I. INTRODUCTION
Solving the energy and environmental issues via semiconductor photocatalytic technology has attracted wide attention in the past decades. Reference Chen, Zhang and Lee1,Reference Zou and Zhang2 Enormous effects have been devoted to develop visible-light-induced photocatalysts such as BiOX (X = Cl, Br, I), Reference Chang, Huang, Cheng, Sui, Sha, Ji, Deng and Yu3 Bi2MoO6, Reference Zhang, Xu, Zhao and Zhu4 BiVO4, Reference Ou, Nie, Zhong, Zhang and Zhong5 Bi2WO6, Reference Zhang and Zhu6 In2S3, Reference Chen, Liu and Gao7 ZnIn2S4, Reference Chai, Peng, Zeng, Zhang and Liu8 AgBr, Reference Xiao, Ge, Han, Li, Zhao, Xin, Fang, Wu and Qiu9 Ag3PO4, Reference Bi, Ouyang, Umezawa, Cao and Ye10 Ag2CO3, Reference Yang, Li, Wang, Wu, Chang and Tang11 AgVO3, Reference Zhao, Guo, Faiz, Yuan, Sun, Wang, Deng, Zhuang, Li, Wang, He and Yang12 and g-C3N4, Reference Cao, Low, Yu and Jaroniec13 considering full harvesting of solar light. Among these catalysts, Ag3PO4 has been seemed as a very promising candidate for photocatalytic applications because of its good photodegradation organic dyes capacity. However, bare Ag3PO4 is prone to photocorrosion and decomposing to low active Ag in the process of photoreaction, which could seriously deteriorate its photocatalytic activity. Reference Wang, Cheng, Yu, Liu and Fan14 To solve this problem and improve stability, coupling Ag3PO4 with other semiconductors to formation composites has been extensively developed, for instance, Ag3PO4/TiO2, Reference Zhang, Li and Zhang15 Ag3PO4/ZnO, Reference Liu, Wang, Xu, Chen and Fu16 Ag3PO4/SnO2, Reference Zhang, Zhang, Huang, Liu and Kang17 Ag3PO4/Bi2MoO6, Reference Lin, Hou, Jiang, Lin, Wang and Che18 Ag3PO4/Bi2WO6, Reference Fu, Xu, Chen, Lei and Zhang19 Ag3PO4/WO3, Reference Xu, Zhao, Xu, Chen, Huang, Li, Song, Zhang and Li20 Ag3PO4/g-C3N4, Reference Liu, Qi, Lu, Lin, An, Liang and Cui21 Ag3PO4/BiVO4, Reference Qi, Gu, Zhu, Wu, Wu, Long and He22 and so on. The well-matched energy bands’ structure of these composites is beneficial for the separation and migration of electron–hole pairs and then boosting the photoactivity and photostability.
The layered structure of BiOX (X = Cl, Br, I) gives high carrier mobility and little recombination of electron–hole pairs, which make it become an excellent photocatalyst. However, the photocatalytic performance of BiOX should be further improved from the practical applications. Until now, a large number of BiOX-based composites such as BiOCl/g-C3N4, Reference Lei, Jin, Zhang, Xu, Gao and Fu23 BiOI/TiO2, Reference Teng, Zhou, Jin, Luo, Xu, Guan, Wang and Yang24 BiOI/Bi2WO6, Reference Xiang, Ju, Wang, Sun, Zhang and Yu25 BiOBr/ZnFe2O4, Reference Kong, Jiang, Xiao, Lu, Jones and Edwards26 BiOBr/Bi2WO6, Reference Xia, Di, Yin, Xu, Zhang, Xu, Xu, Li and Ji27 BiOBr/BiVO4, Reference Li, Zhang, Bu and Chen28 BiOBr/BiMoO6, Reference Miao, Yin, Peng, Huo and Li29 and BiOBr/g-C3N4 Reference Sun, Zhang, Xiong, Zhao, Dong, Wang and Ho30 have been reported, which exhibit the improved photocatalytic activity than that of single BiOX. Recently some research groups have combined BiOX with Ag3PO4 to fabricate BiOX/Ag3PO4 composites. The resultant photocatalysts (BiOCl/Ag3PO4, Reference Cao, Dong, Cao and Wang31 BiOBr/Ag3PO4, Reference Mehraj, Mir, Pirzada and Sabir32 BiOI/Ag3PO4 Reference Wang, Cheng, Meng, Feng, Yang and Sun33,Reference Cui, Si, Zheng, Mi, Fa and Jia34 ) display the outstanding photoactivity and photostability. Based on the aforesaid reports, construction of BiOX/Ag3PO4 composites is a practicable and convenient approach to improve the photocatalytic performances of Ag3PO4 and BiOX.
