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A Comparison Between Experimental and Broken Symmetry Density Functional Theory (BS-DFT) Calculated Electron Paramagnetic Resonance (EPR) Parameters of the S 2 State of the Oxygen Evolving Complex of Photosystem II in its Native (Calcium) and Strontium Substituted Form. Nathan J. Beal, Thomas A. Corry and Patrick J. O’Malley * School of Chemistry, The University of Manchester, Manchester M13 9PL, UK. ABSTRACT A comparison between experimental and Broken Symmetry Density Functional Theory (BS-DFT) calculated hyperfine couplings for the S 2 state of the oxygen evolving complex (OEC) has been performed. The effect of Ca substitution by Sr combined with the protonation state of two terminal hydroxo or aqua ligands, W1 and W2, on the calculated hyperfine couplings of 55 Mn, 13 C, 14 N, 17 O and 1 H nuclei has been investigated. Our findings show best agreement with experiment for OEC models which contain a hydroxide group at the W2 position and a 1
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Page 1:  · Web viewA Comparison Between Experimental and Broken Symmetry Density Functional Theory (BS-DFT) Calculated Electron Paramagnetic Resonance (EPR) …

A Comparison Between Experimental and Broken Symmetry Density

Functional Theory (BS-DFT) Calculated Electron Paramagnetic

Resonance (EPR) Parameters of the S2 State of the Oxygen Evolving

Complex of Photosystem II in its Native (Calcium) and Strontium

Substituted Form.

Nathan J. Beal, Thomas A. Corry and Patrick J. O’Malley*

School of Chemistry, The University of Manchester, Manchester M13 9PL, UK.

ABSTRACT

A comparison between experimental and Broken Symmetry Density Functional Theory

(BS-DFT) calculated hyperfine couplings for the S2 state of the oxygen evolving complex

(OEC) has been performed. The effect of Ca substitution by Sr combined with the

protonation state of two terminal hydroxo or aqua ligands, W1 and W2, on the calculated

hyperfine couplings of 55Mn, 13C, 14N, 17O and 1H nuclei has been investigated. Our

findings show best agreement with experiment for OEC models which contain a hydroxide

group at the W2 position and a water molecule at W1. For this model the agreement

between calculated and experimental data for all hyperfine couplings is excellent. Models

with a hydroxide group at W1 are particularly poor models. Sr substitution has a minor

influence on calculated hyperfine couplings in agreement with experimental

determinations. The sensitivity of the hyperfine couplings to relatively minor changes in

the OEC structure demonstrates the power of this methodology in refining the details of its

steric and electronic structure which is an essential step in formulating a complete

mechanism for water oxidation by the OEC.

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INTRODUCTION

Photosystem II (PSII) is a multi-unit pigment protein complex found in the thylakoid

membrane of organisms that perform oxygenic photosynthesis. One of its key functions is

the accumulation of visible light driven oxidising equivalents on its donor side leading to

oxidation of water to molecular oxygen in its oxygen evolving complex (OEC).1–9 Only

recently has the fundamental atomic-level detailed molecular structure of this important

biological complex been successfully revealed. The 2011 X-ray study by Umena et al. and

the subsequent X-Ray Free Electron Laser (XFEL) crystal structure helped to provide an

atomic-level high resolution structure,10,11 which provides a primary landmark for any

suggested proposals regarding the molecular structure and mechanism of the OEC.1,12–14

The structure of the dark adapted state, Figure 1, showed that the OEC was a Mn4CaO5

cluster arranged in a distorted chair form with four terminal oxygen atoms presumably

water or hydroxide, labelled W1-W4, directly coordinated to the OEC.10 Two of these can

be confidently assigned as water molecules W3 and W4 ligated to the Ca2+ ion and the

other two W1 and W2 are either water or hydroxide ligands to the MnA ion. It has been

suggested that some of these OEC coordinated water or hydroxide molecules may serve as

substrates for water splitting.15,16 Various studies have highlighted an important role for the

calcium ion in the oxygen formation reaction with removal of the calcium ion found to

block the Sn state transition beyond the S2 state resulting in a complete loss of oxygen

evolving activity.17,18 Cation substitution experiments have shown that the only other cation

to restore oxygen evolution was strontium albeit at a reduced activity (approximately half

that of the native OEC).19–22

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Figure 1. Structure of the model used in this study for the OEC found in dark-adapted PSII generated from PDB ID: 4UB6. The protein residues are labelled along with the Mn and Ca bound aqua ligands. Colour coding: manganese (pink), oxygen (red), nitrogen (purple), carbon (yellow) and calcium (white). Hydrogen atoms are omitted for clarity.

Substituting calcium for strontium has been reported to slightly modify the EPR

parameters of the S2 state,19,23 and additionally the substitution has been found to have an

effect on several carboxylate stretching modes of the S2−S1 FTIR difference spectra.24–28

These results imply that the calcium ion performs more than simply a structural role in the

OEC and may be mechanistically involved.

The improved structural information provided by the high resolution crystal structures has

provided the key and necessary underpinning for the mechanism of oxygen formation to be

investigated in greater detail with theoretical methods or other experimental techniques.

6,7,29–36 This report focuses on the S2 state for both native (Ca) and Sr substituted systems.

