Supplementary material for González-Luque (2000) Proc. Natl. Acad. Sci. USA 97 (17), 9379-9384.
Table 3.
S0, S1, S2 state averaged CASSCF and CASPT2 total and relative (DE) energies for the PSB11 model 1Structure | State | CASSCF au | CASPT2 au | w * | D E eV(kcal mol-1) |
Planar FC | S 0 | -441.14129 | -442.43024 | 0.680 | 0.00 (0.00) |
S 1 | -441.01678 | -442.33585 | 0.663 | 2.57 (59.3) | |
S 2 | -440.98174 | -442.29793 | 0.662 | 3.60 (83.0) | |
Planar SP | S 0 | -441.11745 | -442.41907 | 0.674 | 0.30 (7.0) |
S 1 | -441.03140 | -442.34230 | 0.666 | 2.39 (55.2) | |
S 2 | -440.99894 | -442.31735 | 0.655 | 3.07 (70.8) | |
Twist 8° | S 0 | -441.11771 | -442.41923 | 0.675 | 0.30 (6.9) |
S 1 | -441.03144 | -442.34220 | 0.666 | 2.40 (55.4) | |
S 2 | -440.99895 | -442.31737 | 0.644 | 3.07 (70.8) | |
Twist 18° | S 0 | -441.11491 | -442.41689 | 0.674 | 0.36 (8.4) |
S 1 | -441.03193 | -442.34276 | 0.666 | 2.38 (54.9) | |
S 2 | -440.99632 | -442.31532 | 0.155 | 3.12 (72.1) | |
Twist 44° | S 0 | -441.10537 | -442.40855 | 0.673 | 0.59 (13.6) |
S 1 | -441.03556 | -442.34661 | 0.666 | 2.28 (52.6) | |
S 2 | -440.98781 | -442.30735 | 0.512 | 3.34 (77.0) | |
Twist 68° | S 0 | -441.08366 | -442.38714 | 0.671 | 1.17 (27.0) |
S 1 | -441.04185 | -442.35860 | 0.666 | 1.95 (45.0) | |
S 2 | -440.97429 | -442.28905 | 0.411 | 3.84 (88.6) | |
Twist 90° CI | S 0 | -441.07403 | -442.36984 | 0.672 | 1.64 (37.8) |
S 1 | -441.04919 | -442.37170 | 0.665 | 1.59 (36.7) | |
S 2 | -440.97446 | -442.27591 | 0.224 | 4.20 (96.9) |
The basis set used is ANO-S (see Computational Methods for details).
*Weight of the CASSCF reference function (i.e., the zero-order function) in the first-order function.
CASPT2 refers to standard CASPT2 results with no level shift applied. In four cases, due to the occurrence of intruder states, calculations using a level shift of 0.1 au also were carried out [CASPT2 (LS = 0.1 au)]. It was done to check how "reasonable" the standard CASPT2 results are when the reference weight is low ( results). It was concluded, that in spite of the low weights, the corresponding results can be confidently used. Another possibility is to use the LS = 0.1 au results for those () cases. A full calibration vs. the variation of the LS parameter (LS = 0.0, 0.1, 0.2, 0.3, 0.4) has not been performed.