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Critical damping of first and second sound at a smectic A-nematic phase transition
F. Jähnig
To cite this version:
F. Jähnig. Critical damping of first and second sound at a smectic A-nematic phase transition. Journal
de Physique, 1975, 36 (4), pp.315-324. �10.1051/jphys:01975003604031500�. �jpa-00208256�
315
CRITICAL DAMPING OF FIRST AND SECOND SOUND
AT A SMECTIC A-NEMATIC PHASE TRANSITION (*)
F. JÄHNIG
Max-Planck-Institut für biophysikalische Chemie
34 Göttingen-Nikolausberg, Germany (Reçu le 15 juillet 1974, révisé le 2 décembre 1974)
Résumé.
2014On étudie à partir d’une théorie hydrodynamique généralisée les modes propres au
voisinage de la transition de phase smectique A-nématique. Il est nécessaire de tenir compte des
mouvements non hydrodynamiques du paramètre d’ordre du smectique et du directeur qui se ralen-
tissent à la transition de phase. Ceci conduit, en accord avec les résultats expérimentaux existants,
à une anisotropie spéciale de l’atténuation du premier son et du deuxième son. On discute la dépen-
dance en température de l’atténuation critique en la comparant aux résultats expérimentaux récents
sur les viscosités critiques.
Abstract.
2014Starting from a generalized hydrodynamic theory the eigenmodes in the vicinity
of a smectic A-nematic phase transition are derived. It is necessary to take account of the non-
hydrodynamic motions of the smectic order parameter and the director which slow down at the
phase transition. This leads to a special anisotropy of the critical damping of first and second sound which agrees with existing experimental results. The temperature dependence of the critical damping
is discussed in comparison with recent experimental results on the critical viscosities.
LE JOURNAL DE PHYSIQUE TOME 36, AVRIL 1975,
Classification Physics Abstracts
7.130
1. Introduction.
-Considerable work has been done to investigate the smectic A-nematic phase
transition. Up to now mainly the pretransitional
effects due to fluctuations of the smectic order para- meter in the nematic phase have been considered.
They show up statically in the divergence of some of
the Frank elastic constants at the phase transition TAN,
as predicted theoretically by de Gennes [1], and dynamically in the divergence of some of the Leslie
viscosities, as predicted by Jâhnig and Brochard [2]
[JB] and McMillan [3]. The dynamical behaviour
of a smectic A on both sides of the phase transition
was treated by Brochard [4] applying dynamical scaling theory. She was mainly interested in the temperature dependence of the critical eigenmodes
in the hydrodynamic regime and their wave vector dependence in the critical regime. In the present paper we want to investigate in more detail the aniso-
tropic properties of the eigenmodes in the smectic
phase in the hydrodynamic regime. Special attention
will be given to the critical damping of first and second sound.
As a theoretical framework we use the unified (*) Supported by the Deutsche Forschungsgemeinschaft.
Presented partially at the Fifth International Conference on
Liquid Crystals, Stockholm, June 17-21, 1974.
hydrodynamic theory for crystals, liquid crystals and liquids of Jâhnig and Schmidt [5] [JS]. They gave
already the application to nematics. For our problem
this has to be generalized to include the complex
smectic order parameter t/J. Its magnitude §o is a nonhydrodynamic variable. Its phase is a nonhydro- dynamic variable in the nematic phase, but in the smectic phase it is a hydrodynamic variable, the displacement u, of the layers. The orientational
displacements of the molecules, the director displa-
cements «5n_b behave in the opposite sense being a hydrodynamic variable in the nematic phase and a nonhydrodynamic variable in the smectic phase (more exactly the transverse part of c5n .L). As the nonhydrodynamic variables slow down at TAN they
have to be included in the set of dynamical variables
for our problem. As a special case, the theory pre- sented includes also the hydrodynamics of smectics A which has already been given by de Gennes [6], and
more recently by Martin, Parodi and Pershan [7]
as one application of their unified hydrodynamic theory.
