Open Access Article
Yana Reva‡
a,
Jonas Färber‡
a,
Yifan Bo
a,
Maximilian A. Thiele
a,
Christian Hankeb,
Ayşe Günay-Gürer
a,
Maximillian Herm
a,
Johannes A. C. Barthb and
Dirk M. Guldi
*a
aDepartment of Chemistry and Pharmacy, Profile Center FAU Solar, Interdisciplinary Center for Molecular Materials (ICMM), Friedrich-Alexander-Universität Erlangen-Nürnberg, 91058 Erlangen, Germany. E-mail: dirk.guldi@fau.de
bDepartment Geographie und Geowissenschaften, Geozentrum Nordbayern, Friedrich-Alexander-Universität Erlangen-Nürnberg (FAU), Schlossgarten 5, 91054, Erlangen, Germany
First published on 15th May 2026
In this study, we investigated the mechanistic factors that govern the selective photocatalytic reduction of CO2 over protons within a simple π-conjugated N-heterocycle, proflavine. Diluted conditions, where aggregates of 65 nm are formed, favored the selective CO2 photo-reduction, while the gradual transition to concentrated conditions enabled photo-reductive H2 generation. Proton reduction is coupled to larger aggregates, in which an alternative photo-relaxation pathway is active. We used transient absorption spectroscopy to corroborate that at low proflavine concentrations the presence of an electron donor triggers the one-electron reduced proflavine to perform the direct CO2 reduction. At high proflavine concentrations, protonation of the one-electron reduced proflavine was favored due to a positive shift in basicity in larger aggregates with sizes over 1 µm. In turn, H2 abstraction began with a pair of one-electron reduced, protonated, intermediates. Our study demonstrates an effective approach to limiting water reduction, a key challenge in advanced metal-free organic photocatalysis.
In photo-redox reactions, photocatalysts are excited, subsequently reduced by a suitable electron donor to finally produce a catalytically active species, that reduces the substrate by direct electron transfer.3,4 The primary activation is crucial and involves bending of CO2 and overcoming the negative reduction potential of −1.9 V vs. NHE.5 Chemisorptive activation appears essential to lower the activation barrier and facilitate CO2 reduction.6 By tuning the electron-donating strength, light-activated reduction of the photocatalyst governs both its interactions with CO2 and the subsequent substrate reduction. In contrast, protonation of the reduced photocatalyst deactivates the CO2 reduction pathway, lowers its electronegativity, and creates favorable conditions for proton reduction and, therefore, H2 generation.7
With a focus on the competing CO2 and H+ reduction, any change in the photocatalyst concentration commonly affects both pathways in the same way.8–10 The scenario changes, however, as soon as aggregation comes into play. In metal-based photocatalysts, aggregation enhances the catalytic CO2 reduction efficiency, while minimizing the competing water reduction.11,12 A similar balance in organic, metal-free catalysts has not yet been extensively investigated, highlighting a significant knowledge gap. The intrinsic proton affinity of organic materials and pKa shifts in aggregated systems13–15 collectively suggest that aggregation is crucial for determining the photocatalytic selectivity. One prominent example of an efficient metal-free CO2 reducing photocatalyst is covalent organic frameworks (COFs). COF's selective photo-reduction of CO2 in aqueous solutions using visible light is remarkable.16–18 COFs, which are constructed from π-conjugated N-heterocycles, are of particular interest here. For instance, Fu et al. found, that metal-free triazine-based COFs drive a clear-cut photocatalytic conversion of CO2 to methanol, producing only trace amounts of H2.19 Hereby, π-conjugated N-atoms, which serve as photocatalytic centers in the triazine-building blocks,20 play a crucial role.
In this work, we address the nuanced interplay between aggregation and selectivity in the reduction of CO2 over protons. The model system proflavine – a π-conjugated N-heterocycle was utilized. Considering both, the ability to form aggregates21 and a suitable pH window to tune the de-/protonation of the active photoreduced species,22,23 proflavine represents an excellent model.
