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The problem of orientational order in tilted smectic phases : a high resolution neutron quasi-elastic

scattering study

A.J. Dianoux, H. Hervet, F. Volino

To cite this version:

A.J. Dianoux, H. Hervet, F. Volino. The problem of orientational order in tilted smectic phases : a high resolution neutron quasi-elastic scattering study. Journal de Physique, 1977, 38 (7), pp.809-816.

�10.1051/jphys:01977003807080900�. �jpa-00208642�

(2)

THE PROBLEM OF ORIENTATIONAL ORDER

IN TILTED SMECTIC PHASES :

A HIGH RESOLUTION NEUTRON QUASI-ELASTIC SCATTERING STUDY

A. J. DIANOUX

Institut

Laue-Langevin, 156X,

38042 Grenoble

Cedex,

France

H. HERVET

Laboratoire de la Matière

Condensée, Collège

de

France, place Marcelin-Berthelot,

75231 Paris Cedex

05,

France

and F. VOLINO

Institut

Laue-Langevin, 156X,

38042 Grenoble

Cedex,

France

and

Groupe

de

Dynamique

des Phases

Condensées,

Laboratoire de

Cristallographie (*) U.S.T.L., place

E.

Bataillon,

34060

Montpellier Cedex,

France

(Reçu

le

20 janvier 1977, accepté

le 30 mars

1977)

Résumé. 2014 On présente des résultats de diffusion incohérente quasi

élastique

de neutrons, à

haute résolution, dans les

phases

smectiques H surfondue, VI et VII du

téréphtal-bis-butyl-aniline

(TBBA). Le facteur de structure

elastique

incohérent 2014 EISF 2014 et la forme des raies sont

analysés

à

l’aide de modèles qui incluent la

possibilité

d’un ordre orientationnel autour du

grand

axe. Les conclu-

sions sont les suivantes :

(i) Dans la

phase

H, les molécules toument uniformément autour de leur

grand

axe, sur une échelle de temps de 10-11 s, ce qui

n’implique

aucun ordre orientationnel des

dipôles.

(ii) Dans la

phase

VI, les molécules se réorientent, sur la même échelle de temps,

probablement

par sauts de 03C0 autour du

grand

axe, ce qui, comme

précédemment n’implique

aucun ordre orientationnel des

dipôles.

(iii) Dans la phase VII, il n’y a

plus

de mouvements rotationnels de

grande amplitude

sur une

échelle de temps de 10-11 s.

De (i) et (ii), on conclut que les

phases smectiques

inclinées ou non inclinées doivent être caracté- risées par un critère autre que l’existence ou l’absence d’une forte interaction

dipolaire

entre les

molécules.

Abstract. 2014

High

resolution neutron

quasi-elastic

scattering data in the

supercooled

smectic H, smectic VI and smectic VII

phases

of

terephtal-bis-butyl-aniline

2014 TBBA - are presented. The elastic incoherent structure factor 2014 EISF 2014 and the line

shapes

are

analyzed

in terms of models

permitting

orientational

ordering

around the

long

axis. The conclusions are :

(i) In the H

phase,

the molecules rotate

uniformly

around their

long

axis, on a time scale of 10-11

s, implying

no orientational order of the

dipoles.

(ii) In the VI phase, the molecules

probably

reorient, on the same time scale,

by jumps

of 03C0 around

the long axis, again

implying

no orientational order of the

dipoles.

(iii) In the VII phase,

large amplitude

rotational motions on a time scale of 10-11 s do not exist any more.

From (i) and (ii), it is concluded that the tilted or non-tilted smectic

phases

should be characterized

by a criterion other than the existence or non-existence of a strong intermolecular

dipole-dipole

interaction.

Classification

Physics Abstracts

7.130 - 7.114

(*) Associe au (’.N.R.S. (La 233).

