N. Pegiosa,
V. Bliznukb,
S. Prüntec,
J. M. Schneiderc,
R. Palkovits*a and
K. Simeonova
aDepartment of Heterogeneous Catalysis, Chemical Technology (ITMC), RWTH Aachen University, Worringerweg 2, Aachen 52074, North Rhine-Westphalia, Germany. E-mail: Palkovits@itmc.rwth-aachen.de
bDepartment of Electrical Energy, Metals, Mechanical Construction & Systems (EEMMeCS), Group Metals Science & Technology, Tech Lane Ghent Science Park – Campus A, Technologiepark 903, B-9052 Gent, Belgium
cMaterials Chemistry, RWTH Aachen, Kopernikusstr. 16, Aachen 52074, Germany
First published on 2nd January 2018
Dry reforming of methane (DRM) enables an efficient utilization of two abundant greenhouse gases by converting them into syngas, a versatile feedstock for chemical synthesis. Aiming for high catalyst performance and enhanced coke resistance, different preparation techniques of La-promoted Ni/γ-Al2O3 catalysts for DRM were compared facilitating structure–performance correlations. The studied synthesis techniques comprehend incipient wetness impregnation and co-precipitation as well as alternative techniques such as spray drying. All catalysts were fully characterized before and after reaction by N2-physisorption, XRD, H2-TPR and STEM-EDX elemental mapping. Additionally, a thorough investigation of carbon deposits has been carried out by TGA/DSC and STEM-EDX, respectively. The different preparation techniques led generally to very different physical properties, structure, chemical species and anti-coking properties of the catalyst. However, some catalysts with similar physicochemical characteristics differed in catalytic performance and coking resistance. Superior catalytic performance could be reached for catalysts prepared by spray drying and related to excellent Ni dispersion, strong metal–support interaction and very low coke formation of only 2.7% of the catalyst weight. After 6 h time on stream only minor sintering occurred, with few Ni nanoparticles up to 10 nm.
CO2 + CH4 ↔ 2CO + 2H2, ΔHo298 K = +247 kJ mol−1 | (1) |
CH4 ↔ C + 2H2, ΔHo298 K = +75 kJ mol−1 | (2) |
2CO ↔ CO2 + C, ΔHo298 K = −172 kJ mol−1 | (3) |
CO2 + H2 ↔ H2O + CO, ΔHo298 K = +41 kJ mol−1 | (4) |
Therefore, this study focusses on Ni on γ-Al2O3 promoted with lanthanum. La is commonly used to form perovskite-like structures. Whereas in this study, La is envisioned as a textural promoter to enhance nickel dispersion and to accelerate carbon deposits removal, respectively. Numerous studies, both experimental,29–31 and computational (DFT),31–34 suggest that a reduced Ni-nanoparticle size enhances activity and minimizes carbon formation. Especially a Ni particle size of less than 5 nm appears advantageous for coke-resistant catalysts.34 Despite intensive research in the field, the influence of preparation techniques on catalyst properties and the associated performance in DRM has been investigated rarely. In order to address these, we compared seven La-promoted Ni/γ-Al2O3 catalysts prepared by a wide range of different synthetic techniques, all aiming at obtaining catalysts with high specific surface area and high active metal dispersion. The methods comprehend incipient wetness impregnation and co-precipitation as they are commonly used in the literature providing decent catalytic results towards DRM. Spray drying was also utilized since the achieved Ni dispersion is excellent. To the best of our knowledge, spray drying has been rarely used for Ni-based catalysts in DRM. Additionally, we modified spray drying and co-precipitation by combining them with physical mixture and an ethanol suspension approach. In this way, we could also evaluate the influence of ethanol as a suspension medium on the properties of the catalyst. Furthermore, feed ratio of CO2:CH4 = 2:1 was utilized since higher partial pressure of CO2 in the feed was found to suppress sintering and coke formation.35,36 We focused on structural and physico-chemical characterization of these materials before and after testing, as well as their activity and stability in DRM. Together with a throughout analysis of carbon deposits, a correlation between the impact of preparation techniques on catalyst properties and their catalytic performance and coking behavior became evident.
