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The Cavity Approach for Metastable Glassy States Near Random First Order Phase Transitions

T. Kirkpatrick, D. Thirumalai

To cite this version:

T. Kirkpatrick, D. Thirumalai. The Cavity Approach for Metastable Glassy States Near Random First Order Phase Transitions. Journal de Physique I, EDP Sciences, 1995, 5 (7), pp.777-786.

�10.1051/jp1:1995168�. �jpa-00247102�

(2)

J. Phys. I France 5

(1995)

777-786 JULY 1995, PAGE 777

Classification Physics Abstracts

75.10N 64.60M 64.70P

The Cavity Approach for Metastable Glassy States Near Random First Order Phase llYansitions

T.R.

Kirkpatrick

and D. Thirumalai

Institute for Physical Science and Technology, University of Maryland, College Park, Maryland 20742, U-S-A-

(Received

23 January1995, received in final form 5 April 1995, accepted 7 April

1995)

Abstract. Ii is shown that trie cavity method developed to describe equilibrium states in trie mean-field Ising spin glass model con be generalized to describe metastable stores in trie mean-field Potts glass. Trie crucial input is trie existence of an extensive number of statistically

similar but incongruent metastable states with

a weighted Gaussian free energy distribution. It is

argued that the inherent quenched randomness m trie Potts glass Hamiltonian is net important for most of the arguments and that this approach provides insight into recent work on trie

structural glass problem.

1. Introduction

In ibis paper we show how trie

Onsager (reaction

field

approach)

or

cavity

method

developed iii

to describe

equilibrium

states in trie mean-field

Ising

spin

glass

model [2] con be modified to describe metastable

glassy

states near random first-order

phase

transitions. For concreteness we

focus on trie mean-field p-state Potts

glass (PG)

model

(with

p

>4)

where trie metastable states have been well characterized

by

orner methods

(3,4]. However,

we stress that trie ideas behind this

approach

are rather

generic

and in

particular they

do non

depend

in a sensitive way on trie fact that trie PG Hamiltonian bas

quenched

randomness built into it. As a consequence, we

argue that trie ideas

presented

here con be used to understand some work [Si on trie structural

glass problem

which bas no

quenched

randomness.

Trie

general

type of system and situation we bave m mmd is trie

following.

First, trie system is above its

equilibrium (ideal) glass

transition temperature which we denote

by TK,

or

by

trie

Kauzmann temperature

(in general

TK may be ai zero

temperature). Second,

trie

incipient phase

transition is most

naturally

described

by

a

probability

measure for a random order parameter with zero mean. Trie usual observable order parameter is trie average of a

squared

random variable referred to

commonly

as trie Edwards-Anderson order parameter, q (2]. Ai

TK,

q

jumps discontinuously

from zero to a finite value at a random first-order

phase

transition.

For ail temperatures greater thon

TK,

but less thon a temperature denoted

by

TA, there exists

locally

stable

glassy

metastable states. In mean-field models these states are

infinitely long- lived,

whereas in

short-ranged

models

they

can

presumably

be

theoretically

well-defined

by neglecting droplet

fluctuations or

activated, A,

transport. For trie systems we consider, there

Q Les Editions de Physique 1995

(3)

exists an extensive number of

statistically

similar but

incongruent

states (6] metastable states below TA and ii is these states that are considered in this paper. Because of trie extensive

solution

degeneracy,

these states are

expected

to control trie

dynamical

behavior of trie

glass

for ail T < TA

13,4, ii.

In trie above

description: (1)

An extensive number of solutions occurs when the

logarithm

of trie number of states scales with the system size,

(2)

Two states are

statistically

similar when

they

have the same value of q,

(3)

States are

incongruent

when the

overlap

function

(Eq. (3.6))

is zero.

The ideas behind the cavity

approach

are as follows.

Imagine

an

N-spin (or N-partiale)

system and add a new one to it. One then tries to determine the statistical mechanics of the

(N +1)

spm system

by studying

the response of the

N-spin

system to the additional

spin.

In

general,

one can

imagine

two types of

important

fluctuations that act on the added spin. First, even if there is a

single

unique state

(as opposed

to

configuration)

of the N and N

+1-spin

system, there will be a

fluctuating magnetic

field felt

by

the additional spin due to thermal fluctuations in the

N-spin

system.

