Search results for "PHOTOMULTIPLIER"

showing 10 items of 194 documents

Wearable, Fiber-less, Multi-Channel System for Continuous Wave Functional Near Infrared Spectroscopy Based on Silicon Photomultipliers Detectors and …

2019

Development and in-vivo validation of a Continuous Wave (CW) functional Near Infrared Spectroscopy (fNIRS) system is presented. The system is wearable, fiber-less, multi-channel (16×16, 256 channels) and expandable and it relies on silicon photomultipliers (SiPMs) for light detection. SiPMs are inexpensive, low voltage and resilient semiconductor light detectors, whose performances are analogous to photomultiplier tubes (PMTs). The advantage of SiPMs with respect to PMTs is that they allow direct contact with the scalp and avoidance of optical fibers. In fact, the coupling of SiPMs and light emitting diodes (LEDs) allows the transfer of the analog signals to and from the scalp through thin …

PhotomultiplierSpectroscopy Near-InfraredOptical fiberMaterials scienceDynamic rangebusiness.industryDetectorBrainElectroencephalographySignal Processing Computer-Assisted01 natural scienceslaw.invention010309 opticsWearable Electronic Devices03 medical and health sciences0302 clinical medicineSilicon photomultiplierAnalog signallaw0103 physical sciencesOptoelectronicsPhotonicsbusinessOptical filter030217 neurology & neurosurgery2019 41st Annual International Conference of the IEEE Engineering in Medicine and Biology Society (EMBC)
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Sedimentation and Fouling of Optical Surfaces at the ANTARES Site

2003

ANTARES is a project leading towards the construction and deployment of a neutrino telescope in the deep Mediterranean Sea. The telescope will use an array of photomultiplier tubes to detect the Cherenkov light emitted by muons resulting from the interaction with matter of high energy neutrinos. In the vicinity of the deployment site the ANTARES collaboration has performed a series of in-situ measurements to study the change in light transmission through glass surfaces during immersions of several months. The average loss of light transmission is estimated to be only ~2% at the equator of a glass sphere one year after deployment. It decreases with increasing zenith angle, and tends to satur…

PhotomultiplierTransmission lossEquatorMineralogyFOS: Physical sciencesAstrophysics[SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph]Neutrino telescopeAstrophysics01 natural scienceslaw.inventionTelescope[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Phenomenology (hep-ph)law0103 physical sciencesfouling; neutrino telescope; sea water properties; sedimentation; undersea cherenkov detectors14. Life underwater010306 general physicsCherenkov radiationZenithPhysicsUndersea Cherenkov detectors[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)Sea water propertieAstronomy and AstrophysicsFoulingSedimentationHigh Energy Physics - Phenomenology[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Física nuclearNeutrinoSedimentation
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Background light in potential sites for the ANTARES undersea neutrino telescope

2000

The ANTARES collaboration has performed a series of {\em in situ} measurements to study the background light for a planned undersea neutrino telescope. Such background can be caused by $^{40}$K decays or by biological activity. We report on measurements at two sites in the Mediterranean Sea at depths of 2400~m and 2700~m, respectively. Three photomultiplier tubes were used to measure single counting rates and coincidence rates for pairs of tubes at various distances. The background rate is seen to consist of three components: a constant rate due to $^{40}$K decays, a continuum rate that varies on a time scale of several hours simultaneously over distances up to at least 40~m, and random bur…

PhotomultiplierTrigger rateContinuum (design consultancy)Neutrino telescopeFOS: Physical sciencesAstrophysicsAstrophysics01 natural sciencesCoincidenceHigh Energy Physics - Experiment[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Experiment (hep-ex)0103 physical sciencesMetre14. Life underwater010306 general physicsPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)AstronomyAstronomy and AstrophysicsConstant rate13. Climate actionFísica nuclearBackground lightAstroparticle Physics
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First results of the Instrumentation Line for the deep-sea ANTARES neutrino telescope

2006

In 2005, the ANTARES Collaboration deployed and operated at a depth of 2500 m a so-called Mini Instrumentation Line equipped with Optical Modules (MILOM) at the ANTARES site. The various data acquired during the continuous operation from April to December 2005 of the MILOM confirm the satisfactory performance of the Optical Modules, their front-end electronics and readout system, as well as the calibration devices of the detector. The in-situ measurement of the Optical Module time response yields a resolution better than 0.5 ns. The performance of the acoustic positioning system, which enables the spatial reconstruction of the ANTARES detector with a precision of about 10 cm, is verified. T…

Photomultiplierneutrino astronomy; photon detection; underwater detectorPositioning systemInstrumentationAstrophysics::High Energy Astrophysical PhenomenaNeutrino astronomy Underwater detector Photon detectionFOS: Physical sciencesAstrophysics01 natural sciencesneutrino astronomy[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciencesCalibrationAngular resolution010306 general physicsRemote sensingAstroparticle physicsPhysicsunderwater detector[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsDetectorAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsAstronomySITEAstronomy and AstrophysicsLIGHTPHOTON DETECTIONNEUTRINO ASTRONOMYFísica nuclearUNDERWATER DETECTORNeutrino astronomy
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P-on-N and N-on-P silicon photomultipliers: an in-depth analysis in the continuous wave regime

2013

We report on the electrical and optical comparison, in the continuous wave regime, of two novel classes of silicon photomultipliers fabricated in planar technology on silicon P-type (N-on-P class) and N-type (P-on-N class) substrates respectively.

