| Cumulant Analysis of Charge Recombination Kinetics in Bacterial Reaction Centers Reconstituted into Lipid Vesicles Biophysical Journal, Volume 79, Issue 3, 1 September 2000, Pages 1171-1179 Gerardo Palazzo, Antonia Mallardi, Mauro Giustini, Debora Berti and Giovanni Venturoli Abstract The kinetics of charge recombination between the primary photoxidized donor (P) and the secondary reduced quinone acceptor (Q) have been studied in reaction centers (RCs) from the purple photosynthetic bacterium incorporated into lecithin vesicles containing large ubiquinone pools over the temperature range 275K≤T≤307K. To account for the non-exponential kinetics of P re-reduction observed following a flash, a new approach has been developed, based on the following assumptions: 1) the exchange of quinone between different vesicles is negligible; 2) the exchange of quinone between the Q site of the RC and the quinone pool within each single vesicle is faster than the return of the electron from the primary reduced acceptor Q to P; 3) the size polydispersity of proteoliposomes and the distribution of quinone molecules among them result in a quinone concentration distribution function, P(Q). The first and second moments of P(Q) have been evaluated from the size distribution of proteoliposomes probed by quasi-elastic light scattering (mean radius, 〈R〉=(50±15) nm). Following these premises, we describe the kinetics of PQ recombination with a truncated cumulant expansion and relate it to P(Q) and to the free energy changes for QQ→QQ electron transfer () and for quinone binding () at Q. The model accounts well for the temperature and quinone dependence of the charge recombination kinetics, yielding =−7.67±0.05kJmol and =−14.6±0.6kJmol at 298K. Abstract | Full Text | PDF (161 kb) |
| Residual Water Modulates QA-to-QB Electron Transfer in Bacterial Reaction Centers Embedded in Trehalose Amorphous Matrices Biophysical Journal, Volume 85, Issue 4, 1 October 2003, Pages 2760-2775 Francesco Francia, Gerardo Palazzo, Antonia Mallardi, Lorenzo Cordone and Giovanni Venturoli Abstract The role of protein dynamics in the electron transfer from the reduced primary quinone, , to the secondary quinone, , was studied at room temperature in isolated reaction centers (RC) from the photosynthetic bacterium by incorporating the protein in trehalose water systems of different trehalose/water ratios. The effects of dehydration on the reaction kinetics were examined by analyzing charge recombination after different regimes of RC photoexcitation (single laser pulse, double flash, and continuous light) as well as by monitoring flash-induced electrochromic effects in the near infrared spectral region. Independent approaches show that dehydration of RC-containing matrices causes reversible, inhomogeneous inhibition of -to- electron transfer, involving two subpopulations of RCs. In one of these populations (i.e., ), the electron transfer to is slowed but still successfully competing with recombination, even in the driest samples; in the other (i.e., ), electron transfer to after a laser pulse is hindered, inasmuch as only recombination of the state is observed. Small residual water variations (∼7wt %) modulate fully the relative fraction of the two populations, with the active one decreasing to zero in the driest samples. Analysis of charge recombination after continuous illumination indicates that, in the inactive subpopulation, the conformational changes that rate-limit electron transfer can be slowed by >4 orders of magnitude. The reported effects are consistent with conformational gating of the reaction and demonstrate that the conformational dynamics controlling electron transfer to is strongly enslaved to the structure and dynamics of the surrounding medium. Comparing the effects of dehydration on → recombination and → electron transfer suggests that conformational changes gating the latter process are distinct from those stabilizing the primary charge-separated state. Abstract | Full Text | PDF (283 kb) |
| Quinone-Dependent Delayed Fluorescence from the Reaction Center of Photosynthetic Bacteria Biophysical Journal, Volume 79, Issue 1, 1 July 2000, Pages 14-25 Kinga Turzó, Gábor Laczkó, Zoltán Filus and Péter Maróti Abstract Millisecond delayed fluorescence from the isolated reaction center of photosynthetic bacteria was measured after single saturating flash excitation and was explained by thermal repopulation of the excited bacteriochlorophyll dimer from lower lying charge separated states. Three exponential components (fastest, fast, and slow) were found with lifetimes of 1.5, 102, and 865ms and quantum yields of 6.4×10, 2.2×10, and 2.6×10 (pH 8.0), respectively. While the two latter phases could be related to transient absorption changes, the fastest one could not. The fastest component, dominating when the primary quinone was prereduced, might be due to a small fraction of long-lived triplet states of the radical pair and/or the dimer. The fast phase observed in the absence of the secondary quinone, was sensitive to pH, temperature, and the chemical nature of the primary quinone. The standard free energy of the primary stable charge pair relative to that of the excited dimer was −910±20 meV at pH 8 and with native ubiquinone, and it showed characteristic changes upon pH and quinone replacement. The interaction energy (∼50 meV) between the cluster of the protonatable groups around GluL212 and the primary semiquinone provides evidence for functional linkage between the two quinone binding pockets. An empirical relationship was found between the free energy of the primary quinone and the rate of charge recombination, with practical importance in the estimation of the free energy levels from the easily available lifetime of the charge recombination. The ratio of the slow and fast components could be used to determine the pH dependence of the free energy level of the secondary stable charge pair relative to that of the excited dimer. Abstract | Full Text | PDF (180 kb) |
Copyright © 2000 The Biophysical Society. All rights reserved.
