DOI:
10.1039/C6RA13022D
(Paper)
RSC Adv., 2016,
6, 83471-83481
Light-driven removal of rhodamine B over SrTiO3 modified Bi2WO6 composites
Received
19th May 2016
, Accepted 31st July 2016
First published on 16th August 2016
Abstract
SrTiO3/Bi2WO6 hybrids were hydrothermally prepared and structurally examined by means of various chemical and physical techniques. Formation of heterojunction is well confirmed via HRTEM, XPS and PL and contributes immensely to the enhanced catalytic function of a composite in an assay of Rhodamine B (Rh B) photodegradation due to accelerated migration and separation of charge carriers at it. Among as-prepared samples, Bi2WO6 loaded with 8 wt% SrTiO3 proves most photocatalytically active in light of a top degradation rate (D) of ca. 98.4% and a peak apparent kinetic rate (k) of 0.0463 min−1. Besides, h+ and ·OH turn out to be the major reactive species for Rh B degradation. Finally, based on theoretical and experimental results, a possible reaction mechanism was proposed.
1. Introduction
Semiconductor-based photocatalysis demonstrates its predominance over thermal and electrocatalysis by its unique properties such as environmental compatibility and resource conservation on account of substitution of solar energy for non-renewable energy and absence of additional heat suppliers in most cases. Therefore, it has been extensively explored and has found versatile application in H2 evolution,1–6 dye degradation7–10 and CO2 immobilization.11,12 Undoubtedly, engineering and fabrication of a highly active semiconductor photocatalyst as an efficient energy converter center at this process. Among well-exploited promoter options, SrTiO3, a typical cubic perovskite, has been proposed for use as an excellent n-type semiconductor material on account of a collection of outstanding physical and chemical performances including but not limited to (a) excellent (photo)chemical and thermal durability, (b) intriguing structural, electronic and optical attributes such as powerful reducibility of electrons on its conduction band (ECB = −0.8 eV (ref. 13)) and (c) facile synthesis with various existing methods from earth-abundant feedstocks, thus it witnesses huge significant progresses in artificial photosynthesis and environmental purification.14 Nevertheless, it falls short of response to visible light due to unduly wide bandgap (ca. 3.1 eV) and suppressed recombination of photogenerated exactions that are urgent for its application.15 To address these issues, numerous attempts on its structural and chemical modification have been made.14,16
Structural modification is put to effect by introduction of porous some structures (e.g. mesoporous-assembled SrTiO3 (ref. 17)) or designated shapes (e.g. SrTiO3 spheres18 and nanocubes19) on micro/nano scale. Generally, these samples are seldom visible-light-driven despite enhanced photocatalytic function available under UV irradiation. As a most promising alternative, chemical modification consisting mainly of chemical doping14,16 and construction of heterostructure20 enables a red shift of optical absorption to visible light and prompt separation of photoinduced charges, favorable for elevated light-simulated catalytic performance. With regard to contribution to the aforementioned behaviors, constructing SrTiO3-based hybrid materials takes the lead. Visible-light-responsive semiconductors involving g-C3N4,20 Cu2O,21 NiFe2O4 (ref. 22) and BiVO4 (ref. 23) were reported to function as good building blocks to construct functional assemblies with SrTiO3. Notably, amongst the semiconductors, bismuth tungsten (Bi2WO6), the simplest member among Aurivillius family oxides with general formula Bi2An−1BnO3n+3 (A = Ca, Sr, Ba, Pb, Bi, Na and K; B = Ti, Nb, Ta, Mo, W and Fe), has triggered keen interest among scholars on photocatalysis in view of (1) its unique layer structure composed of corner-sharing WO6 octahedral sheets and bismuth oxide sheets,24 (2) excellent visible-light-induced semiconducting behavior with tunable optical harvesting and separation efficiency of electron–hole pairs via morphological and chemical modification and desirable chemical stability25,26 and (3) effortless preparation through hydrothermal treatment from widely available raw materials.26,27 Such characteristics provide ample options to