Search results for " Detectors"

showing 10 items of 2027 documents

The ATLAS Simulation Infrastructure

2010

52 páginas, 10 figuras, 18 tablas.-- This article is distributed under the terms of the Creative Commons Attribution Noncommercial License.-- et al. (The ATLAS Collaboration).

LibraryPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and Detectorscomputer.software_genre01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Statistical physicsDetectors and Experimental TechniquesSimulaciónphysics.ins-detDetectors de radiació/dk/atira/pure/subjectarea/asjc/2200/2201PhysicsLarge Hadron ColliderAtlas (topology)4. EducationAcceleradors de partículesATLAS experimentDetectorSettore FIS/01 - Fisica SperimentaleInstrumentation and Detectors (physics.ins-det)ATLASGridSimulation softwareTile CalorimeterPhysical SciencesMontecarlo simulationLHCReal-time computingFOS: Physical sciencesATLAS experimentddc:500.2530High-Energy Physics0103 physical sciencesFysikddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]High Energy PhysicsMonte-Carlo010306 general physicsPartonEngineering (miscellaneous)Ciencias ExactasGEANT4EventATLAS detector010308 nuclear & particles physicsFísicaATLAS experiment; Montecarlo simulation; LHCGrid computingInterfacingHigh Energy Physics::Experiment/dk/atira/pure/subjectarea/asjc/3100/3101computer
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Light Dark Matter Search with Ionization Signals in XENON1T

2019

We report constraints on light dark matter (DM) models using ionization signals in the XENON1T experiment. We mitigate backgrounds with strong event selections, rather than requiring a scintillation signal, leaving an effective exposure of (22±3) tonne day. Above ∼0.4 keVee, we observe <1 event/(tonne day keVee), which is more than 1000 times lower than in similar searches with other detectors. Despite observing a higher rate at lower energies, no DM or CEvNS detection may be claimed because we cannot model all of our backgrounds. We thus exclude new regions in the parameter spaces for DM-nucleus scattering for DM masses mχ within 3–6 GeV/c2, DM-electron scattering for mχ>30 MeV/c2, a…

Light Dark Matter TPC Ionization Axion-Like particlesCosmology and Nongalactic Astrophysics (astro-ph.CO)PhotonFOS: Physical sciencesGeneral Physics and AstronomyS030DI5S029AECAstrophysics01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)S030DE5Ionization0103 physical sciencesionization[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsAbsorption (electromagnetic radiation)Light dark matterscintillation counterPhysicsDark Matter WIMP Dark-Matter detectors Time-projection chamber detectorsScintillationScatteringbackgrounddark matter: massphotonscatteringS029HPHS030DN5* Automatic Keywords *Scintillation counterElementary Particles and Fieldsaxion-like particles[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Event (particle physics)absorptionAstrophysics - Cosmology and Nongalactic Astrophysics
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The Design and Sensitivity of JUNO's scintillator radiopurity pre-detector OSIRIS

2021

The European physical journal / C 81(11), 973 (2021). doi:10.1140/epjc/s10052-021-09544-4

Liquid scintillatorPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and Detectorsscintillation counter: liquidmeasurement methodsQC770-798Astrophysics01 natural sciencesthorium: nuclidedesign [detector]neutrinoRadioactive purityPhysicsLow energy neutrinoJUNOliquid [scintillation counter]biologySettore FIS/01 - Fisica SperimentaleDetectorInstrumentation and Detectors (physics.ins-det)3. Good healthQB460-466Physics::Space Physicsnuclide [uranium]FOS: Physical sciencesScintillatornuclide [thorium]530NONuclear physicsPE2_2uranium: nuclideNuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesddc:530Sensitivity (control systems)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsJUNO neutrino physics liquid scintillatorEngineering (miscellaneous)background: radioactivitydetector: designMeasurement method010308 nuclear & particles physicsradioactivity [background]biology.organism_classificationsensitivityHigh Energy Physics::ExperimentReactor neutrinoOsiris
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Precise measurement of $2\nu\beta\beta$ decay of $^{100}$Mo with the CUPID-Mo detection technology

2020

We report the measurement of the two-neutrino double-beta ($2\nu\beta\beta$) decay of $^{100}$Mo to the ground state of $^{100}$Ru using lithium molybdate (\crystal) scintillating bolometers. The detectors were developed for the CUPID-Mo program and operated at the EDELWEISS-III low background facility in the Modane underground laboratory. From a total exposure of $42.235$ kg$\times$d, the half-life of $^{100}$Mo is determined to be $T_{1/2}^{2\nu}=[7.12^{+0.18}_{-0.14}\,\mathrm{(stat.)}\pm0.10\,\mathrm{(syst.)}]\times10^{18}$ years. This is the most accurate determination of the $2\nu\beta\beta$ half-life of $^{100}$Mo to date. We also confirm, with the statistical significance of $>3\sigm…

