Electron–nuclear cusp check for self-consistent field wave functions for the neutral atoms from helium to uranium

1986 ◽  
Vol 64 (10) ◽  
pp. 1351-1352 ◽  
Author(s):  
William M. Westgate ◽  
Albert D. Byrne ◽  
Vedene H. Smith Jr. ◽  
Alfredo M. Simas

The values of the electron density ρ(0), its derivative at the nucleus ρ′(0), and the electron (e)–nuclear (n) cusp ratio Cen = –ρ′(0)/2Zρ(0) are evaluated for the popular self-consistent field functions of Clementi and Roetti (helium to xenon) and McLean and McLean (cesium to uranium). The Cen's for these functions exhibit deviations from the exact value of one.

1989 ◽  
Vol 67 (5) ◽  
pp. 543-543 ◽  
Author(s):  
William M. Westgate ◽  
Albert D. Byrne ◽  
Vedene H. Smith Jr. ◽  
Alfredo M. Simas

1991 ◽  
Vol 94 (10) ◽  
pp. 6708-6715 ◽  
Author(s):  
Thilo Busch ◽  
Alessandra Degli Esposti ◽  
Hans‐Joachim Werner

1972 ◽  
Vol 50 (7) ◽  
pp. 708-709 ◽  
Author(s):  
K. M. S. Saxena

Accurate numerical Hartree–Fock (HF) self-consistent-field (SCF) wave functions have been obtained for La+(4ƒ16S)3F and 1F, Tm+(4ƒ136S)3F and 1F, and Yb(4ƒ146S)2S rare-earth ions. In general, the total energy values have an accuracy of seven figures, the virial theorem is satisfied to seven significant digits, and the radial wave functions are self-consistent and without tail oscillations to three decimals. Several Hartree–Fock parameters are also evaluated with these functions.


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