Abstract
Photocatalytic hydrogen evolution is considered as one of the promising pathways to settle the energy crises and environmental issues by utilizing solar energy. In this paper, noble-metal-free Ni2P was used as cocatalyst to enhance g-C3N4 for photocatalytic hydrogen production under visible light irradiation (λ > 420 nm). Characterization results indicated that Ni2P nanoparticles were successfully loaded onto g-C3N4, which can significantly contribute to accelerate the separation and transfer of photogenerated electron. The hydrogen evolution rate reached ∼ 270 µmol h−1 g−1 and the apparent quantum yield (AQY) was ∼ 2.85% at 420 nm. Meanwhile, there is no obviously decrease of the hydrogen production rate even after 36 h under visible light illumination. In addition, the mechanism of photocatalytic hydrogen evolution was also elaborated in detail.
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1 Introduction
With aim to solve the urgent energy crisis and environmental issues in the worldwide, numerous novel and clean energy technologies were proposed [1,2,3]. Compared with these technologies, photocatalytic water splitting into hydrogen is widely considered as an ideal process for inexhaustible solar energy storage using semiconductors as photocatalysts [4,5,6]. As we all known, the photoelectrochemical cell (PEC) system for water splitting on TiO2 photoanode under UV light has been first developed by Fujishima and Honda in 1972 [7]. Due to the obvious shortcomings of TiO2 photocatalyst, such as wide band gap and low quantum yields [8,9,10]. Therefore, seeking a visible light responded photocatalyst for hydrogen generation, which possesses the characteristic of high efficiency and good stability, has become a new research hot topic in the field of solar energy conversion [11].
Very recently, a conjugated metal-free photocatalyst for hydrogen evolution, namely graphitic carbon nitride (g-C3N4), has drawn intensive interdisciplinary attentions owing to their moderate band gap (Eg = 2.7 eV), suitable band-edge positions, physicochemical stability, and fascinating electronic property and so forth [12,13,14]. Nevertheless, the fast recombination rate of photo-generated electron–hole pairs and low quantum efficiency restricted the photocatalytic performance of g-C3N4 [15, 16]. To date, a great deal of attempts has been made to enhance the photocatalytic hydrogen evolution in water of g-C3N4. For example surface modification [17], nano/mesoporous structures introduction [18, 19], metal element doping [15, 20], nonmetal elements doping [21], hetero-structured fabrication [22, 23], and so on. Among these strategies, loading cocatalysts on the surface of g-C3N4, is considered as one of the most efficient method to promote the charge separation efficiency and provides active sites for H2 production reaction [24, 25].
More recently, development of transition metal phosphide (CoP, Ni2P, Cu3P, Fe2P, MoP) to replace noble metal cocatalysts (including Pt, Au, Rh, Ru) for water splitting catalysis receives considerable attentions from researchers owing to their special metallicity and electrical conductivity [26,27,28,29,30,31]. At present, Ni2P has been used as excellent cocatalyst for semiconductor photocatalyst. For instance our group reported that Ni2P as a cocatalyst onto CdS NRs for photocatalytic hydrogen evolution rate reached ~ 1200 µmol h−1 mg−1 visible light, which shows extraordinarily high activity and great stability [26].
Herein, in this work, we report the noble-metal-free Ni2P as an active cocatalyst on g-C3N4 semiconductors surface by in situ phosphidation method, and the hydrogen production rate has greatly improved irradiated with visible light and the AQY was ∼ 2.85% at λ = 420 nm. Photoluminescence (PL) spectra and photoelectrochemical properties revealed that Ni2P can rapidly transfer the photogenerated charge carriers of g-C3N4 and is a proven efficient cocatalyst for photocatalytic hydrogen production. Furthermore, the photocatalytic hydrogen evolution mechanism based on Ni2P/g-C3N4 composition was proposed and also discussed in detail.
2 Experimental Details
2.1 Reagents
All the reagents (analytical grade), including sodium sulfide nonahydrate (Na2S·9H2O, 98.0% purity), nickel nitrate hexahydrate [Ni(NO3)2·6H2O, 98% purity], anhydrous sodium sulfate (Na2SO3, 97.0% purity), urea [CO(NH2)2, 99% purity], sodium hypophosphite (NaH2PO2·H2O, 99% purity), and ascorbic acid (C6H8O6, 99.7% purity), triethanolamine (C6H8O6, 98% purity), were all purchased from Aldrich or Aladdin Reagent Co., Ltd. (China) and used without further purification.
