Search results for "Lier"

showing 10 items of 906 documents

The PANDA DIRC Detectors at FAIR

2017

The PANDA detector at the international accelerator Facility for Antiproton and Ion Research in Europe (FAIR) addresses fundamental questions of hadron physics. An excellent hadronic particle identification (PID) will be accomplished by two DIRC (Detection of Internally Reflected Cherenkov light) counters in the target spectrometer. The design for the barrel region covering polar angles between 22 deg. to 140 deg. is based on the successful BABAR DIRC with several key improvements, such as fast photon timing and a compact imaging region. The novel Endcap Disc DIRC will cover the smaller forward angles between 5 deg. (10 deg.) to 22 deg. in the vertical (horizontal) direction. Both DIRC coun…

PhotomultiplierPhotonPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsFOS: Physical sciences01 natural sciencesParticle identification030218 nuclear medicine & medical imaging03 medical and health sciences0302 clinical medicineOpticsDetection of internally reflected Cherenkov light0103 physical sciencesNuclear ExperimentInstrumentationMathematical PhysicsPhysicsSpectrometer010308 nuclear & particles physicsbusiness.industryDetectorInstrumentation and Detectors (physics.ins-det)Facility for Antiproton and Ion ResearchMicrochannel plate detectorHigh Energy Physics::Experimentbusiness
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Lowering the radioactivity of the photomultiplier tubes for the XENON1T dark matter experiment

2015

The low-background, VUV-sensitive 3-inch diameter photomultiplier tube R11410 has been developed by Hamamatsu for dark matter direct detection experiments using liquid xenon as the target material. We present the results from the joint effort between the XENON collaboration and the Hamamatsu company to produce a highly radio-pure photosensor (version R11410-21) for the XENON1T dark matter experiment. After introducing the photosensor and its components, we show the methods and results of the radioactive contamination measurements of the individual materials employed in the photomultiplier production. We then discuss the adopted strategies to reduce the radioactivity of the various PMT versi…

PhotomultiplierPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)530 PhysicsDark matterPhotodetectorchemistry.chemical_elementFOS: Physical sciencesGermanium01 natural sciencesAtomicRecoilOpticsXenonParticle and Plasma Physics0103 physical sciencesNuclear010306 general physicsEngineering (miscellaneous)physics.ins-detInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsQuantum Physics010308 nuclear & particles physicsbusiness.industryDetectorMolecularInstrumentation and Detectors (physics.ins-det)Nuclear & Particles Physics3. Good healthchemistrybusinessAstrophysics - Instrumentation and Methods for Astrophysicsastro-ph.IM
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The liquid-argon scintillation pulseshape in DEAP-3600

2020

AbstractDEAP-3600 is a liquid-argon scintillation detector looking for dark matter. Scintillation events in the liquid argon (LAr) are registered by 255 photomultiplier tubes (PMTs), and pulseshape discrimination (PSD) is used to suppress electromagnetic background events. The excellent PSD performance of LAr makes it a viable target for dark matter searches, and the LAr scintillation pulseshape discussed here is the basis of PSD. The observed pulseshape is a combination of LAr scintillation physics with detector effects. We present a model for the pulseshape of electromagnetic background events in the energy region of interest for dark matter searches. The model is composed of (a) LAr scin…

PhotomultiplierPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsDark matterFOS: Physical scienceslcsh:AstrophysicsScintillatorWavelength shifter01 natural sciencesParticle detectorDEAPOptics0103 physical scienceslcsh:QB460-466lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsEngineering (miscellaneous)PhysicsScintillation010308 nuclear & particles physicsbusiness.industryInstrumentation and Detectors (physics.ins-det)Scintillation counterlcsh:QC770-798businessEuropean Physical Journal C: Particles and Fields
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Time imaging reconstruction for the PANDA Barrel DIRC

2020

The innovative Barrel DIRC (Detection of Internally Reflected Cherenkov light) counter will provide hadronic particle identification (PID) in the central region of the PANDA experiment at the new Facility for Antiproton and Ion Research (FAIR), Darmstadt, Germany. This detector is designed to separate charged pions and kaons with at least 3 standard deviations for momenta up to 3.5 GeV/c, covering the polar angle range of 22$^{\circ}$-140$^{\circ}$. An array of microchannel plate photomultiplier tubes is used to detect the location and arrival time of the Cherenkov photons with a position resolution of 2 mm and time precision of about 100 ps. The time imaging reconstruction has been develop…

PhotomultiplierPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsFOS: Physical sciences01 natural sciencesParticle identification030218 nuclear medicine & medical imaging03 medical and health sciences0302 clinical medicineOpticsDetection of internally reflected Cherenkov light0103 physical sciencesNuclear ExperimentInstrumentationMathematical PhysicsCherenkov radiationPhysics010308 nuclear & particles physicsbusiness.industryDetectorReconstruction algorithmInstrumentation and Detectors (physics.ins-det)Facility for Antiproton and Ion ResearchMicrochannel plate detectorHigh Energy Physics::Experimentbusiness
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Measurement of the atmospheric muon flux with a 4 GeV threshold in the ANTARES neutrino telescope

2010

A new method for the measurement of the muon flux in the deep-sea ANTARES neutrino telescope and its dependence on the depth is presented. The method is based on the observation of coincidence signals in adjacent storeys of the detector. This yields an energy threshold of about 4 GeV. The main sources of optical background are the decay of 40K and the bioluminescence in the sea water. The 40K background is used to calibrate the efficiency of the photo-multiplier tubes.

PhotomultiplierPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAtmospheric muonsFOS: Physical sciencesLINECosmic rayPotassium-4001 natural sciencesParticle detectorNuclear physicsPOTASSIUM-40NEUTRINO TELESCOPESatmospheric muons; depth intensity relation; potassium-400103 physical sciencesDepth intensity relation14. Life underwater010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)ATMOSPHERIC MUONSPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsPotassium-40DetectorAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsPERFORMANCEDEPTH INTENSITY RELATIONLIGHTNeutrino detector13. Climate actionddc:540Física nuclearHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]SYSTEMLepton
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Transmission of light in deep sea water at the site of the Antares neutrino telescope

2005

The ANTARES neutrino telescope is a large photomultiplier array designed to detect neutrino-induced upward-going muons by their Cherenkov radiation. Understanding the absorption and scattering of light in the deep Mediterranean is fundamental to optimising the design and performance of the detector. This paper presents measurements of blue and UV light transmission at the ANTARES site taken between 1997 and 2000. The derived values for the scattering length and the angular distribution of particulate scattering were found to be highly correlated, and results are therefore presented in terms of an absorption length lambda_abs and an effective scattering length lambda_sct^eff. The values for …

PhotomultiplierPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsNeutrino telescopeAstrophysicsLambda01 natural sciencesLight scattering[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Sea water properties: absorption and transmission of lightHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesAngular resolution07.89.+b 29.40.Ka 42.25.Bs 42.68.Xy 92.10.Bf 92.10.Pt 95.55.Vj010306 general physicsCherenkov radiationPhysicsneutrino telescope undersea Cherenkov detectors sea water properties absorption and transmission of lightUndersea Cherenkov detectors[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsScatteringAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsAttenuation lengthSea water properties: absorption and transmission of light.Astronomy and AstrophysicsScattering lengthabsorption and transmission of lightHigh Energy Physics - Phenomenology13. Climate actionFísica nuclearsea water propertiesAstroparticle Physics
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Comments on 'SPICE Model of Photomultiplier Tube Under Different Bias Conditions'

2021

[EN] The paper ¿SPICE Model of Photomultiplier Tube Under Different Bias Conditions¿ is commented. We revisit the mathematical formulation to compensate for some ambiguities in the original manuscript, and point out some inconsistencies in the results and reproducibility of the simulations, as well as in the optimized parameters originally obtained with the PSPICE simulation engine. All simulations are recalculated with the NGSPICE software using the corrected parameters and compared against the original figures. The reproducibility of our simulations is independently verified with PSPICE, as well as by numerically solving the analytical system of non-linear equations using Newton¿s method …

PhotomultiplierReproducibilityComputer sciencebusiness.industrySpiceModels matemàticsNumerical modelsSoftwareFISICA APLICADAPoint (geometry)Electrical and Electronic EngineeringMATLABbusinessMATEMATICA APLICADAInstrumentationcomputerSimulationcomputer.programming_language
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Operation of silicon photomultipliers as photosensors of liquid xenon detectors

2016

Silicon Photomultipliers as photosensors for liquid xenon detectors are an attractive alternative to photomultiplier tubes: liquid xenon detectors employed in low background experiments or compact Compton cameras can take advantage of the small sensor mass and dimensions, the larger light collection coming from a more packed tiling of the readout plane, and possibly a smaller cost per area. We investigate the operation in liquid xenon of samples developed by Ketek GmbH. To provide sensitivity to the liquid xenon scintillation light wavelength, 178 nm, the inactive entrance layer of the device has been thinned. The operation of such devices at temperatures as low as −100°C has been verified,…

PhotomultiplierScintillationMaterials sciencePhysics::Instrumentation and Detectors010308 nuclear & particles physicsbusiness.industryAstrophysics::Instrumentation and Methods for Astrophysicschemistry.chemical_elementPhotodetectorSubstrate (electronics)01 natural sciencesOutgassingXenonSilicon photomultiplierOpticschemistry0103 physical sciencesOptoelectronicsPhotonics010306 general physicsbusiness2016 IEEE Nuclear Science Symposium, Medical Imaging Conference and Room-Temperature Semiconductor Detector Workshop (NSS/MIC/RTSD)
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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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