Search results for "Neutrino detector"

showing 10 items of 222 documents

Experimental searches on sterile neutrinos

2015

While neutrino oscillations among the three active neutrino flavors are by now well established, several anomalies observed at relatively short baselines in oscillation experiments hint towards the existence of one or more additional sterile neutrino flavors. As a consequence, several experiments are in preparation that are dedicated to test the sterile neutrino hypothesis. The present contribution gives an overview of the on-going experimental efforts, highlighting the two projects that are foreseen to start in 2015: SOX deploying a radioactive neutrino source at short distance from the BOREXINO detector at LNGS, and STEREO searching for sterile neutrino oscillations at short distance from…

PhysicsSterile neutrinoParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoHigh Energy Physics::PhenomenologySolar neutrino problemNuclear physicsNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationBorexinoProceedings of XIIth International Conference on Heavy Quarks & Leptons 2014 — PoS(HQL2014)
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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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ERRATUM: "Search for High-Energy Muon Neutrinos from the "Naked-Eye" GRB 080319B with the Icecube Neutrino Telescope" (2009, ApJ, 701, 1721)

2009

We have noticed some mistakes in formulae (A2) and (A5) in the appendix of our paper. The errors are not present in the code used in the analysis and hence none of the plots or results is affected. The correct formulae are below.

Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Muon[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Solar neutrino[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]AstronomyAstronomyAstronomy and AstrophysicsAstrophysicsSolar neutrino problem01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Neutrino detectorSpace and Planetary Science0103 physical sciencesNaked eyeNeutrinoNeutrino astronomy010306 general physicsGamma-ray burstGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)
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IceCube: A multipurpose neutrino telescope

2008

IceCube is a new high-energy neutrino telescope which will be coming online in the near future. IceCube will be capable of measuring fluxes of all three flavors of neutrino, and its peak neutrino energy sensitivity will be in the TeV–PeV range. Here, after a brief description of the detector, we describe its anticipated performance with a selection of physics topics: supernovae, extraterrestrial diffuse and point sources of neutrinos, gamma-ray bursts, neutrinos from WIMP annihilation, and cosmic ray composition.

Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoGeneral Physics and AstronomyAstrophysics7. Clean energy01 natural sciencesWIMP0103 physical sciencesNeutrinos010306 general physicsCosmic rays; Neutrinos; WIMPsCosmic raysPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsAstronomySolar neutrino problemWIMPsCosmic neutrino backgroundNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomy
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A method for detection of muon induced electromagnetic showers with the ANTARES detector

2012

The primary aim of ANTARES is neutrino astronomy with upward going muons created in charged current muon neutrino interactions in the detector and its surroundings. Downward going muons are background for neutrino searches. These muons are the decay products of cosmic-ray collisions in the Earths atmosphere far above the detector. This paper presents a method to identify and count electromagnetic showers induced along atmospheric muon tracks with the ANTARES detector. The method is applied to both cosmic muon data and simulations and its applicability to the reconstruction of muon event energies is demonstrated. © 2012 Elsevier B.V. All rights reserved.

Physics::Instrumentation and DetectorsAtmospheric muonsDecay productsNeutrino telescopeElectromagnetic shower identification01 natural sciences7. Clean energyneutrino telescope electromagnetic shower identification high energy muons energy reconstruction; high energy muons; neutrino telescope; electromagnetic shower identification; energy reconstructionMuon neutrinoNEUTRINO TELESCOPE010303 astronomy & astrophysicsInstrumentationEnergy reconstructionPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorAstrophysics::Instrumentation and Methods for AstrophysicsDetectorsHigh energy muonNeutrino detectorMuon colliderNeutrino astronomyFísica nuclearNeutrinoNeutrino telescope; Energy reconstruction; High energy muonsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaFLUXNuclear and High Energy PhysicsParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Charged current[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayMuon neutrinoNuclear physicsElectromagnetism0103 physical sciencesHigh energy physicsneutrino telescope electromagnetic shower identification high energy muons energy reconstructionInstrumentation and Methods for Astrophysics (astro-ph.IM)MuonANTARES010308 nuclear & particles physicsCharged particles[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]FISICA APLICADATEVPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNeutrino astronomyNeutrino telescopesElectro-magnetic showersHigh energy muons
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Synchronization of the distributed readout frontend electronics of the Baby MIND detector

2017

Baby MIND is a new downstream muon range detector for the WGASCI experiment. This article discusses the distributed readout system and its timing requirements. The paper presents the design of the synchronization subsystem and the results of its test.

Physics::Instrumentation and DetectorsComputer sciencebusiness.industryDetectorReadout electronicsSynchronizationNeutrino detectorBackplaneNuclear electronicsHigh Energy Physics::ExperimentElectronicsbusinessDownstream (networking)Computer hardware
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Neutrino probes of the nature of light dark matter

2011

Dark matter particles gravitationally trapped inside the Sun may annihilate into Standard Model particles, producing a flux of neutrinos. The prospects of detecting these neutrinos in future multi-\kton{} neutrino detectors designed for other physics searches are explored here. We study the capabilities of a 34/100 \kton{} liquid argon detector and a 100 \kton{} magnetized iron calorimeter detector. These detectors are expected to determine the energy and the direction of the incoming neutrino with unprecedented precision allowing for tests of the dark matter nature at very low dark matter masses, in the range of 5-50 GeV. By suppressing the atmospheric background with angular cuts, these t…

