Open Access Article
Qing
Han†
ab,
Haimiao
Jiao†
b,
Lunqiao
Xiong
b and
Junwang
Tang
*b
aKey Laboratory of Cluster Science, Ministry of Education of China, Key Laboratory of Photoelectronic/Electrophotonic Conversion Materials, School of Chemistry and Chemical Engineering, Beijing Institute of Technology, Beijing 100081, China
bDepartment of Chemical Engineering, University College London, London WC1E 7JE, UK. E-mail: junwang.tang@ucl.ac.uk
First published on 3rd November 2020
Photocatalytic ammonia (NH3) synthesis from N2 and water driven by solar energy is a sustainable and environmentally friendly technology, which has gained considerable attention in recent years. In this review, the recent development in the fundamental understanding of photocatalytic NH3 synthesis and the methods of precise NH3 detection are summarized. More importantly the strategy for surface engineering and interface engineering of photocatalysts toward photocatalytic NH3 production has been thoroughly analyzed with the aim to stimulate critical thinking about the effective methodology for catalyst modification instead of exploring new materials. At the end the challenges and a few concerns are raised from the current reports and future perspectives in this research field are discussed targeting to clarify the reliability and reproducibility of the photochemical process and to direct the future research direction, such as flow reactor design and in-depth understanding of the underlying reaction pathway.
Currently, there are a few green routes reported for ammonia synthesis. One is biological nitrogen fixation which mostly relies on diazotrophs in nature.8 Another one is electrochemical reduction of N2, which uses electricity to produce NH3.9,10 Compared with the stringent conditions of biological nitrogen fixation and the requirement of highly conductive electrolytes and costly electrodes used in electrochemical reduction of N2, photocatalytic ammonia synthesis using sustainable solar energy operated under either aqueous or gaseous conditions is rather different, maybe also economical, from the other methods. If the efficiency of solar driven NH3 synthesis could be dramatically improved, this method has strong potential to replace the current Haber–Bosch process. Photocatalytic reduction of N2 to produce NH3 by utilizing photocatalysts and water, driven by renewable solar energy, has huge potential, and thereby is very significant.11–17 Since the seminal work of Schrauzer and Guth in 1977,17 in which the potential of the TiO2 photocatalyst for N2 reduction with water and N2 was revealed, various semiconductors have been studied for the photocatalytic production of NH3, such as ZnO, Fe2O3, Ga2O3, W18O49, BiOBr, BiOCl, CdS, layered double hydroxides, polymeric carbon nitride and so on.18–25 The main challenges for the photocatalytic synthesis of NH3 are the chemical adsorption and activation of N2. To boost the efficiency of NH3 photosynthesis, the exploitation of highly active photocatalytic materials is crucial. Through surface/interface engineering of various photocatalysts, the photocatalytic reaction pathways can be modulated, therefore enhancing the N2 reduction reaction activity.
Complementary to other reviews in which different photocatalysts are summarized,6,13,18,19,22 this crucial review tries to avoid simply listing a large population of materials and mainly concentrates on recent advances and understanding in two fast moving areas, i.e. surface engineering and interface engineering, which have been proved to be efficient strategies to improve most photocatalysts’ activity for NH3 synthesis, including defect engineering, morphology engineering, cocatalyst loading, and junction structure. The materials stated here are representative and highly efficient. Thus, this review aims at providing a comprehensive understanding of the rational design of highly efficient photocatalysts for N2 photoreduction. Apart from this, the recent understanding of the photocatalytic mechanism of NH3 synthesis and the methods to precisely evaluate the catalytic performance of a photocatalyst in NH3 synthesis will be discussed. Future research directions for further development of the photocatalytic synthesis of NH3 and some concerns will be highlighted at the end.
| 2N2 + 6H2O → 4NH3 + 3O2 |
In this artificial photosynthesis, there are two interlinked conversion processes, water splitting and N2 reduction reaction (NRR).26 As shown in Fig. 1a, upon light irradiation, photoinduced electrons generated from photocatalysts populate the conduction band, leaving holes in the valence band. Subsequently, the escaped electrons diffuse across to the reactive sites on the surface of photocatalysts. The adsorbed N2 and H2O are catalyzed by these electrons and holes into NH3 and O2, respectively, along with the generation of the byproduct H2. Thus the key point for this process is not only to design a highly active photocatalyst but also to achieve high selectivity to NH3 instead of H2 gas as indicated in Fig. 1a.
