Synthesis and characterization of M1-CNs
The LASM strategy for the synthesis of M1-CNs is shown in Fig. 1a. Briefly, the metal–ligand chelates were prepared by regulating the solution temperature, pH value, and types of metal salts and ligands. Then, a mixed solution of the metal–ligand chelates and cyanuric acid was added to a melamine solution to prepare the metal–containing supermolecule via hydrogen bond assembly among the metal–ligand chelates, melamine and cyanuric acid. After the pyrolysis of the supermolecule at a high temperature under an Ar flow, the M1-CN was obtained38. The X-ray diffraction (XRD) pattern and Fourier-transform infrared spectroscopy (FTIR) spectrum of the supermolecule (Supplementary Fig. 1) were different from those of the raw materials. Furthermore, the inerratic microrod morphology of the supermolecule was dissimilar from those of melamine and cyanuric acid (Supplementary Fig. 2), confirming the supermolecule formation39,40. The colour of the sample and its XPS spectrum and elemental mapping show the homogeneous distribution of Cu in the Cu-containing supermolecule (Supplementary Fig. 3). In addition, the FTIR and XPS spectra demonstrated the presence of citric acid in the supermolecule (Supplementary Figs. 1b and 4). The roles of the supermolecule in the LASM strategy were then investigated by a series of experimental measurements. Thermogravimetry–differential scanning calorimetry (TG–DSC) analysis showed that the supermolecule has a higher decomposition temperature than melamine and cyanuric acid (Supplementary Fig. 5) because of its hydrogen bonds, as they prevent the fusion of supermolecule units under high temperatures and ensure the formation of CN (Supplementary Fig. 6a,b) (ref. 36). Hence, the metal atoms can be fixed during calcination to avoid their migration and aggregation. As a comparison, melamine easily melted during thermal polymerisation (Supplementary Fig. 6c,d), resulting in metal-atom agglomeration, even with a Cu content of 6.8 wt% (Supplementary Fig. 7). As a result, the samples obtained from the supermolecule displayed higher surface areas and pore volumes than the bulk CN that was derived from pure melamine (Supplementary Fig. 8 and Table 1). Moreover, the ligand plays a crucial role in ensuring the control and high loading of the metals in M1-CNs. Additionally, the convenient operation and low cost of this method allowed for hundred-gram-scale syntheses of M1-CNs (Supplementary Fig. 9), suggesting that the LASM strategy possesses great potential for industrial applications.
The XRD patterns and FTIR spectra confirmed that the support of Cu1-CN is CN (Supplementary Fig. 10) (ref. 41). Except for the characteristic XRD peaks of CN, no other peaks were detected for Cu1-CN, indicating the absence of crystals of Cu or its compounds42. Furthermore, Cu1-CN demonstrates a nanosheet structure with a thickness of approximately 10 nm (Fig. 1b and Supplementary Fig. 11), with no observable Cu nanoparticles. The uniform dispersion of the Cu atoms in Cu1-CN was verified by elemental mapping (Fig. 1c). The aberration-corrected high-angle annular dark-field scanning transmission electron microscopy (AC-HAADF-STEM) image clearly depicts high-density bright dots corresponding to Cu atoms without metal clusters and/or nanoparticles on the CN (Fig. 1d). The K-edge X-ray absorption near edge structure (XANES) spectrum of Cu in Cu1-CN (Fig. 1e) revealed that the Cu oxidation state is between those of Cu2O and CuO (Cuδ+, 1 < δ < 2) (ref. 43,44). The charge was balanced by the loss of the H atom of CN (Supplementary Fig. 12). The Fourier-transformed k3-weighted X-ray absorption fine structure (XAFS) spectrum of Cu1-CN (Fig. 1f) showed a solitary peak at 1.43 Å, which can be assigned to the Cu–N first coordination shell. Unlike that of Cu foil, the XAFS spectrum of Cu1-CN did not exhibit a Cu–Cu coordination peak at 2.22 Å, indicating the absence of Cu clusters or nanoparticles in Cu1-CN. From the wavelet transform (WT) contour plots (Supplementary Fig. 13), only the intensity maximum of the Cu–N bond at 4.18 Å−1 was observed for Cu1-CN. Notably, it was different from the Cu–Cu bond peak at 7.02 Å−1 observed for the Cu foil. Cu within Cu1-CN was determined to have a coordination number of approximately 3 and a bond length of 1.86 Å (Supplementary Table 2), demonstrating that the Cu atoms were each coordinated with three N atoms. These results indicate that Cu1-CN was successfully prepared using the developed LASM strategy.
