To improve the separation efficiency of photo-generated charge carriers, we first introduce the rGO onto substrate g-C₃N₄ to form n% GCN composite. After the optimization of rGO introduction on the substrate g-C₃N₄, the electron mediator nZVI was then introduced to form n% IGCN composite.

The substrate g-C₃N₄, which is named MCB_0.07, was prepared by melamine (2 g), cyanuric acid (1.93 g), and barbituric acid (0.07 g) according to our previous study (Zheng et al., 2016). Then, the rGO was introduced on the basis of MCB_0.07 (n% GCN, n stood for the mass ratio of graphene oxide (GO) to melamine). Melamine (2 g), cyanuric acid (1.93 g), barbituric acid (0.07 g) and a certain volume of GO dispersion liquid were added into the anhydrous ethanol of 40 ml. The powder was first stirred for 3 h (500 r/min) at 25°C, then ultrasonic treatment for 3 h, and finally dried in 70°C oven to obtain gray-white powder without liquid. The gray-white powder was then transferred into a covered alumina crucible and calcined in a muffle furnace at 550°C for 4 h with a heating rate of 2.3°^°C/min. After natural cooling, the obtained solid is grounded into powder, which was denoted as n% GCN. In order to prove that GO was thermally reduced to rGO at high temperatures, the GO dispersion was dried in an oven at 70°C, and heated in a muffle furnace at 550°C for 4 h with a heating rate of 2.3°^°C/min.

The nZVI modification was introduced on the basis of 7.5% GCN (n% IGCN, n was the mass ratio of nZVI and n% GCN) by a facile ultrasonication-assisted chemisorption method. All n% IGCN samples were freshly prepared to prevent the oxidation of nZVI. Specifically, a certain amount of 7.5% GCN and nZVI were dispersed in 10 ml of ultrapure water (ultrapure water was under N₂ gas flow in advance) to prepare n% IGCN stock solution. Before the photocatalytic experiment, the n% IGCN stock solution was ultrasonicated for 1 min (KQ-300DE, 60 kHz) to achieve a uniform suspension. The synthesized schematic of the n% IGCN photocatalyst is shown in Figure 1.

The surface micro-morphology of samples was detected by field emission scanning electron microscopy (FE-SEM, Sigma 300, Germany) equipped with energy dispersive X-ray spectroscopy (EDS), and transmission electron microscopy (TEM, JEM-2100, Japan). The specific surface area of the samples was determined at 77 K using a gas adsorption instrument (NOVA-2000e, United States) after vacuum degassing under 300°C for 12 h, then pore structure was calculated. The crystal structures of samples were investigated using an X-ray diffractometer (XRD, Rigaku Dmax-2500, Japan) with Cu-Kα radiation (λ = 1.5406 Å) in the scanning range of 2θ = 5–90°. Fourier transform infrared spectroscopy (FTIR, Nicolet iS5, United States) measurement was carried out to characterize the functional groups in the 400–4,000 cm⁻¹ range, and prepare KBr for use as a blank control group.

The valences and existing forms of the elements on the samples were analyzed using X-ray photoelectron spectroscopy (XPS, EscaLab Xi+, United States) with monochromated Al-Kα radiation (hυ = 1,486.6 eV) as the excitation source, and the binding energy values were calibrated concerning C1s = 284.80 eV. All the binding energies of functional groups were determined according to the NIST XPS Database. All materials were vacuum freeze-drying for 24 h to remove the interference of residual H₂O and prevent the oxidation of some components. The diffuse reflectance spectroscopy (DRS, UV-3600, Japan) was used to further evaluate the optical properties of the catalysts with BaSO₄ as the background level. The detailed calculation method of band gap (Eg) was given in Supplementary Text S1.

Photoluminescence (PL, FLS-980, GBR) spectra were obtained with an excitation wavelength of 345 nm and an emission range between 400 and 650 nm to determine the transport characteristics of charge carriers. The transient photocurrent responses and electrochemical impedance spectroscopy (EIS) were measured with an electrochemical analyzer (CS310H, China). The measurement method was given in Supplementary Text S2.

