Open Access Article
Bhawna
Rawat
a,
Ankita
Kumari
b,
Manvi
Sachdeva
a,
Himanshu
Bhatt
a,
Dibyajyoti
Ghosh
b,
Hirendra N.
Ghosh
*c,
Rajenahally V.
Jagadeesh
*de and
Kamalakannan
Kailasam
*a
aInstitute of Nano Science and Technology (INST), Knowledge City, Sector 81, SAS Nagar, Manauli PO, 140306 Mohali, Punjab, India. E-mail: kamal@inst.ac.in
bDepartment of Chemistry, Indian Institute of Technology, Delhi, Hauz Khas, New Delhi 110016, India
cSchool of Chemical Sciences, National Institute of Science and Education Research (NISER), Bhubaneshwar, Odisha 752050, India
dLeibniz-Institut für Katalyse, Albert-Einstein-Straße 29a, 18059 Rostock, Germany
eNanotechnology Centre, Centre for Energy and Environmental Technologies, VŠB–Technical University of Ostrava, Ostrava-Poruba, Czech Republic
First published on 2nd September 2025
Sunlight-driven integration of photocatalytic CO2 reduction with biomass feedstock valorization constitutes a highly efficient strategy for the synergistic production of multi-electron products and high-value fine chemicals, adhering to photo-chemical circular economy and sustainability. To date, no halide perovskite has been utilized for CO2 reduction coupled with biomass oxidation as the development of more stable, efficient, reusable, and non-toxic halide perovskites continues to be challenging. Herein, we report the room-temperature synthesis of methylammonium tin bromide (MA2SnBr6) quantum dots (QDs), a vacancy-ordered hybrid halide perovskite (HHP), without additional capping agents. These novel QDs maintain structural integrity in air, moisture, and polar solvents, addressing a significant issue associated with halide perovskites. Remarkably, the MA2SnBr6 QDs remain stable under ambient conditions even after 1 year, as confirmed by PXRD analysis. Interestingly, MA2SnBr6 achieved exceptionally high electron consumption rates (Re) of 5110 μmol g−1 h−1 and 12
383 μmol g−1 h−1 for CO2 reduction under simulated and natural sunlight, respectively, outperforming previous systems. In situ transient studies demonstrate that the photogenerated electrons of MA2SnBr6 diffuse from the conduction band to trap states, reducing CO2, while synergistically photogenerated holes oxidize biomass-derived alcohols. Additionally, in situ EPR experiments were performed to unravel mechanistic insights. Computational studies identify the Br p-orbitals of MA2SnBr6 as the reaction centre for CO2 reduction. Consequently, this work introduces a lead-free, single-component material that operates without a co-catalyst, sacrificial agent or redox additive, offering a promising path towards achieving photoredox processes in a more sustainable and efficient manner.
Broader contextThe most challenging aspect and bottleneck in photocatalysis is the effective employment of charge carriers in the most sustainable manner for synergistic reduction and oxidation processes while achieving a robust catalyst without the use of co-catalysts, sacrificial agents, or redox additives. Particularly, in tackling excessive CO2 emissions, solar energy provides a sustainable route to transform CO2 into fuels, achieving carbon neutrality. Photocatalytic CO2 reduction in synergism with biomass valorization under sunlight offers a highly effective approach towards “Photo-biorefinery.” This study also breaks the perception of the instability of halide perovskites for photocatalytic organic transformation and photoredox reactions. Halide perovskites are widely explored for CO2-to-CO conversion; however, deep-reduced fuels, such as CH4, still face a challenge with perovskites. This study not only presents the facile mechanochemical synthesis of novel lead-free hybrid halide perovskites in MA2SnBr6 QDs, but also addresses the limitation of conventional halide perovskites—particularly their instability, toxicity, low efficiency, and poor reusability. Eventually, the single-component perovskite achieved record-high production of CO and CH4 under natural sunlight, even without any co-catalyst or sacrificial agent—outperforming the existing halide perovskite photocatalysts. These findings uniquely couple the production of fine chemicals, such as vanillin, veratraldehyde, and 2-phenoxy-1-phenylethanone, with the generation of solar CO and CH4 fuels, thus achieving a “photo-chemical circular economy.” |
Halide perovskites have emerged as promising advanced materials,5 which find increasing applications in catalysis.6 Their remarkable properties such as high absorption coefficient, exceptional charge carrier mobility, long diffusion length, highly crystalline structure and low binding energy of excitons, as well as tuning of band gap by changing the halide, established them as highly essential materials, opening new opportunities in catalysis.7 Despite significant achievements in halide perovskite-based materials, still advancements have to be made to maintain their stability and non-toxicity, thereby enhancing their broad applicability.7,8 To achieve this, a major focus is on replacing the A cation in the ABX3 structure of perovskites. The scientific focus was also shifted majorly towards the replacement of the B cation,9 which stands for Pb in many of the previously reported works as Pb-based perovskites are toxic for our precious nature. Therefore, the development of lead-free halide perovskites without compromising their properties and efficiency is of prime importance. In this regard, we turned our interest to focus on the preparation of lead-free perovskite materials and their applications.
