1. Introduction
Greenhouse gas emissions from fossil fuel combustion and industrial processes have emerged as a primary driver of the current environmental crisis. The increasing atmospheric concentration of pollutants such as carbon dioxide and methane results in a pronounced climate change. Addressing this crisis requires a transition to low-carbon energy systems combined with coordinated international policy efforts to ensure long-term environmental sustainability[
1]. This challenge has motivated the development of catalytic technologies designed to convert greenhouse gases into valuable chemical feedstocks. In this scenario, the dry reforming of methane (DRM: CH₄ + CO₂→2H₂ + 2CO) has attracted growing attention because it simultaneously consumes CH₄ and CO₂ to produce synthesis gas (CO + H₂), a key intermediate for downstream processes such as Fischer-Tropsch synthesis, methanol synthesis, and hydrocarbon upgrading[
2,
3]. However, the practical implementation of DRM faces significant challenges, including the high temperatures required to activate stable reactants and the catalysts deactivation through carbon deposition and metal sintering[
4,
5].
Nickel-based catalysts are widely regarded as the most economical and industrially viable materials for DRM, offering high intrinsic activity for C–H bond activation at a significantly lower cost than noble metals such as Ru, Rh, or Pt[
6]. Nevertheless, their application remains limited by rapid deactivation caused by carbon formation[
7], the growth and agglomeration of Ni nanoparticles, and interactions leading to inactive phases. To mitigate these issues, the development of advanced materials that can stabilize Ni particles, improve reducibility, and enhance coke resistance has become a key research focus[
8,
9,
10]. Among the reported catalytic systems for methane dry reforming, CeO₂ has emerged as a promising support for Ni active sites owing to its excellent redox properties and oxygen storage capacity, which promote the removal of carbon deposits, enhance catalyst stability, and mitigate coke formation[
11,
12,
13]. The Ce³⁺/Ce⁴⁺ redox cycle enables lattice oxygen to participate in the oxidation of CH₄, generating oxygen-deficient CeO₂₋ₓ species that can be reoxidized by CO₂, thus preserving the catalytic performance and extending the lifetime of the Ni/CeO₂ catalytic system.
Hybrid SiO₂-CeO₂ mixed oxides represent a particularly attractive support for Ni-based catalysts[
14,
15,
16]. Silica provides high surface area, thermal stability, and well-controlled porosity[
17,
18], while ceria contributes oxygen mobility and redox activity that facilitate carbon oxidation and CO₂ activation[
19]. The combination of these two oxides can therefore enhance nickel dispersion, strengthen metal-support interactions, and improve resistance to carbon deposition during DRM[
20,
21]. Importantly, both the ceria content and the support synthesis method significantly influence the physicochemical properties of SiO₂-CeO₂ systems, affecting parameters such as surface area, degree of Ni-support interaction, oxygen vacancy concentration, and reducibility[
22,
23,
24].
In this study, we systematically investigate the influence of CeO₂ content (5-30 wt%) and the support synthesis method (sol-gel vs. wetness impregnation) on the structural, textural, and catalytic properties of Ni/SiO₂-CeO₂ catalysts for methane dry reforming. SiO₂-CeO₂ composites were prepared using either sol-gel route or wetness impregnation, followed by the incorporation of nickel via wetness impregnation. Comprehensive physicochemical characterization, including X-ray diffraction (XRD), N₂ physisorption, and H₂ temperature-programmed reduction (H₂-TPR), was performed to elucidate structural evolution, porosity, and reducibility. Catalytic performance was evaluated between 450 and 800 °C using a CH₄/CO₂ mixture, and spent catalysts were examined by thermogravimetric analysis (TG) and XRD to evaluate carbon deposition and phase stability. By correlating preparation methods, ceria content, and reaction performance, this work provides new insight into the design of Ni-based catalysts with enhanced coke resistance and improved stability for DRM.
