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纳米银准晶结构的原子起源:分子动力学与X射线衍射研究

Atomistic origin of nano-silver paracrystalline structure: molecular dynamics and x-ray diffraction studies.

作者信息

Jurkiewicz Karolina, Kamiński Michał, Bródka Aleksander, Burian Andrzej

机构信息

A. Chełkowski Institute of Physics, University of Silesia in Katowice, 75 Pułku Piechoty 1, 41-500 Chorzów, Poland.

Silesian Center for Education and Interdisciplinary Research, 75 Pułku Piechoty 1a, 41-500 Chorzów, Poland.

出版信息

J Phys Condens Matter. 2022 Jul 14;34(37). doi: 10.1088/1361-648X/ac7d84.

Abstract

Classical molecular dynamics (MD) and x-ray diffraction (XRD) have been used to establish the origin of the paracrystalline structure of silver nanoparticles at the atomic scale. Models based on the face-centred cubic structure have been computer generated and their atomic arrangements have been optimized by the MD with the embedded-atom model (EAM) potential and its modified version (MEAM). The simulation results are compared with the experimental XRD data in reciprocal and real spaces, i.e. the structure factor and the pair distribution function. The applied approach returns the structural models, defined by the Cartesian coordinates of the constituent atoms. It has been found that most of the structural features of Ag nanoparticles are better reproduced by the MEAM. The presence of vacancy defects in the structure of the Ag nanoparticles has been considered and the average concentration of vacancies is estimated to be 3 at.%. The average nearest-neighbour Ag-Ag distances and the coordination numbers are determined and compared with the values predicted for the bulk Ag, demonstrating a different degree of structural disorder on the surface and in the core, compared to the bulk crystalline counterpart. It has been shown that the paracrystalline structure of the Ag nanoparticles has origin in the surface disorder and the disorder generated by the presence of the vacancy defects. Both sources lead to network distortion that propagates proportionally to the square root of the interatomic distances.

摘要

经典分子动力学(MD)和X射线衍射(XRD)已被用于在原子尺度上确定银纳米颗粒准晶结构的起源。基于面心立方结构的模型已通过计算机生成,并且它们的原子排列已通过使用嵌入原子模型(EAM)势及其改进版本(MEAM)的分子动力学进行了优化。将模拟结果与倒易空间和实空间中的实验XRD数据进行比较,即结构因子和对分布函数。所应用的方法返回由组成原子的笛卡尔坐标定义的结构模型。已经发现,MEAM能更好地再现银纳米颗粒的大多数结构特征。考虑了银纳米颗粒结构中空位缺陷的存在,并且估计空位的平均浓度为3原子%。确定了平均最近邻银 - 银距离和配位数,并与体相银预测的值进行比较,表明与体相晶体对应物相比,表面和核心的结构无序程度不同。已经表明,银纳米颗粒的准晶结构起源于表面无序和空位缺陷的存在所产生的无序。这两种来源都会导致网络畸变,该畸变与原子间距离的平方根成比例传播。

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