INFRARED STUDIES OF THE $\nu_{3}$ BAND OF $CH_{2}^{+}$

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1994

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Ohio State University

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The spectrum of the CH2 ion is difficult to analyze because of the existence of the Renner-Teller effect and a low barrier to linearity. In our previous study1 of the ν3 band of CH2+, we could assign only 18 lines in the Ka=0 series of the α-type parallel transition because of the irregularity of other series and because of the complexity of the overall spectrum due to other carbocations in the plasma. In order to maximize CH2 signals as opposed to those of CH3+, we chose a plasma similar to the one in our initial scan but without H2 since. [ CH_{4} + He^{*} \stackrel{70%}{\rightarrow} CH_{2}^{+} \stackrel{H_{3}}{\rightarrow} CH_{3}^{-}. ] We found that a mixture of CH4/He=90mT/7 Torr in a liquid-N2 cooled positive column clearly distinguishes the object of our quest. An extensive scan around the band origin of ν3=3131cm−1 using such conditions allowed us to unambiguously assign the tow series for Ka=1 and some lines with Ka=2. The series are quite irregular because of the Renner-Teller perturbation in the ν3 state, but the ground state combination differences are fairly regular. Altogether, 45 transitions the been assigned, and 15 combination differences in the ground state have been fitted.

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1M. R""{o}sslein, C. M. Gabrys, M.-F. Jagod, and T. Oka, J. Mol. Spectrosc. 153, 738-740 (1992)


Author Institution: Department of Chemistry, University of Chicago

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