Reducing CO2 to CO and H2O on Ni(110): The Influence of Subsurface Hydrogen
Source abstract
Abstract
Subsurface hydrogen atoms are relatively high-energy species located below metal surfaces that are readily produced when H, H +, or high-pressure H 2 interacts with the surface under the right conditions. These species can get involved in catalytic processes associated with hydrogenation reactions, either as spectator species, in which they modify the energetics of reactions occurring on the surface, or directly as a reactant for hydrogenation reactions. In this study, we investigate two mechanisms, associative or redox, in CO 2 conversion to CO through the reverse water–gas shift (RWGS) reaction on Ni(110) in the presence of a high density of subsurface hydrogen using spin-polarized periodic density functional theory. The results indicate that subsurface H atoms play an important role for this reaction, both as spectators which lower the energies of barriers and intermediates and as reactants for hydrogenation reactions. The most favorable RWGS pathway involves CO 2 dissociation to CO + O followed by hydrogenation to give CO + H 2 O. Direct associative hydrogenation of CO 2 to give COOH and then CO + H 2 O can also occur, and this is found to be a more important reaction than hydrogenation of CO 2 to give HCOO, and then formic acid as the latter product has a high desorption energy that can result in decomposition.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Catalytic Processes in Materials Science · Advanced Chemical Physics Studies · Catalysis and Oxidation Reactions
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Department of Chemistry, Northwestern University, Evanston, Illinois 60208-3113, United States
Funding
Air Force Office of Scientific Research
References (42)
Show source-provided references
1. 10.1016/S0167-5729(96)00007-610.1016/S0167-5729(96)00007-6 ↗
2. 10.1016/S0360-0564(02)47006-X10.1016/S0360-0564(02)47006-X ↗
3. 10.1021/acs.iecr.5b0056310.1021/acs.iecr.5b00563 ↗
4. 10.1016/0304-5102(91)85070-I10.1016/0304-5102(91)85070-I ↗
5. 10.1021/jp052355g10.1021/jp052355g ↗
6. 10.1016/j.molcata.2012.08.01610.1016/j.molcata.2012.08.016 ↗
7. 10.1016/j.susc.2009.01.02110.1016/j.susc.2009.01.021 ↗
8. 10.1016/j.susc.2014.04.00610.1016/j.susc.2014.04.006 ↗
9. 10.1063/1.168093510.1063/1.1680935 ↗
10. 10.1016/0039-6028(89)90039-310.1016/0039-6028(89)90039-3 ↗
11. 10.1016/S0039-6028(00)00457-X10.1016/S0039-6028(00)00457-X ↗
12. 10.1063/1.190294310.1063/1.1902943 ↗
13. 10.1021/ar970030f10.1021/ar970030f ↗
14. 10.1103/PhysRevLett.67.92710.1103/PhysRevLett.67.927 ↗
15. 10.1016/j.susc.2012.02.02710.1016/j.susc.2012.02.027 ↗
16. 10.1103/PhysRevB.76.19542510.1103/PhysRevB.76.195425 ↗
17. 10.1021/ja802554g10.1021/ja802554g ↗
18. 10.1103/PhysRevB.82.16540310.1103/PhysRevB.82.165403 ↗
19. 10.1021/jz900221c10.1021/jz900221c ↗
20. 10.1021/jz500767510.1021/jz5007675 ↗
21. 10.1021/jacs.5b1336610.1021/jacs.5b13366 ↗
22. 10.1103/PhysRevB.54.1116910.1103/PhysRevB.54.11169 ↗
23. 10.1016/0927-0256(96)00008-010.1016/0927-0256(96)00008-0 ↗
24. 10.1103/PhysRevB.50.1795310.1103/PhysRevB.50.17953 ↗
25. 10.1103/PhysRevB.59.175810.1103/PhysRevB.59.1758 ↗
26. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
27. 10.1103/PhysRevB.13.518810.1103/PhysRevB.13.5188 ↗
28. 10.1063/1.132967210.1063/1.1329672 ↗
29. 10.1063/1.132322410.1063/1.1323224 ↗
30. 10.1063/1.45944410.1063/1.459444 ↗
31. 10.1016/j.commatsci.2005.04.01010.1016/j.commatsci.2005.04.010 ↗
32. 10.1002/jcc.2057510.1002/jcc.20575 ↗
33. 10.1088/0953-8984/21/8/08420410.1088/0953-8984/21/8/084204 ↗
34. 10.1063/1.355371610.1063/1.3553716 ↗
35. 1996
36. 10.1016/j.catcom.2015.10.03410.1016/j.catcom.2015.10.034 ↗
37. 10.1063/1.494300210.1063/1.4943002 ↗
38. 10.1039/dc987840035910.1039/dc9878400359 ↗
39. 10.1063/1.368025610.1063/1.3680256 ↗
40. 10.1063/1.481110910.1063/1.4811109 ↗
41. 10.1016/j.jcat.2010.09.00710.1016/j.jcat.2010.09.007 ↗
42. 10.1063/1.187867210.1063/1.1878672 ↗