Search results for "Names"

showing 10 items of 6843 documents

Polarization angle dependence of the breathing modes in confined one-dimensional dipolar bosons

2021

Probing the radial collective oscillation of a trapped quantum system is an accurate experimental tool to investigate interactions and dimensionality effects. We consider a fully polarized quasi-one dimensional dipolar quantum gas of bosonic dysprosium atoms in a parabolic trap at zero temperature. We model the dipolar gas with an effective quasi-one dimensional Hamiltonian in the single-mode approximation, and derive the equation of state using a variational approximation based on the Lieb-Liniger gas Bethe Ansatz wavefunction or perturbation theory. We calculate the breathing mode frequencies while varying polarization angles by a sum-rule approach, and find them in good agreement with re…

[PHYS.COND.GAS]Physics [physics]/Condensed Matter [cond-mat]/Quantum Gases [cond-mat.quant-gas]FOS: Physical sciences02 engineering and technology01 natural sciencescollective modesBethe ansatzSupersolidsymbols.namesakedipolar gas supersoliddipolar gas0103 physical sciencesQuantum systemtrapped atoms010306 general physicsWave functionUltracold atoms - Dipolar atoms - Luttinger liquidsBosonPhysicsCondensed Matter::Quantum Gasesdipolar interactionsBrewster's angle021001 nanoscience & nanotechnologyPolarization (waves)3. Good healthsupersolidQuantum Gases (cond-mat.quant-gas)Quantum electrodynamicssymbols0210 nano-technologyHamiltonian (quantum mechanics)Condensed Matter - Quantum Gases
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Titan's 3-micron spectral region from ISO high-resolution spectroscopy

2006

Abstract The near-infrared spectrum of Titan, Saturn's largest moon and one of the Cassini/Huygens' space mission primary targets, covers the 0.8 to 5 micron region in which it shows several weak CH 4 absorption regions, and in particular one centered near 2.75 micron. Due to the interference of telluric absorption, only part of this window region (2.9–3.1 μm) has previously been observed from the ground [Noll, K.S., Geballe, T.R., Knacke, R., Pendleton, F., Yvonne, J., 1996. Icarus 124, 625–631; Griffith, C.A., Owen, T., Miller, G.A., Geballe, T., 1998. Nature 395, 575–578; Griffith, C.A., Owen, T., Geballe, T.R., Rayner, J., Rannou, P., 2003. Science 300, 628–630; Geballe, T.R., Kim, S.J.…

[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]PhysicsSolar SystemHaze010304 chemical physicsInfraredSingle-scattering albedoAstronomyAstronomy and AstrophysicsTholin01 natural sciences7. Clean energysymbols.namesake[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]13. Climate actionSpace and Planetary SciencePlanet0103 physical sciencessymbolsMixing ratioTitan (rocket family)010303 astronomy & astrophysicsIcarus
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Titan's surface and atmosphere from Cassini/VIMS data with updated methane opacity

2013

International audience; We present an analysis of Titan data acquired by the Cassini Visual and Infrared Mapping Spectrometer (VIMS), making use of recent improvements in methane spectroscopic parameters in the region 1.3-5.2 μm. We first analyzed VIMS spectra covering a 8 × 10-km2 area near the Huygens landing site in order to constrain the single scattering albedo (ω0) of the aerosols over all of the VIMS spectral range. Our aerosol model agrees with that derived from Huygens Probe Descent Imager/Spectral Radiometer (DISR) in situ measurements below 1.6 μm. At longer wavelengths, ω0 steadily decreases from 0.92 at 1.6 μm to about 0.70 at 2.5 μm and abruptly drops to about 0.50 near 2.6 μm…

[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph][PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]Haze010504 meteorology & atmospheric sciencesOpacity[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Single-scattering albedoAstronomy and AstrophysicsTholinAstrophysicsAtmospheric sciences01 natural sciencesSpectral lineAerosolsymbols.namesake13. Climate actionSpace and Planetary Science0103 physical sciencessymbolsAtmosphere of TitanTitan (rocket family)010303 astronomy & astrophysicsGeology0105 earth and related environmental sciences
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Inhomogeneous speed effects on H-2 vibrational line profiles in ternary mixtures

