Abstract
IR-UV double resonance spectroscopy has been used to characterize hindered internal rotor states (nK = 00, 11, and 10) of the CN-Ne complex in its ground electronic state with various degrees of CN stretch (νCN) excitation. Rotationally resolved infrared overtone spectra of the CN-Ne complex exhibit perturbations arising from Coriolis coupling between the closely spaced hindered rotor states (11 and 10) with two quanta of CN stretch (νCN = 2). A deperturbation analysis is used to obtain accurate rotational constants and associated average CN center-of-mass to Ne separation distances as well as the coupling strength. The energetic ordering and spacings of the hindered internal rotor states provide a direct reflection of the weakly anisotropic intermolecular potential between CN X 2Σ+ and Ne, with only an 8 cm-1 barrier to CN internal rotation, from which radially averaged anisotropy parameters (V10 and V20) are extracted that are consistent for νCN = 0-3. Complementary ab initio calculation of the CN X 2Σ+ + Ne potential using MRCI+Q extrapolated to the complete one-electron basis set limit is compared with the experimentally derived anisotropy by optimizing the radial potential at each angle. Experiment and theory are in excellent accord, both indicating a bent minimum energy configuration and nearly free rotor behavior. Analogous experimental and theoretical studies of the CN-Ne complex upon electronic excitation to the CN B 2Σ+ state indicate a slightly more anisotropic potential with a linear CN-Ne minimum energy configuration. The results from these IR-UV double resonance studies are compared with prior electronic spectroscopy and theoretical studies of the CN-Ne system.
| Original language | English |
|---|---|
| Article number | 184308 |
| Journal | Journal of Chemical Physics |
| Volume | 134 |
| Issue number | 18 |
| DOIs | |
| Publication status | Published - 14 May 2011 |
Bibliographical note
Publisher Copyright:© 2011 American Institute of Physics.
ASJC Scopus subject areas
- General Physics and Astronomy
- Physical and Theoretical Chemistry
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