Search results for "Mixing"

showing 10 items of 795 documents

Nonlinear Disorder Mapping Via Three-Wave Mixing in Quadratic Crystals

2010

Nonlinear optics Three-wave mixing Image analysis
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Guided-wave frequency doubling in surface periodically poled lithium niobate: competing effects

2007

We carried out second-harmonic generation in quasi-phase-matched ? -phase lithium niobate channel waveguides realized by proton exchange and surface periodic poling. Owing to a limited ferroelectric domain depth, we could observe the interplay between second-harmonic generation and self-phase modulation due to cascading and cubic effects, resulting in a nonlinear resonance shift. Data reduction allowed us to evaluate both the quadratic nonlinearity in the near infrared as well as the depth of the uninverted domains. © 2007 Optical

Nonlinear optics integrated opticsMaterials scienceGuided wave testingbusiness.industryLithium niobateNonlinear opticsSecond-harmonic generationPhysics::OpticsFOS: Physical sciencesStatistical and Nonlinear PhysicsHarmonic generation and mixingSettore ING-INF/01 - ElettronicaFerroelectricityAtomic and Molecular Physics and Opticschemistry.chemical_compoundOpticschemistryPeriodic polingNonlinear resonanceHigh harmonic generationbusinessPhysics - OpticsOptics (physics.optics)
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Mean-Field Calculation Based on Proton-Neutron Mixed Energy Density Functionals

2014

We have performed calculations based on the Skyrme energy density functional (EDF) that includes arbitrary mixing between protons and neutrons. In this framework, single-particle states are generalized as mixtures of proton and neutron components. The model assumes that the Skyrme EDF is invariant under the rotation in isospin space and the Coulomb force is the only source of the isospin symmetry breaking. To control the isospin of the system, we employ the isocranking method, which is analogous to the standard cranking approach used for describing high-spin states. Here, we present results of the isocranking calculations performed for the isobaric analog states in $A = 40$ and $A = 54$ nuc…

Nuclear Theory (nucl-th)Nuclear Theoryproton-neutron mixingisobaric analog statesNuclear TheoryFOS: Physical sciencesNuclear Experimentenergy density functionals
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Population of a low-spin positive-parity band from high-spin intruder states in 177Au: The two-state mixing effect

2020

The extremely neutron-deficient isotopes 177,179Au were studied by means of in-beam ?-ray spectroscopy. Specific tagging techniques, ?-decay tagging in 177Au and isomer tagging in 179Au, were used for these studies. Feeding of positive-parity, nearly spherical states, which are associated with 2d3/2 and 3s1/2 proton-hole configurations, from the 1i13/2 proton-intruder configuration was observed in 177Au. Such a decay path has no precedent in odd-Au isotopes and it is explained by the effect of mixing of wave functions of the initial state. © 2020

Nuclear and High Energy Physics? rays179AuPopulation177Au7. Clean energy01 natural scienceskultaIn-beam spectroscopyγ rays0103 physical sciencesMixing effect010306 general physicsWave functioneducationSpectroscopyNuclear Experimenttwo-state mixingPhysicsisotoopiteducation.field_of_studyin-beam spectroscopyIsotope010308 nuclear & particles physicsAu-177Parity (physics)Au-179lcsh:QC1-999gamma raysTwo-state mixingAtomic physicsydinfysiikkalcsh:Physics
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Seasonal dependence in the solar neutrino flux

1999

MSW solutions of the solar neutrino problem predict a seasonal dependence of the zenith angle distribution of the event rates, due to the non-zero latitude at the Super-Kamiokande site. We calculate this seasonal dependence and compare it with the expectations in the no-oscillation case as well as just-so scenario, in the light of the latest Super-Kamiokande 708-day data. The seasonal dependence can be sizeable in the large mixing angle MSW solution and would be correlated with the day-night effect. This may be used to discriminate between MSW and just-so scenarios and should be taken into account in refined fits of the data.

