Abstract
In order to shed light on metal-dependent mechanisms for O-O bond cleavage, and its microscopic reverse, we compare herein the electronic and geometric structures of O2-derived binuclear Co(III)- and Mn(III)-peroxo compounds. Binuclear metal peroxo complexes are proposed to form as intermediates during Mn-promoted photosynthetic H2O oxidation, and a Co-containing artificial leaf inspired by Nature’s photosynthetic H2O oxidation catalyst. Crystallographic characterization of an extremely activated peroxo is made possible by working with substitution inert, low-spin Co(III). Density functional theory (DFT) calculations show that the frontier orbitals of the Co(III)-peroxo compound differ noticeably from the analogous Mn(III)-peroxo compound. The highest occupied molecular orbital (HOMO) associated with the Co(III)-peroxo is more localized on the peroxo in an antibonding π*(O-O) orbital, whereas the HOMO of the structurally analogous Mn(III)-peroxo is delocalized over both the metal d-orbitals and peroxo π*(O-O) orbital. With low-spin d6 Co(III), filled t2g orbitals prevent π -back-donation from the doubly occupied antibonding π*(O-O) orbital onto the metal ion. This is not the case with high-spin d4 Mn(III), since these orbitals are half-filled. This weakens the peroxo O-O bond of the former relative to the latter.
Introduction.
Photosynthesis is one of the most important biochemical processes for maintaining aerobic life on this planet.1,2 This process involves capturing solar energy in chemical bonds via the catalytic oxidation of H2O, the extraction of electrons, and formation of O2 as a by-product.3–6 Nature had three billion years to refine this highly efficient Mn-containing catalyst, which is referred to as the oxygen evolving complex (OEC). The OEC consists of a CaMn3O4 cubane with a dangling Mn ion. Insights into the mechanism of water oxidation and O2 evolution, as well as its microscopic reverse, would contribute to the development of solar fuel cells. The O–O bond forming step is not well understood7 since it follows the rate-determining step in the mechanism.8–12 An unobserved Mn-peroxo intermediate is proposed to form,9–11 followed by the rapid release of O2.13 Despite the fundamental importance of manganese-dioxygen chemistry, it remains relatively unexplored.14–16 Small molecules provide an advantage in that lower temperatures can be accessed by using organic solvents, thereby providing an opportunity to observe metastable intermediates. Mononuclear Mn-peroxo complexes include side-on η2-bound peroxo [MnIII(O2)(13‐TMC)]+,17 and [MnIII(O2) 4-N4py]+.18 There are fewer examples of binuclear Mn peroxo compounds, and no examples of Mn clusters containing a coordinated peroxo. Our group reported the first example of a spectroscopically and structurally characterized, metastable binuclear peroxo-bridged Mn(III) complex derived from dioxygen.14,19 In addition, we have examined the effect of coordination environment on peroxo O-O bond lengths.20
The inherent instability and reactive nature of dinuclear Mn(III)-peroxo complexes, both posited in nature and their synthetic analogues, renders the experimental investigation of their electronic and geometric structures difficult. Most of the reported complexes are mononuclear Mn(III)-peroxo compounds with a peroxo moiety bound in a side-on (η2) binding mode.15,21–24 There are very few examples of structurally characterized multi-nuclear Mn(III)-peroxo complexes.25,26 We reported the first crystallographically characterized binuclear example, {[MnIII(SMe2(6-Me-DPEN))]2(µ-O2)}2+ (1) derived from O2. [MnII(SMe2(6-Me-DPEN))]+ (2) binds dioxygen, the microscopic reverse of photosynthetic O2 evolution by the OEC, on the millisecond timescale to form a superoxo intermediate, which then converts to 1, en route to a binuclear µ-oxo end-product, {[MnIII(SMe2(6-Me-DPEN))]2(µ-O)}2+ (3).26 The isolation of peroxo complex 1 was possible because the rate-determining step was determined to be the O–O bond cleaving step.26 The N-heterocycles (NAr) of [MnII(SMe2(6-Me-DPEN))]+ (2) can be derivatized providing a convenient method for determining how steric and electronic properties affect the stability of metastable dioxygen intermediates.19 Manganese dioxygen intermediates are not observed in the absence of steric bulk, for example with a H-substituent in the 6-position, [MnII(SMe2(6-H-DPEN))]+ (4), or with primary amines in the ligand scaffold, [MnII(SMe2N4(tren))]+ (5). Our group has shown that steric bulk increases metal ion Lewis acidity by lengthening metal-ligand bonds, resulting in a stronger peroxo O-O bond.27
More recent work by our group has led to the observation of two new metastable peroxo intermediates formed in the reaction between O2 and thiolate-ligated Mn(II) derivatives (Figure 1) of 2, [MnII(SMe2(6-MeO-DPEN))]+ (6) and [MnII(SMe2(quinoEN))]+ (7).19,26 Changing the steric bulk and electron donor character of the ligand was shown to affect the barriers to O2 binding and release, as well as O–O bond cleavage.17 The less sterically encumbered 6-MeO-pyridine complex 6 binds O2 more readily than the other derivatives, 2 and 7, and O2 release from the superoxo is more favored. In addition, the 6-MeO-pyridine complex forms a total of four metastable intermediates with dioxygen, two of which follow a peroxo, en route to a mono oxo-bridged dimer product.19 Thiolate ligands (RS−) were incorporated, because they have been shown to lower the activation barrier to O2 binding,28,29 as well as provide a convenient spectroscopic handle for observing reactive dioxygen intermediates.30
Figure 1.