Biophysical Journal, Volume 79, Issue 3, 1237-1252, 1 September 2000
doi:10.1016/S0006-3495(00)76378-8
Biophysical Theory and Modeling
Alexander O. Goushcha*, †,
,
, Valery N. Kharkyanen‡, Gary W. Scott† and Alfred R. Holzwarth*
* Max-Planck-Institut für Strahlenchemie, Ruhr 45470, Germany
† Department of Chemistry, University of California at Riverside, Riverside, California 92521 USA
‡ Institute for Physics, National Academy of Science–Ukraine, Kyiv 252028, Ukraine
Address reprint requests to Dr. Alexander O. Goushcha or Prof. Gary W. Scott, Dept. of Chemistry, University of California at Riverside, Riverside, CA 92521. Tel.: 909-787-4732; Fax: 909-787-4713.Biological energy conversion and storage take place through elementary events of charge transport in biomolecules. Transient, localized charges interact with ionized, polarizable, or dipolar structural elements of the macromolecule to perturb cofactor and/or protein structural modes. These interactions couple localized electron states to nuclear degrees of freedom that may be reduced to a single (generalized) coordinate (see, e.g., Agmon and Hopfield, 1983). This coordinate may be either collective or localized, corresponding in the latter case to motion of specific structural groups. Characteristic relaxation times of structural motion may vary widely, facilitating either an adiabatic or a non-adiabatic elementary charge transfer event in the biomolecule (see Hoff and Deisenhofer, 1997, for a review). The present work focuses on effects that occur during multiple, sequential charge transfer events when structural relaxation is significantly slower than the charge transfer rate itself.
The relevance of slow structural dynamics to the function of biological charge transfer system function has been demonstrated many times. Photosynthetic reaction centers (RCs) exhibit a long-lived, structural relaxation for minutes after completion of electron transfer (ET) (Puchenkov et al,Kalman and Maroti, 1997). Numerous studies of bacteriorhodopsins indicate slow (tens of seconds) structural motions induced by a proton flux (Nagel et al,Sass et al). Long-lived structural modes are also important for the function of cytochrome oxidases (Einarsdottir et al) and ATPases (Noji et al). For such modes, transient, localized charges interact with structural elements of the biomolecule, and the effects of these interactions accumulate during successive events. Accumulated structural changes produce feedback on the charge transfer rate. Thus, slow conformational modes function as control modes to determine long-time biomolecule behavior (Haken, 1983). The action of a charged particle flux on slow conformational modes and structural feedback on charge transfer rate constants produce non-linear, self-regulation effects (Chinarov et al,Tributsch and Pohlmann, 1998,Goushcha et al,Gushcha et al). These self-regulation processes should be quite important for the function of charge transfer biomolecules, modulating the charge-transfer rate. To describe these effects, we propose a self-consistent, adiabatic theory of charge transfer and structural motion. This theory develops a correlation of structural dynamics and electron transfer, ensuring a correct statistical description of electron-conformational dynamics in macromolecules by considering system diffusion along an effective adiabatic potential. This approach generalizes an adiabatic theory for a single ET event to the case of multiple, successive ET events, each of which induces small but long-lived structural changes that accumulate to influence subsequent events.
We develop this theory for photosynthetic reaction centers, but most of our results can be readily generalized to other macromolecular charge transfer systems. For an intact photosynthetic system, charge separation efficiency is determined by the quantum yield of the primary charge separation event and the lifetime of the charge-separated state. The term “efficiency of charge separation” emphasizes that the average survival time of this state, as in isolated RCs, is the determining factor in intact systems, in which the quantum yield of the primary charge separation event is ≈1. (see Wraight and Clayton, 1973).
In this paper, we proceed as follows: 1) In the next (first) section, we develop a theory for a two-state charge-transfer system and for the more general case of a finite number of charge-transfer states. We show that the survival time of the charge-separated state reflects the light-induced structural changes of the system. 2) In the second section, we develop a general, kinetic description of the electron-conformational interaction in macromolecular systems. We show that slow, structural dynamics determine self-regulation effects in biomolecules. 3) In the third section, we analyze the dependence of stationary-state structural variable values with light intensity. 4) Finally, in the fourth section we apply the theory to photosynthetic RC recombination kinetics and quasi-stationary-state, light-induced effects.
