Influence of the loading methods of Ni species in Ni/CeO2 catalysts on the performance of CO methanation

Runran WANG Qiyue JIAO Ruifang LI Hong WANG Hongwei WANG Yali BAO Qi WANG Xiaoyan WANG

Citation:  Runran WANG, Qiyue JIAO, Ruifang LI, Hong WANG, Hongwei WANG, Yali BAO, Qi WANG, Xiaoyan WANG. Influence of the loading methods of Ni species in Ni/CeO2 catalysts on the performance of CO methanation[J]. Chinese Journal of Inorganic Chemistry, 2026, 42(5): 1026-1038. doi: 10.11862/CJIC.20250364 shu

Ni/CeO2催化剂中Ni物种负载方式对CO甲烷化性能的影响

    通讯作者: 汪琪, qiwang127@imut.edu.cn
    王晓燕, rain20030000072@imut.edu.cn
  • 基金项目:

    内蒙古自治区自然科学基金 2025QN02071

摘要: 为提升Ni基催化剂在CO甲烷化反应中的低温活性与抗烧结性能,采用水热法构建了具有限域结构的介孔CeO2载体,并系统比较了等体积浸渍法、共沉淀法及双(环戊二烯)镍升华法3种Ni负载方式对催化性能的影响。借助X射线衍射(XRD)、N2吸附-脱附、氢气程序升温还原(H2-TPR)、X射线光电子能谱(XPS)和透射电子显微镜(TEM)等表征手段,揭示了不同负载方法对Ni物种分散度、颗粒尺寸及金属-载体相互作用的关键调控作用。结果表明,3种方法制备的介孔Ni/CeO2催化剂均因载体的限域效应而表现出优异的抗烧结性能,但三者的低温活性存在显著差异,主要取决于Ni的存在状态。其中,通过双(环戊二烯)镍升华法制备的NC-B催化剂中Ni物种与载体相互作用较弱,还原后形成高度分散的金属Ni纳米颗粒,这增加了低温活性位点数量,从而在300 ℃下实现了98%的CO转化率与100%的CH4选择性,展现出最优的低温CO甲烷化性能。

English

  • As the global energy structure transforms, the strategic importance of clean and low-carbon natural gas has become increasingly prominent[1-2]. CO methanation technology converts coal gasification syngas into synthetic natural gas, serving as a crucial bridge linking the coal chemical industry with clean energy[3-4]. This technology not only alleviates pressure on natural gas supply but also achieves clean and efficient conversion of coal resources, holding significant value in the energy and environmental sectors. Consequently, it has garnered considerable attention from both academic and industrial circles[5-6].

    The core of CO methanation technology lies in developing high-performance catalysts. Although precious metal catalysts offer superior performance, their high cost limits widespread application[7-8]. Nickel (Ni)-based catalysts are widely used due to their high activity and low cost, but suffer from low-temperature deactivation and high-temperature sintering[9-10]. The performance of Ni-based catalysts is primarily governed by the dispersion, particle size of the active Ni component, and its interaction with the support[11-12]. For instance, Li et al.[10] investigated the effect of Ni particle size on CO methanation by preparing a series of Ni@Al2O3-n catalysts. The study revealed that catalysts featuring medium‑sized Ni nanoparticles exhibited high activity at 260 ℃, achieving complete CO conversion rate alongside excellent coking resistance. Xu et al.[13] prepared Ni/SiO2 catalysts via a combustion-impregnation method. By controlling the combustion process, they obtained small Ni particles with an average size of approximately 6 nm. Hydrogen temperature-programmed desorption (H2-TPD) characterization confirmed that this approach significantly improved Ni dispersion and enhanced reactant activation capacity, resulting in outstanding low-temperature activity and CH4 selectivity for CO2 methanation.

