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A molecular theory of surface tension in nematic liquid crystals

J.D. Parsons

To cite this version:

J.D. Parsons. A molecular theory of surface tension in nematic liquid crystals. Journal de Physique,

1976, 37 (10), pp.1187-1195. �10.1051/jphys:0197600370100118700�. �jpa-00208515�

(2)

A MOLECULAR THEORY OF SURFACE TENSION

IN NEMATIC LIQUID CRYSTALS

J. D. PARSONS

Departamento

de Fisica Universidade Federal de Santa Catarina

Florianópolis, Trindade,

Brasil 88000

(Reçu

le

2 fevrier 1976, accepte

le 10 mai

1976)

Résumé. - On calcule la tension superficielle à la surface libre d’un cristal liquide nématique en

utilisant

l’approximation

de Fowler, Kirkwood et Buff pour l’interface et une approximation de champ moyen pour la fonction de distribution de deux molécules. En prenant une interaction de Van der Waals entre molécules, on trouve que : a) les molécules préfèrent toujours être orientées dans le plan de la surface; b) il y a un saut de la tension de surface à la transition

nématique-isotrope,

mais elle est inférieure dans la phase nématique ; c) on peut observer un excès d’ordre en surface qui persiste dans la masse de la phase isotrope. On calcule les expressions générales du paramètre d’ordre

en surface à

partir

d’arguments d’énergie libre. On discute l’effet d’interactions entre moments

dipolaires permanents et l’on trouve que des molécules uniaxiales doivent être parallèles à la surface.

Abstract. - The surface tension at the free surface of a nematic liquid crystal is computed using

the Fowler-Kirkwood-Buff

approximation

to the interface, and a mean field approximation to the

molecular pair distribution function. It is found for a Van der Waals interaction between molecules that : a) the molecules always

prefer

an orientation in the

plane

of the surface; b) there is a gap at the

nematic-isotropic phase transition, but the surface tension is less in the nematic

phase;

c) there may be observable excess surface order which persists into the bulk

isotropic

phase. General expressions

are given for the surface order parameter using free energy arguments. The effect of a permanent dipole interaction on the surface tension is considered, and it is found for uniaxial molecules, that this interaction also leads to the condition that the molecules be parallel to the surface.

Classification

Physics Abstracts

7.130

1. Introduction. - The surface

region

and surface tension in nematic

liquid crystals

is at present rather

poorly

understood.

Experiments

so far

performed

show several

interesting

effects :

a)

Orientation at the free surface : The molecules of

some nematics

(e.g. PAA)

tend to lie in the

plane

of the

nematic-air free surface

[1-3]. However,

the orien- tation of MBBA has been measured to lie at a finite

angle

which is

slightly temperature dependent [3].

Several nematics which have a low temperature smectic A

phase

seem to have a

perpendicular

orien-

tation in the nematic

phase just

above the transition

[4].

b)

Behaviour of surface tension at the nematic-

isotropic

transition temperature : The

early

measu-

rements

[5, 6]

show that the surface tension is discon- tinuous at the transition. Recent work

[7, 8]

has

shown that in certain cases the

discontinuity

is nega-

tive,

and the surface tension is less in the nematic

phase.

c)

Free surface disclinations : In several nematics

having

a low temperature smectic C

phase,

discli-

nations in the orientation appear

just

before the nematic-smectic C transition

[4].

Molecular theories of surface tension in nematics

are difficult because of the

anisotropic pair

interac-

tions between molecules.

Recently,

a

general

expres- sion for the surface tension of a

polyatomic

fluid

has been derived and

applied

to calculate the

dipole- dipole

contribution to the surface tension of low vapor pressure water

[9].

