Guangsheng Guo,
Kuo Lian,
Lijuan Wang,
Fubo Gu*,
Dongmei Han and
Zhihua Wang*
State Key Laboratory of Chemical Resource Engineering, Beijing University of Chemical Technology, Beijing, 100029, China. E-mail: gufb@mail.buct.edu.cn; zhwang@mail.buct.edu.cn; Tel: +86 10 64445927
First published on 23rd October 2014
Perovskite-type metal oxides have been regarded as promising materials for solar cells and catalysts. However, they suffer from a major challenge due to their low specific surface area. In this work, high specific surface area LaMO3 (M = Co, Mn) hollow spheres were synthesized by a hard template method. The influence of the reactant ratios on the properties of the products was investigated. The formation of La2O3, Co3O4 or MnO2 prevented the growth of LaMO3, which resulted in variations in the composition, morphology, specific surface area, surface chemistry and catalytic activity of the products. An acid washing process could remove La2O3 and Co3O4, which led to the enhancement of the specific surface area of LaCoO3. Due to the high reactant concentration and the slow heating rate, multishelled LaMnO3 hollow spheres with a high specific surface area of 42.6 m2 g−1 were formed, which showed the best catalytic activity in methane combustion.
Hollow materials with low density and high specific surface area have attracted much attention. Template-directed route has been considered as an effective strategy to synthesize hollow materials. Diverse hollow spheres, such as Co3O4, TiO2, WO3, In2O3 and Eu3+-doped Y2O3 with high specific surface areas have been synthesized by carbon sphere template method.12–16 However, perovskite-type hollow spheres have rarely been reported.
In this work, high specific surface area LaMO3 (M = Co, Mn) hollow spheres were synthesized by carbon sphere template method. The effects of reactant ratio on the composition, morphology, specific surface area and surface chemistry of the products were investigated. Acid washing process was used to further enhance the specific surface areas of the products.17,18 In addition, catalytic combustion of methane has several advantages compared to the conventional combustion, such as low temperature and high efficiency, which effectively abates thermal NOx formation.19 The performance of the synthesized LaMO3 (M = Co, Mn) hollow spheres in the catalytic combustion of methane was evaluated.
A typical preparation procedure for LaCoO3 hollow sphere was as follows: firstly, a certain amount of La(NO3)3·6H2O and Co(NO3)2·6H2O were dissolved in 40 mL deionized water. The ion concentration of lanthanum was 0.5 M. The molar ratio of lanthanum and cobalt was 1:
1, 1
:
1.5, 1
:
2, 1
:
3 and 1
:
5. Secondly, carbon spheres (0.2 g) were dispersed in the nitrate solution with ultrasonicating for 30 min, and then sealed in a 100 mL Teflon-lined autoclave at 180 °C for 6 h. The precursors were obtained by centrifugation, washing with distilled water and ethanol for three cycles, and then dried in an oven at 80 °C for 12 h. Finally, the LaCoO3 precursors were calcined at a ramp of 5 °C min−1 from RT to 400 °C and then kept at 400 °C for 2 h, and then at a ramp of 5 °C min−1 from 400 °C to 700 °C for 4 h in air. The obtained products were washed with 0.2 M acetic acid with vigorous stirring for 60 min. Then the products were washed with distilled water, centrifuged and dried. The samples obtained with the reactant ratios of 1
:
1, 1
:
1.5, 1
:
2, 1
:
3, 1
:
5 of lanthanum and cobalt were denoted as LC-1, LC-1.5, LC-2, LC-3, LC-5. The corresponding acid washing samples were denoted as WLC-1, WLC-1.5, WLC-2, WLC-3, WLC-5, respectively.
