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HAL Id: jpa-00247991

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Submitted on 1 Jan 1994

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Orientational instability of nematics under oscillatory flow

A. Krekhov, L. Kramer

To cite this version:

A. Krekhov, L. Kramer. Orientational instability of nematics under oscillatory flow. Journal de

Physique II, EDP Sciences, 1994, 4 (4), pp.677-688. �10.1051/jp2:1994155�. �jpa-00247991�

(2)

Classification

Physics Abstracts 61.30G 47.20

Orientational instability of nematics under oscillatory flow

A-P-

Krekhov(~)

and L.

Kramer(2)

(~) Institute of Physics, University of Bayreuth, D-95440 Bayreuth, Germany

(~) Physics Department, Bashkirian Research Center, Russian Academy of Sciences, 450025 Ufa, Russia

(Received

27 October 1993, revised 5 January1994, accepted 6 January1994)

Abstract. Generalizing a recently introduced approximation scheme valid when the director relaxation time is large compared to the inverse frequency of an oscillatory flow, we derive equa- tions for the time-averaged torques on the director for a prescribed plane shear flow. Whereas for a linear flow field

(simple

Couette flow) the average torques vanish, one has for Poiseuille flow

(and

more general flow

fields)

torques that tend to orient the director essentially

perpendicular

to the flow plane. For flow-aligning materials the orientation parallel to the flow is also

(weakly)

stable. Including the effect of homeotropic surface alignment we estimate the threshold of the oscillation amplitude for the out-of-plane transition. The results are essentially recovered

land improved)

by direct numerical simulations.

1. Introduction.

Liquid crystals

exhibit

interesting

flow

phenomena

due to the

coupling

between the director and

velocity

field. The flow

properties

of a nematic

liquid crystal

are characterized

by

Leslie viscosity coefficients al,

, a6, of which two, a2 and 03, describe the

coupling

between flow and director orientation [1-3]. For a

steady velocity

field

viz) along

the z-axis

(plane

shear

flow)

the director will tend to

align

in the shear

plane ix

y

plane)

at an

angle

bfl = tan~l

(a3 /02)~/~

with the z-axis if a3

la2

> 0, which is

usually

the case [4, 5].

However,

in some materials one has

a31a2

< 0

(especially

near the transition to a smectic

phase)

and then instead of flow

alignment

one has a

tumbling

motion [6]. In the usual situation where the director is

aligned

at the surfaces of a

liquid crystal layer

such

hydrodynamic

torques can lead to orientational instabilities. A recent review of these effects is

given

in [7].

When the

velocity

field oscillates

periodically

and

symmetrically

around zero the situation becomes more

complicated.

In a

previous

paper we have

given

an account of much of the

existing

work on this

subject,

which we will not repeat here [8]. We have also introduced

a method based on a two-time scale

analysis

to extract the slow

averaged dynamics

of the director under a

prescribed oscillatory

shear flow field. The director motion was restricted

(3)

to the shear

plane.

In this paper we

generalize

the treatment to include

out-of-plane

director motion. The

general averaging

method for the director

equations

are

presented

in section 2 and

we

apply

it in section 3 to the

simplest small-amplitude plane

Poiseuille flow.

Surpflzingly

the

problem

can

again

be solved

analytically.

For the case of

homeotropic

director

alignment

the critical flow

amplitude

for the

out-of-plane

transition is calculated. The numerical simulations

presented

in section 4 confirm the

analysis

and extend them to

arbitrary

flow

amplitude.

In

section 5 we comment our results with a view on

possible experiments

and

give

an outlook for future work. Some detailed

analytic

formulas are

presented

in the

Appendix

A.

2. Basic

equations.

We consider a nematic

layer

of thickness d confined between two infinite

parallel plates.

The z-axis of a Cartesian coordinate system is chosen normal to the

bounding plates,

the

oscillating

flow in the z-direction and the

origin

in the center of the

layer.

With this choice one can write for the director i1 and

velocity

Q

n~ = cos b cos

#,

n~ = sin

#,

n

z = sin b cos

#,

U~ "

U(t, Z),

Uy "

U(t,

Z), Uz " 0,

ill

where

b, #,

u, u are functions of t and z. In

general,

a full solution of the four

coupled_

hydrodynamic equations

for

b, #,

u and u [1, 2] with

time-periodic boundary

conditions for

u(t, z)

at z =

+d/2 (Couette flow)

or

time-periodic

pressure

gradient 8P/8z (Poiseuille flow), u(t,

z

=

+d/2)

m o and appropriate

boundary

conditions for

b, #

is

quite

a formidable task.