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| Fig. 1 (a) Photocatalytic synthesis of NH3 in water. (b) The proposed mechanisms for photocatalytic N2 reduction consisting of the dissociative pathway, the associative alternating pathway, and the associative distal pathway. Reproduced from ref. 27 with permission from ACS Publication. (c) The proposed mechanism of surface-hydrogenation over noble metal doped photocatalysts for NRR. Reproduced from ref. 28 with permission from ACS Publication. | ||
Up to now, the mechanisms for N2 reduction to NH3 on photocatalysts have been divided into two categories based on the surface adsorption characteristics of catalysts: N-hydrogenation (Fig. 1b) and surface-hydrogenation (Fig. 1c).27,28 For the N-hydrogenation mechanism, there are two different pathways for NRR, dissociative and associative pathways. In the dissociative pathway, the N2 triple bond is broken before hydrogenation, followed by hydrogenation of the N-adatoms into NH3 on the catalyst surface. The Haber–Bosch process is proved to be the dissociative pathway, which requires prohibitively high energy to cleave the N
N bond. Compared with the dissociative pathway, the associative pathway without the breaking of the N
N bond is generally used and accepted far more in the photocatalytic NRR. The nitrogen surface adsorption configuration determines the associative pathways for NRR; as shown in Fig. 1b, the hydrogenation of the adsorbed N2 preferentially occurs at the terminal-site N owing to its relatively low steric hindrance for both the associative alternative pathway and the associative distal pathway. Having generated the first NH3, the other N begins a new hydrogenation circulation to produce a second NH3. It is actually impossible to identify the N2 configurations due to the fact that they are favored equally by the catalysts.
Recently, a novel surface-hydrogenation mechanism for NRR has been proposed (Fig. 1c),28 in which the adsorbed H+ is reduced into *H first, and then N2 molecules react with surface *H to generate *N2H2, and finally the formed *N2H2 intermediates are reduced into NH3. The first step is the trigger step, which enables the NRR to occur at a low potential. Furthermore, the second step is the rate determining step because it needs to conquer a high energy barrier (Ea) to break the N
N bond. The Ea of hydrogen evolution reaction is always lower than that of NRR, and therefore the NH3 production rate is relatively low.
As a complete cycle indicated in Fig. 1a is the ideal process but very challenging, in most cases (or in the majority of the reported cases), a half reaction was investigated in which N2 was reduced to NH3 in the presence of an efficient hole scavenger which was oxidized other than water oxidation. This half reaction is relatively easy and can be used to preliminarily scan different photocatalysts for N2 reduction. Bear in mind that this half reaction has advantages but does not indicate whether the photocatalyst selected is good for a complete cycle as indicated in Fig. 1a. The subsequent discussion will underline this in order to remind the audience of the large difference between a half reaction and the complete cycle.
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| Fig. 2 Photographs of NH3 solution with different concentrations (0, 1.2, and 4 mg L−1 from left to right) when (a) mixing with Nessler's reagent and (b) adding 4 μg L−1 formaldehyde into the above ammonia solution with Nessler's reagent. Measured results of NH3 concentration using (c) Nessler's reagent and d) ion chromatography methods. Reproduced from ref. 29 with permission from ACS Publication. (e) The NH3 concentration evolution with time tested by ion chromatography. Inset in (e): UV-vis absorption spectra tested with the indophenol reagent with the characteristic adsorption peak of 630 nm wavelength. Reproduced from ref. 30 with permission from ACS Publication. | ||
Extensive studies on the determination of NH3 have revealed that the indophenol blue method, Nessler's reagent method, and the ion chromatography method are accurate when the concentration of NH3 is less than 500 μg L−1, but the indophenol blue method tends to be less accurate at higher concentrations or under acidic conditions. Besides, the presence of carbonyl compounds from scavengers will enhance light adsorption in Nessler's reagent method, thus leading to an interfered detection of NH3. Thus, to guarantee accuracy and reliability of NH3 quantification, at least two detection methods such as the ion chromatography method and Nessler's reagent method are recommended. Furthermore, because of trace NH3 in the ambient atmosphere, it is necessary to test the isotopically labeled 15N2 to confirm the source of nitrogen in the product.
