DOI:
10.1039/D4NJ03048F
(Paper)
New J. Chem., 2024, Advance Article
Highly efficient g-C3N4 catalysts derived from various precursors for aflatoxin B1 degradation under visible light
Received
5th July 2024
, Accepted 30th August 2024
First published on 2nd September 2024
Abstract
Aflatoxin B1 (AFB1), a mycotoxin commonly found in foodstuffs, poses significant health risks when ingested through contaminated food sources. Therefore, it is imperative to devise a safe and efficient method for AFB1 degradation. Graphitic carbon nitride (g-C3N4) stands out as an exceptionally stable, non-toxic, and economical photocatalyst, which is widely used in photocatalysis. In this study, we explored the photocatalytic performance of four g-C3N4 catalysts derived from different precursors (dicyandiamide (D-CN), melamine (M-CN), thiourea (T-CN), and urea (U-CN)) in AFB1 degradation under visible light. Notably, the U-CN catalyst displayed an impressive degradation rate of 93.5% for AFB1 within 30 min, outperforming M-CN (82.5%), T-CN (78.5%), and D-CN (46.2%). This superior performance is attributed to its inherent porous structure, enlarged specific surface area, and reduced electron–hole pairs’ recombination rate. Additionally, our investigation identified ˙O2− as the primary active species in AFB1 degradation. Furthermore, we explored the degradation pathway of AFB1 and its associated inactivation mechanism mediated by the U-CN catalyst. This work provides a theoretical foundation for developing highly efficient photocatalysts in AFB1 degradation.
1 Introduction
Food security is a pivotal issue that must be addressed in the progression of human development. Amid the intricate processes of food production, transportation, and storage, the persistent threat of mycotoxin contamination remains a significant concern. Consuming contaminated food can inflict harmful effects on the human body, and AFB1 stands out as a particularly alarming contaminant among all known mycotoxins.1 AFB1, a highly toxic carcinogen produced by fungi and parasitic molds, has been categorized as a Group 1 carcinogen by the International Agency for Research on Cancer. It possesses formidable biological toxicity and teratogenicity, posing a grave threat to both humans and animals.2 AFB1 can maintain its structural stability under extreme conditions, rendering it difficult for the human body to metabolize or eliminate through the circulatory system.3 Hence, our primary focus lies in discovering a safe and reliable method to degrade AFB1 in food, ensuring food safety and protecting public health.
In recent years, numerous methods have been developed for AFB1 treatment, including UV light irradiation,4 gamma ray radiation,5 ozone treatment,6 and others. Nonetheless, these approaches are often accompanied by substantial drawbacks, including significant energy consumption and suboptimal removal efficiency. In contrast, photocatalytic technology offers a promising solution. This innovative method harnesses the power of sunlight to activate semiconductor materials, generating numerous reactive species that engage in oxidation–reduction reactions with pollutants, effectively breaking down their structure for degradation.7 Photocatalytic technology stands out as a low-energy, recyclable, and environmentally friendly approach commonly employed for the elimination of pollutants in various environments.8
g-C3N4 has garnered considerable attention in photocatalysis for its remarkable attributes, including its simplicity in preparation, cost-effectiveness, and robust thermal stability.9–11 Notably, the photocatalytic activity of g-C3N4 is heavily contingent upon the precursors in its synthesis. The common precursors for the fabrication of g-C3N4 encompass thiourea, melamine, urea, and dicyandiamide. These precursors, owing to their variations in chemical element composition, impart significant disparities in the morphology, structural configuration, and ultimately affect the photocatalytic performance of g-C3N4.11,12 For instance, Shirman et al.13 explored the photocatalytic hydrogen evolution activity of palladium-loaded g-C3N4 derived from distinct precursors, revealing that cyanuric dicyandiamide derived g-C3N4 displayed slightly superior catalytic activity than that of urea derived g-C3N4. Chand et al.12 discovered that urea derived g-C3N4 possessed a higher catalytic activity for carbon dioxide conversion compared to those derived from melamine, thiourea, and dicyandiamide. Jung et al.14 found that cyanuric dicyandiamide derived g-C3N4/ZnO composites achieved the highest methylene blue photodegradation efficiency. Liang et al.15 noted significant differences in the photocatalytic reduction of Cr(VI) using g-C3N4 synthesized from dicyandiamide, urea, melamine, and thiourea, where urea derived g-C3N4 nanosheets emerged as the most efficient catalyst in Cr(VI) reduction. Shao et al.16 found that the presence of trace sulfur in thiourea derived g-C3N4 induced higher asymmetry in its structural units, resulting in the highest activity for piezoelectric reduction of KMnO4. However, there has been a lack of reports exploring the effect of g-C3N4 prepared from varying precursors on the photocatalytic degradation of AFB1.