Chemdraw depictions of [MnII(SMe2(6-Me-DPEN))]+ (2), [MnII(SMe2(6-H-DPEN))]+ (4), [MnII(SMe2(6-MeO-DPEN))]+ (6), and [MnII(SMe2(quinoEN))]+ (7), [MnII(SMe2N4(tren))](PF6) (5) and [CoII(SMe2N4(tren))](PF6) (8).
The photosynthetic OEC’s dioxygen evolving properties can also be mimicked by cobalt complexes, the most notable example being Nocera’s bioinspired artificial leaf.5,31 Discrete molecular Co4O4 cubane clusters, such as [Co4O4(OAc)4(py)4]+, have also been shown to evolve O2 upon the addition of OH−.32 A Co-peroxo is proposed to form as an intermediate, however, it was not observed. The mechanism is proposed to involve an oxidized trapped valence CoIII2CoIV2 cubane cluster, and coupling between two oxyls on an adjacent CoIV2 pair (O-CoIV-CoIV-O → •O-CoIII-CoIII-O• to afford an unobserved CoIII-O-O-CoIII peroxo.31
The mechanism for the O–O bond forming step is likely to be different for Co and Mn, given that the oxo wall separates them:33 the former is almost certain to proceed via an oxyl coupling mechanism,12 whereas the latter could proceed via a nucleophilic attack mechanism involving M-OH (M= Ca(II) or Mn(III)) and Mn(V)=O intermediates.34 Developing a better understanding of the geometric and electronic structural differences between small molecule Mn(III) and Co(III) peroxo complexes, and the properties critical to O2 release,12 is likely to shed more light on these reactions, and provide insight into metal-dependent mechanisms. There are many examples of synthetic Co(II) complexes that readily react with molecular O2 at room temperature to form isolable dinuclear µ-peroxo Co(III) complexes, including a crystallographically characterized pac-man Schiff-base calixpyrrole-ligated binuclear Co(III) peroxo,35 and a crystallographically characterized fused pincer-ligated binuclear Co(III) peroxo complex.36–41 However, there are few (if any) structurally analogous pairs of binuclear µ-peroxo-bridged Co(III) and Mn(III) complexes. Whereas Mn(III) peroxo complexes are metastable, the added stability of low-spin d6 transition-metal complexes is likely to stabilize a small molecule Co(III) peroxo, making it easier to obtain a structure. Described herein, is a crystallographically characterized, O2-derived thiolate-ligated Co(III)-μ-peroxo complex, which is structurally analogous to our previously reported series of O2-derived Mn peroxo complexes.19,26
Experimental.
General Methods.
All manipulations were performed using Schlenk line techniques or under a N2 atmosphere in a glovebox. Reagents and solvents purchased from commercial vendors were of highest available purity and were used without further purification unless otherwise noted. MeOH (Na) and MeCN (CaH2) were dried and distilled prior to use. Acetonitrile, Diethyl ether, and THF were rigorously degassed and purified using solvent purification columns housed in a custom stainless-steel cabinet and dispensed by a stainless-steel Schlenk-line (GlassContour). [CoII(SMe2N4(tren))](PF6) (8) was prepared according to literature procedures.42 NMR spectra were recorded on a Bruker DPX 500 FTNMR spectrometer and referenced to the residual protio solvent. Electrospray-ionization mass spectra were obtained on a Bruker Esquire Liquid Chromatograph-Ion Trap mass spectrometer. Cyclic voltammograms were recorded in MeCN solutions with Bu4N(PF6) (0.100 M) as the supporting electrolyte, using an EG&G Princeton Applied Research potentiostat with a glassy carbon working electrode, an SCE reference electrode, and a platinum auxiliary electrode. Electronic absorption spectra were recorded using a Hewlett-Packard 8453 diode array spectrometer. Elemental analyses were performed by Atlantic Microlab, Inc. (Norcross, GA).
Synthesis of [CoIII(SMe2N4(tren))]2(trans–µ–1,2–O2)(PF6)2•MeCN (9).
Reduced [CoII(SMe2N4(tren))](PF6) (8) (317 mg, 0.71 mmol) was dissolved in 100 mL of acetonitrile. The solution was exposed to air at room temperature and left to stir overnight. The dark red solution was evaporated to dryness, and the resulting red powder was washed with diethyl ether over a frit. The remaining solid was dissolved in 10 mL acetonitrile and layered with 30 mL of diethyl ether. The two layers were allowed to diffuse overnight at −40 ˚C to afford red crystals of 9. ESI-MS: Calculated m/z for [C22H50Co2N8O2S2]2+ or [C11H25CoN4OS]+ = 320.1 found m/z = 320.0. Electronic Absorption Spectrum (MeCN): λmax (nm) (ε(M−1cm−1)): 270(6500). 1H NMR (500 MHz, CD3CN) δ ppm 1.45 (s, 6H), 2.05 (s, 3H), 2.44 (s, 2H), 2.72 (dd, J = 11.07, 4.37 Hz, 2H), 2.78 (q, J = 6.38 Hz, 2H), 3.00 (s, 2H), 3.33 (dd, J = 12.00, 5.44 Hz, 2H), 3.40 (t, J = 8.50, 8.50 Hz, 2H), 3.66 (t, J = 7.22, 7.22 Hz, 2H). Reduction Potential (MeCN, vs. SCE): +220 mV (reversible). Elemental Analysis for C22H50Co2F12N8O2P2S2 Calcd: C, 28.39; H, 5.42; N, 12.04. Found: C, 28.86; H, 5.41; N, 12.92.
