Synthesis and structure of the catalysts: Two methods were used to integrate Cu into the ZIF-8 MOF: ion exchange (Fig. 1a, Fig. S1-S2) and conventional wet impregnation. To prepare the ion exchanged catalyst (Cu/ZIF-8|IE|), we introduced the ZIF-8 MOF in an ethanol solution of Cu(NO3)2. Then, the sample was washed in a Soxhlet with ethanol to remove the metal not strongly anchored to the MOF. In this way, we incorporated up to 12 wt.% of Cu in the MOF (Table 1). During ion exchange treatment, defects are generated in the MOF structure, and parts of linkers can be released.20 These missing linkers can be observed using infrared spectroscopy (Fig. 1d), where the broadband centered at 1311 cm−1 is observed because of linker deficiency. In the same figure, no peak between 1100 and 1150 cm−1 was observed, indicating metallic defects were not present. These missing linkers were replaced via hydroxyl groups, as can be seen by IR (broad band between 3250 and 3700 cm−1, Fig. S3). Note that Cu is anchored to these hydroxyl group ligands (Fig. 1a).
The samples were then subjected to reduction treatment at different temperatures to reduce Cu2+ to small Cu metallic clusters and characterized using XRD (Fig. 1b). The diffractograms do not change even when the sample was reduced at 723 K. This indicates that the sample was extremely stable under the reduction conditions. Only a small shift of the peaks is seen before reducing the sample, thus reinforcing the idea that Cu is incorporated into the structure after reduction treatment. Cu phases were not reported even after reduction at 723 K, which could be attributed to the fact that Cu particles are highly dispersed in the catalyst. However, the diffraction pattern of the sample prepared by wet impregnation Cu/ZIF-8|IM| (Fig. S4) shows that the MOF degrades during the impregnation process and that the structural detriment is even more accentuated when reduced at 523 K. Peaks belonging to crystalline Cu can be seen using the wet impregnation method. It is interesting to know that the structural arrangement of the prepared Cu/ZIF-8|IE|R catalyst did not change after being stored (in a glass vial) for more than three years, explaining its long shelf-life (Fig. S5).
Thermogravimetric studies then demonstrated the high stability of these materials (Fig. S6). Nitrogen adsorption isotherms (Fig. 1c) of the catalysts demonstrated that the exchange method developed in this study was essential for achieving the proper dispersion of Cu species in the ZIF-8 structure without considerably decreasing the specific surface area of the MOF. Synthesis of the same catalyst using the traditional impregnation method led to MOF degradation and a loss of all accessible porosity (no proper hysteresis is seen).22–25
Morphology of the catalysts: From the TEM analysis of ZIF-8 before and after Cu exchange and reduction (Fig. 2a, Fig. 2b, and Fig. S7), we could not detect Cu nanoparticles of sufficient size that could be differentiated from that of the ZIF-8 crystals. This confirms that the Cu species are highly dispersed (ultra-small or sub-nanometric level) throughout the MOF structure and provides evidence that the Cu particles are stabilized (as metallic species observed by XPS; Fig. 3e) into the ZIF structure. For comparison, the sample prepared by the traditional impregnation method demonstrated large Cu particles (Fig. S8). HAADF (Fig. 2d and Fig. 2e), along with STEM-EDX of the ion exchange sample, showed a uniform distribution of all elements (Zn, O, N and C) in the ZIF-8 structure with rhombic dodecahedron morphology. Furthermore, the presence of Cu species within the MOF crystal was clearly visible.
Surface acid-base and metal properties of the catalysts: The basicity and acidity of the catalysts were analyzed using CO2 temperature programmed desorption (CO2-TPD) and NH3-TPD techniques. As shown in Fig. 3a, the sample prepared using the ion exchange method after reduction (Cu/ZIF-8|IE|R) had higher basicity than ZIF-8 alone. It is well known that ZIF-8 interacts very weakly with CO2. This increase in basicity after incorporating Cu may be attributed to the presence of –OH groups generated during the exchange reaction (Fig. S3 and Scheme 1). The sample prepared via impregnation also showed higher basicity than ZIF-8. We attributed this to the decomposition of the material via reduction. Using NH3-TPD (Fig. 3b), we observed an increase in the acidity of the samples with the introduction of Cu. However, this increase is much more accentuated in the case of the impregnated sample, as its decomposition leads to the formation of acid sites, as shown in Fig. 1.
