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缺氧对WO激发态动力学的影响及其对光催化的意义。

Effect of oxygen deficiency on the excited state kinetics of WO and implications for photocatalysis.

作者信息

Sachs Michael, Park Ji-Sang, Pastor Ernest, Kafizas Andreas, Wilson Anna A, Francàs Laia, Gul Sheraz, Ling Min, Blackman Chris, Yano Junko, Walsh Aron, Durrant James R

机构信息

Department of Chemistry , Imperial College London , London , SW7 2AZ , UK . Email:

Department of Materials , Imperial College London , London , SW7 2AZ , UK.

出版信息

Chem Sci. 2019 May 9;10(22):5667-5677. doi: 10.1039/c9sc00693a. eCollection 2019 Jun 14.

DOI:10.1039/c9sc00693a
PMID:31293751
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC6563783/
Abstract

Oxygen vacancies are widely used to tune the light absorption of semiconducting metal oxides, but a photophysical framework describing the impact of such point defects on the dynamics of photogenerated charges, and ultimately on catalysis, is still missing. We herein use WO as a model material and investigate the impact of significantly different degrees of oxygen deficiency on its excited state kinetics. For highly oxygen-deficient films, photoelectron spectroscopy shows an over 2 eV broad distribution of oxygen vacancy states within the bandgap which gives rise to extended visible light absorption. We examine the nature of this distribution using first-principles defect calculations and find that defects aggregate to form clusters rather than isolated vacancy sites. Using transient absorption spectroscopy, we observe trapping of photogenerated holes within 200 fs after excitation at high degrees of oxygen deficiency, which increases their lifetime at the expense of oxidative driving force. This loss in driving force limits the use of metal oxides with significant degrees of sub-stoichiometry to photocatalytic reactions that require low oxidation power such as pollutant degradation, and highlights the need to fine-tune vacancy state distributions for specific target reactions.

摘要

氧空位被广泛用于调节半导体金属氧化物的光吸收,但是一个描述此类点缺陷对光生电荷动力学以及最终对催化作用影响的光物理框架仍然缺失。我们在此使用WO作为模型材料,并研究显著不同程度的氧缺陷对其激发态动力学的影响。对于高度缺氧的薄膜,光电子能谱显示在带隙内氧空位态有超过2 eV的宽分布,这导致了扩展的可见光吸收。我们使用第一性原理缺陷计算来研究这种分布的性质,发现缺陷聚集形成簇而不是孤立的空位位点。使用瞬态吸收光谱,我们观察到在高度缺氧情况下激发后200 fs内光生空穴的俘获,这增加了它们的寿命,但以氧化驱动力为代价。这种驱动力的损失限制了具有显著亚化学计量比的金属氧化物在需要低氧化能力的光催化反应(如污染物降解)中的应用,并突出了针对特定目标反应微调空位态分布的必要性。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f9f2/6563783/a2bee41f51fa/c9sc00693a-f5.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f9f2/6563783/a2bee41f51fa/c9sc00693a-f5.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f9f2/6563783/9f1208f2dedf/c9sc00693a-f1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f9f2/6563783/31e4c517fe97/c9sc00693a-f2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f9f2/6563783/e4c4ba2ab91b/c9sc00693a-f3.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f9f2/6563783/a2bee41f51fa/c9sc00693a-f5.jpg

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