A series of SACs were then prepared and characterised to verify the versatility of the LASM strategy. We found that this strategy could precisely and continuously control the metal contents of the M1-CNs; Cu1-CN is used as an example for the following discussion. A series of Cu1-CNs with different Cu contents were prepared by changing the copper salt and melamine molar ratios. XRD patterns and TEM images (Supplementary Fig. 14) revealed that none of the Cu1-CNs contained Cu nanoparticles42. All the Cu atoms (bright dots highlighted by yellow circles in Supplementary Fig. 15) in the Cu1-CNs showed excellent dispersion without clusters, even when the Cu content was as high as 9.75 at.% (or 34.3 wt%) (Fig. 1d), which is consistent with the XAFS results (Fig. 1f). Notably, this Cu loading (9.75 at.% or 34.3 wt%) is the highest metal loading reported thus far45–47. Furthermore, the Cu contents of the Cu1-CNs correlate well with the added dosage of copper salt (Fig. 1g), indicating that the developed strategy provides excellent control of the metal loading in SACs. When citric acid was not introduced during SAC preparation, the loading of Cu became very low and uncontrollable (Fig. 1g). Additionally, the UV-visible absorption peak of Cu2+ showed an obvious red shift when citric acid was added (Supplementary Fig. 16) but no changes occurred when cyanuric acid was added, proving that citric acid can coordinate with Cu2+ to form a metal–ligand chelate37,48. Then, the metal–ligand chelate was introduced into the supermolecule via hydrogen bonding, which was confirmed by XPS, elemental mapping, and FTIR (Supplementary Figs. 1, 3, and 4). Overall, the ligand plays a key role in providing controllable, high metal loadings for the preparation of M1-CNs. The developed LASM protocol can precisely and continuously control the metal loadings in M1-CNs over a large range.
Next, the LASM strategy was extended to prepare M1-CNs with different metals by changing the metal precursor species (e.g. Mn(Ac)2, Co(NO3)3, or FeCl3) and/or organic ligands (e.g. citric acid or oxalic acid); these were selected based on the stability of the resultant metal–ligand coordination complex (see the Supplementary Information for the detailed syntheses of M1-CNs (M = Cr, Mn, Fe, Co, Ni, Zn, Pd, Ag, or Cd)) (ref. 37). The TEM images and XRD patterns of the as-prepared M1-CNs (Supplementary Fig. 17) revealed that they possessed no metal nanoparticles or metallic crystals. The AC-HAADF-STEM images of all the M1-CNs (Fig. 2) clearly indicated high-density bright dots representing the metal atoms, as well as an absence of metal clusters and/or nanoparticles. Furthermore, the X-ray absorption spectroscopy (XAS) results verified the monodispersity of metal atoms without M–M bonds in the M1-CNs (Supplementary Fig. 18). These results demonstrate that the developed LASM strategy can serve as a universal protocol for SAC preparation.
This strategy could also be used to successfully synthesise multi-metal SACs. Specifically, dual-metal SAC Fe1/Cu1-CN and triple-metal SAC Cu1/Zn1/Ag1-CN were prepared and characterised. The TEM images of Fe1/Cu1-CN (Fig. 3a and Supplementary Fig. 19) showed no metal nanoparticles or clusters; this result was supported by their XRD patterns. In addition, elemental mappings of Fe and Cu in Fe1/Cu1-CN exhibited the same distribution ranges as C and N (Fig. 3b), indicating that Fe and Cu were homodispersed in Fe1/Cu1-CN. The contents of Fe and Cu were 1.67 and 7.93 wt% (Supplementary Table 3), respectively. Bright dots representing Fe and Cu atoms were clearly observed in the AC-HAADF-STEM image of Fe1/Cu1-CN (Fig. 3c), suggesting that these atoms did not cluster and were atomically dispersed in Fe1/Cu1-CN. Furthermore, the XAFS spectrum of the as-prepared Fe1/Cu1-CN sample revealed the dispersions of its metal atoms (Fig. 3d,e). Specifically, no Fe–Fe or Cu–Cu bonds were observed, indicating that both Fe and Cu were atomically dispersed in Fe1/Cu1-CN. In addition, the XANES spectra revealed the oxidation states of Fe (Feδ+, 2 < δ < 3) and Cu (Cuδ+, 0 < δ < 1), which were ascribed to the strong interactions of these metals with CN (Fig. 3f) (ref. 43). For Cu1/Zn1/Ag1-CN, the TEM image and XRD pattern confirmed that no metal nanoparticles were present in the sample (Supplementary Fig. 20). According to the elemental mappings (Supplementary Fig. 21), the Cu, Zn, and Ag atoms had the same distributions as C and N, demonstrating that the three metals were uniformly distributed in Cu1/Zn1/Ag1-CN. Furthermore, the results of inductively coupled plasma-atomic emission spectrometry (ICP-AES) confirmed the presence of Cu, Zn, and Ag in the Cu1/Zn1/Ag1-CN sample (Supplementary Table 4). The AC-HAADF-STEM image of Cu1/Zn1/Ag1-CN (Supplementary Fig. 22) revealed all the metals to be atomically dispersed, confirming the successfully preparation of this triple-metal SAC. The results obtained for Fe1/Cu1-CN and Cu1/Zn1/Ag1-CN verify that multi-metal SACs can be prepared via the proposed LASM strategy.
