Introduction

Water pollution has posed a potential threat to human health by the food chain system, thus it is particularly significant to develop some reliable methods to resolve water pollution problem [14]. By far, adsorption, coagulation, biological treatment, chemical oxidation, electrochemical treatment, and heterogeneous photocatalytic oxidation technology have been established for water purification [59]. Among the above techniques, TiO2-based heterogeneous photocatalysis has received much attention due to its low cost, strong oxidation ability, nontoxicity, chemical stability, biocompatibility, and simplicity of operation [1015]. However, TiO2 has a wide band gap (3.2 eV for anatase and 3.0 eV for rutile) and can only respond in the ultraviolet (UV) light region, which restrict its practical application in wastewater treatment [1620]. Therefore, it is imperative and challenging to develop new and efficient visible-light-responsive photocatalysts.

Ternary chalcogenide compounds possess narrow band gap, high stability, and strong visible-light absorption and thus have received tremendous attention in recent years [2123]. Stannum indium sulfide (SnIn4S8) is a common ternary chalcogenide semiconductor and exhibits potential application in photocatalysis [24, 25]. However, single SnIn4S8 semiconductors usually possess a small specific surface area and fast electron–hole recombination, and the photocatalytic activity of silver-based catalysts is diminished during recycling process, which would depress their photocatalytic efficiency and restrict practical application. To solve these problems, integrating SnIn4S8 with other proper semiconductors or supports is an effective and feasible strategy for high photocatalytic efficiency.

Graphitic carbon nitride (g-C3N4), a metal-free polymeric semiconductor, has drawn extensive attention due to its nontoxicity, low cost, suitable band position, excellent electrical conductivity, good thermal–chemical stability, excellent optical performance, and strong absorption of visible light, and has been regarded as a promising visible-light-responsive photocatalyst or an excellent support for many photocatalysts [2630]. Herein, we first presented low-temperature co-precipitation strategy for the fabrication of g-C3N4/SnIn4S8 composites in this study. The physicochemical and electrochemical properties of g-C3N4/SnIn4S8 composites were studied. The effect of g-C3N4 content on PL intensity, photocurrent intensity, and the photocatalytic activities of g-C3N4/SnIn4S8 composites under visible-light irradiation was also systematically investigated. Moreover, the possible photocatalytic mechanism of g-C3N4/SnIn4S8 was provided.

Experimental

Materials

Tin (IV) chloride pentahydrate (SnCl4·5H2O) and indium (III) chloride tetrahydrate (InCl3·4H2O) were purchased from Aladdin Chemistry Co. Ltd. (Shanghai, China). Thioacetamide (TAA) was purchased from China National Medicine Group Chemical Reagent Co., Ltd. (Shanghai, China). Dicyandiamide, urea, p-benzoquinone (BQ), isopropanol (IPA), and triethanolamine (TEOA) were purchased from Sinopharm Chemical Reagent Co., Ltd. (Shanghai, China). Ethanol was supplied by Shantou Xilong Chemical Co., Ltd. (Shantou, China). Methyl orange (MO) was obtained from Shanghai Jingxi Chemical Technology Co., Ltd. (Shanghai, China). All the reagents were of analytical grade and used as received without further purification. Water was purified using a Milli-Q water system (Bedford, USA).

Preparation of g-C3N4

The g-C3N4 was prepared by pyrolysis of urea and dicyandiamide in air atmosphere. 3.5 g urea and 1.5 g dicyandiamide were firstly milled for 30 min, then transferred in a muffle furnace, and heated to 530 °C for 4 h to complete the reaction [31].

Preparation of g-C3N4/SnIn4S8 composite via a low-temperature co-precipitation approach

0.421 g of SnCl4·5H2O (1.2 mmol) and 1.409 g of InCl3·4H2O (4.8 mmol) were dissolved in 96 mL of anhydrous ethanol under continuous magnetic stirring, and then 0.9 g TAA (12 mmol) was added to the above solution. Afterwards, a certain amount of g-C3N4 was added to the solution. The mixture solution was stirred until a transparent solution was formed, then the above solution was transferred to a 150-mL round-bottom flask with a reflux condenser, placed in a thermostatic bath at 70 °C for 3 h under continuous magnetic stirring, and cooled to room temperature naturally. The obtained yellow precipitate was filtered, washed with distilled water and absolute ethanol several times, and finally dried at 80 °C for 12 h. The samples with different g-C3N4 content were designated as pure SnIn4S8, 5 % g-C3N4/SnIn4S8, 10 % g-C3N4/SnIn4S8, 15 % g-C3N4/SnIn4S8, 20 % g-C3N4/SnIn4S8, 30 % g-C3N4/SnIn4S8, and 40 % g-C3N4/SnIn4S8.