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The S2 state is the best characterised Sn state in the Kok cycle, especially in terms of EPR

spectroscopy.16,37–49 X-band EPR spectra of the S2 state exhibits a multiline signal at g ≈ 2,

originating from an S = 1/2 ground state, most likely with a MnIII(MnIV)3 distribution of

oxidation states although other assignments have been discussed at length in the

literature.29,35,50,51 Sometimes accompanying this signal at g ≈ 2 is a broad signal occurring

at g ≥ 4.1 attributed to an S = 5/2 spin state of the OEC.52 The presence of the multiline

signal indicates an antiferromagentically coupled mixed valence manganese cluster,

resembling the multiline signal of synthetic or biological dinuclear MnIIIMnIV complexes.53–

55 In addition to the metal hyperfine couplings of the S2 state, ligand hyperfine couplings,

e.g. 17O, 14N, 1H and 13C have been used to provide insight into the molecular and

electronic structure of the OEC.16,38,40,56,57 As the S2 state is the best characterised state of

the Kok cycle in terms of experimental EPR data it therefore provides a good test of

computational results on model complexes for both native and Sr substituted forms of the

OEC. A large number of computational studies are currently being applied to OEC models

but it is important to limit the suitability of such models and the conclusions drawn from

them to well determined experimental parameters, something which is not widely adhered

to. As we will show in this study, correct prediction of EPR parameters provides very

rigorous constraints on proposed models of the S2 state and such restraints are essential

before models can be used further in the S-state cycle progression. In particular, the study

focuses on the protonation states of the two MnA ligated oxygen atoms, W1 and W2 using

both native and Sr substituted models. As mentioned above, crystallographic studies

cannot distinguish hydroxide and water ligands and while protonated states for both waters

are energetically and structurally similar, we show that the protonation state can be clearly

deciphered by its effect on the EPR hyperfine couplings of the manganese ions in the

cluster and its associated ligands. Earlier reports44 on this problem for smaller Ca models

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have indicated that W1 and W2 are aqua and hydroxo ligands respectively in the S2 state.

This was based solely on the ability of the model to reproduce the experimental 55Mn HFCs

for a small model of the open cubane form. There is however not a complete consensus on

this particular protonation pattern58 and further investigations are required using larger

models of both the open and closed cubane forms and extending the range of comparison

between calculated and experimental HFCs. In this report therefore we extend this analysis

to both open and closed cubane forms of S2 using an extensive model incorporating in

particular the crucial redox active YZ residue and extend the analysis beyond 55Mn HFCs to

the ligand 17O, 14N, 13C and 1H nuclei. In addition we include a similar analysis and

comparison for Sr substituted S2 models.

COMPUTATIONAL DETAILS

The geometries of all the models studied were optimised in their respective high spin states

using the BP86 functional, 59,60 utilising the zeroth-order regular approximation (ZORA)

Hamiltonian to include scalar relativistic effects.61–63 ZORA adapted segmented all-electron

relativistically contracted (SARC) basis sets were employed for all atoms,64 ZORA

versions of the def2-SVP basis sets were used for C and H atoms with ZORA versions of

the def2-TZVP basis set used for all other atoms with f functions removed.65 The

computational time of the calculations was decreased by invoking the resolution of identity

approximation (RI) along with decontracted auxillary def2-TZVP/J coulomb fitting basis

sets.66–68 The optimizations also included the third generation (D3) semi-empirical van der

waals corrections proposed by Grimme.69,70 Increased integration grids (grid 4 and grid x4

in orca convention) and tight SCF convergence criteria were used throughout the

calculations. The Heisenberg exchange coupling constants, hyperfine and nuclear

quadrupole coupling values were calculated for all atoms of interest using the broken

symmetry DFT methodology using the hybrid meta-GGA TPSSh functional with the chain

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of spheres (RIJCOSX) approximation to exact exchange using the same decontracted

auxillary basis sets that were used in the geometry optimization steps.71,72 Initial broken

symmetry guesses were constructed using the ‘flipspin’ feature of ORCA.73 Calculation of

the hyperfine and quadrupole tensors used basis sets developed by Neese et al. based on

the SARC def2-TZVP for the Mn, N and O atoms and def2-TZVP(-f) for all other

atoms.68,74 The integration grids were increased to an integration accuracy of 11 and 9 for

Mn, N and O respectively. Picture change effects were applied for the calculation of

hyperfine and nuclear quadrupole tensors. Heisenberg exchange coupling constants were

calculated using the methodology proposed by Pantazis et al.75 The calculated 55Mn

isotropic hyperfine couplings were scaled by a factor of 1.47 to account for the known spin

polarisation deficiency in the calculation of the Fermi contact term.76,77 This factor has been

validated for 6 models of mononuclear, dinuclear and tetranuclear manganese complexes

(see Table S1 in supporting information; structures are shown in Figure S1). Convergence

to the correct BS and HS states in all calculations was confirmed by examination of the

calculated Mulliken spin populations.

Model Systems

The model systems studied were constructed using starting coordinates taken from two

crystal structures of the OEC of PSII available in the literature (PDB ID: 4UB6 (native

PSII isolated from Thermosynechococcus vulcanus) and 4IL6 (Sr-substituted PSII isolated

from Thermosynechococcus vulcanus)).11,78

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Figure 2. Numbering scheme for the constructed cluster models of the OEC. Colour coding: manganese (pink), calcium/strontium (white), oxygen (red), nitrogen (purple), carbon (yellow). Hydrogen atoms omitted for clarity. The complete model used for the calculations is given in Figure S1 of the Supporting Information.

