Search results for "multipole"

showing 5 items of 105 documents

Relativistic multipole operators for semileptonic weak and electromagnetic nuclear reactions.

1989

We discuss multipole operators that arise in a relativistic analysis ofsemileptonic weak and electromagnetic interactions with nuclei. Thesesingle-particle operators are evaluated between relativistic nucleon boundstates that are solutions to the Dirac equation with potentials of the formproduced by the sigma-..omega.. model. The reduced matrix elements aregiven in terms of easily programmable radial integrals and can be applied to anumber of reactions such as elastic and inelastic electron scattering, realphoton processes, ..beta.. decay, and charged lepton capture as well as moreexotic interactions such as charged and neutral current neutrino reactions. Asa specific example, we calculate …

Semileptonic decayPhysicsElastic scatteringNuclear and High Energy PhysicsParticle physicsNeutral currentNuclear TheoryInelastic scatteringsymbols.namesakeQuantum electrodynamicsDirac equationsymbolsNeutrinoMultipole expansionLeptonPhysical review. C, Nuclear physics
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Fano-resonances in High Index Dielectric Nanowires for Directional Scattering

2018

High refractive index dielectric nanostructures provide original optical properties thanks to the occurrence of size- and shape-dependent optical resonance modes. These modes commonly present a spectral overlap of broad, low-order modes (\textit{e.g}. dipolar modes) and much narrower, higher-order modes. The latter are usually characterized by a rapidly varying frequency-dependent phase, which - in superposition with the lower order mode of approximately constant phase - leads to typical spectral features known as Fano resonances. Interestingly, such Fano resonances occur in dielectric nanostructures of the simplest shapes. In spheroidal nanoparticles, interference between broad magnetic di…

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics][SPI.OPTI] Engineering Sciences [physics]/Optics / Photonic[SPI.NANO] Engineering Sciences [physics]/Micro and nanotechnologies/MicroelectronicsMie scatteringNanowireFOS: Physical sciencesPhysics::OpticsApplied Physics (physics.app-ph)02 engineering and technologyDielectric01 natural sciences010309 opticsMesoscale and Nanoscale Physics (cond-mat.mes-hall)0103 physical sciences[SPI.NANO]Engineering Sciences [physics]/Micro and nanotechnologies/Microelectronics[PHYS.COND.CM-MSQHE]Physics [physics]/Condensed Matter [cond-mat]/Mesoscopic Systems and Quantum Hall Effect [cond-mat.mes-hall]Physics[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]Condensed Matter - Mesoscale and Nanoscale PhysicsCondensed matter physicsScatteringFano resonancePhysics - Applied PhysicsCondensed Matter::Mesoscopic Systems and Quantum Hall Effect021001 nanoscience & nanotechnology[PHYS.COND.CM-MSQHE] Physics [physics]/Condensed Matter [cond-mat]/Mesoscopic Systems and Quantum Hall Effect [cond-mat.mes-hall]Dipole[SPI.OPTI]Engineering Sciences [physics]/Optics / Photonic0210 nano-technologyMultipole expansionMagnetic dipole
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The non-Gaussian distribution of galaxies gravitational fields

2016

We perform a theoretical analysis of the observational dependence between angular momentum of the galaxy clusters and their mass (richness), based on the method introduced in our previous paper. For that we obtain the distribution function of astronomical objects (like galaxies and/or smooth halos of different kinds) gravitational fields due to their tidal interaction. Within the statistical method of Chandrasekhar we are able to show that the distribution function is determined by the form of interaction between objects and for multipole (tidal) interaction it is never Gaussian. Our calculation permits to demonstrate how the alignment of galaxies angular momenta depend on the cluster richn…

galaxies: general — galaxies: formationAngular momentumCosmology and Nongalactic Astrophysics (astro-ph.CO)GaussianFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencessymbols.namesakeGravitational field0103 physical sciences010303 astronomy & astrophysicsChandrasekhar limitGalaxy clusterAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesGalaxyDistribution functionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)symbolsMultipole expansionAstrophysics - Cosmology and Nongalactic Astrophysics
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Quarkonium suppression in heavy-ion collisions: an open quantum system approach

2016

We address the evolution of heavy-quarkonium states in an expanding quark-gluon plasma by implementing effective field theory techniques in the framework of open quantum systems. In this setting we compute the nuclear modification factors for quarkonia that are $S$-wave Coulombic bound states in a strongly-coupled quark-gluon plasma. The calculation is performed at an accuracy that is leading-order in the heavy-quark density expansion and next-to-leading order in the multipole expansion. The quarkonium density-matrix evolution equations can be written in the Lindblad form, and, hence, they account for both dissociation and recombination. Thermal mass shifts, thermal widths and the Lindblad …

heavy ion: scatteringNuclear TheoryHigh Energy Physics::Latticequarkonium: productionhiukkasfysiikka01 natural sciences7. Clean energyHigh Energy Physics - ExperimentOpen quantum systemHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Bound stateEffective field theory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear Experiment[ PHYS.NUCL ] Physics [physics]/Nuclear Theory [nucl-th]quark gluon: plasmaPhysicsLindblad equationquarkonium: suppressionopen quantum systemsQuarkoniumHigh Energy Physics - PhenomenologyQuantum electrodynamicsquarkoniummomentum: diffusion[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]FOS: Physical sciencesdissociationMomentum diffusionNuclear Theory (nucl-th)[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]Quantum mechanics0103 physical sciencesplasma: expansionparticle physics010306 general physicsheavy quark: momentumta114010308 nuclear & particles physicsHigh Energy Physics::Phenomenologynuclear matter: effectrecombinationUpsilon(10020)evolution equation[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Quark–gluon plasma[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::ExperimentMultipole expansionUpsilon(9460)
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Shape Sensitivity Analysis and Gradient-Based Optimization of Large Structures Using MLFMA

2014

A fast method for computing the action of shape-differentiated electric field integral equation (EFIE) system matrix to a vector is derived exploiting the multilevel fast multipole algorithm (MLFMA). The proposed method is used in conjunction with the adjoint-variable method (AVM) to compute the shape gradient of arbitrary objective functions depending on shape of a metallic scatterer. The method is demonstrated numerically by optimizing the shape of a parabolic reflector illuminated with a half-wave dipole.

ta113DipoleParabolic reflectorGradient based algorithmMathematical analysisShape gradientSensitivity (control systems)Electrical and Electronic EngineeringElectric-field integral equationMultipole expansionAction (physics)MathematicsIEEE Transactions on Antennas and Propagation
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