Spectral insights into active matter: Exceptional Points and the Mathieu equation
Horst-Holger Boltz, Thomas Ihle
TL;DR
The paper explains the universal scaling observed in noisy, aligning active matter by mapping the free one-particle Fokker-Planck operator to the Mathieu equation with an imaginary parameter $q=2k\,\mathrm{Pe}$. Through perturbation theory and Mathieu-function theory, it identifies a cascade of exceptional points that governs the spectral structure, yielding exact exponents: in the small-$q$ limit, $\alpha_{\text{low}}=2$ and $\beta_{\text{low}}=1$; in the large-$q$ limit, $\alpha_{\text{high}}=1/2$ and $\beta_{\text{high}}=-1/8$, with a universal high-activity projection $\sim q^{-1/8}$. These spectral insights, extended to mean-field interactions, predict the scaling of the critical coupling $\Gamma_c \sim q^{\gamma}$ with symmetry-dependent exponents $\gamma$, capturing the two regimes observed in simulations for polar and higher-symmetry alignments. The work reveals a dynamical phase-transition-like mechanism rooted in non-Hermitian spectral topology, offering a rigorous foundation for non-equilibrium scaling laws in active matter and suggesting broad applicability to mode selection and density-order coupling. Overall, it connects perturbative analysis, exceptional-point cascades, and Mathieu-function asymptotics to provide exact, universal scaling predictions for noisy active systems.
Abstract
We show that recent numerical findings of universal scaling relations in systems of noisy, aligning self-propelled particles by Kürsten [Kürsten, arXiv:2402.18711v2 [cond-mat.soft] (2025)] can robustly be explained by perturbation theory and known results for the Mathieu equation with purely imaginary parameter. In particular, we highlight the significance of a cascade of exceptional points that leads to non-trivial fractional scaling exponents in the singular-perturbation limit of high activity. Crucially, these features are rooted in the Fokker-Planck operator corresponding to free self-propulsion. This can be viewed as a dynamical phase transition in the dynamics of noisy active matter.
