1. Introduction
CO
2 is the highest oxidation state of carbon, which plays a key role in affecting the carbon cycle in nature. Photocatalytic CO
2 reduction into value-added hydrocarbon fuels including CH
4, CH
3OH, and C2 products, as well as CO, which is one of the most important resources for industrial carbonization and an efficient reducing reagent, is of great promise in clean energy conversion to solve the energy shortage crisis and severe environmental issues [
1,
2]. However, its C=O bonds are extremely stable thermodynamically for breaking, leading to low conversion efficiency and selectivity to the desired product. Various materials have been developed to improve photocatalytic CO
2 conversion efficiency, including metals, metal oxides, nitrides, sulfides, chalcogenides, organic polymers, and perovskite materials [
3,
4,
5,
6,
7,
8,
9,
10,
11]. Many of them have shown limits, such as high cost, lengthy and complex synthesis process, long-term instability, and low catalytic activity. Recently, perovskite materials have been widely considered as rising photocatalysts for photocatalysis due to a wide range of benefits over conventional semiconductors, including their diversity, suitable energy band alignment, rapid charge transfer, and excellent optical properties [
12,
13]. Among the various perovskite materials, halide perovskite has been invoked as an emerging class of semiconducting photocatalyst, due to its extraordinary properties like cost-effectiveness, easy synthesis process, visible light absorption, high CO
2 adsorption surface area, surface disorders for charge trapping, and tunable structure [
14,
15,
16,
17,
18]. However, due to the ionic properties of halide perovskite, these materials usually have poor stability. The structural features of perovskites experience swift degradation under different stress conditions such as moisture, UV light, oxygen, and high temperature, hindering their practical application in photocatalysis. Various approaches including the integration of multiple capping agents/stabilizers and encapsulation into porous materials have been developed to tackle this limit [
19,
20,
21,
22]. Moreover, quantum dots (QDs) refer to the particles with the uniform size distribution in the range of 2–10 nm, which have shown significantly improved performances over the bulk materials in catalysis, especially in solar energy conversion, due to the unique advantages including tunable and size-dependent electronic properties, extended light-harvesting region, and quantum confinement effect. However, the small particle size also leads to high energy of its surface atoms so that the aggregation of those QDs is inevitable.
In recent years, metal–organic frameworks (MOFs) have shown specific merits as the host to incorporate and stabilize perovskite materials owing to their unique properties including robust frameworks, high specific surface area, adjustable pore size and structure, and massive catalytic active sites [
23,
24,
25], rendering the resulting perovskite/MOF composites with improved stability and reduced perovskite particle sizes [
26,
27,
28]. Chang et al. reported the first example of incorporating MOF with perovskite to enhance the crystallinity of the perovskite in 2015 using a one-step deposition method [
29]. The perovskite crystals were formed both on the surface and inside the pores of the MOF. Early works about the perovskite/MOF composites in photocatalysis were reported in the late 2010s. Su and co-workers grew the zinc/cobalt-based imidazolate framework (ZIF) on the surface of CsPbBr
3 QDs, resulting in a largely enhanced moisture stability for up to 10 days [
30]. The CsPbBr
3@ZIF-67 composite could produce CO and CH
4 with yields of 2.301 µmol and 10.537 µmol g
–1, respectively, with an electron consumption rate (
Relectron) of 29.630 µmol g
–1 h
–1, while the pure CsPbBr
3 gave an
Relectron of 11.14 µmol g
–1 h
−1. The recycling test of CsPbBr
3@ZIF-67 was monitored for 18 h without significant decay. Later in 2019, Lu and co-workers reported the encapsulation of MAPbI
3 QDs in the pores of a Fe-porphyrin-based MOF of PCN-221(Fe
x) [
27]. The highest CO
2 photoreduction was detected for MAPbI
3@PCN-221(Fe
0.2), showing a high yield of 1559 µmol g
–1 in 80 h including 34% CO and 66% CH
4, and
Relectron of 129.0 µmol g
–1 h
−1. Zhong and co-workers prepared a CsPbBr
3 QDs/UiO-66(NH
2) nanojunction which could catalyze CO
2 conversion under visible light irradiation, giving the highest CO yield of 98.57 μmol g
−1 and CH
4 yield of 3.08 μmol g
−1 in 12 h, which is much higher than that of pure CsPbBr
3 QDs and UiO-66(NH
2) [
31]. Its
Relectron was 18.5 μmol g
−1 h
−1. More recently, Su and co-workers reported a ternary CsPbBr
3/Au/PCN-333(Al) hybrid, showing a 100% CO selectivity with a yield of 186.15 μmol g
−1 in a 3 h reaction [
32].
