1 Introduction

Global warming continues to drive the scientific community towards catalytic solutions aimed at converting greenhouse gases into non-greenhouse gases. In this endeavor, the process of dry reforming of methane (DRM) emerges as a particularly insightful and valuable approach. In the current landscape, there exists a repertoire of both novel and established metal-based catalysts (such as Pt, Pd, Rh, Ru, Co and Ni) that hold the potential to effectively convert greenhouse gases like CO2 and CH4 into syngas, utilizing both thermal and non-thermal processes [1, 2]. Among these catalysts, those based on low-cost active sites, particularly Ni, hold substantial promise. Notably, Ni demonstrates an interaction energy with CH4 that is 25 times higher than that of Co [3, 4], rendering it a particularly attractive choice for catalytic applications in this context.

The active site Ni plays a crucial role in achieving effective dispersion and stabilization over appropriate support, particularly under the conditions of high-temperature DRM reactions. The choice of support material also significantly influences the catalytic performance of Ni. For instance, Ni supported on materials like titania, magnesia, alumina and zirconia exhibits a stronger interaction between the metal and the support, in comparison to Ni supported on silica, yttria, and ceria catalysts [5,6,7]. The formation of a metal support interface by NiO-MgO solid solution was frequently reported even at the lowest MgO loading [8]. Reduction of NiO-MgO under hydrogen surges small and stable Ni crystallites [9]. Further surface basicity and small dispersed Ni crystallites make NiO-MgO based catalyst a potential DRM catalyst with strong inhibition of carbon deposit [10]. Alumina-supported Ni catalyst has high thermal sustainability and great holding capacity of Ni [11, 12]. Zirconia-supported Ni catalyst has drawn the interest of the catalyst community due to the presence of dual acid–base sites, redox capability and maintaining high H2/CO ratio (> 0.9) during DRM [13,14,15]. However, there are certain limitations associated with supported Ni catalysts. For instance, when Ni is supported on titania, the catalyst may encounter issues such as phase transitions in TiO2 phases and reduced activity in DRM due to partial coverage of active Ni sites by titania [16]. Similarly, when Ni is supported on MgO, challenges arise at higher calcination or pretreatment temperatures (> 700 °C) where the 5NiO-MgO solid solution becomes less reducible, resulting in larger Ni particle sizes and subsequent sintering [17, 18]. The activity of Ni catalysts supported on alumina could be hindered by factors such as limited diffusion of catalytically active Ni species within the alumina lattice, surface acidity and substantial coke deposition [19, 20]. Moreover, zirconia-supported Ni catalysts could face significant phase transitions of the zirconia phase at elevated DRM temperatures [21, 22].

At this point, two distinct approaches can be pursued. The first involves the addition of a small quantity of a second metal oxide (promoter) to the supported Ni catalyst, which significantly enhances its catalytic activity for DRM. However, this approach necessitates a precise synthetic strategy to achieve optimal loading, ensuring that the promoter does not obstruct the active catalytic sites. The second route involves utilizing a dual metal oxide support, thereby leveraging the strengths of each metal oxide to overcome any limitations inherent to the other. Among the options of titania, MgO, alumina and zirconia as supports, MgO stands out due to its cost-effectiveness.

In this context, we have prepared a support comprising 80wt% MgO combined with 20wt% of another metal oxide, chosen from among alumina, zirconia and titania. Each of these components possesses unique attributes; titania exhibits both rutile and anatase phases and is redox and acidic in nature, ZrO2 displays both monoclinic and tetragonal phases and is redox and neutral, while Al2O3 is non-reducible but characterized by its acidic properties. The notable drawback of magnesia-supported Ni catalysts lies in their inferior reducibility and sintering susceptibility at elevated temperatures. Hence, investigating the role of a suitable metal oxide co-support that can compensate for MgO’s limitations in the support becomes an intriguing path of exploration. Consequently, Ni dispersed over dual supports (MgO + TiO2, MgO + Al2O3, MgO + ZrO2) has been thoroughly examined for its performance in the DRM reaction. The investigation employs various characterization techniques, including X-ray diffraction (XRD), surface area and porosity analysis, RAMAN spectroscopy, transmission electron microscopy, temperature-programmed reduction/desorption/oxidation and thermogravimetric analysis. The thorough evaluation of the most synergistic metal oxide to complement MgO as a support for the Ni catalyst in DRM promises to deliver profound insights. The robust data correlations established herein are poised to significantly advance the development of a catalyst that holds the potential to be both economically viable and effective for large-scale DRM applications within the industrial domain.