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01977003807080900

(3)

810

1. Introduction. - The

problem

of the nature of

molecular

ordering

in the tilted smectic

phases

has

been,

in the

past

few years, the

subject

of conside- rable

work,

both

theoretically

and

experimentally,

and the answer is still controversial. The former

microscopic

mean field theories

of Meyer

and McMil-

lan

[1]

for the smectic C and H

phases

and that of

Meyer [2]

for the smectic H and VI

phases

contain

orientational

ordering

of the molecules around their

long

axis as a fundamental feature. This

ordering

is

linked to the existence of a

strong

intermolecular

dipole-dipole interaction,

which

plays

an essential

role in these

theories,

as

being responsible

for the

tilted character of these

phases. Although

some authors

have claimed to have observed some

ordering,

the

published X-ray [3],

NMR

[4, 5, 6],

ESR

[7],

Raman

[8]

and neutron

[9, 10, 11]

results do not support the existence of such an

order,

at least in some C and H

phases. Consequently,

other theories have been deve-

loped

which do not contain this feature

[12, 13].

However,

this

negative

result is not

yet

well

accepted,

as could be noticed at the VIth International

Liquid Crystal Conference, Kent,

Ohio

(1976).

For

studying

this

problem,

incoherent neutron

quasi-elastic scattering (NQES)

is

certainly

one of

the most

powerful

tools since it can

probe

both the

geometry

and the

dynamics

of the molecular

motions, provided

these are

sufficiently rapid (- lO-11 s) [14].

This is the case for the

typical

mesogen

terephtal-bis- butyl-aniline (TBBA).

In a series of papers, we have

presented NQES

results in the

crystalline [15]

and the

various smectic

phases

of TBBA

[9-11, 14, 16].

Analysis

in terms of the elastic incoherent structure factor

(EISF)

have

suggested

that :

(i)

In the C and H

phases,

the molecules rotate

rapidly

around their

long axis,

with some

additional, rapid

fluctuations of this axis about its

equilibrium position.

(ii)

In the VI

phase, rapid

rotational motion still

exists,

but it should be less

uniform

than rotational diffusion - or

jump

motion among six

equivalent positions

around the

long

axis. The existence of an

orientational

ordering

around the

long

axis may

explain

this feature.

In this paper, we present a more detailed

NQES study

of the

supercooled H,

VI and VII

phases [3]

of

TBBA,

aimed at the

problem

of the orientational order.

Here,

not

only

the EISF but also the line

shapes

are

analyzed

in terms of models

permitting

orienta-

tional

ordering

around the

long

axis. The results

essentially

confirm our

previous conclusions; namely,

no

ordering

in the H

phase

and

possible,

but

weak,

order in the VI

phase.

Because of this

weakness,

we

propose an alternative

(and

in our

opinion

more

realistic)

model for the VI

phase,

where the molecules

are allowed to

flip by x

around their

long axis,

as has

been

suggested

for a non-tilted smectic E

phase [17].

In section

2,

we present theoretical models which

are used to describe the

possible physical

situations

and write down the

corresponding

incoherent neutron

scattering

laws. In section

3,

the

experimental

results

are

presented

and some results are extracted from an

analysis

in terms of the

experimental

EISF. In sec-

tion

4,

the same data are

analysed

in terms of the

complete scattering

laws. In section

5,

conclusions are

drawn and discussed in terms of other

experimental

results.

2. Theoretical models and incoherent neutron

scattering

laws. - In these

models,

we assume that

(i)

the molecules are fixed in a three-dimensional

lattice, (ii)

that a

body

axis can be defined and

(iii)

that the

molecules can rotate about it.

Any

translational motion of the centre of mass is assumed to occur on a different time scale to rotation

(much longer

for

self-diffusion,

much shorter for

vibrations). According

to the

microscopic

theories

[1, 2],

the molecules are

submitted to a

potential

of the form

where T is the azimuthal

angle

around the

long

axis.

This

potential

describes the

dipole-dipole

interaction which tends to

align

the

dipoles

towards a fixed

direction,

taken as

origin (T

=

0).

In a

NQES

expe-

riment,

one follows the

protons

which are attached

to the molecules. These protons are

generally

not

situated on the

long

axis but at a distance a. To

analyse

the

NQES data,

we should thus calculate the incohe- rent

scattering

law for a

particle undergoing

random

motion on a circle of radius a and submitted to the

potential given by

eq.

(1).

In a

previous

paper

[18],

FIG. 1. - The first non-zero order parameter yN = (cos Ncp >

versus yg, for a circular random motion in an N-fold cosine poten- tial : eq. (5) of the text.

