Novel visible-light-driven Fe2O3/Ag3VO4 composite with enhanced photocatalytic activity toward organic pollutants degradation

Yuanguo Xua, Liquan Jinga, Xiao Chena, Haiyan Jib, Hui Xu*a, Hongping Lia, Huaming Li*a and Qi Zhangc
aSchool of Chemistry and Chemical Engineering, School of Pharmacy, Jiangsu University, Zhenjiang 212013, PR China. E-mail: lhm@ujs.edu.cn; xh@ujs.edu.cn
bSchool of Materials Science & Engineering, Jiangsu University, Zhenjiang 212013, P. R. China
cHainan Provincial Key Lab of Fine Chemistry, Hainan University, Haikou, Hainan 570228, P. R. China

Received 1st November 2015 , Accepted 14th December 2015

First published on 17th December 2015


Abstract

In this study, a new type of high-performance visible light photocatalyst Fe2O3/Ag3VO4 was prepared by a two-step method. Fe2O3 was prepared by a solvothermal method first and then the Fe2O3/Ag3VO4 photocatalyst was synthesized with different mass ratios by a simple chemical precipitation method. Powder X-ray diffraction (XRD), scanning electron microscopy (SEM), X-ray energy dispersive spectrometry (EDS), transmission electron microscopy (TEM), Fourier transform infrared spectroscopy (FT-IR), UV-vis absorption spectroscopy (in DRS mode), and electrochemical impedance spectroscopy (EIS) were applied to characterize the as-prepared samples. The results showed that the as-prepared photocatalyst was uniform in the shape of particles. Photocatalytic properties of the as-prepared samples were evaluated by degrading RhB under visible light. The results showed that 1% Fe2O3/Ag3VO4 composite presented the highest photocatalytic activity. After 60 min, 96.1% of RhB was degraded by 1% Fe2O3/Ag3VO4 composite. Finally, trapping experiments confirmed that the hole (h+) and superoxide free radical (˙O2) were the main active species in degrading RhB.


1. Introduction

Over the past few years, semiconductor nanocrystals have been considered applicable for solving the problems of water pollution and energy crisis.1–3 Anatase-type TiO2 has outstanding photocatalytic activity in degrading organic pollutants. However, the photocatalytic activity of TiO2 is limited by wide band gap energy and fast recombination of photogenerated carriers.4,5 Therefore, numerous visible-light-active photocatalysts have been developed to overcome these limitations. Recently, Ag-based semiconductor photocatalysts, such as Ag2CO3, Ag2WO4, Ag3PO4 and Ag3VO4, have been studied in the application of environmental treatment and water purification.6–9 Among them, the monoclinic scheelite Ag3VO4 has a narrower band gap (∼2.2 eV), which endows it with a greater spectral response for visible light. It has a special band structure: the Ag 5s orbitals hybrid with V 3d orbitals, constituting the conduction band of Ag3VO4. The valence band of Ag3VO4 is composed of O 2p6 orbitals hybridized with the entirely filled Ag 3d10 orbitals, which could form a valence band at a more positive energy level than that of O 2p6 and enhance the mobility of photoexcited holes for the oxidation of organic pollutants.10–12 However, the photocatalytic activity of pure Ag3VO4 is limited due to its high electron–hole recombination rate, and only a small portion of the photogenerated electrons are transferred to the surface of the catalyst to drive the photocatalytic activity. Therefore, the importance of effective electron transfer has been widely studied.

To improve these shortcomings, researchers have carried out modifications on pure Ag3VO4. As far as we know, composites of Ag3VO4 and other oxide catalysts have been reported with enhanced photocatalytic activity, such as Gd2O3/Ag3VO4, NiO/Ag3VO4, Co3O4/Ag3VO4. These composites could increase the separation efficiency of electron–hole and thus enhance the photocatalytic activity.11,13,14 In addition, some oxide catalysts, such as MgFe2O4, ZnFe2O4, NiTiO3 and CoTiO3, have been reported to improve the photocatalytic activity of Ag3VO4.15–18 The results showed that Ag3VO4 can be modified by oxide, improving the photocatalytic performance. The method is promising and can be continued.

