Yang Genga,
Haili Huanga,
Xiaoling Chena,
Hongyu Dinga,
Shijian Yanga,
Fudong Liu†
b and
Wenpo Shan*a
aJiangsu Key Laboratory of Chemical Pollution Control and Resources Reuse, School of Environmental and Biological Engineering, Nanjing University of Science and Technology, Nanjing 210094, China. E-mail: wenposhan@hotmail.com; Fax: +86 25 84315173; Tel: +86 18012920637
bMaterials Sciences Division, Lawrence Berkeley National Laboratory, Berkeley 94720, California, USA
First published on 4th July 2016
In this study, W0.1TiOx and CeaW0.1TiOx (a = 0.1, 0.2, 0.5, 1.0) catalysts were prepared by a novel stepwise precipitation approach. The CeaW0.1TiOx catalysts showed much better activities and N2 selectivity than W0.1TiOx. Particularly, the Ce0.2W0.1TiOx (CeO2/WO3–TiO2) catalyst showed excellent catalytic performance in a broad temperature range from 200 to 450 °C, under a high GHSV condition of 400000 h−1. Characterizations revealed that the novel preparation approach can achieve highly dispersed Ce species on the surface of the catalyst, and the Ce species could induce enhanced charge imbalance, superior redox functions, and outstanding adsorption and activation properties for NOx and NH3, which is the main reason for the highly efficient NOx abatement capability of the CeO2/WO3–TiO2 catalyst.
Increasingly stringent emission legislations for NOx in mobile applications will require the use of intensification of NOx reduction aftertreatment technology, which requires that the SCR catalyst should work efficiently under high space velocity conditions.4 For the purpose of obtaining higher deNOx efficiency, great efforts have recently been focused on the optimization of the SCR catalysts for broadening the active deNOx temperature window as widely as possible.2
Many types of vanadium-free catalysts, including oxides and zeolites, based on transition metals and/or rare earth metals have been studied for the NH3-SCR reaction.6,7 Several transition metals such as Fe,8 Mn,9 and Cu10 have been used in NH3-SCR catalysts, while the investigation of rare earth metals for NH3-SCR were mainly focused on Ce.11 Ce has been shown to be an outstanding component in the support of NH3-SCR catalyst.12 Ce is also a very effective promoter for NH3-SCR catalysts, such as V2O5–WO3/TiO2,13 Fe-ZSM-5,14 and Mn based low temperature SCR catalysts.15–17 In addition, Ce-based composite oxide catalysts, such as Ce–Ti,18 Ce–W,19 Ce–Mo,20 Ce–W–Ti,21 and Ce–Cu–Ti22 oxides, were shown to be very effective for NH3-SCR reaction. In our previous study, a high-efficient Ce–W–Ti oxide catalyst was prepared by a novel stepwise precipitation approach.23 This catalyst showed excellent catalytic performance, with superior low-temperature NOx conversion, high N2 selectivity and broad operation temperature window. Even under an extremely high space velocity condition of 1000000 h−1, the catalyst could still be highly effective for NOx conversion to N2. In this study, we furtherly characterized this catalyst using various techniques and investigated the effects of Ce species on the catalyst for NH3-SCR.
Before NH3-SCR performance test, the powder samples were pressed, crushed and sieved to 40–60 mesh. The SCR performance tests of the sieved powder catalysts (0.06 mL, about 0.07 g) were carried out in a fixed-bed quartz flow reactor at atmospheric pressure. The performance test in this study was carried out under simulated conditions, which is not directly adapted to the NH3-SCR process in realistic conditions. The reaction conditions were controlled as follows: 500 ppm NO, 500 ppm NH3, 5 vol% O2, N2 balance, and 400 mL min−1 total flow rate. The effluent gas, including NO, NH3, NO2 and N2O, was continuously analyzed by an online FTIR gas analyzer (Nicolet Antaris IGS analyzer) equipped with a gas cell of 200 mL volume and 2 m path length and a liquid nitrogen cooled MCT-A detector. The concentration data were collected after 0.5 h when the SCR reaction reached a steady state.
Powder X-ray diffraction (XRD) measurements of the samples were carried out on a computerized Bruker-AXS D8 diffractometer with Cu Kα (λ = 0.15406 nm) radiation. The data of 2θ were collected at 8° min−1 from 20 to 80°.
