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Debye-Waller like broadening of the susceptibility peak in CeRu2Si2

L. Puech

To cite this version:

L. Puech. Debye-Waller like broadening of the susceptibility peak in CeRu2Si2. Journal de Physique

I, EDP Sciences, 1991, 1 (7), pp.979-984. �10.1051/jp1:1991176�. �jpa-00246389�

(2)

Classification

PhysicsAbsmacis

75.30M-63.20K-63.20L

Show Communication

Debye.Wailer like broadening of the susceptibility peak in

CeRu2S12

L. Puech

Centre de Recherches sur les ltBs Basses

lbm~dratures,

BP 166J~ 38042 Grenoble Cedex, France

(Received 5Apfil

199«

accepted

13

Mqy 1991)

R6sum6. Los

phonons thermiques

sont

peut

dtre

responsables

de

l'dlargissement

de la transi- tion

pseudo-mdtamagndtique,

observ6

lorsque

la temperature augmente, dans le

compass

fermions lourds

CeRu2S12.

Nous montrons que la

largeur

de la transition observde rdcemment k trds basse

temp6rature

sur la

magn6tostriction,

est en fait en

T~;

avec un

pr6facteur compatible

avec les fluctua- tions de densit6 dues aux

phonons thermiques.

Nous montrons que le

couplage magnon-phonon

est trds fort la

transition,

si bien que les

phonons

de

point

z6ro peuvent y

jouer

un role

important.

Abstract. Thermal

phonons

may be

responsible

for the observed

broadening,

with

increasing T,

of the

pseudolmetama gnetic

transition in the

heavy

fermion

compound CeRu2S12.

The width of the

peak

in the

magnetcstriction coefficient, recently

measured at low temperature, is shown to be

proportional

to

T~;

the

prefactor being compatible

with the

density

fluctuations due to thermal

phonons.

The

phonon-magnon coupling

is shown to be

extremely large

at the transition, sc that zero

point phonons

may

play

there a central role.

1. Introduction.

Since the

pionneering

work of references

[1-3],

many

experiments

have been devoted to the

study

of

thermodynamic, microscopic

and

transport properties

of the

heavy

fermion

compound CeRu2S12.

At low

temperature

and zero

applied magnetic field,

the

system

enters the so called

heavy

fermion

regime, according

to the

large

linear term 7 of the

specific

heat

(7

=0.35

J/mol K~) [1,4].

No

long

range order has been detected in the pure

compound,

but short range anti-

ferromagnetic (A~F)

correlations exist between Ce ions

[5].

When a

magnetic

field is

applied,

the

susceptibility

x exhibit a

large

increase around

Bc,

this is called the

pseudo metamagnetic

tran- sition

[2]. (Bc

=7.8 T at the lowest

temperatures). Correspondingly

the A~F fluctuations

rapidly disappear

when

crossing Bc [5].

Much work has been done to

clarify

what

happens

at

Bc.

It is well established that 7 increases

by

at least

609b,

and that x

apparently gets extremely large

at

Bc, provided

T is low

enough [6],

suggesting

the

possibility

of a transition at zero

temperature,

for which x would

diverge

at T = 0.

(3)

980 JOURNAL DE PHYSIQUE I N°7

Theoretical

approaches generally require

the

vicinity

of some

unstability

due to volume

changes

[7j

or

towards'magnetically

ordered

phases [8,9],

for

predicting

the

pseudo-metamagnetism.

In these

cases there is no transition and 7 and X should

extrapolate

to finite

values,

but in a

temperature

range that has still to be

predicted.

Among

the

experiments performed

on the

compound,

those

involving

ma

gneto-volumic

effects have been very

spectacular

and

useful;

we summarize them here.

Apparently,

the main effect of the

pressure

P on the

magnetic properties

of thin

compound

h a

strong

renormalisation of the energy scales

[3,10,11], especially

of the

magnetic

field B necessary to obtain a

given magnetization

M

usually expressed

in Bohr ma

gneton (pB)

per Ce ion:

m =

I

= m

l~olp~) (i)

In thb

expression,

the field scale B"

(P), changes

with P

by large

amounts, caracterized

by

Q = fij~O

~ = 170

MBar~~

B"

may be chosen as

Bc(P)

or I

/xo(P),

the inverse of the

susceptibility

B" P

at low field.