Hematite (Fe2O3) is one of the most important visible-light-responsive semiconductor materials under ambient conditions. It has the advantages of low cost, abundance, high chemical stability and environmental friendly features.19,20 However, it also suffers from high electron resistance and high charge recombination rate.21,22 Thus, great efforts have been made to synthesize Fe2O3–Ag-based nanocomposites to increase the photocatalytic ability of Ag-based photocatalysts. Zhang et al.23 synthesized AgCl/iron oxide composites with enhanced photocatalytic activity towards rhodamine B (RhB) under visible light irradiation, which is due to the coupling action between the narrow band gap of hematite (Fe2O3) and the electron acceptor of AgCl. Fe2O3–AgBr nonwoven cloth was fabricated and its photocatalytic degradation abilities for rhodamine B (RhB) dyes and parachlorophenol (4-CP) were significantly enhanced, which resulted from the synergistic effects between Fe2O3 and AgBr.24 Some studies have also reported that Fe2O3 has been used as a shell in the hybrid. Yang et al.25 prepared a TiO2 core followed by a hydrothermal reaction for the α-Fe2O3 shell. The enhanced photoactivity was attributed to the matching energy levels of the two materials. Huang et al.26 synthesized core–shell structured Ag/AgBr@Fe2O3 with enhanced photoactivity for degrading methyl orange and bisphenol A, as well as for killing Escherichia coli. Zhang et al.27 prepared Co3O4 as the core and Fe2O3 as the shell. The hybrid showed enhanced gas sensing performance. All these studies demonstrated that Fe2O3 can be used as a good material to modify other photocatalysts and the hybrid showed enhanced performance.

Based on the abovementioned analysis, it is feasible to apply the Fe2O3/Ag3VO4 compound in the field of photocatalysis. In addition, the cost of Fe2O3 is very less, and it has the potential to be widely used to modify other materials. To the best of our knowledge, there is no report on the fabrication of coupled Fe2O3/Ag3VO4. In this paper, we report a low-temperature method to synthesize Fe2O3/Ag3VO4 composite by a chemical precipitation method. The as-prepared photocatalysts were studied for the degradation of potential toxic and carcinogenic RhB dye under visible light irradiation.28 The results demonstrated that the introduction of Fe2O3 can improve the photocatalytic activity of Ag3VO4. 1% Fe2O3/Ag3VO4 exhibits the highest photocatalytic performance, and the degradation efficiency could reach 96.1% in 60 minutes. According to the results of trapping experiments, the hole (h+) and superoxide free radical (˙O2) are the main active species in the process of photocatalytic degradation of RhB. Finally, a possible photocatalytic mechanism was proposed.

2. Experiment

2.1 Materials

All the starting materials in the experiment were purchased commercially and used without further purification.

The synthesis of Fe2O3 is similar to our previous report.26 Typically, 8.08 g Fe(NO3)3·9H2O was dissolved in 80 mL ethylene glycol (EG) with magnetic stirring. Then, 7.20 g CH3COONa and 2.00 g polyethylene glycol-600 (PEG-600) were added into the solution and the stirring was continued for 1.5 h to obtain a homogeneous suspension, which was then transferred into several 25 mL Teflon-lined autoclaves, followed by treatment at 200 °C for 22 h. After allowing them to cool naturally, the products were washed 10 times thoroughly with pure water and ethanol. They were then dried at 60 °C overnight. Second, the as-prepared Fe2O3 precursor was calcined in air atmosphere at a temperature of 500 °C for 2 h.

2.2 Synthesis of Fe2O3/Ag3VO4

A certain amount of Fe2O3 (Fe2O3[thin space (1/6-em)]:[thin space (1/6-em)]AgNO3 = 0.5%, 1%, 2%, 3%, 5%, 10% in mass ratio) was added to distilled water by ultrasonication for 30 min. Then, 0.24 g AgNO3 was added into the aforementioned solution with magnetic stirring at 0 °C for 30 min. 0.1884 g Na3VO4·12H2O was dissolved in 40 mL H2O at 0 °C. Subsequently, the prepared Na3VO4·12H2O aqueous solution was mixed into the abovementioned solution to obtain a suspension by mechanical stirring at 0 °C for 60 min. The obtained products were centrifuged and washed three times with deionized water and ethanol, and dried at 60 °C overnight. According to this method, the samples of Fe2O3/Ag3VO4 with different mass ratios were recorded as Fe2O3/Ag3VO4 (0.5%), Fe2O3/Ag3VO4 (1%), Fe2O3/Ag3VO4 (2%), Fe2O3/Ag3VO4 (3%), Fe2O3/Ag3VO4 (5%) and Fe2O3/Ag3VO4 (10%). Ag3VO4 was obtained in the absence of Fe2O3 by the same method.

2.3 Characterization

XRD patterns of the samples were obtained on an X-ray diffractometer (Bruker D8) with Cu Kα radiation (λ = 1.5418 Å) in the range of 2θ = 10–80°. Scanning electron microscopy (SEM) analysis was carried out on a tungsten filament SEM (Hitachi S-3400N) equipped with an energy-dispersive X-ray spectroscope (EDS) running at an acceleration voltage of 10 kV. Transmission electron microscopy (TEM) was carried out with a JEOL-JEM-2010 (JEOL, Japan) operated at 200 kV. Infrared (IR) spectra of all the catalysts (KBr pellets) were recorded on the Nicolet Model Nexus 470 IR equipment at room temperature. The surface compositions and chemical state of the composites were detected by X-ray photoelectron spectroscopy (XPS) analysis (Thermo ESCALab MKII X-ray photoelectron spectrometer using Mg Kα radiation). The UV-vis absorption spectra (in DRS mode) of the samples were obtained on a UV-vis spectrophotometer (UV-2450, Shimadzu Corporation, Japan) using BaSO4 as the reference. The electrochemical impedance spectroscopy (EIS) was carried out on an electrochemical work-station (CHI 660B Chenhua Instrument Company).

