Search results for "Oscillations"

showing 10 items of 238 documents

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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Precise measurement of the neutrino mixing parameter θ23 from muon neutrino disappearance in an off-axis beam

2014

New data from the T2K neutrino oscillation experiment produce the most precise measurement of the neutrino mixing parameter theta_{23}. Using an off-axis neutrino beam with a peak energy of 0.6 GeV and a data set corresponding to 6.57 x 10^{20} protons on target, T2K has fit the energy-dependent nu_mu oscillation probability to determine oscillation parameters. Marginalizing over the values of other oscillation parameters yields sin^2 (theta_{23}) = 0.514 +0.055/-0.056 (0.511 +- 0.055), assuming normal (inverted) mass hierarchy. The best-fit mass-squared splitting for normal hierarchy is Delta m^2_{32} = (2.51 +- 0.10) x 10^{-3} eV^2/c^4 (inverted hierarchy: Delta m^2_{13} = (2.48 +- 0.10) …

Particle physicsGeneral PhysicsPhysics MultidisciplinaryMODELSGeneral Physics and AstronomyFOS: Physical sciencesMASS01 natural sciences09 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]SCATTERINGMuon neutrino010306 general physicsNeutrino oscillationDETECTORMixing (physics)01 Mathematical SciencesPhysicsNeutronsScience & Technology02 Physical Sciences010308 nuclear & particles physicsScatteringOscillationhep-exPhysicsFísicaT2K CollaborationPhysical SciencesSYMMETRIESHigh Energy Physics::ExperimentNeutrinoHigh energy physics Mixing Parameter estimation Parameter extractionConfidence limit Energy dependent Neutrino oscillations Off-axis neutrino beam Oscillation parameters Oscillation probabilities Precise measurements Statistical uncertaintyBeam (structure)Energy (signal processing)
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Search for coherent charged pion production in neutrino-carbon interactions

2005

We report the result from a search for charged-current coherent pion production induced by muon neutrinos with a mean energy of 1.3 GeV. The data are collected with a fully active scintillator detector in the K2K long-baseline neutrino oscillation experiment. No evidence for coherent pion production is observed and an upper limit of $0.60 \times 10^{-2}$ is set on the cross section ratio of coherent pion production to the total charged-current interaction at 90% confidence level. This is the first experimental limit for coherent charged pion production in the energy region of a few GeV.

Particle physicsMesonPhysics::Instrumentation and DetectorsNeutrino-nucleus reactionsFOS: Physical sciencesGeneral Physics and Astronomyddc:500.201 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)PionExperiment-HEP0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationNuclear ExperimentNuclear ExperimentCharged currentPhysicsMuonTamura Norio010308 nuclear & particles physicsNeutrino oscillationsFísica田村 詔生Production (computer science)High Energy Physics::ExperimentNeutrinoLepton
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Axion cold dark matter: Status after Planck and BICEP2

2014

We investigate the axion dark matter scenario (ADM), in which axions account for all of the dark matter in the Universe, in light of the most recent cosmological data. In particular, we use the Planck temperature data, complemented by WMAP E-polarization measurements, as well as the recent BICEP2 observations of B-modes. Baryon Acoustic Oscillation data, including those from the Baryon Oscillation Spectroscopic Survey, are also considered in the numerical analyses. We find that, in the minimal ADM scenario, the full dataset implies that the axion mass m_a = 82.2 pm 1.1 {\mu}eV (corresponding to the Peccei-Quinn symmetry being broken at a scale f_a = (7.54 pm 0.10)*10^10 GeV), or m_a = 76.6 …

Particle physicsNuclear and High Energy PhysicsCold dark matterCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)INFLATIONPlanckAxionPhysicsSpectral indexHigh Energy Physics::PhenomenologyFísicaPlanck temperatureINVISIBLE AXIONBARYON ACOUSTIC-OSCILLATIONS; DIGITAL SKY SURVEY; INVISIBLE AXION; COSMOLOGY; INFLATION; DISTANCEBaryonHigh Energy Physics - PhenomenologyCOSMOLOGYDISTANCEsymbolsDark energyAstronomiaDIGITAL SKY SURVEYBARYON ACOUSTIC-OSCILLATIONSAstrophysics - Cosmology and Nongalactic Astrophysics
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Absence of a day-night asymmetry in the7Be solar neutrino rate in Borexino

