1. Introduction
Photosynthesis utilizes the solar energy absorbed by pigments and transferred in form of electronic excitation energy to photosynthetic reaction center (RC) [
1,
2,
3,
4,
5], common to all photosynthetic species, where it is converted into a charge gradient needed for long term storage of solar energy. The RC from the purple bacterium
Rhodobacter (
Rba.)
sphaeroides includes eight pigment molecules classified into four groups: special pair of bacteriochlorophylls (P), two accessory BChls (B), two bacteriopheophytins (I) and two ubiquinones (Q) (
Figure 1, [
6]). While P and B are located at the periplasmic side of the membrane, and Q at the cytoplasmic side, I is placed approximately half-way across the membrane. A slight asymmetry in the structure of the RC leads to a similar asymmetry in the energy levels of the pigments leading to a highly dominant (A branch) and a non-dominant (B branch) path for charge separation. However, the design can be nearly completely reversed by changes of some crucial amino acids [
7]. The proximity between the BChls in the special pair and between the B
A and I
A pigments suggests strong interaction between their excited states, leading to coherent sharing of the excitation energy [
8,
9]. Similarly, the charge separated state produced initially (~3 ps) after decay of P* is a mixture of vibrationally hot P
+B
A− and P
+I
A− states, which then relaxes within ~1 ps into the cool P
+I
A− state [
10]. The subsequent electron transfer to Q
A with a lifetime of ~200 ps produces a membrane-spanning radical pair P
+Q
A– that is stable on a millisecond timescale.
The energetics, kinetics and pathway of electron transfer centred at I
A are exposed to protein environment and dynamics [
11]. Several evidence have been accumulated in favour of time-dependent relaxations of the P
+I
A─ state (
Figure 2). Based on very fast (1-10 ns) decay of fluorescence, the free energy difference between P* and P
+I
A─ was estimated between 210 and 260 meV in accordance with 250-260 meV obtained from effects of magnetic fields and temperature on the fast (~ 50 μs) decay of the excited
3P triplet state [
12]. Quinone replacement studies indicated that RCs may undergo on the micro- and millisecond time scale further relaxations which increase the free energy difference up to 340 meV after initial charge separation [
13]. However, additional studies are required to test the upper limit of energetic relaxation of the P
+I
A─ state and to distinguish from those of the P
+Q
A─ states.
The anionic states formed during electron transfer induce not only reorganization of the protein environment [
14], but also out-of-plane distortion of the chlorin ring [
15]. Two distinct conformations of I
A•– were reported in spectroscopic studies of RC from
Rba. sphaeroides [
16]. Recently, the XFEL (X-ray free electron) structures revealed how the charge separation process was stabilized by protein conformational dynamics [
17].
The perturbation of the free energy level of the P
+I
A─ charge-separated state can be attributed to nearby amino acids whose contributions have been thoroughly studied [
18] but not always fully understood [
19]. One highly examined residue has been the tyrosine at site M210 because it lies between P and the initial electron acceptors and is a key residue involved in the initial forward electron transfer. Mutant RCs have altered rates of the initial electron transfer (reviewed in [
20,
21]). Theoretical studies indicates that the magnitude and orientation of the hydroxyl dipole of tyrosine M210 may play an important role in energetic stabilization of P
+I
A– [
22]. Indeed, changes of the orientation of this tyrosine’s hydroxyl dipole slowed the electron transfer significantly [
23]. Different mutations at M214 near I
A decreased the rate of I
A– → Q
A electron transfer resulted in competition with the charge recombination between P
+ and I
A– and in a drop of the overall yield of charge separation [
24]. The effects correlated with the volume of the mutant amino acid side chains. Similar results were obtained when the native bacteriopheophytin was replaced by BChl [
25]. The perturbation of the electronic environment in the vicinity of P
+I
A–, and Q
A, affected both the extent and time scale of the dielectric relaxation. A 4-fold decrease in the electron transfer rate from I
A– to Q
A and similar decrease in the recombination rate P
+Q
A– → PQ
A were observed in RC lacking the H subunit (LM dimer). It was interpreted as the increased flexibility in the region around Q
A and the associated shifts in the reorganization energy of the electron transfers relative to that of the native RC [
26].
The light-induced P
+I
– and P
+Q
– dipoles are stabilized both by release of H
+ ions to the periplasmic side, by uptake of H
+ ions from the cytoplasmic side of the RC and by internal proton rearrangement, which processes have not only energetic, but temporal and structural constrains, as well. The flash-induced P
+ state results in very limited proton release [
27] and consequently in very small energetic stabilization of the dipole. Continuous illumination, however, produces significant release of protons, up to six protons per RC for a 300 s light exposure [
28]. The observed very slow charge recombination and proton release/uptake kinetics pointed to cascade of lengthy conformational changes together with suspected formation of a hydrogen-bond network between P
+ and the periplasmic aqueous phase [
29,
30]. On the other end of the dipole, the H
+ uptake in response to the immediate (within 200 ps) formation of P
+Q
A− was found to be rate-limited by intraprotein conformational process [
31]. In native RC, the lifetime of P
+I
A– (
τI~13 ns) is much shorter than the time required for protonation to accommodate the dipole. The relatively slow response of protonation prohibits the stabilization via proton rearrangement. In AQ substituted RC, however, the lifetime of P
+I
A– is increased significantly to
τI·(1+
K2)~1 ms, where
K2 (~ exp(Δ
GAI/
kBT) denotes the equilibrium constant between P
+Q
A– and P
+I
A– states [
32]. Although in small fraction of RCs, the increased lifetime of P
+I
A– state makes possible to observe the stabilization through protonation.