The XPS data were obtained on a Scanning X-ray Microprobe (ESCALAB 250, Thermo-VG Scientific) using Al Ka radiation (1486.7 eV). Binding energies of Ce 3d, W 4f, Ti 2p and O 1s were calibrated using C 1s peak (BE = 284.8 eV) as standard.
The surface morphology and elemental composition of the samples were studied using a scanning electron microscope (SEM, FEI Quanta 250F) combined with an energy dispersive X-ray (EDX) attachment. The accelerating voltage was 9.0 kV.
The H2-TPR tests were carried out on a Micromeritics AutoChem_II_2920 chemisorption analyzer. The samples (100 mg) in a quartz reactor were pretreated at 400 °C in a flow of air (50 mL min−1) for 1 h and cooled down to room temperature. Then H2-TPR was performed in 10 vol% H2/Ar gas flow of 50 mL min−1 at a heating rate of 10 °C min−1.
The NOx-TPD and NH3-TPD were performed using the same reaction system as catalytic performance tests. A typical experiment of NOx-TPD used 300 mg sample and a gas flow rate of 200 mL min−1. The experiment consisted of four stages: (1) degasification of the catalyst under N2 at 350 °C for 1 h, (2) adsorption of 500 ppm NO and 5 vol% O2 at 50 °C for 1 h, (3) isothermal desorption under N2 at 50 °C for 1 h, and (4) temperature-programmed desorption under N2 at 10 °C min−1 up to 500 °C. A typical experiment of NH3-TPD used 100 mg sample and a gas flow rate of 200 mL min−1. The experiment procedure of NH3-TPD was similar with that of NOx-TPD, but in stage (2) the adsorption was carried out under 500 ppm NH3 condition.
The N2O production over the samples during the catalytic performance test is shown in Fig. 1(B). We can see that, the addition of Ce remarkably inhibited the formation of N2O during NH3-SCR. At 350 °C, the N2O production over W0.1TiOx reached 37.4 ppm. When a small amount of Ce was added, the N2O production over Ce0.1W0.1TiOx dropped to be just 2.7 ppm. The peak value of N2O over W0.1TiOx at 350 °C was resulted from the competition between non-selective catalytic reduction reaction (NSCR reaction, 4NO + 4NH3 + 3O2 → 4N2O + 6H2O) and SCR reaction (4NO + 4NH3 + O2 → 4N2 + 6H2O).24,25
The NH3 conversions over the samples during the tests are shown in Fig. 1(C). Below 350 °C, the NH3 conversion over each CeaW0.1TiOx catalyst was very similar with the corresponding NOx conversion, indicating that the NO and NH3 were almost consumed with the same molar ratio. Above 350 °C, all of the NH3 conversions over CeaW0.1TiOx catalysts kept to be 100%, which is associated with the oxidation of NH3 in addition to SCR reaction. The NH3 conversion over W0.1TiOx at 350 °C was almost the same as the NO conversion, indicating that the two N atoms in N2O were mainly due to the coupling of one nitrogen atom from NH3 and another one from NO.26 A comparative investigation of the N2O formation mechanisms during NH3-SCR over Ce0.2W0.1TiOx and W0.1TiOx demonstrated that CeO2 is very effective for enhancing SCR reaction rate and thus depressing the NSCR reaction due to the competition between these two reactions.24
Fig. 2 NO2 production during separate NO oxidation reaction over W0.1TiOx and CeaW0.1TiOx catalysts. Reaction conditions: [NO] = 500 ppm, [O2] = 5 vol%, N2 balance and GHSV = 400000 h−1. |
Sample | BET surface area (m2 g−1) | NOx desorption (μmol g−1) | NH3 desorption (μmol g−1) |
---|---|---|---|
W0.1TiOx | 167.2 | 5.6 | 487.6 |
Ce0.1W0.1TiOx | 160.5 | 14.0 | 419.7 |
Ce0.2W0.1TiOx | 173.6 | 24.2 | 449.0 |
Ce0.5W0.1TiOx | 127.5 | 6.7 | 391.9 |
Ce1.0W0.1TiOx | 8.9 | 7.7 | 366.2 |
The XRD results of the samples are shown in Fig. 3. Only anatase TiO2 was detected in W0.1TiOx. With the addition of Ce, the crystallization of anatase TiO2 got weaker and weaker, but still no Ce or W species was observed in Ce0.1W0.1TiOx or Ce0.2W0.1TiOx. With further increase of Ce, clear cubic CeO2 was observed in Ce0.5W0.1TiOx and Ce1.0W0.1TiOx and Ce2WO6 was observed in Ce1.0W0.1TiOx. The coexistence of Ce with W and Ti species in Ce0.2W0.1TiOx could significantly inhibit the crystallization of Ti species, and the Ce and W species were probably existed as amorphous phase or crystallite phase with very small particle size, which will lead to highly dispersed active species.30 In such case, it is reasonable to see high efficient NOx conversion over Ce0.2W0.1TiOx together with no clear XRD diffraction peak of Ce or W species.
