论文标题

干燥颗粒流的弱非静态浅层模型

A weakly non-hydrostatic shallow model for dry granular flows

论文作者

Garres-Díaz, José, Fernández-Nieto, Enrique D., Mangeney, Anne, de Luna, Tomás Morales

论文摘要

考虑到垂直加速度,提出了一个非静态深度平均模型。考虑了基于$μ(i)$流变的可变摩擦系数。该模型是从局部参考系统中的渐近分析中获得的,在局部参考系统中,与静液压相比,非静态贡献应该很小。压力的非静态对应物可以写为两个术语的总和:一个对应于应力张量,另一个与垂直加速度相对应。此处介绍的模型是弱非静态静态的,因为由于其复杂的实施,与应力张量相关的非静态贡献未被考虑。提出了一种简单有效的数值方案。它由三步分裂过程组成,并基于静水重建。两个关键点是:(i)在解决非静态压力之前必须考虑摩擦力。否则,无法确保不可压缩的条件; (ii)在处理摩擦力时,静水压力和非静态压力都被考虑。然后,基于几个数值测试,包括颗粒状塌陷实验实验,对模型和数值方案进行验证。分析了非静态术语和坐标系统(笛卡尔或本地)的选择的影响。我们表明,非静态模型对坐标系的选择不太敏感。通常,与静液压模型相比,这里引入的非静态模型可以更好地再现颗粒状塌陷实验。一个重要的结果是,模拟的质量剖面直至沉积物和前速度。如预期的那样,对于斜坡的小值,非静压压力的影响显示为更大。

A non-hydrostatic depth-averaged model for dry granular flows is proposed, taking into account vertical acceleration. A variable friction coefficient based on the $μ(I)$ rheology is considered. The model is obtained from an asymptotic analysis in a local reference system, where the non-hydrostatic contribution is supposed to be small compared to the hydrostatic one. The non-hydrostatic counterpart of the pressure may be written as the sum of two terms: one corresponding to the stress tensor and the other to the vertical acceleration. The model introduced here is weakly non-hydrostatic, in the sense that the non-hydrostatic contribution related to the stress tensor is not taken into account due to its complex implementation. A simple and efficient numerical scheme is proposed. It consists of a three-step splitting procedure, and it is based on a hydrostatic reconstruction. Two key points are: (i) the friction force has to be taken into account before solving the non-hydrostatic pressure. Otherwise, the incompressibility condition is not ensured; (ii) both the hydrostatic and the non-hydrostatic pressure are taken into account when dealing with the friction force. The model and numerical scheme are then validated based on several numerical tests, including laboratory experiments of granular collapse. The influence of non-hydrostatic terms and of the choice of the coordinate system (Cartesian or local) is analyzed. We show that non-hydrostatic models are less sensitive to the choice of the coordinate system. In general, the non-hydrostatic model introduced here much better reproduces granular collapse experiments compared to hydrostatic models. An important result is that the simulated mass profiles up to the deposit and the front velocity are greatly improved. As expected, the influence of the non-hydrostatic pressure is shown to be larger for small values of the slope.

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