cooperation over land access; Australia -the Australian Research Council; Braz…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsAstronomyPerformance of High Energy Physics Detector01 natural sciences7. Clean energyEtc)030218 nuclear medicine & medical imaging0302 clinical medicineFront-end electronics for detector readoutAPDsInstrumentationphysics.ins-detPhoton detectors for UVMathematical PhysicsInstrumentation et méthodes en physiqueEBCCDsVisible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc)electronicsSettore FIS/01 - Fisica SperimentaleCalibration and fitting methods; Performance of High Energy Physics Detectors; Photon detectors for UVPhoton 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 AstrophysicsSi-PMTsInstrumentation and Detectors (physics.ins-det)charged particleAPDs; Calibration and fitting methods; Performance of High Energy Physics Detectors; Photon detectors for UV; CCDs; Cluster finding; CMOS imagers; EBCCDs; EMCCDs; Etc); Front-end electronics for detector readout; Pattern recognition; G-APDs; Si-PMTs; Visible and IR photons (solid-state) (PIN diodesAugerobservatorydensity [muon]Pattern recognition cluster finding calibration and fitting methodG-APDsChristian ministryupgradeddc:620Astrophysics - Instrumentation and Methods for Astrophysicsperformanceatmosphere [showers]Land accessCherenkov counter: waterairAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencesVisible and IR photons (solid-state) (PIN diodes03 medical and health sciencesPolitical sciencePattern recognition0103 physical sciencesmuon: densityFront-end electronics for detector readout; Pattern recognitionphotomultiplier: siliconHigh Energy Physicscosmic radiation: UHE[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ddc:610CMOS imagersInstrumentation and Methods for Astrophysics (astro-ph.IM)Engineering & allied operationsscintillation counterCalibration and fitting methodsshowers: atmosphere010308 nuclear & particles physicswater [Cherenkov counter]Cluster findingAutres mathématiquesCCDsEMCCDsResearch councilefficiencyExperimental High Energy Physicssilicon [photomultiplier]Performance of High Energy Physics DetectorsHigh Energy Physics::ExperimentHumanitiesRAIOS CÓSMICOSastro-ph.IM
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The analog Resistive Plate Chamber detector of the ARGO-YBJ experiment

2015

The ARGO-YBJ experiment has been in stable data taking from November 2007 till February 2013 at the YangBaJing Cosmic Ray Observatory (4300 m a.s.l.). The detector consists of a single layer of Resistive Plate Chambers (RPCs) (6700 m2) operated in streamer mode. The signal pick-up is obtained by means of strips facing one side of the gas volume. The digital readout of the signals, while allows a high space–time resolution in the shower front reconstruction, limits the measurable energy to a few hundred TeV. In order to fully investigate the 1–10 PeV region, an analog readout has been implemented by instrumenting each RPC with two large size electrodes facing the other side of the gas volume…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAir shower detectionFOS: Physical sciencesCosmic raySTRIPSCalorimetrySignallaw.inventionOpticsObservatorylawAir shower detection RPC detector CalorimetryCosmic-ray observatoryphysics.ins-detInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsResistive touchscreenbusiness.industryDetectorSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)Core (optical fiber)RPC detectorbusinessAstrophysics - Instrumentation and Methods for Astrophysicsastro-ph.IM
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Results from a calibration of XENON100 using a source of dissolved radon-220

2017

A Rn 220 source is deployed on the XENON100 dark matter detector in order to address the challenges in calibration of tonne-scale liquid noble element detectors. We show that the Pb 212 beta emission can be used for low-energy electronic recoil calibration in searches for dark matter. The isotope spreads throughout the entire active region of the detector, and its activity naturally decays below background level within a week after the source is closed. We find no increase in the activity of the troublesome Rn 222 background after calibration. Alpha emitters are also distributed throughout the detector and facilitate calibration of its response to Rn 222 . Using the delayed coincidence of R…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsDark matterFOS: Physical scienceschemistry.chemical_elementRadon01 natural sciencesCoincidenceNuclear physicsRecoilOpticsXenonXENON DARK MATTER WIMPS CALIBRATION RADON0103 physical sciencesCalibration[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsPhysics010308 nuclear & particles physicsbusiness.industryDetectorAstrophysics::Instrumentation and Methods for AstrophysicsOrder (ring theory)Instrumentation and Detectors (physics.ins-det)chemistryHigh Energy Physics::Experimentbusiness
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Absolute momentum calibration of the HARP TPC

