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Hydrodynamic equations for self-propelled particles:microscopic derivation and stability analysis

机译:自推进颗粒的流体动力学方程:微观推导和稳定性分析

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Considering a gas of self-propelled particles with binary interactions, we derivethe hydrodynamic equations governing the density and velocity fields from themicroscopic dynamics, in the framework of the associated Boltzmann equation.Explicit expressions for the transport coefficients are given, as a function of themicroscopic parameters of the model. We show that the homogeneous statewith zero hydrodynamic velocity is unstable above a critical density (whichdepends on the microscopic parameters), signalling the onset of a collectivemotion. Comparison with numerical simulations on a standard model of self-propelled particles shows that the phase diagram we obtain is robust, in thesense that it depends only slightly on the precise definition of the model. Whilethe homogeneous flow is found to be stable far from the transition line, itbecomes unstable with respect to finite-wavelength perturbations close to thetransition, implying a non-trivial spatio-temporal structure for the resultingflow. We find solitary wave solutions of the hydrodynamic equations, quitesimilar to the stripes reported in direct numerical simulations of self-propelledparticles.
机译:考虑到具有二元相互作用的自推进颗粒气体,我们在相关的Boltzmann方程的框架内从微观动力学推导了控制密度场和速度场的流体动力学方程式,并根据微观参数给出了输运系数的明确表达式。模型的我们表明,在临界密度以上(取决于微观参数),流体动力学速度为零的均匀状态是不稳定的,这标志着集体运动的开始。与自推进颗粒的标准模型上的数值模拟进行比较表明,我们获得的相图是稳健的,因为它仅在很小程度上取决于模型的精确定义。虽然均质流在远离过渡线的地方很稳定,但对于靠近过渡的有限波长扰动来说却变得不稳定,这意味着所得流具有非平凡的时空结构。我们发现了流体动力学方程的孤立波解,这与自推进粒子的直接数值模拟中报告的条纹非常相似。

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