construct a broad set of Bi2WO6-based (photo)catalytic systems for CO2 utilization,24,28 environmental pollutant consumption29,30 and H2 and/or O2 evolution.31 For example, Ma et al.32 developed a novel visible-light-excited trinary Z-scheme composite g-C3N4/RGO/Bi2WO6 (RGO = reduced graphene oxide) via a hydrothermal route for dechlorination and degradation of 2,4,6-trichlorophenol (TCP). The composite (D = 98%) turned out to be much preponderant in catalytic property relative to its reference samples (D = 52%, 58% and 62% for Bi2WO6, g-C3N4 and Bi2WO6/g-C3N4, respectively) attributed to the efficient visible-light utilization efficiency and the construction of Z-scheme system using RGO as a charge transmission bridge between the g-C3N4 and the Bi2WO6. The author highlighted that accelerated separation and migration of photoinduced electrons and holes were accompanied by unaltered redox ability of these excitons accumulated in the conduction band (CB) of g-C3N4 and in the valence band (VB) of Bi2WO6 for Z-scheme mechanism. However, in the absence of RGO, a flow of charge carriers along the double-transfer path is prone to take place,33,34 indicative of the key role RGO played. The double-transfer path equally allows encouraged splitting of excitons at the expense of their redox capacity, leading to raised light-driven catalytic performance. The two mechanisms are also suitable to other Bi2WO6-based hybrids.35,36 Nevertheless, the double-transfer mechanism attracts much more attention than Z-scheme path. Therefore, we try to develop an unreported double-transfer mechanism by coupling SrTiO3 with Bi2WO6 to offer enhanced catalytic performance in Rh B removal compared with the individuals in this paper.
Herein, SrTiO3/Bi2WO6 heterojunctions were synthesized via a simple two-step hydrothermal process for the first time. Besides, they were characterized by means of XRD, TEM, SEM, XPS, DRS, BET and PL. Construction of heterostructure is well-certificated and holds the main part in elevated photocatalytic function of Rh B removal. Among as-prepared samples, Bi2WO6 decorated with 8 wt% SrTiO3 loading is the optimal sample (D = 98.4% and k = 0.0463 min−1), far outperforming those of Bi2WO6 (D = 86.0% and k = 0.0218 min−1). Furthermore, h+ and ·OH are confirmed as the major reactive species for this process. Finally, a possible reaction mechanism was proposed.
2. Experimental
2.1. Chemicals
Bismuth nitrate (Bi(NO3)3·5H2O), sodium tungstate (Na2WO4·2H2O), sodium hydroxide (NaOH), titanium tetrachloride (TiCl4), strontium hydroxide (Sr(OH)2·8H2O), anhydrous ethanol (CH3CH2OH) and hydrochloric acid (HCl) were purchased from Shanghai Chemical Reagent Company in analytical grade, and used as received without further purification. Deionized water was used throughout the whole experiment.
2.2. Synthesis
2.2.1. Synthesis of SrTiO3. The synthetic procedure of SrTiO3 was described elsewhere.37 Briefly, to homogeneous mixture of hydrochloric solution (2.3 mL, 2 M) and titanium tetrachloride (1.1 mL) was dropwise added aqueous strontium hydroxide (0.27 M, 40 mL) under constant agitation. The resulting mixture was hydrothermally treated at 180 °C for 48 h. After cooling to the room temperature naturally, the obtained precipitate was centrifuged, washed with distilled water and ethanol 4 times, dried at 80 °C and then well-ground for further use.
2.2.2. Synthesis of SrTiO3/Bi2WO6 heterojunctions. In situ growth of Bi2WO6 on the surface of SrTiO3 via hydrothermal method was performed as follows. First, an appropriate amount of SrTiO3 was suspended in aqueous Bi(NO3)3·5H2O (0.25 M, 40 mL) under vigorous stirring. Subsequently, aqueous Na2WO4·2H2O (0.25 M, 20 mL) was introduced dropwise into the resulting suspension above. After the agitation for 0.5 h, the obtained mixture underwent hydrothermal treatment at 180 °C for 12 h. Upon cooling to the ambient temperature, the crude product was collected via centrifugation, rinsed with distilled water and ethanol several times, dried at 80 °C for 4 h and thoroughly ground into powder. According to the steps above, by changing the amount of SrTiO3, a series of composites with various mass ratio of SrTiO3 to Bi2WO6 or SrTiO3 loading (x = 1, 8, 10, and 15 wt%) were synthesized. Similarly, Bi2WO6 and SrTiO3 were fabricated as reference samples.
