催化学报  2020, Vol. 41 Issue (1): 154-160      DOI: S1872-2067(19)63475-3   PDF    
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本文作者相关文章
Dashuai Li
Yu Huang
Songmei Li
Changhua Wang
Yingying Li
Xintong Zhang
Yichun Liu
Thermal coupled photoconductivity as a tool to understand the photothermal catalytic reduction of CO2
Dashuai Li, Yu Huang, Songmei Li, Changhua Wang, Yingying Li, Xintong Zhang, Yichun Liu     
Key Laboratory of UV-Emitting Materials and Technology of Chinese Ministry of Education, Northeast Normal University, Changchun 130024, Jilin, China
* Corresponding author. Changhua Wang, Tel/Fax: +86-431-85099772; E-mail:wangch100@nenu.edu.cn;
Xintong Zhang, Tel/Fax: +86-431-85099772; E-mail: xtzhang@nenu.edu.cn
These authors contribute equally to this work
This work was supported by the Natural Science Foundation of China (51072032, 51372036, 51102001), the Key Project of Chinese Ministry of Education (113020A), the 111 project (B13013), and Jilin Province Science and Technology Development Plan (20180101175JC, 20160520170JH)
Abstract: Photocatalysis shows great promise in the field of solar energy conversion. One of the reasons for this is because it promotes the development of multi-field-coupled catalysis. In order to explore the principles of multi-field-coupled catalytic reactions, an in situ multi-field-coupled characterization technique is required. In this study, we obtained hydrogenated ST-01 TiO2 and observed enhanced catalytic activity by thermal coupled photocatalysis. In situ photoconductivity was employed to understand the activity enhancement. The effects of the reaction temperature, reaction atmosphere, and oxygen vacancy (Ov) on the photoconductivity of TiO2 were studied. After coupling thermal into photoconductivity measurement, highly active Ov-TiO2 displayed rapid decay of photoconductivity in a CO2 atmosphere and slow decay of photoconductivity in a N2 atmosphere. These phenomena revealed that photothermal coupling assisted the detrapping of electrons at the Ov surface and promoted electron transfer to CO2, which clearly explained the high photothermal catalytic activity of Ov-TiO2. This study demonstrated that photoconductivity is a useful tool to help understand photothermal catalytic phenomena.
© 2020, Dalian Institute of Chemical Physics, Chinese Academy of Sciences.
Published by Elsevier B.V. All rights reserved.
Key words: Photoconduction    Photothermalcatalytic    Titanium dioxide    Oxygen vacancy    Carbon dioxide reduction    
利用光热耦合下的光电导研究TiO2光热催化还原CO2
李大帅, 黄誉, 李松美, 王长华, 李莹莹, 张昕彤, 刘益春     
东北师范大学紫外光发射材料与技术教育部重点实验室, 吉林长春 130024
摘要:利用太阳能缓解能源危机和解决环境污染,是当前和未来的全球性课题.其中,光催化技术的研究步伐日渐加快.这不仅体现在光催化材料种类的增加,更体现在以光催化为基础的多场协同催化,特别是光热耦合作用成为增强光催化性能的一种高效、可靠的方法.氧空位的引入不仅可以拓宽催化剂对可见光的吸收、抑制载流子的复合、促进反应物的吸附以及降低反应的活化能,而且对于光热协同催化效率的提升有着重要的贡献.然而,目前光热协同催化的表征多局限于常规的光催化手段.开展光热耦合下的测量技术对深刻理解光热催化是十分必要的.本文研究温度、气氛、氧空位浓度对TiO2光电导的影响,构建光电导与光热催化活性之间的关系.我们将商用的ST-01 TiO2制成浆料,利用丝网印刷法将浆料覆盖在刻有沟槽的FTO上,并通过N2/H2混合气不同温度退火,得到不同氧空位含量的TiO2薄膜(Ov-TiO2).采用紫外-可见光谱(UV-Vis),拉曼光谱(Raman),电子顺磁共振(ESR)等手段对样品进行了表征.结果表明,N2/H2退火温度越高,氧空位浓度越高.我们对不同浓度氧空位的样品进行了光催化及光热协同催化CO2还原实验.结果表明,适量氧空位的样品(H2-150)光催化还原CO2性能最差,但光热协同催化还原CO2的性能最佳.我们对其光电导值的衰减情况进行了分析,看到H2-150样品在CO2气氛、光热条件下,电导衰减加快.由于光电导的衰减是由电荷复合和电荷参与的表面反应共同决定的,为确定是哪一因素决定了电导的衰减,我们进一步测试了H2-150样品在N2气氛下的电导衰减情况.结果发现,H2-150样品在N2气氛、光热条件下电导衰减反而变慢.这表明,造成H2-150样品在CO2气氛、光热条件下的电导衰减加快是光热条件下CO2还原速率加快,也验证了H2-150具有较好的光热催化CO2活性.与H2-150样品不同的是,大量氧空位样品(H2-350)在CO2气氛、光热条件下电导衰减反而变慢,我们认为这是由于H2-350存在深能级缺陷,在热的作用下会将捕获的电子释放,因此延缓了光电导的衰减.但由于深能级电子的还原能力较弱,所以H2-350样品的光热CO2还原活性稍逊于H2-150.综上所述,在光热电导与光热催化相关的研究中,我们证实了在Ov-TiO2中被捕获的电子在热激发下可再次向导带弛豫,从而解释了Ov-TiO2优异的光热催化性能.因此,光热电导的研究在理解光热催化方面具有重要的前景.
关键词光电导    光热协同催化    二氧化钛    氧空位    二氧化碳还原    

