0000000000946730

AUTHOR

J. J. Evans

showing 8 related works from this author

Results of the search for neutrinoless double-βdecay inMo100with the NEMO-3 experiment

2015

The NEMO-3 detector, which had been operating in the Modane Underground Laboratory from 2003 to 2010, was designed to search for neutrinoless double $\beta$ ($0\nu\beta\beta$) decay. We report final results of a search for $0\nu\beta\beta$ decays with $6.914$ kg of $^{100}$Mo using the entire NEMO-3 data set with a detector live time of $4.96$ yr, which corresponds to an exposure of 34.3 kg$\cdot$yr. We perform a detailed study of the expected background in the $0\nu\beta\beta$ signal region and find no evidence of $0\nu\beta\beta$ decays in the data. The level of observed background in the $0\nu\beta\beta$ signal region $[2.8-3.2]$ MeV is $0.44 \pm 0.13$ counts/yr/kg, and no events are obs…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsSignal region01 natural sciencesBeta decayLower limitNuclear physicsMAJORANADouble beta decay0103 physical sciencesUnderground laboratoryBeta (velocity)Neutrino010306 general physicsPhysical Review D
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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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Spectral modeling of scintillator for the NEMO-3 and SuperNEMO detectors

2010

We have constructed a GEANT4-based detailed software model of photon transport in plastic scintillator blocks and have used it to study the NEMO-3 and SuperNEMO calorimeters employed in experiments designed to search for neutrinoless double beta decay. We compare our simulations to measurements using conversion electrons from a calibration source of $\rm ^{207}Bi$ and show that the agreement is improved if wavelength-dependent properties of the calorimeter are taken into account. In this article, we briefly describe our modeling approach and results of our studies.

Nuclear and High Energy PhysicsPhotomultiplierTechnologyPhysics - Instrumentation and DetectorsPhotonPhysics::Instrumentation and DetectorsCODEFOS: Physical sciencesScintillator01 natural sciencesHigh Energy Physics - ExperimentPhysics Particles & FieldsNuclear physicsHigh Energy Physics - Experiment (hep-ex)Photomultiplier0202 Atomic Molecular Nuclear Particle And Plasma PhysicsDouble beta decay0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]CalibrationPlastic scintillators[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNuclear Science & TechnologyInstrumentationInstruments & InstrumentationScintillationphysics.ins-detPhysicsScintillationScience & Technology010308 nuclear & particles physicshep-exPhysicsMO-100DetectorInstrumentation and Detectors (physics.ins-det)Double beta decayNuclear & Particles PhysicsCalorimeterPhysics NuclearPhysical SciencesGEANT 4DOUBLE-BETA DECAYOptical photon transport
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PINGU: a vision for neutrino and particle physics at the South Pole

2017

The Precision IceCube Next Generation Upgrade (PINGU) is a proposed low-energy in-fill extension to the IceCube Neutrino Observatory. With detection technology modeled closely on the successful IceCube example, PINGU will provide a 6Mton effective mass for neutrino detection with an energy threshold of a few GeV. With an unprecedented sample of over 60,000 atmospheric neutrinos per year in this energy range, PINGU will make highly competitive measurements of neutrino oscillation parameters in an energy range over an order of magnitude higher than long-baseline neutrino beam experiments. PINGU will measure the mixing parameters $\theta_{\rm 23}$ and $\Delta m^2_{\rm 32}$, including the octan…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsmixing [neutrino]atmospheric neutrinos; IceCube Neutrino Observatory; neutrino oscillations; PINGU; Nuclear and High Energy Physicspole7. Clean energy01 natural sciencesPINGUIceCube Neutrino ObservatoryIceCubeHigh Energy Physics - ExperimentObservatoryPhysicssolar [WIMP]precision measurementAstrophysics::Instrumentation and Methods for Astrophysicsoscillation [neutrino]solar [dark matter]atmosphere [neutrino]threshold [energy]mass difference [neutrino]atmospheric neutrinosobservatoryHigh Energy Physics - PhenomenologyUpgradeNeutrino detectorupgradeNeutrinoKM3NETperformanceParticle physicsNuclear and High Energy Physicssupernova [neutrino]particle identification [neutrino/tau]Astrophysics::High Energy Astrophysical PhenomenaSUPERNOVA DETECTIONIceCube Neutrino Observatory0103 physical sciencesOSCILLATIONSmass: low [dark matter]unitarityddc:530010306 general physicsNeutrino oscillationneutrino oscillations010308 nuclear & particles physicsAstronomysensitivityKM3NeTPhysics and Astronomymass [neutrino]beam [neutrino]High Energy Physics::ExperimentgalaxyATMOSPHERIC NEUTRINOSMATTERSYSTEMLeptonmixing angle [neutrino]experimental results
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Detailed studies of $^{100}$Mo two-neutrino double beta decay in NEMO-3

2019

The full data set of the NEMO-3 experiment has been used to measure the half-life of the two-neutrino double beta decay of $^{100}$Mo to the ground state of $^{100}$Ru, $T_{1/2} = \left[ 6.81 \pm 0.01\,\left(\mbox{stat}\right) ^{+0.38}_{-0.40}\,\left(\mbox{syst}\right) \right] \times10^{18}$ y. The two-electron energy sum, single electron energy spectra and distribution of the angle between the electrons are presented with an unprecedented statistics of $5\times10^5$ events and a signal-to-background ratio of ~80. Clear evidence for the Single State Dominance model is found for this nuclear transition. Limits on Majoron emitting neutrinoless double beta decay modes with spectral indices of …