In this study, urea, melamine, thiourea, and dicyandiamide were used as precursors to synthesize four g-C3N4 catalysts via thermal polymerization approach. The comprehensive discussions of the morphologies, structural integrities, electrochemical properties of these g-C3N4 catalysts were conducted. Their photocatalytic efficiencies were evaluated through AFB1 degradation under visible light. Subsequently, the products generated from the photocatalytic degradation process were subjected to the UHPLC-Q Exactive MS system, thereby inferring potential AFB1 degradation pathways and proposing relevant mechanisms. This study provides valuable insights into the influence of precursors in g-C3N4 synthesis on AFB1 degradation.
2 Experimental sections
2.1 Chemicals
The AFB1 standard was obtained from J&K Scientific. Urea and thiourea were acquired from Guangdong Guanghua Technology Co., Ltd, while melamine and dicyandiamide were purchased from Shanghai Macklin Biochemical Co., Ltd. Analytical-grade isopropyl alcohol (IPA) and 1,4-benzoquinone (BQ, C6H4O2) were provided by Aladdin Biochemical Technology Co. We also procured EDTA-2Na from Tianjin Aopusheng Chemical Co., Ltd. For high-performance liquid chromatography (HPLC) analysis, we utilized HPLC-grade methanol sourced from Thermo Fisher Scientific. Deionized water was used in all experiments.
2.2 Preparation of respective catalysts
The catalysts were synthesized using thermal polymerization method. Specifically, a precise amount of precursor, including urea, melamine, thiourea, or dicyandiamide, was transferred into a ceramic crucible and then positioned in a muffle furnace. The temperature was gradually raised to 550 °C and held constant for 4 h in air. After cooling down to room temperature, the sample was collected and ground thoroughly to obtain g-C3N4. The g-C3N4 derived from urea, melamine, thiourea, and dicyandiamide were designated as U-CN, M-CN, T-CN, and D-CN, respectively.
2.3 Characterizations
To analyze the crystal phases of the catalysts, X-ray diffraction (XRD, Bruker D8-Advance, Germany) was employed. The morphology and particle size of the catalysts were characterized using field emission scanning electron microscopy (FESEM, SU8010, Hitachi, Japan) and transmission electron microscopy (TEM, JEM 2100F). Additionally, elemental analysis was conducted via X-ray photoelectron spectroscopy (XPS, EscaLab-250Xi, USA). The specific surface area and pore size of the catalysts were determined using the Brunauer–Emmett–Teller (BET) system (BET, Bei-Shi-De 3H-2000PS2, Beijing). To investigate the light absorption property of the catalysts, UV-Vis diffuse reflectance spectroscopy (UV-Vis DRS, UV-3600Plus, Shimadzu, Japan) was utilized. The photoluminescence (PL) spectrum (λex of g-C3N4 is 380 nm) of the catalysts was recorded using a fluorescence spectrophotometer (F-4600, Hitachi, Japan). Electron paramagnetic resonance (EPR) tests were conducted on a Bruker EPR EMXplus spectrometer (Bruker, Germany) with DMPO as the spin-trapping agent. Furthermore, the identification and confirmation of degradation products were carried out using a Thermo UltiMate 3000 UHPLC-Q mass spectrometry system (Thermo Fisher Scientific, Waltham, MA, USA).
2.4 Photocatalytic measurement
Using a 300 W Xe lamp coupled with a cut-off filter (λ ≥ 420 nm, PLS-SXE 300, Beijing PerfectLight Co. Ltd., China), the photocatalytic degradation efficacy of an AFB1 aqueous solution (100 mL, 1 μg mL−1) by 2 mg of catalysts was evaluated. Before irradiation, the mixture solution was stirred in darkness for 30 min to attain adsorption–desorption equilibrium. During irradiation, 50 μL of the supernatant were withdrawn every 5 min and diluted to 4 mL using 70% HPLC-grade methanol. This photocatalytic irradiation process spanned 30 min. Analysis was conducted using a high-performance liquid chromatography system (Beijing Mingnike P2000), equipped with a C18 column (254 mm × 4.6 mm × 5 mm, Leena) and a UV-visible detector. The HPLC conditions were set as follows: A mobile phase consisting of 70% methanol in water, a flow rate of 1.0 mL min−1, and a detection wavelength of 365 nm. The AFB1 removal efficiency (Y) was determined utilizing the following equation:
Y = (1 − CtVt/C0V0) × 100% |
In this equation, C0 (μg mL−1) and V0 (mL) represent the initial AFB1 concentration and volume, respectively. Ct (μg mL−1) and Vt (mL) correspond to the AFB1 concentration and volume after the degradation process.
