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HAL Id: jpa-00208523

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Submitted on 1 Jan 1976

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Double spin one-half lattice gas model

J. Sivarditre

To cite this version:

J. Sivarditre. Double spin one-half lattice gas model. Journal de Physique, 1976, 37 (11), pp.1267-

1277. �10.1051/jphys:0197600370110126700�. �jpa-00208523�

(2)

DOUBLE SPIN ONE-HALF LATTICE GAS MODEL

J.

SIVARDITRE

Departement

de Recherche

Fondamentale,

Centre d’Etude Nucléaires de Grenoble 85

X,

38041 Grenoble

Cedex,

France

(Reçu

le 5 avril 1976,

accepté

le

25 juin 1976)

Résumé. 2014 Nous présentons un modèle cellulaire à double spin un-demi, qui reproduit le compor-

tement

thermodynamique

d’un alliage binaire recuit dont les deux composantes sont magnétiques.

L’hamiltonien

ferromagnétique

du type Ising est traité dans

l’approximation

du champ moléculaire.

Divers diagrammes de phases sont obtenus, présentant des points critiques de démixion, des lignes critiques magnétiques, des points triples et tricritiques. La mise en ordre

magnétique

peut favoriser

ou retarder la séparation de phase induite par les forces interatomiques, et peut même provoquer

une

séparation

de phases dans une solution idéale. Les résultats de

Blume-Emery-Griffiths

sont

retrouvés dans le cas une des composantes de l’alliage n’est pas

magnétique.

Le modèle décrit

également les mélanges de liquides nématiques.

Abstract. 2014 A double spin one-half lattice gas model is introduced in order to simulate the ther-

modynamical behaviour of annealed binary alloys, the two constituents of which are magnetic.

The ferromagnetic Ising-like Hamiltonian is solved in the molecular field approximation. Various types of phase diagrams are found, exhibiting critical points for

phase

separation, magnetic cri-

tical lines, triple and tricritical points. Magnetic ordering may hinder or enhance phase separation

induced by interatomic interactions, or even induce it in an ideal mixture. The Blume-Emery-Griffiths

results are recovered in a particular case. The model may apply to the description of liquid

crystal

mixtures and the interplay between phase separation and nematic ordering.

Classification Physics Abstracts

8.514

1. Introduction. - The

thermodynamical

beha-

viour of many

cooperative physical

systems can be simulated

by

a

spin - 1/2 Ising

model. The

following phenomena

can be

described,in

this manner :

magnetic

or nematic

ordering, condensation, freezing,

and

phase separation [1-3]. They

are characterized

by

a

single

order parameter. Other

physical

systems are characterized

by

two

kinematically coupled

order parameters and the

interplay

of two

cooperative

processes, for instance a He3-He4 mixture

[4],

or a

binary

mixture at variable pressure

[5]. They

can be

simulated

by

a

spin -

1

Ising

model. More

compli-

cated systems, characterized

by

three order parameters,

can be simulated

by

a

spin - 3/2 Ising

model

[6].

In this paper, we

investigate

the

applications

of a

double

spin - 1/2 Ising

model. This model describes

some systems characterized

by

two

kinematically independant

order parameters. The paper is

organized

as follows. In section

2,

we show how our lattice gas model

applies

to

magnetic

or nematic

binary

mixtures.

The Hamiltonian is constructed in section

3,

and solved

in the molecular field

approximation

in section 4.

Phase

diagrams

are discussed in sections 5

(ideal mixtures)

and 6

(non-ideal mixtures).

2. Lattice model for

binary

mixtures. - We consi-

der here

liquid

or solid

binary mixtures,

both atoms A

or B

being magnetic.

Two

spins 1/2

are introduced

at each site of the lattice - or in each cell of the lattice gas

description

of the fluid. The first one, ai = ±

1/2, gives

the

type

of atom, A or

B,

which is found at the site or in the cell i. All sites or cells are

occupied,

so

that the pressure is

kept

constant. The second

spin,

Ti = ±

1/2, gives

the

orientation, positive

or nega-

tive,

of the

magnetic

moment : atoms A and B are

supposed

to have the same

magnetic

moment. The two

order parameters are : M

=== ( ai >

and

Q = Ti >.