For the synthesis of LaMnO3, a certain amount of La(NO3)3·6H2O and Mn(NO3)2 (50 wt% aqueous solution) were dissolved in 40 mL deionized water. The ion concentration of lanthanum was 1 M. The reactant ratios of lanthanum and manganese were 1:
1, 1
:
2, 1
:
3, 1
:
4, 1
:
5 and 1
:
6. Carbon spheres (0.2 g) were dispersed in the nitrate solution with ultrasonicating for 30 min, and then sealed in a 100 mL Teflon-lined autoclave at 180 °C for 6 h. The precursors were obtained by centrifugation, washing with deionized water, and then dried in an oven at 80 °C for 12 h. The obtained LaMnO3 precursors were calcined in two steps: (i) firstly, calcinated in a N2 flow of 50 mL min−1 at a ramp of 1 °C min−1 from RT to 300 °C, and then kept at 300 °C for 3 h. Finally, cooled to 50 °C in same atmosphere; (ii) the obtained sample was calcinated in an air flow of 50 mL min−1 at a ramp of 1 °C min−1 from RT to 300 °C, and held at 300 °C for 2 h. Then, calcinated at the same ramp from 300 to 700 °C and maintained at 700 °C for 3 h. The samples obtained with the reactant ratios of 1
:
1, 1
:
2, 1
:
3, 1
:
4, 1
:
5, 1
:
6 of lanthanum and manganese were denoted as LM-1, LM-2, LM-3, LM-4, LM-5, LM-6, respectively.
The phase composition of the samples was characterized by X-ray diffraction (XRD) performed on D/max2500VB2+/PC X-ray diffractometer using graphite monochromatized Cu Kα radiation (λ = 0.15406 nm). The morphology of the products was observed by Hitachi H-800 transmission electron microscopy (TEM). Energy dispersive X-ray spectrometer (EDX) of the samples was recorded on S-4700 scanning electron microscope (SEM) with EDX Octane Super. The Brunauer–Emmett–Teller (BET) specific surface area was determined using an AutoChem Sorption Analyzer (NOVA-1200). Hydrogen temperature programmed reduction (H2-TPR) was performed using an Automated Catalyst Characterization System (AutoChem II 2920 V3.05, Micromeritics Instrument Corporation). The XPS analysis was performed using a Thermo ESCALAB 250 analyzer. The binding energies for each spectrum were calibrated using a C1s spectrum of 284.6 eV. Fourier transform infrared (FT-IR) spectrum was recorded on a Bruker Vector 22 FT-IR spectrophotometer using a KBr pellet.
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Fig. 1 TEM images of LaCoO3 hollow spheres: (a) LC-1, (b) LC-1.5, (c) LC-2, (d) LC-3, (e) LC-5 and LaMnO3 hollow spheres: (f) LM-3, (g) LM-4, (h) LM-5, (i) LM-6. |
The TEM images of the LaMnO3 prepared with the reactant ratios of lanthanum and manganese from 1:
3 to 1
:
6 is shown in Fig. 1f–i. The LM-5 shows uniform hollow spheres with a diameter of ca. 200 nm, and the thickness of the shells is ca. 20 nm. The size of the hollow spheres (180 nm) is reduced to about 60% of the original size of template spheres. This reduction is mainly due to the shrinkage of template because of further carbonization of organic matters and the densification of the products during the thermal treatment.21 Comparing with LaCoO3, LaMnO3 shows a multishelled hollow structure (Fig. 1i). The difference is from the programmable heating process. Dong et al. have found low heating rate can result in multishelled ZnO hollow spheres.22 In this work, the lower heating rate can result in two or three layers of LaMnO3 hollow spheres. Moreover, when the concentration of metal salts is higher, more metal ions can be adsorbed on the surface of carbon spheres, which is helpful to form multishelled structures.
Fig. 2a shows XRD patterns of LC-1, LC-1.5, LC-2, LC-3 and LC-5. LC-1 is composed of LaCoO3 and La2O3. The obtained LC-1.5 sample is assigned to perovskite-type LaCoO3 phase (JCPDS PDF# 48-0123), and no impurity peak is found. When the molar ratio of lanthanum and cobalt is higher than 1:
1.5, a mixed phase of LaCoO3 and Co3O4 is formed. These results indicate that the adsorption ability of the carbon spheres to lanthanum and cobalt ions may be different. The similar results appear in the synthesis of LaMnO3.
Fig. 2b shows the XRD patterns of the as-prepared LaMnO3. By contrasting the standard XRD pattern of LaMnO3 (JCPDS PDF# 82-1152), the diffraction peaks of LM-5 can be indexed to rhombohedral structure. When the molar ratio of lanthanum and manganese is lower than 1:
5, La2O3 will appear in the products. With the increasing of manganese, the peak intensities of La2O3 decrease obviously. In addition, the mean grain sizes of the samples were estimated using the Debye–Scherrer equation. The crystallite size of LM-5 is 16.8 nm, which is much smaller than other LaMnO3,23,24 suggesting that carbon sphere template method can greatly reduce the crystallite size. The EDX images of LM-1 to LM-6 are shown in Fig. S2,† which indicate the La/Mn atom ratios of LM-1 to LM-6 are 1
:
0.37, 1
:
0.69, 1
:
0.80, 1
:
0.90, 1
:
1.07 and 1
:
1.35, respectively.
