Haiming
Yan
,
Teng
Liu
,
Yu
Lv
,
Xianglan
Xu
,
Junwei
Xu
,
Xiuzhong
Fang
and
Xiang
Wang
*
Key Laboratory of Jiangxi Province for Environment and Energy Catalysis, School of Chemistry and Chemical Engineering, Nanchang University, Nanchang, Jiangxi 330031, P.R. China. E-mail: xwang23@ncu.edu.cn
First published on 10th January 2024
To elucidate the valence state effect of doping cations, Li+, Mg2+, Cr3+, Zr4+ and Nb5+ with radii similar to Sn4+ (CN = 6) were chosen to dope tetragonal SnO2. Cr3+, Zr4+ and Nb5+ can enter the SnO2 lattice to produce solid solutions, thus creating more surface defects. However, Li+ and Mg2+ can only stay on the SnO2 surface as nitrates, thus suppressing the surface defects. The rich surface defects facilitate the generation of active O2−/Oδ− and acid sites on the solid solution catalysts, hence improving the reactivity. On the solid solution catalysts active for propane combustion, several reactive intermediates can be formed, but are negligible on those with low activity. It is confirmed that for propane combustion, surface acid sites play a more vital role than active oxygen sites. Nevertheless, for CO oxidation, the active oxygen sites play a more vital role than the acid sites.
Due to its abundant lattice and surface defects/vacancies, tetragonal rutile SnO2, as an n-type semiconducting oxide, finds applications in gas sensors, solar cells, semiconductor devices, and electrode materials.21–23 Previous investigations have validated that the surface defect enables the adsorption and activation of gaseous O2, thus resulting in the generation of abundant active O2− and O22− sites,24–26 whereas these surface oxygen species on pure SnO2 can be relinquished when calcined at temperatures exceeding 300 °C, which thus limits its redox property and reactivity.27,28 The incorporation of secondary metal ions in the SnO2 matrix has been reported to effectively stabilize the surface-active oxygen sites. For example, former studies have demonstrated that the introduction of Cu2+, Fe3+, Cr3+, Ta5+, Ce4+ and Nb5+ in the SnO2 lattice to form solid solutions not only improves the concentration of active surface oxygen sites but also stabilizes them at temperatures higher than 300 °C, due to the formation of more lattice/surface defects and charge imbalance.28–33
The utilization of solid solutions with diverse chemical compositions is crucial for a wide range of catalytic reactions, and has gained significant attention.16,34 As indicated by previous investigations, the formation of steady solid solutions can only be achieved if the two cations possess similar radii and electronegativities.35,36 The additive materials alter the bulk structure and surface defects of the host matrix, which depends on their ionic radii and valence states.
Nevertheless, the effect of doping ions with varied valence states on the structure and reactivity of solid solution catalysts has not yet been investigated systematically. Researchers still lack clear understanding of some important fundamental scientific issues. Aiming to resolve this problem, Li+, Mg2+, Cr3+, Zr4+ and Nb5+ cations with different valence states but having radii similar to Sn4+ have been selected to modify SnO2 by using a sol–gel method, with the expectation to incorporate them into the lattice of SnO2 to obtain solid solutions. The prepared catalysts are tested via CO and propane oxidation to elucidate their surface-active sites and reactivity from different angles. Indeed, it was discovered that while Cr3+, Zr4+ and Nb5+ can be successfully doped in the SnO2 matrix to achieve solid solutions, Li+ and Mg2+ cannot enter the SnO2 lattice because the valence state deviation is too large. Moreover, we found that for CO oxidation, the active surface oxygen sites play a more critical role than the surface acid sites. However, for propane oxidation, the surface acid sites play a more crucial role than the active surface oxygen sites.