(4)

we have solved this

problem

in the case of a more

general potential

of the form

In what

follows,

we

give

the results relevant to our present

problem.

The rate

equation governing

the

probability

function

Gs(lp,

lpo,

t)

which is the

probability

of

finding

the

particle

at 9 at time t if it was at To at t =

0,

was chosen to be of the

Debye

type,

namely

where

Dr

is a rotational diffusion coefficient and 2

yN

the relative barrier

height

defined

by

The

first

non-zero order parameter yN is defined

as the average value of cos

N(p

and we have

where the I are modified Bessel functions of first kind.

Figure

1 shows the curve yN versus

yN

calculated

from eq.

(5).

The neutron incoherent

scattering

law can be calculated. The result

is,

for a

powder

form

sample

with

and

where

jo

is the

spherical

Bessel function of order zero.

In these

expressions :

(i) Ap

and

Vnp

are the

eigenvalues

and

eigenvectors

of the

(infinite)

matrix M whose terms are

(m, n >, 1)

(ii)

P, and

Wnp

are the

eigenvalues

and

eigenvectors

of the

(infinite)

matrix N whose terms are

(m, n >, 1)

(iii) T pn

are the elements of the matrix T such that

where the elements of the matrix 0’ are

(m, n >, 1)

(iv) U pn

are the elements of the matrix U such that

(5)

812

where the elements of the matrix Q’ are

(m, n > 1)

In items

(iii)

and

(iv),

the

argument

of the Bessel functions I is

yfv.

It is

interesting

to consider the two limit-

ing

cases

y%

= oo and

y%

= 0. For

y%

= oo we recover the

jump

model among N

equidistant

sites on a circle

[19, 20].

The

scattering

function

is,

in this case

with

and

For yN

=

0,

we recover the rotational diffusion model on a

circle,

which

clearly,

is

independant

of N.

This case is in fact identical to the case

y%

= oo and N = oo so that we have :

In other

words,

when the number of wells is

large,

the

scattering

law is almost

independant

of this number and of the barrier

height.

In

practice,

for TBBA in the Sm H

phase,

a

jump

model between six sites and the rotational diffusion model are indiscernable from one another for

Q

1.2

A-1 [9].

For N =1 or

2,

this is

no

longer

the case and this fact will be used to

analyse

the

present NQES

data. This is

why

we

give

a few more

results

concerning

these two cases. For N =

1,

whatever

y’,

no

approximate expression

for the

scattering

law

(eq. (6))

exists.

However,

in this case it is clear that the two matrices M and N are identical

(since

m - N is

never

negative). Hence,

eq.

(6)

can be written in a

slightly

more compact form. For N >

1,

on the contrary,

an

approximate

form for eq.

(6)

can be written as soon as

yN

is

sufficiently large.

For N =

2, when y2

> 1.2

(corresponding

to an order parameter Y2

= (

cos 2

qY ) = 0.5), only

the lorentzian

corresponding

to

À1

can

be retained in eq.

(6)

since all the other ones are much broader

(at

least 10

times)

and can thus be considered

as

contributing

to a flat

background.

We can then write :

with

The functional form of eq.

(20)

is identical to that of eq.

(15)

for N = 2. The

quantity D, A,

can thus be

identified for

large y2,

to the

jump

rate between the two

equilibrium positions.

For the

proofs

of all the statements made in this

section,

the reader is referred to ref.

[18].

3.

Experimental

results and

analysis

in terms of the

EISF. - As in our

previous

work

[9 -11],

the

sample

studied was the

partially

deuterated derivative of TBBA we called DTBBA

(completely

deuterated on

the

butyl chains,

in order to render their motion invisible to

neutrons),

in

powder

form. The

sample

environment is described in ref.

[9].

The

NQES

expe-

riments

were

performed using

the

time-of-flight

spec-

(6)

trometer IN 5 installed at the cold source of the reactor of the Institute

Laue-Langevin.

The incident

wavelength

used was 11.0

A, yielding

an elastic

energy resolution function of Aco 20.0

J.l.e V (1 J.l.eV

= 1.52 x

109 rad . s-’)

FWHM

(compared

to Aco 33

J.l.eV

in ref.