Consider first the average lifetime of the charge-separated state for a simple system consisting of a photodonor D and an acceptor A, both inserted into a suitable matrix. The scheme of electron transfers in this system may be described by
![]() | (1) |
Let ρ(t, D) and ρ(t, A) be the normalized populations of the states, DA and D+A−, respectively, at time t. Then these quantities satisfy simple coupled differential rate equations for a fixed structure of the system:
![]() |
![]() |
![]() |
![]() |
![]() | (4) |
![]() | (5) |
![]() |
![]() | (6) |
The efficiency of charge separation under stationary-state illumination with a single photoactivated electron that transfers between a finite number of localized electron states is defined as the ratio of the stationary state probability of charge separation to the number of charge separation events per unit time
![]() | (7) |
![]() | (8) |
![]() | (9) |
What physical mechanisms may correlate macromolecular structural dynamics with photoactivated charge transfer along a cofactor chain? The following facts are relevant:
Statements 1–3 require no additional discussion. Support for statement 4, although previously discussed, is now amplified. For a system with a finite number of localized electron states but with no interactions with its surroundings, electron motion should be completely coherent and may be described in terms of a non-equilibrium density matrix as periodic oscillations of the electronic populations of these states (Landau and Lifshitz, 1965). However, absolute coherence of photoelectron motion is destroyed by interaction with thermal oscillations of the nuclei with relaxation times of ≈10−13–10−11 s. This means that non-diagonal elements of the density matrix may be neglected for slow steps of charge separation. The non-adiabatic description given by Fermi's Golden Rule is appropriate for this type of donor-acceptor transition (Landau and Lifshitz, 1965). The theory of non-adiabatic transitions has been well-developed in solid state physics by Förster, Dexter, and Galanin (Förster, 1949,Dexter, 1953,Galanin, 1951). An appropriate description of elementary steps of electron transfer in chemical and biological systems was given by Levich and Dogonadze, 1959,Marcus, 1956,Marcus and Sutin, 1985; and Jortner, 1976. See also the review by Hoff and Deisenhofer, 1997. It was shown that, in the high temperature limit, the rate constant ωij of ET between the ith and jth cofactors depends exponentially on both the donor-acceptor distance Rij and the value of (λij+ΔGij°)2/λij, in which λij is the nuclear reorganization energy and ΔGij° is the standard Gibbs free energy difference between the donor and acceptor levels (Marcus, 1956,Marcus and Sutin, 1985). This means that either a change in the distance between cofactors on the order of ∼1Å or a change in the macromolecule structure such that (λij+ΔGij°)2/λij changes by more than kBT may cause a significant difference in ωij.
The generalization of the Marcus expression for the rate constant of non-adiabatic ET in continuous media to the case of any solvent model shows that the rate constant for charge transfer may be expressed in terms of a function of the free energy difference between electron-localized donor and acceptor sites produced by a fluctuating polar medium (Tachiya, 1993). This approach leads to a Gaussian-like dependence of the charge transfer rate constant on the local electrostatic potential of the medium. Many current theories of charge transfer reactions in proteins are based on a similar evaluation of the probability distribution for a free energy difference ΔVij between product and reactant states (Warshel, 1982,Parson et al,Tachiya, 1993,Bandyopadhyay et al,Warshel and Parson, 1991,Webster et al). Such an approach not only provides for a correct molecular dynamic calculation of the potential surfaces of the reactant and product states, but also enables prediction of the influence of adiabatic structural motions. Molecular dynamic simulations show that photoinduced charge separation in photosynthetic reaction centers occurs in much shorter times than those required for the system to approach conformational equilibrium after the charge transfer step (Parson et al). Recent molecular dynamics studies also show that, for long-range electron transfer in proteins, cooperation between vibrational modes of the intervening medium and the transferring electron (inelastic ET) may significantly facilitate the ET reaction, even making it an activationless process (Daizadeh et al,Medvedev and Stuchebrukhov, 1997). The resulting analytical, modified Marcus expression for the ET rate constant, using a diabatic model of electron tunneling in fluctuating medium, shows that the activation energy may be significantly reduced due to inelastic interaction with phonons. This description is similar to the idea of adiabatic self-organized ET in an active medium (Tributsch and Pohlmann, 1998,Gushcha et al).
Adiabatic theories of particle transfer over a potential barrier lead to a Kramers-type dependence of the reaction rate constant, one that depends exponentially on the barrier height Eb (Kramers, 1940). Kramers’ theory came from an assumption of a linear interaction between the particle and its environment. Recent studies by Tributsch show that a nonlinearity with energy of frictional force dependence may result in a greatly increased probability of escape from a potential well (Tributsch and Pohlmann, 1998). In this description, the rate constant ωij depends exponentially on (α/2)(Eb−ELC)2, with α being a coupling coefficient with the medium and ELC denoting the mean energy of exchange between the particle and medium during oscillation. This idea has been substantiated analytically for the problem of particle escape over a potential barrier in the case of strong interactions between the particle and structural modes of the surroundings (Čapek and Tributsch, 1999). The authors gave a description of uphill particle transfer for the simplest case. In this case, the coupling of the transferred particle to its surroundings was assumed to be mediated by only one specific mode, localized in the vicinity of the transferred particle. Exact calculations for more realistic cases of many interacting modes were not performed, but expected results for such calculations should be qualitatively the same, providing support for the phenomenological result obtained earlier (Tributsch and Pohlmann, 1998).