For

simplicity

we will here treat

u(t, z)

as a

prescribed 2x/w-periodic

function in t with

u(t

+

x/w,z)

=

-u(t, z),

so that the

time-average

<

u(t,z)

>= 0. In the same

spirit

we set u

=

0. This should be a

good

approximation for small oscillation

amplitudes A/d

< I

(A

is the maximum

displacement

in the

oscillatory flow)

because the director distortion is small.

Moreover,

for

larger amplitudes

the

approximation

should still be reasonable for low

frequencies

such that the viscous

penetration depth fi,

where o is a

typical viscosity,

is

larger

than

the thickness d. Then the flow field is distorted

by

the fact that the effective shear

viscosity

is

z-dependent

as a result of the director distortion. The distortion is

(presumably)

not very

significant,

except

maybe

for Couette

flow,

where the undistorted flow field

(constant velocity gradient)

does not lead to any effect

(see below).

With the dimensionless variables

I

= wt, I

= z

Id,

fi

=

u/dw, (2)

the

equations

for

b(t, z), #(t, z)

can now be written as [1-3]

~,t

~(~)U

z ~~[~ll(bi

~)~,zz

+

a2(bi

~)~~z ~ ~l3(~i

~)~,zz

+

a4(~i ~)~~z

~

a5(~i~)~,z~,zji (~)

#,t K'(b)M(#)u,z

=

e~[bi(b, #)b,zz

+

b2(b, #)9)~

+

b3(~, ~)~,zz

+

b4(~,

@~~z +

b5(~, @~,z~,zj, (~)

where the tiides have been omitted and

K(b)

=

(I

cos~ b sin~

9) Ill Ii, M(#)

=

~

sin

#

cos

#,

2 1

=

o31a2,

e~

=

I/(Tdw),

Td

='fid~ /Kii, (5)

(4)

the notation h, +

8h/8i, h'( f)

+

8h/8 f

has been used

throughout

and

a,(b, ii, b;(b, #)

are

al16, ii

= cos~b + k2

sin~

b + (k3 k2

sin~

bcos~

#, a216, #)

= [k2 + (k3

k2)

cos~

ii

sin b cos

b, a316,

WI

= k2

ii

sin b cos b tan

#,

a41b,

WI =

(2k2

k3

iii

sin b

cosb,

a516,

WI =

-2[cos~

b + k2

sin~

b +

2(k3

k2

sin~

bcos~

#]

tan

#, bi16,

WI = (k2

ii

sin b cos b sin

#

cos

#,

b216,WI = [sin~b + k2 cos~b +

2(k3 k2) sin~

bcos~

#]

sin

#

cos

#,

b316,

ii

= sin~b + k2 cos~b + (k3

ii sin~

bcos~

#,

b416, 11 =

-(k3 ii sin~

b sin

#

cos

#,

b516,11

= -2 sin b cos

b(k2

k3 cos~

# sin~

WI,

(6)

and

k,

=

K,,/Kii.

Since the

frequency

of

oscillatory

flow w is

usually

much

larger

than the inverse director relaxation time I

/Td (I /Td

~

10~~ s~~ for d

= 100

pm)

we may assume e~ < I.

Neglecting

in a first step the terms on the

right-hand

side of

equations (3, 4),

the

remaining

first-order

ordinary

differential equations can be solved and the solution bo is obtained

implicitly

from

/°° (

=

glt,z), glt, z)

=

/~

dtu

z(t, z), (7)

so that bo "

bol~, glt, z))

is a

periodic

function in t. Note that for the

flow-alignment

case,

1 > 0,

K(b)

vanishes at b

=

+bfl

and

(7)

cannot be used for ~

= +bfl

(then

bo +

+bfl).

In

principle,

the

b-integral

in

(7)

can be solved

analytically

and

bo(~, g)

can be

expressed

in terms of

elementary

functions [9] but for our purpose this is not needed. Then the solution

lo

can be obtained from

~° /l~

-

~ dtK~(b°)Uz

= in

ill°1

(81

and

#o(x,~,g(t,z))

is also a

periodic

function in t. We choose the

origin

of t such that

g(t

=

o)

= 0 so that one has

bo(t

=

0)

= j

#o(t

=

o)

= x.