2000

International audience; A study of speed inhomogeneous broadening of the hydrogen vibrational line profiles in the collisional regime for ternary mixtures is reported. The Q(1) line of H-2 in H-2-Ar-N-2, H-2-He-Ar, and H-2-He-N-2 mixtures is investigated by high resolution stimulated Raman spectroscopy for various concentrations and temperatures. A model, successfully used for binary mixtures, is extended to ternary mixtures. An excellent agreement is obtained between theory and experiment for H-2-Ar-N-2, by using the collisional parameters previously obtained from binary mixtures study. For H-2-He-Ar and H-2-He-N-2, H-2-He collisions play a "hardening" effect in the H-2 soft speed memory m…

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]010504 meteorology & atmospheric sciencesHydrogenHEAnalytical chemistryGeneral Physics and Astronomychemistry.chemical_element01 natural sciencesMolecular physicsPARAMETERSsymbols.namesakeDEPENDENCE0103 physical sciencesCOLLISION REGIMECoherent anti-Stokes Raman spectroscopyPhysical and Theoretical Chemistry010306 general physicsSpectroscopy0105 earth and related environmental sciences[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]ChemistryN-2Spectral line shapeDOPPLERXEsymbolsHardening (metallurgy)SHAPERaman spectroscopyTernary operationRaman scattering
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Speed-dependent line profile: A test of a unified model from the Doppler to the collisional regime for molecule-molecule collisions

2000

International audience; A speed-dependent line profile combining soft and hard fully correlated Dicke-narrowing collisions was recently successfully tested on Ar-broadened H-2 spectra in a wide density and temperature range. A further test for mixtures of H-2 in nitrogen molecules (instead of Ar atoms) is presented. This test is also based on high resolution Raman investigation of the isotropic Q(1) line of H-2 from low to high density at various temperatures. The same consistency of the speed-dependent line profile as for H-2-Ar is obtained for H-2-N-2 through a remarkable agreement with all the data by using a unique set of four parameters (the collisional width and shift, the kinetic fre…

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]Analytical chemistryGeneral Physics and AstronomyKinetic energy01 natural sciencesSpectral linePARAMETERSsymbols.namesakeASYMMETRIES0103 physical sciencesSHIFTPhysical and Theoretical Chemistry010306 general physicsLine (formation)[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]010304 chemical physicsChemistryIsotropyCHANGING COLLISIONSCharacteristic velocityN-2BROADENED HFXELINESHAPEsymbolsSHAPEAtomic physicsDoppler effectRaman scatteringDoppler broadeningAR
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Suppression of plasma contribution in femtosecond degenerate four-wave mixing (fs-DFWM) at high intensity

2007

Femtosecond degenerate four-wave mixing (fs-DFWM) experiments in CO2 exhibit a strong background due to plasma produced at high intensity (≥20 TW/cm2), when significant molecular alignment is likely to arise. This perturbing phenomenon renders the measurements of alignment very difficult. It is shown that the plasma contribution can be avoided by employing perpendicular polarizations for the two pump pulses. The effect is explained on the basis of the different diffraction angles between signals produced by molecular alignment and plasma. Copyright © 2007 John Wiley & Sons, Ltd.