    Mesoporous ceria (CeO2) demonstrates significant potential in catalysis due to its well-ordered pore structure, high specific surface area, tunable pore size, unique Ce4+/Ce3+ redox pair, and outstanding oxygen storage/release capabilities[14-16]. The well-defined mesoporous structure facilitates mass transfer and stabilizes loaded metal nanoparticles through spatial confinement, significantly enhancing catalytic performance by leveraging their small size and surface effects[17-19]. Furthermore, the strong interaction between CeO2 and metal components can further enhance the dispersion and stability of the active phase. However, current research has primarily focused on regulating Ni loading, CeO2 morphology, or adding additives, while the impact of the loading method—a critical parameter affecting Ni dispersion—remains understudied. Studies indicate that different loading methods alter the spatial distribution, particle size, and dispersion of Ni species within the structured channels, thereby influencing the catalyst′s methanation activity, selectivity, and sintering resistance[20]. Niu et al.[21] prepared two Ni/CeO2 catalysts using incipient wetness impregnation and combustion methods, respectively. The combustion method produced smaller, more highly dispersed NiO nanoparticles. The rapid, self-sustaining redox reactions during combustion effectively suppressed NiO migration and agglomeration, resulting in a catalyst with outstanding catalytic activity and stability for the dry reforming of methane (DRM). Chen et al.[22] prepared three Ni/SiO2 catalysts using ammonia evaporation, impregnation, and sol-gel methods. It was found that the catalyst prepared by ammonia evaporation had smaller Ni particles, stronger metal-support interaction, and abundant Ni‑O‑Si units on its surface, which significantly improved the catalyst′s anti-sintering performance. However, the catalyst prepared by impregnation had poor catalytic performance due to the uneven distribution of nickel species, large particles, and weak metal-support interaction.

    Therefore, this study aims to investigate the influence of different loading methods on the microstructure and CO methanation performance of Ni catalysts supported on mesoporous CeO2. By systematically comparing the structure-activity relationships of Ni/CeO2 catalysts synthesized via three distinct methods, this work elucidates how loading methods precisely regulate key structural parameters—such as Ni species dispersion and particle size—to determine macroscopic catalytic performance, including low-temperature activity, selectivity, and long-term coking resistance. These findings provide crucial theoretical foundations and experimental support for designing next-generation, highly efficient, and stable industrial methanation catalysts.

    Nickel nitrate hexahydrate (Ni(NO3)2·6H2O, AR), cerium nitrate hexahydrate (Ce(NO3)3·6H2O), bis(cyclopentadienyl)nickel (AR), citric acid monohydrate (AR), and hexadecyl trimethyl ammonium bromide (CTAB, AR) were purchased from Shanghai Titan Technology Co., Ltd., China.

    1.2.1   Preparation of mesoporous CeO2 support

    Ce(NO3)3·6H2O, citric acid, and CTAB were mixed in a molar ratio of 5∶1∶1 under continuous stirring. Ammonia solution was slowly added to adjust the system pH to 9. The mixture was stirred in a water bath for 2 h, then transferred to a polytetrafluoroethylene-lined high-pressure reactor and crystallized at 120 ℃ for 12 h. The product was filtered and washed three times alternately with anhydrous ethanol and distilled water, and dried in a forced-air oven for 12 h. Finally, it was calcined in a muffle furnace at 300 ℃ for 5 h (heating rate: 5 ℃·min-1 to obtain pale yellow mesoporous CeO2 powder, designated as CeO2-0.

    1.2.2   Preparation of comparative CeO2 support

    The obtained CeO2-0 was calcined at 1 000 ℃ for 4 h in a muffle furnace (heating rate: 5 ℃·min-1). The resulting reference sample was designated as CeO2-1.

    1.3.1   Preparation of the catalysts by incipient wetness impregnation

    For a nominal NiO loading (mass fraction) of 20%, the corresponding amount of Ni(NO3)2·6H2O was weighed and dissolved in 100 mL of distilled water (or anhydrous ethanol) to prepare the impregnation solution. Then, 2 g of the prepared mesoporous CeO2-0 support was weighed. The incipient wetness impregnation method was applied by adding the solution dropwise to the support. After ultrasonic-assisted impregnation at room temperature for 24 h, the sample was dried in a forced-air oven at 80 ℃ for 24 h. Subsequently, it was calcined at 550 ℃ for 4 h (heating rate: 1 ℃·min-1), yielding catalysts with 20% NiO loading, designated as NC-W and NC-E (W denoted deionized water as the dispersant, E denoted anhydrous ethanol as the dispersant).

