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arXiv 0802.1001cond-mat.stat-mechcond-mat.soft
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关于中等密度颗粒气体中爱因斯坦关系破坏的一个注记

A note on the violation of the Einstein relation in a driven moderately dense granular gas

Vicente Garzo

摘要:

在Enskog动力学方程的背景下,在$d$维驱动中等密度颗粒气体的爱因斯坦关系进行了分析。Enskog方程忽略了速度相关性,但保留了体积排阻效应产生的空间相关性。正如所预期的,存在与扩散$D$和迁移率$μ$相关的爱因斯坦关系式$ε=D/(T_0μ)\neq 1$的故障,$T_0$是杂质的温度。动力学理论的结果还表明,爱因斯坦关系的破坏仅仅是由于杂质粒子参考态的强非麦克斯韦行为。随着固体体积分数和非弹性的增加,$ε$与1的偏差变得更加显著,特别是当系统由高斯恒温器的作用驱动时。这一结论定性地与最近对稠密气体的一些模拟一致[Puglisi { \em et al.},2007 { \em J. Stat.机械。} P08016],尽管在计算机模拟中观察到的偏差比从Enskog动力学理论中获得的偏差更重要。理论和模拟之间的定量差异的可能原因进行了讨论。

英文摘要:

The Einstein relation for a driven moderately dense granular gas in $d$-dimensions is analyzed in the context of the Enskog kinetic equation. The Enskog equation neglects velocity correlations but retains spatial correlations arising from volume exclusion effects. As expected, there is a breakdown of the Einstein relation $ε=D/(T_0μ)\neq 1$ relating diffusion $D$ and mobility $μ$, $T_0$ being the temperature of the impurity. The kinetic theory results also show that the violation of the Einstein relation is only due to the strong non-Maxwellian behavior of the reference state of the impurity particles. The deviation of $ε$ from unity becomes more significant as the solid volume fraction and the inelasticity increase, especially when the system is driven by the action of a Gaussian thermostat. This conclusion qualitatively agrees with some recent simulations of dense gases [Puglisi {\em et al.}, 2007 {\em J. Stat. Mech.} P08016], although the deviations observed in computer simulations are more important than those obtained here from the Enskog kinetic theory. Possible reasons for the quantitative discrepancies between theory and simulations are discussed.

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