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Non linearities close to the thermal threshold in a planar nematic liquid crystal
E. Dubois-Violette, F. Rothen
To cite this version:
E. Dubois-Violette, F. Rothen. Non linearities close to the thermal threshold in a planar nematic liquid crystal. Journal de Physique, 1979, 40 (10), pp.1013-1023. �10.1051/jphys:0197900400100101300�.
�jpa-00209178�
Non linearities close to the thermal threshold in a planar
nematic liquid crystal
E. Dubois-Violette
Laboratoire de Physique des Solides, Université Paris-Sud, Centre d’Orsay, 91405 Orsay, France
and F. Rothen
Institut de Physique Expérimentale, Université de Lausanne, CH 1015 Lausanne Dorigny, Switzerland
(Reçu le 12 avril 1979, accepté le 29 juin 1979)
Résumé.
2014On étudie les non-linéarités dans l’instabilité thermique induite dans un échantillon nématique planaire
chauffé par en bas. On caractérise d’abord le comportement critique en utilisant un modèle avec des conditions
aux limites libre-libre. On étudie ensuite les propriétés au-dessus du seuil en utilisant un développement en pertur- bation. On montre que le premier coefficient R(1) du développement du nombre critique est nul. On calcule l’ampli-
tude des perturbations au-dessus du seuil et on trouve que pour la plupart des nématiques la bifurcation est normale.
Abstract.
2014We study non linearities in the thermal instability induced by heating a nematic liquid crystal from
below. First a model with free-free boundary conditions is studied. Critical behaviour of the free-free model is
analysed. Properties above the threshold are determined with use of perturbation analysis. One shows that the first expansion coefficient R(1) of the critical number vanishes. One determines in an approximate manner the amplitude of the disturbances above the threshold and finds that for most nematics the bifurcation is normal.
Classification
Physics A6stract,s
61.30
-47.20
1. Introduction.
-In previous works [1], [2], [3],
one of us (E.D.V.) has studied the thermal stability
of a planar or homeotropic nematic sample submitted
to a thermal gradient. Here we shall only consider
the stationary instability which appears in a planar sample heated from below with a periodic pattern
corresponding to rolls with a wavelength of the
order of the sample thickness d. We shall consider neither the stationary instability which occurs in a homeotropic sample heated from above nor the oscillatory one when heated from below [4]. A standard
normal mode linear analysis has allowed to determine the threshold [5]. Experimentally one gets results above the threshold which remain unexploited in a
linear analysis.
A study of non linearities has been performed
elsewhere [10] in a liquid crystal for the case of an instability induced by a simple shear where a homo-
geneous distortion of the nematic appears. In this paper we shall give an approximate method in order
to estimate the disturbance amplitude close to the
threshold and study the nature of the bifurcation.
If the threshold corresponds to a normal bifurcation (see Fig. 2b) the amplitude of the disturbances decays slowly as one approaches the threshold. In the vicinity
of the bifurcation, perturbation methods can be used
to describe the system and to determine the amplitude
of the disturbances. Such a description, valid for
small disturbances, has been sketched for an isotropic liquid by Landau [7] and Stuart [8] and is related in a
review paper [9].
Let A be the amplitude of a disturbance (for example
the fluid velocity) that becomes unstable at the
Fig. 1.
-A planar nematic sample is submitted to a thermal gra- dient. The temperature of the lower plate is Tr + AT and the tem- perature of the upper one is Tr. ç is the angle in the plane xOz of the molecules with the x direction.
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:0197900400100101300
threshold. In our case the threshold will be characte- rized by the temperature difference AT between the two plates of the sample (Fig. 1). As long as we are
concerned with the stationary case where no oscilla-
tions occur (exchange of stability) one can consider
the amplitude A and the time evolution rate 0’ as real.
Close to the bifurcation one assumes that the evo-
lution equation of A is of the following form :
0’ characterizes the slowing down of the disturbances close to the transition and is of the form [11]
R is some dimensionless parameter. R - Rc cha°rac-
terizes the departure from the threshold Rc. In our
case one can define R = Ô.T/Ô.Tc.
For AT > 0394Tc, 03C3 is positive and fluctuations grow
exponentiàlly. On the contrary, for 0394T AT,,, u 0
and there is a damping of the disturbances.
’t 0 is a positive quantity determined by the linear theory, which defines the linear growth rate of the
disturbances near the threshold.
kc is the wave vector of the marginally stable state
at R = Rc. Above the threshold, perturbations with k # kc can occur for an infinite horizontal layer :
this is described by the second term of the right hand
side of eq. B(1.2). The influence of lateral boundaries will depend on a characteristic length 03BE defined in [11] :
where 03BEo is determined by the linear theory.
