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Strong Electronic Interaction with Oxygen Vacancies Enriched Cobalt-Oxide Support Boost the CO Production Yield of Nickel-Hydroxide Nanoparticles

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13 December 2024

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14 December 2024

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Abstract

The catalytic conversion of carbon dioxide (CO2) into carbon monoxide (CO) via the reverse water-gas shift (RWGS) reaction offers a promising pathway toward a sustainable carbon cycle. However, the competing Sabatier reaction presents a significant challenge, underscoring the need for highly efficient catalysts. In this study, we developed a novel catalyst comprising cobalt-oxide-supported nickel-hydroxide nanoparticles (denoted as Co@Ni). This catalyst achieved a remarkable CO production yield of ~5,144 μmol gcatalyst⁻¹ at 573 K, with a CO selectivity of 77%. These values represent 30% and 70% improvements over carbon-supported Ni(OH)2 (Ni-AC) and CoO (Co-AC) nanoparticles, respectively. Comprehensive physical characterizations and electrochemical analyses reveal that the exceptional CO yield of the Co@Ni catalyst stems from the synergistic electronic interactions between adjacent active sites. Specifically, cobalt-oxide domains act as electron donors to Ni sites, facilitating efficient H2 splitting. Additionally, the oxygen vacancies in cobalt oxide enhance CO2 adsorption and promote subsequent dissociation. These findings provide critical insights into the design of highly efficient and selective catalysts for the RWGS reaction, paving the way for advancements in sustainable carbon utilization technologies.

Keywords: 
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1. Introduction

The increasing concentration of atmospheric carbon dioxide (CO2) has driven the need for sustainable technologies that can effectively reduce CO2 emissions while simultaneously generating value-added products. Among these, the catalytic conversion of CO2 into carbon monoxide (CO) through the reverse water-gas shift (RWGS) reaction has emerged as a promising pathway. CO, as a key building block for synthetic fuels and chemicals, plays a central role in the production of hydrocarbons via processes like Fischer-Tropsch synthesis. [1,2,3,4] Moreover, RWGS serves as a crucial step in the establishment of a closed carbon cycle, offering a practical route to recycle CO2 and reduce environmental impacts.
Despite its potential, the RWGS reaction faces several challenges, particularly due to the competitive Sabatier reaction, which favors the production of methane (CH4) at lower temperatures. [5,6] This competition often limits the efficiency and selectivity of CO production. [7] Therefore, the development of catalysts that can selectively promote CO2 reduction to CO, while suppressing undesirable side reactions, is critical. Such catalysts must exhibit high activity, robust stability, and precise control over reaction intermediates to achieve the desired selectivity under mild reaction conditions.
Transition metal-based catalysts, particularly nickel (Ni) and cobalt (Co), have been extensively explored for CO2 reduction due to their favorable activity and tunable electronic properties. [8,9,10,11] However, their performance in RWGS reactions is often constrained by limited CO selectivity and poor stability under reaction conditions. Recent studies have highlighted the importance of structural and electronic modifications, such as the incorporation of oxygen vacancies and synergistic bimetallic interactions, in overcoming these limitations. [12,13,14] Oxygen vacancies play a vital role in activating CO2, facilitating its adsorption and dissociation, while adjacent active metal domains, such as Ni, are highly effective for H2 splitting. [15,16]
In this work, we address these challenges by developing a novel catalyst comprising nickel hydroxide nanoparticles supported on cobalt oxide enriched with oxygen vacancies (denoted as Co@Ni). This catalyst leverages the electronic and synergistic interplay between Co and Ni active sites to enhance both CO2 activation and H2 dissociation. Our results demonstrate that Co@Ni achieves a CO production yield of ~5144 μmolgcatalyst-1 at 573 K, outperforming carbon-supported Ni(OH)2 (Ni-AC) and CoO (Co-AC) catalysts by 30% and 70%, respectively. By integrating physical characterization with electrochemical analyses, we elucidate the mechanism behind this enhanced performance, providing valuable insights into the design of advanced catalysts for RWGS reactions.

2. Experimental

2.1. Preparation of Co@Ni Catalyst

The synthesis of carbon supported Co@Ni binary catalysts was carried out through a sequence of steps involving chemisorption, galvanic replacement, and wet chemical reduction of metal ions with precise control over reaction parameters on the active carbon support. Before synthesis the support material (i.e. active carbon (AC)) was surface functionalized by previously reported method. [17] The synthesis process began by preparing a slurry with 3 g of AC, which was sonicated for 30 minutes. Following this, 0.1 M of 3.055 g aqueous cobalt chloride hexahydrate (CoCl2·6H2O) solution was added, and the mixture was sonicated for an additional 30 minutes. The solution was then stirred at 600 rpm for 4 hours. To facilitate reduction, an excess amount of sodium borohydride (NaBH4) was introduced into the mixture. After that 0.1 M of 3.055 g of nickel chloride hexahydrate (NiCl2·6H2O) solution was added, which was reduced by the excess amount of NaBH4 added in the previous step. The resulting product was separated via centrifugation and thoroughly washed sequentially with deionized water, ethanol, and acetone to ensure purity. Finally, the as-prepared material was dried in a vacuum at 70 °C for 24 hours. The resulting sample was labelled as Co@Ni.

