2.1. Catalyst Synthesis and Fresh Catalyst Characterization
A series of catalysts involving 12 wt.% Ni-3 wt.% Cu as the supported metals and different zeolitic materials—namely, SAPO-11, SAPO-34, ZSM-5, and ZSM-22—as the carrier were prepared via incipient wetness impregnation employing the materials and methods described in
Section 3.1. The synthesized catalysts were analyzed by means of inductively coupled plasma mass spectrometry (ICP-MS) to experimentally determine their metal loadings. The results of these tests, which are summarized in
Table A1 within
Appendix A, show that the experimental loadings obtained are close to the nominal loadings targeted.
The textural properties of the bare supports employed and of the catalysts synthesized were determined by means of N
2-physisorption, the results of these measurements being included in
Table 1. The data in
Table 1 clearly show that the textural properties of the bare zeolitic supports vary widely. For instance, surface area, which follows the trend ZSM-22 < SAPO-11 < ZSM-5 < SAPO-34, ranges from 59.6 to 525.7 m
2/g. Unsurprisingly, the surface area of the supported metal catalysts is lower than that of the bare supports, since metal deposition causes some degree of pore filling.
The X-ray diffractograms of the catalysts synthesized are included in
Figure A1 within
Appendix A. The diffraction peaks so denoted are attributed to NiO, peaks at 37.3°, 43.3°, and 62.9°, respectively, representing its (111), (200), and (220) planes [
22]. The fact that no peaks associated with Cu species were observed can be attributed to the lower Cu loading and/or to Cu species being highly dispersed, which is in agreement with previous reports on NCSAPO-11 [
15]. The Scherrer equation was applied to the diffraction peak at 43.3° to determine the average NiO particle size, which afforded the values included in
Table 1. The average NiO particle size ranges from 21.9 to 28.4 nm and it follows the trend NCZSM-22 < NCSAPO-11 ≈ NCSZM-5 < NCSAPO-34. Notably, the latter trend is the same as that observed for the surface area of the bare supports, which is at odds with the fact that carriers with a higher surface area would be expected to stabilize supported metals in the form of smaller particles and suggests the presence of amorphous and/or sub-nanometric Ni species not detected by means of XRD. Additional information regarding metal dispersion was acquired through H
2 pulse chemisorption measurements, which resulted in the data included in
Table 2. The trend observed for H
2 uptake and metal-specific surface area—namely, NCSAPO-34 < NCSAPO-11 < NCSZM-5 < NCZSM-22—is also indicative of the metal dispersion trend followed by these catalysts.
More detailed information regarding the elemental composition and chemical environment of the surface of the catalysts surveyed was acquired via X-ray photoelectron spectroscopy (XPS) measurements, which were performed after reducing the catalysts using the conditions and approach described in
Section 3.2.
Table 3 summarizes the results of these analyses in terms of the surface concentration and oxidation state of the supported metals, while
Table A2 and
Table A3 in
Appendix A provide more detailed information vis-à-vis the elemental surface composition and the supported metal species of the catalysts as determined via XPS. Full scans as well as Ni and Cu 2p regions of X-ray photoelectron spectra are included in
Figure A2,
Figure A3 and
Figure A4 within
Appendix A. The XPS analysis of NCSAPO-11 and NCZSM-5 clearly showed that the entirety of Ni is present in the metallic state in these two catalysts. Similarly, the low intensity of the Ni 2p
3/2 satellite peak in the spectra of NCSAPO-34 and NCZSM-22 suggests that Ni is mostly reduced in these two formulations. However, the inhomogeneous character of these two samples precludes the neutralization of charging effects, which cause peak broadening and the appearance of a supplemental peak in the spectra of NCZSM-22 and NCSAPO-34, respectively, and make it impossible to accurately determine Ni
0 concentration.