2.5 Electrochemical measurements
In the CHI660E electrochemical system (CH Instruments Ins.), a three-electrode cell configuration is employed, consisting of an Ag/AgCl reference electrode and a Pt counter electrode. In addition, a 300 W Xe lamp (λ > 400 nm) was used as the light source. The working electrode is prepared as follows: Firstly, 4 mg of the samples is dispersed in 4 mL of ethanol with ultrasonication for 2 h to obtain a homogeneous solution. Subsequently, 50 μL of the above solution is pipetted onto an ITO glass substrate (1.0 cm × 1.5 cm), and this process is repeated three times after each drying cycle. Finally, transient photocurrent response measurements and electrochemical impedance spectroscopy (EIS) are conducted using 0.5 M Na2SO4 solution as the electrolyte.
2.6 Photocatalytic stability test
Utilizing U-CN samples which exhibited the optimal photocatalytic performance for stability testing. We conducted four consecutive cycles of photocatalytic degradation experiments on AFB1 by U-CN catalysts. For each cycle, 100 mL of AFB1 solution (1 μg mL−1) was used. After 30 min of photocatalytic reaction, the U-CN catalysts were retrieved and alternately rinsed with deionized water and ethanol. The U-CN catalysts were then dried at 60 °C for subsequent reuse. This process was repeated until four cycles of photocatalytic degradation experiments were completed.
3 Results and discussion
3.1 XRD analysis and FT-IR analysis
The XRD patterns present in Fig. 1(a) carefully illustrate the diffraction peaks of U-CN, M-CN, T-CN, and D-CN, revealing their respective crystallinities and structural characteristics. These XRD patterns reveal that all g-C3N4 samples exhibited two remarkably distinct characteristic peaks at 12.8° and 27.4°, precisely aligning with the standard card of g-C3N4. Notably, the diffraction peak situated near 12.8° is attributed to the intralayer long-range atomic order, stemming from the hydrogen bonding present in g-C3N4.17 Conversely, the pronounced peak observed around 27.4° corresponds to the interlayer periodic stacking along the c-axis, which is induced by the stacking of conjugated aromatic systems within g-C3N4.18,19 FT-IR analysis was employed to identify the functional groups present in U-CN, M-CN, T-CN, and D-CN. As depicted in Fig. 1(b), the samples derived from four precursors exhibited characteristic FT-IR spectra of g-C3N4. Prominent absorption bands were distinctly observed at 811 cm−1, 1200–1700 cm−1, and 3000–3500 cm−1.16 Specifically, the sharp band near 811 cm−1 corresponds to the stretching vibrations of the distinctive tri-s-triazine units within the g-C3N4 structure.15,20 The absorption peaks spanning around 1200–1700 cm−1 are attributed to the presence of C–N and CN bonds in the aromatic nitrogen–carbon heterocycles.21 Furthermore, the distinctive absorption peaks between 3000–3500 cm−1 originate from the stretching vibrations of –OH and –NH groups,22 which can be partially attributed to uncondensed amine groups and water molecules adsorbed on the surface of the catalysts.23 In summary, Fig. 1 confirmed that g-C3N4 samples derived from different precursors were successfully prepared.
|
| Fig. 1 (a) XRD patterns and (b) FT-IR spectra of U-CN, M-CN, T-CN, and D-CN. | |
3.2 Morphological structures
As depicted in Fig. 2, FESEM was utilized to analyze the morphological structures of four g-C3N4 samples derived from various precursors. In Fig. 2(a), U-CN exhibits a loose mesh-like structure, featuring irregular pore sizes, potentially enhancing its specific surface area. Meanwhile, M-CN presents a large, blocky sheet structure with a relatively smooth surface (Fig. 2(b)). T-CN displays a layered structure adorned with numerous particles of varying sizes scattered across its surface (Fig. 2(c)). D-CN shows a flattened layered structure with a reduced number and size of particles on its surface (Fig. 2(d)). The TEM result in Fig. 2(e) further reveals a loose mesh-like configuration of U-CN, comprising numerous overlapping nanosheets of varying sizes and curvature.
