THE CHEMISTRY OF THE SUPERHEAVY ELEMENTS .1. PSEUDOPOTENTIALS FOR 111AND 112 AND RELATIVISTIC COUPLED-CLUSTER CALCULATIONS FOR (112)H-2, AND (112)F-4(, (112)F)
M. Seth et al., THE CHEMISTRY OF THE SUPERHEAVY ELEMENTS .1. PSEUDOPOTENTIALS FOR 111AND 112 AND RELATIVISTIC COUPLED-CLUSTER CALCULATIONS FOR (112)H-2, AND (112)F-4(, (112)F), The Journal of chemical physics, 106(9), 1997, pp. 3623-3632
One- and two-component (spin-orbit coupled) relativistic and nonrelati
vistic energy adjusted pseudopotentials and basis sets for the element
s 111 and 112 are presented. Calculations on the positively charged mo
nohydride of the recently discovered superheavy element 112 are report
ed. Electron correlation is treated at the multireference configuratio
n interaction and coupled cluster level and fine structure effects are
derived from a single-reference configuration interaction treatment.
Relativistic effects decrease the (112H+ bond distance by 0.41 Angstro
m. This bond contraction is similar to the one calculated recently for
(111)H [Chem. Phys. Lett. 250, 461 (1996)]. As a result the bond dist
ance of (112H+ (1.52 Angstrom) is predicted to be smaller compared to
those of the hydrides of the lighter congeners HgH+ (1.59 Angstrom), C
dH+ (1.60 Angstrom) and similar to that of ZnH+ (1.52 Angstrom). We pr
edict that (112H+ is the most stable hydride in the Group 12 series du
e to relativistic effects. As in the case of (111)H the relativistic i
ncrease of the stretching force constant is quite large, from 1.5 to 4
.3 mdyn/Angstrom at the coupled cluster level. The trend in the;dipole
polarizabilities of the Group 12 elements is discussed. Relativistic
and electron correlation effects are nonadditive and due to the relati
vistic its contraction (n = 7 for 112), correlation effects out of the
(n - 1)d core are more important at the relativistic than the nonrela
tivistic level. We also,show evidence that element 112 behaves like a
typical transition element, and as a consequence. the high oxidation s
tate +4 in element 112 might be accessible. (C) 1997 American Institut
e of Physics.