In this work, BiOBr/Ag3PO4 composites were synthesized by a convenient in situ deposition of Ag3PO4 nanoparticles on BiOBr microsheets and applied into photocatalytic degradation of RhB solution under visible light illumination. Remarkably improved photocatalytic performance was realized in comparison with single BiOBr and Ag3PO4. In addition, the effect of composition ratio on photocatalytic activity was investigated.
II. EXPERIMENTAL SECTION
A. Materials preparation
BiOBr microsheets were synthesized according to the previous report. Reference Jiang, Yang, Yang, Kong, Jones, Xiao and Edwards35 Briefly, 0.970 g Bi(NO3)3·5H2O was added into 3 mL acetic acid (HAc) to form a transparent solution. The solution was mixed with 30 mL deionized water including 0.240 g KBr by magnetic stirring for 30 min. After that, the mixture was transferred into a 50 mL Teflon-lined stainless steel autoclave and heated at 160 °C for 6 h. After being cooled to room temperature, the products were obtained by centrifugation, washed with deionized water and ethanol for three times, and then dried at 80 °C for 12 h.
For the fabrication of BiOBr/Ag3PO4 composites, the appropriate amount of BiOBr was ultrasonically dispersed into 30 mL deionized water for 30 min. Then 0.170 g AgNO3 was added into the BiOBr suspension. The pH value of mixture was changed to 7.00 by dilute ammonium hydroxide. After stirring another 30 min, 20 mL deionized water containing 0.127 g Na3PO4·12H2O was introduced into the above mixture. Subsequently, the mixture was stirred for 4 h in the dark at ambient temperature. Then, the wet powders were collected, centrifuged, washed with ethanol and deionized water, and dried at 60 °C for 6 h. According to this procedure, different theoretical weight ratios of BiOBr/Ag3PO4 samples from 10 wt% to 70 wt% BiOBr in the composites were synthesized through tuning the BiOBr amounts. For comparison, the bare Ag3PO4 was also fabricated in terms of the same steps except the addition of BiOBr.
B. Material characterization
X-ray diffraction (XRD) was performed by a Bruker D8 Advance X-ray diffractometer (Bruker Corporation, Karlsruhe, Germany) with Cu Kα irradiation (λ = 0.154178 nm). The morphology of samples was conducted by Hitachi S-3000N scanning electron microscope (SEM; Hitachi Co. Ltd., Tokyo, Japan) and JEM 2100F high resolution transmission electron microscope (HRTEM; JEOL Ltd., Tokyo, Japan). The X-ray photoelectron spectroscopy (XPS) test was recorded on a VG Multilab 2000 (Thermo Fisher Scientific, Waltham, Massachusetts) with Al Kα source. The Fourier transform infrared (FTIR) spectra of samples were carried out using a Thermo Nicolet Avatar 360 spectrometer (Thermo Fisher Scientific). Raman spectra were examined by a Renishaw RM-1000 spectrometer (Renishaw plc, Gloucestershire, United Kingdom). The UV–vis diffuse reflectance absorption spectra (UV-DRS) were monitored on a Purkinje General TU-1901 spectrophotometer. The photoluminescence spectra (PL) were measured using a Varian Cary Eclipse fluorescence spectrophotometer (Varian, Palo Alto, California).