2. Results and Discussion
SiO₂-CeO₂ mixed oxides (SiCe) were developed as supports for Ni-based catalysts to be used in syngas production via methane reforming with carbon dioxide. These SiCe supports were designed to stabilize Ni dispersed nanoparticles, with enhanced catalytic activity and improved resistance to coke formation during high-temperature reforming process.
SiCe powders were synthesized using two distinct strategies: the sol-gel route (SiCe5-30-SG) and the wetness impregnation method (SiCe5,30-WI).
To investigate the influence of support composition, four SiCe materials with ceria contents of 5, 10, 20, and 30 wt% were synthesized using the sol-gel method. A pure SiO₂ support was also prepared both as a reference material and as the bare support for the synthesis of two additional SiCe supports with CeO2 contents of 5 and 30% by the wetness impregnation method (SiCe5-WI, SiCe30-WI).
The supported Ni catalysts (5 wt%), prepared by wetness impregnation of SiCe powders, were labeled as NiSi, NiSiCe5-SG, NiSiCe10-SG, NiSiCe20-SG, NiSiCe30-SG, NiSiCe5-WI, and NiSiCe30-WI.
Ni catalysts were analyzed by X-ray powder diffraction (
Figure 1) to investigate the structural properties. The recorded patterns of most samples display the characteristic reflections of CeO₂ at 28.5°, 33.0°, 47.5°, and 56.3° 2θ, assigned to the (111), (200), (220), and (311) planes of its fluorite-type cubic structure (ICSD No. 28753, space group
Fm–3m).
In contrast, when the sol-gel method was applied to prepare the material with the lowest CeO2 content, NiSiCe5-SG, the corresponding XRD pattern shows barely visible CeO₂ diffractions, suggesting the presence of ceria as highly dispersed phase as well as fine nanometric domains embedded within the amorphous silica network. The XRD patterns of the calcined catalysts clearly display NiO reflections consistent with ICSD reference No. 24018. The primary NiO peaks are detected at 37.2°, 43.3°, and 62.9° 2θ, corresponding to the (111), (200), and (220) planes, respectively. Interestingly, as the ceria content increases, these peaks become less intense and broader, indicating that NiO particles are more finely dispersed on the supports with higher CeO₂ loadings.
NiO mean crystal sizes were calculated by Scherrer equation, and the values are listed in
Table 1. An effect of the catalyst composition on the structural properties was observed. NiSi, without ceria, exhibits the largest NiO crystallite size (22.7 nm). With the incorporation of CeO₂ into the silica matrix a systematic reduction in NiO crystallite size was observed. At low ceria loadings (NiSiCe5-SG and NiSiCe10-SG), the NiO mean size decreases to approximately 17.0-16.6 nm, followed by a further reduction to 15.7 nm for NiSiCe20-SG. The smallest NiO crystallites (11.8 nm) were obtained for NiSiCe30-SG. This progressive decrease in NiO crystallite size suggests that the presence of ceria effectively inhibits NiO crystal growth, likely because of strengthened metal-support interactions and enhanced dispersion of Ni species promoted by CeO₂. A similar effect was registered also for the wet impregnated samples, NiSiCe5-WI, and NiSiCe30-WI, showing smaller and better dispersed NiO crystallites at higher CeO
2 loadings.
N₂ physisorption measurements were performed on the investigated catalysts to evaluate their textural properties, including specific surface area (SSA), pore volume and mean pore size (
Table 1). The specific surface area (SSA) of the catalysts differs significantly based on the CeO₂ content and the preparation method. The bare silica-supported catalyst (NiSi) shows a high surface area of 242 m²/g, a pore volume of 0.50 cm³/g, and a mean pore diameter of 16.4 nm. When CeO₂ is incorporated using the sol-gel method, there is a notable impact on the textural properties. At a low CeO₂ content (NiSiCe5-SG), the SSA increases to 310 m²/g; however, the pore volume decreases significantly to 0.16 cm³/g, and the mean pore diameter drops to 2.73 nm. This suggests the formation of a finer pore structure, likely due to the well-dispersed ceria within the silica matrix. When the CeO₂ content is increased further (NiSiCe10-30-SG), there is a gradual reduction in surface area and pore volume, accompanied by a slight increase in pore diameter at higher loadings. This likely indicates a modification of the pore structure or aggregation of the CeO₂ particles. On the other hand, catalysts prepared by wetness impregnation (NiSiCe5-WI and NiSiCe30-WI) maintain higher pore volumes (0.48-0.52 cm³/g) and larger pore sizes (14.9-17.7 nm), which reflects the preservation of the original silica pore structure. These findings suggest that the preparation method plays a significant role in the dispersion of CeO₂ and the resulting textural properties of the Ni/SiO₂-CeO₂ catalysts.
