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The Potts spin-glass in a transverse field

Yadin Goldschmidt

To cite this version:

Yadin Goldschmidt. The Potts spin-glass in a transverse field. Journal de Physique I, EDP Sciences,

1992, 2 (1), pp.31-39. �10.1051/jp1:1992116�. �jpa-00246460�

(2)

Classification Phydcs Abstracts

05.20 05.30 75.50L

The Potts spin-glass in

a

transverse field

Yadin Y. Goldschmidt

Department of Physics and Astronomy, University ofPittsburgh,

Pittsburgh,

PA 15260, U-S-A-

(Received

23 July 1991, accepted 20

September 1991)

Abstract. ln this paper we derive an expression for the free energy of the infinite ranged quantum Potts spin-glass in

a transverse field using the replica method and the Suzuky-Trotter

formula. Results are obtained for general p

(number

of Potts

states)

and explicit calculations

are done for p

= 3

using

exact spin summations for M < 8 where M is the size of the lattice in the Trotter direction. The phase diagram is obtained and is also compared with results for the

static approximation which is non trivial even in the paramagnetic phase.

I Introduction.

The

investigation

of the quantum

spin-glass

model attracted much attention

recently [1-17].

It has been found that quantum

tunneling

has a

disordering

ef§ect similar to the temperature.

In the case of the

Ising

model in a transverse

field,

the transverse field simulates the effect of

tunneling

in proton

glasses

[3]. It has been found that this

field,

when strong

enough, destroyes

the

spin- glass phase

even at T

= 0~ but the nature of the

spin-glass phase,

when it

exists,

for the case of the infinite range

model,

is very similar to the classical case

(r

=

0)

and is characterized

by

a Parisi order paramater

q(z) (or alternatively by

a non trivial distribution of

overlaps P(q)) [18]. Experimental

realizations of proton

glass

occur in random mixtures of ferroelectric and antiferroelectric materials [3], and it has been

proposed recently

that the

quantum Heisenberg spin-glass

may

play

a role for some range of

doping

in the

newly

discovered

high-n

materials

(in

the

insulating phase)

[19].

The classical infinite

ranged

Potts

spin glass

has some

interesting

features which have been

investigated

in recent years [20,

21].

In

particular

for p > 4

(p

is the number of Potts

states)

the

spin-glass

transition has some first order

features,

and for any p > 3 the order parameter

q(z)

has a

particularly simple

form for some range of temperatures below Tg [21].

In this paper we

generalize

the

Ising

model in a transverse field to the case of the Potts model with

general

p and use the

replica

method and the

Suzuky-Trotter

formula

[22,

23] to map the model into an

equivalent

classical system. The Potts model in a transverse field which represent

tunneling

between the p

equivalent

Potts states is

quite

non trivial. Even the static

approximation

in the

paramagnetic phase

is difficult to

implement

for

general

p.

(3)

32 JOURNAL DE PHYSIQUE I N°1

After

deriving

some

general

results we concenrate on the case p

= 3 where the transition is

expected

to be of second order for any value of the transverse field r

(we verify

this

explicitly

for M =

2).

We first determine the location of the

phase boundary using

the static

approximation.

We then carry out exact

spin

summations up to M < 8 and

extrapolate

the results to M = oc

using

the

I/M~

law [24]. The result obtained

by

this method for the

rc(T

=

0)

is found to be lower than static

approximation

result which is known from the

Ising

case to over-estimate the value of the transverse field necessary to

destroy

the transition at T

= 0.

Finally,

We

point

out

questions

and directions for future research.

2. The free energy and order paranJeters for

general

p.

Following

the discussion in reference [25] we consider the

following

Hamiltonian for the Potts model in a transverse field:

p-I p-I

~f =

~

j,,

£(u±u,)m r£ ~

vp

(i)

iJ i J i

(ij) m=0 I m=0

Here

(ij)

is a summation over all distinct

pairs

of

sites,

and it is a summation over all sites.

V and U are site variables

(operators)

which on a

given

site

satisfy

the

Zp algebra

VU =

e~~~'/PUV, V+U

=

e~~'/PUV+,

VP

= UP

=

(2)

In a

particular representation

in which U is

diagonal

one has

U

nj

=

e~'+ nj,

n = 0,

, p

(3j

V

n) =I

n +

ii

and

PI

= 0)

(4)

Jij

are random variables which for

simplicity

can be chosen to

satisfy

a Gaussian

probability

distribution of width

J/@

and mean Jo

IN

where N is the total number of sites.

