2.2. XRD, XPS, and HAADF-STEM
X-ray diffractograms of the supported Ni catalysts and calcined supports are shown in
Figure 1. Calcined boehmite, Ni/Al
2O
3, Siral-5, and Ni/Siral-5 display closely similar patterns that contain predominantly peaks characteristic of γ-Al
2O
3 at 37°, 46°, and 68° [
16]. There are no discernible differences between the diffractograms of the Ni-containing catalysts and the corresponding calcined supports. The diffractograms of Siral-30 and Ni/Siral-30 are nearly identical, displaying a very broad feature at ~25° characteristic of amorphous silica and broad peaks characteristic of γ-Al
2O
3. The structure of Siral-30 is consistent with γ-Al
2O
3 nanoparticles covered with an amorphous SiO
2 layer [
8,
9]. We infer that the Siral-30 support is biphasic, comprising separate SiO
2 and Al
2O
3 nanoparticles consistent with HAADF-STEM (vide infra). In contrast, Siral-70 and Ni/Siral-70 display an intense broad XRD peak at ~25° and a barely detectable γ-Al
2O
3 peak at ~68°. We infer from the strong peak for an amorphous SiO
2-containing phase and the near absence of crystalline γ-Al
2O
3 XRD peaks that Siral-70 comprises a bulk ASA phase containing tetrahedrally coordinated Al
3+ centers [
13]. SiO
2 displays only an intense broad band at ~25° assigned to an amorphous phase. In addition, small narrow peaks at 37°, 42°, and 53° that correspond to the [111, 200, 220] Bragg reflections of NiO, respectively, ref. [
17] are observed in the XRD patterns of Ni/SiO
2 and Ni/Siral-70. In contrast, we do not observe NiO XRD peaks for the Ni/Siral-30 catalyst, indicating that any particles are smaller than the Debye-Scherrer limit.
The Si/Al ratios of the catalysts and calcined support measured by XPS are compared to the corresponding bulk values in
Table 2. The XPS (surface) values increase monotonically with bulk Si/Al, but in all instances the surface is more enriched in Si than the bulk. This is not surprising because the supports were synthesized by grafting a SiO
2 precursor onto boehmite. The positive deviation of the surface Si/Al ratios from the bulk increases as bulk Si/Al ratios decrease; i.e., the lower the total percentage of SiO
2, the more concentrated it is at the particle surfaces. The (Si/Al)
S value of Ni/Siral-70 comes closest to approximating that of the bulk, indicating that the distribution of Al
3+ and Si
4+ ions is more nearly homogeneous. The surface-to-bulk composition ratio (Ni
S/Ni
B) provides a measure of Ni
2+ species dispersion, which decreases monotonically with (Si/Al)
S for the supported catalysts (
Table 2). The 2.5 wt.% Ni/SiO
2 catalyst prepared by IWI shows negligible Ni 2p photoemission intensity because of its low loading and NiO dispersion (vide infra). Conversely, the Ni
S/Ni
B ratio for Ni/Al
2O
3 is the largest and nearly unity, suggesting that the bulk and surface Ni concentrations are closely similar. The lower, albeit similar, Ni
S/Ni
B values demonstrated by Ni/Siral-5 and Ni/Siral-30 evidence intermixing of Ni and Al-Si oxide species. The Ni/Siral-70 catalyst has a significantly lower Ni
S/Ni
B ratio, consistent with larger NiO crystallites. Previous research has established that larger NiO crystallites are produced on aluminosilicate supports with higher Si/Al ratios [
18].
