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HAL Id: jpa-00246766

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Dynamics of the commensurate-incommensurate phase transition in C2O4D ND4, 1/2 D2O: a polarized Raman

study under pressure

M. Krauzman, A. Colline, D. Kirin, R. Pick, N. Toupry

To cite this version:

M. Krauzman, A. Colline, D. Kirin, R. Pick, N. Toupry. Dynamics of the commensurate- incommensurate phase transition in C2O4D ND4, 1/2 D2O: a polarized Raman study under pressure.

Journal de Physique I, EDP Sciences, 1993, 3 (4), pp.1007-1029. �10.1051/jp1:1993180�. �jpa-00246766�

(2)

Classification

Physics

Abstracts

33.20F 64,70R 64.60C

Dynamics of the commensurate-incommensurate phase

transition in C~04D ND4, 1/2 D~O

: a

polarized Raman study

under pressure

M, Krauzman

(~),

A, Colline

(~),

D, Kirin

(2),

R, M. Pick

(I)

and N,

Toupry (~)

(~)

D6partement

de Recherches

Physiques (*),

Universit6 P, et M, Curie, 75252 Paris Cedex 05, France

(2) Institut Ruder Boskovic, 41000

Zagreb,

Croatia

(Received 5 June J992,

accepted

in

final

form 28 October

1992)

R6sum6. Les spec~es Rarnan

polaris6s

de basse

frdquence

de AHOD ont 6t6 d6terrr1n6s h 6,4 kbar dons les

phases

norrrale et incommensurable.

L'analyse

des deux

pics

centraux visibles

dans les deux

phases,

et des trois

phonons

acoustiques rendus visibles dons la distorsion incommensurable, corrobore les r£sultats obtenus r6cemment par diffusion de neutrons dons la

phase

norrrale [10], et 6tend ceux-ci h la

phase

incommensurable, En

particulier,

l'dvolution du temps de r6sidence des ions

ND(

dons cette demi~re

phase,

ddterrr1n6e h

pant

de

plusieurs expdriences, indique

un accroissement notable de la bam~re de

potentiel

par rapport h la

phase

norrrale.

Abstract, Polarized low frequency Rarnan spectra of AHOD have been measured at 6,4 kbar both in the normal and in the incommensurate

phases,

The evolutions of two central

peaks,

visible in the two

phases,

and of the flwee acoustic modes made active

by

the incommensurate distortion

have been

analyzed.

The results are in good agreement with the values deduced from a recent

neutron experiment in the normal

phase [10],

and extend them to the incommensurate one. In

particular,

the

ND(

residence time is determined

through

various methods in the latter

phase,

and

provides

evidence for an increase of the barrier

height

with respect to the disordered

phase.

1. Introduction.

Ammonium Oxalate

hemihydrated, NH~C~O~H, H~O (in

short

AHO)

and its

fully

deuterated 2

analog (AHOD)

have been

recently

the

subject

of several

investigations

motivated

by

their remarkable

phase diagram,

This

diagram

has been constructed from Raman

experiments [1-3]

up to 8 kbar and down to 80 K, The nature of the

phases

involved has been established

through

(*) U-R-A- 71.

(3)

a series of X

Ray [4-5],

Brillouin

[6]

and elastic neutron

[7] scattering

measurements and

figure

I

reproduces

our present

knowledge

of the

phases appearing

in AHOD, Phase I

belongs

to the

D(((Pmnb )

space group with Z

=

8 formula units per cell, The

phase

I-II transition is

equitranslational,

and of the second order type, Phase II

belongs

to the

Cl

~ PI ~~

l space group and the elastic constant

C55

tends to zero at the

phase

transition.

n

Phase I-III transition is also second order, while

phase

III-II transition is first order. It was established

[3-7]

that

phase

III is incommensurate with wavevector qo =

3c*,

where 3 is a function of pressure

only,

3

increasing

from 0.04

[8]

in the

vicinity

of the critical pressure

P~

to

approximately

0.23 at 8 kbar. Furthermore, from a

polarization analysis

of the Raman

spectra [3],

it was concluded that the variable which freezes in

phase

III

transforms,

in

phase I,

as the v~

representation [9]

of qo.

These

experiments

have

suggested

that the two second-order

phase

transitions have the same

origin

and can be understood in the

following

way. In the

high

temperature

phase

I, the 8

ND(

cations lie on a mirror

plane [4]

and thus form two distinct families, One of them is disordered

[4],

and the two

symmetrical positions

of each cation with respect to this statistical mirror

plane

may be

represented by

the two values of a

pseudospin.

For each lattice

cell,

one

2

can form four different linear combinations of these

pseudospins,

each of them

transforming

as a different irreducible

representation

of the

crystal point

group. One of these

combinations,

which will

play

the

major

role

here,

transforms as the

B~~ representation,

and we shall, in accordance with

[10],

call

~r)

this linear combination in the

L~ cell,

and

~r~(q)

its Fourier

transform

(up

to

phase

factors

[10]

which are irrelevant for the

present discussion).

