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Vibrational spectra and structural parameters of some XNCO and XOCN (X = H, F, Cl, Br) molecules
Authors:James R Durig  Xiaohua Zhou  Diepngan Nguyen
Institution:a Department of Chemistry, University of Missouri-Kansas City, Kansas City, MO 64110, USA
b Departments of Chemistry and Physics, The University of the South, Sewanee, TN 37383, USA
Abstract:Ab initio calculations with full electron correlation by the perturbation method to second order and hybrid density functional theory calculations by the B3LYP method utilizing the 6-31G(d), 6-311+G(d, p), and 6-311+G(2d, 2p) basis sets have been carried out for the XNCO and XOCN (X = H, F, Cl, Br) molecules. From these calculations, force constants, vibrational frequencies, infrared intensities, Raman activities, depolarization ratios, and structural parameters have been determined and compared to the experimental quantities when available. By combining previously reported rotational constants for HNCO, ClNCO and BrNCO with the ab initio MP2/6-311+G(d, p) predicted structural values, adjusted r0 parameters have been obtained. The r0 values for BrNCO are: r(Brsingle bondN) = 1.857(5); r(Ndouble bond; length as m-dashC) = 1.228(5); r(Cdouble bond; length as m-dashO) = 1.161(5) Å; BrNC = 117.5(5) and NCO = 172.3(5)°. For ClNCO the determined r0 parameters are in excellent agreement with the previously determine rs values, whereas those for HNCO the HNC angle is larger with a value of 126.3(5)° compared to the previous reported value of 123.9(17)°. However, considering the relatively large uncertainty in the value given initially the two results are in near agreement. Structural parameters are also estimated for FNCO and XOCN (X = H, F, Cl, Br). The centrifugal distortion constants have been calculated and are compared to the experimentally (XNCO: X = H, Cl, Br) determined values. Predicted values for the barriers of linearity are given for both the XNCO (X = H, F, Cl, Br) molecules and the results were compared to the corresponding isothiocyanate molecules. The predicted frequencies for the fundamentals of the XNCO molecules compare favorably to the experimental values but some of the predicted intensities differ significantly from those in the observed spectra. The two OCN bends for HOCN have been assigned and the frequencies for the two corresponding fundamentals of DOCN are predicted.
Keywords:Ab initio calculations  Infrared and Raman spectra  r0 Structural parameters  XNCO and XOCN (X     H  F  Cl  Br) molecules
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