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. 2021 Jan 15;1(2):2000052. doi: 10.1002/smsc.202000052

ReS2 Nanosheets with In Situ Formed Sulfur Vacancies for Efficient and Highly Selective Photocatalytic CO2 Reduction

Yanzhao Zhang 1, Dazhi Yao 1, Bingquan Xia 1, Haolan Xu 2, Youhong Tang 3, Kenneth Davey 1, Jingrun Ran 1,, Shi-Zhang Qiao 1,
PMCID: PMC11935916  PMID: 40212464

Abstract

Artificial photosynthesis can provide valuable fuels and positively impact greenhouse effects, via transforming carbon dioxide (CO2) and water (H2O) into hydrocarbons using semiconductor‐based photocatalysts. However, the inefficient charge‐carrier dissociation and transportation as well as the lack of surface active sites are two major drawbacks to boosting their activity and selectivity in photocatalytic CO2 reduction. Recently, ReS2 has received tremendous attention in the photocatalysis area due to its intriguing physicochemical properties. Nevertheless, the application of ReS2 in photocatalytic CO2 reduction is scarcely covered. Herein, a heterojunction formed between ReS2 nanosheets and CdS nanoparticles is reported, achieving an apparently raised CO production of 7.1 μmol g−1 and high selectivity of 93.4%. The as‐prepared ReS2/CdS heterojunction exhibits strengthened visible‐light absorption, high‐efficiency electron–hole pair separation/transfer, and increased adsorption/activation/reduction of CO2 on in situ created sulfur vacancies of ReS2, thus all favoring CO2 photoreduction. These are corroborated by advanced characterization techniques, e.g., synchrotron‐based X‐ray absorption near‐edge structure, and density functional theory–based computations. The findings will be of broad interest in practical design and fabrication of surface active sites and semiconductor heterojunctions for applications in catalysis, electronics, and optoelectronics.

Keywords: CO2 photoreduction, heterojunctions, ReS2 , sulfur vacancies, transition metal dichalcogenides


Herein, a heterojunction formed between ReS2 nanosheets and CdS nanoparticles exhibits enhanced photocatalytic CO production together with excellent CO production selectivity. Advanced characterization, e.g., synchrotron‐based X‐ray absorption near‐edge structure, and theoretical computations disclose that the pronounced electronic coupling between ReS2 and CdS and in situ generated sulfur vacancies contribute to the apparently improved light‐induced CO2‐to‐CO conversion performance.

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1. Introduction

CO2 emission leads to severe global greenhouse effect. Therefore, various strategies have been developed to relieve this process, including CO2 fixation and cyclic utilization.[ 1 , 2 , 3 , 4 ] Meanwhile, the application of clean and renewable energy to fix CO2 can not only promote the carbon cycle but also relieve the global energy crisis. Semiconductor‐based photocatalytic carbon dioxide (CO2) conversion represents a carbon‐neutral and sustainable strategy to generate fuels and chemicals using renewable and clean solar energy.[ 1 , 2 , 3 , 4 , 5 ] This process is fundamentally impacted by three steps: 1) light absorption to excite semiconductor‐based photocatalysts, 2) photogenerated electron–hole pair separation and transfer efficiency, and 3) redox reactions on the surface of the photocatalyst.[ 6 , 7 ] To improve photocatalytic CO2 reduction, researchers have generally focused on approaches including introducing defects in the crystal lattice,[ 8 , 9 , 10 , 11 , 12 , 13 ] loading metal cocatalysts,[ 14 , 15 ] exposing highly active facets,[ 16 , 17 ] and fabricating heterojunctions.[ 7 , 18 ] Among these, forming heterojunctions in composites is deemed as an effective strategy due to efficient suppression of charge carrier recombination and highly promoted migration efficiency.[ 19 , 20 ] Some cocatalysts broaden the light absorption spectrum to utilize long‐wavelength light.[ 21 , 22 ] However, CO2 molecules are highly thermodynamically stable with a bond energy of 750 kJ mol−1 for C—O.[ 6 ] This implies that the dissociation of CO2 requires high energy via conventional methods.[ 6 ] The activation of CO2 molecules on the surface of photocatalysts relies on various active sites, e.g., functional groups, frustrated Lewis pairs, single atoms and vacancies. These possess an affinity for CO2 and water (H2O) adsorption and activation. These are however rare on the perfect surfaces of photocatalysts. The deliberate creation of active sites on the surfaces of photocatalysts is therefore a major research approach to practically realize effective photocatalysis.[ 6 ]

