On the structural parameters and vibrational spectra of some XNCS and XSCN (X = H, F, Cl, Br) molecules

被引:37
|
作者
Durig, JR [1 ]
Zheng, C [1 ]
Deeb, H [1 ]
机构
[1] Univ Missouri, Dept Chem, Kansas City, MO 64110 USA
关键词
ab initio calculations; infrared and Raman spectra; r(0) structural parameters; XNCS and XSCN (X=H; F; Cl; Br); molecules;
D O I
10.1016/j.molstruc.2005.06.034
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
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 XNCS and XSCN (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 HNCS, CISCN and BrSCN with the ab initio MP2/6-31 I + G(d,p) predicted parameters, adjusted r(0) parameters have been obtained. The structural parameters for isothiocyanic acid are: r(H-N) = 0.996(5)angstrom; r(N=C) = 1.208(3) angstrom; r(C = S) = 1.568(3) angstrom; angle HNC = 132.0(5)degrees; angle NCS = 172.9(5)degrees. These reported angles have much lower uncertainties than those previously reported from the microwave data alone. The ab initio predicted barrier to molecular linearity of HNCS is 917 + 44 cm (-1) which is in excellent agreement with the experimental value of 900 + 200 cm(-1). The r(0) parameters for CISCN are: r(Cl-S) = 2.023(5); r(S-C) = 1.694(3); r(C N)=1.156(3)angstrom; angle CISC=99.6(5) and angle SCN=174.4(5)degrees and for BrSCN are: r(Br-S)=2.197(5); r(S-C)=1.681(3); r(C N)=1.158(3)angstrom; angle BrSC=99.5(5) and angle SCN=174.7(5)degrees. Structural parameters are also estimated for HSCN and FSCN. The predicted frequencies for the fundamentals of HNCS and DNCS compare favorably to the experimental values but several of their predicted intensities differ significantly from the observed spectra. The frequencies for the reported bending modes of CISCN and BrSCN do not agree with the predicted values and further experimental studies are needed for providing confident assignments for these fundamentals. (c) 2005 Elsevier B.V. All rights reserved.
引用
收藏
页码:78 / 92
页数:15
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