Hydrogen temperature-programmed reduction (H₂-TPR) analysis was performed on Ni-supported catalysts to investigate the effect of ceria content on the reducibility and Ni-support interactions. The observed features reflect the reduction of Ni²⁺ to Ni⁰ and Ce⁴⁺ to Ce³⁺ (
Figure 2) as confirmed by the experimental H₂ consumption values that are in agreement with full reduction of Ni
2+ to metallic Ni and reduction of Ce⁴⁺ to Ce³⁺, that completely occurs at ceria loadings ≤ 10 wt%.
NiO particles with moderate interaction with the support are reduced in the range of 300-400 °C, whereas NiO strongly interacting with the support occurs at higher temperatures. The TPR profile of NiSi shows broad asymmetric peaks centred at ~350 °C and ~600°C, whereas the high-temperature peak can be ascribed to the reduction of small NiO particles strongly interacting with the silica surface, which are difficult to reduce, while the low-temperature peak corresponds to larger NiO crystallites with weaker interaction, more characteristic of bulk NiO[
24,
25].
CeO₂-containing catalysts display further reduction features between 400 and 700 °C, which can be assigned to the reduction of surface and bulk ceria (Ce⁴⁺ → Ce³⁺).
The catalytic activity of the NiSiCe(5-30)-SG catalysts was evaluated in the dry reforming of methane (DRM) reaction under temperature-gradient conditions ranging from 450 to 750 °C (
Scheme 1,
Figure 3). The results indicate an increase in CH
4 conversion in the following order: NiSi > NiSiCe5-SG > NiSiCe20-SG > NiSiCe30-SG > NiSiCe10-SG.
The highest activity of NiSi can be related to the presence of NiO particles resulting in weaker metal-support interactions. These features allow more reducible Ni species, which improve the overall catalytic activity. A high catalytic activity was noted for the material with the lowest CeO₂ content NiSiCe5-SG. This could likely be attributed to the combination of well-dispersed ceria domains and the presence of moderately interacting NiO species, as indicated by H₂-TPR analysis. Additionally, the improved oxygen mobility linked to finely dispersed ceria may also facilitate enhanced carbon removal (see TGA profile,
Figure 4a), contributing to sustained catalytic activity.
As the CeO₂ content increases beyond 10 wt%, the catalytic activity decreases. This behaviour can be due to the stronger Ni-support interactions induced by ceria, which lead to the formation of highly stabilized and less reactive NiO species. These factors can limit the amount of active Ni⁰ available on the surface of the catalyst under reaction conditions. Interestingly, the NiSiCe30-SG catalyst performs better than NiSiCe20-SG for CO₂ conversion but shows slightly reduced performance in methane conversion. This suggests that oxygen mobility and CO₂ activation, both promoted by higher ceria contents, compensate partially for the stronger metal-support interaction at elevated CeO₂ loading.
The results demonstrate that the catalytic performance of the NiSiCe(5-30)-SG series is strongly influenced by the ceria content, which affects Ni dispersion, reducibility, and the extent of Ni-support interactions. Lower ceria contents promote, upon reduction, the formation of active Ni⁰ species while still providing enough redox functionality to assist in carbon removal. Higher ceria loadings likely promote strong interactions between oxidized NiO species and the ceria bulk, rendering the Ni active sites poorly accessible on the catalyst surface and consequently reducing catalytic activity.