    1.3.2   Preparation of the control sample by incipient wetness impregnation

    Following the same procedure as in section 1.2.1, but using the prepared CeO2-1 support. An equal volume of the prepared Ni(NO3)2·6H2O solution dissolved in ethanol was added to the support using the volume-equivalent impregnation method. After ultrasonic impregnation at room temperature for 24 h, the sample was dried in a forced-air drying oven at 80 ℃ for 24 h. After removal, the sample was calcined at 550 ℃ for 4 h (heating rate of 1 ℃·min-1), yielding a reference catalyst with 20% NiO loading (designated as NC-1).

    1.3.3   Preparation of NC-B catalyst by bis(cyclopentadienyl)nickel

    1.644 g of bis(cyclopentadienyl)nickel and 2 g of the prepared mesoporous CeO2-0 support were placed into a quartz reaction tube. Under vacuum, the mixture was heated at 1 ℃·min-1 to 120 ℃ and held for 24 h. After cooling to room temperature, the sample was dissolved in ethanol, magnetically stirred for 4 h, centrifuged, washed, dried overnight, and finally calcined in a muffle furnace at 500 ℃ for 4 h (heating rate: 1 ℃·min-1) to obtain the catalyst, designated as NC‑B, where B denoted bis(cyclopentadienyl)nickel sublimation loading[23].

    1.3.4   Preparation of NC-C catalyst by the co-precipitation method

    A stoichiometric ratio control method was adopted. The dosage of Ni(NO3)2·6H2O was calculated based on 20% NiO loading in the final product. Ce(NO3)3·6H2O, Ni(NO3)2·6H2O, citric acid, and CTAB were weighed in a molar ratio of 5.2∶3∶1∶1, and homogeneous mixing of the precursor system was achieved under continuous stirring. Ammonia solution was added dropwise until the system pH reached 9. The mixture was stirred in an 80 ℃ water bath for 2 h, then transferred to a polytetrafluoroethylene-lined high-pressure reactor and crystallized at 120 ℃ for 12 h. The product was vacuum-filtered, and the precipitate was washed alternately three times with anhydrous ethanol and distilled water, followed by drying for 12 h. Calcination was performed in a muffle furnace: first at 300 ℃ for 5 h (heating rate: 1 ℃·min-1), then at 550 ℃ for 4 h (heating rate: 1 ℃·min-1). The resulting catalyst powder was designated NC-C (C denoted the co-precipitation method).

    X-ray diffractometer (XRD) patterns were recorded on a Bruker D8 X-ray diffractometer using Cu radiation (λ=0.154 06 nm) operated at 40 kV and 100 mA. Data were collected in a 2θ range of 5° to 90° with a step size of 3 (°)·min-1. A Rigaku D/MAX-2500/PC X-ray diffractometer was used for small-angle XRD analysis in the range of 0.5° to 5° with a step size of 1 (°)·min-1. Crystallite sizes were estimated using the Scherrer equation:

    $ D=Kλ/(βcos θ) $

    (1)

    where D is the crystallite size (nm), K is the Scherrer constant (0.89), λ is the X-ray wavelength (0.154 nm), and β is the full width at half maximum (FWHM).

    X-ray photoelectron spectroscopy (XPS) analysis was performed on a PHI 5000 VersaProbe Ⅱ X-ray photoelectron spectroscopy (Japan) using monochromatic Al radiation (=1 486.1 eV) with an energy resolution of 50 eV. The binding energy was calibrated using the C1s peak at 284.6 eV to analyze the elemental composition and valence states of the samples.

    Transmission electron microscope (TEM) and high-resolution transmission electron microscopy (HRTEM) images were obtained using a JEM-2010HR transmission electron microscope (JEOL, Japan) operated at 200 kV with a point resolution of 0.23 nm. The sample powder was ultrasonically dispersed in anhydrous ethanol, and a drop of the suspension was deposited onto a carbon-coated copper grid, dried, and observed under vacuum to examine morphology, pore structure, and the distribution and size of Ni nanoparticles.

    N2 adsorption-desorption isotherms were measured at -196 ℃ using a Micromeritics ASAP-2020 analyzer. Before testing, samples underwent vacuum degassing pretreatment at 200 ℃, followed by static nitrogen adsorption at -196 ℃ (liquid nitrogen). Specific surface area was calculated using the Brunauer-Emmett-Teller (BET) method. Pore volumes and pore size distributions were derived from the adsorption branch using the Barrett-Joyner-Halenda (BJH) model.

