Erika
Keil
a,
Ajeet
Kumar
a,
Lena
Bäuml
b,
Sebastian
Reiter
b,
Erling
Thyrhaug
a,
Simone
Moser
c,
Christopher D. P.
Duffy
d,
Regina
de Vivie-Riedle
b and
Jürgen
Hauer
*a
aTechnical University of Munich, TUM School of Natural Sciences, Department of Chemistry, Lichtenbergstrasse 4, 85748 Garching, Germany. E-mail: juergen.hauer@tum.de
bDepartment of Chemistry, Ludwig-Maximilians-Universität München, Butenandtstr. 11, 81377 Munich, Germany
cInstitute of Pharmacy, Department of Pharmacognosy, University of Innsbruck, Austria
dDigital Environment Research Institute, Queen Mary University of London, London E1 4NS, UK
First published on 27th November 2024
Chlorophylls are photoactive molecular building blocks essential to most photosynthetic systems. They have comparatively simple optical spectra defined by states with near-orthogonal transition dipole moments, referred to as Bx and By in the blue/green spectral region, and Qx and Qy in the red. Underlying these spectra is a surprisingly complex electronic structure, where strong electronic-vibrational interactions are crucial to the description of state characters. Following photoexcitation, energy-relaxation between these states is extremely fast and connected to only modest changes in spectral shapes. This has pushed conventional theoretical and experimental methods to their limits and left the energy transfer pathway under debate. In this work, we address the electronic structure and photodynamics of chlorophyll a using polarization-controlled static – and ultrafast – optical spectroscopies. We support the experimental data analysis with quantum dynamical simulations and effective heat dissipation models. We find clear evidence for B → Q transfer on a timescale of ∼100 fs and identify Qx signatures within fluorescence excitation and transient spectra. However, Qx is populated only fleetingly, with a lifetime well below our ∼30 fs experimental time resolution. Outside of these timescales, the kinetics are determined by vibrational relaxation and cooling. Despite its ultrashort lifetime, our theoretical analysis suggests that Qx plays a crucial role as a bridging state in B → Q energy transfer. In summary, our findings present a unified and consistent picture of chlorophyll relaxation dynamics based on ultrafast and polarization-resolved spectroscopic techniques supported by extensive theoretical models; they clarify the role of Qx in the energy deactivation network of chlorophyll a.
Despite their structural diversity, all Chls share two prominent spectral bands: the lowest energy Q-band (550–720 nm) and the Soret- or B-band (350–480 nm). Historically, these bands have been characterized using the Gouterman four-orbital model of the π–π* transitions in porphyrins.9,10 In this model, the Q-band consists of two distinct electronic states, which we name Qx,el and Qy,el. Their indices relate to the direction of the respective transition dipole moment within the plane of the macrocycle (Fig. 1a). Later, increasingly sophisticated quantum chemical calculations and experiments aimed to refine the assignment of the observed absorption bands to the two electronic states. However, the energetic position of the Qx,el state remained ambiguous. In 2013, Reimers et al.3 proposed a new band assignment based on vibronic coupling, mixing the states within the Q-band. We refer to the states after incorporating such coupling effects as Qx and Qy. This coupling strongly influences the spectral properties of Chl a. For example, the angle between the Qx and Qy transition dipole moments would naively be expected to be close to 90°, but the experimentally measured value for Chl a is ∼70–78°.11,12 In several subsequent two-dimensional electronic spectroscopy (2DES) studies, vibronic coupling was discussed as the basis of fast signal oscillations,13,14 the vibronic origin of which was proven by polarization-controlled studies.7 A similar conclusion was reached from theoretical studies, where it was shown that the Qx and Qy potential energy surfaces do not cross in an energetically accessible region, and non-adiabatic coupling facilitates ultrafast population transfer across the potential energy surfaces.5 Previous to 2DES studies, results from transient absorption (TA) spectroscopy were interpreted so that Qx → Qy transfer shows a strong and unusual solvent dependence, with Qx-lifetimes ranging from 100–250 fs in different solvents.8,15
In this work, we reinterpret the internal conversion dynamics of Chl a, as determined by TA spectroscopy with ∼20 fs excitation and ultra-broadband probing. To offer a comprehensive picture of the relevant deactivation pathways in Chl a, we perform TA experiments exciting the B and the Q-band selectively and compare our results with theoretical models. We can unambiguously determine a B → Q transfer time of ∼100 fs from our experimental data and corroborate our findings using theoretical models. We also show that coupling effects within the Q bands lead to almost instantaneous intraband relaxation.
