Nitrogen oxides (NOx), which arise from automobile exhaust gas and the combustion of fossil fuels, are a major source of air pollution. They are responsible for photochemical smog, acid rain, ozone depletion, and greenhouse effects [1, 2]. Selective catalytic reduction of NOx by NH3 (NH3-SCR) is currently regarded as the most promising technology for removing NOx from the exhaust of vehicles and stationary combustion processes. A typical commercial catalyst for NH3-SCR is V2O5-WO3(MoO3)/TiO2 [3, 4]. However, inevitable problems related to the toxicity of vanadium species, high conversion of SO2 to SO3, and the relatively narrow window temperature for this catalyst have led to increased interest in developing novel, highly active, stable, environmentally friendly, and vanadium- free NH3-SCR catalysts for controlling NOx emissions.
CeO2 is a key component in automotive three-way catalysts for the treatment of exhaust gases owing to its large oxygen storage capacity and excellent redox properties [5, 6]. However, it is well known that both redox and acidity is necessary in NH3-SCR catalysts [7, 8]. The redox properties of the catalyst appear to be a key factor in controlling the reactivity of de-NOx catalysts at low temperatures, while surface acidity plays an important role in the SCR reaction at high temperatures [9, 10, 11]. Because ceria is a basic solid [12], it is inevitable that its redox properties and acidity must be adjusted to obtain a wide operating temperature window for CeO2-based NH3-SCR catalysts for reducing NOx emissions. For example, Shan et al. [13] reported a novel Ce-W mixed oxide catalyst that exhibited nearly 100% NOx conversion in a wide temperature range from 250 to 425 °C, in which the W species increased the amount of Brönsted and Lewis acid sites on the catalyst surface. The modification was not only beneficial in improving the low-temperature activity of the catalyst by facilitating “fast SCR” reaction, but also enhanced its activity at high temperature by inhibiting the unselective oxidation of NH3 [14, 15]. Furthermore, modification of CeO2 with niobate has also been revealed to be an effective method of improving NH3-SCR activity, ascribed to the resulting significant increase in surface acidity [16]. Si et al. [17, 18] showed that sulfate and nickel modifications effectively enhanced the activity and selectivity of ceria-zirconia catalysts for NH3-SCR. The nickel modification improved the Lewis acidity of the CeO2-ZrO2 catalysts, while Brönsted acid sites formed by the sulfate modification facilitated ammonia adsorption instead of ammonia oxidation at high temperatures. Furthermore, Si et al. [19, 20] reported that a zirconium phosphate@Ce0.75Zr0.25O2 catalyst exhibited high NH3-SCR activity within a wide temperature range of 250-450 °C. Loading zirconium phosphate onto Ce0.75Zr0.25O2 was found to reduce the strong interaction between phosphate and cerium as well as introduce acid sites onto the surface of the Ce0.75Zr0.25O2. Very recently, Li et al. [21, 22] reported that a Ce-P-O catalyst prepared by a hydrothermal method showed excellent NH3-SCR activity and K2O and SO2/H2O resistance within a broad temperature range, and thus displayed promise for the de-NOx process of stationary sources at medium or high temperatures. However, the structure of these Ce-P-O catalysts was not confirmed, and thus the structure-activity relationship remained unclear.
In this work, a series of H3PO4-modified CeO2 samples were prepared by impregnation of ceria with phosphoric acid solution and evaluated for NH3-SCR. We found that H3PO4 had a significant promotional effect on the CeO2 catalyst toward the NH3-SCR reaction. The bulk and surface structures of this catalyst were characterized using different methods. Furthermore, the structure-activity relationship of the H3PO4- modified catalysts was thoroughly investigated.
CeO2 was prepared using the citric acid method previously described in the literature [17]. A certain amount of Ce(NO3)3·6H2O was dissolved in distilled water and then mixed with aqueous citric acid to produce a solution with a citric acid to total metal ions ratio of 1.1:1. The solution was stirred vigorously at room temperature for at least 1 h, and then the water was removed by evaporation. The resulting solid was decomposed to produce the oxide by annealing in air at 200 °C. The obtained oxide was then ground and further calcined at 500 °C for 3 h in a muffle oven.
H3PO4-modified CeO2 samples were prepared by wet incipient impregnation of the prepared ceria with H3PO4 solution. The obtained mixture was first dried at 110 °C overnight and then calcined at 500 °C for 3 h in static air. The resulting catalysts were denoted as xH3PO4-yCeO2, where “x/y” denotes the P/Ce molar ratio.