In the ground state at pH 7, proflavine exists primarily in its single protonated form, as (Pf-H)+ (Fig. 1a).24–28 Following photoexcitation at 443 nm and intersystem crossing (ISC) under deoxygenated conditions, the long-lived triplet excited state (T1)(Pf-H)+ emerges.27,29 In the presence of an electron donor, such as TEOA, (T1)(Pf-H)+ with an energy of 2.17 eV accepts an electron and is transformed into the reduced (Pf-H)˙ (Fig. 1a). Because of its reduction potential of −1.57 V vs. SHE (Pf-H)˙ is active in numerous photo-redox reactions.22,24,30–33 The reduced species exhibits a pKa value of 4.5 and, therefore, forms (Pf-H2)˙+ under acidic conditions (Fig. 1a).23 Noticeably, electron-rich and conjugated nitrogen atoms are present. Thus, we hypothesise that (Pf-H)˙ chemisorbs CO2 at the electron-deficient carbon site and then facilitates its reduction. Additionally, aggregate formation is thought to be beneficial for altering its proton affinity, a key step for protonation and thus for H2 generation.
Considering the aforementioned results, we not only infer two different photo-relaxation pathways, but also their dependence on the photocatalyst concentration. To elaborate on the nature of the concentration-dependent CO2/H+ reduction selectivity, dynamic light scattering (DLS) was measured under optimized photocatalytic conditions, with a (Pf-H)+ concentration ranging from 1.6 to 850 µM (Fig. 1d). At concentrations below 52 µM, (Pf-H)+ forms aggregates with an average size of 65 nm in the presence of 4.28 vol% TEOA and 0.55 M KH2PO4 (pH 7). At 52 µM dihydrogen is generated and the aggregate size notably increases. At 1000 µM, where photocatalysis yields solely H2, the average size of the aggregates reached 1 µm. The absorption spectra of (Pf-H)+ across different concentrations were examined (Fig. S4). Starting at around 52 µM, a stepwise blue-shift in the absorption maximum from 445 to 441 nm along with the emergence of a shoulder at 482 nm were observed. This supports the notion that aggregates are growing when a critical concentration of (Pf-H)+ is passed (Fig. 1e). To this end, photocatalytic tests using 1000 µM (Pf-H)+ in aqueous solutions containing 4.28 vol% TEOA were conducted and the pH was changed from 6.5 to 10 by varying KH2PO4 (Fig. S5). Importantly, below a pH of 7 all photo-products relate to the H+ reduction. Going beyond a pH of 7, CO2 reduction products were found next to those stemming from H+ reduction.|| Aggregation has caused a shift in the pKa of the active species, (Pf-H)˙. A stronger basicity facilitates the protonation, on one hand, and enhances H2 generation, on the other hand.
Further, mass spectrometry with the chemically generated (Pf-H)˙ was conducted and a mass of 209.01 m/z was found in the negative ion mode. This is in good agreement with the corresponding isotope pattern (Fig. S7).** Additionally, a titration of (Pf-H)˙ under inert atmosphere corroborates the 446 nm fingerprint of protonation below a pH of 4.5. Corresponding titration curves and spectra are all gathered in Fig. S9. In another experiment, we saturated a (Pf-H)˙ solution with CO2 and noted a red-shift of the absorption to 443 nm. Implicit is the re-oxidation of (Pf-H)˙ and regeneration of (Pf-H)+ (Fig. S10). Moreover, the gaseous products generated upon CO2 saturation of (Pf-H)˙, namely CO and CH4, were analysed. This data was compared with that recorded for a CO2-saturated solution of (Pf-H)+ at 25 µM, which lacked any CO2 reduction (Fig. S11). (Pf-H)˙ showed a striking kinetic selectivity: while it exhibited high stability against re-oxidation by O2 (only 2% re-oxidized after 24 hours in 99.9% O2), it underwent full and instant re-oxidation when exposed to CO2, confirming the CO2 pathway's kinetic preference (Fig. S12). Given the absence of an electron donor, buffer or photoirradiation, CO and CH4 unambiguously stem from the direct CO2 reduction. Hence, we postulate that (Pf-H)˙ is a key species in the photocatalytic CO2 reduction.
To provide unambiguous evidence for the carbon conversion pathway, we monitored the 13C/12C ratios in both CO2 and CH4 using wavelength-scanned cavity ring-down spectroscopy. The 13C/12C ratios are expressed in a delta notation as a permille deviation from Vienna Pee Dee Belemnite (i.e. δ13C in ‰ VPDB) as standard. They were determined for CO2 and CH4 in the complete photocatalytic system and solutions in the absence of an electron donor, buffer or photoirradiation (Table S1).†† The originally added CO2 had a δ13C value of −41.6‰. It was only upon CO2 addition together with all other additives that we found significant CH4 yields. Under these conditions, δ13CCO2 decreased by a maximum of 7.0‰. At the same time, any detectable CH4 was around an average of −37.3‰. From these findings we conclude that CH4 stems from CO2 reduction with a preferential uptake of 13C. Additionally, the 13C/12C ratios for any dissolved organic carbon (doc) were measured by isotope ratio mass spectrometry with and without irradiation (Table S2). Our δ13Cdoc measurements lacked any deviations, but differed noticeably from the δ13C of generated CH4. Negligible differences in δ13Cdoc – with and without irradiation – coupled with their significant deviations from δ13CCH4 confirms that CH4 is not a by-product of any organic material decomposition.
