Modeling chiral active particles: from circular motion to odd interactions
Lorenzo Caprini, Alessandro Petrini, Umberto Marini Bettolo Marconi
TL;DR
The paper addresses how chiral active particles, which exhibit circular trajectories, generate non-conservative odd (transverse) interactions that break mirror symmetry. It develops microscopic models spanning circular self-propelled motion, coarse-grained transverse forces, and granular spinner-based odd interactions, showing how inertia and chirality cooperate to produce a novel BIO (bubbles induced by odd interactions) phase—an inhomogeneous state with particle-free bubbles and edge currents. The work derives both numerical phase diagrams and analytical insights, including an instability condition $m C_0 = \beta_1 \tau_I^2 C_1^2$ and a critical scaling $\omega_c^2 \sim m\epsilon/(\tau_I^2 \sigma^2)$, revealing how increasing inertia lowers the threshold chirality for BIO. Spatial velocity correlations show a finite-$q^*$ signature and oscillatory real-space behavior, supporting a non-equilibrium phase transition separate from classical MIPS. Overall, the BIO phase uncovers a new class of collective behavior in chiral active matter driven by odd interactions, with open questions about a full hydrodynamic or kinetic description and potential experimental realizations.
Abstract
In this paper, we discuss microscopic models for chiral active particles, i.e., rotating active units that exhibit circular or spinning motion. While non-chiral active particles are typically governed by self-propulsion and conservative interactions, the rotating motion of chiral particles generates additional non-conservative forces that cannot be derived from a potential. These manifest as effective transverse forces, acting perpendicular to the line connecting the centres of two interacting particles, and are referred to as odd interactions, because they break the mirror symmetry of the system. Here, we demonstrate that odd interactions arise from a limiting case of a well-established model describing spinning granular objects. In addition, we show that these models for chiral active objects give rise to a novel collective phenomenon that emerges uniquely from transverse forces and, hence, chirality. Specifically, the system undergoes a transition from a homogeneous phase to an inhomogeneous one characterised by regions depleted of particles, referred to as bubbles. This collective behaviour, termed BIO (bubbles induced by odd interactions), is a general emergent phenomenon arising from chirality and odd interactions. In this work, we review theoretical approaches to this problem, including a scaling argument and predictions for spatial velocity correlations that account for the BIO phase. Finally, we outline perspectives and open challenges concerning this collective phenomenon.