Powder X-ray diffraction (XRD) patterns were obtained using a D/Max-IIB diffractometer and Cu Kα radiation (λ = 1.5406 Å). The working voltage and current of the X-ray tube were 40 kV and 30 mA, respectively. The samples were scanned within the range 2θ = 10°-80° at a scanning rate of 5°/min.
Infrared spectra were recorded with a Fourier-transform infrared (FT-IR) spectrometer (Bruker Vertex 70 FTIR) using the KBr wafer technique for sample preparation.
Raman spectra were recorded on a Raman 960 FT-Raman spectrometer using a laser with an excitation wavelength of 1064 nm and a resolution of 8 cm-1. All Raman spectra presented in this paper are original and unsmoothed.
X-ray photoelectron spectroscopy (XPS) was conducted on a scanning X-ray microprobe (Thermo ESCALAB 250) using Al Ka radiation (1486.7 eV). The binding energies of Ce 3d, P 3p, and O 1s were calibrated using the C 1s peak (BE = 284.8 eV) as standard.
The specific surface areas of the samples were obtained from N2 adsorption-desorption analysis at -196 °C using a Micromeritics ASAP 2010. The catalyst samples were degassed at 250 °C overnight prior to the N2 physisorption.
Pyridine-IR spectra were recorded on a Nicolet 410 FT-IR spectrometer. The samples were heated at 200 °C for 30 min and then cooled to room temperature in vacuum of 10-4 mmHg. The pre-treated samples were exposed to pyridine as the probe molecule at room temperature, after which the pyridine was evacuated at 100 °C. All the IR measurements were performed at room temperature.
Temperature-programmed desorption of NH3 (NH3-TPD) was performed using a quadrupole mass spectrometer to record the signals of NH3 (m/z = 15 for NH). Prior to the TPD experiments, the samples (50 mg) were pretreated at 500 °C in a flow of pure Ar for 1 h and allowed to cool to room temperature. The samples were then exposed to a flow of 1000 ppm NH3/Ar at room temperature for 2 h, followed by Ar purge for another 1 h. Finally, the temperature was raised to 800 °C in flowing Ar at a rate of 10 °C /min.
For the H2 temperature-programmed reduction (H2-TPR) experiments, the samples (50 mg) were pretreated at 500 °C in a flow of air for 1 h and allowed to cool to room temperature. The temperature was then raised to 900 °C at a rate of 10 °C/min in a flow of 5 vol% H2/Ar. A thermal conductivity cell was used to detect the consumption of H2.
SCR activity measurements of the catalysts were performed in a fixed-bed quartz flow reactor. The reaction conditions were as follows: 500 ppm NO, 500 ppm NH3, 5% O2, Ar balance, GHSV = 20000 mL/(g·h). The gas concentrations in the outlet stream were continuously monitored with an online quadrupole mass spectrometer (QIC-20, Hiden, UK). The following ion peaks (m/z) were monitored to determine the concentration of products and reactants: 15 (NH3), 30 (NO), 44 (N2O), and 46 (NO2). NOx conversion was calculated as XNOx= (1 - [NOx]out/[NOx]in) × 100%, and N2 selectivity was calculated as SN2 = 1 - 2[N2O]out/([NOx]in - [NOx]out + [NH3]in - [NH3]out) × 100%, where [NOx] = [NO] + [NO2].
The catalytic performance of the pure and H3PO4-modified CeO2 catalysts for NH3-SCR of NO in the presence of oxygen are shown in Fig. 1. As expected, the pure CeO2 showed very poor NOx conversion throughout the whole temperature range and poor N2 selectivity at temperatures higher than 400 °C. The poor high-temperature SCR activity of CeO2 was attributed to the strong redox properties of ceria, which led to the over-oxidation of NH3 by gaseous oxygen [23, 24, 25]. However, the catalytic efficiency was significantly improved after H3PO4 modification, and the loading of H3PO4 played a pivotal role in broadening the operating temperature window. The window was greatly broadened as the P/Ce molar ratio was increased from 1:10 to 1:1, and more than 80% NO conversion was achieved in the temperature range of 250-550 °C over the H3PO4-CeO2 sample. However, upon higher H3PO4 loading, such as for the 1.5H3PO4-CeO2 sample, the low-temperature SCR activity was decreased slightly in comparison with that of H3PO4-CeO2.