The surface of carbon sphere is hydrophilic with OH− groups, which can absorb metal ions. LaMO3 hollow spheres are formed by absorption of La3+, Co3+ and Mn3+ on the carbon spheres due to the electrostatic interaction and coordination with surface hydroxyl groups, and subsequently removed the templates by calcinations. When the molar ratio of lanthanum and manganese is lower than 1:
3, the hollow structure can't be obtained, which possibly results from the different adsorption ability of carbon spheres to metal ions. From our experiment, the adsorption ability of La3+ on the surface of carbon spheres is stronger than that of Co3+ and much stronger than Mn3+. When the ratio of La3+ and Mn3+ is lower than 1
:
3, more La2O3 is formed which prevents the growth of LaMnO3. Therefore, the hollow structure can't be obtained. Moreover, the adsorption ability can be weakened by ion concentration. When Mn3+ concentration is relatively high, the adsorption amounts of La3+ and Mn3+ on the surface of carbon spheres will be close. When the molar ratio of Mn3+ and La3+ is close to 5, relatively pure LaMnO3 can be obtained.
The nitrogen adsorption–desorption isotherms of LaMnO3 hollow spheres indicate that all these samples show the characteristic of mesoporous structures in Fig. S3.† The isotherm of LM-5 can be categorized as type IV with a distinct hysteresis loop, which is the characteristic of mesoporous structure. The pore parameters and specific surface areas of LaMnO3 are summarized in Table 1. The specific surface areas are different between LM-5 and other LaMnO3, demonstrating that the hollow structure is varied by the ratio of lanthanum and manganese. LM-5 has a largest specific surface area of 42.6 m2 g−1 with a pores size distribution of 10–20 nm (Fig. S3b†), and the other samples exhibits lower specific surface areas from 22 to 34 m2 g−1. The excess lanthanum or manganese results in the formation of La2O3 or Mn2O3, which prevents the formation of LaMnO3 hollow spheres, and reduces the specific surface area of the products.
Catalyst code | Crystallite size (nm) | Specific surface area (m2 g−1) | Average pore size (nm) | Pore volume (cm3 g−1) |
---|---|---|---|---|
LC-1.5 | 18.2 | 12.3 | 55.2 | 0.036 |
LC-1 | 19.0 | 13.0 | 61.7 | 0.042 |
LC-2 | 17.8 | 15.5 | 69.2 | 0.068 |
LC-3 | 16.4 | 18.6 | 65.3 | 0.075 |
LC-5 | 16.2 | 21.2 | 72.1 | 0.085 |
LM-1 | 17.2 | 23.0 | 55.9 | 0.064 |
LM-2 | 16.7 | 22.4 | 67.7 | 0.074 |
LM-3 | 16.4 | 27.9 | 70.7 | 0.098 |
LM-4 | 16.4 | 34.4 | 75.7 | 0.130 |
LM-5 | 16.8 | 42.6 | 75.4 | 0.153 |
LM-6 | 17.1 | 33.5 | 86.8 | 0.146 |
WLC-1.5 | 17.7 | 17.2 | 70.3 | 0.088 |
WLC-1 | 15.8 | 20.4 | 68.6 | 0.102 |
WLC-2 | 15.9 | 24.9 | 71.9 | 0.090 |
WLC-3 | 14.2 | 28.9 | 72.5 | 0.124 |
WLC-5 | 11.6 | 37.9 | 79.8 | 0.157 |
Fig. S4,† 3a and b are the XPS spectra of the as-prepared LaCoO3 samples. As Fig. S4† shown, the LC-1 sample exhibits well-defined doublets for this La 3d core-level. According to the fitting procedure carried out, the main peak for the spin–orbit component,25 at 835.3 eV, can be detected. This contribution implies the presence of La2O3 (835.7 eV).26 The main peak of the LC-1.5 sample can be detected at 834.5 eV, displaces to higher value with respect to that observed in LaCoO3 (833.9 eV), indicative of the contribution of La2O3 specie on the surface of catalyst. LC-2, LC-3, LC-5 are observed with binding energies of 833.9 eV, 833.4 eV, 833.7 eV, respectively, indicates that the presence of La3+ in LaCoO3 (833.9 eV). Fig. 3a shows the Co 2p core-level spectra of the products. LC-1 and LC-1.5 exhibits a Co 2p3/2 peak at a binding energy of 779 eV, lower than the one typically reported.27 In addition, the absence of shake-up peaks in the spectra indicates the LaCoO3 phase. The Co 2p profiles of LC-2, LC-3 and LC-5 derived from LaCoO3 display satellite lines around 790 eV which is the fingerprint of Co3O4 species. Fig. 3b shows the O1s spectra of LaCoO3. From the spectra, two kinds of oxygen species are observed with binding energies of 528.7–529.2 eV and 531.3–531.5 eV. These energies can be attributed to the surface lattice oxygen (Olatt) and the surface adsorbed oxygen (Oads) species.28,29 The Oads/Olatt molar ratios are irregular for the untreated samples because of the impurities of La2O3 and Co3O4.
