4.6 Article

Confined active Brownian particles: theoretical description of propulsion-induced accumulation

Journal

NEW JOURNAL OF PHYSICS
Volume 20, Issue -, Pages -

Publisher

IOP Publishing Ltd
DOI: 10.1088/1367-2630/aa9d4b

Keywords

active matter; active Brownian particle; microswimmer; confinement; trapping

Funding

  1. Deutsche Forschungsgemeinschaft (DFG) [SPP 1726]

Ask authors/readers for more resources

The stationary-state distribution function of confined active Brownian particles (ABPs) is analyzed by computer simulations and analytical calculations. We consider a radial harmonic as well as an anharmonic confinement potential. In the simulations, the ABP is propelled with a prescribed velocity along a body-fixed direction, which is changing in a diffusive manner. For the analytical approach, the Cartesian components of the propulsion velocity are assumed to change independently; active Ornstein-Uhlenbeck particle (AOUP). This results in very different velocity distribution functions. The analytical solution of the Fokker-Planck equation for an AOUP in a harmonic potential is presented and a conditional distribution function is provided for the radial particle distribution at a given magnitude of the propulsion velocity. This conditional probability distribution facilitates the description of the coupling of the spatial coordinate and propulsion, which yields activity-induced accumulation of particles. For the anharmonic potential, a probability distribution function is derived within the unified colored noise approximation. The comparison of the simulation results with theoretical predictions yields good agreement for large rotational diffusion coefficients, e.g. due to tumbling, even for large propulsion velocities (Peclet numbers). However, we find significant deviations already for moderate Peclet number, when the rotational diffusion coefficient is on the order of the thermal one.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.6
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available