Ni 2p XP spectra of the Ni/Al
2O
3 and Ni/Siral catalysts and a NiO standard are shown in
Figure 2. The spectrum of bulk NiO (
Figure 2A) shows a well-resolved 2p
3/2 and 2p
3/2 spin-orbit doublet with strong shake-up satellite features [
19]. In addition, the NiO spectrum contains a characteristic 2p
3/2 feature at 854 eV associated with multiplet splitting. In contrast, this distinguishing feature is not observed in the spectrum of Ni/Al
2O
3 nor in the spectra of Ni/Siral-5 and Ni/Siral-30. The XP spectrum of Ni/Siral-5 is similar to Ni/Siral-30, albeit with a somewhat lower signal-to-noise ratio (
Figure 2B). The XP spectrum of Ni/Siral-70 has a significantly lower S/N ratio, and the broad, poorly unresolved peaks suggest the presence of multiple Ni
2+ species. The Ni 2p
3/2 peaks of Ni/Al
2O
3 and Ni/Siral-30 appear at 855.8 and 856.9 eV, respectively, with satellites at ~862 and 863 eV, respectively. The Ni 2p
3/2 binding energy for Ni/Al
2O
3 closely matches typical literature values for NiAl
2O
4 (~856 eV) [
20,
21]. Interestingly, an additional ~1 eV shift of the Ni 2p
3/2 peak to higher binding energy (relative to NiO) is observed for the Ni/Siral catalysts (
Figure 2B). Apparently, there is a range of Ni 2p
3/2 binding energies for NiAl
2O
4 that may be related to impurities (e.g., Si) or Ni
2+ in specific crystallographic sites (i.e., spinel or inverse spinel). For example, Jimenez-Gonzalez et al. assigned Ni 2p
3/2 peaks between 856 and 857 eV to NiAl
2O
4 species in Ni/Al
2O
3 methane-reforming catalysts that had been activated at 850 °C [
22].
More detailed analyses of the XP spectra of NiO powder, Ni/Al
2O
3, and Ni/Siral-30 in the Ni 2p
3/2 region are presented in
Figure 3, including Gaussian-Lorentzian fits of the main peaks, shake-up satellites, and multiplet splitting features. Multiplet splitting is only observed for the standard, suggesting that these catalysts do not contain bulk-like NiO crystallites. The spectrum of Ni/Al
2O
3 comprises well-resolved primary and satellite peaks. The spectrum of Ni/Siral-30 is similar; however, the peaks are broader and less well-resolved. The peak broadening may be intrinsic, arising from a range of Ni
2+ environments, or may be associated with sample charging during XPS measurements.
HAADF-STEM images and EDX maps of the Ni/SiO
2, Ni/Siral-70, and Ni/Siral-30 catalysts are shown in
Figure 4. The bright 20–30-nm particles in
Figure 4A are NiO crystallites on SiO
2, as confirmed by the EDX map and consistent with XRD (
vide supra). The HAADF-STEM image of Ni/Siral-70 (
Figure 4B) contains smaller 10–20 nm NiO crystallites, as corroborated by the EDX map. In contrast, the HAADF-STEM image and EDX map (
Figure 4C) of Ni/Siral-30 comprise small (<2-nm) NiO clusters (nanoparticles) that appear to be uniformly dispersed over the support; however, this observation does not exclude the presence of a surface NiAl
2O
4 layer or mononuclear Ni
2+ complexes. Previously, STEM images of a 5 wt.% Ni/Siralox-30 catalyst by Moussa et al. showed sub-5 nm NiO nanoparticles in addition to larger (>10 nm) NiO particles [
9]. Their commercial Siralox-30 support was produced by calcination at ~900 °C and has a lower surface area than our Siral-30 support, which was calcined at 500 °C.
2.3. H2 TPR
H
2 TPR was used to investigate the impact of the support Si/Al ratio on Ni
2+ speciation and reducibility, including the degree of interaction between Ni
2+ ions and the support surface. TPR profiles of the catalysts and a NiO standard are presented in
Figure 5. The main TPR peak for bulk NiO is narrow and appears at ~400 °C. The reduction of Ni
2+ to Ni
0 should yield a H/Ni ratio of 2, the value obtained for the NiO standard. The H/Ni values obtained for the catalysts (
Table 1) are within the expected range, although there is considerable variation. We infer from the TPR peak temperatures that Ni
2+ ion reducibility increases with increasing support Si/Al ratio due to changes in Ni
2+ speciation [
20,
23]. Reduction of Ni/SiO