2 Experimental

2.1 Material

Nickel nitrate hexahydrate [Ni (NO3)2.6H2O, 98%, Alfa Aesar], γ-Al2O3 (Norton chemical process Product Corp, Ohio, USA), ZrO2 (Daiichi Kigenso Kagaku Kogyo Co-LTD, Japan), TiO2 (Aeoxide TiO2 P25, Evonik Industries, Essen Germany) and SiO2 (SoSal, Hamburg, Germany). MgO from BDH.

2.2 Catalyst Preparation

80wt% MgO + 20wt%MOx (M = Al, Zr, Ti) mixed oxide supports were prepared by mixing appropriate amounts of metal oxides and then after calcining for 5 h at 600 °C. 5wt% Ni loading was introduced by impregnating Ni (NO3)2·6H2O solution over MgO + MOx (M = Al, Zr, Ti) support under stirring conditions. The prepared paste was dried at 120 °C for 20 h and then calcined for 5 h at 600 °C. The catalyst is abbreviated as 5Ni/MgO, 5Ni/MgO + Al2O3, 5Ni/MgO + TiO2, 5Ni/MgO + ZrO2.

2.3 Catalyst Characterization

Transmission electron microscopy (TEM), X-ray diffraction (XRD), Raman spectroscopy, H2 temperature-programmed reduction (H2-TPR), CO2 temperature-programmed desorption (CO2-TPD) and Thermogravimetric analysis (TGA) were used to characterize the catalysts. The Supporting Information (S1) provides a thorough explanation of the instruments and the characterization process.

2.4 Catalyst Activity Test

The dry reforming of the methane reaction was conducted in a stainless-steel fixed tube reactor (PID Eng. and Tech Micro Activity Reference, 9.1 mm internal diameter. and 30 cm length) over 0.1 g catalysts at 700 °C under 1 atm pressure. An axially positioned K-type (stainless sheathed) thermocouple monitors the catalyst bed temperature. Prior to the catalytic experiments, the catalyst is reduced at 600 °C for 60 min under H2 (flow rate of 20 mL/min). The packed reactor was fed a mixture of gases in the proportions of 3:3:1 CH4/CO2/N2, with a volume flow rate of 70 mL/min and an hourly gas velocity of 42,000 mL/gcat. h. The product gas stream was examined using a GC (GC-2014 Shimadzu, columns: Porapak Q and Molecular Sieve 5A) equipped with a thermal conductivity detector. H2 yield percent and CO yield percent are calculated from the following formula.

$${\text{H}}_{2} {\text{Yield }}\% = \frac{{\left( {{\text{n}}_{{{\text{H}}_{2} }} } \right)_{{{\text{out}}}} }}{{2 \times \left( {{\text{n}}_{{{\text{CH}}_{4} }} } \right)_{{{\text{in}}}} { }}} \times 100$$
$${\text{CO Yield }}\% = \frac{{\left( {{\text{n}}_{{{\text{CO}}}} } \right)_{{{\text{out}}}} }}{{\left( {{\text{n}}_{{{\text{CH}}_{4} }} } \right)_{{{\text{in}}}} { } + \left( {{\text{n}}_{{{\text{CO}}_{2} }} } \right)_{{{\text{in}}}} { }}} \times { }100$$

where, \({({{\text{n}}}_{{{\text{H}}}_{2}})}_{{\text{out}}}\) is Mole of H2 in product (outlet), \({({{\text{n}}}_{{{\text{CH}}}_{4}})}_{{\text{in}}}\) is mole of CH4 in inlet, \({({{\text{n}}}_{{\text{CO}}})}_{{\text{out}}}\) is mole of CO in product (outlet) and \({({{\text{n}}}_{{\text{CO}}})}_{{\text{in}}}\) is mole of CO2 in inlet.

