Search results for " mixing"

showing 10 items of 270 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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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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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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Exact relativistic beta decay endpoint spectrum

2007

5 pages, 3 figures.-- PACS nrs.: 14.60.Pq; 13.30.-a; 23.40.-s; 23.40.Bw.-- ISI Article Identifier: 000250620900070.-- ArXiv pre-print available at: http://arxiv.org/abs/0706.0897

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsFOS: Physical sciences[PACS] Neutrino mass and mixingelectron and muon captureHigh Energy Physics - Phenomenology (hep-ph)FactorizationDouble beta decayNuclear Experiment (nucl-ex)Neutrino oscillationNuclear ExperimentPhysics[PACS] β decay[PACS] Decays of baryonsSpectrum (functional analysis)[PACS] β decay; double β decay; electron and muon captureFísicaBeta decay[PACS] Weak-interaction and lepton (including neutrino) aspects of β decayHigh Energy Physics - Phenomenologydouble β decayYield (chemistry)High Energy Physics::ExperimentNeutrinoKATRIN
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Constraining the invisible neutrino decay with KM3NeT-ORCA

2019

Several theories of particle physics beyond the Standard Model consider that neutrinos can decay. In this work we assume that the standard mechanism of neutrino oscillations is altered by the decay of the heaviest neutrino mass state into a sterile neutrino and, depending on the model, a scalar or a Majoron. We study the sensitivity of the forthcoming KM3NeT-ORCA experiment to this scenario and find that it could improve the current bounds coming from oscillation experiments, where three-neutrino oscillations have been considered, by roughly two orders of magnitude. We also study how the presence of this neutrino decay can affect the determination of the atmospheric oscillation parameters $…

Nuclear and High Energy PhysicsParticle physicsSterile neutrinoPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaNeutrino masses and mixingScalar (mathematics)FOS: Physical sciences01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationNeutrino decayMajoronPhysics010308 nuclear & particles physicsOscillationNeutrino oscillationsHigh Energy Physics::Phenomenologylcsh:QC1-999High Energy Physics - PhenomenologyKM3NeTHigh Energy Physics::ExperimentNeutrinoNeutrino telescopeslcsh:PhysicsPhysics Letters
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Search for heavy neutrinos mixing with tau neutrinos

2001

We report on a search for heavy neutrinos ($\nus$) produced in the decay $D_s\to \tau \nus$ at the SPS proton target followed by the decay $\nudecay$ in the NOMAD detector. Both decays are expected to occur if $\nus$ is a component of $\nu_{\tau}$.\ From the analysis of the data collected during the 1996-1998 runs with $4.1\times10^{19}$ protons on target, a single candidate event consistent with background expectations was found. This allows to derive an upper limit on the mixing strength between the heavy neutrino and the tau neutrino in the $\nus$ mass range from 10 to 190 $\rm MeV$. Windows between the SN1987a and Big Bang Nucleosynthesis lower limits and our result are still open for f…

Nuclear and High Energy PhysicsParticle physics[PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex]ProtonFOS: Physical sciences01 natural sciences7. Clean energyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Big Bang nucleosynthesisTau neutrino0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsMixing (physics)PhysicsRange (particle radiation)010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísica3. Good healthneutrino mixing; neutrino decayHigh Energy Physics::ExperimentNeutrinoAnomaly (physics)Event (particle physics)Particle Physics - Experiment
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