The introduction of the displacement u., yields
an elastic coupling between translational and orien- tational displacements, and anisotropy in compres- sional behaviour, as shown in section 2. Dynamically
it implies a further dissipative process, the permea-
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01975003604031500
tion. This effect is introduced together with the set
of equations of motion for all dynamical variables in section 3.
The influence of the thermodynamic fluctuations of the modulus of the order parameter on the dyna-
mics of a smectic A will be taken into account by
the critical contributions to the elastic constants and viscosities. The critical contributions calculated
by JB for T > TAN have the same critical behaviour at T TAN. An additional contribution exists below
TAN which is shown to diverge also in the same way.
These effects will be discussed together with the generalization of the work of JB to compressible
systems in Section 4.
The eigenmodes are presented and discussed as to their critical behaviour in section 5. Finally,
in section 6 the results for the damping of first and second sound are compared with experimental results.
In this connection we also discuss some recent expe- rimental results on the critical behaviour of the twist viscosity y1.
2. The elastic energy.
-To derive the elastic energy Fel of a smectic A phase we define the dila-
tion 0 (in volume), the displacement u. of the layers lying in the xy plane, and the angular displacements [5]
CPx and CPy of the axes of the molecules. In the general expression for the elastic energy Fei as a quadratic
function of the strains
only the terms including 0, Uz, CPx or (py have to be
kept as finite contributions. Because of the appea-
rance of the strain r which is typical for smectics [8]
we show the derivation of the elastic energy in some
detail.
In general the elastic energy can be written as
where Gijk is the Levi-Civita tensor. P, nô, IIaJ, and Tij
are defined as conjugate variables and can be express- ed as
For the uniaxial symmetry of a smectic A phase the nonvanishing components of the elasticity tensors C, E, G, and H are [8]
The components of Kijkl are the Frank elastic cons- tants [5]. A further condition on the elastic constants is imposed by the invariance of the elastic energy under a homogeneous rotation of the layers and the
molecules (staying normal to the layers in equili- brium)
The constants Ci, El, E2, E3 and H2 have to be set equal to zero as they give rise to terms containing
variables other than 0, uZ, and p y. Eqs. (2.2) then yield
where we have substituted C2 = C, E5 = B, and Hl = H. As 1Ij in eq. (2. 5) has no diagonal part,
P can be identified with the pressure, and the stress
acting on the centers of mass of the molecules is
given by
The result for the elastic energy is, if we further-
more introduce the director n = no + ôn, with bnx = (py and ôny = - PX,
with
The elastic constants Hi = G describe the elastic
coupling between the centers of mass and the axes
of the molecules, by which smectics differ from nema- tics. In nematics, this coupling is purely dissipative
and the viscosities y, and 72 are the dissipative coun- terparts to Hl and G, respectively.
JS set up a unified hydrodynamic theory without introducing displacements. For a definite phase, meaningful displacements can be defined and used to express the elastic energy. This is shown for a
smectic A phase in Appendix A, the result being
eq.(2.6).
317
In order to investigate our system in the vicinity
of the smectic A-nematic phase transition, we must generalize the elastic energy to include the smectic order parameter t/J. This generalization has already
been given by de Gennes [1] in form of a Ginzburg-
Landau expression
where qS = 2 nld, and d the interlayer distance.
In the ordered phase the complex order parameter
can be decomposed into its magnitude t/lo, and its phase determined by the displacement u.,
Inserting this equation into eq. (2. 8) it is easily seen
that the energy connected with the variables 0, Uz, and c5n.l is identical to the above result eq. (2.6),
under the substitutions
3. The équations of motion.
-For the determina- tion of the eigenmodes we need the equations of
motion for the dynamic variables by which we
describe our system. These are the particle density p
or the dilation 0 related by p = po(1 - 0), the
momentum p, the angular displacements qJx and qJy, the displacement Uz, and the magnitude t/J 0 of the
order parameter. We shall neglect thermal variables.