2.4 Photocatalytic activity measurement

The photocatalytic performance of the as-prepared catalysts was evaluated by the degradation of rhodamine B (RhB) under visible light irradiation using a 300 W xenon lamp with a 420 nm cutoff filter as the light source. 0.05 g of photocatalyst was placed into 100 mL (10 mg mL−1) aqueous solution of RhB in a Pyrex reaction vessel. Prior to irradiation, the suspensions were magnetically stirred for 30 min to ensure adsorption–desorption equilibrium between photocatalysts and RhB solution in the dark. During the photodegradation process, about 4 mL of suspensions were collected from each sample at given time intervals of visible-light irradiation, followed by centrifugation for 3 min. Then, the concentration was tested by a Shimadzu UV-2450 spectrophotometer at 553 nm, which is the maximal absorption band of RhB.

2.5 Photoelectrochemical measurements

EIS was investigated with an electrochemical analyzer (CHI660B, Chen Hua Instruments, Shanghai, China) in a standard three-electrode system, which used a platinum wire as the counter electrode, a saturated calomel electrode (SCE) as the reference electrode and an ITO as the working electrode. Typically, 5 mg of sample powder was dispersed ultrasonically in 1 mL ethylene glycol, and 20 μL of the resulting colloidal dispersion was drop-cast onto a piece of ITO slice with a fixed area of 0.5 cm2 and dried at 80 °C. A 500 W Xe arc lamp was utilized as the light source. Electrochemical impedance spectra (EIS) were obtained in a frequency range from 0.01 Hz to 100 kHz at 0.24 V, and the amplitude of the applied sine wave potential in each case was 5 mV. A 0.1 M Na2SO4 aqueous solution was used as the impedance liquid.

3. Result and discussion

3.1 XRD analysis

Fig. 1 shows the XRD patterns of Fe2O3, Ag3VO4 and a series of Fe2O3/Ag3VO4 composites. As can be seen in Fig. 1a, the diffraction peaks of Fe2O3 at 24.16°, 33.16°, 35.62°, 40.88°, 49.54°, 54.06°, 57.60°, 63.86°, and 63.98° can be indexed to (012), (104), (110), (113), (024), (116), (018), (214), and (300) planes, which correspond to α-Fe2O3 (JCPDS no. 33-0664).29 The characteristic diffraction peaks (Fig. 1b) for Ag3VO4 were detected at 19.46°, 31.00°, 31.08°, 35.18°, 36.02°, 39.10°, 41.26°, 48.60°, 51.54° and 54.14°, which were matching well with the (011), (−121), (121), (301), (202), (022), (400), (−322), (132), and (331) planes of Ag3VO4 (JCPDS no. 43-0542).17 As shown in Fig. 1c–f, for the XRD of the Fe2O3/Ag3VO4 composites, the diffraction peaks of Ag3VO4 appeared and did not shift, indicating that the combination of Fe2O3 and Ag3VO4 was not in the lattice, but only on the surface. In addition, the diffraction peaks of Fe2O3 in the complexes are not obvious with Fe2O3 content less than 10%. Therefore, the existence of Fe2O3 was confirmed by EDS, TEM, IR and XPS analyses.
image file: c5ra22912j-f1.tif
Fig. 1 XRD spectra of Fe2O3 (a), Ag3VO4 (b), 0.5% Fe2O3/Ag3VO4 (c), 1% Fe2O3/Ag3VO4 (d), 5% Fe2O3/Ag3VO4 (e), and 10% Fe2O3/Ag3VO4 (f).

3.2 SEM-EDS and TEM analysis

The morphology and composition of the samples were determined by SEM, TEM and EDS. In Fig. 2A and B, it can be observed that Fe2O3 and Ag3VO4 appear as nanoparticles with a size of less than 100 nm. The 1% Fe2O3/Ag3VO4 composite (Fig. 2C) displays a morphology similar to them. It is difficult to distinguish Fe2O3 from the Ag3VO4 particle from the SEM images. Thus, the EDS of the 1% Fe2O3/Ag3VO4 composites was carried out; the results (Fig. 2D) displayed that the Fe element was detected in addition to the original Ag, V and O elements in Ag3VO4. It revealed that Fe2O3 existed in the 1% Fe2O3/Ag3VO4 sample. Furthermore, TEM was used to distinguish the introduced Fe2O3. The TEM image in Fig. 2E shows that the Ag3VO4 exists as nanoparticles with diameters about 5–50 nm, and they tend to reaggregate together. The granular morphologies of Fe2O3 (Fig. 2F) are regular, angular and even a few hexagonal nanoparticles appear. As shown in Fig. 2G, it is a little difficult to distinguish the whole Fe2O3 particles from the Ag3VO4 particles.
image file: c5ra22912j-f2.tif
Fig. 2 SEM images of pure Fe2O3 (A), Ag3VO4 (B), 1% Fe2O3/Ag3VO4 (C) and EDS spectrum of 1% Fe2O3/Ag3VO4 (D) and TEM images of Ag3VO4 (E), pure Fe2O3 (F) and 1% Fe2O3/Ag3VO4 (G).

