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Accurate Complete Basis Set Extrapolation of Direct Random Phase Correlation Energies

机译:直接随机相位相关能量的精确完整基集外推

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The direct random phase approximation (dRPA) is a promising way to obtain improvements upon the standard semilocal density functional results in many aspects of computational chemistry. In this paper, we address the slow convergence of the calculated dRPA correlation energy with the increase of the quality and size of the popular Gaussian-type Dunning's correlation consistent aug-cc-pVXZ split valence atomic basis set family. The cardinal number X controls the size of the basis set, and we use X = 3-6 in this study. It is known that even the very expensive X = 6 basis sets lead to large errors for the dRPA correlation energy, and thus complete basis set extrapolation is necessary. We study the basis set convergence of the dRPA correlation energies on a set of 65 hydrocarbon isomers from CH4 to C6H6. We calculate the iterative density fitted dRPA correlation energies using an efficient algorithm based on the CC-like form of the equations using the self-consistent HF orbitals. We test the popular inverse cubic, the optimized exponential, and inverse power formulas for complete basis set extrapolation. We have found that the optimized inverse power based extrapolation delivers the best energies. Further analysis showed that the optimal exponent depends on the molecular structure, and the most efficient two-point energy extrapolations that use X = 3 and 4 can be improved considerably by considering the atomic composition and hybridization states of the atoms in the molecules. Our results also show that the optimized exponents that yield accurate X = 3 and 4 extrapolated dRPA energies for atoms or small molecules might be inaccurate for larger molecules.
机译:直接随机相位近似(dRPA)是在计算化学的许多方面获得对标准半局部密度函数结果的改进的有前途的方法。在本文中,我们解决了随着流行的高斯型Dunning的相关一致aug-cc-pVXZ分裂价原子基集族的质量和尺寸的增加,所计算的dRPA相关能量的缓慢收敛。基数X控制基集的大小,在这项研究中我们使用X = 3-6。众所周知,即使非常昂贵的X = 6基集也会导致dRPA相关能量的较大误差,因此必须进行完整的基集外推。我们研究了从CH4到C6H6的65种碳氢化合物异构体上dRPA相关能的基集收敛性。我们使用自洽的HF轨道,基于方程的CC类形式,使用高效算法计算迭代密度拟合的dRPA相关能量。我们测试了流行的反三次方,优化的指数以及反幂公式,以进行完整的基集外推。我们发现,基于优化的逆功率外推法可提供最佳能量。进一步的分析表明,最佳指数取决于分子结构,并且通过考虑分子中原子的原子组成和杂交状态,可以显着改善使用X = 3和4的最有效的两点能量外推法。我们的结果还表明,对于原子或小分子而言,产生精确X = 3和4外推dRPA能量的优化指数可能不准确。

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