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Impurity and defect interactions during laser thermal annealing in Ge

机译:Ge中激光热退火过程中的杂质和缺陷相互作用

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摘要

The microscopic mechanisms involving dopants, contaminants, and defects in Ge during pulsed melting laser thermal annealing (LTA) are investigated in detail. Samples both un-implanted and implanted with As or B are processed by LTA as well as characterized in terms of chemical (ID and 3D), electrical, and strain profiling. The clustering of As is directly measured by 3D chemical profiling and correlated with its partial electrical activation along with a reduction of the lattice strain induced by As atoms. A semi-quantitative microscopic model involving the interaction with mobile As-vacancy (AsV) complexes is proposed to describe the clustering mechanism. Boron is shown to follow different clustering behavior that changes with depth and marked by completely different strain levels. Oxygen penetrates from the surface into all the samples as a result of LTA and, only in un-implanted Ge, it occupies an interstitial position inducing also positive strain in the lattice. On the contrary, data suggest that the presence of As or B forces O to assume different configurations with negligible strain, through O-V or O-B interactions for the two dopant species, respectively. These data suggest that LTA does not inject a significant amount of vacancies in Ge, at variance with Si, unless As atoms or possibly other n-type dopants are present. These results have to be carefully considered for modeling the LTA process in Ge and its implementation in technology.
机译:详细研究了在脉冲熔融激光热退火(LTA)过程中Ge中涉及掺杂剂,污染物和缺陷的微观机理。通过LTA处理未植入和已植入As或B的样品,并根据化学(ID和3D),电学和应变分析进行表征。通过3D化学分布图直接测量As的团簇,并将其与部分电活化以及As原子引起的晶格应变降低相关联。提出了一个半定量微观模型,该模型涉及与移动式As-空位(AsV)配合物的相互作用。硼表现出不同的聚集行为,该行为随深度而变化,并具有完全不同的应变水平。 LTA的作用是使氧气从表面渗透到所有样品中,并且仅在未注入的Ge中,氧气占据间隙位置,从而在晶格中引起正应变。相反,数据表明,As或B的存在分别通过两种掺杂物的O-V或O-B相互作用迫使O采取应变可忽略的不同构型。这些数据表明,除非存在As原子或可能存在其他n型掺杂剂,否则LTA不会在与Si不同的情况下向Ge中注入大量的空位。在为Ge中的LTA过程建模及其技术实现时,必须仔细考虑这些结果。

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  • 来源
    《Journal of Applied Physics》 |2016年第4期|045702.1-045702.9|共9页
  • 作者单位

    CNR-IMM MATIS and Dipartimento di Fisica e Astronomia, Universita di Padova, Via Marzolo 8, 35131 Padova, Italy;

    CNR-IMM MATIS and Dipartimento di Fisica e Astronomia, Universita di Catania, Via S. Sofia 64, 95123 Catania, Italy;

    CNR-IMM MATIS and Dipartimento di Fisica e Astronomia, Universita di Padova, Via Marzolo 8, 35131 Padova, Italy,IM2NP, CNRS-Universites d'Aix-Marseille et de Toulon, Case 142,13397 Marseille Cedex 20, France;

    CNR-IMM, Z.I. Ⅷ Strada 5, 95121 Catania, Italy;

    CNR-IMM, Via del Fosso del Cavaliere 100, 00133 Roma, Italy;

    CNR-IMM MATIS and Dipartimento di Fisica e Astronomia, Universita di Padova, Via Marzolo 8, 35131 Padova, Italy;

    CNR-IMM MATIS and Dipartimento di Fisica e Astronomia, Universita di Padova, Via Marzolo 8, 35131 Padova, Italy;

    IM2NP, CNRS-Universites d'Aix-Marseille et de Toulon, Case 142,13397 Marseille Cedex 20, France;

    IM2NP, CNRS-Universites d'Aix-Marseille et de Toulon, Case 142,13397 Marseille Cedex 20, France;

    CNR-IMM MATIS and Dipartimento di Fisica e Astronomia, Universita di Catania, Via S. Sofia 64, 95123 Catania, Italy;

    CNR-IMM MATIS and Dipartimento di Fisica e Astronomia, Universita di Padova, Via Marzolo 8, 35131 Padova, Italy;

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