3 Results and Discussion

3.1 Characterization Results and Discussion

N2 adsorption isotherm, porosity distribution profiles and surface parameters of the 5Ni/MgO and 5Ni/MgO + MOx (M = Al, Zr. Ti) catalysts are shown in Fig. 1. All catalysts exhibit a type IV isotherm with an H1 hysteresis loop, confirming the presence of mesopores [23] (Fig. 1a–d). Notably, the incorporation of 20wt% ZrO2 to MgO results in a slightly lower surface area, pore olume and pore diameter for the 5Ni/MgO + ZrO2 catalyst than 5Ni/MgO catalyst, whereas the incorporation of 20wt% TiO2 along with MgO leads to a marginally higher surface area for the 5Ni/MgO + TiO2 catalyst compared to the 5Ni/MgO catalyst (Fig. 1e). The use of 20wt% alumina combined with 80wt% magnesia as a support is particularly noteworthy. The 5Ni/MgO + Al2O3 catalyst demonstrates a surface area that is 1.5 times higher and a relatively greater pore volume than that of the 5Ni/MgO catalyst. The rise in surface area after calcination in 5Ni/MgO + Al2O3 may be attributed to acid–base interaction of Al2O3-MgO, dispersion of acidic oxide Al2O3 over basic oxide MgO and loss of dangling hydroxyls [24, 25]. The distribution of pore sizes across the catalyst surface is depicted through the dV/dlogW versus W plot. Remarkably, the majority of pores observed in the 5Ni/MgO + Al2O3 catalyst have a size of 145 nm, which surpasses that of the other catalysts.

Fig. 1
figure 1

ad N2 adsorption isotherm and porosity distribution profiles (inset) of 5Ni/MgO and 5Ni/MgO + MOx (M = Al, Zr. Ti) catalysts. e The surface area, pore volume and pore diameter of 5Ni/MgO and 5Ni/MgO + MOx (M = Al, Zr. Ti) catalysts

The X-ray diffraction patterns of Ni/MgO and Ni/MgO + MOx (M = Al, Zr. Ti) catalysts are presented in Fig. 2. The diffraction patterns for the magnesia-supported Ni catalyst and the 5Ni/MgO + Al2O3 catalyst are identical (Fig. 2a). The Ni/MgO catalyst exhibits diffraction peaks corresponding to the cubic MgNiO2 phase (at Bragg’s angle 2θ = 36.8°, 42.7°; JCPDS reference number: 00-024-0712) and cubic MgO phase (at 2θ = 36.8°, 42.7°, 62.1°, 74.5°, 78.43°; JCPDS reference number: 01-075-0447). In the literature, cubic NiO peaks were reported at about 37.2° and 43.28°. In the case of the formation of NiO-MgO solid solution, the diffraction pattern about 43.28° is shifted to a lower angle (43.12°) [26]. Here, the diffraction pattern of the Ni/MgO catalyst is shifted to more lower angle (42.7°), indicating a proper mixing of cubic NiO and cubic MgO phase and the organization new cubic MgNiO2 phase. Intriguingly, upon introducing 20wt% alumina along with 80% magnesia in support, the intensity of diffraction patterns decreases and shifts to a lower Braggs’ angle. This shift indicates reduced crystallinity and an expansion of the cell parameter in the 5Ni/MgO + Al2O3 catalyst (Fig. 2b). Remarkably, the phases related to Al2O3 and NiAl2O4 that are typically observed in alumina-nickel-based catalyst systems are obviously absent. This phenomenon may be attributed to the diminished acid profile of alumina caused by basic MgO, which potentially hinders the formation of alumina-related phases [27]. Fahad et al. also found the loss of crystallinity upon dignifying the acid profile of alumina by basic lanthana [20]. Here also, the acid profile of alumina may also be diminished with basic MgO, which may retard the formation of alumina-related phases.

Fig. 2
figure 2

X-ray diffraction profile of a 5Ni/MgO and 5Ni/MgO + Al2O3 catalyst, b 5Ni/MgO and 5Ni/MgO + MOx (M = Al, Zr. Ti) catalysts, c 5Ni/MgO + ZrO2 catalyst, d 5Ni/MgO + TiO2 catalyst

