The accurate calculation and prediction of the bond dissociation energies in a series of hydrocarbons using the IMOMO (integrated molecular orbital plus molecular orbital) methods

Citation
T. Vreven et K. Morokuma, The accurate calculation and prediction of the bond dissociation energies in a series of hydrocarbons using the IMOMO (integrated molecular orbital plus molecular orbital) methods, J CHEM PHYS, 111(19), 1999, pp. 8799-8803
Citations number
30
Categorie Soggetti
Physical Chemistry/Chemical Physics
Journal title
JOURNAL OF CHEMICAL PHYSICS
ISSN journal
00219606 → ACNP
Volume
111
Issue
19
Year of publication
1999
Pages
8799 - 8803
Database
ISI
SICI code
0021-9606(19991115)111:19<8799:TACAPO>2.0.ZU;2-P
Abstract
The IMOMO (integrated molecular orbital+molecular orbital) method was used to accurately calculate and compare with the experiment for the single-bond C-H and C-C bond dissociation energies of a series of hydrocarbons, R-1-R- 2--> R-1+R-2, where R-1 is H or CH3, while the largest R-2 considered is 1, 1-diphenylethyl, C(C6H5)(2)(CH3). While the geometries and zero point vibra tional energies were obtained at the hybrid density function (B3LYP/6-31G) level for the real system, a small system, H-CH3 or CH3-CH3, was used as th e "model" in the IMOMO energy calculation, for which a high level method is used. Of a large number of IMOMO combinations tested, the combination of t he modified Gaussian-2 method (G2MSr) with the restricted open-shell second -order Moller-Plesset perturbation method (ROMP2), the IMOMO(G2MSr:ROMP2/6- 31G(d)) method, yields the best results, and can be used for bond dissociat ion energy predictions of very large molecules. Finally, the IMOMO(G2MSr:RO MP2/6-31G(d)) method was used to predict the C-H bond dissociation energy i n H-C(C6H5)(3) and the C-C bond dissociation energy in CH3-C(C6H5)(3), neit her of which is available experimentally. These predicted values are 75.9 a nd 64.1 kcal/mol, respectively, which are smaller than any other C-H and C- CH3 BDE studied in this paper. (C) 1999 American Institute of Physics. [S00 21-9606(99)30643-7].