Search results for "LOCI"

showing 10 items of 1277 documents

Superluminal two-color light in multiple Raman gain medium

2014

We investigate theoretically the formation of two-component light with superluminal group velocity in a medium controlled by four Raman pump fields. In such an optical scheme only a particular combination of the probe fields is coupled to the matter and exhibits superluminal propagation, the orthogonal combination is uncoupled. The individual probe fields do not have a definite group velocity in the medium. Calculations demonstrate that this superluminal component experiences an envelope advancement in the medium with respect to the propagation in vacuum.

PhysicsQuantum PhysicsSuperluminal motionbusiness.industryFOS: Physical sciencesInterference (wave propagation)Raman gainAtomic and Molecular Physics and OpticsOpticsQuantum Gases (cond-mat.quant-gas)Group velocityQuantum Physics (quant-ph)businessPhase conjugationCondensed Matter - Quantum GasesOptics (physics.optics)Raman pumpEnvelope (waves)Physics - Optics
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Rising time of entanglement between scattering spins,

2009

We investigate the time evolution of entanglement in a process where a mobile particle is scattered by static spins. We show that entanglement increases monotonically during a transient and then saturates to a steady-state value. For a quasi-monochromatic mobile particle, the transient time depends only on the group-velocity and width of the incoming wavepacket and is insensitive to the interaction strength and spin-number of the scattering particles. These features do not depend on the interaction model and can be seen in various physical settings.

PhysicsQuantum Physicsquantum information theory transport in mesoscopic structuresSpinsCondensed matter physicsCondensed Matter - Mesoscale and Nanoscale PhysicsScatteringWave packetTime evolutionFOS: Physical sciencesQuantum entanglementCondensed Matter PhysicsSpin quantum numberElectronic Optical and Magnetic MaterialsQuantum mechanicsMesoscale and Nanoscale Physics (cond-mat.mes-hall)ParticleGroup velocityQuantum Physics (quant-ph)
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Description and evolution of anisotropy in superfluid vortex tangles with counterflow and rotation

2006

We examine several vectorial and tensorial descriptions of the geometry of turbulent vortex tangles. We study the anisotropy in rotating counterflow experiments, in which the geometry of the tangle is especially interesting because of the opposite effects of rotation, which orients the vortices, and counterflow, which randomizes them. We propose to describe the anisotropy and the polarization of the vortex tangle through a tensor, which contains the first and second moments of the distribution of the unit vector ${\mathbf{s}}^{\ensuremath{'}}$ locally tangent to the vortex lines. We use an analogy with paramagnetism to estimate the anisotropy, the average polarization, the polarization fluc…

PhysicsQuantum fluidTangentAngular velocityCondensed Matter PhysicsMathematics::Geometric TopologyElectronic Optical and Magnetic MaterialsTangleVortexSuperfluidityexamine several vectorial and tensorialClassical mechanicsUnit vectorQuantum mechanicsAnisotropySettore MAT/07 - Fisica Matematica
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Quark masses and the chiral condensate with a non-perturbative renormalization procedure

1999

We determine the quark masses and the chiral condensate in the MSbar scheme at NNLO from Lattice QCD in the quenched approximation at beta=6.0, beta=6.2 and beta=6.4 using both the Wilson and the tree-level improved SW-Clover fermion action. We extract these quantities using the Vector and the Axial Ward Identities and non-perturbative values of the renormalization constants. We compare the results obtained with the two methods and we study the O(a) dependence of the quark masses for both actions.

PhysicsQuarkNuclear and High Energy PhysicsParticle physicsquark masses QCD latticeHigh Energy Physics::LatticeHigh Energy Physics - Lattice (hep-lat)High Energy Physics::PhenomenologyFOS: Physical sciencesFísicaQuenched approximationLattice QCDFermionAtomic and Molecular Physics and OpticsAction (physics)FIS/02 - FISICA TEORICA MODELLI E METODI MATEMATICIRenormalizationHigh Energy Physics - LatticeBeta (velocity)High Energy Physics::ExperimentNon-perturbative
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Photometric and Hα Observations of LSI+61°303

1994

The Be massive X-ray binary LSI+61°303 is a 26.5 days periodic radiosource (Taylor & Gregory, 1984), exhibiting radio outbursts maxima between phases 0.6-0.8. Evidence of a photometric period of similar value has also been reported (Paredes & Figueras, 1986; Mendelson & Mazeh, 1989). The previous spectroscopic radial velocity observations of Hutchings & Crampton (1981) are in agreement with the radio period, and give support to the presence of a companion. We present new optical and infrared photometric observations and high resolution Hα spectra of LSI+61°303.

