1. Introduction
The fast-growing global economy has resulted in a vast number of industries, many of which directly or indirectly generate various environmental pollutants, which can cause serious threats to society’s well-being and the development of a sustainable future [
1]. Therefore, there is no question that these pollutants must be tackled to overcome their many undesirable consequences. Among many remediation strategies to address environmental pollutants, semiconductor-based solar photocatalysis, which utilizes the abundant solar energy irradiated by the sun to decompose environmentally polluting organic and inorganic species via various light-induced redox reactions over semiconductor materials, is quite promising [
2]. While many semiconducting materials, such as TiO
2, ZnO, and SnO
2, have been extensively studied for this purpose, their large band gap energy hinders the absorption of visible light and results in inefficient utilization of solar energy to photocatalyze reactions over these materials.
Graphitic carbon nitride (g-C
3N
4), a low-cost metal-free polymeric semiconductor with great thermal and chemical stability and good electronic structure and photoactivity in the visible region of electromagnetic radiation, has recently emerged as a promising visible-light photocatalyst for degradation of various pollutant using sunlight, and thus stimulated intensive research works [
2,
3]. g-C
3N
4 materials are often synthesized by treating certain nitrogen-rich organic precursors at high-temperature. However, g-C
3N
4 materials synthesized via high-temperature thermal treatment of precursors such as cyanamide, dicyandiamide, melamine, thiourea and urea generally possess non-porous structure and relatively low surface area because these precursors tend to undergo a high degree of polycondensation at high temperature [
4,
5]. Thus, finding synthetic methods and/or precursors that can lead to advanced g-C
3N
4 materials with high surface area and large porosity is of paramount importance, since these structural features provide the materials with more accessible catalytically active sites and better pathways for mass transport of reactants and products and thus improved photocatalytic performances for decontamination of pollutants, water splitting, carbon dioxide reduction, etc. [
2,
6,
7].
Meanwhile, although g-C
3N
4 has a good band gap energy (2.7 eV) for visible-light photocatalysis, with conduction band (CB) and valence band (VB) potentials located at ca. –1.1 eV and ca. +1.6 eV vs normal hydrogen electrode (NHE), respectively [
5], its photo-induced electron-hole pairs still suffer from rapid recombination even when high surface area and large porosity are introduced into the material. As a result, g-C
3N
4‘s charge carriers are often unable to participate in many photocatalytic reactions and the material shows poor photocatalytic activity [
1]. In order to improve charge separation as well as light absorption over g-C
3N
4, many strategies have been developed. For example, some improvement in the optical properties and electronic structures of g-C
3N
4 have been realized by depositing metal particles on it [
8], doping or co-doping heteroatoms (metals or nonmetals) on it [
6,
9,
10], combining it with carbon materials [
11] and constructing heterojunctions over its structures [
12]. In the case of metal deposition, the immobilized metal particles on the surfaces of g-C
3N
4 increase charge separation, usually by capturing the photogenerated electrons and preventing them from combining with the holes. For this, noble metals such as Au [
13], Pt [
14], Pd [
15] and Ag [
16] have particularly been used, and their hybrid products with g-C
3N
4 have shown superior photocatalytic performances. Compared with noble metals, non-noble metals such as Cu are more appealing to use for these purposes because they are more Earth-abundant and can be combined with g-C
3N
4 to yield low-cost hybrid materials for a broad range of applications [
17,
18]. In terms of the potential applications of such g-C
3N
4-based semiconductor composite materials, pollutant degradation is of particular interest. In fact, g-C
3N
4-based materials have been demonstrated to degrade a variety of organic contaminants, including methyl orange, methylene blue and rhodamine B [
5].
Over the past few years, melamine has been successfully used as precursor to synthesize g-C
3N
4 materials by thermal condensation [
19,
20]. Melamine has some advantages, especially compared with cyanamide precursors that are more commonly used to make g-C
3N
4. It is nontoxic and inexpensive. Furthermore, it is less likely to produce toxic and flammable byproducts if additional solution-phase nanocasting synthetic steps, e.g., rigid template materials (such as mesoporous or colloidal SiO
2) to create nanopores in g-C
3N
4, are included [
4].