Furthermore, the addition of 20wt% titania alongside 80% magnesia leads to a further decrease in the crystallinity of the 5Ni/MgO + TiO2 catalyst, coupled with a shift to a relatively higher Bragg’s angle (Fig. 2e). This shift indicates partial contraction within the crystals. Previously, the calcination temperature above 500 °C was reported for the formation of NiTiO3 phases over titanium and Ni-based material [28]. Here also, along with cubic MgNiO2 phase and MgO phases, 5Ni/MgO + TiO2 has additional peaks for rhombohedral NiTiO3 phase (at Bragg’s angle 2θ = 24.1°, 33°, 35.7°, 40.9°, 49.4°, 54.01°, 62.45°, 64.07°; JCPDS reference number: 00-033-0960). The 5Ni/MgO + TiO2 catalyst is also populated by rutile TiO2 phase (at 2θ = 27.5°, 36.1°, 41.3°, 54.4°, 56.7°, 69.1°; JCPDS reference number: 01-073-1765) and anatase TiO2 phase (at 2θ = 25.36°, 37.9, 48.1°, 54°, 55.2°; JCPDS reference number: 01-073-1764). Raman band of 5Ni/MgO + TiO2 also confirms the presence of anatase TiO2 phase (Raman band at 399 cm−1 (B1g), 518 cm−1 (B1g) and 639 cm−1 (Eg)) and rutile phase (Raman band at 447 cm−1 (Eg)) [29] (Fig. S3a). Interestingly, NiTiO3 phase is observed in XRD but not in Raman results. It has been previously reported that the crystallization of NiTiO3 initiates at 550–600 °C, while the ordering of the short-range NiTiO3 structure begins at 650–700 °C [30, 31]. In our catalyst synthesis procedure, the calcination temperature is set at 600 °C. As a result, the rhombohedral NiTiO3 phase is detectable through XRD but not through Raman spectroscopy. Upon the incorporation of 20wt% ZrO2 along with 80% alumina support, the intensity of the diffraction peaks corresponding to the cubic MgNiO2 phase and cubic MgO phases is minimized in the 5Ni/MgO + ZrO2 catalyst (Fig. 2c). Additionally, the 5Ni/MgO + ZrO2 catalyst exhibits new diffraction peaks for monoclinic ZrO2 (at 2θ = 24.1°, 28.2°, 31.5°, 34.2°, 35.3°, 49.3°, 50.2°; JCPDS reference number: 00-007-0343). The monoclinic zirconia phase is further validated by the presence of characteristic Raman bands at 179 cm−1, 379 cm−1, 476 cm−1, 536 cm−1, 559 cm−1, 610 cm−1 and 636 cm−1 [32,33,34] (Fig. S3b).

The H2-temperature programmed reduction profiles of 5Ni/MgO and 5Ni/MgO + MOx (M = Al, Zr. Ti) catalysts are shown in Fig. 3a. The MgO-supported Ni catalyst reducibility pattern can be broadly categorized into two regions. Firstly, a broad reduction peak is observed below 600 °C, attributed to reducible NiO interacting with support with moderate strength. Secondly, another broad peak is evident above 600 °C, corresponding to reducible NiO exhibiting a strong interaction with the support [35]. Previously, the peak of about 800 °C was reported for the reduction of Ni+2 located in the subsurface layer of MgO. It shows a very strong interaction between NiO and MgO [10]. XRD results show the presence of MgNiO2 phase where Ni+2 is in very strong interaction with MgO. So, the peak in the higher temperature (~ 800 °C) can be attributed to the reduction of Ni+2 from the MgNiO2 phase.

Fig. 3
figure 3

a H2-temperature programmed reduction of 5Ni/MgO and 5Ni/MgO + MOx (M = Al, Zr. Ti) catalysts. b CO2-temperature programmed desorption of reduced-5Ni/MgO and reduced-5Ni/MgO + MOx (M = Al, Zr. Ti) catalysts. c cyclic H2TPR-CO2TPD-H2TPR profile of 5Ni/MgO. d cyclic H2TPR-CO2TPD-H2TPR profile of 5Ni/MgO + Al2O3. e cyclic H2TPR-CO2TPD-H2TPR profile of 5Ni/MgO + TiO2. f reducibility profile after sequential treatment with oxidizing and reducing gas of 5Ni/MgO and 5Ni/MgO + MOx (M = Al, Zr. Ti) catalysts

Remarkably, when the catalyst support includes 20wt% ZrO2 and 80wt% MgO, the intensity of both reduction peaks is notably decreased in the 5Ni/MgO + ZrO2 catalyst. Conversely, with the incorporation of 20wt% alumina alongside magnesia in the support, the intensity of the first reduction peak is diminished, while the second reduction peak is evidently intensified and broadened in the 5Ni/MgO + Al2O3 catalyst. This observation implies the prevalence of a higher concentration of “strongly interacted NiO species” over the 5Ni/MgO + Al2O3 catalyst compared to both the 5Ni/MgO + ZrO2 and 5Ni/MgO catalysts. Additionally, the 5Ni/MgO + TiO2 catalyst displays an additional distinct reduction peak at 655 °C, corresponding to the reduction of NiTiO3 [28]. This observation is consistent with the detection of the NiTiO3 phase in XRD analysis for the 5Ni/MgO + TiO2 catalyst.

