jcis_lohi01
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ournal of Colloid and Interface Science 242, 15 (2001)
oi:10.1006/jcis.2001.7894, available online at http://www.idealibrary.com on
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Oscillatory Driven Cavity with an Air/ Water Interface and an InsolubleMonolayer: Surface Viscosity Effects
Juan M. Lopez and Amir H. Hirsa
Department of Mathematics, Arizona State University, Tempe, Arizona 85287-1804; andDepartment of Mechanical Engineering, Aeronautical Engineerin
and Mechanics, Rensselaer Polytechnic Institute, Troy, New York 12180-3590
Received April 5, 2001; accepted July 30, 2001
Flow in a planar cavity bounded by stationary side walls, a flat
as/liquid interface covered by an insoluble monolayer, and driven
y sinusoidal motion of the floor is examined numerically. N avier
tokes computations with the BoussinesqScriven surface model
re presented utilizing the equation-of-state measured for a vita-
min K1 monolayeron the air/water interface. The results identify a
ange of initial surfactant concentration for which the surface ve-
ocity is sensitive to the surface viscosity B (sum of surface shear
nd dilatational viscosities) down to 102 surface Poise. Thus, the
udy suggests a practical method for determining surface viscosi-
es consisting of the measurement of the motion of a tracerparticle
n the interface and comparisons with numerical computations at
arious values ofB. C 2001 Academic Press
Key Words: insoluble surfactants; nonlinear equation-of-state;
urface dilatational viscosity.
1. INTRODUCTION
There is much interest in gas/liquid interfaces, e.g., air/water,
ue in part to the recent interest in microfluidic systems, which
re gaining technological importance. When there is a free sur-
ace in the system (which in some cases is unavoidable, espe-ially when channel walls are not fully wetting, and in many
ases essential, e.g., for gas analysis using microchannels), then
he coupling between the interface and the bulk flow needs to
e considered. When the length scales are small, then interfa-
ial effects can dominate effects of gravity and other forces. For
ery small length scales, the effect of intrinsic surface viscosities
surface shear, s, and surface dilatational, s) can dominate the
ffect of surface elasticity (surface tension gradients). Of the two
urface viscosities, surface shear viscosity has been consistently
measured for a variety of surfactant systems using differenttech-
iques (1, 2). However, the same is not true of the surface dilata-onal viscosity. Determination ofs is difficult since its effects
are coupled to surface tension, both in the normal and tangetial stress balances. General agreement between measureme
of s with different techniques have yet to be demonstrat
(3); results varying by several orders of magnitude have be
reported (2), as well as negative values ofs (4). Most indi
tions are that s may be many orders of magnitude larger th
s (58), so it is important to develop techniques to measur
reliably.
Either the tangential or the normal stress balance may be u
to determine s. One of the techniques that utilizes the norm
stress is the maximum bubble pressure method (9). This tec
nique is not applicable to the measurement of s for insolu
(Langmuir) monolayers, which are of interest to this study. Althe complexities resulting from gradients in surfactant distrib
tion on thesurface of thebubble,e.g.,development of shear str
along the surface, have not been addressed and may account
some of the discrepancies seen between different measureme
of s. Other methods that try to determine s are drop def
mation techniques, but they are not easy to apply to insolub
systems. Although in principle it is possible to spread an ins
uble monolayer on an order 1-mm drop, it is difficult to kno
how much material is present on the surface. Thus, these tec
niques have been primarily applied to soluble systems (101
For larger drops, distortions due to gravity become increasinimportant and the technique requires a microgravity enviro
ment (13). These techniques all assume spherical symmetry,
in practice there is always a lip (e.g., in pendant drop, maxim
bubble pressure method, etc.), so the role of tangential str
may remain unaccounted for.