2.3. Photocatalytic test
Photocatalytic activities of SrTiO3/Bi2WO6 heterojunctions were evaluated by photocatalytic degradation of Rh B under simulated sunlight. A 500 W Xe lamp without any UV cutoff filter was used as a light source. A mixture of a composite (0.2 g) and aqueous Rh B (30 mg L−1, 250 mL) was magnetically stirred for 60 min in dark to establish the adsorption–desorption equilibrium between them. Afterwards, the reaction was allowed for 90 min with light and stirring on. The temperature control of the whole system at ca. 25 °C was achieved by a flow of cooling water. At intervals of 15 min, 5 mL of suspension was collected and centrifuged to remove composite particles. The concentration of the remaining supernatant was determined by concentration-dependent absorbance on a UV spectrophotometer. Rh B degradation rate (D) and apparent rate constant (k) as indicators of photocatalytic performance of as-prepared samples can be calculated from the following equations: |
D = (1 − C/Ce) × 100%
| (1) |
where Ce (mg L−1) and C (mg L−1) respectively denote the equilibrium concentration in dark and instantaneous concentration after a period of time t (min) under irradiation.
2.4. Characterization
X-ray diffraction (XRD) patterns were collected on a Bruker D8-Discover instrument with Cu-Kα radiation (λ = 1.54178 nm). Morphology and size of samples were observed through transmission electron microscopy (TEM, FEI Tecnai G2-F30) and field-emission scanning electron microscopy (SEM, JSM-7800F). Chemical composition was determined via X-ray photoelectron spectroscopy (XPS) (VG Multiab-2000) using a PHI Quantum 2000 XPS system with a monochromatic Al-Ka source and a charge neutralizer. UV-vis diffuse reflection spectroscopy (DRS) was measured with a Shimadzu UV 3600 spectrometer. Photoluminescence (PL) spectra were taken at room temperature on a fluorospectrophotometer (Fluoromax-4) using a Xe lamp as an excitation source. The BET surface areas of the samples were obtained from a Micromeritics ASAP 2020M system at liquid nitrogen temperature (77 K).
3. Results and discussion
3.1. XRD analysis
XRD investigation is conducted to unequivocally illuminate the crystal structures of as-prepared samples. Typical XRD patterns of these samples are summarized in Fig. 1, along with the standard curves of orthorhombic-phase Bi2WO6 (JCPDS no. 73-1126) and cubic-phase SrTiO3 (JCPDS no. 35-0734). With regard to bare Bi2WO6 (Fig. 1a), a series of narrow, sharp characteristic peaks located at 28.4, 32.8, 47.1, 55.9 and 58.6° are separately assigned to (113), (200), (220), (313) and (226) planes. Perfect accordance of these peaks with their counterparts in the standard Bi2WO6 curve indicates the sample with orthorhombic phase. For another thing, interplanar spacing of (113) and (200) planes are in several estimated as 0.316 and 0.273 nm. In the case of pristine SrTiO3 (Fig. 1f), main diffraction peaks at 32.4, 39.9, 46.5, 57.7 and 67.6° correspond to the (110), (111), (200), (211) and (220) planes, respectively. It can be identified as a sample with cubic perovskite structure in comparison with those in standard pattern of cubic-phase SrTiO3. Also, the (110) plane has a interplanar spacing of ca. 0.276 nm. In terms of SrTiO3/Bi2WO6 hybrids (Fig. 1b–e), the major diffraction signals analogous to pure Bi2WO6 are evidently observed, suggesting that crystal structure of Bi2WO6 is insensitive to SrTiO3 loading. Besides, characteristic peaks associated with SrTiO3 are scarcely visible, possibly ascribed to low SrTiO3 loading in the composites, which is similar to those described by Ge et al.34 and Liu et al.15