XPS analysis of all the catalysts was performed for each element, and the results are shown in Fig. 3 and Fig. S9. The Zn 2p core level spectra of all samples (Fig. 3c) revealed the presence of Zn (II) species in the catalysts with binding energy (BE) peaks at 1021.4 eV and 1044.5 eV.27 In the Auger spectra of the ZIF-8 and Cu/ZIF-8|IE| samples (Fig. 3d), the Zn Auger region consisted of two peaks at 498 eV and 495 eV because of Zn2+ and Zn0, respectively. The presence of Zn0 in both samples before any reduction treatment can be ascribed to photoreduction from the highly energetic X-rays used in the XPS technique.18 After reduction at 523 K in H2, the main peak at 498 eV was more pronounced and contained a small shoulder at 495 eV, indicating that some of the Zn2+ sites might have been reduced during hydrogenation.
The Cu 2p spectrum (Fig. 3e) of the Cu/ZIF-8|IE| sample confirms the presence of oxidized Cu2+ species with satellite peaks.28,29 After reduction at 523 K (Cu/ZIF-8|IE|R), the CuO species were reduced to metallic Cu species, as confirmed by the presence of a peak at932 eV (Fig. 3e). The small peak is attributed to Cu2+ from CuO that can be attributed to the outer layer of the sample from atmospheric oxygen exposure during sample preparation and transfer to the XPS apparatus.30 The absence of a shakeup satellite peak at 947.6 eV confirms the absence of Cu+ species on the surface. Compared to bulk Cu0 with Cu 2p1/2 at 952.5 eV, the Cu-ion exchanged sample demonstrated a lower Cu binding energy (Cu 2p1/2 at 951.7 eV). This likely resulted from electron injection from the conduction band of ZnO2 to CuO, and provides evidence for a strong interaction between Cu and Zn species.18,31 The same was confirmed with Auger spectroscopy (Cu LMM) of these samples (Fig. 3f). No peak for Cu+ was observed near 570 eV, and the peak at 568 eV confirms the presence of predominately Cu0 species on the reduced catalyst.32
The relative surface compositions obtained from this analysis demonstrated remarkably higher surface oxygen concentration after the ion exchange procedure (Table S2). After reduction, a slight decrease in surface oxygen concentration was observed. Both results were in good correlation with the in situ DRIFTS results in which an intense vibrational band due to –OH stretching was observed after Cu exchange and the subsequent reduction reaction (Fig. 4b). Note that the reduction of the sample in H2 resulted in an additional O 1s peak near 533 eV because of the superficial –OH groups (Fig. S9).
Local environments of Cu and Zn: To determine the local arrangements of Cu and Zn species, XAS analysis was performed on Cu-ZIF-8|IE| and after aging the sample in the CO2+H2 reaction mixture under working conditions (Fig. 4a) for 100 h. The two resulting spectra are completely different. The freshly prepared sample and the sample after CO2+H2 treatment show the typical XANES profiles of Cu2+ and Cu0, respectively.33,34 This is also observed in the curves of the first derivative of the XANES spectra. As shown in Fig. 4b, the derivative spectrum of the freshly prepared sample presents a weak peak at ~8977 eV for the dipole-forbidden 1s → 3d transition and the main peak at ~8986.6 eV for dipole-allowed 1s → 4p transition, which is characteristic of Cu2+.35 For the characteristics of the 1s → 4p transition, the Cu2+ species in the freshly prepared sample demonstrate a positive energy shift of ~1.0 eV compared to Cu2+ in Cu(OH)2, indicating that a part of the Cu2+ species is in a distorted state.36 The derivative spectrum of the used sample demonstrates an edge-energy feature at ~8979 eV for the 1s → 4p transition, which is characteristic of reduced Cu.37 All these results agree with the XPS results (Fig. 3).
For Zn K-edge XANES spectra (Fig. 4c), we see that both spectra are highly similar and correspond to the published spectra of ZIF-8. This indicates that the local environment of Zn mainly comprises ZnN4.38 In other words, most Zn is part of the ZIF-8 structure. After subtracting the spectrum of the catalyst before using it from the sample after treatment, we see that a small peak appears at 9662 eV, indicating that the Zn white line is altered during the CO2 reduction reaction. This Zn white line observation has been previously reported in other Cu/ZnO systems.33,39 In this study, this change was attributed to the formation of interfaces between reduced Cu and partially reduced Zn<2+.39 These results agree with the Zn 2p XPS spectra in Fig. 3c.
