Table 2.
(Activation/Reaction) Potential Energies, Enthalpies and Free Energies of the π(SFeIII = 5/2)-Controlled H-Atom Abstraction from the Native Substrate by the (SyrB2)FeIV═O and (TMG3tren)FeIV═O Species; the Intrinsic Reaction Barriers Are Also Given (All Values Are in kcal mol−1)
system | ΔE≠/ΔH≠/ΔG≠ | ΔE°/ΔH°/ΔG° | ΔE≠intr/ΔH≠intr/ΔG≠intr |
---|---|---|---|
(SyrB2)FeIV═Oa | 23.1c/18.9/19.8 | 3.9/0.6/2.3 | 21.1/18.6/18.6 |
(TMG3tren)FeIV═Ob | 25.3/21.6/21.4 | 5.9/3.2/0.5 | 22.3/20.3/21.6 |
Within the cluster model from Figure 9, the second-shell residue Arg254 appears to sterically destabilize the transition state/product relative to the reactant by ~ 3–4 kcal mol−1. Here, the DFT results are presented for the cluster model in the absence of this Arg residue. For the energetics of the Arg-including cluster model of the active site from Figure 9, see Table S1.
Calculated at the same level of theory as SyrB2 (described in Computational Details) but with a dielectric constant of ε = 35.7 mimicking the solvation effect of acetonitrile.
The Fe–O bond length at the TS for HAA is ~ 1.8 Å (Figure S9). For this Fe–O bond distance, the excited dxzπ* → dz2σ* state (active in HAA) is calculated at the CASPT2 level of theory to lie ~ 10 000 cm−1 (~ 28 kcal mol−1) above the ground state minimum (Figure 8). This energy difference includes (i) the ground-state Fe–O distortion that is associated with the energy increase by ~ 5000 cm−1 (~ 14 kcal mol−1) and (ii) the excitation from the ground state to the dxzπ* → dz2σ* state that requires an additional amount of ~ 14 kcal/mol. The difference of ~ 28 kcal mol−1 taken from Figure 8 relative to the DFT-calculated π-controlled HAA barrier of ~ 23 kcal mol−1 (ΔE‡ for comparison to PES calculations) reflects the interaction of the FeIV═O moiety with the substrate C–H bond.