Per E. M. Siegbahn*
Department of Organic Chemistry, Arrhenius Laboratory, Stockholm University, SE-106 91, Stockholm, Sweden. E-mail: per.siegbahn@su.se
First published on 15th January 2021
During the past 20 years, quantum chemistry has grown to be a significant part in the investigation of mechanisms for redox-active enzymes. In our group we have developed an approach that has been applied to a large number of such systems. Hybrid density functional theory (hybrid DFT) has from the start of these investigations been the leading electronic structure tool. An understanding of how the method works in practice has significantly improved the accuracy and applicability. During the past ten years, it has been found that the results for redox enzymes mainly depend on the chosen fraction of exact exchange in the functional, and that a choice of 15% has worked best. The idea has therefore been to vary that fraction over a reasonable range and study the relative energy dependence. For modeling the enzymes, a cluster approach has been developed. In the present review the development of the method we used is described from its start in work on photosystem II, fifteen years ago. Examples from a few recent applications are described, where the metals have been iron, nickel, copper, cobalt or manganese. The results are in excellent agreement with available experiments, and a large number of new predictions have been made.
The early applications of hybrid DFT on transition metal containing systems often gave rather accurate energies, which was surprising for many. However, there were sometimes quite large errors that obscured the picture. For example, the binding energy of small molecules to transition metal centers could be underestimated by more than 10 kcal mol−1 compared to very accurate ab initio values. During the first period of DFT applications, entropy effects were not included either, and that made the origin of the errors in the applications less obvious, since there were cancellation effects. Suggestions were made that the errors could be due to dispersion, which are not included in DFT, but dispersion effects were at that time expected to be rather small. Instead, the errors were suggested to come from missing multi-reference effects. The solution to the problem came around 2005 when dispersion effects were systematically studied and empirical methods to accurately take care of them were developed.5 It turned out that the inclusion of dispersion effectively removed the large errors of 10 kcal mol−1 also for transition metal complexes.6 At the same time, it was realized that entropy effects sometimes also needed to be included. The approach most commonly used was to only include the entropy effects in the binding or release of substrates. The approximation made was to assume that only the translational entropy of the substrate was lost upon binding.
Another line of progress concerned the modeling of the enzymes. Two different approaches were tried. In one of them, the entire enzyme was included using the QM/MM (Quantum Mechanics/Molecular Mechanics) method.7 A small QM model of the active site was generally used. In the second approach a much larger QM part was used but without the surrounding MM region of the enzyme.8 This was termed the cluster approach, and is the one that has been used in the studies reported in the present paper.
Perhaps the most important progress in modeling the energetics for redox enzymes, was the deeper understanding of how hybrid DFT works in practice. As will be described below, it was realized that for redox active enzymes, the most sensitive parameter for the relative energies is the fraction of exact exchange used in the functional. Furthermore, the empirical finding was that the optimal fraction was always in the range 10–20%, and also that the relative energies vary essentially linearly with the percentage used.9 This realization also led to a useful way of estimating the accuracy of the results.
In the present review, examples will be described on applications with the hybrid DFT method with a fraction of exact exchange as described above, using the cluster model of the enzyme. The enzymes for which the approach has been applied include the most important enzymes in biology, such as Photosystem II (PSII), nitrogenase and Cytochrome c Oxidase (CcO).10 Excellent results have been obtained in comparisons to experiments, sometimes performed years after the theoretical predictions of the mechanisms were made. A general area for the applications, where this strategy has been applied recently, concerns the enzymes that are most important in a fossil-free and environmental context, such as the ones used in H2 production and CO2 fixation.
An important part of the calculations on the mechanisms of the transition metal containing enzymes discussed here was to consider also the reduction/oxidation (redox) steps. Including these steps has quite generally not been done in most applications by other groups. When the charge of a model changes, after the release or acceptance of a single electron or a proton, the electrostatic effects are very large and they reach far away from the active site. Models of the present size are therefore not appropriate for describing those cases. However, when the redox steps are proton-coupled (PCET), the charge of the active site does not change and the long-range effects are therefore minor. Fortunately, most redox steps in enzymes are of that type. If they are not proton-coupled, an empirical scheme has to be adopted, described in detail below for the case of water oxidation in PSII. Since the enzyme surrounding is essentially the same for all the four redox steps in PSII, only one experimental parameter is needed to describe the long range effects of these steps. The energies for the redox coupled electron transfer steps are then obtained from the experimental redox potential of the substrate, that gives the driving force for the reaction.
