Search results for " Detector"

showing 10 items of 2719 documents

Rapid online solid-state battery diagnostics with optically pumped magnetometers

2020

Applied Sciences 10(21), 7864 (2020). doi:10.3390/app10217864

Battery (electricity)Physics - Instrumentation and DetectorsAtomic Physics (physics.atom-ph)Power storageComputer scienceMagnetometerFOS: Physical sciencesApplied Physics (physics.app-ph)02 engineering and technology010402 general chemistrymagnetization01 natural scienceslcsh:Technologylaw.inventionPhysics - Atomic Physicslcsh:Chemistrylawrapid online diagnosticsGeneral Materials ScienceInstrumentationlcsh:QH301-705.5Fluid Flow and Transfer Processesatomic magnetometerbusiness.industrylcsh:TProcess Chemistry and TechnologyGeneral EngineeringElectrical engineering600Instrumentation and Detectors (physics.ins-det)Physics - Applied Physics021001 nanoscience & nanotechnologylcsh:QC1-9990104 chemical sciencesComputer Science ApplicationsState of chargelcsh:Biology (General)lcsh:QD1-999lcsh:TA1-2040Solid-state batterysolid-state battery0210 nano-technologybusinesslcsh:Engineering (General). Civil engineering (General)ddc:600Atomic magnetometerlcsh:Physicsmagnetic susceptibility
researchProduct

In-flight calibration of the ROSAT HRI ultraviolet sensitivity

2000

Comparing measured and estimated count rates of a few selected sample stars, we confirm the validity and provide the in-flight calibration of the ROSAT HRI UV/visible effective area model in Zombeck et al. The count rate estimates for Betelgeuse derived with this model are in agreement with the measured HRI upper limit. This result is also confirmed in an erratum by Berghöfer et al. aimed at revising their previous calculation, which was overestimated by more than 2 orders of magnitude. Adopting this ROSAT HRI UV/visible effective area model and measured UV/visible spectra of a set of sample stars covering the range of Teff 3000-40,000 K, we have built the calibration curves to estimate UV/…

BetelgeusePhysicsInstrumentation: detectorK-type main-sequence starAstronomyAstronomy and AstrophysicsAstrophysicsStars: late-typemedicine.disease_causeUltraviolet: starStars: early-typeStarsSpace and Planetary ScienceROSATmedicineCalibrationX-rays: starSensitivity (control systems)UltravioletNuclear and High Energy Physic
researchProduct

Position-sensitive neutron detector

2002

Abstract A position-sensitive neutron detector has been developed for use in nuclear physics research. The detector consists of a ∅5.5 cm×100 cm long quartz tube filled with liquid scintillator viewed from both ends by photomultipliers and enclosed in a light-tight titanium container. The properties of the detector were determined both experimentally and by Monte Carlo simulations (EFEN code). A time resolution of 0.4 ns was reached resulting in the position resolution of less than 4 cm. The neutron registration efficiency varies from 36% to 20% within neutron energy range 1–10 MeV and is practically independent of the position along the detector length. Good n–γ separation is achieved for …

Bonner spherePhysicsNuclear and High Energy PhysicsPhotomultiplierPhysics::Instrumentation and Detectorsbusiness.industryNuclear TheoryMonte Carlo methodDetectorScintillatorNeutron temperatureNuclear physicsOpticsNeutron detectionNeutronNuclear ExperimentbusinessInstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
researchProduct

Neutron fluence spectrometry using disk activation

2009

Abstract A simple and robust detector for spectrometry of environmental neutrons has been developed. The technique is based on neutron activation of a series of different metal disks followed by low-level gamma-ray spectrometry of the activated disks and subsequent neutron spectrum unfolding. The technique is similar to foil activation but here the applied neutron fluence rates are much lower than usually in the case of foil activation. The detector has been tested in quasi mono-energetic neutron fields with fluence rates in the order of 1000–10000 cm −2  s −1 , where the obtained spectra showed good agreement with spectra measured using a Bonner sphere spectrometer. The detector has also b…

Bonner spherePhysicsRadiationSpectrometerPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFluenceNuclear physicsNeutron fluxNeutron cross sectionNeutron detectionNeutronAtomic physicsNuclear ExperimentInstrumentationNeutron activationRadiation Measurements
researchProduct

Multi-channel search for squarks and gluinos in root s=7 TeV pp collisions with the ATLAS detector at the LHC

