Search results for " Instrumentation."

showing 10 items of 712 documents

Twin GEM-TPC prototype (HGB4) beam test at GSI and Jyväskylä : a development for the Super-FRS at FAIR

2017

The FAIR[1] facility is an international accelerator centre for research with ion and antiproton beams. It is being built at Darmstadt, Germany as an extension to the current GSI research institute. One major part of the facility will be the Super-FRS[2] separator, which will be include in phase one of the project construction. The NUSTAR experiments will benefit from the Super-FRS, which will deliver an unprecedented range of radioactive ion beams (RIB). These experiments will use beams of different energies and characteristics in three different branches; the high-energy which utilizes the RIB at relativistic energies 300-1500 MeV/u as created in the production process, the low-energy bra…

Radioactive ion beamsPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsSeparator (oil production)hiukkaskiihdyttimet01 natural sciences7. Clean energy114 Physical sciencesParticle identificationNuclear physics0103 physical sciencesElectronicsNuclear ExperimentdetectorsPhysicsta114010308 nuclear & particles physicsProjectileI.2.7Detectorparticle acceleratorsilmaisimetAntiprotonPhysics::Accelerator PhysicsF.2.2Beam (structure)
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Radon and material radiopurity assessment for the NEXT double beta decay experiment

2015

Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAM

Radon mitigationPhysics - Instrumentation and DetectorsNuclear engineeringchemistry.chemical_elementFOS: Physical sciencesRadon7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)XenonCambres d'ionitzacióDouble beta decayGamma detectors (HPGe)0103 physical sciencesGamma spectroscopyNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentDetectors de radiació010308 nuclear & particles physicsIonization chambersCanfranc Underground LaboratoryMaterial radiopurityFísicaTime-Projection Chamber (TPC)Instrumentation and Detectors (physics.ins-det)Double beta decaySemiconductor detectorchemistry13. Climate actionNuclear countersEnvironmental scienceNeutrino
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TASISpec—A highly efficient multi-coincidence spectrometer for nuclear structure investigations of the heaviest nuclei

2010

TASISpec (TASCA in Small Image mode Spectroscopy) combines composite Ge- and Si-detectors for a new detector setup aimed towards multi-coincidence gamma -ray, X-ray, conversion electron, fission fragment, and a-particle spectroscopy of the heaviest nuclei. It exploits the TASCA separator's unique small image focal mode, i.e. the fact that evaporation residues produced in fusion-evaporation reactions can be focused into an area of less than 3 cm in diameter. This provides the possibility to pack detectors in very close geometry, resulting in an unprecedented detection efficiency of radioactive decays in prompt and delayed coincidence with implanted nuclei. Crown Copyright (C) 2010 Publis…

Recoil separatorsNuclear and High Energy PhysicsalphaFissionElectronandAccelerator Physics and Instrumentationconversion electronNuclear physicsImage modespectroscopy at recoil separatorsgamma-rayNuclear ExperimentSpectroscopyClover Ge detectorInstrumentationSpontaneous fissionPhysicsdetectorSpectrometerDetectorGamma rayDecay tagging spectrometerCluster Ge detectorSi stripAtomic physicsNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Dichroic atomic vapor laser lock with multi-gigahertz stabilization range

2016

A dichroic atomic vapor laser lock (DAVLL) system exploiting buffer-gas-filled millimeter-scale vapor cells is presented. This system offers similar stability as achievable with conventional DAVLL system using bulk vapor cells, but has several important advantages. In addition to its compactness, it may provide continuous stabilization in a multi-gigahertz range around the optical transition. This range may be controlled either by changing the temperature of the vapor or by application of a buffer gas under an appropriate pressure. In particular, we experimentally demonstrate the ability of the system to lock the laser frequency between two hyperfine components of the $^{85}$Rb ground state…

