Collective behaviour of active colloids

cosmos 24th November 2017 at 4:39pm
Active colloid

See Active colloid, Self-diffusiophoresis, Self-propelled particle. See also Collective hydrodynamics of active entities, Self-assembly of active colloids

City of microbes!

Recent review: Emergent behavior in active colloids

Dynamic self-organization of motile components can be observed in a wide range of length scales, from bird flocks (ref) to bacterial colonies (ref, ref) and assemblies of motor and structural proteins (ref). The fascination with these phenomena has naturally inspired researchers to use a physical under-standing of motility to engineer complex emergent behaviors in model systems that promise revolutionary advances in technological applications if combined with other novel biomimetic functions, such as signal processing and decision making (see Swarm robotics), or replication (see Self-replication of information-bearing nanoscale patterns).

Biological components pose inevitable limitations on this task, while chemical [ 14 ], mechanical [ 15 ], or externally actuated [ 16 ] imitations appear more promising

Individual and collective behavior of artificial swimmers: "Janus particles"

Transport and Collective Dynamics in Suspensions of Confined Swimming Particles

Emergent, Collective Oscillations of Self-Mobile Particles and Patterned Surfaces under Redox Conditions

Emergent Cometlike Swarming of Optically Driven Thermally Active Colloids

Collective behaviour of thermally active colloids. This model doesn't consider the dependence of the interaction on the relative orientation of the colloids. This effect is incorporated in their later model described in the paper on chemotactic colloids, and on optically driven thermally active colloids

Clusters, asters, and collective oscillations in chemotactic colloids

Phoretic mechanisms of self-propelled colloids

Behaviour of a single chemotactic colloid in an external substrate concentration gradient

Theory of phoretic mechanisms of self-propelled colloids

Collective behaviour

FROM CHEMOTAXIS TO COLLECTIVE MOTION

Effective interactions of active colloids

They consider the former in the paper, and look at pairwise interactions.

Stochastic equations of motion

Constructing a Langevin equation using the drift terms derived in here, which depend on

note product gradient: gradient in product concentration. Extra terms were added because the coefficients Φ0,α0\Phi_0, \alpha_0, etc. only take an external ss gradient into account, and now we also have external pp gradients produced by the other catalytic colloids.

These equations can also be derived phenomenologically following from symmetry principles (see citations in paper), but one doesn't get expressions for the coefficients.

Concentration fields

The substrate and product fields (ss, and pp) are themselves determined by the distribution of colloid positions and orientations. The substrate is consumed and the product is generated at the rate

Q(r,t)=κ(s)αXαδ(rrαXα)σ(Xαn^)Q(\mathbf{r}, t) = \kappa(s) \sum_\alpha \int _{|\mathbf{X}_\alpha|} \delta (\mathbf{r} - \mathbf{r}_\alpha -\mathbf{X}_\alpha) \sigma(\mathbf{X}_\alpha \cdot \hat{\mathbf{n}})

Evolution equation of concentration fields is obtained depending on averaged colloid number density and orientation density. The steady state is the considered, and the Fourier transform is applied to obtain information on the length scale of the interaction, expressed in the screening length.

Saturated vs unsaturated regime. MM curve? Refers to Michaelis-Menten rule in Enzyme kinetics. Saturated and unstaturated regimes refer to regimes where κ(s)\kappa(s) (which has the MM form) is saturated vs unsaturated.

Colloid number density ρ\rho and orientation density w\mathbf{w} (averaged equations)

These are obtained from the Langevin equations above. For the orientational equations, the averaged equation involves higher moments, and a closure condition needs to be imposed to express them in terms of lower moments (mean field approximation). See Supplementary Material in paper.

The equations for ρ\rho and w\mathbf{w} depend on the gradients of ss and pp, while the equilibrium ss and pp fields depend on ρ\rho and w\mathbf{w}. The two equations can be combined to obtain closed equations for ss and pp with complicated effective interactions, which give rise to a rich diversity of possible phases, depending on the several parameters in the model. The main two regimes are:

Unsaturated

Saturated

Formation of asters (i.e. star-like formations, I think)...