2012

We report on a search for the day-night asymmetry of the Be-7 solar neutrino rate measured by Borexino at the Laboratori Nazionali del Gran Sasso (LNGS), Italy. The measured value, Adn=0.001 +- 0.012 (stat) +- 0.007 (syst), shows the absence of a significant asymmetry. This result alone rejects the so-called LOW solution at more than 8.5 sigma. Combined with the other solar neutrino data, it isolates the Large Mixing Angle (LMA) -- MSW solution at DeltaChi2 > 190 without relying on the assumption of CPT symmetry in the neutrino sector. We also show that including the day-night asymmetry, data from Borexino alone restricts the MSW neutrino oscillations to the LMA solution at 90% confidence l…

Particle physicsNuclear and High Energy PhysicsNeutrino oscillationPhysics::Instrumentation and Detectorsmedia_common.quotation_subjectSolar neutrino01 natural sciencesAsymmetrySolar neutrinoNuclear physicsDay-night effect0103 physical sciences010306 general physicsNeutrino oscillationNuclear Experimentday–night effectBorexinomedia_commonPhysicsneutrino oscillations010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaSolar neutrino problemNeutrino detectorsolar neutrinosMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoCPT violation
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Neutrino oscillations and Non-Standard Interactions

2017

Current neutrino experiments measure the neutrino mixing parameters with an unprecedented accuracy. The upcoming generation of experiments will be sensitive to subdominant effects that can give information on the unknown neutrino parameters: the Dirac CP-violating phase, the mass ordering and the $\theta_{23}$ octant. Determining the exact values of neutrino mass and mixing parameters is crucial to test neutrino models and flavor symmetries. In the first part of this review, we summarize the current status of neutrino oscillation parameters. We consider the most recent data from solar experiments and the atmospheric data from Super-Kamiokande, IceCube and ANTARES. We implement the data from…

Particle physicsPhysics::Instrumentation and DetectorsMaterials Science (miscellaneous)Physics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaBiophysicsGeneral Physics and AstronomyFOS: Physical sciencesCHOOZ7. Clean energy01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Violació CP (Física nuclear)neutrino physics0103 physical sciencesPhysical and Theoretical Chemistry010306 general physicsNeutrino oscillationMathematical PhysicsPhysicsGauge bosonneutrino oscillationsnon-standard neutrino interactions010308 nuclear & particles physicsneutrino massesElectroweak interactionHigh Energy Physics::Phenomenologylcsh:QC1-999leptonic CP violationHigh Energy Physics - PhenomenologyNeutrino detector13. Climate actionMINOSHigh Energy Physics::ExperimentNeutrinolcsh:Physics
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Searches for Sterile Neutrinos with the IceCube Detector

2016

The IceCube neutrino telescope at the South Pole has measured the atmospheric muon neutrino spectrum as a function of zenith angle and energy in the approximate 320 GeV to 20 TeV range, to search for the oscillation signatures of light sterile neutrinos. No evidence for anomalous $\nu_\mu$ or $\bar{\nu}_\mu$ disappearance is observed in either of two independently developed analyses, each using one year of atmospheric neutrino data. New exclusion limits are placed on the parameter space of the 3+1 model, in which muon antineutrinos would experience a strong MSW-resonant oscillation. The exclusion limits extend to $\mathrm{sin}^2 2\theta_{24} \leq$ 0.02 at $\Delta m^2 \sim$ 0.3 $\mathrm{eV}^…

Particle physicsSterile neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciencesHigh Energy Physics - ExperimentMiniBooNENuclear physicsHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all)0103 physical sciencesOSCILLATIONSddc:550Muon neutrino010306 general physicsNeutrino oscillationZenithHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMuon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyMODELNeutrino detectorPhysics and Astronomy13. Climate actionHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaEnergy (signal processing)SYSTEM
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Effects of triplet Higgs bosons in long baseline neutrino experiments