Herein, we show that melamine and colloidal silica nanoparticles with different sizes can be used, as precursor and hard templates, respectively, to produce mesoporous g-C
3N
4 (mpg-C
3N
4) materials with three-dimensionally interconnected frameworks, large surface areas and high porosities. The mass ratio of melamine-to-silica nanoparticles is found to be crucial in the formation of high surface area and desirable pore sizes in the final g-C
3N
4 materials. The pore size in the materials was easily tailored (to be around 12, 22, 47 or 79 nm) simply by changing the sizes of the silica nanoparticles used as templates during the synthesis. By functionalizing the surfaces of the mpg-C
3N
4 materials with Cu nanoparticles, mpg-C
3N
4 materials decorated with Cu nanoparticles are produced. The Cu-decorated mpg-C
3N
4 composite material are then demonstrated, for the first time, to serve as efficient photocatalysts for degradation of tartrazine yellow, a colorful azo-dye that is widely used as a colorant in various food and pharmaceutical products in many countries, but is also implicated in causing allergies, hyperactivity and even cancer if consumed in excess, and is banned in some countries as a result [
21].
3. Results and Discussion
The synthetic procedures that were employed to make the set of mesoporous C
3N
4 and Cu-decorated mesoporous C
3N
4 materials (denoted as
y-mpg-C
3N
4-
x and Cu-22-mpg-C
3N
4 respectively) are illustrated in
Scheme 1 and also described in the Experimental section above. First, an optimal mass ratio of melamine-to-silica nanoparticles that can render the material with high surface area and desired pore sizes, replicating the sizes of the silica nanoparticles templates, was determined. Briefly, melamine was mixed with different amounts of 12 nm colloidal silica templates and the solvent was evaporated resulting in melamine/silica nanoparticles composite materials. After subjecting the composite materials to thermal condensation and removing the silica templates from the carbonized composite products, a set of 12-mpg-C
3N
4−
x materials was obtained, in which
x represents the mass ratio of melamine-to-silica nanoparticles used (0.25, 0.5, 1, or 4). Another set of materials,
y-mpg-C
3N
4-1, where
y represents the size of colloidal silica templates, was synthesized using 22, 47 or 79 nm silica nanoparticles as templates with an optimized
x value (
x = 1). Two different amounts of Cu
2+ (5 or 10 wt.%) were then deposited onto the surfaces of one of the mpg-C
3N
4 materials, 22-mpg-C
3N
4-1. After reducing the Cu
2+ ions with NaBH
4, photocatalytically active Cu-modified mpg-C
3N
4 materials, denoted 5Cu-22-mpg-C
3N
4-1 and 10Cu-22-mpg-C
3N
4-1, respectively, were obtained.
The structures of 12-mpg-C
3N
4−
x were first investigated by N
2 porosimetry. The results showed that the surface area and porosity of the materials depended on the initial mass ratio of melamine-to-colloidal silica (12 nm) templates used to synthesize the materials (
Figure 1). Bulk g-C
3N
4, which was synthesized without using colloidal silica templates, exhibited low surface area (3 m
2/g) and non-porous structure (0.04 cm
3/g). When colloidal silica nanoparticles templates were used, the surface area of the materials first increased, from 7 m
2/g for 12-mpg-C
3N
4-0.25 (which was synthesized using melamine-to-silica nanoparticles mass ratio of 0.25) to 136 m
2/g for 12-mpg-C
3N
4-1 (which was synthesized using melamine-to-silica nanoparticles mass ratio of 1), but then decreased to 9 m
2/g for 12-mpg-C
3N
4-4 (which was synthesized using the highest ratio of melamine-to-silica nanoparticles of 4). The pore volume of the materials exhibited a similar trend, namely, it first increased from 0.06 cm
3/g for 12-mpg-C
3N
4-0.25 to 0.27 cm
3/g for 12-mpg-C
3N
4-1, but then decreased to 0.05 cm
3/g for 12-mpg-C
3N
4-4). It is also worth noting that only 12-mpg-C
3N
4-1 (the pore sizes of which are centered at ca. 11.7 nm) showed pores close to the size of colloidal silica templates used to synthesize the material. Low or high melamine-to-silica mass ratio (i.e.,
x = 0.25 or 4) did not result in materials the pore size of which directly correspond to each silica nanoparticle; in both cases, the materials were largely non-porous and had a small amount of large pores.