Characterization

X-ray diffraction (XRD) patterns of samples were obtained using a Rigaku D/max 2200 PC automatic X-ray diffractometer (Rigaku, Japan). Transmission electron microscopy (TEM, Hitachi, Japan) and scanning electron microscopy (SEM, Shimadzu, Japan) were used to observe the morphology of the samples. Energy-dispersive spectrometry (EDS, Shimadzu, Japan) was used to confirm the existence of SnIn4S8 and g-C3N4. The specific surface area and pore structures of samples were determined using a GEMINI VII 2390 surface area and porosity analyzer (Micromeritics, USA). The reflectance spectra were obtained using a UV-2550 scan UV–Vis spectrophotometer (Shimadzu, Japan) equipped with a Labsphere diffuse reflectance accessory. The photoluminescence (PL) emission spectra were obtained using F-7000 fluorescence spectrophotometer (Hitachi, Japan).

Photocatalytic activity measurement

The photocatalytic activities were evaluated by decomposing MO under visible-light irradiation. A 300 W Xe lamp with a 400 nm cut-off filter was used as the visible-light source. For the typical photocatalytic experiments, 30 mg of photocatalyst was added into 160 mL of 10 mg/L MO solution. Before irradiation, the suspensions were magnetically stirred in the dark for 40 min to reach adsorption–desorption equilibrium. In the dark reaction, 4 mL suspension was sampled at different time intervals and centrifuged immediately to remove suspended photocatalyst powders. The concentration of MO was analyzed using a UV–Vis spectrophotometer at 463 nm.

Regeneration and reuse of spent g-C3N4/SnIn4S8 composite photocatalyst

The spent g-C3N4/SnIn4S8 catalysts were recovered from the mixture solution by centrifugation, regenerated by washing with water and ethanol, and then dried at 80 °C for 4 h. The regenerated g-C3N4/SnIn4S8 catalysts were reused for MO degradation under similar reaction conditions as with the fresh catalysts.

Results and discussion

XRD analysis

The crystal structure of g-C3N4, pure SnIn4S8, and 15 % g-C3N4/SnIn4S8 composite was characterized by XRD (Fig. 1). Pure SnIn4S8 and 15 % g-C3N4/SnIn4S8 have similar XRD patterns. The main diffraction peaks at about 2θ = 28.6° and 50.4° are observed, which can be indexed to the (600) and (001) crystalline planes of tetragonal phase of SnIn4S8, respectively. Moreover, it is interesting to note that no g-C3N4 diffractions are found in the XRD pattern of g-C3N4/SnIn4S8 composite, possibly due to the low loading content of g-C3N4 or the highly dispersed g-C3N4 on SnIn4S8.

Figure 1
figure 1

XRD patterns of g-C3N4, pure SnIn4S8, and 15 % g-C3N4/SnIn4S8

Morphology analysis of pure SnIn4S8 and g-C3N4/SnIn4S8

The morphologies of pure SnIn4S8 and 15 % g-C3N4/SnIn4S8 are shown in Fig. 2. Pure SnIn4S8 is composed of a large amount of 3D hierarchical network-like spheres with a diameter ranging from 1 to 2 µm. An enlarged view of an individual SnIn4S8 sphere shows that the network-like superstructure of pure SnIn4S8 is constructed by numerous bending two-dimensional nanosheets with a thickness of about 20 nm. In case of 15 % g-C3N4/SnIn4S8, the thickness of nanosheets becomes obviously thinner, and hierarchical pores between nanosheets become obviously larger compared with pure SnIn4S8. The thinner nanosheets and larger hierarchical pores are beneficial for the multiple scattering of light and light-harvesting capacity, thus it is expected that this structure would improve the photocatalytic activity of g-C3N4/SnIn4S8.