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Fig. 3 XPS spectra of the as-prepared LaCoO3 of Co2p (a), O1s (b) and LaMnO3 of Mn 2p3/2 (c), O1s (d). |
Fig. 3c and d shows the Mn 2p3/2 and O1s XPS spectra of the LaMnO3, respectively. There are Mn4+ and Mn3+ species as well as Olatt and Oads species on the surfaces of LaMnO3.30,31 The surface atomic ratios of Mn4+/Mn3+ and Oads/Olatt have an important impact on the catalytic performance of LaMnO3. The ratios of Oads/Olatt of LM-1, LM-2, LM-3, LM-4, LM-5 and LM-6 are 0.21, 0.37, 0.48, 1.13, 1.39 and 1.02, respectively. LM-5 shows the highest Oads/Olatt ratio. The ratios of Mn4+/Mn3+ of LM-1, LM-2, LM-3, LM-4, LM-5 and LM-6 are 0.39, 0.32, 0.54, 0.57, 0.53 and 0.51, respectively. It is found that the surface atomic ratios of lanthanum and manganese of LM-5 is lower than 1, suggesting the presence of Mn enrichment on the surfaces of the samples. Such phenomena are also reported by other literature.32 The differences in surface atomic ratio of Mn4+/Mn3+ of LaMnO3 samples is due to the different reactant ratio of lanthanum and manganese.33
Fig. 4a shows the H2-TPR profiles of the as-prepared LaCoO3. It can be observed that for LC-1 and LC-1.5, there are two major signals with shoulders in all products, which correspond to two consecutive reduction steps. These two steps have been previously discussed in the literatures.34,35 The low-temperature peak is associated to the first reduction step of Co3+ to Co2+. Whereas the second reduction step at high temperature is ascribed to the irreversible reduction of Co2+ in the oxygen deficient perovskite to Co0. For LC-2, LC-3 and LC-5, the reduction peaks are observed at lower temperatures, which are attributed to the reduction of the absorbed oxygen and Co3O4.
Fig. 4b shows the H2-TPR profiles of LaMnO3. LaMnO3 also exhibit stepwise reduction. LaMnO3 show a low temperature reduction peak at 300 °C with a shoulder at 400 °C. The reduction peak at 300 °C is due to the reduction of Mn4+ to Mn3+ and the removal of non-stoichiometric oxygen and adsorbed oxygen species.36 The shoulder at 300 °C is due to the single-electron reduction of unsaturated coordination Mn3+, whereas the reduction peak above 650 °C is due to the reduction of the remaining Mn3+.37 The two reduction temperatures (400 °C and 750 °C) of the LM-1 sample are higher and sharper than those of other LaMnO3 samples. When the ratio of lanthanum and manganese is 1:
1, there is less Mn4+ in sample which shows a less H2 consumption. With the increase of the ratio, the two reduction temperatures shift to lower temperature. LM-5 shows the excellent low-temperature reducibility (320 °C and 690 °C). In addition, the reduction peaks of LM-6 are observed at lower temperatures which are attributed to the reduction of absorbed oxygen and MnO2.