2 occurs over a broad temperature range centered around 400 °C. The breadth of the TPR peak (compared to bulk NiO) may be attributed to the crystallite size distribution (as observed by STEM-EDX) and degree of interaction with the support [
21]; however, some have suggested that non-stoichiometric NiO (that contains Ni
3+ ions) and Ni
2O
3 species also may contribute [
22]. The TPR profile of Ni/Siral-70 is broad and complex, comprising at least three peaks associated with different Ni
2+ species. Fitting reveals a peak at 400 °C assignable to NiO (and consistent with our XRD results), a second peak at 530 °C, and a very broad peak at ~650–700 °C. By comparison to the reduction temperatures of Ni
2+ in Beta zeolite and Ni/SiO
2-Al
2O
3, the 530 °C band is assigned to isolated Ni
2+ ions on the support [
23,
24]. The broad high-temperature peak is suggestive of either NiO nanoparticles interacting strongly with the support or surface Ni aluminate species. The TPR profile of Ni/Siral-30 displays an increasing signal beginning around 500 °C, rising to a broad maximum around 700 °C. In contrast, Ni/Siral-5 does not evidence a significant reduction below ~600 °C. Instead, Ni/Siral-5 exhibits high-temperature H
2 uptake that does not return to baseline at 800 °C; thus, a H/Ni ratio less than 2 is expected. The TPR profile of Ni/Al
2O
3 exhibits a small peak at ~530 °C and strong, overlapping but clearly discernible components at 690 °C and 800 °C. Ni/Al
2O
3 catalysts prepared by IWI and calcined at 500 °C can contain difficult-to-reduce surface NiAl
2O
4 spinel (tetrahedral Ni
2+) and inverse-spinel (octahedral Ni
2+) species [
20,
21]. The X-ray diffractogram of Ni/Al
2O
3 did not show evidence of bulk NiAl
2O
4, but the Ni 2p XP spectrum of Ni/Al
2O
3 is fully consistent with NiAl
2O
4. Moreover, the high-temperature TPR peaks are closely similar to those assigned by Boukha et al. [
20] to the reduction of Ni
2+ ions in NiAl
2O
4. The small peak at ~530 °C could be assigned to isolated Ni
2+ ions and/or NiO nanoparticles interacting strongly with the support.
2.4. NH3 TPD
NH
3 TPD profiles are shown in
Figure 6A for (1) γ-Al
2O
3 derived by calcining boehmite at 500 °C and (2) a Ni/Al
2O
3 catalyst prepared by IWI of the resulting support with subsequent calcination at 500 °C. The NH
3 TPD profiles are closely similar and characterized by an asymmetric peak at 200–300 °C with a high-temperature tail. The surface acidity of γ-Al
2O
3 is typically attributed to surface Al-OH groups (weak BAS) and coordinatively unsaturated (
cus) tetrahedral Al
3+ sites (Lewis acid sites, LAS) based on FTIR measurements of basic probe molecules [
25,
26]. Ni/Al
2O
3 displays substantially more NH
3 desorption than γ-Al
2O
3, consistent with the presence of Ni
2+ LAS. NH
3 TPD profiles for the calcined Siral supports and the Ni/Siral catalysts are shown in
Figure 6B. Siral-70 and Siral-30 demonstrate ~0.45 mmol/g NH
3 desorption, and Ni/Siral-5 slightly less (~0.40 mmol/g). Although the Siral supports exhibit similar densities of total acid sites, the relative contributions of BAS and LAS are expected to vary with the Si/Al ratio [
13]. Siral-5 and Siral-30 exhibit desorption bands similar to γ-Al
2O
3 characterized by a peak at ~180 and one at ~275 °C that tails off at high temperature. Siral-70 has a smaller low-temperature (180 °C) peak and another at 310 °C arising from strong BAS, i.e., Si-OH-Al moieties [
27]. Siral-70 also has a weak high-temperature TPD peak at ~550 °C, consistent with strong LAS. Ni/Siral-5 and Ni/Siral-30 exhibit greater NH
3 desorption peak areas than the corresponding supports, consistent with adsorption on BAS and Ni
2+ LAS [
20]. Conversely, Ni/Siral-70 demonstrates a substantially lower NH
3 desorption peak area than the bare support. Notably, the BAS peak at 310 °C is strongly suppressed, and it seems reasonable to infer that Ni
2+ species exchange with protons during catalyst preparation. These BAS in Siral-70 are probably associated with interstitial Al
3+ and act as Ni
2+ grafting sites.