The most salient feature of the data in
Table 3 is the surface concentration of the metals, which follows the trend NCSAPO-34 > NCZSM-22 >> NCSAPO-11 > NCZSM-5. However, the surface concentration of Cu
0 shows a slightly different trend—namely, NCZSM-22 > NCSAPO-34 > NCZSM-5 > NCSAPO-11—which confirms that the reducibility of the surface metals varies across these catalysts. Indeed, the trend observed vis-à-vis the fraction that Cu
0 represents of the total surface metal is NCSZM-5 > NCSZM-22 > NCSAPO-34 > NCSAPO-11. Admittedly, it is difficult to relate particle size information estimated from XRD, metal-specific surface area results from H
2 pulse chemisorption, and surface concentration data on the supported metals derived from XPS. This can be attributed to the heterogeneity of Ni and Cu species expected to result from the deposition of these metals via impregnation on the zeolitic materials employed, since Ni and Cu can be expected to be present not only as nanoparticles but also as amorphous clusters and/or sub-nanometric species at different locations of the carriers. For instance, the fact that the Cu
2O signal is observed at much higher binding energy than usual—see
Table A3 and
Figure A4 in
Appendix A—may suggest an ionic Cu species exchanged on zeolitic Brønsted acid sites. Nevertheless, the results above provide valuable insights regarding the size of metal nanoparticles, metal-specific surface area, as well as the surface concentration and oxidation state of the supported metals.
The acidity of the catalysts used in this study was assessed by means of ammonia temperature-programmed desorption (NH
3-TPD) given the importance of surface acidity to several reactions and phenomena of interest, including isomerization and cracking as well as coke-induced deactivation. In terms of total acidity, the catalysts followed the trend NCSAPO-34 > NCSAPO-11 > NCZSM-5 > NCZSM-22 (see
Table 2), which is in overall agreement with previously reported acidity trends for the bare supports [
23,
24]. In contrast with previous reports focused on the bare supports, most acidity was found to be associated with weakly acidic sites (from which ammonia desorbs below 250 °C) albeit a smaller number of sites of medium acidity (from which ammonia desorbs between 250 and 400 °C) were also found to be present (see
Figure 1). The fact that strongly acidic sites (displaying higher NH
3 desorption temperatures) were not observed can be attributed to the fact that these sites would represent the main adsorption and anchor sites for metal precursors and particles, respectively. Thus, any strongly acidic sites—along with most sites of medium acidity—would be occupied during catalyst synthesis, leaving only weakly acidic sites and the relatively small number of sites of medium acidity observed.
2.2. BG Conversion to SAF
The BG sample used in this study was analyzed via gas chromatography (GC) and found to be composed entirely of C18 and C16 FFAs as shown in
Table A4 in
Appendix B. This feed was upgraded over the catalysts synthesized using the equipment and methods described in
Section 3.3, the experimental approach employed used for the GC analysis of both the feed and the reaction products being described in
Section 3.4. The results of these upgrading experiments and analyses are summarized in
Table 4. Saliently, both BG conversion and the fraction of aviation fuel-range alkanes (C8–C16 hydrocarbons) in the reaction products follow the trend NCSAPO-11 < NCSAPO-34 < NCZSM-5 ≈ NCZSM-22, which suggests that 12 wt.% Ni-3 wt.% Cu catalysts supported on the socony mobil zeolites tested afford better results that the corresponding formulations involving the silicoaluminophospate zeotypes essayed. Parenthetically, the inferior conversion of NCSAPO-11 is likely not due to its relatively low concentration of surface Ni
0 and Cu
0 (see
Table 3), which represent the active sites for the deCO
x reactions. Indeed, NCZSM-5 affords quantitative conversion despite displaying a slightly lower concentration of Ni
0 than NCSAPO-11 and the second lowest concentration of Cu
0 of all catalysts tested. Similarly, differences in conversion cannot be assigned to the surface Ni
0/Cu
0 concentrations of these catalysts, since the ratios for NCSAPO-11 and NCZSM-5 are 10.5 and 3.0, respectively. Instead, differences in conversion can be attributed—at least in part—to the propensity of these formulations towards fouling and coking (see
Section 2.3). ZSM-supported catalysts also afford better results than SAPO-supported formulations in terms of the selectivity to the hydrocarbon families comprising aviation fuel, since the catalyst supported on SAPO-11 and SAPO-34 displayed almost identical selectivity of ~88.5% n-alkanes, ~7.5% iso-alkanes, ~2.5% cycloalkanes, and ~1.5% aromatics. In contrast, the catalysts supported on ZSM-5 and ZSM-22 showed lower selectivity to n-alkanes and higher selectivity to the other hydrocarbon families comprising aviation fuel. Among these, NCZSM-5 afforded the highest selectivity to iso-alkanes and cycloalkanes, as well as a yield of aromatics within the 8–25% specified for aviation fuel [
25].
To elucidate the fate of the oxygen atoms in the BG feed, the gas stream produced during the upgrading of BG over NCZSM-5 was analyzed with a refinery gas analyzer (RGA) and found to contain 0.45% CO and 0.26% CO
2 as the only oxygen-bearing compounds, which is unsurprising since deoxygenation proceeds via deCO
x. The other compounds detected by the RGA were hydrogen (the reaction atmosphere) and C1–C6 hydrocarbons resulting from CO
x methanation and/or the cracking of alkyl chains, which is consistent with previous reports [
26].