Thus,

from

(7), (8)

bo oscillates around ~ and

lo

around x,

but,

in

general,

< bo

>#

~ and <

lo >#

x. We conclude from

(7), (8)

that

neglecting

the elastic

coupling

leads to a continuous two-parameter

family

of

periodic

oscillations of b and

#

that can be

parametrized by

the

"phases"

~ and x. The

only

fixed points

are #o " o, bo =

+bfl

and

#o

=

x/2.

One

easily

sees from

equation (8)

that the

trajectories

in the

#,

b

plane

are

given by

~~

~~~~~/~~

~~~

In

figures

la and 16 we have

plotted

the

trajectories

for two cases with I > o and I < o,

respectively.

The three

trajectories correspond

to ~ =

x/2

and x

=

x/18, x/6

and

x/4, but,

as seen from

equation (9),

other combinations of ~ and x lead to the same curves.

Depending

on the

amplitude

a

only

part of the curves are

actually

traced out

by

the director. For

large

a and I > o the oscillations saturate at the

flow-alignment angles

whereas for I < o the director motion is in

principle

unbounded

(extend Fig.

lb

periodically).

A similar behavior

was obtained

previously

[9].

In order to

investigate

the influence of the elastic

coupling

in equations

(3, 4)

we use the method of

multiple-scale analysis

[10].

By introducing

a '~slow" time T

=

e~t,

that modulates

JOURNAL DE PHY~)QUE II -T 4 N'4 APRIL 19~4 ~

(5)

r/4 y=n/4

_,,...,__

=~~~8

_."" '".._ ~)

n/6 :/

,---,, "_

.~ ," ',

./ ,' ',

:" l' ',

n/12

,' ',

/ ,

l~o

0

6tj

__... ....___

:.." "". b)

:. ...

:." "...

:.' "..

n/6 _.." "...

,

...

:" ,' ,, "..

:.' ,, , ..

, , ...

, ,

, ,

n/12 ,' ',

,,

o

0 n/2 R

6~

Fig. I. Trajectories in #o,Ho plane obtained from equation (9) for 1 > 0

(a)

and 1 < 0

(b).

the

periodic

behavior on the "fast" time

scale,

so that b

=

b(t,z,T), #

=

#(t,z,T)

and

at

- at +

e~8T,

one can formulate a

systematic perturbation expansion

of the form

b

= bo +

ebi

+ e~b2 +

,

#

=

#o

+

e#i

+ e~#2 +

,

(lo)

where all functions

b,,

#, are

periodic

in t. At order e° one has the solutions

(7, 8)

where the

"phases"

~ and x are now allowed to

depend

on z and slow time T and are undetermined at this order. At first order in e one has

~

~~~

~' ~

-K'~bo

)~j~~)~~ at K'(bo M'(~o )u zj'

~~~~

where L is the linear operator of the

perturbational equations

and we can choose

(bi

" o,

ii

"

o). Finally,

at order e~ we find

~

b2 ~bo,T

+

albo,zz

+

a2b(,z

~

a3~0,zz

+

a4~(,z

~

5b0,z~0,z)

