Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/105670
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Type: Journal article
Title: Ti₃C₂ MXene co-catalyst on metal sulfide photo-absorbers for enhanced visible-light photocatalytic hydrogen production
Other Titles: Ti(3)C(2) MXene co-catalyst on metal sulfide photo-absorbers for enhanced visible-light photocatalytic hydrogen production
Author: Ran, J.
Gao, G.
Li, F.
Ma, T.
Du, A.
Qiao, S.
Citation: Nature Communications, 2017; 8(1):13907-1-13907-10
Publisher: Nature Publishing Group
Issue Date: 2017
ISSN: 2041-1723
2041-1723
Statement of
Responsibility: 
Jingrun Ran, Guoping Gao, Fa-Tang Li, Tian-Yi Ma, Aijun Du and Shi-Zhang Qiao
Abstract: Scalable and sustainable solar hydrogen production through photocatalytic water splitting requires highly active and stable earth-abundant co-catalysts to replace expensive and rare platinum. Here we employ density functional theory calculations to direct atomic-level exploration, design and fabrication of a MXene material, Ti3C2 nanoparticles, as a highly efficient co-catalyst. Ti3C2 nanoparticles are rationally integrated with cadmium sulfide via a hydrothermal strategy to induce a super high visible-light photocatalytic hydrogen production activity of 14,342 μmol h-1 g-1 and an apparent quantum efficiency of 40.1% at 420 nm. This high performance arises from the favourable Fermi level position, electrical conductivity and hydrogen evolution capacity of Ti3C2 nanoparticles. Furthermore, Ti3C2 nanoparticles also serve as an efficient co-catalyst on ZnS or ZnxCd1-xS. This work demonstrates the potential of earth-abundant MXene family materials to construct numerous high performance and low-cost photocatalysts/photoelectrodes.
Rights: © The Author(s) 2017. This work is licensed under a Creative Commons Attribution 4.0 International License. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in the credit line; if the material is not included under the Creative Commons license, users will need to obtain permission from the license holder to reproduce the material. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/
DOI: 10.1038/ncomms13907
Grant ID: http://purl.org/au-research/grants/arc/DP160104866
http://purl.org/au-research/grants/arc/DP140104062
http://purl.org/au-research/grants/arc/DP130104459
Published version: http://dx.doi.org/10.1038/ncomms13907
Appears in Collections:Aurora harvest 3
Physics publications

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