Jiquan
Huang
*ab,
Ting
Lv
a,
Qiufeng
Huang
a,
Zhonghua
Deng
a,
Jian
Chen
b,
Zhuguang
Liu
b and
Guo
Wang
*ab
aFujian Science & Technology Innovation Laboratory for Optoelectronic Information of China, Fuzhou, 350108, P. R. China. E-mail: hjq@fjirsm.ac.cn; guowang@fjirsm.ac.cn
bKey Laboratory of Optoelectronic Materials Chemistry and Physics, Fujian Institute of Research on the Structure of Matter, Chinese Academy of Sciences, Fuzhou, 350002, P. R. China
First published on 21st October 2020
The simultaneous realization of visible light response and high photocatalytic activity remains a challenging task for TiO2 despite extensive research. Herein, (Nb,Rh) codoping is adopted to extend the absorption band of anatase TiO2 into the visible-light region. Meanwhile, the dependence of the electronic structure, visible-light absorption, and photocatalytic performance on the dopant ratio as well as doping concentration is studied. Open shell t2g5 Rh(IV) and closed shell t2g6 Rh(III) coexist in Rh-doped TiO2, and the codoped Nb promotes a change in valence state from Rh(IV) to Rh(III). Rh(III) is the main active species in charge of the excellent photocatalytic performance, while Rh(IV) doping introduces electron/hole recombination centres. However, surprisingly, a trace of Rh(IV)-doping contributes to a decrease in electron transfer resistance and an increase in donor density, which help to improve photocatalytic performance. By virtue of the controlled content of Rh(III) and Rh(IV), Ti1−2xNbxRhxO2 exhibits a high hydrogen evolution rate of ∼9000 μmol g−1 h−1 in methanol solution, along with a remarkable photocurrent density of ∼9 μA cm−2 under visible-light irradiation, which are about 170 and 30 times higher than those of pristine TiO2 nanorods, respectively.
By virtue of its inexpensive, nontoxic, stable and durable qualities, TiO2 exhibits outstanding UV photocatalytic performance.14–16 Great progress has been made in developing TiO2-based semiconductors for photocatalytic water splitting. One-dimensional (1D) anatase TiO2 nanostructures (such as nanotubes, nanorods, and nanowires) are of particular interest due to their high surface area, abundant surface active sites, efficient electron/hole separation, and the great oxidizing ability of photogenerated holes.15–18 For example, a high STH conversion efficiency of 1.05% was achieved in a cross-linked TiO2 nanowire photoanode,19 and a photon-to-current conversion efficiency of nearly 100% at 330 nm was achieved in Pd-sensitized TiO2 nanotube arrays.15 Very recently, we reported the fabrication of dendritic nanorod arrays with an H2 evolution rate of 44.7 mmol g−1 m−2 under simulated sunlight and an apparent quantum yield of 63.8% at 365 nm.20 However, the STH conversion efficiency of TiO2 is still too low to meet the target value for possible commercial applications, since a wide bandgap of 3.2 eV (for anatase) prevents it from harvesting visible light (note: UV and visible light account for 5% and 52% of the solar spectrum, respectively).15–17 Thus, it is of great importance to broaden the light absorption from UV to the visible-light region.
Many strategies have been explored to break through the limitations of the wide bandgap, one of which is doping.21 Doping of appropriate element(s) into the TiO2 crystal lattice creates donor or acceptor levels in the forbidden gap.22 Many metal and non-metal elements, such as Fe, Zr, Cr, Al, V, Rh, Ru, Mo, C, N, F, B, Si, and P, have been proved to be effective dopants for enhancing visible-light absorption.21–25 However, it is found that the expected significant improvements in STH conversion efficiency were not achieved, and even the photocatalytic activity under UV light declined drastically, due to an increase in electron/hole recombination.22 Obviously, both the limited absorption of visible light and the fast recombination of photoinduced electron/hole pairs must be addressed to improve the STH conversion efficiency. In this regard, one notable discovery is that a trivalent Rh(III) dopant with a d6 electron configuration can bring about an in-gap donor level without introducing additional recombination centres.26 The electron transition from the Rh(III) donor level to the conduction band (CB) makes Rh-doped TiO2 a highly active visible-light-driven photocatalyst.16,26–29 Furthermore, Rh(III) doping can even promote electron–hole separation while increasing the photo-induced carrier density.16 However, in Rh-doped TiO2 (and titanates such as SrTiO3), Rh ions prefer to exist in the form of Rh(IV) rather than Rh(III) for charge neutralization.27 Rh(IV) has an open shell t2g5 configuration, which leads to paramagnetic dopant centres acting as trapping sites.26 Therefore, additional compensating dopants such as Sb(V), Nb(V), and Ta(V) should be presented to suppress the oxidation of Rh(III) to Rh(IV). Recently, we reported the fabrication of an (Nb,Rh) codoped TiO2 semiconductor (Ti0.996Nb0.002Rh0.002O2 nanorods) by a two-step method.16 This photocatalyst displays ultra-high activity whether under ultraviolet or visible light. Its H2 production rate is far superior to that of undoped TiO2 nanorods, (Sb,Rh) codoped rutile TiO2, or Pt-loaded P25, which implies that (Nb,Rh) codoping into TiO2 (and titanate) is rather efficient for the development of a visible-light-responsive photocatalyst with a high quantum yield and high STH conversion efficiency.