Lithium molybdatePhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Analytical chemistry[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]nucl-ex01 natural sciencesAtomicchemistry.chemical_compoundParticle and Plasma Physicstwo-neutrino double-beta decay scintillating bolometers0103 physical sciencesddc:530Beta (velocity)Nuclear[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNuclear ExperimentEngineering (miscellaneous)physics.ins-detS076H2NPhysicsQuantum Physics010308 nuclear & particles physicsPhysicsMolecularBeta decayNuclear & Particles Physics3. Good healthchemistrydouble beta decays bolometersUnderground laboratoryGround state
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Characterization of a medium size Xe/TMA TPC instrumented with microbulk Micromegas, using low-energy gamma-rays

2014

NEXT-MM is a general-purpose high pressure (10 bar, $\sim25$ l active volume) Xenon-based TPC, read out in charge mode with an 8 cm $\times$8 cm-segmented 700 cm$^2$ plane (1152 ch) of the latest microbulk-Micromegas technology. It has been recently commissioned at University of Zaragoza as part of the R&D of the NEXT $0\nu\beta\beta$ experiment, although the experiment's first stage is currently being built based on a SiPM/PMT-readout concept relying on electroluminescence. Around 2 million events were collected during the last months, stemming from the low energy $\gamma$-rays emitted by a $^{241}$Am source when interacting with the Xenon gas ($\epsilon$ = 26, 30, 59.5 keV). The localized…

MECANICA DE LOS MEDIOS CONTINUOS Y TEORIA DE ESTRUCTURASDrift velocityPhysics - Instrumentation and DetectorsXenonTime projection chambersDouble-beta decayNuclear physicschemistry.chemical_element01 natural sciencesMicrobulkNuclear physicsTECNOLOGIA ELECTRONICASilicon photomultiplierXenon0103 physical sciencesTrimethylamineDiffusion (business)010306 general physicsInstrumentationMathematical PhysicsDetectors de radiacióPhysicsAtmospheric pressure010308 nuclear & particles physicsGamma rayMicroMegas detectorHigh pressurechemistryTime projection chamberNuclear countersFísica nuclearMicromegasBar (unit)
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Present Status and Future Perspectives of the NEXT Experiment

2014

Gómez Cadenas, Juan José et al.

MECANICA DE LOS MEDIOS CONTINUOS Y TEORIA DE ESTRUCTURASNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsArticle SubjectDouble beta decay experimentchemistry.chemical_elementFOS: Physical sciencesNEXT7. Clean energy01 natural sciencesSignalMathematical SciencesTECNOLOGIA ELECTRONICANuclear physicsXenonDouble beta decay0103 physical sciences010306 general physicsphysics.ins-detPhysicsTime projection chamberIsotope010308 nuclear & particles physicsDetectorInstrumentation and Detectors (physics.ins-det)lcsh:QC1-999chemistryPhysical SciencesFísica nuclearlcsh:PhysicsEnergy (signal processing)
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NEXT-100 Technical Design Report (TDR). Executive summary

2012

[EN] In this Technical Design Report (TDR) we describe the NEXT-100 detector that will search for neutrinoless double beta decay (ßß0v) in 136XE at the Laboratorio Subterráneo de Canfranc (LSC), in Spain. The document formalizes the design presented in our Conceptual Design Report (CDR): an electroluminescence time projection chamber, with separate readout planes for calorimetry and tracking, located, respectively, behind cathode and anode. The detector is designed to hold a maximum of about 150 kg of xenon at 15 bar, or 100 kg at 10 bar. This option builds in the capability to increase the total isotope mass by 50% while keeping the operating pressure at a manageable level. The readout pla…

MECANICA DE LOS MEDIOS CONTINUOS Y TEORIA DE ESTRUCTURASPhotomultiplierPhysics - Instrumentation and DetectorsBar (music)Time projection chambersFOS: Physical scienceschemistry.chemical_elementWavelength shifterTracking (particle physics)7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentTECNOLOGIA ELECTRONICAHigh Energy Physics - Experiment (hep-ex)chemistry.chemical_compoundXenonOptics0103 physical sciences010306 general physicsInstrumentationMathematical PhysicsPhysicsTime projection chamber010308 nuclear & particles physicsbusiness.industryDetectorFísicaTetraphenyl butadieneDetectorsInstrumentation and Detectors (physics.ins-det)Gas detectorsDetectors de gasoschemistryDetector design and construction technologies and materialsbusinessJournal of Instrumentation
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Initial results of NEXT-DEMO, a large-scale prototype of the NEXT-100 experiment

2013

NEXT-DEMO is a large-scale prototype of the NEXT-100 detector, an electroluminescent time projection chamber that will search for the neutrinoless double beta decay of Xe-136 using 100-150 kg of enriched xenon gas. NEXT-DEMO was built to prove the expected performance of NEXT-100, namely, energy resolution better than 1% FWHM at 2.5MeV and event topological reconstruction. In this paper we describe the prototype and its initial results. A resolution of 1.75% FWHM at 511 keV (which extrapolates to 0.8% FWHM at 2.5 MeV) was obtained at 10 bar pressure using a gamma-ray calibration source. Also, a basic study of the event topology along the longitudinal coordinate is presented, proving that it…