The bilinear interaction energy between two

pseudospins

can be written in terms of these linear

combinations, Let us call

Jd(q)w k~ Td(q), (1)

(where k~

is the Boltzmann

constant)

the Fourier transform of this interaction energy between two ad variables

belonging

to different cells. The model

proposed

in

[3]

for the two second- order transitions of

figure

I is that the same variable

~r~(q

drives the two transitions, and that :

a) Td(q) depends only

on pressure its maximum

simply

moves from q = 0 below the critical pressure

P~,

to a wave vector

along c*,

above

P~.

b)

For all values of q, and in

particular

for q in the

vicinity

of the direction of

c*,

there exists

a strong linear

coupling

between

~r~(q)

and a

pseudo

transverse acoustic

phonon

with normal mode coordinate

Q(q),

the elastic limit of which for q -

0, qflc*

is the e~~ shear

(which

transforms,

in this

limit,

as the

B~~ representation).

This model

agreed,

inter alia, with the Raman detection

[3],

in

phase

III, of two low

frequency

excitations which were identified as two acoustic

phonons

with wave vectors qo. These two excitations were

mostly

studied in

AHO, though

some measurements were also

performed

on AHOD

[I],

From the

polarization

in which

they

were

detected,

and from their

frequencies

which could be related to the known elastic constants of AHO in

phase

I, one of these excitations was found to be the LA

phonon,

which

appeared

in the ac

polarization,

while the second one, ab

polarized,

was identified as the b

polarized

TA

phonon,

A weaker

signal,

aa

polarized,

at the same

frequency

as this TA

phonon

was also

detected,

and attributed to a

polarization leakage

the absence of a lower

frequency signal

in that

geometry

led the auth6rs of

[3]

to

conjecture

that the

coupling

of ~r~

(qo )

with

Q (qo )

was so strong that the

frequency

of the a

polarized

TA

phonon

remained too low to be detected with their

equipment

in the whole

temperature

domain accessible in

phase

III,

Neutron inelastic

scattering experiments [10] (here

after referred to as

I)

have been

recently

(4)

performed

in

phase

I of

AHOD,

at 0 kbar and 5 kbar at some

temperatures

above

(including

close

to)

the second-order

phase

transition.

They

confirmed the

predictions a)

and

b)

of the

preceding

model but also showed that, at 5

kbar,

the a

polarized

TA

phonon

branch

essentially

did not

soften, except

in the immediate

vicinity

of q =

0,

contrary to the

hypothesis

made in

[3].

This

implied

that, if w~~ is the

frequency

of a

phonon

on this TA branch, and v is the

mean residence time of an individual

ND(

ion in one of its two orientational

wells,

the

relationship

w~~ v ~ l is fulfilled for most of the

phonons

of that branch in the whole

phase

I ; values of v

(T)

consistent with this

inequality

were in fact deduced from the 5 kbar

experiment.

The purpose of this Raman paper is twofold. First, we wish to confirm the value of this mean residence

time,

which can be deduced from the

study

of a central

peak,

as was shown in

[2],

This central

peak

is related to the individual

pseudospin dynamics,

and appears in two different

polarizations,

which

probe

the

dynamics

of two different collective

variables, ~r~(q)

and

~r~(q) [10],

in the q =

0 limit. Due to

improvements

of our Raman

equipment,

and to the construction of a new pressure cell

[I Ii,

such measurements, which were

formerly possible only

at zero pressure and for strong

signals [2]

are now

feasible,

under pressure, With an increased accuracy, whatever the

polarization

geometry, and can be made both in

phases

I and III.

They

will

provide

us with information on v

(T)

in both

phases

on an AHOD

crystal

of the

same

origin

and

quality

as that used in

[10].

We also wish to

clarify

the

origin

of the weak low

frequency signal

with aa

polarization

obtained in

[3]

at the same

frequency

as the b

polarized

TA

phonon,

It was found in

[10]

that the two bare elastic constants

C44

and

C~5

have

approximately

the same value ; this

suggested

that the aa

polarized signal

could be due to the a

polarized

TA

phonon

and not to a

polarization leakage

of the other TA

phonon,

With the

improved quality

of our

equipment,

it is also

possible

to check this

point,

and this will also represent an

independent

way of

measuring v(T)

in

phase

III,

In order to illustrate the various aspects of this

work,

our paper is

organized

as follows, In section

2,

we

briefly

discuss the

dynamics

of all the low

frequency

excitations which could be visible in a Raman

scattering experiment,

first in

phase I,

and second in

phase III,

where the

new

couplings provided by

the

freezing

of an incommensurate distortion lead to a much more

complex

discussion. Section 3 is devoted to the

description

of the Raman

experiments performed

at 6.4 kbar and of the

tecllniques

used to extract numerical information on the

various spectra we are interested in. The

qualitative

thermal behaviour of these spectra is discussed in section 4 and found to agree with the

predictions

of section 2. The

quantitative analysis performed

in section 5 and the discussion of these results show that a coherent

picture

of the

phase

I-III transition and of the

dynamics

of the relevant excitations can

presently

be

made.