M will be called the concentration and is in fact the deviation from

equiconcentration, Q

is the magne-

tization ;

the concentration xA in A is

given by :

xA =

1/2

+ M.

A

binary

fluid mixture of

elongated

molecules may be described in the same way. The first

spin a gives

the type of molecule A or B found in a

given

cell of the

lattice-gas

model

representing

the

fluid,

the second one

z the orientation of the molecule : molecules A and B

are

supposed

to take

only

two orientations.

Q

is here

the nematic order

parameter

or orientation.

Various

isotropic

and

anisotropic

interactions will be introduced between the atoms or molecules A and

B,

and the

possible phase diagrams

will be

given.

We are

mainly

interested in the

interplay

between

the two

cooperative phenomena : phase separation

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:0197600370110126700

(3)

TABLE I

Interactions in a

binary

mixture

oj’magnetic

atoms

A and B

and

magnetic (or nematic) ordering.

In the

following,

we concentrate on

magnetic systems.

3. Double

spin

one half hamiltonian. - The inter- actions between

magnetic

A and B atoms are defined

in table I. The

following projection

operators are introduced :

The Hamiltonian of the system is then :

Introducing Zi

= ai Ti and the chemical

potentials

,uA and MB, we obtain :

A

change

of notation is now introduced :

JAA, JBB

and

JAB

are interatomic

(isotropic)

interac-

tions, independant

of the

spin orientation; jAA, jBB

and

JAB

are

purely magnetic

interactions. All interac- tions are taken to be

positive,

so that no sub-lattice

structure has to be introduced.

We define now the interactions

K, J, L, k, j

and 1:

and :

K is the mean interatomic interaction in an

equiatomic

mixture. J measures the

tendancy

to

phase separation

in a

non-magnetic

mixture. L measures the

difference

between the pure A and B constituents

(for

instance

the difference between their cohesive forces if A and B

are solids or their critical

temperatures

if A and B are

liquids). Similarly k

is the mean

magnetic

interaction in an

equiatomic mixture, j

measures the

tendancy

to

phase separation

due to

magnetic

interactions and I measures the difference between the

magnetic

critical

temperatures

of the two constituents. We note that :

and :

Using

the notations

(5), (6)

and :

(4)

the Hamiltonian JC becomes :

In the absence of

magnetic interactions,

Je reduces to a

spin

one-half

Ising

Hamiltonian :

If A and B are identical

atoms, JC

reduces

similarly

to :

4. Molecular field

equations

of state. - In order to

obtain

phase diagrams,

we treat the Hamiltonian

(10)

in the molecular field

approximation.

At the first

stage, we introduce two molecular fields

H6

and

Ht

and two order parameters M

= ai >

and

Q = ti ),

The molecular field Hamiltonian is then :

with :

H6

and

Ht

are determined

using

the variation

principle

for the free energy

[7] :

From

(14)

and

(15),

we obtain the two

equations

of

state. Similar

equations

have been found

by Pople

and Karasz

[8]

in their

study

of

liquid

solid transitions of molecular

crystals.

These

equations

however do not

provide

a correct

description

of the system.

Indeed, equation (15b) ,

can be written :

where :

is the mean

magnetic

interaction in a

homogeneous phase

of concentration M. But the

approximation :

(Ji

Ti > = (Ji > ii ) neglects

the fact that the

magnetizations QA

and

QB

of the two

types

of atoms

are not

necessarily

the same. This is true

only

if

jAA

=

jBB

=

JAB or j

= I =

0,

and if so,

phase

sepa- ration and

magnetic ordering

do not interfere.

The

system

is in fact characterized

by

three inde-

pendant

order parameters

M, Q

and R.

According

to

(1),

the contribution of the A and B atoms to the

magnetization

are

given by :

and

respectively. Q

=

QA

+

QB

is then the

magnetization,

and R describes the difference between the

magnetiza-

tions of the A and B atoms. The system

might

also be

described

by

a

spin - 3/2 Ising

model since each atom may be found in one of four different states :

M, Q

and R would be

replaced dipolar, quadrupolar

and

octupolar

order

parameters (see Appendix 1).

The correct molecular field Hamiltonian is then :

The

corresponding partition

function

Zo

is

given by :

and the free energy

by :

The conditions :

give

the

following

values of the molecular fields :

whence the three

equations

of state :

(5)

and the free energy :

with :

Alternative

expressions

of the

equations

of state are

given

in

appendix

2.

