Search results for "Thermodynamic equilibrium"

showing 10 items of 80 documents

D2/H2 adsorption selectivity on FAU zeolites at 77.4 K: Influence of Si/Al ratio and cationic composition

2018

Abstract Equilibrium D2/H2 adsorption selectivity was determined at 77.4 K below 1000 hPa for a series of FAU type zeolites X exchanged with different cations (Li+, Na+, K+, Mg2+, Ca2+, Ba2+ and Mn2+). In addition NaY, DAY (dealuminated Y) and pure silica CHA and MFI zeolites were studied. Two experimental approaches were used to determine the D2/H2 adsorption selectivity: direct determination at the thermodynamic equilibrium from manometric coadsorption experiments and calculations by Ideal Adsorbed Solution Theory (IAST) from single gas adsorption isotherms. While these two approaches are not in quantitative agreement, they reveal similar trends. At low loading (  MnX > LiX > CaX ≈ NaX > …

LangmuirThermodynamic equilibriumChemistryCationic polymerizationHigh loading02 engineering and technologyGeneral Chemistry010402 general chemistry021001 nanoscience & nanotechnologyCondensed Matter Physics01 natural sciences7. Clean energy0104 chemical sciencesAdsorption selectivity[CHIM.THEO]Chemical Sciences/Theoretical and/or physical chemistryAdsorption13. Climate actionMechanics of MaterialsPhysical chemistry[CHIM]Chemical SciencesGeneral Materials ScienceComposition (visual arts)0210 nano-technologySelectivityComputingMilieux_MISCELLANEOUS
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Experimental signature of optical wave thermalization through supercontinuum generation in photonic crystal fiber

2009

International audience; We report an experimental, numerical and theoretical study of the incoherent regime of supercontinuum generation in a two zero dispersion wavelengths fiber. By using a simple experimental setup, we show that the phenomenon of spectral broadening inherent to supercontinuum generation can be described as a thermalization process, which is characterized by an irreversible evolution of the optical field towards a thermal equilibrium state. In particular, the thermodynamic equilibrium spectrum predicted by the kinetic wave theory is characterized by a double peak structure, which has been found in quantitative agreement with the numerical simulations without adjustable pa…

LightThermodynamic equilibriumOptical fieldSpectrum Analysis Raman01 natural sciences010309 opticssymbols.namesakeOptics0103 physical sciencesFiber Optic TechnologyScattering RadiationComputer Simulation010306 general physicsPhysics[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]Photons[ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]business.industryTemperatureNonlinear opticsModels TheoreticalAtomic and Molecular Physics and OpticsSupercontinuumWavelengthsymbolsbusinessRaman scatteringDoppler broadeningPhotonic-crystal fiber
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The Hamburg/ESO R-process Enhanced Star survey (HERES):XI. The highly r-process-enhanced star CS 29497-004

2017

We report an abundance analysis for the highly r-process-enhanced (r-II) star CS 29497-004, a very metal-poor giant with Teff = 5013K and [Fe/H]=-2.85, whose nature was initially discovered in the course of the HERES project. Our analysis is based on high signal-to-noise, high-resolution (R~75000) VLT/UVES spectra and MARCS model atmospheres under the assumption of local thermodynamic equilibrium, and obtains abundance measurements for a total of 46 elements, 31 of which are neutron-capture elements. As is the case for the other 25 r-II stars currently known, the heavy-element abundance pattern of CS 29497-004 well-matches a scaled Solar System second peak r-process-element abundance patter…

MODEL ATMOSPHERESSolar SystemPopulation II [stars]Thermodynamic equilibriumMETAL-POOR STARSFOS: Physical sciencesAstrophysicsStar (graph theory)01 natural sciences7. Clean energySpectral lineGalactic halochemically peculiar [stars]CORE-COLLAPSE SUPERNOVAELABORATORY TRANSITION-PROBABILITIES0103 physical sciencesEXPERIMENTAL OSCILLATOR-STRENGTHShalo [Galaxy]NeutronEARLY GALAXY010306 general physics010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSSolar and Stellar Astrophysics (astro-ph.SR)PhysicsPROCESS-RICHGALACTIC CHEMICAL EVOLUTIONAstronomy and Astrophysicsindividual: CS 29497-004 [stars][PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Astrophysics - Astrophysics of Galaxiesabundances [stars]StarsHIGH-ENTROPY-WIND[PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Astrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)r-processNEUTRON-CAPTURE
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On the structural aspects of solid solutions of enantiomers: an intriguing case study of enantiomer recognition in the solid state

