Search results for " oscillation"

showing 10 items of 845 documents

Magnetic breakdown and charge density wave formation: a quantum oscillation study of the rare-earth tritellurides

2020

The rare-earth tritellurides ($R$Te$_3$, where $R$ = La, Ce, Pr, Nd, Sm, Gd, Tb, Dy, Ho, Er, Tm, Y) form a charge density wave state consisting of a single unidirectional charge density wave for lighter $R$, with a second unidirectional charge density wave, perpendicular and in addition to the first, also present at low temperatures for heavier $R$. We present a quantum oscillation study in magnetic fields up to 65T that compares the single charge density wave state with the double charge density wave state both above and below the magnetic breakdown field of the second charge density wave. In the double charge density wave state it is observed that there remain several small, light pockets…

Quantum phase transitionPhysicsCondensed matter physicsStrongly Correlated Electrons (cond-mat.str-el)Rare earthQuantum oscillationsFOS: Physical sciencesModel systemFermi surface02 engineering and technologyMagnetic breakdown021001 nanoscience & nanotechnology01 natural sciencesCondensed Matter - Strongly Correlated ElectronsEffective mass (solid-state physics)0103 physical sciences010306 general physics0210 nano-technologyCharge density wave
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Constraining nonstandard neutrino-quark interactions with solar, reactor and accelerator data

2009

We present a reanalysis of nonstandard neutrino-down-quark interactions of electron and tau neutrinos using solar, reactor and accelerator data. In addition updating the analysis by including new solar data from SNO phase III and Borexino, as well as new KamLAND data and solar fluxes, a key role is played in our analysis by the combination of these results with the CHARM data. The latter allows us to better constrain the axial and axial-vector electron and tau-neutrino nonstandard interaction parameters characterizing the deviations from the Standard Model predictions.

QuarkHistoryNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsPhase (waves)FOS: Physical sciencesElectronEducationStandard ModelPhysics::GeophysicsHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Charm (quantum number)Nuclear Experiment (nucl-ex)Neutrino oscillationNuclear ExperimentSolar and Stellar Astrophysics (astro-ph.SR)BorexinoSolar dataPhysicsNeutral currentHigh Energy Physics::PhenomenologyFísicaComputer Science ApplicationsHigh Energy Physics - PhenomenologyAstrophysics - Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentNeutrino
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Improved global fit to Non-Standard neutrino Interactions using COHERENT energy and timing data

2020

We perform a global fit to neutrino oscillation and coherent neutrino-nucleus scattering data, using both timing and energy information from the COHERENT experiment. The results are used to set model-independent bounds on four-fermion effective operators inducing non-standard neutral-current neutrino interactions. We quantify the allowed ranges for their Wilson coefficients, as well as the status of the LMA-D solution, for a wide class of new physics models with arbitrary ratios between the strength of the operators involving up and down quarks. Our results are presented for the COHERENT experiment alone, as well as in combination with the global data from oscillation experiments. We also q…

QuarkNuclear and High Energy PhysicsParticle physicsPhysics beyond the Standard ModelFOS: Physical sciences7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityNeutrino Physics010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsScatteringOscillationForm factor (quantum field theory)High Energy Physics - PhenomenologyBeyond Standard Modellcsh:QC770-798Solar and Atmospheric NeutrinosNeutrinoEnergy (signal processing)
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Search for the exotic Θ+ resonance in the NOMAD experiment

2006

12 pages, 16 figures.-- PACS nrs.: 13.15.+g; 13.60.Le; 13.87.Fh; 14.40.Ev.-- ISI Article Identifier: 000243973100007.-- ArXiv pre-print available at: http://arxiv.org/abs/hep-ex/0612063.-- et al.

QuarkParticle physicsPhysics and Astronomy (miscellaneous)Protonneutrino; nutrino oscillations; quarksElectromagnetic Calorimeter7. Clean energy01 natural sciencesParticle identificationHigh Energy Physics - ExperimentNuclear physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Muon neutrino010306 general physicsEngineering (miscellaneous)Charged currentPhysicsNeutral current010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaTransition Radiation DetectorPositive-strangenessBaryonPhotoproductionHigh Energy Physics::ExperimentNeutrinoParticle Physics - ExperimentCharged Current Interactions
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Neutrino Mass Ordering from Oscillations and Beyond: 2018 Status and Future Prospects

2018

The ordering of the neutrino masses is a crucial input for a deep understanding of flavor physics, and its determination may provide the key to establish the relationship among the lepton masses and mixings and their analogous properties in the quark sector. The extraction of the neutrino mass ordering is a data-driven field expected to evolve very rapidly in the next decade. In this review, we both analyze the present status and describe the physics of subsequent prospects. Firstly, the different current available tools to measure the neutrino mass ordering are described. Namely, reactor, long-baseline (accelerator and atmospheric) neutrino beams, laboratory searches for beta and neutrinol…