For reaching a high accuracy of the results, it is import to have a saturated basis set for describing the electronic structure. For the determination of the structures, a medium size basis set (LACVP*) has been found to be enough.13 For the optimized structures, single point calculations were done with a large basis set, with cc-pvtz(-f) for the non-metal atoms, and with LAV3P* for the metals. The programs used have been Jaguar14 and Gaussian.15
Fig. 1 An optimized structure of the active site (OEC) of PSII. Atoms outside the active site are not shown. |
O2 formation was known to occur after four flashes of light. The intermediate states are termed S-states. For a rather small model of 50 atoms, the key S4 step of O–O bond formation was investigated for a structure derived from the calculations. After many attempts, a transition state was obtained in 2006, which was much lower in energy than the other possibilities tried.19 In fact, the transition state (TS) was so low, that it was immediately realized that it was most probably similar to the one actually used in PSII, even though the model was quite small. Surprisingly, the O–O bond was formed between two oxo ligands, one of them with a high spin, therefore termed an oxo–oxyl mechanism. The leading experimental suggestion at the time was instead an outside water attack on a Mn(V)-oxo ligand,20 which by the DFT calculations19 was found to have a much higher barrier. The high barrier for the water attack mechanism has been confirmed more recently in 2017 by DFT.21 Important for the low barrier of the oxo–oxyl mechanism is that the spins for the atoms involved, the two oxygens and two manganese atoms (Mn1 and Mn4) are alternating, which allowed for a smooth formation of the O–O bond. The TS structure obtained is shown in Fig. 2. For the acceptance of that mechanism, it was important to refine the structure of the active site, which was done a few years later in 2008.22,23 One major finding by the DFT calculations was the presence of an additional bridging oxo ligand, not present in the original X-ray structure. The additional oxo ligand was found to be of key importance for the mechanism.
Fig. 2 An optimized TS structure of the active site of PSII. Only the most important atoms are shown. |
To fully understand the mechanism of water oxidation, it was necessary to energetically follow the entire catalytic cycle, which includes also the oxidation steps.23,24 That had never been done before in any theoretical study for an enzyme. One important factor was to obtain the cost for releasing a (H+,e−)-couple from the OEC, where the electron should go to the P680+ oxidant and the proton should go to water. The approach adapted for PSII was to use the experimental redox potential of 0.8 V for the substrate reaction:
2H2O + 4hν → O2 + 4H+ + 4e− |
Using the measured redox potential of 1.25 V for P680, the highest one in nature, this led to a driving force for the catalytic cycle of −41.5 kcal mol−1. The actually calculated energies for releasing a single (H+,e−)-couple could then be adjusted to match that driving force. An almost equivalent way to reach a similar driving force is to use the experimental energy for a proton in water of −264.0 kcal mol−1, combined with the adjustment of the redox potential to the standard hydrogen electrode (4.281 V). That approach works since the number of electrons and protons released are the same. As noted above, the release of a neutral entity does not have any long-range effects and models with 150–300 atoms, and even smaller ones, were therefore adequate. This is not the case if a single electron or proton is released, in which case the long range effects are very large. To describe those effects would have required much larger models than the ones used, but there was an alternative. Assuming that the structure of the enzyme outside the model is reasonably similar in each transition, a single experimental result is enough for obtaining a good estimate for the effect of the surrounding of the model used. The approach for PSII was to use observations for the S1 to S2 transition, where it was known that only an electron and no proton was released, combined with the fact that there should be only a small driving force for the transition, in order not to waste energy. It is important to note that simply using the experimental value for the redox potential of the oxidant, does not work in the case of the S1 to S2 transition in PSII using limited models because of the unknown and large long-range effects from outside the model.25
There was still one problem that needed to be resolved, and that was the most important one. It was found that the computed values for the release of a (H+,e−)-couple were very sensitive to the DFT functional used. To attack that problem in a systematic way, the experience obtained from using the B3LYP functional for redox active systems was used. As mentioned in Section II, it was discovered that the results were almost exclusively dependent on the fraction of exact exchange used. Therefore, this fraction could be varied to obtain what was known from experiments. For PSII, it was found that a fraction of 15% was optimal. Varying this fraction by changing it to 10 and 20% also gave an estimate of the accuracy of the results. To identify how well the different fractions of exchange in the functionals worked, there was at the time no experimental redox potentials available for comparison, so instead a few qualitative experimental results were used. The most important experimental result was the simple fact that the states from S0 to S3 had been observed. That meant that the energies for those states have