Search results for "antineutrino"

showing 10 items of 28 documents

Measurement of the atmospheric ?µ energy spectrum from 100 GeV to 200 TeV with the ANTARES telescope

2013

Atmospheric neutrinos are produced during cascades initiated by the interaction of primary cosmic rays with air nuclei. In this paper, a measurement of the atmospheric energy spectrum in the energy range 0.1-200 TeV is presented, using data collected by the ANTARES underwater neutrino telescope from 2008 to 2011. Overall, the measured flux is similar to 25 % higher than predicted by the conventional neutrino flux, and compatible with the measurements reported in ice. The flux is compatible with a single power-law dependence with spectral index gamma (meas)=3.58 +/- 0.12. With the present statistics the contribution of prompt neutrinos cannot be established.

Astrofísica:Desenvolupament humà i sostenible::Medi ambient [Àrees temàtiques de la UPC]Physics and Astronomy (miscellaneous)Raigs còsmicsFluxOceanografia7. Clean energy01 natural scienceslaw.inventionlawUnderwater acousticsEnergy range 0.1 to 200 TeVNeutrino TelescopePhysicsRange (particle radiation)Spectral index[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]atmospheric neutrinoNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsLorentz Invariance ViolationFLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]OscillationsSoroll -- Aspectes ambientalsAstrophysics::High Energy Astrophysical PhenomenaCosmic rayddc:500.2MACRONuclear physicsTelescopeMUONSSEARCH0103 physical sciencesNeutrinsNeutrinos010306 general physicsEngineering (miscellaneous)Cosmic raysDETECTOR:Física::Acústica [Àrees temàtiques de la UPC]ANTARESAtmospheric neutrino antineutrino010308 nuclear & particles physicsAntares telescopeHigh Energy Physics::Phenomenology[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]13. Climate actionFISICA APLICADAlorentz invariance violation; neutrino oscillation; muonsHigh Energy Physics::ExperimentEnergy (signal processing)Bar (unit)European Physical Journal C
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SOX: search for short baseline neutrino oscillations with Borexino

2015

International audience; The Borexino detector has convincingly shown its outstanding performances in the low energy regime through its accomplishments in the observation and study of the solar and geo neutrinos. It is then an ideal tool to perform a state of the art source-based experiment for testing the longstanding hypothesis of a fourth sterile neutrino with ~ eV(2) mass, as suggested by several anomalies accumulated over the past three decades in source, reactor, and accelerator-based experiments. The SOX project aims at successively deploying two intense radioactive sources, made of Cerium (antineutrino) and Chromium (neutrino), respectively, in a dedicated pit located beneath the det…

HistoryParticle physicsSterile neutrinochromium: nuclidePhysics::Instrumentation and DetectorsSolar neutrino[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyEducationNuclear physicsPhysics and Astronomy (all)0103 physical sciencesddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationBorexinoactivity reportPhysics010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyneutrino: particle sourceSolar neutrino problemneutrino: sterilesensitivityComputer Science ApplicationsNeutrino detector13. Climate actioncerium: nuclideMeasurements of neutrino speedHigh Energy Physics::ExperimentBorexinoneutrino: oscillationNeutrinoantineutrino: particle source
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The high precision measurement of the 144Ce activity in the SOX experiment

2015

International audience; In order to perform a resolutive measurement to clarify the neutrino anomalies and to observe possible short distance neutrino oscillations, the SOX (Short distance neutrino Oscillations with BoreXino) experiment is under construction. In the first phase, a 100 kCi (144)Ce-(144)Pr antineutrino source will be placed under the Borexino detector at the Laboratori Nazionali del Gran Sasso (LNGS), in center of Italy, and the rate measurement of the antineutrino events, observed by the very low radioactive background Borexino detector, will be compared with the high precision (< 1%) activity measurement performed by two calorimeters. The source will be embedded in a 19 mm …

HistoryParticle physicsWater flowPhysics::Instrumentation and Detectorstungstenwater[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesParticle detectorEducationPhysics::GeophysicsthermalNuclear physicsPhysics and Astronomy (all)alloy0103 physical sciencesddc:530010306 general physicsNeutrino oscillationNuclear Experimentbackground: radioactivityBorexinoPhysics010308 nuclear & particles physicsprecision measurementcalorimeter: designDetectorantineutrinoComputer Science ApplicationsGran SassoceriumflowMeasuring instrumentHigh Energy Physics::ExperimentBorexinoneutrino: oscillationNeutrinoLepton
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The $^{144}$Ce source for SOX

2015

International audience; The SOX (Short distance neutrino Oscillations with BoreXino) project aims at testing the light sterile neutrino hypothesis. To do so, two artificials sources of antineutrinos and neutrinos respectively will be consecutively deployed at the Laboratori Nazionali del Gran Sasso (LNGS) in close vicinity to Borexino, a large liquid scintillator detector. This document reports on the source production and transportation. The source should exhibit a long lifetime and a high decay energy, a requirement fullfilled by the (144)Ce-(144)Pr pair at secular equilibrium. It will be produced at FSUE “Mayak” PA using spent nuclear fuel. It will then be shielded and packed according t…

HistorySterile neutrinoParticle physicsenergy: decay[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]Scintillator01 natural sciences7. Clean energyEducationNuclear physicsPhysics and Astronomy (all)0103 physical sciencesddc:530010306 general physicsNeutrino oscillationparticle sourceBorexinoPhysicslifetimenucleusSecular equilibriumneutrino: sterileantineutrinosensitivitySpent nuclear fuelComputer Science ApplicationsGran SassoceriumDecay energyradioactivityBorexinoneutrino: oscillationproductionNeutrino
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Solar neutrino detectors as sterile neutrino hunters

2016

International audience; The large size and the very low radioactive background of solar neutrino detectors such as Borexino at the Gran Sasso Laboratory in Italy offer a unique opportunity to probe the existence of neutrino oscillations into new sterile components by means of carefully designed and well calibrated anti-neutrino and neutrino artificial sources. In this paper we briefly summarise the key elements of the SOX experiment, a program for the search of sterile neutrinos (and other short distance effects) by means of a (144)Ce-(144)Pr anti-neutrino source and, possibly in the medium term future, with a (51)Cr neutrino source.