[9-11]).

Two kinds of run

were

performed

for 24 temperatures between 102 and 68 OC in the

supercooled

Sm

H,

Sm VI and

Sm VII

phases.

In the first kind of run, the spectra

were recorded for six

scattering angles corresponding

to

(elastic) Q

values between 0.5 and 1.05

A-l.

Such

runs needed rather

large counting

times and were

performed only

for a few temperatures. In the second kind of run,

only

two spectra were

recorded, using

many counters for

each, corresponding

to average

Q

values of 0.78 and 1.03

A-1 (AQ

= ± 0.03

A-1).

In all cases, care was taken in

changing

the tempe-

rature between two runs. Indeed it turned out that the Sm VI

phase

could be missed if the

temperature

was

changed

too

rapidly.

In

particular,

we found it

important

to

stay

a

relatively long

time

(-

1

hour) just

above the normal

crystal-Sm

H transition tem-

perature

( x 114 C)

before

gently cooling

the

sample further,

first in the

supercooled

Sm H

phase

and then

into the Sm VI

phase. Figure

2 shows a

typical NQES spectrum

obtained in the Sm VI

phase

at

78°C, together

with the instrumental resolution function. It

clearly

shows a

sharp peak reproducing

the

resolution

function

superimposed

on a broad

component, as

expected [9-11].

Since these two

components

are well

separated,

the

experimental

EISF

(i.e.

the relative

intensity

of the

sharp peak

to the total

(quasi-elastic) intensity)

can be deduced. This was

done

using

the computer method described in ref.

[11].

The results of this

analysis

are summarized in

figure

3

FIG. 2. - Typical NQES spectrum for DTBBA in the smectic VI

phase. Temperature T = 78 °C, momentum transfer Q = 1.03 A - 1.

The corresponding instrumental energy resolution function is also shown.

FIG. 3. - Experimental EISF of DTBBA B’ersus temperature deduced from NQES spectra taken at Q = 1.03 A-1. The error

bars depict the uncertainty inherent to the method for extracting

the EISF. The limits correspond to a pessimistic and an optimistic evaluation of the intensity in the wings of the spectra. On the left hand side of the figure is indicated the theoretical value of the EISF for the jump model among N sites on a circle (yg = oo) : eq. (16) of the text, averaged over the five kinds of protons of the DTBBA molecule, calculated for Q = 1.03 A-’. Point D : N 1, point C :

N = 2, point B : N = 3 and point A : NN 4, 5 ..., oo. Point A also corresponds to the rotational diffusion model (yN = 0). Varying yN, the theoretical EISF should vary between : D and A for N = 1,

C and A for N = 2, B and A for N = 3, etc...

where we have

plotted the, experimental

EISF for

the spectra taken at

Q

= 1.03

A-1,

versus

tempe-

rature. It is seen that the EISF increases as the tem-

perature

is

decreased,

with definite

jumps

between 90

and 89 °C and between 70 and 68 °C. Let us

analyse

these data in terms of the models

presented

in section 2.

Since the DTBBA molecule contains

only

five kinds

of proton, all located on the

body,

the theoretical

expressions (6)

to

(8),

and

(15)

to

(21)

should be

averaged

over the

corresponding

five

gyration

radii ai.

These are,

assuming

that the

body

is

rigid,

in its trans-

conformation, 2.33, 1.90, 1.52,

2.33 and 1.90

A [11].

In what

follows,

when

referring

to these

expressions,

we shall

always

assume that such an average has been

performed.

On the left hand side of

figure 3,

we have

indicated,

for a few values of

N,

the range in which the theoretical EISF

(eq. (7))

can vary with

yg,

for

the value

Q

= 1.03

A- 1.

The limit

yg

= 0 is the same

for all N

(point A).

The limits

yN -

oo are calculated

from eq.

(16).

It is seen that for N >-

4,

all are

practi- cally

the same and

correspond

to

point A,

N = 3

corresponds

to

point B,

N = 2 to

point

C and N = 1

to

point

D. With these

indications,

some conclusions

can

immediately

be drawn :

(i)

Down to 90 OC - the

supercooled

H

phase

-

we have N

large, suggesting

uniaxial rotational

motion,

but no, or very

weak,

orientational

ordering

(7)

814

in the sense of the theories of ref.

