Search results for "DETECTOR"

showing 10 items of 3491 documents

Simulations on time-of-flight ERDA spectrometer performance

2016

The performance of a time-of-flight spectrometer consisting of two timing detectors and an ionization chamber energy detector has been studied using Monte Carlo simulations for the recoil creation and ion transport in the sample and detectors. The ionization chamber pulses have been calculated using Shockley-Ramo theorem and the pulse processing of a digitizing data acquisition setup has been modeled. Complete time-of-flight–energy histograms were simulated under realistic experimental conditions. The simulations were used to study instrumentation related effects in coincidence timing and position sensitivity, such as background in time-of-flight–energy histograms. Corresponding measurement…

010302 applied physicsPhysicsta114SpectrometerPhysics::Instrumentation and Detectorsbusiness.industryInstrumentationMonte Carlo methodDetector7. Clean energy01 natural sciencesMonte Carlo simulationsNuclear physicsTime of flightRecoilOpticsData acquisitiontime-of-flight spectrometers0103 physical sciencesIonization chambersimulations010306 general physicsbusinessInstrumentationReview of Scientific Instruments
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A graphene-based neutral particle detector

2019

A neutral particle detector is presented, in which the traditionally used target material, indium tin oxide (ITO), is replaced by graphene. The graphene-based detector enables collinear photodetachment measurements at a significantly shorter wavelength of light down to 230 nm compared to ITO-based detectors, which are limited at 335 nm. Moreover, the background signal from the photoelectric effect is drastically reduced when using graphene. The graphene based detector, reaching 1.7 eV further into the UV energy range, allows increased possibilities for photodetachment studies of negatively charged atoms, molecules, and clusters.A neutral particle detector is presented, in which the traditio…

010302 applied physicsRange (particle radiation)Materials sciencePhysics and Astronomy (miscellaneous)business.industryGrapheneDetector02 engineering and technologyPhotoelectric effect021001 nanoscience & nanotechnology01 natural sciencesSignallaw.inventionIndium tin oxideWavelengthlaw0103 physical sciencesOptoelectronics0210 nano-technologybusinessNeutral particleApplied Physics Letters
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Development of hard x-ray photoelectron SPLEED-based spectrometer applicable for probing of buried magnetic layer valence states

2016

Abstract A novel design of high-voltage compatible polarimeter for spin-resolved hard X-ray photoelectron spectroscopy (Spin-HAXPES) went into operation at beamline BL09XU of SPring-8 in Hyogo, Japan. The detector is based on the well-established principle of electron diffraction from a W(001) single-crystal at a scattering energy of 103.5 eV. It's special feature is that it can be operated at a high negative bias potential up to 10 kV, necessary to access the HAXPES range. The polarimeter is operated behind a large hemispherical analyzer (Scienta R-4000). It was optimized for high transmission of the transfer optics. A delay-line detector (20 mm dia.) is positioned at the exit plane of the…

010302 applied physicsSpectrum analyzerRadiationPhysics - Instrumentation and DetectorsSpin polarizationSpectrometerScatteringbusiness.industryChemistryFOS: Physical sciencesPolarimeterInstrumentation and Detectors (physics.ins-det)Condensed Matter Physics01 natural sciencesAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsOpticsX-ray photoelectron spectroscopyElectron diffraction0103 physical sciencesPhysical and Theoretical Chemistry010306 general physicsSpectroscopybusinessSpectroscopy
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Simplified feedback control system for scanning tunneling microscopy

2021

A Scanning Tunneling Microscope (STM) is one of the most important scanning probe tools available to study and manipulate matter at the nanoscale. In a STM, a tip is scanned on top of a surface with a separation of a few \AA. Often, the tunneling current between tip and sample is maintained constant by modifying the distance between the tip apex and the surface through a feedback mechanism acting on a piezoelectric transducer. This produces very detailed images of the electronic properties of the surface. The feedback mechanism is nearly always made using a digital processing circuit separate from the user computer. Here we discuss another approach, using a computer and data acquisition thr…