|
| Fig. 2 FESEM images of (a) U-CN (b) M-CN (c) T-CN (d) D-CN, (e) TEM image of U-CN. | |
3.3 XPS analysis
The XPS analysis of U-CN, M-CN, T-CN, and D-CN provides their oxidation states and surface chemical composition. As depicted in Fig. 3(a), the XPS survey spectra reveal that the as-synthesized g-C3N4 samples primarily consist of C, N, and O elements. Notably, the O elements can be attributed to the adsorption of H2O on the catalysts’ surface.24 The high-resolution of C 1s XPS spectrum reveals two distinct peaks centered at 288.2 eV and 284.8 eV (Fig. 3(b)). The peak at 288.2 eV corresponds to the sp2 N–CN bond, which is indicative of the graphitic carbon nitride structure. In contrast, the peak at 284.8 eV represents the C–C bond, potentially originating from adventitious carbon contamination.25 Moreover, Fig. 3(c) displays the N 1s XPS spectra of the four g-C3N4 samples. All four samples exhibit peaks located at 404.2 eV, 401.3 eV, 400.2 eV, and 398.7 eV. These peaks correspond to π excitation,26 –NH2, tertiary nitrogen N–(C)3, and C–NC bonds,25 respectively, providing a comprehensive understanding of the nitrogen bonding configurations within the g-C3N4 samples. The C 1s and N 1s peaks of U-CN exhibit significant deviations relative to those of M-CN, T-CN, and D-CN, aligning with the findings of XRD analysis. XRD and XPS results confirm that U-CN possesses a lower crystallinity, which in turn affects its electron energy level distribution, ultimately leading to the observed peak shifts.27
|
| Fig. 3 The XPS (a) survey spectra and high-resolution spectra of (b) N 1s, (c) C 1s. | |
3.4 BET analysis
In order to gain a profound comprehension of the specific surface area and pore architecture of four g-C3N4 samples, N2 adsorption–desorption isotherms and pore size distributions were carefully assessed. As illustrated in Fig. 4(a), the N2 adsorption–desorption isotherms for four g-C3N4 samples exhibit characteristic H3 hysteresis loops, signifying a type IV isotherm pattern.28 Fig. 4(b) reveals that all the samples possess mesoporous structures.29 In Table 1, U-CN stands out with a remarkable specific surface area of 100.5 m2 g−1 and pore volume of 0.7998 cm3 g−1 compared to the other samples. This enhancement can be attributed to the pyrolysis process of urea, during which a self-sustaining atmosphere is created by the liberation of significant amounts of pyrolysis gases, including NH3, H2O, and CO2. These gases function as soft templates, facilitating the development of a porous structure that enhances the specific surface area and contributes to the formation of a more elaborate porous architecture.30 Fundamentally, a larger specific surface area often correlates with an increased number of reactive sites, which is favourable for photocatalytic degradation.
