Search results for "Spatial"

showing 10 items of 2121 documents

Impact-parameter dependent nuclear parton distribution functions: EPS09s and EKS98s and their applications in nuclear hard processes

2012

We determine the spatial (impact parameter) dependence of nuclear parton distribution functions (nPDFs) using the $A$-dependence of the spatially independent (averaged) global fits EPS09 and EKS98. We work under the assumption that the spatial dependence can be formulated as a power series of the nuclear thickness functions $T_A$. To reproduce the $A$-dependence over the entire $x$ range we need terms up to $[T_A]^4$. As an outcome, we release two sets, EPS09s (LO, NLO, error sets) and EKS98s, of spatially dependent nPDFs for public use. We also discuss the implementation of these into the existing calculations. With our results, the centrality dependence of nuclear hard-process observables…

PhysicsPower seriesNuclear and High Energy PhysicsParticle physicsta114Nuclear Theory010308 nuclear & particles physicsFOS: Physical sciencesObservableParton01 natural sciencesNuclear Theory (nucl-th)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Distribution functionPion0103 physical sciencesProduction (computer science)Spatial dependenceImpact parameterNuclear Experiment010306 general physicsParticle Physics - Phenomenology
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EPS09s and EKS98s: Impact parameter dependent nPDF sets

2013

In our recent study we have determined two new spatially dependent nuclear PDF (nPDF) sets, EPS09s and EKS98s. With these, the hard-process cross-sections can be calculated in different centrality classes consistently with the globally analyzed nPDFs for the first time. The sets were determined by exploiting the $A$-systematics of the globally fitted nPDF sets, EPS09 and EKS98. For the spatial dependence of the nPDFs we used a power series ansatz in the nuclear thickness function $T_A$. In this flash talk we introduce the framework, and present our NLO EPS09s-based predictions for the nuclear modification factor in four centrality classes for inclusive neutral pion production in p+Pb collis…

PhysicsQuantum chromodynamicsPower seriesNuclear and High Energy PhysicsParticle physicsLarge Hadron Colliderta114Nuclear Theory010308 nuclear & particles physicsFOS: Physical sciencesFunction (mathematics)01 natural sciencesNuclear Theory (nucl-th)Nuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Pion0103 physical sciencesSpatial dependenceImpact parameterNuclear Experiment010306 general physicsParticle Physics - PhenomenologyAnsatzNuclear Physics A
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Absolute instability in backward wave four-wave mixing: spatial effects

2010

The spatial distribution of new beams generated above the threshold of absolute instability of two counterpropagating incoherent light waves is studied and compared with the results of calculation.

PhysicsScatteringbusiness.industryWave propagationNonlinear opticsStatistical and Nonlinear PhysicsPolarization (waves)InstabilityAtomic and Molecular Physics and OpticsComputational physicsFour-wave mixingOpticsLight beamSpatial frequencybusinessJournal of the Optical Society of America B
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Spatial correlation of laser-generated electrons and holes in quantum wells

1995

The spatial correlation of hot electrons and holes generated by light in a semiconductor quantum well (QW) is studied. For hot electron-hole pairs in a polar material, this correlation is determined by the interaction with LO-phonons. We analyze the distribution F N (r, K) of electrons and holes which are created in a given light absorption process, with respect to their relative separation r and total quasimomentum ħK, after the emission of a number N of LO-phonons. The relationship between the spatial distribution of electrons and holes in these intermediate states and the cross-section of multi-phonon resonant Raman scattering (MPRRS) is established. Spatial correlation effects are stron…

PhysicsSpatial correlationbusiness.industryQuantum-confined Stark effectElectronCondensed Matter PhysicsLaserSpatial distributionElectronic Optical and Magnetic Materialslaw.inventionsymbols.namesakeSemiconductorlawsymbolsAtomic physicsbusinessRaman scatteringQuantum wellphysica status solidi (b)
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Wavelength-multiplexed computational temporal ghost imaging

2017

Ghost imaging is a novel imaging technique based on correlation measurements between a structured illumination pattern (the reference) and the total intensity transmitted or reflected by an object [1]. The reference illumination patterns may be either randomly generated by a spatially incoherent light source, or pre-programmed e.g. with a spatial light modulator. Light transmitted (or reflected) by the object is measured by a single-pixel “bucket” detector with null spatial resolution. A unique feature associated with ghost imaging is that (i) neither the bucket detector nor the reference measurement caries enough information to retrieve the object shape and (ii) it is insensitive to distor…

PhysicsSpatial light modulatorNull (radio)business.industryDetector02 engineering and technologyGhost imaging021001 nanoscience & nanotechnology01 natural sciences010309 opticsWavelengthOpticsFeature (computer vision)Temporal resolution0103 physical sciences0210 nano-technologybusinessImage resolution2017 Conference on Lasers and Electro-Optics Europe & European Quantum Electronics Conference (CLEO/Europe-EQEC)
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Second order diffractive optical elements in a spatial light modulator with large phase dynamic range

2013

International audience; A study of the diffraction efficiency of a spatial light modulator with a large dynamic phase range is reported. We use a phase-only device that reaches 4π phase modulation depth for the wavelength of 454 nm. This allows operating phase-only diffractive optical elements in the second harmonic diffraction order, instead of in the usual first diffraction order. This type of implementation shows advantages in terms of resolution and diffraction efficiency. Experimental results are reported for blazed diffractive gratings and diffractive lenses.

