Kinetic theory of chiral active disks: Odd transport and torque density

R Raphaël Maire (Department of Condensed Matter, University of Barcelona 1 , 08028 Barcelona,) A Alessandro Petrini (Sapienza University of Rome 2 , IT-00185 Rome,) U Umberto Marini Bettolo Marconi (Department of Physics, University of Camerino) L Lorenzo Caprini (Department of Physics, University of Rome La Sapienza)

Abstract

Parity-odd transport is a central signature of chiral fluids, yet analytical predictions are sparse. Here, we introduce a minimal two-dimensional hard-disk gas in which chirality arises solely from a collision-induced transverse impulse. Motivated by granular spinners, collisions are dissipative and inject orbital angular momentum through a fixed tangential “kick” at contact. Starting from a Boltzmann–Enskog description, we derive nonlinear hydrodynamic equations for density, momentum, and temperature and show that chirality generates an antisymmetric homogeneous stress corresponding to a nonzero torque density. In the dilute limit, a Chapman–Enskog expansion yields analytical predictions for transport coefficients, including odd viscosity, odd thermal conductivity, and odd self-diffusivity, in good agreement with numerical simulations. This minimal kinetic model can serve as a foundation for systematic coarse-graining of chiral fluids and as a tractable benchmark for gaining insight into odd transport across a broader class of chiral systems.

Article Details

Volume / Issue Vol. 165, Issue 3
Published July 21, 2026
ISSN 0021-9606
Publisher American Institute of Physics

Journal Info

The Journal of Chemical Physics

American Institute of Physics

ISSN: 0021-9606 Physical Sciences

Authors (4)

R

Raphaël Maire

Department of Condensed Matter, University of Barcelona 1 , 08028 Barcelona,

A

Alessandro Petrini

Sapienza University of Rome 2 , IT-00185 Rome,

U

Umberto Marini Bettolo Marconi

Department of Physics, University of Camerino

L

Lorenzo Caprini

Department of Physics, University of Rome La Sapienza