Search results for "Line broadening coefficients"

showing 3 items of 3 documents

Line broadening coefficient calculations for methane perturbed by nitrogen

2010

Abstract We report semiclassical line broadening calculations for methane perturbed by nitrogen at room temperature. For this, we have developed a symmetrized version of the Robert and Bonamy theory. The interaction potential was built from electrostatic (octopole and hexadecapole for methane, quadrupole for nitrogen) and atom–atom contributions. The relative (classical) trajectories of the molecules were computed in the frame of the usual parabolic model, through analytical formula. High orders of developments had to be used for the short range molecular interactions. As a consequence, a combination of symbolic computation and source code generation was employed to implement practical calc…

Line broadening coefficients010504 meteorology & atmospheric sciencesAbsorption spectroscopyNitrogenSemiclassical physics7. Clean energy01 natural sciencesSpectral lineMethanechemistry.chemical_compound0103 physical sciences[ PHYS.PHYS.PHYS-GEN-PH ] Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Perturbation theoryPhysics::Chemical PhysicsSpectroscopy010303 astronomy & astrophysicsInfrared spectroscopySpectroscopy0105 earth and related environmental sciencesLine (formation)PhysicsRadiationAtomic and Molecular Physics and Optics[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]chemistryQuadrupoleAtomic physicsMethane
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Calculated line broadening parameters for methane perturbed by diatomic molecules

2013

International audience; We report semiclassical line broadening calculations for methane perturbed by diatomic molecules: nitrogen, N2, oxygen, O2 and hydrogen, H2, at room temperature. For this, we have developed a symmetrized version of the Robert and Bonamy theory. The interaction potential was built from electrostatic (octopole and hexadecapole for methane, quadrupole for the diatomic molecules) and atom-atom contributions. The relative (classical) trajectories of the molecules were computed in the frame of the usual parabolic model, through analytical formula. High orders of developments had to be used for the short range molecular interactions in the case of N2 and O2. For H2, a lower…

Line broadening coefficients010504 meteorology & atmospheric sciencesHydrogen[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]Nitrogenchemistry.chemical_elementInfrared spectroscopySemiclassical physics02 engineering and technology7. Clean energy01 natural sciencesMethanechemistry.chemical_compound[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]Diatomic moleculesMoleculePhysical and Theoretical ChemistryInfrared spectroscopySpectroscopy0105 earth and related environmental sciencesLine (formation)Physics021001 nanoscience & nanotechnologyDiatomic moleculeAtomic and Molecular Physics and OpticsOxygenchemistryQuadrupoleAtomic physics0210 nano-technologyMethaneHydrogen
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Calculated Line Broadening Coefficients in the nu2 Band of CH3D Perturbed by Helium

2003

International audience; Line broadening coefficients have been calculated, at room temperature, for lines in the P and R branches of the nu2 band of monodeuterated methane. A properly symmetrized semiclassical model with parabolic relative trajectories has been used. Two interaction potential models have been considered. The first is a Lennard-Jones type atom-atom potential, while the second one was derived from ab initio calculations. The calculated line widths were compared to the available experimental data and a satisfactory agreement was found, although the model contains no other adjustable parameters than the four atomic Lennard-Jones ones. Nonetheless, failures of calculations have …

PhysicsLine broadening coefficients010304 chemical physicsCondensed matter physics[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]Semiclassical physicschemistry.chemical_elementQuantum numberSemiclassical calculations01 natural sciences7. Clean energyAtomic and Molecular Physics and OpticsCH3DInteraction potentialchemistry[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]Ab initio quantum chemistry methods0103 physical sciencesPhysics::Atomic and Molecular ClustersPhysical and Theoretical ChemistryAtomic physics010303 astronomy & astrophysicsSpectroscopyHeliumLine (formation)
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