Greg M. Anderson,
Iain Cameron,
John A. Murphy* and
Tell Tuttle*
WestCHEM, Department of Pure and Applied Chemistry, University of Strathclyde, 295 Cathedral Street, Glasgow, G1 1XL, UK. E-mail: john.murphy@strath.ac.uk; tell.tuttle@strath.ac.uk
First published on 18th January 2016
The utilization of computational methods to predict reactivity is an increasingly useful tool for chemists to save time and materials by screening compounds for desirable reactivity prior to testing in the laboratory. In the field of electron transfer reactions, screening can be performed through the application of Marcus Hush theory to calculate the activation free energy of any potential reaction. This work describes the most accurate and efficient approach for modelling the electron transfer process. In particular, the importance of using an electron transfer complex to model these reactions rather than considering donor and acceptor molecules as separate entities is highlighted. The use of the complex model is found to produce more accurate calculation of the electron transfer energy when the donor and acceptor spin densities are adequately localised.
Over recent years, a number of research groups have published results demonstrating the ability of a wide range of organic molecules (Scheme 1), in the presence of a strong base (most commonly potassium tert-butoxide), to promote the formation of biaryl products from haloarenes in the absence of any transition metal catalyst.9–18 This research has stemmed from the initial findings of Itami et al.,19 who demonstrated that aryl iodides could be coupled to heteroarenes such as pyridine (used as the reaction solvent) in the presence of potassium tert-butoxide. The proposal of Studer and Curran,20 that these reactions proceed by the base-promoted homolytic aromatic substitution (BHAS) cycle is widely accepted (Scheme 2).
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Scheme 1 Examples of organic molecules shown to promote biaryl coupling reactions in the presence of potassium tert-butoxide. |
Our research group has a strong interest in the application of organic reagents in electron transfer reactions, and has developed a number of neutral organic super electron donors (SED's) that are capable of performing a variety of chemical reductions.21 We have recently proposed the structures for the active electron transfer reagents in a number of these metal-free coupling reactions, based on experimental observations.22,23 For example, donor 19 and/or it's corresponding monoanion has been shown to form from 1 under the reaction conditions employed.22 This was demonstrated by the isolation of the neutral oxidised form of 19 upon quenching with iodine. Traditionally, neutral SED's such as 21 are formed prior to use by reaction of the corresponding disalt, in this instance 20, with sodium hydride.24 However, we have also demonstrated that the disalt 20 can be used directly under the conditions typically used for these metal-free coupling reactions to afford the desired product, indicating the ability of potassium tert-butoxide to generate the organic SED 21 in situ (Scheme 3).22
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Scheme 3 Proposed SED formed from reaction of 1,10-phenanthroline 1 with potassium tert-butoxide (a) and examples of a disalt precursor and neutral SED's used within our research group (b). |
In order to move this chemistry forward, it is desirable to design and develop new, more powerful electron donors that allow the electron transfer to occur at lower reaction temperatures and widen the current substrate scope of aryl iodides and, in some cases, aryl bromides to a broader selection of aromatic substrates. The ability to mediate these transformations at lower reaction temperatures with aryl chlorides would allow for greater competition with transition metal-based reaction conditions. Encouraging steps towards this level of reactivity have already been demonstrated by Dyker et al.,25 who have recently developed a neutral tetra(iminophosphorano)-substituted bispyridinylidene donor with a redox potential exceeding that of neutral organic donors previously developed within our group. This new donor was capable of reactivities previously only accessible using our donors under photoactivated reaction conditions. An attractive means of aiding the design process is the application of computational methods to screen potential electron donors, and their precursors, to determine whether or not they are viable candidates.