Finally

a summary of this work, as well as some

concluding

remarks are done in

section 6.

2. Low

frequency

excitations visible

by

Raman

spectroscopy.

A review.

This section is devoted to a brief review of the effects which have been detected in our Raman

experiments

on AHOD under pressure,

performed

both in

phase

I and in

phase III,

in the low

frequency region.

For temperatures above the

transition, light couples only

to excitations at q =

0, and,

in the

frequency regime studied,

no

dynamics

other than the

pseudospin

one is accessible, Below the

transition,

on top of the same

dynamics, light couples primarily

to the excitations at ± qo, and the latter

comprise

both the

spin dynamics

and the acoustic

phonons.

Except

for one

special scattering

geometry, in the incommensurate

phase,

these

dynamics

are

not

linearly coupled,

so that the situation will tum out to be

relatively simple,

On the other hand,

through

the incommensurate modulation, the

pseudospins

at q = qo are

coupled,

in

phase III,

to other low

frequency excitations,

and we shall have to

explain why

these spectra

can nevertheless be understood in terms as

simple

as in the

high temperature phase.

(5)

2.I THE PHASE I SftUATION. As recalled in the

Introduction,

in the

high

temperature

phase,

in each

elementary cell,

4

ND(

ions exhibit orientational disorder,

They

all

belong

to the same

family,

and, inside one

primitive cell,

one can form four different linear combinations of the

corresponding pseudospins,

which transform

respectively

as the

B~~, A~, Big

and

B~~ representations

of the

crystal point

group

[2]

; these combinations have been labeled

respectively

~r~, ~r~, ~r~ and ~r~ in I.

Only

the last two are Raman active and we shall discuss in tum their

spectra.

2,I.I The

B~~ pseudospin.

The free energy related to the ~r~

pseudospins

and to the

transverse acoustic

phonons, Q (q ),

to which

they

are

linearly coupled

has been discussed in I.

When

specialized

to wave vectors q

parallel

to

c*,

this free energy, limited to its harmonic

part,

reads :

Fd

=

z ik~ (T

Td

(q)) ~r~(q) ~r~(-

q

)

+

idq iQ (q)

~r

(- q)

c-c-

i

+

o] q2 Q (q) Q (-

q)1

~

(2)

where :

~r~(q)

is the Fourier transform of

~r).

Q(q)

is the normal coordinate of the a

polarized

TA

phonon

with sound

velocity

ilo.

d is a constant which

couples

these two

variables, while,

in the

approximation

used in

I, T~(q) reads,

for

qflc

:

T~(q)=

-A

(B-c)cos~j~-Kcosq.c (3)

where

A, B, C,

K are interaction energy constants related to different ty1Jes of

neighbours

of a

given pseudospin. d,

as well as the coefficients ofT~

(q ) depend

on pressure

only,

and d is

large enough

to increase the transition

temperature

from

T~(0 )

= 65 K to

Tf

=

160 K at 0 kbar and from

T~(qo )

= 57 K to

T(

= 137.5 K at 5 kbar for instance.

Writing

for the

equations

of motion of these two variables

Q

and ~r~.

~

~F

= w

2

Q (q )

~

~~

=

i w

k~

Tv ~r~

(q ) (4)

where v is an individual

pseudospin

mean residence time, one obtains for the

pseudospin dynamics

:

lad (q,

w

)

ad

(q,

W

) *>

=

(I

+ n

(w ) )

3m

l~

~ ~

(5)

