Search results for "Cherenkov light"

showing 10 items of 14 documents

Tau neutrinos in the next decade: from GeV to EeV

2022

Tau neutrinos are the least studied particle in the standard model. This whitepaper discusses the current and expected upcoming status of tau neutrino physics with attention to the broad experimental and theoretical landscape spanning long-baseline, beam-dump, collider, and astrophysical experiments. This whitepaper was prepared as a part of the NuTau2021 Workshop.

HIGH-ENERGY NEUTRINOSMAGNETIC-MOMENTAstrophysics and AstronomyNuclear and High Energy PhysicsRADIO PULSESPhysics::Instrumentation and Detectorstau neutrinosFOS: Physical sciencesCHERENKOV LIGHT YIELDGeV530High Energy Physics - Experimenttau neutrino theorySubatomär fysikHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)neutrino experimentsSubatomic Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530Particle Physics - PhenomenologyAIR-SHOWERSLEPTON FLAVORastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)hep-exPhysicshep-phtau neutrinos; neutrino experiments; tau neutrino theorylandscapeCOSMIC-RAYSHigh Energy Physics - PhenomenologyQUANTUM-GRAVITYCHARGED-PARTICLES[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]beam dumpPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentLORENTZ VIOLATION[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical PhenomenaParticle Physics - Experiment
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Time calibration of the ANTARES neutrino telescope

2011

The ANTARES deep-sea neutrino telescope comprises a three-dimensional array of photomultipliers to detect the Cherenkov light induced by upgoing relativistic charged particles originating from neutrino interactions in the vicinity of the detector. The large scattering length of light in the deep sea facilitates an angular resolution of a few tenths of a degree for neutrino energies exceeding 10 TeV. In order to achieve this optimal performance, the time calibration procedures should ensure a relative time calibration between the photomultipliers at the level of ~1 ns. The methods developed to attain this level of precision are described.

Optical telescopesPhysics - Instrumentation and Detectors[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and Detectors01 natural sciencesOptimal performanceHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Calibration procedureDimensional arraysAngular resolution[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutrino energyNEUTRINO TELESCOPE010303 astronomy & astrophysicsPhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)Deep seaNeutrino detectorRelative timeCalibrationFísica nuclearNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsTime calibrationPhotomultiplier[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Cherenkov lightAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesScattering lengthNeutrino TelescopesOptical telescopeNuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Tellurium compounds0103 physical sciencesOptical systemsCalibrationAngular resolution14. Life underwater[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Instrumentation and Methods for Astrophysics (astro-ph.IM)DETECTORCherenkov radiationtime calibration; neutrino telescopes; antaresANTARES010308 nuclear & particles physicsNeutrino interactionsAstronomyElementary particlesAstronomy and AstrophysicsPhotomultipliersFISICA APLICADAHigh Energy Physics::ExperimentUNDERWATER DETECTORNeutrino telescopesSYSTEM
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LeptonInjector and LeptonWeighter: A neutrino event generator and weighter for neutrino observatories

2021

We present a high-energy neutrino event generator, called LeptonInjector, alongside an event weighter, called LeptonWeighter. Both are designed for large-volume Cherenkov neutrino telescopes such as IceCube. The neutrino event generator allows for quick and flexible simulation of neutrino events within and around the detector volume, and implements the leading Standard Model neutrino interaction processes relevant for neutrino observatories: neutrino-nucleon deep-inelastic scattering and neutrino-electron annihilation. In this paper, we discuss the event generation algorithm, the weighting algorithm, and the main functions of the publicly available code, with examples.

Particle physicsPhysics::Instrumentation and DetectorsComputer scienceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and AstronomyCHERENKOV LIGHT YIELDWeighting01 natural sciencesHigh Energy Physics - Experiment010305 fluids & plasmasStandard ModelHigh Energy Physics - Experiment (hep-ex)Neutrino interactionHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsCherenkov radiationEvent generatorEvent generator; Neutrino generator; Neutrino interaction; Neutrino simulation; WeightingGenerator (computer programming)hep-exEvent (computing)ICEHigh Energy Physics::PhenomenologyDetectorhep-phComputational Physics (physics.comp-ph)Quantitative Biology::GenomicsHigh Energy Physics - Phenomenologyphysics.comp-phHardware and ArchitectureHigh Energy Physics::ExperimentNeutrino simulationNeutrino generatorEvent generatorNeutrinoPhysics - Computational PhysicsLeptonComputer Physics Communications
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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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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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The Endcap Disc DIRC detector of PANDA

2019

Abstract At the international FAIR laboratory, an upcoming significant enlargement of the GSI installations near Darmstadt, Germany, the PANDA antiproton experiment will investigate fundamental questions of hadron physics in the charm quark energy range. Antiprotons in the 1.5 to15 GeV/c momentum range will interact with gas jet or pellet fixed targets. The Endcap Disc DIRC (Detection of Internally Reflected Cherenkov light) covers the forward endcap solid angle of the PANDA target spectrometer to positively identify charged kaons. Monte-Carlo simulations indicate that from 1 up to 4 GeV/c one can achieve kaon–pion separation with a separation power of at least 3 standard deviations. For th…