2.2 Synthesis of the Photocatalysts
g-C3N4 was synthesized by a slightly modification based on a previous reports [32, 33]. In a typical procedure, 4.00 g of urea was calcined at 550 °C for 4 h in N2 atmosphere, and the resultant product was obtained after milling.
g-C3N4 was decorated with different amount of Ni2P were synthesized by annealing the mixture of Ni(NO3)2·6H2O, NaH2PO2·H2O and g-C3N4 in inert atmosphere. The content of Ni2P in the obtained samples was 0 wt%, 0.3 wt%, 0.62 wt%, 3.36 wt%, 5.98 wt% and 13.38 wt%, which were determined by ICP-AES measurements, and denoted as NC-1, NC-2, NC-3, NC-4, NC-5, and NC-6, respectively. For comparison, Ni2P nanoparticles were also prepared using the same method in the absence of g-C3N4.
3 wt% Pt/g-C3N4 was synthesized through photodeposition process using H2PtCl6 as Pt source according to the previously reported literature [34].
2.3 Characterization
All the photocatalyst samples were systematically investigated by powder X-ray diffraction (XRD, D/max-TTR III, 5° min−1 from 10° to 70° in 2θ), Scanning electron microscope (SEM, SIRION200, equipped with an electron diffraction), Transmission electron microscopy (TEM, JEM-2010, acceleration voltage of 200 kV), High-resolution transmission electron microscopy (HR-TEM, JEM-2010, acceleration voltage of 200 kV), UV–Vis spectrometer (SOLID 3700) and X-ray photoelectron spectroscopy (XPS, ESCALAB 250).
2.4 Photocatalytic Hydrogen Production Reactions
The photocatalytic activity reactions were performed in a 50 mL flask with magnetic stirring at room temperature using A 300 W xenon lamp as the irradiation source, which equipped with a UV cut-off filter (λ > 420 nm), and the photocatalytic hydrogen production was quantified by gas chromatography (GC, SP6890, TCD detector, high purity N2 as a carrier gas, 5 Å molecular sieve column). For long-term photocatalytic stability under visible light irradiation, 5.0 mg of the photocatalyst sample was ultrasonic dispersed in 20 vol% TEOA aqueous solution in 250 mL flask. The apparent quantum efficiency was calculated using a 300 W Xe lamp with a band-pass filter (λ = 420 nm). A calculation of AQY was performed using following equation.
3 Results and Discussion
The crystal structure of pure g-C3N4, pure Ni2P and Ni2P/g-C3N4 composites with different amount of Ni2P contents (0 wt%, 0.3 wt%, 0.62 wt%, 3.36 wt%, 5.98 wt%, and 13.38 wt%) were studied by X-ray diffraction. As shown in Fig. 1, the characteristic peaks at 2θ values of 13.08° and 27.4° can be indexed to (100) and (002) crystalline planes of pure g-C3N4, with graphitic structure (JCPDS#87-1526) [12], and the characteristic peaks at 2θ values of peaks at 40.6°, 44.5°, 47.3°, 54.1°and 72.1°can be indexed to (111), (110), (201), (210), and (300) planes of hexagonal pure Ni2P (JCPDS#74-1385) [35]. Meanwhile, the g-C3N4/Ni2P samples with different amount of Ni2P contents (NC-1, NC-2, NC-3, NC-4 and NC-5) display similar XRD pattern with pure g-C3N4, and no obvious change can be found with the Ni2P, probably due to its low content and strong diffraction peaks of the pure g-C3N4. This result also indicated that the crystal structure of pure g-C3N4 was not changed after modification with Ni2P.
The morphologies and material compositions of pure g-C3N4 and sample NC-4 were further identified by SEM, TEM and EDX. As shown in Fig. 2a, pure g-C3N4 displays a typical lamellar structure, and the sample NC-4 has a structure of nanoparticles closely anchored on the surface of the g-C3N4 nanosheets (Fig. 2b, c). In addition, the EDX spectrums (Fig. 2d) clearly reveal the existence of Ni and P elements, suggesting that Ni2P nanoparticles were successfully loaded onto the g-C3N4 surface. From the TEM image of sample NC-4 (Fig. 2e), it is found that Ni2P nanoparticles are deposited on g-C3N4 surface evenly. Figure 2f shows the HR-TEM image of Ni2P composites. The lattice fringes of 0.51 nm can be assigned to the (100) plane of hexagonal pure Ni2P [36]. Thus, these results further show that Ni2P nanoparticles were successfully loaded onto the g-C3N4 nanosheets.