Equations (23)

have two types of solutions :

1) Q

= R =

0 and M given by

and : O O

This solution describes a

paramagnetic

mixture.

2) Q, R

and M different from zero

(magnetic mixture)

and in

general R # MQ.

The solution

-

Q, - R,

M describes a

magnetic

domain with

magnetization

in the

opposite

direction.

Suppose

that H- ± oo. Then M = ±

1/2,

R = +

Q/2 and,

as

expected

since the mixture contains no B

(or A)

atoms :

If

only

one solution

(M, Q, R)

of

equations (23a) (23b)

and

(23c)

is found at a

given temperature

T for

given

values

of J, k, l, j

and

H,

it

represents

a

homogeneous

mixture. If n solutions

(Mi, Q1, R1), (M2, Q2, R2), ...

are found with the same free energy,

they

represent n

homogeneous phases

at

equilibrium.

Consequently,

in order to determine the

phase diagram

of the

mixture,

we choose fixed values of the

, interactions

J, k, l, j

and of the field

H,

and look for a

first-order transition as T is varied. The two solutions at

equilibrium

determine either two

magnetic phases

with different

compositions,

or a

magnetic phase

and

a

paramagnetic phase.

CRITICAL LINE. - Phase

separation gives

rise to a

critical

point given by : kTc

= 2 J. The onset of

magnetism gives

rise to a critical line. Its

equation

can

easily

be found from

equations (23b)

and

(23c)

with

Q

and R ~ 0.

Writing :

we obtain ’ :

whence a relation between

Q

and R near the critical line :

and the

equation

of the critical line in the

(M, T) plane :

from which we find as

expected : 1 /Bi

=

2 jAA

for

(6)

TRICRITICAL POINT. - In order to locate a

possible

tricritical

point,

we

perform

a Landau

expansion

of the

free energy :

we obtain for J = 0 :

with :

Me being

the value of M at the critical

point.

The cri-

tical line is

given by

the condition :

b2

= ac, or :

which is

equivalent

to

(30),

and the relation between

Q

and R near the critical line

by :

which is

equivalent

to

(29)

when

(30)

is satisfied.

Q4 is

given by :

x

and y are

defined

by (27).

The tricritical

point,

if

it

exists,

is defined

by (30)

and the condition : (P4 = 0.

When

(30)

is

satisfied,

x

and y

may be

replaced by :

with :

More

complicated

results are found for J different from zero.

5. Phase

diagrams

of ideal mixtures

(J = 0).

-

5.1 PARTICULAR

CASE : j

= 1 = 0

UAA = jBB

=

JAB).

- The mixture is ideal

(no phase separation

can be

induced

by

interatomic

interactions),

and the A and B

atoms have the same

magnetic properties.

The magne- tic critical

temperature :

kT = 2 k is

independant

of

M,

and lines of constant H are

parallel

to the T axis

in the

(M, T) plane.

When

CA

and

CB

are the critical

points

of pure A and

B,

the critical line

CA CB

is a

straight

line..

5.2 PARTICULAR CASE : k = l =

j.

- In this case, B atoms are

non-magnetic : jAB

=

jBB

= 0 or :

JBB

=

JBB

and

JAB

=

JAB.

This is

equivalent

to the

Blume-Emery-Griffiths [4]

or

Hintermann-Rys [9]

model. The Hamiltonian

(10)

becomes :

The system is characterized

by only

two order para- meters : the concentration M

= 6i, >

and the magne- tization of A atoms :

QA

=

1 j2(Q

+ 2

R)

since :

QB

=

(Q -

2

R)/2

= 0

(from (22)

we see also that

Hi

= 2

H,).

Indeed the

equations

of state as

given

in

appendix

2

immediately

become :

Q = 2 R,

and

whence :

and :

From

(43)

with

QA ~ 0,

we deduce the

equation

of the

magnetic

critical line :

in agreement with

(30).

The tricritical

point

is

easily

located from

(36), (37)

and

(38) :

B =

0, x

= y whence : 12

M’+8M+1=0

and

M = - 1/6 (Fig. 1).

Phase

separation

is

magnetically

induced.

.