    Hydrogen temperature-programmed reduction (H2-TPR) experiments were conducted on a PX200 apparatus. Approximately 50 mg of catalyst (80 mesh) was loaded into a U-shaped quartz reactor. The sample was first purged with N2 at room temperature for 30 min. The gas was then switched to a H2/Ar mixture (1∶9, V/V), and the temperature was ramped from room temperature to 900 ℃ at a rate of 10 ℃·min-1.

    Catalytic performance was evaluated using a WFSM-3060-DL fixed-bed reactor system (Tianjin Xianquan Co., Ltd.). Product analysis was performed online using an SP-2100A gas chromatograph (Beijing Beifeng Ruili Co., Ltd.) equipped with a thermal conductivity detector (TCD).

    Typically, 0.3 g of catalyst (60-80 mesh) was loaded into the reactor. Before reaction, the sample was purged with nitrogen for 10 min, then reduced at 500 ℃ for 1 h under a high-purity H2 atmosphere. The temperature was subsequently lowered to 200 ℃ under the same H2 atmosphere before switching to a mixed gas (CO/H2/Ar, 18∶54∶28, V/V). The temperature was raised to 800 ℃ at a rate of 10 ℃·min-1. Products were collected and analyzed simultaneously at 50 ℃ intervals from 200 to 800 ℃.

    In the gas chromatography (GC) analysis, Ar was used as the carrier gas. The support gas was Ar at a flow rate of 30 mL·min-1. The thermal conductivity detector (TCD) was set at 150 ℃. The column was TDX-01, the column oven temperature was set at 130 ℃, the injector temperature was set at 130 ℃, the pre-column pressure was set at 0.2 MPa, and the make-up pressure was set at 0.15 MPa.

    The activity calculation formula is as follows:

    $ X_{\rm CO}=(M_{\rm CO, in}-M_{\rm CO, out})/M_{\rm CO, in}×100\% $

    (2)

    $ {Y}_{\rm C{H}_{4}} = {M}_{\rm C{H}_{4}, out} /M_{\rm CO, in}×100\% $

    (3)

    $ {S}_{\rm C{H}_{4}} = {M}_{\rm C{H}_{4}, out} /(M_{\rm CO, in}-M_{\rm CO, out})×100\% $

    (4)

    where XCO, $ {Y}_{\rm C{H}_{4}} $, and $ {S}_{C{H}_{4}} $ are the CO conversion rate (%), the CH4 yield (%), the CH4 selectivity (%), respectively; MCO, in, MCO, out, and $ {M}_{\rm C{H}_{4}, out} $ are the molar flow rates of CO in the inlet stream (mol·min-1), CO in the outlet stream (mol·min-1), and CH4 in the outlet stream (mol·min-1), respectively.

    2.1.1   Textural characteristics analysis

    Fig.1a shows the small-angle XRD pattern of the CeO2-0 support prepared by hydrothermal synthesis. A distinct characteristic diffraction peak at 2θ≈0.8° corresponds to mesoporous materials[24], confirming the mesoporous structure of the CeO2‑0 support. Fig.1b showed that all samples exhibited characteristic diffraction peaks corresponding to the cubic fluorite structure of CeO2. The CeO2 diffraction peaks for NC‑E were more intense and sharper. This is attributed to the successful encapsulation of most NiO species within the mesoporous channels of CeO2, which ensures the high dispersion of NiO and also promotes the formation of long-range lattice order in the CeO2 framework during calcination, resulting in the significantly enhanced and sharper diffraction peaks observed in the NC‑E sample[25].

    Figure 1

    Figure 1.  (a) Small-angle XRD pattern of CeO2-0 and (b) XRD patterns of the samples

    Fig.2 presents the N2 adsorption‑desorption isotherms and corresponding pore size distributions for the CeO2-0 support, NC-C, NC-B, NC-W, and NC-E. As shown in Fig.2a, all samples exhibited type Ⅳ isotherms with H3-type hysteresis loops[26], further confirming that CeO2-0 is a typical mesoporous material, consistent with the small-angle XRD results. This also indicated that loading metallic Ni did not alter the mesoporous structure of the support. The H3-type hysteresis loops at high relative pressures (p/p0>0.75) suggest the presence of slit-shaped pores[27-28]. The BJH pore size distribution curves in Fig.2b reveal that the mesopores of the CeO2-0 support were mainly concentrated in the 3-5 nm and 7-8 nm ranges. The pore sizes of NC-C, NC-B, NC-W, and NC-E were primarily distributed between 5 and 15 nm, indicating the presence of stacked pore channels and distinct mesoporous characteristics[29]. Furthermore, as listed in Table 1, NC-C, NC-B, NC-W, and NC-E retained high specific surface areas inherited from the support. This increased surface area facilitates the dispersion of Ni species, thereby enhancing catalytic performance.