2.2. Physical and Structural Characterizations

To analyze the physical properties of the control samples and Co@Ni catalyst, a combination of microscopy and X-ray spectroscopy techniques were utilized. High-resolution transmission electron microscopy (HRTEM) was performed at the Electron Microscopy Center of the National Taipei University of Technology (NTUT), Taiwan, to examine the crystal structure and surface morphology of the synthesized materials in their pristine states. Crystallographic characteristics were studied using X-ray diffraction (XRD) measurements, carried at beamline BL-O1C1 of the Taiwan Light Source (TLS) at the National Synchrotron Radiation Research Center (NSRRC), Taiwan. X-ray absorption spectroscopy (XAS) was performed at beamline BL-17C1 of the NSRRC to further explore the electronic structure and coordination environment of the samples.

2.3. CO2 Conversion Performance Analysis

The catalytic performance of the Co@Ni catalyst, along with the control samples, for CO2 conversion was assessed following a protocol described in a previously published study. [18] In detail, the gas chromatography (GC) analysis was conducted using an Agilent 7890 instrument equipped with a Valco PDHID detector (pulsed discharge helium ionization detector, model D-3-I-7890, VICI, USA). A test sample comprising 12 mg of catalyst and 23 mg of silicone gel was thoroughly mixed and loaded into a glass tube with dimensions of 100 mm in length, an inner diameter of 2 mm, and an outer diameter of 3 mm. The reaction was performed under constant pressure conditions, regulated by a pressure control module (PCM, Agilent). Ultra-high-purity helium (99.9995%) served as the carrier gas at a flow rate of 30 mL min⁻¹. The gas products, after passing through the packed reactor bed, were analyzed using the GC system, following a temperature-programmed desorption (TPD) protocol. The oven temperature was increased from 273 K to 573 K at a ramp rate of 20 K min⁻¹, and the separated components were detected by the PDHID detector. To eliminate any moisture from the reaction system, nitrogen gas (N2) was first flowed through the reactor at 50 mL min⁻¹ for 1 hour at room temperature. Subsequently, a gas mixture containing CO2-H2 with a ratio of 1:3 was introduced into the reaction bed at a flow rate of 20 mL min⁻¹, with the temperature set between 273 K and 573 K. At each temperature step, the system was held isothermal for 30 minutes, and the resulting gas products were analyzed using the GC system.