Catalyst | Preparation technique | Step 1 | Step 2 | Step 3 |
---|---|---|---|---|
a Overnight at 80 °C.b At 800 °C in air for 8 h (10 K min−1). | ||||
IW3M | Incipient wetness impregnation | Ni(NO3)2·6H2O and La(NO3)3·6H2O dissolved in water and impregnated on γ-Al2O3 | Dried overnighta and calcinedb | — |
SD3M | Spray drying | Ni(NO3)2·6H2O, La(NO3)3·6H2O and Al(NO3)3·9H2O dissolved in water and then spray dried | — | |
CP3M | Co-precipitation | Ni(NO3)2·6H2O, La(NO3)3·6H2O, Al(NO3)3·9H2O dissolved in water and mixed with NaOH(aq). Filtered and washed | — | |
SD + SolidMix | Spray drying/physical mixture | Ni(NO3)2·6H2O and La(NO3)3·6H2O dissolved in water and then spray dried | Physical mixture with γ-Al2O3 and calcinedb second time | |
SD + suspension | Spray drying/ethanol suspension | Ni(NO3)2·6H2O and La(NO3)3·6H2O dissolved in water and then spray dried | Ethanol suspension with γ-Al2O3, drieda and calcinedb second time | |
CP + SolidMix | Co-precipitation/physical mixture | Ni(NO3)2·6H2O and La(NO3)3·6H2O dissolved in water and mixed with NaOH(aq). Filtered and washed | Physical mixture with γ-Al2O3 and calcinedb second time | |
CP + suspension | Co-precipitation/ethanol suspension | Ni(NO3)2·6H2O and La(NO3)3·6H2O dissolved in water and mixed with NaOH(aq). Filtered and washed | Ethanol suspension with γ-Al2O3, drieda and calcinedb second time |
The catalyst denoted as SD3M was synthesized by the standalone preparation technique of spray drying, utilizing a 3-metal solution. 0.5 g of Ni(NO3)2·6H2O, 0.74 g of La(NO3)3·6H2O and 7.36 g of Al(NO3)3·9H2O (Sigma Aldrich, ≥98.0) were dissolved in 230 mL distilled water to form a solution of 0.1 M concentration based on the total amount of metal nitrates. The solution was then fed with a constant rate of 3 mL min−1 into a spray dryer (BÜCHI Mini-Spray-Dryer B-290) with N2 as carrier gas at 4 mL min−1 and air as drying gas at 550 L min−1 at 140 °C. The obtained material was dried overnight and calcined.
The catalyst denoted as CP3M was synthesized by co-precipitation, utilizing a 3-metal solution. 0.5 g of Ni(NO3)2·6H2O, 0.74 g of La(NO3)3·6H2O and 7.36 g of Al(NO3)3·9H2O were dissolved in 250 mL distilled water and heated to 50 °C. 185 mL of 0.4 M NaOH were added and stirred for 30 min. The formed precipitate was cooled to room temperature, filtered and washed multiple times with distilled water. The obtained material was dried and calcined as already indicated.
The catalysts denoted as SD + SolidMix and SD + suspension were synthesized by applying the combined techniques of spray drying/physical mixture and spray drying/ethanol suspension, respectively. 2.0 g of Ni(NO3)2·6H2O and 2.96 g of La(NO3)3·6H2O were dissolved in 137 mL distilled water to form a solution of 0.1 M concentration based on the total amount of metal nitrates. The rest of the procedure is identical to the one applied to SD3M catalyst. After calcination, half of the collected material was physically mixed with 2 g of γ-Al2O3 to obtain SD + SolidMix catalysts, whereas the other half was suspended in ethanol with 2 g of γ-Al2O3 and after agitation for 30 minutes dried to produce the SD + suspension catalyst. Both materials were finally calcined.
The catalysts denoted as CP + SolidMix and CP + suspension were synthesized by combining co-precipitation and physical mixture, and co-precipitation- and ethanol suspension, respectively. 2.0 g of Ni(NO3)2·6H2O and 2.96 g of La(NO3)3·6H2O were dissolved in 67 mL of distilled water and heated to 50 °C. 225 mL of 0.2 M NaOH were added and stirred for 30 min. The formed precipitate was quenched to room temperature, filtered and washed multiple times with distilled water. The obtained material was dried overnight and calcined. Half of the collected material was physically mixed with 2 g of γ-Al2O3 to obtain the CP + SolidMix catalyst, while the other half was suspended in ethanol with 2 g of γ-Al2O3, agitated for 30 minutes and dried to obtain the CP + suspension catalyst. Both materials were finally calcined.