1 Introduction

Multiple-field-coupled catalysis combined with photocatalysis is attracting increasing interest since it performs better than photocatalysis alone [1-3]. Recently, photothermal coupling has proved to be an efficient and reliable approach to improve the photocatalytic efficiency and promote the development of photothermal catalysis [4-9]. Understanding how a photothermal catalyst works requires knowledge of photocatalysis. However, present characterizations of photocatalyst systems at room temperature are insufficient to understand the effect of photothermal coupling in photothermal catalysis. In this regard, a photothermal coupled characterization technique is required to understand the mechanism of photothermal catalysis.

Photoconductivity measurement is a promising tool to detect photogenerated charge carriers, since a change in photocurrent is closely related to free carrier density [10]. Moreover, in situ thermal coupled photoconductivity can be easily achieved by integrating a heating unit in the photoconductivity test chamber. Pomoni et al. [11] studied the effect of temperature on the transient photoconductivity of a TiO2 film. They suggested that the transient photoconductivity of a nanocrystalline TiO2 film in vacuum was governed by the thermal release of electrons from the trap states in the bandgap. Liu et al. [12-14] successfully employed in situ temperature-dependent photoconductivity to understand the photocatalytic degradation of gaseous formic acid in air. They revealed that the electron transfer was determined by the interface transfer of electrons to O2 rather than by the transport. Therefore, in situ thermal coupled photoconduction can be used to study the separation, recombination, and interfacial reactions of photogenerated charges, which in turn would be useful in understanding the mechanism of photocatalysis and photothermal catalysis.

The photocatalytic activity of semiconductor oxides can be successfully enhanced by crystal facet modulation [15, 16], surface modification [17], formation of Z-scheme [18] or S-scheme heterojunctions [19, 20], and introduction of oxygen vacancies (Ov) [21-24]. Of these methods, introduction of Ov not only extends the visible light absorption range of the semiconductor [25] but also inhibits carrier recombination [26]. Ov can also promote the adsorption of reactants and decrease the activation energy of the reaction [27]. More importantly, Ov has been found to endow the photocatalyst with photothermal catalytic activity. Thus, an Ov-type semiconductor oxide is deemed as an ideal model to study the photothermal catalytic process [28, 29].