To test our hypothesis of near-instantaneous Qx → Qy transfer, we go beyond global analysis of TA data and search for Qx-signals using polarization-selective spectroscopy, followed by isolation of polarization-associated spectra.16 Given reported Qx lifetimes of up to several hundreds of femtoseconds,15 we should observe x-polarized stimulated emission (SE) from Qx, along with Qx ground-state bleach (GSB) and excited-state absorption (ESA). While we successfully isolate the GSB signature of Qx, we find no sign of x-polarized SE or ESA features to indicate a transiently populated Qx state. We attribute this to vibronic mixing and rule out the conventional interpretation of Qx as a state with up to 300 fs lifetime.15 Instead, we offer an interpretation of the kinetic components found in TA based on intra-molecular vibrational redistribution and subsequent vibrational cooling, as described by an effective model.
The paper is structured as follows: to identify GSB signatures of Qx, we first analyze polarization-associated spectra derived from cryogenic fluorescence excitation spectra (“Assignment of Qx and Qy transitions”). Direct excitation of Qx is a non-ideal starting ground for studying dynamics, as the absorption features of Qx and Qy overlap strongly. Instead, we excite the B-band and try to isolate transient Qx features. We compare these results with TA data after direct Qx/Qy excitation (“Ultrafast relaxation dynamics of Chl a”).
Similarly to the dissection of linear spectra, we attempt to isolate Qx- and Qy-related excited state absorption features in transient absorption anisotropy (TAA) (“Isolating Qx-features by polarization control”) and compare our measured results to theoretical predictions (“System and system-bath relaxation dynamics at different timescales”). We show that neither TA experiments with sub 20 fs pump pulses nor polarization-controlled experiments can establish a timescale for Qx → Qy transfer. Instead, our work offers a new perspective on the energy transfer dynamics in Chl a. We relate the experimentally observed ultrafast dynamics to solvent relaxation processes and obtain a robust and consistent picture supporting strong mixing between Q-states.
Alongside the excitation and emission spectra, Fig. 1b also shows fluorescence anisotropy traces. The emission anisotropy (rem, blue line) was measured for λexc = 660 nm, while the fluorescence excitation anisotropy (rexc, orange line) was measured for λEm = 690 nm. In the Q band region, rexc of the main transition centered at 670 nm is almost flat. It reaches a value of 0.35, indicating near-parallel emission and absorption dipoles. As emission occurs from Qy, this band must be y-polarized. The same high value is obtained from rem upon excitation at 660 nm, proving the measurements to be consistent. While the main transition at 670 nm belongs to Qy, rexc shows clearly that the high-energy side of the Q band region contains contributions from electronic states with different polarizations, as anisotropy values here are as low as zero.
