0000000000200437

AUTHOR

Irina Mocioiu

showing 12 related works from this author

Volume IV The DUNE far detector single-phase technology

2020

This document was prepared by the DUNE collaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. The DUNE collaboration also acknowledges the international, national, and regional funding agencies supporting the institutions who have contributed to completing this Technical Design Report.

Technology530 Physicsmedia_common.quotation_subjectNeutrino oscillations liquid Argon TPC DUNE technical design report single phase LArTPCElectronsFREE-ELECTRONS01 natural sciences7. Clean energy09 Engineering030218 nuclear medicine & medical imagingStandard Model03 medical and health sciencesneutrino0302 clinical medicineLIQUID ARGON0103 physical sciencesGrand Unified TheoryHigh Energy PhysicsAerospace engineeringInstrumentationInstruments & InstrumentationMathematical Physicsmedia_commonPhysicsScience & Technology02 Physical Sciences010308 nuclear & particles physicsbusiness.industryDetectorLıquıd ArgonfreeNuclear & Particles PhysicsSymmetry (physics)UniverseLong baseline neutrino experiment CP violationAntimatterNeutrinobusinessEvent (particle physics)
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First results on ProtoDUNE-SP liquid argon time projection chamber performance from a beam test at the CERN Neutrino Platform

2020

The ProtoDUNE-SP detector was constructed and operated on the CERN Neutrino Platform. We thank the CERN management for providing the infrastructure for this experiment and gratefully acknowledge the support of the CERN EP, BE, TE, EN, IT and IPT Departments for NP04/ProtoDUNE-SP. This documentwas prepared by theDUNEcollaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. This work was supported by CNPq, FAPERJ, FAPEG and FAPESP, Brazil; CFI, IPP and NSERC, Canada; CERN; MSMT, Czech Republi…

TechnologyHIGH-ENERGYPhysics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsfar detectorbeam transportNoble liquid detectors (scintillation ionization double-phase)Cms Experıment01 natural sciences7. Clean energy09 EngineeringParticle identificationHigh Energy Physics - Experiment030218 nuclear medicine & medical imagingHigh Energy Physics - Experiment (hep-ex)0302 clinical medicineNoble liquid detectors (scintillationDetectors and Experimental TechniquesInstrumentationInstruments & Instrumentationphysics.ins-dettime resolutionMathematical PhysicsPhysics02 Physical SciencesTime projection chamberLarge Hadron ColliderDetectorInstrumentation and Detectors (physics.ins-det)double-phase)Nuclear & Particles PhysicsLIGHTNeutrinoParticle Physics - ExperimentperformanceNoble liquid detectors(scintillation ionization double-phase)noiseCERN LabLarge detector systems for particle and astroparticle physics Noble liquid detectors (scintillation ionization double-phase) Time projection Chambers (TPC)530 Physicsenergy lossTime projection chambersFOS: Physical sciencesParticle detectorNuclear physics03 medical and health sciencesneutrino: deep underground detector0103 physical sciencesionizationDeep Underground Neutrino ExperimentHigh Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]signal processingactivity reportScience & Technology010308 nuclear & particles physicshep-exLarge detector systems for particle and astroparticle physicsTime projection Chambers (TPC)530 Physiksensitivitycalibrationtime projection chamber: liquid argonExperimental High Energy PhysicsLarge detector systems for particle and astroparticle physicsingle-phase)Large detector systems for particle and astroparticle physics; Noble liquid detectors (scintillation ionization double-phase); Time projection Chambers (TPC)High Energy Physics::Experimentphoton: detectorparticle identificationcharged particle: irradiationBeam (structure)
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Neutrino interaction classification with a convolutional neural network in the DUNE far detector

2020

The Deep Underground Neutrino Experiment is a next-generation neutrino oscillation experiment that aims to measure CP-violation in the neutrino sector as part of a wider physics program. A deep learning approach based on a convolutional neural network has been developed to provide highly efficient and pure selections of electron neutrino and muon neutrino charged-current interactions. The electron neutrino (antineutrino) selection efficiency peaks at 90% (94%) and exceeds 85% (90%) for reconstructed neutrino energies between 2–5 GeV. The muon neutrino (antineutrino) event selection is found to have a maximum efficiency of 96% (97%) and exceeds 90% (95%) efficiency for reconstructed neutrino…