Photocatalytic degradation experiments were conducted in a photochemical reaction apparatus (66924-1000HX-R1, Newport, United States) with direct research grade arc lamp source equipped with an ozone-free xenon lamp (1000 W) (6295NS, Newport, United States), liquid filter (6213NS, Newport, United States), and a 400 nm filter to filter infrared and UV light out. The reaction temperature was maintained at 25 ± 0.2°C by a circulating water system. The distance between the light source and the liquid surface was 13.5 cm. The intensity of light with a wavelength greater than 400 nm (λ > 400 nm) was 220.3 mW/cm². The photocatalytic reaction was carried out in a 300 ml jacket beaker. The initial concentration of phenol or different antibiotics (OFL, NOR, and CIP) was 10 mg/L, and the pH was maintained at 7.0 by adding phosphate buffer solution (PBS). The photocatalyst loading was 1 g/L, and the solution was magnetically stirred at 500 r/min. The solution and photocatalyst were mixed at dark for 20 min to reach adsorption-desorption equilibrium before the photocatalytic reaction. During the photocatalytic reaction under light irradiation, a certain amount of liquid sample was collected at regular time intervals and stored in a 4°C refrigerator after passing through a 0.22 μm filter membrane for further analysis.

Scavenger tests were employed by quenching selected reactive species generated in the photocatalytic system to study the contribution of a specific reactive species to the degradation of pollutants. The isopropyl alcohol (IPA), L-histidine (L-His), p-Benzoquinone (BQ), catalase, and ethylenediaminetetraacetic acid disodium salt dihydrate (EDTA-2Na) were used to quench the •OH, ¹O₂, •O₂ ⁻, H₂O₂, and h⁺, respectively. The concentration of IPA, L-His, and catalase was 0.1 mol/L, 10 mmol/L, and 1,000 U/mL, respectively. The concentrations of BQ and EDTA-2Na were 4 mmol/L, respectively. The inhibition rate of the scavenger to the reaction is shown in Eq. 1: R = N 0 − N a N 0 (1) Where N₀, N_a is the degradation percentage of pollutants with and without adding scavenger, respectively.

The concentration of phenol was determined by 4-aminoantipyrine spectrophotometry (HJ503-2009). The dissolved organic carbon (DOC) of the solution was determined by total organic carbon analyzer (Vario TOC, Germany). The temperature, pressure, and flow rate of the combustion tube were set at 850 ± 1°C, 1,000 ± 30 Pa, and 180 ± 5 ml/min, respectively. The water sample was tested after passing through a 0.22 μm membrane.

The concentrations of OFL, NOR, and CIP were analyzed using high performance liquid chromatography (HPLC, 1,260 Infinity II, United States) equipped with Venusil MP C18 reversed-phase chromatographic column (4.6 mm × 250 mm × 5 μm). The specific HPLC analysis method of OFL, NOR, and CIP were summarized in Supplementary Table S1.

The fluoride ion concentration was detected by ion chromatography (IC, Dionex ICS-1100, United States) equipped with AS23 (4 nm × 250 nm) column.

The regenerated photocatalysts were collected by using a 0.22 μm membrane, washed with ultrapure water for several times with ultrasonication, and dried at 105°C for 24 h. The regenerated photocatalysts were then used to degrade OFL, NOR, and CIP for multiple cycles as described in Section 2.3.

The loading of rGO and nZVI was optimized using phenol degradation kinetics as a performance indicator. 0%–10% rGO was introduced for the synthesis of n% GCN, and then 0%–15% nZVI was applied for the synthesis of n% IGCN. The degradation of phenol on various composites is shown in Supplementary Figures S1, S2 and Supplementary Tables S2, S3. It showed that 7.5% GCN and 10% IGCN had the highest degradation effects on phenol under the visible light (λ > 400 nm), which were 79.7% and 86%. Compared to the 72.7% degradation of phenol by MCB_0.07, the removal efficiency of n% GCN and n% IGCN has been effectively improved.