Catalysts | Coordination number (CN) | Dopant ionic radius (Å) | Sn/M molar ratioa | Lattice parameters | Average crystallite sizeb (nm) | Average grain sizec | Surface area (m2 g−1) | ||
---|---|---|---|---|---|---|---|---|---|
a = b (Å) | c (Å) | α = β = γ (°) | |||||||
a Measured via ICP. b Calculated using the Scherrer equation with the XRD (110) peak of SnO2. c Measured via HRTEM. | |||||||||
SnO2 | 6 | 0.69 | — | 4.806 | 3.211 | 90 | 7.2 | — | 24.2 |
Li–SnO2 | 6 | 0.76 | 8.0/1 | 4.778 | 3.225 | 90 | 6.9 | — | 26.8 |
Mg–SnO2 | 6 | 0.72 | 7.0/1 | 4.746 | 3.210 | 90 | 4.8 | 4.9 | 42.6 |
Cr–SnO2 | 6 | 0.62 | 8.9/1 | 4.767 | 3.201 | 90 | 5.4 | 5.8 | 40.5 |
Zr–SnO2 | 6 | 0.72 | 9.0/1 | 4.810 | 3.212 | 90 | 6.1 | 6.2 | 30.7 |
Nb–SnO2 | 6 | 0.64 | 9.0/1 | 4.796 | 3.206 | 90 | 5.8 | 6.1 | 32.3 |
Theoretically, to effectively establish a solid solution between two metal oxides, the two metal cations must have a similar radius and electronegativity.31,35 The Sn4+ cations in rutile SnO2 have a coordination number (CN) of 6 and possess an ionic radius of 0.69 Å. The XPS analysis in this study has confirmed the predominant presence of the doping metal cations such as Li+, Mg2+, Cr3+, Zr4+ and Nb5+. Further details of these findings will be described in the XPS section. If these cations possess a CN of 6, their radii will be 0.76, 0.72, 0.62, 0.72 and 0.64 Å, respectively, which are similar to that of Sn4+. According to the basic requirement, it is theoretically feasible to generate stable solid solutions between SnO2 and these cations, whereas the valence states of all cations differ from Sn4+ except for Zr4+, thus potentially affecting the generation of a solid solution structure.
Hence, the catalysts were subjected to Raman analysis for further clarification. The Raman spectra of pure SnO2, as illustrated in Fig. 1(b), exhibit an Eg peak at 476 cm−1, a prominent A1g peak at 633 cm−1, and a minor B2g peak at 775 cm−1.25 Analogously, all the modified catalysts also show these three typical Raman bands, confirming that SnO2 could still be in the crystalline phase. However, the Eg, A1g and B2g peaks of Cr3+, Zr4+ and Nb5+-doped samples are shifted and broadened in contrast to those of pure SnO2, which may be attributed to variations in the SnO2 lattice parameters and the presence of surface vacancies/defects resulting from a solid solution structure.30 In contrast, the samples doped by Li+ and Mg2+ show spectra similar to that of individual SnO2 without evident peak shift and broadening, and a characteristic peak of nitrate was observed around 1075 cm−1.37 This suggests the presence of Li+ and Mg2+ on the surface of SnO2 as nitrates rather than their incorporation into its matrix to produce a solid solution structure. Although Li+ and Mg2+ have radii similar to that of Sn4+, their valence states are very different from that of Sn4+, which may result in too big difference in electronegativity to generate a solid solution structure.
To validate this further, Mg–SnO2 and Zr–SnO2, the two typical samples, were calcined at higher temperatures of 800 and 1000 °C, and analysed via XRD and Raman spectroscopy. As depicted in Fig. 1(a′), the tetragonal rutile SnO2 phase remains the sole crystalline phase for Zr–SnO2, providing evidence for the generation of a stable solid solution structure, whereas for the Mg–SnO2 sample, when being calcined at 1000 °C, a new Mg2SnO4 phase appears, accompanying the disappearance of the surface Mg(NO3)2 species, which is also confirmed by the Raman results shown in Fig. 1(b′). This testifies again that for the Mg-doped samples, Mg(NO3)2 is present on its surface rather than being incorporated into the matrix of SnO2. Without the restriction of the crystal lattice, Mg(NO3)2 reacted with SnO2 at high temperature to produce the Mg2SnO4 compound.38 Indeed, this has confirmed that Cr3+, Zr4+ and Nb5+ are incorporated into the lattice of tetragonal SnO2 to form solid solutions, while Mg2+ and Li+ are present on the surface as nitrates.
All the modified samples exhibit larger surface areas and smaller crystallite sizes than pure SnO2 (Table 1). The solid solution structure typically hinders the crystallization of materials due to disparities in radius and charge distribution.29,39 Therefore, it is not difficult to understand that Cr–SnO2, Zr–SnO2 and Nb–SnO2 have improved surface areas. For Li–SnO2 and Mg–SnO2, although a solid solution structure is not formed, the dispersion of Li and Mg nitrates on the surface can also hinder the crystallization process, thereby resulting in improved surface areas.40
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Fig. 2 HRTEM images and particle size distribution profiles: (a) Mg–SnO2; (b) Cr–SnO2; (c) Zr–SnO2; (d) Nb–SnO2. |
The STEM-mapping images in Fig. 3 reveal a nearly uniform distribution of Sn, M, and O across all the samples, further supporting the presence of Cr3+, Zr4+ and Nb5+ in the SnO2 matrix to generate stable solid solutions, but Mg2+ stays on the surface of SnO2 in the form of highly dispersed nitrate.