FIG. 1. - Phase diagram of the Blume-Emery-Griffiths model

with J=O, k=l=j=4 U AD = jDD = 0) CA and CD are the magnetic critical points of pure A and B. The critical line CA C’

is a straight line, C’ is the tricritical point. Lines of constant H are

shown. P, and P 2 are two phases at equilibrium : only P2 is magnetic.

(7)

The

particular

case k

= j

= - 1 describes AB mixtures in which the A atoms are

non-magnetic : Q

= - 2

R, QA

= 0.

Suppose

now that A is

magnetic

and B is a vacancy : the mixture is a

magnetic

gas, the pressure of which can vary

[5].

whence :

The interactions

J AA and jAA

lead to condensation and

ferromagnetism respectively.

The pressure P is the

opposite

of the

grand partition

function qJ.

From

(24)

and

(45),

we deduce :

with :

whence :

in

agreement

with the results of ref.

[4].

5.3 GENERAL CASE. - We note that for J =

0, equations (23b)

and

(23c)

do not contain

M,

so that

they

can be solved

separately. Knowing

a solution

(Q, R),

M is then calculated from

equation (22a).

For H = 0, M = 4 QR and :

,

In the

following

we

always

take :

2jAA

= 32

(magnetic

critical

temperature

of pure

A)

and vary

JAB

and

jBB (see

Tables II and

III).

TABLE II

’Magnetic

interactions in

symmetrical

mixtures

TABLE III

Magnetic

interactions in

asymmetrical

mixtures

Symmetrical

mixtures

(1

=

0).

- The case k =

16, j

= 1 = 0 has been considered above : the critical line

CA CB

is

parallel

to the M axis in the

(M, T) plane.

If

JAB> jAA = jBB’

the critical line

CA CB

exhibits

a maximum

Cmax

at

FIG. 2. - Phase diagram of an ideal magnetic mixture with : k = 20,1= 0, j = 14 jAB > jAA = iBB)’ CA CB is the critical line.

The mixture is homogeneous at any temperature and lines of constant H are shown.

There is no tricritical

point

and the mixture is

always homogeneous :

in

fact,

the onset of

ferromagnetism

favors

homogeneity.

If

jAA

=

jBB

>

jAB

>

0,

the critical line

CA Cl

exhibits a minimum

Cmin

at M = 0

(Fig.

3a : k =

10, j

=

6).

Moreover

phase separation

is found at lower

temperature

in the

magnetic phase :

the critical

point

C is the maximum of a second branch of the critical line situated in the unstable

region

bounded

by

the binodal curve.

According

to

(48), kTc.,. =

2 k

and

kTc

=

2 j.

(8)

FIG. 3. - a) Phase diagram of an ideal magnetic mixture with : k = 10, 1 = 0, j = 6 (j,, = 7BB > jAB > 0). Phase separation is found in the magnetic region : P, and P2 are two magnetic phases

at equilibrium, C is the critical point. The second branch of the

critical line is represented in dashed, lines of constant H are shown.

b) Phase diagram for : k = 8,1= 0, j = 8 (jAB = 0). The critical line is made of two straight lines CA C and CCB. The critical line and

the binodal curve have a common point C.

If

jAB

=

0,

the critical line

CA CB

is made of two

straight

lines which cross at M = 0

(Fig.

3b : k

= j

=

8).

The minimum critical

point

is at the

top

of the binodal

curve.

If JAB = k - j 0, or k j,

and k >

0,

a

phase diagram

similar to that of

figure

3a is found. However

Q = 0

and R =A 0

along Cmin

C

(we

have now :

kTcmin

=

2 j

and

kTc

= 2

k) :

since the mixture is

equiatomic,

atoms A and B have

opposite magneti-

zations

QA

= R and

QB = - R,

so that the net

magnetization

is zero.

If I JAB is

small

(k

>

0), phase separation

is found

below

kTc : coexisting phases

have different concen-

trations and are

partially

ordered both

cristallogra- phically

and

magnetically. If I JAB

is

large (k 0),

atomic

ordering

and

antiferromagnetism

are

expected

at low

enough temperatures.

Asymmetrical

mixtures

(10 0).

- We consider first

the

case : j

= 0 or :

2 jpB

=

jAA

+

iBB’ If

for instance k = 12 and 1 = 2

(Fig. 4),

no

phase separation

is

found in the

magnetic phase

even at very low tempe-

ratures.

