NASA Ames Research Center, Moffett Field, California 94035-1000, USA.
J Chem Phys. 2011 Dec 28;135(24):244310. doi: 10.1063/1.3671389.
Highly correlated ab initio quartic force fields (QFFs) are used to calculate the equilibrium structures and predict the spectroscopic parameters of three HC(2)N isomers. Specifically, the ground state quasilinear triplet and the lowest cyclic and bent singlet isomers are included in the present study. Extensive treatment of correlation effects were included using the singles and doubles coupled-cluster method that includes a perturbational estimate of the effects of connected triple excitations, denoted as CCSD(T). Dunning's correlation-consistent basis sets cc-pVXZ, X = 3,4,5, were used, and a three-point formula for extrapolation to the one-particle basis set limit was used. Core-correlation and scalar relativistic corrections were also included to yield highly accurate QFFs. The QFFs were used together with second-order perturbation theory (PT) (with proper treatment of Fermi resonances) and variational methods to solve the nuclear Schrödinger equation. The quasilinear nature of the triplet isomer is problematic, and it is concluded that a QFF is not adequate to describe properly all of the fundamental vibrational frequencies and spectroscopic constants (though some constants not dependent on the bending motion are well reproduced by PT). On the other hand, this procedure (a QFF together with either PT or variational methods) leads to highly accurate fundamental vibrational frequencies and spectroscopic constants for the cyclic and bent singlet isomers of HC(2)N. All three isomers possess significant dipole moments, 3.05 D, 3.06 D, and 1.71 D, for the quasilinear triplet, the cyclic singlet, and the bent singlet isomers, respectively. It is concluded that the spectroscopic constants determined for the cyclic and bent singlet isomers are the most accurate available, and it is hoped that these will be useful in the interpretation of high-resolution astronomical observations or laboratory experiments.
高相关的从头 quartic 力场 (QFF) 被用于计算 HC(2)N 三种异构体的平衡结构并预测其光谱参数。具体来说,本研究包括基态准线性三重态和最低环状和弯曲单线态异构体。使用包含对连接三重态效应的微扰估计的单双激发耦合簇方法 (CCSD(T)) 包括对关联效应的广泛处理。使用 Dunning 的相关一致基组 cc-pVXZ,X = 3,4,5,并使用三点点公式进行单粒子基组极限外推。还包括核心相关和标量相对论修正以产生高度准确的 QFF。QFF 与二阶微扰理论 (PT)(正确处理费米共振)和变分方法一起用于求解核薛定谔方程。三重态异构体的准线性性质是有问题的,结论是 QFF 不足以正确描述所有基本振动频率和光谱常数(尽管一些不依赖于弯曲运动的常数可以通过 PT 很好地再现)。另一方面,这种方法(QFF 与 PT 或变分方法一起)导致 HC(2)N 的环状和弯曲单线态异构体具有高度准确的基本振动频率和光谱常数。三种异构体都具有显著的偶极矩,分别为 3.05 D、3.06 D 和 1.71 D,用于准线性三重态、环状单线态和弯曲单线态异构体。结论是确定的环状和弯曲单线态异构体的光谱常数是最准确的,希望这些常数将有助于解释高分辨率天文观测或实验室实验。