[1]

and

[2].

The

lowest value of the EISF at 102 °C

compared

to that

at 90 °C can be attributed to a kind of motion other than rotation around the

long

axis. In ref.

[11],

we

assumed that the effect was due to fluctuations of this axis.

(ii)

Between 89° and 70 OC - the Sm VI

phase

-

since the

experimental points

lie between A and D

(case

N =

1),

some finite orientational order in the

sense of the theories of ref.

[1]

and

[2]

may exist.

However,

the

points

also lie between A and C

(case

N =

2),

so that a

symmetrical

model where the mole- cules

jump by 7r

around the

long

axis is also

possible.

(iii)

Below 70 OC - the Sm VII

phase

-

only

the

case N = 1 is

possible, although

it is difficult to conclude in this case whether the measured EISF is

meaningful (the

broadened contribution in the spectra is in fact very

weak).

4.

Analysis

in terms of the

complete scattering

laws :

order parameters and correlation times. - In this

section,

we take

advantage

of the fact that

(i)

for

each temperature, many spectra are available for

different Q

values and

(ii)

that formal

expressions

for

the incoherent

scattering

laws are

available,

to

confirm the above

conclusions,

deduce order parame- ters and correlation times and try to discriminate between the two

possible

models for the Sm VI

phase.

We shall thus discuss the cases N = 1 and N = 2 for the smectic H and VI

phases.

4.1 CASE N = 1. - This case

corresponds

to the

microscopic

theories of ref.

[1]

and

[2],

where the

molecules are allowed to

perform large

and over-

damped

oscillations around the

long

axis about the

direction qJ

= 0. We have fitted the

scattering

law

given by

eq.

(6)

for N = 1

simultaneously

to all the

spectra obtained in one run, for all temperatures.

The fitted parameters are

y’, 1 Dr,

a flat

background

and a

Debye-Waller

factor. The

fitting procedure

is

described in ref.

[15].

The computer time turned out to be rather

large

due to the fact that the

large

matrices

M and N

(truncated

at a dimension s -

20, typically)

have to be

diagonalized

many times.

Figure

4 shows

the results for the order

parameter

yi

= (

cos T

>,

related to

T’ by

eq.

(5) (or Fig. 1).

It is seen that this

model

yields :

(i)

cos

o > --

0 in the

supercooled

H

phase, (it) ( cos T > varying

from 0.2 to 0.5 in the Sm VI

phase.

This

corresponds

to average

angular

fluctua-

tions

of ±

80 to ± 60° about the

equilibrium position.

Figure

5 shows the

corresponding

values found

for

the correlation time

Dr 1.

4.2 CASE N = 2. - This case

corresponds

to a

model in which the

dipoles play

no

role,

as in the

non-tilted Sm B and Sm E

phases.

The molecules are

FIG. 4. - Values of the order parameters y for the models N = 1 and N = 2, versus temperature, obtained by fitting eq. (6) or eq. (20), according to the case, simultaneously to all the spectra obtained in a run at a given temperature. The white symbols correspond to

runs with two spectra, the black symbols to runs with six spectra.

The circles stand for the model with N = 1, the squares for the model with N = 2. The corresponding mean angular fluctuation

amplitude Acp is also indicated for each case.

FIG. 5. - Values of the correlation time of the motion for models N = 1 and N = 2, versus temperature, obtained by fitting eq. (6)

or eq. (20), according to the case, simultaneously to all the spectra obtained in a run at a given temperature. The circles stand for the

quantity Di of the model N = 1, the squares stand for the quan-

tity (Dr A 1) of the model N = 2. It is seen that whatever the model, the correlation times are roughly the same within 50 %

and that no discontinuity is apparent at the Sm H-Sm VI transition.

allowed to oscillate about two

opposite equilibrium positions (T

= 0 and T =

a)

and to

jump

between

these two

positions.

We have fitted eq.

(6)

for N = 2

to the same data. The result for the order parameter Y 2

= (

cos 2 cp

B

related to

y2 by

eq.

