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Orientational optical non-linearity near the instability of nematic liquid crystal flow over an inclined plane

Yu. S. Chilingaryan, R.S. Hakopyan, N.V. Tabiryan, B. Ya. Zel’Dovich

To cite this version:

Yu. S. Chilingaryan, R.S. Hakopyan, N.V. Tabiryan, B. Ya. Zel’Dovich. Orientational optical non-

linearity near the instability of nematic liquid crystal flow over an inclined plane. Journal de Physique,

1984, 45 (3), pp.413-420. �10.1051/jphys:01984004503041300�. �jpa-00209771�

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Orientational optical non-linearity near the instability

of nematic liquid crystal flow over an inclined plane

Yu. S. Chilingaryan, R. S. Hakopyan, N. V. Tabiryan and B. Ya. Zel’dovich (*)

Physics Department of Yerevan State University, 375049, Yerevan, U.S.S.R.

(Reçu le 20 avril 1983, révisé le 7 octobre, accepté le 27 octobre 1983)

Résumé.

2014

On étudie le problème de l’écoulement d’un nématique sur un plan incliné. Dans le cas où le directeur est ancré sur la surface du plan incliné perpendiculairement à la direction de la gravité et à celle de l’écoulement, on prédit une instabilité spécifique de l’orientation dont on calcule le seuil. On étudie la non-linéarité optique d’orien-

tation du nématique au voisinage du seuil de l’instabilité d’écoulement.

Abstract.

2014

The problem of the gravity flow of nematic liquid crystal (NLC) mesophase over an inclined plane is investigated. In the case when the director of NLC is strongly anchored on the inclined plane surface perpendi-

cular to the gravitational force and flow direction, a specific orientational instability arises for which the flow threshold value is obtained. Orientational optical non-linearity at the threshold of NLC flow instability is investi-

gated.

Classification Physics Abstracts

47 . 20 - 61. 30G

1. Introduction.

The coupling, via viscous stresses, between the direc- tor n and the flow velocity v, is one of the factors which determines the original hydrodynamic properties of

nematic liquid crystals (NLC) [1-5]. Due to this coupl- ing, viscous flow such as simple shear flow or Poi- seuille flow can become unstable even for very low

(10-3-10-4) Reynolds numbers. The instability phe-

nomena of these viscous flows were investigated experimentally and theoretically in detail [1-5]. In particular two types of instabilities are mentioned.

The first one corresponds to a distortion of the director which is uniform in the plane (no; vo) composed of the

undisturbed director and the flow direction. The second one corresponds to a so-called roll instability (with the roll axis parallel to the flow direction Oy).

Both instabilities arise at several critical values of shear rate and the threshold of the first type of insta-

bility is lower than the threshold of the second type.

The problem of ordinary viscous fluid flow over an

inclined plane is well known (see [6], § 5). If the boun-

dary conditions on the lower plane correspond to

strong anchoring but the upper surface of the fluid is free, the velocity profile has the form of the parabola

(*) Institute on Problems in Mechanics, prospect Ver- nadskovo, 101, 117526, Moscow, U.S.S.R.

and it is easy to obtain the dependence of the steady

state thickness of the layer on flow.

The theoretically predicted and experimentally

verified orientational optical non-linearity of liquid crystals [7, 8] is a matter of intensive investigations at

present. In particular in several works (see [9, 10] and

the references therein) NLC optical non-linearity

near the Fredericks transition induced by a magnetic

or electric field is discussed, as well as near phase

transitions between liquid crystals modifications.

In the present paper we consider the problem of

NLC flow on an inclined plane assuming the conditions

of zero velocity and strong anchoring on the plane.

It is shown that for the definite geometry a specific

orientational instability arises at some threshold

value of flow. This threshold value and distortion

profiles are obtained for the case when the velocity

and director distortions are uniform in the plane (no; vo). The orientational optical non-linearity at the

threshold of the considered type instability of NLC

flow over the inclined plane is discussed.

2. Recording of boundary conditions.

A quantity Q (em 3 /s) of the liquid crystal, which is

contained in the xy plane and has a width along the

x axis given by l, continuously flows along the y axis

which is inclined at an angle a with respect to the

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01984004503041300

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414

Fig. 1.