kB(T T~(q)) iwkB

TV

~~~~

*o

q W ~

For q -

0,

as the

spectrum

is studied

only

in a

frequency

range for which w »

do

q, the last term in the denominator of

equation (5)

is

negligible,

and the latter reduces to its first two terms, which leads to a Lorentzian central

peak

for the response function.

2.1.2 The

Bi

~

pseudospin.

Let us call

~r~(q)

the Fourier transform of the

corresponding pseudospin

variable. For

qfc*,

them exists no acoustic

phonon

which transforms

as

~r~(q)

and the

only

relevant

part

of the free energy is

simply

:

F~

=

z ik~(T Tc (q)) ~rc(q) ~rc(- q)1 (6)

q

(6)

where

k~ T~(q

is the

corresponding

interaction energy.

Calculating

this interaction energy

by taking

into account the same

pseudospin

interactions as those used to obtain

T~(q),

one

finds,

for

qflc*

T~(q)=

-A+

(B-C)cos~'~-Kcosq.c, (7)

2

Making

use of an

equation

of motion similar to

equation (4) yields,

for this

pseudospin

response function :

(«c(q, W) «c(q, W)*)

=

(i

+

n(w ))

am

~

~~

~

~

~ ~

(8)

I,e, to another central

peak,

with an

expression

identical to the

simplified equation (5) except

for the

change

of

T~(q)

into

T~(q),

2.2 THE PHASE III INCOMMENSURATE CASE. The situation in the incommensurate

phase

is

more

complex,

as one can detect excitations both at q = qo and at q =

0, Let us start with the first ones, As was shown e,g, in

[12],

the Raman tensors which

couple

an excitation at q = qo with the incident

light

are

proportional

to the order

parameter

~ =

(~r~(q~))

and the Raman

intensities,

at any

frequency,

of the excitations detected

through

this mechanism will be

proportional

to

~~,

Let us

discuss,

in tum, the various

spectra

which can be detected in

AHOD.

2,2,1 The LA

phonon

and the b

polarized

TA

phonon. Along

c

*,

the

pseudospins

transform

respectively

as the v~

representation

of the group of q~ for the two

pseudospin

variables

~r~(q )

and

~r~(q )

and as the r~

representation

for

~r~(q

and ~r~

(q ),

The LA

phonon

transforms

as v~ and the b

polarized

TA

phonon

as v~

[9],

These two

phonons

are thus not

coupled

to any

pseudospin

:

then,

one

expects

their

frequency

to be

temperature independent,

and their linewidth

quite

narrow as for any acoustical

phonon, Furthermore,

as shown in

[3],

the LA

phonon

must appear in the ac

polaTization,

and the b

polarized

TA

phonon

in the ab

polarization,

2,2,2 The a

polarized

TA

phonon

and the ~r~

(q ) dynamics.

In order to obtain the

dynamics

of these two variables at ± q~, the usual Landau type treatment

[13]

of the statics and of the

dynamics

of soft variables close to an incommensurate

phase

transition must be

performed, Stating

that the

driving

mechanism of this

phase

transition is the ad

(q)

variable and

adding

to the free energy

(Eq, (2))

a fourth order term in this variable, the latter can be written as ;

F~

=

z

kB

(T Td(q)) "d(q) "d(- q)

+

q

+

Z ( "d(qi ) "d(q2) "d(q3 ) "d(q4)

3

(qi

+ q2 + q3 +

q4)

qt.q~.q3.q4

+

j z q(Q (q)

«

(- q)

c.c.

)

+

z *# q~ Q (q) Q (I q) (9)

where b is a

coupling

constant which

depends

on the four q~ vectors and

which,

in this subsection, will be used

only

for qi, q~, q~ and q~ in the

vicirdty

of ± qo,

Writing

that the transition which takes

place

at qo leads to an

equilibrium

state

yields

:

'7~ =

("d(qo))

~

=

~

kB lTd(qo) Tj

+

~~

m

~/ [Tt Tj (ioa)

I

*o

(7)

iQ(qo)j

=

j i"d(qo)j (lob)

with :

bi

« b

(qo,

qo, qo,

qo). (i i)

In the mean field

approximation,

below this

transition,

two of the four

spin

variables

appearing

in the second term of

equation (9)

must be taken at their

equilibrium value,

while the other

spin

or

phonon

variables are taken as the fluctuations around their

equilibrium

values. The

bi

terms, then,

couple

q

= qo + h to q = qo +

h,

whatever h,

through

a term

proportional

to

~ ~, while

«~(q)

and

Q (q)

are still

coupled by

the d term. There are thus four variables which

are

linearly coupled,

the

dynamics

of which are

degenerate

in

pair

for h

=

0,

in the absence of the ~~

coupling,

To understand the solutions of the

dynamical equations

for q

= qo, it is useful to

study them,

first for h x

0,

and then to let h tend to zero.

Let us make use of this classical

method, choosing

for

simplicity

h to be

parallel

to

c*,

and let us take the

pseudospin amplitude

and

phase

mode variables as

dynamical variables,

Q~(h)

=

fi j«d(q0

+

h)

e~'~

«d(~

q0 +

h) e~~j (12b)

2 where :

(~r~(qo))

= ~ e~~

(13)

with similar

expressions

for the

phonon amplitude

and

phase

mode variables,

Using

equation (4)

and

postulating

that a part of the response function is located in the

vicinity

of

w =

0,

while the other part appears in the

vicinity

of too

=

do

qo, one

obtains, through

a

calculation which is

briefly

sketched in the

Appendix,

the

following

results.

Vicinity of

too =

do

qo, Two excitations have their spectrum in the

vicinity

of the

unperturbed

TA

phonon frequency

in the h

- 0 limit. One is of the

amplitudon

type, and its spectrum is

proportional

to :