In this study, the in situ thermal coupled photoconductivity of Ov-TiO2 was used to correlate photoconductivity with the photothermal catalytic reduction of CO2. The effects of temperature and atmosphere on the photoconductivity were investigated to understand the photothermal catalytic of CO2 reduction. Moreover, Ov-TiO2 samples with different Ov contents were compared on the basis of their photoconductivity and photothermal catalytic activity to reveal the role of Ov in enhancing CO2 reduction. The aim of this study was to use photoconductivity to elucidate the mechanism of the photothermal catalytic reduction of CO2.

2 Experimental
2.1 Preparation of TiO2 film

To fabricate the TiO2 film, commercial ST-01 TiO2 (Japan, Ishihara Sangyo) was used to prepare a TiO2 slurry. The detailed preparation is shown in the supporting information. The TiO2 slurry was coated on fluorine-doped tin oxide (FTO) glass (2.5 cm × 2.5 cm) with an etched channel (77.52 μm × 2.5 cm), followed by temperature-programmed annealing in a muffle furnace up to 500 ℃. The TiO2 film was then heated in a N2/H2 atmosphere (10% H2, 90% N2) at 150 and 350 ℃, respectively. This was denoted as H2-150 and H2-350 respectively. The TiO2 film without the N2/H2 treatment was denoted as "Unannealed."

2.2 Photoconductivity test

Scheme 1 shows the device structure used for the photoconductivity measurements. The test chamber was connected to an electrochemical workstation (Keithley 2400 Sourcemeter), which was used to observe the changes in photocurrent. A heating plate was integrated at the bottom of the chamber, and the temperature was controlled using a thermocouple. The chamber contained shielded wires connected to an external electrochemical workstation for the accurate measurement of photoconductivity. UV light (Hayashi LA-410UV lamp) was irradiated through a circular quartz window (diameter, 4.5 cm) from the top of the chamber, with a light intensity of 20 mW/cm2.

Scheme 1. Schematic illustration of the device structure used for photoconductivity measurements.

Before the measurements, the chamber was pre-aerated by CO2 or N2 for 20 min to remove the air in the reactor. The flow rate of the gases was controlled by a digital gas mass flow meter and maintained at 2 L/min. Each set of measurements was commenced in a dark state for 0 to 20 s. The UV light source was then switched on at 20 s and turned off at 100 s. The measurements were conducted at room temperature and 120 ℃, respectively. The temperature of the different samples was monitored by an infrared camera. The infrared thermograms of the Unannealed, H2-150, and H2-350 samples are shown in figure S1. As can be seen, the temperature changes in the samples were primarily due to the heating of the external hot plate, while the irradiation of the external light resulted in only a small additional increase in temperature.

The photocurrent was measured and defined using the following formula [14]:

(1)

Here, U is the voltage applied by an electrochemical workstation, σ is the conductivity, L is the channel width, and A is the cross-sectional area of the TiO2 film. The applied voltage, U, was set at 1.5 V. Since the photocurrent is proportional to conductivity, the change regularity of photocurrent represents a change in conductivity. Hence, the photocurrent is directly used and not converted to photoconductivity.

2.3 Photocatalytic and photothermal catalytic reduction of CO2

In the photocatalytic test, ST-01 film was put into an airtight reactor. After sealing the reactor, carbon dioxide gas was bubbled for 20 min to expel the air from the reactor (2 L/min). The film was then irradiated by 20 mW/cm2 UV light for 3 h. A Shimadzu 2400 gas chromatograph was used to measure the yield of CO.

The photothermal catalytic experiment was similar to the above photocatalytic experiment. The schematic of the reactor is shown in Scheme 2. The difference between the two setups was that in the photothermal catalytic process, external heating was applied and the temperature was controlled at 120 ℃.