|
| Fig. 4 (a) N2 adsorption–desorption isotherms and (b) BJH pore size distribution curves of U-CN, M-CN, T-CN, and D-CN. | |
Table 1 Physical properties of U-CN, M-CN, T-CN, and D-CN
Sample |
Specific surface area (m2 g−1) |
Pore size (nm) |
Total pore volume (cm3 g−1) |
U-CN |
100.5 |
31.8 |
0.7998 |
M-CN |
20.1 |
30.4 |
0.1526 |
T-CN |
25.2 |
39.0 |
0.2452 |
D-CN |
12.8 |
32.9 |
0.1054 |
3.5 UV-vis DRS analysis
To investigate the optical properties of U-CN, M-CN, T-CN, and D-CN, their UV-vis DRS absorptions were measured. As depicted in Fig. 5(a), the UV-vis DRS absorption spectra reveal that all g-C3N4 samples can exhibit visible light response. Fig. 5(b) further illustrates the corresponding band gaps of respective samples. g-C3N4 is direct semiconductor, and its band gap can be calculated via the Kubelka–Munk equation31: αhν = A(hν − Eg)n/2. Where h represents the Planck constant, ν is the photon frequency, A is the proportionality constant, α is the photopic absorption coefficient, and Eg denotes the band gap. Therefore, the band gap for U-CN, M-CN, T-CN, and D-CN was determined to be 2.72 eV, 2.60 eV, 2.54 eV, and 2.47 eV, respectively. Notably, U-CN exhibited a larger band gap compared to the other g-C3N4 samples, potentially attributed to quantum size effects.32
|
| Fig. 5 (a) UV-vis DRS spectra and (b) (αhν)1/2 vs. hν plots of U-CN, M-CN, T-CN, and D-CN. | |
3.6 MS and PL analysis
The photocatalytic activity of semiconductors is intricately linked to their light harvesting capabilities and band gap characteristics. Consequently, we also examined the Mott–Schottky (MS) curves of U-CN, M-CN, T-CN, and D-CN. As evident in Fig. 6(a), the positive slope of the MS curves for all samples suggests that the g-C3N4 samples derived from different precursors are n-type semiconductors.33,34 The flat band potential (Efb) of U-CN, M-CN, T-CN, and D-CN is −0.65 V, −0.58 V, −0.46 V, and −0.62 V (vs. Ag/AgCl), respectively. Upon reviewing the reported XPS VB spectra of g-C3N4, we can deduce that the VB-Ef potentials for U-CN, M-CN, T-CN, and D-CN are 2.28 eV, 2.22 eV, 2.32 eV, and 2.22 eV,15 respectively. Employing the established methodologies,33,35 we have calculated the valence band (VB) position for these materials, which is 1.63 V for U-CN, 1.64 V for M-CN, 1.86 V for T-CN, and 1.60 V for D-CN. Furthermore, by combining the calculated band gaps with the empirical formula: EVB = ECB + Eg, we determined the conduction band (CB) position of U-CN, M-CN, T-CN, and D-CN to be −1.09 V, −0.96 V, −0.68 V, and −0.87 V, respectively.
|
| Fig. 6 (a) Mott–Schottky (MS) curves and (b) PL spectra of U-CN, M-CN, T-CN, and D-CN. | |
The electron–hole separation efficiency in U-CN, M-CN, T-CN, and D-CN samples was thoroughly analyzed via photoluminescence spectroscopy. As depicted in Fig. 6(b), the PL emission peak's intensity at 470 nm follows the sequence of D-CN > M-CN > T-CN > U-CN for the g-C3N4 samples derived from respective precursors. Conventionally, a lower PL intensity signifies a higher efficiency in charge carrier separation and a reduced recombination rate, thereby indicating superior photocatalytic activity of the catalyst.32,36 Notably, U-CN exhibits a lower fluorescence intensity, which can be attributed to its loose mesh-like structure compared to M-CN, T-CN, and D-CN. The loose mesh-like structure facilitates the rapid transfer of electrons to the catalyst surface and accelerates the separation of photogenerated carriers.
3.7 Electrochemical results
As depicted in Fig. 7(a), all g-C3N4 catalysts exhibit commendable photocurrent responses, with U-CN showing the highest photocurrent. Notably, U-CN displays the most robust photocurrent response, signifying its exceptional photogenerated carriers’ separation efficiency,37 which aligns with the PL results. In Fig. 7(b), the radius's trend of the EIS Nyquist curves for four g-C3N4 samples is as follows: U-CN < M-CN < T-CN < D-CN. Conventionally, a smaller Nyquist curve radius indicates a lower charge transfer resistance in the catalysts, favoring enhanced charge mobility and consequently pointing to a superior separation efficiency of photogenerated carriers.32,37 These findings further reinforce that U-CN possesses the highest electron–hole pair separation efficiency, which can effectively enhance its photocatalytic degradation performance.