to be descending. Also, the energy difference between the S-states should not be very large since the driving force for the entire reaction is rather small. Only B3LYP with 15% was found to give a reasonable energy diagram in agreement with these qualitative experimental findings. Very large errors in the diagrams could be seen using significantly different fractions of exchange in the functionals or using other functionals.25 Since the redox potential for Mn(III) to Mn(IV) enters three times, the error in the redox potential will be multiplied by three from start to end in the energy diagram. Functionals without exact exchange, frequently used in the literature, also gave very large errors. It should be emphasized, that the large number of predictions finally made from the calculations using 15% include many previously unknown facts. For example, the structures and energies for the S0 to S4 states were predicted. For the S0 to S3 states, the predicted structures were found to be in excellent agreement with experiments from free electron laser (X-FEL) experiments performed years later in 2015–2018.26–28 However, the most important prediction was the one for the mechanism for O–O bond formation, see above.19 The actual mechanism could not be directly compared to experiments since the active S4 state is not possible to observe experimentally due to its high energy. Instead, detailed spectroscopic results for the lower S-states could be used to experimentally verify the mechanism in 2011–2012. Of largest importance here were water exchange and EPR experiments.29,30 In the context of modeling mechanisms for redox enzymes, it should finally be noted that it has very surprisingly been found that a fraction of 15% exact exchange is nearly optimal also for all other redox enzymes studied so far, see further below.
Fig. 3 An optimized structure of the active site of CcO, obtained after the cleavage of the O–O bond of O2. |
The mechanism for proton pumping is the most interesting and challenging problem in CcO. The question is how the active site, situated between the inside and the outside of the membrane, is able to pump protons through a channel which is situated outside the active site. Therefore, the chemistry at the active site must be able to direct the protons from the inside to be either consumed in the active site to produce water, or to be pumped across the membrane against the chemical gradient. It has been demonstrated experimentally that for one O2, there are four protons pumped (Hp), and four protons consumed to form water.34
O2 + 8H+ + 4e− → 2*H2O + 4*Hp + ΔE |
This means that two protons have to be transferred from the inside for every electron entering the active site, one for pumping and the other one for consumption. To understand that problem, applications of the methods described here were not enough. Another, more global, approach was also needed. The key was to construct energy diagrams for the entire pumping process, which required use of all available experimental information.35 In particular, the most useful information came from time resolved kinetic experiments.36
It was found necessary to construct very complicated energy diagrams in order to understand proton pumping. The details of the suggested pumping process can be found in the respective papers.10,35 One important realization was that the directions of the protons in the pathways can be determined by long range electrostatic effects from the active site. The charge of the active site has to change in a systematic way, which depends on the number of electrons and protons in the active site. To find the effects from the charges on the different transition states, simple electrostatic models were used, essentially depending only on the distances as given by the X-ray structure, and on the dielectric constant. The different pathways can be divided into allowed, leading to pumping, and non-allowed (leakage) pathways. The accuracy for the differences in energy for the different pathways has to be very high and was not reachable by quantum chemical models alone, but also had to include information from the kinetic experiments mentioned above.36 It was finally possible to rationalize all the experimental observations.10,35 More recently, it was also possible to suggest an explanation for how altogether four protons were pumped for each O2 and why two proton channels had to be used, as observed by experiments.37
Fig. 4 The FeMo-cofactor in Mo-nitrogenase that reduces N2 to NH3.38 |
Apart from the structure of E0, the kinetics of the mechanism has also been determined in detail.41 The most important conclusion was that the activation of N2 occurs after four initial reduction steps in the catalytic cycle. The intermediate states are termed E0 to E4. The overall reaction in Mo-nitrogenase is,
N2 + 8(H+,e−) + 16ATP → 2NH3 + H2 + 16(ADP + Pi) |
A surprise in this reaction is that one H2 is produced in addition to ammonia. Even though the ground state structure has been known for decades, only pieces of the nitrogen activation mechanism has so far been determined from experiments. For example, no other structure than the one for E0 has been determined. The most important finding for the mechanism was made by EPR for the active E4 state.42 It was shown that there are two bridging hydrides, that leave as N2 becomes activated. Therefore, the experiment gives for the first time, an explanation for the release of one H2 for every N2 that is activated. The process was found to be easily reversible in E4. With two hydrides after four reduction steps, the remaining two reductions should lead to two protonations, suggested to be on the sulfides.
