粒子间正面低速碰撞的分子动力学模拟

Yuki Yoshida, Eiichiro Kokubo, Hidekazu Tanaka
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引用次数: 0

摘要

颗粒接触模型对于粉末模拟非常重要。虽然已经提出了多种接触模型,但其有效性尚未得到很好的证实。因此,我们进行了分子动力学(MD)模拟来澄清粒子的相互作用。我们模拟了撞击速度小于声速百分之几的两个颗粒的正面碰撞,以研究颗粒间作用力和替代系数(COR)与撞击速度和颗粒半径的关系。在这项研究中,我们处理了半径为 10-100 nm 的粒子并进行了模拟。我们发现,颗粒间的作用力在加载和卸载阶段之间表现出滞后性。较大的冲击速度会导致强烈的滞后和塑性变形。在所有冲击速度和颗粒半径下,恢复系数都小于约翰逊-肯德尔-罗伯特理论给出的数值。非弹性接触模型无法再现我们的模拟结果。特别是,当冲击速度超过一定值时,COR 会明显降低。即使是包含塑性变形的接触模型也无法解释这种显著的能量耗散。我们还发现,COR 随颗粒半径的增大而增大。我们还发现,以前的接触模型(包括塑性变形)虽然与极低冲击速度下的 MD 结果一致,但无法解释 MD 模拟中获得的强大能量耗散。因此,我们构建了一个新的耗散接触模型,其中耗散力随碰撞产生的应力而增加。与传统模型相比,新的应力依赖模型在更大的冲击速度范围内成功地再现了我们的 MD 结果。此外,我们还提出了另一种更简单的耗散接触模型,它也能再现 MD 结果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Molecular dynamics simulations of head-on low-velocity collisions between particles
The particle contact model is important for powder simulations. Although several contact models have been proposed, their validity has not yet been well established. Therefore, we perform molecular dynamics (MD) simulations to clarify the particle interaction. We simulate head-on collisions of two particles with impact velocities less than a few percent of the sound velocity to investigate the dependence of the interparticle force and the coefficient of restitution (COR) on the impact velocity and particle radius. In this study, we treat particles with a radius of 10-100 nm and perform simulations. We find that the interparticle force exhibits hysteresis between the loading and unloading phases. Larger impact velocities result in strong hysteresis and plastic deformation. For all impact velocities and particle radii, the coefficient of restitution is smaller than that given by the Johnson-Kendall-Robert theory. An inelastic contact model cannot reproduce our MD simulations. In particular, the COR is significantly reduced when the impact velocity exceeds a certain value. This significant energy dissipation cannot be explained even by the contact models including plastic deformation. We also find that the COR increases with increasing particle radius. We also find that the previous contact models including plastic deformation cannot explain the strong energy dissipation obtained in our MD simulations, although they agree with the MD results for very low impact velocities. Accordingly, we have constructed a new dissipative contact model in which the dissipative force increases with the stress generated by collisions. The new stress dependent model successfully reproduces our MD results over a wider range of impact velocities than the conventional models do. In addition, we proposed another, simpler, dissipative contact model that can also reproduce the MD results.
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