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arXiv 1306.4692physics.flu-dyncond-mat.soft
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柔性细丝的沉降

The sedimentation of flexible filaments

Lei Li, Harishankar Manikantan, David Saintillan, Saverio E. Spagnolie

摘要:

本文用解析和数值方法研究了柔性细丝在粘性流体中的沉降动力学。沉积刚性杆的研究情况相比,细丝的顺应性的引入被证明会导致显着的改变,在长时间的沉积方向和细丝的几何形状。通过平衡零雷诺数流动的细长体理论中的粘性力、弹性力和重力来开发模型,并且细丝动力学的特征在于无量纲的弹性重力数。考虑了非均匀和均匀横截面厚度的细丝。在弱柔性制度,多尺度渐近展开用于获得细丝的平移,旋转和形状的表达式。这些都显示出与完整的数值模拟非常匹配。此外,我们表明,与刚性对应物不同,沉降柔性细丝的轨迹仅限于其包络由弹性引力数确定的云。在高度灵活的制度,我们表明,沿其长轴沉降的细丝是容易屈曲不稳定。线性稳定性分析提供了色散关系,清楚地说明了在屈曲过程中压缩应力和恢复弹性力的竞争效应。的不稳定性旅行作为一个波沿长丝的重力方向相反,因为它的增长和预测的增长率相比,有利的数值模拟。控制方程的线性本征模也进行了研究,这与模拟中出现的有限振幅屈曲形状吻合得很好。

英文摘要:

The dynamics of a flexible filament sedimenting in a viscous fluid are explored analytically and numerically. Compared to the well-studied case of sedimenting rigid rods, the introduction of filament compliance is shown to cause a significant alteration in the long-time sedimentation orientation and filament geometry. A model is developed by balancing viscous, elastic, and gravitational forces in a slender-body theory for zero-Reynolds-number flows, and the filament dynamics are characterized by a dimensionless elasto-gravitation number. Filaments of both non-uniform and uniform cross-sectional thickness are considered. In the weakly flexible regime, a multiple-scale asymptotic expansion is used to obtain expressions for filament translations, rotations, and shapes. These are shown to match excellently with full numerical simulations. Furthermore, we show that trajectories of sedimenting flexible filaments, unlike their rigid counterparts, are restricted to a cloud whose envelope is determined by the elasto-gravitation number. In the highly flexible regime we show that a filament sedimenting along its long axis is susceptible to a buckling instability. A linear stability analysis provides a dispersion relation, illustrating clearly the competing effects of the compressive stress and the restoring elastic force in the buckling process. The instability travels as a wave along the filament opposite the direction of gravity as it grows and the predicted growth rates are shown to compare favorably with numerical simulations. The linear eigenmodes of the governing equation are also studied, which agree well with the finite-amplitude buckled shapes arising in simulations.

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