In the present work, we fabricated a series of anatase phase (Nb,Rh) codoped TiO2 nanorods to gain insight into the maximum improvement in photocatalytic performance. The factors that control visible-light absorption, carrier transfer and recombination, and the H2 evolution rate were revealed by regulating the dopant rations and doping concentrations, as well as tailoring the morphology and crystal phase. It is expected to provide a useful reference for evaluating the potential industrial application of (Nb,Rh) codoped TiO2-based photocatalysts in this study.
Sample name | Chemical composition | Major valence state of Rh | H2 evolution rate (μmol g−1 h−1) |
---|---|---|---|
TNR | TiO2 | — | 52 |
N6TNR | Ti0.994Nb0.006O2 | — | 86 |
N6R3TNR | Ti0.991Nb0.006Rh0.003O2 | Rh3+ | 2681 |
N6R6TNR | Ti0.988Nb0.006Rh0.006O2 | Rh3+ | 9194 |
N3R6TNR | Ti0.991Nb0.003Rh0.006O2 | Rh3+/Rh4+ | 4170 |
R6TNR | Ti0.994Rh0.006O2 | Rh4+ | 622 |
N3R3TNR | Ti0.994Nb0.003Rh0.003O2 | Rh3+ | 6788 |
N9R9TNR | Ti0.982Nb0.009Rh0.009O2 | Rh3+ | 6015 |
N12R12TNR | Ti0.976Nb0.012Rh0.012O2 | Rh3+ | 3576 |
N15R15TNR | Ti0.97Nb0.015Rh0.015O2 | Rh3+ | 2045 |
N20R20TNR | Ti0.96Nb0.02Rh0.02O2 | Rh3+ | 1485 |
The evolution of the morphology with calcination temperature is presented in Fig. 2 and Fig. S1.† It is found that the phase transformation from titanate to TiO2 under calcination is accompanied by the collapse of nanotubes. At 500 °C, nanotubes had completely transformed into nanorods with diameters of about 7 nm and lengths of tens to hundreds of nanometers (Fig. 2a and b). The HRTEM images (Fig. 2b) revealed two sets of lattice fringes with the same spacing of 0.35 nm and an angle of ∼82°, which correspond to the (101) and (011) planes of anatase phase. Fig. S1g† shows the HRTEM image of the end face of a nanorod. High-density dislocations were observed. Since the nanorods are formed by the inward collapse and reconstruction of nanotubes (Fig. S1a–g†), the generation of large-scale crystal defects is inevitable. During the high-temperature calcination, although some of the crystal defects will be eliminated and the crystallinity will be improved, the migration of high-concentration dislocations will also lead to the fracture of the nanorods. At a higher calcination temperature of 700 °C, the length of most nanorods was found to be shorter than 70 nm, and quasi-spherical and elongated nanoparticles were also found (Fig. 2c). The HRTEM image (Fig. 2d) reveals the coexistence of anatase and rutile. (101) diffraction planes of the anatase phase were clearly displayed in a rod-like nanocrystal. In addition, two sets of lattices with spacings of 0.23 and 0.32 nm were observed in another nanoparticle, which can be ascribed to the (200) and (110) planes of the rutile phase, respectively. As the calcination temperature was further raised to 900 °C, only quasi-spherical (or elongated) particles were observed (Fig. 2e). Fig. 2f shows the EDX elemental mapping of N15R15TNR, where the homogeneous distribution of Ti, Nb and Rh elements highlighted the formation of (Nb,Rh)-codoped TiO2 without local aggregation or second phases.
