Stabilization of discotic liquid organic thin films by ITO surface treatment
Source abstract
Abstract
Discotic liquid crystals (LCs) are promising materials in the field of electronic components and, in particular, to make efficient photovoltaic cells due to their good charge transport properties. These materials generally exhibit a mesophase in which the disk-shaped molecules can selfassemble into columns, which favorize charge displacement, and may align themselves uniformly on surfaces to form well-oriented thin films. In order to orientate such a columnar thin film on an indium tin oxide (ITO) substrate, the film is heated up to the temperature range of the isotropic liquid phase and subsequently cooled down again. This treatment may lead not only to the desired alignment, but also to dewetting, which leads to an appreciable inhomogeneity in film thickness and to short circuits during the realization of photovoltaic cells. In this article, we describe how this dewetting and the film morphology can be influenced by ITO surface treatments. The chemical modifications of the surface by these treatments were studied by X-ray photoelectron spectroscopy (XPS). Such ITO treatments are shown to be efficient to prevent thin film dewetting when combined with rapid cooling through the isotropic-to-LC phase transition.
Source: openaire · Quality: candidate unverified · Source record ↗
Research context
OpenAlex topics: Fluid Dynamics and Thin Films · Liquid Crystal Research Advancements · Block Copolymer Self-Assembly
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (33)
Show source-provided references
1. Kim · Opt. Mater. · 2002 · 21 · 43910.1016/S0925-3467(02)00179-9 ↗
2. Lee · Curr. Appl. Phys. · 2001 · 1 · 10710.1016/S1567-1739(00)00020-1 ↗
3. Yanagi · Adv. Funct. Mater. · 2003 · 13 · 76710.1002/adfm.200304418 ↗
4. Yang · Nat. Mater. · 2005 · 4 · 3710.1038/nmat1285 ↗
5. van de Craats · Adv. Mater. · 1999 · 11 · 146910.1002/(SICI)1521-4095(199912)11:17<1469::AID-ADMA1469>3.0.CO;2-K ↗
6. Schmidt-Mende · Phys. E · 2002 · 14 · 26310.1016/S1386-9477(02)00400-9 ↗
7. Petritsch · Synth. Met. · 1999 · 102 · 177610.1016/S0379-6779(98)01035-2 ↗
8. B. Kippelen, S. Yo, B. Domercq, C.L. Donley, C. Carter, W. Xia, B.A. Minch, D.F. O’Brien, N.R. Armstrong, NCPV and Solar Program Review Meeting, Denver, 21–23 March, 2003, p. 431.
9. Oukachmih · Sol. Energy Mater. Sol. Cells · 2005 · 85 · 53510.1016/j.solmat.2004.05.012 ↗
10. Grelet · Europhys. Lett. · 2006 · 73 · 71210.1209/epl/i2005-10459-5 ↗
11. Séguy · J. Appl. Phys. · 2001 · 89 · 544210.1063/1.1365059 ↗
12. Hassheider · Angew. Chem. · 2001 · 113 · 211910.1002/1521-3757(20010601)113:11<2119::AID-ANGE2119>3.0.CO;2-G ↗
13. Kim · Synth. Met. · 2000 · 111–112 · 36910.1016/S0379-6779(99)00329-X ↗
14. P.G. de Gennes, F. Brochard-Wyart, D. Quere, Gouttes, Bulles, Perles et Ondes, Belin, Paris, Collection Echelles, 2002.
15. Wu · 1982
16. Zhong · Phys. Status Solidi A · 2003 · 198 · 19710.1002/pssa.200306583 ↗
17. Kim · J. Korean Phys. Soc. · 2002 · 41 · 39
18. Ip · Synth. Met. · 2003 · 138 · 10710.1016/S0379-6779(02)01299-7 ↗
19. Clark · Thin Solid Films · 1980 · 70 · 26110.1016/0040-6090(80)90367-3 ↗
20. Nguyen · Synth. Met. · 2003 · 138 · 11310.1016/S0379-6779(02)01301-2 ↗
21. Yu · Appl. Phys. Lett. · 2001 · 78 · 259510.1063/1.1367897 ↗
22. Kim · Chem. Phys. Lett. · 1999 · 315 · 30710.1016/S0009-2614(99)01233-6 ↗
23. Kim · Synth. Met. · 2000 · 101 · 11110.1016/S0379-6779(98)01127-8 ↗
24. Chaney · Appl. Surf. Sci. · 2001 · 180 · 21410.1016/S0169-4332(01)00347-6 ↗
25. Chaney · Appl. Surf. Sci. · 2003 · 218 · 25910.1016/S0169-4332(03)00617-2 ↗
26. Ma · Thin Solid Films · 2000 · 371 · 14010.1016/S0040-6090(00)00994-9 ↗
27. Donley · Langmuir · 2002 · 18 · 45010.1021/la011101t ↗
28. Israelachvili · 1992
29. Reiter · Langmuir · 1999 · 1 · 255110.1021/la981470y ↗
30. Sarlah · 2001
31. Seemann · J. Phys. C: Condens. Matter · 2001 · 13 · 4925
32. Seemann · J. Phys. C: Condens. Matter · 2005 · 17 · 267
33. Sarlah · Mol. Cryst. Liq. Cryst. · 2001 · 364 · 44310.1080/10587250108025014 ↗