2.1. Catalytic Activity
The prepared catalysts were studied in the combustion reaction of chlorobenzene (CB). The results of the catalytic activity are shown in
Figure 1 and
Table 1, the temperature values corresponding to the 50% conversion of CB (T
50), the 90% conversion of CB (T
90), and the balances of carbon and moles of Cl
2 produced after reaction are reported.
The small differences observed in the T90 values do not present a linear relationship with the increase or decrease in Fe content in the perovskite. However, T50 values decrease with the increase in Fe content. The catalyst that presented the lowest T50 was LaCo0.25Fe0.75O3, whereas the lowest T90 was determined with LaCo0.75Fe0.25O3. At low temperatures, the structures with the highest Fe content resulted in more activity, whereas at high temperatures (from 400 °C), the most active structures were those with the lowest content of this cation.
To corroborate that the catalysts completely convert the CB to its complete combustion products, the total carbon balances were carried out by the indirect method through the valuation of carbonates retained in a trap solution placed at the outlet of the reactor. The carbon balance closed between 0.1 and 0.3%, values that are considered within the error allowed in the calculation of this magnitude (
Table 1). In the same way, the analysis of Cl
2(g) was carried out as an oxidation product of this type of Cl-VOC. Considering that 1.18 × 10
−3 moles of this compound should be obtained as a product under the reaction conditions, the number of moles of Cl
2(g) obtained from this measurement correlated perfectly with the moles of this oxidation product considering a CB complete oxidation (
Table 1).
Kamal et al. reported the CB combustion using mixed oxide-type catalysts (Co
3O
4/Alumina and SnO/MnO/TiO/CrO). They observed that the main cause of deactivation was the saturation of chlorine on the surface and the subsequent formation of intermediates such as organic acids and oxychlorides of the corresponding metals. As was explained in this work, these intermediaries could become more dangerous than the Cl-VOCs to be eliminated [
13]. Rochard et al. detected the formation of intermediates such as benzyl alcohol and toluene during the CB combustion using spinel and perovskite-type catalysts (Mn
0.75Co
2.25O
3 and La
0.9Sr
0.1CoO
3). These intermediates caused the loss of the catalysts’ activity and were the subject of further study due to their high persistence and toxicity compared to that of the VOCs under study [
14]. In the present work, although some minimal differences can be distinguished in the balances of total carbon and Cl
2 that could be associated with the adsorption of Cl on the surface of the catalyst once the reaction has finished, the balances and the total conversion indicated that there was no formation of intermediates or oxychlorides at the end of the reaction test, unlike previously published works. It is worth mentioning that the formation of intermediates at low reaction temperatures cannot be discarded as in situ spectroscopy techniques should be necessary to corroborate it. In addition, the stability of the catalysts was studied under the same reaction conditions but at a fixed temperature, corresponding to the 100% conversion of CB.
Figure 2 shows the variation of the chlorobenzene conversion as a function of time.
As can be seen, the catalyst that began to deactivate in the shortest time was LaCoO3, showing a conversion below 50% after approximately 54 h, while the one that deactivated more quickly (around 45 h) was the catalyst that does not have cobalt in its structure, LaFeO3. On the other hand, the most stable catalysts were those with the lowest Fe content (25% and 50%, respectively). The LaCo0.5Fe0.5O3 catalyst began to deactivate after 50 h, reaching a value of 50% conversion at 65 h. On the other hand, the LaCo0.75Fe0.25O3 catalyst presented excellent stability, maintaining the CB conversion at 100% during the 100 h of reaction without presenting deactivation over time.
A similar study carried out by Wang et al. showed CB conversion to 100% during 9–10 h using Fe-mixed oxide-type catalysts doped with Ni. In this case, despite the excellent results reported, they associated the low stability with the accumulation of Cl in the active sites [
15]. Liu et al. reported a stability of 100% CB conversion for 20 h using perovskite-type catalysts (SmMnO
3) in different proportions of the cations. In this work, these authors informed that a higher proportion of acid sites improved the catalytic capacity, and they also observed that the deactivation of this type of catalyst occurred due to surface poisoning by residual Cl as a product of the combustion reaction [
16]. Effectively, these recently published results evidence the excellent stability of the catalysts presented in our work. In general, the catalysts’ stability increased in the following order: LaFeO
3 ˂ LaCoO
3 ˂ LaCo
0.25Fe
0.75O
3 ˂ LaCo
0.5Fe
0.5O
3 ˂ LaCo
0.75Fe
0.25O
3. In order to find the reason for this catalyst stability order, an exhaustive characterization was created and discussed in the following sections.