For molecules with

pair

interactions

depending only

on the center of mass vector R and

on the Euler

angles [10] (Q, 0, 03C8) describing rigid body

rotations between the molecules relative to their centers of mass, the result for the surface tension is :

where R = r2 - ri is the center of mass vector, and where the

pair potential U12 depends

on R and the

internal states

e1, 62

which denote the Euler

angles :

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:0197600370100118700

(3)

1188

d3ei

=

sin oi doi dcpi dgii. p(2)

is the

pair,

or doublet

distribution function defined so that

gives

the average number of

pairs

of

molecules,

one

of internal state

61

and within

d3r,

of rl, the other of internal state

e2

and within

d3r2

of r2’ We define the distribution function

g (2) by

the relation

where p is the

singlet

distribution

function,

or number

density

of the fluid. In

(1),

the z axis is chosen to be normal to the free

surface,

which we shall

conveniently

fix at z=0.

From

(1)

and

(2)

we see that at the

nematic-isotropic transition,

y will

change abruptly

because of the two factors in the

pair

distribution function :

a)

The

nematic-isotropic

transition is

always

first

order with a discontinuous

change

in the

density

p.

Since the

density

is

larger

in the nematic

phase,

this

will lead to a gap in y with y also

larger

in the nematic

phase. However,

the

density discontinuity

at the

transition is very

small,

0.3

% being

a

typical

value.

Since y oc

p2,

this

implies

that the gap

Any

in the surface tension at the transition will be no more than about 0.6

%

due to the

density discontinuity.

b)

There is also a

sharp discontinuity

in the distri- bution function

g (2)

at the

transition,

due

mainly

to the

discontinuity

in the orientational order parameter.

Using

a Van der Waals interaction for

U12,

and a

mean field

approximation,

we will show that the gap

in y

due to this

discontinuity

should be

larger

than

that due to the

density discontinuity.

The surface tension will also

depend

on the orien-

tation of the molecules at the free

surface,

since the interaction

potential

is

anisotropic,

and

depends

on

the direction of the center of mass vector R as well

as its

magnitude.

In the bulk

phase

we know that the nematic state is characterized

by long

range orienta-

tional order

along

a certain direction

given by

a unit

vector n. In the absence of boundaries and external volume torques, the direction of n is

completely arbitrary :

the free energy of the nematic does not

depend

on n but

only

on the

degree

of order S

along

n.

However,

the free surface breaks the translational symmetry, so that the surface free energy will

depend

on

n . k,

where k is the normal to the surface. It is

important

to realise that this is

essentially

a geome- trical

effect,

and not due to any

special

interaction between molecules at the surface. Therefore we

expect

an

anisotropic

surface energy even in the case of an

isotropic

surface

(e.g. glass,

an

isotropic liquid, etc.) and,

in

particular,

even in the case of a

nematic-vapor

surface. Since the bulk free energy is still

independent

of n, the total free energy

(bulk plus surface)

will

be minimized for the value of

n.k

which minimizes y.

Below we show that for a Van der Waals interaction between

anisotropic molecules,

y is minimized when

n . k

= 0 i.e. when the molecules lie in the

plane

of

the free surface.

2. Interaction

potential.

- In this section we consi- der the form of

U12 in (1),

when the molecules interact

through

the induced

dipole-dipole

term of the Cou-

lomb interaction

(Van

der Waals

forces).

This inte- raction was used

by

Maier and

Saupe [11]

in their

treatment of the

nematic-isotropic phase

transition.

In this section we assume that the molecules have no

permanent

dipole

moments. This interaction will be discussed in section 6.

The

starting point

is the interaction energy between two molecules as

given

in the second order pertur- bation

theory :

where 1 0(1) >, 1 0(2) >

are the

ground

states of mole-

cules 1 and

2, and ,u(1) >, v(2) >

are excited states of

energy

E,

and

Ev. Euv = Ell + Ev

and we assume all

molecules are in their electronic

ground

states.

Finally,

H’ is

given by

a

dipole-dipole

interaction :

ql, qk are

charges

at

positions

xi, xk in the

molecule,

and R is the center of mass

separation

between molecules.