-

Geometry : liquid crystal with thickness h flows

along the direction ey over an inclined plane which makes

angle a with the horizontal. The boundary conditions cor-

respond to no

=

ex.

horizontal. Then at not very high flow velocities (i.e. for not very high Q) steady liquid flow with a

thickness h occurs. If the boundary conditions on the inclined plane (plane z = 0) correspond to a director

orientation along ey (no

=

ey) or along ez (no

=

ez),

then in the whole volume except in a boundary layer

of width ç, where

the molecules will be reorientated by the flow, making

an angle 0s = arctg (--’3/a2) with the axis ey and stay in the plane (y, z). Here K is the average elastic cons-

tant and q the viscous coefficient for the corresponding geometry.

We shall discuss in detail the situation when, on the boundary z

=

0 molecules are anchored along

ex (n°

=

ex). On the same surface the condition on the flow velocity v is v (z

=

0)

=

0. The boundary condi-

tions on the free surface z = h have the form

where Ki are the Frank constants; and (Ja is the sur-

face tension anisotropy. At the free surface the shear stress vanishes and this leads to the first condition in

(1). The two last conditions are obtained by consider- ring the addition to the surface part of the free energy

depending on the orientation having the form A =

0.5 6a(nez)2 [12, 15, 16]. ca = 0 if the surface does not influence the director orientation. In the other limit (fa -> oo the surface strictly orients the director in the

layer plane (if (fa > 0) or perpendicular to it (if 7a 0).

Since we consider a situation where the undisturbed director direction is planar and homogeneous over

the whole volume of the NLC, it is necessary to consi-

der 6a > 0. In this case the orienting action of the free surface supports the director planar orientation.

Such a situation can be experimentally realized with the nematic PAA for example [17,18].

When the flow is very weak the above mentioned orientation (n°

=

ex) will be unperturbed over the

whole volume due to elastic effects. The viscous torque

acting on the director is zero and the viscosity, measur-

ed in this geometry, is fla = 0.5 a4. If we consider the inclined plane to be infinitely long, we obtain from

(A. 14) for velocity profile.

Then the pressure distribution is

It is easy to define the relation between the steady

state thickness h of LC and its quantity of flow Q, giving on the upper part of inclined plane :

All these expressions coincide with those for an ordi- nary liquid by a suitable definition of viscous cons-

tant na-

3. The system of linearized hydrodynamic equations.

Consider a light wave with wave vector and polariza-

tion vector lying in the plane (X, Z), so that K = (Kx, 0, KJ, E

=

(Ex, 0, EJ, and which is incident on

the described system. At sufficiently high flow velo-

cities the stationary profiles of velocity (2) and direc-

tor no are disturbed even without the presence of an

electromagnetic wave.

Let us denote by bn = (0, n r n _,), bv = (’Dx’ ’Dy, CU,- )

and P the orientation, velocity and pressure distur- bances. Equations coupling these disturbances can be obtained by linearizing (A. 12), (A. 14) and the equa- tion of uncompressibility OVi/OXi == Oi Vi = 0. We

carry out the linearization for the problem which is homogeneous in the inclined plane, i.e. we do not

discuss the domain structure (010y

=

0), and the roll

instability (%x = 0). Then we obtain the following

system of equations :

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where the symbol * means complex conjugation; ga = ell jj

-

E1 is the anisotropy of the mesophase dielectric

constant at the light frequency; S is the velocity gradient of the undisturbed flow along z :

fla’ fib are the Miesowicz viscosity coefficients :

The director perturbations lead to the field modification in the medium. However we can consider that in the

equations (4a)-( 4 f) E const. because we are interested in weak perturbations of the director proportional

to the light intensity. In the same approximation the director reorientation does not give rise to an Ey component

of the light field and therefore there is only y component of the torque acting on the director. Thus we only consi-

der (for the stationary problem) the z-dependence of the disturbances. In this case, as for the simple shear or

Poiseuille flows problems, one can show that ’U’y = ’U’z

=

p

=

0 everywhere, which corresponds to a distur-

bance of v(z) of the form bv = ex’U’x(z). From the equation (4c) and boundary conditions at z = 0 and z = h

we have :

With equation (6), equations (4a) and (4b) take the form :

Performing the transformation :

We obtain the dimensionless equations :

In this notation 4J., is determined from the equation :

where CÜx = h.1 (13 I crJx/K1.

