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He对星际PO(XΠ)的碰撞激发:新的从头算势能面和散射计算

Collisional excitation of interstellar PO(XΠ) by He: new ab initio potential energy surfaces and scattering calculations.

作者信息

Lique François, Jiménez-Serra Izaskun, Viti Serena, Marinakis Sarantos

机构信息

LOMC - UMR 6294, CNRS-Université du Havre, 25 rue Philippe Lebon, BP 1123, 76 063 Le Havre cedex, France.

出版信息

Phys Chem Chem Phys. 2018 Feb 21;20(8):5407-5414. doi: 10.1039/c7cp05605b.

Abstract

We present the first ab initio potential energy surfaces (PESs) for the PO(XΠ)-He van der Waals system. The PESs were obtained using the open-shell partially spin-restricted coupled cluster approach with single, double and perturbative triple excitations [UCCSD(T)]. The augmented correlation-consistent polarized valence triple-zeta (aug-cc-pVTZ) basis set was employed supplemented by mid-bond functions. Integral and differential cross sections for the rotational excitation in PO-He collisions were calculated using the new PES and compared with results in similar systems. Finally, our work presents the first hyperfine-resolved cross sections for this system that are needed for accurate modelling in astrophysical environments.

摘要

我们展示了PO(XΠ)-He范德瓦尔斯体系的首个从头算势能面(PESs)。这些势能面是通过开壳层部分自旋限制耦合簇方法结合单、双及微扰三激发[UCCSD(T)]得到的。采用了增强相关一致极化价三重ζ(aug-cc-pVTZ)基组,并辅以键中函数。利用新的势能面计算了PO-He碰撞中转动激发的积分和微分截面,并与类似体系的结果进行了比较。最后,我们的工作给出了该体系首个超精细分辨截面,这对于天体物理环境中的精确建模是必需的。

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