TORSIONAL SPLITTINGS IN $v_{9}^{+}v_{4}$ OF $C_{2}H_{6}$

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1987

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Ohio State University

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Torsional splittings in the torsional hot band v9+v4 of C2H6 have been measured in the P and R branch sub-bands from R15 to P16. Every transition is split into a non-degenerate and a doubly degenerate component with appittings generally near 0.086cm−1. Individual splittings vary between extrcames of 0.235cm−1 and −.079cm−1 (splitting is of opposite phase). The detailed behavior of the splitting is deseribed quantitively by the zeroth order torsional Hamiltonian for ν9. HTOR(9)=APγ2+V62(9)(1−cos⁡6γ). together with the xy Coriolis Interaction operator(1) HCOR−2Bζ4,9xy[(2A)1/2Pγ(JQ9++J+Q9−)−(2A)−1/2sin⁡6γ6(JP9++J+P9−)] connecting ν9+ν4 and the excited torsional states 2νh,3νh,4νh,5νh, and 6νh. Of these, interactions with the nearaby 4νh and 5νh states contribute very significantly to the splittings. Interactions of ν9+ν4 with nνh (n=odd) are nominally forbidden (g + u) in the high barrier limit, corresponding to a rigid molecule. Such interactions are not strictly forbidden, however, but are allowed only in doubly degenerate torsional states, with matrix elements which increase rapidly with torsional quantum number. The zeroth order splitting (0.086cm−1) and the Coriolis interaction constant (ζ4,9xy) and torsional matrix elements consistent with the spectra are predicted extremely well by the coefficients determined from the analysis of splittings in the ν9 band of ethane(1).

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1 J. Susskind, D. Reuter, D. E. Jennings, S. J. Daunt, W. E. Blass, and G. W. Halsey, J. Chem. Phys., 77, 2728 (1982)


Author Institution: NASA GSFC.; Molecular Spectrosocopy Laboratory, Dept. of Physics and Astronomy, University of Tennessee, Knoxville. TN 37996

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