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首页> 外文期刊>The journal of physical chemistry, A. Molecules, spectroscopy, kinetics, environment, & general theory >Accurate Pair Interaction Energies for Helium from Supermolecular Gaussian Geminal Calculations
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Accurate Pair Interaction Energies for Helium from Supermolecular Gaussian Geminal Calculations

机译:从超分子高斯Geminal计算计算出准确的氦原子对相互作用

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Nonrelativistic clamped-nuclei pair interaction energy for ground-state helium atoms has been computed for 12 interatomic separations ranging from 3.0 to 9.0 bohr.The calculations applied the supermolecular approach.The major part of the interaction energy was obtained using the Gaussian geminal implementation of the coupled-cluster theory with double excitations(CCD).Relatively small contributions from single,triple,and quadruple excitations were subsequently included employing the conventional orbital coupled-cluster method with single,double,and noniterative triple excitations [CCSD(T)] and the full configuration interaction(FCI)method.For three distances,the single-excitation contribution was taken from literature Gaussian-geminal calculations at the CCSD level.The orbital CCSD(T)and FCI calculations used very large basis sets,up to doubly augmented septuple-and sextuple-zeta size,respectively,and were followed by extrapolations to the complete basis set limits.The accuracy of the total interaction energies has been estimated to be about 3 mK or 0.03% at the minimum of the potential well.For the attractive part of the well,the relative errors remain consistently smaller than 0.03%.In the repulsive part,the accuracy is even better,except,of course,for the region where the potential goes through zero.For interatomic separations smaller than 4.0 bohr,the relative errors do not exceed 0.01%.Such uncertainties are significantly smaller than the expected values of the relativistic and diagonal Born-Oppenheimer contributions to the potential.
机译:计算了基态氦原子的非相对论性钳位核对相互作用能,计算范围为3.0至9.0 bohr的12个原子间间隔,计算采用了超分子方法,其中相互作用能的主要部分是使用高斯双生子实现的。耦合簇理论与双激发(CCD)。随后,采用传统的轨道耦合簇方法对单,双和非迭代三重激发[CCSD(T)]进行了单,三和四重激发的相对较小贡献。在三个距离上,单次激励贡献来自文献CCSD级别的高斯-基元计算。轨道CCSD(T)和FCI计算使用非常大的基集,直到双倍增加的七进制-和六元组-Zeta大小,然后外推到完整的基本设置极限。在势阱的最小值处,总相互作用能估计约为3 mK或0.03%。对于势阱的吸引部分,相对误差始终小于0.03%。在斥力部分,精度甚至更高,当然,对于势能为零的区域而言。对于小于4.0 bohr的原子间间距,相对误差不超过0.01%。这种不确定性远小于相对论和对角Born-Oppenheimer的期望值对潜力的贡献。

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