To gather additional information on the photoreduction mechanism proflavine was deposited onto a platinum surface and electrochemical operando Raman spectroscopy was conducted. The aqueous phase was purged with CO2 and KH2PO4/K2HPO4 were added to adjust the pH to 7. Broad fingerprints between 750 and 1750 cm−1 were taken as evidence for the proflavine stability at 0 V vs. Ag/AgCl. Under reductive conditions, that is, −1.5 V vs. Ag/AgCl, new features emerged as evident from the corresponding differential spectrum. Compared to reference measurements at 0 V vs. Ag/AgCl, the spectral changes at −1.5 V vs. Ag/AgCl revealed broad signals with distinguishable peaks around 1307 and 2208 cm−1, corresponding to symmetric –C–O stretching vibration of a carboxylate-like species (CO2 adsorption) and –C
O stretching vibration (CO adsorption), respectively (Fig. S13). These features are the crucial intermediates in the formation of CO and CH4. Their presence confirms the successful adsorption and subsequent reduction of CO2 by proflavine.
EAS-1, for which a lifetime of 3.8 ps was determined, showed excited state absorptions (ESAs) at 400 nm, ground state bleaching (GSB) at 445 nm, and stimulated emission (SE) at 515 nm. All of them are in excellent agreement with the steady state absorption and fluorescence spectra of (S0)(Pf-H)+ (Fig. S17). As the decay of EAS-2 is outside the fs-TA timescale, we conducted additional ns-TA experiments. ns-TA spectra were also fitted obtaining two EASs, that is, EAS-2 and EAS-3 (Fig. S18). The characteristics of EAS-2, which include ESA at 400 nm, GSB at 445 nm, and SE at 515 nm, are like those of EAS-1. From the similarity between EAS-1 and EAS-2 it was concluded, that the two are a vibrationally hot singlet excited state (Shot1)(Pf-H)+ and a vibrationally relaxed singlet excited state (Srel1)(Pf-H)+, respectively. After 4.7 ns, SE is replaced by ESAs < 390 nm and between 500 and 750 nm. These comprise EAS-3 and feature a lifetime of 29.2 µs. In line with sensitization experiments using (Ir[dF(CF3)ppy]2(dtbpy))PF6 as a triplet sensitizer,34 EAS-3 is attributed to the triplet excited state – (T1)(Pf-H)+.§§ All reference experiments are summarized in Fig. S19–S21.
In the next set of our experiments TEOA was added: 25 µM (Pf-H)+, 0.55 M KH2PO4, and 4.28 vol% TEOA. On the fs-TA timescale, the only fully resolvable EAS was that of EAS-1 with 450 nm GSB and 515 nm SE. It is the (Shot1)(Pf-H)+ (Fig. S22). Its lifetime is with 7.5 ps slightly longer than the reference experiments. On the ns-TA timescale, the data was taken and best deconvoluted when using a three species kinetic model (Fig. 2). EAS-2 is also like in the experiments without TEOA – albeit being lower in intensity – identified as (Srel1)(Pf-H)+. It takes 4.5 ns, by which EAS-2 gives place to EAS-3, namely a localized (T1)(Pf-H)+. Notably, (T1)(Pf-H)+ is in the presence of TEOA shorter-lived than in the absence of TEOA; 4.5 versus 29.2 µs.
To gather insights into the TEOA-induced quenching of (Pf-H)+, we conducted ns-TA at different TEOA concentrations. The pH was kept constant at 7 by means of adjusting the KH2PO4 concentrations. Results were quantitatively treated with the Stern–Volmer relationship, τ0/τ = 1 + KSV[TEOA], in which KSV is the Stern–Volmer constant, [TEOA] is the concentration of TEOA, and τ0 and τ are the (T1)(Pf-H)+ lifetimes in the absence and presence of TEOA, respectively. The linear relationship was ascribed to the dynamic electron-transfer quenching of (T1)(Pf-H)+ by TEOA.¶¶ With the KSV of 16.4 M−1 the bimolecular quenching rate constant (Kq) was calculated to be 5.6 × 105 M−1 s−1 (Fig. S23). A low Kq is attributed to the partial protonation of TEOA at pH 7 due to a pKa value of 7.76, lowering the concentration of its unprotonated, electron-donating form. Therefore, the presence of protonated TEOA limits the rate constant well below the diffusion-controlled limit.