Several approaches have been developed to decompose optical spectra by leveraging the information on transition dipole moment (TDM) directions available from anisotropies.21–23 Most commonly, in the absence of a macroscopically oriented sample, these methods “project” the isotropic spectrum into contributions either parallel or orthogonal to a reference TDM. For excitation anisotropy measurements, this reference is the TDM of the emissive transition, while for emission anisotropy, the reference TDM is that of the pumped transition. In many cases, however, the TDMs of a given molecule are not exactly orthogonal, and the decomposition of the spectra in orthogonal components is not ideal. As earlier work has shown that the Chl a Qx and Qy TDMs are not orthogonal,11 this type of spectral decomposition will not result in optimal separation of the contributions. In a recent study, we developed a slightly modified decomposition approach, which is suitable for systems where TDMs are not orthogonal.16 In this approach, we can cleanly separate spectral contributions not only when the underlying TDMs are at an angle θ = 90°, but at any angle θ = 90° − β. The parameter angle β introduced here can be thought of as the rotation angle of an orthogonal molecular coordinate system defined by the reference TDM. For details, we refer to the corresponding publications.16,24
In Fig. 1c we show the decomposition of the Chl a excitation spectrum into components polarized parallel (here: Sy, blue in Fig. 1c) and orthogonal (here: Sx, red) to the emissive transition (Qy fluorescence) according to the procedure outlined above. We note that besides Qx features, Sx also contains signals with a TDM parallel to Bx, while Sy contains both Qy and By contributions. If we assume orthogonal Qx and Qy transitions (corresponding to β = 0), we clearly achieve sub-optimal separation of the spectrum with noticeable contamination of the Sx spectrum by features associated with the y-polarized transitions (see Fig. S1†). Increasing the value of β to 17°, however, maximizes the 670 nm peak in the Sy spectrum and simultaneously achieves optimal separation of the spectrum into “pure” but overlapping Qx and Qy contributions, each with their respective vibronic progressions. Note that both the Sx spectral maximum at approximately 640 nm and the relative angle between Qx and Qy of θ = 90 − β = 73° are in good agreement with previously reported results.4 In essence, polarization-associated analysis of Chl a excitation spectra is a straightforward and effective way of isolating overlapping Qx and Qy ground state transitions.
To better elucidate the mechanism of energy transfer dynamics in Chl a, we perform TA experiments under different excitation conditions (B- and Q-band excitation) and in various solvents (acetone, ethanol (EtOH), and benzonitrile (BN)). In particular, we expect to observe direct evidence of B → Q transfer and to understand the origin of the reported solvent dependence of the Qx → Qy energy transfer step. In the following, we show a representative set of data for Chl a in acetone. The corresponding plots for the other two solvents are shown in ESI Fig S2 and S3.† Absorption and pump pulse spectra are shown in Fig. 2a (Fig. S2†). Chirp-corrected TA data in magic angle (MA) configuration after B- and Q-band are shown in Fig. 2b and c, and the global analysis results are shown in Fig. 2d and e (Fig. S3†). The lifetimes corresponding to the individual spectral components are reported in each panel. Only the evolution-associated spectra (EAS) are shown for simplicity, while the decay-associated spectra for all solvents are shown in ESI Fig. S4.†
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Fig. 2 Absorption spectrum of Chl a in acetone plotted against the pump spectra for B-band (blue line) and Q-band (red line) excitation (a). Chirp-corrected TA data for both excitation conditions are shown in (b) and (c). Visible changes in the dynamics are present after B excitation, with a clear increase of the Q-band GSB signal over time, but this is not true after Q excitation. The EAS and lifetimes extracted from global analysis of Chl a in acetone are shown in (d) after excitation in the B-band and in (e) after excitation in the Q band. The corresponding plots for Chl a in EtOH and benzonitrile are shown in Fig. S2.† |
In the case of B-band excitation (Fig. 2b and d), the best fit is achieved with four kinetic components. The shortest component has a lifetime of ∼110 fs (black line), with negligible solvent dependence. It is characterized by a decrease and blue shift of the signal in the B-band region (430 nm) and a concomitant increase of the main Q-band signal (660 nm). This behavior is consistent with B → Q transfer, and the B → Q transfer time agrees with previously reported values.8 The second component (dark blue line) shows minimal spectral evolution; the only noticeable feature is a slight broadening of the Qy band. From the global fits, it appears to be strongly solvent-dependent, varying from ca. 400 fs (BN, cf. Fig. S3†) to 2 ps (acetone). Notably, the amplitude of this component is near-negligible, and it is not associated with any spectral evolution typical of state-to-state energy transfer. As changes to small-amplitude components do not substantially affect the goodness-of-fit, the lifetime associated with this component is inevitably highly uncertain. As such, although this component appears to exhibit some solvent dependence, we do not make strong quantitative claims about this behavior. We emphasize, however, that this component does not contain significant changes to stimulated emission or excited state absorption, implying that it is not related to population transfer. The third kinetic component (red line), with a lifetime of about 7–11 ps, correlates with a narrowing of the Qy band and an increase in its amplitude. Finally, the last kinetic component (light blue line, fixed to 5 ns) is readily assigned to the excited state lifetime of Chl a as known from fluorescence lifetime measurements.26
In the case of Q-band excitation (Fig. 2c and e), only three components are necessary to obtain a satisfactory data fit. We again observe an ultrafast component of 100–300 fs (black line) that was previously assigned to Qx → Qy transfer.8,15 If this component was associated with population transfer, we would expect a signal decrease in the 520–630 nm Qx-region concomitant with an increase in the Qy ground-state bleach (GSB)/stimulated emission (SE) amplitude around 660 nm. As in the B-band excitation case, however, we do not observe any such features, leaving this component inconsistent with a population transfer process. An intermediate 1.5–15 ps component (red line) with extremely small amplitude similarly does not relate to significant spectral changes, suggesting a small structural reorganization process. The longest component is again the excited state lifetime of Chl a, fixed at 5 ns (light blue line).