Record lockingMaterials sciencePhysics - Instrumentation and DetectorsAtomic Physics (physics.atom-ph)Buffer gasFOS: Physical sciencesDichroic glass01 natural sciencesphysics.atom-phlaw.inventionPhysics - Atomic Physics010309 opticsEngineeringlaw0103 physical sciencesPhysics::Atomic Physics010306 general physicsInstrumentationHyperfine structurephysics.ins-detApplied PhysicsRange (particle radiation)business.industryInstrumentation and Detectors (physics.ins-det)LaserAtomic vaporPhysical SciencesChemical SciencesOptoelectronicsphysics.opticsGround statebusinessPhysics - OpticsOptics (physics.optics)
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XENON100 dark matter results from a combination of 477 live days

2016

We report on WIMP search results of the XENON100 experiment, combining three runs summing up to 477 live days from January 2010 to January 2014. Data from the first two runs were already published. A blind analysis was applied to the last run recorded between April 2013 and January 2014 prior to combining the results. The ultra-low electromagnetic background of the experiment, ~$5 \times 10^{-3}$ events/(keV$_{\mathrm{ee}}\times$kg$\times$day) before electronic recoil rejection, together with the increased exposure of 48 kg $\times$ yr improves the sensitivity. A profile likelihood analysis using an energy range of (6.6 - 43.3) keV$_{\mathrm{nr}}$ sets a limit on the elastic, spin-independe…

Scattering cross-sectionPhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsProton010308 nuclear & particles physicsDark matterFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)01 natural sciences7. Clean energyXENON DARK MATTER WIMP TPCNuclear physicsRecoilWIMPLikelihood analysis0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Sensitivity (control systems)010306 general physicsEnergy (signal processing)Astrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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Energy and time resolution for a LYSO matrix prototype of the Mu2e experiment

2016

We have measured the performances of a LYSO crystal matrix prototype tested with electron and photon beams in the energy range 60$-$450 MeV. This study has been carried out to determine the achievable energy and time resolutions for the calorimeter of the Mu2e experiment.

Scintillating crystalNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsFOS: Physical sciencesElectronCalorimetry01 natural sciencesLyso-High Energy Physics - ExperimentNuclear physicsMatrix (mathematics)High Energy Physics - Experiment (hep-ex)Optics0103 physical sciencesMu2eInstrumentationNuclear and High Energy Physic010302 applied physicsPhysicsRange (particle radiation)Calorimeter (particle physics)010308 nuclear & particles physicsbusiness.industryAvalanche photodiodeInstrumentation and Detectors (physics.ins-det)Avalanche photodiodePhysics::Accelerator PhysicsbusinessEnergy (signal processing)
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Ionization and scintillation response of high-pressure xenon gas to alpha particles

2013

High-pressure xenon gas is an attractive detection medium for a variety of applications in fundamental and applied physics. In this paper we study the ionization and scintillation detection properties of xenon gas at 10 bar pressure. For this purpose, we use a source of alpha particles in the NEXT-DEMO time projection chamber, the large scale prototype of the NEXT-100 neutrinoless double beta decay experiment, in three different drift electric field configurations. We measure the ionization electron drift velocity and longitudinal diffusion, and compare our results to expectations based on available electron scattering cross sections on pure xenon. In addition, two types of measurements add…

Scintillation (physics)IonizationMECANICA DE LOS MEDIOS CONTINUOS Y TEORIA DE ESTRUCTURASPhysics - Instrumentation and DetectorsMaterials scienceIonitzacióPhysics::Instrumentation and DetectorsFOS: Physical scienceschemistry.chemical_elementElectronCharge transportNuclear excitation01 natural sciences7. Clean energyHigh Energy Physics - ExperimentTECNOLOGIA ELECTRONICAHigh Energy Physics - Experiment (hep-ex)Gaseous detectorsXenonComptadors de centelleigIonization and excitation processesIonization0103 physical sciencesPhysics::Atomic and Molecular ClustersNuclear Experiment (nucl-ex)010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Nuclear ExperimentInstrumentationMathematical PhysicsHeliumDetectors de radiacióScintillationTime projection chamber010308 nuclear & particles physicsFísicaMultiplication and electroluminescence in rare gases and liquidsInstrumentation and Detectors (physics.ins-det)Alpha particleDouble-beta decay detectorschemistryNuclear countersScintillation counterExcitació nuclearAtomic physicsAstrophysics - Instrumentation and Methods for Astrophysics
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Improved Upper Limit on the Neutrino Mass from a Direct Kinematic Method by KATRIN