Nuclear and High Energy PhysicsAstrofísica nuclearSolar neutrinoFluxFOS: Physical sciencesContext (language use)AstrophysicsAtmospheric sciencesAstrophysicsPartícules (Física nuclear)LatitudeHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)medicineNeutrinsNeutrinosNeutrino oscillationPhysics::Atmospheric and Oceanic PhysicsMixing (physics)ZenithParticles (Nuclear physics)PhysicsAstrophysics (astro-ph)High Energy Physics::PhenomenologyFísicaSeasonalitySolar neutrino problemmedicine.diseaseAtomic and Molecular Physics and OpticsHigh Energy Physics - PhenomenologyEnvironmental scienceNuclear astrophysicsHigh Energy Physics::ExperimentEvent (particle physics)
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Role of dense matter in collective supernova neutrino transformations

2008

6 pages, 2 figures.-- PACS nrs.: 14.60.Pq; 97.60.Bw.-- ArXiv pre-print available at: http://arxiv.org/abs/0807.0659

Nuclear and High Energy PhysicsElectron densityParticle physicsQuantum decoherenceNeutrino mass and mixing[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Critical phenomenaAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences[PACS] SupernovaeAstrophysics[PACS] Neutrino mass and mixingAstrophysics01 natural sciences7. Clean energy[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesddc:530010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsAstrophysics (astro-ph)High Energy Physics::PhenomenologyFísica3. Good healthSupernovaHigh Energy Physics - PhenomenologySupernovae14.60.Pq 97.60.Bw[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::ExperimentNeutrinoEarly phaseDense matter
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Scalar mesons moving in a finite volume and the role of partial wave mixing

2012

Phase shifts and resonance parameters can be obtained from finite-volume lattice spectra for interacting pairs of particles, moving with nonzero total momentum. We present a simple derivation of the method that is subsequently applied to obtain the pi pi and pi K phase shifts in the sectors with total isospin I=0 and I=1/2, respectively. Considering different total momenta, one obtains extra data points for a given volume that allow for a very efficient extraction of the resonance parameters in the infinite-volume limit. Corrections due to the mixing of partial waves are provided. We expect that our results will help to optimize the strategies in lattice simulations, which aim at an accurat…

Nuclear and High Energy PhysicsNuclear TheoryMesonpartial waveFOS: Physical sciencesSpectral lineNuclear Theory (nucl-th)phase shiftisospinHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)Lattice (order)mixingddc:530latticepi piPhysicsFinite volume methodScatteringscatteringHigh Energy Physics - Lattice (hep-lat)Físicascalar mesonpi KHigh Energy Physics - Phenomenology* Automatic Keywords *Data pointfinite sizeIsospinQuantum electrodynamics
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Flavour in heavy neutrino searches at the LHC

2012

Heavy neutrinos at the TeV scale have been searched for at the LHC in the context of left-right models, under the assumption that they couple to the electron, the muon, or both. We show that current searches are also sensitive to heavy neutrinos coupling predominantly to the tau lepton, and present limits can significantly constrain the parameter space of general flavour mixing.

Nuclear and High Energy PhysicsParticle physicsLHC (Large Hadron Collider)Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHeavy neutrinoFOS: Physical sciencesContext (language use)ElectronParameter space01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsMixing (physics)PhysicsMuonLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinoLepton
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Neutrino phenomenology and stable dark matter with A4

2011

We present a model based on the A4 non-abelian discrete symmetry leading to a predictive five-parameter neutrino mass matrix and providing a stable dark matter candidate. We found an interesting correlation among the atmospheric and the reactor angles which predicts theta_23 ~ pi/4 for very small reactor angle and deviation from maximal atmospheric mixing for large theta_13. Only normal neutrino mass spectrum is possible and the effective mass entering the neutrinoless double beta decay rate is constrained to be |m_ee| > 4 10^{-4} eV.

Nuclear and High Energy PhysicsParticle physicsLepton mixingDark matterDiscrete symmetriesFOS: Physical sciencesElementary particle01 natural sciences7. Clean energyNuclear physicsEffective mass (solid-state physics)High Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciencesDark matterNeutrinoless double beta decay010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsFlavor symmetriesNeutrino massesMassless particleHigh Energy Physics - PhenomenologyMass spectrumNeutrinoPhysics Letters B
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Admixture of quasi-Dirac and Majorana neutrinos with tri-bimaximal mixing

2011

7 páginas, 1 tabla.-- El Pdf es la versión pre-print: arXiv:1104.4961v2

Nuclear and High Energy PhysicsParticle physicsNeutrino hierarchyDiscrete symmetriesFOS: Physical sciences01 natural sciencesUpper and lower boundsHigh Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciencesTri-bimaximal mixingNeutrino masses and mixingsNeutrinoless double beta decay010306 general physicsMixing (physics)Majorana equationPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFlavor symmetries3. Good healthMassless particleMAJORANAHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinoLepton
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