Conversions and selectivities were calculated through the equations
(5) |
(6) |
(7) |
(8) |
(9) |
(10) |
(11) |
IW3M | SD3M | CP3M | SD + SolidMix | SD + suspension | CP + SolidMix | CP + suspension | |
---|---|---|---|---|---|---|---|
Surface area (m2 g−1) | 98.8 | 9.8 | 97.0 | 127.4 | 138.1 | 118.3 | 118.8 |
Total pore volume (cm3 g−1) | 0.42 | 0.01 | 0.21 | 0.41 | 0.45 | 0.37 | 0.37 |
Average pore size (Å) | 102 | 27 | 52 | 94 | 96 | 96 | 95 |
XRD measurements were also carried out (see ESI†) for all freshly calcined catalysts. IW3M, SD3M and CP3M exhibited very low crystallinity, which was not expected due to the harsh calcination conditions of 800 °C for 8 h. Literature reports suggest that γ-Al2O3 appears at temperatures between 350 and 1000 °C when formed from crystalline37 or amorphous38 precursors. More studies should be performed in order to understand better this observation. XRD patterns of these three catalysts showed reflections with relatively low intensity related to γ-Al2O3 as well as NiAl2O4, respectively. The other materials possessed a higher degree of crystallinity emphasized by more intense reflexes corresponding to γ-Al2O3 and NiAl2O4. More specifically, all four materials exhibited distinguishable reflexes of γ-Al2O3 (more pronounced at 32.7°, 39.5°, 45.5°, 60.6° and 66.9° 2-theta) and NiAl2O4 (at 37.2° and 78.5° 2-theta), respectively. For the catalysts prepared with the combined preparation techniques crystallinity of La2O3 and/or La(OH)3 was emphasized by reflexes found at 47.3° and 58.5° 2-theta. Furthermore, no reflections attributable to the NiLa2O3 perovskite-like structure were observed. This comes in good agreement with studies, reporting that high calcination temperature would favor perovskite-like structure formation but also an appropriate ratio of Ni and La is needed.39
H2-TPR profiles of the calcined catalysts showed a great variation of the reducibility of the catalysts (Fig. 1). H2 uptake for each catalyst and temperature range was calculated and presented in Table 3. Concerning Ni-based catalysts supported on γ-Al2O3, 4 different species with increasing reduction temperature have been reported: Ni-α species [300–500 °C] that correspond to reducing bulk NiO with very low interaction with γ-Al2O3, Ni-β1 species [500–600 °C] that correspond to NiO interacting moderately with γ-Al2O3, Ni-β2 [600–900 °C] that correspond to non-stoichiometric spinel species with strong interaction with the support and finally Ni-γ species [600–900 °C] that correspond to bulk NiAl2O4 species.40–42 Signals corresponding to reduction of La species did not occur because of the high reduction temperature of lanthanates.43,44 The results obtained are in reasonable agreement with the reduction temperatures of the different Ni species, though some signals overlap and shift from the reported values. This observation can be attributed to the presence of the textural La-promoter. For catalysts IW3M and SD3M, reduction started at temperatures higher than 650 °C suggesting that only spinel species strongly interacting with the support and no separate NiO were available. We observed a comparable H2-TPR profile for CP3M; however, also small amounts of reducible NiO species potentially exhibiting a moderate support interaction appear. For SD + SolidMix, SD + suspension, CP + SolidMix and CP + suspension the acquired profiles differ significantly possessing two major peak regions; between 300 and 500 °C signals can be mainly attributed to Ni-α (bulk NiO species), whereas Ni-β1 species – smaller NiO domains moderately interacting with the γ-Al2O3 support – cause signal at temperature of 450 to 620 °C, respectively. Interestingly, these catalysts did not possess species causing high reduction temperatures of above 650 °C. Moreover, the H2-TPR profile of SD + SolidMix differs to some extent from SD + suspension although the NiO and La2O3 species were prepared for both cases in one step by spray drying. This could be attributed to the different preparation technique of introducing γ-Al2O3, physical mixture and ethanol for SolidMix and suspension, respectively.