C. Photocatalytic degradation
The photocatalytic activities of BiOBr/Ag3PO4 composites were evaluated by the degradation of Rhodamine B (RhB) solution under visible light irradiation using a 500 W xenon lamp (Changzhou Yuyu Electro-Optical Device Co. Ltd, Changzhou, China) as a light source with a 420 nm cut-off filter. In each experiment, 50 mg of catalyst was added in 100 mL of RhB aqueous solution (1.0 × 10−5 mol/L). Before illumination, the suspensions were stirred in the dark for 30 min to establish the adsorption–desorption balance. At 5 min intervals, about 4 mL suspensions was collected and centrifuged at 10,000 rpm for 10 min to remove the catalyst. The concentration of RhB was determined by measuring the UV–vis spectra of the maximum absorption wavelength using a TU-1810 spectrophotometer.
D. Photoelectrochemical measurement
The electrochemical impedance spectroscopy (EIS) measurement was carried out using an electrochemical system (CHI 760D, CH Instruments Co. Ltd., Shanghai, China) in a three-electrode cell constituted of the working electrode, a platinum foil as the counter electrode, a Ag/AgCl electrode as the reference electrode, and 0.1 mol/L Na2SO4 solution as the electrolyte. For the preparation of working electrodes, 20 mg of as-prepared catalysts was ultrasonically dispersed in a mixture solution of 1 mL ethanol and 0.1 mL nafion aqueous solution (5 wt%) for 30 min. After that, 0.1 mL suspension was spread on an indium tin oxide (ITO) glass with a fixed area of 1 cm2 and dried in air at ambient temperature.
III. RESULTS AND DISCUSSION
Figure 1 shows the XRD of BiOBr, Ag3PO4 and 30 wt% BiOBr/Ag3PO4 composite. From the BiOBr diffraction pattern, all the detectable peaks could be assigned to the tetragonal phase BiOBr (JCPDS NO. 73–2061) with well resoluble (001), (002), (011), (012), (110), (003), (112), (004), (014), (114), and (212) reflections, in consistent with the previous report. Reference Jiang, Yang, Yang, Kong, Jones, Xiao and Edwards35 It is noteworthy that the intensities of (001), (002), (003), and (004) crystal planes obviously increase comparing with the standard card, implying that the BiOBr products preferentially grow along the (001) plane. The characteristic peaks of pristine Ag3PO4 could well correspond to the cubic phase of Ag3PO4 (JCPDS, No. 06–505). Reference Bi, Ouyang, Umezawa, Cao and Ye10 As for the 30 wt% BiOBr/Ag3PO4 composite, it presents the coexistence of BiOBr and Ag3PO4 crystal phases. No impurity phases of Ag, AgBr, or BiPO4 occur in the BiOBr/Ag3PO4 composite. In addition, the diffraction peak intensities of BiOBr distinctly fade away, which could be due to the Ag3PO4 nanoparticles tightly enwrapping the surface of BiOBr, then decreasing the diffraction peak intensities of BiOBr.
XRD patterns of BiOBr, Ag3PO4 and 30 wt% BiOBr/Ag3PO4 composite.
Figures 2(a)–2(d) reveals the SEM images of BiOBr, Ag3PO4 and 30 wt% BiOBr/Ag3PO4 composite. The single BiOBr shows the evident two-dimensional (2D) sheet-like structure with the diameter of 1–3 µm and thickness of 50–100 nm, in agreement with the previous report. Reference Jiang, Yang, Yang, Kong, Jones, Xiao and Edwards35 Pure Ag3PO4 exhibits irregular nanoparticle-like morphology with the diameter of 50–100 nm. As for the 30 wt% BiOBr/Ag3PO4 composite, it is composed of the microsheets and nanoparticles, which are respectively ascribed to BiOBr and Ag3PO4. Moreover, these granular Ag3PO4 are mainly attached on the surface of BiOBr microsheets. The microstructure of 30 wt% BiOBr/Ag3PO4 composite is investigated by HRTEM observations. Figure 2(e) identifies that the Ag3PO4 nanoparticles are intimately adhered on the surface of BiOBr, in accordance with the SEM measurement. In Fig. 2(f), the interplanar spacings of lattice fringes are determined to be 0.230 and 0.270 nm, assigning to the (112) plane of BiOBr and the (210) plane of Ag3PO4, respectively.
