Relativistic well‐tempered Gaussian basis sets for helium through mercury
Relativistic well‐tempered Gaussian basis sets for helium through mercury
复制标题
氦到汞的相对论调和高斯基组
DOI:
10.1063/1.456797
复制
发表时间:
1989
影响因子:
4.4
通讯作者:
O. Matsuoka
中科院分区:
文献类型:
--
作者:
Satosi Okada;O. Matsuoka
Exponent parameters of the nonrelativistically optimized well‐tempered Gaussian basis sets of Huzinaga and Klobukowski have been employed for Dirac–Fock–Roothaan calculations without their reoptimization. For light atoms He (atomic number Z=2)–Rh (Z=45), the number of exponent parameters used has been the same as the nonrelativistic basis sets and for heavier atoms Pd (Z=46)–Hg(Z=80), two 2p (and three 3d) Gaussian basis functions have been augmented. The scheme of kinetic energy balance and the uniformly charged sphere model of atomic nuclei have been adopted. The qualities of the calculated basis sets are close to the Dirac–Fock limit.