(5) (or Fig. 1),

is also shown in

figure

4. It is seen that :

(i) (

cos 2

T > --

0 in the

supercooled

H

phase.

This result was

expected

from the case N =

1,

since all the models are identical for

yg

= 0.

(8)

(ii) (

cos 2

T >

varies from 0.7 to - 1.0 in the

Sm VI

phase.

This

corresponds

to average

angular

fluctuations of z ± 200 to

nearly

0 about each

equi-

librium

position.

In

fact,

to obtain these

results,

we used the

approximate scattering

law

given by

eq.

(20) since

cos 2

T >

was

expected

to be

high.

On

figure

5 are also shown the

corresponding

corre-

lation times

(Dr Â.1)-1.

In both cases, N = 1 and N =

2,

the

quality

of the

fit was found to be

equally good,

as can be seen on

figure

6.

FIG. 6. - Example of the quality of the fit obtained. The crosses are

experimental corresponding to a temperature of 73°C. The full line is either the best fit of eq. (6) for N = 1, corresponding to

yl = 0.44, Dr = 3.3 x 10-11 s, or to eq. (20) (N = 2), corres- ponding to Y2 = 0.97 and (Dr A 1) = 2.0 x 10-11 s. The number

of counts has been normalized so that it makes sense to compare the amplitudes of the four spectra.

5. Discussion.

2013 1)

For the smectic H

phase,

we

confirm,

in the

supercooled

state, our

previous

conclu-

sions obtained in the normal state

[9, 10], namely

that

(i)

the molecules rotate around their

long. axis,

in contradiction to the arguments

against

rotation of de Vries

[21]

and

(ii)

no, or very

weak,

orientational

ordering exists,

in the sense of the

Meyer-McMillan [1] ]

and

Meyer [2]

theories for this

phase.

On the contrary,

they

agree with most of the conclusions deduced from results obtained with other

spectroscopic

tech-

niques [3-8].

In

particular,

we wish to mention the

X-ray

results

[3]

which indicate the existence of three

equivalent

orientations for the molecules around their

long

axis

(X-ray

data cannot

distinguish

between

static and

dynamic disorder),

and a theoretical cal- culation

[22],

which can

reproduce

rather

accurately

the

X-ray

patterns

using

a model

assuming only

steric hindrance between the

phenyl rings.

In other

words,

the molecular order in the tilted smectic H

phase

of TBBA appear to be the same as that

expected

for a non-tilted Sm B

phase.

2)

For the smectic VI

phase,

the existence of a

broadened

component

in the

NQES

spectra

is,

in

our

opinion,

a

proof

that some rotational random motion similar to that

existing

in the H

phase,

still

exists. In that sense, we are at variance with the conclusions drawn from DMR

[6]

and Raman

[8]

works where it is

suggested

that the motion freezes

on

cooling

to the

phase

VI. On the contrary, we are

not in contradiction

(i)

with the

picture suggested by X-ray

diffraction -

only

the average orientation of the molecules is seen

there; (ii)

with the weak entropy

change

AS = 0.34

Ro

measured at the

Sm H - Sm VI transition

[2]

- one would

expect

S >

Ro Log 1.1 Ro

if a

complete freezing

occur-

ed

(although

this argument may be

questioned) ; (iii)

with proton

spin-lattice

relaxation measure- ments

[23]

which show

only

a very weak

change

at

the H-VI transition

indicating

that no

major change

in the nature and the time scale of the motions occur.

The

question

left is thus to discuss

which,

of the two

possible

models we propose and which are consistent with our present

NQES data,

is the more realistic.

Since the fit of both models is

equally good,

we

should look to other results to answer this

question.

In our

opinion,

there are

(at least)

two reasons for

believing

that the model

corresponding

to N = 2 is

the correct one. The first reason is theoretical.

Although

our data do not

disagree

with the existence of an orientational order as

predicted by

the

Meyer theory [2],

this

theory

also

predicts

a similar

(but weaker)

order in the

higher

temperature Sm H

phase.

However,

we have seen that such order does not seem to exist in the H

phase,

i.e. that the

dipole-dipole

interaction is not dominant in this

phase.