Activity and stability in the CO2 hydrogenation to methanol reaction: The prepared catalysts were screened below 10% CO2 conversion levels under 50 bar pressure (Fig. S10 and Fig. S11). The main reduction products were methanol and CO at every temperature screened. Irrespective of the different temperatures and pressures used for the Cu/ZIF-8|IE|R catalyst, we did not detect any methane production, and the testing with different particle sizes (Fig. S12) confirmed no diffusion limitations for our catalyst. The synthesized Cu/ZIF-8|IE| catalyst by the ion exchange method showed sustained activity for more than 100 h of reaction time with no significant changes in selectivity after the initial induction period of around 70 h (Fig. 5a). Depending on the exact catalyst, various induction periods were required before methanol formation to allow the catalysts to complete the necessary structural rearrangements.12,40 Remark: The Cu/ZIF-8|IE|R synthesized by the ion exchange method required approximately 70 h for induction. Increasing the reduction time during the catalyst synthesis step did not result in any differences in terms of Cu morphology, as shown in Fig. 1b. However, after more than 70 h in the reaction mixture (CO2+H2), Cu nanoparticles could be seen from powder XRD and HAADF-STEM-EDX analyses (Fig. 5d and Fig. 5f, respectively). The catalyst showed >90% selectivity throughout the course of the CO2 reduction reaction, greatly outperforming the standard Cu-Zn-Al catalyst for both selectivity (>90% vs 60%) and reaction rate (2.2 gmethanol gmetal-1 h-1 vs 1.4 gmethanol gmetal-1 h-1) under similar reaction conditions.
The prepared Cu/ZIF-8|IE| displayed significantly higher methanol selectivity and corresponding space-time yield (STY) than Cu/ZIF-8|IM| and the benchmark Cu-Zn-Al. The parent ZIF-8 did not show any activity (results not presented) under the experimental conditions employed. The higher selectivity of CO over the Cu/ZIF-8|IM| catalyst is due to the agglomeration of large-sized Cu particles on the ZIF-8 MOF (Fig. S8). The higher methanol selectivity observed over the Cu-ion-exchanged sample should be attributed to the presence of finely dispersed Cu nanoparticles (Fig. 5e, Fig. 5f), leading to a higher CO2-adsorption capacity (Table S1) from the increased availability of surface hydroxyl species observed from both, XPS (Table S2) and in situ DRIFTS (Fig. 6b).
As shown in Fig. S11, the reaction temperature significantly affected the reduction product selectivity over the Cu/ZIF-8|IE| catalyst. The trend observed here correlates well with equilibrium concentrations under a similar protocol (Fig. S13). As observed in both cases, an inverse relationship is observed between methanol and CO selectivity as the reaction temperature increases from 498 to 573 K. Optimized methanol production was observed at 523 K, above which the catalyst showed more CO production with high CO2 conversion. The decline in methanol selectivity at higher temperatures can be explained by the endothermic reverse water–gas shift (rWGS) pathway (CO production) is thermodynamically more favorable at high temperatures, enhancing the production of CO over methanol.41,42
The chemical environment (XPS; Fig. 5c and Fig. S14), catalyst structure (from XRD; Fig. 5c), and catalyst morphology (Fig. 5e, Fig. 5f) after 100 h reaction time are compared with that of the reduced form of the catalyst. The powder XRD analysis of Cu/ZIF-8|IE|R after the reaction showed a small diffraction peak at 2θ = 43.5° (Fig. 5d), confirming metallic Cu presence. The surface compositions obtained from the XPS analysis (Table S2) showed a slight decrease in the surface oxygen with no changes to the Cu/Zn ratio before and after the CO2 reduction reaction, confirming no loss of Cu species during CO2 conversion. Therefore, after exposure to the reaction mixture (in situ reduction), further clustering of the finely dispersed Cu in the ZIF-8 MOF occur, leading to the formation of Cu nanoparticles (Fig. 5g) as seen in the HAADF-STEM-EDX analysis of the catalyst after 100 h of time on stream.