~2

~~0,T

+

blbo,zz

+

b2b(,z

~

b3~0,zz

+

b4~(,z

~

bsbo,z~0,z

~~~j

where a, =

a,(bo,40),

b,

=

b,(90,40).

Since L has the two null

eigenvectors 8~(90,#o)

and

8~(90, 40)

one has two

solvability

conditions for the

inhomogeneous

linear

equations (12)

which take on the form

<

V+[F

>=

0,

<

W+[F

>=

0, (13)

where F is the

right-hand

side of

equation (12)

and we define the scalar

product

<

V[U

>=

) ~~~~ dt(ViUi

+

V2U2). (14)

K t

(6)

Here

V+,

W+ are two

linearly independent

null

eigenvectors

of the

adjoint

operator L+

L+(j+,j+)=0, L+(W/,W/)=0,

L+

-

(K,,ilii~llll°1"

~

a~

ri~g~~~,~l~~u l

(IS)

One

easily

finds

V~

=

(),°)

,

W~

=

~-g~~((

,

)) (16)

,n ,n ,x o,x

Using

the fact that

(90, lo) depends

on z and T

only through

~, x and g, equations

(13)

can

be cast into the form of evolution

equations

for the

phases

~ and x

~J,T = Bi + Ci~J,z +

Dix,z

+

Ei~J,zz

+

Fix,~~

+ GiJ~)~ +

Hix)z

+

IiJ~,zx,z (17)

x,T =

82

+ C2~,= +

D2x,z

+

E~~,z~

+

F~x,~~

+ G~~)~ +

H~x)z +12~,zx,z (18)

where

B,, C,,..

,

I~ are scalar

products involving

the functions ~, x,

90, lo,

g,z and g,zz. The

expressions

are

given

in the

Appendix. Equations (17, 18)

describe the slow evolution of the

phases

~ and x. Bi, 82 are in

general

nonzero if g is

spat1ally varying,

I.e. if u

zz

#

0

(see Appendix).

Nonzero Bi and 82 means that there are net bulk torques

acting

on ~ and x. If

spatia1variations

of ~ and x

play

no role the stationary solutions of

(17, 18)

are

simply given

by

the zeros of

Bi,

82.

3.

Small-amplitude oscillatory

Poiseuille flow.

Let us consider more

explicitly

the case of small

g(t, z),

which

essent1ally

amounts to A

Id

< I, where A is the maximum

displacement

in the

oscillatory

flow. Then one has from equations

(7, 8)

for 90 and

#o

up to the second order in g

90 = ~J +

K(~J)g

+

K~(~J)K(~J)g~

+

,

40

= x +

K'(~J)M(x)g

+

)lK"(~J)K(~J)

+

K/~(~J)M'(x)lM(x)g~

+

(19)

The

simplest

situation is obtained for

plane oscillatory

Poiseuille flow:

u =

a(4z~ 1)

cost, g = 8az sin t.

(20)

Then Bi, 82 have no

explicit

z

dependence

and for

spat1ally

uniform ~, x equations

(17, 18)

with

(19, 20)

lead to

~,T "

a~B1(~, X),

Xi

"

a~B2(~, X), (21)

where the functions

fli(~/, x), fl2(~/, x)

are obtained from the

general expressions (Appendix) ti (~, x)

=

3211ai (~, x)

+

a5(~, x)M(x)iK'(~)K(~)

+

a2(~, x)K~(~)

+a3(~, x)M(x)iK"(~/)K(~/)

+

K'~(~/)M'(x)1

+

a4(~/, x)iK~(~/)M(x)i~i,

£2(~, x)

=

3211bi (~, x)

+ b5

(~, x)M(x)iK'(~)K(~)

+

b2(~, x)K~(~)

+b3(~, x)M(x) ill" (~)K(~)

+

K'~ (~)M'(x)1

+

b4(~, x) iK'(~)M(x)i~i (22)

The a,, b, are defined in

(6).

(7)

For

in-plane

motion, I-e- x

= o one has

82(x

=

0)

= 0 and

fli lx

"

0)

=

16[(cos~

~ + k3

sin~ ~)K~ (~)l'. (23)

In the

flow-alignment

case

(I

>

o) fli(x

=

o)

has three zeros

corresponding

to two stable

equilibria

at ~ = 0 and ~

=

x/2,

and an unstable