Then, using new variables U = a2/3.(ii, + nz), W = a2/3.(ii, - nz) and X

=

all3 Z from (9) we obtain two

uncoupled equations :

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416

The boundary conditions (1) in new variables take the form :

where X1

4. Investigation of flow instability.

General solutions of equations (11 a) and (llb) without an external electromagnetic wave are expressed through

the Airy functions Ai(X ) and Bi(X) [20] :

where A1, A2, B1 and B2 are arbitrary constants. From the boundary conditions (12) we get four homogeneous equations for four unknowns A1, B1, A2 and B2. This system has non-trival solution when its determinant is zero.

Thus we shall find an equation for critical X1, i.e. for critical flow Qc :

where

D1, D2 are constants connected with Az(O) and Bi(O) :

Critical thickness he and flow Q, are expressed through the root Xl of equation (14) :

Consider the influence of the surface forces on the value of the threshold. We present the numerical solutions of equation (14) for the cases far = 0 and Ea -+ oo because we do not know the value of NLC surface tension

anisotroPYO"a.If.Ea = 0 we get from ( 14) (F1 + D 1 ) (F2 + D 1 )

=

0 and, because F 1 (XJ is positive for all Xl > 0

we have F2 = - D1 and, therefore, X@ = 1.98. For example from (16) we obtain h’ 3 sin a = 23.5 gm and cor-

respondingly the critical flow Q 0 "/l l-- 1.04 x lO- 5 cm2 s-t for the parameters characteristic for LC p = 1 g/cm3, K1 = 6 x 10-’ dyne, K2

=

4 x 10-’ dyne, Ila = 0.25 poise, fib = 0.4 poise, a2 = - 0.77 poise, CX3

= -

0.012

poise [ 11 ].

When Ea -+ oo from equation (14) we get F1 = F2, therefore X c = 2.347. We have h 3 sin a 27.85 um

and correspondingly for critical flow we obtain Qoo/l ~ 1.7 x 10- 5 cm2 s-1 for above mentioned parameters.

We obtained that the threshold in the case (Ja -+ oo is somewhat greater than in the case ca = 0. This is connected with the circumstance that the surface force supporting the director undisturbed orientation increases with the increase of the a..

Knowing Xi we can obtain the disturbances profiles near the threshold, up to an indefinite constant multi-

plier. To an accuracy of two decimal places we find :

where A and B are arbitrary constants.

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Let us note that at z = 0 X = X 1 and at z = h X = 0.

’Ù’ x can be found from equation (10) by integrating.

The profiles of disturbances nY’ iíz and ctJ x at Ea = 0, ooare given in figure 2. As can be seen on figure 2 the profile of nz essentially depends on the value of ca in contrast to the quantities ny and ’BJx. This is connected with

the given boundary conditions (1). For obtaining the steady state amplitudes of disturbances above the threshold it is necessary to solve a non-linear problem. We will not discuss such a problem in this paper.

5. Orientational optical non-linearity near a flow instability.

Dividing both parts of equations (l la) and (lib) by I we get equations whose solution is given by the Airy func-

tions Ai(X ), Bi(X ) and Gi(X ) :

where A1, A2, B1 and B2 are constants to be determined from the boundary conditions (12).

Near the threshold of the instability which would have the flow on the inclined plane without a light field, they have the form

where i

In particular in the case of Ea = 0, inserting numerical values for the parameters in (18) and omitting higher order

terms, we have :

When X. 0 0 the critical index for all four parameters AI, A2, B1 and B2 is the same and is equal to - 1. For example when Ma --> oo we have :

Fig. 2.

-

Disturbance profiles nY’ nz at I a

=

0 (a) and ¿a -+ oo (b). Disturbance profile of ’BJ x (c).

