Abstract
This paper proposes using the configurational temperature for quantifying how far an active-matter system is from thermal equilibrium. We measure this “distance” by the ratio of the systemic temperature to , where is the canonical-ensemble temperature for which the average potential energy is equal to that of the active-matter system. is “local” in the sense that it is the average of a function, which depends only on how the potential energy varies in the vicinity of a given configuration. In contrast, is a global quantity. The quantity is straightforward to evaluate in a computer simulation; equilibrium simulations in conjunction with a single steady-state active-matter configuration are enough to determine . We validate the suggestion that quantifies the deviation from thermal equilibrium by data for the radial distribution function of the 3D Kob-Andersen and 2D Yukawa active-matter models with active Ornstein-Uhlenbeck and active Brownian Particle dynamics. Moreover, we show that , structure, and dynamics of the homogeneous phase are all approximately invariant along the motility-induced phase separation boundary in the phase diagram of the 2D Yukawa model. The measure is not limited to active matter and can be used for quantifying how far any system involving a potential-energy function, e.g., a driven Hamiltonian system, is from thermal equilibrium.
- Received 17 December 2022
- Accepted 23 January 2023
DOI:https://doi.org/10.1103/PhysRevE.107.024610
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