The classic example that utilizes the tangential stress balan
to determine s is the longitudinal wave method (14). This tec
nique is based on theory that assumes an inertialess limit, hen
the restriction to small barrier speed/frequency. Small barr
speed/frequency is also necessary to avoid making transve
waves as the theory is based on an essentially flat interfaWhen small frequency is used, then the effect of elasticity c
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ominate the effect of surface viscosities (the product of Boussi-
esq number and capillary number being small), so errors in
etermining elasticity (e.g., deviations in the equation-of-state)
may lead to large errors in s. Another method using the tangen-
al stress balance employs a transient vortex flow and simulta-
eously measures the surfactant concentration on the interface,
(x , t), and the surface velocity, us(x, t), at a given location x
8). The problem with the transient vortex method is that theow is not time-periodic, so one cannot do phase averaging. As
result, there are large inaccuracies (at least 50% noise level)
n the determination of surface viscosities. Further, the simulta-
eous measurement of both c and us is technically challenging,
specially since nonlinear optics had to be used to measure c.
We propose a cavity-driven flow; by changing from a barrier-
riven flow, we can drive the system at higher Reynolds numbers
based on frequency and amplitude) and still avoid complicated
urface deformation problems.
. EQUATIONS GOVERNING THE DRIVEN CAVITY FLOW
The flow consists of fluid of density , molecular viscosity
and kinematic viscosity = /), contained in a rectangular
egion of width 2L and depth H, and driven by the horizontal
armonic oscillation of the bottom boundary. The top surface
f the fluid is exposed to air and has an insoluble monolayer on
he interface. Initially, everything is at rest, and the surfactant
monolayer is uniformly distributed. At time t= 0, the bottom
late is set to oscillate with horizontal velocity U sin(2 t).
n this study, we consider the two-dimensional problem that is
nvariant in the transverse direction and neglect viscous coupling
n the air side.The governing equations are the two-dimensional Navier
tokes equations, together with the continuity equation and ap-
ropriate boundary and initial conditions. It is convenient to use
streamfunctionvorticity formulation, where the nondimen-
onal velocity vector and the corresponding(scalar) vorticityare
(u, v) = (y ,x ), = x x yy .
We use H as the length scale and the viscous time H2/ as the
me scale. The two-dimensional NavierStokes equations, with
hese scalings, reduce to the evolution equation for the vorticity:
t +y x x y = x x + yy . [1]
nitially, everything is at rest and the monolayer is uni-
ormly spread; (x, y, 0) = (x, y, 0) = 0 and c(x, 0) = c0.
he boundary conditions on the solid boundaries are no-
ip; for the two stationary vertical walls at x = L/H,
(L/H, y, t) = x (L/H, y, t) = 0 and hence (L/H,
, t) = x x (L/H, y, t). For the oscillating bottom,
(x, 0, t) = 0and y (x, 0, t) = Re sin(2 Ret); the two gov-
rning parameters are Re = UH/, the scaled velocity ampli-
ude of the floor, and Re = H2
/, the scaled frequency of theoor oscillation. The vorticity is (x, 0, t) = yy (x, 0, t). On
the air/water interface, being a material surface, (x, 1, t) =
by continuity with its value on the sidewalls, which is set
zero without loss of generality. We assume that the interface
flat, and hence the contact angle at the air/water/solid cont
line is 90 (in a physical laboratory experiment, the location
the contact line can be fixed by depositing a nonwetting paraf
film above the interface on the vertical walls (15); also, t
Froude number, Fr= 2
/g H
3
, for water at room temperatuand a depth H 1 cm, is only about 103). This leaves t
condition for the vorticity on the interface to be specified.
We model the interface using the BoussinesqScriven co
stitutive relation (16). In planar two-dimensional systems w
a flat interface, only the tangential stress balance plays a d
namic role (2). The tangential stress balance is, noting that
the interface v = 0:
(x, 1, t) = uy (x, 1, t) = C1x
Busx
x
,
where C = /H0 is the capillary number, is the s
face tension which varies with surfactant concentration c, 0(c = 0),B = (s + s)/H is the Boussinesq number cor
sponding to the sum of the surface shear and dilatational v
cosities (in general, also functions of c), scaled by H, a
us(x, t) = u(x , 1, t). In (15), we determined that an insolub
monolayer comprised of vitamin K1, for concentrations up
1 mg/m2, had negligible surface shear viscosity. In this stud
we shall treat B as constant since its functional dependence o
is not known a priori. This linearization is self-consistent as t
computational results indicate that variations in c in both tim
and space are small for the parameter ranges considered. T
reduces the surface viscosity term in Eq. [2] to Bus
x x . For we utilize the equation-of-state measured for water/vitamin
in (15). This equation-of-state is plotted in Fig. 1, along with
FIG. 1. Measured equation-of-state (open symbols) for a vitamin K1 mo
layer on air/water interface at 23C (15), together with the curve fit givenEq. [3].