Relectron was calculated to be 124.1 μmol g
−1 h
−1. As listed, the conversion efficiency and the stability and reusability of photocatalytic CO
2 reduction catalyzed by perovskite/MOF composite is still relatively low. The research on the development of perovskite/MOF composite towards its application in CO
2 photoreduction is still at an early stage and needs epic improvement. In addition, the precise control of the perovskite location in the MOF host is still challenging with random occasions neither inside the pore nor on the surface, leading to low photocatalysis efficiency and product selectivity.
In this work, we report a facile in situ growth method to encapsulate the perovskite quantum dots (QDs) into the pores of MOFs. A series of xMAPbBr3@MIL-101(Cr) (MA = CH3NH3+, x = 8%, 9%, 11%, 14%) composites were prepared. The confined environment limits the growth of the perovskite QDs, resulting in an average size of 2–3 nm, which showed superiority for catalysis. The composites also display improved light harvesting, charge separation, and transfer, as well as enhanced lifetime of excited electrons. As a result, in photocatalytic CO2 reduction, 11%MAPbBr3@MIL-101(Cr) composite displayed an extraordinary performance with a total CO and CH4 yield of 875 μmol g−1 in 9 h, and impressive stability in an as long as 78 h test without structural and morphologic decomposition compared to that of the pure MAPbBr3. Moreover, we also reveal a novel mechanism for the photocatalytic CO2 reduction catalyzed by these perovskite@MOF composites that, through the precise control of the location and amount of the encapsulated perovskite QDs in the MOF pores, the product selectivity could be switched from a CO dominant mode in those with perovskites encapsulated in the mesopores of MIL-101(Cr) to a CH4 dominant one for those with perovskites encapsulated in both meso- and micropores.
2. Results and Discussion
MIL-101(Cr), constructed via the reaction between the Cr
3+ node and the terephthalate ligand, was chosen as the host MOF in this study owing to its robust property and massive meso- and micropores which are accessible for the perovskite precursors [
33,
34,
35,
36,
37]. The confined growth of the perovskite QDs could be protected by the MOF matrix from leaching and decomposition. As depicted in
Scheme 1, MAPbBr
3@MIL-101(Cr) composites were prepared using a two-step deposition strategy, during which the pristine species for the in situ nucleation of MAPbBr
3 QDs were sequentially introduced and self-assembled in the pores of MIL-101(Cr). By adjusting the usage of PbBr
2 and MABr, the MAPbBr
3 content in the composites could be tuned. For example, in the
xMAPbBr
3@MIL-101(Cr) (
x = 8%, 9%, 11%, 14%) composites, the percentage numbers represent the actual weight percent of MAPbBr
3 determined by inductively coupled plasma optical emission spectrometer (ICP-OES) analysis and calculated by Equation (S1), which are 8.29%, 9.02%, 11.17%, and 13.95%, respectively (
Table S1).
From the wide-angle PXRD patterns of MIL-101(Cr),
xMAPbBr
3@MIL-101(Cr), and MAPbBr
3 bulk composites in
Figure 1a, it is clear that the characteristic peaks of MIL-101(Cr) and MAPbBr
3 match well with the simulated patterns prepared from the crystal structures (CCDC 605510 and 1446529), indicating the good purity and crystallinity of the prepared samples. After the introduction of MAPbBr
3 QDs, the typical patterns of MIL-101(Cr) remain unchanged, suggesting the undisturbed integrity of the host MOF. In addition, the characteristic peaks of MAPbBr
3 QDs are not observed in all
xMAPbBr
3@MIL-101(Cr) composites, probably owing to the small sizes confined in the pores of MIL-101(Cr).
