Search results for "Spectral"

showing 10 items of 3116 documents

Measurements and calculations of Stark broadening parameters for the N I multiplet (1D)3s2D–(1D)3p2Do

2014

Calculations of line broadening parameters of a doubly excited N I transition, based on atomic structure data (taken from the literature), are reported. The obtained results were used for a critical analysis of formerly published experimental data, based on spectra measured in our laboratory. These measured spectra were then again analyzed and new broadening parameters were determined and compared with results of calculations.

Physicssymbols.namesakeStark effectExcited statesymbolsAtomic physicsCondensed Matter PhysicsMultipletMathematical PhysicsAtomic and Molecular Physics and OpticsSpectral lineLine (formation)Physica Scripta
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Stark broadening of hydrogen spectral lines with fine structure effects

2004

Formalism and numerical code have been elaborated for calculation of hydrogen line profiles in conditions of plasma in which Stark broadening and fine energy splitting are comparable and it is not possible to neglect either of them. It corresponds to the range of electron densities $10^{11} < N_e ({\rm cm}^{-3}) < 10^{15}$ . Lamb shift and spontaneous emission effects have also been included. Computer simulation method was applied in the calculations. Final results have been compared with experimental and theoretical findings by other authors.

Physicssymbols.namesakeStark effectOptical physicssymbolsHydrogen lineSpontaneous emissionElectronAtomic physicsHydrogen spectral seriesHyperfine structureAtomic and Molecular Physics and OpticsLamb shiftThe European Physical Journal D - Atomic, Molecular and Optical Physics
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Energy gap of intermediate-valentSmB6studied by point-contact spectroscopy

2001

We have investigated the intermediate valence narrow-gap semiconductor ${\mathrm{SmB}}_{6}$ at low temperatures using both conventional spear-anvil type point contacts as well as mechanically controllable break junctions. The zero-bias conductance varied between less than $0.01 \ensuremath{\mu}\mathrm{S}$ and up to 1 mS. The position of the spectral anomalies, which are related to the different activation energies and band gaps of ${\mathrm{SmB}}_{6},$ did not depend on the the contact size. Two different regimes of charge transport could be distinguished: Contacts with large zero-bias conductance are in the diffusive Maxwell regime. They had spectra with only small nonlinearities. Contacts…

Physicssymbols.namesakeValence (chemistry)Condensed matter physicsBand gapFermi levelsymbolsDensity of statesQuasiparticleConductanceAtomic physicsSpectroscopySpectral linePhysical Review B
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Fourier-transform spectroscopy and coupled-channels deperturbation treatment of theA 1Σ+–b 3Πcomplex of KCs

2010

The laser-induced fluorescence (LIF) A {sup 1{Sigma}+}-b {sup 3{Pi}{yields}}X {sup 1{Sigma}+} spectra of the KCs molecule were recorded in a near infrared region by a Fourier-transform spectrometer with a resolution of 0.03 cm{sup -1}. Overall more than 200 collisionally enhanced LIF spectra were rotationally assigned to {sup 39}K{sup 133}Cs and {sup 41}K{sup 133}Cs isotopomers yielding more than 3400 rovibronic term values of the strongly mixed singlet A {sup 1{Sigma}+} and triplet b {sup 3{Pi}} states with the uncertainty of 0.003-0.01 cm{sup -1}. Experimental data massive starts from the lowest vibrational level v{sub A}=0 of the singlet and nonuniformly covers the energy range E is an e…

Physicssymbols.namesakesymbolsSinglet stateAtomic physicsSpectroscopyGround stateQuantum numberHamiltonian (quantum mechanics)Potential energyOmegaAtomic and Molecular Physics and OpticsSpectral linePhysical Review A
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Diagrammatic expansion for positive spectral functions beyond GW : Application to vertex corrections in the electron gas

2014

We present a diagrammatic approach to construct self-energy approximations within many-body perturbation theory with positive spectral properties. The method cures the problem of negative spectral functions which arises from a straightforward inclusion of vertex diagrams beyond the GW approximation. Our approach consists of a two-steps procedure: we first express the approximate many-body self-energy as a product of half-diagrams and then identify the minimal number of half-diagrams to add in order to form a perfect square. The resulting self-energy is an unconventional sum of self-energy diagrams in which the internal lines of half a diagram are time-ordered Green's functions whereas those…

Physicsta114Spectral propertiesFOS: Physical sciencesElectronic structureCondensed Matter PhysicsImaging phantompositive spectral functionsElectronic Optical and Magnetic MaterialsSettore FIS/03 - Fisica della Materiaelectron gasCondensed Matter - Other Condensed MatterTheoretical physicsDiagrammatic reasoningAb initio quantum chemistry methodsHomogeneousQuantum mechanicsCoulombFermi gasOther Condensed Matter (cond-mat.other)Physical Review B
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Optical spectroscopy of X-ray sources in the Taurus molecular cloud: discovery of ten new pre-main sequence stars

