Energetics and optical properties of nitrogen impurities in SrTiO3 from hybrid density-functional calculations
Source abstract
Abstract
Semiconductor photocatalysts that can produce hydrogen from water splitting are of great interest. Among the various possibilities, nitrogen (N)-doped $\mathrm{SrTi}{\mathrm{O}}3$ is a promising candidate for hydrogen evolution under visible-light irradiation. In this study, hybrid density-functional calculations are employed to investigate the stability and impact of nitrogen impurities on the electronic and optical properties in $\mathrm{SrTi}{\mathrm{O}}3$. We find that the substitutional N on O site (${\mathrm{N}}_{\mathrm{O}}$) is a deep acceptor in $\mathrm{SrTi}{\mathrm{O}}3$. Moreover, ${\mathrm{N}}_{\mathrm{O}}$ predominates over other N-related defects under equilibrium growth conditions in $n$-type $\mathrm{SrTi}{\mathrm{O}}3$. Our results reveal that ${\mathrm{N}}_{\mathrm{O}}$ gives rise to visible-light absorption in agreement with experimental observations. In addition, we find that hydrogen can bind to ${\mathrm{N}}_{\mathrm{O}}$, forming ${\mathrm{N}}_{\mathrm{O}}\ensuremath{-}{\mathrm{H}}i$ complex which leads to a blueshift in the optical absorption. Other N configurations can also contribute to optical absorption in the visible range. The vibration frequencies of different N configurations are provided to support identification using vibrational spectroscopy techniques.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Electronic and Structural Properties of Oxides · Advanced Photocatalysis Techniques · Semiconductor materials and devices
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (44)
Show source-provided references
1. 10.1038/238037a010.1038/238037a0 ↗
2. 10.1002/adma.20110275210.1002/adma.201102752 ↗
3. 10.2138/am-2000-041610.2138/am-2000-0416 ↗
4. 10.1021/jp049556p10.1021/jp049556p ↗
5. 10.1021/jp025548210.1021/jp0255482 ↗
6. 10.1016/S1010-6030(03)00442-810.1016/S1010-6030(03)00442-8 ↗
7. 10.1021/jp062487p10.1021/jp062487p ↗
8. 10.1039/c2ta00450j10.1039/c2ta00450j ↗
9. 10.1063/1.240318110.1063/1.2403181 ↗
10. 10.1016/j.jssc.2013.08.00110.1016/j.jssc.2013.08.001 ↗
11. 10.1016/j.jeurceramsoc.2004.07.02710.1016/j.jeurceramsoc.2004.07.027 ↗
12. 10.1016/j.apcatb.2004.03.00810.1016/j.apcatb.2004.03.008 ↗
13. 10.1016/j.jallcom.2008.04.07810.1016/j.jallcom.2008.04.078 ↗
14. 10.1016/j.solidstatesciences.2008.04.01010.1016/j.solidstatesciences.2008.04.010 ↗
15. 10.1021/la035312510.1021/la0353125 ↗
16. 10.1016/j.jphotochem.2004.02.02210.1016/j.jphotochem.2004.02.022 ↗
17. 10.1016/j.apsusc.2013.03.00710.1016/j.apsusc.2013.03.007 ↗
18. 10.1126/science.106105110.1126/science.1061051 ↗
19. 10.1016/j.commatsci.2013.06.00910.1016/j.commatsci.2013.06.009 ↗
20. 10.1021/jp902567j10.1021/jp902567j ↗
21. 10.1039/C4CP02856B10.1039/C4CP02856B ↗
22. 10.1039/C4RA07289H10.1039/C4RA07289H ↗
23. 10.1021/acs.jpcc.5b0666710.1021/acs.jpcc.5b06667 ↗
24. 10.1039/b922399a10.1039/b922399a ↗
25. 10.1016/j.cplett.2012.11.00510.1016/j.cplett.2012.11.005 ↗
26. 10.1016/j.ijhydene.2012.05.03810.1016/j.ijhydene.2012.05.038 ↗
27. 10.1088/0022-3727/40/23/01110.1088/0022-3727/40/23/011 ↗
28. 10.1002/adma.20100360310.1002/adma.201003603 ↗
29. 10.1039/c2cp23348g10.1039/c2cp23348g ↗
30. 10.1063/1.156406010.1063/1.1564060 ↗
31. 10.1016/0927-0256(96)00008-010.1016/0927-0256(96)00008-0 ↗
32. 10.1103/PhysRevB.50.1795310.1103/PhysRevB.50.17953 ↗
33. 10.1063/1.141576610.1063/1.1415766 ↗
34. 10.1016/0025-5408(73)90130-X10.1016/0025-5408(73)90130-X ↗
35. 10.1103/PhysRevB.90.08520210.1103/PhysRevB.90.085202 ↗
36. 10.1103/RevModPhys.86.25310.1103/RevModPhys.86.253 ↗
37. 10.1002/pssb.20104628910.1002/pssb.201046289 ↗
38. 10.1063/1.327404310.1063/1.3274043 ↗
39. 10.1103/PhysRevLett.106.06680110.1103/PhysRevLett.106.066801 ↗
40. 10.1103/PhysRevB.89.07520210.1103/PhysRevB.89.075202 ↗
41. 10.1103/PhysRevB.85.12520510.1103/PhysRevB.85.125205 ↗
42. 10.1016/j.apsusc.2008.07.15910.1016/j.apsusc.2008.07.159 ↗
43. 10.1103/PhysRevB.68.07520610.1103/PhysRevB.68.075206 ↗
44. 10.1016/j.commatsci.2010.01.02410.1016/j.commatsci.2010.01.024 ↗