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Fig. 2 TEM (a, c and e) and HRTEM (b and d) images of N6R6TNR calcined at 500 °C (a and b), 700 °C (c and d) and 900 °C (e). (f) STEM-EDS elemental mapping of N15R15TNR calcined at 500 °C. |
Fig. 3 shows the effect of calcination temperature on the photocatalytic activity. When the calcination temperature was in the range of 400–700 °C, the hydrogen evolution rate of N6R6TNR was at least two orders of magnitude higher than that of TNR, indicating that (Nb,Rh)-codoping is an effective strategy to improve the photocatalytic activity of TiO2. For both samples, the photocatalytic activity reached a maximum at 500 °C, and fell sharply when the temperature was higher than 600 °C. Generally, the performance of a photocatalyst depends largely on crystallinity, particle size and shape, specific surface area, and crystal structure (e.g., anatase, rutile and brookite phases for TiO2).34 For example, (i) high crystallinity and small particle size are often required for inhibiting the bulk recombination of photogenerated carriers; (ii) a higher surface area means more surface active site for redox reactions; (iii) compared with zero-dimensional (0D) nanoparticles, 1D nanostructures exhibit advantages such as enhanced light absorption and excellent charge transport;15–18 (iv) among the three allotropic crystalline forms of TiO2 (anatase, rutile, and brookite), the photocatalytic activity of the anatase phase is generally considered to be the highest. In this study, compared with samples obtained by calcining at higher temperature, the nanotubes obtained at 400 °C possessed the highest specific surface area. However, their crystallinity was also the lowest, which led to a lower hydrogen generation rate than that of nanorods obtained at 500 °C. As the temperature was further increased (T > 500 °C), the hydrogen generation rate decreased, even though the crystallinity increased. This indicated that the contribution of crystallinity was no longer dominant, and the importance of other factors (such as morphology, surface area, and A–R transformation) increased. As more and more nanorods broke into 0D nanoparticles at T > 600 °C (Fig. 2 and S1†), the hydrogen generation rate decreased sharply, indicating that the photocatalytic performance of 1D nanorods is far superior to that of 0D nanoparticles. It is noticed that, for N6R6TNR, the hydrogen generation rate decreased from 8035 μmol g−1 h−1 at 600 °C (anatase) to 51 μmol g−1 h−1 at 900 °C (rutile). Similarly, we also synthesized Ti0.99Nb0.005Rh0.005O2 0D nanoparticles by a simple sol–gel–calcination method. The average particle size increased slightly from 15 nm at 600 °C (anatase) to 20 nm at 900 °C (rutile), while the corresponding hydrogen generation rate decreased obviously from 440 μmol g−1 h−1 (600 °C) to 9 μmol g−1 h−1 (900 °C). Obviously, the A–R transformation has a significant impact on the photocatalytic performance. The anatase phase exhibits much higher photocatalytic activity than the rutile phase. Therefore, the preparation of Rh3+-doped rutile TiO2 through high-temperature calcination is not a good choice for achieving excellent performance. In contrast, the synthesis of anatase TiO2-based 1D nanostructures with high crystallinity is meaningful, but is also very difficult to achieve. In recent years, we have made many attempts to prepare high-quality TiO2-based nanotubes with little success. In this study, under the balance of various factors, the sample calcined at 500 °C exhibited the best performance for hydrogen evolution. Therefore, in the following studies, the calcination temperature was set to 500 °C.
As mentioned above, the photocatalytic performance of TiO2 can be greatly improved by (Nb,Rh) codoping. Undoubtedly, this improvement is related not only to the calcination temperature, but also to the doping concentration of both Nb and Rh. In order to optimize the performance, under the premise that the calcination temperature has been fixed (i.e., 500 °C), our strategy is to determine the preferred Nb/Rh mol ratio before determining the total doping concentration.
Fig. 4 shows the solid state UV-Vis absorption spectra of TiO2-based photocatalysts with different Nb/Rh ratios. Both TNR and N6TNR exhibited an absorbance edge at ∼385 nm and hardly absorb visible light, indicating that Nb5+ doping cannot contribute to the visible photocatalytic activity of TiO2. For N6R3TNR, N6R6TNR, and N3R6TNR, intensive absorption from 385 to 530 nm was observed, which can be attributed to the electronic excitation from the in-gap Rh3+ donor level to the CB.16,35 For R6TNR, the presence of a broad absorption peak with wavelength greater than 500 nm can be assigned to the electronic transition from the valence band (VB) to Rh4+ unoccupied levels.16,35,36 Additionally, the significant absorption between 400 and 500 nm implied the possible existence of Rh3+ in this sample. By comparing the absorption spectra between 500 and 600 nm (corresponding to the Rh4+ level), it is inferred that the Rh4+ content (relative to Rh3+) was increasing in the order of R6TNR > N3R6TNR > N6R6TNR > N6R3TNR, which can be further confirmed by XPS detection.