equilibrium

at the

flow-alignment angle

~ = 9fl =

tan~~(a31a2)~/~

[8]. For

non-flow-aligning

nematics

(1

<

0)

there remains an

unstable

equilibrium

at ~ = 0 and a stable one at ~

=

x/2.

By linearizing 82

around x

= 0

((x(

«

ii

one can

study

the

stability

with respect to out-

of-plane

motion. For the

typica1relations

between the elastic constants

K22

<

Kii

<

K33

and

(I(

< I one finds that in the case 1 > 0 the

equilibrium point (~

= 0, x =

0)

is stable with respect to

out-of-plane

motion and

(~

= 9fl, x =

0), (~

=

x/2,X

"

0)

are unstable. For the

case 1 < 0 the

in-plane

motion is

always

unstable.

Out-of-plane equilibrium points

of

equations (21)

can be

easily

found for ~

=

x/2.

Then

Bi(~

"

x/2)

= 0 and

fl2(~

"

x/2)

=

~~

sin x cos

x[(k3

k2 + 1 k2

lk3)

cos~ x I

sin~ x] (24)

(1- 1)2

has zeros at x =

0, x/2

and for 1 > 0 also at

xo "

tan~~(~/(k3

k2 + k2

lk3)/1). (25)

Finaliy

another

equilibrium

point

(~i,

xi

),

with ~i " 9fl, xi *

x/4

appears in the case 1 > 0.

Complete phase diagrams

which show the

trajectories

of the system

(21)

are

plotted

schemat-

ically

for the cases 1 > 0 and 1 < 0 in

figure

2a and

figure 2b, respectively.

For 1 > 0 one has

two attractors, but since for

typical

nematics 9fl is

small,

one expects the solution

(~

= 0,X

"

0)

to be very

weakly

stable

(small

domain of

attraction) compared

to

(~

=

x/2,

x

=

xo).

For

1 < 0

only

the fixed

point

x

=

x/2

is stable. In both cases

(~

=

x/2,

x =

0)

is unstable with respect to out-of-

plane

motion.

The above

analysis

shows the

possibility

of a

(spatially homogeneous)

transition to out-of-

plane motion,

but it cannot

give

a threshold because

(stabilizing) boundary

conditions on the

director are not included. We now take into account

homeotropic boundary alignment

in an

approximate

manner within our scheme.

Returning

to the evolution

equations (17, 18)

and

linearizing

with respect to x around

(~

=

x/2,

x

=

0)

one obtains with

(19, 20)

x,T "

a~bx a~izx,z

+

/x,zz, (26)

where

"

~i

~jj2

(~3 ~2 + ~2 ~~3 Ii

?

"

11

~>)2

l~~~~ + ~~

~~l'

/

= k3

(27)

The

boundary

conditions for x at z = +

1/2

are

x(z

= +

1/2)

= 0. The modal solutions of equation

(26)

are of the form

x =

exP(aT)U(z) (28)

and

u(z)

satisfies the differential equation u"

fl2zu'+

au

= 0,

u(z

=

+1/2)

= 0,

(29)

(8)

n/2 n/2

I x

z z

0 0 O O

0 6jj n/2 0 n/2

aj ~j

Fig. 2. Phase diagrams for the spatially uniform solutions of evolution equations for 1 > 0

(al

and 1 < 0

(b).

where

o =

a~il / al /, fl

=

a~il /. (30)

2 With the transformation u

=

exp(flz~ /2)w(z)

this equation can be reduced to

w" +

[a

+

fl fl~z~]w

= o,

w(z

=

+1/2)

= o.

(31)

It is well-known that for this

problem

there is a minimum

eigenvalue

o +

fl

that is real and

positive.

The solution of

(31)

can be

expressed

in terms of a confluent

hypergeometric

function

ill]

