THE TORSIONAL SPECTRUM OF $CH_{3}CO_{3}$ AND $C_{2}O_{6}$

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1989

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Ohio State University

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We have recorded the far-infrared spectrum of CH3CO3 and C2O6 in the regions of the forbidden torsional fundamentals under relatively large pressure-pathlength conditions. The observations were made using a modified Bomem spectrometer, with an absorption path of 20 m, a temperature of 230 K, pressures of 50-80 torr, and a resolution of 0.01cm−1. The most prominent features of the spectra are the unresolved Q-branches of the various torsional components of the ν4−1−0 band of C2O6 with an origin at about 208.5cm−1, and of the ν6=1−0 band of CH3CO3 with an origin at about 252.70cm−1. To lower frequencies there are the partially-resolved Q-branches of the ν−2−1 hot bands at about 193.0cm−1 for C2O6 and 227.9cm−1 for CH3CO3. The P- and R-branches of the fundamental consist of peaks about 0.2cm−1 wide due to unresolved clusters. These peaks can be followed up to J=30 in both branches. We have also recorded both low (230 K) and room temperature spectra of the lowest lying allowed fundamental bands around 594cm−1(C2O6) and 679cm−1(CH3CO3) with a resolution of 0.0013cm−1. Over 1000 transitions have been identified in the PP−,RR−,PR, and RP-branches for each molecule. In addition, the millimeter wave spectrum of CH3CO3 has been recorded at around 240-360 GHz in the v6−0 and 1 torsional states for several R-branch transitions. K-splitting has been observed for both states, but not σ-splitting. We will present results for the ground vibrational state of both isotopes based on the analysis of the torsional fundamental together with combination differences obtained from the lowest lying allowed fundamentals and their corresponding hot bands.

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Author Institution: Herzberg Institute of Astrophysics, National Research Council of Canada; Department of Physics, University of British Columbia

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