2.2. Physicochemical Characterization of the Catalysts
The results of the S
BET analysis are presented in
Table 2. The isotherms could be classified according to the IUPAC as type 3 at low pressures and type 5 at high pressures, being in all cases mesoporous materials, since all the isotherms presented H3-type hysteresis.
The partial substitution of the B position by 25% of Fe slightly increased the original surface area of the LaCoO
3 catalyst. At higher substitution percentages, the surface areas decreased due to the change in geometry that occurs in the structure, although the variations do not reflect a linear relationship. The largest surface area was reported for the catalyst with 25% Fe, corresponding to the catalyst that presented the best activity in the catalytic reaction. Although the reaction under study is a surface reaction, it is clear that the little variation in the surface areas in the fresh and pos-reaction structures (
Table 2) indicates that the catalytic activity cannot be fully attributed to surface area variations.
Figure 3A shows the XRD pattern of the LaCo
1−xFe
xO
3 phases from x = 0 to x = 1. The end members of the family match with the trigonal (
Rc) and orthorhombic (
Pbnm) structures for LaCoO
3 and LaFeO
3, respectively. The mixed Co/Fe phases in these symmetries display that for x = 0.25 and 0.50, it remained as trigonal (
Rc), whereas, for x = 0.75, it stabilized as orthorhombic (
Pbnm). This tendency can be observed in
Figure 3B, where an enlargement of the main peak area can be observed. To confirm these observations, all patterns were refined with the Rietveld method using the
Fullprof software. The Rietveld refinements are illustrated in
Figure S1 (Supplementary Materials). The unit-cell parameters obtained from Rietveld refinements are listed in
Table 3, and the volumes normalized with Z are plotted in
Figure S2.
It can be seen that as the substituted Fe content increased (0 ≤ x ≤ 0.5), the lattice parameters increased, as did the cell volume, which was expected due to the difference in ionic radii (Ri) between Co and Fe: Ri (Co2+) = 0.74 Å, Ri (Co3+) = 0.63 Å, Ri (Fe2+) = 0.76 Å, Ri (Fe3+) = 0.64 Å, and then decreased with a higher degree of substitution (x = 0.75) approaching the LaFeO3 value.
The best deactivation resistance of these solids was observed in the LaCo
0.75Fe
0.25O
3 perovskite, which would indicate that the rhombohedral geometries showed greater stability, maintaining the crystallinity of the solid that only differs from the orthorhombic one due to the coordination distortion of Fe compared to Co [
17]. Given that the reducibility of perovskites depends on the crystalline structure, temperature programmed reduction (TPR) tests were also performed to obtain information about the oxidation state of the cations present in the structure.
Figure 3 shows the TPR curves of the synthesized perovskites:
The LaCoO
3 catalyst presented a reduction profile similar to those reported in the literature for the same phase [
18]. The curve presented two main reduction zones, one from 200 °C to 450 °C and the other from 500 °C to 700 °C. The first corresponds to the reduction of Co
3+ to Co
2+, whereas the second is attributed to the reduction of Co
2+ to Co
0 [
19]. As mentioned by Ciambelli et al. [
20] and Barbero et al. [
21], Fe
3+ would not be reduced under the experimental conditions of the TPR measurement. In agreement with these results, the green curve in
Figure 4 is observed to be completely flattened. Only the reduction of Fe
4+ to Fe
3+ would be expected if Fe
4+ were present.