3. Results and Discussion

3.1. Physical Structure Inspections

Figure 1a shows the HRTEM image of active carbon supported cobalt oxide (Co-AC). Accordingly, the cobalt oxide is grown in form of amorphous nanosheets on the AC support with a d-spacing of 0.234 nm, which is corresponding to the CoO (222) plane. [19] The fuzzy Forward Fourier Transformation (FFT) pattern in the absence of clear bright spots further confirms the amorphous nature of CoO nanosheets. On the other hand, as shown in Figure 1b, the nickel-hydroxide (Ni(OH)2) nanoparticles with the d-spacing of 0.232 ( corresponds to the (013) plane of Ni(OH)2) have been grown with more crystallinity. [20] Such a scenario has been complimentary confirmed by the hexagonal FFT patterns with twin bright spots. For Co@Ni, it is evident from Figure 1c that the Ni(OH)2 nanoparticles (indicated by brown box) are grown on amorphous nanosheets. Herein its worth noticing that the Co@Ni exhibits increased d-spacing of 0.260 nm along with ring like FFT pattern with multiple bright spots. These two observations integrally confirm the limited extent of heteroatomic intermixing between Ni and Co domains.
The X-ray diffraction (XRD) spectra of control samples and Co@Ni were further analyzed to confirm the above discussed HRTEM observations about crystal structure. As shown in Figure 2, the peaks X1, X2 and X3 are corresponding to the different planes of active carbon support. Unsurprisingly, the Co-AC does not shows any additional diffraction signals compared to active carbon support, confirming that CoO nanosheets are grown in amorphous phase and consistent with aforementioned HRTEM observations. On the other hand, Ni-AC and Co@Ni samples exhibit prominent peaks A1 and A2, which are, respectively, corresponding to the (20-22) and (0004) planes of Ni(OH)2. More interstingly, the suppressed peak intensities of Co@Ni as compared to Ni-AC can be attributed to the partial oxidation of Ni due to the heteratomic intermixing with CoO. These observations are in good agreement with HRTEM findings.
The electronic localization from Co-to-Ni domains in Co@Ni catalyst was elucidated by conducting X-ray absorption spectroscopy (XAS)at Co and Ni K-edges. Figure 3a shows the normalized X-ray absorption near-edge structure (XANES) at Co K-edge. Notably, compared to the CoO, the shift of inflection point X to higher energy values confirms the severe electron relocation from Co-to adjacent domains (Ni in this case). [21] Given that the whiteline intensity is directly related to the presence of surface chemisorbed oxygen on the surface of catalyst. [22] However, the Co@Ni catalyst exhibits the suppressed whiteline intensity (HA) as compared to standard CoO. With the additional Ni(OH)2 in Co@Ni system, such an observation indicates the presence of abundant oxygen vacancies in cobalt-oxide support. [23] The aforementioned scenarios are further confirmed by analyzing the XANES spectra of Co@Ni catalyst at Ni K-edge. As shown in Figure 3b, as compared to standard Ni(OH)2, the shift of inflection point X position to the lower energy values along with suppressed whitleline intensity (HB), confirms the increased electron density around Ni-atoms in Co@Ni and can be attributed to the stron electron relocation from Co-to-Ni domains. [22] These observations are in good agreement with the results of Co K-edge XAS analysis. Moreover, the Co@Ni share the similar peak positions with Ni(OH)2 in XANES as well as Fourier-transformed extended X-ray absorption fine structure (FT-EXAFS) spectra (Figure S1) confirming that Ni is present in form of Ni(OH)2. [24]
The surface chemcial identities and structural configuration of Co@Ni were further confirmed by the electrochemical analysis Figure 4a represents the cyclic voltammetry (CV) curves of control samples and Co@Ni samples. All the CV curves were obtained in the N2 saturated 0.1 M KOH electrolyte. Accordingly, all the three samples show flattened CV profiles upto 0.90 V vs RHE. Suggesting their inert nature. Such a scenario is obvious due to severe surface oxidation. At higher potential regions, the prominent peaks in the forward scan are correspond to the oxide/hydroxide formation, while the oxide reduction in the backward scan. Herein, it’s worth noticing that the Co@Ni samples shows peaks (C1-C3-C4) corresponding to the Co-AC (A1-A3) as well as corresponding to the Ni-AC (B1), confirming that Ni(OH)2 nanoparticles are grown on CoO nanosheets. Furthermore, the CO-tolerance of Co@Ni is confirmed by the CO-stripping curves. As shown in Figure 4b, the Co@Ni catalyst shows the CO oxidation peak (O) at lowest potential as compared to Co-AC (M) and Ni-AC (N), indicating the better CO tolerance of Co@Ni.

3.2. Catalytic Activity in CO2 Conversion

The catalytic activites of Co@Ni as well as Co-AC and Ni-AC in CO2 conversion performances were assessed with the help of a flow reactor system within the temperature range of 273 K to 573 K under atmospheric pressure and reaction gas atmosphere of H2/CO2 (3/1). As shown in Figure 5a, At 573 K, Co-AC demonstrates a significantly higher CO production yield, while the CH₄ concentration is almost null (Figure 5b), indicating the predominance of the reverse water-gas shift (RWGS) reaction over CO₂ methanation. This behavior is likely due to the absence of active sites for H₂ dissociation in Co-AC. It is well-documented that metal oxides with abundant oxygen vacancies are effective in facilitating CO₂ activation but are generally inactive for H₂ splitting. [16] In contrast, a significant rise in CH₄ production yield (1142 μmol g⁻¹ of catalyst) is observed for Ni-TiO₂, suggesting that Ni sites favours the H2 splitting. Previous studies have highlighted the role of oxygen vacancies in promoting CO₂ dissociation, while Ni-hydro(oxide) nanoparticles are known to reduce to metallic Ni at 573 K in a hydrogen-rich environment. [15] Thus, it can be inferred that during CO₂ methanation on Ni-TiO₂, oxygen vacancies aid CO₂ dissociation, while adjacent metallic Ni domains facilitate H₂ dissociation. The Co@Ni catalyst shows a 30% increase in CO production yield with the CO selectivity of 77% as compared to Ni-TiO₂, likely due to the additional CO₂ activation sites provided by CoO.

