Effective scheme to determine accurate defect formation energies and charge transition levels of point defects in semiconductors
Source abstract
Abstract
We propose an effective method to accurately determine the defect formation energy ${E}_{\mathrm{f}}$ and charge transition level $\ensuremath{\varepsilon}$ of the point defects using exclusively cohesive energy ${E}_{\mathrm{coh}}$ and the fundamental band gap ${E}_{\mathrm{g}}$ of pristine host materials. We find that ${E}_{\mathrm{f}}$ of the point defects can be effectively separated into geometric and electronic contributions with a functional form: ${E}_{\mathrm{f}}=\ensuremath{\chi}{E}_{\mathrm{coh}}+\ensuremath{\lambda}{E}_{\mathrm{g}}$, where $\ensuremath{\chi}$ and $\ensuremath{\lambda}$ are dictated by the geometric and electronic factors of the point defects ($\ensuremath{\chi}$ and $\ensuremath{\lambda}$ are defect dependent). Such a linear combination of ${E}_{\mathrm{coh}}$ and ${E}_{\mathrm{g}}$ reproduces ${E}_{\mathrm{f}}$ with an accuracy better than 5% for electronic structure methods ranging from hybrid density-functional theory (DFT) to many-body random-phase approximation (RPA) and experiments. Accordingly, $\ensuremath{\varepsilon}$ is also determined by ${E}_{\mathrm{coh}}/{E}_{\mathrm{g}}$ and the defect geometric/electronic factors. The identified correlation is rather general for monovacancies and interstitials, which holds in a wide variety of semiconductors covering Si, Ge, phosphorenes, ZnO, GaAs, and InP, and enables one to obtain reliable values of ${E}_{\mathrm{f}}$ and $\ensuremath{\varepsilon}$ of the point defects for RPA and experiments based on semilocal DFT calculations.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Machine Learning in Materials Science · Electronic and Structural Properties of Oxides · 2D Materials and Applications
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (43)
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1. 10.1103/RevModPhys.86.25310.1103/RevModPhys.86.253 ↗
2. 10.1103/PhysRevB.78.23510410.1103/PhysRevB.78.235104 ↗
3. 10.1002/pssb.20104621010.1002/pssb.201046210 ↗
4. 10.1103/PhysRevLett.101.04640510.1103/PhysRevLett.101.046405 ↗
5. 10.1103/PhysRevB.81.08521210.1103/PhysRevB.81.085212 ↗
6. 10.1103/PhysRevB.81.20511810.1103/PhysRevB.81.205118 ↗
7. 10.1002/pssb.20104619510.1002/pssb.201046195 ↗
8. 10.1103/PhysRevLett.102.02640210.1103/PhysRevLett.102.026402 ↗
9. 10.1103/PhysRevB.77.15521110.1103/PhysRevB.77.155211 ↗
10. 10.1103/PhysRevLett.83.235110.1103/PhysRevLett.83.2351 ↗
11. 10.1103/PhysRevB.74.12110210.1103/PhysRevB.74.121102 ↗
12. 10.1002/pssb.20104614910.1002/pssb.201046149 ↗
13. 10.1103/PhysRevLett.108.25640310.1103/PhysRevLett.108.256403 ↗
14. 10.1103/PhysRevB.90.05411510.1103/PhysRevB.90.054115 ↗
15. 10.1103/PhysRevLett.108.06640410.1103/PhysRevLett.108.066404 ↗
16. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
17. 10.1063/1.220459710.1063/1.2204597 ↗
18. 10.1016/j.cpc.2009.06.02210.1016/j.cpc.2009.06.022 ↗
19. 10.1063/1.47293310.1063/1.472933 ↗
20. 10.1103/PhysRevLett.107.24550110.1103/PhysRevLett.107.245501 ↗
21. 10.1103/PhysRevLett.108.23640210.1103/PhysRevLett.108.236402 ↗
22. 10.1103/PhysRevLett.111.04550110.1103/PhysRevLett.111.045501 ↗
23. 10.1063/1.240466310.1063/1.2404663 ↗
24. 10.1002/jcc.2474410.1002/jcc.24744 ↗
25. 10.1007/s10853-012-6595-810.1007/s10853-012-6595-8 ↗
26. 10.1103/PhysRevB.46.481610.1103/PhysRevB.46.4816 ↗
27. 10.1016/0022-3697(84)90043-X10.1016/0022-3697(84)90043-X ↗
28. 10.1002/pssb.222179012610.1002/pssb.2221790126 ↗
29. 10.1088/0953-8984/16/4/00110.1088/0953-8984/16/4/001 ↗
30. 10.1016/S0921-4526(01)00908-510.1016/S0921-4526(01)00908-5 ↗
31. 10.1103/PhysRevLett.56.219510.1103/PhysRevLett.56.2195 ↗
32. 10.1103/PhysRevB.52.1654210.1103/PhysRevB.52.16542 ↗
33. 10.1103/PhysRevLett.81.39310.1103/PhysRevLett.81.393 ↗
34. 10.1103/PhysRevLett.83.345410.1103/PhysRevLett.83.3454 ↗
35. 10.1103/PhysRevB.54.1116910.1103/PhysRevB.54.11169 ↗
36. 10.1103/PhysRevLett.113.04680410.1103/PhysRevLett.113.046804 ↗
37. 10.1103/PhysRevB.81.11512610.1103/PhysRevB.81.115126 ↗
38. 10.1063/1.486350210.1063/1.4863502 ↗
39. 10.1021/nn501226z10.1021/nn501226z ↗
40. C. Kittel · 2004
41. 10.1103/PhysRevB.74.24511510.1103/PhysRevB.74.245115 ↗
42. 10.1103/PhysRevLett.68.279810.1103/PhysRevLett.68.2798 ↗
43. G. D. Watkins · 1986