2021 Volume 18 Pages 196-214
In the present study, we provide a reformulation of the theory originally proposed by Förster which allows for simple and convenient formulas useful to estimate the relative contributions of transition dipole moments of a donor and acceptor (chemical factors), their orientation factors (intermolecular structural factors), intermolecular center-to-center distances (intermolecular structural factors), spectral overlaps of absorption and emission spectra (photophysical factors), and refractive index (material factor) to the excitation energy transfer (EET) rate constant. To benchmark their validity, we focused on the EET occurring in C-phycocyanin (C-PC) chromophores. To this aim, we resorted to quantum chemistry calculations to get optimized molecular structures of the C-PC chromophores within the density functional theory (DFT) framework. The absorption and emission spectra, as well as transition dipole moments, were computed by using the time-dependent DFT (TDDFT). Our method was applied to several types of C-PCs showing that the EET rates are determined by an interplay of their specific physical, chemical, and geometrical features. These results show that our formulas can become a useful tool for a reliable estimation of the relative contributions of the factors regulating the EET transfer rate.
We propose a logarithmic reformulation of the original Förster theory leading to a simple set of formulae useful to accurately estimate the relative contributions of transition dipole moments of donor and acceptor (chemical factors), their orientation factors (structural factors), intermolecular center-to-center distances (structural factors), spectral overlaps of absorption and emission spectra (photophysical factors), and refractive index (material factor). These allow for the calculation of excitation energy transfer (EET) rate constant and a molecular-level interpretation providing a microscopic insight into the mechanism details. By focusing on the EET in C-phycocyanin chromophores, we show that our formulae are well suited to estimate the relative contributions to the EET rate constant.
Photosynthesis is the key mechanism responsible for the conversion of sunlight into energy and this energy is exploited by both terrestrial plants and algae. Phycobiliproteins (PBPs) are pigment proteins which play a pivotal role in photosynthesis as the light-harvesting components in cyanobacteria and red algae [1]. PBPs are water-soluble and, at variance with carotenoids, cannot exist within the membrane. As a consequence, they assemble into clusters which adhere to the membrane and are generally referred to as phycobilisomes. PBPs are heterodimers composed of α and β subunits, each of which possesses one to three open-chain covalently attached tetrapyrrole or phycobilins via thioether bonds to the apoprotein [2–4]. Another important role of PBPs is to convey the light energy to chlorophylls and finally to the photochemical reaction center for photosynthesis [5,6].
Phycobilins act as chromophores, the light-capturing moiety in photosynthesis. Major phycobilins include R-phycoerythrin (R-PE), B-phycoerythrin (B-PE), C-phycocyanin (C-PC), and allophycocyanin (APC) [7–9]. Their photophysical features, and in particular the absorption and fluorescence spectra, have been extensively investigated [10–22]. The common photophysical features of phycobilins can be summarized into one high absorption in the Q-band at around 700 nm and a large number of small absorption peaks in the Soret band at around 400 nm. They are typically classified in terms of their spectral features; R-PE and B-PE with λmax=540–570 nm, C-PC with λmax=610–620 nm, and APC with λmax=650–655 nm, where λmax is the wavelength of the band maximum in the Q-band [23,24]. These differences are known to be induced by different π-conjugation lengths in the tetrapyrrole rings [25]. In addition, because of their similarities in structure and function, it is assumed that they have a common ancestral gene [26].
Although the crystal structures of the PBPs have been intensively investigated over the years using X-rays, it is still difficult nowadays to unravel, for instance, how many phycobilins a given PBP contains. The C-PC system, targeted in the present study, is a peculiar phycocyanin which contains only phycocyanobilin chromophores. C-PC is composed of two homologous subunits; the α-chain with one phycocyanobilin attached at cysteine 84 and the β-chain with two phycocyanobilins attached at cysteines 84 and 155 [27–30]. These two homologous subunits form αβ monomers, aggregate into (αβ)3 trimers, and furthermore into disc-shaped (αβ)6 hexamers, the functional unit of C-PC.
Historically, Schirmer and coworkers determined the crystal structure of the biliprotein C-PC from the thermophilic cyanobacterium Mastigocladus laminosus by X-ray diffraction with a resolution of 3 Å for the first time [31]. In that work, it was found that the protein consists of three identical (αβ)-units which are arranged around a threefold symmetry axis to form a disc of the approximate dimensions of 110 Å×30 Å with a central channel of 35 Å diameter. This aggregation form was supposed to be identical to the one found in the rods of native phycobilisomes. To date, these findings are the most important structural features reported for C-PC.
Subsequent accurate X-ray structural studies of C-PC from a variety of organisms were reported. In general, almost all these studies have shown that the overall sequences of the C-PC complexes are very similar, albeit slight differences in their biophysical and biochemical properties [28–30,32–45].
Nield and coworkers reported a 1.45 Å resolution for the three-dimensional structure of C-PC from Synechococcus elongatus [33], which was the best possible resolution at the date of the publication of that work. They found that C-PCs are covalently bound to the protein via cysteines α-84, β-84, and β-155. The positions of α-84 and β-84 are similar to those of the heme-binding sites of myoglobin, with the thioether bonds in the R stereo-isomer conformation. The β-155 binding site is located in a short insertion loop not found in the α subunit. Its thioether bond has a typical S stereo-isomer conformation. All three pyrrole tetrapyrrole rings show a Z configuration on the D ring. The structures are analogous to those of the Cyanidium caldarium [28]. The difference stems from the different packing arrangement at the interface between the trimers, arising from the lack of conservation of the amino acid sequences [29].
Concerning the functional properties of PBP, crucial factors determining the efficiency of photosynthesis are the efficient collection of sunlight suitable for exciting the reaction centers of the system and, consequently, to transfer these excitation energies toward the photosynthetic pigment antennas. This process is termed electron energy transfer (EET) [46]. The EET process consists of the absorption of light by one pigment and the transfer of the resulting excitation energy to one or more other pigments. Phycobilisomes are efficient energy transducers, transferring the absorbed light to the photosystem II with an efficiency greater than 95% [47,48].
Several investigations of the EET in C-PC [30,49–64], done with picosecond fluorescence measurements, have shown that EET occurs from high (sensitizing) to low (fluorescing) energy phycobilins on isolated phycocyanin aggregates, which are fast components (10–80 ps), accompanied by a much longer decay of ~1–2 ns, corresponding to the normal radiative emission from the fluorescing chromophores.
