First-principles analysis of the intermediate band inCuGa1−xFexS2
Source abstract
Abstract
We present a comprehensive study of the electronic, magnetic, and optical properties of ${\mathrm{CuGa}}_{1\ensuremath{-}x}{\mathrm{Fe}}x{\mathrm{S}}2$, as a promising candidate for intermediate-band (IB) solar cells. We use hybrid exchange-correlation functional within the density functional theory framework, and show that Fe doping induces unoccupied states 1.6--1.9 eV above the valence band. The IBs significantly enhance the optical absorption in lower energy part of the spectrum. We find that at moderate $n$-type co-doping concentration, the added charge occupies part of the IB in the gap, but large concentrations lower the energy of the occupied IB toward the valence band. Moreover, we show that Fe impurities tend to cluster within the compound and they choose antiferromagnetic ordering. The findings can have a significant effect in understanding this material and help to synthesize more efficient IB solar cells.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Chalcogenide Semiconductor Thin Films · Quantum Dots Synthesis And Properties · Copper-based nanomaterials and applications
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (35)
Show source-provided references
1. 10.1103/PhysRevLett.78.501410.1103/PhysRevLett.78.5014 ↗
2. 10.1038/nphoton.2012.110.1038/nphoton.2012.1 ↗
3. 10.1063/1.290121310.1063/1.2901213 ↗
4. 10.1063/1.173603410.1063/1.1736034 ↗
5. 10.1103/PhysRevB.90.07515410.1103/PhysRevB.90.075154 ↗
6. 10.1039/C4RA10007G10.1039/C4RA10007G ↗
7. 10.1002/pssa.20122872110.1002/pssa.201228721 ↗
8. 10.1038/srep0128610.1038/srep01286 ↗
9. 10.1016/j.tsf.2010.12.13610.1016/j.tsf.2010.12.136 ↗
10. 10.1021/jp909895q10.1021/jp909895q ↗
11. 10.1016/j.tsf.2010.09.03910.1016/j.tsf.2010.09.039 ↗
12. 10.1016/j.solmat.2010.06.01910.1016/j.solmat.2010.06.019 ↗
13. 10.1016/j.tsf.2007.12.08510.1016/j.tsf.2007.12.085 ↗
14. 10.1021/jp077418510.1021/jp0774185 ↗
15. 10.1016/j.tsf.2006.12.17010.1016/j.tsf.2006.12.170 ↗
16. 10.1002/pssa.20056617910.1002/pssa.200566179 ↗
17. 10.1088/1674-4926/35/1/01300210.1088/1674-4926/35/1/013002 ↗
18. 10.1016/j.solener.2014.02.04610.1016/j.solener.2014.02.046 ↗
19. 10.1002/pip.119710.1002/pip.1197 ↗
20. 10.1143/JPSJ.36.161810.1143/JPSJ.36.1618 ↗
21. 10.1002/pssa.221048025510.1002/pssa.2210480255 ↗
22. 10.7567/JJAPS.19S3.10110.7567/JJAPS.19S3.101 ↗
23. 10.1143/JJAP.28.1210.1143/JJAP.28.12 ↗
24. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
25. 10.1063/1.156406010.1063/1.1564060 ↗
26. 10.1063/1.220459710.1063/1.2204597 ↗
27. 10.1103/PhysRevB.5.500310.1103/PhysRevB.5.5003 ↗
28. 10.1103/PhysRevB.4.246310.1103/PhysRevB.4.2463 ↗
29. 10.1103/PhysRevB.53.779210.1103/PhysRevB.53.7792 ↗
30. 10.1016/j.jpcs.2005.09.02910.1016/j.jpcs.2005.09.029 ↗
31. 10.1016/j.tsf.2006.12.08310.1016/j.tsf.2006.12.083 ↗
32. 10.1103/PhysRevB.50.1795310.1103/PhysRevB.50.17953 ↗
33. 10.1103/PhysRevB.54.1116910.1103/PhysRevB.54.11169 ↗
34. 10.1103/PhysRevB.84.08514510.1103/PhysRevB.84.085145 ↗
35. 10.7567/JJAPS.39S1.20810.7567/JJAPS.39S1.208 ↗