The model calculations for the mechanism had to start with a rather limited amount of experimental information, as described above. The ground state structure is known to high precision, and it is known both from experiments and theory to have an oxidation state of Mo3+ 3Fe2+ 5Fe3+. If this fact is combined with the conclusions from the EPR experiments, the oxidation state of the active E4 state obtained after four reductions, should be the same as the one for E0. This is very surprising since the lowest reductant in nature is used and still, the state that reduces N2 should have such a high oxidation state with five Fe3+. To reduce N2, a very low redox state was instead expected. That expectation was confirmed by the calculations, which did not lead to any activation of N2 using the suggested redox state. Furthermore, the suggested structure led to very unstable hydrides, which were found to leave the cofactor in a very exergonic step, which does not match the experimental observations of a reversible step.
The initial model calculations led to the conclusion that the cofactor needs to be reduced further. The question was where the protons, that always accompany the reductions, should go. It was found that it was not energetically possible to continue protonating the sulfides. Instead, an unexpected protonation of the carbide was possible. By protonating the carbide, it was actually possible to make four additional reductions, altogether eight from the ground state E0.43,44 The conclusion that eight reductions from E0 is needed to activate N2 may appear to be in contradiction with the kinetic experiments, which suggest that N2 should be activated after four reductions. However, the conclusion from the kinetic experiments were made under the assumption that there are no activation steps prior to catalysis. The conclusion from the model calculations was thus that there are four initial activation steps, termed A0 to A4, which lead to a formation of a terminal CH3, which should be the new E0. The oxidation state reached for E4 is then Mo3+ 7Fe2+, without any Fe3+. The optimal structure was found to have two bridging hydrides, in agreement with the suggestion by the EPR experiments. The hydrides are bound inside the cluster, in the region where the carbide was previously bound. The structure obtained for E4 is shown in Fig. 5.
It was found that the hydrides leave as H2 in a reductive elimination (re) step, in agreement with the EPR suggestion. The importance of that step is that it creates a very low redox state with Mo3+ 5Fe2+ 2Fe1+, which allows N2 to be reduced. It is also important that H2 does not form from a hydride and a proton, an hp, step, which would only lead back to E2. The calculations indeed found a barrier for the re step which is lower than the hp step, again in agreement with the analysis of the EPR experiments. After a rotation of the homocitrate, N2 binds as shown in Fig. 6.
Again, the calculations find that a fraction of exact exchange of 15% does give a reasonable energy diagram for the entire mechanism, all the way to the formation of two NH3 from one N2.43 In order to test the conclusion that activation steps are really needed, calculations have also been done for the experimentally suggested E4 state with other fractions of exact exchange,9 and with other functionals.45 It was shown that, in fact, no other DFT functional can reproduce the mechanism obtained by experiments using only four reductions before E4. All of them give a much too exergonic release of H2 to be compatible with a reversible step when N2 binds.