PhysicsRadial velocityInfraredHigh resolutionAstrophysicsMaximaSpectral line
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A detailed spectroscopy of the carbon-rich star BD +57° 2161

2005

An LTE abundance analysis based on high-resolution spectra is presented for the carbon-rich star BD +57° 2161, whose evolutionary status is unknown. With [C/Fe] = +0.4 dex and a mean s-process overabundance of [s/Fe] ≃ +1.5 dex the peculiar atmospheric composition of BD +57° 2161 is confirmed. The 12 C/ 13 C abundance ratio was found to be about 10. The mild iron deficiency, [Fe/H] = -0.2, supports the idea that BD +57° 2161 could be an old-disk-population object. Radial-velocity measurements confirm the binary nature of the star. Therefore the peculiar chemical composition could be due to the mass transfer from the secondary - AGB star in the past. Orbital parameters are estimated for anot…

PhysicsRadial velocitySpace and Planetary ScienceAsymptotic giant branchAstronomy and AstrophysicsAstrophysicsSpectroscopys-processStellar evolutionChemical compositionCarbon starSpectral lineAstronomy & Astrophysics
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KINETICS OF CRYSTAL GROWTH LIMITED BY RANDOM VELOCITY FIELDS

2008

A spherical growth process controlled by velocity fluctuations of particles of a saturated solution is investigated. Velocity fluctuations are modeled by a Gaussian random field. The interface evolution is determined by a Langevin-type equation with a multiplicative random field, which in the case of the quasi-homogeneous random Gaussian field is equivalent to Fokker–Planck dynamics. We analyze numerically the Fokker–Planck equation and compare growth kinetics in the case of noisy (i.e. space-independent) fluctuations. It is shown that for a large class of spatially correlated velocity fluctuations, the growth kinetics is universal, i.e. it does not depend on the details of statistics of f…

PhysicsRandom fieldField (physics)Applied MathematicsGaussianKineticsDynamics (mechanics)Multiplicative functionGaussian random fieldsymbols.namesakeFlow velocityModeling and SimulationsymbolsStatistical physicsEngineering (miscellaneous)International Journal of Bifurcation and Chaos
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Semi-global simulations of the magneto-rotational instability in core collapse supernovae

2009

Possible effects of magnetic fields in core collapse supernovae rely on an efficient amplification of the weak pre-collapse fields. It has been suggested that the magneto-rotational instability (MRI) leads to rapid field growth. Although MRI studies exist for accretion discs, the application of their results to core collapse supernovae is inhibited as the physics of supernova cores is substantially different from that of accretion discs. We address the problem of growth and saturation of the MRI by means of semi-global simulations, which combine elements of global and local simulations by taking the presence of global background gradients into account and using a local computational grid. W…

PhysicsResistive touchscreenMagnetohydrodynamics (MHD):ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Otras [UNESCO]Astrophysics (astro-ph)supernovae : general [Stars]magnetic fields [Stars]FOS: Physical sciencesAstronomy and AstrophysicsAngular velocityMechanicsAstrophysicsMagnetohydrodynamics (MHD); Instabilities; Stars : supernovae : general; Stars : magnetic fieldsAstrophysicsInstabilityMagnetic fieldSupernovaAmplitudeSpace and Planetary ScienceDispersion relationInstabilitiesUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::OtrasUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::EstrellasSaturation (chemistry):ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellas [UNESCO]
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Dynamics of a flexible ferromagnetic filament in a rotating magnetic field.

2017

Flexible magnetic filaments have garnered considerable attention as prospective materials for the creation of different microdevices. We describe a theoretical model of a ferromagnetic filament and derive its equations of motion by variational techniques. The numerical algorithm used to solve the filament dynamics in magnetic fields of different configurations is described. It is found that in a rotating field the filament transitions between synchronous and asynchronous regimes with respect to the rotating field, similarly to a rigid magnetic dipole. The mean angular velocity of the filament is well described by a relation valid for a rigid magnetic dipole with quantitative differences att…

PhysicsRotating magnetic fieldCondensed matter physicsField (physics)Equations of motionAngular velocity02 engineering and technology021001 nanoscience & nanotechnology01 natural sciences010305 fluids & plasmasMagnetic fieldQuantitative Biology::Subcellular ProcessesProtein filamentFerromagnetism0103 physical sciences0210 nano-technologyMagnetic dipolePhysical review. E
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Electro-kinetics of charged-sphere suspensions explored by integral low-angle super-heterodyne laser Doppler velocimetry

2012

We investigated the flow behaviour of colloidal charged-sphere suspensions using a newly designed integral low-angle super-heterodyne laser Doppler velocimetry instrument, which combines the advantages of several previous approaches. Sample conditions ranged from strong electrostatic interactions with pronounced short-range order to individual particles with no spatial correlations. The obtained power spectra correspond to diffusion broadened velocity distributions across the complete sample cross section. The excellent performance of the instrument is highlighted in detail by the example of electro-kinetic flow of suspensions in a closed cell of a rectangular cross section. We demonstrate …

PhysicsScatteringbusiness.industryLaser Doppler velocimetryCondensed Matter PhysicsElectrostaticsSpectral lineCharacterization (materials science)Cross section (physics)OpticsFlow (mathematics)General Materials Scienceddc:530Diffusion (business)business
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