|
| Fig. 7 (a) Transient photocurrent response and (b) electrochemical impedance spectroscopy (EIS) of U-CN, M-CN, T-CN, and D-CN. | |
3.8 Photocatalytic performance
The photocatalytic degradation of AFB1 was conducted utilizing U-CN, M-CN, T-CN, and D-CN as catalysts. Given the remarkable stability of AFB1 in aqueous solutions, its concentration remains largely unchanged under visible light irradiation.38,39 As depicted in Fig. 8(a), the photocatalytic degradation efficiency of AFB1 by various g-C3N4 follows the order of U-CN > M-CN > T-CN > D-CN. Notably, U-CN emerges as the most effective catalyst with a remarkable AFB1 removal rate of 93.5% for 100 mL of AFB1 (1 μg mL−1) within 30 min, significantly outperforming M-CN (82.5%), T-CN (78.5%), and D-CN (46.2%). This outstanding photocatalytic performance of U-CN aligns perfectly with the findings from transient photocurrent response, EIS, and PL analysis, confirming its superior efficiency in electron–hole pairs’ separation. Additionally, upon reaching adsorption–desorption equilibrium in darkness, the AFB1 concentration in the U-CN suspension is notably lower than that of the other three samples, due to U-CN's largest specific surface area and higher density of active adsorption sites for the substrate. In general, the AFB1 removal by all g-C3N4 samples is mainly due to photocatalytic degradation. To further analyze the degradation kinetics, the kinetic equation ln(Ct/C0) = kt was applied. Where Ct (mg L−1) represents the AFB1 concentration at time t, C0 (mg L−1) is the initial AFB1 concentration, and k (min−1) is the first-order rate constant. As presented in Fig. 8(b) and Table 2, the photocatalytic degradation processes of U-CN, M-CN, T-CN, D-CN samples adhere to a pseudo-first-order kinetic model, and sample U-CN has the largest k value of 0.08856 min−1.
|
| Fig. 8 (a) The photocatalytic degradation rates and (b) the corresponding first-order kinetics of AFB1 by U-CN, M-CN, T-CN, and D-CN. | |
Table 2 k value and R2 of respective samples
Sample |
R2 |
k (min−1) |
U-CN |
0.99747 |
0.08856 |
M-CN |
0.99759 |
0.02824 |
T-CN |
0.99335 |
0.02199 |
D-CN |
0.98190 |
0.00769 |
We delved deeper into the characteristics of U-CN, which exhibits the highest photocatalytic efficiency, examining the mass of U-CN on the photocatalytic degradation of AFB1 (Fig. 9(a)) and the effect of distinct pH values on the degradation rate of AFB1 by U-CN (Fig. 9(c)). Notably, an increase in the mass of U-CN catalyst led to a continuous enhancement in the degradation rate of AFB1. This enhancement can be attributed to the provision of more active reaction sites as the catalyst concentration rises.40 However, after surpassing a catalyst mass of 2 mg, further increments in catalyst's concentration yield diminishing returns in terms of enhancing the degradation rate. This is likely due to the fact that an excessive amount of catalyst may hinder the utilization of visible light and mass transfer during the photocatalytic degradation process.41 Additionally, changing the pH of the solution has a substantial impact on the AFB1 degradation. Since the lactone ring of AFB1 molecules is prone to disruption in alkaline solutions, alkaline conditions were not considered in this study.42 Instead, we focused on the impact of pH values ranging from 3 to 7.43 Under these conditions, the degradation rate of AFB1 by U-CN follows this order: pH = 7 > pH = 5 > pH = 3. This trend can be explained by the fact that under acidic conditions, more H+ ions tend to eliminate ˙OH radicals.44 Their kinetics of photocatalytic reactions both align with a pseudo-first-order kinetic model (Fig. 9(b) and (d)), indicating a consistent relationship between reaction rate and reactant concentration.
|
| Fig. 9 (a) Photocatalytic degradation rate of AFB1 with different masses of U-CN and their (b) first-order kinetics, (c) photocatalytic degradation rate of AFB1 by U-CN under different pH conditions and their (d) first-order kinetics. | |
3.9 Photocatalytic stability test
To evaluate the photostability and reusability of U-CN for AFB1 degradation, this study undertook four consecutive cycles of photocatalytic degradation. Notably, U-CN catalyst sustained a commendable degradation efficiency towards AFB1 after four cycles (Fig. 10(a)), with even the fourth cycle achieving a degradation rate of 85% within 30 min. The slight decline in degradation efficiency throughout the cycling experiments can be attributed to two factors. Firstly, the main reason is that the amount of catalyst (2 mg) is too small, which makes it difficult to recover after the photocatalytic reaction, resulting in a decrease in degradation efficiency. Secondly, the catalyst becomes contaminated by the intermediate products generated during the AFB1 degradation process.45 Upon scrutinizing the FT-IR spectra before and after the cycling experiments (Fig. 10(b)), it is evident that the structure of U-CN remains intact after four cycles. This is evident from the absence of notable shifts or variations in the absorption peaks at 811 cm−1 and within the range of 1200–1700 cm−1. Nonetheless, an increase in the intensity of the absorption peak at 3200–3500 cm−1 is discernible, which can be attributed to the adsorption of intermediates generated during the AFB1 degradation process onto the surface of the catalyst. This observation is consistent with the subsequent SEM findings. A comparative analysis of the SEM images before and after four cycles reveals that U-CN's morphology remained largely unchanged (Fig. 10(c) and (d)), indicating that sample U-CN has a good photostability and reusability. However, a notable presence of new granular substances is observed, which can be attributed to the adsorption of AFB1 intermediates onto the surface of U-CN. As can be seen from Table 3, the U-CN catalyst has high efficiency for AFB1 degradation compared to other reported g-C3N4-based catalysts. It means that the U-CN catalyst can effectively solve the actual AFB1 contamination problem.