Figure 1b shows the small-angle (1~10°) XRD patterns of MIL-101(Cr) and
xMAPbBr
3@MIL-101(Cr) samples, in which the intense peaks demonstrate the mesoporous structure of these samples. The characteristic diffraction peaks of MIL-101(Cr) shift slightly to larger angles with increasing the MAPbBr
3 encapsulation content; while the peak intensity decreases. It is due to the influence of the occupation of QDs in the MOF pore to the crystal structures [
37]. These observations imply the encapsulation of MAPbBr
3 QDs in the mesopores of MIL-101(Cr) while keeping intact the high crystallinity of MIL-101 [
33,
34,
37].
Subsequently, the nitrogen adsorption–desorption isotherms and the pore size distribution of MIL-101(Cr) and
xMAPbBr
3@MIL-101(Cr) recorded at 77 K and 1 atm are shown in
Figure 2. The N
2 adsorption–desorption isotherms of
xMAPbBr
3@MIL-101(Cr) display type I and type IV isotherms with narrow H4 hysteresis loops similar to that of the pristine MIL-101(Cr), indicating the co-existence of micro- and mesopores in these samples (
Figure 2a). The BET-specific surface areas of MIL-101(Cr) and
xMAPbBr
3@MIL-101(Cr) (
x = 8%, 9%, 11%, 14%) composites calculated by Brunauer–Emmett–Teller equation are 2714.0, 1426.4, 1319.5, 975.5, and 936.8 m
2 g
−1, respectively. The total pore volume values of MIL-101(Cr) and
xMAPbBr
3@MIL-101(Cr) composites determined by using the adsorption branch of N
2 adsorption–desorption isotherm at P/P
0 = 0.95 are 1.28, 0.72, 0.63, 0.49, and 0.47 cm
3 g
−1, respectively. The results indicate that upon the encapsulation of MAPbBr
3 QDs, both the N
2 uptake capacity and the total pore volume decreased largely with increasing the perovskite content, but a saturation phenomenon occurred after 14% MAPbBr
3 QDs were encapsulated in MIL-101(Cr), which gave about 65% and 63% decreases for the specific surface area and total pore volume, respectively. Moreover, it could be observed from the corresponding micro- and mesopore volumes in
Table S2 that the major part of MAPbBr
3 QDs first fulfill the mesopores as the QDs contents increased to 9% to reach a maximum and then started to occupy the micropores as the QDs content further increased to 14% with a satisfactory encapsulation. The CO
2 adsorption isotherms of these samples in
Figure S1 also show a decreasing trend upon increasing the content of perovskite QDs in the MIL-101(Cr) pores that are consistent with the N
2 adsorption results, confirming the location of the QDs.
The encapsulation of MAPbBr
3 QDs inside the MIL-101(Cr) pores was further evidenced by IR spectra. As compared with the spectrum for MIL-101(Cr), the new peaks around 1257 nm
−1 appeared for all halide perovskite-based samples, which can be assigned to the CH
3-NH
3+ rock vibration (
Figure S2) [
38]. These results demonstrate that the targeted
xMAPbBr
3@MIL-101(Cr) composite system has been successfully constructed.
11%MAPbBr
3@MIL-101(Cr) was chosen as a typical sample to evaluate the influence of encapsulating perovskite QDs into the MOF pores on the microstructure and morphology based on the following reactivity study, showing the best photocatalytic CO
2 reduction activity and stability. SEM and TEM images of the pristine MIL-101(Cr) show a classical octahedral morphology with smooth surfaces and a diameter of ca. 700 nm, consistent with the previous reports [
33,
34]. After encapsulation, the well-maintained octahedron indicates structural integrity (
Figure 3a). No obvious particles could be detected either on the surfaces or inside the octahedron, probably due to the short detection time since MIL-101 is highly sensitive to the electron beam which would cause the collapse of the structure. The HAADF-STEM image clearly shows white bright spots evenly distributed in octahedral particles with an average particle size of about 2–3 nm, which matches the mesoporous pore sizes (29 Å and 34 Å) of MIL-101(Cr) (