2018

Structural aspects of solid solutions of enantiomers have been considered and the corresponding definitions of type 1 and type 2 solid solutions have been revised based on the available structures reported in the literature. Examples of both types are presented indicating that (e.g., type 1 solid solutions) there is a straightforward relationship between the particular structural aspects and the enantiomer miscibility limits in the solid state. Furthermore, enantiomer recognition in a type 2 solid solution formed by the enantiomers of a pharmaceutically active ingredient, pimobendan, has been studied in more detail. It was found that upon rapid crystallization from a solution a structure po…

Materials science010405 organic chemistryThermodynamic equilibriumCrystal growthGeneral Chemistry010402 general chemistryCondensed Matter Physics01 natural sciencesMiscibility0104 chemical scienceslaw.inventionlawComputational chemistryPhase (matter)General Materials ScienceEnantiomerCrystallizationSingle crystalSolid solutionCrystEngComm
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Experimental and theoretical studies of Stark profiles of Ar I 696.5 nm spectral line in laser-induced plasma

2019

Abstract We report the results of the Stark profile studies of the 696.543 nm Ar I spectral line in laser-induced plasma generated by a nanosecond Nd:YAG laser radiation at 532 nm in argon at reduced pressure. Plasma diagnostics was performed with the use of the laser Thomson scattering method, free from assumptions about the plasma thermodynamic equilibrium, its composition but also independently of plasma emission spectra. The profiles were investigated in wide range of electron densities and temperatures, from 2.81 · 1022 m − 3 to 5.69 · 1023 m − 3 and from 10 430 K to 73 400 K, respectively. Stark profiles were calculated using a semi-classical method as well as by N-body numerical simu…

Materials science010504 meteorology & atmospheric sciencesStark broadeningThomson scatteringThermodynamic equilibrium01 natural sciencesSpectral linesymbols.namesake[PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]Physics::Plasma Physicscomputer simulationsLaser-induced plasmaEmission spectrumThomson scatteringComputingMilieux_MISCELLANEOUSSpectroscopy0105 earth and related environmental sciencesRadiationPlasmaAtomic and Molecular Physics and OpticsStark effectlaser-induced plasmasymbolsElectron temperaturePlasma diagnosticsAtomic physicsComputer simulationsJournal of Quantitative Spectroscopy and Radiative Transfer
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Helium gas pressure cell for pressures up to 1 kbar (0.1 GPa) in conjunction with the cold head of a closed-cycle He refrigerator

1997

A helium gas pressure cell for pressures up to 1 kbar (0.1 GPa) has been developed in conjunction with a closed-cycle He refrigerator allowing variable temperatures between 15 and 300 K. Both cell and refrigerator are equipped with optical windows suitable for photophysical measurements, such as temperature- and pressure-dependent absorption spectroscopy or laser flash photolysis. Examples of measurements on iron(II) spin-crossover systems are given. In these compounds, comparatively small external pressures induce significant changes in the thermodynamic equilibrium as well as in the relaxation dynamics.

Materials scienceAbsorption spectroscopyThermodynamic equilibriumApplied MathematicsConjunction (astronomy)Refrigerator carThermodynamicsLaserlaw.inventionlawddc:540Head (vessel)Relaxation (physics)Flash photolysisInstrumentationEngineering (miscellaneous)
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Phase separation of binary mixtures in thin films: Effects of an initial concentration gradient across the film.