~~~~~°

~~ ~

~~~°

~~ ~~

l~

~

2

~

2

k~

(T~

T)

+

k~

(T~

T~(qo))

I

wk~

Tv

(14)

The

intensity

of this spectrum is

proportional

to ~~. It represents the

dynamics

of an acoustic

phonon coupled

to a diffusive

pseudospin,

this

coupling becoming

smaller as T

decreases,

because the real part of the

pseudospin dynamics

increases with T~ T, while its

imaginary

part increases

exponentially through

the temperature

dependence

of v. It is Raman active in any of the three

diagonal polarizations.

The second excitation is of the

phason type,

in the h

- 0

limit,

both

through

its

eigenvector,

which is a linear combination of the two

phase

mode

variables,

and

through

the

algebraic expression

of its spectrum which reads

~~~~~~

~~ ~

~~~~~

~~

~j(

~j_

~

~2

~~~~

k~(T(qo)

T~) I

wk~

Tv

(8)

Indeed,

as for any

phase mode,

the real part of the term in

d~

does not

depend

on

temperature (compare Eqs. (14)

and

(15)).

As this mode is not Raman

active,

it will be of no interest here.

Vicinity of

w

= 0. It was shown in I that the

pseudospin dynamics

becomes

critical,

I-e-

gives

rise to a central

peak

with HWHM

tending

to zero, in the

vicinity

of the normal- incommensurate

phase transition,

for q in the

vicinity

of qo. Below T~, in the same manner as for the excitations in the

vicinity

of the bare

phonon frequency

discussed above, the two

corresponding

diffusive modes at ± qo

couple

into an

amplitudon

type central

peak,

and a

phason

type central

peak

; this is shown in the

Appendix,

and was

briefly discussed, recently,

in

[14].

The

amplitudon

type central

peak

has an

intensity proportional

to :

'l~SA«(W)

=

'l~il

+

n(w)13m

~

hi

'l

iWkBTT (16)

Its

integrated intensity

is thus

proportional

to

k~ T,

I-e- non critical close to T

= T~ while its linewidth is

proportional

to T T~

similarly

to the

phonon

type

amplitudon (Eq. (14)),

this

spectrum

has a

diagonal polarization,

and could

thus,

be detected a

priori,

in any of these

polarizations.

In

fact,

we have not detected

it, and,

as will be shown in section

6,

this is due to its too small

HWHM,

in the whole temperature range studied.

As for the

phason

type central mode

(Eq. (A7),

second

line)

it has, in a

light scattering experiment,

a linewidth much narrower than the central

peak

of

equation (16).

This excitation is thus not detectable

by

Raman spectroscopy even if its Raman

activity

is not

identically equal

to zero, as is

presumably

the case if one makes use of arguments similar to those used for the

displacive phason [12].

2.2.3 The

Bi~ pseudospin

variable spectrum. The

spectrum

of the

~r~(q)

variable in the

vicinity

of q = 0 was

already discussed,

above the

phase

transition, in subsection 2.1.2. We must reconsider the situation below the

phase transition,

because the

freezing

of the

pseudospin

at ± qo

couples

this variable to

pseudospins

in the

vicinity

of ± 2 qo.

Indeed, taking

into account

only

the terms which lead to such a

coupling,

and

limiting

the

pseudospin

wave

vectors to be

along

the c*

axis,

the relevant part of the free energy reads :

F~

=

zkB(T- T~(q)) ~r~(q) «~(- q)

+ q

~c

+

Z

~ "c(qi "c(q2) "d(q3) "d(q4)

3

(qi

+ q2 + q3 +

q4) (1?)

q; q2. q3. q4

where b~ is a function of the four wave vectors. In the mean field harmonic

approximation,

below T~,

~r~(q~)

and

~r~(q~)

will be

replaced by

their thermal mean value, with

amplitude

~. If one takes q~ = q~ = ± qo this term

simply

renormalizes the

k~ (T T~(q ))

term,

adding

to it a term

equal

to

b[

~ ~, which in view of

equations (6)

to

(8),

modifies the thermal evolution of the

corresponding

central

peak.

If,

on the other

hand,

one

considers,

for

instance,

q~ = q~ = qo, the

corresponding

term

couples

the

dynamics

of

~r~(q)

with that of

~r~(q

2

qo) through

a term

proportional

to

b[

~~; a similar

coupling

exists with

~r~(q

+ 2

qo)

for q~ = q4 " qo. Nevertheless, if q is in the

vicinity

of the Brillouin zone center, T~

(q )

x

T~(q

+ 2

qo)

m

T~(q

2

qo).

This means that

the bare

dynamics

of

~r~(q)

is not

degenerate

with that of

~r~(q

± 2

qo).

In a

perturbative approach,

this

gives only

a correction in

~~

to the

dynamics

of

~r~(q),

an effect which can be

neglected

with

respect

to the

b[

~ ~ correction described above.

(9)

Thus

equation (7) yields

:

(«c (q,

W

)

«c

(q,

W

)*)

=

Ii

+ n

(w )j

am

~ ~

(18)

with :

bi

m bc

«c(q) «c(- q) «d(qo) «d(- qo)

q - o.

