
物理化学学报 >> 2024, Vol. 40 >> Issue (1): 2304004.doi: 10.3866/PKU.WHXB202304004
所属专题: 多物理场能源催化转化
张城城1,2,†, 吴之怡2,†, 沈家辉2, 何乐2,*(
), 孙威1,*(
)
收稿日期:2023-04-03
修回日期:2023-05-05
录用日期:2023-05-08
发布日期:2023-08-21
通讯作者:
Email: sunnyway423@zju.edu.cn; Tel.: +86-571-87951667 (孙威)lehe@suda.edu.cn (何乐)
作者简介:†These authors contributed equally to this work.
基金资助:
Chengcheng Zhang1,2, Zhiyi Wu2, Jiahui Shen2, Le He2,*(
), Wei Sun1,*(
)
Received:2023-04-03
Revised:2023-05-05
Accepted:2023-05-08
Published:2023-08-21
Contact:
Email: sunnyway423@zju.edu.cn; Tel.: +86-571-87951667 (Wei Sun)lehe@suda.edu.cn (Le He)
Supported by:摘要:
人口的快速增长和高能源需求产业造成了严重的环境问题。太阳能等替代性的清洁能源对于缓解能源危机和温室效应至关重要。光催化是一种很有前途的方法,但它在转化率、效率和规模化方面存在局限性。光热催化则结合了光化学和光热效应,是在温和条件下有效催化化学反应的新概念。近年来,与传统的光热催化剂相比,硅纳米结构阵列在光热CO2还原反应中表现出独特的催化性能优势。作为一种平台,它表现出优异的光收集能力、高比表面积以及多样化的材料复合选择。本文综述了光热催化CO2转化的概念和原理,硅纳米结构阵列的功能,以及利用硅纳米结构阵列在光热催化CO2转化方面的最新进展,最终将为高性能纳米结构阵列光热CO2催化剂的发展方向提供指导。
张城城, 吴之怡, 沈家辉, 何乐, 孙威. 硅纳米结构阵列:光热CO2催化的新兴平台[J]. 物理化学学报, 2024, 40(1), 2304004. doi: 10.3866/PKU.WHXB202304004
Chengcheng Zhang, Zhiyi Wu, Jiahui Shen, Le He, Wei Sun. Silicon Nanostructure Arrays: An Emerging Platform for Photothermal CO2 Catalysis[J]. Acta Phys. -Chim. Sin. 2024, 40(1), 2304004. doi: 10.3866/PKU.WHXB202304004
Fig 2
(a) Diffuse reflectance spectra of Ni/Nb2C and Ni/Nb2O5. (b) The CO2 conversion rate of Ni/Nb2C under different illumination intensities. (c) Schematic of the nanoscale greenhouse effect in Ni@p-SiO2. (d) The photothermal catalytic activity of Ni@p-SiO2 under different illumination conditions. (e) The mid-gap energy states near the CB and VB edges of the In2O3−x/In2O3 heterostructure. (f) TEM images of Pd0.82Ni0.18-SiO2. (a, b) Adapted from American Chemical Society publisher 75. (c, d) Adapted from Springer Nature publisher 76. (e) Adapted from Springer Nature publisher 85. (f) Adapted from John Wiley and Sons publisher 86."
Fig 3
(a) The absorption spectra of different support catalysts. (b) Methanation rates over Ru-based catalysts on the SiNW, glass and polished Si supports. (c) Methanation rates under the dark and solar-simulated irradiation. The inset shows the calculation of activation energy in the light and dark. (d) Schematic illustration of light filter experimental apparatus. (e) A comparison between the absorption spectrum of In2O3−x(OH)y and the solar irradiance spectrum. (f) 13CO production rates of In2O3−x(OH)y/SiNW, bilayer In2O3−x(OH)y/SiNW, and In2O3−x(OH)y/glass in the dark and under illumination, with or without external heating. (a–d) Adapted from John Wiley and Sons publisher 101. (e, f) Adapted from American Chemical Society publisher 102."
Fig 5
(a) Schematic illustration of the thinning strategy for thermal management. (b) Surface temperatures and (c) Catalytic performances of nanocone arrays catalysts with different substrate thicknesses. (d–g) SEM images of ncRuO2/i-Si-o with different magnifications. (a–c) Adapted from Royal Society of Chemistry publisher 104. (d–g) Adapted from John Wiley and Sons publisher 107."
Fig 7
(a) Photomethanation rates over Ru/i-Si-o and Ru/SiO2-o under different incident light intensities. (b) The incident light spectra for tests performed without a filter and with a 495 nm high-pass cut-off filter. (c) Diffuse reflectance spectra of different cobalt catalysts. (d) Scheme showing the growth process of Co-PS@SiO2. (e) The Fourier transform curves of the EXAFS spectra at the Co K-edge for Co-PS@SiO2. (a, b) Adapted from Energy Environ. Sci., Royal Society of Chemistry publisher 108. (c–e) Adapted from John Wiley and Sons publisher 109."
Table 1
Performance of various silicon nanostructure arrays-based catalysts in photothermal CO2 hydrogenation."
| Catalyst | Light source | H2 : CO2 | RCO2 (mol∙gcat −1∙h−1) | Reference |
| Ru/SiNW | 300 W Xe light (0.32 W∙cm−2) | 4 : 1 | 1.1 × 10−4 | |
| In2O3−x(OH)y/SiNW | 300 W Xe light (2.0 W∙cm−2) | 1 : 1 | 2.2 × 10−5 | |
| SNAs@Co | 300 W Xe light (2.5 W∙cm−2) | 1 : 1 | 4.3 × 10−1 | |
| SiNCs@Co | 300 W Xe light (2.5 W∙cm−2) | 1 : 1 | 1.78 | |
| ncRuO2/i-Si-o | 300 W Xe light (2.2 W∙cm−2) | 4 : 1 | 4.4 × 10−3 | |
| Ru/i-Si-o | 300 W Xe light (2.5 W∙cm−2) | 4 : 1 | 2.8 × 10−3 | |
| Co@SiO2-array | 300 W Xe light (2.4 W∙cm−2) | 1 : 1 | 4.1 × 10−2 | |
| Co-PS@SiO2 | 300 W Xe light (2.5 W∙cm−2) | 1 : 1 | 0.60 |
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