    Figure 2

    Figure 2.  (a) N2 adsorption-desorption isotherms and (b) pore size distribution curves of the samples

    Table 1

    Table 1.  Physicochemical properties of catalysts prepared by different loading methods
    下载: 导出CSV
    Catalyst Crystallite size of CeO2/nm Mesoporous content/% SBETa/(m2·g-1) $ {n}_{C{e}^{3+}} $/($ {n}_{C{e}^{3+}} $+$ {n}_{C{e}^{4+}} $)/%
    CeO2⁃0 7.0 62.78 147
    NC⁃C 9.0 92.4 104 34.61
    NC⁃B 12.0 95.04 107 37.22
    NC⁃E 28.3 86.84 91 28.33
    NC⁃W 35.4 93.46 91 28.02
    NC⁃1 65.08 9

    Table 1 lists the average particle sizes of each catalyst calculated using the Scherrer equation. The results showed that the average particle size of all catalysts was larger than that of the pure CeO2-0 support. After secondary calcination, the particle sizes of the samples increased.

    2.1.2   Analysis of redox properties

    The H2-TPR results in Fig.3a revealed that the mesoporous CeO2-0 support exhibited reduction peaks at approximately 500 and 790 ℃, attributed to the reduction of surface-adsorbed oxygen and bulk lattice oxygen, respectively. The surface oxygen species on CeO2-0 enhance the electron transfer capacity on the catalyst surface, thereby boosting catalytic activity[30]. The large peak area for surface oxygen reduction indicates an abundance of surface oxygen species, making CeO2-0 an ideal support for Ni-based methanation catalysts.

    Figure 3

    Figure 3.  (a) H2-TPR curves of the catalysts; (b) Survey, (c) Ce3d, and (d) Ni2p XPS spectra of the catalysts

    Reduction peaks above 700 ℃ are attributed to the CeO2-0 support. The reduction curves of NC-E and NC-W were similar, both exhibiting reduction peaks corresponding to weakly interacting NiO species at approximately 260 and 375 ℃. Combined with XRD particle size analysis, NC-W exhibited increased particle size after reduction and significantly smaller reduction peak areas, indicating encapsulation of NiO by the support, which reduces the amount of reducible NiO species. The H2-TPR results demonstrated that different preparation methods significantly influenced the morphologies of NiO species and their interaction strength with the CeO2-0 support.

    The reduction curves of catalyst NC-B exhibited peaks at approximately 240 and 300 ℃, attributed to α-NiO with weak interactions with the support[31]. Compared to other catalysts, the reduction peaks of NC-B shift to lower temperatures, indicating abundant NiO species with weaker support interactions, leading to the formation of highly dispersed Ni nanoparticles that provide more active sites. In contrast, NC-C showed a NiO reduction peak only at 380 ℃, the highest temperature among all catalysts, indicating strong NiO-CeO2 interactions. The reduced Ni species in NC-C also maintained strong interactions with the support, enhancing their resistance to sintering.