 |
| Fig. 1 XRD patterns of (a) Bi2WO6, (f) bare SrTiO3, and ((b)–(e)) SrTiO3/Bi2WO6 heterojunctions with 1, 8, 10, 15 wt% SrTiO3 loading, respectively. | |
3.2. SEM, TEM and hydrothermal synthesis mechanism analysis
3.2.1. SEM and TEM analysis. A meticulous comparison on surface morphology and particle size of as-prepared samples are thoroughly made by means of SEM and TEM graphs presented in Fig. 2. Fig. 2a exhibits homogeneous and shaggy microspheres (ca. 6 μm in size) composed of Bi2WO6 sheets, which can be seen more clearly in the inset. In Fig. 2b, bare SrTiO3 displays quasi-spherical particles with a smooth surface and a narrow size distribution from 50 to 310 nm. Fig. 2c describes surface-rough and subsphaeroidal SrTiO3/Bi2WO6 particles in the size range of ca. 2–4 μm. The magnified graph reveals SrTiO3 pellets randomly “suspended” in the ocean of Bi2WO6 sheets (insets in Fig. 2c). HRTEM of 8 wt% SrTiO3/Bi2WO6 in Fig. 2d displays a clear fringe with lattice spacing of 0.315, 0.271 and 0.275 nm respectively indexed as (113) and (200) planes of Bi2WO6 and (110) plane of SrTiO3, which is in good agreement with XRD results. Therefore, structural preservation of the two individuals occurs before and after their combination. More importantly, the image provides a convincing evidence for construction of the intimate contact on nanoscale level between SrTiO3 and Bi2WO6, opening a door to elevated photocatalytic function by perfecting transmission paths of excitons.
 |
| Fig. 2 SEM of Bi2WO6 (a) and SrTiO3 (b) and SEM (c) and HRTEM (d) of 8 wt%-SrTiO3/Bi2WO6. | |
TEM-EDX mapping serves as a powerful tool in analysis of elemental component and distribution of samples. To obtain the knowledge above, mapping of 8 wt%-SrTiO3/Bi2WO6 sample (Fig. 3) is provided for detailed discussion, coupled with the selected TEM area for EDX mapping analysis (Fig. 3a). Remarkably, Sr and Ti dominates the quasi-spherical area with an even distribution (Fig. 3e and f), leaving the other behind for Bi and W (Fig. 3c and d). Also, O fills the whole area. Due to definition of SrTiO3 and Bi2WO6 as quasi-spherical and sheet-like powder by SEM observations, it can be concluded that Sr and Ti mainly exist in SrTiO3 and Bi and W in Bi2WO6. In other words, the two plain components only closely contacts with each other at their interfaces with little elemental exchange.
 |
| Fig. 3 (a) TEM image and ((b)–(f)) the corresponding EDX mapping of O, Bi, W, Ti and Sr, respectively, for 8 wt% SrTiO3/Bi2WO6. | |
3.2.2. Synthesis mechanisms of samples. It is well-known that synthesis mechanisms of samples enable profound insights of their preparations. Detailed description of related mechanisms are as follows.
