2.1. Composition, Structure, and Morphology
In order to examine the morphological features of the samples, the samples were observed by SEM. As can be seen in
Figure 1a, g-C
3N
4 directly obtained by calcination from melamine shows a large bulk structure, which is due to the stacking of g-C
3N
4 layers caused by the interlayer van der Waals force. After thermal treatment in air, the g-C
3N
4 sample presents a measure of spalling owing to the corrosion on the edge of g-C
3N
4 by oxygen at high temperatures. From
Figure 1b, it can be clearly seen that the g-C
3N
4 bulk became smaller after thermal treatment without any other change in morphology. However, the sample treated with ammonium molybdate solution, as shown in
Figure 1c,d, displays a more obvious lamellar structure, which can be attributed to the escape of NH
3 from the thermal decomposition of ammonium molybdate. In addition, it can be seen from
Figure S1 in the
Supporting materials that with increasing amounts of the applied ammonium molybdate, the size of the resultant g-C
3N
4 nanosheets gradually decreases.
In order to further examine the morphology and elemental composition of the samples, TEM characterization was carried out. Compared with the sample CNH (see
Figure 1e), the sample treated with ammonium molybdate exhibits a clearer exfoliation between the layers (
Figure 1f). Meanwhile, TEM mapping scanning was performed on the area of
Figure 1f, and the results are shown in
Figure 1g. As is seen, four elements of C, N, O, and Mo were identified by the system. Among them, the distributions of C and N elements are consistent with the shape of g-C
3N
4 nanosheets as shown in
Figure 1f. However, the Mo and O elements are only of a small amount and evenly distributed on the surface of the g-C
3N
4 nanosheets. In order to find out the scattering feature of molybdenum oxide on the g-C
3N
4 nanosheets, with a small piece of sample at this position, high-resolution TEM (HRTEM) characterization was carried out. Through the HRTEM image (
Figure 1h), it can be observed that some quantum dots with a diameter of about 2–3 nm are distributed on the surface of the nanosheets. Although their crystallinity is not very fine, a small number of lattice stripes can still be identified on the quantum dots, which could be indexed to the MoO
2 (110) crystal plane. From the above results, it can be inferred that the thermally treated g-C
3N
4 is effectively exfoliated into thinner nanosheets, and a small amount of MoO
2 quantum dots are loaded on the surface of the g-C
3N
4 nanosheets.
Typical XRD patterns of the bulk g-C
3N
4, CNH, and CNM sample are shown in
Figure 2a. It can be seen from this figure that all the samples contain the two characteristic peaks of g-C
3N
4. The peak around 13.2° is indexed to the (100) crystal plane of g-C
3N
4 (0.671 nm), which represents the tri-s-triazine repeating unit in the g-C
3N
4 plane, while the peak around 27.6° is attributed to the (002) crystal plane of g-C
3N
4 (0.323 nm), signifying the interlayer stacking conjugated aromatic system of g-C
3N
4 in the vertical direction [
13,
16]. Remarkably, compared with those of bulk g-C
3N
4, the strengths of these two peaks of the other samples are relatively low. This result can be interpreted as the spalling between g-C
3N
4 layers and plane fracturing, which would cause the structural damage of the g-C
3N
4 crystal [
12]. Obviously, due to the interlayer separation caused by the escape of NH
3, the four composite samples from CNM-1 to CNM-8 have weaker XRD peaks, and this fact further verifies that the processes presented in this work can peel g-C
3N
4 effectively. However, the peak of MoO
2 cannot be identified from these patterns because MoO
2 in these samples exists in the form of quantum dots with a high degree of dispersion, poor crystallinity, and a small molar fraction. In order to confirm the phase composition of molybdenum oxide in the samples, a large number of composite samples were collected from the Al
2O
3 ceramic boat after the synthesis processes, and another 3 h of thermal treatment under air was performed, which was intended to thermally decompose g-C
3N
4 for enriching molybdenum oxide. The enriched samples were characterized by XRD, and the result is shown in
Figure 2b. It can be clearly seen in this figure that the peaks corresponding to the MoO
2 phase are consistent with standard PDF card no. 78-1072.