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Fig. 4 CO and propane oxidation performance on the catalysts. (a) CO conversion; (b) Arrhenius plots for CO conversion; (c) propane conversion; (d) Arrhenius plots for propane conversion. |
Samples | R w (10−5 mmol g−1 s−1) | R s (10−6 mmol s−1 m−2) | E a (kJ mol−1) | |||
---|---|---|---|---|---|---|
CO | Propane | CO | Propane | CO | Propane | |
a R w, the differential rates normalized by catalyst weight. Measured at 180 °C for CO oxidation and at 300 °C for propane combustion. b R s, the differential rates normalized by catalyst surface area. Measured at 180 °C for CO oxidation and at 300 °C for propane combustion. | ||||||
SnO2 | 2.81 | 4.08 | 1.16 | 1.67 | 64.2 | 92.1 |
Li–SnO2 | 0.74 | 3.70 | 0.28 | 1.38 | 72.4 | 96.9 |
Mg–SnO2 | 1.15 | 7.43 | 0.27 | 1.59 | 64.2 | 84.7 |
Cr–SnO2 | 15.00 | 14.00 | 3.69 | 3.46 | 42.5 | 74.0 |
Zr–SnO2 | 2.86 | 4.93 | 0.93 | 1.66 | 62.8 | 90.0 |
Nb–SnO2 | 32.32 | 9.92 | 10.00 | 3.07 | 36.9 | 81.6 |
Interestingly, the results in Fig. 4(c) and (d) demonstrate that the sequence of both overall and intrinsic activity for propane deep oxidation differs from that observed in CO oxidation. The overall activity is sequenced as Cr–SnO2 > Nb–SnO2 > Zr–SnO2≈ SnO2 > Mg–SnO2 > Li–SnO2. Basically, the intrinsic activity judged by Rs obeys the same sequence. Cr–SnO2 shows much higher activity than Nb–SnO2 and other catalysts, which suggests that for propane deep oxidation, the surface acid sites might play a more vital role than the active oxygen species. Therefore, it is proposed that surface acid sites could play a more critical role here, which can adsorb and activate those organic molecules with rich electrons, such as propane molecules in this work.46,47
Catalysts | H2 uptake amount (mmol g−1) | O/Sn atomic ratio | O2 desorption amount (μmol g−1) | |||
---|---|---|---|---|---|---|
Below 350 °C | Above 350 °C | α | β | α + β | ||
SnO2 | 0.14 | 13.27 | 2.0 | 0.62 | 36.86 | 37.48 |
Li–SnO2 | 0.06 | 12.67 | 2.1 | 0.37 | 31.83 | 32.20 |
Mg–SnO2 | 0.05 | 12.11 | 2.0 | 0.47 | 35.41 | 35.88 |
Cr–SnO2 | 0.63 | 11.13 | 1.9 | 2.66 | 36.84 | 39.50 |
Zr–SnO2 | 0.18 | 11.81 | 2.0 | 0.60 | 37.17 | 37.77 |
Nb–SnO2 | 0.80 | 11.62 | 2.0 | 3.08 | 38.65 | 41.73 |
EPR experiments were thus carried out using some typical samples to identify the facile oxygen species. The catalysts exhibit two bands at g = 2.004 and 2.002, as depicted in Fig. 5(b), which are assignable to surface O2−.48 The order of the peak integrated areas is as follows, Nb–SnO2 > Cr–SnO2 > SnO2> Mg–SnO2, in agreement with the CO oxidation activity sequence. The existence of surface O2− suggests that it may serve as one of the significant oxygen centres for CO oxidation.
The broad and significant reduction peak above 400 °C can be attributed to the reduction of Sn4+ to Sn0,24,25 which is further validated by the O/Sn molar ratio around 2 as shown in Table 3. With the doping of Nb5+ and Cr3+ to form solid solutions, the mobility of the lattice oxygen is obviously increased, thus becoming easier to be reduced.