Transition metal dichalcogenides (TMDs) have received significant attention in catalysis, rechargeable batteries, and sensing devices.[ 23 , 24 , 25 , 26 , 27 , 28 ] For example, Zhou et al. reported that FeS ultrathin nanosheets on a carbon fiber cloth achieved highly efficient hydrogen evolution due to the phase transition triggered by illumination at room temperature.[ 29 ] Similarly, Fu et al. prepared MoReS3 with a layered structure, a new type of TMDs, and it showed excellent hydrogen evolution in electrocatalysis.[ 30 ] As a new type of TMDs, ReS2 has been studied in photocatalytic hydrogen evolution (PHE), both experimentally and theoretically.[ 31 , 32 , 33 , 34 , 35 , 36 , 37 , 38 ] Zhang et al.[ 34 ] reported that ReS2 exhibited significant performance in PHE, a two‐electron catalytic reaction. This is because free electrons are captured by tightly bound excitons to form trions that constrain recombination and thereby promote performance. The corresponding computation indicates that the adsorption energy of the H atoms exhibits a small absolute value (−0.5 eV), revealing the highly efficient PHE performance. With a narrow bandgap of 1.7 eV, ReS2 possesses strong absorption in the visible‐light range, thus benefiting photocatalytic activity. In addition, ReS2 exhibits an automatic transition of hydrophobicity–hydrophilicity before and following visible‐light illumination.[ 35 ] This is because defects on its surface change the adsorption configuration of H2O and oxygen (O2) to form hydroxyl groups leading to the transmission of hydrophilicity.[ 35 ] This adsorption configuration impacts adsorption of CO2 and H2O in CO2 photoreduction. Zhou et al.[ 36 ] reported that Re sites can absorb hydrogen as the intermediate for CO2 hydrogenation. Findings suggest ReS2 nanosheets (NSs) are a potential photocatalyst for CO2 reduction. A drawback however with most TMDs is that the reactive sites are located at the edge of the NSs, because of the hanging bond created by breakage of the bond between the transmitting metal and sulfur. These limited active sites on the edge and inert surface elsewhere are a significant impediment to applying TMDs as photocatalysts. Therefore, the activation of the inert surface through the introduction of defects on ReS2 NSs is regarded as an effective strategy to boost their photocatalytic performance.

Herein, we report a simple self‐assembly approach to synthesize a heterojunction composed of ReS2 NSs and CdS nanoparticles (NPs) for photocatalytic CO2 reduction. The optimized ReS2/CdS heterostructure exhibits a boosted photocatalytic CO2‐to‐CO conversion activity of 7.1 μmol g−1 accompanied by a high selectivity of 93.4%. The enhanced performance is aroused by high‐efficiency interfacial charge transfer between ReS2 and CdS as well as in situ formed sulfur vacancies on the ReS2 surface. Results from advanced characterizations, e.g., synchrotron‐based X‐ray absorption near‐edge structure (XANES), together with X‐ray photoelectron spectroscopy (XPS), confirm the strong electronic coupling between ReS2 and CdS. Density functional theory (DFT)‐based computations highlight the adsorption and activation of CO2 on the ReS2 surface with in situ formed sulfur vacancies based on electron transfer and change in C—O bond length and angle. Our work will be of immediate practical interest to a wide range of researchers for the design and synthesis of nanostructured materials in the field of energy conversion and storage.

2. Results and Discussion

ReS2 NSs were prepared by exfoliating commercial bulk ReS2 under ultrasonication in deionized water, and CdS NPs were fabricated by a hydrothermal method. Then, the heterojunctions of ReS2 and CdS were synthesized by physical mixing. The as‐prepared samples were denoted as CdS, CR4, CR8 and CR12, respectively, according to the added volumes of ReS2 NSs suspension (0, 4, 8 and 12 mL, respectively). The X‐ray diffraction (XRD) patterns of all the as‐prepared samples are shown in Figure S1, Supporting Information. The pattern displayed is ascribed to cubic‐phase CdS (PDF #10‐0454). A weak peak at 14.6° is attributed to the presence of ReS2 NSs. The intensity of this peak is enhanced with increasing content of ReS2 in the heterojunction. No apparent alteration of peak positions and intensities is observed for cubic‐phase CdS after its combination with ReS2, suggesting the weak interaction formed via physical mixing at room temperature does not change the crystal structure.

