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Computational Dispersion Rheology, Faculty of Science and Technology, University of Twente, 7500 AE Enschede, The Netherlands
Correspondence: Address reprint requests to W. K. den Otter, Faculty of Science and Technology, University of Twente, PO Box 217, 7500 AE Enschede, The Netherlands. E-mail: w.k.denotter{at}utwente.nl.
| ABSTRACT |
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| INTRODUCTION |
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A flat or weakly undulating bilayer oriented parallel to the xy plane (see Fig. 1) can be exposed to two distinct flow deformations, as illustrated in Fig. 2. The first flow field,
describes the linear velocity profile of a regular shear flow with a shear rate
Following the convention in the literature on sheared block copolymers (16
), this flow is referred to as a perpendicular shear flow. The resistance of the bilayer against this flow is characterized by a two-dimensional surface viscosity,
s, which, analogous to the regular three-dimensional viscosity, relates the shear force per unit of length of bilayer to the shear rate. Note that both leaflets of the bilayer move in unison under this field. In the so-called parallel flow field,
on the other hand, the two monolayers of the bilayer are sliding past one another as two flat rigid objects with velocities
A friction coefficient,
, is defined by the ratio between the sliding force per unit of bilayer area and the velocity difference between the two leaflets.
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Viscosity measurements by pulling a tether from a vesicle, for instance, are hampered by the above effects. It proves more convenient, therefore, to deduce the viscosity from the translational and rotational diffusion coefficients of fluorescent transmembrane tracer particles in a quiescent bilayer (see Waugh (14
) and references cited therein) using a Stokes-Einstein type expression derived for this particular system by Saffman (17
). Saffman elegantly solved Stokes' equations of the creeping flow around a cylinder (i.e., the tracer) moving in a thin sheet of viscous liquid (i.e., the bilayer), by emphasizing the role played by the liquid, of viscosity
w, on either side of this sheet. Falling ball viscosimetry (18
), in which a microsphere moving under gravity is constrained to a bilayer vesicle, is essentially based on the same theory. An independent validation of the Saffman-Einstein expression for use with bilayers is therefore welcomed.
Friction coefficients have been measured by pulling a thin tether from a vesicle (10
12
,15
), where the sharp change in curvature at the vesicle-tether junction induces a velocity difference between the inner and outer layers. A second method focuses on the slip occurring when amphiphiles flow through an hourglass-shaped fusion pore from a bilayer under low surface tension to a bilayer under a higher tension (19
). The wide range of the few reported friction coefficients illustrates the complexity of (the interpretation of) these ingenious measurements, and the sensitivity to the amphiphiles used in the experiment.
The objective of this article is to establish methods to determine both the shear viscosity and the friction coefficient of a bilayer by means of computer simulations on the molecular level. Bilayers have been the subject of numerous modeling studies, which for the most part focused on the equilibrium properties and on the self-assembly from a disordered amphiphilic solution (20
25
). To the best of our knowledge, the flow behavior of a bilayer has never been simulated at this level. Because our aim here is to develop and validate new techniques, we opted for a relatively simple and fast coarse-grained amphiphilic model known to reproduce realistic thermodynamic properties (26
30
). No claims are made to the applicability of the model to calculate realistic values of dynamical properties. Our aim is to develop methods and to test the applicability of the Saffman-Einstein equation. The model and other simulation details are summarized in the "Setup" section. Results are presented in the "Results" section, where we describe the response of the bilayer, and of the individual amphiphiles, to the applied flow fields. We end with a discussion of the applied methods, and a comparison with the available experimental data, in the "Discussion and Conclusions" section.
| SETUP |
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The simulation model we used was developed by Goetz and Lipowsky (27
,28
). They chose an amphiphilic architecture in which the head is represented by a single bead (h) and the tail is reduced to four beads (t) representing roughly three CH2 units each. The solvent consists of loose water beads (w), corresponding with two water molecules. Interactions between like particles, as well as the hydrophilic head-water interactions, are modeled by a Lennard-Jones potential,
LJ(r) = 4
[(r/
)12 (r/
)6], with
= 2 kJ/mol and
= 1/3 nm. The hydrophobic tail-water and tail-head interactions are modeled by a purely repulsive potential,
rep(r) =
[r/(1.05
)]9. The nonbonded forces are implemented in a shifted-force fashion, ensuring a smooth truncation of the energy and the force at the cut-off distance of 2.5
. The particles of the amphiphilic molecules are held together by harmonic bond potentials,
bond(l) = 5000
2(l
)2. An angle potential between every set of three consecutively bonded particles,
angle(
) = 2
[1 cos(
)], introduces a bending stiffness. There are no dihedral potentials. All particles have the same mass m of 36 a.u., and the number density is 2 particles per 3
3. In all our simulations the temperature T was 325 K, or 1.35
/kB with kB Boltzmann's constant, and was maintained by means of a Nosé-Hoover thermostat. The time step used in the Verlet leapfrog scheme was
/500, where
is the unit of time. Previous simulations with this CG model showed that its equilibrium area, elastic modulus, bending rigidity, and line tension coefficient compare favorably with experimental data (26
30
). All simulations were run using the DL_POLY_2.0 package (34
), tailored to the specifications of the problem.