In this context, the catalyst is subjected to reduction prior to the DRM reaction, ensuring that the catalyst’s surface exclusively presents active sites for CH4 decomposition. Furthermore, the basicity of the reduced catalyst surface plays a pivotal role in its potential interaction with CO2. Hence, after comprehending the reducibility profile of the catalyst, it becomes essential to delve into its basic profile subsequent to reduction. To achieve this, a CO2-temperature programmed desorption (CO2-TPD) analysis of the reduced catalyst is conducted and depicted in Fig. 3b. The basic profile of the reduced catalyst is summarized into three distinct regions. Peaks appearing at around 150, 280 and 560 °C correspond to the interaction of CO2 with weak basic sites (associated with surface hydroxyl groups) [36, 37], moderate-strength basic sites (involving surface oxygen anion) [35, 38] and strong basic sites, respectively [39, 40]. It is worth noting that the CO2-TPD profile of the reduced 5Ni/MgO + Al2O3 catalyst exhibits a subtle shift towards relatively lower temperatures.

NiO undergoes a transformation upon reduction into metallic Ni, providing the active sites for the subsequent DRM reaction. During this process, CH4 is decomposed into CHx and H2 over the metallic Ni sites, while CO2 ideally oxidizes CHx species. Over time, as the reaction progresses within the catalyst chamber, both oxidizing CO2 gas and reducing H2 gas (a product of the DRM reaction) are present. This dynamic interplay of CO2 and H2 can potentially lead to modifications in the concentration and strength of active sites, primarily the metallic Ni species. To gain deeper insights into the exact nature of the active sites under oxidizing and reducing gas environments, we have conducted cyclic sequential experiments involving hydrogen temperature-programmed reduction (H2-TPR), CO2 temperature-programmed desorption (CO2-TPD) and another H2-TPR step (Figs. 3c–e, S4). In this sequential experiment, the catalyst is initially reduced under H2 (H2-TPR), followed by an oxidative step under CO2-TPD. Subsequently, the catalyst is subjected to another H2 environment for potential re-reduction (H2-TPR).

Through this sequential treatment involving reducing and oxidizing gases, a notable shift in the reducibility pattern of all catalysts towards the 200–300 °C range is observed. This shift indicates that the catalysts exhibit enhanced reducibility under the influence of the oxidizing/reducing gas mixture that is characteristic of the DRM reaction. This suggests that the active sites on the catalyst are readily accessible even at relatively lower temperatures under these oxidizing and reducing conditions. Furthermore, the intensity of this reduction peak follows the order: 5Ni/MgO + Al2O3 > 5Ni/MgO + TiO2 > 5Ni/MgO + ZrO2 > 5Ni/MgO (Fig. 3f). Remarkably, the reducibility pattern of 5Ni/MgO + Al2O3 under oxidizing and reducing gas environments stands out with a single intense reduction peak observed at 244 °C. This contrasts with the other catalysts, which exhibit split peaks at the same temperature. This unique pattern points to the presence of a specific type of active site on the 5Ni/MgO + Al2O3 catalyst under oxidizing and reducing gas conditions.

During the DRM reaction, the CHx species oxidation delay can lead to carbon deposit accumulation on the catalyst surface. The extent of carbon deposition that can be oxidized by oxygen is reflected in the weight loss profiles of the spent catalysts under thermogravimetry analysis (Fig. 4a). Notably, the 5Ni/MgO + TiO2 catalyst exhibits a substantial weight loss of approximately ~ 74%, indicating a significant presence of active carbon or oxidizable carbon deposits. In contrast, the remaining catalysts show weight losses ranging from 11 to 13%, suggesting lower levels of carbon deposits. It is worth noting that the 5Ni/MgO + TiO2 catalyst might also contain inert carbon species that remain unoxidized during the TGA analysis.

