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首页> 外文期刊>The journal of physical chemistry, A. Molecules, spectroscopy, kinetics, environment, & general theory >Improved correlation energy extrapolation schemes based on local pair natural orbital methods
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Improved correlation energy extrapolation schemes based on local pair natural orbital methods

机译:基于局部对自然轨道方法的改进相关能量外推方案

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It is well-known that the basis set limit is difficult to reach in correlated post Hartree-Fock ab initio calculations. One possible route forward is to employ basis set extrapolation schemes. In order to avoid prohibitively expensive calculations, the highest level calculation (typically based on the "gold standard" coupled cluster theory with single, double, and perturbative triple excitations, CCSD(T)) is only performed with the smallest basis set, and the remaining basis set incompleteness is estimated at a lower level of theory, typically second-order M?ller-Plesset perturbation theory (MP2). In this work, we provide a comprehensive investigation of alternative schemes where the MP2 extrapolation is replaced by the coupled-electron pair approximation, version 1 (CEPA/1) or the local pair natural orbital version of this method (LPNO-CEPA/1). It is shown that the MP2 method achieves apparent accuracy only due to error cancellation. Systematically more accurate results at small additional computational cost are obtained if the MP2 step is replaced by LPNO-CEPA/1. The errors of LPNO-CEPA/1 relative to canonical CEPA/1 are negligible. Owing to the highly systematic nature of the deviations between canonical and LPNO methods, basis set extrapolation reduces the LPNO errors in the total energies by 1 order of magnitude (~0.2 kcal/mol) and errors in energy differences to essentially zero. Using the CCSD(T)/LPNO-CEPA/1-based extrapolation scheme, new reference values are proposed for the recently published S66 set of interaction energies. The deviations between the new values and the original interactions energies are mostly very small but reach values up to 0.3 kcal/mol.
机译:众所周知,在相关的Hartree-Fock后从头算中,很难达到基集极限。一种可能的前进途径是采用基集外推方案。为了避免计算量过高,仅使用最小的基集执行最高级别的计算(通常基于具有单,双和扰动三重激发的“金标准”耦合簇理论CCSD(T)),并且剩余的基集不完备性是在较低的理论水平(通常是二阶M?ller-Plesset微扰理论(MP2))下估计的。在这项工作中,我们对替代方案进行了全面的研究,其中MP2外推被该方法的耦合电子对逼近版本1(CEPA / 1)或本地对自然轨道版本(LPNO-CEPA / 1)取代。结果表明,MP2方法仅由于消除了错误而获得了明显的准确性。如果将MP2步骤替换为LPNO-CEPA / 1,则可以以较小的额外计算成本获得系统上更准确的结果。相对于规范的CEPA / 1,LPNO-CEPA / 1的误差可以忽略不计。由于规范方法和LPNO方法之间的偏差具有高度系统性,因此基集外推法将总能量中的LPNO误差降低了一个数量级(约0.2 kcal / mol),并且能量差的误差基本降至零。使用基于CCSD(T)/ LPNO-CEPA / 1的外推方案,为最近发布的S66相互作用能集提出了新的参考值。新值和原始相互作用能之间的偏差大部分很小,但最高可达0.3 kcal / mol。

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