Figure 3 (inset) reports the H
2/CO molecular ratio values as a function of temperature in the range 500-750 °C.
The H
2/CO values decreased with increasing temperature, dropping from above 2 at 500 °C to approximately 1-0.8 in the 650-750 °C range. The temperature-dependent evolution of the H₂/CO ratio can be attributed to the occurrence of additional reactions during the DRM test[
6]. Specifically, the exothermic Boudouard reaction (2CO ↔ C + CO
2), which is favored at lower temperatures, leads to CO consumption, and thus contributes to the higher H₂/CO ratio. In contrast, endothermic reactions such as the reverse Boudouard reaction and the reverse water-gas shift (RWGS) reaction (CO
2 + H
2 ↔ CO + H
2O) enhance CO formation at higher temperatures, thereby reducing the H₂/CO molar ratio[
6,
25,
26].
After DRM reaction, the spent catalysts were characterized by TGA and XRD analyses. The extent of carbon deposition on the spent NiSi and NiSiCe (5-30)-SG catalysts was determined by thermogravimetric (TG) analysis, as shown in
Figure 4a. The weight losses associated with carbon combustion ranged from approximately 18.5 wt% for NiSiCe5-SG to 2.8 wt% for the least active NiSiCe10-SG. Carbon oxidation occurred within the temperature range 586-703 °C, indicating, for NiSi, the coexistence of carbon species with different structural features (
e.g., amorphous carbon). These results highlight the correlation between catalytic performance and carbon formation.
According to the TG analysis, the XRD patterns of NiSiCe (5-30)-SG powders after DRM under a temperature gradient show a diffraction peak at 26.5° (2θ), corresponding to graphitic carbon (
Figure 4b). In addition, metallic nickel was clearly detected in the spent catalysts, identified by the (111), (200), and (220) reflections at 2θ = 44.4°, 51.8°, and 76.3°, respectively. The absence of CeO₂ diffraction peaks after DRM was observed for all the samples and has also been reported in the literature for Ni/SiO₂–CeO₂ catalysts[
27,
28]. This result was ascribed to the catalyst reduction pre-treatment at 750 °C under 5% H₂/He carried out before DRM test. The reducing atmosphere induced Ce⁴⁺ → Ce³⁺ reduction and the formation of oxygen vacancies, disrupting the long-range crystallinity of the fluorite structure.
Given the high catalytic activity of NiSi observed during the DRM carried out at gradient temperature, together with the limited extent of carbon deposition, a long-term stability test was conducted at 700 °C for 24 h after prior reduction at 750 °C for 1 h under a flow of 5% H₂/He. As shown in
Figure 5, both CH₄ and CO₂ conversions exhibit a slight increase during the initial hours on stream, followed by stable values over the entire 24 h time-on-stream test. CO
2 conversion values were higher than those recorded for CH
4. This behaviour is consistent with the literature and can be explained by the occurrence of the reverse water gas shift reaction (RWGS: CO
2 + H
2 ↔ CO + H
2O)[
25].
CO₂ conversion rapidly reaches approximately 70% and remains essentially constant thereafter, indicating steady catalytic performance. Likewise, CH₄ conversion increases to about 55% in the early stage of the reaction and subsequently stabilizes, with no evidence of deactivation. The absence of any progressive decline in conversion for either reactant points to good catalyst stability under the investigated conditions and is consistent with the limited carbon deposition observed during the test at gradient temperature.