Scheme 2. Schematic illustration of the reactor used for the photothermal catalytic reduction of CO2.
3 Results and discussion

It is well reported that ST-01 is composed of an anatase phase [30, 31]. During the preparation of the TiO2 slurry and the N2/H2 treatment, no significant structural changes in TiO2 were observed in the X-ray diffraction (XRD) patterns (Fig. S2) as well as in the UV/vis spectra (Fig. 1(a)) and Raman spectra (Fig. 1(b)). However, electron spin resonance spectroscopy (ESR) (Fig. 1(c)) was able to distinguish three typical samples. The sample after hydrogen annealing showed a distinct signal at g = 2.002, where a higher annealing temperature led to a stronger signal. The signal at g = 2.002 is a characteristic feature of the ·O2- radicals generated from the interaction of the absorbed atmospheric O2 with the surface Ov sites [21, 22, 32-34]. Therefore, Ov was successfully introduced into the H2-150 and H2-350 samples. Yan et al. [35] also proposed that a vacuum or a reducing atmosphere could produce Ov, which is consistent with our results. Integral processing on the ESR signals was performed to compare the Ov in different samples quantitively. The number of spin electrons over the Unannealed, H2-150, and H2-350 samples were 5.3×10-9, 1.11×10-8, and 3.24×10-8 mol/g, respectively. Assuming that all spin electrons originated from Ov, the ratio of Ov concentration for the Unannealed, H2-150, and H2-350 samples was found to be 1 : 2.08 : 6.09.

Fig. 1. UV-vis spectra (a), Raman spectra (b), and ESR spectra (c) of the samples with different annealing temperatures.

Fig. 2 shows the catalytic reduction of CO2 via photocatalysis and photothermal catalysis, respectively. It was observed that CO was the sole product, and no CH4 was produced. This agrees with most reported results that a cocatalyst-free TiO2 system is not suitable for CH4 production due to the difficulty of multiple electron/proton transfer [36-40]. By carefully comparing CO yields, several interesting conclusions can be drawn. Firstly, thermal coupled photocatalysis for all samples significantly improved the CO yield in comparison with photocatalysis, suggesting that photothermal coupling is a powerful tool for enhancing CO2 reduction with a photocatalyst. Secondly, for photocatalysis, the introduction of Ov, unfortunately, brings a lower CO yield, with the H2-150 sample giving the lowest CO yield. This suggests that Ov is not conducive to enhanced photocatalysis. Contrary to this finding, the introduction of Ov enhances the CO yield for photothermal catalysis, with the H2-150 sample providing the highest CO yield. There is no significant activity loss after four experimental runs (Fig. S3), which suggests that Ov is suitable for enhanced photothermal catalysis. Thus, photothermal catalysis was found to be superior to photocatalysis with regards to CO2 reduction, and Ov was found to improve the activity of TiO2 in photothermal catalysis.

Fig. 2. CO yield obtained from the carbon dioxide reduction of different samples, with a UV light intensity of 20 mW/cm2, PC refers to photocatalysis carried out at room temperature, and PTC refers to photothermal catalysis carried out at 120 ℃.

As was discussed, in the photocatalytic reduction of CO2, Ov helps adsorption of CO2 and enhances CO yield. The CO2 adsorption behavior for hydrogenated TiO2 was then investigated. Fig. S4 shows that the CO2 adsorption ability follows the order: H2-350 > H2-150. However, the photothermal catalytic activity of H2-350 is lower than that of H2-150. Thus, it can be deduced that the photothermal catalytic activity is not solely governed by CO2 adsorption.

To investigate the causes for the enhanced activity of photothermal coupling and Ov, photoconductivity measurements at different conditions were performed. When comparing the photoconductivity at room temperature and 120 ℃ (Fig. 3, inset), it was found that all samples exhibit higher photoconductivity at 120 ℃. The increased photoconductivity is believed to result from the accelerated transfer of electrons from the bulk to the surface at elevated temperatures. Due to the increased number of electrons at the surface per unit time, the probability of electron/proton-coupled reduction of CO2 is enhanced. This is consistent with the enhanced activity observed in photothermal catalysis that is not seen in photocatalysis (Fig. 2).

Fig. 3. The normalized photoconductivity response after the UV light was switched off at RT (blue line, RT refers to room temperature) and HT (orange line, HT refers to 120 ℃), in a carbon dioxide atmosphere. (a) Unannealed sample; (b) H2-150 sample; (c) H2-350 sample. The dynamic change of the actual conductivity in a carbon dioxide atmosphere is given as an inset.

