Cation Vacancies Mediate Thermochemical Water Splitting with Iron Aluminates
Source abstract
Abstract
Solar thermochemical water splitting enables hydrogen production by cycling metal oxides between reduced and oxidized states, typically through an oxygen vacancy mechanism. However, recent experimental work suggests that cation vacancies have a greater influence on the redox behavior of iron aluminate spinels used in water splitting. This remains debated, as calculations predict that such cation vacancies are thermodynamically unfavorable. In the current work, we show that Fe vacancies in (Fe ζ Al 1−ζ ) 3 O 4 become accessible only when facilitated by inversion between Fe and Al. This antisite disorder lowers the formation energy of octahedral Fe vacancies in Al-rich spinels (ζ = 1/3) from over 3 eV to just 0.62 eV when one-third of the cation sites are inverted, allowing high Fe vacancy concentrations under oxidizing conditions. This mechanism supports high H 2 yields up to 361 μmol/g, consistent with experimental observations. Our findings support the notion that solar thermochemical water splitting can occur through a cation vacancy mechanism. They also clarify how site inversion, vacancy energetics, and defect interactions each contribute to redox performance, offering general design principles for identifying and optimizing materials that operate through cation vacancy cycling.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Chemical Looping and Thermochemical Processes · Iron oxide chemistry and applications · High-Temperature Coating Behaviors
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
University of Minnesota
Department of Chemical Engineering and Materials Science
Solar Energy Engineering Laboratory, Department of Mechanical and Process Engineering
ETH Zürich
Department of Chemical and Biological Engineering
University of Colorado
Funding
University of Minnesota
References (56)
Show source-provided references
1. 10.1016/j.rser.2013.08.05010.1016/j.rser.2013.08.050 ↗
2. 10.1002/wene.17410.1002/wene.174 ↗
3. 10.1021/acsenergylett.1c0075810.1021/acsenergylett.1c00758 ↗
4. 10.1002/wene.52810.1002/wene.528 ↗
5. 10.1002/ente.20210022210.1002/ente.202100222 ↗
6. 10.1016/j.mattod.2014.04.02510.1016/j.mattod.2014.04.025 ↗
7. 10.1016/S0360-3199(01)00177-X10.1016/S0360-3199(01)00177-X ↗
8. 10.1016/j.apenergy.2015.12.10610.1016/j.apenergy.2015.12.106 ↗
9. 10.1016/0038-092X(77)90102-510.1016/0038-092X(77)90102-5 ↗
10. 10.1016/S0038-092X(98)00092-910.1016/S0038-092X(98)00092-9 ↗
11. 10.1002/9781119752097.ch110.1002/9781119752097.ch1 ↗
12. 10.1016/j.solener.2005.12.00510.1016/j.solener.2005.12.005 ↗
13. 10.1039/C1EE02620H10.1039/C1EE02620H ↗
14. 10.1021/cm503131p10.1021/cm503131p ↗
15. 10.1016/j.ijhydene.2017.06.09810.1016/j.ijhydene.2017.06.098 ↗
16. 10.1002/adts.20200011210.1002/adts.202000112 ↗
17. 10.1126/science.119783410.1126/science.1197834 ↗
18. 10.1021/acs.energyfuels.9b0271410.1021/acs.energyfuels.9b02714 ↗
19. 10.1021/acs.chemmater.6b0118210.1021/acs.chemmater.6b01182 ↗
20. 10.1021/acs.chemmater.0c0291210.1021/acs.chemmater.0c02912 ↗
21. 10.1021/jacs.1c0557010.1021/jacs.1c05570 ↗
22. 10.1039/D3EE00234A10.1039/D3EE00234A ↗
23. 10.1021/acs.chemmater.2c0305410.1021/acs.chemmater.2c03054 ↗
24. 10.1021/acscatal.4c0335710.1021/acscatal.4c03357 ↗
25. 10.1016/j.ijhydene.2010.01.14010.1016/j.ijhydene.2010.01.140 ↗
26. 10.1021/acs.chemmater.5b0391110.1021/acs.chemmater.5b03911 ↗
27. 10.1126/science.123945410.1126/science.1239454 ↗
28. 10.1039/C5EE01979F10.1039/C5EE01979F ↗
29. 10.1016/j.cej.2020.12601510.1016/j.cej.2020.126015 ↗
30. 10.1016/j.cej.2020.12442910.1016/j.cej.2020.124429 ↗
31. 10.1016/j.joule.2023.07.01610.1016/j.joule.2023.07.016 ↗
32. 10.1039/D1EE02679H10.1039/D1EE02679H ↗
33. 10.1002/bbpc.1982086020510.1002/bbpc.19820860205 ↗
34. 10.1021/acs.chemmater.1c0104910.1021/acs.chemmater.1c01049 ↗
35. 10.1038/144327b010.1038/144327b0 ↗
36. 10.1103/RevModPhys.86.25310.1103/RevModPhys.86.253 ↗
37. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
38. 10.1103/PhysRevB.57.150510.1103/PhysRevB.57.1505 ↗
39. 10.1103/PhysRevB.87.24120110.1103/PhysRevB.87.241201 ↗
40. 10.1103/PRXEnergy.3.01300810.1103/PRXEnergy.3.013008 ↗
41. 10.1038/s41467-018-06682-410.1038/s41467-018-06682-4 ↗
42. 10.1021/je000236i10.1021/je000236i ↗
43. 10.1111/j.1151-2916.1980.tb09856.x10.1111/j.1151-2916.1980.tb09856.x ↗
44. 10.2138/am-1998-9-101810.2138/am-1998-9-1018 ↗
45. 10.1021/acsami.0c0281910.1021/acsami.0c02819 ↗
46. 10.1103/PhysRevLett.65.35310.1103/PhysRevLett.65.353 ↗
47. 10.1016/j.cpc.2023.10866410.1016/j.cpc.2023.108664 ↗
48. 10.1039/c2ee22090c10.1039/c2ee22090c ↗
49. 10.1016/0927-0256(96)00008-010.1016/0927-0256(96)00008-0 ↗
50. 10.1063/1.481232310.1063/1.4812323 ↗
51. 10.1016/j.commatsci.2012.10.02810.1016/j.commatsci.2012.10.028 ↗
52. 10.1088/1361-648X/ac944010.1088/1361-648X/ac9440 ↗
53. 10.1007/BF0264570910.1007/BF02645709 ↗
54. 10.1039/B009288F10.1039/B009288F ↗
55. 10.1007/s11663-015-0493-910.1007/s11663-015-0493-9 ↗
56. 10.1016/S0167-2738(02)00873-110.1016/S0167-2738(02)00873-1 ↗