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418

6. Discussion.

NLC flow on an inclined plane is considered in the present paper. The instability of such a flow corresponding to

director disturbance depended only on the z coordinate transverse to the layer is investigated. The physical

reason for the instability is the decrease in the effective viscosity with a decrease of the angle between the director and velocity [ 13], and this decrease is the same for positive and negative bn. Mathematically this is connected with

inequalities a2 0, a3 0, a2 I > I a3 I which are valid for most of NLC.

.

On the other hand, orientational forces in the absence of the flow try to hold the director strictly homoge-

neous over the whole volume. When the value of flow (or thickness) is above its critical value, the elastic forces cannot hold stable the homogeneous distribution of the director.

On the contrary in the problem with strong anchoring of the director on the inclined plane perpendicular to

the plane (no

=

ez) or along the flow (no

=

ey) the effective viscosity decrease takes place in the first order of bn,

i.e. it is sensitive to the sign of bn. As usual in these problems, the director disturbances 3n - V appear at small

flows, i.e. the reoriention effect here has no threshold behaviour. Large director disturbances (3n - 1) appear here

approximately at the same value of flow at which the instability arises in the problem with no = ex’

Orientational optical non-linearity near (but below) the instability point of the described type is considered in the present paper. It is shown that perturbations of the NLC dielectric constant bgik

=

ga(n9 I n k + ni no ) critically increases near the threshold of the flow instability as 3£ - (Qc - Q )-1.

Let us give numerical estimations. For a = 0 i.e. in the absence of the flow, for the wave incident angle in the

medium 300 and for the LC-parameters h £ 10-2 CM, Ba = 0.7, K - 10 - 6 dyne we obtain that the director reorientation to an angle - 0.1 rad in the x, z plane is achieved for the incident beam power density

P - 0.1 kW/cm2. Such a power density is available for usual c.w. lasers. The increase of a and the approach to

the hydrodynamic flow instability threshold at a fixed thickness leads to the decrease by a factor 6c/(6c " Q )

in the power density, required for the given director reorientation.

From our point of view it will be interesting to experimentally find the predicted instability, to measure its

threshold and to investigate orientational optical non-linearity near the instability point.

Acknowledgments.

The authors are grateful to G. E. Volovik and E. I. Kats for useful discussions.

Appendix.

DISSIPATIVE FUNCTION FOR UNIAXIAL NEMATICS TAKING ACCOUNT OF THE HYDRODYNAMIC MECHANISM OF RELAXATION.

-

In order to obtain the expression for the dissipative function of uniaxial nematics, let us use the properties which the material must have :

1. As free energy F, dissipative function R also must be even in n (n is NLC director).

2. If the velocity gradients and the velocities themselves are not very high, it will be sufficient to let R depend on

terms of the order (ðVi/ðxk)2 and less.

3. R must vanish when the liquid uniformly rotates as a whole because it is clear that under such rotation there must not be any friction in the liquid. Therefore the dissipative function can depend only on the tensor dij and the

vector X which become zero for such a rotation :

4. There must not be terms in R not depending on dij and JM because at v = const. and dn/dt = 0, R must

vanish.

5. The dissipative function must be non-negative and therefore cannot consist of terms linear in dij and X.

The most general form of the dissipative function (of uniaxial NLC) having the above mentioned properties is

For uncompressible NLC (did = 0) we have

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Since n2 = 1 the Lagrangian of NLC can be written as :

The first term represents the kinetic energy density (p is the density); Fd-Frank’s elastic energy; F f-describes the

free energy of interaction between the director and the external field; Fo-the internal free energy depending on density. In (A. 4) we also introduce notations h-Lagraqge multiplier, P-hydrostatic pressure and u-the linear

displacement of the liquid particle, du/dt - v.

The equations of motion can be obtained from (A. 2), (A. 4) and from the variational equation :

Here qi = ni, Ui,

The obtained equation are called the Ericksen, Leslie and Parodi (ELP) equations. Before writing down

these equations let us give the expression for the viscous stress tensor :

Comparing (A. 6) with known (see for example [11]) expressions for U’ki we obtain the relations between the Leslie and Jli coefficients :

It is seen from (A. 7) that the Parodi relation (a6

=

a2 + a3 + a5 ) is only the result of dissipative function (A. 3 ) consisting of only five independent terms. Insertion of the sixth coefficient leads to the additional relation.

