Control of film orientation: a parametric study of laser ablated FTO filmson a-, c- and r-cut sapphire substrates by X-ray diffraction

Citation
Z. Dai et al., Control of film orientation: a parametric study of laser ablated FTO filmson a-, c- and r-cut sapphire substrates by X-ray diffraction, THIN SOL FI, 349(1-2), 1999, pp. 51-55
Citations number
23
Categorie Soggetti
Apllied Physucs/Condensed Matter/Materiales Science","Material Science & Engineering
Journal title
THIN SOLID FILMS
ISSN journal
00406090 → ACNP
Volume
349
Issue
1-2
Year of publication
1999
Pages
51 - 55
Database
ISI
SICI code
0040-6090(19990730)349:1-2<51:COFOAP>2.0.ZU;2-B
Abstract
Parametric work has been done to prepare FeTiO3 (FTO) thin films on A-, C-, and R-cut sapphire substrates. We have found that the preparation of highl y oriented FTO films on different cut substrates is strongly dependent on s ubstrate temperature, laser energy density and gas pressure. The orientatio ns of FTO thin film can be controlled both by varying substrate cut directi on and laser energy density. By varying the substrate cut directions, epita xial thin films with high quality have been successfully grown on both A- a nd C-cut sapphire substrates with different substrate temperatures. The ori entation control can also be realized by changing laser energy density, and we have grown both (11 (2) over bar 0) and (0006) oriented films on A-cut substrates with different laser energy densities. Higher laser energy densi ty developed the tendency of film growth along the (0006) direction on A-cu t substrates. At the same time, higher laser energy density enhances (0006) film growth on C-cut sapphire too. We have also found that epitaxial films can be grown on A-cut sapphire substrates in a quite large temperature ran ge from 450 to 600 degrees C. However, we have not got epitaxial film on R- cut sapphire substrate in a quite wide temperature range from 300 to 600 de grees C. Probably it can be grown at a higher temperature which now is not accessible to our PLD system. (C) 1999 Elsevier Science S.A. All rights res erved.