journal article·2019-08-21

Mimicking π Backdonation in Ce-MOFs for Solar-Driven Ammonia Synthesis

Congmin Zhang, Yanling Xu, Chade Lv, Xin Zhou, Yu Wang, Weinan Xing, Qingqiang Meng, Yi Kong, Gang Chen

ACS Applied Materials & Interfaces· Volume 11· Issue 33
Publisher page

Abstract

π Backdonation is the core process to break through the kinetically complex and energetic hurdle for catalyzing effectively the NH3 synthesis but only occurs on certain transition metals with empty and filled d orbitals. Herein, mimicking π backdonation enables MOF-76(Ce) materials to convert N2/NH3 effectively. Note that, by virtue of the intrinsic mechanism of ligand-to-metal charge transfer, metal cerium species in MOF-76(Ce) serve as an electron sink for accumulating the photogenerated electrons. Taken together, experimental and theoretical analyses reveal that such metal cerium species with coordination unsaturated state (Ce-CUS) on a MOF-76(Ce) nanorod surface can also provide unoccupied and occupied 4f orbitals to accept from and then donate electrons back to nitrogen molecules. Remarkably, it shows outstanding photocatalytic nitrogen reduction performance with high average NH3 yield (34 μmol g–1 h–1) under ambient conditions. This work provides fresh insights into rational designing and engineering highly active catalysts with rare earth elements.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Ammonia Synthesis and Nitrogen Reduction · Advanced Photocatalysis Techniques · Metal-Organic Frameworks: Synthesis and Applications

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Department of Materials Chemistry, School of Chemistry and Chemical Engineering, Harbin Institute of Technology, Harbin 150001, P. R. China

College of Biology and the Environment, Nanjing Forestry University, Nanjing 210037, China

Funding

National Natural Science Foundation of China

References (31)

Show source-provided references
1. 10.1002/adma.20160479910.1002/adma.201604799 ↗
2. 10.1002/smtd.20180038810.1002/smtd.201800388 ↗
3. 10.1002/smtd.20180035210.1002/smtd.201800352 ↗
4. 10.1039/c7mh00557a10.1039/c7mh00557a ↗
5. 10.1039/C4CS00085D10.1039/C4CS00085D ↗
6. 10.1021/ja512491v10.1021/ja512491v ↗
7. 10.1021/jacs.7b0663410.1021/jacs.7b06634 ↗
8. 10.1021/jacs.7b0521310.1021/jacs.7b05213 ↗
9. 10.1126/science.aaq168410.1126/science.aaq1684 ↗
10. 10.1039/c6ta09275f10.1039/c6ta09275f ↗
11. 10.1002/smtd.20180038610.1002/smtd.201800386 ↗
12. 10.1039/c2ee22310d10.1039/c2ee22310d ↗
13. 10.1021/acscatal.6b0049010.1021/acscatal.6b00490 ↗
14. 10.1126/science.aat975010.1126/science.aat9750 ↗
15. 10.1039/C8QO00893K10.1039/C8QO00893K ↗
16. 10.1002/adma.20170366310.1002/adma.201703663 ↗
17. 10.1039/c4cs90059f10.1039/c4cs90059f ↗
18. 10.1002/adma.20170450110.1002/adma.201704501 ↗
19. 10.1021/jacs.8b0361310.1021/jacs.8b03613 ↗
20. 10.1002/ejic.20100054110.1002/ejic.201000541 ↗
21. 10.1103/PhysRevB.50.1795310.1103/PhysRevB.50.17953 ↗
22. 10.1103/PhysRevB.48.1311510.1103/PhysRevB.48.13115 ↗
23. 10.1103/PhysRevB.71.04110210.1103/PhysRevB.71.041102 ↗
24. 10.1002/cssc.20150157410.1002/cssc.201501574 ↗
25. 10.1021/acsami.7b0355510.1021/acsami.7b03555 ↗
26. 10.1016/j.cattod.2014.07.02810.1016/j.cattod.2014.07.028 ↗
27. 10.1021/acs.jpcc.6b0249010.1021/acs.jpcc.6b02490 ↗
28. 10.1039/C5TA01738F10.1039/C5TA01738F ↗
29. 10.1021/jacs.5b0310510.1021/jacs.5b03105 ↗
30. 10.1002/anie.20180153810.1002/anie.201801538 ↗
31. 10.1002/adma.20170177410.1002/adma.201701774 ↗