In general, the reduction temperatures shifted to higher temperatures as the Fe content increased, being the displacement more significant in the reduction of Co
3+/Co
2+ than in the case of Co
2+/Co
0, where it is practically observed that the peak of reduction disappears, indicating that the insertion of Fe stabilizes cobalt in its Co
3+/Co
2+ states. This fact could explain the better behavior of the structures containing Fe in the catalytic reaction. The peak at low temperatures could also be assigned to the transition from Fe
4+ to Fe
4+/Fe
3+; the second, to Fe
4+/Fe
3+ towards Fe
3+. As there is Co in the samples, both peaks would be masked by the reduction of Co
3+ to Co
2+, which also appears in the temperature range from 150 °C to ∼450 °C [
19]. One peak at ∼240 °C is distinguishable in the perovskite with 50% Fe and could indicate the existence of Fe
4+ for this degree of Co substitution, being masked in the rest of the samples by the greater intensity of the reduction of Co
3+ to Co
2+. The incorporation of Fe affects the first reduction stage, modifying the splitting of the first peak of LaCoO
3 perovskite and showing only one peak, probably avoiding an intermediate reduction state. It is also observed that the second reduction peak was displaced at ∼600 °C when the Fe content was increased. This peak, which was assigned to the reduction of Co
2+ to Co
0, decreased in intensity with increasing amounts of Fe and disappeared when the substitution level reached 50%. Furthermore, this peak could also be attributed to the reduction of Fe
n+ to Fe
0 as it was described by Merino et al. [
19], where it was found that this happened when iron was present as free iron oxide outside the perovskite structure. However, the presence of free Fe
2O
3 was ruled out, as pure diffractograms were observed for the perovskite phases obtained. Therefore, only the reduction of Co and a decrease in hydrogen consumption were observed with the increase in iron content, which could indicate the presence of Co
2+ together with Co
3+, as shown in
Table 2 (H
2 consumption). Goldwasser et al. [
22] stated that perovskite structures are more easily reduced when Fe is replaced by Co. However, in our reaction, the opposite effect was observed. This could explain the fact that the extremes (pure Fe and Co perovskites) did not lead to greater stability in the reaction but that a combined composition of cations gave greater resistance effects that were evidenced in the catalytic stability results. In spite of these partial results, a deeper study of the oxidation states of iron and cobalt is essential to know the physicochemical reasons for the high stability of the catalyst. Therefore, Mössbauer and X-ray photoelectronic spectroscopies were used to analyze the redox behavior.
Figure 5 shows the Mössbauer spectra at 298 K and 12 K of the four perovskites with iron. The spectrum corresponding to LaFeO
3 presents a sextet with narrow absorption peaks and a horizontal baseline. These aspects are typical of a solid with magnetic ordering; LaFeO
3 is antiferromagnetically ordered below ≅ 477 °C, without magnetic relaxation and with environments of Fe ions very similar to each other. The hyperfine parameters obtained from the fitting are presented in
Table 4 and
Table 5. These correspond to Fe
3+ ions octahedrally coordinated with a high spin configuration, and they are very similar to those previously reported by other authors for LaFeO
3 [
23,
24]. The value of the quadrupole shift (2ε), nearly equal to zero, indicates that the octahedral environment is highly symmetric. In addition, a central signal (δ = 0.3 mm/s) with a contribution of 1–2% is detected, which could be assigned to a Fe
3+ paramagnetic impurity not detected by XRD due to its low concentration.
Replacing 25% Fe with Co produces a significant change in the spectrum: the peaks broaden considerably and the baseline curves. This behavior indicates that the Fe3+ ions have different environments and that the system undergoes magnetic relaxation phenomena. The change is drastic for the other two compositions, where a complete collapse of the magnetic ordering occurs. Magnetic relaxation can occur by superparamagnetism phenomena or by spin–spin or spin–lattice relaxation. Superparamagnetism manifests itself when the size of the particles is very small, in the nanometer range. In these samples, this effect could be neglected taking into account that they have been calcined at 750 °C and that the XRD diagrams show narrow lines. For this reason, the results can be attributed to modifications in the spin–spin or spin–lattice relaxation modes caused by the replacement of Fe by Co.
The spectra were measured again at 12 K to go below the temperature region where spin dynamics occur and thus to obtain more information. In
Figure 5B, it can be seen that LaCo
0.25Fe
0.75O
3 presents a complete magnetic blocking at this temperature; LaCo
0.5Fe
0.5O
3 still undergoes relaxation phenomena (curved background), whereas LaCo
0.75Fe
0.25O
3 starts to experience the beginning of a magnetic blocking. A similar qualitative effect was reported by Berry et al. for LaCo
0.5Fe
0.5O
3 and LaCo
0.90Fe
0.10O
3 [
25] and by Troyanchuk et al. for LaCo
0.9Fe
0.1O
3 and LaCo
0.6Fe
0.4O
3 [
26]. In both cases, the mixed perovskites were obtained by the ceramic method.