The presence of a quadratic term in eq. (1.1) depends on the symmetry properties of the convection pattern corresponding to the change A ~- A.
If a # 0 the bifurcation is not normal : deviations
can be amplified under the linear threshold (Fig. 2a).
There is hysteresis between Ro and Rc.
The situation is similar to a first order phase tran-
sition when a cubic term appears in the expansion of
the free energy. In section 4 we shall demonstrate that in our case no such quadratic term is present and for similar symmetry properties every even power of A vanishes in eq. (1.1) (a = c = 0...). One is left with a discussion on the sign of the coefficient b :
-
For b 0 one can reach a stationary stable
solution
which decreases as (R - Rc)1/2 close to the threshold.
This case corresponds to a direct bifurcation and reminds a second order phase transition behaviour where the order parameter would be the velocity.
The behaviour is compatible with mean field theory
where the critical exponent fl = 1/2. Here we shall
Fig. 2.
-Different bifurcations. a) The bifurcation is inverse due to the non equivalence of fluctuations A and - A in the system.
b) The bifurcation is normal. The amplitude goes continuously to
zero as one approaches the threshold. c) The bifurcation is inverse.
A and - A are equivalent, but the system is unstable against distur-
bances of finite amplitude. The doted lines correspond to an unstable
branch. The full line corresponds to a stable branch.
not consider the thermal fluctuations close to the threshold as introduced by several authors in isotropic liquids [12], [13]. An estimation of these fluctuations close to the threshold of an instability induced by a
shear in a nematic liquid crystal indicates that they
are likely not observable [10].
-For b>0
Eq. (1.1) has two kinds of solutions. One solution goes to zero as Q tends to zero and corresponds to an
unstable branch as indicated with a doted line on
figure 2c.
For R > Ro = R, - b’12 yro ’, one gets finite
amplitude instabilities corresponding to a stable
branch (full line on figure 2c). At 6 = 0 the amplitude
is A = ± Jbjy (y is supposed to be positive). This
case corresponds to an inverse bifurcation and hyste-
resis is expected between Ro and R,,. This situation may be compared to a first order phase transition.
An important point in order to determine the nature
of the transition is the sign of the b coefficient. The
condition a = 0, b 0 is necessary to get a normal
bifurcation. This condition will be the right one if one
proves that the threshold determined by the linear
theory is the correct one. A criterium of global stability
such as the energy method [6] will give such a proof.
But as long as the experimental results agree with those determined by the linear theory we shall assume this
last point to be true. Then the nature of the bifurcation will be determined by the sign of the coefficient b.
Let us now indicate how we shall proceed for such a
determination. From a mathematical point ofview, the
resolution of the problem depends strongly on the boundary conditions. For isotropic liquids a stress-
free boundary model (we shall refer as free-free case)
is very popular since it leads to very simple mathema-
tical solutions [9]. In nematics the free free case also
leads to simple analytical solutions. In section 2 we
shall develop the analysis of the free-free case and give
the solutions of the linear problem. We will also cha-
racterize the critical behaviour and determine the two
quantities ro and 03BEo. In section 3 we present the general features of the non linear formulation. In section 4 we develop a perturbation analysis in order
to demonstrate that R(l) = 0. Then we present an approached method in order to compute the dis- turbance amplitudes and to determine the nature of the bifurcation.
2. Critical behaviour of the linear régime.
-From
a formal point of view, the hydrodynamic equations governing a disturbance away from the basic flow
can be written under the form
where £ is a linear differential operator and NU represents the non linearities. U is a vector notation.
In our case the U components (p represent 0 the
(03B8 ~ vz) vz
temperature disturbance 0, the angle (p between the director and the x direction (Fig.1 ) and the velocity v,,.
As we are concemed with a stationary instability, DUIat = 0.
Linearized hydrodynamic equations governing the stability of the conductive state have been given in
ref. [5]. Let us define the temperature at the lower plate
as
and at the upper plate as
AIT > 0 (or AT 0) will l correspond to a sample
heated from below (or from above). The temperature
gradient at the threshold is
Using eqs. (2.1), (2.2), (2.3), (2.4) and notations of ref. [5] one can explicitly write the linear problem
£U(1) = 0 as :
with
The operator 04 has been obtained after elimination of the pressure from the force components fx and fz.
11 p is defined by the above expression. The transverse velocity v,, also disappears with use of the continuity equation
where the derivate a/ax has been used in order to eliminate vx.