To investigate the distribution of Fe2O3, EDS elemental mapping of 1% Fe2O3/Ag3VO4 was carried out and the results are shown in Fig. 3. The image demonstrates the X-ray signal coming from Fe, Ag, O and V elements, which are represented by yellow, green, red and blue color, respectively. It is clear that the Fe element dispersed well. Considering that the Fe is present in the form of Fe2O3, it can be confirmed that the Fe2O3 is well-dispersed in the hybrid.


image file: c5ra22912j-f3.tif
Fig. 3 The SEM image of 1% Fe2O3/Ag3VO4 (A) and the corresponding EDS elemental mapping of Fe (B), Ag (C), O (D) and V (E) elements.

3.3 IR analysis

Fig. 4 shows the IR spectra of pure Fe2O3, Ag3VO4, and a series of Fe2O3/Ag3VO4 composites. For Fig. 4a, the absorption peaks at 531 and 465 cm−1 in the low frequency region are the Fe–O–Fe stretching vibration band, suggesting that the synthesized sample is α-Fe2O3.30–33 In the spectrum of pure Ag3VO4 (Fig. 4b), three main absorption peaks at 918, 844, and 696 cm−1 can be clearly observed. The absorption belt at 918 cm−1 is because the tetrahedral VO43− condensation formed symmetric and asymmetric stretching vibration of the coke vanadium ion VO3 group, and the absorption peak at 696 cm−1 is the asymmetric stretching vibration of V2O74−.34–36 It can be seen that the absorption peaks of Ag3VO4 appear in Fig. 4c–f, and there is no shift. When the content of Fe2O3 is less than 5%, the characteristic absorption peaks of Fe2O3 in Fig. 4c, 3d and e are not observed, which may be due to the low content of Fe2O3. When the mass fraction of Fe2O3 reached 10%, the absorption peaks of Fe2O3 appeared at 525 and 455 cm−1. In addition, the absorption peaks showed a little blue shift when compared to the pure Fe2O3. The results may be due to the interaction between Fe2O3 and Ag3VO4.
image file: c5ra22912j-f4.tif
Fig. 4 IR spectra of Fe2O3 (a), Ag3VO4 (b), 0.5% Fe2O3/Ag3VO4 (c), 1% Fe2O3/Ag3VO4 (d), 5% Fe2O3/Ag3VO4 (e), 10% Fe2O3/Ag3VO4 (f).

3.4 XPS analysis

XPS analysis was used to investigate the element compositions and the valencies of the surface elements of Ag3VO4 and Fe2O3/Ag3VO4. Fig. 5A shows the survey spectrum of Fe2O3/Ag3VO4 composite (10%). It is obvious that the sample consists of Ag, V, Fe, O and C. The C element is ascribed to the XPS instrument itself. Fig. 5B–E show the high resolution XPS spectra of Ag 3d, V 2p, O 1s, Fe 2p and Ag 3s of the samples. Fig. 5B displays the high-resolution spectra for Ag 3d; the center of the two peaks at 368.16 and 374.24 eV can be attributed to the Ag 3d5/2 and Ag 3d3/2 in Ag3VO4.10,37 When Fe2O3 was introduced, the center of the Ag 3d5/2 peak did not shift obviously, while the peak at 374.24 eV shifted to 374.15 eV. As shown in Fig. 5C, two typical peaks for V 2p were 516.91 and 524.55 eV, which correspond to V 2p3/2 and V 2p1/2. This indicated that in both samples V exists as V5+. The peak at 516.91 eV shifts to 516.80 eV.10,13,37,38 Furthermore, O 1s spectra exhibit the peak at 530.18 eV, which shifted to 530.08 eV, as shown in Fig. 5D.37 According to the XPS results of Ag 3d, V 2p and O 1s, it can be inferred that there is a weak interaction between Fe2O3 and Ag3VO4 in Fe2O3/Ag3VO4 composite synthesized by chemical adsorption. Fig. 5E shows the high resolution spectrum of Fe 2p and Ag 3s. The four peaks around 711.3 eV, 719.0 eV, 724.2 eV and 734.6 eV are ascribed to the Fe 2p3/2, Fe 2p3/2 satellite, Fe 2p1/2 and Fe 2p1/2 satellite, respectively.39 The shakeup satellite peak at around 719.0 eV is a characteristic of the Fe3+ species.40 The typical peak at 717.3 eV can be assigned to the binding energies of Ag 3s.13,41
image file: c5ra22912j-f5.tif
Fig. 5 The survey spectra of Fe2O3/Ag3VO4 (A) and the high resolution XPS spectra of Ag 3d (B), V 2p (C), O 1s (D), Fe 2p and Ag 1s (E).