The decay of photoconductivity on the photoconductivity curve can provide valuable information. As shown in Fig. 3(a) and (b), both unannealed and H2-150 samples displayed an accelerated decay with the increase in temperature in a CO2 atmosphere. In principle, the decay of photoconductivity is induced by either charge recombination or a charge-involved surface reaction. Since the photoconductivity is measured in CO2, the photogenerated electrons tend to be captured by CO2, which partly contributes to decreased photoconductivity. In this regard, the accelerated decay means a higher capacity for CO2 reduction with a catalyst at higher temperatures. Therefore, the Unannealed and H2-150 samples have great potential to be activated at 120 ℃. However, the H2-350 sample displays a slower decay at elevated temperatures, as shown in Fig. 3(c). It is due to the structural difference between the H2-350 sample and the Unannealed and H2-150 samples that a higher content of Ov is present in H2-350 [41-43]. When considering the energy required for electron detrapping from the defect state to the conduction band by thermal excitation, the electrons trapped at a shallow level rather than a deep level are most likely to be excited to the conduction band [44-46]. It is well known that CO2 reduction is a multi-electron reduction process. The electrons located at the conduction band of TiO2 are thermodynamically allowed to reduce CO2 to CO. However, the electrons trapped at a deep level are unlikely to participate in CO2 reduction due to them being in lower energy state than that required for CO production. Therefore, the slower decay of photoconductivity in H2-350 is believed to partly result from the weaker reduction ability of the electrons at a deep energy level. The results are consistent with the enhanced activity in the photothermal catalysis results of H2-150 as compared to the photothermal catalysis results of H2-350 in Fig. 2. A sample of H2-550 was also prepared, and its photoconductivity was measured (Fig. S5). The decay trend of the photoconductivity of H2-550 under the atmosphere of CO2 and N2 was the same as that of H2-350. Hence, H2-350 was regarded as a standard sample with a high concentration of Ov for a photoconductivity study.

To further prove that the faster decay of photoconductivity results from the catalytic reduction of CO2 rather than charge recombination, photoconductivity measurements under a N2 atmosphere was performed. As shown in Fig. 4, the decay of thermal coupled photoconductivity of the H2-150 and the H2-350 samples was slower in a N2 atmosphere compared to a CO2 atmosphere. The H2-150 sample, in particular, shows a significant difference in the decay of photoconductivity under CO2 as compared to the N2 atmosphere. However, this slower decay of photoconductivity under a N2 atmosphere is not observed for unannealed TiO2. The mechanism diagram for this is shown in Scheme S1. According to the analysis of the changes in photoconductivity in the CO2 atmosphere and N2 atmosphere, the results can be interpreted in two ways. On the one hand, the charge recombination of the H2-150 sample and the H2-350 sample does not decrease upon thermal activation, since it benefits from the introduction of Ov. On the other hand, the photogenerated electrons trapped by Ov can be released to the conduction band. This detrapping of electrons can accelerate surface reactions.

Fig. 4. The normalized photoconductivity response after the UV light was switched off at RT (blue line, RT refers to room temperature) and HT (orange line, HT refers to 120 ℃), in a N2 atmosphere. (a) Unannealed sample; (b) H2-150 sample; (c) H2-350 sample. The dynamic change in conductivity in the N2 atmosphere is given as an inset.

Several conclusions can be drawn above from the photoconductivity test: (1) Thermal coupled photoconductivity is higher than room-temperature photoconductivity for the unannealed TiO2 and Ov-TiO2; (2) The accelerated decay of photoconductivity for Ov-TiO2 in the simulated photothermal reaction implies a promoted charge-involved surface reaction; (3) The slower decay of photoconductivity for Ov-TiO2 implies thermal detrapping of electrons at Ov.

