The precursor of peroxotungstic acid was prepared by the sol-gel method.^[18] According to the literature method, PCN-250 crystal can be easily prepared by solvothermal method with 3,3',5,5'-azobenzenetetracarboxylate (H₄ABTC) as an organic linker and Fe₃-μ₃-oxo as a metal cluster.^[15] Taking PCN-250 as a platform, ultra-small WO₃ nanoclusters were encapsulated to construct a W@P-x Z-type heterojunction composite photocatalyst (Figure 1, and Supporting Information (SI) Figure S1). A series of W@P-x were synthesized, the addition of peroxotungstic acid and PCN-250 are summarized in Table S1 (SI). Scanning electron microscopy (SEM; Figure S2) image reveals that the pristine PCN-250 exhibits a well-defined octahedral morphology with an average size of 8.0 µm.^[16] The high-resolution transmission electron microscopy image (HRTEM; Figure 1b) reveals an octahedral morphology with smooth surfaces, suggesting minimal WO₃ recrystallization on the PCN-250 surface. High-angle annular dark field scanning transmission electron microscopy (HAADF-STEM) characterization confirms the successful confinement and encapsulation of WO₃ nanoclusters within the PCN-250 (Figures 1c and 1d). In W@P-2 composites, WO₃ nanoclusters with diameters ranging from 0.8 to 1.4 nm are uniformly distributed in PCN-250. Applying the same synthetic approach to a porous carbon support results in the formation of W@C composites, wherein smaller WO₃ nanoclusters with an average diameter of ≈0.6 nm are uniformly dispersed (Figure S3). The elemental mapping of W@P-2 demonstrates that Fe, W, C, N and O elements are uniformly dispersed in the composite catalyst (Figures 1e~1i). These findings validate the efficacy of the proposed synthesis strategy for encapsulating ultrasmall WO₃ nanoclusters within the porous architecture of PCN-250.^[20-21]

Powder X-ray diffraction (PXRD) patterns of the as-prepared W@P-x samples (Figures 2a and S4) show excellent agreement with the simulated pattern. The PXRD pattern of W@P-2 exhibits only PCN-250 characteristic diffraction peaks,^[21-22] indicating homogeneous dispersion of WO₃ within the PCN-250. The remarkable stability of WO₃ nanoclusters in acidic media motivated the use of aqua regia treatment on W@P-2 to isolate the crystalline WO₃ nanoclusters. As revealed in Figure S5, three peaks at 16.5°, 25.6° and 34.1° are attributable to the (020), (111), and (200) reflections of WO₃•H₂O, respectively, demonstrating the presence of WO₃•H₂O in W@P-2. Additionally, the PXRD pattern of W/P-2 exhibits distinct peaks at 22.9° and 24.1°, which can be indexed to the (001) and (200) planes of WO₃, respectively, confirming the presence of its characteristic crystal structure (Figure S4).^[23] PXRD analysis confirms the uniform dispersion of WO₃ nanoclusters within the pores of PCN-250.^[20]

The optical absorption properties of W@P-2 were characterized by ultraviolet-visible (UV-vis) absorption spectroscopy. Figures 2b and S6 reveal that the UV-vis absorption edge of W@P-2 extends to 800 nm, almost covering the entire visible light region. As shown in Figures 2c and S7, the fourier transform infrared (FTIR) spectra of W@P-2, W/P-2, PCN-250 and WO₃ revealed characteristic W-O-W stretching vibrations at 953 and 819 cm^－1.^[17,21] The W-O-W stretching vibration in W@P-2 exhibits a blueshift to higher wavenumbers. This spectral change is attributed to modifications in the bond vibrational mode induced by electronic interactions, suggesting a close association between the PCN-250 framework and the WO₃ nanoclusters. Thermogravimetric analysis (TGA) performed in air revealed distinct thermal decomposition profiles for W@P-2 and pristine PCN-250 (Figure 2d), which conclusively indicates the successful incorporation of WO₃.^[15]