~~~~ ~~~

~~'~ ~' '~~~~'

~~~~

From the

boundary

conditions for w one has the

following

equation for

o(fl)

The

dependence

of

a(fl)

obtained from the numerical solution of

equation (33)

is

plotted

in

figure

3. From

equation (30)

follows a =

cfl

a where c

=

2ili,

=

al /.

Thus for

a >

cfl

one has a < o and

perturbations

of x

decay

in

time,

while for a <

cfl

the

growth

rate is positive. The critical value fl~ and the

corresponding

threshold

amplitude

a~

=

fill

of

the

oscillatory

flow can be found from the intersection of the universal curve

a(fl) (Fig. 3)

and the

straight

line a

=

cfl

whose

slope depends

on

liquid crystal

material parameters. For

example,

with the MBBA

liquid crystal

parameters Kii " 6.66 x

lo~~~, K22

" 4.2 x

lo~~~,

K33

" 8.61 x

10~~~N,

02

" -lloA x

lo~~,

a3 " -1.I x

lo~~Ns/m~ [12,

13]

one has a~

= o.4.

Thus for a < a~ the

growth

rate is

negative

and

in-plane

motion is stable

becoming

unstable for a > a~. From equation

(27)

one sees that I has a small influence on the threshold as

long

as

iii

< 1.

(9)

1o o

80

o= cJ

60

~

40

20

~~0.0 5.0 lo 0 15.0 20 0

fi

Fig. 3. Dependence of

a(fl)

corresponding to the minimum eigenvalue equation

(31).

4. Numerical simulations.

In order to test the

analytical

results direct finite-difference simulations of the basic

equations (3, 4)

for the Poiseuille

velocity

field

(20)

were

performed. Homeotropic boundary

conditions

for the director 9

=

x/2,

# = 0 at z =

+1/2

and MBBA parameters were used. We indeed found the

instability

of the

in-plane

motion. The

out-of-plane

distortion of the director can be described

by

the

angle

#m

corresponding

to the

midplane

z = o

(there

the

angle

is time

independent

since for Poiseuille flow

u,z(z

=

o)

=

0).

In

figure

4 we show

ii

as a function of the flow

amplitude

a for different

frequencies

of the

oscillatory

flow. Near threshold one has

#m

+~

(a a~)~/~

so the bifurcation is

supercritical leading

to a continuous

change

of #m with a.

The critical

amplitude

a~ decreases

slightly

with

increasing

flow

frequency,

but remains

higher

than the value a~

= oA obtained from the

analytical approximation.

The

discrepancy

is not

alarming given

that in the

analytic approach

we assumed a~ < I. Moreover the

homeotropic boundary

conditions for 9 are

only

satisfied in the average in the

analysis.

Numerical simulations of

equations (3, 4)

with

homeotropic boundary

conditions for pre- scribed

oscillatory

Couette flow

u =

a(z

+ cost

(34)

2

confirms that there is no

out-of-plane instability

up to

high

flow

amplitudes.

5. Discussion.

Our

investigation

shows that for

plane oscillatory

Poiseuille flow in a

homeotropically

oriented

sample

one has a transition to

out-of-plane

motion

through

a

supercritical

bifurcation. Our

treatment is valid in the

frequency

range

I/Td

< w <

a/pd~

where o is the effective shear

(10)

06

- f=10 Hz

- f=50 H2

H- f=100 Hz

-f=500 Hz

0.4

cv E

£+

0.2

~'~

55 60 0.65 0.70 0 75

a

Fig. 4. Dependencies of

#(z

= 0) on the amplitude of oscillatory Poiseuille flow for different

frequencies.

viscosity, and then the threshold

amplitude

is

proportional

to the

layer

thickness d and

indepen-

dent of w with corrections of the order

(Tdw)~~/~

due to the

boundary layers.

For

flow-aligning

nematics the

homogeneous

orientation

parallel

to the

velocity

field is

linearly stable,

but

large

fluctuations in the flow

plane beyond

the

flow-alignment angle might

destabilize the state

(see Fig. 2a).

For such materials

(homogeneous)

orientation

perpendicular

to the flow

plane

can in

principle

also become

unstable,

but the

hydrodynamic

torques are small in this situation and the attractor near

by.

For

non-flow-aligning

nematics the orientation

parallel

to the

velocity

field can become

unstable,

but

again

the

hydrodynamic

torques are small. For such materials the orientation

perpendicular

to the flow

plane

is

absolutely

stable.

Clearly

these results differ

considerably

from what is known for

steady

flow [7].

We have not

investigated stability

with respect to

spatially periodic

fluctuations. From the results for

elliptic

shear flow [14] we expect that

out-of-plane

motion can

undergo

such an

instability leading

to a

periodic

roll pattern.

For

simple oscillatory

Couette flow no

instability

is found within our framework. This ap- pears to remain true when

spatially periodic

fluctuations are considered [14] unless inertial

terms are

included,

which

surprisingly

appear to be

responsible

for an

instability

at low fre-

quencies (down

to below loo

Hz) [15-17].

Actually

inclusion of inertial terms into our treatment is

straightforward

as

long

as the oscillation

amplitudes

are small. Then the restriction w «

a/pd~

is overcome and in the

high- frequency

range the

small-amplitude approximation

is in fact

expected

to be valid. Then also

oscillatory

Couette flow should lead to average torques and

possibly

to a

spatially homogeneous

reorientation. Work in this direction is in progress. Moreover we

hope

to be able to

generalize

our method to include corrections to the

velocity

field

resulting

from director distortions in a self-consistent manner.

Clearly

it would be

interesting

to test our

predictions experimentauy,

and we

suggest doing

(11)

this with

homeotropic

director

alignment.

When

oscillatory

Poiseuille flow is induced in a thin slab in the usual way

by application

of a pressure difference one must be aware of the fact that as a result of

compressibility

the pressure

decays along

the flow direction z on a

length

b

+~

d/pc~/(3wa))

where c is the sound

velocity

and o a

typical

shear

viscosity

[18]. Since b » d for all reasonable

frequencies, experiments

should nevertheless be

possible.

The

decay

is avoided when Poiseuille flow is induced

by oscillating

in

parallel

both

plates

of an

open-ended

slab.

Finally

let us

point

out that effects related to the one treated

here,

where

systematic

forces result from

oscillatory

and

spatially varying

excitation, are known in Plasma

Physics

under the name of

"ponderomotive

forces"

(see

e.g.

[19]).

Acknowledgments.

We wish to thank A. Buka and H. Schamel for

helpful

discussions. Financial support from Deutsche

Forschungsgemeinschaft (SFB213

and

Graduiertenkolleg

"Nichtlineare

Spektroskopie

und

Dynamik", Bayreuth)

are

gratefully acknowledged.

One of us

(A.K.)

wishes to thank the

University

of

Bayreuth

for its

hospitality.

Appendix.

The

solvability

conditions

(13)

with definition ofthe scalar

product (14)

and

linerly independent

null

eigenvectors

of the

adjoint

operator

(16)

take on the form

~

)~0,T

>"<

)[a190,zz

+ a29~,z ~ ~l3~0,zz +

a4~~,z

~ ~l590,z~0,z) >1

(~~)

,n ,n

~

)§~0,T

> <

