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HAL Id: jpa-00207374

https://hal.archives-ouvertes.fr/jpa-00207374

Submitted on 1 Jan 1973

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The homogeneous helimagnet and the liquid-solid transition

J. Villain

To cite this version:

J. Villain. The homogeneous helimagnet and the liquid-solid transition. Journal de Physique, 1973,

34 (2-3), pp.211-216. �10.1051/jphys:01973003402-3021100�. �jpa-00207374�

(2)

THE HOMOGENEOUS HELIMAGNET AND THE LIQUID-SOLID TRANSITION

J. VILLAIN

Institut

Laue-Langevin,

Grenoble

(Reçu

le 26

juin 1972)

Résumé. 2014 On examine la

possibilité

d’une transition avec une

susceptibilité

infinie pour q ~ 0 dans un milieu

homogène.

Dans le cadre d’un modèle

précis (§ 2)

on montre

(§ 4)

que seule une

faible

singularité

peut exister, et

probablement

pas

d’infinité ;

la

singularité

forte

apparait à q

= 0

et pour une

quantité qui

n’est pas la

susceptibilité (§ 3).

On

prévoit

un résultat

analogue

dans le

cas des

liquides (§

1 et

5).

Abstract. 2014 The

possibility

of a transition with an infinite

susceptibility

at

non-vanishing q

in an homogeneous medium is

investigated.

In the frame of a

precise

model

(§ 2)

it is shown

4)

that

only

a weak

singularity

can occur, and

probably

no

infinity ;

the strong

singularity

appears at q = 0 for a

quantity

which is not the

susceptibility (§ 3).

A similar result is

conjectured

for the

compressibility

of

liquids (§

1 and

5).

Classification Physics Abstracts

15.00 - 14.80

1. Introduction. - It has been

suggested [1] ]

that the

pair

correlation function of a metastable

liquid might

become

long

range at some

tempera-

ture

TL

where the

liquid

becomes unstable. More

recently,

the

dynamical aspect

of this

instability

was

investigated [2], [3] and,

very

recently, experiments

were

performed

to check this

theory by measuring

the static and

dynamic scattering

factors of neutrons

[4].

S(q)

and

S(q, w). S(q)

is

expected

to become infinite at

TL

for some value qL

of q,

and

S(qL, w)

is

expected

to have a

vanishing

width at

TL (infinite

De Gennes

narrowing).

Experimentally TL

could not be reached

[4],

and

possibly

there are fundamental reasons for

that,

at least for a

simple liquid ;

but we do not wish to

consider this

problem :

we

only

mention

[5]

that

symmetry

does not exclude a second order transition for some well-defined pressure at which the 3rd order terms in the

thermodynamic potential

vanish

accidentally.

Our

problem

is the

following :

assume

that

TL

can be

reached,

then what is the

type

of the

singularity ?

For T N

TL and q N qL

the

following approximate

formula has been

suggested [1 ], [2] :

with K2 = A(T - TL). A

and B are constants. The factor K at the numerator is

lacking

in reference

[3],

but is necessary because

S(g)

has to be

integrable [6].

Thus, S(g)

turns out to be

proportional

to

b(q - gL)

at

T,,

so that the

singularity

of

S(q)

at the

instability temperature

is found to be much

sharper

than in

usual transitions

[5],

where

1 /S(q)

remains

analytic

at

TL.

On the other

hand,

there are reasons to believe that on the

contrary, S(q)

is smoother than usual :

indeed,

assume that at

TL,

the

liquid

becomes

locally

solid

like,

in

agreement

with the ideas of references

[1 ]

and

[2].

For a solid

S(q) _ Mft d(q - t),

where t

r

are

reciprocal

lattice vectors. For a

given

orientation of the solid germs, one

expects,

at

TL :

by analogy

with the usual Ornstein-Zernike

formula ;

but in the

present

case it is necessary to average

on the orientations of i for a

given 1 I 1

= qL :

This

simple

minded

argument

will now be

put

into a more

sophisticated

form.