The oxygen characteristics of the catalysts have been analysed from different perspectives using O2-TPD. The desorption peaks observed in Fig. S1 (ESI†) can be categorized into two groups: one group, denoted as α type, occurs in the temperature range of 50–200 °C and corresponds to the release of loosely bonded surface oxygen;24,49 while the other group, referred as β type, appears between 200 and 700 °C and is associated with the release of surface lattice O2−.24,49 As quantified in Table 3, the integrated areas of the α peak for Cr–SnO2 and Nb–SnO2 show significant improvement, indicating the presence of a larger amount of surface facile oxygen compared to individual SnO2. For Li–SnO2 and Mg–SnO2, the amount of this part of oxygen species becomes smaller. The variation in the integrated areas of the β peak exhibits a comparable trend, indicating that the surface lattice oxygen of Cr–SnO2 and Nb–SnO2 becomes also more mobile. However, since most of the surface lattice oxygen releases at much higher temperature, it is believed that the surface facile oxygen could contribute predominantly to the reactions. The amount of the desorbed facile oxygen is sequenced as Nb–SnO2 > Cr–SnO2 > SnO2 ≈ Zr–SnO2> Mg–SnO2> Li–SnO2, being consistent with the CO oxidation performance.
In contrast, the in situ DRIFTS results in Fig. 6(d) obtained with Mg–SnO2 exhibit that no any surface Oδ− (0 < δ < 1) is present, and the generation of surface O2− species is also negligible, which explains its poor oxidation activity. In brief, the in situ DRIFTS results have substantiated that besides surface O2− species, Oδ− (0 < δ < 1) might be another kind of facile oxygen sites contributing to the reactions for those samples possessing a solid solution structure.
The XPS O 1s peaks are thoroughly analysed based on the in situ DRIFTS and EPR results. The unsymmetrical O 1s peak, as depicted in Fig. 7, can be fitted into three peaks centered at approximately 530.0, 531.0, and 533.0 eV, corresponding to the surface lattice O2−, CO32−/OH− and O2− anchored on the defects of the surface.52,53 The O2−/O2− ratios have been calculated in Table S1 (ESI†) to discern the effect of different dopants on the quantity of surface-active oxygen. Interestingly, the ratios are sequenced as Nb–SnO2 > Cr–SnO2 > Zr–SnO2 ≈ SnO2 > Mg–SnO2> Li–SnO2, well consistent with the O2-TPD and CO oxidation activity order. Nb–SnO2 and Cr–SnO2, the two samples with a solid solution structure, show much higher O2−/O2− ratios than pure SnO2. In contrast, the doping of Zr4+ into the SnO2 lattice improves the O2−/O2− ratio only slightly. This seems to imply that doping the SnO2 lattice with cations having varied valence states (Cr3+ and Nb5+) can create more surface defects than doping with cations having the same valence state (Zr4+), thus inducing the creation of a larger amount of surface-active oxygen anions. Notably, Li–SnO2 and Mg–SnO2 possess lower O2−/O2− ratios than pure SnO2, testifying that the Li and Mg nitrates dispersed finely on the surface can suppress surface defects. The observed O2−/O2− ratio change achieved via XPS is in agreement with the H2-TPR, O2-TPD, and EPR results, demonstrating consistency with the catalytic activity, especially for CO oxidation.
Sample | NH3 desorption amount (×10−2 mmol g−1) | Relative propane desorption amount (a.u.) |
---|---|---|
SnO2 | 0.74 | 25.27 |
Li–SnO2 | 2.01 | 28.37 |
Mg–SnO2 | 2.61 | 30.85 |
Cr–SnO2 | 5.20 | 100 |
Zr–SnO2 | 1.09 | 23.95 |
Nb–SnO2 | 3.67 | 65.87 |
The quantification results in Table 4 demonstrate that a solid solution sample with more surface defects generally owns a larger amount of surface acid sites. The previous reports indicated a strong correlation between the quantity of surface Lewis acid sites and surface defects.29,55,56 Fig. S4(b) (ESI†) displays the propane-TPD profiles, and the quantification results in Table 4 prove that the desorption amount of propane follows the same trend, which indicates that the two types of molecules share the same kind of adsorption sites. The relationship between the desorption amount of propane and the number of surface acidic sites is clearly positively correlated, as demonstrated in Fig. 8. Therefore, surface acidity is considered crucial for propane deep oxidation.