From a theoretical standpoint, the EET among weakly coupled pigments was originally formulated by Thomas Förster [65,66]. The Förster theory has often been applied to the interpretations of the experimental results, proving its versatility and reliability [67]. Since the original formulation of the Förster theory, several developments have been proposed and the EET rate constants have been calculated using these new sophisticated formulations [68–76].
Although it is currently possible to quantitatively estimate the EET rate constant, it is not necessarily clear which physical and chemical factors contribute to it and to which extent. Thus, despite being quantitatively accurate, it remains difficult to extract a precise microscopic picture suitable, for instance, to unravel at a molecular level, the experimental investigation aimed at controlling the energy transfer dynamics of a Förster resonance energy transfer (FRET) for a coupled pair of chromophores embedded in a tunable sub-wavelength Fabry-Pérot resonator [77] or for enhancing the FRET rate in several FRET-based applications [78]. Regarding the specific context of photosynthesis, a variety of EET theoretical formulations have been applied to study this process in pigments, and this is the case of C-PCs [79–83]. The attention received by this specific system worldwide stems from the fact that C-PC pigments are the major phycobiliprotein in a wealth of cyanobacteria [84] and a secondary phycobiliprotein in some red algae [85], as mentioned. Moreover, they can also be used as natural dyes in the food industry and pharmaceuticals products [86]. From direct single-molecule measurements of C-PC in EET, by monitoring the fluorescence emission from single photosynthetic antenna proteins in a free solution over a long time and within the FRET theoretical framework, it has been found that there are transitions among many different photophysical states exhibiting distinct EET pathways among the embedded pigments [87]. These numerical findings would not be accessible by bulk studies underscoring the importance of a molecular approach.
Given the present scenario of the state of the art for EET in C-PC as summarized, it would be useful to have a suitable theoretical tool to obtain both quantitative information on the EET, namely the rate constant, and a molecular-level picture of the mechanism to interpret experiments and to provide a guideline for more practical applications.
To this aim, we reformulated the original Förster theory into a set of simple formulas of directly understandable physical/chemical meaning suitable to estimate the relative contributions of the transition dipole moments of the donor and acceptor (chemical factors), their orientation factors (intermolecular structural factors), intermolecular center-to-center distances (intermolecular structural factors), spectral overlaps of the absorption and emission spectra (photophysical factors), and refractive index (material factor) thus allowing for the calculation of the EET rate constant. As a benchmark of this reformulation, we applied our formulas to the EET occurring in C-PC chromophores. The pristine structures of the C-PC chromophores, whose initial molecular structures were taken from [33], were fully optimized at the density functional theory (DFT) level, and using these resulting geometries, we computed the absorption and emission spectra along with the transition dipole moments within the time-dependent DFT (TDDFT). These results were used to apply our Förster theory reformulation to extract the EET rates and estimate quantitatively the relative contributions of the physical quantities involved in the EET process. It turns out from our results that the EET rates are determined by a balance of the specific physical, chemical, and geometrical features of the C-PCs. These numerical examples show that our approach can potentially become a powerful tool to discriminate the relative importance of the various processes influencing the targeted system. Furthermore, this approach can provide a deeper insight into the phenomena taking place in the system. This shows that our formulas are indeed useful and provide a reasonable estimation of the relative contributions to the EET transfer rate.
All the quantum chemistry calculations performed in this study have been done with the GAUSSIAN16 program package [88]. Geometry optimizations of the ground state were performed at the standard DFT framework, whereas the first excited states were obtained within the TDDFT approach [89,90]. For the exchange and correlation interactions, we used the hybrid functional B3LYP [91] and the electronic wavefunctions were represented on a 6-31G(d) basis set for both the ground and excited states during all the structural relaxations. Instead, for a refinement of the related electronic properties, namely the absorption, emission and transition dipole moments, a larger 6-311+G(d,p) basis set was used with no symmetry constraints. The protein environment around the chromphores was described by a polarizable continuum model (PCM) by setting the dielectric constant ε equal to 4.0 [92]. This approximation has been routinely adopted before and carefully benchmarked [93–96], and. we provide support to the appropriateness of this approximation in the Supporting Information. All the optimized structures represent stable local minima of the potential energy surface (PES) as confirmed by a normal modes analysis. The initial molecular structure of C-PC was obtained from the Protein Data Bank [PDB ID: 1JBO] [33]. The missing hydrogen atoms were added using GaussView 6.1 [97].
b. Calculations of EET rate constants based on the Förster theoryThe original formulation of the Förster theory is based on the assumption of a weak coupling, and within this ansatz the EET rate constant, KFörster, from donor to acceptor is given by [98]:
(1) |
where J is the spectral overlap which can be calculated as
(2) |
and the subscripts D and A denote the donor and the acceptor, respectively. The quantities NA and ND are the normalization factors expressed as
(3) |
(4) |
In the above equations, ν is the frequency of light in wavenumber units (cm–1) and fA(ν) and fD(ν) are the line shapes of the adsorption spectrum of the acceptor and the emission spectrum of the donor, respectively. The integration limits, a and b, are appropriately chosen such that fA(ν) and fD(ν) become almost zero in the low and high frequency limits.
The spectral overlaps, J, were obtained by integrating fA(ν), fD(ν), and fA(ν)fD(ν) according to Eqs. (2), (3), and (4) in the range from a=500 nm to b=1200 nm (or 8.3×103 cm–1 to 2.0×104 cm–1). The spectral shapes, f(ν), including both of fA(ν) and fD(ν), were assumed to be a superposition of the Gaussian line-shapes defined by
(5) |
where f(ν) is the oscillator strength of the absorption (emission) spectrum, fmax is its maximum, νmax is the frequency at the maximum oscillator strength, and FWHM is the full width at half maximum. FWHM was set to 4000.0 cm–1 in all the computational absorption and emission spectra presented in this study [82,98].
In the dipole-dipole approximation, VF can be written as
(6) |
In this equation, |μD| and |μA| are the magnitudes of the transition dipole moments of D and A, respectively, which are separated by the intermolecular center-to-center distance R. In the denominator of Eq. (6), n is the refractive index of the surrounding medium [99]. The value
(7) |
was used [100], where n is the refractive index of the protein medium. The transition dipole moments were calculated using the Multiwfn program [101].