In order to verify the hypothesis that NiSiCe-SG catalysts exhibit lower activity than the corresponding NiSi sample due to the strong Ni-CeO₂ interaction, the catalyst with the highest ceria content, NiSiCe30-SG, was subjected to a redox treatment (TPR-TPO-TPR). In details, after a first TPR, the sample was oxidized from room temperature up to 600 °C (hold time 1h) using a 5% O₂/He mixture (v/v, 30 mL/min), then cooled to room temperature under helium and, finally, a second TPR was registered. This procedure was carried out to investigate changes in the reducibility of oxidized Ni species. In
Figure 6a, the second reduction profile was compared with the first one, already shown in
Figure 2. An evident change of the second reduction profile of NiSiCe30-SG was registered in comparison with the first TPR. After the redox treatment (TPR-TPO-TPR), the second H₂-TPR profile shows a marked shift of the main reduction feature toward lower temperatures, with the maximum now centered around 450-500 °C and a narrower distribution of reduction peaks. This behavior suggests a partial weakening of the metal-support interaction and an increased fraction of more easily reducible Ni
2+ and Ce
4+ species formed upon reoxidation. The enhanced reducibility, observed in the second TPR, indicates that the redox cycling modifies the nature of the Ni species, likely promoting changes at the Ni-CeO₂ interface, which may have implications for the catalytic performance of the NiSiCe30-SG system. Based on the so far reported results, a fresh portion of the NiSiCe30-SG catalyst was subjected to a first reduction at 750 °C for 1 h under 5% H₂/He, then after cooling to room temperature under inert gas, the sample was oxidized at 600 °C 1h, therefore, again reduced at 750 °C 1h. The long-term stability test was finally carried out at 700 °C for 24 h (
Figure 6b). Both reactants, CH₄ and CO₂, exhibit relatively high initial conversions, followed by a rapid decline during the first few hours on stream. CO₂ conversion decreases sharply from its initial value to approximately 40-45% within the first 2-3 h, whereas CH₄ conversion shows an even more pronounced early drop, falling from about 55-60% to below 30% over the same period.
The initially high activity indicates that the second reduction treatment is beneficial for the reorganization of the Ni active sites, which are likely more dispersed and more accessible on the catalyst surface. However, the catalyst undergoes rapid deactivation within the first 1-2 h, probably due to modifications of the active sites, such as metal sintering, which affect CH₄ activation more severely than CO₂ activation. After this transient period, both conversion curves gradually approach a quasi-steady state. Between approximately 6 and 24 h on stream, CO₂ conversion stabilizes at around 23-27%, while CH₄ conversion levels off at lower values, ca. 14-17%. Throughout the entire test, CO₂ conversion remains consistently higher than that of CH₄, in agreement with previous observations (see
Figure 3 and
Figure 5). In the
Figure 6b (inset), the CH₄ and CO₂ conversion profiles recorded at 700 °C over the same NiSiCe30-SG catalyst after a single reduction treatment at 750 °C, are displayed during the first 5 h of reaction. This behavior confirms the poor catalytic activity previously observed under temperature-programmed conditions. In this case, CO₂ conversion decreases modestly from ~15% to ~10% within the first hour and then remains nearly constant, whereas CH₄ conversion stays close to ~5% over the entire 5 h interval.
The influence of the support synthesis method on the catalytic performance was evaluated for NiSiCe5-WI and NiSiCe30-WI catalysts by performing gradient temperature tests between 450 °C and 750 °C. For reference, the catalytic results of the corresponding sol-gel (SG) samples (Figure 3) are included in Figure 7a, providing a comprehensive comparison of all catalysts prepared from SiCe supports with 5 wt% and 30 wt% ceria. Both NiSiCe5-WI and NiSiCe30-WI exhibit higher CH₄ conversions than NiSi and the NiSiCe(5-30)-SG samples, with NiSiCe5-WI achieving the highest conversion. The H
2/CO values for both the NiSiCe-WI catalysts lie between 0.7 and 0.8 in the 500–700 °C range, remaining lower than those of the SG series samples. At 750 °C, the curves intersect those of NiSi and the NiSiCe-SG at the same value of 1 (see inset,
Figure 7a).
The spent NiSiCe5,30-WI catalysts were subsequently characterized by XRD and TG analyses, which revealed the presence of carbon deposits (
Figure 7b and
Figure 8b). The XRD patterns again displayed the main diffraction peak of graphitic carbon, while CeO₂ diffraction peaks were not detected, according with previous findings.