Based on N
2 porosimetry results presented above, the processes leading to the formation of mpg-C
3N
4 and Cu-loaded mpg-C
3N
4 were proposed as illustrated in
Scheme 2. For the lowest mass ratio of melamine-to-silica nanoparticles (
x = 0.25, where the mass of silica nanoparticles is much higher than that of melamine), the carbonized material does not maintain its porous structure after removal of silica due to the insufficient amount of melamine and the small amount of carbon product forming from it, which can easily collapse. The small proportion of large pores in it seem to replicate some aggregated silica nanoparticles templates. For the highest mass ratio of melamine-to-silica nanoparticles (
x = 4), the lack of many silica nanoparticles templates can inhibit the formation of carbon structures around the particles and thereby the formation of porous carbon structure in the material. In addition, the formation of compact g-C
3N
4 shells around the silica spheres templates, due to the relatively higher amount of melamine used for the synthesis, can prevent ammonium hydrogen difluoride from reaching the silica templates and etching them all. As a result, the silica templates cannot all be removed from the carbonized product and porous structures cannot be formed in this material. This was actually corroborated by thermogravimetric analysis (TGA) (
Figure S1), which clearly revealed that 12-mpg-C
3N
4-4 had higher amount of residue associated with silica (ca. 6.79 wt.%) compared with 12-mpg-C
3N
4-1 (ca. 1.12 wt.%). However, the low surface area in the former was likely to be caused also by the lack of porous structure in the material, since most of the silica was removed, despite a large amount of it being left behind, and yet the material showed low surface area. Based on the above results, the optimal mass ratio of melamine-to-silica nanoparticles for the synthesis of high surface area mpg-C
3N
4 materials with desired pore sizes, i.e., pores corresponding to the size of the silica nanoparticles, was determined to be around 1.
The synthetic procedure was easily extended to produce a series of
y-mpg-C
3N
4-1 materials with different pore sizes (with
y = 12, 22, 47 or 79 nm, representing the different sizes of silica nanoparticles used as templates to create the pores) (
Figure 2). When the sizes of the silica nanoparticles templates used to synthesize the materials were increased, the surface areas of the
y-mpg-C
3N
4-1 materials slightly decreased (from 136 m
2/g to 73 m
2/g), but their corresponding pore volumes increased (from 0.27 cm
3/g to 1.05 cm
3/g). Quantitative results obtained by N
2 porosimetry analyses of the materials are compiled in
Table 1 and
Table 2.
The structures of
y-mpg-C
3N
4-1 materials were further examined by transmission electron microscope (TEM) (
Figure 3a–d). When
x = 1, the material showed pores with sizes of ca. 12 nm (
Figure 3a), corroborating the pore size obtained by N
2 porosimetry for this material (12-mpg-C
3N
4-1) earlier (
Table 1). The TEM images of the
y-mpg-g-C
3N
4-1 materials, which were synthesized by keeping the same
x value but by changing the sizes of the silica nanoparticles templates, clearly showed that all the materials possessed nanoporous structures. However, their pore sizes were highly dependent on the sizes of the silica templates used to synthesize them, and generally increased as the sizes of colloidal silica templates were increased from 12 nm to 79 nm. In addition, TEM images were also acquired for 5Cu-22-mpg-C
3N
4-1 and 10Cu-22-mpg-C
3N
4-1 (
Figure 3e,f). The images of these materials showed many dark spots or areas associated with Cu species. Overall, the N
2 porosimetry and TEM results above clearly indicated that mesoporous g-C
3N
4 materials with high surface area and mesopore sizes could be produced by a facile synthetic method using melamine as precursor and a proper amount of silica nanoparticles as templates. Furthermore, the pore sizes in the materials could be tuned by varying the sizes of the silica nanoparticles used as templates to synthesize the materials.
Since 22-mpg-C
3N
4-1 and Cu-22-mpg-C
3N
4-1 were used as representative materials to evaluate the photocatalytic activity of Cu-doped mpg-C
3N
4 materials for degradation of tartrazine yellow dye, the following characterizations were carried out only for these two materials. Upon increasing the relative amount of Cu
2+ ions used to synthesize the different Cu-22-mpg-C
3N
4-1 materials, the colors of the samples slowly changed from yellow to light green (
Figure 4a). UV-Vis diffuse reflectance spectroscopy (DRS) was used to determine the optical properties of these materials between 250 nm to 800 nm (
Figure 4b). The intrinsic absorption edge of 22-mpg-C
3N
4-1 was found to be ca. 459 nm, which is in line with the value reported for g-C
3N
4 materials in the literature [
22]. After decorating its surfaces with 5 wt.% and 10 wt.% of Cu (producing 5Cu-22-mpg-C
3N
4-1 and 10Cu-22-mpg-C
3N
4-1 materials), the absorption edge shifted to higher wavelengths, to ca. 498 nm and ca. 514 nm, respectively, and the intensity of the absorption band increased; this suggests that the modification of mpg-C
3N
4 with Cu, at least, up to 10 wt.% enhances the material’s ability to absorb visible light [
23].
