Tin Gallium Oxide Epilayers on Different Substrates: Optical and Compositional Analysis

Author:

Hunter Daniel. A.1,Naresh‐Kumar Gunasekar12,Edwards Paul R.1,Makydonska Olha1,Massabuau Fabien C. P.1,Hatipoglu Isa345,Mukhopadhyay Partha5,Schoenfeld Winston V.5,Martin Robert W.1ORCID

Affiliation:

1. Department of Physics SUPA University of Strathclyde Glasgow G4 0NG UK

2. School of Physics and Astronomy Cardiff University Cardiff CF24 3AA UK

3. Photonics Application and Research Center Gazi University Ankara 06500 Turkey

4. Department of Photonics Faculty of Applied Sciences Gazi University Ankara 06500 Turkey

5. CREOL The College of Optics and Photonics University of Central Florida Orlando FL 32816 USA

Abstract

Electron beam techniques have been used to analyze the impact of substrate choice and growth parameters on the compositional and optical properties of tin gallium oxide [(SnxGa1−x)2O3] thin films grown by plasma‐assisted molecular beam epitaxy. Sn incorporation and film quality are found to be highly dependent on growth temperature and substrate material (silicon, sapphire, and bulk Ga2O3) with alloy concentrations varying up to an x value of 0.11. Room temperature cathodoluminescence spectra show the Sn alloying suppressing UV (3.3–3.0 eV), enhancing blue (2.8–2.4 eV), and generating green (2.4–2.0 eV) emission, indicative of the introduction of a high density of gallium vacancies (VGa) and subsequent VGa–Sn complexes. This behavior was further analyzed by mapping composition and luminescence across a cross section. Compared to Ga2O3, the spectral bands show a clear redshift due to bandgap reduction, confirmed by optical transmission measurements. The results show promise that the bandgap of gallium oxide can successfully be reduced through Sn alloying and used for bandgap engineering within UV optoelectronic devices.

Funder

Engineering and Physical Sciences Research Council

Publisher

Wiley

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