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Crystal Research and Technology |
Cryst. Res. Technol. 40, 1003 (2005) - Abstract -
Homoepitaxy of ZnTe on (100) oriented substrates: Technology issues and MOVPE growth aspects
M. Traversa, N. Lovergine, P. Prete*, L. Tapfer**, and A. M. Mancini
Dip. di Ingegneria dell’Innovazione, Università di Lecce, Via Arnesano I-73100 Lecce, Italy
*IMM-CNR, Sez. di Lecce, Via Arnesano I-73100 Lecce, Italy
**ENEA/UTS-MAT, Centro Ricerche di Brindisi, S.S. 7 “Appia”, km 714, I-72100 Brindisi, Italy
| Keywords | ZnTe, homoepitaxy, High Resolution X-Ray Diffraction, surface morphology, defects, MOVPE |
| PACS | 68.55.Jk, 78.55.Et, 81.05.Dz, 81.15.Gh |
| DOI | 10.1002/crat.200410476 |
The metalorganic vapour phase epitaxy of ZnTe on single crystal (100)ZnTe:P wafers is reported. The technological steps to prepare a substrate surface suitable for the high quality homoepitaxy of ZnTe are identified and optimised in terms of structural and morphological properties of overgrown epilayers. Removal of ~7 μm of material from the ZnTe:P wafers by chemical etching in 1% Br2-methanol solution proved necessary to achieve a sufficiently smooth and homogeneous surface; in-situ H2 heat treatment of the wafers at 350°C immediately before growth ensures optimal desorption of residual oxides, allowing epilayer crystalline quality comparable to the substrate. However, the structure of epilayers degrades for growth temperatures (TG) above 350°C due to the occurrence of stacking faults (SFs) within ~200-300 nm from the epilayer-substrate interface. Accordingly, the epilayer band-edge luminescence vanishes below 350 nm, indicating a worsening of the material radiative efficiency in very thin epilayers.
The epilayer surface morphology is the result of a complex interplay between SF nucleation and Te:Zn ad-atom stoichiometry during growth. Almost featureless morphologies are obtained for growth at 350°C, i.e. under nearly stoichiometric surface conditions. Pyramid-like hillocks develop instead for TG ≥ 360°C, corresponding to Te-rich surface conditions, their density rapidly increasing up to around 9x106 cm-2 at TG

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