The orientation factor, κ, is expressed as
(8) |
where α is the angle between the two transition dipole moments and β1 and β2 are the angles between the dipoles 1 and 2 and the line joining them, respectively. The value of |κ| ranges from 0 to 2. This situation is depicted in Figure 1.
Schematic picture showing the geometric configurations of the transition dipole moments of D (donor) and A (acceptor), μD and μA, respectively. R is the intermolecular center-to-center distance between D and A. α is the angle between the two transition dipole moments and β1 and β2 are the angles between dipoles 1 and 2, respectively, and the line joining them R.
Finally, the transfer time τ was calculated as
(9) |
where
The aim of our study is to reformulate the above quantities, κ, μD and μA, n2, R, J, VF, KFörster, and τ, expressed by the Eqs. (1), (6), and (9), into comparable quantities which would be difficult to compare because of their different units and physical meaning.
We start by defining the general idea of “contribution factor”. In this respect, a physical quantity, a, which depends on some other physical variables, b1, b2, b3, etc., can be written as a function of these arguments, namely
(10) |
In our specific case, we assume that a and bi’s are positive numbers. We assume that only one of the arguments, for instance bi, is rescaled by some positive dimensionless constant Bi,
(11) |
that is,
(12) |
and that as a result, the logarithm of a increases by a factor δlog10a common to all the bi’:
(13) |
We can then define
(14) |
as a contribution factor of a with respect to bi. This definition of the measure of the contribution factor,
(i) The logarithmic increase of a defined by Eq.(13) is proportional to and directly determined by the logarithmic increase of only one of the two variables defined by Eq.(12). Therefore, the contribution factor defined by Eq.(14) determines the amount of the contribution of the physical quantity, bi, to a. Hence,
(ii) The contribution factor defined by Eq.(14) does not depend on any variables other than bi.
(iii) The dimensionless logarithmic version of the quantities log10Bi’s, which pertain to the different physical dimensions, are the ones that can be directly compared instead of the original bi.
To simplify our formulation and to make the different quantities less heterogeneous, we adopt the following fundamental units:
(15) |
for κ, μD and μA, n2, R, J, VF, KFörster, and τ, respectively. They are defined by
(16) |
(17) |
(18) |
(19) |
(20) |
(21) |
(22) |
(23) |
and
(24) |
Using these definitions of the fundamental units, a simple substitution of Eqs.(16)–(23) into Eqs.(1) and (6) provides the following expression:
(25) |
Here, κ, μD and μA, n2, R, J, VF, and KFörster, are measured with respect to their own fundamental units, κ(0), μ(0), n(0)2, R(0), J(0), V(0), and K(0), according to the definitions (16)–(22). Computing the logarithm of both sides of Eq.(25) leads to
(26) |
Here, we have assumed that μD, μA, n2, R, J, VF, and KFörster (or
By multiplying |κ|, |μD|, |μA|, J, R, and n2 by some arbitrary constants, Cκ, CμD, CμA, CJ, CR, and Cn2, and KFörster we can rewrite these terms as
(27) |
(28) |
(29) |
(30) |
(31) |
and
(32) |
where
(33) |
(34) |
(35) |
(36) |
(37) |
and
(38) |
Since we aim at calculating the contribution factors defined by Eq. (14), we have to compute
(39) |
and
(40) |
in which case, by substituting Eq.(39) into Eq.(26), one finds
(41) |
(42) |
(43) |
(44) |
(45) |
and
(46) |
for the initial values of κ, μD, μA, J, R, and n2, respectively. Therefore, substituting Eqs.(41)–(46) into Eq.(11), Cκ, CμD, CμA, CJ, CR, and
(47) |
(48) |
(49) |
(50) |
(51) |
and
(52) |
Substituting Eqs. (39) and (40) and Eqs.(47)–(52) into Eq.(27)–(32), respectively, leads to
(53) |
(54) |
(55) |
(56) |
(57) |
and
(58) |
where we have introduced the following shorthand notations,
(59) |
(60) |
(61) |
(62) |
(63) |
(64) |
and
(65) |
Substituting Eqs. (53)–(58) and Eq.(65) into Eq.(26), it turns out that
(66) |
On the other hand, substituting Eqs.(22) and (24) into Eq.(9) leads to
(67) |
Equations (53)–(58) and Eq.(66) suggest that For, Fdip,D, Fdip,A, Fover, Fdis, and Fref, which are the quantities dependent on the systems considered, are the magnitudes of the independent linear contributions of |κ|, |μD|, |μA|, J, R, and n2 to KFörster, respectively.
We stress the four following points:
(i) the dimensionless logarithms of For, Fdip,D, Fdip,A, Fover, Fdis, and Fref always sum to unity according to Eq. (66).
(ii) Here and below, the physical and chemical quantities which are the argument of the logarithm are always dimensionless as pointed out above.
(iii) Each logarithm of For, Fdip,D, Fdip,A, Fover, Fdis, and Fref is divided by the common factor, Cnorm. Therefore, we cannot only estimate the separate contributions of |κ|, |μD|, |μA|, J, R, and n2 to KFörster, which are dependent on the system considered, but we can also observe that these quantities are normalized in the sense that the simple summation of the logarithms has to be equal to 1 for any system (see Eqs. (53)–(58) and Eq.(66)), and (iv). From Eq.(66), it can be remarked that if one term of the left-hand side of Eq.(66) is greater than 1/6=0.17, this term positively contributes to the EET rate. On the other hand, if it is lower than 1/6=0.17, this same term contributes negatively to the EET rate. This is a consequence of the fact that the six terms on the left-hand side of Eq.(66) always sum to unity and they have all the same relative weight.
(iv) Since we can separate the contributions of the transition dipole moments of D and A (chemical factors), their orientation factors (intermolecular structural factors), the intermolecular center-to-center distances (intermolecular structural factors), the spectral overlaps of absorption and emission (photophysical factors), and refractive index (material factor) in the form of a linear sum of the respective terms, the fundamental theory, which approximates the electronic coupling interaction VF by the transition dipole approximation derived above, allows a straightforward estimation of each contribution to the EET rate. This is a practical advantage compared to the more sophisticated methods proposed in the literature [102,103]. Indeed, these methods do not explicitly calculate the single contributions of |κ|, |μD|, |μA|, R, and n2 but directly the electronic coupling VF. However, from this global coupling term, it is nearly impossible to unravel the single contributions and their relative importance in the EET process.