Particle physicsS029MTPhysics and Astronomy (miscellaneous)FOS: Physical sciencesElementary particle[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]nucl-exinvariance: Lorentz01 natural sciences7. Clean energyneutrinoless double beta decaydecay modesPhysics Particles & Fieldsdouble-beta decay: (0neutrino)SEARCHDouble beta decay0103 physical sciencesground stateNuclear Experiment (nucl-ex)010306 general physics0206 Quantum PhysicsEngineering (miscellaneous)Nuclear ExperimentMajoronS076H2NPhysicsScience & TechnologyHALF-LIFE010308 nuclear & particles physicsPhysicsMO-100High Energy Physics::PhenomenologyNuclear & Particles PhysicsMajoronviolation: Lorentznucleus: transitionSTATESstatisticsPhysical Sciences0202 Atomic Molecular Nuclear Particle and Plasma Physicsspectralelectron: energy spectrumHigh Energy Physics::ExperimentNeutrinoGround stateEnergy (signal processing)Radioactive decayLepton
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Search for neutrinoless double-beta decay ofMo100with the NEMO-3 detector

2014

We report the results of a search for the neutrinoless double-$\beta$ decay (0$\nu\beta\beta$) of $^{100}$Mo, using the NEMO-3 detector to reconstruct the full topology of the final state events. With an exposure of 34.7 kg.y, no evidence for the 0$\nu\beta\beta$ signal has been found, yielding a limit for the light Majorana neutrino mass mechanism of $T_{1/2}(0\nu\beta\beta)>1.1 \times 10^{24}$ years (90% C.L.) once both statistical and systematic uncertainties are taken into account. Depending on the Nuclear Matrix Elements this corresponds to an upper limit on the Majorana effective neutrino mass of $ < 0.3-0.8$ eV (90% C.L.). Constraints on other lepton number violating mechanisms of 0$…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsElectron01 natural sciencesBeta decayLepton numberNuclear physicsMAJORANADouble beta decay0103 physical sciencesBeta (velocity)Neutrino010306 general physicsEnergy (signal processing)Physical Review D
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Combined sensitivity to the neutrino mass ordering with JUNO, the IceCube Upgrade, and PINGU

2020

Physical review / D 101(3), 032006 (1-19) (2020). doi:10.1103/PhysRevD.101.032006

Physics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsantineutrino/e: energy spectrumJoint analysishiukkasfysiikka7. Clean energy01 natural sciencesString (physics)PINGUHigh Energy Physics - ExperimentSubatomär fysikHigh Energy Physics - Experiment (hep-ex)neutrino: atmosphereSubatomic Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Particle Physics Experimentsneutrino: massphysics.ins-detPhysicsJUNOPhysicsneutriinotoscillation [neutrino]Instrumentation and Detectors (physics.ins-det)massa (fysiikka)atmosphere [neutrino]tensionneutrino: nuclear reactormass difference [neutrino]ddc:UpgradePhysique des particules élémentairesnuclear reactor [neutrino]proposed experimentNeutrinoperformanceParticle physicsAstrophysics::High Energy Astrophysical Phenomenaneutrino: mass differenceFOS: Physical sciencesddc:500.25300103 physical sciencesEnergy spectrumIceCube: upgradeOSCILLATIONSddc:530Sensitivity (control systems)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationenergy spectrum [antineutrino/e]hep-ex010308 nuclear & particles physicssensitivityPhysics and Astronomymass [neutrino]stringupgrade [IceCube]High Energy Physics::ExperimentReactor neutrinoneutrino: oscillationMATTER
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Computational Techniques for the Analysis of Small Signals in High-Statistics Neutrino Oscillation Experiments

2020

The current and upcoming generation of Very Large Volume Neutrino Telescopes – collecting unprecedented quantities of neutrino events – can be used to explore subtle effects in oscillation physics, such as (but not restricted to) the neutrino mass ordering. The sensitivity of an experiment to these effects can be estimated from Monte Carlo simulations. With the high number of events that will be collected, there is a trade-off between the computational expense of running such simulations and the inherent statistical uncertainty in the determined values. In such a scenario, it becomes impractical to produce and use adequately-sized sets of simulated events with traditional methods, such as M…

data analysis methodNuclear and High Energy PhysicsMonte Carlo methodFVLV nu TData analysis; Detector; KDE; MC; Monte Carlo; Neutrino; Neutrino mass ordering; Smoothing; Statistics; VLVνTData analysisKDEFOS: Physical sciences01 natural sciencesIceCubeHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)statistical analysisnumerical methods0103 physical sciencesStatisticsNeutrinoddc:530Sensitivity (control systems)MC010306 general physicsNeutrino oscillationInstrumentation and Methods for Astrophysics (astro-ph.IM)InstrumentationMonte CarloPhysicsVLVνT010308 nuclear & particles physicsOscillationStatisticsoscillation [neutrino]ObservableDetectorMonte Carlo [numerical calculations]WeightingNeutrino mass orderingPhysics and AstronomyPhysics - Data Analysis Statistics and ProbabilityPhysique des particules élémentairesNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsMATTERData Analysis Statistics and Probability (physics.data-an)SmoothingSmoothing
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