Coarsening Dynamics in the Vicsek Model of Active Matter

preprint2019arXivOpen access

Abstract

We study the flocking model introduced by Vicsek in the "coarsening" regime. At standard self-propulsion speeds, we find two distinct growth laws for the coupled density and velocity fields. The characteristic length scale of the density domains grows as Lρ(t)∼tθρL_ρ(t) \sim t^{θ_ρ} (with θρ≃0.25θ_ρ\simeq 0.25), while the velocity length scale grows much faster, viz.viz., Lv(t)∼tθvL_{v}(t) \sim t^{θ_v} (with θv≃0.83θ_v \simeq 0.83). The spatial fluctuations in the density and velocity fields are studied by calculating the two-point correlation function and the structure factor, which show deviations from the well-known Porod's law. This is a natural consequence of scattering from irregular morphologies that dynamically arise in the system. At large values of the scaled wave-vector, the scaled structure factors for the density and velocity fields decay with powers −2.6-2.6 and −1.52-1.52, respectively.

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