SUBMILLIMETER WAVE SPECTRA OF NCS

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Date

2003

Authors

Maeda, A.
Habara, H.
Amano, T.

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Ohio State University

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Abstract

Rotational spectra of NCS in the excited bending vibrational states have not been analyzed in detail, because of difficulty in analysis due to large Renner - Teller effect and anharmonic interactions. We have extended the observation of the pure rotational spectra of NCS in the v2=1 as well as in the X2Π ground state up to J=53.5 in the submillimeter wave region. For the ground state, the analysis was straightforward. The measured transition frequencies were fit to a standard effective Hamiltonian for 2Π vibronic states, and the improved molecular constants including the higher order centrifugal distortion constants were obtained. The v2=1 vibronic state splits into four vibronic sub-states, 2Δ5/2,2Δ3/2,μ2Σ and κ2Σ. As a first attempt, the Δ and Σ states were fitted separately to effective Hamiltonians. The least square fittings converged by including various effective parameters concerned with the P-type doubling. However, the physical significance of these higher order parameters is not clear. It is found that the spin rotation coupling constant, γ, and the Λ-type doubling constants, p, q, are significantly different from those for the ground state. We have attempted to analyze the Δ and Σ states simultaneously by taking into account the perturbations from higher vibrational states. An isotopic species, NC34S, in the X2Π3/2 state has also been measured and r0 structure is derived to be r0(NC)=1.1805(1) {\AA}and r0(CS)=1.63212(7)\AA.

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aNASDA postdoctral fellow


Author Institution: Institute for Astrophysics and Planetary Sciences, Ibaraki University

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