2013

A search for supersymmetric particles in final states with zero, one, and two leptons, with and without jets identified as originating from b-quarks, in 4.7 fb[superscript −1] of √s = 7 TeV pp collisions produced by the Large Hadron Collider and recorded by the ATLAS detector is presented. The search uses a set of variables carrying information on the event kinematics transverse and parallel to the beam line that are sensitive to several topologies expected in supersymmetry. Mutually exclusive final states are defined, allowing a combination of all channels to increase the search sensitivity. No deviation from the Standard Model expectation is observed. Upper limits at 95 % confidence level…

Brookhaven National LaboratoryParticle physicsPhysics and Astronomy (miscellaneous)Supergauge TransformationsContext (language use)ddc:500.253001 natural sciencesStandard ModelSet (abstract data type)CurrentsPions0103 physical sciencesddc:530Sensitivity (control systems)WeakHigh Energy Physics010306 general physicsEngineering (miscellaneous)QCCiencias ExactasPhysicsproton–proton collisionsHadron-Hadron ScatteringLarge Hadron ColliderATLAS detector010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleHigh Energy Physics::PhenomenologyFísicaSupersymmetryATLASgluinosHADRON-HADRON COLLISIONSExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGsquarksHigh Energy Physics::ExperimentSupersymmetryLHCEvent (particle physics)LeptonModel
researchProduct

Search for Gravitational-wave Signals Associated with Gamma-Ray Bursts during the Second Observing Run of Advanced LIGO and Advanced Virgo

2019

We present the results of targeted searches for gravitational-wave transients associated with gamma-ray bursts during the second observing run of Advanced LIGO and Advanced Virgo, which took place from 2016 November to 2017 August. We have analyzed 98 gamma-ray bursts using an unmodeled search method that searches for generic transient gravitational waves and 42 with a modeled search method that targets compact-binary mergers as progenitors of short gamma-ray bursts. Both methods clearly detect the previously reported binary merger signal GW170817, with p-values of <9.38 10-6 (modeled) and 3.1 10-4 (unmodeled). We do not find any significant evidence for gravitational-wave signals associate…

Burst astrophysicAstrofísicaneutron star: binary010504 meteorology & atmospheric sciencesBinary numberAstrophysics01 natural sciencesLIGOQCSUPERNOVArelativistic jetsQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01counterpartGRBGravitational waves (678)Physical SciencesRELATIVISTIC JETSAstrophysics - High Energy Astrophysical PhenomenaGravitational waveGravitationstarsblack-holeAstrophysics::High Energy Astrophysical PhenomenaGeneral Relativity and Quantum Cosmology (gr-qc)precursor activityGravitational wavesSettore FIS/05 - Astronomia e AstrofisicasupernovaCORE-COLLAPSEGamma-ray burstGravitational wave sourcesScience & TechnologyVirgoRCUKAstronomy and AstrophysicsHigh energy astrophysics (739)RedshiftDewey Decimal Classification::500 | Naturwissenschaften::520 | Astronomie Kartographiedetector: sensitivityVIRGOSpace and Planetary Sciencegravitational radiation: emissionBLACK-HOLEddc:520Gravitational wave astronomyGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]STARSGravitacióAstronomySignalGeneral Relativity and Quantum CosmologyBurst astrophysicslocalizationemission010303 astronomy & astrophysicsPhysicsDetectorGamma-ray bursts (629)[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave sourcePRECURSOR ACTIVITYGamma-ray burstsLIGO (920)High energy astrophysicsdata analysis methodBurst astrophysics (187)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstAstronomy & AstrophysicsMASSgravitational radiation: direct detectionGravitational wave astronomy Gravitational wave sources LIGO; Gravitational waves Gamma-ray bursts Burst astrophysics High energy astrophysicsGravitational wave astronomy (675)electromagnetic field: production0103 physical sciencesnumerical calculationsGRB; gravitational waves; LIGO; VirgoSTFC0105 earth and related environmental sciencesgravitational wavesneutron starsGravitational waveCOUNTERPARTgravitational radiationLIGOcore-collapsegravitational radiation detectorGravitational wave sources (677)radiationNeutron starPhysics and AstronomymassRADIATIONEMISSIONGravitational wave astronomy; Gravitational wave sources; LIGO; Gravitational waves; Gamma-ray bursts; Burst astrophysics; High energy astrophysics
researchProduct

