A. Ricca et Cw. Bauschlicher, SUCCESSIVE OH BINDING-ENERGIES OF M(OH)(N)(-3 AND M=SC, TI, V, CO, NI, AND CU() FOR N=1), The journal of physical chemistry. A, Molecules, spectroscopy, kinetics, environment, & general theory, 101(47), 1997, pp. 8949-8955
The M(OH)(n)(+) geometries, for n = 1-3, have been optimized and the z
ero-point energies computed using the B3LYP approach. The calculations
show that strong bonds are formed for the early metals, and much weak
er bonds are formed for the late metal atoms. The successive OH bond e
nergies have been computed at the CCSD(T) level for n = 1 and 2. The M
+-OH bond energies are in good agreement with the guided ion beam resu
lts. This implies that the CID values for TiOH+, VOH+, and CoOH+, and
the photodissociation value for CoOH+ are accurate, but that the CID v
alues for ScOH+ and NiOH+ are too small. The B3LYP binding energies ar
e found to be in qualitative agreement with the CCSD(T) results. The r
elative size of the first and second OH binding energies at the B3LYP
level disagrees with the CCSD(T) for Sc+, Ti+, and V+ The B3LYP result
s show that the third OH binding energy for Ti+ and V+ will be large (
85 kcal/mol, or more), while for the remaining systems the third OH is
electrostatically bound, with a binding energy of only about 30 kcal/
mol.