2018

The triplet scalars $(\Delta=\Delta^{++},\Delta^{+},\Delta^{0})$, utilized in the so-called Type-II seesaw model to explain the lightness of neutrinos, would generate nonstandard interactions (NSI) for neutrino propagating in matter. We investigate the prospects to probe these interactions in long baseline neutrino oscillation experiments. We analyze the upper bounds that the proposed DUNE experiment might set on the nonstandard parameters and numerically derive upper bounds, as function of the lightest neutrino mass, on the ratio the mass $M_\Delta$ of the triplet scalars and strength $|\lambda_\phi|$ of the coupling $\phi\phi\Delta$ of the triplet $\Delta$ and conventional Higgs doublet $…

Particle physicsVIOLATIONPontecorvo–Maki–Nakagawa–Sakata matrixFOS: Physical scienceshiukkasfysiikkaComputer Science::Digital Libraries114 Physical sciences7. Clean energy01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)effective field theory0103 physical sciences010306 general physicsNeutrino oscillationBosonPhysicsLEFT-RIGHT SYMMETRYneutrino oscillationsPARITYta114010308 nuclear & particles physicsHiggsin bosoniHigh Energy Physics::PhenomenologyneutriinotParity (physics)Coupling (probability)extensions of Higgs sectorHigh Energy Physics - PhenomenologyHiggsin bosonitHiggs bosonDOUBLY-CHARGED HIGGSHigh Energy Physics::ExperimentNeutrinoLepton
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Novel modes of rhythmic burst firing at cognitively-relevant frequencies in thalamocortical neurons.

2008

It is now widely accepted that certain types of cognitive functions are intimately related to synchronized neuronal oscillations at both low (alpha/theta) (4-7/8-13 Hz) and high (beta/gamma) (18-35/30-70 Hz) frequencies. The thalamus is a key participant in many of these oscillations, yet the cellular mechanisms by which this participation occurs are poorly understood. Here we describe how, under appropriate conditions, thalamocortical (TC) neurons from different nuclei can exhibit a wide array of largely unrecognised intrinsic oscillatory activities at a range of cognitively-relevant frequencies. For example, both metabotropic glutamate receptor (mGluR) and muscarinic Ach receptor (mAchR) …

Periodicity* Cognition* Acetylcholine; * Metabotropic glutamate receptor; * Lateral geniculate nucleus; * Intralaminar nucleus; * Oscillations; * EEG; * Cognition; * Perception; * Memory* EEGAction PotentialsSettore BIO/09 - FisiologiaIon ChannelsArticle* PerceptionBurstingThalamusBiological Clocks* Lateral geniculate nucleuMuscarinic acetylcholine receptorNeural PathwaysmedicineAnimalsHumans* Metabotropic glutamate receptorMolecular BiologyCerebral CortexNeurons* OscillationChemistryGeneral Neuroscience* Intralaminar nucleuGlutamate receptorReceptors NeurotransmitterElectrophysiology* MemoryMetabotropic receptormedicine.anatomical_structure* AcetylcholineMetabotropic glutamate receptorWakefulnessNeurology (clinical)NeuronNeuroscienceDevelopmental Biology
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Steady states and nonlinear buckling of cable-suspended beam systems

2018

This paper deals with the equilibria of an elastically-coupled cable-suspended beam system, where the beam is assumed to be extensible and subject to a compressive axial load. When no vertical load is applied, necessary and sufficient conditions in order to have nontrivial solutions are established, and their explicit closed-form expressions are found. In particular, the stationary solutions are shown to exhibit at most two non-vanishing Fourier modes and the critical values of the axial-load parameter which produce their pitchfork bifurcation (buckling) are established. Depending on two dimensionless parameters, the complete set of resonant modes is devised. As expected, breakdown of the p…

Perturbation (astronomy)010103 numerical & computational mathematicsBiparametric resonance; Cable-suspended beam; Nonlinear oscillations; Pitchfork bifurcation; Stationary solutions; Suspension bridgeCable-suspended beam01 natural sciencesBiparametric resonanceNonlinear oscillationssymbols.namesakeStationary solutions0101 mathematicsNonlinear bucklingNonlinear OscillationsPhysicsMechanical EngineeringPitchfork bifurcationMechanicsCondensed Matter PhysicsSuspension bridge010101 applied mathematicsPitchfork bifurcationFourier transformBucklingMechanics of MaterialssymbolsAxial loadDimensionless quantity
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