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About the influence of deposited nitride layers on oxide precipitation after RTA pre-treatment

机译:关于RTA预处理后沉积的氮化物层对氧化物沉淀的影响

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In order to elucidate the influence of stress and in-diffused nitrogen on oxide precipitation after rapid thermal annealing (RTA), we carried out experiments with one-side and double-sided nitride layers accompanied by simulation models which help to understand the behavior of intrinsic point defects, nitrogen, and strain. We found that the presence of a nitride layer of any thickness, within the rage which we investigated, in direct contact with the silicon surface is sufficient to markedly change the precipitation behavior of interstitial oxygen after RTA at 1175 and 1250℃. The presence of the nitride layer during the stabilization and growth of the oxide precipitates is not of any influence on the precipitation behavior. Therefore, the RTA of wafers covered with silicon nitride is the crucial step controlling the bulk microdefect (BMD) depth profiles. A 10 nm oxide between silicon substrate and nitride layer prevents any change of the BMD depth profile. Only in a direct contact with the nitride layers the vacancy supersaturation, which enhanced the oxide precipitation compared to wafers without nitride layers, was generated. Nitrogen peaks below the silicon surface generated by in-diffusion of nitrogen during RTA lead lo an enhanced oxygen precipitation only for RTA at 1250 ℃ and not for RTA at 1175 ℃. We propose a model based on very tiny coherent a-Si_3N_4 precipitates generated at nitrogen-vacancy (NV) complexes which can act as nucleation sites for oxygen precipitation. Because the stability of NV seems limited to temperatures above 1200 ℃, it would not be effective for RTA at 1175℃. RTA treatment of silicon wafers with one-sided nitride layers at 1250℃ leads to very sharp and small defect denuded zones in subsequent annealing and would be suitable for proximity gettering. The depth of the denuded zone is nearly independent of the thickness of the nitride layer.
机译:为了阐明应力和扩散态氮对快速热退火(RTA)后氧化物沉淀的影响,我们对单面和双面氮化物层进行了实验,并辅以模拟模型,以帮助理解本征行为。点缺陷,氮和应变。我们发现,在我们研究的范围内,与硅表面直接接触的任何厚度的氮化物层的存在都足以显着改变RTA在1175和1250℃后间隙氧的沉淀行为。在氧化物沉淀物的稳定和生长期间氮化物层的存在对沉淀行为没有任何影响。因此,覆盖有氮化硅的晶圆的RTA是控制体微缺陷(BMD)深度分布的关键步骤。硅衬底和氮化物层之间的10 nm氧化物可防止BMD深度分布的任何变化。仅在与氮化物层直接接触时,才产生空位过饱和,与没有氮化物层的晶片相比,空位过饱和增强了氧化物的沉淀。在RTA期间,氮在氮中的扩散会在硅表面下方产生一个氮峰,从而导致仅在1250℃的RTA而不是1175℃的RTA处增加的氧沉淀。我们提出了一种基于氮-空位(NV)络合物产生的非常细小的相干a-Si_3N_4沉淀物的模型,该沉淀物可以充当氧沉淀的成核位点。由于NV的稳定性似乎仅限于1200℃以上的温度,因此对于1175℃的RTA无效。在1250℃下对具有单面氮化物层的硅晶片进行RTA处理会在随后的退火过程中产生非常尖锐且很小的缺陷剥蚀区,适合于近距离吸杂。剥蚀区的深度几乎与氮化物层的厚度无关。

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