The Marcus theory for electron transfer is commonly applied to the study of a number of different chemical systems, ranging from the work of Kochi et al. on the study of ion pair intermolecular electron transfers26–28 to the study of lithium–air batteries by Banerjee and co-workers.29 Similarly, this theory has also been applied within a biochemical context and Blumberger has recently published an excellent review article in which QM/MM has been applied to calculate the energetics for the electron transfer in a modified cytochrome c system.30
Within our own lab, we have previously used computational methods to investigate the relative abilities of neutral SED's to reduce aryl halides.31 In using related methods within this work to investigate the potential ability of candidate organic electron donors, our aim is to ensure that the assumptions made in these calculations are valid. Notable differences between the previous work and the present work are the choice of solvent (previously N,N-dimethylformamide was used; present reactions are performed in benzene) and the charge state of the electron donors (the present proposed electron donors are anionic or dianionic in nature). One crucial aspect of these differences is the treatment of the donor and acceptor molecules as a single complex. The use of electron transfer complexes versus Nelsen's four-point method32 may play a more significant role when considering non-neutral donors and acceptors. Therefore, it is necessary to determine which model most accurately predicts reaction energetics by comparison with experimental observation, as summarised in Fig. 1 below. In addition to this, the formation of the proposed donors by reaction with potassium tert-butoxide is also investigated to determine how effectively the potential donors can be formed under standard reaction conditions. The use of donor–acceptor complexes in Model 2 does not consider the effects of extrinsic factors discussed by Himmel,33 such as solvent reorganisation. However, given the larger solvent exclusion afforded by considering the full complex and the use of a continuum solvent approach, the effect of this approximation should be minimised.
![]() | (1) |
The potential energy surface of two half reactions can be considered as separate parabolas, and thus Marcus Hush theory can be illustrated as per Fig. 2. The intersection of these parabolas represents the activation free energy ΔG*, while the energy difference between the two minima represents the relative free energy ΔGrel. The reorganisation energy λ is interpreted as the vertical energy difference between the minimum of the product curve and the point where the reactant curve overlaps with this on the potential energy surface.
The total reorganisation energy of the system λ is comprised of the internal reorganisation λi (electron donor and acceptor molecules) and the external reorganisation energy λo (i.e., the reorganisation of the solvent in response to the electron transfer). Research published by Kochi26–28 and Banerjee29 has demonstrated that in calculating the overall reorganisation energy, the internal reorganisation energy has a more significant influence on the total reorganisation energy relative to the external reorganisation energy. The opposite of this was observed in Blumberger's study on biological systems.30 However, the current systems under study exist in a non-strongly coordinated medium and as such are more akin to the systems studied by Kochi26–28 and Banerjee.29 Therefore, with this in mind, (eqn (1)) can be reduced to the following (eqn (2)), accounting only for the internal reorganisation energy contribution:
![]() | (2) |
The internal reorganisation energy is calculated as follows (eqn (3)):
![]() | (3) |
λi(D) = (ES(RP) − ES(RS)) + (EP(RS) − EP(RP)) | (4) |
An analogous equation can be written for the electron acceptor. In the above equation, ES(RP) is the energy of the species with the starting electron configuration and the product geometry; ES(RS) is the energy of the optimised starting species; EP(RS) is the energy of the species with the product electron configuration and the starting geometry and EP(RP) is the energy of the optimised product species.
For calculations where electron transfer complexes are used, (eqn (3)) there is only one set of energies (where previously there were independent energies for the respective donor and acceptor molecules) thus affording (eqn (5)) simply as:
λi = λi(DA) | (5) |
The calculated electron transfer energetics for Model 1 (Table 1) show that the activation free energies (ΔG*) for donors 21–23 would result in minimal conversion to the product under the reaction conditions (130 °C in a high-pressure reaction vessel for 3–5 hours). This is most evident for donor 21, which has a calculated activation energy of 54.2 kcal mol−1 (Table 1). Donors 22 and 23 are also predicted to have high reaction barriers (40.2 and 39.5 kcal mol−1 respectively) using Model 1. Moreover, the highly endergonic nature of these reactions implies that even if the electron transfer occurs, the intermediate would be very short lived before collapsing to the reactant state despite the partial cleavage of the C–I bond. Therefore, electron transfer is considered to be extremely unfavourable under the Model 1. However, experimentally, 21–23 are efficient (super) electron donors.