In our current work, we aimed to address four major challenges of the perovskite's domain, namely stability, reusability, toxicity, and efficiency of hybrid halide perovskites (HHPs).10 To tackle these issues, we synthesized a vacancy-ordered HHP, specifically MA2SnBr6 QDs, which had not been explicitly synthesized so far. MA2SnBr6 was synthesized via a greener approach, a simple yet effective solvent-free mechanochemical synthesis at room temperature without the use of additional capping agents. Interestingly, the synthesized MA2SnBr6 QDs maintained structural integrity in air and moisture, addressing a common issue with HHPs. To our surprise, these QDs are also stable in polar solvents such as isopropanol, ethanol, and acetonitrile, overcoming a major challenge typically encountered with halide perovskites. Remarkably, the significance of QDs is now widely recognized, as emphasized by the 2023 Nobel Prize in Chemistry awarded for the discovery and synthesis of QDs, highlighting their wide-ranging applications. Inspired by this notable achievement, the potential use of the synthesized air and moisture-resistant MA2SnBr6 QDs has been investigated for the photocatalytic conversion of renewable resources, including carbon dioxide and biomass-derived compounds, under sunlight, mimicking the process of artificial photosynthesis.
Therefore, for performing artificial photosynthesis, MA2SnBr6 QDs were applied for the simultaneous photocatalytic reduction of CO2 into CO and CH4 and oxidation of biomass-based alcohols and lignin model compounds to carbonyl compounds under natural sunlight. In this context, halide perovskites have been considerably explored for photocatalytic CO2 reduction;11 however, the majority of these relied on Pb-based perovskites,12–36 which are not compatible with the sustainability goals of carbon capture, utilization, and fixation.11 Further, previous studies employed co-catalyst-loaded perovskites,12,13,19,29 ternary systems,23,25,32,37 and complex heterojunctions37–43 to increase the photocatalytic activity, yet not succeeded in a promising manner. Moreover, the complex synthesis procedure of these photocatalytic systems makes them economically non-viable, thereby limiting their potential for large-scale process. Additionally, the full potential of halide perovskites has not been realized because they were not employed for the simultaneous photo-reduction of CO2 and photo-oxidation of biomass-based feedstocks. Thus, during the photo-reduction of CO2, the unutilized photogenerated holes are employed for oxidation reactions. In response, MA2SnBr6 QDs serves as Pb-free, single-component systems offering a synergistic way for utilizing photogenerated electrons for CO2 reduction to CO and CH4, while performing the conversion of biomass-derived compounds using photogenerated holes. Thus a sustainable pathway has been adapted without loading any co-catalyst and even without any sacrificial agent.