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]Diffraction02 engineering and technology01 natural sciencesMolecular physicssymbols.namesakeOpticsIonization0103 physical sciencesGeneral Materials Science010306 general physicsSpectroscopyMixing (physics)[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]business.industryChemistryDegenerate energy levelsPlasma021001 nanoscience & nanotechnologyFemtosecondsymbols0210 nano-technologybusinessRaman spectroscopyFemtochemistryJournal of Raman Spectroscopy
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Theoretical principles of near-field optical microscopies and spectroscopies

2000

International audience; This paper deals with the principles of detection of optical signals near a surface in a manner permitting the mapping of the distribution of the fields close to various kinds of illuminated samples. We begin with a discussion of the main physical properties of the optical fields near a surface in the absence of any probe tip. This mainly concerns phenomena involving evanescent waves for which the local decay lengths are governed not only by the sizes but also by the intrinsic properties of the surface structures. The interpretation of the detection process is reviewed on the basis of a discussion about the possibility of establishing direct comparisons between exper…

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]ELECTRODYNAMICSEvanescent wavePOLARIZATIONGeneral Physics and AstronomyNear and far field02 engineering and technology01 natural scienceslaw.inventionSCANNING TUNNELING MICROSCOPESINGLE MOLECULESsymbols.namesakeOpticslaw0103 physical sciencesSCATTERINGPhysical and Theoretical ChemistryFLUORESCENCE010306 general physicsPhysics[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]SURFACE-STRUCTURESLocal density of statesLIGHT CONFINEMENT[ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]SELF-CONSISTENTbusiness.industryScattering021001 nanoscience & nanotechnologyPolarization (waves)Maxwell's equationsRESOLUTIONsymbolsNear-field scanning optical microscopeScanning tunneling microscope0210 nano-technologybusiness
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All-fibered high-quality low duty-cycle 160-GHz femtosecond pulse source

2008

International audience; In this paper, we report the experimental demonstration of an all-optical fiber-based 160-GHz femtosecond pulse source exhibiting a duty cycle as low as 1/17. The 380-fs wellseparated Gaussian pulses are generated thanks to the strong temporal compression of an initial beat-signal propagating into three distinct segments of optical fiber. Experimental results are supported by numerical simulations based on the generalized nonlinear Schrödinger equation. (© 2008 by Astro Ltd., Published exclusively by WILEY-VCH Verlag GmbH & Co. KGaA)

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]Femtosecond pulse shapingOptical fiberPhysics and Astronomy (miscellaneous)GaussianFemtosecond02 engineering and technology01 natural scienceslaw.invention010309 opticssymbols.namesake020210 optoelectronics & photonicsQuality (physics)Opticslaw0103 physical sciences0202 electrical engineering electronic engineering information engineeringInstrumentationNonlinear Schrödinger equationComputingMilieux_MISCELLANEOUSPhysics[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]business.industryLow duty cyclePulse compressionDuty cyclePulse compressionFemtosecondsymbolsNonlinear optics in fibersOptoelectronicsbusiness
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Real time measurement of long parabolic optical similaritons

2008

International audience; Long optical similaritons using a Raman fibre amplifier are generated. These pulses, with a highly parabolic profile, are monitored in real time on a high speed oscilloscope. Tunability of both the temporal and spectral widths of the pulses is then investigated.

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]Materials science02 engineering and technologyRaman amplifier01 natural sciencesOptical fibre amplifiers010309 opticssymbols.namesake020210 optoelectronics & photonicsOptics0103 physical sciencesSpectral width0202 electrical engineering electronic engineering information engineeringElectrical and Electronic EngineeringOscilloscopeLaser beamsOptical amplifierOptical similaritons[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]business.industryPulse measurementFibre amplifiersymbolsRaman spectroscopybusinessOptical amplifier
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Parabolic pulse generation through passive reshaping of gaussian pulses in a normally dispersive fiber

2007

We numerically and experimentally demonstrate that a Gaussian pulse can be reshaped into a pulse with a stable parabolic intensity profile during propagation in normally dispersive nonlinear fibers.

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]Materials scienceGaussianPhysics::Optics02 engineering and technology01 natural sciences010309 opticssymbols.namesake020210 optoelectronics & photonicsOpticsFiber Bragg grating0103 physical sciences0202 electrical engineering electronic engineering information engineeringFiberGaussian processComputer Science::DatabasesComputingMilieux_MISCELLANEOUS[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]Pulse (signal processing)business.industrySecond-harmonic generationNonlinear opticsPulse shapingsymbolsbusiness
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