Equivalently,

this

unusually strong

pressure or volume

dependence

of B"

(P)

may

be

expressed using

a

(dimensionless)

Griineisen

parameter

r =

j~()

=

-~,

where

Ito

is

~

the

compressibility

at zero

magnetic

field. At the

pseudo-metamagnetic

transition around

Bc,

the

susceptibility

[2] x, the

compressibility [13] It,

and the

magnetostriction

coefficient

ill] I[

$,

=

exhibit

strong increase,

in

quantitative agreement

with the

Scaling

Ansatz

equation (I) [11,12]. Up

to now there is no evidence for saturation of the

height

of these maxima at

Bc

when

lowering T; especially

for the recent measurements [6] of

I[

down to 0.12 K These maxima are known to broaden

rapidly

when T

increases,

while their

height

decreases.

Performing

thermal

expansion experiments,

the authors of references

[6, 12]

could determine as a function of

B,

a

caracteristic

temperature TM (B)

at which av

(T, B)

has an extremum

(maximum

for B <

Bc

and minimum for B >

Bc).

Well below

TM(B)

the

system

enters a

degenerate

Fermi

liquid

behaviour where av is linear in

T,

while above

TM

no well defined Fermi

liquid

is observed. This cross-over

temperature

is shown to have a

sharp

minimum at

Bc.

It decreases from 9K at B

=

0,

to less than

0.5K around

B~

and then increases

again.

The

extrapolated

value of av

IT

increases

sharply

when B increases to

Bc, suddenly changes sign

for a field

step

of less than 19b of

Bc,

and then

slowly

increases back to zero. In the narrow range where av

IT changes sign,

it is

yet

not known wether

av

IT

is a discontinuous function of

B,

and a determination of

TM(B)

has to be done.

The aim of this letter is to

give

an

explanation

of the facts

concerning

the T

dependence

of

the maxima of x and

I[,

and for the low values of

TM (B

-~

Bc).

It relies on the fact

that,

since

FB

h

large, relatively

small

density

fluctuations can induce

strong

fluctuations in B*

(P).

Since It increases around

Bc,

fluctuations due to thermal

phonons

are

strongly

enhanced at that

field,

and the

temperature

for which these

phonons

become

important

decreases. The main effect of these fluctuations will be to

spread Bc

in a range of fields of width

proportional

to

FT2ItSH,

that can be

predicted

from first

principles.

A similar

approach

[6] was used to show that the

broadening

of the

anomally

upon

doping

the

compound

with La on the Ce

sites,

may be due to statbtical fluctuation of the La concentration within the

sample.

2. A model for the effect of

photons.

16 investi

gate

the effect of thermal

phonons

on the electronic

properties,

we assume an adiabatic- like

response

of the

heavy

electrons to

density changes,

and a

Debye approdmation

for the lon-

gitudinal phonons:

(4)

In a

region

of the

sample

where the

density change

is

given by

z =

~~,

there will be a local P

renormafisation of B"

by

a factor

exp(-Fz),

and the

magnetization

will be

given by m(B exp(+Fz))

where

m(B)

b the

magnetization

for z = 0 and T = 0.

The

probability density P(z)

of z b assumed to be

Gaussian,

as

given by

the

Debye theory

for T much less than the

Debye temperature (-~100 K), neglecting

the zero

point

motion of the atoms in the

crystaL

The

magnetization

b then

given by:

m(B, T)

=

/ dzP(z)m (Be~~,

T =

0,

z =

0) (2)

There

P(z)

b a Gaussian of width

(z2)