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| Scheme 1 Schematic of (a) the synthesis route followed for MA2SnBr6 QDs, and (b) MA2SnBr6 perovskite QDs applied for photocatalytic CO2 reduction coupled with oxidation of biomass-derived compounds. | ||
The MA2SnBr6 QDs were kept under ambient conditions and PXRD was conducted after one year, where no change was observed in the PXRD pattern of MA2SnBr6, demonstrating the retention of the MA2SnBr6 crystalline structure even after one year (Fig. 1a). The diffuse reflectance UV-vis (DR UV-vis) spectrum of MA2SnBr6 is presented in Fig. 1b, revealing an absorbance onset at 462 nm, and the corresponding Tauc plot indicates a band gap of 2.80 eV (Fig. 1c). To investigate the surface characteristics, initially, a survey scan of MA2SnBr6 was recorded by X-ray photoelectron spectroscopy (XPS). The survey scan showed the presence of C, N, Sn, and Br elements in the perovskite sample with elemental atomic compositions of 25.9%, 13.7%, 11.4%, and 49.0%, respectively (Fig. S2a), confirming the Br-enriched surface in the synthesized MA2SnBr6 material. The high-resolution XPS (HR-XPS) of Sn 3d was recorded, which showed two peaks at binding energies of 487.3 and 495.8 eV corresponding to Sn 3d5/2 and Sn 3d3/2, respectively (Fig. 1d). These peaks confirmed the presence of Sn in the +4 oxidation state. The HR-XPS of Br 3d was deconvoluted into two peaks centered at 69.0 eV and 70.2 eV attributed to binding energies of Br 3d5/2 and Br 3d3/2, respectively (Fig. S2b). Further, the HR-XPS of C 1s was deconvoluted into two peaks centered at 284.7 eV and 286.2 eV corresponding to the C–C/C–H and C–N binding energies, indicating the presence of methyl and methyl ammonium groups, respectively, in MA2SnBr6 (Fig. S2c). The C–N peak also appeared in the N 1s HR-XPS at 402.0 eV, further confirming the presence of methyl ammonium groups (Fig. S2d).
The chemical structure of MA2SnBr6 was also scrutinized by CP/MAS solid-state NMR spectroscopy, where the 119Sn NMR spectra showed a peak with a chemical shift at −1970 ppm (Fig. 1e), indicating the presence of single sites of the Sn atom. Then, 79Br NMR was also recorded to see the bromine environment in MA2SnBr6. Notably, a single peak was observed at 66 ppm (Fig. 1f), stipulating the presence of one type of Br atoms, which are bonded to Sn in the perovskite structure. Next, the 13C NMR spectra showed a peak at a chemical shift of 33.2 ppm (Fig. S3a) which corresponded to the –CH3 group present in the MA2SnBr6 perovskite. In the 15N NMR spectra, the peak observed at 31.7 ppm (Fig. S3b) was attributed to the ammonium group present in MA2SnBr6. Subsequently, the chemical structure of MA2SnBr6 was characterized by ATR-FTIR spectroscopy (Fig. S4), where the stretching frequency at 900 cm−1 was attributed to the rocking vibration of CH3NH3+, the stretching at 1473 cm−1 corresponded to C–H bending, the peak at 1574 cm−1 was assigned to the N–H bending vibration, the peak at 3180 cm−1 was assigned to the N–H asymmetric stretching vibration, and the peak at 543 cm−1 was assigned to the Sn–Br stretching vibration. The Raman spectral analysis was performed to study the vibrational properties of MA2SnBr6, where the Br–Sn–Br asymmetric bending deformation was observed at δ(F2g) = 119.5 cm−1, Sn–Br asymmetric stretching was observed at v(Eg) = 140.7 cm−1 and Sn–Br symmetric stretching was noticed at 185.8 cm−1 (Fig. S5).
In the microscopy study, the FESEM images were acquired to examine the morphology of MA2SnBr6, revealing a particle-like structure (Fig. 2a). To gain a clear insight, transmission electron microscopy (TEM) was performed, unveiling clusters of small particles for the MA2SnBr6 perovskite (Fig. 2b). The high-resolution TEM (HR-TEM) image provided a detailed picture, where it was found that the MA2SnBr6 perovskites were actually QDs. Further analysis of HR-TEM provided d-spacing values of 0.36 nm and 0.28 nm corresponding to the (311) and (040) planes, respectively (Fig. 2d). Additionally, the TEM analysis showed that these QDs have a size range of 3–4.6 nm with an average particle size of 3.8 ± 0.3 nm (Fig. 2f), and the inset of Fig. 2f presents the particle size distribution of MA2SnBr6 QDs. To assess the long-term stability of MA2SnBr6, TEM and HRTEM images of the same sample stored under ambient conditions for one year were recorded (Fig. 2c and 2e), and its morphology and dispersity with as-synthesized MA2SnBr6 were compared. The TEM image of MA2SnBr6 (after one year) shows clusters of small particles (Fig. 2c), and the HR-TEM images reveal agglomerated QDs for MA2SnBr6 (Fig. 2e) with an average particle size of 3.7 ± 0.3 nm comparable to that of the freshly synthesized material. Additionally, the measured lattice fringes exhibited a d-spacing value of 0.36 nm corresponding to the (311) plane and 0.28 nm representing the (040) plane (Fig. 2e). Hence, the morphology, dispersity, and crystallinity of MA2SnBr6 remained well-preserved even after one year of exposure to air and moisture. The observations, supported by PXRD, TEM, and HRTEM analyses, collectively demonstrated the excellent long-term stability of the MA2SnBr6 perovskite.