If so, there

is no strong reason to believe that it becomes a

leading

term in the Sm VI

phase.

The second reason is related to the structure of the VI

phase.

The

X-ray

results

suggest

a

herring-bone

arrangement for the

molecules,

where at the two kinds of sites in the a, b

plane

the

two mean orientations are at + 300 and - 300 with respect to the b direction

[3]. Consequently,

an ave-

rage

angular fluctuation

of ± 80 to ± 60° around each

equilibrium position,

as

predicted by

the model

with N = 1 would

imply

that the two kinds of sites

are

continuously exchanging

on a time scale of

-

10-11

s

(a

fluctuation

just

greater than + 300 would have

implied

the same

result).

Such a motion

is

necessarily

collective

and,

in our

opinion, unlikely

on this time scale. On the contrary, with the model N =

2,

where the molecules are allowed to

flip by

n around their

long axis,

the maximum

angular

fluctuation is

only

± 200. This result agrees with the

symmetry

and the

jump by

n will

only

involve a

(more reasonable)

mononiolecular motion. If thus we

adopt

the model N = 2 for the VI

phase,

the molecular order in the Sm VI

phase

of TBBA appears to be the same as in the non-tilted Sm E

phase,

for which a similar

type of motion has been

suggested,

based on

NQES

results

[17].

This result

is,

in

addition,

more reasonable

when

regarding

the conclusion for the Sm H

phase.

(9)

816

3)

For the Sm VII

phase,

no

large amplitude

rota-

tional

motions,

on a time scale of

10- 11

s, are detected any more. The Sm VI-Sm VII transition thus appears

as a

freezing

of the

jump by

n around the

long

axis.

This result is in

agreement

with proton

spin-lattice

relaxation measurements which exhibit a

large jump

at the Sm VI-Sm VII transition. The nature of the

remaining

motions

compared

to the

crystalline phase

cannot be inferred from the present

experimental

results.

6. Conclusion. - From

high resolution,

incoherent

NQES

on

TBBA, making

the

(weak) assumptions

that

(i)

the molecular

body

is

mainly

in its transcon-

formation on a time scale of

10-11.

s and

(ii)

that the observed

broadening

of the

spectra

is due to rota- tional motion

only,

we have shown

that,

at least for

TBBA,

there is no orientational

ordering

around the

long axis,

as

predicted by

the

microscopic

theories in which the

dipole-dipole

interaction

play

an essential

role,

in the tilted Sm H and Sm VI

phases.

It thus

seems that the tilted and non-tilted smectic

phases

should be characterized

by

a criterion other than the existence or non-existence of a strong

dipolar

inter-

action between the molecules. This result has received

recently

a chemical

confirmation,

where a mesogen, whose molecules have no

dipole

moment on the

body,

has been

synthetized,

and

which,

in

spite

of

this,

presents a smectic C

phase [241

Finally

we want to comment on the conclusions Note added in

proof :

In a recent letter

(SELIGER, J., OSMDKAR,

R.,

2AGAR,

V. and

BLINC,

R.,

Phys.

Rev.

Lett. 38

(1977) 411),

14N nuclear

quadrupole

reso-

nance data in TBBA have been

presented and,

for the H

phase,

it was concluded that the results may be

interpreted

within the

Meyer-McMillan

model. In

we drew in ref.

[16].

That reference

corresponds

in

fact to results

preliminary

to those

presented

here.

The

interpretation

was however somewhat different.

In

particular

for the increase of the EISF as the tem-

perature was lowered in the

supercooled

H

phase,

it was

suggested

that this could

correspond

to some

kind of orientational

ordering announcing

the Sm VI

phase.

In this

analysis

we had

only

considered a

simple

uniaxial rotation of the molecules around the

long

molecular axis. In fact the DTBBA molecule contains five kinds of

protons

and

using

a

unique gyration

radius is

certainly

an

oversimplification.

The

good

agreement at 119 °C with a

simple

uniaxial rotational model was obtained with a

gyration

radius of 2.5

A

which is much

larger

than the average of the

gyration

radii we have used in the

present

work. The rise of the EISF with

decreasing temperature

in the super- cooled H

phase

can thus be

interpreted

as due to

the

freezing

out of the fluctuations of the

long

mole-

cular axis. On the view of the new results of ref.