3.2.2.1 The formation of SrTiO3 spheres. For SrTiO3 spheres, a possible mechanism of their formation begins with gradual hydrolysis of TiCl4 in HCl to TiO2 with elevated alkalinity due to drop-by-drop addition of Sr(OH)2. Afterwards, the obtained TiO2 undergoes dissolution–precipitation route described elsewhere.18,38 Firstly, TiO2 is converted to a dissoluble and highly reactive intermediate Ti(OH)62− upon further addition of Sr(OH)2. Subsequently, the active species immediately combines with Sr2+ to form SrTiO3 nuclei. The hydrothermal condition in this work favors self-assembly of these nuclei to SrTiO3 pellets with a minimum surface energy. The related chemical steps can be represented with the following formulas: |
Ti4+ + 2H2O → TiO2 + 4H+
| (4) |
|
TiO2 + 2OH− + 2H2O → Ti(OH)62−
| (5) |
|
Ti(OH)62− + Sr2+ → SrTiO3 + H2O
| (6) |
3.2.2.2 The formation of Bi2WO6 spheres. According to synthetic process of Bi2WO6 in Section 2.2, total amount of Na2WO4 corresponds just to stoichiometric proportion that completely precipitates Bi3+. Therefore, dissoluble tungstenic acid (H2WO4) and tungstic oxide (WO3) can hardly result. In other words, Bi2WO6 is the only precipitate.39,40 During formation of Bi2WO6 microspheres, Bi3+ species are at first reversibly hydrolyzed to BiONO3. Next, WO42− ions combine with Bi3+, leading to Bi2WO6 nucleation. What's more, hydrothermal route (180 °C, 12 h) enables growth of Bi2WO6 cores to sheets and their subsequent integration into microspheres. These steps can be summarized with the following equations: |
Bi3+ + H2O + NO3− ⇌ BiONO3 + 2H+
| (7) |
|
2Bi3+ + WO42− + 2H2O → Bi2WO6 + 4H+
| (8) |
3.2.2.3 In situ decoration of SrTiO3 pellets with Bi2WO6 microspheres. To begin with, SrTiO3 pellets are constructed following eqn (3)–(6) and serve as a base for their excellent chemical contact with Bi2WO6, leading to elevated separation efficiency of light-induced excitons and thus enhanced photocatalytic performance. Next, entry of Bi3+ precursor into SrTiO3 suspension results in adsorption on the surface of SrTiO3 pellets (SrTiO3·Bi3+) and thus slightly higher binding energy of Bi3+ (Fig. 4d). Moreover, upon addition of WO42− species, they instantly bind with chemisorbed and unbounded Bi3+ to form Bi2WO6 amorphous cores. Finally, these cores are hydrothermally driven to form sheet-like Bi2WO6 and further self-assemble to Bi2WO6 microspheres that wrap SrTiO3 pellets (Fig. 2c). The chemical process except eqn (3)–(6) present below: |
SrTiO3·Bi3+ + WO42− + 2H2O → SrTiO3·Bi2WO6 + 4H+
| (9) |
 |
| Fig. 4 (a) The survey spectrum, ((f)–(h)) O 1s levels of Bi2WO6, SrTiO3 and 8 wt%-SrTiO3/Bi2WO6 and high-resolution XPS spectra of (b) Ti 2p, (c) Sr 3d, (d) Bi 4f, (e) W 4f. | |
3.3. XPS analysis
XPS measurements are implemented to identify the surface composition and chemical state of as-prepared samples. The binding energies obtained in the XPS analysis are calibrated using C 1s peak at 284.6 eV.41 XPS spectra of 8 wt%-SrTiO3/Bi2WO6, SrTiO3 and Bi2WO6 are summarized in Fig. 4. Fig. 4a exhibits a wide scan XPS spectrum for these samples. Sr, Ti and O form SrTiO3 and Bi, W and O constitute Bi2WO6. Interestingly, unlike four other elements, Ti is “absent” for 8 wt%-SrTiO3/Bi2WO6 due to excessive signal overlap of Ti 2p with that of Bi 4d (marked with dashed rectangle). Similar incident occurs to O 1s for SrTiO3 in 8 wt%-SrTiO3/Bi2WO6. In Fig. 4b, the characteristic doublet at 464.0 and 458.3 eV related to Ti 2p1/2 and Ti 2p3/2 indicates the presence of Ti4+ in SrTiO3.13 However, Ti 2p signal at 458.1 eV appears very faint in view of signal overlap as before (see Fig. 4a). Sr2+ in the composite is well-determined by a pair of peaks at 134.0 and 132.3 eV (Fig. 4c) assigned to Sr 3d orbit.15 The binding energies of 159.1 and 164.4 eV (Fig. 4d) are ascribed to the Bi 4f7/2 and Bi 4f5/2, evidencing that Bi in the composite exists in the 3+ oxidation state. The binding energies of 37.4 eV and 35.4 eV (Fig. 4e) separately assigned to W 4f5/2 and W 4f7/2 support W6+ in the hybrid.42 The O 1s spectra seem more complex than those of other elements. To make them understood, they are all well deconvoluted and exhibited in Fig. 4f and g. Evidently, XPS spectrum of O 1s for Bi2WO6 (Fig. 4f) presents a triplet at 532.7, 530.9 eV and 530.0 eV, corresponding to the absorbed oxygen and the lattice oxygen W–O and Bi–O in the framework of Bi2WO6.33,43,44 For SrTiO3 (Fig. 4g), those peaks at 532.3, 530.2 and 529.2 eV are associated with H, Ti and Sr bonded oxygen, respectively.45,46 In the case of the composite (Fig. 4h), O 1s spectrum of SrTiO3 can hardly be observed in light of its relatively low loading (8 wt%) and peak overlap with Bi2WO6 (Fig. 4a). Therefore, only the latter O 1s spectrum can be found. Notably, relative to those of plain Bi2WO6 and SrTiO3, Bi 4f, W 4f, Sr 3d and O 1s spectra of the composite (Fig. 4c–h) sample undergo slight chemical shifts, providing a solid evidence for construction of the heterostructure between plain Bi2WO6 and SrTiO3 as TEM does.