Furthermore, the morphologies and microstructures of CdS NPs, ReS2 NSs, and CR12 are characterized by aberration‐corrected high‐angle annular dark field scanning transmission electron microscopy (HAADF‐STEM), transmission electron microscopy (TEM), and HAADF‐STEM elemental mapping. The HAADF‐STEM image of CdS NPs (Figure  1a) exhibits a lattice spacing value of 0.33 nm, ascribed to the (111) facet of cubic‐phase CdS. In addition, the HAADF‐STEM image of a ReS2 NSs (Figure 1b) shows the typical Re4 diamond chain (DC) structure (yellow dot line square). The spacing values between the Re4 diamond in the a [100] and b [010] directions are 0.35 and 0.31 nm, respectively (Figure 1b). This is also displayed in the simulated atomic structure of the ReS2 monolayer (Figure 1c). It is reported that Re4 DCs can act as reactive sites for water splitting. This is because these favor water adsorption and activation, and possibly assist proton transfer to participate in CO2 photoreduction.[ 33 , 34 ] The thickness of the ReS2 NSs was further confirmed to be 6.5 nm using atomic force microscopy (AFM; Figure 1d). The ultrathin thickness of the ReS2 NSs not only endows them with a large surface area to form strong electronic coupling with other materials, but also increases the number of exposed active sites toward catalytic reactions. The combination of a ReS2 NSs and CdS NPs in CR12 is shown in Figure 1e. Moreover, the HAADF‐STEM image and the corresponding energy dispersive X‐ray (EDX) elemental mapping images further corroborate the hybridization of the ReS2 NSs and CdS NPs (Figure 1f) in CR12. The colors red, yellow, and green in Figure 1f represent, respectively, the distribution of Cd, S, and Re elements, in agreement with the HAADF‐STEM image.

Figure 1.

Figure 1

Aberration‐corrected HAADF‐STEM images of a) CdS NPs and b) ReS2 NSs. c) Simulated model for ReS2. The red and yellow colored spheres denote Re and S, respectively, and the blue‐dotted line denotes the Re4 diamond chain. d) AFM image of ReS2 NSs and measured thickness of ReS2. e) TEM of ReS2 NSs and CdS NPs. f) EDX mapping of CR12 from red‐dotted rectangle of (e).

Moreover, both surface‐sensitive XPS and synchrotron‐based XANES were conducted to disclose the interactions between CdS and ReS2 in CR12. The high‐resolution Re 4f XPS spectrum for CR12 (Figure  2a) showed a shift of 0.5 eV toward the direction of lower binding energy compared with that for pure ReS2 (Figure 2b), suggesting electron transfer from CdS to ReS2 in CR12. In addition, the high‐resolution XPS spectrum of Cd 3 d for CR12 shifts to the direction of higher binding energy (Figure 2c), also indicating the electron migration from CdS to ReS2 in CR12. Furthermore, synchrotron‐based XANES was performed (Figure 2d). The S K‐edge XANES of CR12 indicates a shift toward high photon energy direction, in comparison to that for CdS. This also supports the electron transfer from CdS to ReS2 in CR12.

Figure 2.

Figure 2

a) High‐resolution XPS spectrum of Re 4f for CR12. b) High‐resolution XPS spectrum of Re 4f for ReS2. c) High‐resolution XPS spectrum of Cd 3d for CdS and CR12. d) XANES S K edge of CdS and CR12.

Solid–gas phase photocatalytic CO2 reduction activities of the as‐prepared samples were examined under visible‐light irradiation (λ ≥ 420 nm). As shown in Figure  3a, CdS shows a limited photocatalytic CO2 reduction activity with CO and CH4 production of 2.3 and 1.1 μmol g−1 over 7 h (Figure S2, supporting information). The coupling of ReS2 and CdS (CR4, CR8, and CR12) leads to apparent enhancement of both activity and selectivity in visible‐light‐driven CO2‐to‐CO conversion (Figure 3a). In particular, CR12 shows the highest photocatalytic CO2‐to‐CO conversion activity of 7.1 μmol g−1 and selectivity 93.4%, 309%, and 138% times higher than those of CdS alone. This result for the first time demonstrates that coupling with a ReS2 NS could significantly boost both activity and selectivity in photocatalytic CO2‐to‐CO conversion. In addition, we conducted three blank experiments under the same conditions but purged with ultra‐high‐purity argon gas instead of CO2, without visible‐light illumination and without a photocatalyst, respectively. These contrast experiments show no photocatalytic CO2 conversion performance, suggesting that the products (CO and CH4) are generated from photoinduced CO2 conversion. Furthermore, the stability of CR12 was studied via four‐cycle testing with 7 h per cycle (Figure 3b). No apparent deterioration in photocatalytic CO2 reduction performance of CR12 was found over a 28 h test. The TEM image and EDX spectrum (Figure S3, Supporting Information) of CR12 after photocatalytic CO2 reduction exhibited no obvious difference from those before reaction. This finding suggests that no apparent change in morphology and chemical composition of CR12 occurs after the 28 h photocatalytic reaction.