| Catalyst | Reaction medium | Scavenger | Light source | Ammonia yield | Apparent quantum efficiency (AQE) | Ammonia detection method | Ref. |
|---|---|---|---|---|---|---|---|
| BiOBr-001-OV | N2/H2O (l) | None | λ > 420 nm | 104.3 μmol g−1 h−1 | 0.23% at 420 nm | Nessler's reagent | 31 |
| JRC-TIO-6 | N2/H2O (l) | 2-PrOH | λ > 280 nm | 2.5 μmol g−1 h−1 | Not reported | Indophenol blue method | 32 |
| CuCr-LDH | N2/H2O (l) | None | Full spectrum | 78.6 μmol g−1 h−1 | 2.4% at 400 nm | Nessler's reagent | 34 |
| ZnAl-LDH | N2/H2O (l) | None | UV-vis | 110 μmol L−1 h−1 | 1.77% at 265 nm, 0.56% at 365 nm | Ion chromatography | 35 |
| V-g-C3N4 | N2/H2O (l) | Methanol | λ > 420 nm | 1.24 mmol h−1 gcat−1 | Not reported | Nessler's reagent | 54 |
| mCNN | N2/ethylene glycol (l) | Ethylene glycol | λ > 400 nm | 3.42 mmol g−1 h−1 | Not reported | Nessler's reagent | 55 |
| SCNNSs | N2/H2O (l) | Methanol | Full spectrum | 5.99 mmol h−1 gcat−1 | Not reported | Nessler's reagent | 56 |
| Mo0.1Ni0.1Cd0.8S | N2/H2O (l) | Ethanol | UV | 3.2 mg h−1 gcat−1 | Not reported | Nessler's reagent | 57 |
| 0.2 wt% Fe-doped TiO2 | N2/H2O (g) | None | UV | 11.6 μmol g−1 h−1 | Not reported | Indophenol blue method | 17 |
| 0.4 wt% Co-doped TiO2 | N2/H2O (l) | None | UV | 6.3 μmol g−1 h−1 | Not reported | Indophenol blue method | 17 |
| 0.4 wt% Cr-doped TiO2 | N2/H2O (l) | None | UV | 0.37 μmol g−1 h−1 | Not reported | Indophenol blue method | 17 |
| 0.4 wt% Mo-doped TiO2 | N2/H2O (l) | None | UV | 6.7 μmol g−1 h−1 | Not reported | Indophenol blue method | 17 |
| Fe-Doped TiO2 | N2/H2O (l) | Ethanol | λ = 254 nm | 1.2 mmol L−1 | Not reported | Nessler's reagent | 64 |
| Fe-Doped SrMoO4 | N2/H2O (l) | None | UV-vis | 93.1 μmol g−1 h−1 | Not reported | Nessler's reagent, indophenol blue method | 65 |
| Fe-Doped BiOCl | N2/H2O (l) | None | Full spectrum | 1.022 mmol g−1 h−1 | 1.8% at 420 nm | Indophenol blue method | 66 |
| Mo-Doped W18O49 | N2/H2O (l) | Na2SO3 | Full spectrum | 195.5 μmol g−1 h−1 | 0.33% at 400 nm | Nessler's reagent, ion chromatography | 67 |
| Cu-Doped TiO2 | N2/H2O (l) | None | Full spectrum | 78.9 μmol g−1 h−1 | 0.08% at 600 nm, 0.05% at 700 nm | Nessler's reagent, ion chromatography | 68 |
| FePt@C3N4 | N2/H2 | None | λ > 400 nm | 63 μg h−1 g−1 | 0.15% between 450 and 500 nm | Colorimetric method, ion chromatography | 72 |
| B-Doped g-C3N4 | N2/H2O (l) | Na2SO3 | λ > 400 nm | 313.9 μmol g−1 h−1 | 0.64% at 420 nm | Nessler's reagent | 73 |
| C-Doped TiO2 | N2/H2O (l) | Methanol | λ > 420 nm | 109.3 μmol g−1 h−1 | 2.4% at 400 nm | Ion chromatography | |
| Bi5O7I-001 | N2/H2O (l) | Methanol | 280–800 nm | 111.5 μmol g−1 h−1 | 5.1% at 365 nm | Nessler's reagent | 77 |
| BiOCl-010 | N2/H2O (l) | Methanol | Full spectrum | 92.4 μmol g−1 h−1 | 4.3% at 254 nm | Nessler's reagent | 78 |
| BiO | N2/H2O (l) | None | Full spectrum | 1226 μmol g−1 h−1 | Not reported | Indophenol blue method | 86 |
| Bi5O7Br-NT | N2/H2O (l) | None | λ > 400 nm | 1.38 mmol g−1 h−1 | 2.3% at 420 nm | Nessler's reagent | 87 |
| eBP NFs | N2/H2O (l) | Na2SO3, Na2S·9H2O | λ = 420 nm | 2.37 mmol g−1 h−1 | Not reported | Nessler's reagent | 88 |
| SiO2/C-RP | N2/H2O (l) | None | Full spectrum | 0.73 μmol h−1 | Not reported | Ion chromatography | 89 |
| Ru-Loaded TiO2 | N2/H2O (l) | Methanol | Full spectrum | 29.4 μmol g−1 h−1 | Not reported | Indophenol blue method | 93 |
| Ru-Loaded TiO2 | N2/H2O (l) | Ethanol | Full spectrum | 56.3 μg h−1 gcat−1 | Not reported | Indophenol blue method | 95 |
| Au/TiO2-OV | N2/H2O (l) | Methanol | λ > 420 nm | 78.6 μmol g−1 h−1 | 0.82% at 550 nm | Indophenol blue method | 96 |
| Ti3C2-P25 | N2/H2O (l) | None | Full spectrum | 10.74 μmol g−1 | Not reported | Ion chromatography | 103 |
| Pt-Loaded ZnO | N2/H2O (l) | Na2SO3 | UV | 860 mmol g−1 h−1 | Not reported | Indophenol blue method | 104 |
| SV-1T-MoS2/CdS | N2/H2O (l) | Methanol | 420–780 nm | 8220.83 μmol L−1 h−1 g−1 | 4.424% under simulated solar light | Nessler's reagent | 105 |