These results demonstrate the capability of this novel LASM strategy to successfully synthesize SACs containing either single or multiple metals; this protocol also provides SACs with controllable, high metal loadings and can be implemented on a large scale. The four components greatly contributing to the versatility of this LASM SAC preparation strategy are summarised as follows. First, the metal–ligand complexations regulate the type of incorporated metal, which enables the preparation of SACs containing universal metals and multi-metal SACs. Second, the hydrogen bonds between the metal–organic chelate and melamine components allow for the metal contents in the supermolecule to be adjusted, which realizes controllable and high metal loadings. Third, the enhanced melting point of the raw material, originating from its hydrogen bonds, prevents the migration and agglomeration of metals. Fourth, CN produced in situ provides abundant single-atom fixed sites, which stabilise the single metal atoms. Unquestionably, the developed LASM strategy can provide SACs in addition to those prepared in this study.
Photocatalytic reduction of CO2 to C2H5OH
The photoelectrical properties and catalytic activities of Cu1-CNs were investigated. The single Cu atoms extended the light absorption range of CN and enhanced its absorption coefficient (Supplementary Fig. 23), providing Cu1-CN with an improved solar energy utilisation efficiency. According to the photoluminescence (PL) spectra, Cu1-CN has stronger fluorescence quenching and a shorter fluorescence lifetime than CN (Fig. 4a and Supplementary Fig. 24), indicating that Cu single atoms could remarkably reduce photogenerated charge recombination and accelerate charge separation and migration17,49. As demonstrated by linear sweep voltammetry (LSV) (Fig. 4b), Cu1-CN has a lower initial potential for CO2 reduction than CN under a CO2 atmosphere, indicating that Cu single atoms could reduce the energy barrier of CO2 reduction50. The current of Cu1-CN is larger under a CO2 atmosphere than under N2, indicating that Cu1-CN tends to reduce CO2 rather than H+ (ref. 51,52). Furthermore, Cu1-CN has a higher photocurrent than CN, allowing it to provide more photogenerated charges for redox reactions (Fig. 4c) (ref. 8,53). All these results indicate that Cu1-CN has excellent potential for photocatalytic CO2 reduction.
The photocatalytic products and yields of the as-prepared samples were tested. Owing to its poor absorption and high overpotential, CN showed no photocatalytic CO2 reduction activity (Fig. 4d). However, as Cu is a common CO2 reduction catalyst54,55, the Cu1-CNs did show photocatalytic CO2 reduction activity. CH3OH was the sole reduction product when the Cu single-atom content of Cu1-CN was low. However, upon increasing the Cu content, C2H5OH was produced, indicating that high-density Cu sites play a crucial role in C–C coupling. When the Cu content reached 23.6 wt%, Cu1-CN reduced the CO2 to C2H5OH with 100% selectivity; notably, this is the first report on the catalytic reduction of CO2 to pure C2H5OH using an SAC (Supplementary Table 5) (ref. 56,57). The ultrahigh selectivity of Cu1-CN for C2H5OH is superior to those of most known nanocatalysts (Supplementary Table 6). At ultrahigh Cu contents (34.3 wt%), C2H5OH remains the sole reduction product, but its yield decreases because an excess of Cu atoms can reduce the generation of photo-induced charges and increase their recombination. The oxidative products were confirmed to be O2 and tiny H2O2 (Fig. 4e and Supplementary Fig. 25), indicating that the photogenerated holes were consumed by oxidising water to produce H2O2, which then decomposed to O2. No •OH was detected during the photocatalytic reaction (Supplementary Fig. 26), ruling out the adverse oxidation reaction from •OH. Namely, both the photogenerated electrons and holes can be used for the valuable reactions, indicating that Cu1-CN possesses excellent application potential. Due to the solubility of O2 in water (Supplementary Fig. 27), the ratio of O2 to ethanol was lower than the stoichiometric ratio. To determine the source of C in C2H5OH, a 13C isotope labelling test was performed. When 13CO2 was used, the molecular mass of C2H5OH was confirmed to be 48.1, indicating that the C in C2H5OH come from CO2 rather than Cu1-CN. The long-term stability of Cu1-CN was evaluated by continuous CO2 reduction for 20 h, and there was no obvious decay in either the ethanol or O2 yield (Fig. 4e).