3.5 UV-vis analysis

The UV-vis absorption spectra (in DRS mode) of Fe2O3, Ag3VO4 and Fe2O3/Ag3VO4 composites with different Fe2O3 contents are shown in Fig. 6A. It can be seen that Fe2O3 has good absorption ability in the region of 200–800 nm, especially in the region of 200–600 nm. Similar results have been reported in other studies.42,43 All the composites show strong absorbance in the region of 400–600 nm and the absorbing boundary of the composite and Ag3VO4 is about 470 nm in Fig. 6A. The absorption intensity of the composite is higher than that of the pure Ag3VO4 and increases with increasing Fe2O3 content in the composite in the region of 400–550 nm (the energy used from the visible light in this region is very important). This means that the composite can absorb more light energy than the pure Ag3VO4, which is beneficial to enhance the photoactivity of the composite. To obtain the estimated value of the band gap energies, the absorption onsets of the samples are acquired by linear extrapolation from the plots of (Ahν)2 versus the photon energy () in Fig. 6B. It can be seen that the tangent extrapolation estimate values are 2.01 and 2.30, which correspond to the band gap energies of Fe2O3 and Ag3VO4, respectively. This showed that Ag3VO4 was a direct transition and its band gap energy was around 2.30 eV, which is close to a reported study.18
image file: c5ra22912j-f6.tif
Fig. 6 (A) UV-vis diffuse reflectance spectra of Ag3VO4 and Fe2O3/Ag3VO4 composites with various Fe2O3 contents, (B) (Ahν)2 versus hν curves of Ag3VO4 and 1% Fe2O3/Ag3VO4.

3.6 Photocatalytic decomposition of RhB

The performance of adsorption-photocatalysis of the sample is tested by measuring the degradation rate of RhB in a wastewater model. The adsorption–desorption balance was achieved between the catalyst and RhB for 30 min adsorption process in darkness. Fig. 7 exhibits the photocatalytic performance of Fe2O3/Ag3VO4 composites with different Fe2O3 contents as well as pure Ag3VO4 under visible light irradiation. It can be seen that the RhB is only slightly degraded without any photocatalyst under light irradiation for 120 min, which demonstrates that self-decomposition of RhB can be negligible. Moreover, by increasing the mass fraction of Fe2O3, the photocatalytic activity of the composites increases. 0.5% Fe2O3/Ag3VO4 can degrade 89.1% at 60 min, which is much higher than that degraded by pure Ag3VO4 (which can degrade 65.2% at 60 min). When the Fe2O3 content was increased to 1%, the 1% Fe2O3/Ag3VO4 composite shows the highest activity, which can degrade about 96.1% RhB in 60 min. However, the photoactivity of the composite decreased gradually with further increasing the Fe2O3 content. 2% Fe2O3/Ag3VO4 can degrade 93.6% of RhB, 3% Fe2O3/Ag3VO4 can degrade 84.6% of RhB, 5% Fe2O3/Ag3VO4 can degrade 79.0% of RhB and 10% Fe2O3/Ag3VO4 can degrade only 65.8% at 60 min.
image file: c5ra22912j-f7.tif
Fig. 7 Photocatalytic degradation of RhB in the presence of pure Ag3VO4 and Fe2O3/Ag3VO4 composites, and photolysis of RhB under visible light irradiation. Results are expressed as means ± the standard error from three independent experiments.

3.7 EIS analysis

The electrochemical impedance spectroscopy of pure Ag3VO4 and Fe2O3/Ag3VO4 composites was carried out to investigate the process of electron transfer. Fig. 8 shows that the EIS data fits well with the Rs(Q(RctZw)) equivalent circuit. The diameter of the semicircular part at higher frequencies is equal to the electrochemical reaction impedance, Rct, which reflects the charge transfer rate occurring at the contact interface between the working electrode and electrolyte solution.44 The smaller radius of the Nyquist circle represents the lower charge-transfer resistance.45 Fig. 8 shows that the arc radius on the EIS Nyquist plot of 1% Fe2O3/Ag3VO4 composite is smaller than that of pure Ag3VO4. This means that a faster interfacial charge transfer to electron acceptor occurs, which resulted from effective separation of electron–hole pairs by the introduction of Fe2O3.46,47
image file: c5ra22912j-f8.tif
Fig. 8 Electrochemical impedance spectroscopy of pure Ag3VO4 and 1% Fe2O3/Ag3VO4 composite. The inset shows the equivalent circuit: Rs(Q(RctZw)); Rs: ohmic resistance of the solution, Q: electric double-layer capacitance, Rct: electrochemical reaction impedance, and Zw: solid phase diffusion of optical electron.