In this work we use a phenomenological description for modeling non-equilibrium structural effects that occur during sequential charge transfer through a protein. We take into account dependence of the rate constants ωij on biomolecule structure by coupling to different structural motion. In both the adiabatic and non-adiabatic descriptions, small changes in the values of parameters such as ΔGij°, λij, Eb, ELC, Rij, ΔVij, which might be caused by electron transfer between cofactors, significantly affect the kinetics of the ET. Therefore, we assume that ET rate constants should be expressed as exponential functions of a structural parameter X=X(x1, x2, x3, … , xi, …) that in turn depends on a complete set of structural variables {x1, … , xN}, ωij ∝ exp(−X). The structural factor X is defined by either the adiabatic Eb, ELC, ΔVij, … , or non-adiabatic ΔGij°, λij, Rij, ΔVij, … , parameters of the system. Thus, statement 4 above indicates that charge-conformational interaction, by which ET is coupled to structural dynamics, may significantly affect the main reaction rate. For the simplest two-state system (Eq. (1)) the only kinetic parameter that depends upon macromolecular structure is the recombination rate constant, krec. Thus we write,
![]() | (10) |
A complete set of structural variables {x1, … , xN} may be selected to span the coordinate space in many ways. Here we take the structural variables as a set of variables that are each distinguished by different relaxation times. The fastest variables (τ≤10−13 s) describe fast motion of single atoms and small groups, whereas the slowest variables, with relaxation times longer than a second, describe the global dynamics of macromolecular structural rearrangement.
Let us assume that there exist long-lived, light-induced structural rearrangements of the macromolecule. Because of their long relaxation times, these rearrangements can produce effects that accumulate from one single electron-transfer step to the next. Under stationary-state illumination conditions, accumulated structural changes produce a new, quasi-stable structure. The extent of structural changes depends only upon the illumination intensity. In particular, in the case of a large electron-conformational interaction, a “dark-adapted” conformational state may convert to a completely new conformational state under high-intensity illumination. Furthermore, this new “light-adapted” conformational state may coexist with the “dark-adapted” one over an intermediate range of illumination intensity. This result means that there is a photo-induced bistability of the macromolecular structure. Necessary conditions for realization of such an effect are a strong charge-conformational interaction and a long structural relaxation time relative to localized electron relaxation. The slow structural modes, represented in this theory as “slow, generalized coordinates” function as “control modes.” These modes lead to a self-regulation of the photoexcited electron flux through the macromolecule, as recently demonstrated for photosynthetic RCs (Gushcha et al, Goushcha et al,Goushcha et al). Below we develop a self-consistent, statistical theory of electronic-conformational transitions to describe such effects.
For the theoretical treatment of light-induced structural changes in a macromolecule undergoing photoinduced charge transfer and separation, we use a Langevin equation with two random forces to describe the mechanical motion of a flexible structure (Chandrasekhar, 1943):
![]() |
![]() |
are the sets of structural variables (degrees of freedom; i=1, 2, …) with rates of structural rearrangements; T(
) and V+ (x) are the kinetic and potential energies for structural modes of the photoactivated macromolecule, respectively; and R(
) is a dissipative function of structural motion.The last two terms on the right-hand side of Eq. (11) represent random forces. The first is a random force due to thermal motion. This force acts on the structural variable xi, while the quantity ϑi(t) describes δ-correlated random processes with amplitudes
to model thermal fluctuations of the structural variables. The last term in Eq. (11) is a random force corresponding to interaction of a photoactivated electron with the macromolecular structure. Thus, Fi(t,x) describes a discrete random process:
![]() | (12) |
![]() |
![]() |
![]() |
![]() |
![]() | (15) |
![]() | (16) |
To simplify, we separate the variables {xi} into three groups, depending upon the relative magnitudes of the relaxation time constants τx and τel of the distribution function P(t; n,x) over the structural and electron variables, respectively. Those variables xfast, for which τx ≪ τel, belong to the first group. For the second group (xequal) the time constants are of the same order: τx ∼ τel. The third group is characterized by slow structural motions (xslow) for which τx ≫ τel. The two types of variables, xslow and xequal, should be explicitly retained in a description of self-regulation effects for a system involving photoexcited electron transfer within a flexible structure. However, in the present treatment we retain only xslow, and ignore xequal. The fast variables, xfast, are not important for self-regulation effects, because these variables relax on much shorter time scales. We can integrate over these variables, using the substitution
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![]() |
(t; n,xslow) is the distribution function for electron and slow structural variables.Putting Eq. (17) into Eq. (14) and integrating over xfast, we obtain equations identical to Eq. (14) that are valid for time intervals t ≫ τfast. They may also be derived from Eq. (14) with a simple substitution,
![]() | (18) |
![]() | (19) |
The potential energy expression corresponding to slow structural variables can be easily obtained after substitution of Eq. (17) into Eq. (14) and integrating over xfast,
![]() | (20) |
(xslow)≡Gn (xslow), in which Gn(xslow) is a so-called quasi-free energy for an electronic state n, depends parametrically on the slow structural variables (Stratonovich, 1992,Stratonovich, 1994). This means that
(xslow) represents the standard free energy for the electron state n with respect to the fast structural variables xfast, but it corresponds to the potential energy of electron state n with respect to the slow variables xslow.We further proceed from Eq. (14), taking into account the substitutions (Eq. (18)) and the actual role of the slow variables, xslow, only. Thus we can use an adiabatic approach that enables us to make the following simplification in Eq. (14). [Here we restrict consideration to the simpler case of ordinary slaving (Haken, 1983) in which fluctuations of the fast variable influence the evolution of the slow one only on average, without causing any noticeable fluctuations of the latter. The softer types of slaving will be discussed in a separate paper.]