Fig. 4
figure 4

a Thermogravimetry analysis of spent-5Ni/MgO and spent-5Ni/MgO + MOx (M = Al, Zr. Ti) catalysts. b Raman spectra of spent-5Ni/MgO and spent-5Ni/MgO + MOx (M = Al, Zr. Ti) catalysts

To delve deeper into the characteristics of the carbon deposits, Raman spectra of the spent catalysts were recorded (Fig. 4b). In Raman spectra, the wavenumbers at 1340 + 5 cm−1 and 1570 + 10 cm−1 correspond to the disordered/amorphous/defective carbon (D band) and well-ordered/graphitic carbon (G band), respectively [41]. Additionally, the 2D band is observed at 2673 cm−1 [42]. All these three bands are evident in the case of the spent 5Ni/MgO catalyst. Upon incorporating 20wt% titania with 80wt% MgO in support, the spent-5Ni/MgO + TiO2 catalyst exhibits notably higher intensities for these bands. This indicates that the spent-5Ni/MgO + TiO2 catalyst has the highest amount of disordered/defective and ordered/graphitic carbon deposits.

Upon incorporating 20wt% ZrO2 along with 80wt% MgO in support, the Raman peak intensity decreases compared to the spent 5Ni/MgO + TiO2. Notably, a new peak around 2218 cm−1 emerges in the Raman spectrum of the spent 5Ni/MgO + ZrO2 catalyst. In literature, the stretching mode of sp3-carbon (without hydrogen) has been reported at ~ 2200 cm−1 [43]. A more diverse array of carbon deposits is observed when Ni is supported over a catalyst comprising 20wt% alumina and 80wt% magnesia. The Raman band intensity associated with the peak mentioned above is lower for the spent 5Ni/MgO + Al2O3 than the spent 5Ni/MgO + ZrO2 catalyst. Intriguingly, two new Raman bands, at approximately 1690 cm−1 and 2092 cm−1, are also observed over the spent 5Ni/MgO + Al2O3 catalyst. Raman bands within the 1690–2150 cm−1 range are associated with the presence of non-suspended commensurate, incommensurate (folded) and suspended graphene layers [44].

The Energy Dispersive X-ray (EDX) spectra of 5Ni/MgO and 5Ni/MgO + MOx (M = Al, Zr. Ti) catalysts are shown in Fig. S5. Upon using dual metal oxide supports, the surface enrichment of Ni atoms are recognized over 5Ni/MgO + MOx (M = Al, Zr. Ti) catalyst than 5Ni/MgO catalyst. Out of all the catalysts, the 5Ni/MgO + Al2O3 catalyst has the highest Ni enrichment on its surface. The TEM image of both the fresh 5Ni/MgO + Al2O3 and spent catalyst are shown in Fig. 5. Notably, the average particle size has increased to 4 nm in the spent 5Ni/MgO + Al2O3, compared to the initial size of 3.7 nm observed in the fresh 5Ni/MgO + Al2O3 catalyst.

Fig. 5
figure 5

a TEM image of 5Ni/MgO + Al2O3 at 100 nm scale. b TEM image of 5Ni/MgO + Al2O3 at 50 nm scale. c Particle size distribution of Ni over 5Ni/MgO + Al2O3. d TEM image of spent 5Ni/MgO + Al2O3 at 100 nm scale. e TEM image of spent-5Ni/MgO + Al2O3 at 50 nm scale. f Particle size distribution of Ni over spent-5Ni/MgO + Al2O3

3.2 Activity Results and Discussion

The presence of the cubic MgNiO2 phase is a common feature observed in both the “MgO-supported Ni” and “MgO + MOx (M = Ti, Al, Zr)-supported Ni” catalysts. The catalyst’s metallic Ni components serve as active sites for the decomposition of CH4 and these sites are generated by reducing the catalysts using H2. After reduction, the catalysts exhibit a range of basic sites, varying in strength from weak to strong, which are involved in interacting with CO2. The interplay between CH4 decomposition and CO2 interaction is pivotal in driving the syngas formation pathway.

However, despite these factors, the complexity of the reaction mechanism cannot be fully captured by these conditions alone. This is due to the inherent nature of CO2, which acts as an oxidizing gas and H2, a reducing gas. The presence of these gases in the system can dynamically influence both the population and accessibility of the active sites. The cyclic H2TPR-CO2TPD-H2TPR experiment offers valuable insights into this aspect, revealing an enhancement in the higher threshold of reducibility for both the “MgO-supported Ni” and “MgO + MOx (M = Ti, Al, Zr)-supported Ni” catalyst systems under conditions of both oxidizing and reducing environments during DRM. In essence, as the reaction progresses, the catalysts move back and forth between oxidizing (CO2) and reducing (H2) gas environments. This dynamic equilibrium results in the accessible active sites of "metallic Ni" being made available at considerably lower temperatures, thereby significantly contributing to the effectiveness of the DRM process.

