Photocatalysis has been intensively investigated as it has potential for exploitation in environmental remediation (pollutant degradation) and clean energy production (H2 production, CO2 reduction) [1, 2, 3]. The metal oxide semiconductors, such as TiO2, tungsten oxide (WO3), Bi2O3, and ZnO, have been shown to be efficient as photocatalysts in different processes [4, 5, 6]. Among these metal oxides, WO3 is of great interest because of its attractive properties such as small energy band gap (from 2.4 to 2.8 eV), stable physicochemical properties, non-toxicity, and resistance to photocorrosion [7].
However, a high charge recombination rate of photo-induced electron-hole pairs is a critical drawback in the development of WO3 as an efficient photocatalyst [8]. Several methods have been developed to improve the photocatalytic activity of WO3. Zhang et al. [9] synthesized monoclinic WO3 nanoplates by a one-step template-free hydrothermal route through a topochemical conversion process of H2WO4 nanoplates. The as-prepared m-WO3 nanoplate exhibited a superior photocatalytic activity for the degradation of rhodamine B (RhB) under visible light irradiation. Lin et al. [10] modified WO3 with an ionic liquid [Bmim]I through a facile impregnation method. The presence of a surface-bound imidazolium ring was demonstrated to effectively suppress the recombination of photoexcited electron-hole pairs.
Additionally, it has been shown that proper junctions formed in semiconductor-based photocatalysts could lead to enhanced activity. Oh et al. [11] prepared WO3/MWCNT-TiO2 composites using a modified sol-gel method. It is found that the WO3/MWCNT-TiO2 photocatalyst showed efficient charge separation during UV irradiation. Our previous work [12] indicated that the phase junction formed between the anatase and rutile TiO2 could greatly enhance photoexcited charge migration between the two phases that, in turn, enhanced the charge separation. Recently, Jaroniec et al. [13] proposed a new “surface heterojunction” concept to explain the difference in the photocatalytic activity of anatase TiO2 with co-exposed (001) and (101) facets. The phase junction enhanced charge separation and thus improved photocatalytic efficiency, and has been demonstrated for a variety of materials. α-Ga2O3/β-Ga2O3 [14], α-Bi2O3/β-Bi2O3 [15], and WO3/WO3·H2O [16] phase junction structures have been successfully synthesized and exhibit high photocatalytic activity for H2 production and RhB degradation. Therefore, the formation of the phase junction becomes an efficient way to produce semiconductor metal oxides exhibiting high photocatalytic activity.
WO3 exists mainly in four polymorphs, which are monoclinic, triclinic, orthorhombic, and tetragonal, along with a hexagonal phase [17]. Among these crystalline phases, the monoclinic phase has been reported as the most stable phase [18]. The monoclinic (m-WO3) and hexagonal (h-WO3) phases of WO3 have attracted the most attention because the m-WO3 is an attractive candidate for photocatalytic applications and h-WO3 exhibits an open-tunnel structure and rich intercalation chemistry [19]. We are interested in determining if we can fabricate the phase junction formed between m-WO3 and h-WO3 by a simple method, as well as understanding if the phase junction in WO3 enhances its photocatalytic activity. However, the relationship between the phase junction in WO3 and the photocatalytic activity is not well understood.
Generally, a material with different crystalline phases possesses a different band gap and flat band. Therefore, a phase junction could be built between different crystal phases given the two phases are in close contact, which will lead to efficient electron-hole separation and higher catalytic reactivity [20]. According to Ref. [21], the valence band position and conduction band position of h-WO3 are lower than those of m-WO3, which implies that a phase junction could be established between m-WO3 and h-WO3.
Therefore, this study attempts to fabricate a phase junction in a WO3 photocatalyst, and then to investigate the effect of the phase junction in the WO3 photocatalyst on its photocatalytic activity. The thermal decomposition method was used to fabricate a phase junction in WO3 by tuning the calcination temperature and the calcination time, and the phase junction (m-WO3/h-WO3) formed between hexagonal and monoclinic WO3 demonstrated an enhanced photocatalytic activity for RhB degradation.