3.8 Mechanism of pollutant photodegradation

The photocatalytic stability of Fe2O3/Ag3VO4 was evaluated by the RhB cycle degradation experiments under visible light. As shown in Fig. 9, the photoactivity of Fe2O3/Ag3VO4 can remain very high after three consecutive cycles. Therefore, Fe2O3/Ag3VO4 composite can be used as an effective, stable photocatalyst for the degradation of organic pollutants.
image file: c5ra22912j-f9.tif
Fig. 9 Cycling runs of 1% Fe2O3/Ag3VO4 photocatalyst for RhB degradation.

To explore the photocatalytic mechanism of RhB, a series of active species trapping experiments was carried out. The results of adding different radical scavengers over the Fe2O3/Ag3VO4 photocatalysts under visible-light irradiation are described in Fig. 10. When triethanolamine (a quencher of h+) was added, the photocatalytic degradation of RhB greatly declined compared to the reaction without radical scavengers, which indicates that h+ is the main active species of Fe2O3/Ag3VO4 for the degradation of RhB. Another quencher of h+ (EDTA-2Na) was used to verify this result. The photoactivity is remarkably decreased, which is consistent with the result of triethanolamine addition. Furthermore, when ascorbic acid as a scavenger for ˙O2 is added, the photodegradation process can be inhibited effectively. This suggests that ˙O2 also plays the critical role in the photocatalysis process. Finally, RhB photodegradation is not obviously affected when isopropanol is applied as ˙OH scavenger. Therefore, the ˙OH is not the main active species in the reaction of the RhB degradation. The free radicals trapping experiments indicate that h+ and ˙O2 are the main active species.


image file: c5ra22912j-f10.tif
Fig. 10 Trapping experiment of active species during the photocatalytic degradation of RhB over 1% Fe2O3/Ag3VO4 composites under visible light irradiation.

Based on the results mentioned above, a possible mechanism for the photocatalytic degradation of organic compounds by Fe2O3/Ag3VO4 is proposed. As shown in Fig. 11, both Ag3VO4 and Fe2O3 can be excited to generate electrons and holes under visible light irradiation. ECB and EVB can be calculated according to the formulas: ECB = χEC − 0.5Eg and EVB = ECB + Eg. Eg is the band gap of the semiconductor, ECB is the conduction band potential, EC is the energy of free electrons on the hydrogen scale (4.5 eV), EVB is the valence band potential and χ is the absolute electronegativity of the semiconductor. According to the UV-vis analysis and potential calculation, the ECB of Ag3VO4 was located at −0.01 eV, which was more negative than the CB potential of Fe2O3 (0.37 eV). In addition, the EVB of Ag3VO4 was located at 2.29 eV, which was more negative than the VB potential of Fe2O3 (2.38 eV). Therefore, the photogenerated electrons in the Ag3VO4 particles could be quickly transferred to Fe2O3. The holes generated in the VB of Fe2O3 could easily move to Ag3VO4, which would promote the effective separation of photoexcited electron–hole pairs and decrease the recombination of electron and hole. This is consistent with the result of the EIS analysis. The electrons on the Fe2O3 could combine with oxygen in the solution to form ˙O2. The generated ˙O2 on the CB of Fe2O3 and the hole on the VB of Ag3VO4 would play important roles in the photocatalytic reaction process, leading to enhanced photocatalytic performance.


image file: c5ra22912j-f11.tif
Fig. 11 Schematic of the separation and transfer of photogenerated charges in the Fe2O3/Ag3VO4 composites combined with the possible reaction mechanism of the photocatalytic procedure.

4. Conclusions

In this study, Fe2O3 modified Ag3VO4 photocatalysts with various Fe2O3 contents were successfully prepared by a simple precipitation technique. They were used for the first time as a photocatalyst for the degradation of RhB under visible light irradiation. The photocatalytic degradation activity of Ag3VO4 was greatly improved by Fe2O3 modification. 1% Fe2O3/Ag3VO4 composite showed much higher photoactivity than Ag3VO4 and can degrade 96.1% of RhB in 60 min. According to the results of EIS and the trapping experiments, the introduced Fe2O3 effectively accelerates the separation of photogenerated electrons and holes, leading to enhanced photocatalytic activity. As a result, the Fe2O3/Ag3VO4 photocatalyst is a potential catalyst for the treatment of organic pollutants.

Acknowledgements

This study is financially supported by the National Natural Science Foundation of China for Youths (No. 21407065 and 21507046), the Natural Science Foundation of Jiangsu Province for Youths (BK20140533), China Postdoctoral Science Foundation (No. 2014M551520 and 2015T80514), Jiangsu University Scientific Research Funding (No. 14JDG052).