The XRD patterns of H3PO4/CeO2 samples with various H3PO4 loadings are shown in Fig. 2. For all of the samples, the typical diffraction lines of the cubic CeO2 structure (JCPDS No. 34-0394) were clearly visible. At low P/Ce ratios, no phases except CeO2 were observed, suggesting that the phosphorus species may have been intercalated into the CeO2 lattice structure or existed as amorphous phosphate species. However, with increasing H3PO4 loading, CeP2O7 (JCPDS No. 16-0584) phase appeared in the H3PO4-CeO2 sample, while in the 1.5H3PO4-CeO2 sample, CeP2O7 became the main phase, and weak peaks of monazite CePO4 (JCPDS No. 32-0199), Ce(PO3)3, and Ce(PO3)4 could also be observed [26, 27, 28, 29]. The diffraction peaks of CeO2 in the H3PO4-modifed ceria samples were shifted towards lower 2θ values as the H3PO4 content increased. This may be ascribed to an increase in lattice parameters caused by part of the phosphorus species entering the fluorite structure of ceria [30, 31].
The BET surface areas of the samples are presented in Table 1. The surface area of the catalysts first decreased with increasing P content and then increased at higher P/Ce molar ratio. The lowest surface area appeared at the molar ratio of 1:2. These results indicated that there was no clearly defined relationship between catalytic performance and BET surface area in our study. However, in Li’s work [21, 22], the authors showed that Ce-P-O(h), prepared by a hydrothermal method, was a novel and efficient catalyst for NH3-SCR with NO conversions above 90% within the range of 200-550 °C, a better catalytic performance than our H3PO4-CeO2 catalyst. Although the two catalysts had the same composition (Ce, P, and O), our H3PO4-CeO2 catalyst had a much smaller BET surface area (17.6 m2/g) than that reported for the Ce-P-O(h) catalyst (82.4 m2/g). Thus, the larger specific surface area of Ce-P-O(h) catalyst is the likely reason for its excellent performance.
The Raman spectra of the H3PO4-modified CeO2 samples are displayed in Fig. 3. The band at 465 cm-1 in the spectra of all samples was attributed to the symmetric breathing mode of O atoms around each Ce4+ cation in the cubic CeO2 phase [32, 33]. As the P/Ce ratio was increased from 1/10 to 1.5/1, the intensity of this band at 465 cm-1 decreased monotonously, which meant that the amount of cubic CeO2 phase continuously decreased. Meanwhile, a new weak band appeared at 1034 cm-1, which could be assigned to the symmetric stretching of PO3 terminal groups from cerium pyrophosphate [34, 35]. Further increasing the P/Ce ratio resulted in an obvious increase in the proportion of the cerium pyrophosphate phase, and pyrophosphate became the main phase in the 1.5H3PO4- CeO2 sample, consistent with the XRD result.
Fig. 4 shows the FT-IR spectra of the pure and H3PO4-modified CeO2 catalysts. Several new bands at 470, 532, 748, 954, and 1223 cm-1 appeared in the H3PO4-CeO2 samples as the H3PO4 loading was increased. These bands could be attributed to O-P bonds, while the bands at 1223 and 748 cm-1 could be ascribed to P2O74- and P4O124-, respectively [36, 37, 38, 39, 40]. Additionally, as P/Ce ratio was increased from 1/50 to 1.5/1, the intensity of the bands at 1223 and 748 cm-1 increased monotonically, consistent with the Raman results.