Further, the thermogravimetric analysis (TGA) indicates that MA2SnBr6 exhibits good thermal stability up to 230 °C, after which decomposition begins, attributed to the degradation of the methylammonium group in MA2SnBr6 (Fig. S6a). Next, MA2SnBr6 was dissolved in different polar solvents such as ethanol, isopropanol, acetonitrile, and ethyl acetate, and the collected samples were subjected to PXRD analysis (Fig. S6b). No changes were observed in the PXRD patterns, demonstrating the excellent chemical resilience of the MA2SnBr6 perovskite in polar solvents. Further, the electronic band structure of MA2SnBr6 was deduced from ultraviolet photoelectron spectroscopy (UPS) measurements (Fig. S6c), and the corresponding schematic of the band energy diagram is presented in Fig. S6d.
| Entry | Substrate | Product | Oxidation product | Reduction product | ||
|---|---|---|---|---|---|---|
| Conversion (μmol g−1 h−1) | Selectivity (%) | CO (μmol g−1 h−1) | CH4 (μmol g−1 h−1) | |||
| a Reaction conditions: 5 mg photocatalyst, 5 mL ethyl acetate, 0.05 mmol substrate, CO2 atmosphere, simulated light: 100 mW cm−2, time = 24 h, and temperature = 25 °C; the yield of products was determined by GC and GC-MS analyses. | ||||||
| (1) |
|
|
253 | >99 | 483 | 518 |
| (2) |
|
|
354 | >99 | 779 | 48 |
| (3) |
|
|
63 | >99 | 340 | 64 |
| (4) |
|
|
416 | >99 | 597 | 66 |
| (5) |
|
|
34 | >99 | 539 | 0 |
| (6) |
|
|
117 | >99 | 119 | 238 |
| (7) |
|
|
225 | >99 | 562 | 303 |
| (8) |
|
|
250 | >99 | 275 | 485 |
Here, the synergistic CO2 reduction with biomass-derived alcohol oxidation shows marked differences in product selectivity. These differences can be explained by considering the structural and electronic properties of alcohol substrates, such as resonance (R) and inductive (I) effects. p-Methoxybenzyl alcohol (entry 1) shows nearly equal production of CO and CH4, attributed to the strong +R effect of the methoxy group, which increases the electron density on the benzylic carbon and promotes efficient oxidation, releasing sufficient electrons and protons for CO and CH4 production. A similar trend is observed in the case of p-methylbenzyl alcohol (entry 8), where the +I and hyperconjugative effects of the methyl group promote CH4 production. In contrast, significant CH4 production occurred in the case of p-chlorobenzyl alcohol (entry 7) despite the −I effect of the chloro group, possibly due to its moderate +R effect, which causes partial retention of electron density on the benzylic carbon. Further, benzyl alcohol (entry 6), where no substituent group is present, has higher CH4 formation than CO, indicating favorable proton and electron availability without any significant steric or electronic effect. Substrates such as 2-phenoxy-1-phenyl ethanol (entry 2) and veratryl alcohol (entry 4) exhibit higher CO selectivity, probably due to steric hindrance from bulky substituents and electron delocalization across the aromatic system, which can slow down the rate of oxidation and limit proton release, restricting CO2-to-CH4 conversion. Next, vanillyl alcohol (entry 3) possesses –OH and –OCH3 groups, which make the benzene ring electron-rich and stabilize the radical on the ring itself, diverting oxidation from benzylic position. Moreover, vanillyl alcohol undergoes intramolecular hydrogen bonding, which may hinder the substrate-catalyst interaction, thereby limiting oxidation and making fewer protons available for CH4 production. Notably, in the case of furfuryl alcohol (entry 5), only CO was produced, consistent with the electron-deficient furan ring, exhibiting −I and weak +R effects, which result in poor oxidation efficiency and minimal proton generation. Further, aliphatic alcohols, which are difficult to oxidize, provided corresponding aldehydes and esters in reasonably lower yields (entries 1 and 2, Table S1). In addition, the oxidation of benzylamine resulted in N-benzylidenebenzylamine in quantitative yields (entry 3, Table S1).