SEM images of BiOBr (a) and Ag3PO4 (b); low magnification (c) and high magnification (d) SEM images of 30 wt% BiOBr/Ag3PO4 composite; TEM (e) and HRTEM (f) images of 30 wt% BiOBr/Ag3PO4 composite.
To further detect the chemical composition and valence state of various ingredients, the 30 wt% BiOBr/Ag3PO4 composite was characterized by XPS. From the XPS survey spectrum [Fig. 3(a)], the composite is consisted of Bi, Ag, Br, P, and O elements. Two strong peaks at about 159.3 and 164.6 eV in Fig. 3(b) are respectively attributed to Bi 4f 7/2 and Bi 4f 5/2, indicating that Bi3+ exists in the composites. Reference Huo, Zhang, Miao and Jin36 In the high-resolution Ag 3d XPS spectrum [Fig. 3(c)], the peaks with binding energies of 367.8 and 373.7 eV were attributed to Ag 3d 5/2 and Ag 3d 3/2, implying that Ag+ is existence in the composite. Reference Liu, Wang, Xu, Chen and Fu16 The Br 3d XPS spectrum [Fig. 3(d)] could be fitted as two peaks, and the binding energies at 68.7 and 69.7 eV are assigned with Br 3d 5/2 and Br 3d 3/2. Reference Huo, Zhang, Miao and Jin36 The P 2p XPS peak is found at 132.5 eV [Fig. 3(e)], which could be related to P5+ in the Ag3PO4. Reference Xu, Zhao, Xu, Chen, Huang, Li, Song, Zhang and Li20 As for the O 1s XPS spectrum [Fig. 3(f)], it could be deconvoluted into three peaks at 530.1, 530.7, and 532.0 eV, corresponding to the Bi–O bonds of BiOBr, the PO4 3− bonds of Ag3PO4, and the O–H bonds, respectively. The XPS results illustrate that the composites are constructed with the BiOBr and Ag3PO4.
XPS spectra of 30 wt% BiOBr/Ag3PO4 composite: (a) XPS survey spectrum; (b) high resolution Bi 4f spectrum; (c) high resolution Ag 3d spectrum; (d) high resolution Br 3d spectrum; (e) high resolution P 2p spectrum; (f) high resolution O 1s spectrum.
Figure 4(a) depicts the FTIR spectra of BiOBr, Ag3PO4 and 30 wt% BiOBr/Ag3PO4 composite. The peaks at 3430 and 1660 cm−1 are respectively attributed to the vibration mode of –OH groups derived from the adsorbed H2O molecules. Reference Qi, Gu, Zhu, Wu, Wu, Long and He22 As for bare BiOBr, the featured peak existing at 520 cm−1 is related to Bi–O vibration. Reference Mehraj, Mir, Pirzada and Sabir32 In the case of Ag3PO4, the peak centered at 540 cm−1 is due to O = P–O bonds bending vibration. The absorption peaks around 850 and 1021 cm−1 are assigned to the symmetric and asymmetric vibration of P–O–P bonds. The peak at 1383 cm−1 originates from the P = O bonds vibration. Reference Qi, Gu, Zhu, Wu, Wu, Long and He22 The FTIR spectrum of 30 wt% BiOBr/Ag3PO4 composite substantially remains the characteristic absorption peaks of Ag3PO4. The vibration peaks ascribing to BiOBr are not distinct due to the relatively weak absorption or approaching to the O = P–O bond bending vibration of Ag3PO4.
