Search results for "Spectral"

showing 10 items of 3116 documents

Note on singular Clairaut-Liouville metrics

2008

Computations on Clairaut-Liouville metrics on S^2 with a finite order singularity.

[ MATH.MATH-OC ] Mathematics [math]/Optimization and Control [math.OC]High Energy Physics::Theory[MATH.MATH-OC] Mathematics [math]/Optimization and Control [math.OC][MATH.MATH-OC]Mathematics [math]/Optimization and Control [math.OC]Mathematics::Spectral Theory
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$PT$-symmetry and Schrödinger operators. The double well case

2016

International audience; We study a class of $PT$-symmetric semiclassical Schrodinger operators, which are perturbations of a selfadjoint one. Here, we treat the case where the unperturbed operator has a double-well potential. In the simple well case, two of the authors have proved in [6] that, when the potential is analytic, the eigenvalues stay real for a perturbation of size $O(1)$. We show here, in the double-well case, that the eigenvalues stay real only for exponentially small perturbations, then bifurcate into the complex domain when the perturbation increases and we get precise asymptotic expansions. The proof uses complex WKB-analysis, leading to a fairly explicit quantization condi…

[ MATH.MATH-SP ] Mathematics [math]/Spectral Theory [math.SP]MSC: 35P20 81Q12 81Q20 35Q40Complex WKB analysis[ MATH.MATH-MP ] Mathematics [math]/Mathematical Physics [math-ph]EigenvaluesMathematics::Spectral TheoryPT-symmetryMathematics - Spectral Theory[MATH.MATH-MP]Mathematics [math]/Mathematical Physics [math-ph]35P20 35Q40 81Q12 81Q20Quantization conditonSchrödinger operatorsMathematical Physics[MATH.MATH-SP]Mathematics [math]/Spectral Theory [math.SP]
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Shaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Cascade in Massive Galaxies, Groups, and Clusters

2018

We propose a novel method to constrain turbulence and bulk motions in massive galaxies, groups and clusters, exploring both simulations and observations. As emerged in the recent picture of the top-down multiphase condensation, the hot gaseous halos are tightly linked to all other phases in terms of cospatiality and thermodynamics. While hot halos (10^7 K) are perturbed by subsonic turbulence, warm (10^4 K) ionized and neutral filaments condense out of the turbulent eddies. The peaks condense into cold molecular clouds (< 100 K) raining in the core via chaotic cold accretion (CCA). We show all phases are tightly linked via the ensemble (wide-aperture) velocity dispersion along the line o…

[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics01 natural sciencesSpectral lineGalaxy groupAbsorption (logic)010303 astronomy & astrophysicsLine (formation)hydrodynamicPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Velocity dispersionPhysics - Fluid DynamicsComputational Physics (physics.comp-ph)active [galaxies]astro-ph.COspectroscopic [techniques]Astrophysics - High Energy Astrophysical PhenomenaPhysics - Computational PhysicsAstrophysics - Cosmology and Nongalactic Astrophysics[ INFO ] Computer Science [cs]Cosmology and Nongalactic Astrophysics (astro-ph.CO)astro-ph.GAgalaxies: activeFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsISM [radio lines]0103 physical sciences[ PHYS.PHYS.PHYS-GEN-PH ] Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]/dk/atira/pure/subjectarea/asjc/1900/1912[INFO]Computer Science [cs]Astrophysics::Galaxy Astrophysicsradio lines: ISM010308 nuclear & particles physicsMolecular cloudturbulenceFluid Dynamics (physics.flu-dyn)Astronomy and AstrophysicsAstronomy and AstrophysicAstrophysics - Astrophysics of GalaxiesX-rays: galaxies: clusterGalaxyAccretion (astrophysics)[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]physics.flu-dynphysics.comp-phSpace and Planetary ScienceX-rays: galaxies: clustersAstrophysics of Galaxies (astro-ph.GA)hydrodynamics/dk/atira/pure/subjectarea/asjc/3100/3103galaxies: clusters [X-rays][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]techniques: spectroscopic
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Multispectrum fits for line mixing in the ν3 band Q branch of methane

2003

International audience; First-order line-mixing coefficients and model relaxation matrix element scaling factors have been obtained for allowed transitions in the nu3 band Q branch of CH4 broadened by H2, He, N2, O2, Ar, and CH4. The broadening, shifting, Dicke-narrowing, and line-mixing parameters are determined by simultaneous least-squares fitting of spectra at pressures from 0.014 to 66.66 kPa recorded with a high-resolution difference-frequency laser. These results confirm, improve, and extend a previous analysis of the lower pressure (613.3 kPa) data [A.S. Pine, J. Chem. Phys. 97 (1992) 773] which yielded averaged coefficients of individually fit spectra where adjacent broadened lines…

[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]010504 meteorology & atmospheric sciencesSelf and foreign gas-broadened methane01 natural sciencesMethaneSpectral linelaw.inventionchemistry.chemical_compoundNuclear magnetic resonance[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]law0103 physical sciencesRelaxation matrixPhysical and Theoretical Chemistry010306 general physicsScalingSpectroscopyMixing (physics)0105 earth and related environmental sciencesLine (formation)PhysicsLine mixingLaserAtomic and Molecular Physics and OpticschemistryDicke narrowingLower pressureAtomic physicsJournal of Molecular Spectroscopy
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On the high resolution spectroscopy and intramolecular potential function of SO2