The labelling scheme for all the models (Figure 2) is as follows: the model designators Ca

and Sr correspond to the crystal structure that was used as a starting point for the

calculations. The native PSII 4UB6 is denoted by Ca, while the Sr-substituted PSII 4IL6 is

represented by the label Sr. A second label is used to distinguish between the various

protonation patterns of the water or hydroxide groups (W1 and W2) studied which for

clarity can be seen in Table 1 below.

Table 1. Labelling scheme to distinguish the various protonation states of W1 and W2 in the Ca and Sr models.

Protonation stateLabel W1 W2

1 OH2 OH2 OH OH3 OH OH2

4 OH2 OH2

All the OEC cluster models studied contain the seven directly coordinated amino acid

residues (all found in the D1 protein chain unless otherwise indicated): Asp-170, Glu-189,

His-332, Glu-333, Asp-342, Ala-344 and CP43-Glu-354. Additionally the two fully

protonated water molecules coordinated to the calcium/strontium ion were also included as

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well as the W1 and W2 groups coordinated to MnA. As well as this the models include the

important second sphere residues: Asp-61, Tyr-161, Gln-165, His-190, Asn-298, His-337

and CP43-Arg-357. In addition to this twelve closely associated crystallographic water

molecules as well as partial backbone of Glu-329 was involved, having previously found to

hydrogen bond with His-332.79 Inclusion of Tyr-161(YZ) and its hydrogen bonding partner

His-190 is essential for all S2 models. This is illustrated in Figure 3 where it is shown that

the Highest Occupied Molecular Orbital (HOMO) is located on the phenoxyl head group

of this residue with the HOMO-1 (predominantly anti-bonding dZ2) located on the MnD

III

ion along the Jahn Teller axis. This is in line with the observed subsequent photooxidation

sequence leading first to YZ oxidation to YZ• followed by eventual oxidation of MnD

III to

MnDIV

forming the S3 state. To reduce computational costs all residues were truncated after

the R group, in addition all residues took their standard proton states apart from His-337

where it has been shown a fully protonated histidine is present.79 A representative model is

shown in Figure S1 and coordinates of all models are given in the Supporting Information.

Figure 3. HOMO (a) and HOMO-1 (b) electron density contours for the Ca-1 model. Only selected regions are shown without hydrogen atoms.

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RESULTS AND DISCUSSION

A full detailed analysis of the geometric structures and the Heisenberg exchange couplings

is provided in the Supporting Information. There is little experimental data concerning the

closed form of S2 other than the characteristically broad signal in the EPR spectrum. As a

result, no hyperfine coupling data will be presented for this form.

55Mn Hyperfine Couplings

Table 2 shows the spin projected isotropic and anisotropic hyperfine coupling (HFC)

tensors calculated for the open cubane form Ca models along with several experimental

data sets. At the present time there are numerous sets of experimental hyperfine coupling

tensors obtained from various simulations of the spectra obtained from EPR and ENDOR

experiments. The differences found in the experimental datasets reflect not only variations

in the methodology of the simulations but also aspects of sample origin and preparation. It

should be noted that a change in species from spinach to Thermosynechoccus elongatus

PSII or treatment of the sample with MeOH may have a visible effect on the splitting

pattern in the spectra on the order of ca. 10 MHz for a given HFC value.80 These data sets

will therefore be regarded as a range to compare the calculated results with. All three data

sets featured in Table 2 find one isotropic HFC around 300 MHz. Two of the data sets

feature two HFC near 200 MHz with the remaining HFC being found around 250 MHz.41,81

In contrast, Charlot et al. found two HFCs near to 250 MHz and only a single HFC value

around 200 MHz.82 The additional experimental value of 312 MHz found by Teutloff et al.

from single crystal Q-band ENDOR refers specifically to the largest hyperfine coupling

found in the OEC.80 It is important to note that no experimental studies performed so far

have been able to yield sign information or to assign the HFCs to specific manganese sites

with any certainty.

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Considering firstly the calculated isotropic HFCs for each of the Ca models shows that Ca-

2 and Ca-3 models may be instantly rejected, as both models produce Aiso values for MnA

and MnB which are significantly smaller than shown in any of the experimental datasets.

The model Ca-4 produces isotropic HFCs in better agreement with the experimental values

however MnB and to a lesser extent MnA are still significantly lower than any found

experimentally. An explanation for this behaviour can be seen in the small on-site spin

projection coefficients (see Supporting Information) calculated for these models. In

contrast the model Ca-1 produces isotropic HFC values in very good agreement with the

experimental values with one HFC close to 300 MHz, another HFC was found close to

250 MHz and two HFCs near to 200 MHz (the HFC value of 224 MHz could arguably be

associated to either the 250 MHz or 200 MHz grouping). As has been found previously,

the largest Aiso value is not found for the MnIII ion (MnD) but rather is calculated for a MnIV

ion (MnA). Initially this disagreed with experimentally derived models of the S2 state which

were constructed with knowledge gained from studying mixed valence models.83,84

However there is experimental evidence to support the finding of smaller than expected