Ammonium tungstate hydrate (H40N10O41W12·xH2O, APT) was of analytical grade and used without further purification. For the thermal decomposition method, the white APT powder was calcined at 600-1000 °C for 4 h in a static atmosphere of air, and then was naturally cooled to room temperature. The obtained samples were labeled as WO3-T, where T represents the calcination temperature (°C) used to obtain the samples. APT powders were also calcined at 800 °C for different times from 8 to 30 h and were denoted as WO3-t, where t represents calcination time (h).
Thermogravimetry and differential thermal analysis (TG-DTA) was performed using a TG/DTA-6300 thermal analyzer at the rate of 10 °C/min under air atmosphere (60 mL/min). The structure characterization was carried out by powder X-ray diffraction (XRD) using a Rigaku MiniFlex diffractometer with a Cu Ka radiation source. The morphologies of the samples were investigated using scanning electron microscopy (SEM, Quanta 200 F) and high-resolution transmission electron microscopy (HETRM, JEOL, JEM-2100). X-ray photoelectron spectra (XPS) were obtained using a Thermo ESCALAB 250Xi X-ray photoelectron spectrometer. The BET surface area was determined by N2 adsorption-desorption isotherms using a NOVA 4200e surface area and pore size analyzer from Quantachrome. A Hitachi F-4500 spectrophotofluorometer was used to record the photoluminescence spectra (PL) using an excitation wavelength of 350 nm.
A set of photocatalytic degradation experiments were performed with the following procedure. Photodegradation of RhB was carried out in a 100-mL Pyrex reactor filled with de-ionized water (60 mL) containing RhB (10 mg/L) and the WO3 sample. The suspension was stirred for 30 min in the dark to obtain adsorption-desorption equilibrium of the dye before illumination. After irradiation with a 125-W Hg lamp (λ = 365 nm, Shanghai Feilipu Yaming Lighting Co.), a 3-mL aliquot was taken every 30 min and immediately centrifuged. The RhB concentration in the clear solution was analyzed by optical characteristic absorption (22PC spectrophotometer, Shanghai Lengguang Technology Co., Ltd.) at a wavelength of 553 nm for a RhB solution. The blank experiments without a mercury lamp and without catalysts in the RhB solution under the same conditions are also compared. The blank study shows that mere photolysis can be ignored for RhB.
Fig. 1 shows TG-DTA curves of APT in a dynamic atmosphere of air. The TG curve shows five main mass-loss steps with a total of 11.8% loss of the original mass of APT. Four mass-loss steps totaling 10.6% (2.2% + 2.1% + 1.2% + 5.1% = 10.6%) and four main endothermic peaks at 84, 130, 208, and 275 °C could be observed in the DTA curve, which are attributed to the loss of absorbed water, crystal water, structural water, and loss of ammonia. In addition, two exothermic peaks are observed at 355 and 440 °C. The peak at 440 °C can be attributed to crystallization of the amorphous phase of WO3 [22]. In this study, calcination temperatures higher than 600 °C were chosen to prepare WO3, which facilitated a high degree of crystallinity.
Fig. 2 shows the XRD patterns of APT calcined at different temperatures. When the WO3 sample was calcined at 600 °C, diffraction peaks at 2θ = 23.1°, 23.6°, 24.3°, and 34.1° were observed, which represent the indices of the (002), (020), (200), and (202) planes of m-WO3 (PDF #43-1035), respectively. These results indicate that the WO3-600 °C sample is in the monoclinic phase. Moreover, the XRD peaks are strong and sharp, indicating that the WO3-600 °C sample exhibits high crystallinity. The XRD pattern of the WO3-700 °C sample is almost the same as that for the WO3-600 °C sample. On heating to 800 °C, three weak peaks appear at 2θ = 14.0°, 28.2°, and 36.6°, which arise from h-WO3 (PDF #33-1387), in addition to the typical peaks of the monoclinic phase. This implies the co-existence of hexagonal and monoclinic phases in the WO3-800 °C sample, while m-WO3 is the main constituent in the crystalline phase.
Martínez-de la Cruz et al. [23] prepared m-WO3 particles by the precipitation method using APT as the starting material and PEG as the template and steric stabilizer. It was also found that a long calcination time promoted the formation of the hexagonal structure of WO3 in addition to m-WO3. The XRD peaks of h-WO3 hardly changed for the WO3 sample calcined at temperatures up to 900 °C. However, the intensities of the typical peaks of h-WO3 were decreased for the WO3-1000 °C sample (Fig. 2(b)).