2.5. DRIFTS
The
v(OH) DRIFT spectra of the catalysts after in situ pretreatment at 350 °C are shown in
Figure 7. The spectrum of Siral-70 (
Figure 7A) closely resembles that of amorphous SiO
2, indicating essentially complete encapsulation (coverage) of γ-Al
2O
3 by silica [
13]. Siral-70 exhibits a single sharp
v(OH) peak at 3743 cm
−1 assigned to isolated Si-OH groups, as found on weakly acidic SiO
2 surfaces. Despite its similar IR spectrum, the stronger surface acidity of Siral-70 has been confirmed by NH
3 TPD (this work) and other techniques [
23]. The decreased area of the
v(OH) band associated with vicinal (H-bonded) OH groups (broad maximum at ~3400–3700 cm
−1) on addition of Ni
2+ to Siral-70 can be explained by divalent ion exchange with vicinal (H-bonded) Si-OH groups [
28]. The
v(OH) spectrum of Siral-30 also comprises bands assigned to isolated and vicinal Si-OH species despite its relatively high alumina content (
Figure 7B). Moreover, the Siral-30 surface is substantially more Si-rich than the bulk (
Table 2). Daniell et al. [
13] determined that silicon-aluminum oxides derived from Siral-30 and Siral-40 after calcination at 550 °C were covered by silica-rich layers, as evidenced by a sharp isolated
v(OH) at 3743 cm
−1. These silica-alumina samples exhibited the strongest BAS according to low-temperature CO IR measurements [
13]. Ni/Siral-30 demonstrates a substantial loss of isolated and bridging surface OH groups (based on peak area) when compared to the bare support, evidencing ion exchange of Ni
2+ species. Siral-5 displays primarily bands associated with γ-Al
2O
3 with a minor contribution from isolated Si-OH species at 3747 cm
−1 (
Figure 7C) [
25]. Upon addition of Ni
2+, the DRIFT spectrum indicates loss of isolated and vicinal Si-OH groups and an increase in one type of bridging (vicinal) Al-OH groups. Our results are consistent with previous work indicating that Siral-5 comprises isolated patches of SiO
2 on a γ-Al
2O
3 surface [
14,
16].
The
v(CO) DRIFT spectra of the catalysts after in situ pretreatment at 350 °C and CO adsorption at 20 °C are shown in
Figure 8. The observed peaks arise from CO interacting with Ni
2+ species because they were not observed for the pretreated supports after CO exposure at 20 °C. Only in measurements at sub-ambient temperatures have carbonyl bands (2190–2150 cm
−1) assigned to
cus-surface Al
3+ or BAS been reported [
29]. Moreover, CO does not reduce the Ni
2+ species to Ni
+ under these conditions [
30]. Ni/Siral-70 exhibits a broad band at 2201 cm
−1 that may be composed of several individual components. We assign this peak to CO adsorbed on isolated Ni
2+ ions by comparison to the spectra of CO coordinated to Ni
2+ ions hosted in zeolites, e.g., Ni-Beta [
31]. In comparison, Stoyanova et al. [
23] observed
v(CO) peaks at 2195 and 2191 cm
−1 (depending on Ni loading) for Ni/Siral-70 catalysts (prepared by grafting and IWI) and exposed to CO at sub-ambient temperatures. Ni/Siral-30 displays a medium-intensity
v(CO) band at 2184 cm
−1 with a small shoulder at ~2200 cm
−1. The former may be assigned to CO coordinated to
cus Ni
2+ ions on NiAl
2O
4 crystallite surfaces [
32], and the latter to CO on isolated Ni
2+ ions. Alternatively, the 2184 cm
−1 peak may be assigned to CO adsorbed on NiO nanoparticles [
8,
9], and this assignment is consistent with HAADF-STEM images of this catalyst (
Figure 4C). Ni/Siral-5 exhibits an intense, nearly symmetrical
v(CO) peak at 2184 cm
−1 that may be assigned to
cus Ni
2+ ions on NiAl
2O
4 surfaces or CO on NiO nanoparticles. Unfortunately, HAADF-STEM images of this catalyst are not available. In contrast, Ni/Al
2O
3 exhibits an asymmetric peak centered at 2172 cm
−1 with a second component at ~2184 cm
−1. Because the XPS and TPR results for Ni/Al
2O
3 are fully consistent with NiAl
2O
4, we assign the 2172 cm
−1 peak to CO interacting with
cus Ni
2+ cations on this surface phase. Previous work indicates that SiO
2 interacts with the most reactive surface sites of Al
2O
3, thereby reducing the strength of the Ni
2+-support interaction (relative to γ-Al
2O
3) [
16]. This is consistent with the lower CO DRIFTS frequency for Ni/Al
2O
3 when compared to Ni/Siral-5. The
v(CO) frequencies reflect the Lewis acidity of the Ni
2+ ions in exchange sites (higher frequency = stronger LAS) and indirectly the Bronsted acidity of the original proton exchange sites. The nature of the site (spinel tetrahedral or inverse-spinel octahedral) and the degree of coordinative unsaturation may impact Ni
2+ Lewis acidity and therefore the observed CO stretching frequency. We state with some confidence, however, that the Ni
2+ sites associated with the 2172-cm
−1 band are significantly less Lewis acidic than isolated Ni
2+ species on Siral-70 (or Siral-30).