In order to remove the Co3O4 and La2O3 from LaCoO3, acetic acid was used to dissolve these impurities. Fig. S5† shows the XRD patterns of the acid washing LaCoO3, and all of the samples are perovskite-type LaCoO3 phase. No impure phases corresponding to lanthanum or cobalt oxides are detected. The EDX images of WLC-1, WLC-3 and WLC-5 are shown in Fig. S6,† which show the La/Co atom ratios of WLC-1, WLC-3 and WLC-5 are 1:
1.04, 1
:
1.06 and 1
:
1.02, close to 1
:
1. The average crystal sizes decrease with increasing the amount of the impure oxides, which further results in the increase of specific surface area in Table 1. The small crystal size and large specific surface area are obtained when the content of Co3O4 increased. Similar phenomena were also observed in the preparation of ZrO2 and SnO2 nanoparticles.38,39 The existence of Co3O4 can prevent the growth of LaCoO3 nanocrystals.
After washing, XPS has been used to investigate the surface element compositions and metal oxidation states. Fig. S7,† 5a and b are the XPS spectra of the acid-treated LaCoO3 samples. In Fig. S7†, the samples of WLC-5, WLC-3, WLC-2, WLC-1, WLC-1.5 exhibited binding energies all around 833.9 eV, which implies the presence of species of La3+ only in LaCoO3 (833.9 eV). These results reveal La2O3 can be removed after acid washing, which is in agreement with XRD results (Fig. S5†). Fig. 5a shows the Co 2p core levels for the acid-treated LaCoO3. The spectra have 2p3/2 and 2p1/2 spin–orbit doublet peaks located at 780 and 796 eV, respectively. The absence of the satellite line around 786 and 790 eV which are the finger print of CoO and Co3O4, indicates that Co atoms in these samples are mainly in LaCoO3 phase,40 in accordance with the results of XRD. Fig. 5b illustrates the O1s XPS spectra of the acid-treated LaCoO3. The Oads/Olatt ratios of WLC-1.5, WLC-1, WLC-2, WLC-3, WLC-5 of the samples after acid washing are 0.84, 1.23, 1.25, 1.95, 2.41, indicated that the high specific surface area could significantly enhance the adsorption capability of oxygen.
Fig. 6 shows the H2-TPR profiles of the acid-treated LaCoO3. The temperature of the low-temperature peak (Co3+ to Co2+) of WLC-1.5 is 460 °C. The corresponding TPR peaks shift to a lower temperatures of 428 °C for WLC-1, 414 °C for WLC-2, 410 °C for WLC-3 and 324 °C for WLC-5. The high-temperature peaks (Co2+ to Co0) also shift to a lower temperature. The positions of the reduction peaks are influenced by crystallite size,41 which suggests that the decrease in average crystallite size and increase in specific surface area can enhance the reducibility of Co3+ to Co2+ and Co2+ to Co0.
Catalyst | Temperature (°C) | Reaction rate (×10−3 mmol g−1 s−1) | TOF (molCH4 (molM s)−1) (M = Co or Mn) | |
---|---|---|---|---|
T50 | T90 | 400 °C | 400 °C | |
LC-1 | 599 | 667 | 0.222 | 2.58 × 10−2 |
LC-1.5 | 544 | 623 | 0.318 | 2.83 × 10−2 |
LC-2 | 530 | 605 | 0.448 | 3.19 × 10−2 |
LC-3 | 493 | 588 | 0.841 | 6.38 × 10−2 |
LC-5 | 485 | 578 | 1.04 | 7.96 × 10−2 |
LM-1 | 558 | 647 | 0.358 | 2.15 × 10−2 |
LM-2 | 545 | 628 | 0.414 | 2.84 × 10−2 |
LM-3 | 532 | 594 | 0.683 | 3.53 × 10−2 |
LM-4 | 513 | 580 | 0.750 | 5.17 × 10−2 |
LM-5 | 480 | 570 | 1.24 | 11.43 × 10−2 |
LM-6 | 507 | 582 | 0.907 | 7.68 × 10−2 |
WLC-1 | 525 | 605 | 0.640 | 4.82 × 10−2 |
WLC-1.5 | 570 | 648 | 0.299 | 1.08 × 10−2 |
WLC-2 | 513 | 599 | 0.744 | 5.48 × 10−2 |
WLC-3 | 495 | 589 | 1.15 | 9.48 × 10−2 |
WLC-5 | 479 | 576 | 1.61 | 12.31 × 10−2 |
For the catalytic activities of the acid-treated LaCoO3 (Fig. 8), the catalytic activities of WLC-1.5, WLC-1, WLC-2, WLC-3 and WLC-5 are gradually enhanced with the increase of specific surface area. The catalytic activity of WLC-5 (T50% = 479 °C) are much better than other LaCoO3 because the smallest crystallite size (11.6 nm), highest pore volume (0.157 cm3 g−1), average pore size (79.8 nm) and specific surface area (37.9 m2 g−1). The XPS and H2-TPR results indicate WLC-5 has the highest ratio of Oads/Olatt and the lowest reduction temperature. Sun's report also illustrated high specific surface area, adsorbed oxygen content and good reducibility helped to improve the catalytic activity.42
The different activities are likely related to the difference of the specific surface area. According to the activity data and the mole number of cobalt or manganese in samples, the turnover frequencies (TOFs) are calculated, and the results are shown in Table 2. It can be observed that WLC-5 (12.31 × 10−2 molCH4 (molCo s)−1) and LM-5 (11.43 × 10−2 molCH4 (molMn s)−1) show the highest TOF value in LaCoO3 or LaMnO3 under the temperature of 400 °C. Compared with the other catalysts in Table 3, WLC-5 and LM-5 shows the lower T50% and higher reaction rate.