The morphologies and particle sizes of the WO3-T samples were investigated by SEM (Fig. 3). As shown in Fig. 3(a) and (b), the WO3-600 °C sample consists of dispersed large and fine particles with irregular polyhedral shapes. Bulky components with dimensions up to 10 mm were observed, and the sizes of the fine particles were approximately 200-500 nm for the WO3-600 °C sample. It is obvious that the rod-like components (circled by a dashed line in Fig. 3), assigned to the hexagonal phase, appear in the WO3-800 °C sample (Fig. 3(c) and (d)). This shows the co-existence of the monoclinic and hexagonal phases in the WO3-800 °C sample, which is in agreement with the results from XRD (Fig. 2). Moreover, it can be seen that m-WO3 and h-WO3 particles are in close contact, and m-WO3 particles are located on the surface of h-WO3 particles with a rod-like shape.
Crucial information on the spatial distribution of the h-WO3 and m-WO3 particles was further provided by HRTEM (Fig. 4). The HRTEM image of WO3-800 °C shows an example of the intimate contact between m-WO3 and h-WO3 phases. As shown in Fig. 4, the small particles and rod-like particles exhibit fringes with a lattice spacing of 3.779 and 6.361 Å, respectively, which can be indexed into the (020) atomic plane of m-WO3 and (100) atomic plane of h-WO3, respectively. HRTEM and SEM results (Fig. 3) reveal that the phase junction can be built between the m-WO3 particles and h-WO3 nanorods.
From Fig. 3, no apparent changes in the morphology of the m-WO3 particles were observed in the WO3-1000 °C sample, as compared with the WO3-800 °C sample. However, the samples obtained after calcination at 1000 °C showed a minor tendency to form large agglomerates, as shown in Fig. 3(e). Moreover, it should be noted that it is not easy to observe rod-like particles in the WO3-1000 °C sample, and the number of rod-like particles decreased for WO3-1000 °C as compared with the WO3-800 °C sample, from the SEM image. This result is in agreement with that from XRD (Fig. 2).
It is reported that triangular and hexagonal channels are formed along the structure in h-WO3 bronzes owing to the special arrangement of corner-sharing WO6 octahedra [24]. Alkaline (Na+, K+, Cs+ and so forth) or NH4+ ions are thought to be located in hexagonal channels [25]. Szilágyi et al. [24] studied the formation of h-WO3 during the annealing of hexagonal ammonium tungsten bronze (HATB), which is obtained by heating APT ((NH4)10[H2W12O42]·4H2O) in H2. They proposed that, in general, some ions or molecules were needed in the hexagonal channels to maintain a hexagonal tungsten oxide structure. Moreover, residual NH4+ and NH3 (from APT) in the hexagonal channels seemed to be vital for stabilizing h-WO3: when NH4+ and NH3 were completely released, the hexagonal framework collapsed in an exothermic reaction into m-WO3. Thus, combined with the results from previous studies, h-WO3, which forms at 800 °C, may transform into m-WO3 by increasing the calcination temperature to 1000 °C because of the release of NH4+ ions and NH3 molecules (from APT starting material) in the hexagonal channels at high temperature. Thus, the amount of rod-like h-WO3 decreased for WO3-1000 °C from Fig. 2. Further work is in progress to study the mechanism of the phase transformation between h-WO3 and m-WO3 in our lab.
To further change the phase composition in the WO3 sample, the APT powder was calcined at 800 °C for different times. Fig. 5 displays the XRD patterns of the WO3-t samples. It can be seen that the mixed phases of m-WO3 and h-WO3 were obtained for all the WO3-t samples. WO3-8 h sample is mainly composed of m-WO3 with a small amount of h-WO3. More intense peaks of h-WO3 appeared when the annealing time was increased from 8 to 12 h (Fig. 5(b)), suggesting an increase of h-WO3 content in the mixed phases. However, the diffraction peaks of h-WO3 gradually decreased in intensity after calcination for 12 h. With a further increase of the calcination time up to 24-30 h, WO3 samples were again mainly composed of m-WO3 with a small amount of h-WO3.
