Wüest M. 51 Wykes M. 82 Yamaguchi M. 17 Ybarra G. 129 Yubero F ...
Wüest M. 51 Wykes M. 82 Yamaguchi M. 17 Ybarra G. 129 Yubero F ...
Wüest M. 51 Wykes M. 82 Yamaguchi M. 17 Ybarra G. 129 Yubero F ...
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JUNE 28 WEDNESDAY AFTERNOON<br />
JS1-WeA-P.4 PHOTOLUMINESCENCE AND BAND-SPLITTING IN CDS THIN<br />
FILMS, INFLUENCE OF CDCL 2 AND THERMAL ANNEALING. O. Vigil-Galán, G.<br />
Contreras-Puente, and J. Aguilar-Hernández. Escuela Superior de Física y Matemáticas, Instituto Politécnico<br />
Nacional, México 07738 D.F. J. Vidal-Larramendi, and A. Arias-Carbajal. Univ. de la Habana,<br />
43100, La Habana, Cuba. O. Zelaya-Angel. Departamento de Física, CINVESTAV-IPN, P.O.<br />
Box 14-740, México 07360 D. F.<br />
CdS thin films were deposited on conducting glass substrates by three different techniques: (a)<br />
chemical bath deposition (CBD), (b) close spaced vapor transport (CSVT), and (c) laser ablation<br />
(LA). As-grown and coated with CdCl 2 CdS-samples were thermal treated (TT) in Ar. From optical<br />
absorption measurements the valence band splitting in cubic and hexagonal layers are observed (in<br />
CBD and CSVT films). In the case of CdS films grown by CSVT the hexagonal wurtzite (W) crystalline<br />
phase is observed in as-grown and TT samples, while using CBD as-grown and annealed CdS<br />
films are cubic zincblende (ZB). For LA-CdS samples no band splitting was observed in both asgrown<br />
and annealed samples, these two types of LA-CdS layers have W as crystalline phase. Band<br />
splitting is characterized for the variation of the energy band gap (E g ) shift (ΔE g ) due to the spin-orbit<br />
*<br />
*<br />
interaction with ΔE g = 0.069 eV, where ΔE g → Δ E g<br />
when ZB → W, with Δ E g<br />
= 0.081 eV, the<br />
change is owing to the reordering of splitting levels because of the addition of the crystal field interaction.<br />
The evolution of the crystalline quality and the ΔE g change in the three kinds of grown films,<br />
beside optical absorption measurements, was studied from photoluminescence spectra<br />
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