Identification of reaction intermediates: The structure and stability of the catalysts, and the reaction mechanism, were studied using in situ DRIFT spectroscopy at different pressures (1–25 bar) and temperatures (323–523 K; Fig. 6). ZIF-8 and Cu/ZIF-8|IE|R share identical bands with less intense bands observed in the Cu/ZIF-8|IM|R sample, primarily due to the structural collapse of the MOF. Additionally, a highly intense and broad vibrational band is observed in the range of 3150 to 3700 cm-1 that can be assigned to the –O–H stretching vibrations in –OH/OH2 groups, even after reduction at 523 K (Fig. 6b and Fig. S3). Exploring more deeply, we also collected the IR spectra after introducing the reaction mixture CO2:H2 under 25 bar pressure at the reaction temperature after in situ reduction of the sample. This resulted in new peaks between 3150 and 3700 cm-1, mostly due to the adsorption of reactants and the interaction of CO2 with the surface hydroxyl groups (Fig. 6c and Fig. S3).
We analyzed the reaction mechanism by monitoring the intermediates and products from Cu/ZIF-8|IE|R in CO2+H2 at reaction temperature (523 K) under 25 bar pressure by in situ IR spectroscopy (Fig. 6). We propose the reaction mechanism pathway as depicted in Fig. 6a based on the observed reaction intermediates. These experiments were performed at the limit allowed by the cell for safe operation, which was 25 bar (Fig. S10). The in situ IR spectra of Cu/ZIF-8|IE| (Fig. 6b and Fig. 6c) exposed to the CO2+H2 mixture at different pressures (10–25 bar) showed the formation of CO adsorbed on different Cu sites (Fig. 6e, and Fig. 6f). The increase in the intensity of the vibrational band for CO adsorption with pressure confirms the high activity of CO2 conversion at high pressures. The bands at 2093, 2078, and 2060 cm−1 can be assigned to linearly adsorbed CO molecules on metallic Cu species.26 We also observed methoxy species, i.e., two pairs of bands at 2960–2910 cm−1 and 2865 cm−1, corresponding to the ν(CH3) and δs(CH3) vibrations and bicarbonate/carbonates (Fig. 6d) in the region of 1750–1690 cm−1 and 1680–1600 cm−1.26,43 The bands at 2971, 2930, 2888, and 2750 cm−1 were assigned to the formate (HCOO)−metal species(Fig. 6g).17,44 Additionally, the difference IR spectra also show a gradual increase in CO vibrational band intensity with increasing pressure, confirming high conversion at higher pressures (Fig. 6f). Due to the superimposing features of methanol vibrational bands (–OH and –CH) with that of the surface hydroxyl and methoxy groups, it was challenging to monitor methanol formation in the IR cell directly. Thus, the observed HCOO− species was identified as a possible key reaction intermediate in the current reaction pathway.
Adsorption behavior of CO2 studied by density functional theory (DFT): To understand the adsorption properties of CO2 for a given site, we carried out ab initio calculations using DFT (Fig. 7). Based on the results from XRD, IR, XAS, and XPS, we optimized the structure of the Cu cluster encapsulated on the ZIF-8 through linker vacancies (Fig. S15). In this connection, 4 different (key and possible from the obtained results and reported literature)1,20 cases are considered here to study the adsorption of CO2 on (1) Cu sites on the Cu cluster, (2) Zn2+–O2-–Zn2+ sites in a tridentate complex, (3) Cu/ZnO interfacial Cu–Zn2+ sites, and (4) Cu–O–Zn interfacial site (Fig. 7).
The binding of CO2 is not energetically favored on the Cu metal particle (Fig. 7a), as the adsorption energy (ΔEads) is slightly positive (0.21 eV) and the studied case is also consistent with the weak adsorption of CO2 found on Cu surfaces.26 In addition, no adsorption was observed when CO2 was exposed to bare ZIF-8 (no Cu cluster or linker vacancy), consistent with experimental results where no activity was observed in CO2 hydrogenation. Insignificant CO2 uptake was observed in the CO2-TPD experiments on bare ZIF-8 (Fig. 3a). When considering CO2 adsorption on to the Zn2+-O2- sites (to form a bi/tridentate carbonate with an adjacent Cu cluster; Fig. 7b), an adsorption energy of –1.39 eV was found. The adsorption of CO2 at the Cu–Zn2+ interfacial sites (Fig. 7c) was significantly stronger (ΔEads= −1.62 eV) than the adsorption on the Cu nanoparticles and ZnO nodes. CO2 is stabilized via electron transfer from the Cu nanoparticle to CO2 upon binding C to the metal, along with the stabilization of the negatively charged oxygens by the interfacial Lewis acid Zn2+ and Cu sites. Finally, we can conclude that the Cu-O–Zn site was the most preferred site for CO2 adsorption with an adsorption energy of -2.82 eV (Fig. 7d), whereas the Cu site was the weakest adsorption site.