Rectangular periodic simulation boxes were used, each having a square ground plane of sides L|| parallel to the bilayer and the xy plane, and a height L
perpendicular to these. Initial bilayer-solvent configurations were created by constructing two parallel square lattice layers of straight amphiphilic molecules, 1152 in total, with their heads pointing outward. The 10,800 solvent particles were placed at random in the box, taking care to avoid overlap with the bilayer and with previously inserted solvent particles. The boxes were then energy minimized for a limited number of steps, followed by equilibration runs at the desired temperature. A snapshot of the resulting bilayer box is shown in Fig. 1. On varying L|| it was found that at L|| = 34.9
the bilayer is in the tensionless state, in which the average pressures parallel and perpendicular to the bilayer are identical, to wit,
1.5
3 or 1.4 kbar. The structure factors S of the thermal undulations followed the theoretical prediction for the tensionless state, S(q)
q4, with q a wave vector commensurate with the box dimension L|| (1
,2
,27
). The box height of 20.4
allows the solvent enough freedom to reach an isotropic pressure in the middle between two periodic images of the bilayer (28
).
Simulations under shear rate
were run using Lees-Edwards boundary conditions (35
,36
), such that the flow was directed along the x axis, i.e., such that
For homogeneous solvent boxes the shear direction is of course irrelevant, but this is no longer the case for boxes with a bilayer. A perpendicular flow was generated such that
and a parallel flow such that
Analogous flow fields along the y axis produce identical results. The Nosé-Hoover thermostat (35
) was adapted for these shear conditions, by calculating the temperature from the velocity distribution relative to the local flow field and by rescaling only superficial velocities. In these calculations the flow fields were assumed to be given by appropriate linear expressions, although some runs yielded a distinctly nonlinear profile. Using the actual flow field in the thermostating routine did not significantly change the results. The structure factors S(q) of the thermal undulations of the bilayer still scaled as q4 under shear, suggesting that the flow does not induce any significant tension on the bilayer. After turning on the shear flow, the simulations were continued until all transient effects had died out and a steady laminar flow field had formed, before starting the production runs.
Three techniques were used to determine the overall shear viscosities of the simulated systems (35
). In the nonsheared runs, the viscosity
tot was calculated using the Green-Kubo relation
![]() | (1) |
ß is an off-diagonal (
ß) element of the pressure tensor, V is the volume of the box, and the angular brackets denote a canonical average. For a sheared system the viscosity is defined as the ratio between the total shear force per unit area and the shear rate,
![]() | (2) |
For systems containing a bilayer we use
= x and ß = y or z for the perpendicular and parallel shear flows, respectively. The third method is based on the realization that the rate of energy production,
by the shearing boundaries is easily calculated as the time derivative,
of the extended Hamiltonian of the system plus thermostat, to arrive at
![]() | (3) |
Notice that in the stationary state the energy of the system is constant and therefore
is equal to the rate of energy extraction from the system by the thermostat. A similar approach was recently proposed by Holian (37
). The conversion from total shear viscosities into the viscosity and friction coefficient of the bilayer will be discussed at the appropriate places in the next section.
| RESULTS |
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w of just over 1.0
1/2m1/2
2, virtually independent of the applied shear rate
ranging from zero to 0.2
1. This value translates into 1.3 x 104 Pa s, which amounts to about one-quarter of the experimental viscosity of 5 x 104 Pa s for water at this temperature. The diffusion coefficient of the solvent particles was found to be 0.1
2/
, or 1 x 108 m2/s, which is about four times larger than the experimental self-diffusion coefficient, 2.5 x 109 m2/s, of a water molecule at this temperature.