(19)

In the mean field

approximation

used

here,

~ ~ is

proportional

to T~ T

but,

since the value of

b[

is

unknown,

one can

only predict

the appearance of a second term linear in T in the real

part

of the denominator of

equation (18).

As will be seen in section

4,

in the

present

case, I-e- for AHOD at 6.4

kbar,

it will reverse the

sign

of the coefficient of T. Let us

finally

note

that,

as this

spectrum

was

already

visible

above the

phase transition,

in the ab

polarization,

it will remain visible

through

the same mechanism below T~.

2.2.4 The

B~~ pseudospin

variable at q = 0. In

principle,

the situation is

quite complex

as

one must combine the difficulties met in subsections 2.2. I and 2.2.3

(I.e.

the linear

coupling

between

phonons

and

pseudospins)

on the one

hand,

the

coupling

between the excitations at q, q + 2 qo and q 2 qo and the renormalization of the coefficient

k~(T T~(q)),

on the other

hand. The

analysis

is rather cumbersome but shows that the

only significant

effect is the last one, as was

already

the case for the

«~(q) dynamics,

both the

coupling

with the acoustic

phonons (as

in subsection 2.

I-I)

and the

coupling

with the

pseudospins

at q ± 2 qo

(as

in subsection

2.2.3) being negligible.

One thus

obtains,

in

analogy

with

equation (18)

:

("d(q, W) "d(q,

W

)*)

=

Ii

+

n(w)]

am

~ ~

(20) kB(T Td(q))

+

b2

'l i

wkB

Tr

with :

b(

m b

(q,

q, qo,

qo)

q

- ° ~~~~

b(qi,

q~, q~,

q~) being

defined

by equations (9)

and

(

II

).

Comparing equations (5)

and

(20),

as well as

equations (8)

and

(18),

one sees that the effect of the

phase

transition on the spectra related to the

dynamics

of the

«~(q)

and

«~(q)

pseudospins

at q =

0 is

absolutely

similar. It

simply changes

the

slope

of the coefficient in Tin the real

part

of a

denominator,

thus

changes

the thermal behaviour of the HWHM of the

corresponding

central

peak.

It does not

change

its

polarization properties

so that the

«~(q) dynamics

will still appear in the ac

polarization.

3.

Experiments.

3.I EXPERIMENTAL DEVICE. The present

experiments

have been

performed

with a

8 x 7 x 7

mm~ crystal

of AHOD obtained

by

the

evaporation technique

in the same bath as for

the neutron

experiment

of I. The

sample

was oriented with its a axis

perpendicular

to the

scattering plane,

the

incoming

beam

being parallel

to c and the scattered beam

parallel

to b. A helium pressure cell with three

saphire

windows

containing

the

crystal

was

placed

in a vacuum cryostat with silica windows. Pressure was measured within ± 5 bar

by

a

manganin

resistor in a

secondary

cell, at room temperature, and the temperature of the

crystal

was

probed by

a

Chromel Alumel

thermo-couple

at room pressure inside a 3 mm in diameter

pipe penetrating

(10)

the

sample cavity.

Raman

spectra,

excited

by

the 514.5 nanometer line emitted with a power of 0.I to 0.2 W

by

a

Spectra Physics Argon

ion

laser,

were recorded with a

Coderg

T800

triple spectrometer

modified in order to be driven

by

an IBM AT3 Personal

Computer

which collected and stored the

signal

from a cooled RCA 31034-06

photomultiplier.

Data were taken

during

one

second,

every 0.125 cm~ ~, and the

origin

of the

frequency

scale was checked and

occasionally

shifted within half a step after

comparing

the Stokes and the antistokes part of the

spectra.

All the

experiments

discussed below were

performed

at 6.4

kbar,

between room

temperature

and 78 K

although

some

preliminary

tests were

performed

at a lower pressure to ascertain the

position

of the

phase

II-HI transition for

fully

deuterated AHOD.

Taking

this information into account, the

general

form of the

phase diagram,

as well as the other transition

temperatures

shown in

figure I,

the 6.4 kbar pressure was chosen as a

compromise

between two

opposite points

of view :

The pressure must be as close as

possible

to 5

kbar,

in order to allow for a fruitful

comparison

with the neutron

experiment

of I.

The first order

phase

II-m transition must take

place

below 78

K,

so that the

phase

III

dynamics

can be studied in as

large

a temperature interval as

possible.

iii

i

Z

r0

f

Ii

T

140

~

T K ~

Fig.

1. Phase diagram of fully deuterated AHOD. The transition points have been obtained from

neutron data (round [8] and square [10] dots) and Rarnan data obtained

during

the present set of

experiments

(crosses). Phase III exists only above

P~

= 2,4 kbar and below T~ = 147 K [10].