![]() | (21) |
![]() | (22) |
![]() | (23) |
, and![]() | (24) |
Equations (13), provide the basis for self-regulation of a photoactivated electron flux by slow structural variables of a macromolecule.
Assume that the system can be characterized by a single slow structural degree of freedom: the generalized configurational coordinate x. Then Eq. (23) may be rewritten as:
![]() | (25) |
![]() | (26) |
The quantity VadI(x) serves as the effective adiabatic potential for the slow structural mode. This potential determines the average value of x over the electron distribution function. This potential is of a statistical nature, depending upon a stationary-state distribution of localized electron populations at a fixed structure. This structure is determined and controlled by the illumination intensity, I. For times t>τxslow, stationary-state conditions are reached. The corresponding stationary-state distribution function can be written as
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![]() |
The minima and maxima of this function, xext, define the stationary states of the macromolecule at a fixed I. Thus, the effective adiabatic potential VadI(x) for the open non-equilibrium system described by Eq. (1) is the analog of a standard Gibbs free energy, G°, which determines the probability to find a closed system in a particular equilibrium state with given free energy. The stationary states defined by xext in this open system are the analog of the equilibrium states in a closed system, and the values of xext can be determined from
![]() | (28) |
![]() | (29) |
![]() | (30) |
Thus, we restrict present considerations to a one-dimensional model of slow structural rearrangements induced by a photoinduced charge separation in biomolecules. We treat x as a global configurational coordinate that describes slow photoinduced structural changes. In this case, the structural factor X(x) introduced above may also be identified as a configurational coordinate because as it is well known that the dimension of generalized variables does not affect the calculation of trajectories and free energies (Goldstein, 1980). Consequently, we modify Eq. (10) making the substitution x → X, assuming that the configurational coordinate x is monotonic in configurational space because system energy decreases during relaxation, and slow system diffusion is determined by the trajectory. Note that x does not describe arbitrary structural rearrangements, but only those responsible for slow structural relaxation to a new potential minimum in configurational space. Finally, we obtain:
![]() | (31) |
To determine the light intensity dependence of macromolecule stationary states from Eq. (28) we select, as an example, a harmonic potential with effective elastic constant χ, V+ (x)=χ(x2/2), and, hence an effective adiabatic potential, VadI(x). Such a potential represents Gaussian fluctuations of x around equilibrium (see, e.g., Zusman, 1980). The quantities fn(x) (n=D, A) are defined as additional stochastic forces that act on the configurational coordinate when an electron is localized on cofactors D and A, respectively. We assume that these forces are constant, but not equal to each other. That is, fD(x)=fD=χxD is a force acting on the structure when an electron is localized on donor D; and fA(x)=fA=χxA is a force acting on the structure when an electron is localized on acceptor A. In general, xA≠ xD. The quantity ξ=|xA−xD| characterizes the electron-conformational interaction of the system. It is proportional to the additional force acting on the configurational coordinate in a charge-separated donor-acceptor pair. We assume here that the force constant χ is the same for the charge-neutral and charge-separated states, although this need not necessarily be true (i.e., in general χD ≠ χA). Furthermore, we showed in our recent paper (Goushcha et al) that for photosynthetic bacterial reaction centers the probe potential V+ (x) is probably not harmonic with different curvatures in the charge-neutral (PQAQB) and in the charge-separated (P+QAQB−) states. Parson and co-workers arrived at a similar conclusion in their molecular dynamic studies of the ET reaction P*BH → P+B−H. They showed that the force constant for the P+B−H state is larger than that it is for the P*BH state (Parson et al). In the current work, we explore qualitatively the conditions for non-equilibrium structural transitions and the emergence of new conformational states. For this treatment, the fact that χD ≠ χA is not essential, and we assume that χD=χA≡χ to obtain analytical solutions.
Using expressions for light-dependent, stationary-state electron populations (Eq. (5)), the recombination rate constant dependence on x (Eq. (31)), and stochastic forces (Eqs. (12), and fA,D(x)), the equation defining the stationary states of the system (Eq. (28)) becomes
![]() | (32) |
For this specific example, xext(I) (Eq. (32)) at specific values of ξ was determined in our recent work (Goushcha et al). A small, monotonic, light-induced increase in xext(I) was obtained for the case of a weak interaction, ξ=(xA−xD)≤4. The concomitant increase in the lifetime of the charge separated state, τd, obtained using Eq. (32) is shown in Fig. 1. The smooth, light-induced increase of τd for curves 1 and 2 is due to deformation of the “dark” conformational state. This effect may be described as “self-regulation” of the photoactivated electron transfer rate due to a slow structural deformation, reflecting macromolecule structural changes from an electron-conformational interaction modulated by the photoinduced electron flow.