2019

We report on the neutrino mass measurement result from the first four-week science run of the Karlsruhe Tritium Neutrino experiment KATRIN in spring 2019. Beta-decay electrons from a high-purity gaseous molecular tritium source are energy analyzed by a high-resolution MAC-E filter. A fit of the integrated electron spectrum over a narrow interval around the kinematic end point at 18.57 keV gives an effective neutrino mass square value of (−1.0−1.1+0.9) eV2. From this, we derive an upper limit of 1.1 eV (90% confidence level) on the absolute mass scale of neutrinos. This value coincides with the KATRIN sensitivity. It improves upon previous mass limits from kinematic measurements by almost a …

Semileptonic decayPhysics - Instrumentation and DetectorsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and DetectorsFOS: Physical sciencesGeneral Physics and AstronomyKinematicsElectron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]KATRIN01 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)mass: scaleneutrino: mass: measured0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530S066MAESensitivity (control systems)Limit (mathematics)structure[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentPhysicstritiumPhysicsformationS066M2EInstrumentation and Detectors (physics.ins-det)semileptonic decaysensitivityddc:kinematicsElementary Particles and Fieldselectron: energy spectrumHigh Energy Physics::ExperimentPräzisionsexperimente - Abteilung BlaumNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)Astrophysics - Cosmology and Nongalactic AstrophysicsKATRINexperimental results
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The nearest X-ray emitting protostellar jet observed with HST

2009

The HH 154 jet coming from the YSO binary L1551 IRS5 is one of the closest (about 150 pc) astrophysical jet known. It is therefore a unique laboratory for studies of outflow mechanisms and of the shocks forming at the interaction front between the expanding material and the ambient medium. The substructures (knots) observed within the HH 154 jet were imaged in several spectral bands using the Hubble Space Telescope. This allows us to derive a simple characterization of the physical conditions in different structures as well as to measure the proper motion of the knots in the jet, their flux variability and shock emission over a time base of about ten years. These knots in the jet undergo si…

Shock wavePhysicsProper motionAstrophysics::High Energy Astrophysical PhenomenaAstronomyBinary numberAstrophysicsSpectral bandsSettore FIS/05 - Astronomia E AstrofisicaKnot (unit)Astrophysical jetPlanetary bow shockCoincidentinterplanetary shocks X-ray binaries Astronomical and space-research instrumentationOutflowAstrophysics::Galaxy AstrophysicsAIP Conference Proceedings
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Rapid parameter determination of discrete damped sinusoidal oscillations

2020

We present different computational approaches for the rapid extraction of the signal parameters of discretely sampled damped sinusoidal signals. We compare time- and frequency-domain-based computational approaches in terms of their accuracy and precision and computational time required in estimating the frequencies of such signals, and observe a general trade-off between precision and speed. Our motivation is precise and rapid analysis of damped sinusoidal signals as these become relevant in view of the recent experimental developments in cavity-enhanced polarimetry and ellipsometry, where the relevant time scales and frequencies are typically within the ∼1 − 10 µs and ∼1 − 100 MHz ranges, …

Signal Processing (eess.SP)Accuracy and precisionPhysics - Instrumentation and DetectorsAcousticsPolarimetryFOS: Physical sciences02 engineering and technologyApplied Physics (physics.app-ph)01 natural sciencesSignal010309 opticssymbols.namesakeOptics0103 physical sciencesFOS: Electrical engineering electronic engineering information engineeringElectrical Engineering and Systems Science - Signal ProcessingPhysicsbusiness.industrySpectral densityInstrumentation and Detectors (physics.ins-det)Physics - Applied Physics021001 nanoscience & nanotechnologyAtomic and Molecular Physics and OpticsMicrosecondFourier transformsymbols0210 nano-technologybusinessMatrix methodOptics (physics.optics)Physics - Optics
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