The band gap energy (
Eg) of the materials were calculated based on the spectra obtained with UV-Vis DRS and using the transformed Kubelka–Munk equation (
Figure 4b):
, where
, where
is the incident photon energy,
is the percentage of reflected light,
is the band gap energy and A is constant, the value of which depends on the transition probability [
24,
25]. The value of
for 22-mpg-C
3N
4-1 was determined to be 2.71 eV, whereas the values of
for 5Cu-22-mpg-C
3N
4-1 and 10Cu-22-mpg-C
3N
4-1 were determined to be 2.49 and 2.41 eV, respectively. This result indicates that the value of
decreases as the amount of Cu in mpg-C
3N
4-1 is increased. These results are consistent with those reported for g-C
3N
4 in the literature, where a steady decrease in band gap energy is observed as more metal is loaded on g-C
3N
4 [
26,
27,
28]. Overall, the DRS results suggested that Cu/mpg-C
3N
4 composite materials have significantly improved light absorption; they can thus be potentially better photocatalysts compared with pure g-C
3N
4.
The amount of Cu in Cu-22-mpg-C
3N
4-1 was estimated by comparing the weight of the residue that remained in Cu-mpg-C
3N
4 at the end of thermogravimetric analysis (TGA) in air with respect to that of 22-mpg-C
3N
4-1 (
Figure 5). While 22-mpg-C
3N
4-1 gave ca. 1.12 wt.% residue, which is associated with residual silica, since the C
3N
4 in it should be lost in the form of CO
2 and NO
2 during calcination, 5Cu-22-mpg-C
3N
4-1 and 10Cu-22-mpg-C
3N
4-1 gave ca. 6.07 wt.% and 12.24 wt.% residue, which should be largely due to CuO. From these values, the amounts of Cu in 5Cu-22-mpg-C
3N
4-1 and 10Cu-22-mpg-C
3N
4-1 were determined to be ca. 3.73 wt.% and 8.68 wt.%, respectively. In addition, it is worth noting that the presence of Cu NPs in mpg-C
3N
4 facilitated the materials’ thermal decomposition. While 22-mpg-C
3N
4-1 was stable up to ca. 480 °C in air and decomposed only in the range of 480–625 °C, the Cu-functionalized counterparts, 5Cu-22-mpg-C
3N
4-1 and 10Cu-22-mpg-C
3N
4-1, decomposed in lower temperature ranges of 440–575 °C and 390–560 °C, respectively. Furthermore, the decreased thermal stability of Cu-22-mpg-C
3N
4-1 materials compared with mpg-C
3N
4-1 indirectly indicated the successful decoration of the surfaces of mpg-C
3N
4 with Cu nanoparticles. This is not unprecedented as the presence of Cu (metallic) particles has been reported to facilitate heat transfer during calcination and promote the combustion of g-C
3N
4 [
29].
Powder X-ray diffraction (XRD) patterns of 22-mpg-C
3N
4-1 and Cu-22-mpg-C
3N
4-1 materials were obtained to further characterize the materials (
Figure 6). The XRD patterns of 22-mpg-C
3N
4-1 showed two pronounced diffraction peaks centered at ca. 27.5° and 13.0°, corresponding to the (002) and (100) reflections that are due to the interlayer stacking of the graphite-like, conjugated aromatic systems and the in-plane structure repeating motif of trigonal N-linkages of tri-s-triazene in g-C
3N
4, respectively [
5,
30]. This result indirectly confirmed the formation of g-C
3N
4. While the XRD patterns of both Cu-22-mpg-C
3N
4-1 materials showed the prominent peak associated with C
3N
4, they did not show any diffraction peak associated with Cu species, due possibly to either the small size or the high dispersion of the Cu nanoparticles in them [
28]. There is some evidence, at least, for the latter, based on TEM images (
Figure 2e,f). Energy dispersive X-ray fluorescence (EDXRF) was carried out to further determine the amount of Cu in 10Cu-22-mpg-C
3N
4-1 material (
Figure S2). The result showed that not only Cu was present in the material but also its amount was ca. 14.1 wt.%, which is close to what was used for its synthesis. Small angel X-ray scattering (SAXS) pattern of 22-mpg-C
3N
4-1 material (see
Figure S3) showed a Bragg reflection in 2
-region of 0.15°–0.75°, indicating the presence of some ordered pores with d-spacing of ca. 26.1 nm, which is also in line with the results obtained from TEM images and by N
2 porosimetry.