The photocatalytic degradation of OFL, NOR, and CIP on MCB_0.07, 7.5% GCN, and 10% IGCN are shown in Figure 2. Under visible light (λ > 400 nm) irradiation, the degradation of the antibiotic conformed well to the first-order kinetics. The reaction rate constants of MCB_0.07, 7.5% GCN, and 10% IGCN were 0.0150 min⁻¹, 0.0264 min⁻¹, and 0.0318 min⁻¹ for the degradation of OFL, 0.0122 min⁻¹, 0.0274 min⁻¹, and 0.0450 min⁻¹ for the degradation of NOR, and 0.0158 min⁻¹, 0.0242 min⁻¹, and 0.0406 min⁻¹ for the degradation of CIP, respectively. The degradation rate of 10% IGCN for the three antibiotics was the highest, indicating that the loading of rGO and nZVI can effectively improve the photocatalytic activity of g-C₃N₄. As shown in Supplementary Figure S3, the oxidation of OFL, NOR, and CIP is not complete, which indicates the existence of oxidation intermediates. The photolysis of OFL, NOR, and CIP under visible light irradiation, shown in Supplementary Table S4, are 8.28%, 8.10%, and 9.64%, respectively, which show the little effect on the photocatalytic degradation process.

The adsorption of OFL, NOR, and CIP on synthesized photocatalysts was evaluated under dark conditions. As shown in Supplementary Figure S4, it was found that the adsorption capacity of three quinolone antibiotics for the same photocatalytic material is not much different, but the adsorption capacity of different photocatalytic materials for the three quinolone antibiotics is obviously different. The removal efficiencies of OFL, NOR, and CIP were 14.63%, 14.24%, and 15.90% using MCB_0.07, respectively. Moreover, the removal efficiencies of OFL, NOR, and CIP were 5.88%, 6.91%, and 6.60% using 10% IGCN, respectively. The decreasing adsorption capacity of MCB_0.07, 7.5% GCN and 10% IGCN for fluoroquinolone antibiotics is related to the reduction of active sites due to the loading of rGO and nZVI as shown by the decrease of BET surface area (Supplementary Figure S5) and pore volume (Supplementary Figure S6). The adsorption of OFL, NOR, and CIP on each photocatalyst was comparable and the photocatalytic experiments were conducted after the adsorption reaching the equilibrium. Therefore, the adsorption effect was neglectable to photocatalytic degradation. Secondly, MCB_0.07 has the highest static adsorption rate, but its ability that produces reactive oxygen species is relatively poor. While 10% IGCN has a weak adsorption capacity, it has a solid ability to produce reactive oxygen species (the removal effect of 10% IGCN for three antibiotics was seen in Section 3.3). Therefore, the strong adsorption capacity is not necessarily related to the high organic matter removal capacity.

To observe the morphological and microstructural features of as-prepared samples, scanning electron microscopy (SEM) and transmission electron microscopy (TEM) images were investigated. As shown in Figure 3A, the MCB_0.07 showed an abundant porous structure distributing evenly and densely on the surface, which was consistent with previous studies (Zheng et al., 2016; Chang et al., 2019). The original GO exhibits an irregular layered flaky structure with rough edges and smooth surfaces, shown in Figure 3D (Liu et al., 2017). According to the previous work, after 550°C treatment, GO was reduced to rGO (Shanavas et al., 2019; Hu et al., 2021), while the wrinkles and curls could be observed from rGO (Agarwal and Zetterlund, 2021). However, although the porous structure of 7.5% GCN and the interface between rGO and MCB_0.07 can be observed (Figure 3B), the pore of 7.5% GCN was inapparent and messy than MCB_0.07. This may be due to the introduction of rGO layers, which upset the pore structure of MCB. This was consistent with the Brunauer-Emmett-Teller (BET) results. The pristine nZVI particles exhibit uncontrollable agglomeration, shown in Figure 3E. After loading nZVI on 7.5% GCN to synthesize 10% IGCN, it was observed that nZVI spherical particles were successfully attached to the sheet layer of 7.5% GCN with slight agglomeration (Figure 3C).

The energy dispersive X-ray spectroscopy (EDS) of MCB_0.07, 7.5% GCN, and 10% IGCN composites showed that C and N were uniformly distributed, and O was also presented due to incomplete polymerization of cyanuric acid or barbituric acid on g-C₃N₄ and the residual O-containing functional groups of rGO (Supplementary Figures S7, S8). As shown in Supplementary Table S5, the weight ratio of C and O in 7.5% GCN and 10% IGCN increased, while the weight ratio of N decreased compared with MCB_0.07. This can indicate that rGO was successfully introduced to the sample since rGO has residual O-containing groups (Hu et al., 2021). The presence of about 2.52% Fe on 10% IGCN indicated the successful loading of nZVI, and Fe was also uniformly distributed on the samples.