[11]

and of this paper, based on a more realistic theore- tical treatment

(in particular,

it

clearly

appears now that the

gyration

radius should not be taken as an

adjustable

parameter, as was done in ref.

[16]),

one

should

replace

the conclusions of ref.

[16] by

those

presented

here.

Acknowledgments.

- VVe are indebted to Pr.

P. G. de Gennes for

stimulating

discussions and

reading

the

manuscript.

a

subsequent

paper

(to

be

published)

we have shown

that these data may also be

interpreted

in terms of

a model which is consistent with the

NQES

results.

The reverse however is not true

[10, 11].

For the

VI

phase,

we have shown that both methods lead to

remarkably

consistent conclusions.

References [1] MEYER, R. J. and MCMILLAN, W. L., Phys. Rev. A 9 (1974) 899.

[2] MEYER, R. J., Phys. Rev. A 12 (1975) 1066.

[3] DOUCET, J., LEVELUT, A. M. and LAMBERT, M., Phys. Rev.

Lett. 32 (1974) 301 ;

DOUCET, J., LEVELUT, A. M. and LAMBERT, M., J. Physique

35 (1974) 773 ;

DOUCET, J., LEVELUT, A. M., LAMBERT, M., LIEBERT, L.

and STRZELECKI, L., J. Physique Colloq. 36 (1975) C1-13.

[4] Luz, Z. and MEIBOOM, S., J. Chem. Phys. 59 (1973) 275.

[5] Luz, Z., HEW, R. C. and MEIBOOM, S., J. Chem. Phys. 61 (1974)

1758.

[6] DELOCHE, B., CHARVOLIN, J., LIEBERT, L. and STRZELECKI, L.,

J. Physique Colloq. 36 (1975) C1-21.

[7] MEIROVITCH, E. and Luz, Z., Mol. Phys. 30 (1975) 1589.

[8] DVORJETSKI, D., VOLTERRA, V. and WIENER-AVNEAR, E., Phys. Rev. A 12 (1975) 681.

[9] HERVET, H., VOLINO, F., DIANOUX, A. J. and LECHNER, R. E., J. Physique Lett. 35 (1974) L-151.

[10] HERVET, H., VOLINO, F., DIANOUX, A. J. and LECHNER, R. E., Phys. Rev. Lett. 34 (1975) 451.

[11] VOLINO, F., DIANOUX, A. J. and HERVET, H., J. Physique Colloq. 37 (1976) C3-55.

[12] PRIEST, R. G., J. Chem. Phys. 65 (1976) 408.

[13] CABIB, D. and BENGUIGUI, L., J. Physique 38 (1977) 419.

[14] VOLINO, F., DIANOUX, A. J. and HERVET, H., Proceedings of

the VIth Int. Liq. Cryst. Conf., Kent, Ohio (1976), Mol.

Cryst. Liq. Cryst. 38 (1977) 125.

[15] VOLINO, F., DIANOUX, A. J., HERVET, H. and LECHNER, R. E.,

J. Physique Colloq. 36 (1975) CI-84.

[16] VOLINO, F., DIANOUX, A. J. and HERVET, H., Sol. State Commun. 18 (1976) 453.

[17] LEADBETTER, A. J., RICHARDSON, R. M. and CARLILE, C. J.,

J. Physique Colloq. 37 (1976) C3-65.

[18] DIANOUX, A. J. and VOLINO, F., Mol. Phys. (1977) in print.

[19] BARNES, J. D., J. Chem. Phys. 58 (1973) 5193.

[20] DIANOUX, A. J., VOLINO, F. and HERVET, H., Mol. Phys. 30 (1975) 1181.

[21] DE VRIES, A., J. Chem. Phys. 61 (1974) 2367.

[22] DESCAMPS, M. and COULON, G., Sol. State Commun. 20 (1976)

379.

[23] BLINC, R., LUZAR, M., VILFAN, M. and BURGAR, M., J. Chem.

Phys. 63 (1975) 3445.

[24] GRAY, G. W., private communication.

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