Electron donor | Electron transfer model | |||
---|---|---|---|---|
Model 1 | Model 2 | |||
ΔG* | ΔGrel | ΔG* | ΔGrel | |
21 | 54.2 | 53.2 | 34.1 | 20.3 |
22 | 40.2 | 36.1 | 23.9 | 4.6 |
23 | 39.5 | 33.9 | 27.2 | 14.2 |
The results for Model 2 show that the use of an electron transfer complex produces a significant change in the electron transfer energetics. There is a decrease in the relative free energy of the electron transfer, such that, while still endergonic, the barrier to the reverse reaction is higher (13.0–19.3 kcal mol−1, Table 1) thus making the reverse reaction more difficult relative to Model 1. Moreover, the use of the donor–acceptor complex in the calculation of the electron transfer energetics also results in a significant decrease in the calculated barrier heights by up to 19.3 kcal mol−1 (Table 1). For example, in the case of donor 22 as an example, the activation energy is decreased by 16.3 kcal mol−1, and the relative free energy (ΔGrel) is decreased by 31.5 kcal mol−1, relative to Model 1, resulting in an electron transfer that is only mildly endergonic (ΔGrel = 4.6 kcal mol−1, Table 1). This suggests that the reorganisation of the electron transfer complex is more favourable than the reorganisation of the individual components.
To ensure that the energetics calculated represent the transfer of an electron from the donor to the acceptor, rather than a singlet-to-triplet excitation localised on the electron donor, we probed the HOMO and LUMO of the reactant complex, as well as the spin density of the product complex, the visualisations of which are shown for donor 22 in Fig. 3. Fig. 3a shows that despite the formation of a stable complex, within the reactant complex the HOMO is localised predominantly on the donor molecule, while the Fig. 3b shows that the LUMO is similarly localised on the acceptor. For the product complex (Fig. 3c) the spin density of 2 is distributed relatively evenly across both the donor and acceptor components of the complex (Fig. 3d). A decomposition of the atomic contributions to the spin densities shows that the 1.06 electrons is localised to the acceptor and 0.94 localised across the donor molecule (see ESI Fig. S1 and S3† for corresponding figures of donors 21 and 23).
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Fig. 3 Calculated HOMO (a) and LUMO (b) for the reactant complex and the optimised geometry (c) and calculated spin density (d) for the product complex of donor 22. |
For these proposed donors, three reaction models will be addressed. Model 1, as with the previous section, will again consider the donor and acceptor molecules as separate entities. An alternative to Model 1 will include potassium counter ions (one counter ion for anionic systems, two counter ions for dianionic systems) to balance the charges of these donors, herein referred to as Model 1K. Finally, Model 2 will again represent the calculation of the electron transfer complex, and includes the potassium counter ions to give an overall neutral reaction system.
Electron donor | Model 1 | Model 1K | Model 2 | |||
---|---|---|---|---|---|---|
ΔG* | ΔGrel | ΔG* | ΔGrel | ΔG* | ΔGrel | |
27 | 53.6 | 43.4 | 99.5 | 99.2 | 64.7 | 58.3 |
30 | 50.3 | 38.7 | 92.0 | 91.6 | 64.9 | 58.8 |
33 | 49.6 | 43.5 | 89.7 | 89.6 | 65.7 | 59.5 |
36 | 51.5 | 39.8 | 95.0 | 94.9 | 64.3 | 58.3 |
38 | 49.9 | 44.1 | 85.8 | 88.6 | 65.1 | 58.9 |
40 | 15.3 | −4.0 | 46.7 | 44.8 | 25.5 | 2.9 |
43 | 26.2 | 16.9 | 53.8 | 52.2 | 33.5 | 11.7 |
The inclusion of the potassium counter ion in Model 1K for this series of candidate electron donors, raises the activation and relative free energies significantly. As in Model 1, the amino acid carboxylates are predicted to be inefficient donors, with activation energies, calculated using Model 1K, exceeding 85.0 kcal mol−1 (Table 2). More significantly however, donors 40 and 43 are now also predicted to be inefficient, with their respective activation energies for electron transfer now increased to 44.8 and 52.2 kcal mol−1 (Table 2). This increase across the board in the activation and relative free energies suggests that the simple inclusion of a counter ion to balance the charges in the systems is not beneficial in the calculation of the electron transfer energetics. Therefore, inclusion of the complete donor acceptor complex is required (Model 2) to ensure that the electron transfer energetics are modelled accurately.
