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Effect of antimony segregation on the electronic properties of InAs/InAsSb superlattices

机译:锑隔离对INAS / INASSB超晶格电子特性的影响

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There has been great progress in recent years in advancing the state-of-the-art of Ga-free InAs/InAsSb superlattice (SL) materials for infrared detector applications, spurred by the observation of long minority carrier lifetimes in this material system. However, compositional and dimensional changes through antimony (Sb) segregation alter the detector properties from those originally designed. For this reason, in this work, the authors explore epitaxial conditions that can mitigate this segregation in order to produce high-quality SL materials for optimum detector performance. A nominal SL structure of 7.7 nm InAs/3.5 nm InAs_(0.7)Sb_(0.3) tailored for an approximately six-micron response at 5 K was used to optimize the epitaxial parameters. Since the growth of mixed AsSb alloys is complicated by the potential reaction of As with Sb surfaces, the authors vary the substrate temperature (T_s) in order to control the As surface reaction on a Sb surface. Experimental results indicate that the SL sample grown at the lowest investigated T_s produces the highest Sb-mole fraction x of ~0.3 in InAs_(1-x)Sb_x layers, which then decreases by 21 % as the T_s increases from 395 to 440 °C. This reduction causes an approximately 30 meV blueshift in the position of the excitonic photoluminescence (PL) peak. This finding differs from the results obtained from the Ga-containing InAs/GaSb SL equivalents, where the PL peak position remains constant at about 220 meV, regardless of T_s. The Ga-free SLs generally generate a broader PL linewidth than the corresponding Ga-containing SLs due to the higher spatial Sb distribution at the hetero-interfaces engendered by Sb segregation. In order for this newly proposed Ga-free SL materials to be viable for detector applications, the material problem associated with Sb segregation needs to be adequately controlled and further mitigated.
机译:近年来近年来在推进了对红外探测器应用的无限内部/ INASSB超晶格(SL)材料的最先进的探测器,通过观察本材料体系中的长少数载体寿命来促进的。然而,通过锑(Sb)偏析的组成和尺寸变化改变了最初设计的探测器性能。因此,在这项工作中,作者探讨了可以减轻这种隔离的外延条件,以便生产用于最佳探测器性能的高质量SL材料。用于在5 k下定制大约六微米响应的7.7nm inas / 3.5nm inas_(0.7)Sb_(0.3)的标称SL结构用于优化外延参数。由于混合ASSB合金的生长与与SB表面的潜在反应复杂化,因此作者改变衬底温度(T_S),以便控制在SB表面上的表面反应。实验结果表明,在最低研究的T_S上生长的SL样品在inas_(1-x)sb_x层中产生〜0.3的最高Sb-mole分数x,然后随后将T_S从395增加到440°C增加21% 。这种减少导致激发光致发光(PL)峰的位置约30meV蓝。该发现与从含GA的INAS / GASB SL等同物获得的结果不同,其中PL峰位置在约220meV时保持恒定,无论T_S如何。由于SB偏析发出的异质界面,Ga-Fain的SLS通常产生比相应的GA的SLS更宽的P1线宽。为了使这种新提出的GA-FAL的SL材料可用于探测器应用,需要充分控制和进一步减轻与SB偏析相关的材料问题。

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