HFC for MnIII centres.77 Additionally the results of other computational studies of the OEC

have provided an ever increasing body of computational data which show that the MnIII

centre is not necessarily required to provide the largest HFC value in highly connected

systems as seen in the OEC.29,44,85,86

Turning to consider the anisotropic HFCs produced by model Ca-1, it can be observed

from the experimental simulation data that the anisotropy is more spread out over all the

manganese centres. The computed anisotropic HFCs of MnA and MnD are considerably

larger than those calculated for MnB and MnC and all of the calculated anisotropic HFCs

are in poor agreement with those from experiment. A potential reason for this is the zero-

field splitting related anisotropy transfer which has been neglected in the current study and

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may critically affect the calculated anisotropic HFC data. Efforts to extend the spin

projections schemes to include zero field splitting and zero-field splitting anisotropy

transfer has been presented in the literature but the investigations have only focused so far

on dinuclear MnIIIMnIV complexes.87

Table 2. Calculated spin projected isotropic (Aiso) and anisotropic (Ti) 55Mn hyperfine couplings (in MHz) for the investigated Ca models and comparison with experimental data.

Model Aiso T1 T2 T3

Ca-1

MnA −287 −30 7 23MnB 198 −8 −1 10MnC 224 −5 −1 6MnD −253 −51 −45 96

Ca-2

MnA −78 −1 0 1MnB 65 −2 0 2MnC 193 −3 −1 5MnD −267 −56 −44 99

Ca-3

MnA −82 −5 0 5MnB 71 −2 0 3MnC 190 −4 −1 5MnD −280 −60 −41 101

Ca-4

MnA −179 −4 0 4MnB 145 −5 −1 6MnC 229 −5 −1 7MnD −292 −59 −50 109

Kulik et al.81

1 193 −23 −23 472 205 −20 −20 403 248 −13 −13 274 298 −23 12 12

Peloquin et al.41

1 200 −20 −20 402 217 −17 −17 333 245 −13 −13 254 297 −14 −14 27

Charlot et al.82

1 186 −5 −2 72 243 −26 5 203 257 −32 −17 494 329 −17 −5 22

Teutloff et al.80 1 312 −37 14 22

Table 3 shows the spin projected isotropic and anisotropic HFCs for the Sr models. The

strontium substituted OEC has been investigated to a lesser extent than the native form,

however recent EPR experiments have probed its electronic structure. The available

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experimental data is also included in Table 3. Similar to the native OEC, both of the

experimental data sets feature a HFC near to 300 MHz and a smaller HFC below

200 MHz. The data set of Cox et al. shows a second HFC slightly above 200 MHz and a

final HFC near 350 MHz.23 However the data set of Lohmiller et al. shows the remaining

HFCs to be close together at ca. 220/230 MHz.86 The Sr models display the similar trends

to those observed previously for the Ca models. It can be seen that Sr-2 and Sr-3 display

calculated Aiso values substantially smaller than those observed in the experimental

datasets.

Table 3. Calculated spin projected isotropic (A iso) and anisotropic (Ti) 55Mn hyperfine couplings (in MHz) for the investigated Sr models and comparison with experimental data.

Model Aiso T1 T2 T3

Sr-1

MnA −289 −10 0 10MnB 195 −6 −2 8MnC 234 −5 −2 8MnD −253 −58 −36 93

Sr-2

MnA −51 −1 0 1MnB 46 −2 0 2MnC 242 −5 −2 7MnD −339 −65 −41 106

Sr-3

MnA −94 −7 0 7MnB 81 −3 0 3MnC 237 −6 −2 8MnD −327 −68 −41 109

Sr-4

MnA −176 −2 0 2MnB 141 −5 −1 6MnC 240 −9 −1 10MnD −291 −59 −44 98

Cox et al.23

1 173 −21 −17 372 203 −18 −3 203 243 −26 1 254 332 −39 11 29

Lohmiller et al.86

1 187 −26 −12 372 221 −41 −6 493 232 −31 −19 514 332 −12 −4 15

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Additionally similar to the model Ca-4, the isotropic HFCs calculated for model Sr-4 are

an improvement over the Sr-2 and Sr-3 but the Aiso values for MnA and MnB are in poor

agreement with those found experimentally. The poor agreement for these models can be

attributed again to the small on-site spin projection coefficients found for these models.

Again, the only model which provides reasonable calculated HFCs is that of Sr-1 which

produces isotropic HFCs which coincide with the experimental data very well. Contrasting

the isotropic HFCs calculated for both the Ca-1 and Sr-1 model shows there is little

difference in the calculated HFCs following substitution of the Ca2+ ion. Historically

substitution of the OEC calcium with strontium was thought to change the oxidation state

distribution within the OEC cluster and therefore alter the coordination environment of the

MnIII ion.88 Instead the current thinking supported by experimental and computational

studies in the literature and found in this work is that strontium substitution produces minor

alterations to the manganese tetramer.23,43,89

No specific 55Mn HFCs have been reported for the closed cubane form, so a comparison

between theoretical and experimental values is not possible. The calculated spin projected

55Mn hyperfine couplings for the closed cubane form are presented for Ca-1, Ca-4, Sr-1

and Sr-4 models in Table S11 of the Supporting Information.