FTIR (a) and Raman (b) spectra of BiOBr, Ag3PO4 and 30 wt% BiOBr/Ag3PO4 composite, the partial magnification Raman curves (inset).
Figure 4(b) shows a comparison of the Raman spectra of BiOBr, Ag3PO4 and 30 wt% BiOBr/Ag3PO4 composite. As far as BiOBr, the strong peaks at 115.3 and 165.5 cm−1 (inset) could be attributed to the A1g and Eg internal Bi–Br stretching modes, respectively. Reference Zhang, Li, Wang and Wu37 For Ag3PO4, the peak at 911.5 cm−1 is ascribed to the PO4 3− vibration. Reference Liu, Qi, Lu, Lin, An, Liang and Cui21 In terms of the 30 wt% BiOBr/Ag3PO4 composite, all the Raman bands belonging to BiOBr and Ag3PO4 can be observed. Furthermore, the characteristic peaks assigning to the Bi–Br stretching mode have the slight shifts from 115.3 to 114.5 cm−1 and from 165.5 to 164.7 cm−1, implying the interaction existence between BiOBr and Ag3PO4.
Figure 5 exhibits UV-DRS spectra of BiOBr, Ag3PO4 and 30 wt% BiOBr/Ag3PO4 composite. As shown, BiOBr presents an absorption edge at 435 nm, while Ag3PO4 is 506 nm. According to the equation of E g = 1240/λg, the band gap energies of BiOBr and Ag3PO4 are respectively calculated to be 2.85 and 2.45 eV, where E g is the band gap energy and λg is the absorption edge. The 30 wt% BiOBr/Ag3PO4 composite reveals a combination of the two UV-DRS spectra.
UV–vis diffuse reflectance absorption spectra of BiOBr, Ag3PO4 and 30 wt% BiOBr/Ag3PO4 composite.
The photocatalytic activities of as-prepared samples were evaluated by the photocatalytic degradation of RhB solution. The control experiments and physical mixed sample were carried out in the same photocatalytic reaction. As shown in Fig. 6(a), the RhB molecules are hardly degraded after 30 min visible light illumination without catalysts. Single Ag3PO4 exhibits poor adsorption capacity. During 30 min visible light irradiation, the decolorization percentage of RhB is 16.8%. Pristine BiOBr shows the highest adsorption activity, and the decrease of RhB concentration achieving 36.1% after visible light irradiation for 30 min. The adsorption abilities of BiOBr/Ag3PO4 composites enhance slightly along with increasing the amount of BiOBr in the composites. The decolorization percentages of RhB molecules are about 38.3%, 87.9%, 99.0%, 81.1%, and 68.8% for the 10 wt%, 20 wt%, 30 wt%, 50 wt%, and 70 wt% BiOBr/Ag3PO4 composites after 30 min visible light illumination, respectively. It is obvious that the photocatalytic activities improve with increasing the BiOBr contents in the composites and the 30 wt% BiOBr/Ag3PO4 composite manifests the best photocatalytic performance. Whereas further enhancing BiOBr amounts, the photocatalytic activities decline because the excessive BiOBr in the composites leads to the interfacial contact decrease between BiOBr and Ag3PO4. As for the physical mixed sample (30 wt% BiOBr and 70 wt% Ag3PO4), after 30 min visible light irradiation, the decolorization percentage of RhB is about 74.0%, which is lower than that of in situ prepared 30 wt% BiOBr/Ag3PO4 composite. The results indicate that it is important to construct intimate contact between BiOBr and Ag3PO4 for the improvement of photocatalytic activity. The temporal UV–visible absorption spectral variations of RhB solution over Ag3PO4, 30 wt% BiOBr/Ag3PO4 and BiOBr samples are illustrated in Figs. 6(b)–6(d), respectively. It is evident that the construction of BiOBr/Ag3PO4 composites could markedly boost the photocatalytic activity. It is also found that the maximal absorbance (λmax) has slightly blue shift in the BiOBr sample during visible light illumination, indicating that degradation of RhB molecules is a stepwise removal of the N-ethyl groups over BiOBr photocatalyst.