In principle, three sextets could be detected in each mixed perovskite. However, in the case of LaCo0.75Fe0.25O3, the magnetic relaxation phenomena prevent this detection even at a temperature as low as 12 K. Another aspect to mention is that the tendency in the structures with lower Fe concentrations causes the hyperfine magnetic field to strongly decrease, and the width of the distribution of this parameter increases, indicating the presence of an increasing number of environments with slightly different symmetries.
The LaFeO
3 perovskite has a relatively high antiferromagnetic ordering temperature (T
Neel ≅ 477 °C), which shows very strong exchange interactions between the high-spin Fe
3+ ions. This is reflected in the narrow line sextet of the Mössbauer spectrum obtained at 298 K and shown in
Figure 5A. The changes described as a consequence of the increasing substitution of Fe ions by Co ions (appearance of magnetic relaxation phenomena that culminate in the total collapse of the ordering when the substitution reaches 75%, even at a temperature as low as 12 K) indicate that Co causes a very strong dilution of the magnetic interactions among Fe
3+ ions.
Co is found as Co3+ and/or Co2+ and is located in highly symmetrical octahedral sites surrounded by six oxygen anions. Under these conditions, the possible electronic configurations that it could adopt are:
Co3+:
- high spin: t2g4eg2
- intermediate spin: t2g5eg1
- low spin: t2g6eg0
Co2+:
- high spin: t2g3eg2
- intermediate spin: t2g4eg1
- low spin: t2g5eg0
If for each configuration the corresponding magnetic moment is calculated assuming, in a first approximation, that only the spin magnetic moment is considered: μs = (n(n + 2))0.5μB, (where n is the number of unpaired electrons), the following values are obtained:
Based on this analysis, the drastic effect on the magnetic order produced by the substitution of Fe
3+ by Co would be justified if the latter were found as Co
3+ in a low-spin configuration. Other authors have reached similar conclusions for the LaCo
1–xFe
xO
3–d system
30. Recently, a similar effect has been reported when substituting high-spin Fe
3+ for low-spin Co
3+ on the magnetic properties of α-Fe
2O
3, which also presents an antiferromagnetic ordering [
27].
From these results, it can be inferred that if small amounts of Co
2+ are present surely these ions would have a low spin configuration, as it is the one with the lowest magnetic moment. Due to the existence of Co
2+, the electroneutrality of the system can be preserved by the appearance of oxygen vacancies or by the emergence of abnormally high oxidation states of Fe (Fe
4+). It is now accepted that if Fe
4+ is present in the sample when the temperature is lowered, it undergoes the following disproportionation reaction [
28].
Fe
5+ produces a sextuplet whose hyperfine parameters are: H = 265 kG, δ ≅ 0 mm/s, and ε ≅ 0 mm/s [
29]. This implies that the two most intense peaks of the sextet (peaks 1 and 6) should appear at −4.27 and +4.27 mm/s, respectively (their position is indicated in the 12 K spectra with a red dotted line). Evidently, for LaFe
0.75Co
0.25O
3, the line at +4.27 mm/s is not recorded (a “valley” appears in the spectrum in this region). The line at −4.27 mm/s could be hidden by the line “2” of the Fe
3+ signals. However, if this was the case, the envelope corresponding to those lines should be more intense than the envelope of line “5”, which is not the case. Therefore, the presence of Fe
5+ can be ruled out in this sample. Corroborating this conclusion, the characteristic Fe
4+ singlet at δ ≅ 0.16 mm/s is not recorded in the spectrum at room temperature (its position is indicated by a red dotted line in the spectrum at 298 K).
In the case of LaFe
0.5Co
0.5O
3, although the situation is not as clear as with the previous sample, once again, the presence of the −4.27 mm/s line should generate an asymmetry in the envelope of line “2” with respect to line “5” that is not recorded. Similarly, at 298 K, the existence of an Fe
4+ singlet would produce an asymmetry in the central doublet, with the peak on the left being more intense than the one on the right. Therefore, it could also be concluded that there is no charge compensation due to an increase in the oxidation state of Fe ions. In the case of LaFe
0.25Co
0.75O
3, magnetic relaxation phenomena prevent obtaining this type of conclusion. With this technique, it is possible to study the oxidation states in the bulk, which is why XPS was also carried out to identify the oxidation states on the catalysts’ surface.