010302 applied physicsSuperconductivityPhysics - Instrumentation and DetectorsMaterials sciencebusiness.industrySerial communicationFOS: Physical sciencesWeyl semimetalPort (circuit theory)Instrumentation and Detectors (physics.ins-det)01 natural sciencesPiezoelectricityNoise (electronics)law.inventionCondensed Matter - Other Condensed MatterData acquisitionlawCondensed Matter::Superconductivity0103 physical sciencesOptoelectronicsScanning tunneling microscope010306 general physicsbusinessInstrumentationOther Condensed Matter (cond-mat.other)Review of Scientific Instruments
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ZnMgO-based UV photodiodes: a comparison of films grown by spray pyrolysis and MBE

2016

Detecting the UV part of the spectrum is fundamental for a wide range of applications where ZnMgO has the potential to play a central role. The shortest achievable wavelength is a function of the Mg content in the films, which in turn is dependent on the growth technique. Moreover, increasing Mg contents lead to an electrical compensation of the films, which directly affects the responsivity of the photodetectors. In addition, the metal-semiconductor interface and the presence of grain boundaries have a direct impact on the responsivity through different gain mechanisms. In this work, we review the development of ZnMgO UV Schottky photodiodes using molecular beam epitaxy and spray pyrolysis…

010302 applied physicsTelecomunicacionesMaterials sciencebusiness.industrySchottky diodePhotodetector02 engineering and technology021001 nanoscience & nanotechnology01 natural sciencesPhotodiodelaw.inventionResponsivityWavelengthSemiconductorlaw0103 physical sciencesOptoelectronicsGrain boundary0210 nano-technologybusinessMolecular beam epitaxy
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Oxy-nitrides characterization with a new ERD-TOF system

2017

Abstract A new time-of-flight (TOF) camera was installed on Elastic Recoil Detection (ERD) measurement setup on the Tandem Accelerator at Universite de Montreal. The camera consists of two timing detectors, developed and built by the Jyvaskyla group, that use a thin carbon foil and microchannel plates (MCP) to produce the start and stop signals. The position of the first detector is fixed at 18 cm from the target, while the position of the second detector can be varied between 50 and 90 cm from the first detector. This allows to increase time resolution by increasing the distance between the time-of-flight detectors or to increase solid angle by decreasing the distance. Moving the detector …

010302 applied physicsToF-ERDANuclear and High Energy PhysicsIon beam analysisMicrochannelMaterials scienceta114Physics::Instrumentation and Detectorsbusiness.industryDetectorSolid angleion beam analysis02 engineering and technology021001 nanoscience & nanotechnology01 natural sciencesSignalelastic recoil detectionElastic recoil detectionOpticsPosition (vector)0103 physical sciences0210 nano-technologybusinessInstrumentationEnergy (signal processing)Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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Operational Experience and Performance of the Belle II Pixel Detector

2021

Proceedings of the 29th International Workshop on Vertex Detectors (VERTEX2020), Tsukuba, Japan (Online); Journal of the Physical Society of Japan 34, 010002 (2021). doi:10.7566/JPSCP.34.010002

010308 nuclear & particles physicsComputer sciencebusiness.industry0103 physical sciencesddc:530Computer visionArtificial intelligence010306 general physicsbusiness53001 natural sciencesPixel detectorProceedings of the 29th International Workshop on Vertex Detectors (VERTEX2020)
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Antineutrino monitoring of spent nuclear fuel

2016

Military and civilian applications of nuclear energy have left a significant amount of spent nuclear fuel over the past 70 years. Currently, in many countries world wide, the use of nuclear energy is on the rise. Therefore, the management of highly radioactive nuclear waste is a pressing issue. In this letter, we explore antineutrino detectors as a tool for monitoring and safeguarding nuclear waste material. We compute the flux and spectrum of antineutrinos emitted by spent nuclear fuel elements as a function of time, and we illustrate the usefulness of antineutrino detectors in several benchmark scenarios. In particular, we demonstrate how a measurement of the antineutrino flux can help to…