To calculate the contributions relative to a particular transfer pathway from D to A, e.g., from 1 to 2, the following formulas can be used:
(68) |
(69) |
(70) |
(71) |
(72) |
and
(73) |
Within our proposed framework, from Eqs. (53)–(58) and Eq.(66), we always have
(74) |
The PBP is mainly made up of hexameric and trimeric disks of phycobiliproteins. In Figure 2, the former case, the C-PCs in the (αβ)6 hexameric form, are depicted. In this study, we only focus on the EET pathways among α1-84, β1-84, and β1-155. The intermolecular center-to-center distances between α1-84 and β1-84, β1-84 and β1-155, and α1-84 and β1-155 connected by the purple lines are 50, 34, and 47 Å, respectively.
(αβ)6 hexameric form of C-PCs. The α and β units are shown in green and light blue, respectively. The red C-PCs are those placed in the α unit whereas the gray ones are those placed in the β unit. The figure was based on the pdb data deposited in the Protein Data Bank [PDB ID: 1JBO] [33].
To benchmark our reformulation of the Förster theory, we used the C-PC structures sketched in Figure 3, which are surrounded by the protein environment shown in Figure 4, from which our models are derived. In Figure 3, the molecular geometry in panel (a) is identical to the model used by Ren and coworkers [82] (Fig. 2 in the quoted reference), except for the crucial nearby aspartate residues (Asp-87 for α1-84, Asp-87 for β1-84, and Asp-39 for β1-155) as shown in Figure 4, referred to as PCB as reported in Refs. [64,104]. In Figure 3, the panel labeled as (b) the PCBp model is also adopted here and has already been discussed in a former study [105]. Panel (c) of Figure 3 displays the PCBp model with the added nearby aspartate residue [105], as shown in Figure 4. Panel (d) of Figure 3 shows a molecular structure similar to the one reported in panel (b) of Figure 3; the only difference is that the two propionic acid side-chains of the former are deprotonated for the latter.
Computational models adopted for the structures of (a) PCB, (b) PCBp, (c) PCBp-asp, and (d) PCBp-(1-).
Crystal structure of C-PC monomer from the thermophylic cyanobacterium Synechococcus Elongatus and the locations of α1-84, β1-84, and β1-155, together with their neighboring aspartate residues, Asp-87, Asp-87, and Asp-39, respectively. The molecular groups, which we are interested in, α1-84 and Asp-87, β1-84 and Asp-87, and β1-155 and Asp-39, are colored red, gray, and yellow, respectively. The figure was based on the pdb data deposited in the Protein Data Bank [PDB ID: 1JBO] [33].
Note that the three kinds of subunits, one from the α-subunit and two from the β-subunit, are indicated as PCB1, PCB2, PCB3 for the PCB model, PCBp1, PCBp2, PCBp3 for the PCBp model, PCBp1-asp, PCBp2-asp, PCBp3-asp for the PCBp-asp model, PCBp1-(1-), PCBp2-(1-), PCBp3-(1-) for the PCBp-(1-) model, respectively, according to the labeling adopted in Figure 3 of Ref. [33]. Phycocyanobilins (PCBs), α-84, β-84, and β-155, described in Ref. [94] correspond to PCB1, PCBp1, PCBp1-asp, PCBp1-(1-), PCB2, PCBp2, PCBp2-asp, PCBp2-(1-), and PCB3, PCBp3, PCBp3-asp, PCBp3-(1-), respectively. The total charges of PCB (panel (a)) and PCBp (panel (b)) are +1 [105], those of PCBp-asp (panel (c)) are neutral [82], and those of PCBp-(1-) (panel (d)) are -1. The difference between PCB and PCBp consists of the fact that one β-butylene group is attached to the pyrrole ring A in the former case, while an ethyl group is attached to the pyrrole ring A in the latter case.
One of the most important features of our molecular models is that the main chain of C-PC is composed of four pyrrole rings denoted as A, B, C, and D as shown in Figure 3. The outermost two pyrrole rings, A and D, contain one oxygen atom. On the other hand, each of the other pyrrole rings, B and C, carries a propionic acid side-chain, -CH2-CH2-COOH, except for panel (d) of Figure 3, in which case each of the two propionic acids is deprotonated.
The optimized structures of the PCB model (PCB1, PCB2, PCB3), the PCBp model (PCBp1, PCBp2, PCBp3), and the PCBp-asp model (PCBp1-asp, PCBp2-asp, PCBp3-asp) in the ground and first excited states are shown in Supplementary Figures S1, S2, and S3, respectively. Note that each PCBp-(1-) model is assumed to take the molecular geometry optimized for the corresponding PCBp model in this study. A feature that can be noted is that the molecular backbones composed of pyrrole rings, A, B, C and D are nearly identical in all the cases and the configurations of the two propionic acids (Supplementary Figs. S1 and S2) and those of the aspartate residue (Supplementary Fig. S3) are different for species 1, 2, and 3.
The major differences of the four models shown in panels (a), (b), (c), and (d) of Figure 3 can be summarized in the following three points: (1) the PCB has a longer conjugation length than the PCBp, PCBp-asp, and PCBp-(1-) models, (2) the PCBp-asp model includes the most important weak interaction of PCB with the respective aspartate residues, as shown in Figure 4, (3) the two propionic acids of the PCBp-(1-) model are deprotonated. Therefore, comparisons among the four models can clarify the influence of the congugation length of the chromophore, the role of the weak intreaction with the aspartate residue, and the effects of the deprotonation of the propionic acids.