To investigate the atomic distributions of the metal elements, two techniques (SEM-EDX and XPS) of elemental composition analysis were carried out. The resolution of EDX is over 1 μm in depth, so its result were used to represent the overall status of the sample. For XPS, the detection depth is less than 10 nm, so its result can be used as the surface information of the sample. The analysis results by EDX and XPS are shown in Fig. 5. From the EDX results, we can see that the measured Ce/Ti molar ratios were similar with the added molar ratios. However, the surface Ce/Ti molar ratios for Ce0.2W0.1TiOx, Ce0.5W0.1TiOx and Ce1.0W0.1TiOx measured by XPS were much higher than the corresponding added molar ratios. The comparison of surface and overall Ce/Ti molar ratios clearly indicated the enrichment of Ce on the surface of the catalyst, which demonstrated the structure of the CeO2/WO3–TiO2 catalyst with dispersion of CeO2 on WO3–TiO2. An EDX mapping of the Ce for the Ce0.2W0.1TiOx catalyst in Fig. 6 showed that Ce was distributed evenly.
The NOx-TPD profiles are shown in Fig. 7(A). The first NOx peak of CeaW0.1TiOx at ca. 100 °C was due to the desorption of physisorbed NOx, while the second NOx peak at ca. 275 °C was mainly associated with the decomposition of chemsorbed NOx species.31,32 The two NOx peaks of W0.1TiOx were both observed at lower temperature than those of CeaW0.1TiOx, indicating that the adsorption of NOx on W0.1TiOx was much weaker than those on CeaW0.1TiOx. The adsorbed NOx on W0.1TiOx was obviously less than that on Ce0.1W0.1TiOx or Ce0.2W0.1TiOx, with similar BET surface area, indicating that NOx was mainly adsorbed on Ce sites. The adsorbed NOx on Ce0.5W0.1TiOx and Ce1.0W0.1TiOx were clearly less than that on Ce0.1W0.1TiOx or Ce0.2W0.1TiOx, indicating that the accumulation of Ce on the surface of catalysts with high Ce contents (as detected by XRD) was unfavourable for NOx adsorption. Therefore, highly dispersed Ce species on the Ce0.2W0.1TiOx catalyst is very important for the adsorption and activation of NOx.
It has been indicated that surface acidity plays an important role in the adsorption and activation of NH3, and the SCR reaction in the high-temperature region is likely controlled by the surface acid properties.33,34 Both of W and Ti can play as acid sites for NH3 adsorption during NH3-SCR reaction. Therefore, it is reasonable to see that the addition of Ce induced less NH3 adsorption on CeaW0.1TiOx than that on W0.1TiOx (Fig. 7(B) and Table 1). Furthermore, the addition of Ce led to a shift of NH3 desorption peak to the low temperature from W0.1TiOx to CeaW0.1TiOx. It indicates that the NH3 adsorbed species could be more easily desorbed at low temperature with the addition of Ce. Considering BET surface area for Ce1W0.1TiOx is just 8.9 m2 g−1, the amount of adsorbed NH3 (366.2 μmol g−1) is more than that for monolayer adsorption (considering ≈1019 sites per m2 for a monolayer), indicating the existence of physisorption. In addition, NH3 could be chemically adsorbed on both of the Lewis and Brønsted sites to form NH3ads and NH4+ species, which could both present in the NH3-SCR reaction.35–37 Ce0.2W0.1TiOx exhibited much better NH3 adsorption capacity than other CeaW0.1TiOx catalysts (Table 1). That was probably an important reason for the better NH3-SCR performance of Ce0.2W0.1TiOx.
