1998
DOI: 10.1103/physrevlett.80.4819
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Sound Waves and the Absence of Galilean Invariance in Flocks

Abstract: We study a model of flocking for a very large system ͑N 320 000͒ numerically. We find that in the long wavelength, long time limit, the fluctuations of the velocity and density fields are carried by propagating sound modes, whose dispersion and damping agree quantitatively with the predictions of our previous work using a continuum equation. We find that the sound velocity is anisotropic and characterized by its speed c for propagation perpendicular to the mean velocity ͗ y͘, ͗ y͘ itself, and a third velocity … Show more

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Cited by 136 publications
(257 citation statements)
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“…The analogy is as follows: the Hamiltonian tending to align the spins in the same direction in the case of equilibrium ferromagnets is replaced by the rule of aligning the direction of motion of particles, and the amplitude of the random perturbations can be considered proportional to the temperature for η ≪ 1. From a hydrodynamical point of view, in SPP systems the momentum of the particles is not conserved and -as was pointed out in [18] -the Galilean invariance is broken. Thus, the flow fields emerging in these models can considerably differ from the usual behavior of fluids.…”
Section: Discrete Modelsmentioning
confidence: 99%
“…The analogy is as follows: the Hamiltonian tending to align the spins in the same direction in the case of equilibrium ferromagnets is replaced by the rule of aligning the direction of motion of particles, and the amplitude of the random perturbations can be considered proportional to the temperature for η ≪ 1. From a hydrodynamical point of view, in SPP systems the momentum of the particles is not conserved and -as was pointed out in [18] -the Galilean invariance is broken. Thus, the flow fields emerging in these models can considerably differ from the usual behavior of fluids.…”
Section: Discrete Modelsmentioning
confidence: 99%
“…We therefore conclude that for tori fatter than ξ < ξ c = 5K 3 2K 2 (the last equality holding approximately when K 3 K 2 ), thresholdless active flow will definitely occur. If disclinations are not generated and the aforementioned conditions for the validity of the frozen director approximation hold, then the flow field should be approximately described by our result (15).…”
Section: B Chiral Symmetry Breaking and Flow In Toroidal Shellsmentioning
confidence: 99%
“…At the same time, the far-from-equilibrium nature of active matter leads to exotic phenomena of fundamental interest. Among these are the ability of active fluids to (i) spontaneously break a continuous symmetry in two spatial dimensions [14][15][16][17], (ii) exhibit spontaneous steady-state flow [2,18] in the absence of an external driving force, and (iii) support topologically protected excitations (e.g., sound modes) that originate from time-reversal symmetry breaking [19].…”
Section: Introductionmentioning
confidence: 99%
“…III B, we examine its excitations. Even though our system is overdamped because of the presence of a substrate, the ordered polar flock supports long-wavelength propagating sound modes [42]. The presence of curvature introduces an additional length scale in the problem and gaps the sound spectrum at long wavelengths.…”
Section: Introductionmentioning
confidence: 99%