However,

rather

than

arguing

on the difhcult case of a

liquid,

it is

convenient to define a

precise

model

which, although

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01973003402-3021100

(3)

212

probably academic,

seems to have features similar to those attributed to

liquids

in references

[1 ], [2], [3].

2. The

planar helimagnet

with

isotropic

interactions in a

homogeneous

médium. - We consider a conti- nuous, 2-dimensional vector field in the 3-dimensional space, with energy :

where

J(r)

is a function of r

= 1 r only.

It is assumed

that m(r) 1

=

1,

so that

m(r)

is

completely

defined

by

its

polar angle cp(r) [7].

In the absence of further

prescription,

the model has no

phase

transition : indeed it is the limit of an

increasing density

of

vanishingly

small moments with

vanishingly

small

individual

susceptibility,

so that there is no

phase

transition as can be seen from molecular field appro-

ximation,

which in this case is

rigorous

because of the

large

number of

neighbours [8].

As a

phase

transition is

desired,

the Fourier transform

mq

of

m(r)

will be assumed to vanish

for q greater

than

some cut off qo > QL To sum up, the

prescriptions

are :

In any

physical analogue

of the model

(see § 6),

condition

(4b)

expresses the fact that the number of

degrees

of freedom is of the order of the number of atoms.

Conditions

(4a)

and

(4b)

are

compatible :

it is

indeed sufficient to find

mx(r) satisfying mx(r)

1

and relation

(4b),

then

M2 x(r)

satisfies

(4b),

therefore

m2 y =

1 -

mx

also satisfies

(4b)

and so does my.

2.1 Low TEMPERATURES. - We start with the

assumption (to

be

justified below)

that the

ground

state is a

helimagnetic

structure :

For a

weakly perturbed configuration :

the energy is :

Ô(Pk

and

5(k)

are the Fourier transforms of

ôg(r)

and

J(r) :

The bracket in the above

expression

is

positive (or

zero for k =

0)

and therefore the

helimagnetic

structure is stable at T =

0,

and remains stable at low

temperature

if

(4b)

is

satisfied ;

qL is the maximum of

l(k).

2.2 HIGH TEMPERATURES : : MOLECULAR FIELD APPROXIMATION

(MFA). - Let xq

be the

staggered susceptibility

of the

non-interacting system, only

submitted to conditions

(4) :

where

hq

is the

qth

Fourier

component

of the external field. The effect of Je can be taken into account

by adding

a molecular field 2

3(q) mq

> to

h :

with

The

system

described

by

conditions

(4)

is

roughly equivalent

to an array

of cells

of side

llqo

with

magnetization

of order

1/qo3 ; thé

individual suscep-

tibility

of each cell is

given by

a Curie law : xo ~

f3/qg

and a similar law is

expected

for

xq :

It is seen from

(5)

and

(6)

that the Néel

temperature

is

where qL

maximizes

3(q). Neglecting

the weak

possible

(4)

dependence

of

Xo

on q,

(5)

reads for T N

TN

and so that :

where V is the total volume and

mq the

Fourier

transform of

m(r),

and where

vanishes at

TN.

The factor K of eq.

(1)

is

lacking

at the numerator of eq.

(7),

thus

violating

the sum

rule

2.3 SPHERICAL MODEL. - The

spherical

model

[9], [10]

accounts for eq.

(8) (but

not for the more

general

condition

m2(r) - 1) by using

the

density

matrix :

where V is the volume and :

where the

Lagrange multiplier y

is determined

by :

The critical

temperature TN

=

1 /KB f3N,

determined

by

the

condition Il - 3(q,)

=

0,

is found to be zero, in contradiction with what was shown

above,

para-

graph

2.1.

The best way to describe critical

phenomena

in

our model in a consistent

approximation

is to make

a

change

of

thermodynamical

variables.

3.

Change

of

thermodynamical

variables. - Rather than

m(r),

we wish to introduce the variable :

In terms of the

polar angle Q(r)

of

m(r),

eq.