The quenching of (T1)(Pf-H)+ by the electron donating TEOA resulted in EAS-4, for which a distinct 388 nm ESA and a lifetime outside the time-range of our ns-TA set-up were derived. Considering a significant spectral overlap of the differential (Pf-H)˙ − (Pf-H)+ and EAS-4 as well as the presence of an electron-donating TEOA, EAS-4 is assigned to (Pf-H)˙ (Fig. S24). Fig. 2e summarizes the proposed mechanism for the low concentration experiments – aggregate size 65 nm.
To exclude any impact of TEOA degradation products onto the proposed mechanism, ns-TA was conducted with 25 µM (Pf-H)+ in water, using 4.28 vol% methanol rather than TEOA as electron donor. The raw data was deconvoluted with a kinetic model based on three species (Fig. S25). All three EASs match those discussed when employing electron donating TEOA and, in turn, prove its electron donation.
Global analyses of fs-TA reveal two consecutively emerging EAS, that is, EAS-1 and EAS-2. They correspond to (Shot1)(Pf-H)+ and (Srel1)(Pf-H)+ and match the spectral characteristics seen in the low concentration regime (Fig. S26). It takes 3.2 ps for (Shot1)(Pf-H)+ to interconvert into (Srel1)(Pf-H)+. To determine the lifetime of EAS-2 we conducted ns-TA. Interpretation of the 410 µM (Pf-H)+ ns-TA experiments required a kinetic model based on three species, that is, EAS-2, EAS-3, and EAS-4 (Fig. S27). EAS-2 are similar on the fs- and ns-time scales. The lifetime of (Srel1)(Pf-H)+) is 5 ns. EAS-3 and EAS-4 exhibit similar spectral properties: ESAs < 390 nm and between 500 and 750 nm. To this end, EAS-3 and EAS-4 both are attributed to (T1)(Pf-H)+s; one short-lived with a lifetime of 1 µs, and one long-lived with a lifetime of 33 µs. We hypothesize that the 1 µs component of (T1)(Pf-H)+ is due to triplet–triplet annihilation and that it is activated by the high (Pf-H)+ concentration.
fs-TA spectroscopy of the TEOA-containing aqueous system with 410 µM (Pf-H)+, 4.28 vol% TEOA, and 0.55 M KH2PO4 gives rise to two EASs. For EAS-1, 400 nm ESA and 440 nm GSB are complemented by 515 nm SE (Fig. S28). This (Shot1)(Pf-H)+ lives for 33.3 ps and undergoes relaxation to afford (Srel1)(Pf-H)+. Insights into the decay of (Srel1)(Pf-H)+ came from ns-TA measurements. Fitting the ns-TA spectrum requires the use of four species rather than three like in the absence of TEOA.||||
For EAS-2, once again, 400 nm ESA, 440 nm GSB, and 515 nm SE due to (Srel1) are noted. (Srel1) undergoes intersystem crossing within 4.5 ns to afford (T1)(Pf-H)+ in the form of EAS-3 based on ESAs < 390 nm and between 500 and 750 nm (Fig. 3). Rather than undergoing ground state recovery as in the case of TEOA-free conditions, (T1)(Pf-H)+ decays quickly in the presence of 4.28 vol% TEOA within 2.1 µs. A 35.5 µs lived EAS-4 evolves from the interaction of (T1)(Pf-H)+ with the electron donating TEOA. The most prominent ESAs are discernible at 388 and 450 nm. As shown previously, (Pf-H)˙ protonation causes a rise of a 446 nm feature, which is assigned to (Pf-H2)˙+. To deconvolute the spectral signature of EAS-4, EAS-3 was subtracted from EAS-4. The resulting differential spectrum combines the spectral features of (Pf-H)˙ next to those of (Pf-H2)˙+ (Fig. S30). The final species, namely EAS-5, is an amplification of the 446 nm ESA and, therefore corresponds to a second (Pf-H2)˙+. Its lifetime is outside of the time-range covered by our ns-TA set-up. In stark contrast to the experiments at low (Pf-H)+ concentrations, protonation of (Pf-H)˙ and formation of (Pf-H2)˙+ are observable on the microsecond timescale, due to an increase in proton affinity of the reduced proflavine in the aggregates. Evidently, at the given concentrations a competing photocatalytic path evolves. A somewhat broader size distribution of aggregate sizes at the concentration of 410 µM renders the deconvolution of (Pf-H)˙ and (Pf-H2)˙+ and detection thereof impossible.*** Fig. 3e summarizes the proposed mechanism for intermediate concentrations of proflavine (700 nm-aggregate).