To elucidate the structural and functional implications of WO₃ incorporation, comprehensive characterizations were conducted. N₂ and CO₂ sorption measurements were performed on PCN-250, WO₃, and the composite W@P-2 to characterize their respective porous structures and to evaluate the CO₂ adsorption capacity of W@P-2. The N₂ adsorption-desorption isotherm of W@P-2 was measured at 77 K, yielding a BET surface area of 564.99 m²•g^－1 (Figure S8). Relative to pristine PCN-250 (1190.72 m²•g^－1), W@P-2 exhibits a reduced specific surface area and an increased average pore size, from 0.78 nm (PCN-250) to 0.84 nm (W@P-2) (Figure S9). The experimental results confirm that W@P-2 retains a porous structure, with the pores of PCN-250 being occupied by ultrasmall WO₃ nanoclusters. The CO₂ adsorption capacities of WO₃, pristine PCN-250, and the W@P-2 composite were determined to be 3.45, 63.03, and 42.49 cm³•g^－1, respectively, at 298 K and 101 kPa (Figure S10). This result indicates that the high CO₂ adsorption capacity of W@P-2 facilitates transfer of CO₂ molecules to its active surface, which is conducive to subsequent catalytic processes.^[20]

The enhanced photoelectrochemical properties of W@P-2 were systematically verified. Steady-state photoluminescence (PL) spectra showed significant quenching upon WO₃ integration (Figure S11), suggesting inhibited charge recombination. Measured by time-resolved photoluminescence spectroscopy (Figure S12), the decay lifetime of W@P-2 is 5.23 ns, markedly longer than that of pristine PCN-250 (0.70 ns), indicating more efficient suppression of charge recombination. Consistent with the enhanced charge separation, W@P-2 exhibits a significantly higher photocurrent density than PCN-250 and WO₃ (Figure S13), alongside a smaller semicircle radius in its Nyquist plot (Figure S14), which collectively indicates a lower charge-transfer resistance and more efficient charge migration. Collectively, these results affirm that the synergistic integration of PCN-250 and WO₃ not only maintains a functional porous framework but also significantly promotes light harvesting and the separation of photogenerated charge carriers.

As illustrated in Figure S15, PCN-250 exhibits a band gap of 1.75 eV, whereas WO₃ has a band gap of 2.42 eV. The corresponding conduction band (CB) and valence band (VB) potentials were also determined (Figures S16 and S17). Specifically, the CB and VB of PCN-250 are positioned at －0.75 V and ＋1.00 V (vs. NHE, pH=7.0), respectively. In comparison, WO₃ shows CB and VB potentials of －0.24 V and＋2.18 V, respectively.^[17,23] To probe the chemical composition and interfacial electronic interactions, high-resolution X-ray photoelectron spectroscopy (XPS) was performed on WO₃, PCN-250, and W@P-2. The survey spectrum of W@P-2 (Figure S18) simultaneously displays characteristic signals of Fe, C, O, N, and W, confirming the successful incorporation of WO₃ into the PCN-250 framework. In the high-resolution Fe 2p spectrum (Figure 3a), characteristic doublets corresponding to Fe^2＋ (711.40/725.20 eV) and Fe^3＋ (713.90/730.40 eV) are observed, and these spectral features are preserved in the W@P-2 composite. Similarly, the high-resolution W 4f XPS spectrum of W@P-2 (Figure 3b) exhibits two characteristic peaks at 35.39 and 37.49 eV, which are assigned to W^6＋.^[20] A slight negative shift in the binding energies of both Fe 2p and W 4f is observed. In the C 1s spectrum (Figure S19), peaks corresponding to C—C, C—N, and O—C=O are clearly identified at 284.72, 285.90, and 288.86 eV, respectively. Compared to pristine PCN-250, the N 1s and O 1s peaks in W@P-2 shift to lower binding energies (Figures S20 and S21), indicating an increased electron density within the MOF framework. Conversely, the O 1s peak of W@P-2 shows a positive shift relative to pristine WO₃, suggesting a decreased electron density around WO₃ after composite formation. These results collectively demonstrate an interfacial charge transfer from WO₃ to PCN-250 upon integration, accompanied by the establishment of an effective heterojunction interface in the W@P-2 composite.^[24]