In particular, for the deprotonation of the propionic acids, Zienicke and coworkers experimentally investigated the photo-conversion of phytochrome Agp2 from Agrobacterium tumefaciens, which has a Pfr ground state and a Pr metastable state, by means of UV/visible absorption and resonance Raman spectroscopies [106]. They observed unusual spectral properties of Agp2 Pr induced by the chromophore protonation state and found that the Pfr chromophore is protonated in a range of values of the pH up to 11, while the Pr chromophore has a pKa value of 7.6 and is therefore only partially protonated in neutral pH conditions. On the basis of these results, we can assume that some propionic acids are deprotonated while some others are protonated in the usual protein environment. On these grounds, a comparison between panels (b) and (d) of Figure 3 deserves special attention in terms of the influence of the protonation state of the propionic acids on the EET rate.
c. Absorption and emission spectraThe absorption and emission spectra of the PCB, PCBp, PCBp-asp, and PCBp-(1-) models are shown in Figure 5. To account for the trend observed in the Q band [107,108], the values of the maximum wavelengths of the absorption and emission spectra in this same Q band have been carefully tuned for PCB1, PCB2, PCB3, PCBp1, PCBp2, PCBp3, PCBp1-asp, PCBp2-asp, PCBp3-asp, PCBp1-(1-), PCBp2-(1-), and PCBp3-(1-) and these values are summarized in Supplementary Table S1 together with the Stokes shifts and graphically shown in panel (f) of Supplementary Figure S4.
Calculated absorption and emission spectra of (a) PCB1, PCB2, PCB3, (b) PCBp1, PCBp2, PCBp3, (c) PCBp1- asp, PCBp2-asp, PCBp3-asp, and (d) PCBp1-(1-), PCBp2-(1-), PCBp3-(1-). The calculations were done within the TDDFT framework with a B3LYP functional and the basis set 6-311+G(d,p). FWHM was 4000.0 cm–1.
As a first observation, we noted that the emission spectra are characerized by peaks at wavelengths slightly longer than the corresponding absorption spectra in all the cases shown in Figure 5, Supplementary Table S1, and panel (f) of Supplementary Figure S4. The difference in the position of the two peaks is a typical Stokes shift. From Supplementary Table S1, the Stokes shifts range from 20 nm to 70 nm except for those of the PCBp-(1-)_shift models. Comparing the spectral peaks of the absorption and emission spectra and the Stokes shifts among the geometries shown in Figure 3, the PCBp-asp model reproduces the experimental results better than the other PCB, PCBp, and PCBp-(1-) ones. The wavelengths of the PCBp-(1-) models are slightly shorter than or comparable to the experimental ones and those of the PCBp model. Therefore, we can infer that the deprotonated and protonated propionic acids coexist under the typical experimental conditions and that the photophysical properties do not depend on the protonation state of the propionic acids.
Furthermore, we note that the wavelengths of the absorption and emission spectra undergo a shift toward the shorter values according to the order PCB, PCBp, PCBp-(1-), and PCBp-asp, as shown in panels (a), (b), (c), and (d) of Figure 5. The fact that the PCB system has a conjugation length longer than the other three PCBp, PCBp-asp, and PCBp-(1-) models seems to be the reason for the longer wavelengths of the absorption and emission spectra [104].
The justification in the use of the PCM instead of the real protein environment is reported in Supplementary Text S1.
d. Results of EET rate KFörster/K(0) and transfer time τ/τ(0)We report in Supplementary Tables S2, S3, S4, and S5 all the magnitudes of the orientation factor |κ|/|κ(0)|, the transition dipole moments of D and A, |μD|/|μ(0)| and |μA|/|μ(0)|, the intermolecular center-to-center distance R/R(0), the square modulus of the electronic coupling |VF|2/|VF(0)|2, the spectral overlap J/J(0), the EET rate constant KFörster/K(0), inverse of KFörster/K(0), and Cnorm defined by Eq. (65) for the models, PCB, PCBp, PCBp-asp, and PCBp-(1-) model systems, respectively. This is accompanied by a graphical presentation in panels (a), (b), (c), (d), and (e) of Supplementary Figure S4 of the physical quantities, |κ|/|κ(0)|, |μD|/|μ(0)| and |μA|/|μ(0)|, |μD||μA|/|μ(0)|2, |VF|2/|VF(0)|2, and J/J(0).
From panel (d) of Supplementary Figure S4, we observed that the highest value of |VF|2/|VF(0)|2 is the one corresponding to the PCBp-asp system, whereas it is nearly the same for the PCB and PCBp models and it is much less for the PCBp-(1-) model system. Moreover, |VF|2/|VF(0)|2 is much lower for the D-A pairs, 1-3 and 3-1, than for the D-A pairs, 1-2, 2-1, 2-3, and 3-2. On the other hand, from panels (b) and (c) of Supplementary Figure S4, we noted that |μD|/|μ(0)|, |μA|/|μ(0)|, and |μD||μA|/|μ(0)|2 are slightly lower for the PCBp -asp and PCBp-(1-) model systems than those for the PCB and PCBp systems, in which case they are significantly low for the PCBp-(1-) model system.
From Eq. (6), |VF|2 is determined by |κ|, |μD|, |μA|, and R. By considering that the numerical values of R/R(0) are 96.0, 68.0, and 91.0 for the D-A pairs, 1-2 and 2-1, 2-3 and 3-2, and 1-3 and 3-1, respectively (see Supplementary Tables S2, S3, S4, and S5), it becomes evident that the lowest values of |VF|2 for the D-A pairs, 1-3 and 3-1, are due to the higher value of R/R(0), and simultaneously, to the lower values of |κ|/|κ(0)| and |μD||μA|/|μ(0)|2 for the pairs, 1-3 and 3-1 (see panels (a) and (c) of Supplementary Fig. S4).
In addition, we noted that the values of |VF|2/|VF(0)|2 for the D-A pairs 1-2 and 2-1 are similar for the PCB, PCBp, and PCBp-asp models, whereas those for the PCBp-(1-) model are lower than the other cases. Furthermore, |VF|2/|VF(0)|2 for the D-A pairs 2-3 and 3-2 are the highest for the PCBp-asp system and lowest for the PCBp-(1-) system. Those of the PCB and PCBp models are comparable and lie between those of the PCBp-asp and PCBp-(1-) systems as shown in panel (d) of Supplementary Figure S4. These facts result from the lowest magnitudes of the transition dipole moments for the PCBp-(1-) system, as shown in panels (b) and (c) of Supplementary Figure S4.