3.4. DRS analysis
A remarkable insight into optical property and band gaps of as-prepared samples is available via DRS as illustrated in Fig. 5. In Fig. 5a, bare Bi2WO6 sample is characterized by a strong band-edge absorption in the visible light region with an absorption edge at 430 nm. As for pure SrTiO3, it is endowed with forceful near-visible band-edge absorption and an absorption edge at 396 nm. Noticeably, with respect to the hybrids, typical semiconducting optical harvesting curves stand out. In particular, the x-dependent successively blue shift of these curves in comparison with that of Bi2WO6 indicates a tunable optical property as a third knock-down witness for construction of the heterostructure between the pure components.1,9
 |
| Fig. 5 The optical properties (a) and bandgap energies (b) of as-prepared samples. | |
The bandgap (Eg) of a semiconductor is calculated according to the following equation (Fig. 5b):47–49
where
α,
ν,
Eg and
A represent the absorption coefficient, the light frequency, the band gap and a constant, respectively.
Egs of SrTiO
3 and Bi
2WO
6 are determined to be 3.05 (
n = 4 (
ref. 50)) and 2.88 eV (
n = 2 (
ref. 51)), respectively, which are consistent with the previous reports.
22,23,52 Besides, 8 wt%-SrTiO
3/Bi
2WO
6 corresponds to a hybrid semiconductor with
Eg = 2.93 eV (
n = 2).
3.5. PL analysis
It is well-established that PL intensity functions as an indicator of separation efficiency of light-excited charges in light of origin of PL emission from charge recombination. As a result, PL analyses of SrTiO3, Bi2WO6 and 8 wt%-SrTiO3/Bi2WO6 are conducted and illustrated in Fig. 6. Obviously, all samples are endowed with a peak emission wavelength of ca. 465 nm possibly due to their approximate band gaps (e.g. Eg = 2.88, 3.05 and 2.93 eV respectively for Bi2WO6, SrTiO3 and 8 wt%-SrTiO3/Bi2WO6). In Fig. 6a, typical quenched PL intensity of 8 wt%-SrTiO3/Bi2WO6 indicates enhanced separation efficiency of charge carriers via efficient construction of the heterostructure between Bi2WO6 and SrTiO3. Besides, x-dependent PL intensity observed in Fig. 6b suggests separation efficiency as a function of x. More specifically, enhanced separation efficiency of excitons (decreased PL intensity of samples) coincides with increased x (x ≤ 8 wt%) or diminished x (x > 8 wt%). To conclude, the optimal separation efficiency is achieved at x = 8 wt% and correspond to the peak photocatalytic performance (Fig. 8). The trend is possibly associated with insufficient formation of the heterojunction by excessively low SrTiO3 loading or creation of new recombination sites by its overloading.