The solar-driven photocatalytic CO₂ reduction was performed under ambient conditions with water vapor as the proton source. As shown in Figure S22, the pristine WO₃ exhibited limited photocatalytic activity, with a CO evolution rate of 56.80 μmol•g^－1. The W@P-2 heterostructure demonstrated a notable enhancement in photocatalytic performance under identical conditions, yielding 516.07  μmol•g^－1 of CO following 12  h illumination (Figure  4a) with 100% selectivity toward CO₂. This performance significantly exceeded that of the individual components. Control experiments identified the W@P-2 photocatalyst, incident light, and the presence of water vapor as critical factors governing the high-selectivity CO₂ photoreduction process (Figure 4b). To assess catalytic stability, recycling tests were performed. As shown in Figure 4c, the CO production yield of W@P-2 exhibits no significant decay over five consecutive cycles. Post-recycling SEM and PXRD analyses further confirmed that the W@P-2 retained its original crystal structure and morphology (Figures 4d and S23). These results indicate that W@P-2 maintain the robustness comparable to the as-synthesized material. Furthermore, the composite demonstrates efficient water oxidation capability during photocatalysis. This is corrobor-ated by PL spectral analysis (Figure S24), in which the characteristic emission peak of 7-hydroxycoumarinn at 456 nm verifies the formation of •OH radicals via an •OH-mediated coumarin oxidation pathway, confirming that H₂O oxidation primarily generates •OH. Collectively, the photogenerated electron-hole pairs in W@P-2 possess strong redox capacity, capable of driving both CO₂ reduction and water oxidation effectively.

To probe the reactive intermediates generated during H₂O photooxidation, electron paramagnetic resonance (EPR) spectroscopy was employed using 5,5-dimethyl-1- pyrroline N-oxide (DMPO) as a spin-trap agent. Upon light irradiation, characteristic quartet signals with a 1∶2∶2∶1 intensity ratio were observed in the EPR spectrum (Figure 5a), corresponding to DMPO-•OH adducts and thus confirming the generation of •OH radicals during H₂O photooxidation catalyzed by W@P-2. Under Xe lamp irradiation, photogenerated holes in WO₃ nanoclusters can oxidize H₂O to •OH via the reaction: H₂O→•OH＋H^＋＋ e^－, with a thermodynamic potential of ＋1.99 V (vs. NHE). Concurrently, PCN-250 harvests photons to generate electrons in its conduction band, which reduce CO₂ along the pathway CO₂＋2H^＋＋2e^－→CO＋H₂O (－0.74 V). The interfacial charge-transfer pathway in W@P-2 was further elucidated by in situ irradiated X-ray photoelectron spectroscopy (XPS). As shown in Figure S25, the Fe 2p binding energies shift toward lower values under illumination, suggesting an increase in electron density around the Fe centers. This is attributed to electron transfer from WO₃, as further supported by corresponding shift of the W 4f peaks to higher binding energies (Figure S26), which reflects electron depletion at W sites. These opposite spectral shifts collectively confirm directional electron transfer from WO₃ to PCN-250, consistent with a Z-scheme heterojunction mechanism. To dynamically monitor the evolution of key intermediates during CO₂ photoreduction, in situ diffuse reflectance infrared fourier transform spectroscopy (DRIFTS) was conducted on the W@P-2 catalyst. As shown in Figure 5b, characteristic vibrational bands corresponding to adsorbed CO₂ (*$CO_{2}^{}$ at 1268 and 1680 cm^－1), bidentate carbonate ($b-CO_{3}^{2}$ at 1555 and 1575 cm^－1), monodentate carbonate ($m-CO_{3}^{2}$ at 1495, 1473, 1361 and 1339 cm^－1), and bicarbonate ($HCO_{3}^{}$ at 1651, 1457 and 1417 cm^－1) exhibited progressive intensity enhancement throughout the reaction. The emergence and gradual intensification of absorption bands at 1632, 1540, and 1246 cm^－1 can be unequivocally assigned to the *COOH intermediate. This species has been identified as the rate-determining intermediate for CO generation during photocatalytic CO₂ reduction,^[25-26] indicating that the formation of *COOH constitutes the key kinetic bottleneck in the CO production pathway. Together, these spectroscopic observations confirm the operation of a Z-scheme charge-transfer mechanism within the W@P-2 heterojunction (Figure 5c).