Figure 2
figure 2

SEM images of a pure SnIn4S8 and b 15 % g-C3N4/SnIn4S8 with different magnifications

The microstructure of g-C3N4, pure SnIn4S8, and 15 % g-C3N4/SnIn4S8 composites was further studied by TEM (Fig. 3). The TEM images further confirmed the network-like structure of pure SnIn4S8, and g-C3N4 possessed a loose structure and nanopores with size in the range of 20–50 nm, and it is clear that g-C3N4 was successfully dispersed on SnIn4S8.

Figure 3
figure 3

TEM images of a pure SnIn4S8, b g-C3N4, and c 15 % g-C3N4/SnIn4S8

EDS analysis

The EDS analysis was used to analyze the chemical composition of pure SnIn4S8 and 15 % g-C3N4/SnIn4S8 (Fig. 4). It can be seen from Fig. 4 that pure SnIn4S8 is composed of Sn, In, and S elements. In case of 15 % g-C3N4/SnIn4S8, Sn, In, S, C, and N elements were observed, confirming the formation of g-C3N4/SnIn4S8 composites.

Figure 4
figure 4

EDS patterns of a pure SnIn4S8 and b 15 % g-C3N4/SnIn4S8 composites

Specific surface areas and porous structures

The nitrogen adsorption–desorption isotherm and the pore size distribution curves of pure SnIn4S8 and 15 % g-C3N4/SnIn4S8 composite are shown in Fig. 5. The isotherms of pure SnIn4S8 and 15 % g-C3N4/SnIn4S8 are classified as type IV according to the Brunauer–Deming–Deming–Teller (BDDT) classification, implying the presence of mesopores (2–50 nm). The shape of the hysteresis loop is of type H3, which is associated with aggregates of plate-like particles, giving rise to slit-like pores. Pure SnIn4S8 and 15 % g-C3N4/SnIn4S8 composites possessed broad and bimodal pore size distribution with small mesopores (2–3 nm) and larger ones (5–30 nm). The BET surface areas of pure SnIn4S8 and 15 % g-C3N4/SnIn4S8 composites are 14.49 and 21.33 m2 g−1, respectively. A larger surface area of 15 % g-C3N4/SnIn4S8 provides more surface active sites for the adsorption of the reactive molecules, which is beneficial for the photocatalytic degradation of organic pollutants.

Figure 5
figure 5

a Nitrogen adsorption–desorption isotherms and b pore size distribution curves of pure SnIn4S8 and 15 % g-C3N4/SnIn4S8

Optical properties

The UV–Vis diffuse reflectance spectra of pure SnIn4S8, g-C3N4, and 15 % g-C3N4/SnIn4S8 composite are shown in Fig. 6a. We can see that the absorption edges of 15 % g-C3N4/SnIn4S8 composite shift significantly to longer wavelength, and the absorption intensity of 15 % g-C3N4/SnIn4S8 composite is stronger than that of pure SnIn4S8.

Figure 6
figure 6

a UV–Vis diffuse reflectance spectra and b plots of (αhv)2 versus hv of pure SnIn4S8, g-C3N4, and 15 % g-C3N4/SnIn4S8

The band gap energies of pure SnIn4S8, g-C3N4, and 15 % g-C3N4/SnIn4S8 composite can be estimated from the following equation: (αhv)n = k(hv-Eg), where α is the absorption coefficient, k is a constant, hv is the photonic energy, Eg is the absorption band gap energy, and the value of n is 2 and 1/2 for a direct and an indirect band gap semiconductor, respectively. Plots of (αhv)2 versus hv of the samples are shown in Fig. 6b, and the band gap energies of pure SnIn4S8, 15 % g-C3N4/SnIn4S8, and g-C3N4 are estimated to be about 1.8, 1.68, and 2.58 eV, respectively.

PL emission spectra

The separation efficiency of photogenerated electrons and holes can be investigated by PL emission spectra. Figure 7 represents the PL spectra of pure SnIn4S8 and g-C3N4/SnIn4S8 composites with different g-C3N4 content. Pure SnIn4S8 shows the highest PL intensity, indicating that pure SnIn4S8 exhibits the highest recombination of electrons and holes and the lowest separation efficiency under visible-light irradiation. Moreover, the PL emission intensity of g-C3N4/SnIn4S8 composites is obviously influenced by the content of g-C3N4. With increasing the g-C3N4 content from 0 to 15 %, the emission intensity of g-C3N4/SnIn4S8 composite decreased, but further increasing the g-C3N4 content results in a dramatic increase of PL emission intensity, leading to the lowest PL emission intensity for 15 % g-C3N4/SnIn4S8 composite. Therefore, it is implied that 15 % g-C3N4/SnIn4S8 composite could exhibit the highest separation efficiency of electron–hole pairs under visible-light irradiation.

