Suppr超能文献

用于高效太阳能驱动光催化CO还原的无贵金属高熵合金纳米颗粒

Noble-Metal-Free High-Entropy Alloy Nanoparticles for Efficient Solar-Driven Photocatalytic CO Reduction.

作者信息

Huang Haowei, Zhao Jiwu, Guo Hele, Weng Bo, Zhang Hongwen, Saha Rafikul Ali, Zhang Menglong, Lai Feili, Zhou Yufan, Juan Rubio-Zuazo, Chen Peng-Cheng, Wang Sibo, Steele Julian A, Zhong Fulan, Liu Tianxi, Hofkens Johan, Zheng Yu-Ming, Long Jinlin, Roeffaers Maarten B J

机构信息

cMACS, Department of Microbial, and Molecular Systems, KU Leuven, Celestijnenlaan 200F, Leuven, 3001, Belgium.

State Key Lab of Photocatalysis on Energy and Environment, College of Chemistry, Fuzhou University, Fuzhou, 350116, China.

出版信息

Adv Mater. 2024 Jun;36(26):e2313209. doi: 10.1002/adma.202313209. Epub 2024 Apr 21.

Abstract

Metal nanoparticle (NP) cocatalysts are widely investigated for their ability to enhance the performance of photocatalytic materials; however, their practical application is often limited by the inherent instability under light irradiation. This challenge has catalyzed interest in exploring high-entropy alloys (HEAs), which, with their increased entropy and lower Gibbs free energy, provide superior stability. In this study, 3.5 nm-sized noble-metal-free NPs composed of a FeCoNiCuMn HEA are successfully synthesized. With theoretic calculation and experiments, the electronic structure of HEA in augmenting the catalytic CO reduction has been uncovered, including the individual roles of each element and the collective synergistic effects. Then, their photocatalytic CO reduction capabilities are investigated when immobilized on TiO. HEA NPs significantly enhance the CO photoreduction, achieving a 23-fold increase over pristine TiO, with CO and CH production rates of 235.2 and 19.9 µmol g h, respectively. Meanwhile, HEA NPs show excellent stability under simulated solar irradiation, as well high-energy X-ray irradiation. This research emphasizes the promising role of HEA NPs, composed of earth-abundant elements, in revolutionizing the field of photocatalysis.

摘要

金属纳米颗粒(NP)助催化剂因其增强光催化材料性能的能力而受到广泛研究;然而,它们的实际应用常常受到光照下固有不稳定性的限制。这一挑战激发了人们对探索高熵合金(HEA)的兴趣,高熵合金由于其增加的熵和更低的吉布斯自由能而具有卓越的稳定性。在本研究中,成功合成了由FeCoNiCuMn高熵合金组成的尺寸为3.5纳米的无贵金属纳米颗粒。通过理论计算和实验,揭示了高熵合金在增强催化CO还原中的电子结构,包括各元素的单独作用和集体协同效应。然后,研究了它们固定在TiO上时的光催化CO还原能力。高熵合金纳米颗粒显著增强了CO光还原,与原始TiO相比提高了23倍,CO和CH的产率分别为235.2和19.9微摩尔·克⁻¹·小时⁻¹。同时,高熵合金纳米颗粒在模拟太阳辐射以及高能X射线辐射下均表现出优异的稳定性。这项研究强调了由储量丰富的元素组成的高熵合金纳米颗粒在变革光催化领域方面的广阔前景。

文献AI研究员

20分钟写一篇综述,助力文献阅读效率提升50倍。

立即体验

用中文搜PubMed

大模型驱动的PubMed中文搜索引擎

马上搜索

文档翻译

学术文献翻译模型,支持多种主流文档格式。

立即体验