研究目的
Investigating the effects of ion irradiation on Sb-rich GaSb films deposited by magnetron sputtering, focusing on structural, compositional, and morphological changes.
研究成果
Ion irradiation induces the formation of pores in Sb-rich GaSb films, evolving into a foam-like structure at sufficient fluence. The swelling of the films depends on both irradiation fluence and initial film thickness, with thicker films swelling more. The local atomic structure around Ga atoms changes with irradiation, showing a decrease in Ga–Sb scattering and an increase in Ga–O scattering for higher fluences.
研究不足
The study is limited to Sb-rich GaSb films and does not explore the effects of ion irradiation on stoichiometric GaSb films. The mechanisms governing the formation of porous layers by ion irradiation are still not fully understood.
1:Experimental Design and Method Selection:
GaSb films were deposited by RF magnetron sputtering onto Si (100) and SiO2/Si substrates at room temperature. The films were then irradiated with 17 MeV Au+7 ions at different fluences. Structural, compositional, and morphological characterizations were performed using XRD, RBS, XPS, SEM, and XAFS techniques.
2:Sample Selection and Data Sources:
Films with thicknesses ranging from 20 to 300 nm were selected for irradiation. The base pressure during deposition was lower than 4×10?8 Torr, with a constant Ar flow of 20 sccm and pressure maintained at 2 mTorr.
3:List of Experimental Equipment and Materials:
RF magnetron sputtering system, Tandetron 3MV accelerator for ion irradiation, Siemens D500 diffractometer for XRD, Carl Zeiss Auriga FEG-SEM microscope for SEM, and synchrotron-based techniques for XPS and XAFS analyses.
4:Experimental Procedures and Operational Workflow:
Films were deposited, then irradiated with Au+7 ions at room temperature and normal incidence. Post-irradiation, films were characterized using the aforementioned techniques to analyze structural and compositional changes.
5:Data Analysis Methods:
RBS data were analyzed using the SIMNRA code. XPS spectra were fitted using XPSPeak version 4.1. XAFS spectra were analyzed using the IFEFFIT package.
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