X-ray photoelectron spectroscopy (XPS) analysis was performed to determine the composition of 10Cu-22-mpg-C
3N
4-1 material as well as the chemical states of the elements existing in it. The survey spectrum showed that only C, O, N and Cu were present in the material (
Figure 7a). The C 1s peak in the spectrum showed two peaks centered at ca. 284.3 eV and 288.0 eV, corresponding to sp
2−bonded carbon atoms of C–C and N–C=N groups, respectively (
Figure 7b) [
5]. The N 1s peak in the spectrum was deconvoluted into four peaks with binding energy values of 398.5, 399.9, 401.1 and 404.1 eV, which can be ascribed to sp
2−bonded N atoms of C–N=C species, N atoms in tertiary N–(C)
3 groups, N atoms in N–H moieties and π excitation, respectively (
Figure 7c) [
5,
31]. The oxidation state of Cu was determined on the basis of the position of the Cu 2p
3/2 peak (
Figure 7d). Two peaks at binding energies of ca. 932.4 and 952.2 eV were observed, corresponding to Cu 2p
3/2 and Cu 2p
1/2 of Cu
0 and/or Cu
1+. The additional small peaks observed at ca. 933.9 and 954.0 eV could be assigned to Cu
2+ species, which were likely formed from the oxidation of Cu
0 on the surfaces of the Cu nanoparticles during exposure to air and humidity [
32].
The photocatalytic activities of the materials for degradation of tartrazine yellow dye in solutions, a colorful additive that is widely used in various consumer products worldwide but is also often regarded as a cause of allergies, hyperactivity and even cancer, were evaluated (
Figure 8). The necessary comparative and control experiments were also performed. In one control experiment, the extent of photolysis of tartrazine yellow without the presence of catalyst over an irradiation time of 240 min was found to be only ca. 5.3%. This revealed that the photodegradation of this dye in the absence of a catalyst was very slow. The photodegradation of the dye in the presence of a sample of 22-mpg-C
3N
4-1 was not good either, as only ca. 18.8% tartrazine yellow was photodegraded in the same time period. This suggested that as-synthesized mpg-C
3N
4 was not a good photocatalyst for the degradation of tartrazine yellow. However, the photocatalytic performance of the material for degradation of tartrazine yellow dye in solution was significantly improved after its surfaces were decorated with Cu nanoparticles, especially with about 10 wt.% of Cu nanoparticles. Specifically, the extents of photodegradation of tartrazine yellow dye in 240 min in the presence of 5Cu-22-mpg-C
3N
4-1 and 10Cu-22-mpg-C
3N
4-1 were found to be ca. 32.8% and ca. 81.9%, respectively, which were significantly higher than the one obtained in the presence of 22-mpg-C
3N
4-1. For comparison, the performance of 10Cu-47-mpg-C
3N
4-1 (a material that is synthesized using 47 nm silica nanoparticles as templates but containing the same amount, 10 wt.%, Cu nanoparticles) was also evaluated. This material resulted in ca. 42.5% photodegradation of tartrazine yellow in the same period of time. This material had a surface area is 87 m
2/g, which is lower than that of 10Cu-22-mpg-C
3N
4-1 (i.e., 97 m
2/g). These results suggest that, besides the surface-deposited Cu nanoparticles, higher surface area enhances the ability of Cu-doped mpg-C
3N
4 materials to photocatalytically degrade tartrazine yellow dye in solutions.
During photocatalytic degradation, efficient charge separation is important, because it allows the charges not to be compromised by undesirable charge recombination processes and to participate in various redox reactions. The available photogenerated electrons on the conduction band can then react with O
2 and form superoxide radicals (O
2•−). The resulting superoxide radicals as well as the photogenerated holes will help the photo-oxidative degradation of various compounds [
2,
33,
34]. Unfortunately, plain g-C
3N
4 often suffers from rapid electron-hole recombination, and thus shows negligible photocatalytic activity. However, in the presence of metals such as Cu, which can trap the photogenerated electrons, the recombination rate of the photogenerated electron-hole pairs in g-C
3N
4 is significantly minimized. Hence, not surprisingly, the decoration of mpg-C
3N
4 with Cu nanoparticles facilitated the photodegradation of tartrazine yellow over the materials. In particular, 10Cu-22-mpg-C
3N
4 showed superior photocatalytic activity compared with plain 22-mpg-C
3N
4-1. Although 10Cu-47-mpg-C
3N
4-1 also showed better photocatalytic activity than plain 22-mpg-C
3N
4-1, its activity was inferior to that of 10Cu-22-mpg-C
3N
4-1 (the surface area of which is 97 m
2/g); this was most likely due to its lower surface area (87 m
2/g) and thus less exposed catalytic active sites [
35]. Therefore, it can be said that, in addition to decorating its surfaces with Cu nanoparticles, introducing high surface area in mpg-C
3N
4 can improve the photocatalytic activity of g-C
3N
4 for degradation of tartrazine yellow dye.