We assume that the molecules are uniaxial and

rodlike,

and that the

dipole

moments are induced

only along

the

long

axes of each

molecule,

all off-axis

dipole

moments

cancelling

out. This latter

assumption

is unnecessary if

we are

only

interested in the orientational part of the

interaction,

but it effects the

dependence

on the center of

mass vector R. Write

xi(1)

=

ni(1) il, XK(2)

=

nK(2) e2,

where

ê1

and

e2

are unit vectors

along

the

long

axes of the two

molecules.

Then, putting (4)

into

(3)

we have :

(4)

Since

Eoo E/-Lv,

we have a sum of

negative

terms in

(5).

Hence the interaction can be written as :

where T is the

symmetric

tensor

n

with 1 a unit tensor.

We now average the interaction

(6)

over a distribution of molecules. Introduce a

spherical

coordinate

system with

polar

axis n and express

61

and

e2

in this coordinate system. Since the molecules are

uniaxial,

all azimuthal

angles

Q 1, (P2 are

equally probable.

The average W over these

angles

then works out to be

where the

Tij

are the cartesian

components

of T.

Next,

we average

(8)

over the

polar angles 0,, 02-

From the symmetry of the nematic state, the distribution function

f(0)

is related to the order parameter S

by

In

doing

the average in

(8)

we assume that

f(o1,’ o2)

=

f (o1) f (o2)

with

f(O) given by (9).

This is a mean field

approximation

where local correlations in orientation are

ignored.

With this

approximation,

the interaction

averaged

over all orientations of the two

molecules,

becomes :

Finally,

we must average

(10)

over all orientations of the center of mass vector R. We express R in the same

spherical

coordinate system as before

(with

n the

polar vector).

Let 0 and 0 be the azimuthal and

polar angles

of R. Since the nematic state is

cylindrically symmetric,

all values of 0 are

equally probable,

and an average of

(10)

over this

angle gives,

with the

help

of

(7) :

In their treatment of the bulk

phase,

Maier and

Saupe [11]

assume that all

angles

0 are

equally

pro-

bable,

i.e. the centers of mass of the molecules are

completely random,

even at short range. This

approxi-

mation is in the same

spirit

as the one that invokes the

separability

of

f(01, 02);

i.e.

local,

short range correlations in both

position

and orientation of molecules are

ignored. However,

note that the inte- raction

potential (6)

is a strong function of the direc- tion

of R,

therefore this is

only

a

rough approximation.

With this

assumption cos2 0 >

=

1/3,

so that the

linear term in S

drops

out, and

(11)

reduces to :

which is the well known result that the mean field is

proportional

to

S2.

In

(11)

we see

if cos’ 0 )

>

1 /3 (molecules

tend

to be lined up end to end with

R // n)

then the term

in S is

positive. If cos’ 0 > 1 /3 (molecules

tend

to

align

in

layers

with n 1

R)

then this term is

negative.

On the other

hand,

the term in

S2

is

always positive

and rather insensitive to the direction of R. The interaction

(11)

has an extremum which is a local

minimum when 0 =

n/2,

which favors the

tendency

to order in

layers.

If we have

complete

translational symmetry, the linear term in

(11) dissapears,

but

if this symmetry is broken in some way, this term will determine the translational

symmetry

of the struc-

ture.

One way to break the translational symmetry is

through

an

equilibrium phase

transition. The inte- raction

(11)

suggests that a

possible

low

temperature phase

of a nematic would be characterized

by

a

structure where the molecules tend to form

layers

with nematic

ordering

in each

layer

and with the

planes

of the

layers perpendicular

to n. This is

exactly

(5)

1190

the symmetry of the low temperature smectic A

phase

observed in many materials that form nematics

[12].

Of course, one cannot say whether a

given

nematic

will form such a smectic state

just by looking

at the

interaction

(11). Nevertheless,

the

tendency

to

align

in

layers,

characteristic of the smectic

phase,

is

already

present in the nematic

phase.

We feel that

previous

molecular theories of the smectic A

phase [13, 14]

have not taken

enough

account of the

anisotropy

of

the interaction with respect to the center of mass

vector

R, corresponding

to the linear term in S in

(11).

