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HAL Id: jpa-00246381

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Submitted on 1 Jan 1991

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Zero temperature dynamics of a spin glass chain

P. Krapivsky

To cite this version:

P. Krapivsky. Zero temperature dynamics of a spin glass chain. Journal de Physique I, EDP Sciences,

1991, 1 (7), pp.1013-1018. �10.1051/jp1:1991185�. �jpa-00246381�

(2)

Classification

Physics

Abstracts

05.20

Zero temperature dynamics of

a

spin glass chain

P. L.

Krapivsky

Central

Aerohydrodynamics

Institute,

Academy

of Sciences of the USSR, 140160 Zhukovsky-3, Moscow

region,

U-S-S-R-

(Received

25

February

1991,

accepted

21 March

1991)

Abstract. We consider an

Ising spin glass

chain at zero temperature.

Introducing

a time-

dependence

in the model

by

means of Glauber

dynamics,

we have calculated one-spin and two-

spin

correlation functions

exactly.

For

example,

we have found that if one starts at time

t = 0 with all the

spins aligned,

the

magnetization

evolves as

[I

+ exp

(- t)

+ exp

(-

2

t)]/3.

Our results are valid for a

spin glass

chain with an

arbitrary symmetric

and continuous distribution of

nearest-neighbour

interactions.

1. Introductiton.

In recent years considerable interest has

developed

in the

study

of zero-temperature

dynamics

of

spin glasses

and of neural networks

[1-5]. They

exhibit

qualitatively

the same features

(many

metastable states, remanence

effects, etc.)

as

spin glasses

at low temperatures.

However, they

are much

simpler

to

study

from a theoretical

point

of view because the effect of thermal noise is eliminated.

They

may also have a

practical advantage

if one wants to build

pattern recognition

devices.

The reason that

zero-temperature dynamics

is non-trivial and

interesting

is the existence of

a

huge

number of metastable states

(for

a

review,

see, e-g-,

[6]).

Metastable states are

spin configurations

which are

separated by

energy barriers from other

configurations.

These

metastable states are

responsible

for remanence effects

[7],

very slow relaxations and

sensitivity

to initial conditions.

At the moment, one knows how to calculate the number of metastable states and the sizes of their basins of attraction for a one-dimensional

spin glass

at zero temperature

[8-10].

The

particular dynamics

used in references

[8-10]

was

single spin-flip dynamics.

Some of these results have also been

generalized

to more

complicated dynamics [I I].

All these studies

give important

results

conceming

the remanent

magnetization,

the

residual entropy, etc. at time t

= cc. In this paper, we will

develop

an

approach

to kinetic behaviour of a one-dimensional

spin glass

chain with Glauber

dynamics.

We will consider an

Ising spin glass

chain with Hamiltonian

H=-£J~,~~jS~S~~j, S~=±I. (I)

(3)

1014 JOURNAL DE

PHYSIQUE

I M 7

Our results are

independent

of the details of the distribution

p(/~)

of the

exchange

interactions

/~.

The

only

condition for the result to hold is that the distribution p is

symmetric,

p

/~ )

= p

(- /~),

and does not contain any delta function. So our results will be valid e,g, for

a Gaussian distribution

p(/~)

=

(2wJ~)~~'~ exp(- /(/2J~)

and for a flat distribution

p

(/j

" 0 2

/j /J)

2.

Dynamics.

A linear

Ising spin glass

chain with Hamiltonian

(I)

has no natural intrinsic

dynamics.

One way of

introducing

a time

dependence

in this model is

by

means of Glauber

dynamics [13].

We

postulate

a master

equation

for the

probability P(S, t)

of

finding

a

particular

realization of the chain with

spin configuration

S

=

(S~)

at time t,

P

(S~

=

£

Wk

(S~)

P

(S~) Wk(s)

P

(s)j (2)

In this

equation ll~(S)

denotes the rate for the system to

jump

from a

configuration

S to a

configuration S~

obtained from S

by flipping spin

k. The transition rates

W~(S)

for

going

from S to

S~ obey

the detailed

balancing

condition

w~(sk) Peq(sk)

=

w~(S~ Peq(s~ (3)

so that in the limit t

~ cc the

equilibrium

distribution

P~(S~ ~exp(- H[Sl/l~J

will be attained.

