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首页> 外文期刊>The Journal of Chemical Physics >Accurate prediction of heat of formation by combining Hartree-Fock/density functional theory calculation with linear regression correction approach
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Accurate prediction of heat of formation by combining Hartree-Fock/density functional theory calculation with linear regression correction approach

机译:通过结合Hartree-Fock /密度泛函理论计算和线性回归校正方法来准确预测地层热量

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摘要

A linear regression correction approach has been developed successfully to account for the electron correlation energy missing in Hartree-Fock calculation and to reduce the calculation errors of density functional theory. The numbers of lone-pair electrons, bonding electrons and inner layer electrons in molecules, and the number of unpaired electrons in the composing atoms in their ground states are chosen to be the most important physical descriptors to determine the correlation energy unaccounted by Hartree-Fock method or to improve the results calculated by B3LYP density functional theory method. As a demonstration, this proposed linear regression correction approach has been applied to evaluate the standard heats of formation DeltaH(f)(Theta) of 180 small-sized to medium-sized organic molecules at 298.15 K. Upon correction, the mean absolute deviation for the 150 molecules in the training set decreases from 351.0 to 4.6 kcal/mol and 360.9 to 4.6 kcal/mol for HF/6-31G(d) and HF/6-311+G(d,p) methods, respectively. For B3LYP method, the mean absolute deviations are reduced from 9.2 and 18.2 kcal/mol to 2.7 and 2.4 kcal/mol for 6-31G(d) and 6-311+G(d,p) basis sets, respectively. (C) 2004 American Institute of Physics.
机译:已经成功开发了线性回归校正方法,以解决Hartree-Fock计算中缺少的电子相关能并减少密度泛函理论的计算误差。选择分子中的孤对电子,键合电子和内层电子的数量以及组成原子处于基态的未成对电子的数量作为确定Hartree-Fock无法解释的相关能的最重要的物理描述符。方法或改进结果,可采用B3LYP密度泛函理论方法计算。作为演示,此提议的线性回归校正方法已应用于评估298.15 K下180个小到中型有机分子的标准形成热DeltaH(f)(Theta)。校正后,对于HF / 6-31G(d)和HF / 6-311 + G(d,p)方法,训练集中的150个分子分别从351.0降至4.6 kcal / mol和从360.9降至4.6 kcal / mol。对于B3LYP方法,对于6-31G(d)和6-311 + G(d,p)基集,平均绝对偏差分别从9.2和18.2 kcal / mol减小到2.7和2.4 kcal / mol。 (C)2004年美国物理研究所。

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