The pore structures and BET specific surface area of the as-synthesized samples were further characterized by the N₂ adsorption-desorption isotherm method. As shown in Supplementary Figure S5, MCB_0.07, 7.5% GCN, and 10% IGCN all presented a representative type-IV curve with a high adsorption capacity at high relative pressures, indicating that they all have the highly porous structure (Li et al., 2015). In addition, mesopores were the main pore structure of three photocatalysts (Supplementary Figure S6; Table 1). However, the BET surface area and total pore volume of MCB_0.07, 7.5% GCN, and 10% IGCN showed a decreasing trend. MCB_0.07 showed the highest BET surface area (104.139 m²/g) and pore volume (0.270 cm³/g). Although the BET surface area of GO was determined to be 181.991 m²/g, the BET surface area and total pore volume of 7.5% GCN dropped to 79.558 m²/g and 0.225 cm³/g, respectively. This may be explained by the fact that the pores of MCB_0.07 were destroyed by the rGO lamellar texture (Shao et al., 2016). With further loading of nZVI, nZVI may block the part of the pores on 10% IGCN as a result of the smaller size of nZVI particles (Rao et al., 2021), the BET surface area and total pore volume of 10% IGCN further decreased to 53.739 m²/g and 0.163 cm³/g, respectively. However, the removal efficiency of OFL, NOR, and CIP on 10% IGCN was higher than the other two photocatalysts (Figure 2), which indicated that the enhanced photocatalytic activity of the samples has no direct relationship with the BET surface areas, even though the parts of reactive sites of g-C₃N₄ were sacrificed due to the modification of nZVI and rGO.

The crystal structures of the as-prepared samples are determined by X-ray diffraction (XRD), shown in Figure 4. Two distinct and typical diffraction peaks at 13.0° and 27.34° (ICDD No. 87–1,526) were observed for MCB_0.07, 7.5% GCN, and 10% IGCN, which are indexed to g-C₃N₄. The stronger peak at 27.34° was assigned to (002) crystal plane originating from the interlayer-stacking structure of a conjugated aromatic system (Liu et al., 2019), while the weaker peak at 13.0° corresponded to the (001) crystal plane originated from in-plane structural packing motif of tri-s-triazine units (Chang et al., 2019), respectively. However, the characteristic peaks of 7.5% GCN and 10% IGCN exhibited a slight shift compared with MCB_0.07, which was attributed to the lattice strain generated in the hybridization process of MCB_0.07 and rGO (Chen et al., 2020b). The GO sample presented a strong diffraction peak at 10.8° corresponding to the (001) crystal plane (Feng et al., 2022). Nevertheless, a new diffraction peak at 25.2° is detected after the GO treated under 550°C, shown in Supplementary Figure S9, being in accord with (002) crystal plane (Jaiswal et al., 2020), which provided the evidence for the conclusion that the GO was thermally reduced to rGO. However, the diffraction peaks of rGO were not detected in 7.5% GCN and 10% IGCN. It may be due to the content of rGO being too low to be detected (Tang et al., 2022). After nZVI loaded on 7.5% GCN, three typical diffraction peaks at 44.94°, 65.26°, and 82.46° were observed in the image of 10% IGCN, corresponding to (110), (200), and (211) crystal planes (ICDD No. 87–0722) (Huang et al., 2020), respectively. This indicated that the nZVI was successfully loaded without apparent oxidation, which may be credited with the protective effect of graphene materials on nZVI (Wang et al., 2019).