2.6. EO Catalysis
Temporal conversions and steady-state EO product distributions from the Ni/Siral catalysts at 225 °C, 11 bar, and 6 h
−1 WHSV are presented in
Figure 9. The Ni/SiO
2 and Ni/Al
2O
3 catalysts were inactive (<2% conversion), confirming that NiO crystallites and NiAl
2O
4 have negligible EO activity under these conditions. Ni/Siral-70 was the most active catalyst; however, Ni/Siral-30 also gave comparable (>50%) EO conversion. Catalyst deactivation with time-on-stream (TOS) during these relatively brief runs was insignificant. The oligomer product distribution approximated Schulz–Flory behavior with ~63% butene selectivity. Ni/Siral-70 produced a slightly higher yield of C10 products than Ni/Siral-30. In contrast, Ni/Siral-5 exhibited only ~7% conversion with 80% C4 selectivity; C8 and C10 oligomers were not detected for Ni/Siral-5. The iC4/1C4 ratio [sum of internal C4 isomers to 1-butene] increases linearly with conversion over the Ni/Siral catalysts with a non-zero
y-intercept (
Figure 10). There is also a modest trend of decreasing
cis/
trans ratio with increasing conversion. We infer that
cis/
trans-2-butene and 1-butene are primary EO products [
15,
33,
34]. Isobutene and odd-numbered oligomers require catalysts containing strong BAS and were detected in minor concentrations only over Ni/Siral-30 and Ni/Siral-70.
EO catalysis at 225 °C and 11 bar was investigated using a feed stream containing 44% ethylene, 44% ethane, 4.5% methane, 2% H
2, 4.5% CO
2, 0.9% propylene, and 0.1% CO that was intended to simulate an ethane ODH product stream. Catalyst performance was compared to results obtained using a 50/50 ethylene/N
2 feed under equivalent conditions. The Ni/Siral-5 catalyst gave very low (<10%) ethylene conversion irrespective of the feed mixture (
Figure 9). In contrast, the Ni/Siral-70 catalyst displayed substantial activity with only slight deactivation with TOS. EO conversion over Ni/Siral-70 was nearly equivalent using the simulated ODH product mixture and a 50/50 ethylene/N
2 mixture, indicating a negligible impact of reactive impurities on catalyst performance [
35]. The EO product distributions over Ni/Siral-70 were closely similar to each other; however, the addition of diluents appeared to reduce the chain-growth probability slightly with respect to 100% ethylene. Ethane, methane, and CO
2 were non-reactive diluents, whereas propylene reacted over Ni
2+ oligomerization sites [
36]. The simulated ODH mixture gave lower conversion than the 50/50 ethylene/N
2 mixture over Ni/Siral-30 consistent with the effect of catalyst poisons, e.g., CO. DRIFT spectra of the catalysts (
Figure 8) indicate that both Ni/Siral-30 and Ni/Siral-70 adsorb CO at 20 °C, and although the relevant absorption coefficients are unknown, Ni/Siral-30 does have a substantially smaller initial Ni
2+-CO peak area than Ni/Siral-70. Assuming the active sites to be isolated Ni
2+ ions (vide infra), CO DRIFTS and TPR indicate this species to be less abundant in Ni/Siral-30 than Ni/Siral-70. We suggest that the lower concentration of active sites renders Ni/Siral-30 more susceptible to catalyst poisoning (e.g., by CO) than Ni/Siral-70.