Figure 6,
Figure 7 and
Figure 8 show the results for Co
2p, Fe
2p, and O
1s, and
Table 6 shows the main data extracted from these graphs.
Figure 6 shows the XPS spectrum of the Co
2p signal. The Co
2p3/2 peak can be deconvoluted into two components, at 778 and 781 eV, assignable to the Co2p and Co3p surface species, respectively, whereas the peak around 793.5 eV, which corresponds to Co2p
1/2, can also be deconvoluted into two peaks due to the existence of these two cobalt species. Between 785–790 eV it is possible to appreciate that as Fe substitution increased, the intensity of a satellite peak in that region increased, showing that the structure is ordered in such a way that both Co species and Fe species coexist. Specifically, in the case of the XPS spectra of Co, this peak indicates the existence of Co
2+ as it was described by Wang et al. [
30]. The analysis of the results shows, as expected, a decrease in the Co signals as the Fe content increases. In addition, from
Figure 6, it can be observed how the relative intensity of the satellite peak around 785–790 eV increases with respect to the other Co signals. As already discussed, this positively influences the catalytic reaction considering that this decrease could interfere in the oxidation-reduction process and would cause greater durability of the structure. In addition, the presence of the species that are detected by this technique promotes active oxygen vacancies during the reaction, accelerating the combustion process [
31].
The highest Co
2+/Co
3+ ratio occurs with the lowest and highest percentages of Fe substitution, while the highest Fe
3+/Fe
2+ atomic ratios were obtained in structures with 50% and 100% substitution. However, analyzing
Table 7 as a whole, it is possible to conclude that an intermediate percentage of substitution yields a greater energy difference between the Co
2p(1/2) and Co
2p(3/2) peaks, evidencing the presence of both Co species. These species would present greater participation in the catalytic activity [
18,
30].
Figure 7 shows an intense peak around 710.5 eV, corresponding to Fe2p
3/2 that deconvolves into two possible peaks attributed to Fe
3+ and Fe
2+, which are the most stable states in which this metal can be found in the structure. At higher binding energies, an intense peak around 722.9 eV is also observed, which corresponds to Fe2p
1/2, which also deconvolves into two possible peaks that are masked by its width and which, like the first peak, can be attributed to the coexistence of Fe
3+ and Fe
2+. In the region between 715–721 eV, satellite peaks are observed that correspond to the coexistence of both Fe oxidation states, and also to the possible appearance of metallic Fe in the structure [
32]. The presence of metallic Fe is unlikely in these working conditions. However, it is not possible to rule out the existence of this species that could justify the deactivation of the catalysts by the inactivation of the cations of this metal. As described, the coexistence of different Fe cations is inferred from these results due to the reduction of this species in the perovskite structure, which can influence the catalytic reaction depending on the effect on the rest of the cations that play a fundamental role in the reaction under study.
As noted above, as Fe is incorporated into the structure, surface sites of Co2p are replaced by Fe, and the relative intensity of the satellite peak between 785–790 eV increases with respect to the other Co signals, indicating the presence of Co
2+. This is in correspondence with what was observed for Fe, where the analysis of the results shows an increase in the Fe signals as the Fe content increases. In addition,
Figure 7 shows that the relative intensity of the satellite peak (715–720 eV) increases with Fe content, indicating the coexistence of iron in its 2+ and 3+ states.
The XPS spectra of O
1s shown in
Figure 8 reflect two intense peaks between 528–533 eV, clearly demonstrating the existence of two oxygen species on the surface. The peak with the highest binding energy (530.9–531.2 eV) corresponds to surface oxygens (O
ads) such as
or O
− and (OH)
− hydroxyl anion, while the peak at low binding energies (528.1–528.8 eV) is attributed to O
2−, oxygens of the lattice (O
latt) [
33].