2012

We study the kinetics of phase separation of a binary (A,B) mixture confined in a thin film of thickness $D$ by numerical simulations of the corresponding Cahn-Hilliard-Cook (CHC) model. The initial state consisted of 50$%$ A:50$%$ B with a concentration gradient across the film, i.e., the average order parameter profile is ${\ensuremath{\Psi}}_{\mathrm{av}}(z,t=0)=(2z/D\ensuremath{-}1){\ensuremath{\Psi}}_{g},\phantom{\rule{0.28em}{0ex}}0\ensuremath{\leqslant}z\ensuremath{\leqslant}D$, for various choices of ${\ensuremath{\Psi}}_{g}$ and $D$. The equilibrium state (for time $t\ensuremath{\rightarrow}\ensuremath{\infty}$) consists of coexisting A-rich and B-rich domains separated by interfac…

Materials scienceCondensed matter physicsSpinodal decompositionThermodynamic equilibriumOrder (ring theory)Membranes ArtificialState (functional analysis)Complex MixturesPhase TransitionModels ChemicalMetastabilityDomain (ring theory)PerpendicularComputer SimulationColloidsThin filmPhysical review. E, Statistical, nonlinear, and soft matter physics
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Humidity effects on gravitational settling and Brownian diffusion of atmospheric aerosol particles

1977

The dependency on relative humidity of the settling velocity of aerosol particles in stagnant air and of the diffusion coefficient due to Brownian motion of aerosol particles was computed for six aerosol types and different particles sizes in dry state. The computations are based (1) on mean bulk densities of dry aerosol particles obtained from measurements or from the knowledge of the chemical composition of the particles, (2) on micro-balance measurements of the water uptake per unit mass of dry aerosol substance versus water activity at thermodynamic equilibrium, and (3) on measurements of the equilibrium water activity of aqueous sea salt solutions. The results show a significant depend…

Materials scienceThermodynamic equilibriumDiffusionThermodynamicsHumidityrespiratory systemAtmospheric sciencescomplex mixturesAerosolGeophysicsDeposition (aerosol physics)SettlingGeochemistry and PetrologyParticleRelative humidityPhysics::Atmospheric and Oceanic PhysicsPure and Applied Geophysics PAGEOPH
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High-temperature emission spectroscopy of methane

2008

International audience; A high-enthalpy source (HES) has been developed in Rennes either to heat gases up to 2000K in local thermodynamic equilibrium (LTE) or to generate hypersonic expansions. The HES prototype has been associated with a high-resolution Bruker IFS 120 HR Fourier transform spectrometer to record emission spectra of hot gases, in LTE conditions. A series of emission spectra of methane has been obtained at 1005, 1365, 1485, 1625 and 1820K in the pentad spectral region located around 3000 cm1, at Doppler-limited resolution (0.02 cm1). Spectra have been corrected for the transmission function that strongly affects the infrared radiation emitted by the hot gas. Line-integrated a…

Materials scienceThermodynamic equilibriumInfraredInfrared spectroscopy02 engineering and technology7. Clean energy01 natural sciencesSpectral line0103 physical sciencesEmission spectrumAbsorption (electromagnetic radiation)010303 astronomy & astrophysics[ SDU.ASTR ] Sciences of the Universe [physics]/Astrophysics [astro-ph]Spectroscopy[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Radiation[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]AnharmonicityRotational–vibrational spectroscopyCRESU021001 nanoscience & nanotechnologyAtomic and Molecular Physics and Optics[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Atomic physics0210 nano-technologyMolecular physics
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Entrapment of charged, nonwetting colloids near oil-water interfaces.

2007

Charged, nonwetting colloids with a contact angle $\ensuremath{\theta}=180\ifmmode^\circ\else\textdegree\fi{}$ are attracted to an oil-water interface due to image charge forces. Near the interface, the attractive image charge forces are balanced by repulsive van der Waals forces, and thus the colloids are trapped at a finite distance from the interface. Electrostatic and van der Waals pressure lead to a deformation of the interface in the equilibrium state. For parameters relevant to experiment, however, the effects of the deformed interface are negligible and thus the mutual interactions of such interfacially trapped colloids should be well characterized by electrostatic dipole repulsions.

Materials scienceThermodynamic equilibriumVan der Waals strainMethod of image chargesCondensed Matter::Soft Condensed MatterContact anglesymbols.namesakeDipoleColloidChemical physicssymbolsVan der Waals radiusvan der Waals forceAtomic physicsPhysical review. E, Statistical, nonlinear, and soft matter physics
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