MECANICA DE LOS MEDIOS CONTINUOS Y TEORIA DE ESTRUCTURASPhysics - Instrumentation and DetectorsBar (music)Isòtops radioactius -- DesintegracióTime projection chambersPattern recognition SystemsFOS: Physical scienceschemistry.chemical_elementElectron7. Clean energy01 natural sciencesNuclear physicsTECNOLOGIA ELECTRONICAXenonCambres d'ionitzacióCluster analysisDouble beta decayPattern recognition0103 physical sciencesCalibrationReconeixement de formes (Informàtica)Calibratge010306 general physicsInstrumentationMathematical PhysicsRadioisotopes -- DecayPhysicsCalibration and fitting methodsTime projection chamber010308 nuclear & particles physicsDetectorCluster findingFísicaInstrumentation and Detectors (physics.ins-det)Double-beta decay detectorsAnàlisi de conglomeratschemistryCalibrationEvent (particle physics)Ionization Chambers
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Radiopurity control in the NEXT-100 double beta decay experiment: procedures and initial measurements

2013

[EN] The "Neutrino Experiment with a Xenon Time-Projection Chamber" (NEXT) is intended to investigate the neutrinoless double beta decay of Xe-136, which requires a severe suppression of potential backgrounds. An extensive screening and material selection process is underway for NEXT since the control of the radiopurity levels of the materials to be used in the experimental set-up is a must for rare event searches. First measurements based on Glow Discharge Mass Spectrometry and gamma-ray spectroscopy using ultra-low background germanium detectors at the Laboratorio Subterraneo de Canfranc (Spain) are described here. Activity results for natural radioactive chains and other common radionucl…

MECANICA DE LOS MEDIOS CONTINUOS Y TEORIA DE ESTRUCTURASPhysics - Instrumentation and DetectorsGlow Discharge Mass SpectrometryPhysics::Instrumentation and Detectorschemistry.chemical_elementFOS: Physical sciencesGermanium01 natural sciences7. Clean energyTECNOLOGIA ELECTRONICANuclear physicsCambres d'ionitzacióXenonDouble beta decay0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentInstrumentationDetectors de radiacióMathematical PhysicsPhysicsRadionuclideRadiation calculationsIonization chambers010308 nuclear & particles physicsTime projection Chambers (TPC)Gamma detectors (scintillators CZT HPG HgI etc)FísicaInstrumentation and Detectors (physics.ins-det)chemistryNuclear countersNeutrino
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Conceptual design of the International Axion Observatory (IAXO)

2014

The International Axion Observatory (IAXO) will be a forth generation axion helioscope. As its primary physics goal, IAXO will look for axions or axion-like particles (ALPs) originating in the Sun via the Primakoff conversion of the solar plasma photons. In terms of signal-to-noise ratio, IAXO will be about 4-5 orders of magnitude more sensitive than CAST, currently the most powerful axion helioscope, reaching sensitivity to axion-photon couplings down to a few $\times 10^{-12}$ GeV$^{-1}$ and thus probing a large fraction of the currently unexplored axion and ALP parameter space. IAXO will also be sensitive to solar axions produced by mechanisms mediated by the axion-electron coupling $g_{…

MICROPICPhysics - Instrumentation and DetectorsPhotonaxionsParameter space7. Clean energyHigh Energy Physics - ExperimentDark Matter detectors (WIMPs axions etc.)High Energy Physics - Experiment (hep-ex)Observatoryetc.)Micropattern gaseous detectors (MSGC GEM THGEM RETHGEM MHSP MICROPIC MICROMEGAS InGrid etc)Detectors and Experimental TechniquesInstrumentationMathematical PhysicsPhysicsGEMsolar [axion]Dark Matter Detectors (Wimps Axions etc.)MicroMegas detectorX-ray detectorsInstrumentation and Detectors (physics.ins-det)Dark Matter detectors (WIMPs axions etc.); Large detector systems for particle and astroparticle physics; Micropattern gaseous detectors (MSGC GEM THGEM RETHGEM MHSP MICROPIC MICROMEGAS InGrid etc); X-ray detectors; Instrumentation; Mathematical PhysicssolarobservatoryMICROMEGASMHSPaxion-like particlesproposed experimentaxions ; dark matter detectors ; x-ray detectors ; Micropattern gaseous detectors ; large detector systems for particle and astroparticle physicsMicromegasX-ray detectorParticle physicsoptics [X-ray]FOS: Physical sciencesSuperconducting magnetMicropattern gaseous detectors (MSGCddc:610Axionactivity reportDark Matter detectors (WIMPssuperconductivity [magnet]etc)HelioscopeLarge detector systems for particle and astroparticle physicssensitivityInGridRETHGEMOrders of magnitude (time)axionLarge detector systems for particle and astroparticle physicTHGEMMicropattern Gaseous Detectors (MSGC Gem THGEM Rethgem MHSP Micropic Micromegas In Grid; etc)
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