Spectroscopic constants of the (X)over-tilde((1)A(1)), (a)over-tilde(B-3(1)), and (A)over-tilde(B-1(1)) states of CF2, CCl2, and CBr2 and heats of formation of selected halocarbenes: An ab initio quantum chemical study
K. Sendt et Gb. Bacskay, Spectroscopic constants of the (X)over-tilde((1)A(1)), (a)over-tilde(B-3(1)), and (A)over-tilde(B-1(1)) states of CF2, CCl2, and CBr2 and heats of formation of selected halocarbenes: An ab initio quantum chemical study, J CHEM PHYS, 112(5), 2000, pp. 2227-2238
The geometries, rotational constants, harmonic force constants and frequenc
ies, dissociation and term energies of CF2, CCl2, and CBr2 in their respect
ive (X) over tilde((1)A(1)), (a) over tilde(B-3(1)) and (A) over tilde(B-1(
1)) states, computed by complete active space self-consistent field (CASSCF
), complete active space second-order purturbation (CASPT2), and coupled-cl
uster with single, double and perturbative triple excitations [CCSD(T)] met
hods and cc-pVTZ basis sets, are reported. For CCl2 and CBr2 the barriers t
o linearity are also characterized. The computed spectroscopic constants ar
e in good agreement with the available experimental data. The atomization e
nergies and hence heats of formation at 0 and 298 K of these molecules as w
ell as of CHF, CHCl, and CFCl, all in their lowest singlet ground states we
re also computed by the CCSD(T) method utilizing basis sets ranging from cc
-pVDZ to aug-cc-pVQZ, cc-pCVQZ and G3large, enabling the extrapolation of t
he energies to a complete basis set (CBS) limit and the inclusion of core-v
alence correlation (with the exception of CBr2). Scalar relativistic correc
tions, computed by CASPT2, were also taken into account. The final CBS resu
lts are Delta(f)H(298)(0)(CHF)=147 +/- 4 kJ mol(-1), Delta(f)H(298)(0)(CHCl
)=320 +/- 4 kJ mol(-1), Delta(f)H(298)(0)(CFCl)=29 +/- 4 kJ mol(-1), Delta(
f)H(298)(0)(CCl2)=229 +/- 4 kJ mol(-1), and Delta(f)H(298)(0)(CBr2)=337 +/-
8 kJ mol(-1). The GAUSSIAN-3 (G3) heats of formation of these molecules ar
e within 2 kJ mol(-1) of the CBS values, representing significant improveme
nt over the GAUSSIAN-2 predictions which differ from the CBS results by up
to similar to 10 kJ mol(-1). Similarly, the G3 triplet/singlet energy separ
ations are found to be in good agreement with those obtained at the CCSD(T)
/cc-pVQZ level of theory including core-valence correlation corrections, as
well as experiment. (C) 2000 American Institute of Physics. [S0021-9606(00
)30704-8].