Translational symmetry is also broken at the free surface in the nematic

phase.

Even if all orientations of R are

equally probable

in the

bulk,

this will cer-

tainly

not be true close to the free surface. We will

see below that the linear term in S in

(11)

is crucial

for

determining

both the surface

tension,

and the orientation of molecules at the free surface. So the orientation at a free

surface,

and the

tendency

of the

fluid to form a

layered,

smectic structure are

closely

related. A

study

of the free surface

gives

information

on molecular interactions which are

averaged

out in

the

translationally symmetric,

bulk nematic

phase.

This is also the case in some types of

polar

and asso-

ciated

liquids

which do not have a bulk

liquid crystal phase [15] :

the fluid is

isotropic

far from the

surface,

but there is an

anisotropy

close

enough

to the

surface, corresponding

to a

preferential ordering

of the mole-

cules.

3. The FKB

approximation

for surface tension. - The

general

formula

(1)

for the surface tension is very difficult to use without further

approximation

since the

density profile

and

pair

correlation function are

unknown in the surface

region

where the fluid is

nonhomogeneous. Indeed,

in an exact treatment, the

density profile

cannot be

specified beforehand,

but must be determined as part of the solution

[16].

At lov vapor pressure, the Fowler-Kirkwood- Buff

(FKB) approximation

leads to a

fairly

accurate

estimate of y for

simple

fluids

[17].

We will use the

same

approximation

in

treating

the

nematic-vapor

free surface. The FKB

assumptions

are that :

a)

the

vapor

density

is

negligible,

and

b)

the

density

of the

liquid phase

has the bulk value up to the

(Gibbs’) dividing surface,

which we take at z = 0. These two

assumptions imply :

where Z = zl - Z2’ In addition we assume that

where

1(8)

is

given by (9).

This

approximation

involves

the

following assumptions : a)

the centers of mass

vectors are

isotropic

in the bulk

phase, b)

local

correlations between the orientations of the molecules

are

neglected (a

mean field

approximation),

and

c)

the

z,

dependence

of the distribution function

f(0)

is

ignored.

That

is,

we assume that the order

parameter S

has the bulk value up to the free surface. The first two

assumptions

are

obviously

in the same

spirit

as the

Maier-Saupe theory

for the bulk

phase,

and the last

assumption

is in the same

spirit

as the FKB

approxi-

mation

(13), although

it is much less

obvious,

and in

fact,

as we shall see, contradicts the

boundary

condition on S at the free surface which can be derived from free energy arguments. As with the

density profile,

the detailed form of

S(z) through

the surface

region

must be obtained

self-consistently

in the

solution,

and cannot be

specified

in advance.

Recently,

the

S(z) profile

has been discussed

[18],

but since it

depends

on the unknown

density profile p(z),

the

discussion is

only qualitative.

The

only

other case

that can be treated within the FKB

approximation

is one where

S(z) decays

to the bulk value S in a

characteristic distance

large compared

to the mole-

cular interaction range. This case is discussed in an

appendix

where it is shown that the

parameter S appearing

in y must be taken to be the value of S at the

surface,

and not the bulk value of S.

With these

approximations (1)

reduces to :

with

d2e

= sin 0 dO

d(p,

the

superfluous angle 0 having

been

integrated

out. The interaction

U12

is taken to be

(6)

for Van der Waals forces. Put

(6)

into

(16)

and

integrate

over

d 2e, d2e2 first, keeping

R

constant. We get

where ( W >

is

given by (10).

The surface tension can

be broken up into three terms

in W > :

First assume that n lies

along

the surface normal

(z axis).

We can then express R in terms of

spherical

coordinates with

k

= n as the

polar

vector, and

integrate

over the two

angles e,

0. The first term yo in

(18) easily

works out to be :

(6)

The second and third terms in

(18)

can be

expressed

in terms of the

angular integrals

After a rather tedious

calculation,

one finds that

From

(10), (17),

and

(21)

we get :

hence the surface tension for

perpendicular

orien-

tation is

with Yo

given by (19).