Photomultipliers SiPM detectors continuous waveSettore ING-INF/02 - Campi ElettromagneticiSettore ING-INF/01 - Elettronica
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TRITIUM - A Real-Time Tritium Monitor System for Water Quality Surveillance

2018

In this work the development results of the TRITIUM project is presented. The main objective of the project is the construction of a near real-time monitor for low activity tritium in water, aimed at in-situ surveillance and radiological protection of river water in the vicinity of nuclear power plants. The European Council Directive 2013/51/Euratom requires that the maximum level of tritium in water for human consumption to be lower than 100 Bq/L. Tritium levels in the cooling water of nuclear power plants in normal operation are much higher than the levels caused by the natural and cosmogenic components, and may easily surmount the limit required by the Directive. The current liquid-scint…

Physics - Instrumentation and DetectorsMonitoringNuclear engineeringSurface treatmentFOS: Physical sciences7. Clean energy01 natural scienceslaw.inventionSilicon photomultiplierlaw0103 physical sciencesNuclear power plantWater coolingPrototypes[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physics010308 nuclear & particles physicsbusiness.industryDetectorsInstrumentation and Detectors (physics.ins-det)Nuclear power6. Clean waterElectricity generation13. Climate actionOptical sensorsEnvironmental radioactivityEnvironmental scienceTritiumWater qualitybusinessCoolingPower generation
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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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Baby MIND: a magnetized segmented neutrino detector for the WAGASCI experiment

2017

T2K (Tokai-to-Kamioka) is a long-baseline neutrino experiment in Japan designed to study various parameters of neutrino oscillations. A near detector complex (ND280) is located 280~m downstream of the production target and measures neutrino beam parameters before any oscillations occur. ND280's measurements are used to predict the number and spectra of neutrinos in the Super-Kamiokande detector at the distance of 295~km. The difference in the target material between the far (water) and near (scintillator, hydrocarbon) detectors leads to the main non-cancelling systematic uncertainty for the oscillation analysis. In order to reduce this uncertainty a new WAter-Grid-And-SCintillator detector …

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsFOS: Physical sciencesCosmic rayScintillator01 natural sciences7. Clean energy030218 nuclear medicine & medical imaging03 medical and health sciences0302 clinical medicineSilicon photomultiplierOptics0103 physical sciencesDetectors and Experimental TechniquesNeutrino oscillationphysics.ins-detInstrumentationMathematical PhysicsPhysicsMuon010308 nuclear & particles physicsbusiness.industryDetectorInstrumentation and Detectors (physics.ins-det)Neutrino detectorHigh Energy Physics::ExperimentLarge scale cryogenic liquid detectors [8]NeutrinobusinessJournal of Instrumentation
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Prototype tests for a highly granular scintillator-based hadronic calorimeter

2017

Within the CALICE collaboration, several concepts for the hadronic calorimeter of a future lepton collider detector are studied. After having demonstrated the capabilities of the measurement methods in "physics prototypes", the focus now lies on improving their implementation in "technological prototypes", that are scalable to the full linear collider detector. The Analogue Hadronic Calorimeter (AHCAL) concept is a sampling calorimeter of tungsten or steel absorber plates and plastic scintillator tiles read out by silicon photomultipliers (SiPMs) as active components. The front-end electronics is fully integrated into the active layers of the calorimeter and is designed for minimal power co…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsFOS: Physical sciencesScintillator01 natural sciences7. Clean energylaw.inventionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Silicon photomultiplierOpticslaw0103 physical sciencesElectronicsDetectors and Experimental Techniques010306 general physicsColliderphysics.ins-detPhysicsCalorimeter (particle physics)010308 nuclear & particles physicsbusiness.industryhep-exDetectorInstrumentation and Detectors (physics.ins-det)High Energy Physics::ExperimentbusinessBeam (structure)Particle Physics - ExperimentLepton
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The Monte Carlo simulation of the Borexino detector

2017

We describe the Monte Carlo (MC) simulation package of the Borexino detector and discuss the agreement of its output with data. The Borexino MC 'ab initio' simulates the energy loss of particles in all detector components and generates the resulting scintillation photons and their propagation within the liquid scintillator volume. The simulation accounts for absorption, reemission, and scattering of the optical photons and tracks them until they either are absorbed or reach the photocathode of one of the photomultiplier tubes. Photon detection is followed by a comprehensive simulation of the readout electronics response. The algorithm proceeds with a detailed simulation of the electronics c…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsSolar neutrinoMonte Carlo methodscintillation counter: liquidSolar neutrinosenergy resolution01 natural sciences7. Clean energyLarge volume liquid scintillator detectorHigh Energy Physics - Experiment[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Large volume liquid scintillator detectorsBorexinoPhysicsphotomultipliertrack data analysisDetectorefficiency: quantumddc:540GEANTBorexinoNeutrinophoton: yieldnumerical calculations: Monte CarloPhotomultiplierdata analysis methodenergy lossScintillatorSolar neutrinoprogrammingphoton: reflectionMonte Carlo simulationsNuclear physics0103 physical sciencesphoton: scattering[INFO]Computer Science [cs][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsbackground: radioactivityMonte Carlo simulationdetector: designScintillation010308 nuclear & particles physicsbibliographyAstronomy and AstrophysicscalibrationLarge volume liquid scintillator detectors; Monte Carlo simulations; Solar neutrinos; Astronomy and Astrophysicsattenuation: lengthpile-upelectronics: readout
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