Next, the photoluminescence (PL) study of MA2SnBr6 was carried out at an excitation wavelength (λex) of 350 nm (Fig. 3c). A broad PL spectrum was observed, having a peak maximum of around 440 nm, which could be assigned to trap states. On subsequent addition of pMBA into MA2SnBr6, the PL emission intensity significantly decreased, which infers the participation of charge carriers in the oxidation of pMBA. Fig. 3d shows the time-resolved PL (TRPL) decay profile of MA2SnBr6, which reveals an average charge carrier lifetime of 4.5 ns. Upon the addition of the pMBA substrate, the decay dynamics significantly slowed down, resulting in an increased lifetime to 5.1 ns. The possible reason for this observation is the oxidation of pMBA, which is assisted by photogenerated holes, indicating that pMBA functions as an effective hole scavenger. The delayed dynamics suggest the active participation of photogenerated holes in the oxidation process, where they react with pMBA present in the system, facilitating its oxidation and leading to an increased average lifetime of charge carriers.
The excited-state dynamics of any catalyst significantly influences its photocatalytic activity.46,47 Hence, in order to delve deeper into the excited charge carrier dynamics of MA2SnBr6, we performed ultrafast transient absorption (TA) studies after 400 nm pump excitation. Fig. 4a shows the TA spectra of bare MA2SnBr6 upon 400 nm pump excitation, scanning in the spectral range from 420 nm to 650 nm at different pump–probe delay time scales. The pump fluence of 400 μJ cm−2 was used at which the possibility of auger recombination is negligible (as discussed in SI). The TA spectrum of MA2SnBr6 exhibits a positive absorption band spanning across the entire visible region, which peaked at 450 nm. This positive signal can be attributed to the excited state's absorption (ESA) of trapped charge carriers.48,49 Earlier, O. M. Bakr and co-workers similarly observed a positive band in the visible region upon 380 nm excitation for other lead-free perovskites, CsMnBr3.50 It is intriguing to see that no transient bleaching is observed here, which is possibly due to the presence of a large number of defects in MA2SnBr6.48 Keli Han and co-workers also observed a positive signal for the hydrothermally synthesized lead-free inorganic perovskite (Rb0.75Cs0.25)3InCl6 and attributed this signal to photoinduced absorption from trap states.51
Further, we probed the TA kinetics of pristine MA2SnBr6 at a band maxima position of ∼450 nm (Fig. 4b) to investigate the charge carrier dynamics. The rise time of the signal was found to be 0.3 ps (Table S2), which suggests that there is almost no potential barrier for the trapping of the charge carriers.51 Further, the recovery dynamics were fitted with a bi-exponential function, obtaining two decay components (Table S2): an ultrafast time-scale component τ1 of 5.8 ps and a long lifetime component τ2 >1 ns. Here, the fast recovery component (τ2 = 5.8 ps) can be assigned to the surface defect trapping or cooling of hot self-trapped excitons in MA2SnBr6.48 The long-timescale component (τ2 >1 ns) is ascribed to the charge carrier recombination. Further, we conducted quenching experiments with electron and hole quenchers to determine whether the transient signal originated due to trapped holes or electrons. Fig. 4b and c show the comparative kinetics of bare perovskites before and after adding electron and hole quenchers, respectively. The signal intensity decreased (Fig. S20) in the presence of the electron scavenger, and faster decay dynamics were observed (Fig. 4b). The first recovery component τ1 decreased from 5.8 ps to 4.1 ps after adding the electron scavenger. Photogenerated electrons are scavenged by electron scavengers, leaving fewer electrons to recombine with the holes. Hence, the decrease in the transient signal intensity and faster recovery suggested that the signal corresponds to the trapped electrons. Thus, the transient signal in bare MA2SnBr6 can be easily assigned to ESA from trap states presented near the conduction band edge. However, in the presence of a hole-trapping agent, the decay dynamics became drastically slow (Fig. 4c), which validated the findings of the electron quenching experiment. The hole quencher scavenges the holes, leaving more electrons than holes. Hence, the slower decay observed further confirmed that electrons have a major contribution in the transient absorption signal of MA2SnBr6.