However,

there are then still many ways in which the

W~(S)

can be chosen such that detailed balance condition is satisfied. We shall follow Glauber and choose

~~~

~~

~~~~~ ~~~

~

~~ ~~~

~~~ ~~~

where

1~

~

~k,k+i

+

~k-i,k

1~

~

~k,k+1~ ~k-i,k

~~ ~~

2 ~~ T ~ 2 ~~ T ~

~~ ~~~~

~

~~

~

~

~ ~~~~

~

~

T

~

~

~ ~~~~

Note that

by

the definition

(4)

time is measured in units of

elementary spin flip

time. For a

ferromagnetic Ising

chain e~

= &~ = tanh ~ ~

and

consequently

these rates are identical

2 T

to those of reference

[13].

From the master

equation

we shall derive evolution

equations

for the

spin

correlation functions

iii..

i~

)

m

~j

S~~.

$ P(S~. (6)

s

~

Taking

the time derivative of

equation (6)

and

using

the master

equation (2)

and relations

(4)

one finds

~ n

i <ii in I

= n

<ii in

+

Z

i~ip

I.. ip

+ i

I

+

bi~ I.. tp

i

Ii (7)

p= i

From this

equation

we see that an

advantage

of the choice

(4)

for the transition rates is that the evolution

equations (7)

for

n-spin

correlation functions

(6)

contain

only n-spin

correlation

functions. This makes the

problem

solvable at zero temperature as we shall show below.

(4)

3.

One-spin

correlatiton functions.

At T

=

0 the

dynamics

becomes

extremely simple. Equation (5) implies

~k "

°, ~k

~ S~II

(~k-i,k)

~t

(~k-i,k'

~

'~k,k+1' (8~)

~k

~

°,

~k ~ S~ll

(~k,k+i)

~t

'~k,k+1(

~

'~k-i,k' (8b)

It is therefore convenient to divide all bonds

along

the chain into three

types, namely

strong

bonds,

medium bonds and weak bonds. We say that

J~~~j

is a strong bond if

J~,~

~ j ~ max

( J~

j,~

[, J~

~ j,~~ ~

).

So a bond is strong if

iti

two

neighbouring

bonds are weaker.

Similarly

a bond is weak if its two

neighbouring

bonds are stronger.

Lastly

a bond is a

medium bond if one of its

neighbours

is stronger and the other

neighbour

is weaker. This classification is violated when

[J~

j ~ =

[J~

~

~ j

[,

but our

assumption

that the distribution

p(/~)

does not contain any delta

~function ~shows

that such

a violation occurs with zero

probability.

Further we shall call parts of the chain between two consecutive weak bonds

by

clusters. So the chain is broken into clusters of medium and strong bonds delimited

by

consecutive weak

bonds. A

typical

cluster is

depicted

in

figure

I. It contains the

only

one

strong

bond and an

arbitrary

number of medium bonds.

Zero temperature

dynamics

of

spins

in an

arbitrary

cluster is determined

by

the

spins

of this cluster

only.

So the chain is broken onto a system of

noninteracting

clusters.

Let us consider the kinetic behaviour of

one-spin

correlation function in the cluster

depicted

in

figure

I.

Combining equations (7)

and

(8) gives

( (k)

=

(k)

+

e~(k

+ I

)

at I w k mm

(9a)

~

(k)

=

(k)

+

&~(k

I

)

at m + I w k

w L.

(9b)

Here we have used the notation of

figure I,

L is the

length

of the cluster and

(m,

m + I the

only

strong bond in the cluster.

For

simplicity,

we

stipulate

that at t = 0 the chain is

fully magnetized,

I.e.

(k)

=

I

for all k.

Other initial conditions can also be dealt with- in the

following

we shall denote s

= e~ =

&~~

i and

c~ =

jkj

exp

(t) (10)

Solving (9) yields

c~ = exp

(St)

c~_j = I + e~_j

s(c~- I)

Cm-2 ~ l + ~m-2 + ~m-2

~m-I(Cm

l

~S~)

~~~~~

Cm-3 "1+ ~m-3 + ~m-3 ~m-2

t121+

~m-3 ~m-2 ~m-I

S(C~

I ~S~

l12'),

etc, at km m, and similar results

cm + i = exP

(St)

Cm+2 ~ l +

~m+25(Cm+1~ l) (lib)

c~~~ =1+

&~~~

t +

&~~~ &~~~(c~~j

I

-St),etc.

atkmm+1.

(5)

1016 JOURNAL DE

PHYSIQUE

I M 7

(Jk~i<:(

j

m ml

L

Fig.

I. A

typical

cluster with the strong bond (m, m + ).

These correlation functions become

extremely simple

after an average over the random

couplings. Equations (8) imply

that in such an average

e~'s

in

(I la)

and

&~'s

in

(I16)

take the values ± I with

equal probability

and

independently. Performing

the averages of the solution

(I I)

one finds :

<k)

=

(~~P~~ [1

~~ ~~

~#'~'

'~+

(12)

+

exp(-

2

t)]/2

at k

= m and k

= m +

From the

knowledge

of the kinetic behaviour of

one-spin

correlation functions in a cluster of

length

L, one can deduce the relaxation of the

magnetization

m(t)

= exp

(- t) ~ £ (L

2

) X~

+

[I

+ exp

(-

2

t)] £ X~. (13)

2

~2

Here

X~

is the

density

of clusters of

length L,

which was

computed by

Derrida and Gardner

[10]

X

=

2~(L

I

(L

+ 2

)/(L

+ 3

) (14)

A direct calculation of the sums on the

fight-hand

side of

equation (13)

then

yields

w w

~j (L 2) X~

=

~j X~

=

1/3.