Neutrino Oscillations. Neutrino detectors.Physics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsfar detector01 natural sciencesPhysics Particles & FieldsHigh Energy Physics - Experimentcharged currentHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Particle Physics ExperimentsMuon neutrinoneutrino/e: particle identificationNeutrino detectorsDetectors and Experimental Techniquesphysics.ins-detCharged currentneutrino: interactionInformáticaPhysicsTelecomunicacionesNeutrino oscillationsPhysicsNeutrino interactions neural network DUNE Deep Underground Neutrino ExperimentInstrumentation and Detectors (physics.ins-det)Experiment (hep-ex)Neutrino detectorPhysical SciencesCP violationNeutrinoParticle Physics - ExperimentParticle physicsdata analysis method530 Physicsneural networkAstrophysics::High Energy Astrophysical PhenomenaCONSERVATIONFOS: Physical sciencesAstronomy & AstrophysicsDeep Learningneutrino: deep underground detectorneutrino physics0103 physical sciencesNeutrino Oscillations. Neutrino detectorsObject DetectionNeutrinoCP: violationDeep Underground Neutrino ExperimentHigh Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrinos010306 general physicsNeutrino oscillationneutrino/mu: particle identificationIOUScience & TechnologyDUNENeutrino interactions010308 nuclear & particles physicshep-exHigh Energy Physics::PhenomenologyFísicaNeutrino InteractionDetector530 PhysiksensitivityefficiencyHigh Energy Physics::ExperimentElectron neutrino
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Atmospheric neutrinos in ice and measurement of neutrino oscillation parameters

2010

The main goal of the IceCube Deep Core array is to search for neutrinos of astrophysical origins. Atmospheric neutrinos are commonly considered as a background for these searches. We show that the very high statistics atmospheric neutrino data can be used to obtain precise measurements of the main oscillation parameters.

AstrofísicaNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemCosmic neutrino backgroundHigh Energy Physics - PhenomenologyNeutrino detector13. Climate actionMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomy
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Theory of Neutrinos: A White Paper

2005

During 2004, four divisions of the American Physical Society commissioned a study of neutrino physics to take stock of where the field is at the moment and where it is going in the near and far future. Several working groups looked at various aspects of this vast field. The summary was published as a main report entitled ``The Neutrino Matrix'' accompanied by short 50 page versions of the report of each working group. Theoretical research in this field has been quite extensive and touches many areas and the short 50 page report provided only a brief summary and overview of few of the important points. The theory discussion group felt that it may be of value to the community to publish the e…

Neutrino mass physics; Matter-antimatter asymmetry of the UniverseParticle physicsSupersymmetric Standard ModelPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaElectric-dipole momentsPhysics beyond the Standard ModelFOS: Physical sciencesGeneral Physics and AstronomyTheoretical researchHigh Energy Physics - Phenomenology (hep-ph)White paperSee-saw mechanismneutriniPublicationParticle Physics - PhenomenologyPhysicsLepton-flavor violationDiscussion groupbusiness.industryHigh Energy Physics::PhenomenologyFísicaMatter-antimatter asymmetry of the UniverseDouble beta decaySettore FIS/02 - Fisica Teorica Modelli e Metodi MatematiciEpistemologyElectroweak symmetry-breakingHigh Energy Physics - PhenomenologyLarge extra dimensionsNeutrino mass physicsHeavy Majorana neutrinosHigh Energy Physics::ExperimentRight-handed neutrinoNeutrinoAnomalous magnetic momentWorking groupbusiness
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Gravitational Lensing of Supernova Neutrinos

2006

The black hole at the center of the galaxy is a powerful lens for supernova neutrinos. In the very special circumstance of a supernova near the extended line of sight from Earth to the galactic center, lensing could dramatically enhance the neutrino flux at Earth and stretch the neutrino pulse.

Solar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsGalactic CenterAstrophysics (astro-ph)AstronomyAstronomy and AstrophysicsSolar neutrino problemGalaxySupernovaHigh Energy Physics - PhenomenologyGravitational lensPhysics::Space PhysicsMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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Volume I. Introduction to DUNE

2020

Journal of Instrumentation 15(08), T08008 (1-228) (2020). doi:10.1088/1748-0221/15/08/T08008

detector: technologydeep underground detector [neutrino]530 PhysicsPhysics::Instrumentation and DetectorsData managementmedia_common.quotation_subjectfar detector610Long baseline neutrino experiment CP violation01 natural sciences030218 nuclear medicine & medical imagingNeutrino oscillations. Neutrino Detectors. CP violation. Matter stabilitydesign [detector]03 medical and health sciencesneutrinoneutrino: deep underground detector0302 clinical medicinenear detector0103 physical sciencesDeep Underground Neutrino Experimentddc:610Neutrino oscillationInstrumentationdetector: designMathematical Physicsactivity reportmedia_common010308 nuclear & particles physicsbusiness.industryNeutrino oscillations. Neutrino Detectors. CP violation. Matter stability.DetectorVolume (computing)Modular designtime projection chamber: liquid argonUniversetechnology [detector]liquid argon [time projection chamber]Systems engineeringHigh Energy Physics::ExperimentNeutrino oscillations DUNE technical design report executive summary detector technologiesdata managementNeutrinobusiness
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Atmospheric neutrino oscillations and tau neutrinos in ice