Fig. 5a shows the Rh 3d core level spectra of several doped TiO2 samples with different Nb/Rh ratios. The difference in the outer electron cloud density of Rh ions leads to a lower binding energy for Rh3+ than for Rh4+. For Rh3+ and Rh4+, the 3d5/2 peak was located at 307.7 and 309.3 eV, and the 3d3/2 peak was located at 312.5 and 314.1 eV, respectively. For N6R3TNR, two symmetric peaks were found at 307.7 and 312.5 eV, indicating the sole existence of Rh3+. For N3R6TNR, both Rh 3d5/2 and Rh 3d3/2 peaks can be deconvoluted into two comparable components, indicating the coexistence of Rh3+ and Rh4+ with a ratio close to 1. For N6R6TNR, in addition to Rh3+, a trace of Rh4+ was also detected. In reverse, for R6TNR, the Rh 3d5/2 profile can be fitted with a dominant Rh4+ peak and a secondary Rh3+ peak, implying that it is not a completely isovalent substitution of Rh4+ for Ti4+ in Rh-doped TiO2. This may be due to the fact that the stable oxidation state of Rh is +3. The change in valence state of Rh with Nb/Rh ratio will affect the charge balance, and thus alter the electronic structure of the doped TiO2. Fig. 5b shows the VB spectra. It is found that the Fermi level (EF) was located at about 2.78, 2.98, 2.84, 2.73, 2.25, and 1.97 eV above the valence band maximum (VBM) for TNR, N6TNR, N6R3TNR, N6R6TNR, N3R6TNR, and R6TNR, respectively. In other words, Nb-doping will shift the EF towards the CB while Rh-doping will shift the EF towards the VB. This is because Nb5+ and Rh3+ act as donor and acceptor impurities in TiO2, respectively. The existence of Nb5+ in N6TNR makes it more n-type while Rh3+ in R6TNR makes it more p-type (exhibited as the downward shift of the EF). Based on the aforementioned XPS and UV-Vis observations, a schematic band structure diagram was proposed, as shown in Fig. S4.† For all the samples, the EF was located above the impurity (Rh4+ and/or Rh3+) levels, indicating their n-type semiconductor nature. This may be due to the slight doping and the resultant negligible charge imbalance.
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Fig. 5 Rh 3d core level (a) and valence band (b) spectra for the photocatalysts with different Nb/Rh ratios (calcined at 500 °C). |
It is generally accepted that, in Rh-doped TiO2, Rh(III) is the active species, while Rh(IV) doping introduces additional trapping sites and thus its formation should be avoided. As shown in Fig. 5 and Fig. S4,† Rh(IV) coexists with Rh(III) in the samples with Rh/Nb ≥ 1, and only Rh(III) exists in N6R3TNR. It is thereby anticipated that N6R3TNR may exhibit the highest photocatalytic activity among these samples. But surprisingly, the hydrogen evolution rate of N6R3TNR was only 2681 μmol g−1 h−1, which was much lower than that of N6R6TNR (9194 μmol g−1 h−1) or N3R6TNR (4170 μmol g−1 h−1), as shown in Table 1. One possible explanation is that the Rh content of N6R3TNR is lower than that of the other two samples. However, it is also noticed that the hydrogen evolution rate of N3R3TNR (which has the same Rh doping concentration as N6R3TNR) was about three times that of N6R3TNR. Similar phenomena have also been reported in previous work.35,37 For example, the hydrogen evolution rate of (La,Rh) codoped SrTiO3 (with a constant Rh doping level of 4 mol%) decreases drastically with an increase in the La doping concentration from 4 to 10 mol%.35 To explore the origin of the enhanced performance, EIS measurement was carried out. Fig. 6 and Fig. S6† show the Nyquist plots for (Nb,Rh) co-doped TiO2. As shown in Fig. 6, for samples N6R3TNR, N6R6TNR, and N3R6TNR, N6R3TNR showed the largest semicircles, revealing its highest electron transfer resistance.38,39 In contrast, the smallest semicircular diameter of N3R6TNR indicated that the charge transfer in this sample was easier and more efficient than for the other two samples. Fig. S5† shows the Mott–Schottky plots of these three samples. Linear behaviour was observed when the applied bias ranged from 0 to 0.8 V. The positive slopes indicate that these samples were n-type semiconductors, which was in consistent with the aforementioned analysis (see the proposed band structure diagram in Fig. S4†). The slope for N6R3TNR was larger than that for N6R6TNR or N3R6TNR. It is known that the slope of the Mott–Schottky plot is inversely proportional to the donor density.39,40 Therefore, the larger slope of N6R3TNR suggested its lower donor density. According to the