If the ratio

kll

is lower

(Fig.

5 : k =

9,

1 =

3.5, j

=

0),

a tricritical

point

C’ and

magnetically-induced phase separation

are found : the critical line is

made

of two

branches, CA

C’ and

C1 CB.

Phase

separation disappears

as T -> 0.

If j # 0,

and k ~ I

~ j (Fig. 6),

the

phase diagram

is similar to that of the

Blume-Emery-Griffiths model,

except that the critical line is

composed

of two bran-

ches

CA

C’ and

C1 CB. Figure

7 shows a similar

situation in which the two branches are

straight

lines.

Finally figure

8 shows an

asymmetrical phase diagram

similar to that of

figure

3a : the binodal

curve is not

symmetric

due to the asymmetry of the

magnetic

interactions

(l # 0).

FIG. 4. - Phase diagram of an ideal magnetic mixture with : k = 12, / = 2, j = 0. J_ > JAB> jBB > 0). The mixture is

homogeneous at any temperature.

FIG. 5. - Phase diagram of an ideal magnetic mixture with : k = 9, / = 3.5, j = 0. C’ is a tricritical point.

FIG. 6. - Phase diagram of an ideal magnetic mixture with :

k = 5.25, 1 = 3.75, j = 3.25 ( jAA > An > Aa) C’ is a tricritical

point. The dashed line represents the unstable part of the critical line.

(9)

FIG. 7. - Phase diagram of a magnetic mixture with : k = 5.33, 1 = 2.66, j = 5.33. The critical lines CA C’ and CB C1 are straight

lines. C’ is a tricritical point.

FIG. 8. - Phase diagram of an ideal magnetic mixture with : k = 9, I = l,j = 5. The binodal curve is non-symmetric.

We note that the critical line is

composed

of

straight

lines in various cases.

1)

If k

= j (and

I #

0)

or

jAB

= 0. From

(30)

we

deduce the

equations

of the two branches :

The two branches intersect at the

point :

The

following

cases have been studied : I = 0

(Fig. 3b) ;

2)

If

kj

=

l2.

From

(30)

we deduce :

A

particular

case is

again : k

= I

= j (Fig. 1).

6. Phase

diagrams

of non-ideal mixtures

(,l

=

0).

-

6.1 PARTICULAR

CASE : j

= I = 0. - As

expected

from the above

discussion,

M is solution of

(25a)

and

equations (23b)

and

(23a)

become :

Phase

separation

and

magnetic ordering

are inde-

pendant phenomena :

the

magnetization

of an atom

is

independant

of its chemical nature A or

B and, according

to

(34),

the

magnetic

critical

temperature

is

independant of M : kTQ

= 2 k.

Figure

9 illustrates the

two

possible phase diagrams

in the

(M, T) plane :

C is the critical

point

for

phase separation, kTc

= 2 J.

FIG. 9. - Phase diagram of a magnetic mixture with : j = 1 = 0 (jAA = jBB = As = k) : a) k > J, the critical phase is magnetic;

b) k J. C1 and C2 are two critical points at equilibrium.

6.2 PARTICULAR CASE : k = I =

j.

-

Figure

10

shows a

typical

result

already given

in ref.

[4] :

we

choose : J =

12 ; k

= I

= j

= 4. As T is

lowered, phase separation

is induced either

by

interatomic or

magnetic interactions, according

to the initial concen-

tration. C is the critical

point

for

phase separation,

’r a

triple point.

For

larger

values of

J,

no tricritical

point

is found.

6.3 SYMMETRICAL PHASE DIAGRAMS

(! = 0).

-

j

0 : Phase

separation

induced

by

interatomic inter- actions is hindered

by magnetic

interactions

(Fig. 11).

If J >

k, phase separation

occurs as T is reduced for M = 0. The binodal curve is narrowed as compar- ed to the

non-magnetic

case when the two

phases

at

equilibrium

become

magnetic.

If J k the binodal

curve is

entirely

below the

magnetic

critical curve.

For H =

0,

M and R become different from zero.

Phase

separation

is not found if J

+ j

0.

(10)

FIG. 10. - Phase diagram of the Blume-Emery-Griffiths model with J = 12, k = 1 = j = 4. C is the unmixing critical point. C’

the tricritical point, i the triple point. The dotted line represents the binodal curve in the absence of magnetic interactions.