| NiS/CdS | N2/H2O (l) | None | Full spectrum | 2.8 mg L−1 h−1 | 0.76% at 420 nm | Nessler's reagent | 106 |
| Pt-SACs/CTF | N2/H2O (l) | None | 420–780 nm | 171.4 μmol g−1 h−1 | 1.4% at 420 nm | Nessler's reagent | 107 |
| Ru/RuO2/g-C3N4 | N2/H2O (l) | Methanol | Full spectrum | 13.3 μmol g−1 h−1 | Not reported | Ion chromatography | 108 |
| Fe@graphene | N2/H2, 200 °C | None | 200–600 nm | 420 μg gcat−1 h−1 | Not reported | Indophenol blue method | 110 |
| g-C3N4/Bi2MoO6 | N2/H2O (l) | Methanol | λ > 420 nm | 3271 μmol L−1 g−1 | Not reported | Nessler's reagent | 111 |
| TiO2@C/g-C3N4 | N2/H2O (l) | Methanol | λ > 420 nm | 250.6 μmol g−1 h−1 | 0.14% at 420 nm | Nessler's reagent | 112 |
| Bi2MoO6/OV-BiOBr | N2/H2O (l) | None | Full spectrum | 81.0 μmol g−1 h−1 | Not reported | Nessler's reagent | 116 |
N bonds from 1.078 Å to 1.133 Å, which gave strong evidence for N2 activation over the OVs.31 Theoretical calculations showed that the OV induced defect states could serve as the electron acceptor (Fig. 3a) to effectively suppress the recombination of electrons/holes and enhance the charge transfer from BOB-001-OV to the N2 molecule. Fluorescence spectroscopy showed that the average lifetime (τ) of BOB-001-OV was 2.15 ns, around two times higher than that of BiOBr without OVs (BOB-001-H, Fig. 3b), proving that the OVs could promote the migration of charge carriers. With the function of OVs, BOB-001-OV showed a NH3 yield rate of 104.3 μmol g−1 h−1 under visible light illumination in the absence of organic scavengers and noble-metal cocatalysts (Fig. 3c), and an apparent quantum efficiency (AQE) of 0.23% at 420 nm. Meanwhile, the amount of generated O2 was stoichiometrically approaching 3/4 of the produced NH3, which proved that water could act as an electron donor to achieve a complete chemical cycle in NH3 photosynthesis.
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| Fig. 3 Schematic of the OV-induced enhanced interfacial electron transfer processes over BOB-001-OV. (b) Time-resolved photoluminescence (PL) spectra of BOB-001-OV and BOB-001-H. (c) The photocatalytic NH3 production of BOB-001-OV and BOB-001-H under visible light (λ > 420 nm). Reproduced from ref. 31 with permission from ACS Publication. | ||
Apart from the research on bismuth oxyhalide materials, Shiraishi's group utilized a series of commercial TiO2 to study the effect of OVs on the photoreduction of N2 to NH3.32 A commercial TiO2 of JRC-TIO-6 showed an excellent performance with a steadily increasing NH3 production within 100 h under UV light irradiation in pure water. They proposed that the Ti3+ species formed at the OVs on the surface of TiO2 served as active sites, which could effectively trap the electrons and promote N2 dissociation, resulting in a photocatalytic NH3 production rate of 2.5 μmol h−1.
In order to create the OVs, most studies used oxygen-containing catalysts. In recent years, layered double hydroxide (LDH, Fig. 4a) materials have attracted substantial attention due to their tunable electron structure and low cost.34 Zhang's group firstly used the CuCr-LDH nanosheets (CuCr-NS) with OVs as efficient photocatalysts for NH3 photosynthesis.34 The OVs over CuCr-NS surface were created by the reduction of thickness and the in-plane compressive strain (Fig. 4b). The optimal CuCr-NS exhibited a NH3 production rate of 78.6 μmol g−1 h−1 under full-spectrum irradiation (Fig. 4c), and an AQE of 2.4% at 400 nm. Subsequently, they further reported another work on ZnAl-LDH nanosheets for optimal OVs by incorporating coordinately unsaturated Cuδ+ species.35 The DFT calculations implied that the OVs and Cuδ+ species in ZnAl-LDH could effectively promote N2 adsorption and activation, leading to a remarkable NH3 yield of 110 μmol L−1 h−1 in pure water under UV-vis irradiation. Therefore, the creation of OVs on the surface of photocatalysts paves a way for developing other innovative materials toward photocatalytic N2 reduction.