To confirm this further, in situ DRIFTS experiments by adsorbing NH3 and propane with a reversed order were also carried out. As shown in Fig. 9(b), after adsorbing propane at 50 °C firstly on the cleansed catalyst, three peaks are observed around 1617, 1454, and 1241 cm−1. As labelled in the curves, all of the peaks belong to the dissociative adsorption of propane.59–61 In addition, a gaseous propane vibration peak is detected around 2968 cm−1.62 After introducing NH3, the three characteristic peaks were replaced by the four typical peaks of adsorbing NH3. Therefore, it is strongly proved that both NH3 and propane are adsorbed on the acidic sites, which are crucial to activate propane molecules.
In addition, CO and NH3 adsorption was also investigated using the in situ DRIFTS technique following the same procedures. Basically, a similar phenomenon is observed in the adsorption of NH3 and propane. As demonstrated in Fig. 9(c), after the surface of Cr–SnO2 is pre-saturated by NH3 molecules, it is difficult to adsorb CO molecules. As shown in Fig. 9(d), after the surface of Cr–SnO2 is pre-saturated by CO molecules again, NH3 molecules can drive out the pre-adsorbed CO molecules. Since a CO molecule contains π-back bonding, surface acid sites are necessary for its adsorption/activation. But the surface-active oxygen sites may play a more critical role than the surface acid sites for CO oxidation, as discussed above.
The first series: the sample was initially subjected to a purification process at 500 °C in an Ar flow (30 mL min−1) for 60 minutes, followed by a decrease in temperature to 50 °C. Subsequently, a propane feed mixed with Ar was directed into the cell in the temperature range of 50–300 °C. As shown in Fig. 10(a), at 50 and 100 °C, the surface adsorption of propane is very weak, and gas phase propane is obviously detected at 2968 and 2982 cm−1. However, after the temperature is increased to 200 °C, the initially very weak adsorption peaks can be evidently detected. The peaks observed at 2902 and 2876 cm−1 can be attributed to the C-H vibrations of CH, CH2, or CH3 species, suggesting that propane undergoes adsorption, partial oxidation, and cracking on the catalyst surface.63 At 50 °C, the peak at 1620 cm−1 is assigned to the vibration of the CC bond. When the temperature was increased to 100 °C, it was oxidized to form C
O bonds detected at 1676 cm−1.64 When the temperature is higher than 200 °C, new bands appeared at 1542, 1384, 1351, and 1424 cm−1, which are assigned to vas (COO), δs (CH3), O–C–O bonds in carboxylate species and carbonate species, respectively.64,65 The evidence exhibits that the presence of surface O2− species facilitates the partial oxidation of propane adsorbed on the catalyst. As shown in Fig. S5(a) (ESI†), compared with Cr–SnO2, the formation of those intermediate species is not observed on Mg–SnO2, showing that propane cannot be sufficiently activated under the same condition. However, Fig. S5(b) (ESI†) indicates that much weaker intermediate peaks can still be detected on Nb–SnO2, which indicates that propane can only be mildly activated.
The second series: as displayed in Fig. 10(b-I), full adsorption of propane was carried out at 300 °C to generate the intermediates detected in the first series of experiments. After this, 10% O2/Ar was introduced at the same temperature. As shown in Fig. 10(b-II), the intermediate bands exhibited a quick decrease, particularly those in relation to the oxygenates. This observation provides evidence that these adsorption species may serve as reactive intermediates during propane combustion.
The third series: a batch of fresh catalysts was subjected to the same pretreatment process as in the first series of experiments for surface cleansing, followed by temperature controlling at 300 °C. After being fully oxidized in a 10% O2/Ar feed, Fig. 10(c-I) shows that two groups of peaks around 1000 and 1200 cm−1 appear, corresponding to O2− and Oδ− in a sequence. Afterwards, a propane/Ar stream was switched into the cell. Fig. 10(c-II) shows that the Oδ− sites are used up after 15 minutes but some O2− species remain, implying that the former is more active than the latter. At the same time, the detection of the intermediates observed in the initial series of experiments occurs. This suggests that both Oδ− and O2− sites serve as active centres for propane oxidation, potentially exhibiting higher reactivity compared to the surface lattice O2−.
The fourth series: after cleansing the catalyst, the reaction flow consisting of 5000 ppm propane + 10% O2/Ar was introduced into the cell at 300 °C. As shown in Fig. 10(d), after 5 minutes, the formation of the intermediates is obviously detected as well. In contrast, as shown in Fig. S5(a′) and (b′) (ESI†), the formation of the above intermediates on Mg–SnO2 and Nb–SnO2 is marginal under the same conditions, exhibiting that during the reaction process, propane molecules can only be mildly activated. Different from the second series of experiments, with the co-existence of propane and gaseous O2, these intermediates are always detected. This strongly demonstrates that these surface species are the reaction intermediates for propane combustion, which can be formed, consumed, regenerated, and can reach equilibrium quickly under real reaction conditions with gas phase O2.