X-Ray Crystallographic Structure Determination.
A 0.19 × 0.17 × 0.14 a black prism of [Co(III)(SMe2N4(tren))]2(trans-μ−1,2-O2)(PF6)2•MeCN (9) was mounted on a glass capillary with oil. Data was collected at −143 ˚C on a Nonius Kappa CCD single crystal X-ray diffractometer, Mo Kα-radiation. Crystal-to-detector distance was 30 mm and exposure time was 15 seconds per degree for all sets. The scan width was 2˚. Data collection was 94.5% complete to 29.61˚ in θ and 96.9% complete to 25˚ in θ. A total of 18,295 partial and complete reflections were collected covering the indices, h = −9 to 8, k = −13 to 14, l = −15 to 14. 6,556 reflections were symmetry independent and the Rint = 0.0408 indicated that the data was above average quality (0.07). Indexing and unit cell refinement indicated a triclinic P lattice. The space group was found to be P-1 (No.2). The data for 9 was integrated and scaled using hkl-SCALEPACK.43,44 Solution by direct methods (SHELXS, SIR97) produced a complete heavy atom phasing model consistent with the proposed structure.45,46 The structure was completed by difference Fourier synthesis with SHELXL.47,48 Scattering factors are from Waasmair and Kirfel.11 Hydrogen atoms were placed in geometrically idealized positions and constrained to ride on their parent atoms with C---H distances in the range 0.95–1.00 Angstrom. Isotropic thermal parameters Ueq were fixed such that they were 1.2 Ueq of their parent atom Ueq for CH’s and 1.5 Ueq of their parent atom Ueq in case of methyl groups. All non-hydrogen atoms were refined anisotropically by full-matrix least-squares. Final solution plotted using ORTEP and POV-Ray programs.49,50
Computational Details.
Calculations were performed using the ORCA v.4.0.0 quantum chemistry package developed by Neese and coworkers.51 Geometry optimizations employed the B3LYP hybrid functional and 6–311G basis set for all complexes. Tight convergence criteria were required for self-consistent field (SCF) solutions. The Grid4 (GridX4) integration grid size, and the conductor-like polarizable continuum model (CPCM), were used for geometry optimizations.52
Crystallographic coordinates were used as a starting point for geometry optimizations of peroxo {[CoIII(SMe2N4(tren))]2(trans-µ−1,2-O2)}2+ (9) using the B3LYP/6–311G functional/basis set. Details regarding the theoretical calculations for peroxo-bridged [MnIII(SMe2N4(quinoEN)]2(μ– O2)(BPh4)2 (10) and {[MnIII(SMe2N4(6-MeO-DPEN)]2-(μ–O2)}2+ (11) reported elsewhere.19 Canonical molecular orbital isosurfaces were visualized at an isovalue of 0.03 a0 3 using UCSF Chimera software.53
Results and Discussion.
The reaction between [CoII(SMe2N4(tren))](PF6) (8) and dioxygen (O2) in MeCN at ambient temperature results in a color change from pale yellow to red, with the concomitant growth of peaks at λmax(ε(M−1cm−1)) = 280(11350), 385(3085), and 485(1250) nm (Figure S2). The 1H NMR of this dioxygen product, 9, (Figure S3) only contains peaks in the diamagnetic region of the spectrum, consistent with oxidation of the S = 3/2 Co(II) precursor42 to low-spin (L.S.) S = 0 Co(III). The ESI-MS of 9 (Figure 2) displays peak at m/z = 320.0, consistent with the addition of two oxygen atoms to a dicationic dimer (M + 32, where M= 608.2, z = 2), or the addition a single oxygen atom to a monocationic monomer (M + 16, where M= 304.1. z= 1). These two would be distinguishable based on their isotope distribution pattern. As shown in the simulated spectrum of Figure S1, peaks would be separated by 1/2 mass unit for a dicationic dimer, versus one mass unit for a monocationic monomer. The experimental data would therefore be consistent with the former. This was consistently the case across a wide range of applied skim voltages (4 – 10 V to 30 – 70 V), implying that we are looking at either a Co-peroxo with a remarkably weak O-O bond, or a Co-oxo. The reaction of 8 with isotopically labeled 18O2 results in a peak shift to m/z to 322.0 (M + 18), consistent with incorporation of a one oxygen atom, derived from dioxygen.
Figure 2.
ESI-MS of peroxo-bridged 9 derived from 16O2 (top) and 18O2 (bottom).