14N Hyperfine Couplings

As well as studying the 55Mn hyperfine couplings, further information and insight into the

electronic structure may be provided by the hyperfine interactions of various ligating EPR

active nuclei.90 One such nucleus is the 14N nucleus of the histidine residue (D1-His-332), a

ligand to MnD. Experimentally the HFC for this residue have been used to probe the

oxidation state assignment of the histidine bound metal.38 Additionally Pérez-Navarro et al.

found that the 14N signal observed for the native S2 state from Thermosynechococcus

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elongatus was very similar to that seen in samples of PSII isolated from both higher plants

(spinach) as well as the cyanobacteria Synechosytstis sp. PCC6803, illustrating the high

structural homogeneity of the OEC.40,46,56

Table 4 shows calculated 14N HFC as well as nuclear quadrupole coupling constants for the

Ca models studied in this work. At the present time no information is available regarding

the potential sign of the isotropic HFC. Although computationally the sign of the

calculated 14N isotropic HFC is dependent on the sign of the projection coefficient of MnD.

As a result of the dominant spin polarisation, A iso is positive when the MnD spin is down

and negative when the MnD spin is found to be up. Comparing the calculated and

experimental 14N EPR parameters shows that all models produce an isotropic HFC that is in

good agreement with that found from experiment. This is due to the spin projection

coefficients for MnD in all the models being similar. As a result of this it is expected that all

models produce an isotropic HFC value that agrees well with the experimental HFC.

Turning to consider the anisotropic HFC, it can be seen from Table 4 that in particular

model Ca-1 produces anisotropic HFCs, which are in excellent agreement with those

determined from experiment. The other Ca model results shown in Table 4 show

anisotropic HFCs which are in poorer agreement with those determined from experiment.

Early ESEEM experiments typically simulated the EPR spectra using axially symmetric

HFC tensors;38,40 however more modern measurements have found rhombic HFC

tensors.16,56 The calculations presented here would support the finding of rhombic tensors

for these HFCs.

Table 4. Calculated spin projected isotropic (A iso) and anisotropic (Ti) 14N hyperfine couplings and nuclear quadrupole couplings for the investigated Ca models studied and comparison with experimental data. All values are given in MHz.

Aiso T1 T2 T3 e2Qq/h ηCa-1 −6.08 −1.41 0.18 1.23 −1.56 0.68Ca-2 −5.55 −1.18 0.30 0.88 −1.71 0.54

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Ca-3 −5.99 −1.16 0.25 0.92 −1.54 0.63Ca-4 −6.12 −1.11 0.32 0.79 −1.48 0.78

Exp.56* |6.95| −1.50 0.20 1.30 −1.98 0.82* Similar experimental values have been reported in references 16,91

The calculated nuclear quadrupole coupling constant e2Qq/h is found to be slightly lower

than the experimental value in all Ca models but is similar to those previously found for

superoxidised manganese catalase or other imidazole nitrogen atoms that are coordinated

to metal centres.55,92 The asymmetry parameter η is also found to be under calculated. The

experimental asymmetry parameter of 0.82 is larger than that found in the superoxidised

manganese catalase or other metal-coordinated imidazole ligands.92 It should be noted that

the uncertainties in the asymmetry parameter in the ESEEM simulations are found to be

considerably larger than those for the nuclear quadrupole coupling constant. A good

example of this is the MnIII coordinated histidine in two different manganese catalase

samples (purified from Lactobacillus plantarum and Thermus thermophilus), the measured

asymmetry values were found to disagree significantly although the nuclear quadrupole

coupling constants were found to be very close to each other.92

Table 5. Calculated spin projected isotropic (A iso) and anisotropic (Ti) 14N hyperfine couplings and nuclear quadrupole couplings (in MHz) for the investigated Sr models studied and comparison with experimental data.

Aiso T1 T2 T3 e2Qq/h ηSr-1 −6.0 −1.3 0.1 1.1 −1.72 0.93Sr-2 −5.8 −1.1 0.2 0.9 −1.88 0.75Sr-3 −5.9 −1.1 0.3 0.8 −1.79 0.88Sr-4 −6.1 −1.2 0.3 0.9 −1.72 0.72

Exp.86 |7.3| −1.4 0.1 1.2 |1.98| 0.79

Comparing the calculated and experimental 14N EPR parameters for the Sr models shown

in Table 5 allows additional insight into the electronic structure of the strontium substituted

OEC. It can be seen that in a similar fashion to the Ca models, all the Sr models produce

isotropic HFCs which are found to be close to the reported experimental HFC. The

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anisotropic HFC tensors of model Sr-1 were found to agree very well with those

determined from experiment. However as was seen when studying the Ca models, the

remaining Sr models anisotropic HFCs were found to be in poorer agreement with the

experimental values. The calculated nuclear quadrupolar coupling constant is found to be

calculated in good agreement for all Sr models and is actually calculated in better

agreement with experimental data than the Ca models. Comparing the asymmetry

parameter with the experimental value shows an improvement over the Ca model data,

although Sr-1 and Sr-3 produce asymmetry values which are over calculated. Studying the

Ca-1 and Sr-1 models appears to support the earlier findings that substitution of the

calcium ion with strontium does not significantly perturb the electronic structure of the

MnD ion and by extension the tetranuclear manganese cluster, as there is very little

difference between the calculated isotropic and anisotropic HFCs or in the nuclear

quadrupole coupling constants.

From the analysis of the 55Mn and 14N HFCs above, we can confidently rule out the -2 and

-3 models which contain W1 as a hydroxo group and will confine our further analysis to

the -1 and -4 models.

