Search results for "Dispersion."

showing 10 items of 1094 documents

Role of dispersion on zero-average-index bandgaps

2009

We consider periodic multilayers combining ordinary positive index materials and dispersive metamaterials with negative index in some frequency ranges. These structures can exhibit photonic bandgaps which, in contrast with the usual Bragg gaps, are not based on interference mechanisms. Changing the dispersion models for the constituent metamaterial, we investigate its role in the production of zero-average-index bandgaps. In particular, we show the effect of each constitutive parameter on both bandgap edges. Finally, we give some approximated analytical expressions in terms of average parameters for the determination of the upper and lower limits of the zero-average refractive-index bandgap…

PhysicsCondensed matter physicsbusiness.industryWave propagationBand gapCiencias FísicasPHOTONIC CRYSTALSPhysics::OpticsMetamaterialStatistical and Nonlinear PhysicsInterference (wave propagation)Atomic and Molecular Physics and OpticsNEGATIVE INDEXAstronomíaCondensed Matter::Materials ScienceOpticsPHOTONIC BAND GAPNegative refractionDispersion (optics)MULTILAYERSPhotonicsbusinessRefractive indexCIENCIAS NATURALES Y EXACTAS
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Understanding and controlling N-dimensional quantum walks via dispersion relations: application to the two-dimensional and three-dimensional Grover w…

2013

The discrete quantum walk in N dimensions is analyzed from the perspective of its dispersion relations. This allows understanding known properties, as well as designing new ones when spatially extended initial conditions are considered. This is done by deriving wave equations in the continuum, which are generically of the Schrodinger type, and allows devising interesting behavior, such as ballistic propagation without deformation, or the generation of almost flat probability distributions, which is corroborated numerically. There are however special points where the energy surfaces display intersections and, near them, the dynamics is entirely different. Applications to the two- and three-d…

PhysicsContinuum (topology)General Physics and AstronomyFísicaSpaceType (model theory)Wave equationsymbols.namesakePerspective (geometry)Dispersion relationsymbolsProbability distributionQuantum walkStatistical physicsGrapheneSchrödinger's cat
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Stabilisation of dispersion-managed soliton transmissions by nonlinear gain

1999

Nonlinear gain is shown to be effective in suppressing the radiative background that may not be separated from the signal when the average dispersion is close to zero in dispersion-managed soliton transmissions. By correctly combining nonlinear gain and filtering, the instability introduced by guiding filters can be avoided.

PhysicsControl theoryNonlinear gainDispersion (optics)Radiative transferDispersion managedSoliton (optics)Electrical and Electronic EngineeringSignalInstabilityElectronics Letters
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PECULIAR TRANSVERSE VELOCITIES OF GALAXIES FROM QUASAR MICROLENSING. TENTATIVE ESTIMATE OF THE PECULIAR VELOCITY DISPERSION ATZ∼ 0.5

2016

We propose to use the flux variability of lensed quasar images induced by gravitational microlensing to measure the transverse peculiar velocity of lens galaxies over a wide range of redshift. Microlensing variability is caused by the motions of the observer, the lens galaxy (including the motion of the stars within the galaxy), and the source; hence, its frequency is directly related to the galaxy's transverse peculiar velocity. The idea is to count time-event rates (e.g., peak or caustic crossing rates) in the observed microlensing light curves of lensed quasars that can be compared with model predictions for different values of the transverse peculiar velocity. To compensate for the larg…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsFOS: Physical sciencesAstronomy and AstrophysicsQuasarAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGravitational microlensing01 natural sciencesGalaxyTransverse planeSpace and Planetary Science0103 physical sciencesDispersion (optics)Peculiar velocity010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic AstrophysicsThe Astrophysical Journal
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Systematic variation of the stellar Initial Mass Function with velocity dispersion in early-type galaxies

2012

An essential component of galaxy formation theory is the stellar initial mass function (IMF), that describes the parent distribution of stellar mass in star forming regions. We present observational evidence in a sample of early-type galaxies (ETGs) of a tight correlation between central velocity dispersion and the strength of several absorption features sensitive to the presence of low-mass stars. Our sample comprises ~40,000 ETGs from the SPIDER survey (z<0.1). The data, extracted from the Sloan Digital Sky Survey, are combined, rejecting both noisy data, and spectra with contamination from telluric lines, resulting in a set of 18 stacked spectra at high signal-to-noise ratio (S/N> …