Development of a 3D CZT detector prototype for Laue Lens telescope

2010

We report on the development of a 3D position sensitive prototype suitable as focal plane detector for Laue lens telescope. The basic sensitive unit is a drift strip detector based on a CZT crystal, (similar to 19x8 mm(2) area, 2.4 mm thick), irradiated transversally to the electric field direction. The anode side is segmented in 64 strips, that divide the crystal in 8 independent sensor (pixel), each composed by one collecting strip and 7 (one in common) adjacent drift strips. The drift strips are biased by a voltage divider, whereas the anode strips are held at ground. Furthermore, the cathode is divided in 4 horizontal strips for the reconstruction of the third interaction position coord…

CDTE DETECTORSPhysicsPhysics::Instrumentation and Detectorsbusiness.industryDetectorVoltage dividerGamma ray spectroscopySTRIPSCZT detectorCZT detectors 3D detectors Laue lensCathodeParticle detectorlaw.inventionAnodeLens (optics)TelescopeOpticsHard X- and soft gamma-ray astronomy3D imagingDrift striplawCDZNTEbusiness
researchProduct

ALICE forward rapidity upgrades

2017

Two forward rapidity upgrades of the ALICE apparatus at the LHC are presented: the Muon Forward Tracker (MFT) and the Fast Interaction Trigger (FIT). Their designs are driven by physics performance studies, which have been done using MC simulations. Several prototypes have been tested. Currently the detector design phase has ended. The final layouts, geometries and expected performance figures are presented. The latest developments from the test of the prototypes are discussed. The MFT will improve the performance of the ALICE Muon Spectrometer by adding vertexing capabilities to the system. The elementary component of the MFT is a Monolithic Active Pixel Sensor (MAPS), using the TowerJazz …

CMOS sensorLarge Hadron ColliderMuon Forward TrackerInteraction pointta114Computer sciencebusiness.industryCherenkov detectorFast Interaction TriggerPhysics::Instrumentation and DetectorsMonte Carlo methodDetectorALICE apparatuslaw.inventionOpticslawMicrochannel plate detectorDetectors and Experimental TechniquesbusinessCherenkov radiation
researchProduct

Update on the TowerJazz CMOS DMAPS development for the ATLAS ITk

2019

The upgrade of the ATLAS tracking detector for the High-Luminosity Large Hadron Collider at CERN requires the development of novel radiation hard silicon sensor technologies. For the de- velopment of depleted CMOS sensors for ATLAS we combined small electrodes with minimal capacitance and advanced processing for fully depleted active sensor volume to achieve radiation hard CMOS sensors in line with ATLAS ITk specifications. Based on initial studies on the prototype sensor “TowerJazz Investigator” we have now developed, produced and tested a first full-size depleted CMOS sensor based on the 180nm TowerJazz imag- ing process, the so-called “MALTA” sensor. The sensor combines special low-noise…

CMOS sensorLarge Hadron Colliderbusiness.industryComputer sciencePhysics::Instrumentation and DetectorsDetectorElectronic detector readout concepts (solid-state) ; Front-end electronics for detector readout ; Particle tracking detectors ; Radiation-hard detectorsChipCapacitancemedicine.anatomical_structureUpgradeCMOSAtlas (anatomy)medicineComputerSystemsOrganization_SPECIAL-PURPOSEANDAPPLICATION-BASEDSYSTEMSDetectors and Experimental TechniquesbusinessComputer hardware
researchProduct

Perspectives for CNO neutrino detection in Borexino

2018

International audience; Borexino measured with unprecedented accuracy the fluxes of solar neutrinos emitted at all the steps of the pp fusion chain. Still missing is the measurement of the flux of neutrinos produced in the CNO cycle. A positive measurement of the CNO neutrino flux is of fundamental importance for understanding the evolution of stars and addressing the unresolved controversy on the solar abundances. The measurement of the CNO neutrino flux in Borexino is challenging because of the low intensity of this component (CNO cycle accounts for about 1% of the energy emitted by Sun), the lack of prominent spectral features and the presence of background sources. The main background c…

CNO cycleexperimental methodsneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical Phenomenascintillation counter: liquidSolar neutrinosbismuth: admixtureAstrophysics[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energySolar neutrinoCNO-cycleneutrino: fluxAstrophysics::Solar and Stellar Astrophysics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Stellar evolutionBorexinoliquid scintillatorAstrophysics::Galaxy AstrophysicsPhysicsEnergy distributiondetectorbackgroundbismuth: nuclideCNO cycleNeutrino detector13. Climate actionBorexinoExperimental methodsNeutrino
researchProduct