The equations of motion for the variables 0, p, qJx, and qJy are known from the hydrodynamics of nematics which we will use in the formulation of JS.
The motion of uz, being hydrodynamic below TAN,
was treated within the hydrodynamic theory of Martin, Parodi, and Pershan [7]. With this motion
a further dissipative process is connected, the per- meation. It has not been taken into account by JS
but can easily be treated within their framework
as shown in Appendix B. The result is given by the equation of motion for Uz
where v is the velocity and Âp is the permeation cons-
tant.
The dynamic behaviour of the order parameter t/1 0
is usually assumed to follow a simple relaxation law
The relaxation time i has been discussed by Bro-
chard [4].
Far below TAN one can eliminate the fast non-
hydrodynamic motions of the variables g/o and bOi by the conditions
The latter condition states that the molecules are
fixed normal to the layers. It implies that the trans-
verse part of l5n.l vanishes ; the longitudinal part is still a hydrodynamic variable. Under the conditions eq. (3.3) our theory reduces to the hydrodynamic theory of smectics A.
From the work of JB for T > TAN we know that
the motion of t/J 0’ its dynamical fluctuations, yields
contributions to some of the Frank elastic constants and viscosities which diverge at TAN. For T TAN, essentially the same critical contributions arise from the fluctuations of t/J o. Therefore we will take account
for the motion of t/Jo by keeping these critical contri- butions which will be investigated in more detail
in the next section.
The complete set of equations of motion is then
given by
where the dissipative stress tensor TCij = rc1j + n’ij
was split up into its symmetric and antisymmetric
parts. Explicit expressions for them define the vis- cosities (presented without restriction to critical
ones)
with
(In JS Yi and y2 were called (j and - v, respectively.)
These viscosities are related to the ones used by Mar- tin, Parodi, and Pershan [7] by
4. The critical elastic constants and viscosities.
-Above the phase transition the critical contributions to the Frank elastic constants and the viscosities have been calculated for the incompressible system by JB
where jjj Il = (2 aM v) - 1/2 is the coherence length
in the z direction, z the relaxation time of the order parameter and T the temperature with Boltzmann’s constant KB = 1. Just those viscosities, for which
an elastic counterpart, E4 = G = Hl and E5, has
been introduced in section 2 for the description of
a smetic A, show a critical behaviour.
We don’t want to give a rigorous derivation of the critical effects for T TAN, but rather discuss the
qualitative features. As an example we treat the
critical contributions to y,. Following JB we start
with the expression for the stress tensor compo- nent IIZx, eq. (2. 5c) with the substitution eq. (2.10c).
Splitting up the order parameter t/J 0 in its mean
value t/Joo and the fluctuating part liÍo,
11, "Il, r w , 1.. -,
we find with
The first term 1Ii represents the ordinary hydrody-
namic stress, whereas llzx and 1I.-X are due to fluctua- tions tÍ o.
The last term ÎIZx corresponds to the stress tensor
component used by JB for the calculation of Y1
at T > TAN. Below TAN it will yield a contribution y1 with the same critical behaviour
This symmetry of the fluctuation effects, with respect
to TAN, is already known from the analogous pro- blem of superconductors [9, 10].
The second fluctuating term Îlzx exists only for
T TAN, as it is proportional to yGoo, and gives
rise to an additional critical contribution yi. The
Kubo formula for Yi is given by
This thermal average can most simply be evaluated
on working with the nonhydrodynamic variable tPx = Oxuz + c5nx instead of the variables Uz and c5nx separately. Dynamically px describes a relaxation with
and c5Yl = Yi + 00FF 1, as can be seen from eq. (5. 6).
The static fluctuations of 4>x are given approximately by
Following the lines of JB we get from eq. (4.6)
and with 1 tfro(K) 12 ) ~ (K2 + C-2)- ’ and eq. (4. 8)
Inserting eq. (4.7) this relation is fulfilled for
Critical contributions of this type were introduced first by Landau and Khalatnikov [11]. î, and yi
show the same behaviour, as discussed already for
the Â-transition in He by Hohenberg [12]. The complete
critical contribution at T TAN’
319
therefore has the same critical temperature divergence
as i for T > TAN. This symmetry would also follow from dynamical scaling [4].