More complex behavior of xext(I) occurs in the case of a strong charge-conformational interaction ξ>4. For illumination intensities, IIIcr>I>IIcr, in which
![]() | (33) |
![]() |
![]() | (34) |
![]() | (35) |
The appearance of a new, light-induced stable structural state for ξ>4 and the coexistence of this state with the initial stable state represents a non-equilibrium phase transition of the “monostability-bistability” type (Haken, 1983, Stratonovich, 1994).
The problem of thermodynamic stability of stationary states at coordinates xext(1) (I) and xext(3) (I) and the related problem of thermal fluctuations in the configurational coordinate around stationary-state values can be solved using a distribution function over x of the form P(t, x)=PD(t, x)+PA(t, x) (see Eq. (22)). An evolution equation for this function is described by Eq. (23), where using Eq. (26), the statistical potential VadI(x) (Goushcha et al) is given by
![]() |
![]() |
Previously, we analyzed this expression for many values of the electron-conformational interaction parameter, ξ (Goushcha et al 1999). A second, light-induced potential minimum may appear for ξ>4, a case corresponding to a distribution function PeqI(∞, x) with two maxima (Figure 2A). For ξ<4, the light-induced deformation of the adiabatic potential causes a deformation of the distribution function with only a shift in the distribution maximum toward larger values of the conformational coordinate (Figure 2B). The evolution of the distribution function with light intensity for the case of a weak interaction has been described in the literature. See, e.g., studies of the P+QA−→ PQA reaction in photosynthetic bacterial RCs (Shaitan et al,Uporov and Shaitan, 1990).
The abscissas of the potential VadI(x) extrema determine stationary values xext of the slow configurational coordinate as a function of ξ (see Eq. (35)). The values xext(1)(I) and xext(3)(I) correspond to adiabatic potential minima, whereas xext(2)(I) corresponds to a maximum. The minima determine the conformational states of the macromolecule at steady-state illumination intensity I. The thermodynamic stability of these conformational states is determined by both the depth of the potential minima and the height of the barrier between them.
Often the ensemble properties of macromolecules may be satisfactorily described by the most probable behavior of these macromolecules near potential minima. For this description, we use a conformational approach and introduce the function
![]() | (37) |
States with an x such that x ∈ Ga are treated as the same conformational state, α. The probability of realizing different conformational states is determined by the forward and reverse transition rates over potential barrier (Kramers, 1940,van Kampen, 1992). These probabilities are obtained from Eq. (25) using Eq. (37). Using this conformational approach, the average value of an observable q(t) can be written as
![]() | (38) |
(t, xα) is the average value over electron variables at t in conformational state α.For a system undergoing photoinduced charge separation and described by a double-minimum adiabatic potential, we introduce two distinct conformational states, “light” and “dark,” denoted as l and d, respectively. Providing that the barrier height between the two minima is sufficiently high, then equilibration near the minima may occur without thermally activated transitions between the minima. In this case, the non-equilibrium distribution function for x, corresponding to the evolution Eq. (25), may be written as
![]() | (39) |
The theoretical expression for an experimentally measured quantity, q(t), at steady-state illumination intensity I is
![]() | (40) |
![]() | (41) |
In the final section of this paper, we apply Eqs. (40) to a brief analysis of illumination-dependent absorbance changes in photosynthetic RCs. We also present other recent experimental observations that provide support for the idea of self-regulation phenomena in photosynthetic RCs.
Photosynthetic reaction centers have been among the most comprehensively studied biological systems over the last 30 years (Hoff and Deisenhofer, 1997, and references therein). Many researchers have discussed light-induced conformational transitions in RCs (see, e.g., Graige et al,McMahon et al,Kalman and Maroti, 1997,Kleinfeld et al,Shaitan et al). The charge recombination rate constant in RCs depends on structural coordinates such as the donor-acceptor distance (Kleinfeld et al,Shaitan et al). These authors experimentally determined, in effect, the distribution function for the generalized conformational coordinate both in the dark and under illumination by quenching structural relaxation at cryogenic temperatures. They obtained a light-induced increase in the donor-acceptor distance of ∼1Å. Recent EPR studies of RCs show that light-induced conformational changes are not simple relative translations of the donor and primary quinone acceptor (QA) molecules, but that they are more likely rearrangements of the protein structure (Zech et al). More recent x-ray studies of RCs from Rb. sphaeroides showed a large, ∼5Å, light-induced translation of the secondary quinone acceptor from its location in the dark-adapted system accompanied by a 180° rotation about the isoprene axis (Stowell et al). These authors also reported light-induced changes in the protein structure that affect the protonation of amino acid residues. Recent molecular dynamic calculations demonstrated the existence of two distinctly different binding sites for the neutral secondary quinone QB and semiquinone anion QB− (Grafton and Wheeler, 1999). The authors showed for the first time that the protonation of ASP L213 should occur prior to occupation by QB− of its stable (quasi-equilibrium) site, ∼5Å distant from the site which is at equilibrium for neutral quinone in the dark. Such motion of an ubi-semiquinone QB− from the non-equilibrium position that is characteristic for the dark-adapted structure to a quasi-equilibrium position that is stable for the light-adapted structure indicates the importance of non-equilibrium structural transitions in RCs. These observations explain previously reported light-induced changes in the transient absorption spectrum of Rb. sphaeroides RCs (Kleinfeld et al), but the physical phenomena responsible for these new conformations remained unexplained. Using the theoretical approach described above, we now elucidate reasonable mechanisms that lead to these structural changes in RCs.