Figure 3b) [
37]. In addition, the elemental mapping images of 11%MAPbBr
3@MIL-101(Cr) show that Br, Pb, N, C, and Cr elements are evenly distributed (
Figure 3c–h). These results confirmed the successful encapsulation of MAPbBr
3 QDs inside the pores of MIL-101(Cr).
X-ray photoelectron spectroscopy (XPS) analysis was employed to investigate the surface properties of the composite and the interfacial interaction between MIL-101(Cr) and MAPbBr
3 QDs. The total survey spectra of the samples in
Figure 4a demonstrate the coexistence of Pb, Br, and N elements in all materials. The high-resolution Br 3d XPS spectra are shown in
Figure 4b. The curves for the pure MAPbBr
3 QDs could be deconvoluted into two separated peaks centered at 69.0 and 67.9 eV for the Br 3d
5/2 and 3d
3/2 hybrid orbits, respectively. Positive shifts to higher binding energies of 69.2 and 68.1 eV, respectively, could be found for 9%MAPbBr
3@MIL-101(Cr), which are further shifted to 69.3 eV and 68.2 eV, respectively, for those in 11%MAPbBr
3@MIL-101(Cr). In the Pb 4f XPS spectra of MAPbBr
3 QDs, 9% and 11%MAPbBr
3@MIL-101(Cr) (
Figure 4c), the peaks located at 143.0 and 138.1 eV could be attributed to the binding energies of Pb 4f5/2 and Pb 4f7/2 in the pure MAPbBr
3 QDs, which also shifts to higher bind energies of 143.5 eV and 138.5 eV for 9%MAPbBr
3@MIL-101(Cr) and 143.7 eV and 138.7 eV for 11%MAPbBr
3@MIL-101(Cr), respectively. Meanwhile, a contrary shift to lower binding energies of 0.1 and 0.3 eV could be observed in the Cr 2p
1/2 and 2p
2/3 XPS spectra of the 9% and 11%MAPbBr
3@MIL-101(Cr) samples, respectively, in comparison with those of the pure MIL-101(Cr) sample (
Figure 4d). These XPS results confirm the positive shifts of the Br 3d and Pb 4f binding energies, as well as the negative shift of the Cr 2p upon incorporation of MIL-101(Cr) and MAPbBr
3 QDs compared to the single phase. The systematic shifts vary with the gradual increase of MAPbBr
3 QDs contents in the composites. Therefore, the increased electron cloud density of Cr and reduced electron cloud density of Pb and Br in MAPbBr
3 recommend an electron transfer pathway from Br
− to Cr
3+, leading to the strong coordination between Cr
3+ and Br
- ions and subsequent interaction between MAPbBr
3 and chromium oxide SBU of MIL-101(Cr).
The photocatalytic CO
2 reduction performances of the samples were evaluated subsequently via a gaseous reaction mode by placing the photocatalysts in a sealed Pyrex bottle. This kind of gas–solid reaction system could greatly avoid the leaching issue of the toxic Pb and Cr elements to the environment and the competition reaction of water splitting to produce H
2. The reactor was vacuumed to remove any air inside and filled with CO
2 and a tiny amount of H
2O (10 μL), which would provide vapor under light irradiation. Such a gas–solid reaction system is useful to prohibit the product from the comparative water-splitting reaction [
37].