In situ attenuated total reflectance (ATR)-FTIR was conducted to characterize the reaction intermediates of the photocatalytic CO2 reduction. For a scanning illumination time of 0–96 s, the Cu1-CN spectra (Fig. 4f) displayed two bands at 1079 and 1355 cm− 1, which were ascribed to the C–O stretching vibration of ethanol and the *COOH moiety of the intermediate product, respectively58,59. During illumination, the intensities of the bands at 1580 and 1705 cm− 1, which correlate to carbonate, continuously decreased59; carbonate originates from the adsorption of CO2 onto the alkalescent CN surface owing to residual amino groups. In the photocatalytic process, carbonate was rapidly consumed. When CN was used for CO2 reduction, no intermediates were produced, even after 12 min of illumination (Supplementary Fig. 28). Based on these results, Cu plays an important role in the adsorption and reduction of CO2, which is consistent with the photocatalytic activity analysis (Fig. 4d).
For heterocatalysis, adsorption between the reactants and catalysts is very important. As shown in Fig. 5a, there are no CO2 temperature-programmed desorption (CO2-TPD) signals for the CN sample, indicating that CN has a low CO2 adsorption capacity. When the Cu single atoms were introduced, three strong CO2-TPD signals were detected, and the CO2 desorption temperature of the main peak was as high as 401°C, thus manifesting a strong adsorption energy between CO2 and Cu1-CN. Defect was a common CO2 adsorption sites in reported works60. However, the weaker electron paramagnetic resonance (EPR) signal of Cu1-CN indicates that its defect density is lower than that of CN (Supplementary Fig. 29), which rules out the increase in CO2 adsorption caused by an increase in the number of defects. Hence, CO2 was well adsorbed at the Cu single-atom sites.
Finally, the adsorption energy of CO2 relative to the adsorption site (Fig. 5b) was determined via density functional theory (DFT) calculations to illustrate the photocatalytic reduction of CO2 to ethanol over Cu1-CN. Among the Cu, C, and N sites, we found that the CO2 adsorption energy is the lowest when it is adsorbed on the Cu single atom sites, indicating that CO2 tends to adsorb on the Cu single atoms, in agreement with the experimental results (Fig. 5a). Owing to the weak adsorption capacity (Fig. 5b) and ultrahigh reduction overpotential (Fig. 4b) of CN to CO2, CO2 reduction cannot occur on the CN surface; thus, the CO2 reduction process on CN was not considered. Because the Cu content of Cu1-CN influences the products obtained via CO2 reduction, two Cu1-CNs models with low (approximately 13 wt%) and high (approximately 25 wt%) Cu contents (L-Cu1-CN and H-Cu1-CN, respectively) were constructed (Supplementary Fig. 30), and their reaction pathways were calculated (Fig. 5c). The intermediate product of *CO can only produce *CHO by hydrogenation on the L-Cu1-CN rather than producing *OCCO through C–C coupling, owing to the overlarge distance between Cu active sites. Furthermore, L-Cu1-CN showed a lower uphill energy barrier for the formation of *CHO than that of H-Cu1-CN. For H-Cu1-CN, the uphill energy barrier of *CO and *CO coupling to produce *OCCO (0.284 eV) was much lower than that of *CO hydrogenation to *CHO (1.718 eV). Thus, the ethanol product was obtained with H-Cu1-CN, while methanol was obtained using L-Cu1-CN. Importantly, it is these large energy barrier differences that provide the high selectivity of H-Cu1-CN for producing ethanol.