We now make use of the Suzuki-Trotter formula to map the system into a classical system

plus

an extra '~Trotter" dimension. The effective classical Hamiltonian for the Mth

approxi-

mant is

given by

~

M N

~~~~~~ ~

M

( ( ~"~~'l~~>~J(~)

~ ~

~ $ ~n,(k),n,(k+i)

+

CNM, (5)

with

~ ~

B =

In(

~~'~j~~

),

C =

In(

~ ~'

(6)

e M I P

and 7

=

fly.

In

deriving equation (5)

we have used the identities

exp(7 f

V~)

= 1+ ~~~

f V~' (7)

m=0 P

m=0

(n exp(7 f

V~) n')

=

bn,n,

+

~~~

(8)

m=0 P

(4)

where the

eigenstates n)

of U where defined in

equation (3).

In

equation (5)

the classical variables

n,(k)

take the values

0,

p- I on sites

(I, k)

where k =

I,

,

M labels the Trotter direction and

satisfy

the

periodic boundary

condition in this

"time"

direction. Ultimately

the limit M

- oc must be taken. The

quenched averaging

over

the random bonds is done

by

the use of the

replica

trick

[26].

After some

algebra

we obtain:

"

"

4flln 11 £iQ17'(k> k')12

+

t ~o ~o ~imz<~,j~

no , ~~ ~ ~ ~

-(In~hexp(G) (9)

with

p2 j2

~ "

~ £(~~na

,

(k),na(k+i) +

tl)

+

~ 2 Jf2

~ ~ ~ Qll

(~>

k')(P~n"(k),~ l)(P~n«'(k'),s

~)

a i P

««, ;1, »

+

jjj ii LMI(k)(p&n«~i~,~ i) (lo)

~ ~ i

where the linfit

n - 0 has to be taken. We now define

j~a

(~ ~l) Qaa(~ ~l) (~~)

~8 ~8 '

and reserve the notation

Qff'

for the

case where a

#

o'. Based on the Potts symmetry of the model we look for

stationary

solutions

satisfying

Q(f'

=

Q°°'(pbm

1)

(12)

Rls

=

R°(pb~s

11

(13)

We will further

simplify

the

expression

for the free energy

by making

the

following

assump-

tions and arguments:

First since we are interested

only

in the

spin-glass phase

and not in a

ferromagnetic phase (or

a mixed

phase)

we choose

Jo

to be

negative

such that

Mf(k)

= 0. This choice has also

been used in the classical case

[20, 21].

Next we assume that

Q°°'(k, k')

does not

depend

on the Trotter index. This has also been

used in the

Ising

case and follows from the nature of

Q

as the

spin-glass

order parameter, and it is found to be a consistant solution of the

stationarity

conditions. For

R°(k, k')

we will assume

that it does not

depend

on a since there is no

prefered

direction in

replica

space and that the

dependence

on

k,

k' comes

through

the difference k k'

(because

of translation invariance in the Trotter

direction).

To

simplify

matters we will use a first step

replica

symmetry

breaking

scheme [27] in the

spin glass phase

which for the classical case

(for

p >

2)

is known to be exact in a range of temperature below

Tg.

[21]

Thus one puts a =

(L7)

with L = I,

,

n/m;

7 " 1, m and

Q°°'

"

Q2

L

"

L'>'f # 'f' (141

Q°°'

=

Qii

L

#

L'

(15)

In the classical case for p > 2 one has

Qii

" 0 in a range of temperatures below

Tg.

Since it is not

guaranteed

to hold for r

#

0 we will

keep

the most

general

case

(15).

First step RSB

(5)

34 JOURNAL DE PHYSIQUE I N°1

even if not exact is a

good

first

approximation

to the

spin glass

case as has been found for the

Ising spin glass

in a transverse field [14]

(p

=

2).

We will now use the Wallace-Zia [28]

representation

of the Potts variables as p I dimen- sional vectors

S(n),

n =

0,

,p I.

We have

pbnn,

I =

S(n) S(n') (16)

The free energy

can now be written in the form

p2

j2

~ i

~~

~

~ ~~

~~~~~~2 ~~l) ~(

+

j~2

~~~~

~ ~' ~

ii'

jDP~~z

in

jDP~~y Z'$ (17)