Figure 3.

Figure 3

a) Photocatalytic CO2 reduction activities of CdS, CR4, CR8, and CR12 under visible‐light illumination (λ ≥ 420 nm). b) Photocatalytic CO2 reduction activity of CR12 recycle test with 7 h per cycle test. c) UV–vis diffuse reflectance spectroscopy and band edge for CdS, CR4, CR8, and CR12. d) TSPL spectra for CdS and CR12.

To further investigate the origin of the enhanced activity and selectivity, as well as the reaction mechanism in CR12 for photocatalytic CO2 reduction, both experimental characterizations and DFT‐based theoretical calculations were conducted. The light absorption capacity was studied by UV–vis diffuse reflectance spectroscopy. As shown in Figure 3c, increased absorption in the range of 460–800 nm is attributed to the presence of ReS2 NSs. However, the adsorption edge of CR12 (457 nm) does not display any shift. This finding suggests that the bandgap (2.24 eV) is not changed following combination with the ReS2 NSs. The bandgap of ReS2 NSs is 1.7 eV (Figure S4, Supporting Information). This induces the “bulge” at ≈600–800 nm in the UV–vis spectrum of CR12. Such an improved visible‐light absorption probably contributes to the raised activity in photocatalytic CO2 reduction.

A range of characterization methods, e.g., steady‐state photoluminescence (PL) spectroscopy, transient‐state photoluminescence (TSPL) spectroscopy, electrochemical impedance spectroscopy (EIS), and transient photocurrent (TPC) density measurement, were executed to probe the efficiency of charge‐carrier separation and transportation. The steady‐state PL (Figure S5, Supporting Information) intensity of CR12 is significantly lower than that of CdS. This finding is attributed to the oppressed charge‐carrier recombination after coupling with the ReS2 NSs in CR12. After fitting of the TSPL curves in Figure 3 d, elongated lifetimes of charge carriers (τ 1 = 0.33 ns; τ 2 = 3.44 ns; τ ave = 1.40 ns) for CR12 were observed, in comparison to those for CdS (τ 1 = 0.29 ns; τ 2 = 3.08 ns; τ ave = 1.04 ns). This also supports the more effective dissociation and migration of photogenerated electrons and holes in CR12. Furthermore, the EIS spectra (Figure S6a, Supporting Information) exhibit a smaller semicircle radius for the Nyquist plot together with a decreased charge‐transfer resistance (R t = 4672 Ω) for CR12 in contrast with that of CdS (R t = 4830 Ω). This finding suggests a faster charge‐carrier migration rate in CR12. In addition, CR12 exhibits a greater TPC density than CdS (Figure S6b, Supporting Information). This also confirms the more efficient dissociation of light‐induced excitons, in agreement with the earlier PL and EIS spectra results.

To investigate the CO2 adsorption, activation, and reduction process, XPS and Raman characterizations were conducted for pristine ReS2, RS1, RS2, and RS3 (see details in Section 1.5, Supporting Information). The C 1s peaks in Figure  4a–c mainly consist of a peak located at 284.6 eV, ascribed to the contaminated carbon. All other peaks were calibrated using this peak. After deconvolution of the C 1s peaks in Figure 4a–c, four satellite peaks can be obtained and attributed to C—OH, *COOH, b‐CO2 (chemisorbed and bent CO2), and l‐CO2 (physisorbed and linear CO2), respectively.[ 39 ] Among these adsorption configurations, *COOH is deemed as the precursor for CO, consistent with the major product (CO) of this work.[ 40 , 41 ] The contents (mol%) acquired based on the areas of four satellite C 1s peaks are provided in Table S1, Supporting Information). RS1 shows the highest contents of C 1s peaks associated with *COOH and b‐CO2, in comparison to RS2 and RS3. This is because the water vapor can facilitate the adsorption of CO2.[ 42 , 43 , 44 ] The aforementioned results indicate that the adsorption of CO2 on the surface of the ReS2 NSs is obviously enhanced by visible‐light illumination. To further study the key role of illumination on CO2 adsorption, the high‐resolution XPS spectra of S 2p for pristine ReS2 NSs, RS1, RS2, and RS3 were collected. The ReS2 NSs exhibits two peaks located at 162.05 and 163.18 eV, ascribed to the S 2p 3/2 and S 2p 1/2 (Figure S7, Supporting Information). In comparison, after light illumination, satellite peaks located at 162.7 and 163.85 eV appear (Figure 4d–f), attributed to the presence of sulfur vacancy induced by visible‐light illumination. Moreover, the high‐resolution Re 4f XPS spectrum (Figure S7, Supporting Information) of the pristine ReS2 NSs only exhibits two peaks at 41.65 and 44.06 eV, attributed to the Re 4f 7/2 and Re 4f 5/2 peaks, respectively. In comparison, Re 4f satellite peaks located at lower binding energy positions are observed in the high‐resolution Re 4f XPS spectra of RS1, RS2, and RS3 (Figure S8a–c, Supporting Information), also implying the presence of sulfur vacancies in ReS2 after light illumination. Furthermore, the aberration‐corrected HAADF‐STEM images of RS1 and pristine ReS2 are displayed in Figure S9a,b, respectively. In contrast to pristine ReS2, RS1 exhibits more defects, e.g., vacancies and pores, on its surface after the light illumination. This finding is in agreement with the aforementioned XPS results.