The XPS technique was used to determine the chemical states of WO3 samples. The overview XPS spectrum of the WO3-12 h sample in Fig. 6(a) shows the corresponding peaks of O 1s, C 1s, and W 4f, confirming the existence of W and O elements in the WO3-12 h sample. The fine spectrum in Fig. 6(b) displays two peaks at 35.4 and 37.5 eV, which suggests that the W exists in the W6+ form [26]. These two peaks are attributed to the spin-orbit splitting of the W 4f components (W 4f7/2 and W 4f5/2). For O 1s XPS (Fig. 6(c)), a peak at 530.6 eV was found, which can be assigned to lattice oxygen O2- of WO3 [27]. According to XPS studies, the W/O atomic ratio was estimated to be 1:3, which is consistent with tungsten(VI) trioxide. Therefore, the XPS results agree well with the results from the XRD pattern of the WO3-12 h sample.
The morphologies of the WO3-t samples were determined by the SEM analysis and are shown in Fig. 7. The m-WO3 particles exhibit a bulky shape with heavy aggregates, while h-WO3 particles exhibit a rod-like shape. Therefore, substances containing m-WO3 and h-WO3 can be identified simply by the particle morphology. The WO3-8 h sample (Fig. 7(a)) is composed of m-WO3 particles and some h-WO3 particles. As compared with the WO3-8 h sample, the number of rod-like particles obviously increases for the WO3-12 sample, which is in accordance with the XRD results (Fig. 5). It is shown that h-WO3 particles can be easily observed in the WO3-16 h sample although the number of h-WO3 particles decreases with an increase of the calcination time to 16 h. With a further increase in the calcination time to 30 h, the WO3 products are composed of a large number of m-WO3 particles coupled with a small number of h-WO3 particles, as shown in Fig. 7(g).
The results from XRD, SEM, and HRTEM demonstrate that well-defined m-WO3/h-WO3 phase junctions of WO3 can be fabricated by the phase transformation between m-WO3 and h-WO3. It is observed that the ratio of m-WO3 and h-WO3 in the WO3 products is mainly controlled by the calcination time. Moreover, from SEM and HRTEM images, it can be seen that m-WO3 crystals are sporadically patched on the surface of the h-WO3 rod-like particles, resulting in the exposure of both m-WO3 and h-WO3 on the surface.
RhB was used as a representative organic substance to investigate and compare the photocatalytic activity of the WO3 samples (Fig. 8). The degradation of RhB could be described by the first-order kinetics of ln(Ct/C0) versus reaction time (t): -ln(Ct/C0) = kapt, where kap is the apparent reaction rate constant, and C0 and Ct are the initial concentration and the concentration at reaction time t of RhB, respectively.
After 180 min of irradiation, 41% and 30% of RhB were degraded by the WO3-600 °C and WO3-700 °C catalysts, respectively. The lower degradation ability may be ascribed to the decrease of the surface area from 1.216 to 0.867 m2/g with increasing calcination temperature from 600 to 700 °C. From Table 1, WO3-600 °C, WO3-700 °C, WO3-800 °C, WO3-900 °C, and WO3-1000 °C samples exhibit a photocatalytic performance with kap determined as 0.00298, 0.00198, 0.00383, 0.00440, and 0.00232 min-1. It is observed that the photocatalytic activity increases with increasing calcination temperature to 800 °C. The WO3-900 °C sample exhibits the highest photocatalytic activity although the surface area of the WO3-900 °C sample (0.779 m2/g) is lower than those of WO3-600 °C and WO3-700 °C. Therefore, we concluded that the enhancement in the photocatalytic activity of the WO3-800 °C and WO3-900 °C samples arose from the phase junction between m-WO3 and h-WO3, the presence of which is confirmed by SEM and HRTEM results. The formation of the phase junction may improve the charge separation efficiency of photoexcited electrons and holes in the WO3-800 °C and WO3-900 °C samples. Thus, WO3-800 °C and WO3-900 °C samples show a higher photocatalytic activity than WO3-600 °C and WO3-700 °C containing the monoclinic phase.
By further increasing the calcination temperature to 1000 °C, the photocatalytic activity of WO3-1000 °C (surface area is 0.617 m2/g) decreased. However, the WO3-1000 °C sample shows a comparable photocatalytic activity to WO3-600 °C although the photocatalytic activity of WO3-1000 °C decreases compared with that of WO3-800 °C and WO3-900 °C. From the above discussion, the decrease of the photocatalytic activity for WO3-1000 °C arises from the decrease in the amount of h-WO3 when the calcination temperature is raised to 1000 °C, which decreases the amount of the exposed m-WO3/h-WO3 phase junction.