 |
| Fig. 6 PL patterns of SrTiO3, Bi2WO6 and 8 wt%-SrTiO3/Bi2WO6. | |
3.6. BET and DFT analysis
BET specific surface areas (SBET), N2 adsorption–desorption curves (the red line) and DFT pore-size distributions (the black line) are provided in Fig. 7. To begin with, SBET ascends up to 35.7 m2 g−1 (x ≤ 8 wt%) and then descends (x > 8 wt%) for the composites. The trend agrees well with those of the amount of Rh B (Ad) adsorbed in the dark on the surface of composites, D and k (Fig. 8). In summary, 8 wt%-SrTiO3/Bi2WO6 with a peak SBET provides the optimal photocatalysis, indicating that SBET is beneficial for enhanced photocatalytic performance. Next, according to IUPAC recommendation, Fig. 7 displays typical II isothermal curve. Finally, DFT pore-size distributions confirm samples as mesoporous materials. The samples other than 15 wt%-SrTiO3/Bi2WO6 have a dominate pore size of ca. 3 nm and 4.6 nm. The amount variation tendency of both pores coincides with those of SBET and Ad for the composites.
 |
| Fig. 7 BET specific surface areas (SBET), N2 adsorption–desorption curves (the red line) and DFT pore-size distributions (the black line) of (a) Bi2WO6, (b) 1 wt%-SrTiO3/Bi2WO6, (c) 8 wt%-SrTiO3/Bi2WO6, (d) 10 wt%-SrTiO3/Bi2WO6 (e) 15 wt%-SrTiO3/Bi2WO6 and (f) SrTiO3. | |
 |
| Fig. 8 x-Dependent D, k and Ad over SrTiO3/Bi2WO6 heterojunctions. | |
Besides, adsorption capacity of samples (the amount of adsorbed Rh B in the dark on the surface of the as-prepared samples) is calculated according to the formula Ad = (1 − Ce/C0) × 100%, where Ad, C0 and Ce stand for adsorption capacity of the as-prepared samples, the concentration of original Rh B solution (30 mg L−1) and Rh B equilibrium concentration in dark. Thus, Ad values of samples are obtained and summarized in Fig. 8. Markedly, with regard to the composites, Ad is on the rise to 8.91% (x ≤ 8 wt%) and then decrease to 5.53% (x > 8 wt%), which varies well with SBET (Fig. 7).
3.7. Evaluation of photocatalytic performance
Rh B works as a model contaminant to test photocatalytic activity of as-prepared samples. Fig. 8 displays the effect of x on D, k and Ad. Evidently, the augmented D and k are coincident with increased x up to 8 wt%. Inversely, exorbitant x (8–15 wt%) results in reduced D and k. To conclude, 8 wt%-SrTiO3/Bi2WO6 (D = 98.4% and k = 0.0463 min−1) is much more photocatalytically active than Bi2WO6 (x = 0, D = 86.0%, k = 0.0218 min−1), which derives mainly from perfective separation route of electrons and holes through the interfaces between SrTiO3 and Bi2WO6 as disclosed by highly quenched PL intensity (Fig. 6a), which is in line with the literature results.7,52
Moreover, the sample offers catalytic superiority over any other composite. One of the reasons is possibly associated with best separation efficiency of excitons as PL analysis indicates (Section 3.5). For another, the suitable SBET (Fig. 7) and optical absorption (Fig. 5a) favor Rh B adsorption and activation.
Controlled experiments are crucial for knowledge of the photocatalytic process. As a result, these experiments were conducted (Table 1). Remarkably, 8 wt%-SrTiO3/Bi2WO6 far surpasses plain SrTiO3 and Degussa P25 (Table 1, Title 2 and 3) with reference to light-driven catalytic behavior in virtue of overwhelming advantage of optical response and excitonic splitting. Blank tests (Table 1, Title 4–6) evidence that Rh B photodegradation is certainly a light-stimulated catalytic process rather than a thermal-induced catalytic or self-degradation one.
Table 1 Controlled experiments
Title |
Samples |
Da/% |
Under the condition described in Experimental section. In dark during the whole process. |
1 |
8 wt%-SrTiO3/Bi2WO6 |
98.4 |
2 |
SrTiO3 |
38.1 |
3 |
Degussa P25 |
17.5 |
4 |
None |
0 |
5 |
8 wt%-SrTiO3/Bi2WO6 |
16.3b |
6 |
None |
0b |
3.8. Photostability exploration
Photostability is a considerably critical attribute for an excellent semiconductor material. Therefore, related tests were performed (Fig. 9). Obviously, 8 wt%-SrTiO3/Bi2WO6 maintains chemically (Fig. 9a) and structurally (Fig. 9b) durable after used 4 times. In a word, it is beyond doubt that it deserves an outstanding promoter for the excellent stability toward the sunlight.
