T. Helgaker et al., THE PREDICTION OF MOLECULAR EQUILIBRIUM STRUCTURES BY THE STANDARD ELECTRONIC WAVE-FUNCTIONS, The Journal of chemical physics, 106(15), 1997, pp. 6430-6440
A systematic investigation has been carried out of the accuracy of mol
ecular equilibrium structures of 19 small closed-shell molecules conta
ining first-row atoms as predicted by the following standard electroni
c nb initio models: Hartree-Fock (HF) theory, Moller-Plesset theory to
second, third, and fourth orders (MP2, MP3, and MP4), coupled-cluster
singles and doubles (CCSD) theory; CCSD theory with perturbational tr
iples corrections [CCSD(T)], and the configuration-interaction singles
and doubles (CISD) model. For all models, calculations were carried o
ut using the correlation-consistent polarized valence double-zeta (cc-
pVDZ) basis, the correlation-consistent polarized valence triple-zeta
(cc-pVTZ) basis, and the correlation-consistent polarized valence quad
ruple-zeta (cc-pVQZ) basis. Improvements in the basis sets shorten the
bond distances at all levels. Going from cc-pVDZ to cc-pVTZ, bond dis
tances are on the average reduced by 0.8 pm at the Hartree-Fock level
and by 1.6 pm at the correlated levels. From cc-pVTZ to cc-pVQZ, the c
ontractions are about ten times smaller and the cc-pVTZ basis set appe
ars to yield bond distances close to the basis-set limit for all model
s. The models HF, MP2, and CCSD(T) give improved accuracy at increased
computational cost. The accuracy of the Moller-Plesset series oscilla
tes, with MP3 being considerably less accurate than MP2 and MP4. The M
P2 geometries are remarkably accurate, being only very slightly improv
ed upon at the MP4 level for the cc-pVQZ basis. The CCSD equilibrium s
tructures are only moderately accurate, being intermediate between MP2
and MP3. The accuracy of the CCSD(T) model, in contrast, is high and
comparable to that observed in most experimental studies and it has be
en used to challenge the experimentally determined equilibrium structu
re of HNO. The CISD wave function provides structures of low quality.
(C) 1997 American Institute of Physics.