Abstract
The geometries and relative stabilities of TiH2-6 with Oh and D3h symmetry and of VH-6 with Oh, D3h and C3v symmetry are calculated with ab initio molecular orbital methods using effective core potentials for Ti and V. With inclusion of electron correlation using quadratic CI (QCISD(T)) and coupled cluster (CCSD(T)) theory the D3h form of TiH2-6 is predicted to be slightly (≈3 kcal/mol) lower in energy than the octahedral form. At the same level of theory the C3v form of VH-6 is calculated as ≈50 kcal/mol more stable than the Oh form and ≈3 kcal/mol more stable than the D3h form. Energy calculations using Møller-Plesset perturbation theory show strongly oscillating results at the MP2, MP3 and MP4 level and thus, are not reliable for estimating relative energies of transition metal complexes.
Original language | English |
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Pages (from-to) | 109-117 |
Number of pages | 9 |
Journal | Chemical Physics Letters |
Volume | 194 |
Issue number | 1-2 |
DOIs | |
State | Published - 19 Jun 1992 |
Externally published | Yes |