The molecular structures of the as-prepared samples were further examined by Fourier-transform infrared (FTIR) spectroscopy. As shown in Figure 5, the MCB_0.07, 7.5% GCN, and 10% IGCN showed the typical absorption peaks with g-C₃N₄. The broad peaks between 2,850 and 3,600 cm⁻¹ were from the stretching vibration of O–H bands and N–H components (Wang et al., 2019; Xiao et al., 2021). This indicated that the presence of unpolymerized–NH₂/=NH groups at the defect sites of the aromatic ring in the cyclic g-C₃N₄ structure was identified (Shanavas et al., 2019). Besides, according to the study of (Huang et al., 2021), the incomplete polymerized fragments of g-C₃N₄ play a leading role in the separation of charge carriers. In addition, the peaks at 1,200–1,650 cm⁻¹ can be attributed to the skeletal stretching vibration modes of a heptazine heterocyclic ring (Li et al., 2015) containing the N–(C)3 or bridging C–NH–C units (Kim et al., 2020). The sharp peak at 812 cm⁻¹ was the breathing mode of the tri-s-triazine ring (Xiao et al., 2021). Compared with the GO sample, the characteristic peaks of GO were not detected in the 7.5% GCN and 10% IGCN samples. This may be explained by the carboxyl, carbonyl, and ester bonds on the surface of GO were reduced at 550°C to form rGO. In addition, as a result of the small amount of rGO in 7.5% GCN and 10% IGCN, the typical peaks were not obvious or merged with the peaks of g-C₃N₄. That was mutually supportive of the XRD results.

The compositions and chemical states of 10% IGCN were analyzed by X-ray photoelectron spectroscopy (XPS). As shown in Supplementary Figure S10, 10% IGCN was mainly composed of C, N, O, and Fe. For a closer examination of C, N, O, and Fe peaks, high-resolution XPS scans over C 1s, N 1s, O 1s, and Fe 2p of 10% IGCN sample were obtained, respectively. The high-resolution XPS scans over C 1s of 10% IGCN contained three components located at 284.8, 286.4, and 288.4 eV. The peak at 284.8 eV is assigned to the alkyl carbon (C–C) (Zhou et al., 2018), which may be proof of the interaction between rGO and g-C₃N₄ (Palanivel et al., 2021). The peak of 286.4 and 288.4 eV are assigned to the C–O bonds (Wu et al., 2022b) and sp² carbon (N–C=N) presented in the framework of g-C₃N₄ (Zhou et al., 2018), respectively, as shown in Supplementary Figure S11A. As shown in Supplementary Figure S11B, the high-resolution scans over N 1s peaks could be deconvoluted into three peaks with binding energies of 399, 400.3, and 401.4 eV, corresponding to the aromatic N with sp²-hybridization bonded with C (C–N=C) (Shanavas et al., 2019; Zeng et al., 2020), the N–(C)3 groups at the edges of heptazine units (Xiao et al., 2021), and the amino functions (C–NH) which are derived from the terminal amino groups on the surface (Zhou et al., 2018), respectively. As shown in Supplementary Figure S11C, the high-resolution XPS scans over O 1s of 10% IGCN showed that three typical peaks were found with binding energies located at 529.9, 531.5, and 532.9 eV, respectively. The peak at 529.9 eV attributes to the Fe–O bond (Wang et al., 2021b) because of the partial oxidation of nZVI. In addition, the peaks located at 531.5 and 532.9 eV are associated with the C=O bond and organic C–O bond (Chen et al., 2021) due to incomplete polymerization of cyanuric acid or barbituric acid. Most notably, according to the previous research (Xie et al., 2022), compared with 7.5% GCN, the binding energies of C 1s, N 1s, and O 1s of 10% IGCN exhibited a distinct increase, which revealed that an intense interaction could be found between nZVI and 7.5% GCN rather than a simple physical mixing. The Fe species that existed in 10% IGCN were composed of Fe⁰ and oxidation states (e.g., Fe²⁺ and Fe³⁺) (Supplementary Figures S11C,D). The peaks at 707.2 and 720.4 eV of Fe 2p high-resolution XPS scans corresponded to Fe⁰ 2p_3/2 and Fe 2p_1/2 (Lv et al., 2021), respectively. It indicated that nZVI was loaded successfully. The presence of Fe³⁺ and Fe²⁺ was shown by the peaks of Fe 2p_3/2 and Fe 2p_1/2 at 711.9 and 725.9 eV and 710.6 and 724.3 eV (Ma et al., 2021), which represented that only a small amount of nZVI was inevitably oxidized on the particle surface in the preparation of 10% IGCN because of the high activity of nZVI (Liang et al., 2016; Kong et al., 2021; Rao et al., 2021).

