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arXiv 1407.4202cond-mat.soft
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粘弹性碰撞下颗粒气体中激波不稳定性的演化

Evolution of shock instability in granular gases with viscoelastic collisions

Nick Sirmas, Matei Radulescu

摘要:

粒状介质中的冲击已被证明会产生不稳定性。我们解决的作用,冲击发展的早期阶段对这种类型的不稳定性。我们看看在一个稀释系统的光滑非弹性磁盘,使用离散粒子和连续模拟的活塞驱动的冲击波的演变。为了模拟真实的粒状气体,粘弹性碰撞近似为发生非弹性碰撞所需的冲击速度阈值$u^*$。我们表明,冲击演化的行为是依赖于活塞速度的比例,冲击速度阈值$u_p/u^*$,和恢复系数$\varepsilon$。对于$u_p/u^*=2.0$,我们恢复冲击演化行为类似于在纯非弹性介质中观察到的。其特征在于,在获得展开结构之前,冲击波阵面拉向活塞的时间很短。未观察到$u_p/u^*=1.0$回撤。结果表明,这些较强的冲击,在这一发展阶段的不稳定性的开始。这些结果表明,激波演化的早期阶段在激波不稳定性中起着重要的作用。

英文摘要:

Shocks in granular media have been shown to develop instabilities. We address the role that early stages of shock development have on this type of instability. We look at the evolution of shock waves driven by a piston in a dilute system of smooth inelastic disks, using both discrete-particle and continuum modelling. To mimic a realistic granular gas, viscoelastic collisions are approximated with an impact velocity threshold $u^*$ needed for inelastic collisions to occur. We show that behaviour of the shock evolution is dependent on the ratio of piston velocity to impact velocity threshold $u_p/u^*$, and the coefficient of restitution $\varepsilon$. For $u_p/u^*=2.0$, we recover shock evolution behaving similar to that observed in purely inelastic media. This is characterized by a short period where the shock front pulls towards the piston before attaining a developed structure. No pullback is seen for $u_p/u^*=1.0$. Results show the onset of instability for these stronger shocks during this evolving stage. These results suggest that the early stages of shock evolution play an important role in the shock instability.

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