Upon photoexcitation of RCs from purple bacteria Rhodobacter (Rb.) sphaeroides, a large absorbance decrease is observed in the 865-nm absorption band for the primary donor bacteriochlorophyll dimer (See Clayton, 1965). The absorbance A865(t) depends on the illumination intensity through σ(t),
![]() | (42) |
From Eq. (42) one can easily determine the relationship between the theoretical quantity, σI(t) (see first section) and experimentally measured values of δ(t)=−{[A865(t)−A865(0)]/[A865(0)]}. For stationary-state conditions,
![]() | (43) |
![]() | (44) |
The conclusions drawn above are valid for a system in which both 1) a single photoactivated electron transfers between a finite number of electronic states, and 2) charge trapping by exogenous acceptors is negligible. The first condition is verified for the RCs by the absence of cytochrome c or any other exogenous electron donors that might rapidly reduce the bacteriochlorophyll dimer P+ after initial photoactivation in double-flash experiments. Thus there are no states with doubly reduced quinone acceptors in these experiments. The second condition was verified in recent studies, which showed that large changes in the ET and charge recombination kinetics of RCs upon prolonged illumination are not related to the loss of photochemical activity of the RCs, but rather are due to the formation of new “light-induced” conformations of the RCs (Kalman and Maroti, 1997).
The experimentally measured quantity δ(t) can be calculated with the formalism developed above for the distribution function. Consider a homogeneous sample of isolated RCs at concentration C and optical pathlength l that absorbs with an “ideal” theoretical absorbance A′865=ɛ′865l CδDA, in which δDA=1 for A=D and=0, otherwise. Taking an ensemble average over the distribution of RC electronic and conformational states yields the following result:
![]() | (45) |
![]() | (46) |
Equation (46) may be used to model both transient absorption kinetics and quasi-stationary state effects for RCs. The calculated, light-induced, stationary-state absorption changes of RCs from Eq. (46) reveal nonlinear behavior of δ(∞) and were described theoretically elsewhere (Gushcha et al,Goushcha et al). The parameters xD and xA, discussed above, have a straightforward physical interpretation for RCs: they are generalized configurational coordinates for permanent localization of the photoelectron either on the donor D, as in thoroughly dark-adapted RCs, or on a quinone acceptor, QB or QA, for thoroughly light-adapted RCs, respectively.
Another remarkable property of RC dynamics is the dependence of primary donor recombination kinetics upon illumination conditions (Kleinfeld et al,Shaitan et al,Kalman and Maroti, 1997). For Rb. sphaeroides RCs that lack a secondary quinone acceptor QB, the charge recombination rate constant krec (see Eq. (1)) equals the recombination rate constant kAP=10s−1 for the radical pair D+QA− (Parson and Ke, 1982,Kleinfeld et al). For QB-containing Rb. sphaeroides RCs, electron transfer may be described by a two-level electronic scheme under physiological conditions (Kleinfeld et al,Labahn et al). This situation is also exactly like the one of Eq. (1) with an effective recombination rate constant,
![]() | (47) |
and P+QAQB−. Note that ΔGAB for the non-equilibrium case described in this work is the difference in the quasi-free energies GP+QAQB(x) and GP+QA−QB(x). This difference equals the conventional standard free energy difference ΔGAB° when RCs reach their equilibrium stable state in the dark (when x≡xD).The parameters kAP and ΔGAB/kBT may both be important in modeling the correlation of photoelectron transfer with RC structure. As discussed in the first section, both parameters determine the survival time of the charge-separated state
![]() | (48) |
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Figure 4A shows the primary donor absorbance recovery kinetics, measured at λ=865nm, for RCs from Rb. sphaeroides (wild type, wt) with inhibited QA−→ QB electron transfer. In this case, the recombination kinetics are determined by kAP. Trace 1 of Figure 4A was obtained after flash-activation of a dark-adapted sample, while trace 2 was measured after switching off 2min of background illumination that pre-illuminated the RCs (λ=700–900nm and Iexp=2 mW/cm2). The values kAP observed were 13s−1 and 9s−1 for the dark-adapted sample and the pre-illuminated sample, respectively. Such small but detectable differences in kAP may well be due to light-induced structural changes in the RCs (Kleinfeld et al,Shaitan et al).