The second line corresponds to the heat equation.
The third one reads or yi ax where fy is the total torque
(viscous + elastic + ...) exerted on the molecules for which one assumes an isotropic elasticity cha-
racterized by an elastic-constant K. At threshold a
periodic distortion appears and one looks for solutions which are periodic in x with wave vector qx. For the planar case, the x direction is defined by the molecule
orientation at the upper and lower plates of the sample.
Solutions of system (2.4) depend on the boundary
conditions. Exact solutions have been given in ref. [5].
In order to get tractable non linear calculations, we shall not use the exact solutions but consider some
simplified model. Simple solutions (one mode in z)
are obtained if one considers a stress-free model where all real boundary conditions are taken into account except on the transverse velocity vx. This model usually calledfree-free case has been largely
considered in isotropic liquids [14], [15]. The corres- ponding boundary conditions are :
An exact condition on vx should be :
Such a free-free model largely simplifies the compu- tations, since one easily obtains simple analytical
solutions. This model defined by eq. (2.6) is quite
reasonable for the planar case where the transverse velocity does not play a very important role, since the dominant viscous torque acting on the molecules is a avZ. On the contrary in the homeotropic case the
~x
dominant viscous torque q is ll2 2 az. ~z Viscous effects
are not well described in a model where the z depen-
dence of the vx velocity profile is badly taken into
account. Then this model is not appropriate to describe
the homeotropic configuration. In that case one should
solve the exact boundary condition (2. 7) on Vx.
Solutions of eqs. (2.4) with boundary conditions (2.6) are, apart from a normalization constant,
where
The continuity eq. (2. 5) imposes
2. 1 THRESHOLD. - The compatibility condition of system (2.4) leads to the marginal curve as a function of the parameters x = qx/qz
where
The result (2.9) is an approximation valid when
ka ~ > K (~ is a typical viscosity coefficient). This
last condition is realized for all real systems.
A typical marginal curve is drawn on figure 3.
Computation has been done for MBBA where nume-
rical constants are heat diffusivities
elastic constant A = 6 x 10-’ CGS and viscosities
a6 is determined by the Parodi relation [18]
Fig. 3.
-Theoretical marginal curve of the thermal instability in a
nematic sample in a free-free model. àT > 0 (or 0) corresponds
to a sample heated from below (or above). Point B corresponds to
the threshold with circular rolls..x = qx/qz.
Point B corresponds to the threshold minimum value of ~T of the simplified model
It only gives a crude estimation of the exact threshold
given in [5] which corresponds to (~Tc d 3) = 2.6 x 10- 3 and Xc = 0.95. The discrepancy of the threshold comes
from the fact that a little difference in the estimation
of the qz wave vector modifies strongly (- q4z) the
threshold value. For small values of x, expression (2.9) changes its sign with ax, then point A would correspond
to an instability induced by heating from above (DT 0), with a structure of rolls, deeply flattened
in the x direction. Such a situation has also been
reported in an approximate resolution of the linear threshold with use of a Galerkin method written to the lowest order of the expansion [16]. In such flattened
rolls the velocity gradient ~vxl~z is largely enhanced.
Such a situation cannot be reasonably considered
in a simplified model where the v,, velocity is very
badly sketched. Then in the following we shall restrict
our attention to circular rolls (À-x 1’-1 2 d) correspond- ing to the B point of the diagram and omit the A point
which should be studied in a model taking into account
a more realistic boundary condition on v,,.
2.2 CRITICAL SLOWING DOWN. - Near the threshold the intensity of the scattered light depends
on fluctuations of the director curvature. It is then easy to measure the decay or growth rate of such
disturbances. Near the threshold one expects a linear
growth rate of disturbances Q behaving as R - Rc.
Let us write them as :
where 03B8(1), ~(l) and v(1) z are the solutions given in eqs. (2.8).
0’ is the smallest root of the equation
(one looks here for Q real).
Eq. (2.11) is of the third order in 0’, but the root
width the smallest 1 a is easily determined
Using the inequality k~/ k >> 1 and the expansion
of the marginal curve close to the threshold :
where dqx = qx - q, (q,, is the critical wave vector
corresponding to the critical value Xc = qc/qz), one
obtains
To, which defines the critical slowing down, is obtained by identification with eq. (2.12)
where close to the threshold the last term inside the brakets reads
For circular rolls where x - 1 the last term is
negligible. The sum of the two first terms of eq. (2.14)
is normally positive. ’t 0 is scalled by the time
characteristic of the orientation relaxation.
For the critical value xc = 0.795, 7:o/T = 0.35.