Figure 7
figure 7

PL spectra of pure SnIn4S8 and g-C3N4/SnIn4S8 composites with different g-C3N4 content

Photocurrent analysis

To further confirm the separation efficiency of photogenerated electrons and holes, the transient photocurrent response versus time curves of g-C3N4, SnIn4S8, and g-C3N4/SnIn4S8 composite ITO electrodes under visible-light irradiation were measured (Fig. 8). The photocurrent intensity increased in the order of g-C3N4 < pure SnIn4S8 < 5 % g-C3N4/SnIn4S8 < 10 % g-C3N4/SnIn4S8 < 20 % g-C3N4/SnIn4S8 < 15 % g-C3N4/SnIn4S8, indicating that g-C3N4 content in the composite has an obvious effect on the photocurrent intensity of g-C3N4/SnIn4S8 composite. The photocurrent intensity of g-C3N4/SnIn4S8 composite increased with increasing the g-C3N4 content from 0 to 15 %, but decreased with further increasing the g-C3N4 content from 15 % to 20 %, leading to the highest photocurrent intensity for 15 % g-C3N4/SnIn4S8 composite. The highest photocurrent intensity of 15 % g-C3N4/SnIn4S8 composite further confirmed its highest separation efficiency of electron–hole pairs under visible-light irradiation, which is consistent with PL results.

Figure 8
figure 8

Transient photocurrent response for g-C3N4, pure SnIn4S8, and g-C3N4/SnIn4S8 composites with different g-C3N4 content

Photocatalytic activity

Figure 9 shows the adsorption process in the dark and photocatalytic degradation of MO over pure SnIn4S8, g-C3N4, and g-C3N4/SnIn4S8 composites under visible-light irradiation. The photocatalytic activity of g-C3N4/SnIn4S8 composite is higher than that of pure SnIn4S8 and g-C3N4 and is greatly influenced by the g-C3N4 content. The photocatalytic activity of g-C3N4/SnIn4S8 composite is enhanced with increasing the g-C3N4 content from 5 % to 15 %. When the content of g-C3N4 reaches 15 %, it exhibits the highest photocatalytic activity, giving rise to the almost complete degradation of MO, which is much higher than that of pure SnIn4S8. However, as the proportion of g-C3N4 further increases from 15 to 40 %, the photocatalytic activity decreases gradually though it remains higher than that of pure SnIn4S8. Possible reason is that appropriate amount of g-C3N4 is beneficial for the generation and transfer of photogenerated electrons and holes, while excessive g-C3N4 could shield SnIn4S8 from light as well as promote electron–hole recombination. Therefore, due to the demands of both the charge transfer and light harvesting, the photocatalytic activity of g-C3N4/SnIn4S8 firstly increases and then decreases with increasing g-C3N4 content, which results in the best photocatalytic activity of 15 % g-C3N4/SnIn4S8.

Figure 9
figure 9

Temporal changes of MO concentration in the presence of pure SnIn4S8 and g-C3N4/SnIn4S8 composites with different g-C3N4 content

Photocatalytic mechanism

In order to detect the main reactive species (such as h+, OH, and O2 radicals) of 15 % g-C3N4/SnIn4S8 composite during photocatalytic process under visible-light irradiation, the trapping experiment of h+, OH, and O2 radicals was investigated by adding 1.0 mmol/L TEOA (a quencher of h+), 1.0 mmol/L BQ (a quencher of O2 ), and 1.0 mmol/L IPA (a quencher of OH), respectively. As shown in Fig. 10, the degradation efficiency of MO is 97.63 % in the absence of quenchers. When TEOA, BQ, and IPA scavengers were added, the MO degradation efficiency was reduced to 4.83, 36.4, and 72.1 %, respectively. The results indicated that the main reactive species which play crucial roles in the degradation of MO follow the order of h+ > O2  > OH.