In order to investigate the elemental composition and chemical state of the composite samples, XPS analysis on them was performed. Since the XPS spectra of the prepared series of composite samples are similar, only the spectra of the optimal sample CNM-4 are displayed. Through the XPS survey spectrum (see
Figure S2), it can be seen that the composite sample is composed of C, N, Mo, and O. From the high-resolution spectra (
Figure 3), the chemical state of each element in the composite can be further understood. In the C 1s spectrum (
Figure 3a), two peaks centered at the binding energies of 284.77 and 288.22 eV can be observed in the sample, which are attributed to the free carbon for instrument calibration and the C element in N-C=N, respectively [
26]. For comparison, the high-resolution C 1s spectrum of bulk g-C
3N
4 was also presented in this figure. It is seen that this spectrum has the same peaks at similar positions as that of the optimal sample CNM-4. The only difference between these two spectra is that the binding energy of CNM-4 at 288.22 eV is 0.18 eV higher than that of bulk g-C
3N
4, due to the inductive effect of the O atoms, which are connected to the g-C
3N
4 structure caused by the thermal oxidation process. In addition, in the N 1s spectrum of the sample CNM-4 (
Figure 3b), four peaks with binding energies of 398.69, 399.34, 401.05, and 404.35 eV can be fitted, representing N atoms in C-N=C, N-(C)
3, and C-N-H structures in the g-C
3N
4 framework as well as free N
2 adsorbed from air, respectively [
26]. Similarly, the peaks in the N 1s spectrum representing the g-C
3N
4 structure in the sample CNM-4 are shifted to the high value of binding energies by about 0.3 eV compared with those of bulk g-C
3N
4, which is due to the inductive effect of the O atoms connected with the g-C
3N
4 structure. On the basis of the chemical states of C and N elements discussed above, it can be concluded that the composite does contain g-C
3N
4. As for the Mo 3d spectrum of the optimal sample CNM-4 (
Figure 3c), there are three groups of peaks with binding energy at 230.30 and 233.31 eV, 231.36 and 235.30 eV, as well as 232.27 and 236.37 eV, representing the electron spin splitting of 3d
5/2 and 3d
3/2 of Mo
4+, Mo
5+, and Mo
6+ in the composites, respectively [
20,
27]. The XPS spectrum of the Mo element revealed that the oxidation state of Mo atoms in the composites involved Mo
4+, Mo
5+, and Mo
6+, with the Mo
5+ and Mo
6+ states attributed to the Jahn–Teller effect caused by lattice distortion [
28]. This result is consistent with the XPS Mo spectrum of pure MoO
2, also shown in
Figure 3c. Thus, it can be concluded that the molybdenum oxide in the optimal sample CNM-4 is composed of MoO
2. From the XPS spectrum of O 1s (
Figure 3d), three peaks centered at the binding energies of 520.21, 531.98, and 533.31 eV could be observed, which can be assigned to the oxygen element in MoO
2, the N-C-O structure, and free H
2O, respectively [
27]. Compared with the XPS spectrum of bulk g-C
3N
4, the O peak area representing N-C-O in the sample CNM-4 displays an obvious increase, which can be attributed to the O atoms introduced into the g-C
3N
4 structure by thermal oxidation.
In addition, the content of each element in the prepared samples in this work was calculated based on XPS analysis and is listed in
Table 1. It can be seen that C and N elements account for the main components in each sample, and the atomic ratio of C to N is close to 3:4. Thus, it is believable that the main component of these samples is g-C
3N
4. Furthermore, the content of Mo in these samples increased gradually as the concentration of ammonium molybdate in the precursor solution used for the thermal treatment increased. Additionally, the content of O element is clearly increased, which is more than twice the content of Mo element, indicating that, in addition to the O atoms in the introduced MoO
2, there are additional O atoms in the samples. This result should be attributed to the O atoms introduced into g-C
3N
4 that is combined directly with the g-C
3N
4 structure in the samples by the oxidation reaction during the thermal treatment in air. In addition, the increase in oxidation degree reflects the destruction of the intermolecular force between g-C
3N
4 layers by the gases produced by the decomposition of ammonium molybdate. In other words, when O
2 can enter the g-C
3N
4 layers smoothly, the oxidation process will be further accelerated. In summary, through the XPS analysis of the composite samples, it can be concluded that such samples are composed of O-doped g-C
3N
4 and MoO
2.