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| Fig. 4 (a) Schematic representation of the layered LDH structure with defective MO6 octahedra. (b) Schematic of the in-plane biaxial compressive strain in CuCr-NS. (c) The yield of NH3 over different LDH photocatalysts under visible-light illumination (λ > 400 nm). Reproduced from ref. 34 with permission from Wiley-VCH. | ||
N) and intercalated K+ (mCNN) was prepared as an efficient photocatalyst for NRR.55 Relative to pristine g-C3N4, the absorption spectrum of mCNN was extended to the whole visible region (Fig. 5a), resulting from the π–π* electronic transitions in the conjugated heterocyclic rings and the n–π* electronic transitions at the active N defect sites (–C
N), which indicated that the introduction of the N-defect of –C
N could significantly change the optical properties. Fig. 5b displays the band structures of mCNN and pristine g-C3N4 through the results of experiments. Compared with pristine g-C3N4, a subgap state was presented for mCNN, which could be ascribed to the N defect, resulting in a broad visible-light response. The enhanced EPR intensity (Fig. 5c) of mCNN compared to pristine g-C3N4 was assigned to the strong electron withdrawing groups of –C
N on mCNN, which could delocalize the isolated electrons in mCNN, therefore promoting the separation of photocarriers and increasing the generation of active radical species to boost the activity of NH3 photosynthesis. The rate of NH3 generation of the mCNN photocatalyst was measured to be 3.42 mmol g−1 h−1 with ethylene glycol as a scavenger under visible light irradiation (Fig. 5d), which was much higher than that of pristine g-C3N4 (1.11 mmol g−1 h−1). The DFT calculations revealed that K+ could be linked to the unsaturated C centers by coordination as shown in Fig. 5e, which could adsorb N2 as the lone-pair electrons of nitrogen would fill the empty state in K+ (ΔG = −0.28 eV), followed by the rearrangement of K+ with the C atom and the adsorption of N2 (ΔG = −0.17 eV). Because of the large ion hydration free energy of K+, it could be extracted back into solution, then forming a C2N4 ring (ΔG = 1.64 eV) intermediate which could undergo a MvK process to regenerate –C
N, thereby stabilizing the unsaturated C sites.
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| Fig. 5 (a) UV-vis diffuse reflectance spectra (DRS). (b) Schematic illustration of energy band structures. (c) Room-temperature electron paramagnetic resonance (EPR) spectra. (d) NH3 production rates of g-C3N4 and mCNN. (e) The calculated free-energy changes for the NRR pathway using mCNN. The blue sphere represents N, the grey sphere represents C, the white sphere represents H, and the purple sphere represents K+. Reproduced from ref. 55 with permission from Wiley-VCH. | ||
Apart from the above NVs on the g-C3N4 photocatalyst, carbon vacancies (CVs) on a porous sulfur-doped g-C3N4 (SCNNSs) have also been exploited.56 The introduction of CVs was proved to play the same role as NVs, while the S-doping effect was demonstrated to improve the separation efficiency of photogenerated electron–hole pairs. Taking these advantages, the optimal SCNNSs showed an NH3 production rate of 5.99 mmol h−1 gcat−1.
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| Fig. 6 (a) The N2-TPD of Mo0.1Ni0.1Cd0.8S and Mo0.1Ni0.1Cd0.8S. (b) The relationship of NH3 yield over the obtained photocatalysts and the SV concentration. Reproduced from ref. 57 with permission from The Royal Society of Chemistry. | ||
In another study, Mo was successfully doped into W18O49 nanowires to produce Mo-doped W18O49 nanowires (MWO-1) as shown in Fig. 7a.67 Compared with OV-rich W18O49 nanowires, Mo-doping had many kinds of effects on photocatalytic N2 reduction. Fig. 7b displays the electronic band structures of MWO-1 and W18O49; it is observed that the defect-band center could be shifted to the Fermi level by Mo doping, which provided more energetic electrons for NRR. Theoretical simulations revealed that the Mo–W centers could alter electron distribution, leading to a larger adsorption energy (−2.48 eV) relative to W18O49 with W–W sites (1.65 eV), which was in favor of N2 chemisorption and activation (Fig. 7c). Additionally, the enhanced M–O co-valence caused by Mo doping could effectively promote the electron transfer from metal active centers to adsorbed N2 molecules. Thus, the optimal MWO-1 exhibited an excellent NH3 yield rate of 195.5 μmol g−1 h−1 under full-spectrum irradiation (Fig. 7d), which was 7 times higher than that of W18O49, and also realized a high AQE of 0.33% at 400 nm.