The catalytic activity results for the 5Ni/MgO and 5Ni/MgO + MOx (M = Al, Zr. Ti) catalysts are shown in Fig. 6. The MgO-supported Ni catalyst exhibits a surface area of 55.2 m2/g along with reducible NiO, derived from the cubic MgNiO2 phase, which interacts with surface from moderate to strong strength. This phenomenon of Ni interaction with MgO support has been previously elucidated by Zou et al. through density functional theory and kinetic Monte Carlo simulations [45]. Furthermore, the reduced 5Ni/MgO catalyst is characterized by an array of basic sites spanning from weak to strong strengths, poised for potential interaction with CO2. The reduced catalyst provides access to metallic Ni sites that facilitate the CH4 decomposition process, along with offering basic sites for the interaction of CO2, thereby initiating the dry reforming of methane reaction. Moreover, the shifting balance between oxidizing and reducing environments during the DRM reaction expedites the accessibility of metallic Ni sites at lower temperatures. This synergy culminates in the 5Ni/MgO catalyst, displaying a consistent H2 yield of 70–69% (CO yield of 73–72%) over a duration of 430 min in the time on stream test. Notably, the spent 5Ni/MgO catalyst demonstrates minimal weight loss and a low accumulation of graphitic carbon. The relatively higher CO yield compared to the H2 yield implies the possible occurrence of side reactions, such as the reverse water gas shift reaction, alongside the primary dry reforming of methane reaction.

Fig. 6
figure 6

Catalytic activity results over 5Ni/MgO and 5Ni/MgO + MOx (M = Al, Zr. Ti) catalysts, a H2-yield (%) vs time on stream (TOS), b CO-yield (%) vs time on stream (TOS), c “H2 yield(%) and CO yield (%)” vs time on stream (TOS)

Incorporating 20wt% ZrO2 alongside 80% MgO in the catalyst of 5Ni/MgO + ZrO2 results in a reduction of surface area compared to the 5Ni/MgO catalyst. Additionally, the catalyst exhibits the least crystallinity and a monoclinic phase, a characteristic associated with potential phase transition and catalyst instability [21]. The fresh 5Ni/MgO + ZrO2 catalyst demonstrates inferior reducibility compared to the 5Ni/MgO catalyst. Notably, the reducibility pattern of 5Ni/MgO + ZrO2 does not significantly differ from that of the 5Ni/MgO catalyst under oxidizing and reducing environments during the DRM reaction.

The weight loss profile of the spent 5Ni/MgO + ZrO2 catalyst is akin to that of the spent 5Ni/MgO catalyst, albeit with a relatively higher content of graphitic carbon. The spent catalyst also reveals an additional deposit of sp3-carbon (without hydrogen). The overall impact on the catalytic performance is evident in the H2 yield of the 5Ni/MgO + ZrO2 catalyst, which is only 54% and further decreases to 46% during the 430 min time on stream. The CO yield, similarly, remained between 62 and 56% throughout the 430 min time on stream.

The 5Ni/MgO + TiO2 catalyst exhibits a notably higher surface area compared to the 5Ni/MgO catalyst. This catalyst also features a partially contracted lattice and lower crystallinity in comparison. Additionally, it includes reducible rhombohedral NiTiO3 phases alongside the cubic MgNiO2 phase. Consequently, the 5Ni/MgO + TiO2 catalyst boasts the highest population of catalytically active Ni species (derived from the reduction of both MgNiO2 and NiTiO3) among the various catalyst systems considered for DRM. Moreover, under oxidizing and reducing conditions during the DRM process, the 5Ni/MgO + TiO2 catalyst showcases an enhanced degree of reducibility compared to the 5Ni/MgO + ZrO2 and 5Ni/MgO catalysts.

Turning to the spent catalyst analysis, the TGA and Raman profiles of the spent 5Ni/MgO + TiO2 catalyst reveal a substantial weight loss (73.9%) and the highest accumulation of “graphitic and defective” carbon deposits on the catalyst surface. Despite presenting a greater number of active sites, the catalytic performance of the 5Ni/MgO + TiO2 catalyst is hindered by severe carbon deposition, leading to diminished activity compared to the 5Ni/MgO catalyst. Throughout the 430 min time on stream, the 5Ni/MgO + TiO2 catalyst achieves H2 yields of 63–60% and CO yields of 70–65%.