Based on these findings, the catalytic stability of NiSiCe5-WI and NiSiCe30-WI was further assessed in a 24 h DRM test at 700 °C (
Figure 8a). NiSiCe5-WI exhibited the highest activity, achieving initial CH₄ and CO₂ conversions of 85% and 79%, respectively. These values exceed those obtained under gradient temperature conditions by 39% and 14%, respectively (
Figure 7a), indicating that NiSiCe5-WI performs efficiently at 700 °C during long-term conditions.
Raman spectra of the as-prepared and spent NiSiCe5,30-SG and NiSiCe5,30-WI catalysts were recorded to investigate additional structural features (
Figure 9), complementing the XRD findings. For all samples, the resulting spectra exhibit a peak centered at 483 cm
-1, which is ascribed to the stretching vibration of Si-O-Si bonds[
29].
For the spent catalysts, the intensity of this peak is markedly reduced, suggesting partial coverage or blockage of the silica framework. This effect could be likely caused by carbon deposition formed during the DRM reactions, which can hinder the detection of Si–O–Si vibrations and may also affect the structural integrity and accessibility of the active sites. The F
2g vibration mode of the CeO₂ fluorite structure was clearly detected at ~462 cm⁻¹ for the as-prepared NiSiCe5-WI and NiSiCe30-SG. The sharper peak observed for the as-prepared NiSiCe5-WI is consistent with its higher crystallinity[
30], which can be attributed to the synthesis method. In contrast, the F
2g peak was not detected in the NiSiCe5-SG analogue, reflecting the highly dispersed and poorly crystalline nature of CeO₂ resulting from the sol-gel synthesis of the bare SiCe5-SG support.
Consistently with the XRD analysis, the characteristic F₂g Raman mode of CeO₂ is not clearly detected in the spent catalysts after DRM, which may be attributed to the combined effects of carbon deposition and a reduction in the long-range order of ceria domains during reaction. The D₁ bands observed in the 500-600 cm⁻¹ range are ascribed bulk oxygen vacancies (O
v-b) in the ceria fluorite structure[
31]. These bands reflect the presence of local structural defects in CeO₂, which are likely related to the presence of Ce³⁺ species. Moreover, the D₁ band of the spent catalysts appears more pronounced than in the corresponding as-prepared samples, indicating that DRM conditions induce additional oxygen vacancies and structural disorder. Qualitatively, while the F
₂g band of CeO₂ reflects the long-range fluorite order, the relative prominence of the D₁ band in the spent samples suggests an increase in defect density. Among the catalysts studied, NiSiCe5 WI exhibits the strongest D₁ signal, consistent with a higher concentration of bulk oxygen vacancies, which may contribute to its superior catalytic performance[
32].
Raman spectroscopy was also employed to elucidate the nature and structural order of the carbon deposits on the spent catalysts after DRM focusing on the 1260-1680 cm
-1 Raman shift range (
Figure 10). The spectra of the spent catalysts exhibit the characteristic G band at ~1588 cm⁻¹, associated with the
E2g vibration of sp² carbon, and the D band at ~1309-1352 cm⁻¹, which becomes active in the presence of defects or structural disorder. The I
D/I
G ratio was calculated to assess the degree of disorder versus graphitization in the deposited carbon, as it is widely used to quantify the structural quality of sp² carbon materials[
33,
34].
Higher values denote a more defective carbon network, whereas lower ratios indicate increased ordering. The catalysts recovered after the temperature-gradient test exhibit ID/IG values of NiSiCe5-WI (1.21) > NiSiCe30-SG (1.17) > NiSiCe5-SG (1.14) > NiSiCe30-WI (1.10), indicating that NiSiCe30-WI accumulates the most graphitized carbon. After the long-term stability test, the Iᴅ/Iɢ values converge (1.06 for NiSiCe5-WI and 1.05 for NiSiCe30-WI), suggesting that extended operation promotes the formation of similarly ordered carbon species.