|
| Fig. 10 (a) Photocatalytic degradation rate of AFB1 by U-CN over four cycles, (b) FT-IR results, and SEM images of U-CN (c) before and (d) after four cycles. | |
Table 3 Related reported of photodegradation aflatoxin
Pollutant |
CAFB1 |
VAFB1 |
Catalyst |
Source |
Time |
Degradation rete (%) |
Ref. |
AFB1 |
0.5 μg mL−1 |
100 mL |
g-C3N4 (0.1 mg mL−1) |
Xe lamp 500 W, λ ≥ 400 nm |
120 min |
70.20 |
46 |
AFB1 |
0.54 μg mL−1 |
100 mL |
WO3/RGO/g-C3N4 (0.1 mg mL−1) |
Xe lamp 300 W, λ ≥ 400 nm |
120 min |
92.40 |
47 |
AFB1/AFB2/AFG1/AFG2 |
315.21 μg kg−1 |
|
g-C3N4/NiFe2O4 (2 mg mL−1) |
Xe lamp 300 W, λ ≥ 420 nm |
90 min |
94.10 |
48 |
AFB1 |
0.5 μg mL−1 |
50 mL |
PCL-g-C3N4/CQDs (1 mg mL−1) |
Xe lamp 300 W, λ ≥ 420 nm |
30 min |
96.90 |
49 |
AFB1 |
0.5 μg mL−1 |
50 mL |
PAN-g-C3N4/MoS2 (0.5 mg mL−1) |
Xe lamp 300 W, λ ≥ 420 nm |
60 min |
97.0 |
50 |
AFB1 |
1.0 μg mL−1 |
100 mL |
U-CN (0.02 mg mL−1) |
Xe lamp 300 W, λ ≥ 420 nm |
30 min |
93.5 |
This work |
3.10 Exploring the photocatalytic degradation mechanism
In this study, scavenging experiments were conducted separately for superoxide anion radicals (˙O2−), photogenerated holes (h+), and hydroxyl radicals (˙OH) by introducing 1 mM of benzoquinone (BQ), ethylenediaminetetraacetic acid disodium salt (EDTA-2Na), and isopropanol (IPA). After the addition of BQ, IPA, and EDTA-2Na, the degradation efficiency of AFB1 by U-CN decreased from 93.5% to 56.0%, 78.2%, and 83.2% (Fig. 11(a)), respectively. This indicates that these three types of radicals play a significant role in influencing the photocatalytic performance of U-CN, and ˙O2− is identified as the primary reactive species. This phenomenon may be caused by the fact that the ECB of U-CN is more negative than that of Eθ(O2/˙O2−), which makes it easy for U-CN to generate a large amount of ˙O2−. Under visible light irradiation, U-CN tends to generate electrons (e−) in the CB and generate h+ in the VB. Subsequently, e− in the CB react with O2 to form ˙O2−. It is noteworthy that despite the lower EVB position of U-CN compared to Eθ(˙OH/H2O), precluding direct ˙OH generation on its VB, the degradation efficiency of U-CN significantly decreases upon IPA addition for ˙OH scavenging. This indicates an indirect reaction between ˙O2− and H2O2 may generate a finite amount of ˙OH during U-CN photocatalysis, as reported previously (O2 + e− → ˙O2−, ˙O2− + e− + 2H+ → H2O2, H2O2 + e− → ˙OH + OH−).45,51 These active species then undergo oxidation–reduction reactions with AFB1, ultimately achieving the photocatalytic degradation of AFB1. This process can be succinctly summarized as:
g-C3N4 + hν → g-C3N4 (e− + h+) |
AFB1 + ˙O2− (or h+ or ˙OH) → small molecules |
|
| Fig. 11 (a) Effects of different scavengers on the degradation of AFB1 by U-CN and (b) and (c) ESR spectra of U-CN. | |
Utilizing 5,5-dimethyl-1-pyrroline N-oxide (DMPO) as a trapping agent, ESR analysis identified the presence of ˙O2− and ˙OH during photocatalytic reactions52,53 (Fig. 11(b) and (c)). Notably, no ESR signal was detected in the absence of light, suggesting that U-CN did not generate ˙O2− in dark conditions. However, a significant ESR signal emerged upon exposure to visible light irradiation, indicating the generation of ˙O2− during the photocatalytic process. Similarly, the ESR analysis also revealed the characteristic peak of the ˙OH signal generated by U-CN under visible light irradiation. These results confirmed that the active species of the ˙OH and ˙O2− can be generated during the photocatalytic process.
