Search results for "SPECTRA"

showing 10 items of 3542 documents

A Study Using Sulfur K-Edge XAS of Bitumens, Asphaltenes, Maltenes and their Oxidation Products by Comparison with Model Compounds

1997

High resolution Sulfur K-edge XANES spectra have been recorded at the ESRF on test samples of bitumen, asphaltene and maltene fractions and various model compounds. All these fractions were found to have a low content of sulfidic species as opposed to thiophenic species and it is therefore not surprising that thermally oxidized samples (RTFOT) had also a low content (1%) of sulfoxides. This is indeed consistent with the absence of any detectable S=O signature in the EXAFS spectra which were recorded over more than 1300 eV using the undulator gap scan technique.

X-ray absorption spectroscopyExtended X-ray absorption fine structureK-edgeChemistryAnalytical chemistryGeneral Physics and AstronomyHigh resolutionchemistry.chemical_elementSulfurXANESSpectral lineAsphalteneLe Journal de Physique IV
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Electronic structure of single-crystal rocksalt CdO studied by soft x-ray spectroscopies andab initiocalculations

2008

Soft x-ray emission spectroscopy (XES) and x-ray absorption spectroscopy (XAS) are employed to investigate the occupied and unoccupied electronic structures in rocksalt-phase single-crystal CdO. Resonant XES at the OK edge reveals a clear Cd 4d-O 2p hybridized peak and momentum-dependent coherent contributions to the resonant emission spectra. Good agreement is obtained between the above-threshold XES and XAS spectra, and the calculated O 2p local partial density of states (PDOS). Calculation of the O 2p PDOS was performed within the GW framework of many-body perturbation theory.

X-ray absorption spectroscopyMaterials scienceAbsorption spectroscopyAb initio quantum chemistry methodsAstrophysics::High Energy Astrophysical PhenomenaElectronic structureEmission spectrumPerturbation theoryAtomic physicsCondensed Matter PhysicsSingle crystalSpectral lineElectronic Optical and Magnetic MaterialsPhysical Review B
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Pressure-induced structural changes in α-MoO3 probed by X-ray absorption spectroscopy

2019

The authors are grateful to Prof. Alain Polian for providing NDAC cell. The research leading to this result has been supported by the project CALIPSOplus under the Grant Agreement 730872 from the EU Framework Programme for Research and Innovation HORIZON 2020. The work was supported by philanthropist MikroTik and administrated by the University of Latvia Foundation.

X-ray absorption spectroscopyMaterials scienceAbsorption spectroscopyExtended X-ray absorption fine structureAnalytical chemistryOxide02 engineering and technologyReverse Monte Carlo021001 nanoscience & nanotechnology01 natural sciencesSpectral lineXANESchemistry.chemical_compoundchemistry0103 physical sciences:NATURAL SCIENCES:Physics [Research Subject Categories]010306 general physics0210 nano-technologyAbsorption (electromagnetic radiation)
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XANES and EXAFS modelling of configurational disorder in silver borate glasses

2005

The sensitivity of X-ray absorption spectroscopy (XAS) to the local structure around a selected atomic species (symmetry, distances and angles) is commonly exploited to quantitatively describe systems where all the configurations around the absorbing atoms may be approximated by the mean one. However, in many cases of disordered systems a simple description of the local structure with singleconfiguration models cannot be reconciled with experimental spectra. In this paper the necessity to analyse the XAS spectra by considering a multiplicity of atomic structural configurations is demonstrated in the case of silver borate glasses. The local coordination around Ag cations in (Ag2O.nB2O3) glas…

X-ray absorption spectroscopyMaterials scienceAbsorption spectroscopyExtended X-ray absorption fine structureilver borate glasseschemistry.chemical_elementX-ray absorption spectroscopyCondensed Matter PhysicsMolecular physicsAtomic and Molecular Physics and OpticsXANESSpectral lineCondensed Matter::Materials ScienceX-ray absorption spectroscopy; ilver borate glasses; model structuresK-edgechemistrymodel structuresMultiplicity (chemistry)BoronMathematical Physics
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cis-[(η5-C5H5)Fe(η1-CO)(μ-CO)]2, the poor relative between cis and trans tautomers. A theoretical study of the gas-phase Fe L3-edge and C and O K-edg…

2021

The relative stability of trans-[(η5-C5H5)Fe(η1-CO)(μ-CO)]2 (trans-I) and cis-I tautomers in a vacuum and in solvents with different dielectric constants (e) has been investigated by exploiting density functional theory (DFT). Theoretical results indicate that, in agreement with experimental evidence, trans-I is more stable than cis-I in a vacuum (∼1.5 kcal mol−1; e = 1), while the opposite is true in media with e > 7. Differently from solution, DFT outcomes pertaining to the vapor-phase cis-I ⇆ trans-I equilibrium at T = 368 K, the temperature at which the Fe L2,3-edges and the C and O K-edge X-ray absorption spectroscopy (XAS) data of I have been recorded, ultimately indicate the trans-I …

X-ray absorption spectroscopyMaterials scienceK-edgeAbsorption spectroscopyGeneral Physics and AstronomyPhysical chemistryDensity functional theoryDielectricPhysical and Theoretical ChemistryTautomerSpectral lineCis–trans isomerismPhysical Chemistry Chemical Physics
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Wavelet data analysis of EXAFS spectra

2009

Abstract The application of wavelet transform to the analysis of the extended X-ray absorption fine structure (EXAFS) from perovskite-type compounds is presented on the example of the Re L 3 -edge in ReO 3 and Co K-edge in LaCoO 3 . We propose a modified wavelet transform procedure, which allows better discrimination of the overlapped contributions into the EXAFS signal.