=

~~

~

~

~~~(~,

c

being

the

longitudinal

sound

velocity

10 Mc

(hc)

and V = 50

cm~/mol,

M

= 0.4

kg/mol

the molar volume and mass, and

kB

and h the Boltzmann and Planck constants. We conclude that an

anomaly

at B

=

Bc

will be

spread

on the field axis in a width: S

=

~j

~ =

F2 (z2) ar(T~c~5

lvith the values

given

above and c = I

km/s

this amounts to S

= 1.6 x

10~~T~.

The above

assumptions

indeed

imply

that thermal

phonons

have a

wavelength

and a

period

much

larger

than the characteristic

length

and time involved in the fluctuations of the

spin

sys-

tem

(wavelength,

correlation

length, frequency

and relaxation

time). Actually

these

assumptions

cannot be

justified

on

experimental grounds;

if

they

are wrong ma gnons and

phonons

have to be

treated as

coupled exdtations,

an

approach

which was not

attempted

in this kind of

compounds.

We

finally

note that a rather

big problem

arises when one looks at zero

point phonons.

A quan-

titative estimate of their influence is

given by

the

spreading Szp

due to zero

point

motion. If the entire

spectrum up

to the

Debye

wavector

kD

is taken into acccun~

Szp

is

given by: Szp

=

F(

~

8

~~

This number is very

large: Szp

= 20 for

FB

= 200 and c = I

km/s.

This

large spreading

is

strongly exagerated by

c the fact that the adiabatic

assumption

made above is

certainly

not

tjue

at

kD.

If a cut-off wavevector

kc

is

introduced,

the above result has to be

multiplied by ~

D

3. Technical details.

Equation (2) implicitely

relates measurements of the

magnetization

at different

temperatures.

In the framework of the S.A~ an identical

equation

can be written

replacing

m

by I[ (which

is

proportional

to B

~j ).

We assume this

formula,

and use it for

determining

in a

systematic

way a

broadening

of the

peak

in

I[

of reference

[fl.

This h done in the

following

way: we define the new variables y

= Fz and b: B

=

Boexp(b)

where

Bo

is a reference

magnetic

field.

Equation

(2)

then becomes a

genuine

convolution

product:

(5)

982 JOURNAL DE PHYSIQUE I N°7

where A normalizes the Gaussian on y. For

relating

measurements at a

temperature T2

to the results at a reference

temperature Ti,

we use the fourier transform 1)~

(q, Ti)

of

I[ (b, Ti)

We have:

I[ (b, T2)

=

dq exp(iqb)

exp

(-Sq~/2) ii, (q, 7i) (3)

where S

= S

(T2)

S

(Ti)

Note that neither S

(Ti)

nor

I[(T

=

0)

have to be known for per-

forming

this

analysis,

but that

they

cannot be found from it. The

quality

of the fit

given by (3)

is shown below to be

quite satisfactory provided

the

proper

value of S is chosen. We

performed

this

analysis using

the

experimental

results at

Ti

" 0.34

K,

the lowest

temperature

for which a wide range of fields was

investigated

in reference

[fl.

We use a 512

point FFT

and choose a range of field

larger

than the

peak

in

I[

at 4.2

Xj

but

sufficiently

small for

having

a reasonable accuracy

on B

Bo

= 5 T < B < 11

T, yielding

to a relative accuracy of 1.5x

10~~

on B. We evaluated

l~,~,

the

right

hand of

equation (3)

and compare

l~~~

to the measured

magnetostriction 1[~~~

for

T2 =0.12, 0.2, 0.6, 0.8,

1.3 and 4.2 K and for a very broad range of S

=

52 Si

We define

(~~eas ~~aic)~)

a reduced error A

= ~, ~ that we

plot

versus S for each

T2 (Fig. I).

We can then

meas)

find the value of

Sbest,

that

yields

to the smallest

possible

error

Abest,

and the error bar on

Sbest,

defined as the

region

where A is less than I-I

Abest.

The

quality

of the fits for

T2

>

Ti

may be

appreciated

in the inset of

figure

I. In any case

(Abest)~~

is about

0.I, comparable

to the error bar on the measured

I[.

For

T2

<

Ti, equation (3) magnifies

the

noise,

so that no well defined minimum

appears

in

A; thus,

we choose Sbest as the values for which a linear

regression of1[~~~

verms

1[,~ yields

a

slope equal

to 1+0.I. In this latter case,

Sbest

is

certainly

dominated

by

S

(Ti)

~ T=1.3

T=~.2K

0.8

I

z T=0.8

~ r4~

fl

~

~j

~

~ ~

IT1 io

io-6

~o-5

io-'

1o-3

io-2 io-i

s

Fig.

1. The relative error A on

