J.
Bleibel
*ae,
A.
Domínguez
b,
F.
Günther
c,
J.
Harting
cd and
M.
Oettel
e
aMax-Planck-Institut für Intelligente Systeme, Heisenbergstr. 3, 70569 Stuttgart, Germany. E-mail: bleibel@is.mpg.de
bFísica Teórica, Universidad de Sevilla, Apdo. 1065, 41080 Sevilla, Spain. E-mail: dominguez@us.es
cFakulteit Technische Natuurkunde, Technische Universiteit Eindhoven, Den Dolech 2, 5600MB Eindhoven, The Netherlands
dInstitut für Computerphysik, Universität Stuttgart, Allmandring 3, 70569 Stuttgart, Germany
eInstitut für Angewandte Physik, Universität Tübingen, Auf der Morgenstelle 10, 72076 Tübingen, Germany
First published on 17th February 2014
Under partial confinement, the motion of colloidal particles is restricted to a plane or a line but their dynamics is influenced by hydrodynamic interactions mediated by the unconfined, three-dimensional flow of the embedding fluid. We demonstrate that this dimensionality mismatch induces a characteristic divergence in the collective diffusion coefficient of the colloidal subsystem. This result, independent of the specific interparticle forces in the colloid, is solely due to the kinematical constraint on the colloidal particles, and it is different from the known divergence of transport coefficients in purely one or two-dimensional fluids.
![]() | (1) |
The dynamics of colloidal solutions in confinement or near physical boundaries has also been of long-standing interest. The effect of HI has been investigated theoretically on systems confined between walls,7–9 close to a free interface,10,11 or on solutions with a matrix of fixed obstacles.12 Trapped objects in (fluid) membranes also show peculiar diffusion behavior.13,14 In this communication, we investigate the generic case of partial confinement: one part of the system, namely the colloidal particles, is restricted to move in one or two dimensions, whereas the other part, namely the embedding solvent, evolves in a (essentially unbound) three-dimensional (3D) domain. Examples of experimental realizations of such a partial confinement setup are numerous, e.g., a colloidal monolayer at a fluid interface,15 or particles restricted by optical tweezers to stay in a plane or a line.16 Here we study this problem both theoretically with a simplified model and numerically with simulations of a more complete model. The main result is that the HI induce anomalous fast diffusion.
![]() | (2) |
The particles are acted upon by a thermodynamic generalized force, e.g., Brownian or due to direct particle–particle interactions, and simultaneously transported by the ambient flow in the surrounding 3D fluid. Thus, in the overdamped limit we approximate
v = Γf + u, | (3) |
![]() | (4) |
Notice that is the Oseen tensor for the 3D flow, even though only its evaluation at points of the monolayer plane (z = z′ = 0) is required. The mean-field-like approximations underlying eqn (2)–(4) usually imply a restriction to the “macroscopic” regime of large scales and long times (see ESI, Section 1†).
In the absence of external force fields, the homogeneous, stationary state, ρ(r,t) = ρhom, f(r,t) = 0, u(r,t) = 0, is a possible solution of eqn (2)–(4). By linearizing them about the homogeneous state, one obtains an equation for the evolution of the perturbation δρ(r,t) = ρ(r,t) − ρhom,
![]() | (5) |
In this linear approximation, f can be approximated as a linear functional of ∇δρ in general, so that the first term describes the decay (or growth, in cases of instability) of density fluctuations driven by the force field. The second term accounts for the effect of HI and the key point is to note that ∇ · u ≠ 0 in the 2D layer, that is, the ambient flow at the plane z = 0 induces compression and dilution of the colloidal fluid, although the full 3D ambient flow is not compressible. This is at variance with the phenomenology when ∇ · u = 0 (absence of confinement or full confinement to 2D), under which conditions the effect of the HI appears only as a nonlinear coupling (advection). By introducing the 2D Fourier transform of the fields, eqn (5) can be cast into the form of eqn (1) with D(k) = [1 + g(k)]D0(k) (see ESI, Section 2†). Here D0(k), defined from fk ≈ [D0(k)/Γρhom](−ikδρk), is the diffusion coefficient in the absence of hydrodynamic couplings, the latter being accounted for by the function
![]() | (6) |
The anomalous diffusion is illustrated by means of two physically relevant models lying at opposite extremes. The first case is an ideal gas (no direct interparticle force), for which f = −kBT∇ lnρ and D0(k) = ΓkBT. The Green function G(r,t) of eqn (1) is (see ESI, Section 3†)
![]() | (7) |
The second case is a system of colloidal particles trapped by wetting forces at the interface between two fluids. They deform the interface slightly and an effective mutual interaction of capillary origin arises (see, e.g., ref. 17). In the simplest model (two-body force between capillary monopoles), the pairwise, attractive interaction potential is proportional to the Bessel function K0(r/λ), dependent on the capillary length λ. When λ → ∞, this reduces to the Newtonian gravitational potential in 2D. For realistic configurations (λ ∼ mm, typical particle size ∼ μm), the attraction is extremely long-ranged and one can use the mean-field approximation to compute the force f and derive (see ESI, Section 4†)
![]() | (8) |
Here, is a characteristic time scale and
−1 is a characteristic length scale. Eqn (8) predicts a clustering instability dominated by the large scales (D0(k) < 0 if k <
) provided λ
> 1. For these modes, HI-induced faster evolution is predicted too because, regarding the ambient flow, one can dismiss the tiny interfacial deformation, so that the Oseen tensor in the monolayer plane (see eqn (4)) holds either asymptotically for large separations, or exactly in the absence of a viscosity contrast at the fluid interface.19
(i) HI-enhanced diffusion coefficient in capillary collapse: we check the linear prediction ρk(t) ∝ exp (−D(k)k2t) from eqn (1) for capillary monopoles using tSD simulations. As Fig. 1 illustrates, simulation results are described very well by theory and clearly show the enhancement due to the 1/k divergence of the diffusion coefficient compared with the corresponding results without HI. (The deviations at large values of k/ are due to nonlinear effects, and to corrections to mean-field from the short-range repulsion.)