X-ray absorption spectroscopyMaterials scienceNuclear magnetic resonanceWaveletExtended X-ray absorption fine structureHardware and ArchitectureGeneral Physics and AstronomyWavelet transformAbsorption (electromagnetic radiation)Spectral lineComputational physicsComputer Physics Communications
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Broadband observations of the X-ray burster 4U1705-44 with Beppo SAX

2016

4U 1705-44 is one of the most-studied type I X-ray burster and Atoll sources. This source represents a perfect candidate to test different models proposed to self-consistently track the physical changes occurring between different spectral states because it shows clear spectral state transitions. The broadband coverage, the sensitivity and energy resolution of the BeppoSAX satellite offers the opportunity to disentangle the components that form the total X-ray spectrum and to study their changes according to the spectral state. Using two BeppoSAX observations carried out in August and October 2000, respectively, for a total effective exposure time of about 100 ks, we study the spectral evol…

X-ray bursterAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)AstrophysicsX-rays: general01 natural sciencesSpectral lineAccretion accretion diskStars: individual: 4U 1705-44Settore FIS/05 - Astronomia E Astrofisica0103 physical sciencesBlack-body radiationX-rays: star010303 astronomy & astrophysicsLine (formation)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAccretion (meteorology)010308 nuclear & particles physicsAstronomy and AstrophysicsAstronomy and AstrophysicX-rays: binarieStars: neutronNeutron starSpace and Planetary ScienceReflection (physics)individual: 4U 1705-44; Stars: neutron; X-rays: binaries; X-rays: general; X-rays: stars; Astronomy and Astrophysics; Space and Planetary Science [Accretion accretion disks; Stars]Astrophysics - High Energy Astrophysical Phenomena
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ATHENA WFI optical blocking filters development status toward the end of the instrument phase-A

2018

Copyright 2018 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited. The Wide Field Imager (WFI) is one of the two instruments of the ATHENA astrophysics space mission approved by ESA as the second large mission in the Cosmic Vision 2015-2025 Science Programme. The WFI, based on a large array of depleted field effect transistors (DEPFET), will provide imaging in the 0.2-15 keV band over a 40'x40' field of view, simultaneously with spectrally an…

X-ray detectorCosmic VisionPhotonX-ray detectorWide Field ImagerField of viewCondensed Matter Physic7. Clean energy01 natural sciences010309 opticsX-ray astronomyOpticsSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesAthenaSpectral resolutionElectrical and Electronic EngineeringOptical blocking filter010303 astronomy & astrophysicsPhysicsCMOS sensorbusiness.industryElectronic Optical and Magnetic MaterialDetectorComputer Science Applications1707 Computer Vision and Pattern RecognitionPhoton countingApplied MathematicActive pixel sensor13. Climate actionbusinessDEPFET
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Collinear fast-beam laser spectroscopy

1987

The progress in atomic and molecular spectroscopy has gone hand in hand with improvements of the resolution. Before the tunable narrow-band lasers led to the invention of Doppler-free techniques, spectral lines from cooled hollow-cathode discharges(1) had typical widths larger than 300 MHz, and high resolution was achieved only in rf spectroscopy, e.g., within hyperfine structure multiplets, by the classical techniques like atomic beam magnetic resonance,(2) optical pumρing,(3) or double resonance.(4) While the Doppler broadening $$\delta {v_D} = {v_0}{\left( {{{8kT{\rm{ }}\ln {\rm{ 2}}} \over {m{c^2}}}} \right)^{1/2}}$$ (1) is negligible for resonance frequencies v 0 in the rf regime, the …

X-ray laserPhysicsThermal velocityResonanceNuclear Physics - ExperimentAtomic physicsCoherent spectroscopySpectroscopyHyperfine structureSpectral lineDoppler broadening
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EBIT diagnostics using X-ray spectra of highly ionized Ne

2003

We have carried out a detailed analysis of highly ionized neon spectra collected at the NIST EBIT using an NTD germanium X-ray microcalorimeter developed at the Harvard-Smithsonian Center for Astrophysics [Nucl. Instr. and Meth. A 444 (2000) 156]. Our attention was focused especially on the Ne IX He-like triplet to check electron density diagnostics through the intercombination/forbidden line ratio. We have investigated possible effects of the ion dynamics on the plasma emission line intensities, looking at the dependence of the count-rate and the charge state distribution on the electron beam energy and current. The temperature and spatial distribution of the neon ions, and hence the overl…

X-ray spectraNuclear and High Energy PhysicsElectron densityEBITChemistrySurfaces Coatings and Filmchemistry.chemical_elementFizikai tudományokSurfaces and InterfacesPlasmaIonNeonSettore FIS/05 - Astronomia E AstrofisicaTermészettudományokIonizationAstrophysical plasmaPhysics::Atomic PhysicsEmission spectrumAtomic physicsIonization of atomForbidden mechanismInstrumentationExcitation
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