m

~~~~~

~p-i, jj

~~'~

)exp(- £ z?/2) (~~)

@

~

n>=i I

and

similarly

for

DP~~y. ZH

is

given by

Tt

exp(H)

where

H =

j L(R(I

k k'

1)

Q2)S(n(k)) S(n(k'))+

+

~(

~

S(n(k)) S(n(k

+

1))

+ ~ +

C)

~ P P

+$( Qii

y +

/& z) ~ s(n(k)) (19)

from

equations (17)-(19)

we obtain the

stationarity equations

for the R's and

Q's

q

_ -l~

ji~

(~ij

~~

p

- I

I ~

~yZg

where

(A)H

"

lh[A exp(H)]/lh exp(H) (23)

In the

pararnagnetic phase equation (17)

becomes

Pi

=

(jj~ (p

11

~ R(

k k'

1)~ in zH

(24)

~ ~

kk,

with

H =

~ £

R(I

k k'

I>S(n(k» S(n(k'l>

+

L()S(n(k» S(n(k

+

ii>

+

)

+

Cl (251

(6)

and

R~i

k k' i> "

)iS<n<k» S<n<k'»iH

(26>

In the case that the transition is continuous

<which

for q < 4 is known to be true when r

=

0),

then the

phase boundary

is determiend

by

the condition This is found

by expanding

the

free energy in powers of

Q

and

identifying

the coefficient of the

quadratic term>:

ji £

~<

k k' I> "

TC/J

<27>

k,k'

For the case when the transition is of first order

equation

<27> is no

longer

valid since the location of the transition is no

longer

determined

by vanishing

of the coefficient of the

Q~

term in the

expansion

of the free energy in power of

Q.

In that

case the location of the transition

can be found

by matching

the free

energies

in the

paramagnetic

and in the

spin-glass phases.

3.

Explicit

calculations for p

= 3.

In this section we will carry out

explicit

calculations for the three state Potts model. We will

assume that as in the classical case with r =

0,

the transition is continuous and hence we can

use the condition

(27>.

We have verified that this is the case for M = 2

(see below>

where we

were able to calculate the order parameters

Q2

and

Qii

in the

spin-glass phase.

Before we

proceed

with the exact calculations we will

briefly

describe the results of the static

approximation.

In the static

approximation R(k,

k'> is taken to be

independent

of

k,

k'. We then find that

equation

(24> taken the form

fl f

=

~~~~

R~

7 lim in G <28)

with

G

=

j

Dz 'h

exPl~ £(S(n(kl S(n(k+ Ill 2>+ $4

z

.~lS<n<k»

+

S<n(k+ I»11

(29>

s(o>

=

<v5,o>, s<i>

=

<-(, (>, s<2)

=

<- (, (>

<30)

The trace in

equation (29)

can be obtained from the

eigenvalues

of a 3 x 3 transfer matrix

representing

a I dimensional Potts model. Because of the M

dependence

of B B

--

In(M/r)

for

large M)

and of the

magnetic

field one needs to consider a non- trivial M

- oc limit.

This means that one has to calculate the

I/M

correction to the

eigenvalues li

of the transfer

matrix.

Pitting

li = I +

flui /M

+

O(I /M~

we find

G =

j

Dz

£efl~'

<31)

I

l

with u,

being

solutions of the

equation

u~ 3<(h( I )h(

+

r~)u 2r~ #h(

+

~#hi hi

= 0 <32>

(7)

36 JOURNAL DE PHYSIQUE I N°1

h;

=

J4

z;

(33)

Equation (33)

can be solved

numerically

and

together

with

equations (28) (31)

and the condition R =

I/flcJ

can be used to find the

phase boundary

between the

spin-glass

and

paramagnetic phases.

Here we consider the

limiting

cases of r

= 0 and T = 0.

In the case r = 0 one

easily

find

~~~

"~

~~~'

"~

~~~

~

~~~'

~~

~~~ ~~~

~~~~

p j

=

1p2 j2

j~2

p2 j2

j~ f~ ~

(~~j

~ from which R

= I and also Tc = J. This agrees with known results for the classical case.

In the case Tc - 0 we would like to find r

(Tc)

in that limit. We have to consider the limit flc - oc and R

- 0

(since

Rc

=

I/flcJ

at the

transition)

and thus h; in

equation (32)

are also small. Under these conditions the

largest

solution for

equation (32)

is

um = 2r +

(h(

+

h()

+

= 2r +

J~Rz~

+

(36)

3r 3r

Thus the free energy is

given

in the small T limit

by Pi

=

(~~

R2

3Pr

+

in(1 ~((~ (37)

From this

equation

and the condition ll~ = I

/flcJ

we find

rc(T

"

0)

"

~J (38)

In case of the

Ising

model

(p

=

2)

it is known that the static

approximation

tends to overestimate the value of rc at T =0.

(The

exact value is about

rc(0)

-- 1.51J whereas the static

approximation yields

rc (0> =

2J>.

We now

proceed

to an exact evaluation of the location of the

phase boundary using

exact

spin

summations. We have evaluated the free energy

(24)

and solved for R (( k k' for lattices with the size of the Trotter dimensions up to M = 8

(with periodic b-c-).

For M = 2

we have also solved for the solution in the

spin- glass phase.

In the

spin-glass

one has to carry out the two dimensional

integrals

d~z and

d~y

in

equations <20)-(22)

and the solution is

quite

time

consuming.