To correlate thermal coupled photoconductivity with photothermal catalysis, the mechanism shown in Scheme 3 was proposed. Upon photoexcitation, the electrons of the valence band can be excited to the conduction band or trapped by shallow Ov located below the conduction band. The surface adsorbed CO2 can be reduced by coupled electrons/protons. At this stage, the thermal coupled photoconductivity was increased in comparison to room temperature photoconductivity, due to the combined contribution of photo-induced excitation and thermal-induced detrapping of electrons. When the UV light is switched off, the trapped electrons at Ov gradually recombine with nearby holes at room temperature. The stored electrons seldom transfer to the surface and participate in CO2 reduction, which leads to a slow electron consumption rate by CO2. Therefore, a slower decay of photoconductivity is observed. At a higher temperature, the trapped electrons at Ov tend to escape to the conduction band and are then transferred to the surface, which leads to a faster electron consumption rate by CO2. Hence, a faster decay of photoconductivity is observed.

Scheme 3. Schematic illustration of the thermal coupled photoconductivity of Ov-TiO2 in CO2, (RT refers to room temperature).
4 Conclusions

In summary, thermal coupled photoconductivity was measured to obtain an understanding of the photothermal catalytic reduction of CO2. Photothermal catalysis shows that the introduction of Ov can significantly enhance the CO yield over Ov-TiO2. In comparison to room temperature photoconductivity, thermal coupled photoconductivity of highly active Ov-TiO2 exhibits an accelerated decay in a CO2 atmosphere and a decelerated decay in a N2 atmosphere. With regards to the correlation between thermal coupled photoconductivity and photothermal catalysis, an accelerated electron transfer to CO2 and the detrapping of electrons to the conduction band of TiO2 are confirmed, which provides a reasonable explanation for the superior performance of Ov-TiO2 in photothermal catalysis. This study on thermal coupled photoconductivity could represent a promising method for understanding photothermal catalysis.