From panel (e) of Supplementary Figure S4 and Supplementary Tables S2, S3, S4, and S5, we noted that the magnitudes of J/J(0) are roughly comparable for all the systems, PCB, PCBp, PCBp-asp, and PCBp-(1-). This simply reflects the fact that the linewidth of 4000.0 cm–1 adopted in Figure 5 is so broad that the values of the J/J(0)’s computed by Eq. (2) are nearly identical for all the considered molecular models and calculation levels. If we take this fact into account, KFörster/K(0) might display a trend similar to |VF|2/|VF(0)|2 because KFörster is proportional to the product of |VF|2 and J (see Eq. (1)).
This is indeed the case. The magnitudes of KFörster/K(0) shown in panel (a) of Figure 6 show a trend analogous to the case of |VF|2/|VF(0)|2 reported in panel (d) of Supplementary Figure S4.
Calculated EET rate constants (panel (a)) and transfer times (panel (b)) of PCB, PCBp, PCBp-asp, and PCBp-(1-) model systems adopted in this study. The calculations were carried out at the TDDFT level with a hybrid functional B3LYP for the exchange-correlation and a 6-311+G(d,p) basis set. Experimental results (Exp.) were taken from Ref. [80].
The transfer times for the four systems, PCB, PCBp, PCBp-asp, and PCBp-(1-), calculated according to Eq. (67) are reported in panel (b) of Figure 6. The equation indicates that lower values of KFörster/K(0) lead to higher values of the transfer times, τ/τ(0). Indeed, a simple comparison of panels (a) and (b) of Figure 6 shows that this is the overall picture. The EET rates of the PCBp-(1-) system are the lowest among the four models. The transfer times for PCBp-asp are shorter than those for PCB, PCBp, and PCBp-(1-), as shown in panel (b) of Figure 6. Furthermore, the transfer times for the D-A pair 1-3 are much longer than those for the other D-A pairs, 1-2 and 2-3. It should be stressed that the PCBp-asp model system is able to reproduce the experimental transfer time better than the PCB, PCBp, and PCBp-(1-) models, as shown in panel (b) of Figure 6. Given this scenario, this underlines the importance of the intermolecular interaction between PCB and the aspartate residue for a good reproduction of the experimental EET rates and transfer times, whereas the deprotonation of the propionic acids decreases the EET rates and leads to a much worse estimation of the transfer time for the D-A pair 1-3.
e. Determination of the contributions of orientation |κ|/|κ(0)|, transition dipole moments, |μD|/|μ(0)| and |μA|/|μ(0)|, spectral overlap J/J(0), intermolecular center-to-center distance R/R(0), and refractive index n2/n(0)2 to the EET rate constant KFörster/K(0) according to the Förster theory in the C-phycocyanin chromophoresThe various contributions indicated as For, Fdip,D, Fdip,A, Fover, Fdis, and Fref (see Eqs. (53)–(58)) are shown in panel (a) of Figure 7 for the EET pathways, 1→2, 2→1, 2→3, 3→2, 1→3, and 3→1, for the PCBp-asp system and those are shown in panels (a) of Supplementary Figures S5, S6, and S7 for the PCB, PCBp, and PCBp-(1-) models, respectively. On the other hand, panels (b) of Figures 7 and those of Supplementary Figures S5, S6, and S7 show
Panel (a): For, Fdip,D, Fdip,A, Fover, Fdis, and Fref as obtained from Eqs. (53)–(58) for the EET pathways, 1→2, 2→1, 2→3, 3→2, 1→3, and 3→1, for the PCBp-asp system. Panel (b):
In addition, we noticed that Fdip,D and Fdip,A remain nearly constant while changing the EET pathways. This implies that the variations in the order of the magnitude of |μD|/|μ(0)| and |μA|/|μ(0)| for the different EET pathways are almost negligible as shown in panels (b), and (c) of Supplementary Figure S4. The contributions of Fref are nearly identical in all the cases.
An important point to make in panel (a) of Figure 7 is that For is rather low, yet its sign changes from negative to positive as the EET pathway changes as 1→2, 2→1, 2→3, 3→2, 1→3, and 3→1. This tendency is reflected in the increasing trend of the relative magnitude of
The reason why For increases as the EET pathways evolves along 2→3 and 3→2 to 1→3 and 3→1 can be identified in the fact that |κ|/|κ(0)|, which is lower than 1 for the EET pathways 2→3, 3→2, 1→3, and 3→1, decreases as the EET pathways change from 2→3 and 3→2 to 1→3 and 3→1, as shown in panel (a) of Supplementary Figure S4.
In addition, the reason for the change of sign in the For from the negative to the positive values as the EET pathways proceeds from 1→2 and 2→1 to 2→3 and 3→2 is that |κ|/|κ(0)| is lower than 1 for the EET pathways 2→3 and 3→2, whereas it becomes greater than 1 for the EET pathways 1→2 and 2→1, and Cnorm is negative for the case described in Figure 7, in agreement with Eqs.(53) and (65). All these results indicate that For increases, assuming that the values of which are initially negative, then become positive along the EET pathways going from 1→2 and 2→1 to 2→3 and 3→2.
From panels (a) and (b) of Figure 7, we note that For increases as Fdis decreases, and
The four models shown in Figure 3 are some models of C-PCs currently used for calculations of various properties of C-PCs. As mentioned, the fact that the PCB model system has a conjugation length longer than the PCBp seems to be the reason for the longer wavelengths of the absorption and emission spectra with respect to the former [104]. This leads to quite different relative contributions of the spectral overlap J/J(0) to KFörster/K(0) among the D-A pathways, 2→1, 2→3, 3→2, 1→3, and 3→1, for the PCB and PCBp systems, as shown in panels (b) of Supplementary Figure S5 and Supplementary Figure S6, respectively. In other words, the difference in KFörster/K(0) for the D-A pathways in the PCB and PCBp systems mainly arises from the different relative contributions from the spectral overlap, J/J(0), which in turn originates from the different conjugation lengths. In addition, such a difference leads to a significantly different transfer time for the D-A combination of 1-3 shown by the blue bars in panel (b) of Figure 6 for the PCB and PCBp systems.
Based on these considerations, the comparison between the PCB (panel (a) of Fig. 3) and PCBp (panel (b) of Fig. 3) systems provides a clear example in which the difference in the spectral overlap J/J(0) originating from the different conjugation length plays a key role in discriminating the relative contributions to the EET rate, KFörster/K(0), for the different D-A pathways.