Crystallization from MeCN/Et2O afforded single crystals of 9 suitable for X-ray crystallography. As shown in the ORTEP diagram of Figure 3, {[CoIII(SMe2N4(tren))]2 (trans-µ−1,2-O2)}2+ (9), is binuclear and contains an O2 moiety bridging between two Co ions in a trans-µ−1,2-configuration. The Co–S bond length of 9 (2.2180(9) Å) is 0.083 Å shorter than the reduced precursor 8 (Co–S = 2.3006(7) Å), and the average Co–N bond length distance is 0.173 Å shorter than the corresponding distance in 8. More importantly, the Co–S, average Co-N, and Co-O bond lengths in 9 are comparable (Table 1) to the previously characterized hydroxo complex [CoIII(SMe2N4(tren)) (OH)]+ (12),54 consistent with the oxidation of the high-spin Co(II) (S = 3/2) ion in 8 to a low-spin Co(III) (S = 0) ion in 9. The Co–O bond length in 9 (1.899(2) Å) is comparable to that of 12, as well as other previously reported Co(III) peroxo compounds.36,55,56 The O–O bond length of dicationic 9 (1.482(4) Å) is consistent with a peroxo, but is 0.054 Å longer than that of neutral (B2pz4Py)CoIII-O-O-CoIII(B2pz4Py), which contains two dianionic ligands.51 This indicates that the peroxo in 9 is highly activated. The two halves of the dimer are twisted relative to each other with a dihedral angle of 180°, and the plane containing the Co(III)-O-O-Co(III) core is approximately perpendicular to the plane containing two Co–S bonds. The and Co-O-O bond angle (114°) is more obtuse than the corresponding Mn-O-O angle of 1 (Table 1), but is comparable to most CoIII-peroxo compounds.36,55–62
Figure 3.

ORTEP of peroxo-bridged {[CoIII(SMe2N4(tren))]2 (trans-µ−1,2-O2)}2+ (9) showing 50% probability ellipsoids and the atom labeling scheme. Hydrogens are omitted for clarity.
Table 1.
Selected Bond Distances (Å) and Bond Angles (deg) for [CoII(SMe2N4(tren))](PF6) (8), Peroxo-Bridged [CoIII(SMe2N4(tren))]2(trans-µ−1,2-O2)(PF6)2•MeCN (9), Peroxo-Bridged [MnIII(SMe2N4(6-Me-DPEN))]2(trans-µ−1,2-O2)(BPh4)2•2CH3CH2CN (1), and Hydroxo Bound [CoIII(SMe2N4(tren))(OH)](PF6) (12).54
| 8 (d7, S = 3/2; | 9 (d6, S = 0; | 1 (d4, S = 2; | 12 | |
|---|---|---|---|---|
| M(1)–S(1) | 2.3006(7) | 2.2180(9) | 2.275(11) | 2.217(3) |
| M(1)–N(1) | 2.050(2) | 1.900(2) | 2.040(3) | 1.892(8) |
| M(1)–N(2) | 2.223(2) | 1.978(3) | 2.203(3) | 1.971(8) |
| M(1)–N(3) | 2.107(2) | 1.935(2) | 2.410(3) | 1.935(6) |
| M(1)–N(4) | 2.086(2) | 1.963(2) | 2.492(3) | 1.935(6)* |
| M(1)–O(1) | N/A | 1.899(2) | 1.832(3) | 1.869(6) |
| O(1)–O(1’) | N/A | 1.482(4) | 1.452(5) | N/A |
| M(1)•••O(1’) | N/A | 2.845 | 2.481 | N/A |
| M(1)•••M(1’) | N/A | 4.604 | 4.113 | N/A |
| M(1)–O(1)–O(1’) | N/A | 114.0(2) | 97.5(6) | N/A |
| O(1)–M(1)–S(1) | N/A | 94.88(7) | 85.12(9) | 95.8(2) |
| O(1)–M(1)–N(3) | N/A | 90.9(1) | 92.4(1) | 87.7(2) |
| O(1)–M(1)–N(1) | N/A | 174.24(9) | 165.5(1) | 178.0(3) |
| O(1)–M(1)–N(2) | N/A | 90.61(9) | 111.1(1) | 90.0(3) |
| S(1)–M–N(2) | 163.96(6) | 174.24(7) | 163.3(1) | 174.3(2) |
| S(1)–M–N(3 | 112.25(6) | 94.10(8) | 109.0(1) | 94.23(17) |
| S(1)–M–N(4) | 106.90(6) | 94.05(8) | 105.6(1) | 94.23(17)* |
| N(1)–M–N(4) | 125.14(8) | 92.0(1) | 101.7(1) | 92.17(17)* |
N(4) = N(3’) for this structure, since a crystallographic mirror plane relates the two atoms (N(3) and N(3’).