Figure 5a shows the photocatalytic reduction ability of MAPbBr
3 and
xMAPbBr
3@MIL-101(Cr) in a 9 h reaction, which has been normalized by the content of reactive sites, i.e., the actual halide perovskite content for the composites and the weight for neat MIL-101(Cr). For all samples, the photocatalytic CO
2 reduction products were CO and CH
4. Neither H
2 nor other liquid products including CH
3OH and HCOOH could be detected. Control experiments using N
2 to replace CO
2 gas under the same condition revealed no product. As depicted in
Figure 5a, pure MIL-101(Cr) cannot serve as a photocatalyst in CO
2 reduction with merely no reactivity, while for pure MAPbBr
3, the total production of CO and CH
4 was 107 μmol g
−1. These results indicated that both single-phase samples were inefficient photocatalysts. However, after incorporation, the photocatalytic activity increased significantly even with a small encapsulation amount of MAPbBr
3, i.e., 5% (144 μmol g
−1), as compared with that of MIL-101(Cr). The total gas yields and the CH
4 selectivity increase with increasing halide perovskite contents in
xMAPbBr
3@MIL-101(Cr). The
xMAPbBr
3@MIL-101(Cr) composites (x = 8%, 9%, 11%, and 14%) displayed a total production of CO and CH
4 6–8 times higher than that of pure MAPbBr
3, among which 11%MAPbBr
3@MIL-101(Cr) obtained the highest total yield of 875 μmol g
−1 in 9 h with the CO and CH
4 formation rates of 16.9 and 80.3 μmol g
−1 h
−1, respectively. Notably, CO dominates in the product when the perovskite contents in the composites are less than 11%; while those with perovskite contents above 11% are more preferential for CH
4 production. Interestingly, the selectivity switch happens when the amount and the location of the encapsulated at the number of 11%, which has been demonstrated to include the perovskite QDs in both meso- and micropores of MIL-101(Cr) by N
2 adsorption–desorption and XPS analysis results. In the CO
2 photoreduction of 11%MAPbBr
3@MIL-101(Cr), the CH
4 selectivity is 82.6%, which is a little bit higher than 75.7% for that of pure MAPbBr
3 and much higher than 9.0% for the 5%MAPbBr
3@MIL-101(Cr). Moreover, the surface area of the material normally plays a critical role in catalysis, displaying a positive correlation with the catalysis efficiency. However, in our case, MIL-101(Cr) is inactive although it has the highest surface area. Incorporation with MAPbBr
3 would make the surface area of MIL-101(Cr) less, but the catalytic efficiency of the composites increased a lot. In addition, as for the
xMAPbBr
3@MIL-101(Cr) composites, the surface areas were systematically decreased when increasing the number
x, although their photocatalytic activities showed a volcano-type relationship with the highest CO
2 conversion at the number of 11%.
The electron consumption rate (
Relectron) calculated by Formula (S2) is normally utilized to compare the efficiency in photocatalytic CO
2 reduction. As shown in
Figure S3, 11%MAPbBr
3@MIL-101(Cr) obtained the highest
Relectron value of 676.4 μmol g
−1 h
−1, which is 8.6 and 17-fold higher than the pure MAPbBr
3 (77.8 μmol g
−1 h
−1) and 5%MAPbBr
3@MIL-101(Cr) (40 μmol g
−1 h
−1), respectively. The enhancement of
Relectron is higher than the total gas yield enhancement (8-fold) due to the largely enhanced selectivity toward CH
4, which normally requires 8H
+/8e
- to proceed and should be much harder than the generation of CO thermodynamically. Interestingly, although pure perovskite is more preferential to CH
4 production, the encapsulated composites clearly display a selectivity shift from CO to CH
4 at the dividing point of 9% encapsulation of perovskite, from which the encapsulated perovskite sufficiently occupies the mesopores and start to enter the micropores of MIL-101(Cr), according to the analysis of the N
2 adsorption–desorption isotherms and the pore size distribution.
With an extended reaction time of 27 h, the
xMAPbBr
3@MIL-101(Cr) photocatalyst not only shows well-maintained catalytic activity but also demonstrates high selectivity for CH
4 (
Figure 5b). However, the CH
4 yield decreased slightly, leading to a decrease in the electron consumption rate. In addition, no photosensitizer or sacrificial agent is added to the reaction system, which brings a breakthrough and possibility for the practical application of CO
2 photoreduction. To the best of our knowledge, this result is among the highest values for CO
2 conversion and electron consumption rate of CO
2 photoreduction catalyzed by perovskite-based photocatalytic materials under similar reaction conditions reported so far (
Table S3).
