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氢分子与氦原子碰撞的相互作用诱导偶极子:一种新的用于高温应用的从头算偶极子表面。

Interaction-induced dipoles of hydrogen molecules colliding with helium atoms: a new ab initio dipole surface for high-temperature applications.

机构信息

Department of Chemistry, Michigan State University, East Lansing, Michigan 48824, USA.

出版信息

J Chem Phys. 2012 Jan 28;136(4):044320. doi: 10.1063/1.3676406.

DOI:10.1063/1.3676406
PMID:22299884
Abstract

We report new ab initio results for the interaction-induced dipole moments Δμ of hydrogen molecules colliding with helium atoms. These results are needed in order to calculate collision-induced absorption spectra at high temperatures; applications include modeling the radiative profiles of very cool white dwarf stars, with temperatures from 3500 K to 9000 K. We have evaluated the dipoles based on finite-field calculations, with coupled cluster methods in MOLPRO 2006 and aug-cc-pV5Z (spdfg) basis sets for both the H and He centers. We have obtained values of Δμ for eight H(2) bond lengths ranging from 0.942 a.u. to 2.801 a.u., for 15 intermolecular separations R ranging from 2.0 a.u. to 10.0 a.u., and for 19 different relative orientations. In general, our values agree well with earlier ab initio results, for the geometrical configurations that are treated in common, but we have determined more points on the collision-induced dipole surface by an order of magnitude. These results make it possible to calculate transition probabilities for molecules in excited vibrational states, overtones, and rotational transitions with ΔJ > 4. We have cast our results in the symmetry-adapted form needed for absorption line shape calculations, by expressing Δμ as a series in the spherical harmonics of the orientation angles of the intermolecular vector and of a unit vector along the H(2) bond axis. The expansion coefficients depend on the H(2) bond length and the intermolecular distance R. For large separations R, we show that the ab initio values of the leading coefficients converge to the predictions from perturbation theory, including both classical multipole polarization and dispersion effects.

摘要

我们报告了氢分子与氦原子碰撞的诱导偶极矩 Δμ 的新从头算结果。这些结果是计算高温下碰撞诱导吸收光谱所必需的;应用包括模拟温度从 3500 K 到 9000 K 的非常冷的白矮星的辐射轮廓。我们基于有限场计算评估了偶极矩,使用 MOLPRO 2006 中的耦合簇方法和 H 中心的 aug-cc-pV5Z(spdfg)基组以及 He 中心的 aug-cc-pV5Z(spdfg)基组。我们得到了 8 个 H(2)键长从 0.942 a.u.到 2.801 a.u.、15 个分子间分离距离 R 从 2.0 a.u.到 10.0 a.u.和 19 个不同相对取向的 Δμ 值。一般来说,对于共同处理的几何构型,我们的结果与早期的从头算结果吻合得很好,但我们通过一个数量级确定了碰撞诱导偶极面上更多的点。这些结果使得计算处于激发振动状态、泛音和 ΔJ > 4 的转动跃迁的分子跃迁概率成为可能。我们通过将 Δμ 表示为分子间矢量和 H(2)键轴方向上的单位矢量的取向角的球谐级数,将结果表示为适应对称性的形式,用于吸收线形状计算。扩展系数取决于 H(2)键长和分子间距离 R。对于大的分离距离 R,我们表明领头系数的从头算值收敛于包括经典多极极化和色散效应的微扰理论预测。

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