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| Fig. 7 (a) The scanning TEM (STEM) image and the corresponding elemental mapping of MWO-1. (b) Schematic illustration of the band structures of W18O49 and MWO-1. (c) Schematic simulation for N2 adsorption and activation on the surface active sites of the Mo-doped W18O49 model. (d) The photocatalytic NH3 yield on various catalysts. Reproduced from ref. 67 with permission from ACS Publication. | ||
Furthermore, Cu-doped ultrathin TiO2 nanosheets (TiO2-Vo-strain) were also studied.68 Compared with pristine TiO2, introducing Cu into TiO2 could create abundant OVs and cause lattice distortion and strain effects, resulting in a significant increase of N2 adsorption energy on the surface of TiO2-Vo-strain (−0.37 eV) compared with that of pristine TiO2 (−0.17 eV, Fig. 8a). The increased adsorption energy promoted the electron transfer from TiO2 to N2, thereby breaking the N
N bonds. Meanwhile, the required reaction energy for N2 hydrogenation to N–NH* was only 0.365 eV on TiO2-Vo-strain, which was lower than that on pristine TiO2 (2.115 eV, Fig. 8b). As a result, the optimal TiO2-Vo-strain (6% TiO2) achieved an enhanced NH3 yield rate of 78.9 μmol g−1 h−1 under full solar irradiation, about 5.2 times higher than that of the TiO2 nanosheets with OVs (0% TiO2, Fig. 8c). In addition, the yield rate of O2 (59.1 μmol g−1 h−1) and NH3 mentioned above over TiO2-Vo-strain was close to the stoichiometric ratio of 3
:
4, revealing that the protons in NH3 were from the H2O molecules. Most recently, a novel bimetallic system with Fe–Pt loaded g-C3N4 was used for efficient ammonia synthesis under mild conditions.72 Further investigations proposed that the doping of Pt onto the Fe nanocluster over the surface of g-C3N4 could cause an uplift of the energy band of semiconductors and form a large Schottky barrier, thus leading to an improved separation of photogenerated carriers and enhanced N2 reduction. Accordingly, 0.3 wt% Pt doped on 3 wt% Fe@C3N4 exhibited a high NH3 production rate of 63 μg h−1 g−1 with gaseous H2 and N2 as reactants under visible light irradiation and the AQE was tested to be 0.15% between 450 and 500 nm.
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| Fig. 8 (a) The N2 adsorption energies by DFT calculations on different photocatalysts. (b) The calculated Gibbs free energy for N2 reduction on the (001) surface of different photocatalysts (H: white sphere, Ti: gray sphere, N: blue sphere, O: red sphere). (c) Yield of NH3 over various samples under UV-vis irradiation. Reproduced from ref. 68 with permission from Wiley-VCH. | ||
Apart from metal doping, a metal-free B-doped g-C3N4 nanosheet (BCN) with exposed active N atoms was recently synthesized for highly efficient ammonia synthesis.73 Theoretical studies revealed that the exposed N atoms could be stabilized by B–N–C coordination on BCN, which was different from that in the pristine g-C3N4. The B dopants were proved as active sites for N2 adsorption and activation and could effectively retard charge recombination and improve light utilization. The optimal BCN with 13.8 wt% B-dopants exhibited a remarkable NH3 yield rate of 313.9 μmol g−1 h−1 under visible light irradiation in the presence of Na2SO3 as a hole scavenger, which was much higher than that (32.8 μmol g−1 h−1) over pristine g-C3N4 and also achieved a good QE of around 0.64% at 420 nm. In addition, carbon-doped TiO2 was also reported for N2 photoreduction, which exhibited an NH3 yield rate of 109.3 μmol g−1 h−1.
In another report, Zhang et al. also systematically investigated the influence of {001} and {010} facets of OV-rich BiOCl nanosheets on N2 adsorption and activation.78 Experimental results showed that {010} facet BiOCl nanosheets (BOC-010) exhibited a superior performance with a NH3 yield of 4.62 μmol g−1 h−1, which was around 2.5 times higher than that on {001} facet BiOCl nanosheets (BOC-001, Fig. 9a). Meanwhile, it was observed that N2H4 which served as a main intermediate was accumulated on BOC-010 during N2 photoreduction reaction within 30 min and was consumed gradually to be converted into NH3 (Fig. 9b). Importantly, when N2H4 was used as the reactant, both BOC-010 and BOC-001 showed a similar photocatalytic conversion efficiency of N2H4 under simulated solar irradiation (Fig. 9c), which in turn meant that BOC-010 had a stronger ability to generate N2H4 intermediates. Further DFT calculations revealed that the N2 fixation on BOC-010 followed an alternative pathway with N2H4 as the main intermediate, which could provide a lower energy pathway for N2 fixation via proton-coupled electron transfer compared with that via a distal pathway occurring on BOC-001 facets, thus resulting in enhanced NH3 production (Fig. 9d and e).