010308 nuclear & particles physicsNuclear engineeringDetectorGeneral Physics and AstronomyFluxRadioactive wasteFOS: Physical sciences01 natural sciencesSpent nuclear fuel3. Good healthHigh Energy Physics - ExperimentOverburdenHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesElectromagnetic shieldingEnvironmental scienceNeutrinoNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentLeakage (electronics)
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Cosmic-Ray Anisotropies in Right Ascension Measured by the Pierre Auger Observatory

2020

We present measurements of the large-scale cosmic-ray anisotropies in right ascension, using data collected by the surface detector array of the Pierre Auger Observatory over more than 14 years. We determine the equatorial dipole component, ~d⊥, through a Fourier analysis in right ascension that includes weights for each event so as to account for the main detector-induced systematic effects. For the energies at which the trigger efficiency of the array is small, the “East-West” method is employed. Besides using the data from the array with detectors separated by 1500 m, we also include data from the smaller but denser sub-array of detectors with 750 m separation, which allows us to extend …

010504 meteorology & atmospheric sciencesAstronomyAstrophysicsAstrophysicsanisotropy [cosmic radiation]Amplitude01 natural sciencessurface [detector]010303 astronomy & astrophysicsRight ascensionastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsOBSERVATÓRIOSGalactic CenterAstrophysics::Instrumentation and Methods for AstrophysicsCosmic RaysAugerobservatoryAmplitudePhysics::Space PhysicsAstrophysics - High Energy Astrophysical PhenomenaExtragalactic cosmic rayAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic raycosmic radiation: anisotropyExtragalactic cosmic rayGalactic center0103 physical sciencesHigh Energy PhysicsPierre auger observatory0105 earth and related environmental sciencesPierre Auger Observatorydetector: surfaceFísicaAstronomy and AstrophysicsCosmic rayefficiency [trigger]GalaxyDipole* Automatic Keywords *Space and Planetary ScienceExperimental High Energy Physicstrigger: efficiencyddc:520galaxyDipoleObservatoryEnergy (signal processing)anisotropiesRight ascension[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)dipoleThe Astrophysical Journal
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A Search for Ultra-high-energy Neutrinos from TXS 0506+056 Using the Pierre Auger Observatory

2020

Results of a search for ultra-high-energy neutrinos with the Pierre Auger Observatory from the direction of the blazar TXS 0506+056 are presented. They were obtained as part of the follow-up that stemmed from the detection of high-energy neutrinos and gamma rays with IceCube, Fermi-LAT, MAGIC, and other detectors of electromagnetic radiation in several bands. The Pierre Auger Observatory is sensitive to neutrinos in the energy range from 100 PeV to 100 EeV and in the zenith-angle range from θ = 60° to θ = 95°, where the zenith angle is measured from the vertical direction. No neutrinos from the direction of TXS 0506+056 have been found. The results were analyzed in three periods: One of 6 m…

010504 meteorology & atmospheric sciencesAstronomyAstrophysicspower spectrum7. Clean energy01 natural sciencesIceCubeObservatoryMAGIC (telescope)UHE Cosmic Rays010303 astronomy & astrophysicsHigh energy astrophysics Neutrino astrony Blazars Transient sources Active galaxiesHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEOBSERVATÓRIOSAstrophysics::Instrumentation and Methods for Astrophysicsneutrino: UHEUHE [neutrino]AugerobservatoryHigh energy astrophysics; Neutrino astronomy; Blazars; Transient sources; Active galaxiesNeutrino detectorNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical PhenomenaHigh energy astrophysicsradiation: electromagneticHigh-energy astronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGLASTblazar0103 physical sciencesNeutrinoHigh Energy PhysicsZenithAstrophysique0105 earth and related environmental sciencesPierre Auger ObservatoryFísicaAstronomy and AstrophysicsAstronomiesensitivityMAGICTransient sourcesSciences de l'espaceelectromagnetic [radiation]13. Climate actionSpace and Planetary Sciencegamma rayExperimental High Energy PhysicsActive galaxiesddc:520spectralNeutrino astronomy[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Blazars
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