    2.1.3   Surface phase analysis

    Fig.3b shows the XPS survey spectra of the samples, indicating that the sample primarily composed of Ce, Ni, O, and C elements. Further systematic analysis of the XPS spectra of Ce3d and Ni2p was conducted to clarify the chemical states of the elements. Fig.3c shows the Ce3d XPS spectra of the samples. Due to hybridization between the Ce4f and O2p orbitals, the Ce3d XPS spectra exhibited a complex structure. Through fitting analysis, these spectra can be resolved into eight characteristic peaks, located at binding energies of approximately v0 (882.9 eV), u0 (885.7 eV), v1 (888.6 eV), v2 (897.7 eV), v0′ (901.1 eV), u0′ (903.8 eV), v1′ (907.6 eV), and v2′ (916.7 eV). Among these, u0 and u0′ belong to Ce3+, while v0, v1, v2, v0′, v1′, and v2′ belong to Ce4+. The peaks v2, v1, u0, and v0 at binding energies of 897.7, 888.6, 885.7, and 882.9 eV, respectively, are attributed to the ground state levels of Ce3d5/2. The peaks v2′, v1′, u0′, and v0′ at binding energies of 916.7, 907.6, 903.8, and 901.1 eV correspond to the ground state levels of Ce3d3/2[32]. Among catalysts prepared under different loading methods, the binding energy of Ce3d5/2 was uniformly 888.3 eV. As indicated by the molar ratio of Ce3+ to Ce3+ and Ce4+ [$ {n}_{C{e}^{3+}} $/($ {n}_{C{e}^{3+}} $+$ {n}_{C{e}^{4+}} $)] in Table 1, the predominant valence state of Ce compounds in the catalyst was +4, and NC-B exhibited the highest Ce3+ content. The redox electron pairs formed between Ce3+ and Ce4+ facilitate electron transfer during catalysis, thereby enhancing activity.

    Fig.3d shows the XPS spectra of the Ni2p for the samples. The binding energy of Ni2p3/2 was 855.8 eV, observed within the range of 855.5-856.5 eV, corresponding to the Ni2+ species. The peak at 861.0 eV is attributed to a satellite peak[33]. The Ni2+ peak area across the four catalysts indicates that the NC-C catalyst contained lower NiO content on its surface. Combined with H2-TPR and XRD characterization results, it is inferred that under these conditions, a significant amount of Ni2+ enters the CeO2 lattice, forming strongly interacting Ni-Ce solid solutions with CeO2.

    2.1.4   Morphological analysis

    Fig.4 and 5 show TEM and HRTEM images of the CeO2-0 support and catalysts. As seen in Fig.4a and 4b, although some agglomeration existed, the CeO2 particles showed a relatively uniform size distribution. According to the statistical results in Fig.4c, the particle size distribution was primarily centered around 5 nm, consistent with BJH pore size distribution and small-angle XRD results. The HRTEM image in Fig.4d reveals lattice fringes with spacings of approximately 0.27 and 0.31 nm, corresponding to the (200) and (111) crystal planes of CeO2, respectively, indicating that these were the primary exposed surfaces of the mesoporous CeO2-0[34].

    Figure 4

    Figure 4.  (a, b) TEM and (c, d) HRTEM images of CeO2-0

    Figure 5

    Figure 5.  (a, b) TEM images, (c) HRTEM images, and (d) EDX spectra of catalysts: (a1-d1) NC-W, (a2-d2) NC-E, (a3-d3) NC-B, and (a4-d4) NC-C

    Inset: elemental contents.

    TEM images of the catalysts in Fig.5a1 and 5b1 reveal significant agglomeration of particles in NC-W compared to the support, with sizes ranging from approximately 20 to 40 nm, consistent with XRD particle size analysis. Fig.5c1 showed NiO located at the interfaces between CeO2 particles. Combined with XRD analysis, this indicates that Ni species had entered the CeO2 lattice, leading to increased particle size. Fig.5a2 and 5b2 showed that NiO was uniformly dispersed throughout the NC-E sample. Furthermore, the HRTEM image in Fig.5c2 suggested that most NiO had entered the CeO2 channels and was confined within the mesopores. Fig.5a3 and 5b3 revealed that NC-B exhibited a worm-like mesoporous structure similar to the CeO2-0 support, with a uniform particle size distribution of approximately 8-13 nm. Fig.5c3 showed that NiO had extensively penetrated the support without causing agglomeration. Energy dispersive X-ray spectroscopy (EDX) analysis of the selected region in Fig.5d3 confirmed uniform Ni distribution on the CeO2-0 support. NC-C exhibited a uniform particle size distribution between 7-12 nm while maintaining an intact mesoporous structure (Fig.5a4 and 5b4). Fig.5c4 demonstrated uniform dispersion of NiO, attributed to more homogeneous atomic mixing achieved via the coprecipitation method. Fig.5d4 showed a surface Ni content (mass fraction) of only 2.80%, significantly lower than that of catalysts prepared by other methods (Fig.5d1-5d3), indicating substantial Ni dispersion within the support. Combined with H2-TPR results, it is evident that this Ni exhibits strong interactions with the support, with some Ni species likely incorporated into the CeO2 lattice.