Structure 9 is analogous to our previously reported crystallographically characterized trans-µ−1,2-peroxo bridged Mn(III) complex, {[MnIII(SMe2N4(6-Me-DPEN)]2(trans-µ−1,2-O2)}2+ (1),26 as well as two additional spectroscopically characterized Mn(III)-peroxo compounds, [MnIII(SMe2N4(quinoEN)]2(μ–O2)(BPh4)2 (10) and {[MnIII(SMe2N4(6-MeO-DPEN))]2-(μ–O2)}2+ (11), for which spectroscopically calibrated DFT calculated structures are available (Scheme 1).19 Relative to 1 (1.452(5)), the peroxo O–O bond of bimetallic Co(III)-peroxo 9 is 0.03 Å longer, and closer to that of O22- (1.49 Å),63 indicating that the peroxo is more activated in 9. An activated O–O bond should be susceptible to cleavage, consistent with our inability to observe the intact dimer by mass spectrometry (vide supra). An activated O–O bond should be susceptible to cleavage, consistent with our inability to observe the intact dimer by mass spectrometry. Only half of the dimer, consisting of a monocationic cobalt-oxo, is detected in ESI-MS, even at the lowest applied skim voltage (4 – 10 V) (Figure 2).). Peroxos are π-donors that can be stabilized via the removal of antibonding electron density from the peroxo π* orbitals via π-back-donation into a metal ion t2g d-orbital. With low-spin d6 Co(III), the π-symmetry t2g orbitals are filled, whereas they are half-filled with a high-spin d4 Mn(III) ion. If the t2g orbitals are filled, then this pathway for O–O bond stabilization is not available. In addition, with the cobalt peroxo 9 there are two short H-bonds (N(2)-H(2E)••••O(1’) = 2.051 Å) to the bridging peroxo oxygens (Figure 4), which are absent in the Mn(III) compound. It is possible that these H-bonds also contribute to O–O bond activation in 9. However, there are other examples of bridging Co peroxo compounds lacking H-bonds with similar distances.36,64
Scheme 1.
ChemDraw sketches of {[CoIII(SMe2N4(tren))]2(trans-µ−1,2-O2)}2+ (9),, {[MnIII(SMe2N4(6-Me-DPEN)]2(traans-µ−1,2-O2)}2+ (1),26 {[MnIII(SMe2N4(quinoEN))]2-(μ–O2)}2+ (10),19 and {[MnIII(SMe2N4(6-MeO-DPEN))]2-(μ–O2)}2+ (11).19
Figure 4.

Space-filling diagram of peroxo-bridged {[CoIII(SMe2N4(tren))]2(trans–µ–1,2–O2)}2+ (9) showing N-H hydrogen bonding to the peroxo (red).
We recently showed that metal ion Lewis acidity can influence peroxo O-O bond lengths by facilitating π -back-donation of electron density from the peroxo π* orbital.16,17 Metal ion Lewis acidity was found to depend on the steric properties of the ligand scaffold. Ligands with sterically demanding substituents on the aryl ring (e.g., 2, 5, and 7, Figure 1) were found to possess unusually long M•••NAr distances in the corresponding M(III) derivatives.65 Elongation of the Mn•••NAr distances was shown to increase metal ion Lewis acidity and create a virtual coordinatively unsaturated metal ion.16,17 This facilitates π-back donation from the filled peroxo π*(O-O) orbital to the metal ion, resulting in a shorter peroxo O–O bond.16 With less sterically demanding primary amines (e.g., 5 and 8, Figure 1), on the other hand, M-N (M= Mn or Co) distances in the corresponding M(III) derivatives were found to be significantly shorter.
To gain more insight into the electronic structure differences governing peroxo O–O bond activation, DFT calculations were performed on Co-peroxo 9 and compared to the Broken Symmetry (BS) DFT calculated structures for our previously reported Mn peroxo compounds {[MnIII(SMe2N4(quinoEN))]2-(μ–O2)}2+ (10) and {[MnIII(SMe2N4(6-MeO-DPEN))]2-(μ–O2)}2+ (11) of Scheme 1.19 Complex 9 was geometry optimized using the B3LYP hybrid functional and the 6–311G basis set, yielding metal-ligand and peroxo O-O bond lengths that are in reasonable agreement with crystallographic parameters (maximum bond length deviation of 3.7%) (Figure S4). Notably, the calculated O–O bond length of 1.521 Å supports a more activated peroxo moiety in 9.
The DFT calculated Mulliken charge of the metal ions in 9 (+1.45), 11 (+1.59), and 10 (+1.60) indicate that metal ion metal ion Lewis acidity does not necessarily follow the expected periodic trends Co > Mn. Steric constraints imposed by the ligand elongate two of the Mn•••NAr distances for the Mn-peroxo complexes {[MnIII(SMe2N4(quinoEN))]2-(μ–O2)}2+ (10, Scheme 1) and {[MnIII(SMe2N4(6-MeO-DPEN))]2-(μ–O2)}2+ (11, Scheme 1), and this is reproduced by the calculations. Conversely, the calculated electron density localized on the bridging peroxo oxygens is higher with Co-containing 9 (–0.56), relative to Mn-containing 11 (–0.48) and 10 (– 0.49). This trend reflects the fact that the π*(O–O) orbital that cannot π-back-donate into the filled t2g orbitals of a L.S. d6 Co(III) ion, resulting in a the localization of electron density on the peroxo oxygens and destabilization of the peroxo O-O bond. An analysis of the frontier orbital of both the Co and Mn-peroxo complexes, 9 and 11 (Figure 5), corroborates the strong dependence of the extent of O–O bond activation on the electronic properties of the metal ion. The highest occupied molecular orbital (HOMO) contains significant π*(O–O) character for both Co-peroxo 9 and Mn-peroxo 11. However, the HOMO of Mn-peroxo {[MnIII(SMe2N4(6-MeO-DPEN))]2-(μ–O2)}2+ (11, Scheme 1) is fairly delocalized, extending over both the O–O π* and singly occupied t2g Mn d-orbitals (Figure 5, right). This would be consistent with higher calculated Lewis acidity of the Mn ions as well as the observed stabilization of the peroxo O–O bond. The HOMO of Co-peroxo 9 (Figure 5, left), however, is dominated by the π*(O–O) orbital and predominantly peroxo in character, consistent with lack of π-back-donation into the fully occupied Co t2g d-orbitals (Figure 5). The LUMO of both 9 and 11 is antibonding with respect to the M-O(peroxo) bond.