Further, by increasing the reaction time to 78 h, the CO production increased linearly with a relatively consistent rate of 16.9 μmol g
−1 h
−1, while the CH
4 production rate decreased continuously, as shown in the gas yield versus time curves (
Figure S4). The catalyst collected after photocatalysis was characterized by XRD and SEM, showing well-maintained crystallinity and octahedral morphology (
Figure S5). In addition, such a long runtime with impressive stability is rare in the reported studies of perovskite-involved photocatalysis, probably due to the use of MIL-101(Cr) as the host, which could not only confine the self-growth of the perovskite QDs but also serves as a physical barrier to protect the perovskite under photocatalysis conditions.
To further explore the reason for the remarkably enhanced photocatalytic performance, the negative effect of the surface areas on the catalytic activity, and the switched product selectivity of
xMAPbBr
3@MIL-101(Cr) composites in the CO
2 photoreduction, their light-harvesting ability, energy band structure, electron-charge separation, and transfer efficiency were studied and compared.
Figure 6a shows the light absorption behaviors of
xMAPbBr
3@MIL-101(Cr), MIL-101(Cr), and MAPbBr
3 via UV−vis absorption spectroscopy. The absorption band edge is located at ~550 nm in the UV spectrum of MAPbBr
3 QDs, corresponding to an energy band (
Eg) of 2.25 eV, which is similar to the reported value [
39]. The
xMAPbBr
3@MIL-101(Cr) exhibits similar light-absorption behaviors as compared to the pristine MIL-101(Cr) with strong absorption in the range of 200–400 nm. A slight, but systematic enhancement of the absorption at ~540 nm was observed with increasing MAPbBr
3 contents, probably due to the small ratio of encapsulated perovskite QDs inside the pores of MIL-101(Cr). This result suggests that the photoelectrons in
xMAPbBr
3@MIL-101(Cr) could be easily excited upon visible light irradiation, which benefits the utilization of solar energy. The bandgaps (
Eg) of MIL-101(Cr) and MAPbBr
3 are estimated to be 3.63 and 2.2 eV from the Tauc plots, respectively (
Figure S6a,b); while those for the composites are between 3.4 and 3.6 eV (
Figure S6c–f). Furthermore, the conduction band edge for MIL-101(Cr) and MAPbBr
3 obtained from the Mott–Schottky plots are −1.62 V and −1.00 V vs. NHE, respectively (
Figure S7a,b). Those positive slopes suggest the n-type semiconductor nature of the samples. These results indicate that the photoexcited electrons in MAPbBr
3 have enough driving force to reduce CO
2 to CO (−0.53 V vs. NHE) or CH
4 (−0.24 V vs. NHE) [
17,
19,
40,
41]. Moreover, steady-state PL spectra can also verify the electron transfer property by a much lower PL intensity of the 11%MAPbBr
3@MIL-101(Cr) nanocomposite as compared with MAPbBr
3 QDs (
Figure 6b), suggesting the promoted electron transfer between the single component and thereby improved charge separation of the photoinduced electron–hole pairs.
Time-resolved photoluminescence (TRPL) was conducted to reveal the acceleration of the electron separation and transfer. The decay plots fitted via a multiexponential function show a much longer lifetime of excited electrons for the 11% MAPbBr
3@MIL-101(Cr) (16.64 ns) than the bare MAPbBr
3 (3.35 ns) (
Figure 6c and
Table S2), indicating the greatly suppressed nonradiative recombination upon the encapsulation of MAPbBr
3 QDs inside the MOF pores. The enhanced carrier separation efficiency values of MIL-101(Cr), MAPbBr
3, and xMAPbBr
3@MIL-101(Cr) nanocomposites were further confirmed by other photoelectrochemical properties. The photocurrent density shows the generation of photocurrent upon switching the light-on and -off mode (
Figure 6d). The current densities of
xMAPbBr
3@MIL-101(Cr) nanocomposites are all much higher than MAPbBr
3 QDs and MIL-101(Cr) due to the high charge separation efficiency in those nanocomposites, which elucidates the interaction between MIL-101(Cr) and MAPbBr
3. Among the
xMAPbBr
3@MIL-101(Cr), 11%MAPbBr
3@MIL-101(Cr) reveals the highest photocurrent density. Similarly, electrochemical impedance spectra (EIS) also illustrate the fast kinetic charge transfer behavior of
xMAPbBr
3@MIL-101(Cr) upon illumination. The EIS Nyquist plots of all
xMAPbBr
3@MIL-101(Cr) show a much smaller semicircle arc at high frequencies than the two single components (
Figure 6e). In addition, the semicircle arc of 11%MAPbBr
3@MIL-101(Cr) in the EIS plots is not the smallest, but its slope of the linear line at low frequencies is the highest among all
xMAPbBr
3@MIL-101(Cr) composites, indicating the most efficient ion diffusion during the reactions. These results evidently reveal the efficient charge transfer between MAPbBr
3 QDs and MIL-101(Cr), which offers a brand-new opportunity for perovskite material in photo/optical-related applications.