The oxidation states and composition of the photocatalyst sample NC-4 were further confirmed using XPS spectrum. The survey XPS scan spectrum in Fig. 3a clearly shows the existence of Ni, P, C, O and N elements, as well as O element from the absorbed gaseous molecules. Due to the low content of Ni2P loading, the weak XPS signals were observed for Ni 2p and P 2p, which further confirm the formation of Ni 2p in the hybrids, triazine rings (C–N=C) and the tertiary nitrogen N–(C)3 groups, respectively [37]. In high resolution XPS spectrum of C 1s (Fig. 3b), two deconvolution peaks at 284.6 and 288.0 eV are observed, which are assigned to graphite C–C bonds and sp2-hybridized carbon in N-containing aromatic ring (N–C=N), respectively. The latter is considered as the major carbon species in g-C3N4. For the Ni 2p region, three peaks are seen at 853.2, 856.7 and 862.5 eV (Fig. 3e), which is ascribed to Niδ+ (0 < δ < 2) in Ni 2p, oxidized Ni species (Ni2+) and the satellite of the Ni 2p1/2 peak, respectively. In addition, the other three peaks at 869.5 eV, 874.1 eV and 879.8 eV is corresponding to Niδ+ in Ni 2p, oxidized Ni species and the satellite of the Ni 2p3/2 peak, respectively. For the P 2p energy level (Fig. 3f), the peak at 129.7 eV is a mark of metal-P bonds in metalphosphides (For example, Ni2P), while the peak at 132.9 eV can be attributed to the oxidized P species due to air contact [26].
The light harvesting properties of the pure g-C3N4 and NC-4 were measured by UV–Vis diffuse reflectance spectroscopy and PL spectroscopy. As depicted in Fig. 4a, the pure g-C3N4 sample has a sharp absorption edge at approximately 470 nm, corresponding to a band gap of ∼ 2.65 eV (Fig. 4b), which is consistent with typical C materials in many previous reports [12], No obvious band-gap absorption structure throughout the UV–Vis region is observed for the pure Ni2P nanoparticles, indicating a typical metallic character. As for sample NC-4, the absorption band in the region less than 470 nm is similar to that of pure g-C3N4 and the absorption band in the region from 470 to 700 nm is strengthened because of the presence of Ni2P, indicating that Ni2P was not doped into the g-C3N4 crystal lattice to change its band gap.
Figure 4c shows the PL spectra of pure g-C3N4 and sample NC-4. For pure g-C3N4, at an excitation wavelength of 350 nm, two distinct emission bands peaking at about 450 nm and 490 nm can be observed, which are probably due to near-band emission and surface trap state emission, respectively [38, 39]. The two peaks are remarkably quenched after loading Ni2P onto g-C3N4, probably due to the fast transfer of photogenerated electrons from g-C3N4 to Ni2P, indicating that the Ni2P cocatalyst helps the transfer of charge carriers and slows down the recombination process. The photocatalytic activity for hydrogen production can be improved.
The reducing power of sample NC-4 can be evaluated by using organic electron acceptors methyl viologen dication (MV2+). When the methyl viologen dication (MV2+) was added to an aqueous solution containing TEOA, and 10 µg mL−1 sample NC-4 under visible light irradiation, the solution’s color rapidly changed from light white to blue and a characteristic absorption spectrum of the methyl viologen radical cation (MV+˙) appeared (Fig. 5a). This phenomenon indicated the formation of MV+˙ and the fast electron transfer from the photocatalyst NC-4 to MV2+˙. In addition, a diquat (DQ2+, N,N′-(1,3-propylene)-5,5′-dimethylbipyridine dication) was also used as an electron acceptor, which has a more negative reduction potential (-0.7 V vs. NHE) than MV2+. The result showed a rapid color change from light white to yellowish-brown and the appearance of the characteristic absorption spectrum of DQ+˙, suggesting that the reduction potential of NC-4 is more negative than − 0.7 V versus NHE, and thus the reducing power of the photo-excited electrons is sufficient for H+ reduction to produce H2 (Fig. 5b).
Photocatalytic hydrogen production experiments were carried out in TEOA aqueous solution. The rates of hydrogen production of pure g-C3N4 loaded with different amount of Ni2P were investigated and the results are shown in Fig. 6a. As seen in the results, the hydrogen production rate increases initially and then decreases with the increasing ratio of Ni2P loaded, indicating that Ni2P is an efficient cocatalyst. Nevertheless, excess Ni2P may shield the incident light and may also block the active sites responsible for hydrogen production. Pure Ni2P is not active for hydrogen evolution. Besides, the mechanically mixed sample of pure g-C3N4 and Ni2P exhibits a lower rate of hydrogen production than sample NC-4, highlighting the importance of the close contact between pure g-C3N4 and the Ni2P cocatalyst (Fig. 6b).