2008

We have analyzed optical spectra of 25 X-ray sources identified as potential new members of the Taurus molecular cloud (TMC), in order to confirm their membership in this SFR. Fifty-seven candidates were previously selected among the X-ray sources in the XEST survey, having a 2MASS counterpart compatible with a PMS star based on color-magnitude and color-color diagrams. We obtained high-resolution optical spectra for 7 of these candidates with the SARG spectrograph at the TNG telescope, which were used to search for Li absorption and to measure the Ha line and the radial and rotational velocities; 18 low-resolution optical spectra obtained with DOLORES for other candidate members were used …

Physicstechniques: spectroscopic stars: luminosity function mass function stars: pre-main sequence Galaxy: open clusters and associations: individual: Taurus molecular cloudMolecular cloudAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsStellar classificationSurface gravityAstrophysicsSpectral lineStarsSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsEmission spectrumMain sequenceAstrophysics::Galaxy AstrophysicsLine (formation)
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High-spin states in the neutron-rich A∼100 region

2009

Two experimental setups have been used to study excited states of neutron‐rich nuclei in the A∼100 region. Extended level schemes and lifetime measurements were obtained using deep‐inelastic and fusion‐fission reactions with the CLARA‐PRISMA spectrometer and the Ge‐array GASP respectively. Experimental information from GASP has been used to complement the CLARA‐PRISMA experiment. Time spectra have been used to measure the lifetimes of isomeric states. Preliminary results are presented for 89Rb.

Physicsγ-ray transitionsSpin statesSpectrometerAstrophysics::High Energy Astrophysical PhenomenaLifetimesPRISMA-CLARA spectrometerGASP arrayDeep inelastic scatteringSpectral lineNuclear physicsPhysics and Astronomy (all)Excited stateNuclear fusionNeutronGamma spectroscopyAtomic physicsγ-ray transitions; GASP array; Lifetimes; PRISMA-CLARA spectrometer; Physics and Astronomy (all)Nuclear ExperimentAIP Conference Proceedings
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Electronic States, Absorption Spectrum and Circular Dichroism Spectrum of the Photosynthetic Bacterial LH2 Antenna of Rhodopseudomonas acidophila as …

1999

A new approach that uses a combination of semiempirical configuration interaction method and exciton theory to calculate electronic energies, eigenstates, absorption spectrum and circular dichroism (CD) spectrum of the LH2 antenna of Rhodopseudomonas acidophila is introduced. A statistical simulation that uses experimental homogeneous line widths was used to account for the inhomogeneous line width of the observed spectrum. Including the effect of orbital overlap of the close-lying pigments of the B850 ring and the effect of the pigment protein interaction in the B800 ring allowed a successful simulation of the experimental absorption and CD spectra of the antenna at room temperature. Two e…

Physics::Biological PhysicsCircular dichroismAbsorption spectroscopyChemistryExcitonTransition dipole momentOrbital overlapConfiguration interactionPhotochemistryMolecular physicsSpectral lineSurfaces Coatings and FilmsX-ray magnetic circular dichroismMaterials ChemistryPhysical and Theoretical ChemistryThe Journal of Physical Chemistry B
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Laboratory astrophysics survey of key x-ray diagnostic lines using a microcalorimeter on an electron beam ion trap

2000

Cosmic plasma conditions created in an electron beam ion trap (EBIT) make it possible to simulate the dependencies of key diagnostic X-ray lines on density, temperature, and excitation conditions that exist in astrophysical sources. We used a microcalorimeter for such laboratory astrophysics studies because it has a resolving power ≈1000, quantum efficiency approaching 100%, and a bandwidth that spans the X-ray energies from 0.2 keV to 10 keV. Our microcalorimeter, coupled with an X-ray optic to increase the effective solid angle, provides a significant new capability for laboratory astrophysics measurements. Broadband spectra obtained from the National Institute of Standards and Technology…

Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical Phenomenachemistry.chemical_elementFizikai tudományokAstrophysicsSpectral lineNeonTermészettudományokAtomic processeIonizationPhysics::Atomic PhysicsAtomic dataNuclear and High Energy PhysicPhysicsArgonKryptonAstronomy and AstrophysicsLine: IdentificationPlasmaX-rays: GeneralchemistrySpace and Planetary ScienceAstrophysical plasmaMethods: Laboratory plasmaAtomic physicsElectron beam ion trap
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A class-separability-based method for multi/hyperspectral image color visualization

2010

In this paper, a new color visualization technique for multi- and hyperspectral images is proposed. This method is based on a maximization of the perceptual distance between the scene endmembers as well as natural constancy of the resulting images. The stretched CMF principle is used to transform reflectance into values in the CIE L*a*b* colorspace combined with an a priori known segmentation map for separability enhancement between classes. Boundaries are set in the a*b* subspace to balance the natural palette of colors in order to ease interpretation by a human expert. Convincing results on two different images are shown.

PixelComputer sciencebusiness.industryComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONPalette (computing)Hyperspectral imagingImage segmentationColor spaceVisualizationSegmentationComputer visionArtificial intelligencebusinessSubspace topology2010 IEEE International Conference on Image Processing
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