    Catalytic activity tests for CO methanation were conducted at 0.6 MPa and a gas hourly space velocity (GHSV) of 10 000 mL·g-1·h-1. As shown in Fig.6, the preparation method significantly influenced catalyst activity. The impregnation-prepared catalysts NC-W and NC-E exhibited high CO conversion rate at 250 ℃ but demonstrated poor selectivity, attributed to their larger particle size. Nevertheless, NC-E showed superior activity to NC-W because the use of ethanol as a dispersant improved NiO dispersion compared to water, resulting in smaller particles and more exposed active sites. NC-B exhibited optimal low-temperature activity at 300 ℃, with CO conversion rate rapidly increasing from 14% to approximately 98%. It also demonstrates high CH4 yield and selectivity near 300 ℃. Analysis of its H2-TPR profile suggests that Ni species reduced at low temperatures are key to enhancing low-temperature activity. Literature reports also indicate that α-NiO reduced near 300 ℃ is the primary active component for low-temperature methanation[35]. However, as the temperature increased further, the activity of NC-B decreased significantly, likely due to weak Ni-support interactions leading to Ni sintering under high-temperature conditions. In contrast, NC-C exhibited superior activity above 500 ℃ compared to other catalysts. Combined with H2-TPR results, strong Ni-support interactions were evident in this catalyst. Furthermore, active sites can be replenished through the reduction of some framework NiO during the reaction. Consequently, the catalyst maintained good activity even under high-temperature conditions.

    Figure 6

    Figure 6.  Catalytic activities of catalysts: (a) CO conversion rates, (b) CH4 yields, and (c) CH4 selectivities

    To investigate the stability of catalysts prepared by different methods and clarify the role of the mesoporous structure, a reference catalyst, NC-1, with lower mesoporosity (65.08%), was prepared. Stability tests were conducted at 450 ℃, 0.6 MPa, and a GHSV of 10 000 mL·g-1·h-1. As shown in Fig.7a-7c, NC-B, NC-C, NC-W, and NC-E maintained stable CO conversion rate over 50 h, demonstrating good activity and stability. NC-1 showed a significant decline in both CO conversion rate and CH4 selectivity after approximately 30 h. Based on characterization results, it can be concluded that the confinement effect of the CeO2 mesoporous structure enhances the anti-sintering capability of Ni, effectively maintaining catalyst stability.

    Additionally, stability testing of NC-B was conducted at 300 ℃, 0.6 MPa, and a GHSV of 10 000 mL·g-1·h-1. Results in Fig.7d show that CO conversion rate remained around 98% with CH4 selectivity near 100% throughout the reaction, with no significant activity decline, indicating excellent stability under these conditions.

    Figure 7

    Figure 7.  Stability test of the catalysts: (a) CO conversion rates, (b) CH4 yields, and (c) CH4 selectivities; (d) Stability test of NC-B

    The XRD patterns of catalysts after 50 h of stability testing at 450 ℃ are shown in Fig.8a. Comparison with pre-reaction patterns reveals that after reaction, all catalysts exhibited faint diffraction peaks attributable to graphitic carbon. Among them, the spent NC-B catalyst showed the strongest carbon peak intensity, while support diffraction peaks were significantly weakened due to coking coverage. This indicates that catalysts prepared via the Ni sublimation method demonstrate relatively poor resistance to sintering and coking, attributed to weaker Ni-support interactions. In the spent NC-C and NC-E catalysts, almost no diffraction peaks for Ni or carbon deposits were detected. Based on previous analysis, these catalysts exhibited uniform Ni dispersion within the mesoporous structure or framework, with a significantly higher proportion of Ni exhibiting strong support interactions.

    Figure 8

    Figure 8.  (a) XRD patterns of spent catalysts; (b) TG curves (solid line) and DTG curves (dashed line) of the used NC-E and NC-1

    Analysis of the TG curve in Fig.8b reveals that the spent NC-E catalyst showed no weight loss across the temperature range, whereas the catalyst NC‑1 showed pronounced weight loss between 450-600 ℃. This indicates that the confinement effect of the mesoporous structure effectively suppresses sintering of active components and surface coking formation, thereby enhancing catalyst resistance.