References
[1]
Z. F. Jiang, H. L. Sun, T. Q. Wang, B. Wang, W. Wei, H. M. Li, S. Q. Yuan, T. C. An, H. J. Zhao, J. G. Yu, P. K. Wong, Energy Environ. Sci., 2018, 11, 2382-2389. DOI:10.1039/C8EE01781F
[2]
K. K. Paul, N. Sreekanth, R. K. Biroju, A. J. Pattison, D. Escalera-Lopez, A. Guha, T. N. Narayanan, N. V. Rees, W. Theisc, P. K. Giri, J. Mater. Chem. A, 2018, 6, 22681-22696. DOI:10.1039/C8TA06783J
[3]
J. Ren, S. X. Ouyang, H. Xu, X. G. Meng, T. Wang, D. F. Wang, J. H. Ye, Adv. Energy Mater., 2017, 7, 1601657. DOI:10.1002/aenm.201601657
[4]
J. X. Low, L. Y. Zhang, B. C. Zhu, Z. Y. Liu, J. G. Yu, ACS Sustainable Chem. Eng., 2018, 6, 15653-15661. DOI:10.1021/acssuschemeng.8b04150
[5]
L. Zhang, G. G. Kong, Y. P. Meng, J. S. Tian, L. J. Zhang, S. L. Wan, J. D. Lin, Y. Wang, ChemSusChem, 2017, 10, 4709-4714. DOI:10.1002/cssc.201701472
[6]
L. Wang, Y. Wang, Y. Cheng, Z. Liu, Q. Guo, M. N. Ha, Z. Zhao, J. Mater. Chem. A, 2016, 4, 5314-5322. DOI:10.1039/C5TA10180H
[7]
B. Liu, X. Zhao, C. Terashima, A. Fujishima, K. Nakata, Phys. Chem. Chem. Phys., 2014, 16, 8751-8760. DOI:10.1039/c3cp55317e
[8]
G. Chen, R. Gao, Y. Zhao, Z. Li, G. I. N. Waterhouse, R. Shi, J. Zhao, M. Zhang, L. Shang, G. Sheng, X. Zhang, X. Wen, L. Z. Wu, C. H. Tung, T. Zhang, Adv. Mater., 2018, 30, 1704663. DOI:10.1002/adma.201704663
[9]
W. Zhang, L. Wang, K. Wang, M. U. Khan, M. Wang, H. Li, J. Zeng, Small, 2017, 13, 201602583.
[10]
J. Nelson, A. M. Eppler, I. M. Ballard, J. Photochem. Photobiol. A, 2002, 148, 25-31. DOI:10.1016/S1010-6030(02)00035-7
[11]
K. Pomonia, A. Vomvas, C. Trapalib, Thin Solid Films, 2005, 479, 160-165. DOI:10.1016/j.tsf.2004.12.005
[12]
B. S. Liu, X. L. Wang, L. P. Wen, X. J. Zhao, Chem. Eur. J., 2013, 19, 10751-10759. DOI:10.1002/chem.201300243
[13]
J. J. Yang, B. S. Liu, H. Xie, X. J. Zhao, C. Terashima, A. Fujishima, K. Nakata, J. Phys. Chem. C, 2015, 119, 21711-21722. DOI:10.1021/acs.jpcc.5b06534
[14]
B. S. Liu, J. J. Yang, X. J. Zhao, J. G. Yu, Phys. Chem. Chem. Phys., 2017, 19, 8866-8873. DOI:10.1039/C6CP07328J
[15]
J. Y. Wang, B. S. Liu, K. Nakata, Chin. J. Catal., 2019, 40, 403-412. DOI:10.1016/S1872-2067(18)63174-2
[16]
Y. A. Zhu, Z. Y. Zhang, N. Lu, R. N. Hua, B. Dong, Chin. J. Catal., 2019, 40, 413-423. DOI:10.1016/S1872-2067(18)63182-1
[17]
J. X. Low, B. Cheng, J. G. Yu, Appl. Surf. Sci., 2017, 392, 658-686. DOI:10.1016/j.apsusc.2016.09.093
[18]
J. X. Low, B. Z. Dai, T. Tong, C. J. Jiang, J. G. Yu, Adv. Mater., 2019, 31, 1802981. DOI:10.1002/adma.201802981
[19]
J. W. Fu, Q. L. Xu, J. X. Low, C. J. Jiang, J. G. Yu, Appl. Catal. B, 2019, 243, 556-565. DOI:10.1016/j.apcatb.2018.11.011
[20]
M. Edelmannov, K. Y. Lin, J. C. S. Wu, I. Troppov, L. Čapek, K. Ko, Appl. Surf. Sci., 2018, 454, 313-318.
[21]
L. N. Kong, Z. Q. Jiang, C. H. Wang, F. X. Wan, Y. Y. Li, L. Z. Wu, J. F. Zhi, X. T. Zhang, S. J. Chen, Y. C. Liu, ACS Appl. Mater. Inter., 2015, 7, 7752-7758. DOI:10.1021/acsami.5b00888
[22]
L. N. Kong, C. H. Wang, F. X. Wan, H. Zheng, X. T. Zhang, Appl. Surf. Sci., 2017, 396, 26-35.
[23]