Next, we performed in situ transient studies in the presence of CO2 to examine its reactivity with photo-generated charge carriers in the bare MA2SnBr6 perovskite. Fig. 4d shows the comparative dynamics of bare MA2SnBr6 in the absence and presence of CO2. The decay dynamics becomes faster in the presence of CO2 than in the bare MA2SnBr6 perovskite. The first recovery component τ1 decreased from 5.8 ps in bare MA2SnBr6 to 4.9 ps in the presence of CO2. As explained earlier, the transient signal observed is due to the ESA of trapped electrons. Hence, the faster decay dynamics confirmed the active participation of MA2SnBr6 electrons in the CO2 reduction process,52 as schematically illustrated in Fig. 4f. In addition to that, we conducted ultrafast studies in the presence of pMBA to investigate the mechanism behind its oxidation. Fig. 4e represents the transient dynamics in the presence of pMBA. The slower dynamics was observed in the presence of alcohol substrates. The faster component (τ1) increased from 5.8 ps to 8.8 ps in the presence of pMBA. This delay in recovery suggests that holes are reacting with pMBA present in the system, eventually helping in the formation of pMBAL. Fig. 4f illustrates the photophysical mechanism responsible for the CO2 reduction and pMBA oxidation. The 3.1 eV pump generates the electrons and holes within the conduction and valence bands, respectively. The conduction band electrons diffuse to trap states, which react with CO2 molecules, producing CO and CH4. Conversely, the photogenerated holes react with biomass-derived pMBA to produce pMBAL.
The topographical image of MA2SnBr6 obtained via atomic force microscopy (AFM) is shown in Fig. S21, and its corresponding height profile reveals a thickness of 170 nm. Kelvin probe force microscopy (KPFM) was performed under dark and light conditions to analyze changes in the surface potential (Fig. 5a and c). In the dark, MA2SnBr6 delivers a contact potential difference (CPD) of 350 mV, which increased to 391 mV under illumination (Fig. 5b and d). The surface potential voltage (SPV) is defined as the change in the surface potential in the dark and under light irradiation (SPV = CPDlight – CPDdark), and is related to the photogenerated charge separation. The observed positive increment in CPD after irradiation of light (ΔCPD = 41 mV) suggests a more significant accumulation of photogenerated holes over the MA2SnBr6 surface than in the dark, enhancing exciton separation and improving the photocatalytic activity.53 To delve deeper into the mechanistic insights, the CO2 temperature-programmed desorption (CO2-TPD) analysis was performed to observe the adsorption behavior of CO2 over MA2SnBr6 (Fig. S22). The strong desorption peak observed between 180 and 190 °C indicates chemisorbed CO2 molecules over the surface of MA2SnBr6.
Density functional theory calculations were conducted to optimize the photocatalyst design by simulating the reaction energetics of the CO2 reduction reaction, as shown in Fig. 6d. The optimized structures of the catalyst MA2SnBr6 and various intermediates involved in the reaction pathway are displayed in Fig. 6e, and the plausible mechanism for CO2 reduction on the MA2SnBr6 surface is presented in Fig. 6f. Typically, the photocatalytic CO2 to CO or CH4 reduction steps include the first proton-coupled electron transfer to generate a carboxyl intermediate (*COOH), and subsequently, the second charge transfer (one electron and one proton) for the formation of *CO intermediate as well as the desorption of CO for the final CO product (Fig. 6f, path-1). For CO2 to CH4, the reaction proceeds through path-2: CO2→ COOH*→ CO* → CHO* → CH2O* → CH3O* → CH4. Note that the adsorption energy value is scaled down to 0 eV here to track the energy changes in subsequent steps precisely. The formation of the COOH* intermediate is uphill by 0.18 eV. However, the transformation of COOH* to *CO is slightly downhill in energy by 0.13 eV. The formation of *COOH and its conversion to *CO are critical intermediates that determine the thermodynamics of the reaction pathway. At this stage, two competing possibilities arise: (1) desorption of CO as the final product or (2) the further reduction of *CO to form *CHO, leading to the formation of CH4. DFT calculations reveal that the desorption of CO from the catalytic surface requires an energy input of 0.49 eV, making this step thermodynamically feasible under appropriate reaction conditions. However, the formation of the *CHO intermediate is energetically downhill by −0.38 eV, favoring the progression towards CH4 formation. This downhill energy profile for *CHO formation indicates that, given sufficient energy, the catalyst can selectively drive the reduction pathway toward methane instead of terminating at carbon monoxide.