4. Conclusions

In conclusion, the catalytic conversion of carbon dioxide (CO₂) into carbon monoxide (CO) through the reverse water-gas shift (RWGS) reaction offers a promising pathway for establishing a sustainable carbon cycle. This study successfully developed a cobalt-oxide-supported nickel-hydroxide nanoparticle catalyst (Co@Ni), which demonstrated remarkable performance, achieving a CO production yield of approximately 5144 μmol g⁻¹ at 573 K with a CO selectivity of 77%. This performance represents a significant improvement by 30% and 70% higher than those of carbon-supported Ni(OH)₂ (Ni-AC) and cobalt oxide (Co-AC) nanoparticles, respectively. Detailed physical and electrochemical analyses indicate that the exceptional catalytic activity of Co@Ni stems from the electronic interactions between its active sites. Specifically, cobalt-oxide domains act as electron donors, enhancing hydrogen dissociation at nickel sites, while oxygen vacancies in cobalt oxide promote CO₂ adsorption and subsequent dissociation. These results highlight the potential of rationally designing catalysts with synergistic active sites to achieve enhanced efficiency and selectivity for the RWGS reaction.

Supplementary Materials

The following supporting information can be downloaded at the website of this paper posted on Preprints.org, 1. The electrochemical analysis methods-note-1; 2. The FT-EXAFS spectra at Ni K-edge; Figure.S1.

Author Contributions

Conceptualization, T.-Y.C.; methodology, D.B. and T.F.L.; software, D.B..; validation, D.B., A.B., and A.B.; formal analysis, D.B.; investigation, D.B., T.-Y.C; resources, T-Y.C..; data curation, D.B., T.F.L., A.B.; writing—original draft preparation, D.B.; writing—review and editing, D.B., A.B., A.B., and T.-Y.C.; visualization, D.B.; supervision, T.-Y.C.; project administration, T.-Y.C.; funding acquisition, T.-Y.C. All authors have read and agreed to the published version of the manuscript.

Data Availability Statement

The data presented in this study are available on request from the corresponding author.

Acknowledgments

The authors express their gratitude to the staff of the National Synchrotron Radiation Research Center (NSRRC), Hsinchu, Taiwan for the help in various synchrotron-based measurements. T.-Y. Chen acknowledges the funding support from the National Science and Technology Council, Taiwan (NSTC 113-2112-M-007-014-) and the industrial collaboration projects from the MA-tek (MA-tek 2023-T-004) and the Taiwan Space Agency (TASA-S-1120691). Dinesh Bhalothia acknowledges the funding support (Enhanced Seed Grant) from Manipal University Jaipur.

Conflicts of Interest

The authors declare no conflict of interest.

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Figure 1. The HRTEM images of (a) Co-AC, (b) Ni-AC, and (c) Co@Ni catalyst. The Forward Fourier Transformation (FFT) patterns for the selected regions in the HRTEM images are displayed in the bottom left insets. The d-spacing values were determined using Inverse Fourier-Transformed (IFT) images, accompanied by their corresponding line histograms shown in the insets.
Figure 1. The HRTEM images of (a) Co-AC, (b) Ni-AC, and (c) Co@Ni catalyst. The Forward Fourier Transformation (FFT) patterns for the selected regions in the HRTEM images are displayed in the bottom left insets. The d-spacing values were determined using Inverse Fourier-Transformed (IFT) images, accompanied by their corresponding line histograms shown in the insets.
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Figure 2. X-ray diffraction (XRD) spectra of control samples (AC, Co-AC and Ni-AC) and the Co@Ni. Herein the peaks X1, X2 and X3 are corresponding to the different planes of active carbon, whereas the peaks A1 and A2 are corresponding to the (20-22) and (0004) planes of Ni(OH)2.
Figure 2. X-ray diffraction (XRD) spectra of control samples (AC, Co-AC and Ni-AC) and the Co@Ni. Herein the peaks X1, X2 and X3 are corresponding to the different planes of active carbon, whereas the peaks A1 and A2 are corresponding to the (20-22) and (0004) planes of Ni(OH)2.
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Figure 3. XANES spectra at (a) Co K-edge and (b) Ni K-edge.
Figure 3. XANES spectra at (a) Co K-edge and (b) Ni K-edge.
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Figure 4. (a) The cyclic voltammetry (CV) and (b) CO stripping curves of Co-AC, Ni-AC and Co@Ni.
Figure 4. (a) The cyclic voltammetry (CV) and (b) CO stripping curves of Co-AC, Ni-AC and Co@Ni.
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Figure 5. CO2 Conversion results. (a) CO and (b) CH4 production yields of control samples (Co-AC and Ni-AC) and Co@Ni.
Figure 5. CO2 Conversion results. (a) CO and (b) CH4 production yields of control samples (Co-AC and Ni-AC) and Co@Ni.
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