A. Nikokavoura, C. Trapalis, Appl. Surf. Sci., 2017, 391, 149-174.
[24]
K. Z. Qi, S. Y. Liu, M. Qiu, Chin. J. Catal., 2018, 39, 867-875. DOI:10.1016/S1872-2067(17)62999-1
[25]
T. Wang, W. W. Li, D. D. Xu, X. M. Wu, L. W. Cao, J. X. Meng, Chin. J. Catal., 2017, 38, 1184-1195. DOI:10.1016/S1872-2067(17)62855-9
[26]
L. Li, P. Li, Y. J. Wang, L. Lin, A. H. Shah, T. He, Appl. Surf. Sci., 2018, 452, 498-506. DOI:10.1016/j.apsusc.2018.04.256
[27]
Y. Sohn, W. X. Huang, F. Taghipour, Appl. Surf. Sci., 2017, 396, 1696-1711. DOI:10.1016/j.apsusc.2016.11.240
[28]
X. B. Li, J. Xiong, Y. Xu, Z. J. Feng, J. T. Huang, Chin. J. Catal., 2019, 40, 424-433. DOI:10.1016/S1872-2067(18)63183-3
[29]
X. B. Li, J. Xiong, X. M. Gao, J. T. Huang, Z. J. Feng, Z. Chen, Y. F. Zhu, J. Alloys Compd., 2019, 802, 196-209. DOI:10.1016/j.jallcom.2019.06.185
[30]
S. Moziaa, A. W. Morawski, M. Toyoda, M. Inagaki, Sep. Purif. Technol., 2008, 63, 386-391.
[31]
P. H. Wen, H. Itoh, W. P. Tang, Q. Feng, Langmuir, 2007, 23, 11782-11790. DOI:10.1021/la701632t
[32]
K. Komaguchi, T. Maruoka, H. Nakano, I. Imae, Y. Oyama, Y. Harima, J. Phys. Chem. C, 2010, 114, 1240-245. DOI:10.1021/jp909678e
[33]
I. Nakamura, N. Negishi, S. Kutsuna, T. Ihara, S. Sugihara, K. Takeuchi, J. Mol. Catal. A, 2000, 161, 205-212. DOI:10.1016/S1381-1169(00)00362-9
[34]
S. H. Wei, S. Ni, X. X. Xu, Chin. J. Catal., 2018, 39, 510-516. DOI:10.1016/S1872-2067(17)62968-1
[35]
H. Yu, S. C. Yan, P. Zhou, Z. G. Zou, Appl. Surf. Sci., 2018, 427, 603-607.
[36]
Y. Y. Li, C. H. Wang, M. Song, D. S. Li, X. T. Zhang, Y. C. Liu, Appl. Catal. B, 2019, 243, 760-770. DOI:10.1016/j.apcatb.2018.11.022
[37]
X. Y. Liu, M. Ye, S. P. Zhang, G. C. Huang, C. H. Li, J. G. Yu, P. K. Wong, S. W. Liu, J. Mater. Chem. A, 2018, 6, 24245-24255. DOI:10.1039/C8TA09661A
[38]
A. Y. Meng, L.Y. Zhang, B. Cheng, J. G. Yu, ACS Appl. Mater. Interfaces, 2019, 11, 5581-5589. DOI:10.1021/acsami.8b02552
[39]
T. Yui, A. Kan, C. Saitoh, K. Koike, T. Ibusuki, O. Ishitani, ACS Appl. Mater. Interfaces, 2011, 3, 2594-2600. DOI:10.1021/am200425y
[40]
X. G. Meng, T. Wang, L. Q. Liu, S. X. Ouyang, P. Li, H. L. Hu, T. Kako, H. Iwai, A. Tanaka, J. H. Ye, Angew. Chem. Int. Ed., 2014, 53, 11478-11482. DOI:10.1002/anie.201404953
[41]
L. C. Wang, Y. Wang, Y. Cheng, Z. F. Liu, Q. S. Guo, M. N. Ha, Z. Zhao, J. Mater. Chem. A., 2016, 4, 5314-5322. DOI:10.1039/C5TA10180H
[42]
X. B. Chen, L. Liu, P. Y. Yu, S. S. Mao, Science, 2011, 331, 746-750. DOI:10.1126/science.1200448
[43]
G. B. Zhang, T. F. Xiong, M. Y. Yan, L. He, X. B. Liao, C. Q. He, C. S. Yin, H. N. Zhang, L. Q. Mai, Nano Energy, 2018, 49, 555-563. DOI:10.1016/j.nanoen.2018.04.075
[44]
J. C. Bourgoin, M. Zazoui, Phys. Rev. B, 1992, 45, 11324. DOI:10.1103/PhysRevB.45.11324
[45]
P. Ščajev, S. Miasojedovas, L. Subačius, K. JarašiūnaS, A. V. Mazanik, O. V. Korolik, M. Kato, J. Lumin., 2019, 212, 92-98. DOI:10.1016/j.jlumin.2019.04.018
[46]
L. L. Hou, Z. J. Guan, M. Zhang, C. Q. He, Q. Y. Li, J. J. Yang, Catal. Sci. Technol., 2018, 8, 2809-2817. DOI:10.1039/C8CY00644J