The optical absorption properties of as-synthesized photocatalysts were characterized by measuring the UV-vis diffuse reflectance spectrum (UV-Vis DRS). The spectra (Supplementary Figure S12) indicate that the visible light absorption of MCB_0.07 is greatly enhanced via rGO and nZVI modification. Notably, the absorption edges of MCB_0.07, 7.5% GCN, and 10% IGCN were found to be 460 nm, 468 nm, and 599 nm, corresponding to the band gaps (E_g) of 2.70 eV, 2.65 eV, and 2.07 eV, respectively, which represented that the capability of harvesting and utilizing visible light photons were enhanced obviously. Compared to MCB_0.07, a slightly red shift was observed in 7.5% GCN, which may attribute to the intrinsic absorption of black-colored rGO (Shao et al., 2016) and the enhancement of π-π*conjugation effect by rGO is indispensable for the change (Tang et al., 2022). With further loading of the nZVI, 10% IGCN showed an intensive absorption in visible light region. This is probably relevant to the presence of Fe energy level results in decreasing of the energy gap for electron transition (Kong et al., 2021) and the synergism of rGO and nZVI (Fan et al., 2022), indicating that the introduction of rGO and nZVI play a critical role in improving the absorption capacity of visible light. However, in general, the narrower Eg is, the faster recombination of photo-generated charge carriers is, while 10% IGCN was not affected during, which will be discussed below.

To further explore the photoelectric conversion capability and carrier separation efficiency, transient photocurrent response and electrochemical impedance spectroscopy (EIS) are performed, as shown in Figure 6A. The smaller the radius of the curve is, the lower the charge transfer resistance is. The radius of the curve for MCB_0.07 was the largest and significantly larger than 7.5% GCN, indicating that the introduction of rGO accelerated the rate of charge transfer at the interface of the photocatalysts and reduced the charge transfer resistance of g-C₃N₄ (Jo et al., 2018), which could be attributed to the high charge-carrier mobility capability of the rGO sheets (Tong et al., 2015; Chen et al., 2017). With loading nZVI on 7.5% GCN, the curve radius of 10% IGCN reduced further due to the excellent conductivity of nZVI (Kong et al., 2021). Figure 6B shows that the transient photocurrent responses are recorded by switching the visible-light-on-off for five cycles. In general, the larger the photocurrent density is, the higher the photo-generated carrier mobility is. Obviously, the photocurrent density of 10% IGCN was significantly larger than that of MCB_0.07 and 7.5% GCN, which meant that 10% IGCN had good separation efficiency of photo-induced e⁻- h⁺ pairs. Similarly, the photoluminescence (PL) spectrum result also confirms that 10% IGCN possesses a better photo-generated e⁻-h⁺ separation efficiency (Figure 6C) due to the gradually decreasing fluorescence intensity.

Notably, the narrower E_g of 10% IGCN was prone to induce photo-generated e⁻-h⁺ recombination, but the synergy between g-C₃N₄, rGO, and nZVI could effectively improve the transfer and separation efficiency of e⁻-h⁺ (Wang et al., 2019) and offset the negative effect of narrow E_g, combined with the EIS, transient photocurrent response and PL spectrum results. In addition, although Fe⁰ was oxidized due to inevitable oxidation, ≡Fe^II and ≡Fe^III on the surface of material could capture e⁻ and reduced to Fe⁰, which could improve the e⁻-h⁺ separation.

Under the visible light radiation (λ > 400 nm), the photocatalytic degradation of OFL, NOR, and CIP on 10% IGCN with time is displayed in Figure 7. The results showed that the degradation process of OFL, NOR, and CIP by 10% IGCN conforms to the first-order reaction rate equation (Table 2). The degradation rate of NOR is 0.045 min⁻¹, which is higher than that of CIP (k = 0.0406 min⁻¹) and OFL (k = 0.0318 min⁻¹). Moreover, all three antibiotics had a more significant degradation rate. The difference in degradation rate may be related to the molecular structure and the molecular weight (Fang et al., 2021).

To evaluate the mineralization of antibiotics on 10% IGCN, the change of DOC reaction rate constants in the solution was measured. As Figure 7B shows, the reaction rate constants of DOC for OFL, NOR, and CIP degradation by 10% IGCN were 0.0107 min⁻¹, 0.011 min⁻¹, and 0.0108 min⁻¹, respectively. The reaction rate constants of DOC for the three antibiotics were not significantly different. Compared with the apparent degradation effects of OFL, NOR, and CIP in Figure 7A, the DOC results showed that all three antibiotics had degradation products. However, the oxazinyl in the OFL structure is not easy to break and open (Tian et al., 2020; Zhao et al., 2021), and the cyclopropyl in the CIP structure is not easy to fall off, either (Wang et al., 2018; Bai et al., 2020; Chen et al., 2020a). These molecular structures may have a specific impact on the mineralization of antibiotics.