To further explore the internal pore structure in the composite samples, a set of N
2 adsorption-desorption tests were conducted on bulk g-C
3N
4, CNH, and this series of CNM composite samples. The recorded N
2 adsorption-desorption isotherms are shown in
Figure 4a. Based on them, the specific surface area (S
BET), pore diameter, and pore volume of the samples were calculated. The results are listed in
Table 2, in which the pore diameter distribution is also displayed in
Figure 4b. Firstly, comparing the S
BET values of the samples (see
Table 2) with that of the bulk g-C
3N
4 (12.34 m
2·g
−1), the sample CNH shows a larger S
BET value of 55.65 m
2·g
−1, which can be attributed to the oxidation of g-C
3N
4 by O
2 from air [
13]. The S
BET values of CNM-1, CNM-2, CNM-4, and CNM-8 samples were 102.91, 89.67, 96.17, and 116.32 m
2·g
−1, respectively, which were much larger than those of CN and CNH samples. Based on the above facts, the increase in specific surface area can be attributed to the spalling effect of ammonia produced by the decomposition of ammonium molybdate in the g-C
3N
4 layers and O
2 corrosion of g-C
3N
4 [
14]. Then, the pore size distribution of the samples was examined (see
Figure 4b). Compared with that of the bulk g-C
3N
4, the CNH sample has more pores with a large pore size of about 10~50 nm but fewer pores with a small pore size of roughly 3.833 nm, indicating that partial small pores are expanded into large mesopores under the erosion of O
2. The change of small pores into large pores will lead to an increase in specific surface area and pore volume. Moreover, the pore diameter of the sample CNM-1 increases in both ranges, which can be explained by the fact that the escape of NH
3 produces a large number of micro/mesopores and oxygen corrosion simultaneously. Furthermore, with an increasing concentration of ammonium molybdate in the precursor solution, the pore diameter distribution changed significantly. After examining the pore diameter of CNM-2, CNM-4, and CNM-8, it can be seen that more small-pore-size mesopores and fewer large-pore-size micropores are built in the samples. This phenomenon may be attributed to two factors. On the one hand, because the escape of more ammonia reduced the local oxygen concentration in the sample, the oxidation of g-C
3N
4 was limited, thereby restraining the further expansion of pores. On the other hand, after more MoO
2 was deposed into the large pore, part of the large pore was blocked into small ones. As a result, there are more small pores and fewer large pores after adding more (NH
4)
2MoO
4·4H
2O.
2.2. Synthesis Strategy and Formation Mechanism
According to the above characterization results of the samples, the synthesis strategy and formation mechanism of the CNM composite samples are proposed in
Figure 5. As shown in
Figure 5a, initially, bulk g-C
3N
4 was dispersed in ammonium molybdate solution under stirring in order to fully adsorb MoO
42− and NH
4+ on the g-C
3N
4 sheet. Considering that the radius of NH
4+ is 0.142 nm and that of MoO
42− is 0.192 nm, as well as from XRD data, the calculated radius of the small ring in the g-C
3N
4 sheet is 0.134 nm and the diameter of the large pot is 0.671 nm, the NH
4+ and MoO
42− ions in the precursor solution can only enter into the large pot in the g-C
3N
4 sheet [
29,
30], as shown in
Figure 5b. Then, after centrifugation, the precipitate was collected and dried, obtaining the precursor for the preparation of the target sample. Finally, the precursor was placed in an Al
2O
3 ceramic boat and heated under an air atmosphere in a tube furnace to obtain the target sample. According to thermogravimetric analysis data of the precursors (see
Figure S3), the samples with ammonium molybdate began to lose weight at around 450 °C and completely decomposed after 600 °C, whereas the original g-C
3N
4 sample began to lose weight after 500 °C and completely decomposed at 700 °C. Therefore, it can be deduced that the presence of ammonia would reduce the decomposition temperature and increase the decomposition rate of g-C
3N
4. Based on these facts, the formation mechanism of the present CNM samples can be proposed as follows (
Figure 5b). MoO
42− and NH
4+ ions entered into the interlayer of bulk g-C
3N
4 and further entered into the large pot in the g-C
3N
4 lamellas. In the process of thermal treatment, the ammonium molybdate absorbed between the g-C
3N
4 nanosheets is decomposed. During this process, NH
4+ is transformed into ammonia, and the escape of ammonia will destroy the van der Waals forces between g-C
3N
4 molecular layers, finally leading to exfoliated layers of g-C
3N
4. On the other hand, the amount of ammonia generated in the g-C
3N
4 nanosheets cannot diffuse out immediately and forms a reductive environment. Thus, MoO
42− was decomposed into MoO
3 initially, which was then converted into MoO
2 at 500 °C in the reductive ammonia atmosphere [
28]. At the same time, O
2 in the air flow diffuses into the g-C
3N
4 interlayer and oxidizes g-C
3N
4, forming numerous pores of larger size in g-C
3N
4 (see
Figure 5c). Finally, the proposed g-C
3N
4/MoO
2 composites are formed.