4. Surface tension for

parallel alignment.

- Next

consider the surface tension when the molecules lie in the

plane

of the

surface,

i.e. when n is

along

the x

axis. Since R is

expressed

in terms of

0, 0

in a coordi-

nate system with n the

polar axis,

we can calculate y

by simply interchanging x

and z in the coefficients

(22) (i.e. Ixx

->

Izz, Ixy

->

Izy, etc.). Then, using

the

general

results

(17)

and

(10),

one finds :

We see

that y

II V’ 1. for all values of S. Further- more, the symmetry of the interaction

(10)

rules out a

smaller value

of y

for any other orientation. If there are no external torques

applied,

and the influence of other boundaries is

ignored,

the total free energy

(volume plus surface)

will be minimized when the orientation is

parallel

to the free surface. We conclude

that,

for molecules

interacting

with Van der Waals

forces,

the orientation will tend to be

parallel

to the free surface.

The

result, (25)

also

predicts

a gap in the surface tension vs. temperature curve at the

nematic-isotropic phase

transition

T,,

due to the discontinuous

change

in S there :

where AS =

S(T Tk) - S(T > Tk).

If we assume

that the S in

(25)

is the bulk

value,

then we know that

S(T > Tk)

= 0 and

S(T Tk) N 1/3.

This

gives

a gap of about

10 %

in the surface tension.

Moreover,

the

gap is

negative

- the surface tension is less in the nematic

phase.

We can relate this to molecular interactions as follows : the surface tension is essen-

tially proportional

to the

pair interaction ( W >

averaged

over all orientations. From

(11)

one can see

that W )

will be less in the nematic

phase

when the

linear term in S becomes

negative,

i.e. when the dis- tribution of the centers of mass vectors favors a

layered

like structure close to the free surface. The

decrease

in ( W >

with S

implies

there is less

restoring

force on s,urface molecules in the nematic

phase,

than in the

isotropic phase.

This

implies, ignoring

the

small

density effect,

that y will be less in the nematic

phase.

Note that this can

only happen

when the

orientation is

parallel

to the free

surface;

for a perpen- dicular orientation the surface tension gap would be

positive,

as can be seen from

(24).

We can make some further remarks on the

y(T)

curve away from

Tk.

Since y oc

pe

we expect y to

slowly

increase with

decreasing

temperature due to thermal

expansion.

In fact this is the main temperature

dependence of y in

normal

organic liquids [19].

For a

typical

value of

10-3/deg

for the volume

expansion

coefficient we expect a value

Ayfy = 0.2 %

per

degree.

Now for T

Tk,

we know that

S

increases with

decreasing temperature,

with the rate of increase

being largest

near

Tk.

Since for

parallel orientation,

an

increase in S leads to a decrease in y, it is

possible

that close to

Tk

one may see y

decreasing

with decreas-

ing temperature.

Far below

Tk,

where the order parameter is almost constant, the thermal

expansion

effect will

probably

win out, and y should start to increase

again.

The situation is further

complicated by

the fact that near

Tk

the thermal

expansion

coef-

ficient shows

pretransitional

anomalies. A careful measurement of

y(T)

above

Tk

could

give

information

on the temperature

dependence

and

magnitude

of

the order parameter at the surface

(see

section

5).

The

dependence

of y on an

applied magnetic

field

has received some attention in the literature

[20].

If the field is

applied parallel

to the free surface there should be no bulk

distortions,

and one can see from

(25)

that y should decrease with H because of the increase in S with H. However this effect is very small in nematics because of the small value of the

anisotropy

of the

magnetic susceptibility

and it is not

expected

to be observable.

We have calculated y for

parallel

and for

perpendi-

cular orientation and shown that y || yl. For certain distortion

problems

near the free surface it is of interest to calculate

y(03C8 ) ; where 0

is the

angle

that n

makes with the surface normal

k :

:

cos 0

=

n.k.

