Flocking dynamics with voter-like interactions
We study the collective motion of a large set of self-propelled particles subject to voter-like interactions. Each particle moves on a two-dimensional space at a constant speed in a direction that is randomly assigned initially. Then, at every step of the dynamics, each particle adopts the direction...
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Published in | arXiv.org |
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Main Authors | , |
Format | Paper Journal Article |
Language | English |
Published |
Ithaca
Cornell University Library, arXiv.org
11.04.2019
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Subjects | |
Online Access | Get full text |
ISSN | 2331-8422 |
DOI | 10.48550/arxiv.1608.08231 |
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Summary: | We study the collective motion of a large set of self-propelled particles subject to voter-like interactions. Each particle moves on a two-dimensional space at a constant speed in a direction that is randomly assigned initially. Then, at every step of the dynamics, each particle adopts the direction of motion of a randomly chosen neighboring particle. We investigate the time evolution of the global alignment of particles measured by the order parameter \(\varphi\), until complete order \(\varphi=1.0\) is reached (polar consensus). We find that \(\varphi\) increases as \(t^{1/2}\) for short times and approaches exponentially fast to \(1.0\) for long times. Also, the mean time to consensus \(\tau\) varies non-monotonically with the density of particles \(\rho\), reaching a minimum at some intermediate density \(\rho_{\tiny \mbox{min}}\). At \(\rho_{\tiny \mbox{min}}\), the mean consensus time scales with the system size \(N\) as \(\tau_{\tiny \mbox{min}} \sim N^{0.765}\), and thus the consensus is faster than in the case of all-to-all interactions (large \(\rho\)) where \(\tau=2N\). We show that the fast consensus, also observed at intermediate and high densities, is a consequence of the segregation of the system into clusters of equally-oriented particles which breaks the balance of transitions between directional states in well mixed systems. |
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Bibliography: | SourceType-Working Papers-1 ObjectType-Working Paper/Pre-Print-1 content type line 50 |
ISSN: | 2331-8422 |
DOI: | 10.48550/arxiv.1608.08231 |