With Model 2, we note a significant decrease in the activation and relative free energies relative to Model 1K. However, relative to Model 1, the activation free energies are greater by approximately 10–16 kcal mol−1. For the amino acid carboxylates, this results in activation free energies in the region of 64.0 kcal mol−1, and as such are all considered inefficient donors. This suggests that the singly anionic state investigated is not the experimentally active form of the SED that results from these precursors. Interestingly, with donors 40 and 43, we observe that the predicted activation free energies are once again accessible under the reaction conditions employed, at 25.5 and 33.5 kcal mol−1, respectively. Moreover, the product state for 43 is further stabilised when it is treated as a complex, rather than the individual donor and acceptor molecules (Model 1, Table 2).
As with the neutral donors in the previous section, the reactant complex orbitals and product complex spin densities were investigated, and this yielded an unexpected result for the amino acid carboxylate complexes. A spin density of ∼1 should exist on both the donor and acceptor molecules, in systems such as 30 (Fig. 5a), which is observed (spin densities for the product complexes of all species investigated are available in the ESI, Fig. S4–S21†). However, the spin density on the acceptor molecule is localised onto the iodine atom, which is more typical of a homolytic bond scission of the neutral acceptor molecule rather than the radical anion that would result from electron transfer. This shows that within the singly anionic state these compounds are indeed not acting as electron donors. In contrast, donors 40 and 43, display the expected spin density distribution across the donor and acceptor molecules, illustrated using 43 (Fig. 5b).
In the case of precursors 2–4, there are two options for further deprotonation following the formation of the respective carboxylate anion; C–H deprotonation at the α-carbon (affording proposed donors 28, 31 and 34), or N–H deprotonation at the amine centre (affording proposed donors 29, 32 and 35). Structures 28, 31 and 34 should represent stronger electron donors due to the formation of an electron-rich alkene, analogous to that observed in neutral organic SED's such as 22. However, structures 29, 32 and 35 could still represent active electron donors, despite the fact that the two negative charges in these structures are localised.
The two dimethylated variations of glycine, precursors 24 and 25, can form only one dianionic species each (37 and 39), upon deprotonation of carboxylates 36 and 38, owing to the substitution at the α-carbon and amine positions, respectively. For dianions 41 and 42, the only difference is the presence of an alkene moiety linking the two anionic nitrogen centres, allowing the importance of this to be investigated. Dianion 44, if formed in situ, is predicted to be a powerful electron donor due to its antiaromaticity. This antiaromaticity would be a very strong driving force for electron transfer, as loss of two electrons from this would afford an aromatic species, again drawing similarity to the neutral organic SED's discussed previously.
The calculated energetics for these dianionic organic electron donors are summarised in Table 3. Using Model 1, it is predicted that all dianionic species represent very powerful electron donors, with the highest activation barrier calculated at a mere 2.7 kcal mol−1. This in contrast to the experimental observation that using amino acids 24 and 25 as initiators in biaryl coupling reactions leads to poor yields. This observation implies that dianions 37 and 39, if formed in situ, are inefficient electron donors. We believe that this disagreement between theory and experiment suggests that Model 1 is unable to provide a realistic representation of the electron transfer energetics for these highly charged species.