Despite the thermodynamic feasibility of both pathways, the rate-determining step (RDS) in the CO2 reduction process is the desorption of CO, which requires an energy input of 0.49 eV. This RDS acts as a bottleneck for CO formation, potentially limiting the efficiency of the CO2 reduction when CO is the desired product. However, the experimentally determined band gap of the photocatalyst is 2.8 eV, which is significantly higher than the energy required for CO desorption. Under light illumination, the catalyst generates sufficient photoexcitation energy to overcome the desorption barrier, ensuring that both CO desorption and subsequent *CHO formation become thermodynamically and kinetically favorable. This observation highlights the dual capability of the photocatalyst to selectively produce either CO or CH4, depending on the operating conditions.54 The computational analysis and comparison with experimental findings confirm that the photocatalyst can facilitate both CO and CH4 production.
These insights underscore the importance of catalyst design in tuning the product selectivity for the photocatalytic CO2 reduction reaction. The detailed mechanistic study highlights the dual functionality of the MA2SnBr6 surface in facilitating both CO2-to-CO and CO2-to-CH4 conversions. The localized charge density on Br p-orbitals enhances the catalytic efficiency, and the system's band gap provides sufficient driving force for CO2-to-CO and CO2-to-CH4 conversion. These findings underline the potential of MA2SnBr6 as an efficient photocatalyst for CO2 reduction.
Furthermore, the photocatalytic activity of MA2SnBr6 for CO2 reduction was compared with previously reported perovskites, as shown in Fig. 7 and Table S3. It was observed that most of the prior studies utilized lead-based perovskites, predominantly complex perovskite heterojunctions, and yet suffered a low production rate of CO. Moreover, even after significant attempts, the photoreduction of CO2 to CH4 was still not promising as it is an 8 e− process and demands high energy as compared to the 2 e− reduction process of CO2 to CO. Therefore, addressing the challenge, MA2SnBr6 displayed a remarkable electron consumption rate (Re) of 5110 μmol g−1 h−1 under simulated light and 12
383 μmol g−1 h−1 under natural sunlight, significantly surpassing previously reported halide perovskite-based systems. Consequently, as a lead-free, single-component material, MA2SnBr6 not only achieves a superior CO2 reduction rate with a higher production rate of CO and CH4 but also simultaneously facilitates the photo-oxidation of biomass-derived compounds into value-added chemicals.
![]() | ||
| Fig. 7 Comparison of the electron consumption rate (Re) of previously reported halide perovskites. The referenced articles: ref. [S1–S44]. | ||
383 μmol g−1 h−1 under natural sunlight, significantly surpassing previously reported halide perovskite-based systems. Based on in situ transient absorption, in situ EPR experiments, and computational studies, the detailed mechanism is unravelled for this photo-redox reaction to valorise CO2 and biomass-based feedstocks. Consequently, as a lead-free, single-component material, without any co-catalyst and sacrificial agent, MA2SnBr6 not only achieves significantly higher yields of CO and CH4 but also synergistically facilitates the photo-oxidation of biomass-derived alcohols into valuable chemicals, making a significant contribution towards sustainable solar fuel generation and fine chemical production.
The adsorption-free energy (ΔG*) and adsorption energies of reactants and intermediates were calculated using the following equation:
| ΔG = ΔE + ΔEZPE − TΔS |
| ΔEabs = Eslab(/molecule) − (Eslab + Emolecule) |
:
1 stoichiometric ratio as a starting material and ground in a mortar and pestle. A yellow powder was obtained via this solvent-free and eco-friendly process. The MA2SnBr6 powder was then recrystallized in ethanol to produce MA2SnBr6 crystals.
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