17O Hyperfine Couplings

Rapatskiy et al. performed W-band ELDOR detected NMR on 17O labelled PSII samples

and found three classes of signal in the spectra which were termed strong, intermediate and

matrix.16 The strong signal was found to have an isotropic HFC of magnitude 9.7 MHz and

was experimentally assigned to a μ-oxo bridging oxygen on the basis of HFCs previously

measured for a MnIIIMnIV μ-oxo bridged model complex.16,93 In addition Rapatskiy et al.

used the relative orientations of the 14N and 17O experimental hyperfine tensors to assign

the exchangeable μ-oxo bridging HFC to either O4 or O5, although subsequent 14N

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experiments by Lohmiller et al. found there to be disagreement between the 14N datasets

questioning this assignment.16,86 The intermediate signal produced an isotropic HFC value

of magnitude 4.5 MHz and was assigned to one or both of the terminal water ligands of

MnA. The matrix class of signal was found to possess an isotropic HFC value of magnitude

1.4 MHz and assigned to weakly coupled matrix waters (either manganese or calcium

coordinated).16

Bridging atoms currently highlight a problem in the spin projection techniques currently

used to calculate hyperfine couplings for BS-DFT calculations. Non-bridging ligand nuclei

are normally spin projected using the spin projection coefficients of the metal ion they are

coordinated to. For bridging nuclei a number of solutions have been proposed. The first is

to simply average the two projected hyperfine couplings,94,95 while an alternative approach

is to sum the spin projections.96 From our investigations of several μ-oxo bridged

manganese complexes (see Tables S2 and S3 in Supporting Information) and the results of

Rapatskiy et al. we conclude that the second spin projection technique produces results in

better agreement with experiment.96 A comparison of calculated and experimental 17O

HFCs obtained for the Ca-1 and Ca-4 models is shown in Table 6.

Table 6. Calculated spin projected isotropic (A iso) and anisotropic (Ti) 17O hyperfine couplings (in MHz) for the investigated Ca models and comparison with experimental data.

Label Aiso T1 T2 T3

Ca-1

W1 −1.4 −1.2 0.5 0.7W2 −5.5 −1.1 0.4 0.7O1 0.2 −18.9 −2.9 21.8O2 6.0 −24.6 −7.5 32.1O3 7.3 −12.9 −1.1 16.1O4 1.6 −27.0 7.8 19.2O5 −10.3 −18.6 −10.8 29.4

Ca-4 W1 −1.7 −0.9 0.4 0.5W2 0.3 −1.0 0.3 0.7O1 0.9 −20.7 −1.4 23.2O2 7.0 −19.9 −7.6 27.5O3 7.9 −22.8 3.4 26.2

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O4 −0.4 −13.2 −6.3 19.5O5 −7.7 −12.1 −3.5 15.6

Exp.16|9.7| 4.5 -1.0 -3.4|4.5| 1.2 −0.5 −0.6|1.4| 1.2 −0.6 −0.7

Considering first the calculated results for the μ-oxo bridging atoms (O1 through to O5) the

model Ca-1 produces isotropic HFCs in the range of 0−10 MHz. The calculated isotropic

HFC for O5, -10.3 MHz agrees very well with the experimental value of |9.7| MHz

supporting the experimental assignment made, by Rapatskiy et al.16 The calculated

anisotropic magnitude is however significantly larger than the experimental determination

reported for O5. The isotropic HFCs for the manganese bound W1 and W2 calculated for

Ca-1 are also in very good agreement with the isotropic HFC magnitudes reported for the

intermediate and matrix signals. In addition the magnitude of the anisotropic HFCs, for

both W1 and W2 in the Ca-1 model, were found to agree very well with those determined

from experiment. The calculated isotropic HFCs for the model Ca-1 also correspond well

with those reported by Rapatskiy et al. (4.7 and 1.5 MHz respectively).44 Here agreement

between theory and experiment is much better for the Ca-1 model compared with Ca-4

which again adds further support to this model of the OEC in the S2 state. The calcium

bound waters W3 and W4 are expected to display only small HFCs owing to the absence

spin on the calcium ion.

The isotropic and anisotropic HFCs for the Sr models are given in Table S12 of

Supporting Information and are similar to those calculated for the Ca models.

1H Hyperfine Couplings

Table 7 shows selected 1H HFC calculated for the Ca cluster models as well as recent

HYSCORE data for the native OEC. The spectra reported by Milikisiyants et al. for the

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native OEC showed a number of signals HI – HV originating from interacting protons.91

Milikisiyants et al. assigned the HI and HIII group of protons to fully protonated water

molecules, W1 and W2 directly ligated to MnA of the OEC. The HII proton group was

assigned to the proximal protons of the D1-His-332 residue. The remaining detected proton

signals were attributed to non-specific matrix proton interactions.

Considering the calculated results for model Ca-1, Table 7, it can be seen that the W1

protons HA and HB produce isotropic and anisotropic HFCs in good agreement to those

observed for the HI group of protons, with particular good agreement for HB of W1.