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tted curve given by
= 66.1+ 6.2 tanh(7.5(1 c/1.38)). [3]
Since the vorticity at the interface depends on surface tension
radients, which in turn depend on the surfactant concentration,
we also need to solve an advectiondiffusion equation for the
urfactant concentration,
ct + (c us)x = Pe
1cx x , [4]
where Pe= /Ds is the surface Peclet number and Ds is the dif-
usivity of the surfactant on the interface. Note that [4] is linear in
so there is no need to nondimensionalize c. Conservation of in-
oluble surfactant on the interface is enforced with the zero-flux
onditions cx (L/H, t) = 0. The zero-flux boundary condition
ssumed for insoluble monolayers is realizable in experiment
or low Fr flow by pinning the contact line via the application of
nonwetting film on the sidewall above the waterline (15, 17).The numerical solution of [1] and [4] together with the bound-
ry and interface conditions follows that used in (15, 18).
pecifically, a second-order centered finite-difference spatial
iscretization is used, with nx = 101 and ny = 51 grid points
n the horizontal and vertical directions, respectively, together
with a second-order predictorcorrector scheme for the time
volution. The time step, t, is governed predominantly by the
dvectiondiffusion Eq. [4] for the range of parameters chosen,
ndneedsto be reduced when the surface velocitybecomes small
which is the case when Marangoni stress is large and/or surface
iscosities are large). The smallest value used was t= 107.
3. RESULTS
Equation[2] shows that the stress on the fluid at the interface is
ue to contributions from elasticity and surface viscosity. These
ontributions are qualitatively different in the way they relate to
he thermodynamic state of the interface (via surfactant concen-
ation) and its kinematics (fluid velocity at the interface), and
heir effects are complementary. To leading order, c is essentially
onstant (this is verified numerically for the Re and Re ranges
onsidered). The elastic term depends on the equation-of-state,
s x = ccx ; for small cx , its contribution is greatest for c valueswhere the equation-of-state is steep, i.e., c large, regardless of
ny velocity gradients. On the other hand, the surface viscosity
erm,Busx x , has B essentially constant (for small cx ), but its con-
ibution to the surface stress depends to leading order on surface
elocity variations. These can be made large by appropriate os-
illatory driving. Also, the elastic contribution dominates when
here is large bulk inertia (flow) that drives a concentration gra-
ient and results in a Marangoni stress that brings the surface
elocity to zero. This occurs for adequately large Re and suit-
bly small Re. Whereas, the viscous contribution dominates
when there are large surface velocity gradients, and is relativelynsensitive to concentration gradients.
The objective of the computations presented here is to demo
strate that the flow under consideration is sensitive to surfa
viscosity effects in some range of parameter space. For this fl
to provide a practical experimental technique to measure surf
viscosities,B, we need to show that it is sensitive toB variatio
in a parameter regime accessible to laboratory measureme
with a reasonable signal-to-noise ratio. We begin by noting t
B only appears in the tangential stress balance (2), and its effon this balance may be completely masked by surface tensi
gradient effects. For a given surfactant system (and bulk liqu
e.g., water at room temperature), the only variable available
adjust the relative contributions of Marangoni stress and surfa
viscosities to the stress balance is the length scale H; C
scales with H and B scales with H1, so as H is reduced,
ratio of surface viscosity to elasticity is increased by H2
practical lower limit is H 1 cm, which would limit the Frou
number to 103 and minimize surface deformations. Fo
vitamin K1 monolayer onwater ofdepth 1 cm at 23C, this giv
C = 1.2 106. In the present calculations, we have conside
FIG. 2. Variation of max |us| and c/c0 with c0 (mg/m2) for Re = 1Re = 16, H/L = 1, and B as indicated.