H2-uptake (mmol H2 gcat−1) | ||||||||
---|---|---|---|---|---|---|---|---|
IW3M | SD3M | CP3M | SD + SolidMix | SD + suspension | CP + SolidMix | CP + suspension | ||
Temperature (°C) | 300–500 | 0.49 | 0.28 | 0.20 | 1.82 | 1.56 | 3.47 | 3.14 |
500–600 | 0.39 | 0.23 | 0.50 | 0.47 | 0.32 | 4.02 | 1.87 | |
600–800 | 4.58 | 1.78 | 4.41 | 0.04 | 0.13 | 0.28 | 0.16 | |
Total | 5.46 | 2.29 | 5.11 | 2.32 | 2.01 | 7.77 | 5.17 |
Elemental mapping (EDX) of the materials facilitated insights into element distribution. Fig. 2 provides an overview of Al, La and Ni for IW3M, CP3M, SD + SolidMix and SD + suspension, respectively. For most catalysts, Ni and La signals overlapped suggesting that La indeed acted as a spacer improving NiO dispersion. IW3M and CP3M exhibited a very good metal dispersion with no obvious nanoparticle formation for NiO. In contrast, for SD + SolidMix and SD + suspension, NiO nanoparticles of around 100 nm in size occurred. For SD3M only STEM images are provided, since only elemental line measurements were possible due to high charging and instability of the observed specimen (see ESI†). The utilized preparation technique of spray drying led to formation of spherical particles in the size range of 300 to 1500 nm with a good metal dispersion; NiO, La2O3 and Al2O3 were homogeneously dispersed throughout the formed spherical particles. Literature reports suggest that lower reducibility, namely strong metal–support interaction, could be a direct consequence of high metal dispersion and harsh calcination conditions (800 °C for 8 h).45 This is in good agreement with the H2-TPR profiles and EDX elemental mapping of the freshly calcined catalysts.
Fig. 2 EDX elemental mapping of the fresh calcined catalysts. Color scale, to the left of images, represents intensity of correspondent element characteristic X-ray line. |
(12) |
(13) |
Fig. 3a shows reaction time courses. The standard error of the measurements (S.E.) was calculated to be 0.02 × 10−5 and 0.01 × 10−5 for the reaction rate of CO2 and CH4, respectively; the reaction rate for CH4 always exceeded the one of CO2 suggesting that reverse water–gas shift (RWGS) reaction (eqn (4)) was disfavored at the utilized reaction conditions (800 °C, CO2:CH4 = 2:1, 35000 h−1). Thermodynamic calculations, assuming ΔG° = 0, showed that 820 °C is the upper limiting temperature for RWGS and 640 °C the lower limiting for DRM.48 Comparing the yields of H2 and H2O derived from DRM and RWGS, respectively, at different temperatures it was found that the first was the dominant reaction at temperatures higher than 330 °C with a catalytic system that wasn't reported.49,50
IW3M, SD3M and CP3M exhibited the best catalytic performance concerning both activity and stability throughout the 6 h time on stream (TOS). The final reaction rate of CH4 at 6 h TOS for SD3M was 30.8 × 10−5 mol gcat−1 s−1, surpassing the reaction rate of the other two by more than 3 times, 9.5 × 10−5 and 8.3 × 10−5 mol gcat−1 s−1 for IW3M and CP3M, respectively. In fact, IW3M and SD3M exhibited superior catalytic activity and stability compared to the other catalysts. However, IW3M deactivated over time, whereas SD3M showed stable activity for CO2 over the studied TOS and increasing activity over the first 4 h TOS for CH4. Concerning this initial activation of SD3M, incomplete reduction of the catalyst and subsequently further reduction by H2 derived from CH4 decomposition was ruled out, since the same observation was true for both 2 and 3 h of catalyst reduction before reaction. A possible explanation could be the structural change of the catalysts at 800 °C, revealing more active sites through Ni-nanoparticle migration, leading to higher activity. In the future, this finding will be further investigated. The four catalysts prepared by the combined techniques displayed inferior catalytic activity and stability. Focusing on the final reaction rates of CH4 at 6 h TOS, we identified the following ranking of all 7 catalysts:
SD3M > IW3M > CP3M > CP + suspension > CP + SolidMix > SD + suspension > SD + SolidMix.
