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An extended critical region in swarms

The puzzle

Natural midge swarms show power laws (correlation length ∝ flock size, susceptibility, correlation time) and strong scale-free correlations — signatures of near-criticality — yet three facts sit awkwardly with the usual explanation (an ordering transition, à la Cavagna): swarms live in the disordered phase (low polarization), they form around markers on the ground (so they are not translation-invariant), and their dynamic scaling is imperfect — the normalized dynamic correlation function (NDCCF) collapses onto one curve only for short rescaled times (0<t/ξz<40 < t/\xi^z < 4). The ordering-transition RG gets the dynamic exponent right (z1.35z\approx1.35) but the static exponents wrong (ν0.75,γ1.17\nu\approx0.75,\gamma\approx1.17 vs. observed ν0.35,γ0.9\nu\approx0.35,\gamma\approx0.9), predicts a full NDCCF collapse, and can’t produce the marker/shape phenomenology. This paper offers a different mechanism.

The model: a scale-free-chaos transition

They use the harmonically confined Vicsek model (HCVM) — 3D Vicsek alignment plus a linear spring β\beta that binds the swarm (standing in for the marker) — with alignment noise η\eta and confinement β\beta as control parameters. The HCVM has a scale-free-chaos phase transition: chaotic dynamics (positive Lyapunov exponent) with scale-free correlations (ξN1/3\xi \sim N^{1/3}). Crucially, for finite NN this is not a point but an extended critical region bounded by three scale-free lines on the (η,β)(\eta,\beta) plane — the onset-of-chaos line β0\beta_0 (zero largest Lyapunov exponent), the single-to-multicluster line βc\beta_c, and the maximal-Lyapunov line βi\beta_i — all collapsing onto the β=0\beta=0 axis at the same rate as NN\to\infty.

Power laws, and a bridge to the observable

As η0\eta\to0 the critical lines obey

βj(N;η)=CjN1/(3ν)ηmj,j=0,c,\beta_j(N;\eta) = C_j\, N^{-1/(3\nu)}\,\eta^{m_j}, \qquad j=0,c,

with ξβν\xi\sim\beta^{-\nu}, χβγ\chi\sim\beta^{-\gamma}, τξz\tau\sim\xi^z. Because the exponents drop out of the noise dependence, ν\nu and γ\gamma can be estimated at a fixed NN (you cannot grow the insect count at will) — giving ν0.43\nu\approx0.43, γ0.92\gamma\approx0.92. And the unmeasurable confinement β\beta is found to be proportional to the perception range (the mean nearest-neighbour distance), the same observable control parameter used in the Attanasi–Cavagna finite-size analysis — so the laws can be written in measurable terms.

The key move: mixtures of data

Real swarm data are pooled across different times, atmospheric conditions, species, and NN — so they do not sit at a single control-parameter value. The authors model this as a mixture of simulation data over the extended critical region (varying NN, η\eta, β\beta along β0\beta_0 and βc\beta_c). Applying the same fitting procedures used on real swarms, the mixture reproduces:

  • the static exponents (ν0.43\nu\approx0.43, γ0.92\gamma\approx0.92 vs. observed 0.350.35, 0.90.9);
  • the dynamic exponent (mixture: zLS1.15z_{\text{LS}}\approx1.15, zRMA1.33z_{\text{RMA}}\approx1.33 vs. observed 1.161.16, 1.371.37 — noting LS underestimates zz; on a single line z1z\approx1);
  • the imperfect NDCCF collapse over only a finite time interval — a signature that several timescales are in play near the scale-free-chaos transition (an ordering transition has one timescale → full collapse);
  • the observed swarm shape (a condensed core in an “insect vapour”).

The upshot

The ordering transition between homogeneous, translation-invariant phases does not belong to the universality class of insect swarms; the scale-free-chaos transition — with confinement/markers, chaos, an extended critical region, and multiple timescales — matches both the exponents and the qualitative features. The broader twist for the criticality debate: when a system’s control parameter is unmeasurable or varies across observations, apparent power laws may reflect a mixture over an extended critical region rather than fine-tuning to a single critical point (a cousin of Griffiths-phase / generic scale-invariance ideas).

References

González-Albaladejo & Bonilla (2024), arXiv:2309.05064 · González-Albaladejo, Carpio & Bonilla (2023), Phys. Rev. E 107, 014209 · González-Albaladejo & Bonilla (2023), Phys. Rev. E 107, L062601 · Attanasi et al. (2014), Phys. Rev. Lett. 113, 238102 · Cavagna et al. (2017), Nat. Phys. 13, 914 · Cavagna et al. (2023), Nat. Phys. 19, 1043 · Vicsek et al. (1995), Phys. Rev. Lett. 75, 1226 · Cavagna, Giardina & Grigera (2018), Phys. Rep. 728, 1 · Mora & Bialek (2011), J. Stat. Phys. 144, 268.