On the other hand, panels (b) and (c) of Figure 5 show that the PCBp and PCBp-asp systems have a very different photoresponse; specifically, the absorption and emission wavelengths. This is due to the presence/absence of the weak interaction between the chromophore and aspartate residue, which is similar to the comparison between the PCB and PCBp systems although the chemical origins are different. Unlike the comparison between these PCB and PCBp systems, the difference in the relative contributions of the orientation factors to KFörster/K(0) among the D-A pathways, 2→1, 2→3, 3→2, 1→3, and 3→1, is more important for the PCB system than that from the spectral overlap in the PCBp and PCBp-asp systems, as shown in panels (b) of Supplementary Figure S6 and Figure 7. At the same time, the relative contribution from the center-to-center distance for both the PCBp and PCBp-asp systems proportionately decreases. This compensation leads to the transfer times for the D-A combinations, 1-2, 2-3, and 1-3, which are similar and reproduce the experimental values better for the PCBp and PCBp-asp systems. Conversely, those are rather different between the PCB and PCBp (1-) systems and the PCBp and PCBp-asp systems.
Based on these considerations, the comparison among the systems PCB (panel (a) of Fig. 3), PCBp (panel (b) of Fig. 3), and PCBp-asp (panel (c) of Fig. 3) provides a typical example where the difference in the transfer times originates from the difference in the orientation factor. Moreover, the comparison between PCBp (panel (b) of Fig. 3) and PCBp-asp (panel (c) of Fig. 3) shows that there is a compensation among the factors (orientation factor and center-to-center distance factor in this case), which leads to the similar transfer times for the D-A combinations, 1-2, 2-3, and 1-3.
Finally, the comparison between PCBp (panel (b) of Fig. 3) and PCBp-(1-) (panel (d) of Fig. 3) shows that the deprotonation of the two adjacent propionic acids leads to a decrease of the EET rates, which in turn originates from the small transition dipole moments of the deprotonated PCB systems.
In summary, by using Eqs. (53)–(58) and Eqs.(65)–(74) derived in this study, the following key points have been concluded for the EET in the C-PC chromophores:
(i) The EET rate constant KFörster/K(0) is dominated by the intermolecular center-to-center distance R/R(0).
(ii) The quantities, |μD|/|μ(0)|, |μA|/|μ(0)|, and J/J(0). remain almost constant for any of the EET pathways. This implies that their coontributions to the EET rate constant remain unchanged for any of the EET pathways.
(iii) From (i), (ii), and according to Eq. (65), the change in R/R(0) as shown in panel (a) of Figure 7 is compensated by |κ|/|κ(0)|. Thus, For increases as Fdis decreases, and, analogously,
(iv) The relative contributions of the orientation factors |κ|/|κ(0)| are also non-negligible as reported in panel (b) of Figure 7. This implies that the balance between |κ|/|κ(0)| and R/R(0) determines the EET rate constant KFörster/K(0)in the case of the PCBp-asp system.
(v) The influence of the difference in the conjugation length was evidenced by comparing the PCB and PCBp systems. The longer conjugation length leads to a greater relative contribution from the spectral overlap than from the other factors, which finally results in a longer transfer time.
(vi) The influence of the difference in the orientation factor of the transition dipole moment was rationalized by comparing the PCB system and PCBp and PCBp-asp systems. In this case, such a difference leads to different transfer times.
(vii) The compensation of the factors was found by the comparison between the PCBp and PCBp-asp systems. The contribution of the orientation factor and that of the center-to-center distance compensate each other, which leads to similar transfer times for the D-A combinations, 1-2, 2-3, and 1-3.
(viii) By comparing the PCBp-asp and PCBp-(1-) systems, it turns out that the deprotonation of the two adjacent propionic acids leads to a decrease in the EET rates, and this originates from the lower transition dipole moments of the deprotonated PCBp-(1-) system.
In conclusion, we have shown that a logarithmic reformulation of the original Förster theory (Eq. (1)) allows splitting of all the single contributions, expressed by Eqs. (66) and (74), and this formulation, in turn, leads to a simple linear addition of the separated terms. Each term has an intuitive physical and chemical interpretation and allows to rationalize the various contributions affecting the EET rate constant, which is not necessarily evident if one only relies on the product form of Eq.(1).
Finally, an extension of our method to the case where both the Förster and Dexter theories play a role in the EET process is described in Supplementary Text S2.
In this study, we have shown that a simple logarithmic reformulation of the theoretical approach originally proposed by Förster leads to a set of simple and convenient formulas useful to separate the five different contributions, namely (i) transition dipole moments of the donor and acceptor (chemical factors), (ii) their orientation factors (structural factors), (iii) intermolecular center-to-center distances (structural factors), (iv) spectral overlaps of the absorption and emission spectra (photophysical factors), and (v) refractive index (material factor), all of them involved in the determination of the excitation energy transfer (EET) rate constant. To demonstrate the applicability of this reformulation, we focused on the EET pairs in the C-phycocyanin (C-PC) chromophores. Quantum chemical calculations based on DFT were done to obtain optimized molecular structures. The absorption and emission spectra, and transition dipole moments were evaluated by a TDDFT approach. The obtained results show that our formulas are indeed versatile and provide a deeper insight into the physical and chemical origins contributing to the EET rate.
Our method is prone to become useful for the design of high-efficiency solar cells, artificial photosynthesis systems, etc., because it can quantify the relative magnitudes of the contributions involved in the EET rates and their constructive or destructive effects. This, in turn, allows to unravel which parameters require special attention and optimization.
As an added value, we remark that the method proposed here may become particularly useful if the number of parameters included in the formula of the EET rate increases, since it is not necessarily clear what kind of balance of the parameters determines the EET rate if one makes use of the original formula.
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Front and side views of the optimized geometries for the ground state of PCB1, the first excited state of PCB1, the ground state of PCB2, the first excited state of PCB2, the ground state of PCB3, and the first excited state of PCB3 (Supplementary Fig. S1).
Front and side views of the optimized geometries for the ground state of PCBp1, the first excited state of PCBp1, the ground state of PCBp2, the first excited state of PCBp2, the ground state of PCBp3, and the first excited state of PCBp3 (Supplementary Fig. S2).