2009

Abstract Two weak stretching bands, ν 1  + 3 ν 3 and 3 ν 1  +  ν 3 , of the sulfur dioxide molecule have been recorded at high resolution and analyzed for the first time with using a Fourier transform Bruker IFS-120 HR interferometer. About 1000 transitions with J max .  = 51, K a max . = 16 , and 900 transitions with J max .  = 53, K a max . = 16 have been assigned to the bands ν 1  + 3 ν 3 and 3 ν 1  +  ν 3 , respectively. Analysis of the recorded spectra was made using the model of isolated vibrational states. Parameters obtained from the fit reproduce the initial experimental ro-vibrational energies with the rms deviation of 0.0006 and 0.0012 cm −1 for the bands, 3 ν 1  +  ν 3 and ν 1  …

[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]Analytical chemistryHigh resolution02 engineering and technology01 natural sciencesSpectral linesymbols.namesakeNuclear magnetic resonance[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]High-resolution spectra0103 physical sciencesMoleculePhysical and Theoretical ChemistrySpectroscopySpectroscopyPhysics010304 chemical physicsPotential functionFunction (mathematics)Spectroscopic parameters021001 nanoscience & nanotechnologyAtomic and Molecular Physics and OpticsInterferometryFourier transformSulfur dioxideIntramolecular forcesymbols0210 nano-technology
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Symmetry-adapted tensorial formalism to model rovibrational and rovibronic spectra of molecules pertaining to various point groups

2004

International audience; We present a short review on the tensorial formalism developed by the Dijon group to solve molecular spectroscopy problems. This approach, originally devoted to the rovibrational spectroscopy of highly symmetrical species (spherical tops) has been recently extended in several directions: quasi-spherical tops, some symmetric and asymmetric tops, and rovibronic spectroscopy of spherical tops in a degenerate electronic state. Despite its apparent complexity (heavy notations, quite complex mathematical tools), these group theoretical tensorial methods have a great advantage of flexibility: a systematic expansion of effective terms for any rovib- rational/rovibronic probl…

[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]Rovibrational spectroscopyRovibronic spectroscopySymmetrizationTensorial formalism02 engineering and technologyMolecular spectroscopyPoint group01 natural sciencesSpectral lineTheoretical physics[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]Quantum mechanics0103 physical sciencesPhysics::Atomic and Molecular ClustersMoleculeLineshapesPhysical and Theoretical ChemistrySpectroscopySpectroscopyPhysics010304 chemical physicsDegenerate energy levelsRotational–vibrational spectroscopy021001 nanoscience & nanotechnologyAtomic and Molecular Physics and OpticsFormalism (philosophy of mathematics)Group theory0210 nano-technology
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Embedded multi-spectral image processing for real-time medical application

2016

International audience; The newly introduced Kubelka-Munk Genetic Algorithm (KMGA) is a promising technique for the assessment of skin lesions from multi-spectral images. Using five skin parameter maps such as concentration or epidermis/dermis thickness, this method combines the Kubelka-Munk Light-Tissue interaction model and Genetic Algorithm optimization process to produce a quantitative measure of cutaneous tissue. Up to the present, variant improved KMGA implementations have been successfully realized using the recent parallel computing techniques. However, all these achievements are based on the multi-core CPUs. This results in a quite high cost and low practicability for the hardware …

[INFO.INFO-AR]Computer Science [cs]/Hardware Architecture [cs.AR]Digital signal processorSource code[ INFO ] Computer Science [cs]Computer sciencemedia_common.quotation_subject[INFO.INFO-DS]Computer Science [cs]/Data Structures and Algorithms [cs.DS]Image processing02 engineering and technologyARCHITECTURESLight-Tissue InteractionGenetic algorithm0202 electrical engineering electronic engineering information engineering[INFO]Computer Science [cs]Embedded SystemField-programmable gate arrayFPGA[ INFO.INFO-DS ] Computer Science [cs]/Data Structures and Algorithms [cs.DS]media_commonFlexibility (engineering)Multi-spectral image processingGenetic AlgorithmHigh-Level Synthesis FPGA IMPLEMENTATIONbusiness.industryProcess (computing)020206 networking & telecommunicationsTransplantationMODELComputer engineeringHardware and ArchitectureEmbedded system020201 artificial intelligence & image processing[ INFO.INFO-AR ] Computer Science [cs]/Hardware Architecture [cs.AR]businessHigh-Level SynthesisSoftware
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Dispositifs d’imagerie multi-spectrale pour la détection et le contrôle des adventices

2007

National audience; pas de résumé

[INFO.INFO-TS]Computer Science [cs]/Signal and Image Processing[INFO.INFO-TS] Computer Science [cs]/Signal and Image ProcessingImagerie multi-spectraleAdventices
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Multispectral imaging for computer vision

2018

[INFO.INFO-TS]Computer Science [cs]/Signal and Image Processing[INFO.INFO-TS] Computer Science [cs]/Signal and Image ProcessingMultispectral ImagingImagerie multispectrale
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γ-RAY AND PARSEC-SCALE JET PROPERTIES OF A COMPLETE SAMPLE OF BLAZARS FROM THE MOJAVE PROGRAM

2011

著者人数: 145名

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical Phenomenagalaxies: activePopulationFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesRadio spectrumLuminosityRelativistic beamingquasars: generalgamma rays: galaxiesgalaxies0103 physical sciencesgalaxie [gamma rays]educationBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)radio continuum: galaxiesPhysicseducation.field_of_studygeneral [quasars]general [BL Lacertae objects]010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astronomy and AstrophysicsQuasarBL Lacertae objects: generalgalaxies: jetsgalaxies [radio continuum]BL Lacertae objects: general; galaxies: active; galaxies: jets; gamma rays: galaxies; quasars: general; galaxies quasars: generaljet [galaxies]BL Lacertae objects: general; galaxies: active; galaxies: jets; gamma rays: galaxies; quasars: general; radio continuum: galaxiesSpace and Planetary Scienceactive [galaxies]Spectral energy distributionAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsFermi Gamma-ray Space TelescopeThe Astrophysical Journal
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