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 (). The ordering-transition RG gets the dynamic exponent right () but the static exponents wrong ( vs. observed ), 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 that binds the swarm (standing in for the marker) — with alignment noise and confinement as control parameters. The HCVM has a scale-free-chaos phase transition: chaotic dynamics (positive Lyapunov exponent) with scale-free correlations (). Crucially, for finite this is not a point but an extended critical region bounded by three scale-free lines on the plane — the onset-of-chaos line (zero largest Lyapunov exponent), the single-to-multicluster line , and the maximal-Lyapunov line — all collapsing onto the axis at the same rate as .
Power laws, and a bridge to the observable
As the critical lines obey
with , , . Because the exponents drop out of the noise dependence, and can be estimated at a fixed (you cannot grow the insect count at will) — giving , . And the unmeasurable confinement 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 — 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 , , along and ). Applying the same fitting procedures used on real swarms, the mixture reproduces:
- the static exponents (, vs. observed , );
- the dynamic exponent (mixture: , vs. observed , — noting LS underestimates ; on a single line );
- 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.