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FIG. 3. Profiles of surface velocity, us, and concentration, c, at 10 phases over one oscillation period for Re = 100, Re = 16, H/L = 1, c0 = 2.0 mg/
nd B as indicated.
arious Re and Re with c0 up to 2.25 mg/m2, covering a largeange of the equation-of-state. For each of these parameters,
e have set B = 0, 1, 10, and 100; using our scalings, B = 100
orresponds to (s + s) = 0.9325 g/s (surface Poise). In the
alculations, we have set Pe= 10, which is probably about
wo orders of magnitude too small, but since the surfactant
oncentration gradients are everywhere small for the cases
onsidered, we do not expect the results to be sensitive to Pe.
The flow geometry was selected to accentuate the contribu-
on from surface viscosity. The parameters used to illustrate the
esults are selected with an eventual laboratory experiment in
mind to verify the model and ultimately to measure the surfaceiscosities, B. The depth of the cavity, H= 1 cm, was cho-
en to be as small as possible (in line with the above scaling
rgument), but not so small that Fr becomes large and surface
atness suffers, and surface velocity measurements are diffi-
ult. The frequency of oscillation, Re = 16, was selected to
e large enough to avoid approaching a quasi-static monolayer
18) showed that for steady flow, the effect of surface viscosi-
es is very small at a steady monolayer front), yet small enough
o give adequately large surface velocity and surface velocity
radients and avoid instabilities in the bulk flow. The amplitude
f oscillation, Re = 100, was selected to be large enough to en-
ure a strong surface flow (to keep viscosity in the bulk fluid from
diminishing the surface velocity) and small enough to avoid stabilities in the bulk flow (19). In Fig. 2, the maximum surfa
velocity over a complete period, max |us|, andthe relative chan
in concentration over a complete period, c/c0, are plotted
functions of initial concentration, c0, for B = 0, 1, 10, and 1
in the driven cavity with Re = 100, Re = 16, and H/L =
using a vitamin K1 monolayer. The plot shows that over som
ranges of c0, the effect of surface viscosity is to decrease t
magnitude of the surface velocity, as expected. For c0 < 1
c0 > 1.8 mg/m2, the change in surface velocity is well with
the range that can be sensed in a laboratory measurement. T
change in c is comparatively small, thus use of a constant surfa
viscosity in each calculation is justified.
Profiles ofus and c over one period for a typical set of para
eters (Re = 100, Re = 16, H/L = 1, c0 = 2) are present
in Fig. 3 for B = 0 and B = 100, illustrating the factor of tw
difference in us, which is detectable using now standard flo
measuring techniques.
4. CONCLUSION
The theoretical foundations for a method for determing t
surface dilatational viscosity of insoluble monolayers are p
sented (the planar geometry gives the sum of the surface she
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nd dilatational viscosities and measurements of surface shear
iscosityvia independent established methods canbe used to iso-
ated the surface dilatational viscosity (20)). The time-periodic
ow was chosen to minimize surface deformations and max-
mize gradients of surface velocity. By considering the nondi-
mensionalized tangential stressbalance, we show that theratio of
he surface viscosity term to the elastic term scales as H2, thus
he cavity depth, H, needs to be minimized. NavierStokes com-utations are presented for a physical monolayer on the air/water
nterface; the equation-of-state for vitamin K1 was used in the
alculations since we have already demonstrated that it forms
well behaved monolayer and quantitative comparisons in a
ifferent flow between NavierStokes computations and mea-
urements have already been made for this monolayer (15). For
range of surfactant concentration where surface elasticity is
mall, the method is sensitive down to order 102 surface Poise.
With increasing surface viscosity, the range of concentration for
which theviscosity can be determined increases. Theflow geom-
try and operating conditions for the case presented correspond
o conditions that are presently realizable in the laboratory, and
roduce a stable bulk flow. For these operating conditions, the
omputed amplitudeof themaximum surface velocityis 40 m/s
n the absence of surface shear viscosity and 20 m/s with sur-
ace viscosity of about 1 surface Poise (for a 1-cm-deep channel
with water at room temperature). This difference is readily mea-
urable by video microscopy of a tracer particle on the surface
5). Thus, this study suggests a practical method for determin-
ng surface viscosities, B, consisting of the measurement of the
motion of a tracer particle on the interface and comparisons with
NavierStokes predictions at various values ofB.
ACKNOWLEDGMENT
This work was supported by NSF Grants CTS-9803478 and CTS-989625
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