由粘性无摩擦球组成的多孔尘埃聚集体碰撞增长的阈值速度
Threshold velocity for collisional growth of porous dust aggregates consisting of cohesive frictionless spheres
摘要：
了解尘埃聚集体的碰撞结果以及对组成粒子的材料性质的依赖性对于理解行星形成具有重要意义。最近的数值模拟表明，颗粒间的切向摩擦起着至关重要的作用，在能量耗散在多孔尘埃聚集体之间的碰撞过程中，然而，尘埃聚集体的碰撞增长的摩擦的重要性仍然知之甚少。在这里，我们展示了颗粒间切向摩擦的尘埃聚集体的碰撞增长的影响。我们进行了数值模拟等质量的多孔尘埃聚集体之间的碰撞组成的粘性和无摩擦的球体。系统地改变了碰撞速度和碰撞角度，计算了碰撞生长效率随碰撞速度的变化。我们发现，碰撞增长的阈值速度降低时，尘埃聚集体的摩擦球相比，无摩擦的球体。我们的研究结果突出了切向相互作用对尘埃聚集体碰撞行为的重要性，并指出，阈值速度的预测方程应重建。
英文摘要：
Understanding the collisional outcomes of dust aggregates and dependence on material properties of the constituting particles is of great importance toward understanding planet formation. Recent numerical simulations have revealed that interparticle tangential friction plays a crucial role in energy dissipation during collisions between porous dust aggregates; however, the importance of friction on the collisional growth of dust aggregates remains poorly understood. Here we demonstrate the effects of interparticle tangential friction on the collisional growth of dust aggregates. We performed numerical simulations of collisions between equal-mass porous dust aggregates consisting of cohesive and frictionless spheres. We changed the collision velocity and impact angle systematically and calculated the collisional growth efficiency as a function of the collision velocity. We found that the threshold velocity for collisional growth decreases when dust aggregates are made of frictionless spheres as compared to frictional spheres. Our results highlight the importance of tangential interactions on the collisional behavior of dust aggregates and indicate that the predictive equation for threshold velocity should be reconstructed.
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