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一氧化氮-氪复合物的从头算基态和激发态势能面以及含一氧化氮杂质的氪固体动力学。

Ab initio ground and excited state potential energy surfaces for NO-Kr complex and dynamics of Kr solids with NO impurity.

作者信息

Castro-Palacios Juan Carlos, Rubayo-Soneira Jesús, Ishii Keisaku, Yamashita Koichi

机构信息

Departamento de Física, Universidad de Pinar del Río, Martí 270, Esq. 27 de Noviembre, Pinar del Río, Cuba.

出版信息

J Chem Phys. 2007 Apr 7;126(13):134315. doi: 10.1063/1.2715947.

Abstract

The intermolecular potentials for the NO(X 2Pi)-Kr and NO(A 2Sigma+)-Kr systems have been calculated using highly accurate ab initio calculations. The spin-restricted coupled cluster method for the ground 1 2A' state [NO(X 2Pi)-Kr] and the multireference singles and doubles configuration interaction method for the excited 2 2A' state [NO(A 2Sigma+)-Kr], respectively, were used. The potential energy surfaces (PESs) show two linear wells and one that is almost in the perpendicular position. An analytical representation of the PESs has been constructed for the triatomic systems and used to carry out molecular dynamics (MD) simulations of the NO-doped krypton matrix response after excitation of NO. MD results are shown comparatively for three sets of potentials: (1) anisotropic ab initio potentials [NO molecule direction fixed during the dynamics and considered as a point (its center of mass)], (2) isotropic ab initio potentials (isotropic part in a Legendre polynomial expansion of the PESs), and (3) fitted Kr-NO potentials to the spectroscopic data. An important finding of this work is that the anisotropic and isotropic ab initio potentials calculated for the Kr-NO triatomic system are not suitable for describing the dynamics of structural relaxation upon Rydberg excitation of a NO impurity in the crystal. However, the isotropic ab initio potential in the ground state almost overlaps the published experimental potential, being almost independent of the angle asymmetry. This fact is also manifested in the radial distribution function around NO. However, in the case of the excited state the isotropic ab initio potential differs from the fitted potentials, which indicates that the Kr-NO interaction in the matrix is quite different because of the presence of the surrounding Kr atoms acting on the NO molecule. MD simulations for isotropic potentials reasonably reproduce the experimental observables for the femtosecond response and the bubble size but do not match spectroscopic results. A general overall view of the results suggests that, when the Kr-NO interaction takes place inside the matrix, potentials are rather symmetric and less repulsive than those for the triatomic system.

摘要

已使用高精度的从头算计算方法计算了NO(X 2Pi)-Kr和NO(A 2Sigma+)-Kr体系的分子间势能。分别对基态1 2A'态[NO(X 2Pi)-Kr]采用自旋限制耦合簇方法,对激发态2 2A'态[NO(A 2Sigma+)-Kr]采用多参考单双激发组态相互作用方法。势能面(PESs)显示出两个线性阱和一个几乎处于垂直位置的阱。已构建了三原子体系PESs的解析表达式,并用于对NO激发后掺NO氪基质响应进行分子动力学(MD)模拟。针对三组势能比较了MD结果:(1)各向异性从头算势能[动力学过程中NO分子方向固定并视为一个点(其质心)],(2)各向同性从头算势能(PESs勒让德多项式展开中的各向同性部分),以及(3)根据光谱数据拟合的Kr-NO势能。这项工作的一个重要发现是,为Kr-NO三原子体系计算的各向异性和各向同性从头算势能不适用于描述晶体中NO杂质里德堡激发后的结构弛豫动力学。然而,基态的各向同性从头算势能几乎与已发表的实验势能重叠,几乎与角度不对称无关。这一事实在NO周围的径向分布函数中也有体现。然而,在激发态的情况下,各向同性从头算势能与拟合势能不同,这表明由于周围Kr原子对NO分子的作用,基质中的Kr-NO相互作用有很大差异。各向同性势能的MD模拟合理地再现了飞秒响应和气泡尺寸的实验可观测量,但与光谱结果不匹配。结果的总体概况表明,当Kr-NO相互作用在基质内部发生时,势能相当对称,且比三原子体系的势能排斥性更小。

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