I[ (see text)

is

plotted

ver~us the

spread

S for the temperatures as indi- cated. From this

plot

we find the best fit Sbe~i of the

magnetostriction

and the error

bar,

as indicated

by

the

horizontal dashes. Inset: the fit for T

= 0.8 K.

I[

is

plotted

as fttnction of B. The

experimental

curve can be

distinguished

from the fit,

only

because the noise is

slightly

visible.

(6)

4. Results and discussion.

The results of this

analysis

are

reported

in

figure

2 as

Sbesi

= S

(T2)

S

(Ti)

versus

Tf T).

It is

readily

seen that the

T~

law for

S(T)

is

nicely obeyed

for S

ranging

from -1.7x

10~~

at 0.12 K to 2~5x

10~~

at 4.2 K~

yielding

to

S(T)

=

10~~ T~ (1+0.5).

This value

imply

at

Bc

a sound

velocity

c = I

km/s.

This b smaller than the one

reported [13],

at 1.3 K but we

expect

from the

S.A~ in view of the

magnetostriction

results

[fl,

that a much more

significant softening

exist at low

temperature,

for

good samples.

These facts

imply

that thermal

phonons play

a central role in the

broadening

of the

metamagnetic

transition in

CeRu2S12,

a conclusion in

strong

contrast to the

generally accepted

one, that the

spreading

is due to

exeptionnally

low

energy

scale in the

heavy

electron

problem.

We

emphasize

that this mechanism of

spreading

is

significant

because of its

strong dependence

on F: it is

proportional

to

r~/c5,

and if the S.A~ is true, the

compressibility

at

Bc

is

essentially proportional

to

F2

so that S

«

F7.

With F =200 we

get

an enhancement of the thermal

phonons

contrlution of about 10~~

compared

to nonnal

problems! Finally,

since the

spreading

due to zero

point phonons

is

potentially

very

large,

this

approach

rises the

question

of the role

played by

the zero

point density fluctuations,

in the

magnetic properties

of the

compound.

Namely,

we ask whether zero

point

motion of the Ce ions b

responsible

for the lack of order at low

field,

for the width of the transition at

Bc,

and for the

suppression

of an eventual first order

transition at

Bc

driven

by

volume

changes [7,12].

10"~T~

041 0.I 10 100

T~ K'l

Fig.

2. The

spread (Asbest(

is

plotted

venus

(T~ Tf(

in

log-log

scales. The

T~

law is well verified. The

straight

line

corresponds

to

10~~T'.

See text and

figure

for the

error bars.

Acknowledgements.

J.

Flouquet,

P Haen and A~ Lacerda are

gratefully acknowledged

for

having

involved the author in this field of research.

(7)

984 JOURNAL DE PHYSIQUE I N°7

References

ii]

BEsNus

MJ.,

KAPPUIR

J-P,

LEHMANN P and MEYER

A.,

Sobd State Commm. 55

(1985)

779.

[2] HAEN

P,

FLOUQUET

J.,

LAPIERRE

E,

LUAY

P,

REMENYI G.,L Low

2kmp. Phys.

67

(1987)

391.

[3] VOIRON

J.,

MIGNOT

J-M-,

LUAY

P,

HAEN P and FLcuouET J.,J

Phys.

France 49

(1988)

1555.

[4] FISHER

R~A.,

PHILUPS

N.E.,

MARCENAT

C,, FLOUQUETJ.,

HAEN

P,

LEJAY P and

MIGNOTJ.L.,J Phys.

Co&q.

France 49

(1988)

C8-759.

[5~ RossAr.MIGNOD

J.,

REGNAULT

L.P,

JAOCARD

J-L-,

VETTJER

C.,

LUAY

P,

FLououET

J.,

WALKER

E.,

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JL,J Magm Magm

Mater 76&77

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[6l PAULSEN C., LACERDA A., PUECH

L.,

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P, THOUINCEJ.L.,

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JL,

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907.

[8] UEDA

K.,

YAMAMOTC K and KONNO

R.,

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[9] MIYAKE K and KURAMOTC

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ibid.

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J.M.,

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ill]

PUECH L., MIGNOT

J-M-,

VOIRON

J.,

LUAY

P,

HAEN P and FLououET

J.,

f Low

2kmp. Phys.

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P, FLOUQUETJ.,

VoiRoN J. and OHKAWA Il.,

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I.,

WEBER

D.,

YOSHIzAWA

M.,

LUTHI

B.,

PUECH

L.,

HAEN

P,

FLOUQUET

J.,

BRULS

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JJ.M.,

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