QuarkParticle physicsneutrino masses and flavor mixingCosmology and Nongalactic Astrophysics (astro-ph.CO)Field (physics)lcsh:AstronomyCosmic background radiationneutrino mass orderingFOS: Physical scienceslarge scale structure formation7. Clean energy01 natural sciencesCosmologyPartícules (Física nuclear)lcsh:QB1-991High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNeutrino oscillation010303 astronomy & astrophysicsPhysicsneutrino oscillations010308 nuclear & particles physicslcsh:QC801-809High Energy Physics::Phenomenologyneutrinoless double beta (0vββ) decayAstronomy and AstrophysicsHigh Energy Physics - PhenomenologySupernovalcsh:Geophysics. Cosmic physicscosmic microwave Background (CMB)High Energy Physics::ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic AstrophysicsLeptonFrontiers in Astronomy and Space Sciences
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Neutrino Oscillations in the Dualized Standard Model

1998

A method developed from the Dualized Standard Model for calculating the quark CKM matrix and masses is applied to the parallel problem in neutrino oscillations. Taking the parameters determined from quarks and the masses of two neutrinos: $m_3^2 \sim 10^{-2} - 10^{-3} eV^2$ suggested by atmospheric neutrino data, and $m_2^2 \sim 10^{-10} eV^2$ suggested by the long wave-length oscillation (LWO) solution of the solar neutrino problem, one obtains from a parameter-free calculation all the mixing angles in reasonable agreement with existing experiment. However, the scheme is found not to accommodate comfortably the mass values $m_2^2 \sim 10^{-5} eV^2$ suggested by the MSW solution for solar n…

QuarkPhysicsNuclear and High Energy PhysicsParticle physicsCabibbo–Kobayashi–Maskawa matrixSolar neutrinoHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaDuality (optimization)Solar neutrino problemStandard ModelHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics::ExperimentNeutrinoNeutrino oscillation
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NO nu A plus T2K: The race for the neutrino mass hierarchy

2006

The determination of the ordering of the neutrino masses (the hierarchy) is probably a crucial prerequisite to understand the origin of lepton masses and mixings and to establish their relationship to the analogous properties in the quark sector. Here, we follow an alternative strategy to the usual neutrino--antineutrino comparison in long baseline neutrino oscillation experiments: we exploit the combination of the neutrino-only data from the NOvA and the T2K experiments by performing these two off-axis experiments at different distances but at the same $/L$, where $$ is the mean neutrino energy and $L$ is the baseline. This would require a minor adjustment to the proposed off-axis angle fo…

QuarkPhysicsNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical sciencesHigh Energy Physics - ExperimentStandard ModelNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino detectorCP violationInvariant massHigh Energy Physics::ExperimentFísica nuclearNeutrinoNeutrino oscillationLepton
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Confusing nonzero theta(13) with nonstandard interactions in the solar neutrino sector

2009

Solar and KamLAND data are in slight tension when interpreted in the standard two-flavor oscillations framework and this may be alleviated allowing for a non-zero value of the mixing angle theta_13. Here we show that, likewise, non-standard flavor-changing interactions (FCI), possibly intervening in the propagation of solar neutrinos, are equally able to alleviate this tension and therefore constitute a potential source of confusion in the determination of theta_13. By performing a full three-flavor analysis of solar and KamLAND data in presence of FCI we provide a quantitative description of the degeneracy existing between theta_13 and the vectorial coupling eps_e\tau^dV characterizing the…

QuarkPhysicsNuclear and High Energy PhysicsParticle physicsScatteringSolar neutrinoFOS: Physical sciencesFísicaWeinberg angleHigh Energy Physics - ExperimentHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Astrophysics - Solar and Stellar AstrophysicsMixing (mathematics)Potential sourceHigh Energy Physics::ExperimentNuclear Experiment (nucl-ex)Neutrino oscillationDegeneracy (mathematics)Nuclear ExperimentSolar and Stellar Astrophysics (astro-ph.SR)
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Relating quarks and leptons with the T7 flavour group

2015

In this letter we present a model for quarks and leptons based on T7 as flavour symmetry, predicting a canonical mass relation between charged leptons and down-type quarks proposed earlier. Neutrino masses are generated through a Type-I seesaw mechanism, with predicted correlations between the atmospheric mixing angle and neutrino masses. Compatibility with oscillation results lead to lower bounds for the lightest neutrino mass as well as for the neutrinoless double beta decay rates, even for normal neutrino mass hierarchy.

QuarkPhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physicsHigh Energy Physics::LatticeFlavourHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicalcsh:QC1-999Nuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw mechanismDouble beta decayddc:530High Energy Physics::ExperimentNeutrinoNeutrino oscillationlcsh:PhysicsLepton
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Predictions from warped flavor dynamics based on the T′ family group

2020

We propose a realistic theory of fermion masses and mixings using a five-dimensional warped scenario where all fermions propagate in the bulk and the Higgs field is localized on the IR brane. The assumed $T'$ flavor symmetry is broken on the branes by flavon fields, providing a consistent scenario where fermion mass hierarchies arise from adequate choices of the bulk mass parameters, while quark and lepton mixing angles are restricted by the family symmetry. Neutrino mass splittings, mixing parameters and the Dirac CP phase all arise from the type-I seesaw mechanism and are tightly correlated, leading to predictions for the neutrino oscillation parameters, as well as expected \znbb decay ra…

QuarkPhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyFOS: Physical sciencesFermionType (model theory)01 natural sciencesHigh Energy Physics - PhenomenologyHiggs fieldHigh Energy Physics - Phenomenology (hep-ph)Seesaw mechanism0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationLepton
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