Using the same approaches, the viscosity of a homogeneous liquid of chains of five particles, t5, was found to be
b
2.1
1/2m1/2
2, twice the value obtained for the solvent, again independent of the shear rate. For comparison, the experimental viscosity of a comparable liquid of hydrocarbon chains, n-hexadecane, is about eight times higher (38
). These results indicate that the model is not well suited to aim for dynamical properties in quantitative agreement with experiments. Marrink et al. (24
), following Groot and Rabone (21
), addressed the spurious speedup of their coarse-grained model by introducing an ad hoc scaling factor of four to relate the elapsed simulation time to the real time. An alternative physically sound route to solve the dynamical discrepancy is to maintain the friction and random forces in the equations of motion of the coarse-grained particles. In case these forces grow large relative to the inertial forces, one is of course better off running Brownian dynamics.
Perpendicular shear
Of the two interesting shear directions of a box containing a bilayer, the perpendicularly sheared system will be discussed first. The total viscosity of the system has been calculated for the quiescent box, as well as for those with shear rates ranging from 0.001 to 0.1
1, to be
1.6
1/2m1/2
2 in each case. In the steady state, the velocity distribution of the amphiphilic particles closely follows a linear flow field. This suggests that the bilayer behaves like a regular sheared liquid (be it one in which the molecules are bound to a plane), which is a prerequisite for a well-defined bilayer surface viscosity. Analogous to Eq. 2, the surface viscosity is defined as the total shear force on the bilayer per unit of length, divided by the shear rate,
![]() | (4) |
![]() | (5) |
The last equation defines the shear force on the bilayer, Fbilayer, as the total shear force across the xz plane minus the contribution acting on the solvent, where hs
6.8
is the thickness of the bilayer. The shear viscosity of the bilayer was found to be
20
1/2m1/2
1, or 8.5 x 1013 Pa m s. Fig. 3 reveals a weak dependence of this value on the shear rate, with a reduction by
10% over the entire range covered.
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1.4
1/2m1/2
2, for shear rates ranging from 0.002 to 0.05
1. A similar value was obtained by applying the Green-Kubo relation to the quiescent box. As in the previous section, we now have to convert this number into a property of the bilayer.
Because of the orientation of the bilayer relative to the sheared boundaries, we expect a velocity profile like the one drawn in Fig. 4. The profile in the solvent will be linear, with a slope
different from the imposed shear rate
In the middle of the box the two leaflets of the monolayer are sliding past one another, like two flat solid objects, with velocities
giving rise to a friction force between the two leaflets. The friction coefficient of this motion follows from the shearing force F exerted on the top (bottom) monolayer, by the solvent above (below) the bilayer, according to
![]() | (6) |
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The actually calculated velocity profile (see Fig. 5) shows that the velocity gradient within the bilayer region is considerably smaller than in the solvent, but not zero. This is caused by a convolution of the idealized profile with the thermal undulations of the bilayer. Unfortunately, this renders direct estimates of
v from the velocity profiles highly inaccurate. The shear rate of the solvent at some distance from the bilayer, however, is not affected by these undulations. Under the assumption of stick boundary conditions at the bilayer-solvent interface, we can calculate the slip velocity from
![]() | (7) |
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Alternatively, one could look at the distances traveled by the amphiphilic particles, along the flow direction, over the course of a simulation. This distribution is shown in Fig. 6 for the head particles of the two monolayers, excluding a few that flipped from one monolayer to the other. Because of the covalent bonding, the distributions for the tail particles are virtually identical. From the location of the peak, divided by the length of the simulation, we again obtain
v. The numerical values obtained by both methods agree very well, implying stick boundary conditions at the two bilayer-solvent interfaces. Consequently, the force exerted on the top monolayer by the solvent above the bilayer can be calculated from the shear rate in the solvent,
Inserting these results in Eq. 6, we find a friction coefficient
= 3.7
1/2m1/2
3, or 1.4 x 106 N s m3. As shown in Fig. 7, this value is effectively independent of the slip velocity.
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of the end-to-end vectors r15 of the amphiphiles, i.e., the orientation of the molecule in the plane of the bilayer. In the quiescent box this distribution is homogeneous, as expected for a bilayer in the liquid-crystalline or fluid L
phase. The sheared system, on the other hand, reveals maxima at
= 0 and
rad, indicative of a propensity to tilt along the shear direction. A distribution of the tilt angles, defined as the angle
between the z axis and the projection of r15 on the xz plane, is presented in Fig. 9. The two peaks of the distribution, corresponding to the upper and lower monolayer, lie at 0 and
rad in the quiescent box, and shift by 
under shear. This average tilt is proportional to the slip velocity and the overall shear rate. The length distribution of the end-to-end vectors is not affected by the shear flow.
