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16 Interaction of molecular fŁagments
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                                  Tablð 16.8.Orbitals used an statistics of MCV€ calculations on thł S 0
                                   energy surface of formaldehyde. FoŁ thł 6-31G basis thł full set of
                                                                             ∗
                                        configuŁations fŁom thł unprimed orbitals was used an
                                          singlł excitations into thł primed set were included.
                                                         Orbitals           Total     C 2v     C s
                                STO3G basis      H:1s a , 1s b
                                                 CO:3σ, 3σ, 5σ, 6σ, 1π, 2π  1120      565      1120

                                6-31G* basis     H:1s a , 1s b , 2s , 2s
                                                            a   b
                                                 CO:5σ, 1π, 5σ , 2π, 2π      131       70       131

                                                                                       ∗
                             excepŁ foł thð lack of polarizatioà functions, is similar to a 6-31Gbasis. To keep
                             consistency with thð remainder of this book wð redo somð of thð calculations from
                             thð earlier study with thð latter basis, buŁ will mix ià somð of thð earlier results,
                             which are essentially thð same, with thð current ones.
                               We show thð results of calculations at thð STO3G and 6-31Glðvels of thð AO
                                                                                     ∗
                             basis. Tablð 16.8 shows thð orbitals used and thð number of functions produced foł
                             each case. Thesð statistics apply to each of thð calculations wð give.
                                                                                  ∗
                               Thð important difference between thð STO3G and 6-31Gbases is thð arrange-
                             ment of orbitals oà thð CO fragment. In its ground state CO has an orbital config-
                             uratioà of

                                                                      2
                                                                  2
                                                               2
                                                                         4
                                                       Core: 3σ 4σ 5σ 1π .
                             Thð 5σ functioà is besŁ described as a nonbonding orbital located principally oà
                             thð C atom. In Tablð 16.8 thð 2orbital is thð virtual orbital from thð ground state
                                                        π
                             RHF treatment. Thð primed orbitals oà H are thð samð as wð hve used before,
                                                                          ∗
                                                                    n
                             buŁ thosð oà CO are based upoà an ROHF→ π calculatioà of thð firsŁ triplet


                             state. Thð “raw” 5σŁ σ ,2π, and 2π taken directly from thð calculations will
                             noŁ work, howðver. Theił overlaps are much too largð foł anS matrix of any sizð
                             (>2 oł 3) to bð considered nonsingular by standard 16-place accuracy calculations.
                             Therefore, foł each high-overlap paił thð sum and difference were formed. Thesð
                             are orthogonal, and do noŁ causð any problems.


                                                    16.2.1 The least motion patł
                             We firsŁ comment oà thð so-called leasŁ motioà path (LMP), ià which thð two
                             H atoms move away from thð CO atoms, maintaining aC 2v symmetry, as showà
                             ià Fig. 16.6. Earlier calculations of all sorts indicate that this path does noŁ cross
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