journal article·2019-10-03Open access

Passivating Grain Boundaries in Polycrystalline CdTe

Chuan-Jia Tong, Keith P. McKenna

The Journal of Physical Chemistry C· Volume 123· Issue 39

Abstract

Using first-principles density functional calculations, we investigate the structure and properties of three different grain boundaries (GBs) in the solar absorber material CdTe. Among the low ∑ value symmetric tilt GBs ∑3 (111), ∑3 (112), and ∑5 (310), we confirm that the ∑3 (111) is the most stable one but is relatively benign for carrier transport as it does not introduce any new states into the gap. The ∑3 (112) and ∑5 (310) GBs, however, are detrimental due to gap states induced by Te-Te and Cd-Cd dangling bonds. We systematically investigate the segregation of O, Se, Cl, Na, and Cu to the GBs and associated electronic properties. Our results show that co-doping with Cl and Na is predicted to be a viable approach passivating all gap states induced by dangling bonds in CdTe.
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Research context

OpenAlex topics: Chalcogenide Semiconductor Thin Films · Quantum Dots Synthesis And Properties · Advanced Semiconductor Detectors and Materials

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Affiliations

Department of Physics, University of York, Heslington, York YO10 5DD, United Kingdom

Funding

Engineering and Physical Sciences Research Council

References (41)

Show source-provided references
1. 10.1016/j.cossms.2010.08.00210.1016/j.cossms.2010.08.002 ↗
2. 10.1039/C3EE41981A10.1039/C3EE41981A ↗
3. 10.1021/jz101423s10.1021/jz101423s ↗
4. 10.1021/acs.jpclett.7b0252610.1021/acs.jpclett.7b02526 ↗
5. 10.1016/S0040-6090(00)01725-910.1016/S0040-6090(00)01725-9 ↗
6. 10.1063/1.204253010.1063/1.2042530 ↗
7. 10.1021/acsenergylett.8b0170010.1021/acsenergylett.8b01700 ↗
8. 10.1021/acs.jpclett.9b0076310.1021/acs.jpclett.9b00763 ↗
9. 10.1021/jacs.6b0064510.1021/jacs.6b00645 ↗
10. 10.1038/nenergy.2016.1510.1038/nenergy.2016.15 ↗
11. 10.1063/1.159864110.1063/1.1598641 ↗
12. 10.1063/1.484485510.1063/1.4844855 ↗
13. 10.1103/PhysRevLett.112.15610310.1103/PhysRevLett.112.156103 ↗
14. 10.1021/jp409538p10.1021/jp409538p ↗
15. 10.1088/1361-651X/aaba8710.1088/1361-651X/aaba87 ↗
16. 10.1088/1367-2630/17/1/01302710.1088/1367-2630/17/1/013027 ↗
17. 10.1103/PhysRevB.93.20542610.1103/PhysRevB.93.205426 ↗
18. 10.1103/PhysRevLett.101.15550110.1103/PhysRevLett.101.155501 ↗
19. 10.1016/j.ssc.2012.05.00610.1016/j.ssc.2012.05.006 ↗
20. 10.1088/0268-1242/31/9/09300110.1088/0268-1242/31/9/093001 ↗
21. 10.1016/j.tsf.2016.10.00810.1016/j.tsf.2016.10.008 ↗
22. 10.1021/acs.jpclett.6b0239910.1021/acs.jpclett.6b02399 ↗
23. 10.1063/1.482848410.1063/1.4828484 ↗
24. 10.1002/(sici)1099-159x(199909/10)7:53.3.co;2-g10.1002/(sici)1099-159x(199909/10)7:53.3.co;2-g ↗
25. 10.1016/j.tsf.2006.12.14710.1016/j.tsf.2006.12.147 ↗
26. 10.1016/j.solmat.2012.06.01910.1016/j.solmat.2012.06.019 ↗
27. 10.1016/0040-6090(88)90299-410.1016/0040-6090(88)90299-4 ↗
28. 10.1038/ncomms1253710.1038/ncomms12537 ↗
29. 10.1103/PhysRevB.50.1795310.1103/PhysRevB.50.17953 ↗
30. 10.1103/PhysRevB.59.175810.1103/PhysRevB.59.1758 ↗
31. 10.1103/PhysRevB.13.518810.1103/PhysRevB.13.5188 ↗
32. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
33. 10.1063/1.220459710.1063/1.2204597 ↗
34. 10.1103/PhysRevB.79.22411610.1103/PhysRevB.79.224116 ↗
35. 10.1063/1.494072210.1063/1.4940722 ↗
36. 10.1007/s10853-005-2665-510.1007/s10853-005-2665-5 ↗
37. 10.1103/PhysRevB.78.24532010.1103/PhysRevB.78.245320 ↗
38. 10.1038/nature1059310.1038/nature10593 ↗
39. 10.1088/0965-0393/10/3/20210.1088/0965-0393/10/3/202 ↗
40. 10.1103/PhysRevB.89.03531010.1103/PhysRevB.89.035310 ↗
41. 10.1016/j.commatsci.2016.08.04410.1016/j.commatsci.2016.08.044 ↗