FIG. 11. - Phase diagram of a symmetrical magnetic mixture

with : k = 20, l = 0, j = - 4 ; a) J = 22 ; b) J = 18 The dotted lines represent the binodal curves if j = 0, the dashed line represents

the critical line if J = 0.

j

> 0 : Phase

separation

is enhanced

by magnetic

interactions. Four types of

phase diagrams

are

found

(Fig. 12).

. a)

J is

large : phase separation

is found in the non-

magnetic region

of the

(M, T) plane (Fig. 12a).

b)

For lower values of

J,

a

second

order

phase

transition in M is followed

by

a first-order

phase

transition

in Q

and R as T is decreased for H = 0.

This leads to the

diagram

of

figure

12b :

C’

and

C’

are two tricritical

points, A

is a

quadruple point.

c)

For still lower values of

J,

the two

phase

transi-

tions considered above coalesce and the

diagram

of

figure

12c is obtained. T is a

triple point.

d)

For low values of

J,

the

diagram

is similar to

that of

figure

3a.

6.4 UNSYMMETRICAL PHASE DIAGRAMS

(1

==

0).

Two different situations are shown in

figure

13. For

small values of

J,

the binodal curve is

symmetrical

FIG. 12. - Phase diagram of a symmetrical magnetic mixture with:k=10,1=O,j=6:a)J=15;b)J=l2:CiandCi

are tricritical points : A is a quadruple point; c) J = 9 :

C,

and C2

are tricritical points, i is a triple point; d ) J = 5. In (a), (b) and (c),

the dashed curve represents the unstable part of the magnetic critical curve.

FIG. 13. - Phase diagram of an asymmetrical magnetic mixture

with k = 12, 1 = 2, j = 0 : a) J = 8 : the binodal curve is asymme- trical ; b) J = 14 : below Tc,, the binodal curve is asymmetrical.

The dotted line represents the binodal curve if I = 0.

and is

entirely

below the

magnetic

critical

curve.

For

large

values of

J,

the critical

point

a for

phase

separa- tion is non

magnetic,

and the

magnetic

critical curve

is made of two branches

CA C1

and

CB C2.

(11)

7. Discussion. - We have shown in this paper that the

thermodynamic

behaviour of a mixture of two

magnetic

or nematic

compounds

can be simulated

by

use of a double

spin

one-half

Ising

model with Hamil- tonian

(10).

Such a system is characterized

by

three

order parameters

M, Q

and R but

only

the concen-

tration M and the

magnetization

or orientation

Q

are

generally

observable. Phase

diagrams

similar

to that of He3-He4 mixtures have been obtained :

phase separation

can be

triggered by

interatomic or

intermolecular

interactions,

or

by

the onset of coope- rative

magnetic

or nematic

ordering.

An external

magnetic

field

applied

to a paramagne- tic mixture can also

trigger phase separation.

As discussed

by

Wortis

[10]

our model of a solid

magnetic binary

mixture is valid if the atoms are

mobile and their kinetic energy is

neglected.

Indeed in

the case of a dilute

Ising ferromagnet,

two types of

impurities

must be considered : random

impurities

which are frozen in and mobile

impurities.

In the

first

situation,

the critical

temperature

decreases as the

impurity

concentration is increased until the critical

percolation

concentration : above this

concentration,

the system is

always paramagnetic [ 11 ].

In the second

situation,

a tricritical

point

is found above a certain

impurity

concentration

[10] : phase separation

occurs

at low

temperature,

as in He3-He4 mixtures. The

mobility

of atoms is in fact

implied by

the

pseudo- spin description

of a solid mixture. Our model can

also describe

liquid ferromagnetic alloys :

the

Ising

like character of the

magnetic

interaction is not well

adapted

to such an

isotropic

system, but we are

interested in the

topology

of the

phase diagram

more

than in detailed a

description

of the

magnetic

pro-

perties.

As mentioned

above,

our

lattice-gas

model also

applies

to the

description

of mixtures of nematic

compounds.

The

possibility

of

finding

tricritical

points

in dilute

liquid crystals

has

already

been

suggested [12].