    To evaluate long-term anti-coking performance, TEM analysis was conducted on the four catalysts after 50 h of stability testing, with the results shown in Fig.9. The size and distribution of Ni particles in each catalyst showed no significant changes after reaction, indicating structural stability and excellent sintering resistance during operation. This is primarily attributed to the spatial confinement effect provided by the mesoporous CeO2 support, which effectively suppresses Ni migration and agglomeration at elevated temperatures, ensuring structural integrity during long-term operation.

    Figure 9

    Figure 9.  (a) TEM and (b) HRTEM images of the spent catalysts: (a1, b1) NC-W, (a2, b2) NC-E, (a3, b3) NC-B, and (a4, b4) NC-C

    In this work, a mesoporous CeO2 support with a confined structure was prepared via hydrothermal synthesis. The effects of three Ni loading methods—incipient wetness impregnation, coprecipitation, and bis (cyclopentadienyl)nickel sublimation—on CO methanation performance were systematically compared. Results indicate that all catalysts exhibit excellent sintering resistance due to the support′s confinement effect. However, their coking resistance, catalytic activity, and stability significantly depend on Ni dispersion and metal-support interaction strength.

    Specifically, catalyst NC-B contained abundant weakly interacting NiO species. After reduction, it generated highly dispersed metallic Ni nanoparticles, providing more active sites. It exhibited optimal low-temperature activity, achieving ca. 98% CO conversion rate and ca. 100% CH4 selectivity at 300 ℃. Catalyst NC-E showed high activity and excellent coking resistance across a broad temperature range, owing to uniform Ni distribution within the pores and moderate support interaction. Catalyst NC-C maintained stable activity even at 550 ℃ because Ni is highly embedded into the CeO2 lattice, forming strong interactions. This study clarifies the intrinsic relationship between Ni loading method, Ni-based catalyst structure, and catalyst performance, laying a theoretical foundation for the rational design of high-performance Ni-based methanation catalysts.


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  • Figure 1  (a) Small-angle XRD pattern of CeO2-0 and (b) XRD patterns of the samples

    Figure 2  (a) N2 adsorption-desorption isotherms and (b) pore size distribution curves of the samples

    Figure 3  (a) H2-TPR curves of the catalysts; (b) Survey, (c) Ce3d, and (d) Ni2p XPS spectra of the catalysts

    Figure 4  (a, b) TEM and (c, d) HRTEM images of CeO2-0

    Figure 5  (a, b) TEM images, (c) HRTEM images, and (d) EDX spectra of catalysts: (a1-d1) NC-W, (a2-d2) NC-E, (a3-d3) NC-B, and (a4-d4) NC-C

    Inset: elemental contents.

    Figure 6  Catalytic activities of catalysts: (a) CO conversion rates, (b) CH4 yields, and (c) CH4 selectivities

    Figure 7  Stability test of the catalysts: (a) CO conversion rates, (b) CH4 yields, and (c) CH4 selectivities; (d) Stability test of NC-B

    Figure 8  (a) XRD patterns of spent catalysts; (b) TG curves (solid line) and DTG curves (dashed line) of the used NC-E and NC-1

    Figure 9  (a) TEM and (b) HRTEM images of the spent catalysts: (a1, b1) NC-W, (a2, b2) NC-E, (a3, b3) NC-B, and (a4, b4) NC-C

    Table 1.  Physicochemical properties of catalysts prepared by different loading methods

    Catalyst Crystallite size of CeO2/nm Mesoporous content/% SBETa/(m2·g-1) $ {n}_{C{e}^{3+}} $/($ {n}_{C{e}^{3+}} $+$ {n}_{C{e}^{4+}} $)/%
    CeO2⁃0 7.0 62.78 147
    NC⁃C 9.0 92.4 104 34.61
    NC⁃B 12.0 95.04 107 37.22
    NC⁃E 28.3 86.84 91 28.33
    NC⁃W 35.4 93.46 91 28.02
    NC⁃1 65.08 9
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  • 发布日期:  2026-05-10
  • 收稿日期:  2025-12-08
  • 修回日期:  2026-03-05
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