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首页> 外文期刊>IEEE Transactions on Nuclear Science >Photoluminescence study of gallium vacancy defects in gallium arsenide irradiated by relativistic protons
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Photoluminescence study of gallium vacancy defects in gallium arsenide irradiated by relativistic protons

机译:相对论质子辐照砷化镓中镓空位缺陷的光致发光研究

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摘要

Epitaxially grown n-type gallium arsenide films, doped with silicon to concentrations of 2/spl times/10/sup 15/ and 2/spl times/10/sup 16/ cm/sup -3/ were exposed at room temperature to 200, 350, and 500 MeV proton irradiation at fluences of 3/spl times/10/sup 11/, 10/sup 12/, 10/sup 13/, 3/spl times/10/sup 13/ 10/sup 14/ and 10/sup 15/ cm/sup -2/. The effects of the irradiation were determined through low temperature continuous photoluminescence spectroscopy. Two radiation-induced donor-to-acceptor transitions were observed. The one at 1.476 eV has been associated to the gallium vacancy acceptor (V/sub Ga/) and the other at 1.482 eV to the silicon at the arsenic site acceptor (Si/sub As/). The relative introduction rate of these two defects has been measured in the irradiated samples before and after annealing at 550/spl deg/C for 30 minutes. The introduction rates are higher than those predicted by relativistic elastic scattering cross-section theory in the energy range studied here. We conclude that inelastic scattering contributes to the cross-section. The introduction rates are lower than non-ionizing energy loss (NIEL) calculations in the 200 to 500 MeV energy range. We suggest that the proton inelastic scattering parameter used in NIEL needs revision. The relativistic inelastic scattering formula is closer to experiment than present NIEL calculations.
机译:在室温下将掺有硅的浓度分别为2 / spl次/ 10 / sup 15 /和2 / spl次/ 10 / sup 16 / cm / sup -3 /的外延生长n型砷化镓膜在室温下暴露于200,分别以3 / spl次/ 10sup 11 /,10 / sup 12 /,10 / sup 13 /,3 / spl次/ 10 / sup 13/10 / sup 14 /和10的通量辐照350和500 MeV质子/ sup 15 / cm / sup -2 /。通过低温连续光致发光光谱法确定辐照的效果。观察到两个辐射诱导的供体到受体的转变。一个在1.476 eV处与镓空位受体(V / sub Ga /)相关联,另一个在1.482 eV与砷位点受体处的硅(Si / sub As /)相关联。在550 / spl deg / C退火30分钟之前和之后,在被辐照的样品中测量了这两个缺陷的相对引入率。在此处研究的能量范围内,引入率高于相对论弹性散射截面理论所预测的引入率。我们得出的结论是,非弹性散射会影响横截面。在200到500 MeV的能量范围内,引入率低于非电离能量损失(NIEL)计算。我们建议需要修改NIEL中使用的质子非弹性散射参数。相对论的非弹性散射公式比当前的NIEL计算更接近于实验。

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