It should finally be emphasized, that although the calculations clearly conclude that activation steps before catalysis are needed, the suggestion that the carbide becomes protonated is less certain. Calculations are in progress investigating other possibilities, such as those where the release of H2S is involved. Structures with a missing sulfide have been found by X-ray experiments, but it is not clear that those structures are on the reaction path.
Fig. 7 The X-ray structure of the active site of FeFe-hydrogenase.48 The structure is identified as Hox. |
The formation of H2 requires two reductions, involving proton coupled (H+e−) transfers.
2H+ + 2e− = H2 + ΔE |
There have been many suggestions for the protonation site of the of the structure obtained after the first reduction of Hox, termed Hred. The lowest energy structure, found in essentially all theoretical studies, has a bridging hydride in the Fe-dimer. It is, in fact, much more stable, by 32 kcal mol−1, than the other conformers suggested by experiments. Therefore, the hydride would easily replace the bridging CO. However, vibrational spectroscopy very clearly indicates that there is still a bridging CO in this state, showing that the protonation pathway to the bridging site must be blocked by the enzyme.49 To block such a stable site is a very unusual feature, hardly seen in any other enzyme. Instead, experiments have suggested that the protonation site in the first reduction is either on a ligand of the Fe4S4 cluster,50 or on the ADT ligand of the Fe-dimer.51
Model calculations to find the mechanism for H–H bond formation52 started by investigating the protonation sites suggested for Hred. It turned out that both sites suggested, see above, have very high energies, and they should therefore not be possible to observe, in conflict with the actual experimental observation of that state. Instead, the calculations suggested that a terminal hydride on the empty site of Fed is formed, which is 14 kcal mol−1 more stable than the other suggestions. It should be noted that the bridging hydride state is still 18 kcal mol−1 more stable that the terminal hydride, and therefore, the bridging position still has to be blocked by the enzyme. In the next reduction, forming Hhyd, the proton initially ends up on a cysteine on the Fe4S4 cluster. The observed Hred state gave an energy of −1.0 kcal mol−1 and the one for Hhyd of +3.2 kcal mol−1 compared to the starting Hox state. To form the H–H bond, the added proton in Hhyd moves to the ADT ligand in an endergonic step, which stabilizes the oxidation state of Fed(I), necessary for H–H bond formation. A TS can then be formed either between the proton on ADT and the terminal hydride on Fed, see Fig. 8, or more surprisingly, from a proton on a nearby cysteine and the terminal hydride, see Fig. 9. The latter alternative was actually found to be slightly better by −1.3 kcal mol−1. The barrier is very low, 11.4 kcal mol−1, indicating an extremely fast reaction in agreement with experiments.
As in all the other studies discussed here, the methodology was tested by varying the fraction of exact exchange. Again, the best agreement with experiments was found using 15%, but 10% also gave quite reasonable results. The sensitivity is highest for the Hred intermediate with 8 kcal mol−1 going from 10 to 20%. The sensitivity on the overall barrier height is smaller with only a difference of 1–2 kcal mol−1 going from 10 to 20%. For comparison, calculations were also done for the Hhyd state, using the PW6B95-D3 (ref. 53) and PBE0-D3,54 where the former gave an energy of +12.3 kcal mol−1 and the latter one of +8.3 kcal mol−1 counted from the Hox state. Both these functionals have a higher fraction of exact exchange, higher than the range usually investigated by the present method. Hhyd has been observed and should therefore not have an energy higher than +3 kcal mol−1, probably lower, indicating that those two functionals are not reliable in the case of FeFe hydrogenase.
The most common hydrogenases in nature are ones where the active site has a dimer between nickel and iron, therefore called NiFe hydrogenases. They are mainly used for cleavage of H2, producing protons and electrons. In some of them, the protons are transferred to the outside of the membrane against the gradient, to eventually store energy as ATP. The active site structure, shown in Fig. 10,55,56 has many features in common with the one for FeFe hydrogenase. Most strikingly, there are again ligands which are very unusual in nature, two CN- and one CO bound to the iron. There are also four cysteine ligands, two of them bridging between the metals.
