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氩三聚体转动-振动光谱的计算

Calculation of argon trimer rovibrational spectrum.

作者信息

Karlický Frantisek, Lepetit Bruno, Kalus René, Gadéa Florent Xavier

机构信息

Department of Physics, University of Ostrava, 30 dubna 22, 701 03 Ostrava, Czech Republic.

出版信息

J Chem Phys. 2007 May 7;126(17):174305. doi: 10.1063/1.2721564.

Abstract

Rovibrational spectra of Ar3 are computed for total angular momenta up to J=6 using row-orthonormal hyperspherical coordinates and an expansion of the wave function on hyperspherical harmonics. The sensitivity of the spectra to the two-body potential and to the three-body corrections is analyzed. First, the best available semiempirical pair potential (HFDID1) is compared with our recent ab initio two-body potential. The ab initio vibrational energies are typically 1-2 cm-1 higher than the semiempirical ones, which is related to the slightly larger dissociation energy of the semiempirical potential. Then, the Axilrod-Teller asymptotic expansion of the three-body correction is compared with our newly developed ab initio three-body potential. The difference is found smaller than 0.3 cm-1. In addition, we define approximate quantum numbers to describe the vibration and rotation of the system. The vibration is represented by a hyper-radial mode and a two-degree-of-freedom hyperangular mode, including a vibrational angular momentum defined in an Eckart frame. The rotation is described by the total angular momentum quantum number, its projection on the axis perpendicular to the molecular plane, and a hyperangular internal momentum quantum number, related to the vibrational angular momentum by a transformation between Eckart and principal-axes-of-inertia frames. These quantum numbers provide a qualitative understanding of the spectra and, in particular, of the impact of the nuclear permutational symmetry of the system (bosonic with zero nuclear spin). Rotational constants are extracted from the spectra and are shown to be accurate only for the ground hyperangular mode.

摘要

使用行正交超球坐标以及超球谐函数上的波函数展开,计算了总角动量高达(J = 6)的(Ar_3)的振转光谱。分析了光谱对两体势和三体修正的敏感性。首先,将现有的最佳半经验对势(HFDID1)与我们最近的从头算两体势进行比较。从头算振动能通常比半经验振动能高(1 - 2 cm^{-1}),这与半经验势的离解能稍大有关。然后,将三体修正的Axilrod-Teller渐近展开与我们新开发的从头算三体势进行比较。发现差异小于(0.3 cm^{-1})。此外,我们定义了近似量子数来描述系统的振动和转动。振动由一个超径向模式和一个两自由度超角模式表示,包括在Eckart坐标系中定义的振动角动量。转动由总角动量量子数、其在垂直于分子平面的轴上的投影以及一个超角内动量量子数描述,该量子数通过Eckart坐标系和惯性主轴坐标系之间的变换与振动角动量相关。这些量子数为光谱,特别是为系统的核置换对称性(具有零核自旋的玻色子)的影响提供了定性理解。从光谱中提取了转动常数,结果表明仅对基态超角模式是准确的。

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