Front and side views of the optimized geometries for the ground state of PCBp1-asp, the first excited state of PCBp1-asp, the ground state of PCBp2-asp, the first excited state of PCBp2-asp, the ground state of PCBp3-asp, and the first excited state of PCBp3-asp (Supplementary Fig. S3).
Physical quantities related to the expression of the EET rate as formulated in Eq. (1) for PCB, PCBp, PCBp -asp, and PCBp-(1-): |κ|/|κ(0)|, |μD|/|μ(0)|, |μA|/|μ(0)|, |μD||μA|/|μ(0)|2, |VF|2/|VF(0)|2, J/J(0), and peak wavelengths of absorption and emission spectra in Q band shown Figure 5 and Supplementary Table S1 (Supplementary Fig. S4).
Factors, For, Fdip,D, Fdip,A, Fover, Fdis, and Fref as obtained from Eqs. (53)–(58) for the EET pathways, 1→2, 2→1, 2→3, 3→2, 1→3, and 3→1, and factors,
Factors, For, Fdip,D, Fdip,A, Fover, Fdis, and Fref as obtained from Eqs. (53)–(58) for the EET pathways, 1→2, 2→1, 2→3, 3→2, 1→3, and 3→1, and factors,
Factors, For, Fdip,D, Fdip,A, Fover, Fdis, and Fref as obtained from Eqs. (53)–(58) for the EET pathways, 1→2, 2→1, 2→3, 3→2, 1→3, and 3→1, and factors,
Calculated absorption and emission spectra of PCBp1-(1-)_shift, PCBp2-(1-)_shift, and PCBp3-(1-)_shift (Supplementary Fig. S8).
Factors, For, Fdip,D, Fdip,A, Fover, Fdis, and Fref as obtained from Eqs. (53)–(58) for the EET pathways, 1→2, 2→1, 2→3, 3→2, 1→3, and 3→1, and factors,
EET rates, KFörster/K(0), KDexter/K(0), and KEET/K(0), versus the intermolecular distance R/R(0), in P3HT/PCBM blend (Supplementary Fig. S10).
Relative importance of the physical quantities related to EET rate, KEET/K(0), versus the intermolecular distance R/R(0) in P3HT/PCBM blend (Supplementary Fig. S11).
Maximum wavelengths of absorption and emission spectra, and Stokes shifts in Q band for PCB1, PCB2, PCB3 PCBp1, PCBp2, PCBp3, PCBp1-asp, PCBp2-asp, PCBp3-asp, PCBp1-(1-), PCBp2-(1-), and PCBp3-(1-) shown in Figure 5, and PCBp1-(1-)_shift, PCBp2-(1-)_shift, and PCBp3-(1-)_shift. (Supplementary Table S1).
Magnitudes of orientation factor |κ|/|κ(0)|, transition dipole moments of D and A |μD|/|μ(0)| and |μA|/|μ(0)|, intermolecular center-to-center distance R/R(0), square of the the electronic coupling |VF|2/|VF(0)|2, spectral overlap J/J(0), EET rate constant KFörster/K(0), inverse of KFörster/K(0), and Cnorm for the PCB systems, PCB1, PCB2, and PCB3 (Supplementary Table S2).
Magnitudes of orientation factor |κ|/|κ(0)|, transition dipole moments of D and A |μD|/|μ(0)| and |μA|/|μ(0)|, intermolecular center-to-center distance R/R(0), square of the the electronic coupling |VF|2/|VF(0)|2, spectral overlap J/J(0), EET rate constant KFörster/K(0), inverse of KFörster/K(0), and Cnorm for the PCBp systems, PCBp1, PCBp2, and PCBp3 (Supplementary Table S3).
Magnitudes of orientation factor |κ|/|κ(0)|, transition dipole moments of D and A |μD|/|μ(0)| and |μA|/|μ(0)|, intermolecular center-to-center distance R/R(0), square of the the electronic coupling |VF|2/|VF(0)|2, spectral overlap J/J(0), EET rate constant KFörster/K(0), inverse of KFörster/K(0), and Cnorm for the PCBp-asp systems, PCBp1-asp, PCBp2-asp, and PCBp3-asp (Supplementary Table S4).
Magnitudes of orientation factor |κ|/|κ(0)|, transition dipole moments of D and A |μD|/|μ(0)| and |μA|/|μ(0)|, intermolecular center-to-center distance R/R(0), square of the the electronic coupling |VF|2/|VF(0)|2, spectral overlap J/J(0), EET rate constant KFörster/K(0), inverse of KFörster/K(0), and Cnorm for the PCBp-(1-) systems, PCBp1-(1-), PCBp2-(1-), and PCBp3-(1-). (Supplementary Table S5).
Magnitudes of orientation factor |κ|/|κ(0)|, transition dipole moments of D and A |μD|/|μ(0)| and |μA|/|μ(0)|, intermolecular center-to-center distance R/R(0), square of the the electronic coupling |VF|2/|VF(0)|2, spectral overlap J/J(0), EET rate constant KFörster/K(0), inverse of KFörster/K(0), and Cnorm for the PCBp-(1-)_shift systems, PCBp1-(1-)_shift, PCBp2-(1-)_shift, and PCBp3-(1-)_shift. (Supplementary Table S6).
Numerical calculations were carried out under support from the “Multidisciplinary Cooperative Research Program” at the Center for Computational Sciences (CCS) in University of Tsukuba.
This research was supported by Japan Science and Technology Agency (JST), PRESTO Grant Number JPMJPR19G6, Japan, and Japan Society for the Promotion of Science (JSPS) Grants-in-Aid for Scientific Research (KAKENHI) Grant Numbers JP19H05781, JP20H05088 and JP20H05453. M.B. thanks the HPC Mesocentera at the University of Strasbourg funded by the Equipex Equip@Meso project (Programme Investissements d’Avenir) and the CPER Alsacalcul/Big Data, and the Grand Equipement National de Calcul Intensif (GENCI) under allocation DARI-A0100906092.
The authors declare no conflict of interest.
The manuscript was written through contributions of all authors. K.M., derivations of equations, quantum chemistry calculations, and writing original draft. M.S., conceptualization, investigation, editing and funding acquisition. Y.U, M.B, and Y.S., investigation and editing.