Comparison of photocatalytic activities of different samples for the degradation of RhB solution (a); the temporal UV–vis absorption spectra during the photocatalytic degradation of RhB mediated by Ag3PO4 (b), 30 wt% BiOBr/Ag3PO4 (c), and BiOBr (d), “origin” means the concentration of RhB before absorption equilibrium; recycling photocatalytic degradation of RhB solution (e) and XRD patterns (f) of 30 wt% BiOBr/Ag3PO4 composite before and after photocatalytic reaction.
To study the stability of photocatalysts, the 30 wt% BiOBr/Ag3PO4 composite was reused under the same conditions, as shown in Fig. 6(e). It is clear that the photocatalytic performance has mild reduction after the first run visible light irradiation. However, the photocatalytic efficiency still has 78.5% after four runs of degradation of RhB. The crystalline structures of the recycled 30 wt% BiOBr/Ag3PO4 composite were also investigated, as shown in Fig. 6(f). It can be seen that there are no extra characteristic diffraction peaks in the XRD patterns. The moderate decrease of the diffraction peak intensities indicates the declined crystallinity after photocatalytic reaction. It suggests that the slight photocorrosion has happened.
To clarify the reaction mechanism, 10 mmol/L triethanolamine (TEOA), 10 mmol/L p-benzoquinone (BQ), and 1 mmol/L isopropanol (IPA) were respectively added into the photocatalytic reaction system as the scavengers of holes (h+), superoxide radicals (·O2 −), and hydroxyl radicals (·OH) to investigate the effects of reactive species on photocatalytic degradation of RhB. As shown in Fig. 7(a), the TEOA and BQ lead to the dramatically inhibition of the degradation efficiency of RhB. However, IPA showed a weak constraint on degradation efficiency. The results reveal that h+ and ·O2 − make the crucial roles in the degradation of RhB.
The effect of reactive species on the photocatalytic degradation of RhB solution over the 30 wt% BiOBr/Ag3PO4 composite (a); electrochemical impedance spectra Nyquist plots (b) and PL emission spectra (c) of BiOBr, Ag3PO4 and 30 wt% BiOBr/Ag3PO4 composite.
As we all know that the efficient charge separation and transfer is significant for the improvement of photocatalytic activity. The EIS spectra have been used to study the interfacial charge separation efficiency. From Fig. 7(b), the diameter of Nyquist circle of 30 wt% BiOBr/Ag3PO4 composite is shorter than those of pure Ag3PO4 and BiOBr samples, which means an effective interfacial charge transfer and separation. This result suggests that coupling Ag3PO4 with BiOBr to formation composites is beneficial for the enhancement of photocatalytic activity.
To further illustrate the effective separation of photogenerated charge carriers in the BiOBr/Ag3PO4 composites, the PL spectra measurements were performed at room temperature. Generally, the lower PL intensity, the smaller probability of photogenerated charge carriers recombination. In Fig. 7(c), the PL intensity of 30 wt% BiOBr/Ag3PO4 composite is distinctly weakened, indicating that the recombination of photogenerated charge carriers is greatly restrained. The result also confirms that the BiOBr/Ag3PO4 composite could effectively separate photogenerated electron–hole pairs.