Different preparation techniques have a strong influence on physico-chemical properties and performance of a catalyst.51,52 Mesoporous materials are commonly used due to their high surface area and pore volume as well as their uniform pore size leading to more accessible and exposed active sites.53 This comes in contradiction with our study, where the two worst performing catalysts, SD + SolidMix and SD + suspension, possessed the highest specific surface area with 127.4 and 138.1 m2 g−1, respectively. On the other hand, the specific surface area of SD3M was 14-fold lower than the latter with 9.8 m2 g−1, indicating that achieving high specific surface area was not crucial towards good catalytic performance. An explanation of the observed catalytic behavior of all studied catalysts can be their different reducibility. The first three catalysts, IW3M, SD3M and CP3M, displayed the lowest reducibility especially in the low temperature regions, which points at the very good dispersions of the active metal phase in these materials. This is in good agreement with the TEM investigations of the freshly calcined catalysts (Fig. 2) and literature reports suggesting that the stronger the metal–support interaction, the better the metal dispersion leading to enhanced activity and stability.45,54 However, the following contradictory point should be noted. Strong metal–support interactions causing low reducibility means that Ni2+ is not completely reduced to Ni0. The latter is considered to be the active site for DRM. Consequently, catalysts with less “reduced” active sites lead to higher activity. This is in line with literature reports, suggesting that mixture of Ni2+ and Ni0 could facilitate higher activity compared to samples only containing Ni0.45,55 The reaction rate of CO2 follows the same trend with the one of CH4 and varies from 0.5 to 3.5 × 10−5 mol gcat−1 s−1 among the different catalysts. It is reported that Ni0 formed by NiAl2O4 spinels, namely species with strong metal–support interaction, could accommodate the spill-over H derived by CH4 decomposition. With the assistance of spilt over H, CO2 dissociation rate could be enhanced leading to differences in CO2 activity.56
Despite identical calcination of all catalysts at 800 °C for 8 h, catalysts prepared by the combined techniques possessed significantly lower activity and stability. We relate this observation to phase separation between Ni- and La-oxides during this calcination step and subsequently to the Ni-nanoparticle size. With smaller nanoparticle size better activity and anti-coking properties were achieved.57–59 As confirmed by EDX mapping, individual domains of Ni-rich matter are easily distinguishable. These Ni-rich domains are reduced at lower temperatures (Fig. 1) and lead to formation of bigger agglomerates (Fig. 2) during DRM causing more pronounced coking. In line, higher reducibility suggests weaker metal–support interaction associated to the formation of bigger Ni nanoparticles due to sintering during DRM. The bigger the Ni nanoparticles the lower are the observed coke resistance and catalytic activity, respectively. In order to further point this relationship out, we plotted the final reaction rates of CH4 conversion over the amount of species with strong metal–support interaction (%) for all seven catalysts (Fig. 3b). The trend indicates that the higher the amount of strong metal–support interactions the higher catalytic activity. Two groups of catalyst preparation techniques can be distinguished: (a) standalone preparation techniques (IW3M, SD3M, CP3M) that exhibited superior catalytic results and (b) combined preparation techniques (SD + SolidMix, SD + suspension, CP + SolidMix, CP + suspension) with inferior catalytic results. In a comparative study between two Ce-promoted catalysts prepared by co-impregnation and sequential impregnation, the first was found to perform better towards DRM. This was attributed to closer interaction between promoter and active metal, increasing the redox properties of the catalyst.60 Similarly, for the catalysts prepared by the single preparation technique La, Ni and Al2O3 exhibited stronger interaction than the ones by the combined preparation techniques, leading to better activity and stability.
Selectivities of both H2 and CO (based on total carbon feed, CO2 + CH4) are presented in ESI.† The calculated standard error of the former is 0.17 and for the latter 0.35, respectively. Indeed, the selectivity of H2 varies significantly with the catalysts type. Catalysts prepared with combined preparation techniques exhibited the lowest values compared to IW3M, SD3M and CP3M. The difference in H2 selectivity could be attributed to RWGS and the Boudouard reaction. Reaction rate of CH4 was always higher than the one of CO2 (see ESI†). For the catalysts prepared by a single technique as well as SD + SolidMix and SD + suspension selectivity of hydrogen was higher than the one of CO, indicating that RWGS occurs at a greater extent than the Boudouard reaction. The opposite is suggested for CP + SolidMix and CP + suspension. For CO selectivity, all catalysts possessed stable values at around 50% with the only exception of SD + suspension, which started at 40.3%, increased slightly and then decreased to 42.4% at 6 h TOS. The utilized feed ratio of CO2:CH4 = 2:1 could provide a rationale for the stable value of CO selectivity at around 50% but further investigations are needed to better understand this observation.
