Fluctuations, renormalizations, and a convective instability in driven wet active matter
arXiv:1801.06820 · doi:10.1103/PhysRevFluids.4.024306
Abstract
A scalar model of wet active matter in the presence of an imposed temperature gradient, or chemical potential gradient, is considered. It is shown that there is a convective instability driven by a (negative) activity parameter. In this non-equilibrium steady state the generic long-ranged correlations are computed and compared and contrasted with the analogous results in a passive fluid. In addition, the non-equilibrium Casimir pressure or force is computed. Singularities in various physical quantities as the instability is approached are determined. Finally, we give the generalized Lorenz equations characterizing the fluid behavior above the instability and contrast these equations to the Lorenz equations for the Rayleigh-Bernard instability in a passive fluid.
4 pages
References in corpus (6)
- Spontaneous motion in hierarchically assembled active matter
- Direct measurement of the flow field around swimming microorganisms
- Entropy production in field theories without time reversal symmetry: Quantifying the non-equilibrium character of active matter
- Complex Spontaneous Flows and Concentration Banding in Active Polar Films
- Heat, temperature and Clausius inequality in a model for active brownian particles
- Contractile and chiral activities co-determine the helicity of swimming droplet trajectories
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