The kinetics and stoichiometry of flash-induced proton uptake upon formation of either Q
A− or Q
B− are correlated, suggesting that the same residues respond to the generation of both semiquinone species [
33,
34,
35]. The Q
B domain is rich of protonatable residues that can account for uptake of protons in response to appearance of negative charges on Q
B and Q
A [
36,
37,
38]. The substoichiometric proton uptake and/or internal redistribution of H
+ ions arise largely from the same cast of characters in the Q
B domain and supports the lack of ionizable residues around Q
A and I
A [
37,
39]. However, the interactions within the ionization states of the individual residues in the complex network and between the acidic cluster and the semiquinones are still not reliably accounted for by existing computational and spectroscopic methods. Discrepancies between calculations and experiments (particularly FTIR) remain unresolved for some key residues in the cluster [
40,
41].
Whether I
A‒ can interact with the remote acidic cluster and what are the possible consequences of this interaction are open questions. There are some experimental indications that the acidic cluster may cooperate with the appearance of the negative charge on I
A. Q
A–-induced red shift of the Q
y absorption band of I
A was observed that was pH-dependent and showed the involvement of proton transfer in the protein relaxation [
42]. The absence of the 400 μs component in the relaxation kinetics of the L212Glu-Ala mutant suggested that this residue of the cluster was involved in the relaxation mechanism. The low effective dielectric allows the spread of electric field from I
A− in the membrane further to the Q
B region featured by an unusually high density of ionizable residues with a striking excess of acidic groups. In this way, the cluster of ionizable residues around Q
B should contribute substantially to the partial shielding and stabilization of the light-induced P
+I
A– dipole. However, the direct experimental proof, the mechanism and the extent of the cross-talk have remained unresolved.
Here, we set the aim to get direct experimental evidence to this interaction. The protonation changes in the acidic cluster around QB upon appearance of P+QA– and P+IA– was probed by substitution of the native UQ10 by several low potential analogues of anthraquinone (AQ) and by combined measurements of the delayed fluorescence and charge recombination attributed to P+QA– → PQA. With AQ, as opposed to UQ, the charge recombination occurs through indirect pathway via P+IA– and the rate is sensitive to small perturbations of the free energy states of P+QA– and P+IA–. It is revealed that the free energy levels of P+IA– states were pH-dependent at high (> 10) pH values indicating the participation of residues of high pKa values in the interaction between the acidic cluster around QB and IA─. Relative to P*, the stabilization of the relaxed (ms) state of the P+IA─ dipole compared to that of the hot (ns) state increased more than 50% due to this coupling and to the protonation coupled slow conformational changes.
3. Results
The kinetics of charge recombination were measured in RCs of purple bacterium
Rba. sphaeroides where the native ubiquinone
10 was replaced by low potential anthraquinones at the primary quinone binding site (
Figure 4 top). The charge recombination from the P
+Q
A─ state can follow two parallel routes, and the rate of the observed reaction will be the sum of the rates of the two reactions ([
62], Eq. (1)). The first reaction is a direct tunnelling to the ground state, and the second one is an uphill (indirect) reaction to P
+I
A‒, where P
+Q
A─ pre-equilibrates with P
+IA
─ before decaying to the ground state (
Figure 2). By replacement of various quinones of very different midpoint redox potentials for the native Q
A (UQ
10), P
+Q
A‒ will recombine indirectly via P
+I
A─ if Δ
G*<0.8 eV, and directly if Δ
G*>0.8 eV [
13]. The free energy level of the P
+Q
A─ state relative to that of the P
+I
A─ state can be determined from the relative contribution of the uphill reaction [
13,
48,
63,
64,
65]. In all our cases, faster kinetics were obtained than that with UQ
10 at the Q
A site indicating the contribution of the indirect way of the charge recombination. The lower is the midpoint potential of the anthraquinone, the more significant is the Boltzmann term in Eq. (1), therefore the increase of the rate constant of the back reaction. As the energy gap for the indirect way of recombination depends on the interactions with protonatable groups, the observed rate constants depend not only on the temperature but on the pH, as well. The sharp difference between the pH-dependence of the charge recombination rates for AQ and UQ
10 are demonstrated in
Figure 5. Because the rate of direct charge recombination is hardly controlled by the driving force, very slight pH-dependence can be observed if Q
A is the native ubiquinone. However, if UQ
10 is replaced by AQ, the RC will perform increasing rate of the back reaction upon increasing pH. In contrast to earlier work [
66], no signs of saturation can be seen in the pH range studied here.