Focusing on syngas composition (H2:CO) (Fig. 4), catalysts prepared by the standalone techniques (IW3M, SD3M, CP3M) exhibited the highest values of ca. 0.65 as opposed to catalysts prepared by combined techniques (CP+*, SD+*). The latter showed relatively low values of the H2:CO ratio of about 0.20–0.55, indicating that the RWGS takes place at a higher extent. This is surprising, since RWGS is thermodynamically limited to 820 °C.48 Further studies will aim at an understanding of DRM and RWGS over these materials. H2:CO ratio in the absence of carbon deposits and C2+ should follow the formula;61
(14) |
TGA/DSC analyses in air enabled investigating carbon formation on all seven spent catalysts (Table 4 and see ESI†). Focusing on DSC, exothermic events corresponding to oxidation of different carbon species became evident at different temperatures. DSC signals at 300 to 500 °C and at 550 to 700 °C were related to amorphous and graphitic carbon oxidation, respectively.62–64
IW3M | SD3M | CP3M | SD + SolidMix | SD + suspension | CP + SolidMix | CP + suspension | |
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a Temperature of DSC peaks. | |||||||
Mass loss (%) | 3.9 | 2.7 | 14.4 | 6.4 | 6.0 | 0.1 | 5.1 |
Temperature (°C)a | 300 | 650 | 300, 600 | 500 | 500 | 350 | 350, 600 |
Carbon species | Amorphous | Graphitic | Amorphous graphitic | Amorphous | Amorphous | Amorphous | Amorphous graphitic |
Firstly, amorphous carbon is formed and then, depending on the reaction conditions and the catalytic system, graphitization gradually occurs converting amorphous to graphitic carbon. All seven spent catalysts demonstrated the existence of at least some amount of amorphous carbon. The amount of graphitic carbon varies throughout the catalysts with CP3M exhibiting the highest amount of all seven spent catalysts. SD3M and SD + suspension presented moderate amounts, while the rest of the catalysts exhibited very low or no graphitic carbon. The weight loss due to carbon oxidation was also measured and translated to percentage of carbon deposits. The best performing catalysts, IW3M and SD3M, presented relatively low amounts of carbon at 3.9 and 2.7%, respectively. This is in good agreement with literature reports, suggesting that homogeneity of active sites, as it was confirmed by EDX elemental mapping, could sharply decrease carbon deposits.31 Carbon could be gasified either by O* derived by CO2 decomposition or by H2O produced by RWGS leading to less carbon deposits after reaction. The later is mainly met in steam reforming of methane but with the presence of the produced water during DRM, this is expected to lower the amount of carbon deposits for IW3M and SD3M.65,66
CP3M exhibited the highest amount of carbon of all seven spent catalysts with 14.4%. The catalysts with combined preparation techniques showed relatively low amounts of carbon deposits. CP + SolidMix had practically no carbon deposits, although it exhibited moderate reaction rates compared to the other catalysts indicating carbon free operation at the given reaction conditions. SD + SolidMix and SD + suspension possessed very low activity but relatively high amounts of coke deposits. A possible explanation could be that they started with higher activity that lead to coking and deactivated rapidly before sampling from the online GC.
Further, investigating carbon deposits on all spent catalysts, we found that the higher the amount of strong metal–support interacting species on the fresh catalyst, found by H2-TPR analysis, the less the amount of coke deposits (%) (Fig. 6a). CP + SolidMix exhibited a minimal amount of coke deposits (%) as the reaction rates were also minimal. CP3M had at the same time significantly higher values of both. For the mentioned correlation, we considered these extreme points as outliers. Also, a trend of the nature of the carbon deposits could be identified; the higher the amount of coke deposits (%) the higher the graphitization degree (Fig. 6b). Again, CP3M was not considered for the correlation.