Figure 5.
Frontier orbitals of CoIII(SMe2N4(tren))]2(trans-µ−1,2-O2)}2+(9) (left) and {[MnIII(SMe2N4(6-MeO-DPEN)]2( trans-µ−1,2-O2)}2+ (11)19 visualized at an isovalue of 0.03 a03.
Conclusions.
This work describes the structure and properties of a O2-derived thiolate-ligated, peroxo-bridged Co(III) dimer and provides a comparison with structurally analogous peroxo-bridged Mn(III) dimers. It also provides a rationale for the effects of both electronic structural differences and the ligand scaffold can have on peroxo O–O bond activation. The electronic structure of the metal ion, as well as the metal ion Lewis acidity, are shown to have a profound impact on peroxo O–O bond activation and stability. The lack of steric bulk in the Co peroxo compound is shown to decrease metal center Lewis acidity relative to the Mn peroxo compounds, resulting in a more activated peroxo O-O bond. In addition, with its completely filled -symmetry t2g set of orbitals, the L.S. d6 Co(III) ion is incapable of providing stability to the peroxo O-O bond through -back-donation from the π*(O–O). DFT calculations support this by showing that, with Co(III), the HOMO contains more electron density localized in the peroxo π*(O–O) orbital, relative to the HOMO of the structurally analogous Mn(III) peroxo complex, resulting in a more activated peroxo O-O bond. The substitution-inert character of the Co(III) ion facilitates the isolation of a significantly more activated peroxo, however. Insight into some of the key factors governing O–O bond activation can serve as a benchmark for future small-molecule design.
Supplementary Material
Acknowledgements.
We wish to thank the National Science Foundation for funding (CHE-1664682)
Footnotes
Publisher's Disclaimer: This Author Accepted Manuscript is a PDF file of an unedited peer-reviewed manuscript that has been accepted for publication but has not been copyedited or corrected. The official version of record that is published in the journal is kept up to date and so may therefore differ from this version.
References.
- (1).Leslie M Science 2009, 323 (5919), 1286. [DOI] [PubMed] [Google Scholar]
- (2).Barber J Chem. Soc. Rev 2009, 38 (1), 185. [DOI] [PubMed] [Google Scholar]
- (3).Askerka M; Brudvig GW; Batista VS Acc. Chem. Res 2017, 50 (1), 41. [DOI] [PubMed] [Google Scholar]
- (4).Yano J; Yachandra V Chem. Rev 2014, 114 (8), 4175. [DOI] [PMC free article] [PubMed] [Google Scholar]
- (5).Nocera DG Acc. Chem. Res 2012, 45 (5), 767. [DOI] [PubMed] [Google Scholar]
- (6).Cox N; Pantazis DA; Neese F; Lubitz W Acc. Chem. Res 2013, 46 (7), 1588. [DOI] [PubMed] [Google Scholar]
- (7).Renger G J. Photochem. Photobiol. B Biol 2011, 104 (1–2), 35. [DOI] [PubMed] [Google Scholar]
- (8).Retegan M; Krewald V; Mamedov F; Neese F; Lubitz W; Cox N; Pantazis DA Chem. Sci 2015, 7 (1), 72. [DOI] [PMC free article] [PubMed] [Google Scholar]
- (9).Cox N; Retegan M; Neese F; Pantazis DA; Boussac A; Lubitz W Science 2014, 345 (6198), 804. [DOI] [PubMed] [Google Scholar]
- (10).Brudvig GW Philos. Trans. R. Soc. B Biol. Sci 2008, 363 (1494), 1211. [DOI] [PMC free article] [PubMed] [Google Scholar]
- (11).Dismukes GC; Brimblecombe R; Felton GAN; Pryadun RS; Sheats JE; Spiccia L; Swiegers GF Acc. Chem. Res 2009, 42 (12), 1935. [DOI] [PubMed] [Google Scholar]
- (12).Betley TA; Wu Q; Van Voorhis T; Nocera DG Inorg. Chem 2008, 47 (6), 1849. [DOI] [PubMed] [Google Scholar]
