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金属氮掺杂碳催化剂在CO电还原过程中的可逆结构演变:原位X射线吸收光谱研究

Reversible Structural Evolution of Metal-Nitrogen-Doped Carbon Catalysts During CO Electroreduction: An Operando X-ray Absorption Spectroscopy Study.

作者信息

Hursán Dorottya, Timoshenko Janis, Ortega Eduardo, Jeon Hyo Sang, Rüscher Martina, Herzog Antonia, Rettenmaier Clara, Chee See Wee, Martini Andrea, Koshy David, Roldán Cuenya Beatriz

机构信息

Department of Interface Science, Fritz-Haber Institute of the Max Planck Society, Faradayweg 4-6, 14195, Berlin, Germany.

出版信息

Adv Mater. 2024 Jan;36(4):e2307809. doi: 10.1002/adma.202307809. Epub 2023 Dec 7.

Abstract

Electrochemical CO reduction (CO RR) is a rising technology, aiming to reduce the energy sector dependence on fossil fuels and to produce carbon-neutral raw materials. Metal-nitrogen-doped carbons (M-N-C) are emerging, cost-effective catalysts for this reaction; however, their long-term stability is a major issue. To overcome this, understanding their structural evolution is crucial, requiring systematic in-depth operando studies. Here a series of M-N-C catalysts (M = Fe, Sn, Cu, Co, Ni, Zn) is investigated using operando X-ray absorption spectroscopy. It is found that the Fe-N-C and Sn-N-C are prone to oxide clusters formation even before CO RR. In contrast, the respective metal cations are singly dispersed in the as-prepared Cu-N-C, Co-N-C, Ni-N-C, and (Zn)-N-C. During CO RR, metallic clusters/nanoparticles reversibly formed in all catalysts, except for the Ni-N-C. This phenomenon, previously observed only in Cu-N-C, thus is ubiquitous in M-N-C catalysts. The competition between M-O and M-N interactions is an important factor determining the mobility of metal species in M-N-C. Specifically, the strong interaction between the Ni centers and the N-functional groups of the carbon support results in higher stability of the Ni single-sites, leading to the excellent performance of Ni-N-C in the CO to CO conversion, in comparison to other transition metals.

摘要

电化学一氧化碳还原(CO RR)是一项新兴技术,旨在减少能源部门对化石燃料的依赖,并生产碳中和原材料。金属氮掺杂碳(M-N-C)是用于该反应的新兴且具有成本效益的催化剂;然而,它们的长期稳定性是一个主要问题。为了克服这一问题,了解它们的结构演变至关重要,这需要系统深入的原位研究。在此,使用原位X射线吸收光谱对一系列M-N-C催化剂(M = Fe、Sn、Cu、Co、Ni、Zn)进行了研究。研究发现,即使在CO RR之前,Fe-N-C和Sn-N-C也容易形成氧化物簇。相比之下,在制备好的Cu-N-C、Co-N-C、Ni-N-C和(Zn)-N-C中,相应的金属阳离子是单分散的。在CO RR过程中,除了Ni-N-C之外,所有催化剂中都可逆地形成了金属簇/纳米颗粒。这种以前仅在Cu-N-C中观察到的现象,因此在M-N-C催化剂中普遍存在。M-O和M-N相互作用之间的竞争是决定M-N-C中金属物种迁移率的一个重要因素。具体而言,Ni中心与碳载体的N官能团之间的强相互作用导致Ni单中心具有更高的稳定性,与其他过渡金属相比导致Ni-N-C在CO到CO转化中具有优异的性能。

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