As the amount of Fe in the structure increases, it can be observed that the most intense peak of O1s spectra shifts to higher energies, whereas the less intense one undergoes practically imperceptible changes. Modifications were also observed in the O
ads/O
latt ratio (
Table 6), which decreased while the Fe content in the structure increased.
This decrease can also be explained by the cationic ordering on the surface that competes with the different oxygen species that occupy these sites. The Oads/Olatt ratio is a measure of surface oxygen vacancies that has a marked influence on the oxidation reactions. The highest ratio is not in line with the increase in Fe in the structure, but with an amount of 25% Fe, the Oads/Olatt ratio is the highest in the mixed perovskites, and therefore this could also explain the higher catalytic activity of this catalyst.
Mössbauer spectroscopy and XPS results confirmed that to the extent of the greater substitution of Fe, the cationic environment of Co increased to a point where the presence of Fe became more significant, that is, up to 25% of the insertion of Fe. With a greater percentage of substitution, the structure collapsed its magnetic ordering. The different environments of Fe
3+ varied with increasing substitution and produced changes that influenced the stability of the material in the combustion reaction. With a 25% substitution of Fe, the structure is magnetically and electronically balanced, causing greater resistance during the oxidation process. Based on the redox mechanisms discussed, it is important to analyze the capacity and possible mobility of oxygen in the structure. Thus, an O
2-TPD study was carried out, and the results are shown in
Figure 9.
As shown in
Figure 9, it is possible to differentiate two species of oxygen in the structure: α or surface oxygens that desorb between 200 °C and 400 °C, and β or lattice oxygens that desorb between 500 °C and 800 °C [
34]. The limited amount of surface oxygen is noticeable except in the LaFeO
3 sample. This can be explained assuming that the vacancies on the surface are occupied by the combination of the Fe
3+/Co
3+ cations, leaving the possibility of dynamic exchange between O
ads/O
latt, which is observed and corroborated by the atomic relationships determined by XPS (
Table 7). The lowest O
ads/O
latt ratio is obtained for the LaFeO
3 perovskite, whereas the highest ratios are obtained for the LaCoO
3 and LaCo
0.75Fe
0.25O
3 structures. It is well known that the catalytic combustion process of CVOCs mainly includes breaking the C–C bond (346 kJ mol
−1), C–H bond (411 kJ mol
−1), and C–Cl bond (327 kJ mol
−1). Thermodynamically, the bond energy of the C–Cl bond is lower, so it is easier to break. Chlorobenzene is generally adsorbed and dissociated on surface active sites via a nucleophilic attack on C–Cl bond. Then, the adsorbed species react with active oxygen species to produce CO
2 and H
2O. Simultaneously, the dissociative Cl
– species adsorbed are oxidized into Cl
2 by the surface reactive oxygen species through the Deacon reaction (2HCl + O
2 → Cl
2 + H
2O). Finally, the consumed oxygen species are replenished by the gas-phase oxygen adsorbed on the oxygen vacancies [
35,
36]. Thus, the lattice oxygens play a fundamental role, and that is why the best catalytic behavior corresponds to the highest O
ads/O
latt ratio that occurs in the LaFe
0.25Co
0.75O
3 structure. There is a correspondence between what is observed in
Figure 8 with this O
ads/O
latt ratio, which is why it is justified that the occupancy of the active sites and the amounts of Co ions, which are affected by the insertion of Fe, have important roles in the activity and stability of the catalyst.
2.3. Pos-Reaction Analysis
To determine the possible causes of catalyst deactivation, pos-reaction samples were characterized by XRD, XPS, and S
BET after being evaluated in the chlorobenzene oxidation reaction.
Figure 10 shows the diffractograms of the used catalysts.
No modifications of the structure were detected by XRD. The samples maintained the main peaks of the structures before the reaction, with the exception of the LaCoO
3 catalyst, where a destruction of the structure is observed as the main peak of the perovskite is modified. There are three additional peaks that correspond to the appearance of the LaOCl phase (PDF 96-900-9171), a modification that has been discussed in previous works [
12] and attributed to the absorption of Cl species on the catalyst surface, a situation that in the case of the Fe-containing catalysts did not happen.