The redox property of catalyst is very important for NH3-SCR. Topsøe et al. proposed a well-known catalytic cycle for the SCR reaction involving both acid-based and redox functions.41 Previous studies by Lietti et al. have demonstrated that the redox functions of NH3-SCR catalyst govern the catalytic reactivity in the low-temperature region.34,42 Therefore, the enhanced redox property of Ce0.2W0.1TiOx due to Ce species would beneficial for the low temperature NH3-SCR performance.
The XPS results of O 1s of W0.1TiOx and Ce0.2W0.1TiOx are shown in Fig. 9. The peak of O 1s was fitted into three sub-bands by searching for the optimum combination of Gaussian bands with correlation coefficients (r2) above 0.99. The sub-bands at 529.9–530.4 eV could be attributed to the lattice oxygen O2− (denoted as Oβ). Two shoulder sub-bands at 531.4–531.6 eV and 532.9–533.0 eV are assigned to the surface adsorbed oxygen (denoted as Oα), such as the O22− and O− belonging to defect-oxide or hydroxyl-like group, and chemisorbed water (denoted as O′α), respectively.45,46 The Oα ratio of Ce0.2W0.1TiOx (35.4%) calculated by Oα/(Oα + O′α + Oβ) was much higher than that of W0.1TiOx (12.3%), which means that the introduction of Ce indeed created more surface oxygen vacancies. Oα is usually more reactive than Oβ for oxidation reactions due to its higher mobility.16 Therefore, the enhanced Oα of Ce0.2W0.1TiOx would beneficial for the activation of NO and NH3 in the SCR reaction, and thereby promote the NOx conversion at low temperature.
Before the supply of oxygen was stopped, the NOx conversion over Ce0.2W0.1TiOx was kept at ca. 96% under the reaction conditions (GHSV = 400000 h−1 and temperature = 350 °C). After the supply of oxygen was stopped, the NOx conversion rapidly decreased by ca. 10% in 2 min, and then the decrease rate changed to be steady. After the stop of O2 for 270 min, the NOx conversion gradually decreased to be ca. 12%. Upon resupply of gaseous oxygen, the NOx conversions of Ce0.2W0.1TiOx was recovered to the initial level immediately. This result demonstrated that the lattice oxygen of the catalyst has substantially participated in the NH3-SCR reaction in the absence of gaseous oxygen.47 Under the same reaction condition, the initial NOx conversion over W0.1TiOx was kept at ca. 57%. As soon as the supply of oxygen was stopped, the NOx conversion decreased sharply to be ca. 26%. After the stop of O2 for 180 min, the NOx conversion kept stably to be ca. 8%. Upon resupply of gaseous oxygen, the NOx conversions of W0.1TiOx was also recovered immediately. The results of O2 shut off experiments showed that the W0.1TiOx only contained small amount of lattice oxygen that could be reduced, and lattice oxygen just slightly affect the reaction. However, the introduction of Ce remarkably increased the amount of lattice oxygen that could be reduced, and enhanced lattice oxygen could participate significantly in the SCR reaction.
The W0.1TiOx just exhibited good catalytic performance in the high temperature region above 400 °C. When Ce was added, all of the CeaW0.1TiOx catalysts showed remarkably improved catalytic performance and N2 selectivity. Particularly, the Ce0.2W0.1TiOx (CeO2/WO3–TiO2) catalyst showed excellent catalytic performance in a broad temperature range from 200 to 450 °C, under a high GHSV condition of 400000 h−1.
Characterizations indicated that the CeO2/WO3–TiO2 catalyst prepared by the stepwise precipitation approach can achieve highly dispersed active CeO2 on WO3–TiO2 and intense interaction among Ce, W and Ti species. The Ce species on the catalyst could induce enhanced charge imbalance, superior redox functions, and outstanding adsorption and activation properties of the reactants. That is the reason for the excellent NH3-SCR performance of CeO2/WO3–TiO2 catalyst.
Footnote |
† Current address: BASF Corporation, 25 Middlesex Essex Turnpike, Iselin, New Jersey 08830, United States. |
This journal is © The Royal Society of Chemistry 2016 |