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arXiv 2011.03595physics.chem-ph
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跃迁势耦合簇

Transition-Potential Coupled Cluster

Megan E. Simons, Devin A. Matthews

AI总结:

针对核心空穴光谱计算中的轨道弛豫难题,提出基于跃迁势参考轨道的跃迁势耦合簇方法,其中TP-CCSD(1/2)可在与EOM-CCSD相当的成本下,实现第一行原子分子X射线吸收光谱的高精度计算。

摘要:

计算核心空穴光谱(包括X射线吸收和X射线光电离)中的轨道弛豫问题长期困扰着线性响应方法,包括运动方程耦合簇单双激发方法(EOM-CCSD)。我们未通过引入额外电子关联来解决该问题,而是提出通过使用“跃迁势”参考轨道来显式处理轨道弛豫,由此得到跃迁势耦合簇(TP-CC)方法家族。其中的TP-CCSD(1/2)方法被发现可基本消除轨道弛豫误差,其在核心空穴光谱上达到的精度与EOM-CCSD在价层区域的典型预期精度相当。这些结果表明,对于含第一行原子的分子,可在与EOM-CCSD基本相同的计算成本下得到非常精确的X射线吸收光谱。

英文摘要:

The problem of orbital relaxation in computational core-hole spectroscopies, including x-ray absorption and x-ray photoionization, has long plagued linear response approaches, including equation-of-motion coupled cluster with singles and doubles (EOM-CCSD). Instead of addressing this problem by including additional electron correlation, we propose an explicit treatment of orbital relaxation via the use of "transition potential" reference orbitals, leading to a transition-potential coupled cluster (TP-CC) family of methods. One member of this family in particular, TP-CCSD(1/2), is found to essentially eliminate the orbital relaxation error and achieve the same level of accuracy for core-hole spectra as is typically expected of EOM-CCSD in the valence region. These results show that very accurate x-ray absorption spectra for molecules with first-row atoms can be computed at a cost essentially the same as that for EOM-CCSD.

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