Photocatalytic hydrogen production experiments were further carried out using NC-4 as photocatalyst in different sacrificial electron donors (TEOA, CH3OH, CH3CH2OH, Lactic acid, Ascorbic acid and concentrations of 0.75 M Na2S and 1.05 M Na2SO3 aqueous solution) system. As data shows in Fig. 6c, A maximum hydrogen production rate of ∼ 270 µmol h−1 g−1 can be reached in the presence of 20 vol% TEOA, which is much higher than that of pure g-C3N4, and a little lower than that of 3.0 wt% Pt/g-C3N4(∼ 297 µmol h−1 g−1). All the above results suggest that Ni2P can effectively improve the photocatalytic activity for hydrogen production after the optimal concentration.
The transient photocurrent response curves of the electrodes coated with pure g-C3N4 and sample NC-4 were recorded for several on–off cycles. Figure 6d shows both samples present relatively low currents without light irradiation. Interestingly, an apparent increase of the photocurrent appears when visible light irradiation is turned on. When the working electrode coated with sample NC-4 exhibits a much higher photocurrent than the pure g-C3N4 electrode. The photocurrent response indicates the effective transfer of the photoinduced electrons from the photocatalyst to the back contact. Therefore, Ni2P can efficiently facilitate the transport of photogenerated charge carriers and promote the hydrogen production activity.
Further experiments were performed to measure the AQY and confirm the long-term photocatalytic stability under visible light irradiation. Figure 7a shows that the hydrogen production rate reaches ∼ 143.7 µmol−1 g−1 upon irradiation of 420 nm monochromatic in 6 h, and the values for H2 production are relatively low in the initial few hours due to the induction period. After 6 h, the AQY is maintained at an average value of ∼ 2.85%. Figure 5b shows the long-term stability for photocatalytic hydrogen production. The result shows that there is no significant decrease of the hydrogen evolution rate even after 36 h of illumination. In addition, the XRD spectra of the NC-4 after irradiation show no significant difference from those before irradiation (Fig. 7c), which indicate that the Ni2P/g-C3N4 photocatalyst have good photocatalytic durability and stability.
Based on the above charactertions, a possible photocatalytic mechanism of Ni2P/g-C3N4 was proposed and shown in Scheme 1. When pure g-C3N4 is illuminated by visible light, the electrons in the valence band (VB) will be excited to the conduction band (CB). The photogenerated electrons will either recombine with the holes or transfer to the surface for photochemical hydrogen evolution reactions. As a metallic compound, Ni2P will form a typical metal–semiconductor interface with g-C3N4, and the photogenerated electrons are able to transfer from the semiconductor photocatalyst g-C3N4 to the metallic cocatalyst Ni2P. Thus, loading moderate Ni2P onto g-C3N4 can facilitate the separation of the photogenerated electron–hole pairs in g-C3N4, leading to improved photocatalytic activity.
4 Conclusions
In summary, a novel Ni2P/g-C3N4 photocatalyst was successfully synthesized by a facile phosphidation method. The photocatalytic activity for hydrogen production can be enhanced after the loading of Ni2P onto g-C3N4. The H2 production rate reached ∼ 270 µmol h−1 g−1 under visible light irradiation (λ > 420 nm) and the AQY was ∼ 2.85% at 420 nm. The results indicate that Ni2P, as a noble-metal-free cocatalyst, can efficiently promote the separation of the photogenerated electron–hole pairs in g-C3N4. This work presents the potential of noble metal-free Ni2P as cocatalysts for photocatalysis.
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Acknowledgements
This work was funded by the NSFC (21473170), the Fundamental Research Funds for the Central Universities (WK3430000001, WK2060140015, and WK2060190026), Natural science Fund of of Anhui province (1808085ME139), and The Thousand Young Talents Program.
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Ge, J., Jiang, D., Zhang, L. et al. Embedding Noble-Metal-Free Ni2P Cocatalyst on g-C3N4 for Enhanced Photocatalytic H2 Evolution in Water Under Visible Light. Catal Lett 148, 3741–3749 (2018). https://doi.org/10.1007/s10562-018-2562-6
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DOI: https://doi.org/10.1007/s10562-018-2562-6