The term 1IÀ, eq. (4.4a), and the corresponding
terms of the other stress tensor components are independent of the fluctuations §o and linear in the
displacements. They represent the ordinary hydro- dynamic stresses and will be used in Section 5 for the calculation of the eigenmodes.
If we wanted to calculate the director response function QafJ defined by [2] ]
the fluctuations of Uz arising from the first term in eq. (4.4a) would contribute to Qap. We only
mention that these fluctuations would serve to make the static director response function purely transverse
in the limit q --+ 0
(We introduced the assumption MT = Mv which
can be avoided by a scale transformation in momen- tum space.)
As spatial symmetry does not change at T AN,
the other critical viscosities and elastic constants, eq. (4.1), diverge for T TAN in the same way as for T > TAN.
For a generalization of our results to a compressible
system, it is sufficient to continue the work of JB at T > TAN because of the symmetry of the fluctua- tion effects. The two additional viscosities by which
a compressible system is described in comparison
to an incompressible system are critical
as shown explicitely in Appendix C. ôtll and 8r3 depend on the existence of the coupling constant C.
The critical behaviour of the permeation constant
we take from dynamical scaling [4]
5. The eigenmodes.
-The critical eigenmodes in
the vicinity of the smectic A-nematic phase transition
are the solutions of the equations of motion, eq. (3.4), restricting ourselves to the critical parts of the elastic constants Ki and the viscosities fli and y,. Without loss of generality we can choose the wave vector q to lie in the xz plane, with 0 = (z, q). Then the eigenmodes with q in the xz plane (case 1) and the
others with q perpendicular to it (case 2) are decou- pled.
In case 2 the equations of motion reduce to (the coupling due to the elastic constant H may simply
be taken into account substituting - iWY1’ - iroY2,
-
i(0114 in JS by H - iwc5Yl)
The first eigenmode, eq. (5. la), has zero frequency
which means that this mode is noncritical. It corres-
ponds to the fast shear diffusion mode wF2 of nema-
tics. In eq. (5 .1 b) the elastic terms are of the relative
order Êi q2jH ~ (çq)2. In the hydrodynamic regime jq « 1 the Ki terms can be neglected. Then eq. (5. 1b) yields a relaxational eigenmode
This mode corresponds to the slow director mode WS2 of nematics.
In case 1 the equations of motion are
To simplify the discussion of the eigenmodes we
introduce the assumptions i) A > B, C and ii) B » C.
The first assumption is justified experimentally [16]
and implies the neglect of the constant C ( ~ B).
The second assumption implies the neglect of c5r¡ 1
and c5r¡3. The results in the absence of assumption ii)
will be given later.
As discussed in case 2, the K3 term in eq. (5. 4d)
can be neglected against the H term. Then this equa- tion for the orientational motion decouples from the equations for the translational motion. Substituting
vZ = icz in the dissipative term it reduces to
This equation describes a relaxational mode
in the variable 4>x. It corresponds to the director
mode ws1 of nematics.
We furthermore show that the H term describes
a purely transverse static director response. In the
static limit eq. (5 .4b) yields 0 = 0, and eq. (5 .4c)
and (5.4d) reduce to
Assuming MT = Mv as in eq. (4..14), which means
B = H, we find on eliminating u from eq. (5. 7b)
This result corresponds to the transverse static response function, eq. (4.14), mentioned in connec-
tion with the fluctuations of UZ.
The equations of motion, eq. (5.4), for the varia- bles 0, v,,, vz, and Uz lead to the secular equation
We make the insertion W2 = s2 q2 - iDwq2. For
the velocities we find the well-known equation [6]
Using the assumption A » B the velocities of first and second sound result as
For the damping constant D we obtain the equation (using A > B)
. n v i . i