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Xe-NO(X2Π)范德华配合物相互作用势能的从头算研究:束缚态和全量子及准经典散射。

Ab initio studies of the interaction potential for the Xe-NO(X2Π) van der Waals complex: bound states and fully quantum and quasi-classical scattering.

机构信息

Department of Chemistry and Biochemistry, University of Maryland, College Park, Maryland 20742-2021, USA.

出版信息

J Chem Phys. 2012 Jul 7;137(1):014312. doi: 10.1063/1.4731286.

DOI:10.1063/1.4731286
PMID:22779653
Abstract

Adiabatic potential energy surfaces for the ground electronic state of the Xe⋅⋅⋅NO(X(2)Π) van der Waals complex have been calculated using the spin-restricted coupled cluster method with single, double, and non-iterative triple excitations (RCCSD(T)). The scalar relativistic effects present in the Xe atom were included by an effective core potential and we extended the basis with bond functions to improve the description of the dispersion interaction. It has been found that the global minimum on the A(') adiabatic surface occurs at a T-shaped geometry with γ(e) = 94° and R(e) = 7.46 a(0), and with well depth of D(e) = 148.68 cm(-1). There is also an additional local minimum for the collinear geometry Xe-NO with a well depth of 104.5 cm(-1). The adiabat of A('') symmetry exhibits a single minimum at a distance R(e) = 7.68 a(0) and has a skewed geometry with γ(e) = 64° and a well depth of 148.23 cm(-1). Several C(nl) van der Waals dispersion coefficients are also estimated, of which C(6, 0) and C(6, 2) are in a reasonable agreement with previous theoretical results obtained by Nielson et al. [J. Chem. Phys. 64, 2055 (1976)]. The new potential energy surfaces were used to calculate bound states of the complex for total angular momentum quantum numbers up to J = 7/2. The ground state energy of Xe⋅⋅⋅NO(X(2)Π) is D(0) = 117 cm(-1), which matches the experimental value very accurately (within 3.3%). Scattering calculations of integral and differential cross sections have also been performed using fully quantum close coupling calculations and quasi-classical trajectory method at a collision energy of 63 meV. These calculations reveal the important role played by L-type rainbows in the scattering dynamics of the heavier Rg-NO(X) systems.

摘要

已使用单、双和非迭代三重激发(RCCSD(T))的自旋限制耦合簇方法计算了基电子态的 Xe⋅⋅⋅NO(X(2)Π)范德华复合物的绝热势能面。Xe 原子中的标量相对论效应通过有效核势包含在内,我们通过键函数扩展了基组以改善色散相互作用的描述。已发现 A(')绝热表面上的全局最小值出现在 T 形几何形状,γ(e) = 94°,R(e) = 7.46 a(0),并且势阱深度为 D(e) = 148.68 cm(-1)。对于共线几何 Xe-NO 也存在另一个局部最小值,势阱深度为 104.5 cm(-1)。A(''')对称性的绝热线在距离 R(e) = 7.68 a(0)处表现出单个最小值,并且具有倾斜几何形状,γ(e) = 64°,势阱深度为 148.23 cm(-1)。还估计了几个 C(nl)范德华色散系数,其中 C(6, 0)和 C(6, 2)与 Nielson 等人之前通过理论获得的结果[J. Chem. Phys. 64, 2055 (1976)]相吻合。新的势能面用于计算总角动量量子数高达 J = 7/2 的复合物的束缚态。Xe⋅⋅⋅NO(X(2)Π)的基态能量为 D(0) = 117 cm(-1),与实验值非常吻合(精度在 3.3%以内)。使用完全量子紧密耦合计算和准经典轨迹方法在 63 meV 的碰撞能下也进行了积分和微分截面的散射计算。这些计算揭示了 L 型虹在较重的 Rg-NO(X)系统散射动力学中所起的重要作用。

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