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. 2023 Jan 23;3(2):429–440. doi: 10.1021/jacsau.2c00575

Table 1. d-Orbital Populations on CoII in 1 from Various Methodsa.

d-orbital idealized MM-experimental MM-theoretical ab initio (KD1) ab initio (KD2)
dxz 1 1.05 (13.6%) 1.14 (15.4%) 1.000 1.000
dyz 1 1.38 (17.9%) 1.14 (15.4%) 1.000 1.000
dxy 1 1.47 (19.1%) 1.33 (17.9%) 1.282 1.089
dx2 – y2 2 1.97 (25.5%) 1.75 (23.6%) 1.715 1.903
dz2 2 1.84 (23.8%) 2.06 (27.7%) 2.000 2.000
total 7 7.71 7.43 6.997 6.992
a

For ab initio, the d-orbital populations have been obtained by directly taking the weights of (1) and (2) as the face value of dxy and dx2 – y2. This has been done both for KD1 and KD2. For MM, this is the conversion from refined multipole parameters on CoII. See text for more details.