PXRD data were recorded on an X-ray powder diffractometer (Ultima IV, Rigaku, Japan). The UV-Vis absorption spectra were collected by a UV-Vis spectrophotometer (2550, Shimadzu, Japan). HRTEM images were performed on a transmission electron microscope (JEOL, JEM-2010, Japan). Gas adsorption and desorption isotherms were taken using specific surface and pore size analyzer (BELSORP-max, Microtrac BEL, Japan) and the specific surface areas were detected by the Brunauer-Emmett-Teller (BET) method. Element species and valence analysis were recorded by the XPS spectroscopy (ESCALAB250Xi, Thermo, England). The products of CO₂ photoreduction were analyzed in a gas chromatograph (GC-2014, Shimadzu, Japan) equipped with TCD and FID dual detectors using argon as carrier. EPR spectroscopic measurements were performed on a Bruker EMX Plus-6/1 electron paramagnetic resonance spectrometer (Switzerland) at room temperature. DRIFTS date was performed on a Thermo Scientific Nicolet iS50 transform infrared spectrometer with an in-situ infrared cell and a Calcium fluoride detector (America).

In a typical preparation of PCN-250, Fe(NO₃)₃•9H₂O (14 mg, 0.035 mmol), H₄ABTC (12.5 mg, 0.035 mmol), 6.9 mL of N,N-dimethylformamide (DMF), 1.35 mL of HAc and 0.2 mL of deionized water were added to a 20 mL vial. The mixture was stirred at room temperature for 15 min. Then, the resulting solution was sealed in a 25 mL Teflon-lined stainless-steel vessel and maintained at 140 ℃ for 48 h. After cool down, the red crystals were harvested through centrifugation and washed with DMF for three times, followed by washing with ethanol repeatedly. Finally, the as-obtained product was dried under vacuum at 80 ℃ overnight for further characterization.

In a typical procedure, 2.0 g of Na₂WO₄•2H₂O was dissolved in 80 mL of deionized water in a three-necked round-bottom flask equipped with reflux condenser under stirring. The mixture was heated to 70 ℃, followed by addition of 1.224 g of sodium dodecyl benzene sulfonate (SDBS). After 20 min of controlled agitation, 80 mL of concentrated sulfuric acid was introduced dropwise into the reaction system while maintaining precise thermal regulation of the internal temperature below 100 ℃. Then, the mixture was heated at 160 ℃ for 5.0 h. After cooled to room temperature, the obtained sample was washed with deionized water and ethanol for several times. After vacuum drying at 80 ℃ overnight, the sample was thermally treated in an air atmosphere with a controlled heating ramp of 5 ℃/min, followed by isothermal holding at 350 ℃ for 1 h.

The peroxotungstic acid stock solution was prepared by dissolving 0.4 g of WO₃ in 10 mL of 30% H₂O₂ with constant stirring at 60 ℃ for 5 h. After natural cooling to room temperature, a specific volume of the peroxotungstic acid solution and 25 mg of PCN-250 were added to 10 mL of ethanol (EtOH), followed by continuous stirring at (24±0.5) ℃ for 12 h. To regulate the loading amount of nanoclusters within PCN-250, different volumes of the precursor solution were employed (Table S1). The resulting mixture was evaporated at ambient temperature to yield precipitates, which were washed twice with deionized water. The final products were vacuum-dried at 80 ℃ overnight for subsequent characterization.

A homogeneous suspension was prepared by dispersing 11 mg of WO₃ and 25 mg of PCN-250 in 30 mL of deionized water under continuous stirring. After stirring at room temperature for 30 min, it was transferred to a 50 mL of Teflon-lined stainless-steel vessel and maintained at 120 ℃ for 2 h. After cooling to room temperature, the obtained sample was washed several times with deionized water. The product was dried in vacuum at 80 ℃ overnight, and the obtained powder was collected for further characterization.

The peroxotungstic acid stock solution was prepared by dissolving 0.4 g of WO₃ in 10 mL of 30% H₂O₂ with constant stirring at 60 ℃ for 5 h. After natural cooling to room temperature, 50 μL of peroxotungstic acid solution and 25 mg of porous carbon aerogel were added to 10 mL of EtOH, followed by continuous stirring at (24±0.5) ℃ for 12 h. The resulting mixture was evaporated at ambient temperature to yield precipitates, which were washed twice with deionized water. The final products were vacuum-dried at 80 ℃ overnight for subsequent characterization.

(Zhao, C.)