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Measurements and theoretical calculations of self-broadening and self-shift coefficients in the ν2 band of CH3D
Authors:Adriana Predoi-Cross  Kyle Hambrook  Jean-Pierre Bouanich  D. Chris Benner
Affiliation:a Physics Department, University of Lethbridge, 4401 University Drive, Lethbridge, Alta., Canada T1K 3M4
b Laboratoire de Photophysique Moléculaire, CNRS UPR3361,Université de Paris-Sud, Bâtiment 350, F-91405 Orsay, France
c Department of Physics, The College of William and Mary, Box 8795, Williamsburg, VA 23187-8795, USA
d Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91109-8099, USA
Abstract:In this paper, we report measured Lorentz self-broadening and self-induced pressure-shift coefficients of 12CH3D in the ν2 fundamental band (ν0 ≈ 2200 cm−1). The multispectrum fitting technique allowed us to analyze simultaneously seven self-broadened absorption spectra. All spectra were recorded at the McMath-Pierce Fourier transform spectrometer of the National Solar Observatory (NSO) on Kitt Peak, AZ with an unapodized resolution of 0.0056 cm−1. Low-pressure (0.98-2.95 Torr) as well as high-pressure (17.5-303 Torr) spectra of 12C-enriched CH3D were recorded at room temperature to determine the pressure-broadening coefficients of 408 ν2 transitions with quantum numbers as high as J″ = 21 and K = 18, where K″ = K′ ≡ K (for a parallel band). The measured self-broadening coefficients range from 0.0349 to 0.0896 cm−1 atm−1 at 296 K. All the measured pressure-shifts are negative. The reported pressure-induced self-shift coefficients vary from about −0.004 to −0.008 cm−1 atm−1. We have examined the dependence of the measured broadening and shift parameters on the J″, and K quantum numbers and also developed empirical expressions to describe the broadening coefficients in terms of m (m = −J″, J″, and J″ + 1 in the QP-, QQ-, and QR-branch, respectively) and K. On average, the empirical expressions reproduce the measured broadening coefficients to within 3.6%. A semiclassical theory based upon the Robert-Bonamy formalism of interacting linear molecules has been used to calculate these self-broadening and self-induced pressure-shift coefficients. In addition to the electrostatic interactions involving the octopole and hexadecapole moments of CH3D, the intermolecular potential includes also an atom-atom Lennard-Jones model. For low K (K ? 3) with |m| ? 8 the theoretical results of the broadening coefficients are in overall good agreement (3.0%) with the experimental data. For transitions with K approaching |m|, they are generally significantly underestimated (8.8%). The theoretical self-induced pressure shifts, whose vibrational contribution is derived from results in the QQ-branch, are generally smaller in magnitude than the experimental data in the QP-, and QR-branches (15.2%).
Keywords:Monodeuterated methane   CH3D   Self-broadening   Fourier transform infrared spectroscopy   Spectral lineshape
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