In Fig. 7 the results of the STEM-EDX elemental mapping are presented for five spent catalysts. It is clear that sintering occurs during DRM leading to bigger nanoparticles of Ni for IW3M and CP3M. For these two catalysts, the metal dispersion was very high with no distinguishable Ni particles before reaction. However, after reaction, we observed nanoparticles of 15–70 nm size. SD + SolidMix and SD + suspension displayed the same big Ni-rich domains as observed for the fresh catalysts. No carbon filaments formed for these two materials. Most probably, the nature of the preparation procedure played a crucial role for this behavior; lanthanum and nickel segregated during the first calcination step forming separate domains of NiO and La containing species. We assume that La is present in the form of La2O3. La2O3 in close proximity of the DRM active Ni-rich domains is known to possess high oxidation potential with respect to deposited surface carbon species.21 Therefore, no carbon nanotubes could be observed for SD + SolidMix and SD + suspension. In practice, for the mixed preparations, we obtained La2O3-supported Ni catalysts, where the third phase, γ-Al2O3, is considered to be only a spectator. SD3M exhibited no visible large scale sintering; only some small Ni particles (less than 10 nm in size) were found on the tips of the carbon filaments (Fig. 7). These particles are most probably detached from the support during reaction, suggesting that some small scale phase segregation occurred. This observation is in line with the suggested growth mechanism of carbon nanotubes, where carbon, derived mainly from CH4 dissociation, migrates through the Ni nanoparticle to precipitate at the nickel–support interface. This interfacial carbon built-up pushes the isolated Ni-particles away from the support leading eventually to its deactivation.67 Focusing on the carbon species formed, the STEM results are in reasonable agreement with the ones from TGA/DSC, where for CP3M and SD3M (the catalysts with the highest graphitization degree) carbon nanotubes were found. For the rest of the catalysts with low graphitization degree no carbon nanotubes were observed.
Fig. 7 EDX elemental mapping of the spent catalysts. Color scale, to the left of images, represents intensity of correspondent element characteristic X-ray line. |
The surface chemistry of IW3M and SD3M, the two best performing catalysts, was investigated for both, fresh and spent catalysts by means of XPS analysis (Fig. 8). The most significant difference in surface chemistry between the two catalysts lies in the chemical state of La which was probed by the La 3d5/2 signal (Fig. 8b). Deconvoluted signals of IW3M, for both fresh and spent catalysts, are located at 835.6 eV and attributed to the formation of La(OH)3.68 In contrast, the main La 3d5/2-signal of the fresh and spent SD3M catalyst is positioned at 0.4 eV lower binding energy consistent with the formation of La2O3.68 The Ni 2p3/2 signal (Fig. 8a) overlaps with the La 3d3/2 signal. However, peaks at 856.3 and 856.6 eV clearly indicate the formation of NiAl2O4 for both the fresh and spent catalysts,69–72 while a signals 854.9–855.0 eV may originate from the La 3d3/2 satellite signal68 and/or the Ni 2p3/2-signal which could indicate the formation of NiO.70–72 While for all examined powders the XPS analysis remains inconclusive regarding the potential formation of NiO due to the overlap with the La satellite signal, the formation of NiAl2O4 is evident. Furthermore, the intensity of signals associated with the presence of NiAl2O4 is clearly reduced for the spent catalysts as compared to the fresh state. The Ni 3p signal detected at 68.4 eV and 68.1 eV (Fig. 8c) for the fresh catalysts IW3M and SD3M cannot be detected in the spent state for both materials, indicating a Ni depletion consistent with the concomitant reduction in signal associated with the presence of NiAl2O4. Finally, the Al 2p signals (Fig. 8c) detected at 74.1–74.6 eV for all samples investigated are attributed to the formation of Al2O3.69,72,73 It is reasonable to assume that the detected Na was incorporated during storage of the sample in air prior to the XPS analysis.
Fig. 8 XPS spectra of IW3M and SD3M prior (fresh) and after reaction (spent). (a) Ni 2p3/2- and La 3d3/2-signals (b) La 3d5/2-signals and (c) Al 2p- and Ni 3p-signals. |
Catalyst prepared by spray drying, namely SD3M, showed superior catalytic results irrespective of its low specific surface area compared to materials prepared via more conventional techniques. This superior performance can be attributed to excellent Ni dispersion and strong metal–support interactions leading to very low formation of carbon deposits. These properties also facilitate very stable catalytic activity. In line, catalyst morphology remains intact in the course of the reaction for 6 h time-on-stream in DRM. Overall, spray drying appears promising to further improve the performance of catalysts for DRM. Future studies will focus on optimized spray drying conditions aiming for even higher nickel dispersion, further enhanced metal–support interactions and materials possessing high specific surface areas.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c7ra06570a |
This journal is © The Royal Society of Chemistry 2018 |