In order to define the inequalities arising because of the non-negativity of quadratic form (A. 3) it must be

reduced to the diagonal form. For this, one must separate tensor dij into irreducible components in relation to the one-parameter group of rotation around the axis n (compare with [14]) :

where do

Then for quadratical form (A. 3) we have

The following inequalities are obtained from this :

For obtaining the fifth inequality let us write :

Consequently the fifth inequality has the form :

JOURNAL DE PHYSIQUE.

-

T. 45, N° 3, MARS 1984

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420

For writing the ELP equations we will suggest that the liquid is in the gravitational and electromagnetic fields

where g-the gravitational acceleration, ga = 9 11

-

G 1. is the dielectric permittivity anisotropy. Then equations for

the director components n obtained from (A. 3) and (A. 4) have the form

Varying expressions (A. 3) and (A. 4) by u and using the formula (see [11]) :

We get the balance equation of forces acting on a liquid particle

Equations (A 12) and (A 14), along with the incompressibility condition div v

=

0, constitute a self-consistent system of equations for defining p, v and n.

References

[1] PIERANSKI, P., GUYON, E., Phys. Rev. A 9 (1974) 404.

[2] MANNEVILLE, P. and DUBOIS-VIOLETTE, E., J. Physique

37 (1976) 1285.

[3] JANNOSSY, P., PIERANSKI, P. and GUYON, E., J. Physique 37 (1976) 1105.

[4] MANNEVILLE, P., DUBOIS-VIOLETTE, E., J. Physique 37 (1976) 1115.

[5] DUBOIS-VIOLETTE, E., DURAND, G., GUYON, E., MAN-

NEVILLE, P. and PIERANSKI, P., Liq. Cryst., Solid

state Phys. Suppl. 14 (1978) 147.

[6] LANDAU, L. D. and LIFSHITZ, E. M., Mechanics of

Continuous Media (Oxford, Pergamon Press) 1954.

[7] ZEL’DOVICH, B. Ya., TABIRYAN, N. V., Pisma ZHETF 30 (1979) 510 (JETP Lett. 30 (1979) 478).

[8] ZEL’DOVICH, B. Ya., PILIPETSKI, N. F., SUKHOV, A. V.

and TABIRYAN, N. V., Pisma ZHETF 31 (1980)

287 (JETP Lett. 31 (1980) 263).

[9] HERMAN, R. M., SERINKO, R. J., Phys. Rev. A 19 (1979)

1757.

[10] HAKOPYAN, R. S., TABIRYAN, N. V., ZEL’DOVICH, B. Ya., Cristallografia 28 (1983) 973.

[11] DE GENNES, P. G., The physics of Liquid Crystals (Clarendon Press, Oxford) 1974.

[12] ZEL’DOVICH, B. Ya., TABIRYAN, N. V., ZHETF 79

(1980) 2380 (Sov. Phys. JETP 52 (1980) 1210).

[13] CARLSON, T. and SKARP, K., Mol. Cryst. Liq. Cryst.

78 (1981) 157.

[14] ZEL’DOVICH, B. Ya., ZHETF 63 (1972) 63 (Sov. Phys.

JETP 36 (1973) 39).

[15] MADA, H., Mol. Cryst. Liq. Cryst. 51 (1979) 43.

[16] MADA, H., Mol. Cryst. Liq. Cryst. 53 (1979) 127.

[17] BOUCHIAT, M. A. and LANGEVIN-CRUCHON, D., Phys.

Lett. 34 (1971) 331.

[18] CHIARELLI, P., FAETTI, S. and FRONZONI, L., Lett.

Nuovo Cimento 36 (1983) 60.

[19] ABRAMOWITZ, M. and STEGUN, I. A., Handbook of

Mathematical functions. National Bureau of Stan-

dards, Applied Maths Series 55, Washington DC,

U.S.A., 1964.

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