To further elucidate the degradation mechanism of AFB1 by U-CN, UHPLC-MS analysis was performed. After visible light irradiation, eight intermediate products are identified (Fig. 12(a)–(d)), including C17H18O7 (m/z = 334.11), C14H12O6 (m/z = 276.06), C16H10O6 (m/z = 298.05), C16H12O5 (m/z = 284.07), C14H8O4 (m/z = 240.04), C11H10O3 (m/z = 190.06), C11H12O2 (m/z = 176.08), and C5H6O (m/z = 82.04). Previous researches have highlighted that the toxicity and carcinogenicity of AFB1 primarily originate from its double bonds in the furan and lactone rings.54,55 In general, ˙OH addition reactions tend to occur on unsaturated carbon bonds.56 Consequently, the initial degradation product, C17H18O7, likely forms through addition reactions involving the C8C9 double bond in AFB1's furan ring, as well as reactions with the lactone ring and cyclopentenone group. Upon visible light irradiation, C17H18O7 undergoes ROS reactions and transform into C14H12O6. Another possible degradation pathway involves ˙OH addition reactions on various unsaturated carbon bonds in AFB1, particularly those located at C8C9, owing to the strong conjugated π bonds present at C9bC9c, C5aC5, C4C3b, and C3aC11a.37 This pathway leads to the formation of non-toxic or mildly toxic small molecules through a series of reactions, ultimately contributing to the degradation of AFB1 (Fig. 12(e)). Based on the above analysis, the possible photocatalytic mechanism of AFB1 via U-CN under visible light can be observed in Fig. 12(f).
|
| Fig. 12 (a)–(d) UHPLC-MS spectra of AFB1 degradation products, (e) possible pathway of U-CN degraded AFB1, and (f) possible photocatalytic mechanism of AFB1 via U-CN. | |
4 Conclusion
In summary, this study investigates the synthesis of four distinct g-C3N4 morphologies employing urea, melamine, thiourea, and dicyandiamide as precursors. Furthermore, the photocatalytic properties of these g-C3N4 catalysts, derived from varied precursors, were rigorously evaluated during the AFB1 degradation under visible light. Notably, the g-C3N4 catalyst (U-CN) derived from urea exhibited a remarkable photocatalytic degradation rate (93.5%) of AFB1 within 30 min, which was attributed to its porous structure, large surface area, and reduced electron–hole pairs’ recombination rate. Furthermore, its consistent performance over four consecutive cycles validates that U-CN catalyst has a good photocatalytic stability. We also provided a potential deactivation pathway for AFB1 degradation by U-CN catalyst. This study underscores the critical role of precursor choice in enhancing the photocatalytic property of g-C3N4, thereby laying a theoretical foundation and technological groundwork for designing highly efficient photocatalysts in AFB1 degradation.
Data availability
The data that support the findings of this study are available from the corresponding author upon reasonable request.
Conflicts of interest
There are no conflicts of interest to declare.
Acknowledgements
This work was supported by the National Natural Science Foundation of China (22262025, 21862004, U23A2089), Science and Technology Program of Market Supervision Administration of Guangxi Zhuang Autonomous Region (GXSJKJ2024-13), Scientific Research Foundation for Doctor, Nanning Normal University (No. 602021239253), and BAGUI Scholar Program of Guangxi Province of China. The financial support was gratefully appreciated.
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