Deep-UV Transparent Conducting Oxide La-Doped SrSnO3 with a High Figure of Merit
Source abstract
Abstract
Perovskite stannate SrSnO3 (SSO) is attracting attention as ultraviolet transparent conducting oxides (UV TCOs) due to its ultrawide band gap and high conductivity. Here, we investigate in detail the thickness-dependent electrical, structural, and optical properties of sequentially strain-relaxed La-doped SrSnO3 (SLSO) epitaxial thin films. We find that the SLSO films grow as an orthorhombic Pnma phase with a - a - c + in the c + direction under the tensile strain. With the strain relaxation, as the films become thicker, vertical grain boundaries are created and the orthorhombic phase becomes reoriented to all three possible orientations. Simultaneously, the conductance starts to deviate from the linear behavior with increasing film thickness. Through the analysis of thickness fringes in optical transmittance, we found that a 120 nm thick nominally 4% La-doped SrSnO3 film has a figure of merit (φTC = 2.65 × 10-3 Ω-1) at λ = 300 nm in the deep-UV region, which is the highest value among the well-known candidates for UV TCOs reported to date.
Source: europepmc · Quality: candidate unverified · Source record ↗
Research context
OpenAlex topics: Electronic and Structural Properties of Oxides · ZnO doping and properties · Magnetic and transport properties of perovskites and related materials
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Institute of Applied Physics, Department of Physics and Astronomy, Seoul National University, Seoul 08826, Republic of Korea
Department of Chemical Engineering and Material Science, University of Minnesota, Minneapolis, Minnesota 55455, United States
Department of Physics, Yonsei University, Seoul 03722, Republic of Korea
Funding
National Research Foundation of Korea · Division of Materials Research
References (63)
Show source-provided references
1. 10.1088/0268-1242/29/8/08400410.1088/0268-1242/29/8/084004 ↗
2. Bettles T. · Int. Ultraviolet Assoc. News · 2007 · 9 · 11
3. 10.1111/1541-4337.1264510.1111/1541-4337.12645 ↗
4. 10.1016/j.watres.2016.03.00310.1016/j.watres.2016.03.003 ↗
5. 10.1016/j.watres.2010.11.01510.1016/j.watres.2010.11.015 ↗
6. 10.1002/adom.20180109910.1002/adom.201801099 ↗
7. 10.1002/mame.20130034910.1002/mame.201300349 ↗
8. 10.1111/phpp.1274010.1111/phpp.12740 ↗
9. 10.1016/j.nima.2006.05.15910.1016/j.nima.2006.05.159 ↗
10. 10.1063/1.36267710.1063/1.362677 ↗
11. Neele, F. P.; Schleijpen, J. In Electro-Optical Missile Plume Detection, SPIE Proceedings, 2003; pp 270–280.10.1117/12.487510 ↗
12. 10.1143/APEX.5.08210110.1143/APEX.5.082101 ↗
13. 10.7567/APEX.10.03100210.7567/APEX.10.031002 ↗
14. 10.1016/S0040-6090(03)01158-110.1016/S0040-6090(03)01158-1 ↗
15. 10.1016/S0040-6090(02)00163-310.1016/S0040-6090(02)00163-3 ↗
16. 10.1063/1.346698710.1063/1.3466987 ↗
17. 10.1016/j.jascer.2016.01.00110.1016/j.jascer.2016.01.001 ↗
18. 10.1021/acsami.0c0485410.1021/acsami.0c04854 ↗
19. 10.1038/s42005-020-0372-910.1038/s42005-020-0372-9 ↗
20. 10.1038/nmat449310.1038/nmat4493 ↗
21. 10.1186/s40580-020-00242-710.1186/s40580-020-00242-7 ↗
22. 10.1063/1.133055910.1063/1.1330559 ↗
23. 10.1143/JJAP.47.731110.1143/JJAP.47.7311 ↗
24. 10.1063/1.512841010.1063/1.5128410 ↗
25. 10.1021/acsaelm.0c0080610.1021/acsaelm.0c00806 ↗
26. 10.1116/1.505466610.1116/1.5054666 ↗
27. 10.1039/C4RA02479F10.1039/C4RA02479F ↗
28. 10.1063/1.495886010.1063/1.4958860 ↗
29. 10.1021/ic034551c10.1021/ic034551c ↗
30. 10.1143/APEX.5.06110210.1143/APEX.5.061102 ↗
31. 10.1063/1.493965710.1063/1.4939657 ↗
32. 10.1103/PhysRevMaterials.2.02160110.1103/PhysRevMaterials.2.021601 ↗
33. 10.1063/1.487489510.1063/1.4874895 ↗
34. 10.1016/j.materresbull.2004.11.00410.1016/j.materresbull.2004.11.004 ↗
35. 10.1016/S1466-6049(00)00013-110.1016/S1466-6049(00)00013-1 ↗
36. 10.1088/0022-3727/43/3/03540310.1088/0022-3727/43/3/035403 ↗
37. 10.1016/j.tsf.2011.03.03810.1016/j.tsf.2011.03.038 ↗
38. 10.1088/0022-3727/48/45/45510610.1088/0022-3727/48/45/455106 ↗
39. 10.1016/j.jallcom.2017.05.08010.1016/j.jallcom.2017.05.080 ↗
40. 10.1021/acsami.8b1659210.1021/acsami.8b16592 ↗
41. 10.1063/1.511927210.1063/1.5119272 ↗
42. 10.1016/j.spmi.2021.10702810.1016/j.spmi.2021.107028 ↗
43. 10.1016/j.ceramint.2020.04.05610.1016/j.ceramint.2020.04.056 ↗
44. 10.1021/acs.nanolett.0c0370810.1021/acs.nanolett.0c03708 ↗
45. 10.1021/acsaelm.0c0099710.1021/acsaelm.0c00997 ↗
46. 10.1016/j.optmat.2020.11013910.1016/j.optmat.2020.110139 ↗
47. 10.1063/1.479832510.1063/1.4798325 ↗
48. 10.1186/s11671-020-03390-110.1186/s11671-020-03390-1 ↗
49. 10.1063/1.291741310.1063/1.2917413 ↗
50. 10.1021/acsami.9b0781910.1021/acsami.9b07819 ↗
51. 10.1063/1.497486410.1063/1.4974864 ↗
52. 10.1016/j.jallcom.2005.06.03010.1016/j.jallcom.2005.06.030 ↗
53. 10.1116/1.236275910.1116/1.2362759 ↗
54. 10.1016/j.mee.2007.04.02910.1016/j.mee.2007.04.029 ↗
55. 10.1002/adma.20210596710.1002/adma.202105967 ↗
56. 10.1107/S056774087200797610.1107/S0567740872007976 ↗
57. 10.1063/1.275211810.1063/1.2752118 ↗
58. 10.1016/j.physleta.2008.04.01510.1016/j.physleta.2008.04.015 ↗
59. 10.1016/j.commatsci.2010.09.00310.1016/j.commatsci.2010.09.003 ↗
60. 10.1116/1.495900410.1116/1.4959004 ↗
61. 10.1016/j.cplett.2005.10.12210.1016/j.cplett.2005.10.122 ↗
62. 10.1016/j.jssc.2011.02.00910.1016/j.jssc.2011.02.009 ↗
63. 10.1063/1.32324010.1063/1.323240 ↗