A similar preparation method was also used for the synthesis of a series of
xMAPbI
3@MIL-101(Cr) composites (
x = 9%, 13%, 14%, and 15%, indicating the real weight percentage of MAPbI
3 in the composites). Their physical, morphological, optical, and electrochemical properties were also characterized (
Figures S8–15, Tables S1 and S2). In photocatalytic CO
2 reduction reactions, they were relatively inefficient as compared with those for
xMAPbBr
3@MIL-101(Cr) (
Figures S16–S18).
The band alignment of MAPbBr
3 and MIL-101(Cr) determined from the UV–vis spectra and Mott–Schottky plots is given in
Figure 7. The CB and VB of MaPbBr
3 are in between those for the MIL-101(Cr), suggesting a possible Type I junction formed at the interface of MAPbBr
3 and MIL-101(Cr), in which photogenerated electrons and holes should transfer from MIL-101(Cr) to MAPbBr
3. However, the XPS results reveal the electron transfer pathway from the perovskite to the Cr
3+ of the MOF, which is contrary to the Type I junction character. Therefore, electron paramagnetic resonance (EPR) recorded at 77 K was utilized to monitor the chemical state change of Cr under different conditions. As shown in
Figure 6f, a broad and intense signal at g = 1.98 confirmed the existence of a high-spin S = 3/2 Cr(III) species [
37,
42]. An obvious intensity decrease could be detected for the perovskite-encapsulated sample, probably due to the formation of the EPR silent Cr
2+ from the reduction of Cr
3+ species. Upon irradiation of 11%MAPbBr
3@MIL-101(Cr), the signal assigning to Cr
3+ further decreases, consistent with the electron transfer pathway to form Cr
2+.
In combination with the CO
2 photoreduction results that MIL-101(Cr) with a more negative CB band showed no activity, it could be deduced that the incorporation of the two components does not form a Type I heterojunction (
Figure 7). Electrons on the CB of MAPbBr
3 transfer to the SBU of MIL-101(Cr) first, where Cr
3+ could be reduced to Cr
2+ (
Ered = −0.55 V), and then to the adsorbed CO
2 molecular, leading to the CH
4 (
Ered = −0.24 V) and/or CO (
Ered = −0.53 V) production. On this condition, the SBUs of MOF serve as the functional catalytic sites, which could also unveil the interesting selectivity switch for those
xMAPbBr
3@MIL-101(Cr) composites. When the amount of encapsulated perovskite is less than 9%, their location is mainly in the mesopores of MIL-101(Cr). Upon illumination, the photogenerated electrons transferred from the perovskite QDs to the SBU of MIL-101(Cr) and then participated in CO
2 reduction. Under this condition, CO is the main product since it is dynamically more favorable compared to the formation of CH
4; both the CO
2 conversion and CH
4 selectivity increased with further increasing the encapsulated perovskite content. Up to an 11% encapsulation, the mesopores of MIL-101(Cr) were fully occupied by the QDs; the excess amount of these QDs started to enter the micropores of MIL-101(Cr), as shown in N
2 and CO
2 adsorption analysis results, leading to the lack of space for CO
2 adsorption and its contact with the catalytic active sites, i.e., SBU of MIL-101(Cr). In that case, the perovskite itself functions as the catalytic site for CO
2 photoreduction, revealing the high CH
4 selectivity comparable to that of the pure perovskite material.