Fig. 10 Optimized structure for the active site of NiFe hydrogenase, based on an X-ray-structure.44,45 |
The early studies on the mechanism all converged to essentially the same type of TS for H–H cleavage. H2 enters in between the metals, and is cleaved heterolytically, leading to a bridging hydride and a proton on Cys543, as described in the review mentioned above.46 The TS obtained in the most recent study is shown in Fig. 11.57 The barrier obtained was 15.2 kcal mol−1, in good agreement with experiments. For the barrier height, it was important to include the loss of entropy, which was estimated to be 8.4 kcal mol−1, and which also led to the finding that no bound state for molecular H2 was present, as was also the case for FeFe hydrogenase, discussed above. When the proton bound to the cysteine was released to the outside, a state with Ni(III) was found, and when also the hydride was released a state with Ni(I) was reached, showing the electronic flexibility needed for nickel. Iron stays Fe(II) throughout.
The accuracy of the calculations were as usual tested by varying the exact exchange fraction. It turned out that the energy of one intermediate was quite sensitive to this variation. A fraction of 15% was again shown to be in best agreement with available experimental information, while the use of 10% gave quite erroneous results. The situation is quite different from the one for FeFe hydrogenase.
Another mechanism than the one above has been suggested from experiments for NiFe hydrogenase under certain conditions.58 It was noted that one of the intermediates that should be present in the heterolytic mechanism was sometimes missing. Model investigations were therefore initiated to find a second mechanism.57,59 The mechanism found from the model calculations was one of a homolytic, rather than a heterolytic, cleavage. The optimized TS is shown in Fig. 12. The catalytic cycle for the homolytic mechanism starts out from one intermediate in the heterolytic cycle, where there is a bridging hydride but no proton on the cysteine. The oxidation state of nickel was Ni(III). When the hydride moved to the cysteine, a state with Ni(I) was formed, which was able to cleave H2 homolytically, with a product that had two hydrides, one bridging and one terminal on nickel. The barriers for the two mechanisms were found to be about the same.
Ni,Fe-CODH uses a cofactor with four irons and one nickel as shown in Fig. 13. It can be described as an Fe4S4-cluster in which one iron has been pushed out by a nickel. The X-ray structure has been determined with a high resolution for an intermediate with a bound CO2.61 Apart from the metal cofactor there is a hydrogen-bonded chain with His93 and Asp219 of probable high significance. There is also a positive lysine (Lys563) that can form a strong hydrogen bond to the substrate. Recently, the mechanism was investigated with the methods described in this review.62 The experimentally suggested oxidation state for the structure in the figure is Ni(II)Fe(III)3Fe(II). An important experimental result is that CO2 reduction is reversible.60 That fact can be used also for testing the accuracy of the results, as described below.
Fig. 13 The X-ray structure of the active site for NiFe-CODH, showing the key intermediate with a bound CO2.61 |
Two reductions with additions of (H+,e−)-couples are needed to activate CO2. The products are CO and water.
CO2 + 2H+ + 2e− = CO + H2O |
The structure in Fig. 13 was the starting point for the model calculations. For the mechanism of NiFeCO-DH, it was found that the His, Asp couple was protonated and that one of the sulfides on the NiFe3 cubane was protonated. The first addition of a (H+,e−)-couple led to a protonation of the bound CO2 and a cleavage of the C–O bond. The reduction by itself ws quite sensitive to the fraction of exact exchange, while the cleavage of the C–O bond was entirely insensitive. The barrier was found to vary by only a few tenths of a kcal mol−1 between 10% and 20%. The product has CO bound to nickel, while the OH− was found to be bound to the iron outside the cube. In the next reduction, a water is formed from the OH-ligand on iron. In the final step, which is not a reduction, the CO bound to nickel is replaced by a new CO2 in the preparation for the next catalytic cycle. The computed energy diagram and structures are in good agreement with experimental knowledge, using 15% exact exchange.