Based on the aforementioned experimental results, a possible mechanism is proposed to explicate the improvement of photocatalytic activity of BiOBr/Ag3PO4 composite. As for the semiconductor composites, the band edge potentials make a significant role in determining the flowchart of photogenerated electron–hole pairs. The potentials of the conduction band (CB) and valence band (VB) edge potentials of Ag3PO4 and BiOBr are calculated by Mulliken electronegativity theory E VB = X − E e + 0.5 E g, where E VB is the VB edge potential, X is the electronegativity of semiconductor, which can be expressed as the geometric mean of the absolute electronegativity of constituent atoms. Reference Xia, Di, Yin, Xu, Zhang, Xu, Xu, Li and Ji27 The X values of Ag3PO4 and BiOBr are calculated to be 5.97 and 6.20 eV, respectively. E e is the energy of free electrons on the hydrogen scale (approximately −4.5 eV). The E g values of Ag3PO4 and BiOBr are about 2.45 and 2.85 eV from the UV-DRS measurements, respectively. The E VB of Ag3PO4 and BiOBr are calculated to be 2.69 and 3.12 eV, respectively. The conduction band edge potential (E CB) can be acquired by the formula, E CB = E VB − E g. Accordingly, the E CB of Ag3PO4 and BiOBr are estimated to be 0.24 and 0.27 eV, respectively. As shown in Fig. 8, when the BiOBr/Ag3PO4 composite is illuminated under visible light, both Ag3PO4 and BiOBr can be excited to generate electron–hole pairs. The electrons in the CB of Ag3PO4 can transfer into the CB of BiOBr; meanwhile, the holes in the VB of BiOBr can conveniently migrate into the VB of Ag3PO4. As a result, the electron–hole pairs are efficiently separated between Ag3PO4 and BiOBr; the recombination of electron–hole pairs can be prevented, in agreement with the results of PL and EIS tests. Since the CB potential of BiOBr and Ag3PO4 is more positive than the single electron reduction potential of O2/O2 − (−0.046 eV vs. NHE), Reference Lin, Hou, Jiang, Lin, Wang and Che18 it could not reduce O2 to yield ·O2 − on the surfaces of BiOBr and Ag3PO4. However, the redox potentials of RhB and RhB* are 0.95 and −1.42 eV (vs. NHE), respectively. Reference Xiong, Zhang, Ma and Zhao38 Because of the good adsorption capacity of BiOBr, the excited RhB* molecules can inject the electrons into the CB of BiOBr, then reducing the surface chemisorbed O2 to give ·O2 − via one electron reaction. The VB potential of Ag3PO4 is not more positive than the redox potentials of ·OH/H2O (2.72 eV vs. NHE). It implies that the photogenerated h+ in the VB of Ag3PO4 could not react with H2O to form ·OH. Meanwhile, the production of ·OH on BiOBr is almost impossible because the standard redox potential of BiV/BiIII (1.59 eV vs. NHE) is more negative than that of ·OH/H2O. Reference Jiang, Yang, Yang, Kong, Jones, Xiao and Edwards35 In view of this, the photogenerated holes directly oxidize the RhB molecules in the reaction process.
The proposed mechanism of enhanced photocatalytic activity for the BiOBr/Ag3PO4 composite.
IV. CONCLUSIONS
The BiOBr/Ag3PO4 composites have been synthesized via a facile in situ deposition of Ag3PO4 nanoparticles on BiOBr microsheets and applied into the photocatalytic degradation of RhB solution. The improved photocatalytic activity is achieved over the BiOBr/Ag3PO4 composites in comparison with the single BiOBr and Ag3PO4, which could be attributed to the effective separation and migration of photogenerated electron–hole pairs. PL and EIS measurements demonstrate the efficient separation of photogenerated charge carriers in the BiOBr/Ag3PO4 composites. Additionally, the measurements of radical scavengers suggest that h+ and ·O2 − are the main active species for the degradation of RhB in the current system. The resultant BiOBr/Ag3PO4 composites may have a broad application prospect in the pollutant removal as the highly efficient photocatalysts.
ACKNOWLEDGMENTS
This work was supported by the National Natural Science Foundation of China (No. 51302200), Scientific and Technological Support Project of Hubei Province (No. 2015BAA100), Research and Innovation Initiatives of Wuhan Polytechnic University (Nos. 2016y18 and 2015d4).