Figure 4.

Figure 4

a,d) High‐resolution XPS spectrum for C 1s and S 2p for RS1. b,e) High‐resolution XPS spectrum for C 1s and S 2p for RS2. c,f) High‐resolution XPS spectrum for C 1s and S 2p for RS3. g) Side‐view (elevation) and h) top‐view (plan) of the electron density distribution of absorbed CO2 on Vs‐ReS2. The red, yellow, gray, and brown colored spheres denote O, S, Re, and C atoms, respectively. The isosurface value is set to 0.002e Å−3. i) Schematic of photocatalytic CO2 reduction in CR12 system under visible‐light illumination (λ ≥ 420 nm). The purple, red, yellow, orange, white, and black colored spheres denote Cd, O, S, Re, H, and C atoms, respectively.

These findings are further corroborated by the Raman spectroscopy characterization. Pristine ReS2 displays a typical E g‐like peak at 305 cm−1 (Figure S10, Supporting Information). In contrast, RS1, RS2, and RS3 all exhibit a blueshift of the E g‐like peak. This might be caused by the presence of a sulfur vacancy leading to the mass fluctuation at the S position. In addition, RS1, RS2, and RS3 all exhibit peaks at 1271 cm−1, ascribed to *COOH (Figure S11, Supporting Information).[ 40 , 41 ] In particular, the highest *COOH peak intensity is observed for RS1, compared to those of RS2 and RS3, in coincidence with the aforementioned XPS results (Table S1, Supporting Information). These findings were reinforced in the Fourier transform infrared spectroscopy (FTIR) spectra (Figure S12, Supporting Information). The bands at 1620 cm−1 are attributed to *COOH and the bands at 1404 cm−1 to the symmetric (O—C—O) vibration, indicating the presence of adsorbed CO2 molecules on the surface of the photocatalyst. These findings are consistent with those from the XPS results.

To verify the possible CO2 activation on the ReS2 with the sulfur vacancy (Vs‐ReS2), DFT‐based theoretical computation was conducted to determine the adsorption of CO2 and the local electronic structure. As shown in Figure S13, Supporting Information, the atomic structures for Vs‐ReS2 were constructed and optimized. The adsorption behavior of CO2 on the surface of Vs‐ReS2 was studied (Figure 4g,h). The adsorption energy (E ad) of CO2 on Vs‐ReS2 was found to be −0.82 eV. This value demonstrates that the chemisorption of CO2 on Vs‐ReS2 is favorable.[ 45 , 46 ] The CO2 molecule loses linearity to change α(OCO) to 117.9°, and the two C—O1 and C—O2 bonds are lengthened to 1.209 and 1.398 Å, respectively, thereby denoting activation of the C=O bond on Vs‐ReS2.[ 46 , 47 ]

Bader charge analysis (Figure S14, Supporting Information) was conducted to study the charge distribution on the CO2‐adsorbed Vs‐ReS2 and to investigate the electronic impact. It was found that Re atoms and C atoms are electron deficient, whereas S atoms and O atoms are negatively charged (Figure S14a, Supporting Information). In particular, Re near a sulfur vacancy (Re4, Re7, and Re13) changed more positively when CO2 was absorbed onto Vs‐ReS2 (Figure S14b, Supporting Information).[ 38 , 46 , 47 ] Charge density difference was used to visualize the electron transfer behavior. The findings showed that Re and carbon atoms donate charges to oxygen and that they are positively charged.[ 37 , 46 , 47 ] These findings confirm that Vs‐ReS2 favorably impacts chemisorption and activation of CO2 and electron transfer between CO2 and Vs‐ReS2.