To clarify the impacts of reactive species on the photocatalytic degradation of OFL, NOR, and CIP by 10% IGCN, isopropanol (IPA), L-histidine (L-His), 1,4-benzoquinone (BQ), EDTA-2Na, and catalase was introduced to the reaction system to trap •OH, ¹O₂, •O₂ ⁻, h⁺, and H₂O₂.

As shown in Supplementary Figure S14 and Supplementary Table S6, after adding EDTA-2Na, the degradation kinetics of OFL, NOR, and CIP decreased to 0.0048, 0.0072, and 0.0086 min⁻¹, respectively, indicating that h⁺ played a dominant role during the photocatalytic degradation of the three antibiotics. However, from the perspective of inhibition rate (Supplementary Figure S15), compared with h⁺, the contributions of individual reactive oxygen species (ROS) (•OH, ¹O₂, •O₂ ⁻, and H₂O₂) do not show dramatic differences in the degradation of OFL, NOR, and CIP. In detail, the ROS inhibition rate of OFL, NOR, and CIP followed the orders: •OH (37.78%) > •O₂ ⁻ (32.05%) > H₂O₂ (30.79%) > ¹O₂ (23.84%), •OH (30.22%) > ¹O₂ (24.72%) > H₂O₂ (17.40%) > •O₂ ⁻ (16.79%), and ·•O₂ ⁻ (27.90%) > ¹O₂ (19.57%) > H₂O₂ (15.87%) > •OH (13.86%). It may be explained that the differences in the molecular structures of the antibiotics may cause the different interactions between them and the ROS (Zheng et al., 2016). Furthermore, although the scavengers quenched the target ROS, it affected the formation of other ROS through the free radical chain reaction.

Furthermore, the energy band structure of 10% IGCN was proposed to illustrate the possible photocatalytic degradation mechanism accounting for the enhancing in degradation efficiency and the complicated oxidation process. The E _g of g-C₃N₄ was obtained at 2.70 eV from the UV-Vis DRS results (Supplementary Figure S12B). The conduction band (CB) and valence band (VB) edge potentials of g-C₃N₄ can be estimated according to Supplementary Eqs S4, S6. Combined with XPS valence band spectra (Supplementary Figure S13), the calculated E _CB and E _VB of g-C₃N₄ are −1.12 eV and 1.58 eV, respectively, consistent with previous research (Chang et al., 2019).

Combined with Supplementary Table S7, the possible mechanism is proposed to explain the transformation of photo-induced charge carriers in the photocatalytic system of 10% IGCN. Under the visible light irradiation, the e⁻ of g-C₃N₄ could be promoted to the CB, leaving h⁺ in the VB. However, it should be noted that the VB of g-C₃N₄ (+1.58 eV) was higher than the redox potential of •OH/H₂O (+2.32 eV) as well as •OH/OH⁻ (+1.99 eV), leading to the insufficient oxidation capacity of h⁺ to generate •OH, resulting in only being produced through the free radical chain reaction. Therefore, it provided evidence that the direct oxidation of pollutants induced by h⁺, existing on the surface of the photocatalyst, was the main step in the degradation of OFL, NOR, and CIP. Furthermore, the h⁺ was considered the starting point of the chain reaction, which was the source and necessary factor for producing the ROS (Zheng et al., 2019). As excellent electron mediators, e⁻ could be transferred from CB of g-C₃N₄ to rGO and then to nZVI, which meant that more e⁻ would be involved in the photocatalytic reaction. Moreover, owing to the interfacial interactions and synergistic effect between g-C₃N₄, rGO, and nZVI (Wang et al., 2019), the recombination of e⁻ and h⁺ was largely inhibited, and the utilization of visible light was greatly improved, while the photocatalytic performance was enhanced by the following process. The CB of g-C₃N₄ (−1.12 eV) was lower than the redox potential of O₂/•O₂ ⁻ (−0.33 eV), resulting in the capability to generate •O₂ ⁻, which could be further oxidized into ¹O₂ by h⁺ (¹O₂/•O₂ ⁻ (+0.65 eV)), as well as reduced into H₂O₂ by e⁻ (•O₂ ⁻/H₂O₂ (+0.89 eV)). With the exception of producing the •O₂ ⁻, the O₂ could also capture the e⁻ to generate H₂O₂ (O₂/H₂O₂ (+0.28 eV)). As an electron trapper, H₂O₂ could be dissociated into the •OH (H₂O₂/•OH (+0.38 eV)) using e⁻, which may be an important source of •OH. Although ≡Fe^II or ≡Fe^III could trap e⁻ to some extent to inhibit the oxidation of nZVI (Raha and Ahmaruzzaman, 2020), the nZVI is inevitably oxidized into Fe₂O₃ after the reaction (Supplementary Figure S20), attributing to the strong oxidation of ROS and activity of nZVI (Kong et al., 2021).

