Thermal instability of GaSb surface oxide

K. Tsunoda; Y. Matsukura; R. Suzuki; M. Aoki

doi:10.1117/12.2223583

20 May 2016 Thermal instability of GaSb surface oxide

K. Tsunoda, Y. Matsukura, R. Suzuki, M. Aoki

Proceedings Volume 9819, Infrared Technology and Applications XLII; 98190S (2016) https://doi.org/10.1117/12.2223583
Event: SPIE Defense + Security, 2016, Baltimore, MD, United States

Abstract

In the development of InAs/GaSb Type-II superlattice (T2SL) infrared photodetectors, the surface leakage current at the mesa sidewall must be suppressed. To achieve this requirement, both the surface treatment and the passivation layer are key technologies. As a starting point to design these processes, we investigated the GaSb oxide in terms of its growth and thermal stability. We found that the formation of GaSb oxide was very different from those of GaAs. Both Ga and Sb are oxidized at the surface of GaSb. In contrast, only Ga is oxidized and As is barely oxidized in the case of GaAs. Interestingly, the GaSb oxide can be formed even in DI water, which results in a very thick oxide film over 40 nm after 120 minutes. To examine the thermal stability, the GaSb native oxide was annealed in a vacuum and analyzed by XPS and Raman spectroscopy. These analyses suggest that SbO_x in the GaSb native oxide will be reduced to metallic Sb above 300°C. To directly evaluate the effect of oxide instability on the device performance, a T2SL p-i-n photodetector was fabricated that has a cutoff wavelength of about 4 μm at 80 K. As a result, the surface leakage component was increased by the post annealing at 325°C. On the basis of these results, it is possible to speculate that a part of GaSb oxide on the sidewall surface will be reduced to metallic Sb, which acts as an origin of additional leakage current path.

Citation Download Citation

K. Tsunoda, Y. Matsukura, R. Suzuki, and M. Aoki "Thermal instability of GaSb surface oxide", Proc. SPIE 9819, Infrared Technology and Applications XLII, 98190S (20 May 2016); https://doi.org/10.1117/12.2223583

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