6533b835fe1ef96bd129f6b4

RESEARCH PRODUCT

Helium and Argon Line Broadening in the nu2 Band of CH4

N. M. GrigorovichM. V. TonkovI. M. GrigorievTony Gabard

subject

Materials science010504 meteorology & atmospheric sciences[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]Physics::Instrumentation and Detectorschemistry.chemical_element01 natural sciencesMethaneSpectral linechemistry.chemical_compound[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]0103 physical sciencesPhysics::Atomic and Molecular ClustersPhysical and Theoretical ChemistryPhysics::Chemical PhysicsLine broadeningSpectroscopyHelium0105 earth and related environmental sciencesLine (formation)Argon010304 chemical physicsResolution (electron density)Tetrahedral molecular geometryAtomic and Molecular Physics and OpticschemistryVibration-rotation linesAstrophysics::Earth and Planetary AstrophysicsAtomic physicsMethane

description

Abstract The spectra of the gaseous mixtures CH 4 –He and CH 4 –Ar were obtained in the spectral region 1400–1750 cm −1 with a resolution up to 0.003 cm −1 . Helium and argon pressure broadenings for the vibration–rotation lines of the ν 2 band of CH 4 have been estimated at room temperature for some lines in the P , Q , and R branches. These values were also calculated using the theoretical approach developed by Robert and Bonamy, extended to the case of tetrahedral molecules. The helium data have been found to be in a satisfactory agreement whereas a divergence of calculated and measured broadening coefficients has been evidenced in the case of argon. Simulations of the ν 2 band shapes of methane perturbed by helium have also been performed.

https://hal.archives-ouvertes.fr/hal-01053565