Although the two W1 protons would be expected to be equivalent in an isolated system,

the hydrogen bonding interaction between Asp-61 and HA lowers the calculated Aiso and T

value. Similar behaviour is observed in experimental and computational studies of

ammonia inhibition of the OEC, where ammonia has been to found to replace W1 and

hydrogen bond to the Asp-61 residue.97,98 The Ca-1 model also gives isotropic and

anisotropic HFCs for the W2 HC hydroxide proton in very good agreement with the

experimental results found for the HIII proton group. This result differs with the

experimental interpretation of Milikisiyants et al. who interpreted the HIII proton signal as

arising from a fully protonated W2 water and not a hydroxide group. This interpretation

was due to the observed Aiso values showing agreement to previously published 2D 1H

HYSCORE spectra of a water ligated dimanganese model complex.48,99 It was speculated

that a hydroxo group would give rise to a much larger isotropic HFC but this is not bourne

out by our calculated values. The calculated results for Ca-4 model where W2 is a water

ligand are not in as good agreement with the experimental value, lending extra support for

the hydroxo nature of W2 in the S2 state as already found above. The assignment of the

experimentally observed HII protons to the ring protons of the proximal D1-His332 residue

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is also supported by our calculations. Both protons have small calculated isotropic and

larger anisotropic T values close to the experimental value.

Table 7. Calculated spin projected isotropic (Aiso) and anisotropic (Ti) 1H hyperfine couplings (in MHz) for the investigated Ca-1 and Ca-4 models and comparison with experimental data. T is defined as T = (T1 + T2)/2 = −T3/2

Label Aiso T1 T2 T3 T

Ca-1

W1 HA 1.0 −3.9 −2.7 6.6 −3.3W1 HB 1.7 −5.0 −4.3 9.3 −4.6W2 HC 3.0 −2.0 −1.7 3.8 −1.9W2 HD − − − − −His HE 0.1 −5.0 −1.1 6.2 −3.1His HF −0.8 −4.2 −2.9 7.1 −3.6

Ca-4

W1 HA 0.7 −2.5 −1.6 4.1 −2.0W1 HB 1.6 −3.6 −3.2 6.8 −3.4W2 HC 1.0 −2.5 −2.1 4.6 −2.3W2 HD 1.3 −2.5 −2.1 4.6 −2.3His HE 0.1 −5.6 −1.2 6.8 −3.4His HF −0.9 −4.7 −3.3 8.0 −4.0

Exp.48

HI |1.8| − − − |4.4|HII |0.1| − − − |4.1|HIII |2.6| − − − |1.9|HIV |0.2| − − − |2.3|HV |0.4| − − − |1.4|

Table 8 shows the calculated 1H isotropic and anisotropic HFCs for the Sr models in

addition to HYSCORE data from experimental studies of the Sr substituted OEC. Unlike

the native OEC, Chatterjee et al. only found a single signal, HI, originating from direct

ligation to the OEC. 100 This signal was found to have similar isotropic and anisotropic

HFCs to that seen in the native OEC and assigned to the ring protons of the D1-His-332

residue. In contrast to the native OEC, Chatterjee et al. could find no significant HFCs

signals originating from either the W1 or W2 protons leading them to conclude that Sr

substitution results in a strongly disordered geometry for these water ligands that perturbs

these groups and causes a large modification in their HFCs. 100 The BS-DFT calculated

HFCs for the Sr models are very similar to the native form and would be expected to occur

at similar positions in the experimental spectra. No significant perturbation of W1 and W2

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are observed in our models as was also found in the Sr OEC X-ray crystal structure. As can

be seen in Table 8, the isotropic and anisotropic HFCs calculated for both the W1 protons

(HA and HB) and the W2 hydroxo proton (HC) are similar to those calculated for the Ca-1

analogue model. These calculations in conjunction with those presented earlier would

suggest that Sr substitution has little or no effect on the calculated HFCs of the W1 and W2

groups. We suggest therefore that the lack of detection of experimental signals for the W1

and W2 protons in Sr substituted OEC is due to a detection limitation rather than a major

change in value introduced by Sr substitution.

Table 8. Calculated spin projected isotropic (Aiso) and anisotropic (Ti) 1H hyperfine couplings (in MHz) for the investigated Sr-1 and Sr-4 models and comparison with experimental data. T is defined as T = (T1 + T2)/2 = −T3/2

Label Aiso T1 T2 T3 T

Sr-1

W1 HA 1.0 −4.0 −2.7 6.7 −3.4W1 HB 1.5 −4.3 −4.0 8.3 −4.2W2 HC 3.2 −2.3 −1.5 3.7 −1.9W2 HD − − − − −His HE 0.0 −4.5 −0.8 6.2 −3.1His HF −0.7 −4.3 −3.0 7.3 −3.6

Sr-4

W1 HA 0.9 −2.4 −1.6 3.9 −2.0W1 HB 1.7 −3.8 −3.0 6.7 −3.4W2 HC 0.8 −2.3 −1.8 4.1 −2.1W2 HD 1.8 −2.7 −1.2 3.9 −2.0His HE 0.1 −5.1 −1.2 6.3 −3.2His HF −0.8 −4.1 −3.3 7.4 −3.7

Exp.100H1 ~0 − − − |4.1|HII |0.2| − − − |2.2|HIII |0.2| − − − |1.5|

13C Hyperfine Couplings

Stull et al. used ENDOR spectroscopy to study the S2 state in a PSII preparation where all

alanine carboxylate carbons were 13C labelled as well as a scenario where all carbon atoms

were uniformly 13C labelled. These results were then compared to a bridging carboxylate in

a synthetic dinuclear MnIIIMnIVcomplex.57 These results, published before the 2011

