Bulletin of the American Physical Society
2024 APS March Meeting
Monday–Friday, March 4–8, 2024; Minneapolis & Virtual
Session T31: Phase Separation in Active Matter
11:30 AM–2:18 PM,
Thursday, March 7, 2024
Room: 102C
Sponsoring
Units:
GSNP DSOFT
Chair: Daphne Klotsa, UNC Chapel Hill; Corey O'Hern, Yale University
Abstract: T31.00009 : Thermodynamically consistent lattice Monte Carlo simulation for active particle system
1:30 PM–1:42 PM
Presenter:
Ki-Won Kim
(Seoul National University)
Authors:
Ki-Won Kim
(Seoul National University)
Euijoon Kwon
(Seoul National University)
Yongjoo Baek
(Seoul National University)
Collaboration:
Seoul National University
Lattice-based Monte Carlo methods provide efficient means of computing the universal scaling properties of many-particle systems. For equilibrium systems, there are well-established Monte Carlo methods based on the ensemble theories. In contrast, for active particles, the lack of ensemble theories means that one must rely on the kinetic Monte Carlo (KMC) methods that properly discretize the dynamics in space and time so that the continuum description is restored in an appropriate limit. A recently proposed KMC method achieves this goal by probabilistically mixing ‘passive’ steps with active ones.
However, the method focuses only on the kinetics of the system, completely ignoring its energetics. If one is also interested in calculating the thermodynamic cost of maintaining a certain dissipative structure, a KMC method with well-defined energetics is needed.
In this study, we present a thermodynamically consistent lattice KMC algorithm describing both kinetics and energetics of active particles. Towards this purpose, we construct a model of active lattice gas whose jump probability does not only satisfy the local detailed balance condition but also involves the prefactor which explicitly depends on the self-propulsion. The model correctly reproduces the continuum dynamics in the proper limit, all the while allowing us to quantify how far from equilibrium the system is by calculating the energy dissipation.
We demonstrate that the characteristic phenomena of active matter, such as motility-induced phase separation and current rectification are well reproduced by our model. Moreover, our method reveals which part of the system dissipates more energy as the active particles maintain a nonequilibrium structure.
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