Catalysts | Specific surface area (m2 g−1) | T50 | T90 | Reaction rate (×10−7 molCH4 g−1 s−1)a | Reference |
---|---|---|---|---|---|
a At 400 °C. | |||||
LaMnO3 | 15 | 511 | 599 | 1.39 | 43 |
LaMnO3 | 37 | 521 | 612 | 2.98 | 44 |
LaCoO3 | 5.5 | 560 | 640 | 0.94 | 45 |
La0.5Sr0.5MnO3 | 9.3 | 524 | 575 | 9.28 | 46 |
La0.96Ca0.04CoO3 | 4.3 | 541 | 623 | 0.67 | 47 |
La(Mn,Pd)O3 | 12 | 495 | 586 | 4.46 | 48 |
LaFe0.95Pd0.05O3 | 5.2 | 554 | 638 | 0.89 | 49 |
CexZr1−xO2 | 16.5 | 580 | 680 | 1.86 | 50 |
WLC-5 | 37.9 | 479 | 576 | 16.1 | This work |
LM-5 | 42.6 | 480 | 570 | 12.4 | This work |
Thermal durability of LC-5, WLC-5 and LM-5 were investigated, and the results are shown in Fig. 9. It is seen that the catalytic activity of WLC-5 and LM-5 are stable during 70 h test, with methane conversion keeping at around 99.2% in WLC-5 and 99.4% in LM-5 at the reaction temperature of 650 °C. Compared to WLC-5 and LM-5, LC-5 has the poor thermal durability. The methane conversion of LC-5 decrease after 30 h. This phenomenon may be the result of the small quantities of Co3O4 in LC-5, whose catalyst activity will decrease rapidly at high temperature or in the atmosphere with excessive water vapor. These experimental results indicate that the perovskite-type metal oxides are much more resistant to deactivation than the traditional noble-metal-based catalysts.
![]() | ||
Fig. 9 Methane conversion versus time at the reaction temperature of 650 °C of LC-5, WLC-5 and LM-5. |
Different SO2 poisoning behaviors over perovskites in methane oxidation were reported.51–54 Exposed to 20 ppm of SO2 for 15 h at 550 °C, a loss of 50% and 90% of the initial activity was observed for LaMnO3 and LaCoO3, respectively.51 In our experiments, the sample of WLC-5 was exposed to 100 ppm of SO2 at 600 °C for 3 h. Fig. S8a† shows the catalytic activity of WLC-5 before and after SO2 poisoning. The lost catalytic activity can be observed. T50 of the catalyst increases from 478 °C to 545 °C, and T90 increases from 582 °C to 640 °C, which reveal a loss of 20% of the initial activity. Fig. S8b† is the FTIR spectrum of the catalyst after SO2 poisoned. The peaks at 1064 cm−1, 1128 cm−1, 1190 cm−1 indicate the formation of sulfate, which indicate the destruction of the perovskite structure. This destruction is considered the main reason leading to the deactivation of the perovskite catalyst.
Footnote |
† Electronic supplementary information (ESI) available: Fig. S1–S8. See DOI: 10.1039/c4ra10053k |
This journal is © The Royal Society of Chemistry 2014 |