To isolate Qx-signatures and to determine their transient behavior, we have measured transient absorption anisotropy (TAA) data for Chl a in acetone after B-band excitation. With these data, we can decompose the TA signals into polarized components in an analogous procedure to that described for excitation anisotropy.16,24 In this case, a value of β = 32° is necessary to fully suppress the Qy peak. In the employed representation, Sx contains signals with a TDM parallel to that of Bx, including all Qx features, while Sy contains the Qy and By contributions. Representative spectra are shown for a time delay Δt = 120 fs in Fig. 3a. At this delay time, effects due to pump-and-probe pulse overlap are negligible, and there is already population in the Q-band resulting from B → Q transfer (cf.Fig. 2b and d).
In search for Qx-features, we identify two weak negative peaks at 580 nm (ca. 17200 cm−1) and 625 nm (ca. 16
000 cm−1), matching the Qx features observed in the excitation anisotropy measurements (Fig. 3a, red line and inset). They show an energy spacing of about 1100 cm−1 as calculated by fitting a bi-gaussian function to the peaks (Fig. 3a, inset, black lines), in excellent agreement with magnetic circular dichroism spectra for pentacoordinated Chl a.3
The lineshape of the Sx spectrum remains identical for time delays between 100 fs and several ps (Fig. S5†). This means that while we observe the Qx GSB, no Qx SE (or excited-state absorption (ESA)) features are discernible. We support this statement further by performing a global analysis of the polarization-decomposed TA maps shown in the ESI (Fig. S6†). Similar time constants are needed to fit Sx and Sy, and there is no evidence for a transient population of an excited Qx state.
We further examine the possibility of Qx ESA features by comparing the experimental excited state spectrum to calculations for both B-excitation (Fig. 3b) and Q-excitation (Fig. 3c). The experimental excited state spectrum is determined from the measured TA spectrum by subtracting the GSB.27,28 The latter is approximated by a scaled absorption spectrum. The resulting spectra only contain ESA and SE contributions. We then compare the lineshapes of these spectra at early and late times with calculations for the Qx- and Qy-associated ESA, considering one acetone molecule coordinating to the central Mg of a Chl a molecule. Notably, the excited-state spectrum at early times after B-band excitation has a positive feature at 655 nm which is absent at later times and in the case of Q-band excitation. We attribute this to ESA from the B-band, which is cancelled by the Q-band GSB, explaining why we do not observe this feature in the magic angle TA data in Fig. 2d. While the calculated Qy ESA-peaks correspond to measured features at both early and late times, the features related to Qx ESA are missing. In particular, two intense Qx-features are expected in the 16000–21
000 cm−1 region at early times. However, the measured spectra in this region at early and late times are effectively identical. While ESA from Qy is clearly visible, the lack of excited-state signatures associated with Qx means that Qx is either not significantly involved in the energy relaxation network or its lifetime is shorter than the experimental time resolution.