- (13).Armstrong FA Philos. Trans. R. Soc. B Biol. Sci 2008, 363 (1494), 1263. [DOI] [PMC free article] [PubMed] [Google Scholar]
- (14).Coggins MK; Brines LM; Kovacs JA Inorg. Chem 2013, 52 (21), 12383. [DOI] [PMC free article] [PubMed] [Google Scholar]
- (15).Shook RL; Gunderson WA; Greaves J; Ziller JW; Hendrich MP; Borovik AS J. Am. Chem. Soc 2008, 130 (28), 8888. [DOI] [PMC free article] [PubMed] [Google Scholar]
- (16).Rees JA; Martin-Diaconescu V; Kovacs JA; DeBeer S Inorg. Chem 2015, 54 (13), 6410. [DOI] [PMC free article] [PubMed] [Google Scholar]
- (17).Annaraj J; Cho J; Lee YM; Kim SY; Latifi R; De Visser SP; Nam W Angew. Chemie - Int. Ed 2009, 48 (23), 4150. [DOI] [PubMed] [Google Scholar]
- (18).Geiger RA; Leto DF; Chattopadhyay S; Dorlet P; Anxolabéhère-Mallart E; Jackson TA Inorg. Chem 2011, 50 (20), 10190. [DOI] [PubMed] [Google Scholar]
- (19).Poon PCY; Dedushko M; Sun X; Yang G; Toledo S; Hayes EC; Johansen A; Rees JA; Stoll S; Rybak-Akimova E; Kovacs JA J. Am. Chem. Soc 2019. [DOI] [PMC free article] [PubMed] [Google Scholar]
- (20).Coggins MK; Kovacs JA J. Am. Chem. Soc 2011, 133 (32), 12470. [DOI] [PMC free article] [PubMed] [Google Scholar]
- (21).Seo MS; Kim JY; Annaraj J; Kim Y; Lee YM; Kim SJ; Kim J; Nam W Angew. Chemie - Int. Ed 2007, 46 (3), 377. [DOI] [PubMed] [Google Scholar]
- (22).Vanatta RB; Strouse CE; Hanson LK; Valentine JS J. Am. Chem. Soc 1987, 109 (5), 1425. [Google Scholar]
- (23).Kitajima N; Komatsiizaki H; Hikichi S; Osawa M; Moro-oka Y J. Am. Chem. Soc 1994, 116 (25), 11596. [Google Scholar]
- (24).Singh UP; Sharma AK; Hikichi S; Komatsuzaki H; Moro-oka Y; Akita M Inorganica Chim. Acta 2006, 359 (13), 4407. [Google Scholar]
- (25).Bossek U; Weyhermiiller T; Wieghardt K; Nuber B; Weiss J J. Am. Chem. Soc 1990, 112 (17), 6387. [Google Scholar]
- (26).Coggins MK; Sun X; Kwak Y; Solomon EI; Rybak-Akimova E; Kovacs JA J. Am. Chem. Soc 2013, 135 (15), 5631. [DOI] [PMC free article] [PubMed] [Google Scholar]
- (27).Coggins MK; Martin-Diaconescu V; Debeer S; Kovacs JA J. Am. Chem. Soc 2013, 135 (11), 4260. [DOI] [PMC free article] [PubMed] [Google Scholar]
- (28).Brown CD; Neidig ML; Neibergall MB; Lipscomb JD; Solomon EI J. Am. Chem. Soc 2007, 129 (23), 7427. [DOI] [PMC free article] [PubMed] [Google Scholar]
- (29).Kovacs JA; Brines LM Acc. Chem. Res 2007, 40 (7), 501. [DOI] [PMC free article] [PubMed] [Google Scholar]
- (30).Kovacs JA Acc. Chem. Res 2015, 48 (10), 2744. [DOI] [PMC free article] [PubMed] [Google Scholar]
- (31).Brodsky CN; Hadt RG; Hayes D; Reinhart BJ; Li N; Chen LX; Nocera DG Proc. Natl. Acad. Sci 2017, 114 (15), 3855. [DOI] [PMC free article] [PubMed] [Google Scholar]
- (32).Smith PF; Hunt L; Laursen AB; Sagar V; Kaushik S; Calvinho KUD; Marotta G; Mosconi E; De Angelis F; Dismukes GC J. Am. Chem. Soc 2015, 137 (49), 15460. [DOI] [PubMed] [Google Scholar]
- (33).Holm RH Chem. Rev 1987, 87 (6), 1401. [Google Scholar]
- (34).Gao Y; Åkermark T; Liu J; Sun L; Åkermark B J. Am. Chem. Soc 2009, 131 (25), 8726. [DOI] [PubMed] [Google Scholar]
- (35).Volpe M; Hartnett H; Leeland JW; Wills K; Ogunshun M; Duncombe BJ; Wilson C; Blake AJ; McMaster J; Love JB Inorg. Chem 2009, 48 (12), 5195. [DOI] [PubMed] [Google Scholar]
- (36).Schaefer WP; Marsh RE J. Am. Chem. Soc 1966, 88 (1), 178. [Google Scholar]
- (37).Sykes AG; Weil JA In Progress in Inorganic Chemistry; 1970; Vol. 13, pp 1–106. [Google Scholar]
- (38).Kotani H; Hong D; Satonaka K; Ishizuka T; Kojima T Inorg. Chem 2019, 58 (6), 3676. [DOI] [PubMed] [Google Scholar]