Notes and references

  1. M. Barroso, A. J. Cowan, S. R. Pendlebury, M. Gr€atzel, D. R. Klug and J. R. Durrant, J. Am. Chem. Soc., 2011, 133, 14868–14871 CrossRef CAS PubMed.
  2. S. K Li, F. Z Huang, Y. Wang, Y. H Shen, L. G. Qiu, A. J. Xie and S. J. Xu, J. Mater. Chem., 2011, 21, 7459 RSC.
  3. D. Li, X. C. Duan, Q. Qin, H. M. Fan and W. J. Zheng, CrystEngComm, 2013, 15, 8933–8936 RSC.
  4. L. F. Zhu, D. Q. Huang, J. F. Ma, D. R. Wu, M. R. Yang and S. Komarneni, Ceram. Int., 2015, 41, 12509–12513 CrossRef CAS.
  5. J. X. Wang, P. X. Wang, Y. T. Cao, J. Chen, W. J. Li, Y. Shao, Y. Zheng and D. Z. Li, Appl. Catal., B, 2013, 136–137, 94–102 CrossRef CAS.
  6. H. Xu, J. X. Zhu, Y. X. Song, T. T. Zhu, W. K. Zhao, Y. H. Song, Z. L. Da, C. B. Liu and H. M. Li, J. Alloys Compd., 2015, 622, 347–357 CrossRef CAS.
  7. H. H. Chen and Y. M. Xu, Appl. Surf. Sci., 2014, 319, 319–323 CrossRef CAS.
  8. H. Xu, H. Z. Zhao, Y. H. Song, W. Yan, Y. G. Xu, H. P. Li, L. Y. Huang, S. Yin, Y. P. Li, Q. Zhang and H. M. Li, Mater. Sci. Semicond. Process., 2015, 39, 726–734 CrossRef CAS.
  9. D. P. Das, R. K. Barik, J. Das, P. Mohapatra and K. M. Parida, RSC Adv., 2012, 2, 7377–7379 RSC.
  10. X. C. Tao, Q. Hong and T. Z. Xu, J. Mater. Sci.: Mater. Electron., 2014, 25, 3480–3485 CrossRef CAS.
  11. L. Zhang, Y. M. He, P. Ye, W. H. Qin, Y. Wu and T. H. Wu, Mater. Sci. Eng., B, 2013, 178, 45–52 CrossRef CAS.
  12. J. X. Wang, H. Ruan, W. J. Li, D. Z. Li, Y. Hu, J. Chen, Y. Shao and Y. Zheng, J. Phys. Chem. C, 2012, 116, 13935–13943 CAS.
  13. G. S. Sun, H. Xu, H. M. Li, H. M. Shu, C. T. Liu and Q. Zhang, React. Kinet., Mech. Catal., 2010, 99, 471–484 CAS.
  14. X. X. Hu and C. Hu, J. Chem. Technol. Biotechnol., 2010, 85, 1522–1527 CAS.
  15. L. Zhang, Y. M. He, P. Ye, Y. Wu and T. H. Wu, Catal. Commun., 2013, 30, 14–18 CrossRef CAS.
  16. L. Zhang, Y. M. He, P. Ye, Y. Wu and T. H. Wu, J. Alloys Compd., 2013, 549, 105–113 CrossRef CAS.
  17. B. Inceesungvorn, T. Teeranunpong, J. Nunkaew, S. Suntalelat and D. Tantraviwat, Catal. Commun., 2014, 54, 35–38 CrossRef CAS.
  18. K. Wangkawong, S. Suntalelat, D. Tantraviwat and B. Inceesungvorn, Mater. Lett., 2014, 133, 119–122 CrossRef CAS.
  19. J. Xie, Z. Zhou, Y. W. Lian, Y. J. Hao, P. Li and Y. Wei, Ceram. Int., 2015, 41, 2622–2625 CrossRef CAS.
  20. Y. J. Liu, L. Sun, J. G. Wu, T. Fang, R. Cai and A. Wei, Mater. Sci. Eng., B, 2015, 194, 9–13 CrossRef CAS.
  21. S. C. Han, L. F. Hu, Z. Q. Liang, S. Wageh, A. A. Al-Ghamdi, Y. S. Chen and X. S. Fang, Adv. Funct. Mater., 2014, 24, 5719–5727 CrossRef CAS.
  22. L. M. He, L. Q. Jing, Z. J. Li, W. T. Sun and C. Liu, RSC Adv., 2013, 3, 7438–7444 RSC.
  23. Y. Zhang, Y. R. Zhang and J. Tan, J. Alloys Compd., 2013, 574, 383–390 CrossRef CAS.
  24. H. H. Zhao, L. S. Zhang, X. D. Gu, S. J. Li, B. Li, H. l. Wang, J. M. Yang and J. S. Liu, RSC Adv., 2015, 5, 10951 RSC.
