Search results for "electron neutrino"

showing 10 items of 39 documents

Simulation and optimization of the implantation of holmium atoms into metallic magnetic microcalorimeters for neutrino mass determination experiments

2017

Abstract Several novel experiments designed to investigate the electron neutrino mass in the sub-eV region are based on the calorimetric measurement of the 163Ho electron capture spectrum. For this the 163Ho source, with a required activity of the order of 1 to 100 Bq , needs to be enclosed in the detector, having a volume smaller than 10 − 3 mm 3 . Ion implantation is presently considered to be the most reliable method to enclose this source in the detector homogeneously distributed in a well defined volume. We have investigated the distribution of implanted holmium ions in different target materials and for different implantation energies by means of Monte Carlo simulations based on the S…

010302 applied physicsPhysicsNuclear and High Energy PhysicsElectron captureMonte Carlo methodDetectorchemistry.chemical_element01 natural sciencesIonIon implantationchemistry0103 physical sciencesAtomic physicsNeutrino010306 general physicsHolmiumInstrumentationElectron neutrinoNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
researchProduct

Mu-tau neutrino refraction and collective three-flavor transformations in supernovae

2008

9 pages, 6 figures.-- PACS nrs.: 14.60.Pq; 97.60.Bw.-- ArXiv pre-print available at: http://arxiv.org/abs/0712.1137

AstrofísicaHistoryNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and Detectors[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]FlavourFOS: Physical sciencesAstrophysicsAstrophysics01 natural sciencesPartícules (Física nuclear)Education[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Phenomenology (hep-ph)Tau neutrino0103 physical sciencesRefraction (sound)010306 general physicsNeutrino oscillationPhysicsMuon010308 nuclear & particles physicsAstrophysics (astro-ph)High Energy Physics::PhenomenologySolar neutrino problemComputer Science ApplicationsSupernovaHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Measurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoElectron neutrino
researchProduct

Low-energy Neutrino Astronomy in LENA

2015

LENA (Low Energy Neutrino Astronomy) is a proposed next-generation neutrino detector based on 50 kilotons of liquid scintillator. The low detection threshold, good energy resolution and excellent background rejection inherent to the liquid-scintillator detectors make LENA a versatile observatory for low-energy neutrinos from astrophysical and terrestrial sources. In the framework of the European LAGUNA-LBNO design study, LENA is also considered as far detector for a very-long baseline neutrino beam from CERN to Pyhasalmi ¨ (Finland). The present contribution gives an overview LENA’s broad research program, highlighting the unique capabilities of liquid scintillator for the detection of low-…

LENAPhysicsParticle physicsta114Physics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologySolar neutrino problemPhysics and Astronomy(all)astroparticle physics. underground physicsNuclear physicslow-energy neutrino astronomyNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoNeutrino oscillationElectron neutrinoPhysics Procedia
researchProduct

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
researchProduct

2020 global reassessment of the neutrino oscillation picture

2021

We present an updated global fit of neutrino oscillation data in the simplest three-neutrino framework. In the present study we include up-to-date analyses from a number of experiments. Concerning the atmospheric and solar sectors, we give updated analyses of DeepCore and SNO data, respectively. We have also included the latest electron antineutrino data collected by the Daya Bay and RENO reactor experiments, and the long-baseline T2K and NO$\nu$A measurements. These new analyses result in more accurate measurements of $\theta_{13}$, $\theta_{12}$, $\Delta m_{21}^2$ and $|\Delta m_{31}^2|$. The best fit value for the atmospheric angle $\theta_{23}$ lies in the second octant, but first octan…

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciences01 natural sciences7. Clean energyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)CUOREDouble beta decay0103 physical sciencesNeutrino Physicslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsNeutrino oscillationNOνAPhysicsSudbury Neutrino Observatory010308 nuclear & particles physicsHigh Energy Physics - Phenomenology13. Climate actionBeyond Standard Modellcsh:QC770-798CP violationHigh Energy Physics::ExperimentNeutrinoElectron neutrinoAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
researchProduct

Evidence of Electron Neutrino Appearance in a Muon Neutrino Beam

2013

The T2K Collaboration reports evidence for electron neutrino appearance at the atmospheric mass splitting, vertical bar Delta m(32)(2)vertical bar approximate to 2.4 X 10(-3) eV(2). An excess of electron neutrino interactions over background is observed from a muon neutrino beam with a peak energy of 0.6 GeV at the Super-Kamiokande (SK) detector 295 km from the beam's origin. Signal and background predictions are constrained by data from near detectors located 280 m from the neutrino production target. We observe 11 electron neutrino candidate events at the SK detector when a background of 3.3 +/- 0.4(syst) events is expected. The background-only hypothesis is rejected with a p value of 0.0…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsFOS: Physical sciencesFluxddc:500.201 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Pion0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Momentum rangeMuon neutrino010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsT2K experimentFísicaHigh Energy Physics::ExperimentNeutrinoAbsorption cross-sectionsElectron neutrinoBeam (structure)
researchProduct