Based on the findings from both the experimental studies and theoretical computations, a possible photocatalytic CO2 reduction mechanism is proposed. The conduction band (CB) and valence band (VB) edge positions of CdS and ReS2 are estimated via combining their Mott–Schottky plots (Figure S15, Supporting Information) and UV–vis diffuse reflectance spectrum (Figure S5, Supporting Information). As shown in Figure 4i, CdS and ReS2 form a type I (straddling‐type) heterojunction. Under visible‐light illumination (λ ≥ 420 nm), the CdS NPs are photoexcited and the electrons transfer from the VB to the CB, whereas the photogenerated holes in the VB of CdS will migrate to the VB of ReS2, where H2O molecules are oxidized. Then, photogenerated electrons in the CB of CdS transfer to the CB of ReS2. The ReS2 NSs accommodates abundant active sites for the adsorption, activation, and reduction of CO2 and H2O to evolve CO and CH4 (Equation ((1), (2))–(3)). The most likely pathways for the CO2 photoreduction on the CdS/ReS2 heterojunction are proposed as

*+CO2+e+H+COOH* (1)
COOH*+e+H+CO*+H2O (2)
CO**+CO (3)

The asterisks and vertical arrows, respectively, denote reactive sites and the release of gas.

The presence of ReS2 NSs in CR12 leads to the apparent enhancement in the selectivity of photocatalytic CO2‐to‐CO conversion. This is probably because the electrons in ReS2 can be captured by tightly bound excitons to form trions consisting of two electrons and one hole,[ 34 ] which facilitates the two‐electron reduction reaction of CO2‐to‐CO conversion rather than the eight‐electron reduction reaction of CH4 production.

3. Conclusions

In summary, we have successfully prepared a heterojunction of ReS2 NSs and CdS NPs using a facile self‐assembly method via physical mixing at room temperature. This nanocomposite exhibits a significantly boosted visible‐light photocatalytic CO production of 7.1 μmol g−1 together with an increased CO2‐to‐CO conversion selectivity of 93.4%. Such an improved photocatalytic performance originates from two factors: 1) intimate electronic interaction advancing efficient photogenerated electron–hole separation and migration and 2) in situ generated sulfur vacancies serving as active sites for CO2 adsorption, activation, and reduction to CO. These are verified by both state‐of‐the‐art characterizations, e.g., synchrotron‐based XANES, and theoretical calculations. Our work demonstrates the promising potency of ReS2 in light‐driven CO2 reduction and the intriguing opportunities of applying in situ generated anion vacancies of transitional metal dichalcogenides in catalysis, electronics, and optoelectronics.

Conflict of Interest

The authors declare no conflict of interest.

Supporting information

Supplementary Material

SMSC-1-2000052-s001.docx (5.3MB, docx)

Acknowledgements

This work was supported financially by the Australian Research Council (ARC) through the Discovery Project Program (DP160104866, FL170100154, and DE200100629). The authors thank Dr. Ting Gao, University of South Australia, for the XPS testing and Dr. Ashley Slattery, Adelaide Microscopy, The University of Adelaide, for technical assistance. DFT computations within this research were undertaken with the support of supercomputing resources provided by the Phoenix HPC service at the University of Adelaide. Y.Z. acknowledges financial support from the Australian Government Research Training Program Scholarship (RTP). This research was undertaken on the X‐ray absorption spectroscopy beamline at the Australian Synchrotron, part of ANSTO.

Contributor Information

Jingrun Ran, Email: jingrun.ran@adelaide.edu.au.

Shi-Zhang Qiao, Email: s.qiao@adelaide.edu.au.