Nyquist and Mott–Schottky plots, it is possible to conclude that N6R3TNR possesses higher electron transfer resistance and lower carrier density. On the other hand, the presence of Rh(IV) in N6R6TNR and N3R6TNR induces an increase in the conductivity and carrier density, which allows more efficient charge separation, and allows more electrons and holes (per unit time) to reach the semiconductor surface for photocatalytic water splitting. It is therefore deduced that the existence of a certain amount of Rh(IV) may be beneficial to the improvement of photocatalytic performance. Meanwhile, it should be emphasized again that the Rh(IV) unoccupied level plays the role of a carrier recombination centre. As discussed above, the content of Rh(IV) in N3R6TNR and R6TNR was far higher than that in N3R3TNR and N6R6TNR. However, the hydrogen evolution rate of N3R6TNR (4170 μmol g−1 h−1) was much lower than that of N3R3TNR (6788 μmol g−1 h−1) or N6R6TNR (9194 μmol g−1 h−1), and the hydrogen evolution rate of R6TNR (622 μmol g−1 h−1) was even just about 1/15 of N6R6TNR (see Table 1). Obviously, the concentration of Rh(IV) must be limited to a low level by controlling the Nb/Rh ratio. According to Table 1, the optimal Nb/Rh ratio for achieving excellent photocatalytic activity is around 1. It should be pointed out that the valence state of Rh in a TiO2 lattice depends not only on the Nb/Rh ratio, but also on the preparation methods and conditions (such as calcination temperature and atmosphere). It is thus of little significance to accurately determine the optimal Nb/Rh ratio.
With the determination of calcination (500 °C) and Nb/Rh ratio (1:
1), the dependence of photocatalytic activity on the doping concentration was studied. Fig. 7a shows the hydrogen evolution performance of Ti1−2xNbxRhxO2 nanorods from methanol solution under the full arc irradiation of a Xe lamp. The amount of produced H2 increased almost linearly with irradiation time in the 10 h test, indicating the stability of the (Nb,Rh) codoped TiO2 photocatalysts. The stable hydrogen evolution rate of the samples is presented in Table 1. Obviously, the photocatalytic activity can be greatly improved by slight doping. The hydrogen evolution rate of N3R3TNR (x = 0.003) was 6788 μmol g−1 h−1, which was about 80 times higher than that of undoped TiO2. An ultrahigh evolution rate of 9194 μmol g−1 h−1 was achieved by further increasing the doping concentration to x = 0.006 (N6R6TNR). Thereafter, the photocatalytic performance decreased with increasing doping concentration, but remained above 1400 μmol g−1 h−1 even if the doping concentration reached x = 0.02. Fig. S7† shows the visible-light-driven hydrogen generation over Ti1−2xNbxRhxO2 photocatalysts (λ ≥ 420 nm). N6R6TNR presented the highest hydrogen evolution rate (75 μmol g−1 h−1) among these samples. A further increase in doping concentration led to a progressive downturn in the visible-light activity. The change in photocatalytic activity with doping concentration is related to the recombination of photogenerated electron–hole pairs. As shown in Fig. S8,† the intensity of the PL emission was markedly suppressed with slight doping (x < 0.009). However, the PL intensity increased with a further increase in the doping concentration (x > 0.009). In general, a weaker PL intensity is indicative of a lower recombination rate of photogenerated carriers.41,42 The outstanding H2 evolution performance of N3R3TNR, N6R6TNR, and N9R9TNR correlated well with their much lower electron–hole recombination. Fig. 7b shows transient photocurrent responses under visible-light irradiation (λ ≥ 420 nm). The photocurrent densities of N3R3TNR, N6R6TNR, and N9R9TNR were close, and significantly higher than those of other samples. In other words, the generation and migration rate of electron/hole pairs reached a maximum when the doping concentration fell within the range 0.003 ≤ x ≤ 0.009, which is in accord with the photocatalytic activity. Such a low optimal doping concentration is of great importance for cost saving due to the high price of rhodium.
Footnote |
† Electronic supplementary information (ESI) available: XRD patterns of TiO2-based photocatalysts with different Nb/Rh ratio and doping concentration, TEM and HRTEM images of selected samples calcined at different temperature, Nyquist and Mott–Schottky plots. See DOI: 10.1039/d0nr05695b |
This journal is © The Royal Society of Chemistry 2020 |