Figure 4B shows the primary donor recovery kinetics for RCs from Rb. sphaeroides (wt) that are active in QA−→ QB electron transfer. We used isolated RCs with ∼75% occupation of the QB site with native ubiquinone, without any reconstitution of QB activity. The sample was thoroughly degassed before experiments by multiple freeze-thaw-pump cycles down to 77K and 10−6 torr. This procedure allowed us to avoid photo-oxidation of semiquinones by oxygen or other oxidants during illumination. Trace 1 in Figure 4B corresponds to flash-activated kinetics of a thoroughly dark-adapted sample. Trace 2 was measured after switching off 2min of pre-illumination of the sample with saturating actinic light Iexp=2 mW/cm2 at λ=700–900nm. Curve 1 in Figure 4B may be modeled with a recombination half-lifetime of ∼1s, whereas curve 2 reveals a decay half-lifetime of ∼200s. Such a drastic increase in the average survival time of the charge-separated state for a pre-illuminated sample cannot be explained by a light-induced decrease in the rate constant kAP, which changes only slightly for similar pre-illumination conditions (see Figure 4A). Consequently, this increase in the recombination time constant for a QB-containing sample may reflect a light-induced increase in the value |ΔGAB|/kBT.
In these experiments we assume a closed system with a fixed number of localized electron states and an absence of exogenous donors or acceptors. These assumptions are supported by the following observations. Several minutes after cessation of prolonged illumination, the RCs had undergone complete electron relaxation. Then we applied a saturating illumination flash. In cases of both QB-lacking and QB-containing RCs, the bleaching amplitude caused by this flash was the same as for a dark-adapted sample. Thus, the native activity of the pre-illuminated RCs was restored following charge recombination. However, the recovery kinetics of the primary donor, in response to this illumination flash, were quite different from those of a dark-adapted sample. These kinetics (not shown in Figure 4A) were nearly the same as those obtained for a 2-min, pre-illuminated sample in the case of QB-lacking RCs. For QB-containing RCs, the kinetics were intermediate between those of the thoroughly dark-adapted and of the pre-illuminated sample (trace 3 in Figure 4B). This means that a significant fraction (15–20% for QB-containing RCs) of the RCs remain trapped in a second, light-induced conformation, one with a relaxation time ≥10min for QB-containing RCs. A similar observation was reported by Kalman and Maroti, 1997 who applied much higher intensities of actinic illumination to QB-lacking RCs to saturate the electronic state QA−. This difference in experimental conditions may explain why our results for QB-lacking RCs differ from those of Kalman and Maroti, as well as why our results for QB-containing RCs are similar to theirs, even though they worked with QB-lacking RCs.
As noted above, the effects reported here cannot be explained by formation of states like P+QAQB with the electron having been captured by exogenous acceptors. Nevertheless, we do not completely exclude formation of such states and their influence on the dynamics of the system. This very interesting problem requires special attention, but was not studied in the present work. Additionally, sample preparation protocols involving treatment with detergents play a role in the effects observed. These results are not reported here either, but we plan to report them in subsequent work.
From the comparison of Eq. (47) with Eq. (31) we may assume that for the case of bacterial photosynthetic reaction centers the parameter |ΔGAB|/kBT may be identified with the slow generalized configurational coordinate x. This coordinate reflects slow, light-induced structural rearrangements in QB-containing RCs during system relaxation to its quasi-equilibrium, charge-separated state P+ QAQB−. During relaxation, the system moves along a single trajectory in configurational space with a concomitant decrease in free energy, which remains a single-valued function of x. As already noted, this free energy should be considered as a quasi-free energy with respect to slow relaxation of medium polarization (Stratonovich, 1992,Stratonovich, 1994). The quantity ΔGAB is a single-valued function of the configurational coordinate during system relaxation along a chosen trajectory in configurational space. It should be considered as a quasi-free energy difference for the system, which does not yet reach thermodynamic equilibrium and is still subject to illumination. Hence we define
![]() | (49) |
![]() | (50) |
Therefore, the free energy difference |ΔGAB| increases by ≥130 meV as a result of structural changes caused by multiple successive turnovers of the RC. Note that one may expect even larger light-induced changes in the standard free energy difference, ΔΔGAB°, because the illumination conditions used in our experiments are not necessarily sufficiently intense or prolonged to satisfy RC equilibration near the potential minimum xA. Thus, the generalized configurational coordinate, analogous to the perpendicular coordinate in the Agmon-Hopfield model, Eq. (49), is suitable for analysis of the correlation of structural dynamics and electron states in QB-containing RCs. Several recent papers have shown that slow structural dynamics play an important role in ultrafast charge separation steps in RCs, providing evidence for their adiabatic character and an illumination-controlled drop of the acceptor free energy (Holzwarth and Mueller, 1996,Lin et al). An analysis shows that the structural changes in response to ET in QB-lacking RCs cause a decrease in the free energy gap between donor (DQA) and acceptor (D+QA−) states of 120 meV (McMahon et al), comparable to the above result. Such a decrease in the free energy may be common in many biological charge transfer systems.
In the current paper we have developed a formalism for describing the evolution of open, non-equilibrium biomolecular systems with photoinduced charge separation. Upon steady-state illumination, such a system may have several stationary states, the number and relative thermodynamic stability of which depends on the illumination intensity. The thermodynamic stability of such an open system is determined by Eq. (27), in which the system effective adiabatic potential VadI is used instead of the standard free energy G° to describe equilibrium. Note that the fundamental Gibbs relationship P(G°)=Z−1exp(