  25. Z. Y. Lin, P. Liu, J. H. Yan and G. W. Yang, J. Mater. Chem. A, 2015, 3, 14853–14863 CAS.
  26. S. Q. Huang, Y. G. Xu, Z. G. Chen, M. Xie, H. Xu, M. Q. He, H. M. Li and Q. Zhang, RSC Adv., 2015, 5, 71035–71045 RSC.
  27. J. Cao, Z. Y. Wang, R. Wang, S. Liu, T. Fei, L. J. Wang and T. Zhang, RSC Adv., 2015, 5, 36340–36346 RSC.
  28. B. M. Pirzada, O. Mehraj, N. A. Mir, M. Z. Khan and S. Sabir, New J. Chem., 2015, 39, 7153–7163 RSC.
  29. Y. Y. Xu, G. Y. Zhang, G. X. Du, Y. Q. Sun and D. Z. Gao, Mater. Lett., 2013, 92, 321–324 CrossRef CAS.
  30. J. Dobosz and M. Zawadzki, React. Kinet., Mech. Catal., 2015, 114, 157–172 CrossRef CAS.
  31. M. Alagiri and S. B. A. Hamid, Mater. Lett., 2014, 136, 329–332 CrossRef CAS.
  32. X. Zhang, Y. A. Niu, Y. Li, Y. Li and J. P. Zhao, J. Solid State Chem., 2014, 211, 69–74 CrossRef CAS.
  33. C. M. Huang, G. T. Pan, Y. M. Li, M. H. Li and T. C. Yang, Appl. Catal., A, 2009, 358, 164–172 CrossRef CAS.
  34. M. W. Xue, J. Z. Ge, H. L. Zhang and J. Y. Shen, Appl. Catal., A, 2007, 330, 117–126 CrossRef CAS.
  35. S. M. Wang, Y. Guan, L. P. Wang, W. Zhao, H. He, J. Xiao, S. G. Yang and C. Sun, Appl. Catal., B, 2015, 168–169, 448–457 CrossRef CAS.
  36. F. Kiantazh and A. Habibi-Yangjeh, Mater. Sci. Semicond. Process., 2015, 39, 671–679 CrossRef CAS.
  37. T. T. Zhu, Y. H. Song, H. Y. Ji, Y. G. Xu, Y. X. Song, J. X. Xia, S. Yin, Y. P. Li, H. Xu, Q. Zhang and H. M. Li, Chem. Eng. J., 2015, 271, 96–105 CrossRef CAS.
  38. S. F. Chen, W. Zhao, W. Liu, H. Y. Zhang, X. L. Yu and Y. H. Chen, J. Hazard. Mater., 2009, 172, 1415–1423 CrossRef CAS PubMed.
  39. M. Omran, T. Fabritius, A. M. Elmahdy, N. A. Abdel-Khalek, M. El-Aref and A. E. Elmanawi, Appl. Surf. Sci., 2015, 345, 127–140 CrossRef CAS.
  40. S. Guo, G. K. Zhang, Y. D. Guo and J. C. Yu, Carbon, 2013, 60, 437–444 CrossRef CAS.
  41. H. Xu, H. M. Li, L. Xu, C. D. Wu, G. S. Sun, Y. G. Xu and J. Y. Chu, Ind. Eng. Chem. Res., 2009, 48, 10771–10778 CrossRef CAS.
  42. Y. Liu, Y. X. Yu and W. D. Zhang, Int. J. Hydrogen Energy, 2014, 39, 9105–9113 CrossRef CAS.
  43. J. Theerthagiri, R. A. Senthil, A. Priya, J. Madhavan, R. J. V. Michael and M. Ashokkumar, RSC Adv., 2014, 4, 38222–38229 RSC.
  44. X. H. Kang, J. Wang, H. Wu, I. A. Aksay, J. Liu and Y. H. Lin, Biosens. Bioelectron., 2009, 25, 901–905 CrossRef CAS PubMed.
  45. J. Di, J. X. Xia, Y. P. Ge, H. P. Li, H. Y. Ji, H. Xu, Q. Zhang, H. M. Li and M. N. Li, Appl. Catal., B, 2015, 168–169, 51–61 CrossRef CAS.
  46. B. F. Xin, Z. Y. Ren, P. Wang, J. Liu, L. Q. Jing and H. G. Fu, Appl. Surf. Sci., 2007, 253, 4390–4395 CrossRef CAS.
  47. Q. Wu, J. J. Ouyang, K. P. Xie, L. Sun, M. Y. Wang and C. J. Lin, J. Hazard. Mater., 2012, 199–200, 410–417 CrossRef CAS PubMed.

This journal is © The Royal Society of Chemistry 2016
Click here to see how this site uses Cookies. View our privacy policy here.