HistorySterile neutrinoParticle physicsneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical Phenomena01 natural sciences7. Clean energyEducationPhysics and Astronomy (all)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationnuclideBorexinoPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemneutrino: sterileComputer Science ApplicationspraseodymiumGran Sassoneutrino: detectorNeutrino detectorcerium: nuclideHigh Energy Physics::Experimentneutrino: oscillationNeutrino astronomyNeutrinoantineutrino: particle source[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Sub-percent precision measurement of neutrino oscillation parameters with JUNO

2022

JUNOneutriino-oskillaatioprecision measurementilmaisimettutkimuslaitteetreactor antineutrinoneutriinotneutrino oscillationhiukkasfysiikka
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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
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Theoretical estimates of supernova-neutrino cross sections for the stable even-even lead isotopes: Charged-current reactions

2016

A detailed study of the charged-current supernova electron neutrino and electron antineutrino scattering off the stable even-mass lead isotopes $A=204$, 206, and 208 is reported in this work. The proton-neutron quasiparticle random-phase approximation (pnQRPA) is adopted to construct the nuclear final and initial states. Three different Skyrme interactions are tested for their isospin and spin-isospin properties and then applied to produce (anti)neutrino-nucleus scattering cross sections for (anti)neutrino energies below 80 MeV. Realistic estimates of the nuclear responses to supernova (anti)neutrinos are computed by folding the computed cross sections with a two-parameter Fermi-Dirac distr…

Particle physicsAstrophysics::High Energy Astrophysical PhenomenaNuclear Theoryneutrino-nucleus interactionsElectronelectron neutrino01 natural sciencesNuclear physics0103 physical sciencesNuclear Experiment010306 general physicsNeutrino oscillationsupernova neutrinosCharged currentPhysicsta114010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyscatteringelectron antineutrinoSupernovalead isotopesIsospinQuasiparticleHigh Energy Physics::ExperimentNeutrinoElectron neutrinoPhysical Review C
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Combined Analysis of Neutrino and Antineutrino Oscillations at T2K.

2017

T2K reports its first results in the search for CP violation in neutrino oscillations using appearance and disappearance channels for neutrino- and antineutrino-mode beams. The data include all runs from January 2010 to May 2016 and comprise 7.482 ×10^(20) protons on target in neutrino mode, which yielded in the far detector 32 e-like and 135 μ-like events, and 7.471 × 10^(20) protons on target in antineutrino mode, which yielded 4 e-like and 66 μ-like events. Reactor measurements of sin(2)2θ(13) have been used as an additional constraint. The one-dimensional confidence interval at 90% for the phase δCP spans the range (−3.13, −0.39) for normal mass ordering. The CP conservation hypothesis …

Particle physicsGeneral PhysicsNeutrino oscillations; CP violation; Neutrino detectors530 PhysicsPhysics MultidisciplinaryFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciences7. Clean energy09 EngineeringHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutrino detectors010306 general physicsNeutrino oscillationGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)01 Mathematical SciencesComputingMilieux_MISCELLANEOUSQCPhysicsScience & Technology02 Physical Sciences010308 nuclear & particles physicshep-exNeutrino oscillationsPhysicsCP violationNeutrino detectorantineutrino oscillationsT2K CollaborationPhysical SciencesCP violationNeutrinoPhysical review letters
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A study of quasi-elastic muon neutrino and antineutrino scattering in the NOMAD experiment

2008

We have studied the muon neutrino and antineutrino quasi-elastic (QEL) scattering reactions ($\nu_\mu n\to \mu^- p$ and $\bar{\nu}_\mu p\to \mu^+ n$) using a set of experimental data collected by the NOMAD collaboration. We have performed measurements of the cross-section of these processes on a nuclear target (mainly Carbon) normalizing it to the total $\nu_\mu$ ($\bar{\nu}_\mu$) charged current cross-section. The results for the flux averaged QEL cross-sections in the (anti)neutrino energy interval 3-100 GeV are $\sigma^{qel}_{\nu_\mu} = (0.92 \pm 0.02 (stat) \pm 0.06 (syst))\times 10^{-38} \cm^2$ and $\sigma{qel}_{\bar{\nu}_\mu} = (0.81 \pm 0.05 (stat) \pm 0.08 (syst))\times 10^{-38} \cm…

Particle physicsPhysics and Astronomy (miscellaneous)FOS: Physical sciences01 natural sciences7. Clean energyHigh Energy Physics - ExperimentMiniBooNEHigh Energy Physics - Experiment (hep-ex)muon neutrino; antineutrino scattering0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Bubble chamberMuon neutrinoEngineering (miscellaneous); Physics and Astronomy (miscellaneous)Nuclear Experiment010306 general physicsMass parameterEngineering (miscellaneous)Charged currentPhysics010308 nuclear & particles physicsScatteringHigh Energy Physics::PhenomenologyFísicaDeuteriumHigh Energy Physics::ExperimentNeutrinoParticle Physics - Experiment
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