 |
| Fig. 9 (a) Reuse of 8 wt%-SrTiO3/Bi2WO6 and (b) XRD patterns of fresh and 4th cyclical 8 wt%-SrTiO3/Bi2WO6. | |
3.9. Reaction mechanism
It is well-constructed that identification of primary reactive species in the degradation process enables proposal of reaction mechanism. Thereby, the reactive species trapping experiments were conducted. Ethylene diamine tetra acetic acid (EDTA), isopropanol (IPA) and benzoquinone (BQ) featured as scavengers for hole (h+), hydroxyl radical (OH·) and superoxide radical (·O2−), respectively.53–55 Fig. 10 definitely elucidates the considerably diminished D of 8 wt%-SrTiO3/Bi2WO6 in the presence of EDTA or IPA, circumstantiating h+ and OH· as the main species. Conversely, ·O2− plays minor role in Rh B removal.
 |
| Fig. 10 Various D values of 8 wt%-SrTiO3/Bi2WO6 after introduction of several scavengers. | |
On the other hand, the matched band structures are required for two semiconductors intended for highly efficient assembly of a hybrid. The valence band (VB) and conduction band (CB) potentials can be calculated from the two equations below:56–59
|
EVB = X − Ee + 0.5Eg
| (11) |
where
X represents the absolute electronegativity of semiconductor (
X = 6.36 for Bi
2WO
6 (
ref. 60) and 5.19 for SrTiO
3 (
ref. 37)), which means the atomic electron affinity and the first ionization energy;
Ee is the energy of free electrons on the hydrogen scale (4.5 eV). Accordingly,
ECB and
EVB are respectively calculated to be 0.42 and 3.30 eV for Bi
2WO
6 and −0.83 and 2.22 eV for SrTiO
3.
On basis of the aforementioned discussion, a rational route for migration, isolation and capture of excitons since their birth is put forward as illustrated in Fig. 11. Under simulated sunlight, both Bi2WO6 and SrTiO3 are excited to give birth to elections and holes. Subsequently, they are forced respectively to accumulate in the CB of Bi2WO6 and VB of SrTiO3 due to the potential differences between their CBs (−0.83 and 0.42 eV) and VBs (2.22 and 3.30 eV), leaving their recombination suppressed and their lifetime lengthened as PL results indicate (Fig. 6). Thus, more excitons are allowed to run the photocatalytic reaction, which is mainly responsible for enhanced catalytic function. Next, elections are captured by chemisorbed O2 to convert to OH· by way of ·O2−.61,62 However, holes hardly combine with OH− to form OH· as a result of less positive potential in VB of SrTiO3 (2.22 eV) compared with that of ·OH/OH− (2.38 eV). Therefore, Rh B is transformed to its degradation products mostly via its oxidation by OH· and h+.
 |
| Fig. 11 Reaction mechanism of Rh B removal over 8 wt%-SrTiO3/Bi2WO6 under simulated sunlight. | |
4. Conclusion
SrTiO3/Bi2WO6 composites were prepared via a technically viable two-step hydrothermal method and submitted to structural exploration by means of XRD, TEM, SEM, XPS, DRS, BET and PL. The heterostructure between SrTiO3 and Bi2WO6 is well-constructed and plays the main part in raised photocatalytic behavior in Rh B removal. 8 wt%-SrTiO3/Bi2WO6 is selected as the optimal catalyst (D = 98.4% and k = 0.0463 min−1) among as-prepared samples by perfecting the SrTiO3 loading and optical and electric properties. h+ and OH· as the main species are beyond dispute. Based on the discussion above, a possible reaction was proposed.
Acknowledgements
This work was financially supported by the Fundamental Research Funds for the Central Universities of China (No. 3207045403 and 3207045409), National Natural Science Foundation of China (No. 21576050), Jiangsu Provincial Natural Science Foundation of China (BK20150604) and a Project Funded by the Priority Academic Program Development of Jiangsu Higher Education Institutions (PAPD).
Notes and references
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Footnote |
† These authors contributed equally to this work. |
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