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Initial mass functionDark matterFOS: Physical sciencesAstronomyVelocity dispersionAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics - Astrophysics of GalaxiesGalaxyAbundance of the chemical elementsStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Galaxy formation and evolutionLenticular galaxySolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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SPIDER VIII - Constraints on the Stellar Initial Mass Function of Early-type Galaxies from a Variety of Spectral Features

2013

We perform a spectroscopic study to constrain the stellar Initial Mass Function (IMF) by using a large sample of 24,781 early-type galaxies from the SDSS-based SPIDER survey. Clear evidence is found of a trend between IMF and central velocity dispersion, sigma0, evolving from a standard Kroupa/Chabrier IMF at 100km/s towards a more bottom-heavy IMF with increasing sigma0, becoming steeper than the Salpeter function at sigma0>220km/s. We analyze a variety of spectral indices, corrected to solar scale by means of semi-empirical correlations, and fitted simultaneously with extended MILES (MIUSCAT) stellar population models. Our analysis suggests that sigma0, rather than [alpha/Fe], drives t…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Initial mass functionStellar populationmedia_common.quotation_subjectFOS: Physical sciencesVelocity dispersionAstronomy and AstrophysicsAstrophysicsSpectral lineGalaxyStarsSpace and Planetary ScienceSkyGlobular clustermedia_commonAstrophysics - Cosmology and Nongalactic Astrophysics
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THE ORIENTATION OF GALAXIES IN GALAXY CLUSTERS

2010

We present an analysis of the spatial orientations of galaxies in the 247 optically selected rich Abell clusters, having in the considered area at least 100 members. We investigated the relation between angles giving information about galaxy angular momenta and the number of members in each structure. The position angles of the galaxy major axes, as well as two angles describing the spatial orientation of galaxy plane were tested for isotropy, by applying three different statistical tests. It is found that the values of statistics increase with the amount of galaxies' members, which is equivalent to the existence of the relation between anisotropy and number of galaxies in cluster. The sear…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Plane (geometry)IsotropyFOS: Physical sciencesVelocity dispersionAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGalaxySpace and Planetary ScienceOrientation (geometry)Cluster (physics)AnisotropyGalaxy clusterAstrophysics - Cosmology and Nongalactic AstrophysicsThe Astrophysical Journal
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Peculiarities of coherent optical oscillation in Sn_2P_2S_6 crystals

2010

We show analytically and numerically that the unusual photorefractive nonlinear response of Sn2P2S6 crystals leads to a variety of new features of coherent optical oscillation. In addition to the explanation of the known peculiarities, new features are predicted.

PhysicsDiffractionCondensed matter physicsOscillationPhysics::OpticsNonlinear opticsStatistical and Nonlinear PhysicsPhotorefractive effectFerroelectricityAtomic and Molecular Physics and OpticsFour-wave mixingQuantum mechanicsDispersion (optics)Refractive indexJournal of the Optical Society of America B
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Thermalization of the dispersive three-wave interaction

2007

We investigate the role of dispersion effects on the long-term evolution of the nonlinear three-wave interaction. We show that the three waves exhibit, as a general rule, an irreversible evolution towards a thermodynamic equilibrium state in which they propagate with identical velocities. As a result of this thermalization process, the three-wave system is driven away from spatio-temporal resonance, so that the equilibrium state does not satisfy the (phase-matching) resonant conditions of energy and momentum conservation for the averaged frequencies. Moreover, we show that the interplay between temporal dispersion and spatial diffraction leads to the emergence of a peculiar equilibrium stat…

PhysicsDiffractionThermodynamic equilibriumGeneral Physics and AstronomyEnergy–momentum relationState (functional analysis)01 natural sciencesResonance (particle physics)010305 fluids & plasmasNonlinear systemThermalisationClassical mechanicsQuantum electrodynamics0103 physical sciences010306 general physicsDispersion (water waves)ComputingMilieux_MISCELLANEOUS
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All-incoherent dispersion-compensated optical correlator

2007

We report on a simple, spatially incoherent, wavelength-independent imaging system that, in contrast to the conventional case, exhibits a dispersion-compensated point-spread function. Our hybrid (diffractive-refractive) three-lens imaging configuration thus acts as an all-incoherent dispersion-compensated optical irradiance correlator. So the optical arrangement is well adapted to processing color information (both spatially and temporally incoherent) under natural illumination.

PhysicsDiffractionbusiness.industrymedia_common.quotation_subjectIrradiancePhysics::OpticsAtomic and Molecular Physics and OpticsPtychographyOpticsDispersion (optics)Optical correlatorContrast (vision)businessFresnel diffractionmedia_commonVisible spectrum
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