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Molecular dynamics studies of defect formation during heteroepitaxial growthof InGaN alloys on (0001) GaN surfaces

机译:外延生长过程中缺陷形成的分子动力学研究(0001)GaN表面上的InGaN合金的制备

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摘要

We investigate the formation of extended defects during molecular-dynamics (MD) simulations of GaN and InGaN growth on (0001) and (112¯0) wurtzite-GaN surfaces. The simulated growths are conducted on an atypically large scale by sequentially injecting nearly a million individual vapor-phase atoms towards a fixed GaN surface; we apply time-and-position-dependent boundary constraints that vary the ensemble treatments of the vapor-phase, the near-surface solid-phase, and the bulk-like regions of the growing layer. The simulations employ newly optimized Stillinger-Weber In-Ga-N-system potentials, wherein multiple binary and ternary structures are included in the underlying density-functional-theory training sets, allowing improved treatment of In-Ga-related atomic interactions. To examine the effect of growth conditions, we study a matrix of >30 different MD-growth simulations for a range of InxGa1-xN-alloy compositions (0 ≤ x ≤ 0.4) and homologous growth temperatures [0.50 ≤ T/T*m(x) ≤ 0.90], where T*m(x) is the simulatedmelting point. Growths conducted on polar (0001) GaN substrates exhibit theformation of various extended defects including stacking faults/polymorphism, associated domainboundaries, surfaceroughness, dislocations, and voids. In contrast, selected growths conductedon semi-polar (112¯0) GaN, where the wurtzite-phase stacking sequence is revealed at thesurface, exhibit the formation of far fewer stacking faults. We discuss variations in thedefect formationwith the MD growth conditions, and we compare the resulting simulatedfilms toexisting experimental observations in InGaN/GaN. While the palette of defects observed by MD closelyresembles those observed in the past experiments, further work is needed to achieve trulypredictive large-scale simulations of InGaN/GaN crystal growth using MDmethodologies.
机译:我们研究了在(0001)和( 11 2 0 )纤锌矿-GaN表面。通过向固定的GaN表面依​​次注入将近一百万个单独的气相原子,可以非典型地大规模进行模拟生长。我们应用了与时间和位置有关的边界约束,这些约束改变了气相,近表面固相和生长层的块状区域的整体处理。该模拟采用了新近优化的Stillinger-Weber In-Ga-N系统势能,其中基础的密度泛函理论训练集中包括多个二元和三元结构,从而可以改进In-Ga相关原子相互作用的处理。为了检查生长条件的影响,我们研究了一系列InxGa1-xN合金成分(0≤x≤0.4)和同源生长温度[0.50≤T / T 30种不同MD增长模拟的矩阵* m(x)≤0.90],其中T * m(x)是模拟的熔点。在极性(0001)GaN衬底上进行的生长显示出形成各种扩展缺陷,包括堆垛层错/多态性,相关域边界,表面粗糙度,位错和空隙。相反,选择的增长进行了在半极性( 11 2 0 )GaN,其中纤锌矿相堆叠顺序显示在表面上,形成的堆积断层少得多。我们讨论了缺陷形成与MD的生长条件,我们将模拟结果进行比较电影到InGaN / GaN中现有的实验观察结果。 MD密切观察缺陷的调色板与过去的实验相似,需要进一步的工作才能真正实现使用MD进行InGaN / GaN晶体生长的预测性大规模模拟方法论。

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