Search results for "Dark current"

showing 5 items of 15 documents

Search for Supernova Neutrino-Bursts with the AMANDA Detector

2001

The core collapse of a massive star in the Milky Way will produce a neutrino burst, intense enough to be detected by existing underground detectors. The AMANDA neutrino telescope located deep in the South Pole ice can detect MeV neutrinos by a collective rate increase in all photo-multipliers on top of dark noise. The main source of light comes from positrons produced in the CC-reaction of anti-electron neutrinos on free protons $\antinue + p \to e^+ + n$. This paper describes the first supernova search performed on the full sets of data taken during 1997 and 1998 (215 days of live time) with 302 of the detector's optical modules. No candidate events resulted from this search. The performan…

PhysicsPhysics::Instrumentation and DetectorsMilky WayAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)DetectorFOS: Physical sciencesAstronomyAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGalaxySupernovaPositronHigh Energy Physics::ExperimentNeutrinoCharged currentAstrophysics::Galaxy AstrophysicsDark current
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Silicon photomultiplier properties at cryogenic temperatures

2015

Abstract The properties of different types of silicon photomultipliers (SiPMs) were studied at cryogenic temperatures. In liquid nitrogen at 77 K, problems with quenching in Hamamatsu SiPMs and with the protective epoxy layer, covering Zecotek SiPMs, were observed. Tests with one Zecotek SiPM were successful after removal of the epoxy layer. In liquid helium at 4 K, fast signals with pulse lengths shorter than 50 ns were observed, the dark count rate was below 10 Hz and no after-pulses were detected. The gain, as a function of over-voltage, was comparable to room temperature. The SiPM׳s response to photons was found to be linear with intensity for low light levels and single-photon detectio…

PhysicsQuenchingNuclear and High Energy PhysicsPhotonbusiness.industryLiquid heliumEpoxyLiquid nitrogenlaw.inventionSilicon photomultiplierOpticslawvisual_artvisual_art.visual_art_mediumOptoelectronicsbusinessInstrumentationIntensity (heat transfer)Dark currentNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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A Wavelength-shifting Optical Module (WOM) for in-ice neutrino detectors

2016

7th Very Large Volume Neutrino Telescope Workshop, Rome, Italy, 14 Sep 2015 - 16 Sep 2015 ; The European physical journal / Web of Conferences 116, 01006 (2016). doi:10.1051/epjconf/201611601006

PhysicsTotal internal reflection010504 meteorology & atmospheric sciences010308 nuclear & particles physicsbusiness.industryPhysics::Instrumentation and DetectorsPhysicsQC1-999Astrophysics::High Energy Astrophysical PhenomenaDetectorWavelength shifter01 natural sciencesNoise (electronics)530WavelengthOpticsNeutrino detector0103 physical sciencesddc:530businessCherenkov radiation0105 earth and related environmental sciencesDark current
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Preliminary radiation hardness tests of single photon Si detectors

2010

Single photon Si detectors were fabricated by STMicroelectronics and fully characterized in standard operation conditions and after irradiations. Both single cells and arrays, of dimensions ranging from 5x5 up to 64x64, were electrically tested. The devices operation was studied as a function of the temperature from -25 degrees C to 65 degrees C varying the voltage over breakdown, from 5% up to 20% of the breakdown voltage before and after irradiation using both light ions, 10 MeV B ions to doses in the range 3x10(7)-5x10(10) cm(-2), and X-rays irradiations in the range 0.5-20 krad(Si). Optical characterization was performed using a laser at 659 nm and opportunely chosen filters to vary the…

Physicsbusiness.industryOptical powerSilicon Photomultiplier single photon avalanche diode dark count gain light ion irradiation X-rays irradiationSilicon photomultiplierOpticsSingle-photon avalanche diodeRadiation damageOptoelectronicsBreakdown voltageIrradiationbusinessRadiation hardeningDark current
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Dynamical analysis of electron transport in RF cavities and photomultipliers tubes

2021

El objetivo de este trabajo es el estudio de la dinámica de haces y corrientes de electrones en cavidades aceleradoras de radiofrecuencia (RF) y en tubos fotomultiplicadores. Por una parte, los haces de electrones presentan una gran importancia histórica tanto en aplicaciones directas (televisiones, hornos de microondas, tratamiento del cáncer), como en la generación de radiación sincrotrón. La última generación de fuentes de rayos X muy brillantes se basa en los láseres de electrones libres (XFEL). No obstante, para producir los haces de electrones que emitirán dichos rayos X como radiación sincrotrón, se necesitan campos eléctricos de gran intensidad lo que produce que, debido a la emisió…

secondary electron emissionphotomultiplier tubesBoris methodsimulationselectron transportdark currentsrf cavities
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