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Richtmyer-Meshkov instability for elastic-plastic solids in converging geometries

机译:会聚几何中弹塑性固体的Richtmyer-Meshkov不稳定性

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We present a detailed study of the interface instability that develops at the boundary between a shell of elastic-plastic material and a cylindrical core of confined gas during the inbound implosive motion generated by a shock-wave. The main instability in this configuration is the so-called Richtmyer-Meshkov instability that arises when the shock wave crosses the material interface. Secondary instabilities, such as Rayleigh-Taylor, due to the acceleration of the interface, and Kelvin-Helmholtz, due to slip between solid and fluid, arise as the motion progresses. The reflection of the shock wave at the axis and its second interaction with the material interface as the shock moves outbound, commonly known as re-shock, results in a second Richtmyer-Meshkov instability that potentially increases the growth rate of interface perturbations, resulting in the formation of a mixing zone typical of fluid-fluid configurations and the loss of the initial perturbation length scales. The study of this problem is of interest for achieving stable inertial confinement fusion reactions but its complexity and the material conditions produced by the implosion close to the axis prove to be challenging for both experimental and numerical approaches. In this paper, we attempt to circumvent some of the difficulties associated with a classical numerical treatment of this problem, such as element inversion in Lagrangian methods or failure to maintain the relationship between the determinant of the deformation tensor and the density in Eulerian approaches, and to provide a description of the different events that occur during the motion of the interface. For this purpose, a multi-material numerical solver for evolving in time the equations of motion for solid and fluid media in an Eulerian formalism has been implemented in a Cartesian grid. Equations of state are derived using thermodynamically consistent hyperelastic relations between internal energy and stresses. The resolution required for capturing the state of solid and fluid materials close to the origin is achieved by making use of adaptive mesh refinement techniques. Rigid-body rotations contained in the deformation tensor have been shown to have a negative effect on the accuracy of the method in extreme compression conditions and are removed by transforming the deformation tensor into a stretch tensor at each time step. With this methodology, the evolution of the interface can be tracked up to a point at which numerical convergence cannot be achieved due to the inception of numerical Kelvin-Helmholtz instabilities caused by slip between materials. From that point, only qualitative conclusions can be extracted from this analysis. The influence of different geometrical parameters, initial conditions, and material properties on the motion of the interface are investigated. Some major differences are found with respect to the better understood fluid-fluid case. For example, increasing the wave number of the interface perturbations leads to a second phase reversal of the interface (i.e., the first phase reversal of the interface naturally occurs due to the initial negative growth-rate of the instability as the shock wave transitions from the high-density material to the low-density one). This phenomenon is caused by the compressive effect of the converging geometry and the low density of the gas with respect to the solid, which allows for the formation of an incipient spike in the center of an already existing bubble. Multiple solid-gas density ratios are also considered. Results show that the motion of the interface asymptotically converges to the solid-vacuum case. When a higher initial density for the gas is considered, the growth rate of interface perturbations decreases and, in some situations, its sign may reverse, as the fluid becomes more dense than the solid due to having higher compressibility. Finally, the influence of the Mach number of the driving shock and the yield stress on the mixing-zone is examined. We find that the width of the mixing zone produced after the re-shock increases in proportion to the strength of the incident shock. An increased yield stress in the solid material makes the interface less unstable due to vorticity being carried away from the interface by shear waves and limits the generation of smaller length scales after the re-shock.
机译:我们目前对界面不稳定性的详细研究,该界面不稳定性是在冲击波产生的内向内爆运动过程中,在弹塑性材料的壳体与封闭气体的圆柱形芯之间的边界处发展的。这种配置中的主要不稳定性是当冲击波穿过材料界面时出现的所谓的Richtmyer-Meshkov不稳定性。随着运动的进行,会出现二次不稳定性,例如由于界面加速引起的瑞利-泰勒(Rayleigh-Taylor)和由于固体与流体之间的滑动而引起的开尔文-亥姆霍兹(Kelvin-Helmholtz)。激波在轴上的反射及其在激波向外移动时与材料界面的第二次相互作用(通常称为重新激波)会导致第二次Richtmyer-Meshkov不稳定性,从而可能增加界面扰动的增长率,从而导致形成典型的流体-流体混合区,并失去初始扰动长度尺度。研究这个问题对于实现稳定的惯性约束聚变反应是有意义的,但是它的复杂性和由靠近轴的内爆所产生的材料条件对实验和数值方法都证明是具有挑战性的。在本文中,我们尝试规避与该问题的经典数值处理相关的一些困难,例如拉格朗日方法中的元素反演或变形张量的行列式与密度在欧拉方法中的关系无法维持,以及提供对界面运动期间发生的不同事件的描述。为此,已经在笛卡尔网格中实现了一种多材料数值求解器,用于在欧拉形式主义中及时演化固体和流体介质的运动方程。状态方程是使用内部能量和应力之间的热力学一致超弹性关系得出的。通过使用自适应网格细化技术,可以获得捕获接近原点的固体和流体材料状态所需的分辨率。在极端压缩条件下,变形张量中包含的刚体旋转已显示出对该方法的精度有负面影响,并且通过在每个时间步将变形张量转换为拉伸张量而将其消除。使用这种方法,由于材料之间滑动引起的开尔文-亥姆霍兹数值不稳定性的出现,可以跟踪界面的演化直至无法实现数值收敛。从这一点出发,只能从该分析中得出定性结论。研究了不同的几何参数,初始条件和材料特性对界面运动的影响。对于更好理解的流体情况,发现了一些主要差异。例如,增加界面扰动的波数会导致界面的第二相反转(即,界面的第一相反转自然会由于不稳定性的初始负增长率而发生,因为当冲击波由高密度材料到低密度的一种)。这种现象是由于会聚的几何形状的压缩作用和气体相对于固体的低密度引起的,这允许在已经存在的气泡的中心形成初期的尖峰。还考虑了多种固体气体密度比。结果表明,界面的运动渐近收敛于实心真空情况。当考虑到较高的气体初始密度时,界面扰动的增长率会降低,并且在某些情况下,由于流体由于具有较高的可压缩性而变得比固体更稠密,因此其符号可能会反转。最后,研究了驱动冲击的马赫数和屈服应力对混合区的影响。我们发现,再冲击后产生的混合区域的宽度与入射冲击的强度成比例地增加。固体材料中增加的屈服应力使界面不易由于剪切波将涡旋带离界面而变得不稳定,并限制了再电击后较小长度尺度的产生。

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