Thus we obtain

L=2 L=2

m(t)

=

ii

+

exp(- t)

+ exp

(-

2

t)i13. (15)

Observe that remanent

magnetization

at time t

= cc

equals

to

1/3.

TMs result was first found

by

Femandez and Medina

[12]

and then rederived and

generalized

in references

[8-11].

4.

Two-spin

correlatiton functitons.

We now turn to the calculation of

two-spin

correlation functions at zero

temperature.

For a

pair

of

spins

from distinct clusters one has the obvious result

liJ)

=

Ill lj) (16)

(6)

For a

pair

of

spins

inside a cluster

equations (7)

and

(8)

can be rewritten as

~

c~~ = e~ c~

~ j ~ + ej c~~ ~ j

(I

w I

~

j

w m

) (17a)

dt

~

c~~ = &~ c~ j ~ + &~ c~~ j

(m

+ I w I ~

j

w L

(17b)

dt

~

c~j = e~ c~ ~ i j + &~ c~~ j

(I

w I mm, m + I w

j

w L

) (17c)

dt

with

c~~ =

(ij) exp(2 t). (18)

Hereinafter we assume that I

ij.

Other correlators can be reconstructed from the relations

c~~ = c~~

and c~~

=

exp(2 t).

We

begin by calculating

the

special two-spin

correlation functions in which one

spin belongs

to the strong bond

(m,

m + I

).

From

(17),

a closed system of

equations

is obtained for the

rows

j

= m and

j

= m + I. It is convenient to present these

equations

in a vector form :

with

A~ =

~~+

A~* =

~~

(20)

Cim Cim+1

A~

we determine

directly

from

(17) A~

=

Uexp(2 t)

at s

=

(21a)

A~

=

U +

V[exp(2 t) I]

at s =

(21b)

where we introduced the shorthands

U=

(()

and V=

(~j).

Solving (19)

with the initial conditions

(21) yields

A~ =

Uexp(t) F~(t)

at s =

(22a)

~41 " U exp

(-

t F~

(t

+

Ve~

e

~ j G

~

t)

at s =

(22b)

where

F~(t)=

I +e~t+. +e~..

e~_~t~~~~~/(m-I-I)!+e~.

e~_j

~j

~

t~/nj

n=m-1

and

G~(t)

= 2 exp

(t) ~o ~j t~+

'

+~P/(k

+ + 2p

One can also calculate

two-spin

correlation functions in the columns I =m and

I

= m + I.

They

are described

by

formulas such as

(22a)

and

(22b).

One can further calculate all other

two-spin

correlation functions

recurrently.

For

example,

in the

triangle

I wi <

j

mm, we have

already

found the upper row

j

= m, see

(21)

and

(22). Using (17a)

we then find the correlators in the row

j

= m

I,

etc.

(7)

1018 JOURNAL DE

PHYSIQUE

I M 7

After

performing

the disorder average of these

unwieldy

correlators we arrive at the

extremely

compact final result

(ij)

=

Ii ) (j)

at

(ij)

#

(m

m +

(23)

with

one-spin

correlation functions

given by (12),

and

(m

m +

)

= exp

(-

2

t) (24)

Thus our results

imply

the absence of correlations between

spins

of distinct clusters

(see (16))

and also the absence of correlations between

spins

of the same cluster after

performing

the disorder average

(see (23))

with the

only exception

of

spins

connected

by

a strong bond.

Acknowledgment.

I wish to thank N. Slavnov for warm

hospitality

in Institute of

Computer

Mathematics and Informational

Technologies.

References

[1] PARETTO P., Biol.

Cybernet.

50

(1984)

51.

[2] BIENENSTOCK E., FOGELMAN-SouLiE F. and WEISBUCH G., Disorder

Systems

and

Biological

Organization

(Springer-Verlag,

New York, 1986).

[3] AMIT D. J., GUTFREUND H. and SOMPOLINSKY H.,

Phys.

Rev. A 32

(1985)

1007 ;Ph_vs. Rev. Lett.

55 (1985) 1530.

[4] GARDNER E., DERRIDA B. and MOTTISHAW P., J.

Phys.

France 48

(1987)

741.

[5] HANKEL R. D. and KINzEL W., J. Phys. A 20

(1987)

L 727.

[6] BINDER K. and YOUNG A. P., Rev. Mod. Phys. 58 (1986) 801.

[7] KINzEL W., Phys. Rev. 833

(1986)

5086.

[8] LI T.,

Phys.

Rev. 824

(1981)

6579.

[9] ETTELAIE R, and MOORE M. A., J.

Phys.

Lett. France 46

(1983)

L 893.

[10] DERRIDA B. and GARDNER E., J.

Phys.

France 47

(1986)

959.

[I I]

ETTELAIE R. and MOORE M. A., J. Phys. France 48

(1987)

1255.

j12]

FERNANDEz J. F. and MEDINA R.,

Phys.

Rev. B 19

(1979)

3561.

j13]

GLAUBER R. J., J. Math.

Phys.

4

(1963)

294.

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