References

  • 1. Solomon S., Plattner G. K., Knutti R., Friedlingstein P., Proc. Natl. Acad. Sci. USA 2009, 106, 1704. [DOI] [PMC free article] [PubMed] [Google Scholar]
  • 2. Lewis N. S., Nocera D. G., Proc. Natl. Acad. Sci. USA 2006, 103, 15729. [DOI] [PMC free article] [PubMed] [Google Scholar]
  • 3. Vermeer M., Rahmstorf S., Proc. Natl. Acad. Sci. USA 2009, 106, 21527. [DOI] [PMC free article] [PubMed] [Google Scholar]
  • 4. Pearson P. N., Palmer M. R., Nature 2000, 406, 695. [DOI] [PubMed] [Google Scholar]
  • 5. Meinshausen M., Meinshausen N., Hare W., Raper S. C., Frieler K., Knutti R., Frame D. J., Allen M. R., Nature 2009, 458, 1158. [DOI] [PubMed] [Google Scholar]
  • 6. Zhang Y., Xia B., Ran J., Davey K., Qiao S. Z., Adv. Energy Mater. 2020, 10, 1903879. [Google Scholar]
  • 7. Ran J., Jaroniec M., Qiao S. Z., Adv. Mater. 2018, 30, 1704649. [DOI] [PubMed] [Google Scholar]
  • 8. Jiang Z., Sun W., Miao W., Yuan Z., Yang G., Kong F., Yan T., Chen J., Huang B., An C., Adv. Sci. 2019, 6, 1900289. [DOI] [PMC free article] [PubMed] [Google Scholar]
  • 9. Sato S., Morikawa T., Saeki S., Kajino T., Motohiro T., Angew. Chem., Int. Ed. 2010, 49, 5101. [DOI] [PubMed] [Google Scholar]
  • 10. Zhang Q., Gao T., Andino J. M., Li Y., Appl. Catal., B 2012, 123, 257. [Google Scholar]
  • 11. Li X., Sun Y., Xu J., Shao Y., Wu J., Xu X., Pan Y., Ju H., Zhu J., Xie Y., Nat. Energy 2019, 4, 690. [Google Scholar]
  • 12. Shen M., Zhang L., Wang M., Tian J., Jin X., Guo L., Wang L., Shi J., J. Mater. Chem. A 2019, 7, 1556. [Google Scholar]
  • 13. Gao S., Gu B., Jiao X., Sun Y., Zu X., Yang F., Zhu W., Wang C., Feng Z., Ye B., J. Am. Chem. Soc. 2017, 139, 3438. [DOI] [PubMed] [Google Scholar]
  • 14. Long R., Li Y., Liu Y., Chen S., Zheng X., Gao C., He C., Chen N., Qi Z., Song L., J. Am. Chem. Soc. 2017, 139, 4486. [DOI] [PubMed] [Google Scholar]
  • 15. Cheng X., Dong P., Huang Z., Zhang Y., Chen Y., Nie X., Zhang X., J. CO2 Util. 2017, 20, 200. [Google Scholar]
  • 16. Zhang Y., Wang X., Dong P., Huang Z., Nie X., Zhang X., Green Chem. 2018, 20, 2084. [Google Scholar]
  • 17. Xu H., Ouyang S., Li P., Kako T., Ye J., ACS Appl. Mater. Interfaces 2013, 5, 1348. [DOI] [PubMed] [Google Scholar]
  • 18. Shi H., Chen G., Zhang C., Zou Z., ACS Catal. 2014, 4, 3637. [Google Scholar]
  • 19. Cao S. W., Liu X. F., Yuan Y. P., Zhang Z. Y., Liao Y. S., Fang J., Loo S. C. J., Sum T. C., Xue C., Appl. Catal. B 2014, 147, 940. [Google Scholar]
  • 20. Ran J., Guo W., Wang H., Zhu B., Yu J., Qiao S. Z., Adv. Mater. 2018, 30, 1800128. [DOI] [PubMed] [Google Scholar]
  • 21. Zhao C., Krall A., Zhao H., Zhang Q., Li Y., Int. J. Hydrogen Energy 2012, 37, 9967. [Google Scholar]
  • 22. Yui T., Kan A., Saitoh C., Koike K., Ibusuki T., Ishitani O., ACS Appl. Mater. Interfaces 2011, 3, 2594. [DOI] [PubMed] [Google Scholar]
  • 23. Lin Y. C., Komsa H. P., Yeh C. H., Bjorkman T., Liang Z. Y., Ho C. H., Huang Y. S., Chiu P. W., Krasheninnikov A. V., Suenaga K., ACS Nano 2015, 9, 11249. [DOI] [PubMed] [Google Scholar]
  • 24. Yu Y., Nam G. H., He Q., Wu X. J., Zhang K., Yang Z., Chen J., Ma Q., Zhao M., Liu Z., Ran F. R., Wang X., Li H., Huang X., Li B., Xiong Q., Zhang Q., Liu Z., Gu L., Du Y., Huang W., Zhang H., Nat. Chem. 2018, 6, 638. [DOI] [PubMed] [Google Scholar]