In designing models for CO2 fixation, it is very important to avoid formation of hydrides, which would shortcut the fixation process and instead lead to formation of H2. The pathways for hydride formation were therefore also studied. It was found that the available protons for a possible formation of the hydride were all very strongly bound and can therefore not directly lead to formation of a hydride. However, since a small amount of H2 has been found in NiFe-CODH under certain conditions,63 a process for forming hydrides needed to be explained. The explanation found was that an overreduction could take place to a small extent. With one more reduction, hydrides could form leading to H2 formation.
As mentioned above, the reductions are quite sensitive to the exchange fraction used. However, the variation is very systematic. Each reduction is about 4 kcal mol−1 easier for 10% compared to 15%, and 4 kcal mol−1 harder for 20%. This type of variation is rather common for cases where there is a change of oxidation state of the metals. In order to choose the right fraction for the reduction steps, it is very useful to compare the calculated rates for oxidation and the reverse one of reduction. It has been experimentally found that the rates for reduction and oxidation are similar, with the barrier for oxidation being a few kcal mol−1 lower. It was found that the use of 10% makes the process irreversible, and that fraction should therefore not be used. For 20% the barriers are about the same, which is tolerable, but using 15% reproduces the experimentally found difference in rates very well and is therefore again the best choice.
CO2 + 2e− + H+ = HCOO− |
It can be seen on the overall reaction that there is a complication here that is not present for the other cases discussed in the review. Since the number of protons and electrons involved are not the same, this causes modeling problems. There are two reductions and one of them is therefore not proton coupled, which means that the cost for obtaining an electron has to be estimated for accepting a single electron and that is somewhat uncertain. Therefore, unlike the situation for the hydrogenases, where the only assumption made was a small, reasonable driving force, that procedure would not be enough for Mo-FDH. Instead, the second choice as described for PSII was adopted. That meant the straightforward use of the experimental redox potential, which with a small model may lead to large, somewhat unpredictable long-range effects. Since that approach did not work well for PSII, the value must be taken with caution. For Mo-FDH, it turned out that the approach actually worked very well, which must be considered as being merely a fortunate case. For the purpose of testing the accuracy, it is useful that the reaction has been found to be reversible. If the straight-forward approach had not worked, the value would have to be modified until the reaction became reversible. The work is in progress and will be presented elsewhere.
Fig. 14 The X-ray structure of the active site for a multicopper oxidase.64 |
The mechanism for reduction was found66 to be the same as in the previous studies.68 O2 was found to be bound in the center of the cluster with bidentate bonding to one of the coppers and single bonds to the other ones. The full reduction of O2 requires additions of four (H+e−)-couples.
O2 + 4(H+e−) → 2H2O + ΔE |
Since the reductions are proton coupled, the standard methodology described above can be used. The first reduction became endergonic by +5.1 kcal mol−1, where the proton goes to O2 and the electron to one of the coppers. The O–O bond in O2H was then found to be cleaved in a very exergonic step by −26.7 kcal mol−1. The barrier for that step was found to be 10.9 kcal mol−1. With the endergonicity in the previous steps the total barrier became 16.0 kcal mol−1, in reasonable agreement with experiments, which should be 12–14 kcal mol−1. Three reductions remain to go back to the ground state, two of them exergonic, the last one slightly endergonic.
The above results were obtained with a 15% fraction of exact exchange. With 20%, the total barrier became 20.6 kcal mol−1, significantly worse compared to experiments. For 10%, the barrier became 14.4 kcal mol−1, quite similar to the one for 15%, even slightly better. In conclusion, there were no signs of a breakdown of B3LYP with 15% exact exchange. The results are fully in line with the results for the other enzymes described above.
To obtain agreement with experiments for the oxidation of water was more difficult. To drive the reaction backwards, a high redox potential of 1.25 V was used, and the pH was raised to 10.5. The first three oxidations were unproblematic and became strongly exergonic. At that point a structure was obtained similar to the one for the product of the cleavage of O2H for the reduction. However, trying to go back the same pathway but in the opposite direction as for the reductive cleavage, forming the O–O bond with one oxo and one OH, led to a much too high barrier. However, with the increased redox potential and pH, it was actually possible to oxidize the system even further in an exergonic step. In that step a proton leaves from the water ligand and not from the OH ligand that should form the O–O bond. Reaching a point where two fully deprotonated oxo ligands were formed, was found to be endergonic by +6.9 kcal mol−1. From that point a TS for O–O bond formation between the two oxo ligands was found with a height of only 16.5 kcal mol−1. Adding the endergonicity of +6.9 kcal mol−1 a total barrier of 23.4 kcal mol−1 was obtained, which seems reasonable compared to the results of the electrochemical experiment, where no rate was determined but a very slow reaction was noted.