(3)

reads :

The cosine can be

expanded

in powers of

u(r)

as follows :

cos 1

After

integration

of this

expansion,

the

expansion

of the

integral

contains :

a)

A zero-th order term

which will be

represented by

its Mac Laurin

expansion :

and has a minimum 1

b)

Terms

containing

the derivatives of u,

namely :

a term

proportional

to

(div U)2

For the sake of

simplicity,

the last 3 terms, which

are of

higher

order in u, will be

neglected.

It is relevant to

express

in terms of the Fourier

(5)

214

transform of

u(r) - VQ(r),

which is a vector with

components :

The variable uq =

qqJq

has been introduced because

1 Uq 12 >,

and not

1 qJq 2

> remains finite for q

going

to zero in the limit of infinite volume. a,

y, 03BE

denote the

coordinates : x,

y, z.

Expressing

the term

a)

and the first 2 terms

b)

as

functions of

u,,, inserting

into eq.

(9),

and

integrating

over r and

r’,

we

get :

C, D,

E are constants.

If the ordered

phase,

as was said in

paragraph 2, corresponds

to

u(r)

> =

C’,

the constant E

is

expected

to be

positive

and the

transition,

in terms

of uq, takes

place at q -

0. This transition is of a

very common

type, comparable

for instance to a

Bose

condensation,

since uo becomes

macroscopic (proportional

to the volume

V)

below the transition

temperature TN.

Conventional «

scaling theory

»

[9], [11] ] predicts

above

TN a

correlation function of the

following type :

where q

is a small

positive

coefficient

and f is

a function.

In the

appendix,

the

thermodynamics

of the

system

is

investigated

in the Hartree

approximation

and

eq.

(11)

is derived

microscopically with q

= 0.

4. Correlation-funetion for

m(r).

- We have

given

a consistent

description

of the

system

in terms of

u(r). Unfortunately

the correlation function

(11)

is not

easily

accessible to

experiment (in

the

liquid-

solid

transition, u(r) represents

a vector

joining

2

neighbouring

atoms : see next

section).

It is

therefore of interest to

investigate

the suscep-

tibility m(o) . m(r)

>. It cannot be deduced from

u(O). uer)

> without additional

assumptions,

be-

cause

strictly speaking,

the

knowledge

of

higher

order

correlations,

uuuu

>,

etc., is

required.

To

approximate

these correlations

by

a factorization is not

satisfactory,

as shown in the

appendix.

It seems

preferable

to

apply

the ideas of the «

droplet

model »

[11]

and to assume that at

TN

the

system

is constituted of «

droplets »

which look somewhat like the condensed

phase. Quantitatively,

this idea

is

expressed by

the

following assumption :

P(r)

is

roughly

the

probability

that r

belongs

to

the same «

droplet

» as the

origin. m(r)

and

u(r)

are mean values

corresponding

to

given

values of

m(0)

and

u(O). Comparison

of eq.

(11)

and

(12b) yields :

The case T >

TN

will not be treated for

brevity.

At T

TN, P(r)

has a finite limit for

large

r.

For a

given

value of

u(O) =

u, the average value

of

m(O).m(r)

is from

(12a)

and

(13) :

and

averaging

over the orientations of u

yields :

The Fourier transform of this function is not infinite

at q

= qL,

except if il

=

0,

where the

loga-

rithmic

singularity

of

paragraph

1 is recovered.

5.

Liquids.

- Our model can be

transposed

to

liquids :

the function

g(r),

instead of

being

the

polar angle

of

m(r),

now defines « reticular surfaces »

by

the

equation

cos

qJ(r) =

1. It is also

possible

to

define 3 families of reticular surfaces

corresponding

to 3 variables

qJa(r) (a

=

1, 2, 3).

The atoms would

be located at the intersections of 3 surfaces. A

possible

hamiltonian is :

The hamiltonian

(3)

is a

simplified

version with

only

one function

Q(r).

The ordered

phase

described

in

paragraph

2.1

clearly pictures

a solid since the

reticular surfaces are

parallel planes.

The

description

of the

liquid phase

is very poor, due to the absence of

dynamics

and to the presence of elastic

properties

that a

liquid

has

probably

not.