XPS was used to study the residues of OFL, NOR, and CIP on the surface of 10% IGCN before and after photocatalytic reaction to deduce the possible degradation intermediates. As shown in Figure 8; Supplementary Figures S16, S17, there are indistinct differences in C 1s, N 1s, and O 1s spectra. In contrast, although the Fe 2p spectra show the disappearance of the characteristic peaks of nZVI, it is speculated that the oxidation on the surface of nZVI led to no detection. However, the F 1s spectra showed a considerable change before and after the reaction (from 688.8 eV to 686.6 eV), indicating that the benzene ring attached to the C–F bond occurred as the ring-opening oxidation.

In summary, the possible photocatalytic degradation mechanisms of 10% IGCN in OFL, NOR, and CIP under visible light are proposed in Figure 9. As the main reactive species in the reaction, the h⁺ may attack the C–N bond between the piperazine ring and benzene binding at first (Fan et al., 2020; Hu et al., 2020; Hu et al., 2020; Su et al., 2022), according to the DFT calculation. Moreover, the cleavage on the piperazine ring induced by h⁺ was considered one of the degradation pathways because the two N atoms on the piperazine ring were also the most active sites (Hu et al., 2020; Zhang et al., 2020; Zhao et al., 2021). And then, the products could be further oxidized by •OH and •O₂ ⁻, etc. Moreover, the ring-opening oxidation of the benzene ring (C=C bond) connected by the C–F bond may also be an important step. With the exception of the above conclusion, the defluorination is observed definitely because of the increasing concentration of F⁻ in OFL, NOR, and CIP solution after the photocatalytic reactions (Table 3). •OH and •O₂ ⁻ were important ROS in the defluorination process, but their mechanisms differed. Combined with the contribution of ROS, it is speculated that the fluorine was substituted by •OH directly in the defluorination of OFL and NOR (Jin et al., 2019; Liu et al., 2020; Zhang et al., 2020; Wang et al., 2021a). However, the defluorination process in CIP solution may be triggered by •O₂ ⁻ (Wang et al., 2018), which subsequently underwent •OH substitution, leading to the formation of the defluorination product. It can be seen that the OFL, NOR, and CIP molecules were gradually decomposed by h⁺ and ROS and finally mineralized.

The stability performance of 10% IGCN photocatalyst is tested through the repeating experiment for OFL, NOR, and CIP degradation under the visible light irradiation, shown in Supplementary Figure S18. After four cycles, the removal efficiency of OFL, NOR, and CIP had a decrease from 82.71% to 71.92%, from 91.70% to 82.36%, and from 88.94% to 79.16%, respectively at 60 min, indicating the photo stability of the catalyst. The XRD patterns of the initial and used 10% IGCN composite for OFL, NOR, and CIP degradation were also conducted to further testify the stability of photocatalyst. As illustrated in Supplementary Figure S19, the diffraction peaks of nZVI are weakened, and the new peaks are consistent with Fe₂O₃ (ICDD. No. 39–0238), indicating that nZVI should be surface oxidation rather than complete oxidation, which is mutually explained with XPS results. However, the photocatalytic performance of 10% IGCN did not decrease significantly, which may be due to the existence of heterojunction between Fe₂O₃ and g-C₃N₄ (Shanavas et al., 2019).