The incorporation of 20wt% Al2O3 along with 80wt%MgO brings about significant modifications in the physio-chemical surface composition of the 5Ni/MgO + Al2O3 catalyst. Notably, the catalyst's crystallinity decreases compared to the 5Ni/MgO catalyst, while the lattice is relatively expanded, and the surface area extends to 1.5 times that of 5Ni/MgO. The fresh 5Ni/MgO + Al2O3 catalyst surface exhibits the highest concentration of “strongly interacted reducible-NiO species”. EDX profile showed the highest Ni enrichment on the surface of 5Ni/MgO + Al2O3 catalyst than rest catalysts. Basic sites for CO2 interaction are also accessible at slightly lower temperatures. These surface features contribute to achieving H2 yields of up to 72.5% (with CO yields of up to 76%). Over time, under oxidizing and reducing conditions during DRM, the active sites become accessible at lower temperatures, with the highest accessibility observed over the 5Ni/MgO + Al2O3 catalyst. The spent 5Ni/MgO + Al2O3 catalyst experiences a weight loss of about 12.8%, similar to the spent 5Ni/MgO + ZrO2 catalyst. The type of carbon deposit observed includes graphene layers and sp3-carbon (without hydrogen) but no graphitic carbon. Overall, the catalytic activity remains stable, with H2 yields not dropping below 71% (with CO yields of 74%) during the 430-min time on stream. The catalytic activity of the 5Ni/MgO + Al2O3 catalyst is optimal among the considered catalyst systems.

Comparing the catalytic activity of “metal oxide supported Ni” and “dual metal oxide supported Ni” catalysts for DRM (in terms of H2 yield), as shown in Table 1 [22, 46,47,48,49,50,51,52,53,54,55,56,57,58,59,60], it is evident that the H2 yield achieved by the 5Ni/MgO + Al2O3 catalyst is comparable to that of alumina-supported Ni catalyst [48] and MSN (mesoporous silica new) supported 20wt% Ni catalyst [55]. Notably, the former study employed six times more catalyst for the reaction, and the latter study used four times more Ni loading than the current catalyst in this study.

Table 1 Comparative catalyst activity for dry reforming of methane over closely related catalyst systems

4 Conclusion

The study investigated promotor-free, MgO or MgO + MOx (M = Zr, Ti, Al) supported Ni-based catalyst system for the dry reforming of methane (DRM) to syngas. The reduced MgO-supported Ni catalyst exhibited good reducibility, a wide range of basic sites for CO2 interaction, and active Ni sites derived from cubic MgNiO2. The cyclic H2TPR-CO2TPD-H2TPR experiment highlighted the increased accessibility of active Ni sites under both oxidizing and reducing environments during DRM, leading to a consistent ~ 70% H2 yield over 430 min.

However, the addition of 20wt% ZrO2 led to an unstable catalyst phase, reduced reducibility, and increased graphitic carbon deposition. This resulted in a significantly decreased H2 yield of 46% over the same reaction time. On the other hand, the 5Ni/MgO + TiO2 catalyst showed increased active Ni concentration due to the presence of rhombohedral NiTiO3 along with MgNiO2. It also exhibited enhanced reducibility under both oxidizing and reducing conditions, but extensive coke deposition limited its H2 yield to 60%.

The addition of 20wt% Al2O3 with MgO support significantly modified the physio-chemical surface composition of the catalyst. The 5Ni/MgO + Al2O3 catalyst demonstrated expanded lattice and surface area, a high concentration of “strongly interacted reducible NiO species”, and the highest accessible active sites during DRM. Interestingly, the spent-5Ni/MgO + Al2O3 catalyst did not show a graphitic carbon peak but a carbon peak for graphene layers and sp3-C (without hydrogen). This catalyst maintained a constant H2 yield of 71% (CO yield of 74%) over the 430 min reaction time, making it a promising candidate for DRM applications.

Overall, the study provides valuable insights into the effects of promotor-free Ni-based different catalyst supports and compositions on DRM performance, highlighting the role of reducibility, basicity and coke deposition in achieving sustainable and efficient syngas production.