Search results for "Mixing"

showing 10 items of 795 documents

Search for heavy neutrinos in \(\pi ^{ + } \to \mu ^{ + }\nu \) decay and status of lepton universality test in the PIENU experiment

2019

International audience; In the present work of the PIENU experiment, heavy neutrinos were sought in pion decays \(\pi ^{ + } \to \mu ^{ + }\nu \). No evidence for extra peak was found in the muon kinetic energy spectrum and 90% confidence level upper limits were set on the neutrino mixing matrix \(|U_{\mu i}|^{2}\) in the mass range of 15.7 to 33.8 MeV/c^2, improving an order of magnitude over previous experiments. Current status of lepton universality test is also reported.

PhysicsParticle physicsMuonpi+ --> muon+ neutrinopi: decayneutrino: heavy: search forUniversality (philosophy)Pontecorvo–Maki–Nakagawa–Sakata matrixkineticenergy spectrumKinetic energyPion[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]High Energy Physics::ExperimentNeutrinoneutrino: mixingOrder of magnitudeParticle Physics - ExperimentLeptonexperimental resultslepton: universality
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Determination of the $\theta_{23}$ octant in LBNO

2014

According to the recent results of the neutrino oscillation experiment MINOS, the neutrino mixing angle $\theta_{23}$ may not be maximal ($45^{\circ}$). Two nearly degenerate solutions are possible, one in the lower octant (LO) where $\theta_{23}45^{\circ}$. Long baseline experiments measuring the $\nu_{\mu}\rightarrow\nu_{e}$ are capable of resolving this degeneracy. In this work we study the potential of the planned European LBNO experiment to distinguish between the LO and HO solutions.

PhysicsParticle physicsNeutrino Detectors and TelescopesNuclear and High Energy Physicsta114010308 nuclear & particles physicsOscillationDegenerate energy levelsHigh Energy Physics::PhenomenologyOctant (solid geometry)01 natural sciencesHigh Energy Physics - ExperimentOscillationHigh Energy Physics - PhenomenologyMINOS0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationDegeneracy (mathematics)Mixing (physics)
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The Zee–Babu model revisited in the light of new data

2014

We update previous analyses of the Zee-Babu model in the light of new data, e.g., the mixing angle $\theta_{13}$, the rare decay $\mu\to e \gamma$ and the LHC results. We also analyse the possibility of accommodating the deviations in $\Gamma(H\to \gamma\gamma)$ hinted by the LHC experiments, and the stability of the scalar potential. We find that neutrino oscillation data and low energy constraints are still compatible with masses of the extra charged scalars accessible to LHC. Moreover, if any of them is discovered, the model can be falsified by combining the information on the singly and doubly charged scalar decay modes with neutrino data. Conversely, if the neutrino spectrum is found t…

PhysicsParticle physicsNuclear and High Energy PhysicsLarge Hadron Collider010308 nuclear & particles physicsPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaScalar (mathematics)High Energy Physics::PhenomenologyFOS: Physical sciencesFísicaScalar potential01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesCP violationNeutrino010306 general physicsNeutrino oscillationMixing (physics)Nuclear Physics B
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The earth Mantle-Core effect in charge-asymmetries for atmospheric neutrino oscillations

2002

Earth medium effects in the three-neutrino oscillations of atmospheric neutrinos are observable under appropriate conditions. This paper generalizes the study of the medium effects and the possibility of their observation in the atmospheric neutrino oscillations from the case of neutrinos traversing only the Earth mantle, where the density is essentially constant, to the case of atmospheric neutrinos crossing also the Earth core. In the latter case new resonance-like effects become apparent. We calculate the CPT-odd asymmetry for the survival probability of muon neutrinos and the observable muon-charge asymmetry, taking into account the different atmospheric neutrino fluxes, and show the de…

PhysicsParticle physicsNuclear and High Energy PhysicsMuonPhysics::Instrumentation and Detectorsmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFísicaObservableAsymmetryCore (optical fiber)MomentumMagnitude (astronomy)High Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsNeutrinoMixing (physics)media_commonPhysics Letters B
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A non-resonant dark-side solution to the solar neutrino problem

2001

We re-analyse spin-flavour precession solutions to the solar neutrino problem in the light of the recent SNO CC result as well as the 1258--day Super-Kamiokande data and the upper limit on solar anti-neutrinos. In a self-consistent magneto-hydrodynamics approach the resulting scheme has only 3 effective parameters: $\Delta m^2$, $\mu B_\perp$ and the neutrino mixing angle $\theta$. We show how a rates-only analysis for fixed $\mu B_\perp$ slightly favours spin-flavour precession (SFP) solutions over oscillations (OSC). In addition to the resonant solution (RSFP for short), there is a new non-resonant solution (NRSFP) in the ``dark-side''. Both RSFP and NRSFP lead to flat recoil energy spect…