2. 3 INFLUENCE LENGTH.
-The stability marginal
curve defines the interval of wave vectors qx close to qc where the system is linearly unstable (Fig. 3). At the threshold Rc, for an infinite (without lateral walls) box, the wave vector is well defined and is equal to qc.
For a finite box the amplitude of fluctuations is not any more constant in an horizontal box. It needs to
adjust itself to lateral boundary conditions. The influence of lateral boundaries can be characterized
by an influence length 03BE which behaves like [11]
where Ço results from the expansion of the marginal
curve close to qc (eq. (2.13)).
After some algebra one obtains :
with
This leads for x = Xc to
3. Perturbation approach to non linearities.
-In the case of stationary convection 0’ is real. The steady
state corresponds to the solution of
At the threshold Rc the solutions U(1) of the linear problem are defined by :
Above the threshold, at a value defined by R, U(l) is
neither solution of the linear problem :
nor solution of the non linear one (eq. (3 .1 )). The
non linear terms in eq. (3.1) are very complicated, particularly in liquid crystals. So instead of solving exactly eq. (3.1) we look for approximate solutions.
Different methods can be used. We shall indicate the basic line of two of them we shall use in the follow-
ing. A perturbative method used very often [14], [15]
has allowed to solve the non linear Rayleigh-Bénard
case. It is sketched as follows : one searches solutions U at a given value R, developed as a series of a small
parameter 8
Eq. (3.1) has to be solved at each order of the
expansion. To the first order this reduces to eq. (3.2) and U(l) is the solution of the linear problem. To
higher order, a solubility condition of eq. (3.1 ) reads at order n :
where U(l) is the solution of the adjoint problem :
g(n) denotes the nth order term of g.
In the following we shall consider a roll system with the axis parallel to the y direction and then all
quantities will be y independent.
The scalar product is then defined as :
Ax is the wavelength in an horizontal plane, d is the sample thickness. In the following we shall use the
notations :
Solutions 0(1) of the adjoint t + are defined with the following boundary conditions :
and solutions of system (3.6) with boundary condi-
tions (3.5) read :
where
A complete iterative resolution of the perturbative problem will proceed as follows : to the jth order the solvability condition (3.4) determines R(j-l). The
resolution, at the jth order of eq. (3.1) gives the
solutions U(j) and so on. In the next section we shall
only write the second order term of eq. (3.4) in order
to show how the symmetry properties of the convective flow allow to set R(l) = 0 and then justify the absence of a quadratic term in eq. (1.1). In order to determine the leading term of the disturbances written as
R-R R(2) C R(2) one should solve, , to the second order, , eq. q (3.1) ( )
in order to determine U(2 ) and report the solutions in eq. (3.1) written to the third order in order to calculate R(2). This calls for an exact solution of eq. (3.1). Such perturbative analysis will be developed
in another paper. Here we shall restrict our attention
to a much simpler method which only needs the knowledge of the solutions U(l) and allows to deter-
mine in an approximate manner the disturbance
amplitude and indicates the nature of the bifurcation.
This approximation follows Stuart’s method [8] as exposed in Chandrasekhar’s book [17]. Instead of
solving exactly eq. (3.1) one searches approximate
solutions U. One assumes that, above the threshold, the motions and the distortions of the liquid crystal are
similar to those appearing at the threshold, as is experimentally observed. Then disturbances will be taken of the form
U = AU(l).
Furthermore, one takes into account the modifica- tions of the mean > vertical thermal gradient due
to non linearities. This last point will be exposed in
detail in the next section. But the principal feature is
the following : just at the threshold the mean
vertical thermal gradient is constant. Above the
threshold this gradient is no more constant in the sample thickness but is reduced by convective effects.
In an isotropic liquid this modification depends on the
ratio of the thermal diffusion time Tth and of the
convective time Tconv and reads [17] :
where g(z) is a function of z depending on the fluc-
tuations profiles at the threshold. A similar modi- fication will also appear in nematics. But we shall
see that the essential non linearities will concern the orientation disturbance which is the slowest relaxing
variable.
4. Non linear régime.
-Non linearities in liquid crystals are much more complex than in isotropic liquid. First we get non linearities due to convective terms as in isotropic liquid. The term v.V(v) can in fact be neglected since we are dealing with sample
of large Prandtl number (P - 103). The thermal convective term v.V(T) will reveal also negligible compared with non linear terms characteristic of
liquid crystals. The non linearities are due to the fact that :
-
the viscous stress tensor depends on both the velocity gradient and the director n [18],
-
the elastic stress tensor depends on n,
-