Figure 2 shows the carbon number distribution of the product mixtures resulting from upgrading experiments. Irrespective of the catalyst support employed, most hydrocarbon products were found to be within the C8–C16 range characteristic of aviation fuel (with the remainder being ≥C17 hydrocarbons). However, SAPO-supported catalysts show noticeable differences in terms of the carbon number of the reaction products relative to those obtained over ZSM-supported formulations. Indeed, NCSAPO-11 and NCSAPO-34 yield a considerable and comparable amount of C15 and C11 hydrocarbons, these two carbon numbers representing the most abundant among the products obtained over these catalysts. In contrast, NCZSM-5 and NCZSM-22 afford much lower amounts of C15, since lighter (≤C13) hydrocarbons are favored among which C10 hydrocarbons are the most abundant.
These results cannot be readily explained by the relative acidity of the supports favoring cracking reactions—since ZSM-supported catalysts have a total acidity that is either slightly (NCZSM-5) or much lower (NCZSM-22) than SAPO-supported formulations—albeit this can be attributed to the fact that most of the acid sites in these supports are either weakly or moderately acidic (see
Figure 1) with a relatively low activity towards C-C cleavage [
27,
28]. Instead, these results can be rationalized by invoking the metal-specific surface area of ZSM-supported catalysts, which is much higher than that of their SAPO-supported counterparts (see
Table 2). Indeed, it can be argued that a higher concentration of surface metal sites would increase the metal-catalyzed hydrogenolysis of C–C bonds, which in turn would favor the formation of lighter—at the expense of heavier—hydrocarbons. The relatively low concentration of surface Ni
0 within NCSAPO-11 can only partially explain the lower cracking activity of this catalyst, since NCZSM-5 displays a slightly lower concentration of surface Ni
0 (see
Table 4). In addition to the aforementioned heterogeneity of Ni and Cu species, the lack of a consistent trend in this regard can also be attributed to the relative distribution of these metals on the catalyst surface, since C–C hydrogenolysis reactions require contiguous Ni atoms to be catalyzed [
29] and Cu can disrupt Ni adjacency [
30], curbing cracking reactions through both geometric and electronic effects [
12,
30,
31,
32]. However, the ability of Cu to disrupt Ni adjacency and cracking reactions appears to be limited in these catalysts, since NCSAPO-11 displays a lower cracking activity than NCZSM-5 despite having a much higher surface Ni
0/Cu
0 concentration ratio (10.5 vs. 3.0).
Given that the results in
Table 4 preclude the identification of NCSZM-5 or NCZSM-22 as the most active catalyst (since both formulations afforded quantitative conversion), upgrading experiments were performed in which the amount of BG employed was doubled relative to that specified in
Section 3.3. The results of these experiments are summarized in
Table A5 in
Appendix B. Surprisingly, both catalysts displayed quantitative BG conversion and practically identical selectivity to C8–C16 hydrocarbons under these conditions. An additional effort was made to identify the most active formulation between NCSZM-5 or NCZSM-22 by halving the amount of catalyst relative to the amount used in the experiments that afforded the data in
Table A5. However, conversion remained quantitative, which suggests that testing these catalysts in a fixed-bed reactor, which would allow for additional variables (such as space velocity and time on stream) to be investigated—represents a better approach to enable this comparison. Previous reports on the upgrading of BG over supported Ni-Cu catalysts indicate that fixed-bed reactor experiments are also the best was to study catalyst stability and recyclability [
12]; however, those experiments fall outside of the scope of this work and will be the focus of a future contribution.
2.3. Spent Catalyst Characterization
In an effort to rationalize the results of BG upgrading to SAF, the spent catalysts were analyzed by means of thermogravimetric analysis (TGA). Indeed, TGA offers a way to determine the amount of type of the carbonaceous deposits that accumulate on the catalyst surface in the course of the reaction, which can in turn serve as a gauge for the catalyst deactivation caused by fouling and coking. Parenthetically, coking and fouling represent the main deactivation mechanism for supported Ni-Cu catalysts used for the conversion of oleaginous biomass to fuel-like hydrocarbons, since metal loss due to leaching or even the formation of volatile carbonyls has been found to be negligible [
12,
15]. The results of these TGA measurements are summarized in
Figure 3. Saliently, the spent NCSAPO-11 catalyst displayed the most significant weight loss (~18%), which suggests that fouling and coking could explain (at least in part) the fact that it shows the lowest BG conversion among all catalysts tested. NCSAPO-11 is unique in the sense that it represents the only spent formulation displaying considerable weight losses below 400 °C—which can be assigned to the removal of residual solvent, reactants, products as well as soft coke—as well as weight losses above the same temperature that can be attributed to the combustion of hard coke or graphitic carbon [
33]. Indeed, spent NCSAPO-34 displays the vast majority of its weight loss below 400 °C, whereas spent NCZSM-5 and NCZSM-22 undergo most of their weight loss above this temperature.