- (39).Jin Seog Seo; Hynes RC; Williams D; Chin J J. Am. Chem. Soc 1998, 120 (38), 9943. [Google Scholar]
- (40).Givaja G; Volpe M; Edwards MA; Blake AJ; Wilson C; Schröder M; Love JB Angew. Chemie - Int. Ed 2007, 46 (4), 584. [DOI] [PubMed] [Google Scholar]
- (41).Wang D; Lindeman SV; Fiedler AT Inorg. Chem 2015, 54 (17), 8744. [DOI] [PubMed] [Google Scholar]
- (42).Brines LM; Shearer J; Fender JK; Schweitzer D; Shoner SC; Barnhart D; Kaminsky W; Lovell S; Kovacs J. a. Inorg. Chem 2007, 46 (22), 9267. [DOI] [PMC free article] [PubMed] [Google Scholar]
- (43).Otwinowski Z; Minor W Macromolecular Crystallography, 1st ed.; Sweet RM, Carter CW, Eds.; Acadmic Press: New York, 1997. [Google Scholar]
- (44).Mackay S; Edwards C; Henderson A; Gilmore C; Stewart N; Shankland K; Donald A University of Glasgow; 1997,. [Google Scholar]
- (45).Altomare A; Cascarano G; Giacovazzo C; Guagliardi A; Burla MC; Polidori G; Camalli M J. Appl. Crystallogr 1994, 27 (3), 435. [Google Scholar]
- (46).Altomare A; Burla MC; Camalli M; Cascarano GL; Giacovazzo C; Guagliardi A; Moliterni AGG; Polidori G; Spagna R J. Appl. Crystallogr 1999, 32 (1), 115. [Google Scholar]
- (47).Sheldrick GM University of Göttingen, Germany: 1997,. [Google Scholar]
- (48).Sheldrick GM Acta Crystallogr. Sect. C Struct. Chem 2015, 71 (Md), 3. [DOI] [PMC free article] [PubMed] [Google Scholar]
- (49).Burnett MN; Johnson CK Oak Ridge National Laboratory; Report ORNL-6895 1996,. [Google Scholar]
- (50).Persistence of Vision Pty. Ltd.: Williamstown, Victoria, Australia: 2013,. [Google Scholar]
- (51).Neese F WIREs Comput. Mol. Sci 2012, 2, 73. [Google Scholar]
- (52).Barone V; Cossi M J. Phys. Chem. A 1998, 102 (11), 1995. [Google Scholar]
- (53).Pettersen EF; Goddard TD; Huang CC; Couch GS; Greenblatt DM; Meng EC; Ferrin TE 2004. [Google Scholar]
- (54).Swartz RD; Coggins MK; Kaminsky W; Kovacs JA J. Am. Chem. Soc 2011, 133 (11), 3954. [DOI] [PMC free article] [PubMed] [Google Scholar]
- (55).Nurdin L; Spasyuk DM; Fairburn L; Piers WE; Maron L J. Am. Chem. Soc 2018, 140 (47), 16094. [DOI] [PubMed] [Google Scholar]
- (56).Ramprasad D; Gilicinski AG; Markley TJ; Pez GP Inorg. Chem 1994, 33 (13), 2841. [Google Scholar]
- (57).Rigsby ML; Mandal S; Nam W; Spencer LC; Llobet A; Stahl SS Chem. Sci 2012, 3 (10), 3058. [Google Scholar]
- (58).Ludovici C; Fröhlich R; Vogtt K; Mamat B; Lübben M Eur. J. Biochem 2003, 269 (10), 2630. [DOI] [PubMed] [Google Scholar]
- (59).Howard-Jones AR; Adam V; Cowley A; Baldwin JE; Bourgeois D Photochem. Photobiol. Sci 2009, 8 (8), 1150. [DOI] [PubMed] [Google Scholar]
- (60).Fukuzumi S; Mandal S; Mase K; Ohkubo K; Park H; Benet-Buchholz J; Nam W; Llobet A J. Am. Chem. Soc 2012, 134 (24), 9906. [DOI] [PubMed] [Google Scholar]
- (61).Cho YI; Joseph DM; Rose MJ Inorg. Chem 2013, 52 (23), 13298. [DOI] [PubMed] [Google Scholar]
- (62).Wang HY; Mijangos E; Ott S; Thapper A Angew. Chemie - Int. Ed 2014, 53 (52), 14499. [DOI] [PubMed] [Google Scholar]
- (63).Vaska L Acc. Chem. Res 1976, 9 (5), 175. [Google Scholar]
- (64).Fritch JR; Christoph GG; Schaefer WP Inorg. Chem 1973, 12 (9), 2170. [Google Scholar]
- (65).Coggins MK; Toledo S; Shaffer E; Kaminsky W; Shearer J; Kovacs JA Inorg. Chem 2012, 51 (12), 6633. [DOI] [PMC free article] [PubMed] [Google Scholar]
Associated Data
This section collects any data citations, data availability statements, or supplementary materials included in this article.