Table 2 presents specific surface areas of fresh and used catalysts. It can be highlighted that there are no marked differences between values. In the case of LaCoO
3 and LaCo
0.75Fe
0.25O
3, a small surface area difference of about two units was observed. However, marked differences in pore size and volume can be seen, in all cases attributable to the surface reaction. As was previously mentioned, the LaCoO
3 catalyst is the one that formed the least amount of Cl
2 after the catalytic reaction (see
Table 1) in line with what is observed in
Figure 10. Part of the Cl
2 reaction product remained adsorbed on the catalyst surface, destroying the perovskite structure to form LaOCl.
XPS studies of pos-reaction samples evidenced the presence of Cl on the surface of all catalysts. In the case of perovskites with Fe, the variations in the stability time of the structures and their deactivation could also be associated with the adsorption of Cl on the surface. Although this was not perceptible by XRD due to the low concentration of this species, it was possible to identify the presence of this product as it is shown in
Figure 11.
Two signals can be observed in
Figure 11, one corresponding to Cl2
p1/2 around 195 eV and the other around 199 eV corresponding to Cl
2p3/2. Both signals suggest the presence of the Cl
− ion related to the structure in different ways. As described by Bello et al. [
37], one of the ways in which this ion can be found is bounded to oxygen bounded to one of the metals of the solid (Metal–O–Cl), which is in line with the results observed in the present work. Atomic ratios determined by XPS of the used samples (
Table 8) showed that the highest proportion of Cl appears in the LaCoO
3 catalyst, a structure that is destroyed by the formation of LaOCl, as was observed by the XRD diffractograms. Another way in which this ion can be associated with the structure is directly linked to a metal (Metal–Cl), a relationship that was not found as the formation of any metal chloride was not detected by the techniques used, maybe because the thermodynamic conditions are not favorable for the appearance of these structures or due to the low concentration of this species. From these results, it can be ensured that the deactivation of the catalysts happened due to the surface adsorption of Cl, which can occur both in oxygen vacancies or in some active sites on the surface, in both cases causing lower stability of the catalyst [
38].
Comparing
Figure 6 and
Figure 12, it can be concluded that the Co
2+/Co
3+ ratio decreases once the catalyst is used, with the exception of the LaCo
0.75Fe
0.25O
3 catalyst, which presented the same intensity peak. There were no notable changes for the LaCoO
3 and LaCo
0.75Fe
0.25O
3 catalysts in the case of the satellite peak between 785–790 eV. On the contrary, for LaCo
0.25Fe
0.75O
3 and LaCo
0.5Fe
0.5O
3, an increase in intensity is observed, evidencing a greater presence of Co
2+. The modification in the intensity of this peak suggests a change in the oxidation state that can be related to chlorine adsorption on the surface. These variations can be observed by comparing
Figure 6 with data in
Table 7 and
Table 8.
If
Figure 7 and
Figure 13 are compared, it can be observed that the Fe
3+/Fe
2+ ratio decreases for the used catalysts. It is possible that the behavior of the redox couple and the disposition of the cations were modified when the Cl occupied sites on the surface that were interchangeable in the case of the fresh catalyst. Once the Cl adsorbs to the surface, the states and dispositions of the cations suffer alterations in terms of oxidation state and spatial arrangement, which are clearly reflected in
Table 7.
In the region of 528–533 eV (
Figure 13), an intense peak that corresponds to the oxygens of the lattice is observed. Comparing
Figure 8 and
Figure 14, it is observed that the Oads/Olatt ratio decreases in all cases. This result is consistent with that obtained in the catalytic reaction, considering that combustion requires a constant exchange of different oxygen species. The bonding of chlorine on the surface affects the occupancy of oxygen on the surface, and it avoids the exchange between the oxygens of the lattice and the superficial ones, inhibiting the catalytic activity, which is why the greatest stability is seen in the catalyst with the highest Oads/Olatt ratio.
Based on the previous analyses, it could be concluded that in mixed perovskites, at least in LaCo0.75Fe0.25O3, charge compensation is produced by the generation of oxygen vacancies, attributable to the existence of Co2+ facilitated by the different Fe cations in the structure. The analysis of the magnetic environments, the possible oxidation states of Fe, and the pos-reaction results is in perfect agreement with the best behavior of this catalyst in the catalytic reaction, supporting up to 100 h of time on stream without modifying its original structure. This demonstrates the high stability that Fe in low concentrations provides to the LaCoO3 perovskite.