Figure 10
figure 10

Effect of different scavengers on the MO photodegradation by 15 % g-C3N4/SnIn4S8

According to the band gap energy and Mott–Schottky plot of SnIn4S8 (Fig. 11), the conduction band potential (E CB) and valence band potential (E VB) of SnIn4S8 can be calculated. The flat-band potential (E fb ) of SnIn4S8 can be estimated from the Mott–Schottky equation:

$$ \frac{1}{{C^{2} }} = \frac{2}{{\varepsilon \varepsilon_{o} N_{d} }}\left( {E - E_{fb} - \frac{{k_{\text{B}} T}}{e}} \right), $$

where C is the space charge capacitance, ε is the dielectric constant of the semiconductor, ε 0 is the permittivity of free space, N d is the donor density, E is the applied potential, E fb is the flat-band potential, kB is Boltzmann’s constant (1.38 × 10−23 J K−1), T is the absolute temperature, and e is the electronic charge. The E fb value can be determined by extrapolating the linear part of the curve to \( \frac{1}{{C^{2} }} \) = 0, and the E fb value of SnIn4S8 is about −0.45 V versus the saturated calomel electrode (SCE), and is about −0.21 V versus NHE. Supposing the difference between flat-band potential and conduction band potential can be negligible for n-type semiconductors [32], the E CB value (−0.21 V vs NHE) is approximately equal to the E fb value. The E VB of SnIn4S8 can be calculated by empirical equation (E VB = E CB + E g), and the E VB value of SnIn4S8 is about 1.59 V versus NHE.

Figure 11
figure 11

Mott–Schottky plots for SnIn4S8

Based on the trapping experiment results, E CB and E VB values of SnIn4S8, and the reported literatures, the generation and transfer of the photogenerated holes and electrons in g-C3N4/SnIn4S8 composites are illustrated in Fig. 12. As shown in Fig. 12, under visible-light illumination, the photogenerated electrons (e) and holes (h+) can be excited from the valence band (VB) and conduction band (CB) of g-C3N4 and then transferred to the VB and CB of SnIn4S8, respectively. The accumulated e on the surface of SnIn4S8 can react with adsorbed O2 to form superoxide radicals (O2 ). A majority of O2 radicals play important roles in the MO degradation, and the rest of O2 could further react with H2O to generate hydroxyl radicals (OH), which also have some impact on the degradation of MO. The h+ in the VB of SnIn4S8 can preferentially attack MO adsorbed onto the surface of g-C3N4/SnIn4S8 composites, and then MO can be transformed to degradation products.

Figure 12
figure 12

Photocatalytic mechanism of g-C3N4/SnIn4S8 composite under visible-light irradiation

Regeneration and reuse of spent g-C3N4/SnIn4S8 composite

To test the stability and reusability of 15 % g-C3N4/SnIn4S8, the 15 % g-C3N4/SnIn4S8 composite was reused four times for photocatalytic reaction under the same conditions, and the results are shown in Fig. 13a. There is no obvious decrease in the photocatalytic activity of the 15 % g-C3N4/SnIn4S8 after four consecutive photocatalytic degradation cycles, indicating that the 15 % g-C3N4/SnIn4S8 is stable and can be used repeatedly. Moreover, the structure of the regenerated 15 % g-C3N4/SnIn4S8 after four consecutive cycles was characterized by XRD, and the results are shown in Fig. 13b. It can be seen that there is no significant change of crystal structure, and the main diffraction peaks of the regenerated 15 % g-C3N4/SnIn4S8 are approximately consistent with those of the fresh counterpart.

Figure 13
figure 13

a Regeneration and reuse of 15 % g-C3N4/SnIn4S8 and b XRD patterns of the regenerated 15 % g-C3N4/SnIn4S8 after four consecutive cycles

Conclusions

We first successfully prepared hierarchical network-like g-C3N4/SnIn4S8 composites with visible-light response and high photocatalytic activity by low-temperature co-precipitation method. The band gap energies of g-C3N4, pure SnIn4S8, and 15 % g-C3N4/SnIn4S8 are 2.58, 1.8, and 1.68 eV, respectively. The g-C3N4 content in g-C3N4/SnIn4S8 composites was optimized, and the optimal 15 % g-C3N4/SnIn4S8 composites showed the maximum photocurrent intensity and the best photocatalytic performance with complete degradation of MO within 80 min under visible-light irradiation, which is much higher than that of pure SnIn4S8. The main reactive species which affect MO degradation efficiency follow the order of h+ > O2  > OH, and the possible degradation mechanism was proposed. Moreover, 15 % g-C3N4/SnIn4S8 exhibits excellent reusability and stability without an obvious decrease of photocatalytic activity after four consecutive photocatalytic degradation cycles.