![]() | ||
Fig. 1 Growth of ρk(t) from tSD simulations (symbols) and from linear theory, eqn (1) and (8) (thick lines; thin lines in the absence of HI). See ESI, Section 5.3.† |
(ii) Speedup of nonlinear capillary collapse: a particularly simple limit case of the instability corresponds to , λ → ∞ in eqn (8) (dubbed “cold collapse” in 2D Newtonian gravity), allowing for an exact solution of the nonlinear evolution equations in the absence of HI:18 an initially homogeneous circular patch of particles (top-hat profile) remains top-hat during the evolution towards the simultaneous collapse of all the particles at the center at a time t =
. Fig. 2 addresses the effect of HI on this solution by means of tSD and LB simulations: due to the faster dynamics of the low-k modes induced by HI, the collapse occurs earlier and the top-hat profile is destroyed, with a faster increase of density at the center (clearly seen at time t/
= 0.5), until close-packing effects become important (at t/
= 0.8) and halt the collapse. The agreement between the results from tSD and LB is reassuring that the phenomenological effect by HI is captured already by the Oseen approximation. When the capillary attraction is screened (λ < initial patch radius), the collapse develops a shockwave-like feature at the outer rim.22 As illustrated by Fig. 3, the incorporation of HI does not alter this qualitative spatial structure but the faster time evolution towards the collapse is very prominent.
![]() | ||
Fig. 2 Collapse of an initial top-hat profile (radius R, density ρ0, see ESI, Section 5.3†) for 2D gravity (λ → ∞) without (dashed line, from theory) and with HI (symbols, from tSD and LB simulations). |
![]() | ||
Fig. 3 Same as Fig. 2 but for a larger system (see ESI, Section 5.3†) and screened capillary attraction (λ < ∞) without (open symbols, from BD simulations) and with HI (filled symbols, from tSD simulations). |
(iii) Anomalous diffusion in an ideal gas: we have considered an initial top-hat profile immersed in a homogeneous background. Despite the absence of (static) interactions, the evolution is affected by the HI if a nonvanishing hydrodynamic radius rH of the particles is assumed. This corresponds to the idealized case of, e.g., mutually interpenetrable polymeric particles whose radius of gyration defines rH. Fig. 4 shows the effect of HI by means of simulations and the numerical solution of eqn (2)–(4). One can observe how the HI reduce the diffusion time and induce the development of a tail consistent with the r−3 decay predicted by eqn (7).
![]() | ||
Fig. 4 Diffusion of a top-hat overdensity of ideal gas without (filled symbols, from BD simulations) and with HI (open symbols, from tSD simulations). Lines represent the numerical solution of eqn (2)–(4). For simulation parameters, see ESI, Section 5.3.† |
In conclusion, under partial confinement, i.e., colloidal motion restricted to a plane or a line but with hydrodynamic interactions originating from 3D flow of a surrounding fluid, peculiar collective diffusion properties emerge. Using a mean-field model, we have identified a singularity in the collective long-time diffusion coefficient responsible for anomalous diffusion. The dominating dynamical effect of this singularity has been illustrated by simulation examples of an ideal gas (dilute limit) and a monolayer of capillary monopoles at a fluid interface (long-ranged interparticle attraction) obtained with effectively 2D Stokesian dynamics truncated at the two-body level and with 3D Lattice-Boltzmann/Molecular Dynamics simulations.
Footnotes |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c3sm53043d |
‡ “Short-time” meaning a time much shorter than the diffusion time over a distance of the order of the mean interparticle separation. |
This journal is © The Royal Society of Chemistry 2014 |