To further confirm the phase junction effect of WO3, the photocatalytic activities of WO3-t samples that were calcined at 800 °C for different times were investigated (Fig. 9) because the m-WO3 and h-WO3 phase composition can be carefully controlled by calcination at 800 °C for different times. When the APT powder was calcined at 800 °C for 8-30 h, all samples are in the mixed phases of m-WO3 and h-WO3 from XRD results (Fig. 5), and all the above samples show higher photocatalytic activities compared with WO3-600 °C containing m-WO3 (Fig. 9). Moreover, the photocatalytic activities were improved by gradually increasing the calcination time range from 8 to 12 h. The increase in the photocatalytic activity may mainly arise from the extent of the phase junction when the calcination time is increased from 8 to 12 h because the XRD results indicate that the amount of h-WO3 increases gradually with increasing calcination time. From Table 1, the WO3-12 h sample exhibits the highest photocatalytic activity with kap of 0.01025 min-1. With further increases of the calcination time to 24 and 30 h, the photocatalytic activity decreases.
A mechanism for electron-hole separation and transport of an m-WO3/h-WO3 phase junction is proposed and is shown in Fig. 10. The valence and conduction band potentials of h-WO3 were found to be 3.18 and 0.41 eV [21], whereas these values for m-WO3 were 3.37 and 0.80 eV, respectively [28]. The conduction band (CB) of h-WO3 is lower than that of m-WO3, thus the photo-induced electrons on the conduction band of h-WO3 transfer easily to m-WO3 through the well-developed interface, and the photogenerated holes move in the opposite direction from the electrons. Therefore, the phase junction of m-WO3/h-WO3 could act as an active center for hindering the rapid recombination of photo-induced electron-hole pairs. The electrons accumulated on the CB of m-WO3 can be scavenged by O2 to produce a superoxide radical (•O2-) and hydrogen peroxide (H2O2), which can interact to produce a powerful oxidant (hydroxyl radical, •OH) to decompose RhB. The holes accumulated in the VB of h-WO3 take part in the oxidation process to make OH− or H2O species to produce reactive hydroxyl radicals [29, 30, 31].
To further investigate the effect of the phase junction, PL analysis was applied to reveal the diffusion and recombination process of photogenerated electron-hole pairs. Fig. 11 shows the PL spectra of WO3-600 °C, WO3-800 °C, and WO3-12 h samples. A main peak at approximately 469 nm and several peaks in the range of 400-600 nm were observed in the PL spectrum of WO3-600 °C, which is in agreement with the results from Ref. [32]. In the case of WO3-800 °C and WO3-12 h with an m-WO3/ h-WO3 junction, the shape of the curves is similar to that of WO3-600 °C, whereas the peak intensities significantly decrease.
Generally, a higher PL intensity indicates a higher recombination rate of photoexcited electron-hole, and a lower PL intensity expresses a lower recombination rate of photoexcited electrons and holes [33, 34]. This indicates that the interaction between h-WO3 and m-WO3 in the WO3-800 °C and WO3-12 h samples is favorable for interfacial charge transfer, and thus reduces the recombination rate of electron-hole pairs under light irradiation. Moreover, it can be seen that the PL intensity of the peak at 469 nm of WO3-12 h is weaker than that of the WO3-800 °C sample. This result indicates that WO3-12 h exhibits a lower electron-hole recombination rate than that of WO3-800 °C. Thus, WO3-12 h exhibits higher photocatalytic activity than WO3-800 °C.
WO3 photocatalysts with different crystalline phases were prepared by thermal decomposition of APT at 600-1000 °C for 4 h and 800 °C for 8-30 h. Characterization of crystal structure, morphology, chemical composition, surface area, and optical properties of WO3, together with their relationships with the photocatalytic degradation of RhB, reveal that a phase junction between m-WO3 and h-WO3 of WO3 was fabricated by a thermal decomposition strategy to inhibit the recombination of carriers. The promotion of the photocatalytic performance is mainly ascribed to the enhanced charge separation originating from the phase junction between m-WO3 and h-WO3. This work provides a simple method to design and fabricate the effective WO3-based photocatalyst.