2.3. Photocatalytic H2 Evolution Performance
The photocatalytic performance was evaluated by measuring the photocatalytic hydrogen evolution ability over the samples under visible light, and the results are displayed in
Figure 6.
Figure 6a clearly shows that the HER of the samples CNH and CNM-1 to CNM-8 increases with increasing ammonium molybdate concentration in the pre-cursor solution, reaching a maximum value of 320.8 μmol·g
−1·h
−1 when the ammonium molybdate concentration is 4 mmol·L
−1. However, under the same conditions, the photocatalytic HER of a bulk g-C
3N
4 sample is only 78.4 μmol·g
−1·h
−1. In other words, the performance of the optimal sample CNM-4 in this work is 4.1 times that of bulk g-C
3N
4. Therefore, it can be confirmed that the improved performance of the composite samples is due to the increasing amount of MoO
2 in the samples and their enhanced specific surface area. Compared with CNM-4, the photocatalytic HER of the sample CNM-8 would be significantly reduced because the band gap of C
3N
4 in CNM-8 reaches 3.02 eV, which can only absorb light with a wavelength below 410 nm. However, because a 400 nm filter was used to cut off the UV light source below 400 nm in this work, the shortage of the available light for the sample CNM-8 would certainly result in the decline of its hydrogen evolution performance. Consequently, although a higher concentration of ammonium molybdate can be beneficial for both enhancing the amount of MoO
2 and producing more pores in the sample CNM-8, the intensified oxidation of bulk g-C
3N
4 will widen the band gap of g-C
3N
4, making it impossible to make effective use of visible light. In addition, compared with bulk g-C
3N
4, although the sample CNH will lose partial absorption capacity of visible light sources due to the oxidation of g-C
3N
4, its photocatalytic hydrogen evolution performance was still improved significantly. This result can be attributed to the exposure of more active sites caused by the expansion of a specific surface area. The as-prepared composite samples thermally treated with ammonium molybdate show more excellent photocatalytic hydrogen evolution performance because of their larger specific surface area and more abundant mesopores in the samples. Based on the above results, it can be concluded that the improvement of photocatalytic hydrogen evolution performance of the present g-C
3N
4/MoO
2 composite samples is caused by a synergistic effect of the MoO
2 recombination with g-C
3N
4 and the increase in specific surface area. However, it has to be noted that excessive oxidation will reduce the light absorption range of g-C
3N
4, which will ultimately finally lead to a decline in the photocatalytic hydrogen evolution performance of the samples.
Moreover, whether a photocatalyst can work stably for a long time is also very important for its practical application. Therefore, cyclic stability tests were performed for the optimal sample CNM-4 under the same conditions as described above. Notably, the cyclic stability tests consist of 5 rounds of a 3 h photocatalytic hydrogen evolution process, for which the system should be re-evacuated after each run. From the test results shown in
Figure 6b, it can be concluded that the sample CNM-4 has good stability for photocatalytic hydrogen evolution, since the sample can still maintain stable, high hydrogen evolution efficiency after five rounds of tests.
2.4. Photoelectrochemical Properties
In order to characterize the absorption ability of the prepared materials for light, the UV-Vis absorption spectra of bulk g-C
3N
4, CNH, and all the g-C
3N
4/MoO
2 composite samples were measured.