Detecting the upturn of the solar 8B neutrino spectrum with LENA

2014

LENA ( L ow E nergy N eutrino A stronomy) has been proposed as a next generation 50 kt liquid scintillator detector. The large target mass allows a high precision measurement of the solar 8 B neutrino spectrum, with an unprecedented energy threshold of 2 MeV. Hence, it can probe the MSW-LMA prediction for the electron neutrino survival probability in the transition region between vacuum and matter-dominated neutrino oscillations. Based on Monte Carlo simulations of the solar neutrino and the corresponding background spectra, it was found that the predicted upturn of the solar 8 B neutrino spectrum can be detected with 5 σ significance after 5 years.

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsSolar neutrinoSolar neutrinosFOS: Physical sciencesAstrophysicsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Neutrino oscillationInstrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)PhysicsHigh Energy Physics::PhenomenologyInstrumentation and Detectors (physics.ins-det)Solar neutrino problemlcsh:QC1-999ddc:Neutrino detectorAstrophysics - Solar and Stellar AstrophysicsMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyAstrophysics - Instrumentation and Methods for AstrophysicsElectron neutrinolcsh:PhysicsPhysics Letters B
researchProduct

A search for neutrino–antineutrino mass inequality by means of sterile neutrino oscillometry

2015

The investigation of the oscillation pattern induced by the sterile neutrinos might determine the oscillation parameters, and at the same time, allow to probe CPT symmetry in the leptonic sector through neutrino-antineutrino mass inequality. We propose to use a large scintillation detector like JUNO or LENA to detect electron neutrinos and electron antineutrinos from MCi electron capture or beta decay sources. Our calculations indicate that such an experiment is realistic and could be performed in parallel to the current research plans for JUNO and RENO. Requiring at least 5$\sigma$ confidence level and assuming the values of the oscillation parameters indicated by the current global fit, w…

Nuclear and High Energy PhysicsSterile neutrinoParticle physicsPhysics - Instrumentation and DetectorsElectron captureCPT symmetryFOS: Physical sciencesElectronHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)sterile neutrinoslcsh:Nuclear and particle physics. Atomic energy. RadioactivityNeutrino oscillationPhysicsta114OscillationHigh Energy Physics::PhenomenologyInstrumentation and Detectors (physics.ins-det)oscillation patternHigh Energy Physics - Phenomenologyelectron antineutrinoslcsh:QC770-798High Energy Physics::ExperimentNeutrinoGALLEXelectron neutrinos
researchProduct

Improved limit on the electron-antineutrino rest mass from tritium ß-decay

1993

Abstract The endpoint region of the β-spectrum of tritium was remeasured by an electrostatic spectrometer with magnetic guiding field. It enabled the search for a rest mass of the electron-antineutrino with improved precision. The result is m2v=−39±34stat±15syst(eV/c2)2, from which an upper limit of mv m( T )−m( 3 He )=18 591±3 eV /c 2 .

Nuclear physicsPhysicsNuclear and High Energy PhysicsField (physics)SpectrometerElectron energy spectrumTritiumInvariant massddc:530Limit (mathematics)Atomic physicsElectron neutrino
researchProduct

Search for Electron Antineutrino Appearance at theΔm2∼1  eV2Scale

2009

The MiniBooNE Collaboration reports initial results from a search for nu{sub m}u->nu{sub e} oscillations. A signal-blind analysis was performed using a data sample corresponding to 3.39x10{sup 20} protons on target. The data are consistent with background prediction across the full range of neutrino energy reconstructed assuming quasielastic scattering, 200<E{sub n}u{sup QE}<3000 MeV: 144 electronlike events have been observed in this energy range, compared to an expectation of 139.2+-17.6 events. No significant excess of events has been observed, both at low energy, 200-475 MeV, and at high energy, 475-1250 MeV. The data are inconclusive with respect to antineutrino oscillations suggested …

Nuclear physicsPhysicsNuclear reactionMiniBooNEParticle physicsLiquid Scintillator Neutrino DetectorQuasielastic scatteringGeneral Physics and AstronomyNeutrinoNuclear ExperimentNeutrino oscillationElectron neutrinoLeptonPhysical Review Letters
researchProduct