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arXiv 2008.03237physics.chem-ph
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用于精确处理数百个原子的开壳层分子的显式相关耦合簇方法

Explicitly correlated coupled cluster method for accurate treatment of open-shell molecules with hundreds of atoms

Ashutosh Kumar, Frank Neese, Edward F. Valeev

AI总结:

提出近线性标度的显式相关开壳层CCSD(T)方法,基于DLPNO框架实现与闭壳层形式精确一致,能在3天内处理超550原子系统,生成热计算精度达0.3-0.4 kcal/mol。

摘要:

我们提出了一种近线性标度的显式相关耦合簇单双激发并带有微扰三激发方法(CCSD(T)$_{\overline{\text{F12}}}$)的公式化,用于开壳层物种的高自旋态。该方法基于常规的开壳层 CCSD 形式 [M. Saitow et al., J. Chem. Phys. 146, 164105 (2017)],利用了域局域对自然轨道(DLPNO)框架。使用自旋无关的对自然轨道集合确保了与先前报道的闭壳层形式完全一致,且对计算成本的影响极小(例如,对于 $\text{C}_\text{160}\text{H}_{\text{322}}$ 正烷烃,开壳层形式仅比闭壳层对应形式慢 1.5 倍,测得的尺寸复杂度约为 1.2)。在单台多核计算机上,不到 3 天即可完成对包含超过 550 个原子和 5000 个基函数的开壳层系统在接近完备基组(CBS)极限下的耦合簇能量评估。对于 348 种核心燃烧物种基准集 [J. Klippenstein et al., J. Phys. Chem. A 121, 6580 (2017)] 中最大的 50 个分子,aug-cc-pVTZ DLPNO-CCSD(T)$_{\overline{\text{F12}}}$ 对生成热的贡献与外推的 CBS CCSD(T) 参考值的均方根偏差(RMSD)为 0.3 kcal/mol。对于包含小闭壳层和开壳层分子的更具挑战性的 50 个反应集 [G. Knizia et al., J. Chem. Phys. 130, 054104 (2009)],aug-cc-pVQ(+d)Z DLPNO-CCSD(T)$_{\overline{\text{F12}}}$ 相对于 CBS CCSD(T) 估计值的 RMSD 约为 0.4 kcal/mol。

英文摘要:

We present a near-linear scaling formulation of the explicitly-correlated coupled-cluster singles and doubles with perturbative triples method (CCSD(T)$_{\overline{\text{F12}}}$) for high-spin states of open-shell species. The approach is based on the conventional open-shell CCSD formalism [M. Saitow et al., J. Chem. Phys. 146, 164105 (2017)] utilizing the domain local pair-natural orbitals (DLPNO) framework. The use of spin-independent set of pair-natural orbitals ensures exact agreement with the closed-shell formalism reported previously, with only marginally impact on the cost (e.g. the open-shell formalism is only 1.5 times slower than the closed-shell counterpart for the $\text{C}_\text{160}\text{H}_{\text{322}}$ n-alkane, with the measured size complexity of $\approx1.2$). Evaluation of coupled-cluster energies near the complete-basis-set (CBS) limit for open-shell systems with more than 550 atoms and 5000 basis functions is feasible on a single multi-core computer in less than 3 days. The aug-cc-pVTZ DLPNO-CCSD(T)$_{\overline{\text{F12}}}$ contribution to the heat of formation for the 50 largest molecules among the 348 core combustion species benchmark set [J. Klippenstein et al., J. Phys. Chem. A 121, 6580 (2017)] had root-mean-square deviation (RMSD) from the extrapolated CBS CCSD(T) reference values of 0.3 kcal/mol. For a more challenging set of 50 reactions involving small closed- and open-shell molecules [G. Knizia et al., J. Chem. Phys. 130, 054104 (2009)] the aug-cc-pVQ(+d)Z DLPNO-CCSD(T)$_{\overline{\text{F12}}}$ yielded a RMSD of $\sim$0.4 kcal/mol with respect to the CBS CCSD(T) estimate.

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