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| Fig. 9 Photocatalytic performance for N2 reduction on BOC-001 and BOC-010. The yield comparison of produced (a) NH3 and (b) N2H4 on BOC-001 and BOC-010 under simulated solar light irradiation. (c) The NH3 yield produced from N2H4 BOC-001 and BOC-010 under simulated solar light irradiation. The calculated free energy change for N2 reduction (d) on the (001) surface via a distal pathway and (e) on the (010) surface via an alternating pathway. Reproduced from ref. 78 with permission from The Royal Society of Chemistry. | ||
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| Fig. 10 (a) TEM image of BiO quantum dots. (b) Proposed mechanism for N2 photoreduction on BiO quantum dots. Reproduced from ref. 86 with permission from The Royal Society of Chemistry. (c) TEM image of Bi5O7Br-NT. (d) Yield of NH3 for Bi5O7Br-NT. (e) The wavelength-dependent AQE of Bi5O7Br-NT. Reproduced from ref. 87 with permission from Wiley-VCH. | ||
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| Fig. 11 (a) TEM image of Au/TiO2-OV. (b) Adsorption spectra of different photocatalysts. (c) The proposed schematic for photocatalytic N2 reduction over the Au/TiO2-OV catalyst under visible-light irradiation. (d) Photocatalytic NH3 production with different photocatalysts under visible light irradiation. Reproduced from ref. 96 with permission from ACS Publication. (e) Schematic of the adsorption structure on TiO2 (A), OVs-TiO2 (B) and Ti3C2 MXenes (C). Reproduced from ref. 103 with permission from Elsevier Publication. (f) Schematic for photocatalytic N2 reduction over Fe@graphene photocatalysts. Reproduced from ref. 108 with permission from ACS Publication. | ||
In addition to TiO2-based photocatalysts, Pt-loaded ZnO was reported as an efficient photocatalyst for N2 photoreduction which exhibited an NH3 yield rate of 860 mmol g−1 h−1.104 More recently, O-doped 1T-MoS2 nanosheets with a large amount of SVs (SV-1T-MoS2) were used as cocatalysts over CdS nanorods for photocatalytic N2 reduction.105 The DFT calculations revealed that the SVs and the metal properties of 1T-MoS2 could effectively promote the separation of h+/e− and the presence of SV-1T-MoS2 could also provide abundant active sites, resulting in enhanced N2 adsorption and immobilization. Accordingly, a remarkable performance over the optimal SV-1T-MoS2/CdS was realized with a superior NH3 yield rate of 8220.83 μmol L−1 h−1 g−1 under simulated solar light irradiation. Besides, NiS was also studied as a cocatalyst over CdS nanorods for ammonia photosynthesis.106 The DFT calculation indicated that the NiS cocatalyst could reduce the adsorption energy of N2 from 1.16 eV on the CdS surface to −0.55 eV on the Ni-doped CdS surface. Further characterization revealed that charge separation could also be enhanced by loading NiS on the CdS surface. Because of these properties, a favorable NH3 yield of 2.8 mg L−1 was reported within the first hour in pure water under full-spectrum irradiation. Recently, single-atom Pt modified triazine framework (CTF) nanosheets (Pt-SACs/CTF) were developed for photocatalytic NH3 production.107 It was found that the Pt–N3 sites were formed in Pt-SACs/CTF, leading to more negative conduction band position with accelerated thermodynamics and fast interfacial charge migration ability, and therefore a high NH3 production rate of 171.4 μmol g−1 h−1 under visible light irradiation. Most recently, we synthesized a ternary Ru/RuO2/g-C3N4 system for N2 photoreduction, which exhibited a photocatalytic NH3 yield of 13.3 μmol g−1 h−1 whilst no NH3 could be measured for pure g-C3N4 under the same condition. Such significant improvement in photocatalytic NH3 synthesis for Ru/RuO2/g-C3N4 was not only because of Ru and RuO2 acting as cocatalysts to promote electron and hole transfer respectively, but also due to the advantage of Ru for N2 chemisorption and activation.108 Besides that, carbon-based materials especially graphene are also often used as cocatalysts to prevent the photoinduced electron–hole recombination and promote the electron transfer due to their prominent electrical conductivity.109,110 For instance, a Fe modified three-dimensional graphene (Fe@graphene) photocatalyst was reported for NH3 production.110 In the Fe@graphene system (Fig. 11f), graphene generated hot electrons under light irradiation and transferred those electrons to Fe, while Fe acted as an electron sink and provided the catalytic active sites for the adsorption and activation of N2.
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| Fig. 12 (a) SEM image of TiO2@C/g-C3N4. (b) PL spectra of TiO2@C/g-C3N4 and g-C3N4. (c) Transient photocurrent responses of TiO2@C/g-C3N4 and g-C3N4. (d) The N2-TPD profiles. (e) The yield of produced NH3 under visible light irradiation (λ > 420 nm). Reproduced from ref. 112 with permission from The Royal Society of Chemistry. | ||
This review does not detail different photocatalysts as there are a few reviews on them, but analyses surface engineering and interface engineering in photocatalysts developed recently for the photocatalytic NH3 synthesis, involving oxygen vacancies, nitrogen vacancies, carbon vacancies, sulfur vacancies, metal and non-metal doping, facet modulation, nanostructure engineering, and heterostructure construction such as loading with cocatalysts and modification with other semiconductors, together with the mechanism of N2 reduction reaction and the reliable means for the detection of NH3.