3.2 EXPERIMENTAL TECHNIQUE. At each temperature, the four different

spectra

with

respective polarizations

aa,

ab,

ac and bc were

recorded,

from 150 to 150 cm~ as well as

(he

aa

polarized

spectrum from 840 to 910

cm~~

which contains a

sharp

line near

8~ficm~

~, the

integrated intensity

of which was used as an intemal

intensity

standard. In this

high frequency

range, there also

exists,

in the bc

polarization

a line whose

frequency (851

cm~ ~) is

temperature independent

in

phase I,

and which

splits

into two lines in

phase

III.

The transition

temperature

was

accurately

determined

by recording

the 851 cm

intensity

as a

function of temperature : due to this

splitting,

the 851 cm~

intensity drops rapidly

below the

transition and the same

result,

T~ =135.5 K ± 0.3

K,

was found either

by cooling

or

by

warming

the

sample,

in a

good agreement

with the

extrapolation

of the neutron results

(Fig.

I

).

(11)

Careful

setting

of the

polarizers

resulted in correct

polarizations

as can be checked in

figure

2 which represents, at the temperature T = 78.3 K, far below T~, the Stokes part of the four recorded spectra up to I IO cm~ :

indeed, leakages

from strong lines do not appear in

unallowed

polarizations.

As

expected,

Lorentzian

peaks

appear

only

in the ac and ab

polarizations.

Nevertheless, extemal modes of the

crystal

are located above 50 cm~ ~, and

they

are broad

enough

to

produce

a substantial

(and frequency dependent)

contribution 15 to 20 cm~ below their maximum,

especially

in

phase

I. In order to obtain the pure

pseudospin

dynamics,

it is necessary to subtract this

frequency dependent

«

background

». This was

performed by representing

the

corresponding

extemal modes

by damped oscillators,

charac- terized

by

their

frequency,

linewidth and

intensity

evaluated

by

a fit of the

spectra

above 50 cm~

78.3K 6.Skbar

[

~ ab

~

-

bc

aa

50 ioo

w

(cm-') Fig.

2. Rarnan spectra at T

=

78.3 K and P

=

6.4 kbar in the aa, ac, bc and ab

polarizations.

3.3 AcousTic PHONONS.

IySTRUMENTAL

LINEWIDTH DEcoNvoLuTioN. In order to

study

in

detail the thermal evolution of the acoustic

phonon

lines, it was necessary to deconvolute the latter from the instrumental linewidth ; this deconvolution

plays

no role for the continuous spectra discussed above. It

is,

of course, the deconvoluted values of the linewidths and the

frequencies

of these acoustic

phonons

which are

reported

in

figures

5 to 7.

4.

Qualitative

discussion~

4,I AcousTlc PHONONS.

Figure

3 represents, for the same temperature as in

figure 2,

T

=

78.3

K~T~,

a

portion

of the same spectra,

represented

on an

expanded

scale and

arbitrarily

normalized at the same 885 cm~

peak integrated intensity.

Three

spectra

show the

LA,

the a

polarized

and the b

polarized

TA

phonons respectively

at q = qo. Due to the very

good polarization quality

of our

experimental setting,

there is no

polarization leakage,

while our detection accuracy allows for a resolution of about 1.7 cm ~. In

figure 3,

it appears that the

aa and ab spectra have maxima at different

frequencies. Furthermore,

as can be seen in

figure

4 which shows similar spectra recorded at a

higher

temperature, the two lines have different

linewidths, indicating clearly

that these two spectra do not

correspond

to the same

excitation,

and are thus the two TA modes.

(12)

~

~

i

" ~

§

~

d ~

ac

6.Skbar

l17K

20 50 20 30

w

(cm-')

W

(cm-<

F~g. 3. Fig. 4.

Fig.

3. Enlargement of the low frequency part of figure 2 (presented in a different order). Note the excellent

polarization

of the four spectra.

Fig.

4.

Comparison

of the b and a

polarized

TA

phonons

at 117 K. The latter is broadened by the interaction with the «~

pseudospin.

The

meaningful

results of fits of each line with a

simple damped

oscillator above a linear

background,

convoluted with the

spectrometer

function are

represented

in

figures

5 and 6. In

figure

5, the thermal variation of the three

frequencies

in

phase

III, from 78K up to

T~, is

represented

as

~

for each of the three

phonons.

One sees

that,

while the

frequencies

w

(78 )

of the LA and the b

polarized

TA

phonons practically

do not

change

with

temperature,

the

frequency

of the a

polarized

TA

phonon

decreases when

approaching

T~ from below. A

parallel

type of behaviour can be seen in

figure 6,

where the

corresponding

deconvoluted linewidths

are

plotted

: for the first two

phonons,

the linewidths remain, in the whole

phase III,

smaller than the instrument

resolution,

while this linewidth is

larger

for the a

polarized

TA

phonon,

and increases

notably

when

approaching

the transition temperature.