Fig. 15 Optimized structure of the active site of Acetyl-CoA synthase (ACS) with bound CH3 and CO, based on an X-ray structure.70 |
The catalytic cycle occurs in a complicated sequence of steps, which cannot be described in detail here. The question of the oxidation state of Nip is one of the issues raised for the mechanism of ACS. Therefore, states with Nip(II), Nip(I) and Nip(0) were investigated. The oxidation state of Nid was found to stay Nid(II) with zero spin, in agreement with most suggestions from experiments. Another question has been the order of the binding of CO and CH3 to the complex. It turned out that the order gave very similar rate-limiting barriers. CH3 and CO both bind to Nip, and after that a C–C bond is formed between CO and CH3, with a resulting CO-CH3 ligand bound to nickel. In the next step, the substrate CoA-SH binds to Nip and becomes deprotonated. In the final part of the reaction sequence, a C–S bond is formed leading to the product CoA-S-CoCH3, which leaves the active site. There are five intermediates in that part. Both Nip(I) and Nip(II) were found to be capable of catalyzing the reaction, but not Nip(0). The overall reaction is,
CH3-Co(III)-Cbl + CO + CoA-SH → CoA-S-CH3CO + H+ + Co(I)-Cbl |
The rate-limiting barrier was found to be the delivery of CH3 to Nip from the cobalt in Cbl. The barrier using 15% exact exchange for a triplet state was found to be 14.1 kcal mol−1 in good agreement with experiments. The barriers are very similar for both 10% and 20%. However, for the product the energies differ by about 3 kcal mol−1 between the different exchange fractions, altogether 6 kcal mol−1 between 10% and 20%, with 15% in between, with a linear variation. Since the product has Co(II) while the reactant has Co(III), it is this oxidation state change that leads to the differences. The variation is typical for redox transitions with first row transition metals. For the final part of the reaction forming the C–S bond, there are five intermediates. The use of 15% exchange gives very small energy differences between them of 1–3 kcal mol−1. For 10% and 20%, the energies are also quite similar except for one intermediate. That one occurs for a step where an electron is transferred between Nip(I) and the Fe4S4 cluster, with a corresponding change of redox states. That step is endergonic by +2.5 kcal mol−1 for 10%, exergonic by −1.4 kcal mol−1 for 15%, and exergonic by −6.1 kcal mol−1 for 20%. Since these variations are smaller than the rate-limiting barrier of 14 kcal mol−1, it cannot be definitely concluded which fraction fits experiments best. However, the use of 15% exact exchange gives the smoothest potential surface and should probably be preferred also in this case.
In modeling the enzymes, an approach has been developed the past decades termed the cluster approach. A quantum chemical model of the active site is used with the number of atoms usually in the range 150–300 atoms. This size of cluster should take care of charge effects from the immediate surrounding of the active cofactor. This is usually enough in cases where the charge of the model does not change during the mechanism. That is, for example, the case in the reaction steps where bonds are formed or cleaved and when proton coupled reductions or oxidations occur in the mechanism. When there is a change of charge of the model an empirical scheme is needed. A single empirical parameter is usually enough to describe the long range polarization effects. To take account of strain effects from the enzyme, points along the backbone in the periphery of the model should be fixed. That procedure has been tested by releasing constraints and observing the energetic effects. Usually there were no effect, but if there is a significant effect, a constraint may have to be released.
With the large variety of enzymes where the approach has been tested against experiments with excellent agreement, it is unlikely that many examples will be found where the approach fails. However, a failure can, of course, not be excluded in the future. A close observation of experimental results has to be kept to be aware of possible failures.
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