According to Eq. (1), the free energy gap of the thermal activation Δ
Go(P
+I
A–Q
A → P
+I
AQ
A–) is worth to be introduced instead of the rate constants. The van’t Hoff analysis of the temperature dependence of the measured rate constants offers the difference of the free energy levels of P
+I
A─Q
A and P
+I
AQ
A─ that proves to be slightly pH-dependent in the alkaline pH region (
Figure 6). This is a strong indication that either Q
A─ or I
A─ or both are in interaction with protonatable residues in the RC and the interactions are slightly different. The van’t Hoff analysis of the rate constants of the charge recombination gives information about the pH-dependence of the difference of the free energy levels but not about the pH-shifts of the individual P
+I
A–Q
A and P
+I
AQ
A– states. The observed difference may come exclusively from stabilization of the Q
A– state at low pH or from stabilizations of both states but in different extents. If we intend to distinguish the two effects and to determine the pH-induced displacement of the state of I
A─ separately, the measured values should be corrected to those attributed to Q
A─. We need a different and independent method for the separation. The delayed fluorescence of the bacteriochlorophyll dimer is an appropriate assay. By comparison of the yields of the prompt and delayed fluorescence of P*, the absolute values of the free energy states of the low potential quinones can be obtained.
As the delayed fluorescence comes from the leakage of the charge separated state P
+Q
A─, it will follow the kinetics of charge recombination (
Figure 4 bottom). Because of the relatively slow (about 100 ms) back reaction of RC with native ubiquinone
10, the delayed fluorescence can be measured by mechanical shutter with good signal-to-noise ratio. However, the recombination times become much smaller (in the ms time range) upon replacement UQ
10 by low potential quinones and accordingly the kinetics of the delayed fluorescence will be faster. The slow response of the mechanical shutter will limit the time resolution of the kinetics. The electronic switching of the photomultiplier and time-correlated single photon counting of the signal was used to avoid the artifacts caused by the intense prompt relative to the very weak delayed fluorescence of the sample [
50,
53]. With this method, the charge recombination kinetics can be resolved in the sub millisecond time scale and the free energy level of the P
+Q
A− state relative to that of P*Q
A can be determined from the measurement of the delayed fluorescence of the BChl dimer (see Eq. (2)).
Figure 7 demonstrates these values for RCs where the native UQ
A was substituted by a series of low potential AQ derivatives. The free energies perform either no (1-chloro-AQ) or (above pH 10) slight (
≈ 10-15 meV/pH unit) pH dependence. These values are in good accordance with those of previous measurements [
13,
48]. To verify that the pH dependence observed for rates of charge recombination and intensity of delayed fluorescence were not artifacts of the quinone removal and reconstitution process, they were also measured for RCs reconstituted with UQ
10. The essential pH independence for
kAP(UQ
10) and slight pH-dependence for ∆
GP*A(UQ
10) were in good agreement with those presented earlier [
48,
49,
67].
If the free energy gap between P+IA–QA → P+IAQA– is subtracted from the free energy level of P+QA–, the free energy state of IA─ would be obtained. Comparing the two set of curves for different AQ substituents, the following conclusions can be drawn. 1) It is not expected that the free energy state of IA─ would depend on the chemical nature of the substituent at the QA binding site. However, the free energy levels of IA─ for different substituents are not unified into a single trace but constitute a narrow branch of curves. This will indicate that the lowest level of P+IA– relaxation will depend slightly on the chemical nature of QA. Different QAs will cause different degree of relaxation of P+IA–. 2) The free energy levels of P+IA– show definite pH-decrease at the highly alkaline pH range (pH > 10) in an extent comparable to that of P+QA–. Similar residues of high pKa values may participate in the pH-dependent interaction with the negative charge on QA and IA. Likewise, as for P+QA–, 1-chloro-AQ performs no pH-dependence indicating the possibility of unique binding structure at the QA site which may reduce (block) the electrostatic interactions with the cluster of residues.
The standard free energies between P
+Q
A─/P* and P
+Q
A─/P
+I
A─ obtained from direct measurements of the intensity of the DL and the rates of charge recombination consist of enthalpic (Δ
Ho) and entropic (
T·Δ
So) terms: Δ
Go = Δ
Ho -
T·Δ
So that can be determined from temperature-change measurements [
38]. The enthalpy changes can be obtained from the temperature-dependence of the amplitude (integral) of the decay of the delayed fluorescence as the slopes of the straight lines offer the enthalpy change of the charge separation (van’t Hoff plot,
Figure 8). The thermodynamic parameters for the different quinones in the Q
A site are summarized in
Table 1. The changes of the free energy and the enthalpy of the P* → P
+Q
A─ and P
+I
A─ → P
+Q
A─ transitions are negative for all quinone analogues indicating spontaneous and exothermic reactions, respectively. The entropy changes perform large variations upon quinone substitution and are positive (with assumption of 1-chloro-AQ in the P
+I
A─ → P
+Q
A─ transition) representing increase in the disorder of the system.