To obtain a better understanding of their surface characteristics and concentration of active species, the CeO2-based catalysts were investigated using XPS. The electron-binding energies (BE) of the photoelectron peaks pertaining to Ce 3d, P 2p, and O 1s are shown in Table 1. The obtained values agreed well with those previously reported in the literature [14, 15, 41]. The representative photoelectron peaks of Ce 3d and O 1s for both the pure CeO2 and H3PO4-modified CeO2 samples are depicted in Figs. 5 and 6, respectively. As shown in Table 1, the binding energy of the Ce 3d and O 1s core-levels of the H3PO4-modified CeO2 samples was shifted to higher values with respect to pure CeO2, indicating the interaction between Ce and P species. As shown in Fig. 5, the Ce 3d spectra of the CeO2-based samples with different H3PO4 loadings were very complicated. By performing peak-fitting deconvolution, the Ce 3d spectra could be separated into eight bands. The sub-bands labeled u' and v' represent the 3d104f1 initial electronic state corresponding to Ce3+, while the sub-bands labeled u, u'', u''', v, v'', and v''' represent the 3d104f 0 state of Ce4+ [14, 42]. The Ce3+ ratios of the samples, calculated as Ce3+/(Ce3++Ce4+), are shown in Table 1. The Ce3+ ratio in H3PO4-modified CeO2 was significantly higher than that in CeO2. Meanwhile, it can be seen that the Ce3+ ratio increased remarkably with H3PO4 loading until it reached a maximum for the H3PO4-10CeO2 sample, after which further increases led to a slightly decreased Ce3+ ratio. As indicated by the XRD, IR, and Raman results, besides Ce(IV) pyrophosphate, other phosphates such as the monazite CePO4 phase appeared in the H3PO4-modified CeO2 samples as the H3PO4 loading was increased, which led to an increased Ce3+ ratio. However, the highly stable CePO4 has been claimed to be responsible for the locking of a considerable fraction of the Ce3+/Ce4+ redox couple, which may reduce the redox ability of these catalysts [20].
Fig. 6 shows the O 1s XPS spectra of the samples in the range of 524-542 eV. There were three kinds of oxygen species present in the samples. The peak centered at 531.5 eV was assigned to non-bridging oxygen (P-O), the peak centered at 533.0 eV was caused by bridging oxygen (P-O-P), and the peak centered at 529.5 eV is ascribed to lattice Ce-O [43, 44, 45]. As shown in Fig. 6, the relative intensities of both the P-O-P and P-O contributions increased and the lattice Ce-O peak intensity significantly decreased with increasing H3PO4 content. These results confirm that phosphorus species appeared on the surface of the catalysts after H3PO4 modification as expected.
NH3-TPD is a frequently used method for determining the number of acid sites on solid acid catalysts as well as acid strength distribution. Fig. 7 shows NH3-TPD profiles of the pure CeO2 and H3PO4-modified CeO2 catalysts. Pure CeO2 showed two broad NH3 desorption peaks, one at about 120 °C and the other at around 250 °C, which indicate weak acid strength. However, it is noteworthy that the acid site strength changed significantly after H3PO4 modification. With increasing H3PO4 loading, the weak acid site peak decreased gradually until it completely disappeared, while a peak at around 600 °C, assignable to strong acidity, dramatically increased in intensity. As discussed above, the surface area of the catalysts initially decreased with increasing P content and then increased at higher P/Ce molar ratio (Table 1). The lowest surface area was observed for the sample with a P/Ce molar ratio of 1:2. Moreover, the pore paths accessible by NH3 were partly blocked by the phosphate formed as a result of the P enrichment of the surface of the catalyst. As a result of these two factors, the amount of desorbed NH3 from 1.5H3PO4-CeO2 and H3PO4-2CeO2 was much lower than that from H3PO4- 10CeO2. However, the H3PO4 modification increased the acidic strength of the catalysts, which facilitated the adsorption of NH3 for the catalysts and simultaneously favored the SCR reaction.
The adsorbed pyridine IR technique was used to determine the acidic properties of the CeO2-based catalysts. As shown in Fig. 8, the IR spectra of pyridine adsorbed on CeO2 exhibited bands at 1456, 1485, 1595, 1545, and 1642 cm-1. The bands at 1456 and 1595 cm-1 are assignable to Lewis acid sites, while the band at 1490 cm-1 is mainly attributed to Lewis and Brönsted acid sites, and the bands at 1545 and 1642 cm-1 are caused by Brönsted acid sites [32, 46]. Thus, both Lewis and the Brönsted acid centers were found on the surfaces of the CeO2 catalysts. However, the pyridine-IR profiles exhibited an obvious change after H3PO4 modification. The bands attributed to Brönsted acidic sites showed an obvious increase in intensity with the amount of H3PO4 modification, while the amount of Lewis acidic sites decreased considerably after H3PO4 modification. The enhanced Brönsted acidity is probably connected with POH surface groups on the H3PO4-modified CeO2 catalysts. Although the nature of the NH3 adsorption sites was still under debate, Li et al. [47, 48, 49] showed that Brönsted acid sites efficiently catalyzed the decomposition of ammonium nitrite (an important intermediate in the SCR cycle), which promoted the NH3-SCR reaction. Furthermore, more Brönsted acidic sites might provide more moderate acid sites exhibiting less oxidation activity in comparison with Lewis acid sites, which would be beneficial for avoiding NH3 consumption at high temperatures [17, 25]. Thus, H3PO4 modification enhances the high temperature NH3-SCR activity of CeO2 owing to the higher ratio of Brönsted to Lewis acid centers.