From

(10)

and

(17)

we can see that

only

even powers of

cos #

can enter y, but the

resulting expression

is not

easy to carry out because the interaction

(10)

involves

(7)

1192

the squares of the tensor components

Tij

rather than

these

quantities

themselves. For

qualitative

discus-

sions it may be sufficient to use the

simple expression :

From

(24)

and

(25)

it follows that

In the nematic

phase

where S >

1/3,

it is

important

to

recognize

that this is a very

large

difference in surface

energies;

at most an order of

magnitude

less

than the actual interfacial surface tension of the

liquid.

This means that it will be very difficult to tilt the surface orientation

by

the

application

of bulk torques. For

example,

if one

applies

a

magnetic

field

perpendicular

to the

surface,

the orientation at the surface will be

given by

an

angle t/Jo (measured

with

respect

to the

normal)

of

[21]

where 3 DS 2 ~

k,

where k is a Frank orientation elastic constant

[22].

Now with k ~ 10-6

dynes,

xa N 10-’ c.g.s., H ~ 104

G,

and yl -

Y II N

1

dyne/

cm we find that cos

t/Jo

3 x

10-3,

which is

hardly

observable. So our

theory

suggests that the

general

solutions of the elastic

equations

for the distortions in surface orientation

produced by

volume torques

[21, 23]

will be difficult to observe in the nematic

phase.

The surface orientation is then

subject

to

strong

anchoring :

in

problems involving

orientation at the free

surface,

instead of

minimizing

the bulk

plus

surface free

energies,

one may

simply

minimize

the bulk free energy and

require

that the

boundary

condition

n-k =

0 be satisfied at the free surface.

Instead of

using

bulk torques, one may try to

change

the orientation at the free surface

by using

solid bound- aries.

Suppose

we introduce a thin nematic film on top of a solid that

rigidly

maintains a

perpendicular alignment

of molecules

[24].

For a thin

enough layer,

one may be able to tilt the

alignment

at the free surface.

This

problem

was considered in ref.

[21]

where it

was shown that the

alignment

at the surface satisfies :

where d is the thickness of the film and

using

the same estimates as before. For d >

dc

we

have

approximately parallel alignment

at the surface

(tf 0 ~ x/2),

but for d

dc,

the

alignment

at the free

surface is forced to be

perpendicular

to

satisfy

the

rigid boundary

condition at the solid surface. It would be

interesting

to try to observe this

effect,

as the gap

in y at the transition temperature is very sensitive to the orientation

tf¡ 0’

and even reverses

sign (see

eq.

(24))

for

00 -+

0. The surface tension itself will

depend

on the

layer thickness d, varying from 01,

I

when d >>

dc

to yl when d

dc.

Finally,

it should be

pointed

out that the surface

energy favors

parallel orientation,

but the direction of n within the surface is

arbitrary.

This

degeneracy

is inherent in the

problem,

since what we have chosen

to call the X axis is

arbitrary.

The

degeneracy

will be

removed,

in

practice, by

small

perturbing

forces in

the

bulk,

whose

origin

may come from other boun- daries in the

problem,

or from an external

magnetic

field

applied

in a

given

direction

parallel

to the surface.

5. Excess surface order. - The fact that

Any

0 for the

preferred parallel

orientation also

implies

that there will be excess surface

order,

and

that S #

0

at the surface even above

Tk.

It has been shown elsewhere

[21]

that the

boundary

condition that S must

satisfy

at a

plane

interface is

given by :

where

5(S)

is the volume free energy. To get a

rough

estimate of the

magnitude

of this

effect,

we may use

a Landau

expansion

for

f(S) [25] :

where A =

a(T - Tc*)

with

T * slightly

below the

(first order) phase

transition temperature

Tk,

and

a,

B, C,

D are

positive

constants. Since D >

0,

note that excess surface order can

only

occur when

which is the case for

parallel

orientation. The

equi-

librium

S(z)

must

satisfy

the Euler

Lagrange

equa- tion :

which for

(32) gives

a nonlinear

equation

for

S(z) :

with the

boundary

conditions S

= Sb, dS/dz

= 0

at z = - oo.

