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Bismuth-rich bismuth oxyiodide microspheres with abundant oxygen vacancies as an efficient photocatalyst for nitrogen fixation
Solar-driven reduction of dinitrogen (N 2 ) to ammonia (NH 3 ) is still challenging due to the highly stable N-N triple bond. Herein, orthorhombic phase H-Bi 5 O 7 I microspheres with abundant oxygen vacancies (OVs) were successfully prepared via a simple calcination and hydrogen reduction strategy....
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Published in: | Dalton transactions : an international journal of inorganic chemistry 2020-07, Vol.49 (26), p.9123-9129 |
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Main Authors: | , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | Solar-driven reduction of dinitrogen (N
2
) to ammonia (NH
3
) is still challenging due to the highly stable N-N triple bond. Herein, orthorhombic phase H-Bi
5
O
7
I microspheres with abundant oxygen vacancies (OVs) were successfully prepared
via
a simple calcination and hydrogen reduction strategy. Based on the combined bismuth-rich strategy and the introduction of OVs in H-Bi
5
O
7
I, a remarkable photocatalytic nitrogen fixation performance was achieved under visible light irradiation in the absence of any organic scavengers or noble-metal cocatalysts. H-Bi
5
O
7
I exhibits an NH
4
+
generation rate of 162.48 μmol g
−1
h
−1
, which is 2.0 and 7.4 times higher than that of Bi
5
O
7
I and BiOI. It is because H-Bi
5
O
7
I with abundant OVs has a more proper band gap, better electron capturing ability and more effective separation and transfer rate for the photogenerated charge carriers. This study may provide a new direction and useful insight for the design of defect assisted N
2
fixation photocatalysts.
A combined bismuth-rich and defect introduction strategy was used to prepare the H-Bi
5
O
7
I with abundant oxygen vacancies, which can effectively yield ammonia under visible light without any organic scavengers or noble-metal cocatalysts. |
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ISSN: | 1477-9226 1477-9234 |
DOI: | 10.1039/d0dt01332c |