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首页> 外文期刊>Journal of Applied Physics >Highly mismatched crystalline and amorphous GaN_(1-x)AS_x alloys in the whole composition range
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Highly mismatched crystalline and amorphous GaN_(1-x)AS_x alloys in the whole composition range

机译:在整个组成范围内高度失配的晶体和非晶GaN_(1-x)AS_x合金

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摘要

Alloying is a commonly accepted method to tailor properties of semiconductor materials for specific applications. Only a limited number of semiconductor alloys can be easily synthesized in the full composition range. Such alloys are, in general, formed of component elements that are well matched in terms of ionicity, atom size, and electronegativity. In contrast there is a broad class of potential semiconductor alloys formed of component materials with distinctly different properties. In most instances these mismatched alloys are immiscible under standard growth conditions. Here we report on the properties of GaN_(1-x)As_x, a highly mismatched, immiscible alloy system that was successfully synthesized in the whole composition range using a nonequilibrium low temperature molecular beam epitaxy technique. The alloys are amorphous in the composition range of 0.17 0.2, and to the upward movement of the valence band for alloys with x < 0.2. The unique features of the band structure offer an opportunity of using GaN_(1-x)As_x alloys for various types of solar power conversion devices.
机译:合金化是为特定应用定制半导体材料性能的普遍接受的方法。在整个组成范围内,只有有限数量的半导体合金可以容易地合成。通常,此类合金由在离子性,原子尺寸和电负性方面非常匹配的组成元素形成。相反,存在由具有明显不同性质的组分材料形成的广泛的潜在半导体合金。在大多数情况下,这些错配的合金在标准生长条件下是不溶混的。在这里,我们报告了GaN_(1-x)As_x的性质,这是一种高度失配,不混溶的合金系统,该系统已使用非平衡低温分子束外延技术成功地在整个组成范围内进行了合成。合金在0.17 <x <0.75的范围内是非晶态的,并且在该区域之外是结晶的。无定形膜具有光滑的形态,均匀的组成和清晰的,清晰的光吸收边缘。带隙能量的变化范围很广,从GaN的〜3.4 eV到x〜0.85的〜0.8 eV。带隙的减小主要归因于x> 0.2的合金的导带的向下运动,以及x x <0.2的合金的价带的向上运动。带结构的独特特征提供了将GaN_(1-x)As_x合金用于各种类型的太阳能转换设备的机会。

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  • 来源
    《Journal of Applied Physics 》 |2009年第10期| 103709.1-103709.8| 共8页
  • 作者单位

    Materials Sciences Division, Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, California 94720-8197, USA;

    School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD, United Kingdom;

    Materials Sciences Division, Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, California 94720-8197, USA Materials Science and Engineering Department, University of California, Berkeley, California 94720;

    Advanced Light Source, Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, California 94720-8197, USA Department of Chemistry, University of Nevada Las Vegas, 4505 Maryland Pkwy-Box 454003, Las Vegas, Nevada 89154-4003, USA Institute of Physics, PAS, al. Lotnikow 32/46, 02-668 Warsaw, Poland;

    Advanced Light Source, Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, California 94720-8197, USA;

    Materials Sciences Division, Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, California 94720-8197, USA;

    Department of Physics, SUPA, Strathclyde University, Glasgow G4 ONG, United Kingdom;

    Department of Physics, SUPA, Strathclyde University, Glasgow G4 ONG, United Kingdom;

    Materials Sciences Division, Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, California 94720-8197, USA;

    School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD, United Kingdom;

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