0000000000241027

AUTHOR

M Selvi

showing 2 related works from this author

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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International Scoping Study (ISS) for a future neutrino factory and Super-Beam facility. Detectors and flux instrumentation for future neutrino facil…

2009

Technical report by The ISS Detector Working Group; This report summarises the conclusions from the detector group of the International Scoping Study of a future Neutrino Factory and Super-Beam neutrino facility. The baseline detector options for each possible neutrino beam are defined as follows: 1. A very massive (Megaton) water Cherenkov detector is the baseline option for a sub-GeV Beta Beam and Super Beam facility. 2. There are a number of possibilities for either a Beta Beam or Super Beam (SB) medium energy facility between 1-5 GeV. These include a totally active scintillating detector (TASD), a liquid argon TPC or a water Cherenkov detector. 3. A 100 kton magnetized iron neutrino det…

Particle physicsneutrino factoryCherenkov detectorPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaBeam-line instrumentation (beam position and profile monitorsddc:500.27. Clean energy01 natural sciencesBunch length monitors)law.inventionNuclear physicsneutrinolaw0103 physical sciencesbeam-intensity monitorsneutrino oscillation[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Detectors and Experimental Techniques010306 general physicsInstrumentationbeam-intensity monitorMathematical PhysicsdetectorsPhysicsMuon010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physicsDetectorFísicaBeam-intensity monitorsFIS/01 - FISICA SPERIMENTALENeutrino detectorLarge detector systems for particle and astroparticle physicBeam-line instrumentation (beam position and profile monitorbunch length monitors)Physics::Accelerator PhysicsNeutrino FactoryHigh Energy Physics::ExperimentCloud chamberNeutrinoBeam (structure)
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