Electron donor | Model 1 | Model 1K | Model 2 | |||
---|---|---|---|---|---|---|
ΔG* | ΔGrel | ΔG* | ΔGrel | ΔG* | ΔGrel | |
28 | 0.2 | −64.5 | 33.0 | 22.9 | 15.2 | −14.9 |
29 | 1.8 | −39.1 | 43.9 | 42.3 | 25.9 | 1.3 |
31 | 0.2 | −62.3 | 35.7 | 28.3 | 19.1 | −8.8 |
32 | 1.8 | −41.7 | 38.9 | 35.7 | 25.4 | −1.5 |
34 | 0.6 | −60.2 | 31.5 | 23.2 | 11.3 | −14.0 |
35 | 2.7 | −39.7 | 40.0 | 36.5 | 25.5 | −4.9 |
37 | 1.9 | −40.8 | 43.2 | 41.4 | 30.5 | 3.9 |
39 | 0.7 | −54.9 | 36.2 | 27.7 | 20.3 | −8.0 |
41 | 2.0 | −41.6 | 40.6 | 37.6 | 24.2 | −6.0 |
42 | 0.3 | −71.8 | 27.7 | 18.8 | 3.0 | −25.6 |
44 | 1.1 | −53.6 | 31.6 | 18.5 | 15.0 | −11.8 |
Using Model 1K, some differences become more obvious in the comparison of potential donors formed from amino acids (precursors 2, 3, 4, 24 and 25). With this model, it is apparent that dianions 28, 31, 34 and 39 are all predicted to have activation energies approximately 3–10 kcal mol−1 lower than donors 29, 32, 35 and 37 respectively. This offers support for the proposal that the dianions formed from C–H deprotonation do afford electron donors stronger than those formed from N–H deprotonation of amino acid carboxylates. In the case of the proposed donors 41 and 42, both derived from precursor 6, there is a difference in activation energy of approximately 13.0 kcal mol−1 when the alkene moiety is included in Model 1K. Similar to the amino acid subset, this shows that it is clearly important to have an electron-rich alkene present to delocalise the negative charges. For donor 44, Model 1K predicts an activation energy of 31.6 kcal mol−1, which is achievable under the reaction conditions used.
The use of the donor–acceptor complexes (Model 2) for these systems leads to a significant decrease in both the activation and relative free energies for all the proposed donors relative to Model 1K. As was observed for the monoanionic donors, despite the decrease relative to Model 1K, these energies are greater than those obtained using Model 1. For donors 28, 31, 34 and 39 the activation free energies decrease by approximately 16.0 kcal mol−1 each compared to Model 1K, making all four easily accessible under the reaction conditions. The activation free energies for the corresponding dianions formed by N–H deprotonation (donors 29, 32, 35 and 37) also decrease by approximately 13.0 kcal mol−1 moving from Model 1K to Model 2, again bringing these candidates below the upper limit of activation. Comparing these two subsets, we note that Model 2 maintains the trend that dianions formed from C–H deprotonation of amino acid carboxylates afford more effective electron donors than those formed from N–H deprotonation. This is evidenced by both a lower activation and relative free energy for donors 28, 31, 34 and 39. The two dianions formed from precursor 6 (41 and 42) demonstrate the same trend as was observed using Model 1K, in that the presence of the alkene moiety leads to a more effective electron donor (their respective activation energies amounting to 24.2 and 3.0 kcal mol−1). For dianion 44, derived from a double deprotonation of 26, an accessible activation free energy of 15.0 kcal mol−1 is predicted using Model 2.
With the energetics for the reduction of an aryl iodide by the charged donors 27–44 established, it is clear that the differences in activation energy for the electron transfer from donors derived from both effective and ineffective precursors (based on experimental observation) are not always sufficient to account for the observed difference in activity. For example, using precursor 3 as an additive leads to efficient coupling, while the use of 25 does not. The results from Marcus Hush theory using Model 2 indicate a difference in activation free energy of only 1.2 kcal mol−1 between dianions 31 and 39, indicating that the electron transfer reaction is not the limiting step in these reactions. Therefore, the formation of the active species must be the limiting step for the inactive compounds.
