Pressure and Phase Equilibria in Interacting Active Brownian Spheres
arXiv:1412.5475 · doi:10.1103/PhysRevLett.114.198301
Abstract
We derive from first principles the mechanical pressure , defined as the force per unit area on a bounding wall, in a system of spherical, overdamped, active Brownian particles at density . Our exact result relates , in closed form, to bulk correlators and shows that (i) is a state function, independent of the particle-wall interaction; (ii) interactions contribute two terms to , one encoding the slow-down that drives motility-induced phase separation, and the other a direct contribution well known for passive systems; (iii) is equal in coexisting phases. We discuss the consequences of these results for the motility-induced phase separation of active Brownian particles, and show that the densities at coexistence do not satisfy a Maxwell construction on .
6p (main text) + 4p (SI)
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