All these results agree with the

predictions

of subsections 2.2,I and 2.2.2 : the LA

phonon

and the b

polarized

TA

phonon, decoupled

from the

pseudospins,

must be very narrow and have

frequencies essentially

temperature

independent. Conversely,

the

coupling

of the a

polarized

TA

phonon

with

«~(q)

was

expected

to

slightly

decrease the

phonon frequency

and to increase

notably

its linewidth. This increase of the linewidth

is,

in fact, so

large

that it was

already

noticed in I : in Phase

I, along

the whole c*

direction,

the b

polarized

TA

phonon

was

found to be much narrower at 0 kbar and 300

K,

than the a

polarized

TA

phonon

which was measured at various temperatures both at 0 kbar and 5 kbar.

On the contrary, at 5

kbar,

the

frequency change

of the a

polarized

TA

phonon

with temperature was too small to have been detected

by

neutron

scattering

in

phase

I : one needs the accuracy of Raman spectroscopy to evidence it in

phase

III.

(13)

~

~x>

~

~ TAb

-

LA

~

-

T4

3

d

80 loo

Tt

T(K)

Fig.

5. Thermal variation of the

frequencies

of the three acoustic

phonons

relative to their

respective frequency

at 78 K.

TAb

80 loo 120 Tt

T K

Fig.

6. Deconvoluted linewidth r(T) for the three acoustic

plionons.

The small linewidths of the LA and

TA~

phonons are evaluated with a poor

precision

due to the instrumental resolution ( 1.5 cm- ~).

4.2 THE PSEUDOSPIN DYNAMICS. The evolution of the

pseudospin dynamics

with

temperature

is shown in

figures

7 and 8. In

phase I,

the linewidth of these spectra decreases with

temperature

down to T~, while the

intensity

at w = 0 increases when

approaching

the

phase

I-III transition. Below this

transition,

on both spectra,

opposite

effects are seen for the

(14)

ac

loo Tt

T(K)

Fig.

7. Thermal variation of the width (left scale) and

intensity (fight

scale) of the «~

pseudospin dynamics

as fitted to the ac spectrum.

ab

i-

~

-

5

~

E d

U ~j

~'

-

~

fi

~

loo

T

(

K )

Fig.

8. Same as

figure

7 for the «~

pseudospin dynamics

as fitted to ab spectrum.

(15)

intensities : when still

decreasing

the

temperature,

the

intensity

decreases

again.

But the linewidth still decreases below T~, and saturates, or

slightly

increases

again

near 78 K.

The

high

temperature behaviour was

anticipated

from subsection 2,I. For

instance,

the

spectral

response of the ac spectrum was

predicted,

from

equation (5),

to be

equal

to

~~~

~~

~~~~~~

j~(0 )

2

~

~ 2

~~~~

T ~

j~~(o)

T where R~~ is the

corresponding

Raman tensor.

The individual relaxation time increases when the

temperature

decreases while

~~/~

decreases for

T~T~ >T~(0).

This results in an increase of

I~(0)

and a decrease of the

HWHM,

and the same

is,

of course, true for the ab spectrum.

On the contrary, below T~, the thermal evolution of the HWHM and

of1(0)

could not be

anticipated

from the sole

analysis

of the discussion

performed

in subsections 2.2.3 and 2.2.4.

For

instance,

from

equations (10a), (20)

and

(21),

the

spectral

response of the ac spectrum is

given

below T~

by

:

~~~

~~

~~~~

Mac (T)j~

~ W

T ~

~ ~

c

~~~~

(T)

with :

2

b(

j 2

b(

fa~(T)

=

I + T~

T~(0) (24a)

hi

T

bi

It is the thermal evolution both of

fa~(T)

and of r which fixes the thermal evolution of

Ia~(0)

and of the HWHM. As

b(

is

expected

to be of the same order of

magnitude

as

bi, fa~ (T

is

expected

to increase with

decreasing

temperature, as well as r. The present results indicate that r

increases,

close to T~, faster than

f~~(T)

but slower than

lf~~ (T)]~,

and similar

considerations must hold for the

Bi

~

where

f~~(T)

is

replaced by

12b[

j

2b[

fab(T)

~

i

~

+

y ~

Tt

Tc(o) (24b)

One may

simply

note, at this

point,

that we find here for AHOD at 6.4

kbar,

an evolution of

1(0)

and of the

HWHM,

below as well as above T~, very similar to the results we

reported

in

[2]

at normal pressure for AHO. In

particular,

in these

early experiments,

below the

phase

I-II transition temperature,

1(0)

decreased with

decreasing

temperature while the HWHM still decreased in some temperature range before

increasing again.

In section 5, we shall

show,

that

we find for v

(T),

a thermal evolution similar to the evolution of this residence time in AHO at normal pressure, an evolution which

explains

the behaviour

of1(0)

and of the HWHM.

5.

Quantitative analysis

and discussion.

All our

experimental

results

being

in

qualitative

agreement with the theoretical

predictions,

we

have

proceeded

to their

quantitative analysis.

In the next

subsection,

we shall consider first the

integrated intensity

of the acoustic

phonons

in

phase

III, second the

consistency

of the individual relaxation time measurements in both

phases.

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