(6)

It is not clear whether a more realistic

description

of

a

liquid

would

give

rise to an

instability

of the

type investigated

in this paper, but if it

does,

there is

probably

no

singularity

at finite q in the

compressi- bility,

or a weak one, as discussed in

paragraphs

1

and 3.

Acknowledgments.

- The author is

especially grateful

to Pr. P. G. De

Gennes,

B.

Jancovici,

P. C.

Martin and L. Verlet for their valuable comments and

suggestions. Acknowledgments

are also made

to Dr. Kleban and

Kugler,

and to Pr. Schofield.

Appendix :

The Hartree

approximation

The hamiltonian

(10)

will now be treated in the Hartree

approximation, namely :

In this

approximation,

the correlation function

is,

from

(10)

and standard fluctuation

theory [5] :

The Néel

temperature TN

is defined

by

the

following

relation :

Below

TN,

uo is

given by

the minimization of

(10)

after insertion of

(A.1) :

where Ox is the direction of uo.

Inserting (A. 4)

into

(A. 2) yields :

where ç

is defined

by

the

following integral equation :

When ç

increases from 0 to

00, j (ç)

decreases

from a

positive

value to

0, except

for uo -

0,

then

f(ç)

= 0.

Therefore ç

> 0 for T

TN,

so that the

stability

condition

u _ q uq > > 0 is fulfilled,

in

agreement

with Section 2.1.

Remarks. -

a)

The rotational invariance

requires ôu-L. ôu-L

> = oo, where

buô

is the fluctuation

of uo

perpendicular

to uo >. On the other

hand, u_q.uq

> does not go to zero in the direction

perpendicular

to uo >. This

discontinuity

is

likely

a

spurious

result of the Hartree

approximation,

as it would show up in a similar treatment of an

ordinary, crystalline ferromagnet,

as well.

b)

At

high temperature

the

present approximation predicts u _ q uq

> ~

T¥2.

This result should not be taken too

seriously

because it is not

legitimate

to

neglect

terms of

higher degree

in u in eq.

(10).

If the factorization

(A.l)

is made in formula

(10),

it is

possible

to calculate

m(O). m(r)

>

[7] :

The

integrand

is

positive,

so that the

exponent

decreases when r increases and

m(o) . m(r)

> is a

decreasing

function of r. This result cannot be

accepted

because the same treatment

yields

an

analogous

result for a

crystalline helimagnet,

whereas

m(o). m(r)

> is known to

be,

at

TN,

an

oscillating

function of r in this case. This is the reason

why

the

droplet

model was used in section 4 rather than the Hartree

approximation.

(7)

216

References

[1]

KIRKWOOD J.

G.,

MONROE E., J. Chem.

Phys.

9

(1941)

514.

KIRKWOOD J. G., J. Chem.

Phys.

7

(1939)

919.

[2]

KOBAYASHI K., Technical report of ISSP A 360,

Tokyo (1969).

[3]

SCHNEIDER T., BROUT R., THOMAS H., FEDER J.,

Phys.

Rev. Lett. 25

(1970)

1423.

SCHNEIDER

T., Phys.

Rev., A 3

(1971),

2145.

[4]

SÜCK J. B., GLÄSER W., Communication at the IAEA Conference on Neutron inelastic

Scattering, Grenoble,

March 1972.

[5]

LANDAU L., LIFSHITZ E.,

«Physique Statistique

»,

éditions MIR, Moscou

(1967). Chapter

XII and

§ 140.

[6]

For

example

SJÖLÄNDER

A.,

in « Thermal neutron

scattering

», edited

by

P.

Egelstaff.

Acad. Press, London

(1965).

[7]

SARMA

G.,

Solid State Commun. 10

(1972)

1049.

[8] BROUT R., « Phase transitions »,

Benjamin (1965).

[9] For a recent review on critical

phenomena,

see

STANLEY H. E. « Introduction to

phase

transitions and critical

phenomena

», Clarendon Press

(1971).

[10]

BERLIN T. H., KAC M.,

Phys.

Rev. 86

(1952)

821.

[11]

WILSON K. G.,

Phys.

Rev. Lett.

[12]

FISCHER M. E.,

Physics

3

(1967)

255.

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