2010

The main goal of the IceCube Deep Core Array is to search for neutrinos of astrophysical origins. Atmospheric neutrinos are commonly considered as a background for these searches. We show here that cascade measurements in the Ice Cube Deep Core Array can provide strong evidence for tau neutrino appearance in atmospheric neutrino oscillations. Controlling systematic uncertainties will be the limiting factor in the analysis. A careful study of these tau neutrinos is crucial, since they constitute an irreducible background for astrophysical neutrino detection.

PhysicsAstrofísicaNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical sciencesAstrophysicsSolar neutrino problem01 natural sciencesCosmic neutrino backgroundHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino detector13. Climate actionTau neutrino0103 physical sciencesMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino astronomyNeutrino010306 general physics
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Oscillation effects on high-energy neutrino fluxes from astrophysical hidden sources

2006

High-energy neutrinos are expected to be produced in a vareity of astrophysical sources as well as in optically thick hidden sources. We explore the matter-induced oscillation effects on emitted neutrino fluxes of three different flavors from the latter class. We use the ratio of electron and tau induced showers to muon tracks, in upcoming neutrino telescopes, as the principal observable in our analysis. This ratio depends on the neutrino energy, density profile of the sources and on the oscillation parameters. The largely unknown flux normalization drops out of our calculation and only affects the statistics. For the current knowledge of the oscillation parameters we find that the matter-i…

Nuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics01 natural sciences7. Clean energyPartícules (Física nuclear)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationPhysicsMuon010308 nuclear & particles physicsOscillationAstrophysics (astro-ph)Solar neutrino problemHigh Energy Physics - PhenomenologyNeutrino detector13. Climate actionMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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Neutrino mass hierarchy extraction using atmospheric neutrinos in ice

2008

We show that the measurements of 10 GeV atmospheric neutrinos by an upcoming array of densely packed phototubes buried deep inside the IceCube detector at the South Pole can be used to determine the neutrino mass hierarchy for values of sin^2(2theta13) close to the present bound, if the hierarchy is normal. These results are obtained for an exposure of 100 Mton years and systematic uncertainties up to 10%.

AstrofísicaNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesStatistical analysis010306 general physicsNeutrino oscillationPhysicsHierarchy (mathematics)010308 nuclear & particles physicsAstrophysics (astro-ph)DetectorAstrophysics::Instrumentation and Methods for AstrophysicsHigh Energy Physics - PhenomenologyNeutrino detector13. Climate actionHigh Energy Physics::ExperimentNeutrinoMass hierarchy
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Volume III. DUNE far detector technical coordination

2020

The preponderance of matter over antimatter in the early universe, the dynamics of the supernovae that produced the heavy elements necessary for life, and whether protons eventually decay-these mysteries at the forefront of particle physics and astrophysics are key to understanding the early evolution of our universe, its current state, and its eventual fate. The Deep Underground Neutrino Experiment (DUNE) is an international world-class experiment dedicated to addressing these questions as it searches for leptonic charge-parity symmetry violation, stands ready to capture supernova neutrino bursts, and seeks to observe nucleon decay as a signature of a grand unified theory underlying the st…

Technology530 PhysicsPhysics::Instrumentation and Detectorsmedia_common.quotation_subjectContext (language use)01 natural sciences09 Engineering030218 nuclear medicine & medical imagingneutrino03 medical and health sciences0302 clinical medicine0103 physical sciencesGrand Unified TheoryDeep Underground Neutrino ExperimentHigh Energy PhysicsInstruments & InstrumentationNeutrino oscillations liquid Argon TPC technical design report technical coordinationInstrumentationMathematical Physicsmedia_commonScience & Technology02 Physical Sciences010308 nuclear & particles physicsDetectorVolume (computing)530 PhysikNuclear & Particles PhysicsUniverseSystems engineeringHigh Energy Physics::ExperimentState (computer science)NeutrinoLong baseline neutrino experiment CP violationJournal of Instrumentation
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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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