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1, which corresponds to a slip velocity of
11 x 103
/
, the bilayer becomes unstable. We observed pronounced undulations of the bilayer, amphiphiles piling up to form buds, and the creation of transmembrane pores. Eventually the bilayer is torn apart. A further discussion of these phenomena will be presented elsewhere. | DISCUSSION AND CONCLUSIONS |
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s for coplanar shear deformations and the friction coefficient
between sliding monolayers. Both are obtained by placing the simulation box under a shear flow, with vorticity oriented perpendicular and parallel to the bilayer, respectively. The shear force acting on the bilayer is then easily obtained by subtracting the shear force on the solvent from the total shear force.
The common experimental method to obtain a surface viscosity is to measure the diffusion coefficient D of a tracer particle, a cylinder of radius a with a length equal to the bilayer thickness hs. Assuming the bulk viscosity
w of the surrounding solvent is much smaller (but not zero) than that of the bilayer, Saffman (17
) derived that
![]() | (8) |
0.577 is Euler's constant. In case
this equation also holds when the tracer particle sticks out of the bilayer. Assuming that Eq. 8 may be used even at the molecular level, we set a equal to
and find D = 1.3 x 102
2/
. Both from a direct calculation of the mean square displacements of the amphiphiles in a quiescent bilayer, as well as from the spreading of the distributions in Fig. 6, we find D = 1.8 x 102
2/
. Using half the surface viscosity in Eq. 8, because the diffusing amphiphiles span only half the bilayer (14
, and thus includes the first "solvation shell". Second, the diffusion coefficient calculated from the Saffman equation is relatively insensitive to the surface viscosity, as illustrated by the two calculated values of D.
It is tempting to relate the viscosity
s of the bilayer to the viscosity
b of a bulk liquid of like molecules, in this case chains of five tail particles, t5. This connection appears frequently in the literature (10
,19
), and is given by
s' =
bhs. Inserting numerical values yields
s' = 14
1/2m1/2
1, which amounts to just over two-thirds of the actual value of
s. This difference is due to the lower degree of ordering in the liquid relative to the bilayer, where the amphiphiles are stretched, aligned, and positioned in a near-planar configuration, and to the higher packing density in the bilayer made possible by this ordering.
The effective friction coefficient of a slab of t5 with the same thickness as the bilayer is readily shown to be given by
' =
b/hs (10
,19
). The resulting value of
' = 0.3
1/2m1/2
3, indicated in Fig. 7 by an arrow, amounts to less than one-tenth of the actual bilayer friction coefficient. Here again, the increased ordering in the bilayer relative to the liquid must have caused the difference, which is much more pronounced for
than for
s. Interestingly, on the basis of experimental data for the friction coefficient, Evans and Yeung and co-workers (10
,11
) also arrived at a mismatch by one order of magnitude.
We end with a brief comparison of our numerical results with experimental data. Whereas the model amphiphile possesses only one relatively short tail, experiments have concentrated on phosphatidylcholine PC lipids with two longer tails of typically 18 carbons. It is to be expected, therefore, that the latter yield considerably higher surface viscosities and friction coefficients than the model amphiphiles, even if friction and random forces had properly been included in the model. Reported surface viscosities for lipid bilayers (10
,14
,18
) are of the order of 107106 surface poise (1 sp is equivalent to 103 Pa m s), as compared to the 8.5 x 1010 sp found by the perpendicular shear simulations. Experimental friction coefficients are rare, with 1 x 108 N s m3 reported by Evans and Yeung (10
) and 4.5 x 108 N s m3 by Raphael and Waugh (12
). Chizmadzhev et al. (19
) assumed in their analysis that
b =
'hs =
w'/hs; from their value of
b we arrive at 2 x 109 N s m3 for hs = 4 nm. The parallel shear simulations yield 1.4 x 106 N s m3. In both cases, the simulation results are two to three orders of magnitude lower than the experimental values. As already alluded to, this is a consequence of using a simplified coarse-grained model, which does not discredit the proposed simulation method in any way.
| ACKNOWLEDGEMENTS |
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Submitted on March 11, 2005; accepted for publication May 2, 2005.
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W. K. den Otter and S. A. Shkulipa Intermonolayer Friction and Surface Shear Viscosity of Lipid Bilayer Membranes Biophys. J., July 15, 2007; 93(2): 423 - 433. [Abstract] [Full Text] [PDF] |
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