Sb

is the bulk value

(the

value the order parameter would have if the fluid were

unbounded).

It satisfies :

For T

Tk

the solution which minimizes

(32)

is

(8)

with

For T >

Tk

the solution that minimizes

(32)

is

Sd

= 0.

At T =

Tk

there is a

discontinuity

in

Sb

and the

transition is first order.

An exact solution of

(34)

for all cases would involve

elliptic

functions and would be very difficult to carry out. Here we

only

consider

approximate

solutions

for T >

Tk

and T

Tk.

First suppose T

Tk

so

we are in the bulk nematic

phase.

In

particular,

choose T =

Tc *,

then

A = 0, Sb

=

B jC.

Assume

that the effect of the surface is small and write S

= Sb

+

S’(z)

and linearize

(34)

in

S’(z).

This

gives

a

simple exponential equation

for

S’(z) :

where

a2

=

(3 CSb -

2

CSb)/D

=

B 2/CD

> 0. The solution for S is then

where

So

=

S(O)

is the order at the surface. The interfacial

boundary

condition

(31) along

with

(25)

then

gives

For

yo/Da ->

oo,

So approaches

the

limiting

value

of

3/4.

In

evaluating (39)

we use the

typical

values

C N 1

J/cm3,

D ~

lO-12 J/cm,

yo N 30

ergs/cm’,

Sb

= 0.5. Then

(39) gives So N

0.68 which is about 30

%

excess surface order. The

decay

distance is

a -1 N

100

A

which is

small,

but still much

larger

than the range of interaction of Van der Waals forces

(only

a few

A).

The case T >

Tk

poses more difficulties since

Sb

= 0. A first

integral

of

(34)

is

readily

obtained :

Note that the r.h.s. is

always positive

for A > 0 since this is

just

the free energy of the bulk nematic

phase

which has an absolute minimum at S = 0 when T >

Tk.

Thus

(40) represents

a nonlinear

decay

from

the surface : oscillations in

S(z)

cannot occur.

Using (40)

and the

boundary

condition

(31)

we can get a condition on

So

without

knowing

the

complicated dependence

on z :

Again

when yo -> oo,

So -> 3/4. Eq. (41)

can be

solved

numerically

for

So

at all

temperatures

if the

quantities A, B, C, D,

yo are known. For the values

A/C

=

1/10, B/C

=

1/2,

and yo and D as estimated

before, (41)

has the

approximate

solution of

So

= 0.5

just

above

Tk.

This rather

large

value decreases

roughly inversely

to the temperature difference T -

Tc*.

A more detailed

qualitative

discussion of the excess

order

parameter, taking

into account the fact that the surface

region

is

really

diffuse rather than

sharp,

has been

given

in ref.

[18].

6. Effect of a

permanent dipole-dipole

interaction. - Interactions between permanent molecular

dipoles

are

ignored

in the

theory

of bulk nematics because no

ferroelectric effects have ever been measured in

nematics;

the states n and - n seem to be

completely equivalent.

This

implies

that the molecular distri- bution function

f(O)

has the symmetry property

f(n - 0)

=

f(O),

so that even if the molecules have permanent

dipole

moments, as many

point

up as

point

down on the average and any

long

range ferro- electric effect cancels out.

However,

since a free surface breaks the translational

symmetry,

it is

possible

to

have cos

0 > :0

0 at the

surface,

where there is an

.anisotropy

in

the

distribution of center of mass vectors.

Since

cos

0 >

= 0 in the

bulk,

it must

decay

to zero in a characteristic

distance

from the free surface.

In this section we calculate the contribution to the surface tension

produced by

permanent

dipole- dipole

interactions. We assume that the permanent

dipoles

are

along

the

long

axes of the molecules. Then the interaction is

given by :

where T is

given by (7), and p

is the

dipole

moment of

the molecule.