  • 25. Samadi M., Sarikhani N., Zirak M., Zhang H., Zhang H. L., Moshfegh A. Z., Nanoscale Horiz. 2018, 3, 90. [DOI] [PubMed] [Google Scholar]
  • 26. Martella C., Mennucci C., Lamperti A., Cappelluti E., de Mongeot F. B., Molle A., Adv. Mater. 2018, 30, 1705615. [DOI] [PubMed] [Google Scholar]
  • 27. Yun Q., Lu Q., Zhang X., Tan C., Zhang H., Angew. Chem., Int. Ed. 2018, 57, 626. [DOI] [PubMed] [Google Scholar]
  • 28. Wang X., Li G., Seo M. H., Hassan F. M., Hoque M. A., Chen Z., Adv. Energy Mater. 2015, 5, 1501106. [Google Scholar]
  • 29. Zhou G., Shan Y., Wang L., Hu Y., Guo J., Hu F., Shen J., Gu Y., Cui J., Liu L., Wu X., Nat. Commun. 2019, 10, 399. [DOI] [PMC free article] [PubMed] [Google Scholar]
  • 30. Fu Y., Shan Y., Zhou G., Long L., Wang L., Yin K., Guo J., Shen J., Liu L., Wu X., Joule 2019, 3, 2955. [Google Scholar]
  • 31. Keyshar K., Gong Y., Ye G., Brunetto G., Zhou W., Cole D. P., Hackenberg K., He Y., Machado L., Kabbani M., Hart A. H. C., Li B., Galvao D. S., George A., Vajtai R., Tiwary C. S., Ajayan P. M., Adv. Mater. 2015, 27, 4640. [DOI] [PubMed] [Google Scholar]
  • 32. Tongay S., Sahin H., Ko C., Luce A., Fan W., Liu K., Zhou J., Huang Y. S., Ho C. H., Yan J., Ogletree D., Aloni S., Ji J., Li S., Li J., Peeters F. M., Wu J., Nat. Commun. 2014, 5, 3252. [DOI] [PubMed] [Google Scholar]
  • 33. Zhang Q., Wang W., Zhang J., Zhu X., Fu L., Adv. Mater. 2018, 30, 1704585. [DOI] [PubMed] [Google Scholar]
  • 34. Zhang Q., Wang W., Zhang J., Zhu X., Zhang Q., Zhang Y., Ren Z., Song S., Wang J., Ying Z., Wang R., Qiu X., Peng T., Fu L., Adv. Mater. 2018, 30, 1707123. [DOI] [PubMed] [Google Scholar]
  • 35. Wang W., Zhang J., Zhang Q., Wan S., Zhu X., Zhang Q., Wang W., Zhang Y., Liu Y., Fu L., Adv. Mater. 2018, 30, 1804559. [DOI] [PubMed] [Google Scholar]
  • 36. Zhou Y., Song E., Zhou J., Lin J., Ma R., Wang Y., Qiu W., Shen R., Suenaga K., Liu Q., Wang J., Liu Z., Liu J., ACS Nano 2018, 12, 4486. [DOI] [PubMed] [Google Scholar]
  • 37. Chen B., Li H., Liu H., Wang X., Xie F., Deng Y., Hu W., Davey K., Zhao N., Qiao S. Z., Adv. Energy Mater. 2019, 30, 1970117. [Google Scholar]
  • 38. Pan J., Zhou X., Zhong J., Hu J., Phys. Lett. A, 2019, 31, 125883. [Google Scholar]
  • 39. Favaro M., Xiao H., Cheng T., Goddard W. A., Yano J., Crumlin E. J., Proc. Natl. Acad. Sci. USA 2017, 114, 6706. [DOI] [PMC free article] [PubMed] [Google Scholar]
  • 40. Vasileff A., Zhi X., Xu C., Ge L., Jiao Y., Zheng Y., Qiao S. Z., ACS Catal. 2019, 9, 9411. [Google Scholar]
  • 41. Firet N. J., Smith W. A., ACS Catal. 2017, 7, 606. [Google Scholar]
  • 42. Yazaydin A. O., Benin A. I., Faheem S. A., Jakubczak P., Low J. J., Willis R. R., Snurr R. Q., Chem. Mater. 2009, 21, 1425. [Google Scholar]
  • 43. Yue M. B., Sun L. B., Cao Y., Wang Z. J., Wang Y., Yu Q., Zhu J. H., Microporous Mesoporous Mater. 2008, 114, 74. [Google Scholar]
  • 44. Zhao B., Pan Y. X., Liu C. J., Catal. Today 2012, 194, 60. [Google Scholar]
  • 45. Zhi X., Jiao Y., Zheng Y., Qiao S., Small 2019, 15, 1804224. [DOI] [PubMed] [Google Scholar]
  • 46. Khaledialidusti R., Mishra A. K., Barnoush A., ACS Omega 2019, 4, 15935. [DOI] [PMC free article] [PubMed] [Google Scholar]
  • 47. Li H., Shang J., Ai Z., Zhang L., J. Am. Chem. Soc. 2015, 137, 6393. [DOI] [PubMed] [Google Scholar]

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