PhysicsParticle physicsNuclear and High Energy PhysicsNeutrino mass and mixingCosmologiaMagnetic momentNeutrino oscillationsSolar neutrinosHigh Energy Physics::PhenomenologyFOS: Physical sciencesSolar neutrino problemSpectral linePartícules (Física nuclear)Magnetic fieldBohr magnetonNeutrino magnetic momentsymbols.namesakeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)symbolsPrecessionHigh Energy Physics::ExperimentNeutrinoMixing (physics)
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An invisible axion model with controlled FCNCs at tree level

2015

We derive the necessary conditions to build a class of invisible axion models with Flavor Changing Neutral Currents at tree-level controlled by the fermion mixing matrices and present an explicit model implementation. A horizontal Peccei-Quinn symmetry provides a solution to the strong CP problem via the Peccei-Quinn mechanism and predicts a cold dark mater candidate, the invisible axion or familon. The smallness of active neutrino masses can be explained via a type I seesaw mechanism, providing a dynamical origin for the heavy seesaw scale. The possibility to avoid the domain wall problem stands as one of the most interesting features of the type of models considered. Experimental limits r…

PhysicsParticle physicsNuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsDark matterHigh Energy Physics::PhenomenologyFOS: Physical scienceslcsh:QC1-999Domain wall (string theory)High Energy Physics - PhenomenologySeesaw mechanismHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryStrong CP problemNeutrinoAxionMixing (physics)lcsh:PhysicsPhysics Letters B
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Quantum electrodynamics for vector mesons

2005

Quantum electrodynamics for $\rho$ mesons is considered. It is shown that, at tree level, the value of the gyromagnetic ratio of the $\rho^+$ is fixed to 2 in a self-consistent effective quantum field theory. Further, the mixing parameter of the photon and the neutral vector meson is equal to the ratio of electromagnetic and strong couplings, leading to the mass difference $M_{\rho^0}-M_{\rho^\pm}\sim 1 {\rm MeV}$ at tree order.

PhysicsParticle physicsPhotonMesonGyromagnetic ratioGeneral Physics and AstronomyFOS: Physical sciencesRenormalizationHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Quantum electrodynamicsHigh Energy Physics::ExperimentTree (set theory)Neutral vectorQuantum field theoryMixing (physics)
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Circumstantial Evidence for Rotating Mass Matrix from Fermion Mass and Mixing Data

2002

It is shown that existing data on the mixing between up and down fermion states and on the hierarchical mass ratios between fermion generations, as far as can be so analysed at present, are all consistent with the two phenomena being both consequences of a mass matrix rotating in generation space with changing energy scale. As a result, the rotating mass matrix can be traced over some 14 orders of magnitude in energy from the mass scale of the $t$-quark at 175 GeV to below that of the atmospheric neutrino at 0.05 eV.

PhysicsParticle physicsPhysics and Astronomy (miscellaneous)Scale (ratio)FísicaFOS: Physical sciencesFermionSpace (mathematics)Mass matrixHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Orders of magnitude (time)Mass scaleAtmospheric neutrinoEngineering (miscellaneous)Mixing (physics)Computer Science::Databases
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Updates to the Dualized Standard Model on Fermion Masses and Mixings

2003

The Dualized Standard Model has scored a number of successes in explaining the fermion mass hierarchy and mixing pattern. This note contains updates to those results including (a) an improved treatment of neutrino oscillation free from previous assumptions on neutrino masses, and hence admitting now the preferred LMA solution to solar neutrinos, (b) an understanding of the limitation of the 1-loop calculation so far performed, thus explaining the two previous discrepancies with data, and (c) an analytic derivation and confirmation of the numerical results previously obtained.

PhysicsParticle physicsPhysics and Astronomy (miscellaneous)Solar neutrinoFísicaFOS: Physical sciencesFermionStandard ModelHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)NeutrinoNeutrino oscillationMass hierarchyEngineering (miscellaneous)Mixing (physics)
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Where we are onθ13: addendum to ‘Global neutrino data and recent reactor fluxes: status of three-flavor oscillation parameters’

2011

In this addendum to arXiv:1103.0734 we consider the recent results from long-baseline $\nu_\mu\to\nu_e$ searches at the T2K and MINOS experiments and investigate their implications for the mixing angle $\theta_{13}$ and the leptonic Dirac CP phase $\delta$. By combining the $2.5\sigma$ indication for a non-zero value of $\theta_{13}$ coming from T2K data with global neutrino oscillation data we obtain a significance for $\theta_{13} > 0$ of about $3\sigma$ with best fit points $\sin^2\theta_{13} = 0.013(0.016)$ for normal (inverted) neutrino mass ordering. These results depend somewhat on assumptions concerning the analysis of reactor neutrino data.

PhysicsParticle physicsPhysics::Instrumentation and Detectors010308 nuclear & particles physicsOscillationDirac (video compression format)High Energy Physics::PhenomenologyFlavourFísicaGeneral Physics and AstronomyAddendum01 natural sciences7. Clean energyNuclear physicsHigh Energy Physics - PhenomenologyMINOS0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationMixing (physics)New Journal of Physics
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