The redox properties of the CeO2-based samples were investigated by H2-TPR. The H2-consumption profiles obtained from the TPR experiments are plotted in Fig. 9. As expected, the reduction profile of pure CeO2 exhibited two peaks [17, 50]. The first peak, centered at around 500 °C, was attributed to the reduction of the uppermost layers of Ce4+, while the second peak, at above 800 °C, originated from bulk reduction. However, the H2-TPR profile was significantly affected after H3PO4 modification. The position of the CeO2 reduction peak shifted to higher temperature with increasing H3PO4 content, which indicated that the oxidation ability of the catalysts was decreased. This difference in the redox behavior between the H3PO4-CeO2 catalyst and pure CeO2 may have arisen from interaction between Ce and P species.
Phosphorus species, produced by the decomposition of zinc dialkyldithiophosphate present in engine oil, can lead to the poisoning of automotive catalysts because the formed monazite (CePO4) accumulates on the surface and in the subsurface regions of the three-way catalysts. This deteriorates the oxygen storage and release properties of CeO2 [32, 33, 34]. However, in this work, we found that the addition of H3PO4 to CeO2 catalysts promoted the catalytic efficiency of NH3-SCR, and the operating temperature window was greatly broadened. Based on XRD, IR, Raman spectroscopy, and XPS analyses, it was concluded that in the samples with low P/Ce ratio (<1:2), the phosphorous species were highly dispersed on the surface of the CeO2, while part of the species diffused into the subsurface region and even became incorporated into the CeO2 lattice. The incorporation of P into the CeO2 lattice may occur through substitution of anions with PO43- or P2O74-, which would lead to the formation of Ce(III) and excess oxygen in the lattice [32, 33, 51], consistent with the XPS results shown in Table 1. However, as the P/Ce ratio increased, amorphous pyrophosphates, orthophosphates, and metaphosphate appeared in the samples. With further increases in the H3PO4 loading, crystallization of the amorphous CeP2O7 occurred on the H3PO4-CeO2 sample and a mixture of crystalline CeP2O7, CePO4, Ce(PO3)3, and Ce(PO3)4 was formed on the 1.5H3PO4-CeO2 catalyst, in which CeP2O7 as the main phase. Our previous work has demonstrated that rare earth pyrophosphates used as solid acid catalysts show excellent catalytic performance for the Beckmann rearrangement reaction and the vapor-phase dehydration of glycerol [52, 53]. Furthermore, we found that polyphosphate possessed much stronger surface acidity than CePO4 [53]. Therefore, the increase in acidity on the samples with higher H3PO4 loading may have been caused by the formed crystalline polyphosphate.
As is well known, both redox and acidic properties are necessary for the SCR reaction [7, 8]. Previous studies have showed that the redox properties of a catalyst governs its low-temperature activity, while its surface acidity determined its SCR activity at high temperatures [9, 10, 11].
Besides acid properties, redox properties have been claimed to be another important controlling factor for the De-NOx reaction, especially at high temperatures [1, 3]. A high reaction temperature was unfavorable for NH3 adsorption but promoted H-abstraction of the adsorbed NH3. Strong oxidation ability would result in higher catalytic activity for NH3 oxidation to N2 or even NOx, causing decreases in the NH3-SCR activity and N2 selectivity of the catalyst at high temperatures. The present H3PO4 modification decrease the oxidation ability of the CeO2-based catalysts and inhibited NH3 oxidation on the catalysts. Therefore, the high-temperature NH3-SCR activity and selectivity of the catalysts were improved after H3PO4 modification. In summary, the addition of H3PO4 to CeO2 in the present study increased its acidic strength and modified its redox ability, which led to a very broad operation temperature window.
The addition of H3PO4 to CeO2 enhanced its activity for NH3-SCR remarkably, especially at high temperatures. The modification resulted in an increased acidic strength and reduced redox ability, which were responsible for the very broad operation temperature window of the H3PO4-modified CeO2 catalysts.