In our

simple model,

the

isotropic

to

nematic

phase

transition is a second order one. In real

systems

it is

slightly

first order in the sense that the

discontinuity

in the order

parameter

is small and there

are

significant

fluctuation

phenomena

on both sides

of the transition. We

hope

however that the model will

give

a correct

qualitative description

of the

phase diagram.

First order transitions would be found if the

elongated

molecule were allowed to take three

mutually perpendicular

orientations : the

spin-one-

half

(r)

would be

replaced by

a

spin-one (Potts model).

The

double-spin 1/2

model has been

applied

to the

description

of

magnetic liquids [13], singlet-triplet magnetic

systems

[14],

the

degenerate

Hubbard mo-

del

[15],

Jahn-Teller systems

[16], magnetic

systems

with

spatial degrees

of freedom

[17],

and the Ashkin- Teller model

[18].

It can be

applied

also to the

descrip-

tion of solidification of

liquid-mixtures,

or the nema-

tic-smectic A transition in

liquid crystal

mixtures

[19].

Acknowledgments.

- I thank Prof. J.

Lajzerowicz

for useful comments.

Appendix

1 :

Spin

S =

3/2 description

of a

magnetic

mixture. - A double

spin

one-half manifold is

equi-

valent to a

spin 3/2

manifold. We shall use the follow-

ing relationships :

so that the

dipolar operator

is

given by :

and the

quadrupolar

operator

by :

and the

octupolar

operator

by :

the

eigenvalues

of c are

1/2, - 3/2,

+

3/2, - 1/2.

Reciprocally

we have :

We note that :

of the form

given by

Tahir-Kheli and

Taggart [20].

The

eigenvalues

of r + 2 6i and i - 2 as are

(1, - 1, 0, 0)

and

(0, 0, - 1, 1).

The Hamiltonian

(10), using

the above formula can be written in the form

given by

Tahir-Kheli and

Taggart.

(12)

Appendix

2 : The

equations

of state

(23)

can also be written :

whence :

References

[1] LEE, T. D. and YANG, C. N., Phys. Rev. 87 (1952) 410.

[2] See MONTROLL, E. W., in Brandeis University Summer Institute

in Theoretical Physics (Gordon and Breach, New York) 1968, vol. 2.

[3] See HUANG, K., Statistical Mechanics (Wiley, New York)

1963.

[4] BLUME, M., EMERY, V. J. and GRIFFITHS, R. B., Phys. Rev.

A 4 (1971) 1071.

BERNASCONI, J. and RYS, F., Phys. Rev. B 9 (1971) 3045.

[5] LAJZEROWICZ, J. and SIVARDIÈRE, J., Phys. Rev. A 11 (1975) 2079, 2090, 2101.

MUKAMEL, D. and BLUME, M., Phys. Rev. A 10 (1974) 610.

[6] KRINSKY, S. and MUKAMEL, D., Phys. Rev. B 11 (1975) 399 and B 12, 211.

[7] See SIVARDIÈRE, J. and BLUME, M., Phys. Rev. B 5 (1972) 1126.

[8] POPLE, J. A. and KARASZ, F. E., J. Phys. & Chem. Sol. 18, 28 and 20 (1961) 294.

[9] HINTERMANN, A. and RYS, F., Helv. Phys. Acta 42 (1969) 608.

[10] WORTIS, M., Phys. Lett. 47A (1974) 445.

[11] ELLIOTT, R. J. HEAP, B. R., MORGAN, D. J. and RusH- BROOKE, G. S., Phys. Rev. Lett. 5 (1960) 366.

[12] PAPOULAR, M. and LAHEURTE, J. P., Solid State Commun.

12 (1973) 71.

[13] HONDA, K. and KATO, Y., Phys. Lett. 44A (1973) 497.

[14] PINK, D. A., J. Phys. C 1 (1968) 1248.

[15] CYROT, M. and LYON-CAEN, C., J. Physique 36 (1975) 253.

[16] PYTTE, E. and STEVENS, K. W. H., Phys. Rev. Lett. 27 (1971)

862.

[17] DOMANY, E., Phys. Lett. 49A (1974) 339.

[18] FAN, C., Phys. Lett. 39 (1972) 136.

[19] ALBEN, R., Solid State Commun. 13 (1973) 1783.

[20] TAHIR-KHELI, R. A. and TAGGART, G. B., Prog. Theor. Phys.

42 (1969) 1265.

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