~~~

90,T >-<

)[(bl

jl'~al)~0,zz

+ (b2

l'~a2)~~,z

~

,x , ,x ,x ,n ,n

(b~

jjj a~)io,zz

+ (b~

jj~ a~)ii,z

+ (b~

jj~ a~)90,zio,zi

>,

(36)

, ,n ,n

where a,

=

a~(90, lo),

b, = b~(bo,

lo)

are defined in

(6)

and < F >=

) f/~~~dtf.

From equations

(7, 8j

one has bo =

bo(~,gl,

40 =

40(x,~J,gl,

where J~

=

J~(T,zj,

x

=

x(T,zj,

g =

g(t, z)

and

b0,T

"

b0,q~,T, ~0,T

"

~0,q~,T

+ §$0,XX,Ti

bo,z = bo,~~J,z +

bo,gg,z, 40,z

= 40,~~J,z +

40,xx,z

+

40,gg,z,

bo,zz = bo,~~J,zz + bo,~~~J)z + 2bo,~g~J,zg,z +

bo,gg,zz

+ bo,ggg)z,

40,zz

= 40,~~J,zz + 40,~~~J)z +

40,xx,zz

+

40,xxx)z

+

2jo,~x~J,zx,z

+

2jo,~~J~,~g,~ +

2jo,~~x,zg,z

+

40,gg,zz

+

40,ggg)z. (37j

Then for the coefficients in evolution

equations (17, 18)

one has

i~l

<

)ial(~0,g§,zz

+ b0,gg§~z) ~ ~l2b~,g§~z ~

~l3(~0,g§,zz

+ ~0,gg9~z) +

,n

a4~~,g9~z ~ a5b0,g~0,g9~z) ~i

1~2 " <

)I(~l )~~ ~ll)(b0,g9,zz

~ b0,gg9~z) ~ (~2

l'~a2)b~,g9~z

~

, , ,

(12)

(~3

~'~a3)(~0,g9,zz

+ ~0,gg9~z) + (~4

~'~a4)~~,g9~z

~

o,~ o,~

(b5

°'~a5)90,g40,ggizl

>, o,~

Ci = < 12ai bo,~g +

2a2bo,~bo,g

+

2a340,~g

+

2a440,~40,g

+

a5(bo,~40,g

+

bo,g40,~)lg,z

>, o,~

C2 - <

H12(bi Iii ai)bo,na

+ 2(b2

Iii

a2)bo>nbo,g + 2(b3

ta3)40,ng

+

2(b4

fia4140,~40,g

+ (b5

(°'~ asl(bo,~40,g

+

bo,g40,~llg,z

>,

o,~ o,~

Di = < 12a340,xg +

2a440,x40,g

+

a590,g40,xlg,z

>, o,~

~2

" <

)[~(~3 jl'~ a3)~0,Xg

~ ~(~4

jl'~ a4)~0,X~0,g

+ (b5

jl'~ a5)~0,g~0,X)9,z

~'

