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二维格气模型中的 Kirkendall 效应。

Kirkendall effect in the two-dimensional lattice-gas model.

机构信息

Department of Physics, Chalmers University of Technology, Göteborg, Sweden and Boreskov Institute of Catalysis, Russian Academy of Sciences, Novosibirsk, Russia.

出版信息

Phys Rev E. 2019 Jan;99(1-1):012132. doi: 10.1103/PhysRevE.99.012132.

Abstract

Customarily, the Kirkendall effect is associated with the vacancy-mediated balance of diffusion fluxes of atoms at the interface between two metals. Nowadays, this effect attracts appreciable attention due to its crucial role in the formation of various hollow nanoparticles via oxidation of metal nanocrystallites. The understanding of the physics behind this effect in general and especially in the case of nanoparticles is still incomplete due to abundant complicating factors. Herein, the Kirkendall effect is illustrated in detail at the generic level by performing two-dimensional (2D) lattice Monte Carlo simulations of diffusion of A and B monomers with attractive nearest-neighbor interaction for times up to 10^{7} Monte Carlo steps. Initially, A monomers are considered to form a close-packed array, while B monomers are in the 2D-gas state. The A-B interaction is assumed to be stronger compared to the other interactions, so that thermodynamically the c(2×2) A-B phase is preferable compared to the close-packed A phase (as in the case of metal oxidation). Depending on the relative rate of the diffusion jumps of A and B monomers, the patterns observed at the late stage of the formation of the mixed phase are shown to range from a single array without voids to those with appreciable disintegration of the initial array. In this way, the model predicts a single array with numerous small voids, a few moderate voids, or a single large void inside.

摘要

通常情况下,柯肯达尔效应与两种金属界面处原子扩散通量的空位介导平衡有关。如今,由于其在通过金属纳米晶氧化形成各种空心纳米粒子方面的关键作用,这种效应引起了相当大的关注。由于存在大量复杂因素,人们对这种效应的物理原理的理解(尤其是在纳米粒子的情况下)还不完全。在此,通过对具有吸引力近邻相互作用的 A 和 B 单体的二维(2D)晶格蒙特卡罗模拟,在一般情况下,详细说明了柯肯达尔效应,模拟时间长达 10^{7}个蒙特卡罗步骤。最初,A 单体被认为形成密排排列,而 B 单体处于 2D-气体状态。假设 A-B 相互作用比其他相互作用强,因此从热力学角度来看,与密排 A 相比,c(2×2) A-B 相更可取(就像金属氧化的情况一样)。根据 A 和 B 单体扩散跳跃的相对速率,在混合相形成的后期观察到的模式从没有空洞的单个阵列到初始阵列有明显解体的模式不等。通过这种方式,该模型预测会形成一个具有许多小空洞、几个中等空洞或一个内部大空洞的单一阵列。

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