Based on the in situ DRIFTS results, a possible pathway, propane → propene → acrylaldehyde → acrylic acid → acrylate → CO32− → CO2, is illustrated in Scheme 1.59,60,64 The adsorption of propane molecules on the Cr–SnO2 surface is proposed to be converted into different intermediates, including propylene, acrolein, carboxylate, carbonate species and others. Both the adsorbed Oδ−/O2− species and lattice O2− could be involved in the intermediate formation process, but the Oδ−/O2− anions can react more effectually with the intermediates to produce H2O and CO2.
Therefore, Raman spectroscopy, FTIR spectroscopy and H2-TPR techniques have been used to elucidate the reasons. In comparison with the fresh catalyst, Fig. S7(a) (ESI†) exhibits that the characteristic Raman bands of SnO2 phases disappeared on the partly deactivated catalyst, indicating that its surface composition has been changed. As exhibited in Fig. S7(b) (ESI†), a sulphate peak at 1000 cm−1 is observed obviously via FTIR spectroscopy. Additionally, the H2-TPR results in Fig. S7(c) (ESI†) have proven that the low temperature reducing peak belonging to the surface facile oxygen nearly disappears. This strongly shows that when water vapor and sulphur oxide are co-fed into the reaction flow, some stable surface sulphates are generated, which can damage the surface-active oxygen centres, thus being harmful to the catalytic reactivity.
In turn, these defects/vacancies can promote the generation of a higher concentration of surface-active oxygen species (Oδ− and O2−), which are favourable to CO oxidation and propane combustion.66–69 It is also discovered that for the three solid solution catalysts, if the doping cations (Cr3+ and Nb5+) have more varied valence states than Sn4+, there is a higher formation of surface defects than Zr4+ having the same valence state. Therefore, Nb–SnO2 and Cr–SnO2 possess a higher concentration of surface-active oxygen sites than Zr–SnO2, displaying better oxidation activity.
However, although Li+ and Mg2+ have radii similar to Sn4+ at CN = 6, their valence state deviation is too big to form a solid solution structure, thus Li and Mg nitrates are present on the catalyst surfaces, which can cover and suppress the surface defects/vacancies of SnO2. As a result, Li–SnO2 and Mg–SnO2 exhibit lower oxidation activity than individual SnO2.
Most interestingly, though the concerted interaction between surface active oxygen and acidic sites is important for CO oxidation and propane oxidation, the two kinds of active sites have different weights in the two reactions. Fig. 11(a) displays that the activity of CO oxidation is almost positively correlated to the surface-active oxygen amount but not to the surface acid site amount. This indicates that the surface facile oxygen is more effective for CO oxidation than the surface acidity. However, Fig. 11(b) shows that the propane combustion activity is nearly proportional to the quantity of surface acid sites but not to the quantity of surface-active oxygen sites. This testifies that different from the case of CO oxidation, surface acid sites could play a more crucial role than the active oxygen species for propane combustion.
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Fig. 11 (a) CO oxidation rates versus facile oxygen amount and NH3 desorption amount; (b) propane oxidation rates versus facile oxygen amount and NH3 desorption amount. |
(1) XRD and Raman results have proven that Cr3+, Zr4+, and Nb5+ can be successfully incorporated into the matrix of SnO2 to substitute part of the Sn4+ to form solid solutions, which results in more abundant surface defects. In contrast, due to too big deviation of the valence state from Sn4+, Li+ and Mg2+ cannot enter the lattice of SnO2 but can mainly be present in the form of nitrates on the catalyst surfaces, thus suppressing the surface defects.
(2) The abundant surface defect on the solid solution catalysts promotes the generation of both active surface oxygen (O2− and Oδ−) and acid sites, thus improving catalytic performance. It is concluded that the active oxygen sites play a more critical role than the acid sites for CO oxidation. In contrast, the surface acid sites play a more crucial role than the active oxygen sites for propane combustion.
(3) On the active Cr–SnO2 for propane oxidation, reactive intermediates such as adsorbed propylene, acrylaldehyde, carboxylate etc. can be formed effectively. However, on those catalysts with low activity, the formation of these intermediates is negligible.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d3cp05840a |
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