PhysicsNuclear and High Energy PhysicsLarge Hadron ColliderSpectrometerPhysics::Instrumentation and Detectors010308 nuclear & particles physicsDetectorJet (particle physics)01 natural sciences030218 nuclear medicine & medical imagingCharm quarkNuclear physicsMomentum03 medical and health sciences0302 clinical medicineDetection of internally reflected Cherenkov lightAntiproton0103 physical sciencesPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNuclear ExperimentInstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Recent results with lifetime enhanced microchannel-plate photomultipliers

2018

Abstract The favored photon sensors for the DIRC (detection of internally reflected Cherenkov light) detectors at the PANDA (Anti-proton Annihilation at Darmstadt) experiment at FAIR (Facility for anti-proton and ion research) are micro-channel-plate photomultipliers (MCP-PMTs). The main problem until a few years ago was the limited lifetime of the MCP-PMTs caused by a rapid decrease in quantum efficiency (QE) of the photo cathode (PC) with increasing integrated anode charge (IAC). These limitations are overcome by applying an atomic layer deposition (ALD) coating on the MCPs, as recently done by PHOTONIS and Hamamatsu. During the last years’ tests of lifetime enhanced MCP-PMTs were perform…

PhysicsNuclear and High Energy PhysicsPhotomultiplierPhoton010308 nuclear & particles physicsbusiness.industry01 natural sciencesCathode030218 nuclear medicine & medical imagingAnodelaw.invention03 medical and health sciencesAtomic layer deposition0302 clinical medicineOpticsDetection of internally reflected Cherenkov lightlaw0103 physical sciencesQuantum efficiencyMicrochannel plate detectorbusinessInstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Breakthrough in the lifetime of microchannel plate photomultipliers

2015

Abstract Cherenkov detectors using the DIRC (Detection of Internally Reflected Cherenkov Light) principle are foreseen for particle identification in the P ¯ ANDA experiment at FAIR. Promising sensors for the detection of the Cherenkov light are the so-called micro-channel plate (MCP) photomultipliers (PMT). They have an excellent time resolution, can be operated at high gain for single photon detection and have a high resistivity against magnetic fields. The disadvantage of these devices was their limited lifetime, due to damage by feedback ions on the photocathode. The lifetime of various types of MCP-PMTs from different manufactures has been tested under conditions similar to that in the…

PhysicsNuclear and High Energy PhysicsPhotomultiplierbusiness.industryDetectorPhotocathodeAtomic layer depositionOpticsDetection of internally reflected Cherenkov lightQuantum efficiencyMicrochannel plate detectorbusinessInstrumentationCherenkov radiationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Simulation and reconstruction of the PANDA Barrel DIRC

2014

Hadronic particle identification (PID) in the barrel region of the PANDA experiment at the new Facility for Antiproton and Ion Research in Europe (FAIR) at GSI, Darmstadt will be provided by a DIRC (Detection of Internally Reflected Cherenkov light) counter. To optimize the performance and reduce the detector cost, detailed simulations of different design elements, such as the width of the radiators, the shape of the expansion volume, and the type of focusing system, were performed using Geant. Custom reconstruction algorithms were developed to match the detector geometry. We will discuss the single photon resolution and photon yield as well as the PID performance for the Barrel DIRC baseli…

PhysicsNuclear and High Energy PhysicsPhotonPhysics::Instrumentation and DetectorsCherenkov detectorDetectorBarrel (horology)PID controllerParticle identificationlaw.inventionNuclear physicsDetection of internally reflected Cherenkov lightlawFacility for Antiproton and Ion ResearchHigh Energy Physics::ExperimentNuclear ExperimentInstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Particle Identification with DIRCs at PANDA

2019

The DIRC technology (Detection of Internally Reflected Cherenkov light) offers an excellent possibility to minimize the form factor of Cherenkov detectors in hermetic high energy detectors. The PANDA experiment at FAIR in Germany will combine a barrel-shaped DIRC with a disc-shaped DIRC to cover an angular range of 5 to 140 degrees. Particle identification for pions and kaons with a separation power of 3 standard deviations or more will be provided for momenta between 0.5 GeV/c and 3.5 GeV/c in the barrel region and up to 4 GeV/c in the forward region. Even though the concept is simple, the design and construction of a DIRC is challenging. High precision optics and mechanics are required to…

PhysicsNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsLarge Hadron ColliderPhotonCherenkov detectorbusiness.industryPhysics::Instrumentation and DetectorsDetectorFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)Particle identificationlaw.inventionOpticslawDetection of internally reflected Cherenkov lightHigh Energy Physics::ExperimentParticle beambusinessInstrumentationCherenkov radiation
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