While we can readily explain ultrafast time constants with our quantum dynamics simulations, the dynamics at longer times are not practically accessible with this type of calculation. At these longer timescales, we expect energy redistribution and dissipation to the solvent to be the dominating contributions to the dynamics.28 As such, the bath must be considered when trying to reproduce the longer kinetic components observed in TA.
We construct a simplified numerical model to test our hypothesis of cooling dynamics on multiple timescales. Excitation of Chl a with a visible laser pulse always means that a large amount of energy is deposited into the vibrational modes of the molecule. Energy deposited – directly or indirectly – into a high-lying state of Qy will relax in a non-linear sequence of intra-molecular vibrational redistribution (IVR) events, solute-to-solvent energy transfer, and solvent equilibration. Using an effective molecular temperature Tm (details and modeling parameters in the ESI text, Table T2, Fig. S9 and S10†) that increases with the energy deposited into the system, we predict a molecule-to-solvation shell transfer time of ∼1 ps. This is consistent with observations from our previous work on carotenoids.29–31 The dynamics of Tm are determined by two timescales: τIVR ∼ 1 ps, which accounts for the rise in Tm due to thermalization of the Qy state, and τVC ∼ 7–9 ps, which is the relaxation of the solute due to vibrational cooling (VC) into the solvation shell. The exact values of the time constants vary with the solvent (Fig. 4c and d). The results indicate that the relaxation kinetics are almost independent of whether one excites Qy directly or indirectly via the B-band. However, the maximum Tm reached should be affected by excitation wavelength, as this defines the amount of energy that thermalizes (Fig. 4c and d). As τIVR is associated with heating and τVC with cooling, we expect to observe thermal broadening effects of the Qy-band over ∼1 ps as the maximum Tm is achieved, followed by spectral narrowing over ∼10 ps as the population of low-frequency vibrational modes drops while the solute and first solvation shell re-equilibrate with the bulk solvent. Careful inspection of the decay-associated and evolution-associated spectra (DAS and EAS, respectively) in the Q-band region (Fig. S11†) confirms these predictions for excitation in the B-band, although the observed lineshape changes are minimal. After Q-band excitation, IVR and cooling are much less pronounced. In particular, we do not observe a narrowing in ∼10 ps as expected. Instead, we observe a minimal but continuous redshift typical of Stokes shift dynamics (Fig. S11†).28
An implication of these observations is that none of the time constants found in MA-TA (cf.Fig. 2) can be assigned to Qx → Qy transfer. The small amplitudes and only subtle influence on the spectra of the kinetic components other than the one related to B → Q transfer suggest instead an association with IVR and subsequent heat dissipation to the solvent.
In Fig. 5, we propose a comprehensive scheme for the internal conversion dynamics of Chl a. After the initial B → Q transfer, the state we detect is y-polarized. Therefore, if Qx is participating in the energy transfer as suggested by the quantum dynamics calculations, its relaxation towards a vibrationally hot, y-polarized state must be faster than our time resolution. The relaxation from there to the vibrationally relaxed Qy occurs through IVR, leading to heat exchange with the first solvation shell. Further relaxation to bulk solvent (VC) then occurs on slower timescales. Overall, IVR and VC are sufficient to explain the timescales in the evolution of the Chl a TA spectra beyond the first few hundred fs after B-band excitation: ∼1 ps for IVR to a hot pseudo-thermal state, ∼10 ps for relaxation of the hot thermal state (Fig. 4c and cf.Fig. 2d). The effect of IVR and VC on the lineshape is much less pronounced after Q-band excitation. In this case, the changes in the lineshape can be explained by Stokes shift dynamics.28
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Fig. 5 Vibronic mixing (J) in the Q band leads to strongly coupled states Qx (red) and Qy (blue). Ultrafast transfer via Qx populates a vibrationally excited Qy, which in turn relaxes via intra-molecular vibrational redistribution (IVR), followed by slower equilibration with the surrounding solvent (vibrational cooling VC). The right panel shows a sketch of the spectral profiles of Qx and Qy, as discussed in Fig. 1. |
In summary, our findings shed new light on the internal conversion dynamics in Chl a. Although the heating–cooling cycle on the Qy surface of Chl a is highly complicated and requires further investigation from both experimental and theoretical sides, we reach a good agreement between model and experiment. We present experimental and theoretical evidence for B → Q transfer on a ∼120 fs timescale. The relaxation dynamics in the Q band are dominated by the strong coupling of the Qx and Qy states and occur on a <30 fs timescale. This leads to the absence of x-polarized excited-state signatures in TAA experiments. We attribute this ultrafast Qx lifetime to the small and internal-coordinate-independent energy gap between Qx and Qy. Regardless of its short lifetime, Qx seems important for efficient B → Q relaxation, as the B → Q transfer rate slows down if B/Qx coupling is deactivated. Based on these results, we reinterpret the solvent-dependent, longer time constants found in TA measurements as a combination of IVR, VC, and possibly Stokes shift dynamics on Qy. Overall, our unique combination of extensive theoretical modeling, numerical methods, and highly sensitive TA experiments allows us to paint a clear and consistent picture of the energy transfer in Chl a under the excitation conditions relevant to photosynthetic systems and to shed light on the previously controversial role of the Qx state in the Chl a dynamics.