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Umena et al. crystal structure,10 led to the conclusion that the D1 polypeptide alanine C-

terminus is directly bound to a manganese ion. In the simulations of the ENDOR spectra,

Stull et al. were required to make a number of assumptions in order to interpret the

experimental spectra, namely the dipolar hyperfine couplings were estimated using the

point dipole approximation from the various X-ray structures available at the time

(provided by Loll et al., Guskov et al. and Ferreira et al.).13,101,102 Table 9 summarises the

computational results obtained for the Ca models studied, in comparison with the

experimental data. For carboxylates which bridge two manganese sites, we have utilised

the same spin projection technique used above for spin projecting bridging oxygen nuclei;

the intrinsic hyperfine coupling tensors are spin projected to both of the two manganese

sites and them summed. In the case of terminal or Mn−Ca bridging carboxylates, the 13C

nuclei were spin projected to the directly bonded manganese site.

In both the Loll et al. and Guskov et al. X-ray crystallographic structures, the alanine C-

terminus of the D1 polypeptide chain was bonded to one manganese centre,101,102 unlike the

Ferreira et al. crystal structure, which proposed the alanine C-terminus to be bonded only

to the calcium atom of the OEC.13 The high resolution 2011 Umena et al. structure and

2014 XFEL structure of Suga et al. found the D1-Ala-344 residue to be bonded to both

MnC and the Ca2+ ion of the OEC.10,11

Inspection of the data in Table 9 of the Ca-1 model shows that the Ala-344 residue

provides an isotropic and anisotropic hyperfine coupling which is in good agreement with

the experimental data. Additionally Stull et al. found that in the uniformly labelled sample

there were multiple 13C containing moieties which produced hyperfine couplings similar to

that observed for the Ala-344 labelled example.57 This observation is supported by the

results shown in Table 9, as multiple residues in model Ca-1 provide similar isotropic and

anisotropic hyperfine couplings (Asp-170 and Asp-342) within the joint uncertainties of

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computation and simulation. Schinzel et al 82 also previously compared BS-DFT calculated

13C HFCs with the experimental values. This study was performed before the high

resolution crystal structure of the OEC was available which limited accurate assignment

possibilities.

Table 9. Calculated spin projected isotropic (Aiso) and anisotropic (Ti) 13C hyperfine couplings (in MHz) for the investigated Ca models and comparison with experimental data.

Label Aiso T1 T2 T3

Ca-1

Asp-61 0.0 −0.2 −0.1 0.3Asp-170 1.3 −2.0 −0.7 2.6Glu-189 2.1 −1.3 −1.1 2.4Glu-333 2.6 −3.9 0.2 3.7Asp-342 −1.9 −4.5 −0.5 5.0Ala-344 −1.6 −1.9 −0.7 2.6Glu-354a −4.3 −2.6 0.3 2.3

Ca-4

Asp-61 −0.0 −0.2 −0.1 0.2Asp-170 1.6 −1.4 −0.1 1.5Glu-189 3.0 −1.5 −1.2 2.7Glu-333 1.3 −2.4 0.3 2.2Asp-342 −2.3 −5.9 −0.4 6.3Ala-344 −1.7 −1.7 0.8 0.9Glu-354a −3.6 −2.3 0.4 1.9

Exp.57 -1.0 −2.4 −0.8 3.2a Residue from the CP43 protein chain, all other residues from the D1 protein chain

13C data for the Sr models are similar to the Ca models and are given in the Supporting

Information.

CONCLUSIONS

In this study a thorough BS-DFT analysis of the OEC S2 state 55Mn and ligand hyperfine

couplings was performed investigating the effects of altering the protonation states of the

W1 and W2 ligands. In addition the effect of Sr substitution for Ca was investigated.

Using large geometry optimised cluster models of high resolution dark adapted crystal

structures, we show that slight changes in the structure as a result of altering the

protonation state of the W1 and W2 oxygens had a profound effect on the calculated 55Mn

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HFCs. Such variations arise due to small changes in the Heisenberg exchange coupling

constants which affect the spin projection coefficients. Comparison between experimental

and calculated HFCs for both the native Ca OEC and Sr substituted form clearly show that

W1 is present in the S2 state as a water molecule and W2 is present as a hydroxo.

Substitution of the Ca for Sr has a minor effect on the calculated HFCs showing that the S2

electronic structure of the OEC is not significantly altered by this substitution. The ability

to be able to distinguish between small structural differences such as protonation patterns

using this combination of experimental and BS-DFT calculated EPR parameters

demonstrates the unique ability of this combination of theory and spectroscopy to probe

the OEC electronic structure. Such an analysis can now be confidently applied to the S3

state where it has been found that Ca/Sr substitution gives rise to large differences in its

EPR properties. Probing the electronic origin of such differences can provide a key and

unique insight into the final stages of the water oxidation cycle.

ACKNOWLEDGEMENTS

NJB and TAC acknowledge support from the UK BBSRC Doctoral Training Partnership

(DTP) program.

ASSOCIATED CONTENT

Supporting Information

Additional analysis and discussion of calculated exchange coupling constants, spin

projection coefficients and hyperfine couplings mentioned in manuscript. Available free of

charge at http://pubs.acs.org

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TOC Graphic

S2 Frontier Orbitals

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