journal article·2026-03Open access

Defects Dynamic in Photo‐Excited CeO 2 and their Influence on CO 2 Photoreduction

Rambabu Yalavarthi, Shashi B. Mishra, Olivier Henrotte, Emiliano Cortes

Advanced Functional Materials· Volume 36· Issue 21

Abstract

Abstract Defects play a crucial role in shaping the efficiency and performance of semiconductor‐based technologies. Under illumination, the interaction between photo‐excited charge carriers and defect states in the semiconductor can significantly influence the response of devices and catalysts. Here, an X‐ray photoelectron spectroscopy study conducted under light excitation is presented to track exciton generation and its interaction with defects in CeO 2 , a widely used metal‐oxide support in (photo) catalysis. The light intensity‐dependent measurements reveal that photo‐excited electrons in CeO 2 can effectively reduce Ce 4+ to Ce 3+ . Surface‐enhanced Raman spectroscopy further highlights the critical role of Ce 3+ states in governing charge and energy transport across the CeO 2 ‐molecule interface. Finally, how these photo‐induced states (Ce 3+ ) can be leveraged is demonstrated to control the selectivity in the photocatalytic CO 2 reduction reaction, dramatically influencing the yields of CO, CH 4 , and H 2 .
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Research context

OpenAlex topics: Catalytic Processes in Materials Science · Advanced Photocatalysis Techniques · Electronic and Structural Properties of Oxides

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

Affiliations

Nanoinstitute Munich Faculty of Physics Ludwig‐Maximilians‐Universität München 80539 München Germany

Department of Physics and Astronomy Binghamton University‐SUNY New York 13902 USA

Funding

European Commission · Deutsche Forschungsgemeinschaft

References (47)

Show source-provided references
1. 10.1039/C7EE03639F10.1039/C7EE03639F ↗
2. Zaleska‐Medynska A. · 2018
3. 10.1002/anie.20120719910.1002/anie.201207199 ↗
4. 10.1038/nmat381110.1038/nmat3811 ↗
5. 10.1038/ncomms880010.1038/ncomms8800 ↗
6. 10.1021/acsenergylett.1c0177210.1021/acsenergylett.1c01772 ↗
7. 10.1021/jp502067510.1021/jp5020675 ↗
8. 10.1038/ncomms976910.1038/ncomms9769 ↗
9. 10.1038/nnano.2013.1810.1038/nnano.2013.18 ↗
10. 10.1021/acsenergylett.1c0251610.1021/acsenergylett.1c02516 ↗
11. 10.1039/C9CS00588A10.1039/C9CS00588A ↗
12. 10.1002/smll.20231067710.1002/smll.202310677 ↗
13. 10.1002/adma.20170630010.1002/adma.201706300 ↗
14. 10.1016/j.jpowsour.2020.22908010.1016/j.jpowsour.2020.229080 ↗
15. 10.1073/pnas.190163111610.1073/pnas.1901631116 ↗
16. 10.1002/adma.20160479710.1002/adma.201604797 ↗
17. 10.1038/s41467-017-00710-510.1038/s41467-017-00710-5 ↗
18. 10.1126/science.111395510.1126/science.1113955 ↗
19. 10.1021/jacs.4c0436610.1021/jacs.4c04366 ↗
20. 10.1063/1.514330910.1063/1.5143309 ↗
21. 10.1088/0953-8984/22/22/22320110.1088/0953-8984/22/22/223201 ↗
22. 10.1146/annurev-matsci-062910-10044210.1146/annurev-matsci-062910-100442 ↗
23. 10.1002/adfm.20120061510.1002/adfm.201200615 ↗
24. 10.1038/s41929-023-00970-z10.1038/s41929-023-00970-z ↗
25. 10.1016/j.solener.2022.04.05110.1016/j.solener.2022.04.051 ↗
26. 10.1021/acs.jpclett.1c0000310.1021/acs.jpclett.1c00003 ↗
27. 10.1103/PhysRevB.95.24510110.1103/PhysRevB.95.245101 ↗
28. 10.1002/sia.74020060410.1002/sia.740200604 ↗
29. 10.1002/jrs.298710.1002/jrs.2987 ↗
30. 10.1103/PhysRevB.48.17810.1103/PhysRevB.48.178 ↗
31. 10.1111/j.1151-2916.2002.tb00509.x10.1111/j.1151-2916.2002.tb00509.x ↗
32. 10.1021/la101723w10.1021/la101723w ↗
33. 10.1088/1361-6463/ad42a910.1088/1361-6463/ad42a9 ↗
34. 10.1021/acsnano.4c0267010.1021/acsnano.4c02670 ↗
35. 10.1038/s41467-017-02166-z10.1038/s41467-017-02166-z ↗
36. 10.1002/adfm.20240052310.1002/adfm.202400523 ↗
37. 10.1002/anie.20170518710.1002/anie.201705187 ↗
38. 10.1002/anie.20191337510.1002/anie.201913375 ↗
39. 10.1088/0957-4484/16/9/00610.1088/0957-4484/16/9/006 ↗
40. 10.1103/PhysRevB.68.03510410.1103/PhysRevB.68.035104 ↗
41. 10.1016/S0039-6028(02)02657-210.1016/S0039-6028(02)02657-2 ↗
42. 10.1063/1.280001510.1063/1.2800015 ↗
43. 10.1088/0022-3727/46/49/49530610.1088/0022-3727/46/49/495306 ↗
44. 10.1103/PhysRevB.75.04512110.1103/PhysRevB.75.045121 ↗
45. 10.1007/s00214-005-0641-410.1007/s00214-005-0641-4 ↗
46. 10.1002/pssb.20084441910.1002/pssb.200844419 ↗
47. 10.1038/s41467-021-25007-610.1038/s41467-021-25007-6 ↗