Great progress has been made in the study of photoreduction of N2 to NH3 as briefed in Fig. 13, but there are still many problems, some of which are very critical. First, the majority of the studies so far reported use an efficient and expensive hole scavenger to get long lived photoelectrons for N2 reduction. However, a practical pathway should use water as the only electron donor and to provide protons for the photosynthesis of NH3, as such NH3 synthesis by photocatalysis is scientifically meaningful and economically sustainable. The slow progress linked to this profile is mainly due to the very limited understanding in this field. Second, there are few reports specifying the stoichiometric chemistry in the photochemical process. Without the stoichiometric O2 gas produced, such N2 reduction to NH3 is questionable. Furthermore, as O2 could be leaked from air, the isotopic measurement of O2 production is necessary. In addition, since H2 production would compete with NH3 synthesis, a comprehensive study should detail the selectivity between the two products and discuss the strategy to favor NH3 synthesis. In addition an experimental error bar is very crucial for such NH3 synthesis in order to improve the confidence as almost all studies were carried out in a batch reactor with quite a small amount of NH3 produced, which was quite easy to be interfered by occasional factors.
Apart from the issues mentioned above, photocatalytic NH3 synthesis also faces a few tough challenges. The majority of the studies show that the NH4 amount produced is less than 10 μmol h−1 (instead of the unit of μmol g−1 h−1) when using water as the electron donor and 10 times enhancement is achieved when using an organic hole scavenger. This amount is lower than the NH3 amount in the river water which is about 0.01 mM.118 Besides, since the NH3 yield is extremely easy to be interfered by environmental impurities and different detection agents, it is difficult to obtain reliable and reproducible results by just one analysis method.119 At least two methods have to be applied to prove the consistent results and to improve the reproducibility of the process.
The surface states of a catalyst can dominate its performance, such as surface defects. However, to quantify the correlation of the surface defects with the catalytic activity is very challenging at present. This should be undertaken in the future in order to distinctly guide catalyst surface state control. Furthermore the cocatalyst is another key factor to control both charge separation and catalytic performance. The majority of the cocatalysts reported are either large particles or nanosized particles. Single atomic catalysis is an emerging area, which presents unprecedented activity in some chemical processes. Such unique reaction sites should be introduced to ammonia synthesis with in-depth exploration of their intrinsic function. In addition, a junction structure is widely accepted to help charge separation, which was also reviewed in the previous session. The new design strategy should be applied to construct new junctions, such as polymer and oxide junctions as the former has likely better N2 adsorption due to the potential hydrogen bond between the organic polymer and N2 while the latter has a very positive VB for water oxidation.
The modified catalyst discovery is very informative. Equally, the mechanism and reaction pathways for photocatalytic N2 fixation are scarce and much less investigated, forming an obstacle for the rational design of highly efficient photocatalysts. Currently, most of the given reaction mechanisms and reaction pathways were based on assumptions and lacked solid evidence. Thus, the current catalyst development is more or less a try-and-error process. Some advanced operando technologies in functional characterization should be applied to comprehensively study the reaction pathway such as by time resolved spectroscopy to investigate charge carrier dynamics, and by transient and stationary spectroscopy to observe the reaction intermediates.
In addition, it is of paramount importance to design a flow reaction system for N2 photoreduction. The current reaction system is composed of a batch reactor, which is far from the requirement of the industry. The typical batch reactor is easy to be constructed; however, its efficiency is severely restricted by the low mass transfer between N2 gas and aqueous solution due to the low solubility of N2, thereby resulting in a low photocatalytic efficiency. Besides, NH3 accumulated in the batch reactor during the reaction process will be overoxidized to other byproducts, thereby resulting in a low conversion rate and even bad selectivity. Moreover, based on the industrial viewpoint, it is quite costly to separate the photocatalysts from reactants and products in a batch system. Thus, an intensified flow reactor such as using N2 and water vapor as reactants should be explored to overcome these drawbacks and to meet the industrial requirement in the future, underlining the crucial collaborations between chemical scientists and experts in reaction engineering.
Last, modelling will be expected to combine with experimental results to figure out the reaction mechanism and speed up the rational design of highly efficient photocatalysts. Meanwhile, the big data, together with artificial intelligence (AI) and machine learning (ML), will be a future key research area to improve the reproducibility of the catalyst synthesis, to facilitate catalyst screening, to enhance the experimental safety and to save the experimental costs and time.
Overall, this research field is at an infant state and all these areas should be enhanced in order to improve the NH3 synthesis rate with high reproducibility and reliability of the procedure.
Footnote |
| † Co-first authors: These authors contributed equally to this work. |
| This journal is © The Royal Society of Chemistry 2021 |