,x ,n ,n ,n

El = <

)ia190n

+

a3'0ni

>,

~~ " <

fi~~~~ IIl ~~l~°~

+ ~~~

IIl ~~~'°~l

>'

~1 1

" <

fa3~0,X

~'

o,~

' ~ ~~

~~~

~~ ~~

Gi

= <

£la190,w

+ a~91,~ +

a340,w

+

a441,~

+

asbo,~40,4

>,

o,~

G2 # <

fii~bi Illl al190nn

+ ~b2

Illl a2191n

+ ~b3

IIl a31'°nn

+

(b4

~°'~

a4)#(

+ (b5

~°'~ a5)90

n

lo

n) >,

90~

n

90~

Hi

o,~

H2 = <

ox on o,~

Ii

o,~

12 #

<

fi12~b3

~ Illl

a3)'0nx + 2~b4

-

Illl a4)'°n'°x + ~b5

~

Illl 5)90n'0xi

~~

/

~

/(9)~

~'

~~

/

~

j/(b)l~

~' ~~~~

which

gives

~°'~

~~~~'

~°'~

~~~°~'

~~~~

(13)

Analogously,

an ~° /l~j

=

an In l~l~~l ax

£~° /l~j

- °,

(41)

[j'° d# (bo)j

~~

x

M(41

~~ ~~

K(~)

40,n

=

M(40)~'~~(jj)~~~~, 40,x

=

(~)j~, 40,g

=

M(40)K'(bo). (42) j~~(~i~~~/~~~~~

~~~~~~~~~~~

~°'~~'~°'~~' ~°'"'~°'~~' ~°'~~'

~°~~x,

40,gg, 40,no, 40,xg

are

simply

References

Ill

Ericksen J-L-, Trans. Soc. Rheol. 5

(1961)

23.

[2] Leslie F.M., Arch. Mecll. Anal. 28

(1968)

265.

[3] de Gennes P-G-, The Physics of Liquid Crystals

(Clarendon

Press, Oxford, 1974).

[4] Leslie F-M-, Adv. Liq. Cryst. 4

(1979)

1.

[5] Leslie F-M-, in Theory and Applications of Liquid Crystals, J-L- Ericksen and D. Kinderlehrer

Eds.

(Springer-Verlag,

New York, 1987) p. 235.

[6] Zuniga I, and Leslie F-M-, Liq. Cryst. 5

(1989)

725; Europllys. Lett. 9

(1989)

689.

[7] Leslie F-M-, in Nematics: Mathematical and Physical Aspects~ J-M- Coron et al. Eds., NATO

ASI Series

(Kluwer

Academic Publishers, Dordrecht, 1991) p. 223.

[8] Krekhov A-P-, Kramer L., Buka A. and Chuvyrov A-N-, J. Pllys. II France 3

(1993)

1387.

[9] Clark M-G-, Saunders F-C- Shanks I-A- and Leslie F-M- Mol. Cryst. Liq. Cryst. 70

(1981)

195.

[lo] see e-g- Bender C-M- and Orzag S.A.~ Advanced Mathematical Methods for Scientists and Engi-

neers

(McGraw-Hill,

New York, 1978).

Ill]

see e-g- Abramowitz M. and Stegun I-A-, Handbook of Mathematical Functions

(Dover,

New

York,

1964).

[12] de Jeu W-H-, Classen W-A-P- and Spruijt A-M-J-, Mol. Cryst. Liq. Cryst. 37

(1976)

269.

[13] Kenppe H., Schneider F. and Sharma N-K-, J. Chem. Phys. 77

(1982)

3203.

[14] Dubois-Violette E. and Rothen F., J. Phys. France 39

(1978)

1039;

Sadik J., Rothen F. and Bestgen W., J. Phys. France 42

(1981)

915.

[15] Belova G-N- and Remizova E.N., Akust. Zh. 31

(1985)

289 [Sov. Phys. Acoust. 31

(1985)

171].

[16] Kozhevnikov E-N-, Zh. Eksp. Teor. Fiz. 91

(1986)

1346 [Sov. Phys. JETP 64

(1986)

793].

[17] Hogan S-J-, Mullin T. and Woodford P., Proc. R. Soc. Lond. A 441

(1993)

559.

[18] Blinov L-M-, Davidyan S-A-, Reshetov V-N-, Subachyus D-B. and Yablonskii S-V-, Zh. Eksp. Teor.

Fiz. 97 (1990) 1597 [Engl. Transl.: Sov. Phys. JETP 70 (1990) 902].

[19] G. Schmidt, Physics of High Temperature Plasmas

(Academic

Press, New York, 1979) Chap. 9A.

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