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Scheme 4 Summary of proposed pathways towards the donor candidates investigated in this work. Reactions in blue indicate pathways that were modelled in detail. |
Looking at the energetics for the formation of dianions 28, 31, 34 and 39 (Table 4) it is noted that these reactions are disfavoured when we consider the free energy, with the reverse reaction being strongly favoured. In order to illustrate that the calculated structures represent true maxima and minima, the electronic energies are also provided, which show the relative energy to be lower than the activation energy. Interestingly, for the deprotonation leading to 39, we note that there is an approximate 10.0 kcal mol−1 increase in the activation energy relative to the remaining amino acid dianions (entries 1–3), likely to be a consequence of the additional allylic strain imparted on the molecule in forming the enolate.
Deprotonation reaction step | Gibbs free energy | Electronic energy | ||
---|---|---|---|---|
ΔG* | ΔGrel | ΔE* | ΔErel | |
27 → 28 | 14.7 | 16.2 | 17.1 | 16.2 |
30 → 31 | 13.6 | 15.7 | 16.1 | 15.1 |
33 → 34 | 14.3 | 15.4 | 15.2 | 14.4 |
38 → 39 | 24.4 | 23.2 | 26.7 | 25.6 |
26 → 43 | 3.6 | 0.23 | 5.5 | −0.1 |
43 → 44 | 12.4 | 12.6 | 13.7 | 12.7 |
The instability of the dianions resulting from these deprotonations suggests that for an electron transfer to occur the true activation energy for the electron transfer should include the energy required to reach the dianion, as it will have a limited lifetime once formed. For example, the electron transfer from 31 requires the formation of 31 from 30 in an endergonic reaction of 15.7 kcal mol−1 (Table 4), with the subsequent electron transfer requiring an activation energy of 19.1 kcal mol−1 (Table 3). Therefore, for 3 to act as an electron donor, the initial exothermic reaction to form 30 takes place in a barrierless reaction, which then requires 34.8 kcal mol−1 for the formation of electron donor 31 and the immediate transfer of the electron to the 4-iodoanisole acceptor. If the acceptor is not present then 31 will collapse back to 30 without the transfer of an electron. Nonetheless, the overall barrier for electron transfer of 34.8 kcal mol−1 is still achievable under the reaction conditions, which require the reaction to be performed at 120 °C. A similar analysis applies to donors 28 and 34, which have comparable energetics to 31.
In contrast, for 39, the initial formation of 38 also occurs in a barrierless reaction. However, the increased endergonicity for the formation of 39 (23.2 kcal mol−1, Table 4) results in a significantly larger overall barrier for the electron transfer from 39 of 43.5 kcal mol−1 (23.2 kcal mol−1 for formation of 39 and 20.3 kcal mol−1 for the electron transfer, Table 3). This higher activation energy for the electron transfer is not accessible under the reaction conditions.
For the two deprotonations of precursor 26 (entries 5 and 6), we note two accessible barriers for the first and second deprotonations (3.6 and 12.4 kcal mol−1 respectively). For the deprotonation leading to 44 (entry 6), the electronic energy values again demonstrate that the structures correctly represent a reaction maximum and two reaction minima.
Candidates that are predisposed to form an electron-rich alkene upon reaction with a strong base, such as that found in donors 31, 42 and 43, are able to produce efficient electron donors. The exceptions to this proposition are instances where the precursor has significant substitution on any of the groups α to where the alkene would be formed, such as in the formation of donor 39 which has an overall barrier to electron transfer of 43.5 kcal mol−1.
Footnote |
† Electronic supplementary information (ESI) available: Optimised reaction coordinates and geometries, Model 2 HOMO, LUMO and spin density graphics. See DOI: 10.1039/c5ra26483a |
This journal is © The Royal Society of Chemistry 2016 |