UV-vis spectra were measured on a PerkinElmer Lambda 365 spectrometer. Emission spectra were measured on a Spectrofluorometer FS5 (Edinburgh Instruments). All spectra are background-corrected.
HR ESI-MS (positive ion mode): m/z (found) = 893.5426; m/z (calculated) = 893.5426, Δ = 0.56 ppm.
TA experiments were performed for Chl a in acetone, ethanol (EtOH), and benzonitrile (BN). Chl a was excited in the B and Q bands in separate experiments for all solvents. The pulse duration of the two pump pulses was comparable, with the B-pump at 20 fs and the Q-pump at 15 fs as measured by SD-FROG and SHG-FROG, respectively. The measured and retrieved FROG traces, as well as the retrieved spectral and temporal phase profiles, are shown in the ESI (Fig. S12†). The TA setups used for B- and Q-band excitation have been described in detail before.33,34 Briefly, a 5 kHz, 2.5 mJ, 25 fs amplified laser system (Coherent Legend Elite Duo HE+ Ti:
Sapphire MOPA) is used to seed a 1 m long, commercial hollow-core fiber (HCF) with a core diameter of 250 μm filled with 1 bar of Argon gas. The resulting supercontinuum is either frequency-doubled in an achromatic second-harmonic scheme to yield the B-band pump pulse33 or spectrally filtered to obtain the Q-band pump pulse.34 In the first case, the pump is compressed by a three-prism configuration, while in the second case, the compression is achieved by chirped mirrors. In both experiments, the probe pulse is given by a supercontinuum obtained by seeding a CaF2 crystal with the NIR part of the HCF output. For B-band excitation, a double-chopping scheme was employed to reduce scatter, and the pump energy was 60 nJ per pulse with a focal spot diameter of 200 μm; for Q-band excitation, the pump pulse was not chopped and its energy was 16 nJ per pulse with a focal spot of 140 μm. The data was recorded at MA (54.7°) configuration between pump and probe for B- and Q-pumping. Additionally, datasets with parallel and perpendicular polarization of pump and probe were recorded for B-band excitation of Chl a in acetone in order to calculate the TAA.
Global analysis was performed with the open-source software Glotaran.35,36
Excited state absorption spectra for the optimized geometries were simulated at the double-hybrid TDDFT level using the ORCA 5.0.3 software package.56–58 The SCS-ωPBEPP86 density functional59 was used in the Tamm–Dancoff approximation60 along with the def2-TZVPD61,62 basis. The calculation was accelerated by employing the RIJCOSX approximation63,64 with the def2/J65 and def2-TZVPD/C66 auxiliary basis sets. A tighter-than-usual integration grid (ORCA keyword DefGrid3) and convergence criteria (ORCA keywords VeryTightSCF TightPNO) were employed. The bulk solvent was described implicitly via the linear-response conductor-like polarizable continuum model (LR-CPCM),67,68 assuming equilibrium solvation in the excited state.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d4sc06441k |
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