Tailored Electronic Band Gap and Valance Band Edge of Nickel Oxide via p-Type Incorporation
Source abstract
Abstract
A p-type semiconductor candidate of nickel oxide (NiO) desires longer carrier lifetimes with suitable conduction band edge, which holds a unique advantage to drive the hydrogen evolution toward efficient water splitting. However, a relatively large band gap (∼4 eV) greatly hinders its practical applications. We thus theoretically explore the band edge tailoring of NiO by doping electron-poor S on the sites of O. With the increase of incorporated S density, the electronic band gap ( E g ) of p-type-doped NiO is reduced with the improved valance band maximum (VBM), which is dominated by the emerged S 3p orbital hybridized with Ni t 2g states. Accordingly, the hole transportation might be enhanced due to the enlarged VBM offset between the active layer and NiO 1– x S x . Furthermore, the magnetic momentum per Ni atom increases with the increase of S densities, owing to the p-type-doping-induced majority and minority spin mismatch. It is confirmed that the VBM of NiO with S density lower than 2.08% consists of S 3p and Ni t 2g states with majority spin. Moreover, as a turning point, the special quasirandom structure (SQS) with S density as high as 2.78% shows a balanced spin feature, while the states with minority spin play a predominant role in the VBM with S density higher than 8.33%.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: ZnO doping and properties · Copper-based nanomaterials and applications · Transition Metal Oxide Nanomaterials
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Institute of Materials, Ningbo University of Technology, Ningbo 315211, P. R. China
State Key Laboratory of Advanced Metallurgy, University of Science and Technology Beijing, Beijing 100083, P. R. China
Funding
Natural Science Foundation of Ningbo · Natural Science Foundation of Zhejiang Province · Zhejiang Province
References (50)
Show source-provided references
1. 10.1016/0040-6090(93)90636-410.1016/0040-6090(93)90636-4 ↗
2. 10.1021/acs.jpclett.0c0230410.1021/acs.jpclett.0c02304 ↗
3. 10.1021/acs.jpclett.0c0146710.1021/acs.jpclett.0c01467 ↗
4. 10.1021/acs.jpclett.0c0086510.1021/acs.jpclett.0c00865 ↗
5. 10.1021/acs.jpclett.0c0182210.1021/acs.jpclett.0c01822 ↗
6. 10.1063/1.36494810.1063/1.364948 ↗
7. 10.1016/S0304-8853(98)00089-410.1016/S0304-8853(98)00089-4 ↗
8. 10.1063/1.12130810.1063/1.121308 ↗
9. 10.1109/JSEN.2016.251708510.1109/JSEN.2016.2517085 ↗
10. 10.1166/sl.2017.386410.1166/sl.2017.3864 ↗
11. 10.1039/c1jm13278d10.1039/c1jm13278d ↗
12. 10.1039/C6NR04643F10.1039/C6NR04643F ↗
13. 10.1002/aenm.20170198110.1002/aenm.201701981 ↗
14. 10.1021/acsnano.7b0785610.1021/acsnano.7b07856 ↗
15. 10.1021/acsami.0c1173110.1021/acsami.0c11731 ↗
16. 10.1021/acs.jpclett.0c0042510.1021/acs.jpclett.0c00425 ↗
17. 10.1021/ja711023z10.1021/ja711023z ↗
18. 10.1021/acsami.5b0929110.1021/acsami.5b09291 ↗
19. 10.1007/s10853-006-1153-x10.1007/s10853-006-1153-x ↗
20. 10.1021/acs.jpclett.8b0259110.1021/acs.jpclett.8b02591 ↗
21. 10.1016/j.electacta.2017.09.09110.1016/j.electacta.2017.09.091 ↗
22. 10.1039/C6TC00513F10.1039/C6TC00513F ↗
23. 10.1021/acsenergylett.6b0024110.1021/acsenergylett.6b00241 ↗
24. 10.1103/PhysRevB.69.07541310.1103/PhysRevB.69.075413 ↗
25. 10.1103/PhysRevB.85.11512710.1103/PhysRevB.85.115127 ↗
26. 10.1021/jp502484510.1021/jp5024845 ↗
27. 10.1126/science.aad101510.1126/science.aad1015 ↗
28. 10.1021/am302189410.1021/am3021894 ↗
29. 10.1021/acsami.0c1613910.1021/acsami.0c16139 ↗
30. 10.1021/jp803919b10.1021/jp803919b ↗
31. 10.1021/acs.jpcc.5b1248910.1021/acs.jpcc.5b12489 ↗
32. 10.1021/acsami.7b0602510.1021/acsami.7b06025 ↗
33. 10.1103/PhysRevLett.111.08660210.1103/PhysRevLett.111.086602 ↗
34. 10.1103/PhysRevB.54.1116910.1103/PhysRevB.54.11169 ↗
35. 10.1016/0927-0256(96)00008-010.1016/0927-0256(96)00008-0 ↗
36. 10.1103/PhysRevB.59.175810.1103/PhysRevB.59.1758 ↗
37. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
38. 10.1103/PhysRevLett.65.35310.1103/PhysRevLett.65.353 ↗
39. 10.1103/PhysRevB.42.962210.1103/PhysRevB.42.9622 ↗
40. 10.1103/PhysRevB.69.21420210.1103/PhysRevB.69.214202 ↗
41. 10.1016/j.calphad.2017.05.00510.1016/j.calphad.2017.05.005 ↗
42. Cox P. A. · 2010
43. 10.1103/PhysRevLett.53.233910.1103/PhysRevLett.53.2339 ↗
44. 10.1103/PhysRevB.27.696410.1103/PhysRevB.27.6964 ↗
45. 10.1063/1.166885510.1063/1.1668855 ↗
46. 10.1016/S0039-6028(01)01957-410.1016/S0039-6028(01)01957-4 ↗
47. 10.1103/PhysRevLett.87.08610110.1103/PhysRevLett.87.086101 ↗
48. 10.1103/PhysRevB.62.1639210.1103/PhysRevB.62.16392 ↗
49. 10.1103/PhysRevB.45.161210.1103/PhysRevB.45.1612 ↗
50. 10.1103/PhysRevB.50.825710.1103/PhysRevB.50.8257 ↗