Physics::Instrumentation and DetectorsDark matterFOS: Physical sciences01 natural sciences7. Clean energyStandard ModelNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsLight dark matterParticle Physics - PhenomenologyHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAnnihilationCalorimeter (particle physics)010308 nuclear & particles physicsDetectorFísicaAstronomy and AstrophysicsHigh Energy Physics - PhenomenologyNeutrino detector13. Climate actionHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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Performance study of a 3×1×1 m3 dual phase liquid Argon Time Projection Chamber exposed to cosmic rays

2021

This work would not have been possible without the support of the Swiss National Science Foundation, Switzerland; CEA and CNRS/IN2P3, France; KEK and the JSPS program, Japan; Ministerio de Ciencia e Innovacion in Spain under grants FPA2016-77347-C2, SEV-2016-0588 and MdM-2015-0509, Comunidad de Madrid, the CERCA program of the Generalitat de Catalunya and the fellowship (LCF/BQ/DI18/11660043) from "La Caixa" Foundation (ID 100010434); the Programme PNCDI III, CERN-RO, under Contract 2/2020, Romania; the U.S. Department of Energy under Grant No. DE-SC0011686. This project has received funding from the European Union's Horizon 2020 Research and Innovation program under Grant Agreement no. 654…

Physics::Instrumentation and DetectorsLibrary scienceargon: gas01 natural sciences7. Clean energyNeutrino detectorArgon gasPolitical scienceParticle tracking detectors0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]media_common.cataloged_instanceNeutrino detectors[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]European union010306 general physicsInstrumentationMathematical Physicsmedia_common010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physicsTime projection Chambers (TPC)time projection chamber: liquid argonParticle tracking detectorTime projection chambercosmic radiationLarge detector systems for particle and astroparticle physicyield: stabilityLiquid argonperformance
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Neutrino oscillation studies with IceCube-DeepCore

2016

IceCube, a gigaton-scale neutrino detector located at the South Pole, was primarily designed to search for astrophysical neutrinos with energies of PeV and higher. This goal has been achieved with the detection of the highest energy neutrinos to date. At the other end of the energy spectrum, the DeepCore extension lowers the energy threshold of the detector to approximately 10 GeV and opens the door for oscillation studies using atmospheric neutrinos. An analysis of the disappearance of these neutrinos has been completed, with the results produced being complementary with dedicated oscillation experiments. Following a review of the detector principle and performance, the method used to make…

Physics::Instrumentation and DetectorsSolar neutrinopoleinteraction [neutrino nucleon]PINGU01 natural sciences7. Clean energyneutrino nucleon: interactionIceCubeenergy: thresholdAstronomi astrofysik och kosmologineutrino: atmosphereAstronomy Astrophysics and Cosmologydetector [neutrino]Physicsneutrino: energy spectrumoscillation [neutrino]Astrophysics::Instrumentation and Methods for Astrophysicsatmosphere [neutrino]threshold [energy]mass difference [neutrino]Cosmic neutrino backgroundneutrino: detectorNeutrino detectorPhysique des particules élémentairesMeasurements of neutrino speedNeutrinoperformanceNuclear and High Energy PhysicsParticle physicsAstrophysics::High Energy Astrophysical Phenomenaneutrino: mass differenceddc:500.2530neutrino: energySOUTH-POLE0103 physical sciencesddc:530010306 general physicsNeutrino oscillation010308 nuclear & particles physicsICEenergy spectrum [neutrino]Solar neutrino problemneutrino: mixing anglePhysics and Astronomyenergy [neutrino]High Energy Physics::Experimentneutrino: oscillationNeutrino astronomyMATTERSYSTEMmixing angle [neutrino]experimental results
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The mass-hierarchy and CP-violation discovery reach of the LBNO long-baseline neutrino experiment.

2014

The next generation neutrino observatory proposed by the LBNO collaboration will address fundamental questions in particle and astroparticle physics. The experiment consists of a far detector, in its first stage a 20 kt LAr double phase TPC and a magnetised iron calorimeter, situated at 2300 km from CERN and a near detector based on a high-pressure argon gas TPC. The long baseline provides a unique opportunity to study neutrino flavour oscillations over their 1st and 2nd oscillation maxima exploring the $L/E$ behaviour, and distinguishing effects arising from $\delta_{CP}$ and matter. In this paper we have reevaluated the physics potential of this setup for determining the mass hierarchy (M…

Physics::Instrumentation and Detectorsfar detectorkaukoputket ja teleskoopit7. Clean energyviolation [CP]CP violation; Neutrino Detectors and Telescopes; Oscillation; Nuclear and High Energy PhysicsHigh Energy Physics - Phenomenology (hep-ph)Observatorymass: hierarchy [neutrino]detector [neutrino]QCPhysicsTime projection chamberLarge Hadron ColliderOscillationmagnetization [iron]oscillation [neutrino]High Energy Physics - PhenomenologyCP violationliquid argon [time projection chamber]CP violationNeutrinoParticle physicsNuclear and High Energy PhysicsCERN Lab530 PhysicseducationFOS: Physical sciencesddc:500.2oscillation [flavor]114 Physical sciencesNuclear physicsphase spacenear detectorstatistical analysisiron [calorimeter]Particle Physics - PhenomenologyAstroparticle physicsNeutrino Detectors and Telescopesta114Físicaflavor [neutrino]CP [phase]CERN SPSMODELproposed [observatory]Oscillation13. Climate actionPhase space[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]gas [argon]beam [neutrino]High Energy Physics::ExperimentMATTERneutrino detectorsCP violation.
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