2008

In the HARP experiment the large-angle spectrometer is using a cylindrical TPC as main tracking and particle identification detector. The momentum scale of reconstructed tracks in the TPC is the most important systematic error for the majority of kinematic bins used for the HARP measurements of the double-differential production cross-section of charged pions in proton interactions on nuclear targets at large angle. The HARP TPC operated with a number of hardware shortfalls and operational mistakes. Thus it was important to control and characterize its momentum calibration. While it was not possible to enter a direct particle beam into the sensitive volume of the TPC to calibrate the detect…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsTime projection chambersFOS: Physical sciencesDetector alignment and calibration methods (laserssources particle-beams)ddc:500.2Tracking (particle physics)01 natural sciencesParticle detectorParticle identificationNuclear physics0103 physical sciencesCalibration[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Detector alignment and calibration methodsDetectors and Experimental Techniques010306 general physicsNuclear ExperimentInstrumentationMathematical PhysicsHARPPhysicsMomentum (technical analysis)Spectrometer010308 nuclear & particles physicsDetectorSettore FIS/01 - Fisica SperimentaleFísicaInstrumentation and Detectors (physics.ins-det)Settore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)
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DARWIN: Towards the ultimate dark matter detector

2016

DARk matter WImp search with liquid xenoN (DARWIN) will be an experiment for the direct detection of dark matter using a multi-ton liquid xenon time projection chamber at its core. Its primary goal will be to explore the experimentally accessible parameter space for Weakly Interacting Massive Particles (WIMPs) in a wide mass-range, until neutrino interactions with the target become an irreducible background. The prompt scintillation light and the charge signals induced by particle interactions in the xenon will be observed by VUV sensitive, ultra-low background photosensors. Besides its excellent sensitivity to WIMPs above a mass of 5 GeV/c2, such a detector with its large mass, low-energy …

Physics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsdouble beta decay7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentPhysics Particles & FieldsNeutrino detectorHigh Energy Physics - Experiment (hep-ex)XenonWIMPPHOTOMULTIPLIERAXIONSphysics.ins-detsolar and atmospheric neutrinosPhysicsDark matter detectorTime projection chamberdark matter detectorsPhysicsSolar and atmospheric neutrinoInstrumentation and Detectors (physics.ins-det)Nuclear & Particles PhysicsNeutrino detectorSOLAR NEUTRINOSGASPhysical SciencesNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsGRAN SASSODark matter detectors; Double beta decay; Neutrino detectors; Solar and atmospheric neutrinosDark matterchemistry.chemical_elementFOS: Physical sciencesAstronomy & AstrophysicsLIQUID-XENON DETECTOR0202 Atomic Molecular Nuclear Particle And Plasma PhysicsSettore FIS/05 - Astronomia e AstrofisicaSEARCH0103 physical sciencesIsotopes of xenonZEPLIN-III[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsAxionInstrumentation and Methods for Astrophysics (astro-ph.IM)Science & Technology010308 nuclear & particles physicshep-exAstronomyAstronomy and Astrophysics0201 Astronomical And Space ScienceschemistryHigh Energy Physics::ExperimentSCINTILLATIONneutrino detectorsastro-ph.IMJournal of Cosmology and Astroparticle Physics
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Mini-MALTA: Radiation hard pixel designs for small-electrode monolithic CMOS sensors for the High Luminosity LHC

2020

Journal of Instrumentation 15(02), P02005 (2020). doi:10.1088/1748-0221/15/02/P02005

Physics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsirradiation [n]measurement methods01 natural sciencesdamage [radiation]High Energy Physics - Experimentdesign [semiconductor detector]High Energy Physics - Experiment (hep-ex)n: irradiationupgrade [ATLAS][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Detectors and Experimental TechniquesInstrumentationRadiation hardeningphysics.ins-detMathematical PhysicsFront-end electronics for detector readout ; Particle tracking detectors (Solid-state detectors) ; Radiation-hard detectors ; Solid state detectorsradiation: damageSolid State DetectorsCMOS sensorLarge Hadron Colliderpixel: sizeInstrumentation and Detectors (physics.ins-det)CMOSOptoelectronicsParticle Physics - ExperimentperformancenoiseMaterials science610FOS: Physical sciencesContext (language use)Radiation-hard DetectorsNovel high voltage and resistive CMOS sensors [6]Front-end Electronics for Detector ReadoutRadiationCapacitanceRadiation-hard detectorsemiconductor detector: pixelsize [pixel]electrode: design0103 physical sciencesParticle Tracking Detectors (Solid-state Detectors)ddc:610[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsdesign [electrode]pixel [semiconductor detector]Pixel010308 nuclear & particles physicsbusiness.industryhep-exATLAS: upgradeefficiencyelectronics: readoutbusinessreadout [electronics]semiconductor detector: design
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