Again

we express the

6i

in

spherical

coordinates with

polar

vector n and average

(42)

over the two azimuthal

angles

wi, Q2. The

only surviving

term is :

An average

over 01 and 02 gives

a

factor cos () >2 == G2

in a mean field

approximation. Expressing TZZ

in

polar

coordinates as

before,

the average interaction turns out to be :

As

expected,

for a random distribution of centers of mass,

cos’ 0 )

=

1/3,

and the interaction vanishes in the bulk

phase.

But near the

surface,

the interaction

(44)

will not average out.

(9)

1194

The contribution of the

permanent dipole

interac-

tion to the surface tension is then

where U > = R -3(1 - 3 cos’ 0). Doing

the angu- lar

integrals

as before we find for

perpendicular alignment

and for the

parallel alignment

So we have yd 11 yal and hence the permanent

dipole forces,

like the Van der Waals’

forces,

lead to a

parallel alignment

of molecules at the surface. This appears to rule out the ferroelectric interaction between permanent

dipoles

in the

interpretation

of

the

perpendicular

orientation of MBBA in a thin film with two free surfaces

[2].

We have assumed the

dipole

moment of a molecule

is

along

the

long

axis. If we have

permanent

off axis

dipole

moments which make an

angle

a to the direction

of easy

polarizability

then the molecules are no

longer

uniaxial but biaxial

[26].

In this case, if the

dipole-dipole

interaction is the

only interaction,

the above arguments go

through exactly

as before and

the surface tension is minimized when the

dipole

moments are

parallel

to the surface which means that

the director makes an

angle

a to the surface. When

there are Van der Waals forces present, these will tend

to line up the director

parallel

to the

surface,

so that the actual

angle tf

that n makes with the surface will be less than a. The

angle tf

is thus determined

by

two

competing

forces and will in

general

be

temperature dependent

since the two order parameters S and e may be different functions of temperature. In MBBA the molecules are tilted at an

angle r

750 from the

surface which

depends

upon temperature

[3].

The case

of MBBA would be an

interesting

one to

study

in

detail since we have

experimental

information on y at the transition

[27],

the tilt

angle,

and the electric

dipole

moment

[28].

Other mechanisms that can lead to a tilt in the molecular orientation at the surface are :

a)

Interactions of surface molecules with

impu-

rities

selectively

adsorbed to the surface which tend to

orient the

polar

heads of the molecules and

thereby

cause a term in y which favors

perpendicular align-

ment. In this case, the tilt

angle

would vary with the concentration of the surface

impurities.

b)

The formation of smectic-like

layers

near the

surface, resulting

in a breakdown of the translational symmetry at finite distances from the surface. If the

layers

tend to lie in the

plane

of the free

surface,

as

they

do in

smectics,

this will lead to a

perpendicular

orien-

tation at the surface. This kind of

ordering,

where

one has a non-zero smectic order parameter close to the surface which

decays

to zero in the

bulk,

is ana-

logous

to the case of orientational surface order above the bulk

clearing

temperature where the bulk order parameter vanishes. A better

understanding

of the

relationship

between order and molecular interactions in smectics will

probably

be necessary, before such a

model could be worked out in detail.

Appendix. Spatial dependence

of S. - If there is

excess surface

order,

the order

parameter

will

decay

to the bulk value within a characteristic distance from the surface. In other

words,

the order para- meter, and therefore the

pair

distribution

function, depend

on the coordinate z, in

(1).

We assume the FKB

approximation

and put

(13), (14), (15)

into

(1), where f (0)

is allowed to

depend

on

zl. The

integral

over

d3 R

can be broken up into a

part with Z > 0 and a part with Z 0 :

Since

p(2)

= 0 for zi >

0,

this reduces to :

where

Interchange

the orders of

integration

in

(A. 2),

inte-

grating

over

d3el d3e2

first :

where A and B are

given

in terms of the T tensor

by (10).

Integrate

over z, term

by

term. The first term

just

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