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Transformation from β-Ga2O3 to GaN Nanowires via Nitridation 被引量:1

Transformation from β-Ga2O3 to GaN Nanowires via Nitridation
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摘要 Element doping is an important way to modify the properties of semiconductor materials. In our previous work, it was found that nitrogen-doping in β-Ga2O3 nanowires can induce a novel luminescence emission (around 740 nm) caused by generation of acceptor levels at the middle of the band gap of the β-Ga2O3 nanowires. Here we report that further heavy doping of nitrogen can transform the β-Ga2O3 nanowires completely into wurtzite structured GaN nanowires. Transmission electron microscopy (TEM), x-ray diffraction (XRD) and Raman spectrum are used to evaluate the transition process. Both XRD and Raman analysis reveal that the monoclinic β-Ga2O3 nanowires start phase transformation at a temperature around 850℃ towards wurtzite structured GaN. Our results will be very helpful to profound our understanding of the doping induced effects and phase transformation in semiconductor compounds. Element doping is an important way to modify the properties of semiconductor materials. In our previous work, it was found that nitrogen-doping in β-Ga2O3 nanowires can induce a novel luminescence emission (around 740 nm) caused by generation of acceptor levels at the middle of the band gap of the β-Ga2O3 nanowires. Here we report that further heavy doping of nitrogen can transform the β-Ga2O3 nanowires completely into wurtzite structured GaN nanowires. Transmission electron microscopy (TEM), x-ray diffraction (XRD) and Raman spectrum are used to evaluate the transition process. Both XRD and Raman analysis reveal that the monoclinic β-Ga2O3 nanowires start phase transformation at a temperature around 850℃ towards wurtzite structured GaN. Our results will be very helpful to profound our understanding of the doping induced effects and phase transformation in semiconductor compounds.
出处 《Chinese Physics Letters》 SCIE CAS CSCD 2008年第3期1038-1041,共4页 中国物理快报(英文版)
基金 Supported by the National Natural Science Foundation of China under Grant Nos 50025206, 50472024 and 20151002, and National Basic Research Programme of China under Grant No 2002CB613505. YU Da-Peng is supported by the Cheung Kong Scholar Programme.
关键词 supernova explosion proto-neutron star shock wave supernova explosion, proto-neutron star, shock wave
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