Following its 3 µs lasting decay, ESAs > 500 nm of EAS-4 are formed as (Pf-H2)˙+ grows. For the latter, a lifetime of 43.6 µs was derived. Notably, it was impossible to deconvolute (Pf-H)˙ found at the lower concentrations. We rationalize this fact by a pKa-driven shift towards (Pf-H2)˙+ rather than (Pf-H)˙.
Subsequently, EAS-5 evolves and is linked to the intensification of the ESA > 500 nm. EAS-5 lifetime extends beyond the temporal window of our ns-TA set-up. While the high (Pf-H)+ concentration of 1000 µM leads to strong ground-state absorbance that obscures the near-UV region, the emergence of the (Pf-H2)˙+ ESA is still evident, and its gradual intensification is clearly supported. Consequently, after the initial (Pf-H2)˙+ is produced, a second (Pf-H2)˙+ forms.
Our previous investigations with N-heterocyclic phenazine aggregates demonstrated that TEOA facilitated the formation of the second reduced and protonated phenazine via a chemical reduction that is linked to TEOA's self-oxidation reaction.7 In ns-TA, an intensification of the characteristic ESAs reflects the second reduction and protonation. Seeing a similar behavior in proflavine-aggregates, we conclude that the reduction of (T1)(Pf-H)+ and the formation of (Pf-H)˙ is linked to a positive pKa shift in the 1 µm-aggregates. This facilitates protonation to afford (Pf-H2)˙+. (Pf-H2)˙+ subsequently reacts with a second (Pf-H2)˙+ before H2 is released. Fig. 4e summarizes the proposed mechanism for high concentrations of proflavine – aggregate size of 1 µm.
Once the critical concentration is passed, the formation of H2 starts to compete with the CO2 reduction. This concentration represents a threshold beyond which the degree of clustering gradually increases. Based on fs-TA and ns-TA spectroscopy larger aggregates enforce the protonation of (Pf-H)˙, yield (Pf-H2)˙+, and allow for H2 release upon reaction with a second (Pf-H2)˙+. This reactivity is attributed to a positive shift in the pKa of reduced proflavine at higher degrees of clustering. The intricate nature of this aggregation process provides a fertile ground for further investigation, opening up new avenues for understanding and controlling the mechanism of organic photocatalysts. Fig. 5 summarizes the complete mechanism.
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| Fig. 5 Electronic ground- and excited state square scheme in proflavine at pH 7 in the presence of electron donating TEOA. | ||
Footnotes |
| † Dedicated to Jonathan Sessler on the occasion of his 70th birthday. |
| ‡ These authors contributed equally. |
| § The corresponding values were further used as references and subtracted to reveal the amount of photocatalytically generated products. |
| ¶ The reported product yields are not normalized by turnover number (TON) due to the observed degradation of the photocatalyst over time. This instability implies that the catalyst's activity diminishes throughout the reaction period, making traditional TON calculations unrepresentative of the system's true catalytic efficiency. |
| || The concentration of H2 has remained constant. |
| ** Storing a (Pf-H)˙ solution for 24 h confirmed its inertness in water (Fig. S8). |
| †† The increased concentration of CH4 in the isotopic measurements are explained, as here a different setup was used, which demanded a decreased gas to liquid phase ratio in the containers paired with an increased irradiation surface of the vessels. |
| ‡‡ The gaseous phase was analyzed and the sample was re-purged with CO2 every 30 min. |
| §§ ns-TA in oxygen-free methanol solutions of (Ir[dF(CF3)ppy]2(dtbpy))PF6 and (Pf-H)+ resulted in a 1.38 µs lasting formation of ESAs < 390 and between 500 and 750 nm that decayed with 28.2 µs. |
| ¶¶ In order to reach pH 7, the TEOA-free sample was buffered with KH2PO4 and K2HPO4. Different electrolyte-composition causes an offset of the τ0 value, deviating the linear behavior and, therefore was excluded from fitting. |
| |||| The corresponding time-trace fits and singular value decompositions of the residual matrices corroborate the choice of four (Fig. S29). |
| *** The model fitting with five species does not sufficiently resolve (Pf-H)˙ and (Pf-H2)˙+ separately (Fig. S31). |
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