In short, it can be argued that coking and fouling can only be invoked to explain catalytic activity when the catalyst displays both a relatively low surface area and a high propensity for coking as is the case for NCSAPO-11. All other formulations display a moderate degree of coking (like NCZSM-22), a relatively high surface area (like NCSAPO-34), or both (as is the case for NCZSM-5). The analysis by means of TGA of the catalysts spent in the experiments resulting in the data within
Table A5 seems to corroborate this conclusion, since the weight loss spent NCZSM-22 and NCZSM-5 displayed, respectively, remained unchanged and increased only slightly (see
Figure A5 in
Appendix B) with no impact on conversion. Lastly, it should be noted that the TGA results can only be partially explained invoking acidity. Indeed, the least acidic catalysts—namely, NCZSM-22—displays the lowest degree of fouling and coking as would be expected. However, the extent of coking and fouling observed for the other catalysts does not show a linear relationship with acidity, which suggests that other variables (like the concentration and relative distribution of Ni and Cu on the catalyst surface) are at play.
2.4. Catalyst Recycling Studies
The recyclability of the catalyst that afforded the most promising results—i.e., NCZSM-5 (see
Section 2.2)—was assessed by testing this catalyst in five sequential BG upgrading reactions. Between reactions, the spent catalyst was regenerated through a procedure comprising a calcination step under static air (to remove carbonaceous deposits from the spent catalyst surface) and a reduction step identical to the one used before the first upgrading reaction (to re-reduce the supported metals oxidized during the calcination step). The results of these experiments are summarized in
Figure 4.
Notably, BG conversion remained quantitative across all reaction cycles. Interestingly, the selectivity to C8–C16 hydrocarbons was 100% in cycles 1 and 2, dropped to 86.5 and 82.7% in cycles 3–4 (due to the formation of oxygenates and C19 hydrocarbons) and increased to 98% in cycle 5 (since much less oxygenates and no C19 hydrocarbons were produced in this last cycle). Parenthetically, the oxygenates detected in some products mixtures were aldehydes, alcohols, ethers, and ketones, which are produced in small amounts via the incomplete deoxygenation of FFAs in BG and through condensation reactions involving oxygenated intermediates. Finally,
Figure 4 also shows how the selectivity to the different hydrocarbon families comprising jet fuel (n-alkanes, iso-alkanes, cyclo-alkanes, and aromatics) varied significantly across cycles.
To rationalize these results, the post-mortem of the NCZSM-5 catalyst recovered at the end of the recycling experiments was performed focusing on Ni-specific metal active sites and on surface acid sites associated with the zeolitic support. H2 pulse chemisorption results showed that the metal-specific surface area of the catalyst dropped from 1.414 m2/g in the fresh catalyst to 0.004 m2/g in the catalyst recovered at the end of the recycling experiments, which clearly indicates a loss of metal sites likely due to metal sintering and coking. Similarly, NH3-TPD measurements indicate that the total acidity of the catalyst dropped from 1.44 mmol NH3/g on the fresh catalyst to 0.59 mmol NH3/g on the catalyst recovered at the end of the recycling experiments, which is indicative of a loss of acid sites attributable to the accumulation of recalcitrant coke deposits.
The results of recycling studies and of the post-mortem catalyst characterization suggests that metal sites within NCZSM-5 have a very high intrinsic activity, since conversion remained quantitative despite the loss of most metal sites. Moreover, changes in the amount of metal active sites and surface acid sites are in line with the changes in selectivity observed during the recycling studies, since structural changes are bound to affect the performance of the catalyst in cracking, isomerization, cyclization, and aromatization reactions. In short, although these studies show the recycling stability of the catalyst in terms of conversion, the results also show variance in terms of selectivity, clearly indicating the direction of future work. However, the latter falls outside of the scope of the present contribution and will be the focus of future studies.