Additional EO reactor runs were performed at 120 °C and 26 bar (low-temperature, high-pressure conditions) using fresh catalyst and a 50/50 ethylene/N
2 feed (
Figure 11). Ni/Siral-70 and Ni/Siral-30 gave 6–8% conversion under these conditions, the former being more active. High-pressure and low-temperature operation in the presence of CO was expected to have a deleterious effect on catalyst activity. Follow-on measurements using the simulated ODH feed (
Figure 11) gave very low activity consistent with catalyst poisoning. After a run using the simulated feed at 26 bar, the Ni/Siral-30 catalyst was kept in the reactor and heated to 300 °C in flowing N
2 to ascertain whether thermal catalyst regeneration was possible. For comparison, a fresh Ni/Siral-30 catalyst was tested at 225 °C and 26 bar using a 50/50 ethylene/N
2 feed mixture (denoted Run 1), and catalyst performance was comparable to that obtained using 11 bar of 100% ethane. The regenerated Ni/Siral-30 catalyst, however, gave only ~15% conversion at 225 °C with the simulated feed, and there was significant deactivation with TOS (Run 2). After a second attempted regeneration, the catalyst was tested at 225 °C using a 50/50 ethylene/N
2 feed, and ~30% conversion with relatively stable activity was observed (Run 3). The difference in steady-state conversion observed for Runs 1 and 3 can be explained by assuming a significant fraction of Ni active sites remain poisoned following regeneration at 300 °C. Higher regeneration temperatures or time may be required to restore full catalytic activity. Alternatively, some Ni
2+ sites may have been reduced to Ni
+, and regeneration in air or O
2 might be necessary.
2.7. Nature of EO Active Sites
There is reasonable consensus that the EO active sites in Ni/Siral catalysts comprise isolated Ni
2+ ions grafted to an amorphous SiO
2-Al
2O
3 support [
11,
15]. More specifically, the Ni
2+ grafting sites are conjectured to be vicinal surface Si-OH groups with adjacent interstitial Al
3+ ions that enhance Brønsted acidity [
15]. To our knowledge, ours is the first report of Ni/Siral-70 as an EO catalyst; however, the EO activity of Ni
2+ supported on conventional ASA supports is well-known, and Ni/Siral-70 has been evaluated for the conversion of ethylene to propylene [
23]. Moussa et al. [
9] compared several Ni/aluminosilicate catalysts for EO, including Ni-Beta and Ni/Siralox-30, and they found Ni/Siralox-30 to be among the most active catalysts. It should be noted that Ni/Siralox-30 was prepared using a commercial aluminosilicate support (Siralox-30) that was pre-calcined at temperatures > 550 °C and not derived from calcination of Siral-30 at 500–550 °C in the lab. Our EO data indicate that Ni/Siral-70 exhibits comparable to modestly greater activity than Ni/Siral-30, making it one of the most active Ni aluminosilicate catalysts with greater activity than Ni-Beta [
9,
31]. NH
3 TPD provided evidence for the ion-exchange of Ni
2+ species with surface acid sites during the preparation of this catalyst. A CO DRIFTS peak at ~2200 cm
−1, consistent with isolated Ni
2+ complexes grafted to SiO
2-Al
2O
3, was observed for the Ni/Siral-70 catalyst; however, TPR, XRD, and
v(OH) DRIFTS indicate that this catalyst contains a mixture of Ni
2+ species, including bulk-like (inactive) NiO, isolated Ni
2+ ions, and NiAl
2O
4 species (also thought to be inactive). A contribution from NiO nanoparticles also cannot be excluded. Ni/Siral-30 also has substantial EO activity and contains isolated Ni
2+ species grafted to amorphous SiO
2-Al
2O
3; however, these are a minority species represented by a shoulder near 2200 cm
−1 in the CO DRIFTS spectrum. The main peak at 2184 cm
−1 can be assigned to CO coordinated to
cus Ni
2+ ions on NiAl
2O
4 crystallite surfaces [
32] and/or to CO adsorbed on NiO nanoparticles [
8]. The former species is not expected to be active for EO catalysis; however, the latter has been suggested to show activity arising from
cus Ni
2+ ions [
9]. On the basis of extensive characterization, including low-temperature CO FTIR spectroscopy and extended x-ray absorption fine structure (EXAFS) spectroscopy, Lee et al. [
8] inferred that isolated Ni
2+ species grafted to amorphous SiO
2-Al
2O
3 were the predominant active sites in Ni/Siral-30. We concur with their conclusion; however, isolated Ni
2+ species appear to be less abundant in Ni/Siral-30 than in Ni/Siral-70. Ni/Siral-5 comprises a NiAl
2O
4 surface phase and/or NiO nanoparticles and exhibits very low EO activity. Because Siral-5 consists of γ-Al
2O
3 overlaid with isolated islands of SiO
2, strong interaction of the Ni(NO
3)
2 precursor with γ-Al
2O
3 surfaces during calcination leads to formation of a difficult-to-reduce and EO-inactive NiAl
2O
4 surface phase.