Figure 7a shows the recorded spectra of these samples. As shown in the figure, when compared to bulk g-C
3N
4, after thermal treatment, the resultant samples CNH and CNM would have a lower light absorption capacity due to their widened band gap. Moreover,
Figure 7b displays their corresponding (ahν)
2 versus E
g plots, from which the band gap of the corresponding materials can be obtained. As can be seen, the band gap of the sample bulk g-C
3N
4, CNH, and CNM-1–CNM-8 is 2.78, 2.88, 2.86, 2.94, 2.96, and 3.02 eV, respectively, which can be attributed to the changed structure caused by the increased degree of oxidation on g-C
3N
4. The band gap of g-C
3N
4 is excited by π-π * excitation, in which the conjugated C 2p and N 2p orbitals in the heptazine form the conduction band, while the 2p orbitals of the edge N atoms form the valence band [
31]. However, the oxidation of g-C
3N
4 will break the C=N bond conjugated structure into an N-C-O bond, resulting in an expanded band gap of g-C
3N
4 in the sample. Although the band gap of the samples CNM-1–CNM-4 continues to increase, their light absorption capacity becomes stronger and stronger, which can be attributed to the increased loading amount of MoO
2 in the sample. On the other hand, the sample CNM-8 shows a poor light absorption capacity due to the greatly widened band gap of g-C
3N
4 caused by excessive oxidation.
To explain the photocatalytic activity for hydrogen evolution of the prepared samples, their photoelectric response ability and carrier transport ability were investigated by transient photocurrent response and electrochemical impedance tests.
Figure 8a shows the transient photocurrent response curves of all the samples. From this figure, it can be clearly seen that the optimal sample CNM-4, which presents the highest efficiency for photocatalytic hydrogen evolution, also has the strongest photocurrent response ability. It is easy to understand that its photocurrent intensity is stronger than those of the samples CNM-1 and CNM-2 because it contains more MoO
2. Because the loaded MoO
2 can effectively separate photogenerated electrons and holes, more free electrons will be converted into current without becoming internal energy after the compositing of MoO
2 with g-C
3N
4. However, the photocurrent intensity of CNM-8 with the highest content of MoO
2 is attenuated, which is obviously due to the poor light utilization ability of CNM-8, because it can only make use of the light in the band range between 400–410 nm after the light with a wavelength shorter than 400 nm is filtered. In addition, it is seen that the photocurrent intensity of bulk g-C
3N
4 is stronger than that of the sample CNH, because the widening of the band gap after the oxidation of g-C
3N
4 will result in a poor utilization efficiency of light.
The EIS Nyquist plots of all the samples obtained from the electrochemical impedance test are shown in
Figure 8b. Obviously, the impedance of all the samples after thermal treatment decreased with the increase of the MoO
2 content in them. This phenomenon shows again that the compositing of MoO
2 with g-C
3N
4 is conducive to the transfer of photogenerated carriers through the photocatalyst. Additionally, this result can be attributed to the following two reasons: firstly, MoO
2 has better electrical conductivity than g-C
3N
4, and another reason is that the compositing of g-C
3N
4 with MoO
2 forms a built-in electric field, which is also conducive to charge transmission. The resultant lower impedance is beneficial to improving the transmission efficiency of photogenerated carriers, preventing them from recombination, effectively improving the photocatalytic performance. In addition, the impedances of CNH and CNM-1 are higher than that of bulk g-C
3N
4, which is because the impedance depends on both g-C
3N
4 and MoO
2. The impedance of g-C
3N
4 would be increased after it was oxidized, while the deposition of MoO
2 with good electrical conductivity would decrease the impedance of the samples. The impedance of the samples is actually a balanced result between the oxidation of g-C
3N
4 and the deposition of MoO
2. Consequently, the impedance of CNH is higher than that of bulk g-C
3N
4 due to the oxidation of g-C
3N
4. The impedance of CNM-1 is higher than that of bulk g-C
3N
4 because the deposition of a small amount of MoO
2 cannot compensate for the counteracting effect of the oxidation of g-C
3N
4. In summary, the increase in MoO
2 content in the composites can effectively reduce the impedance of the samples, while the oxidation of g-C
3N
4 will increase the impedance of the samples. Therefore, it is the superposition of the two factors that determines the final impedance of the samples.