PhysicsSpatial light modulatorbusiness.industryDynamic rangeMechanical EngineeringResolution (electron density)Phase (waves)Physics::Optics02 engineering and technology021001 nanoscience & nanotechnologyDiffraction efficiency01 natural sciencesAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic Materials010309 opticsWavelengthOptics0103 physical sciencesOptoelectronicsElectrical and Electronic Engineering[SPI.NANO]Engineering Sciences [physics]/Micro and nanotechnologies/Microelectronics0210 nano-technologybusinessDiffraction gratingPhase modulation
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Time-multiplexed chromatic-controlled axial diffractive optical elements

2010

Programmable diffractive optical elements DOEs with axial response have many interesting applications, including diffractive lenses, axicons, and optical tweezers. In all these cases, it is essential to properly select the modulation configuration of the spatial light modulator SLM where the DOE is displayed, in order to avoid the undiffracted zero order component that appears on axis and overlaps the desired axial response. However, in general, the chromatic dispersion in liquid crystal SLMs prevents the cancellation of the zero order for a broadband light source, thus limiting the possibilities for polychromatic program- mable axial DOEs. We operate a ferroelectric liquid crystal on silic…

PhysicsSpatial light modulatorbusiness.industryFourier opticsGeneral EngineeringPhysics::OpticsAtomic and Molecular Physics and OpticsLiquid crystal on siliconOpticsOptical tweezersDispersion (optics)OptoelectronicsChromatic scalebusinessPhase modulationDiffraction gratingOptical Engineering
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Testing the companion hypothesis for the origin of the X-ray emission from intermediate-mass main-sequence stars

2006

There is no straightforward explanation for intrinsic X-ray emission from intermediate-mass main-sequence stars. Therefore the observed emission is often interpreted in terms of (hypothesized) late-type magnetically active companion stars. We use Chandra imaging observations to spatially resolve in X-rays a sample of main-sequence B-type stars with recently discovered companions at arcsecond separation. We find that all spatially resolved companions are X-ray emitters, but seven out of eleven intermediate-mass stars are also X-ray sources. If this emission is interpreted in terms of additional sub-arcsecond or spectroscopic companions, this implies a high multiplicity of B-type stars. Firm …

PhysicsSpatially resolvedAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsStarsSpace and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsMultiplicity (chemistry)Main sequenceAstrophysics::Galaxy Astrophysics
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Making Mathematics in an Oral Culture: Göttingen in the Era of Klein and Hilbert

2004

This essay takes a close look at specially selected features of the Göttingen mathematical culture during the period 1895–1920. Drawing heavily on personal accounts and archival resources, it describes the changing roles played by Felix Klein and David Hilbert, as Göttingen's two senior mathematicians, within a fast-growing community that attracted an impressive number of young talents. Within the course of these twenty-five years Göttingen exerted a profound impact on mathematics and physics throughout the world. Many factors contributed to the creation of a special atmosphere that served as a model for several other important centers for mathematical research. Göttingen exemplified a dyna…

PhysicsSpoken wordsymbols.namesakeHistory and Philosophy of ScienceMathematics educationsymbolsGeneral Social SciencesEinsteinAtmosphere (architecture and spatial design)Mathematical researchPeriod (music)MathematicsScience in Context
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Mass Segregation in the Open Cluster NGC 2422

2003

UBVRI photometry of the open cluster NGC2422 (age ~10 8  yr) down to a limiting magnitude V ≃ 19 is used to study the cluster spatial distribution and the luminosity and mass functions. From the Color-Magnitude Diagram (CMD), we obtained a list of candidate cluster members based on a photometric criterion. Using a comparison field region and an iterative procedure, a correction for contaminating field stars has been inferred in order to obtain the luminosity and the mass functions in the M=0.4 -3.5 M ⊙ range. By analyzing the spatial distribution, we infer that a non-negligible number of cluster stars lie outside our investigated region. We estimate a correction to the mass function of the …

PhysicsStellar populationGeneral EngineeringAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsSpatial distributionPhotometry (optics)StarsSpace and Planetary ScienceLimiting magnitudeAstrophysics::Solar and Stellar AstrophysicsMass segregationPleiadesAstrophysics::Galaxy AstrophysicsOpen clusterEAS Publications Series
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