The results of the

spin-glass phase

calculation

indicates,

at least for M

= 2,

that:

(a)

The transition is of second order for p

= 3 even for r

#

0;

(b)

The first stage

replica breaking

with

Qii

" 0 is a solution of the

stationarity

condition

for a range of temperatures below

Tc<r)

as it is for r

= 0.

More work has to be done to establish these results for M = oc

although

the results seems

plausible. Assuming

the transition to be continuous we derived the location of the

phase boundary

from the solution of

equations (26)

and

(27).

For temperatures 0.95, 0.9, 0.8, 0.6 we have calculated

rc(T>

for M

= 2, 4, 8. For T

= 0A we evaluated

rc<T>

for M =

4,8.

The values obtained for

rc(T)

as a function of

I/M~

lie on

nearly straight

lines.

(This

is the known

I/M~

law

[24])

and

by

this method we

extrapolated

to M

= cxJ

(allowing

for some small error

bars)).

The results are

displayed

in

figures

I and

figure

2.

Figure

2 shows the location of the

phase boundary

and we see that

rc(T

=

0)

-- 1.05- 1-1This is

compared

with the value of

4/3

obtained from the static

approximation

which is known to overestimate the value of

rc(T)

for small T.

(8)

2.0

Legend 1.8

. T=0.g5

x T=O.g

6 a T=O.8

. T=0.6

1_4 ~"~'~

l.2

~ i.o

0.8

O.6

O.4

O.2

0 O.025 O.OSO 0.075 0.100 O.125 0,150 O,175 0.200 0.225 O.250

1/M62

Fig. 1. rc ~3.

1/M~

foT various values of T for the p

= 3 Potts SG.

1.2

1-o

0.8

~

O.6

O.4

, '

,

O.2 ,

0

0 0.2 0.4 O.6 0.8 1.0 .2

r

Fig. 2. Phase boundary between the

Spin-glass

and paramagnetic phases for the

case p = 3. The

dotted line is a possible extrapolation to T

= 0.

(9)

38 JOURNAL DE PHYSIQUE I N°1

4. Conclusions.

In this paper we extended the

Ising spin-glass

in a transverse field to a p-component Potts model with a transverse field that induces

tunneling

among the p-states. This model may have

experimental

realizations in ferroelectric antiferroelectric mixtures and is also

interesting

from the theoretical

point

view. More work is needed to

investigate higher

p

values, especially

p >

4, where the transition is known to have some first order features for r = 0

[21].

A solution for p

- oc may also be found. These are

projects

for future research.

Acknowledgements.

This work has been

supported by

the National Science Foundation under grant

#

DMR- 90l6907.

Note added in proofs: After the

completion

of this w6rk we became aware of a

preprint by

K. Walasek and K. Lukierska-Walasek who consider the 3 state Potts

glass

in a transverse field.

They

do not use

replicas,

but rather an uncontrolled effective field

approximation

that

neglects

correlations among different components of the

cavity

field. Their result of

rc(0)

= 2

/3

underestimates the value of the critical field at T

= 0.

References

[I]

Bray A. J. and Moore M. A., J. Phys. G13 (1980) L655.

[2] Sommers, J. Ma9n. Mater. 22

(1981)

267.

[3] Pirc R., Tadic B. and Blinc R., Z. Phys. B 61

(1985)

69.

[4] Ishii H. and Yamamoto T., J. Phys. G. 18

(1985)

6225; J. Phys. C 20

(1987)

6053.

[5] Usadel K. D., Solid State Gommun. 58

(1986)

629; Nucl. Phys. B

(Proc. Suppl.)

5A

(1988)

91.

[6] Walasek K, and Lukierska-Walasek K., Phys. Rev. 34

(1986)

4962.

[7] Usadel I<. D, and Schmidtz B., Solid State Commun. 64

(1987)

975.

[8] Dobroslavievic V. and Stratt R., Phys. Rev. B 36

(1987)

8484.

[9] Yokota T., Phys. Lent. A 125

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482.

[10] Ray P., ChakrabaTti B. K, and Chakrabarti A., Phys. Rev. B 39

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3339.

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428; ibid 41

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4858.

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[18] see e.g. Binder I<. and

Young

A. P., Rev. Mod. Phys. 58

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L497, L971, L1169.

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545.

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1454.

(10)

[24] Suzuki M., Quantum Monte Carlo Methods, Springer Series in Solid-State Physics 74, M. Suzuki Ed.

(Springer-Verlag, 1987).

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(1982)

149.

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(1975)

1792.

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13(1980)

L155, L1101, L1887.

[28] Zia R. K. P. and Wallace D. J., J. Phys. A 8

(1975)

1495.

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