2.5. Photocatalytic Mechanism
Based on the results mentioned above and the support of relevant theories, the photocatalytic hydrogen evolution mechanism over the obtained photocatalysts was proposed in
Figure 9. In order to obtain the energy band correlation between g-C
3N
4 and MoO
2 in the figure, with the optimal sample CNM-4 as an example, Mott-Schottky plots, VB-XPS spectra, and UV-Vis absorption spectra were carried out, and the results are displayed in
Figure S4. In this study, the flat band potentials of CNM-4 and MoO
2 can be obtained from the recorded Mott-Schottky plots, which are −0.53 and −0.52 eV, respectively. After eliminating the influence of the potential from the Ag/AgCl reference electrode, their final flat band potential values are −0.31 and −0.30 eV, respectively [
32]. From the VB-XPS spectra, the potential differences in the energy bands of CNM-4 and MoO
2 from the valence band top to the Fermi level are 2.02 and 0.23 eV, respectively [
33]. In general, the flat band potential value is approximately equal to the Fermi level [
32,
34]. Based on the above data, it can be calculated that the valence band values of CNM-4 and MoO
2 are 1.72 and −0.07 eV, respectively. In addition, the band gap of CNM-4 and MoO
2 could be obtained from
Figure 7b and
Figure S4, and the calculated values of their valence bands are −1.24 and −1.80 eV, respectively. Finally, according to the energy band data obtained from the test, the photocatalytic hydrogen evolution mechanism was proposed.
As is seen, three factors are considered to influence the photocatalytic hydrogen evolution performance of g-C3N4/MoO2 composite. The first is the heterojunction between g-C3N4 and MoO2, which can form a built-in electric field there and promote the separation of photogenerated electrons and holes, preventing them from recombination. Under the irradiation of visible light, the photocatalyst was excited to generate lots of free electrons and holes. The photogenerated electrons in the conduction band of g-C3N4 pass across the heterojunctions through the connected Fermi level due to the energy difference between the two sides of the heterojunction into MoO2, which can combine with the holes in the valence band of MoO2, where a depletion layer is formed. As a result, the counteraction of electrons was prevented, thus retaining the holes in the valence band of g-C3N4 and the electrons in the conduction band of MoO2. These free photogenerated electrons will further rapidly move to the Pt particles deposited on the surface of the catalysts and attend to the redox reaction with H+ in the solution to produce hydrogen. Meanwhile, the photogenerated holes in g-C3N4 can react with TEOA to be quenched. Of course, the transfer process of carriers from conduction band to conduction band and/or from valence band to valence band in such a Type II heterojunction may also be in question. Nevertheless, if the electrons in the valence band of g-C3N4 are transferred to the valence band of MoO2, the total oxidation potential of the catalyst will decrease dramatically. As a result, it is unable to react with TEOA. So, such a process was almost impossible during the photocatalytic process over the present composite catalyst. In other words, the formation of heterojunctions promotes the photocatalytic hydrogen evolution of the present composite catalyst.
The second factor is the exfoliation of g-C3N4, which can effectively increase the specific surface area and form numerous mesopores in the catalyst. A larger specific surface area is conducive to the exposure of active sites in a catalyst, and the formation of more mesopores is advantageous to the adsorption of reaction substrates and the release of the formed hydrogen. This point explains the improvement in the photocatalytic hydrogen evolution performance of the samples CNM-1–CNM-8.
Finally, the oxidation of g-C3N4 during thermal treatment causes the π-π conjugated structures in the heptazine group to be destroyed, which will widen the band gap. With the increasing oxidation degree, the band gap of the samples increases gradually. As a result, the band wavelength of visible light that can be used for photocatalytic hydrogen evolution will be narrowed, ultimately degrading the photocatalytic performance of the sample.
In summary, the photocatalytic hydrogen evolution performance of the present g-C3N4/MoO2 samples is affected by three factors: the loading amount of MoO2, the extent of exfoliation, and the degree of g-C3N4 oxidation. Among them, high MoO2 content and full exfoliation are conducive to photocatalysis, but the oxidation of g-C3N4 is also intensified with increasing content of MoO2 in the sample. Therefore, the sample CNM-4 instead of CNM-8 is the optimal sample for photocatalytic hydrogen evolution by adjusting the synthesis and application conditions.