Secondly,

if the order parameter

description

is

intrinsically probabiistic,

as it is in

glasses,

then to obtain observables one must average

over the randomness. Here ii is

important

to

distinguish

between two

possible

sources of randomness. There is the randomness m spin

glasses

due to the presence of

quenched

disorder

m the

microscopic

Hamiltoman. Even if there is a unique macroscopic state for a

given

set of random bonds the local site

magnetization

fluctuates due to this randomness. Trie second type of randomness is more novel and does arise even in

regular Hamiltonians,

1-e-, in those systems where

quenched

interactions are not

explicitly

present. If there are many

macroscopic

states that are

statistically

similar and bave

nearly equal

free

energies

then an externat field cannot be used to

pick

oui a

particular

state and one is forced to average over ail these states. In previous work on trie structural

glass problem

(Si it is trie second type of randomness that is shown to be important. Note that this type of randomness can m

principle

exist even if trie

microscopic

interactions are not random.

Subsequent

to Dur initial work on model Hamiltonians

describing

trie

liquid

to

glass

transition numerous papers bave

recently

aflirmed trie earlier conclusion that

glassy dynamics

can result in systems without

quenched

randomness

[8-12].

In this

paper, we

provide

very

general

arguments that this conclusion is

intimately

tied to trie notion that an intrinsic randomness results due to the presence of a

large

number of

statistically

similar macroscopic states. In the case of spin

glasses

without reflection symmetry these arise

m the temperature range TK < T < TA where TK and TA are the characteristic temperatures introduced earlier.

Explicit

calculations reveal that ii is

precisely

in this temperature range that there are

large

numbers of

macroscopically

well-defined metastable states.

Conceptually,

the situation we are

considering

here dilfers from the

problem

considered before

by

Mézard et ai.

iii

for the

Ising

spin

glass

model because: 1) the states we consider do not have an ultrametric

topology, 2)

for our case, two states

typically

dilfer in free energy

by

an amount

+~O(N~/~)

and the

weighted

distribution of free energy states is Gaussian rather

than

exponential

[4].

Nevertheless,

we shall see that the calculational

methodology developed by

Mézard et ai.

iii

can be

applied

with

appropriate

modifications.

Finally,

we point out that the states we consider are

completely

missed in the usual statistical mechanical

approach

to spin

glasses

[2j.

Physically

this is because the natural order parameter to this

phase

transition

is the Edwards-Anderson parameter which is a

dynarnical

quantity. The plan of this paper is

as follows. In Section 2 we rederive the TAP equations for the PG using the cavity method and obtain an expression for the site

magnetization

m terms of a random

magnetic

field

acting

on that site. In Section 3 we denve the

probability

measure for the random

magnetic

field

and obtain the self-consistent

equation

of state for the Edwards-Anderson order parameter.

This result agrees with that obtained from

approaches [3,4j.

In Section 4 we conclude with a discussion.

(4)

N°7 THE CAVITY APPROACH FOR METASTABLE GLASSY STATES 779

2. Thermal Fluctuation in a

Single

State:

Tap Equations

for trie PG

In this section we use the cavity

approach

to derive the TAP

equations

for the PG. The derivation in a

generalization

of that

given

elsewhere [2] for the mean-field

Ising

spin

glass.

We repeat it here because some of the results are needed in the next section where fluctuations due to solution

degeneracy

are taken into account.

The mean-field or infinite

ranged

PG Hamiltonian is

(3,13],

p-1 l~

"

~ ~ ~çS,asja. (2.1)

~~~

i, j

~

j)

The PG has p components m a

(p-1)-dimensional

vector space. The bonds

(J,j )

are

randomly

distributed

according

to,

P(J,j)

=

~

~ exp

~~j~~j

,

(2.2)

2~rJ

~ ~

2J

with N the number of lattice sites. To suppress a

ferromagnetic

transition one must

properly

fix the average of

J,j.

We avoid this

problem by setting

the

ferromagnetic

order parameter,

N

Ma =

~jm,a

= 0.

(2.3)

~

i=J

equal

to zero. The S,a in

equation (2.1)

are Potts variables chosen from the set

(e(),

é

=

1, 2,.. p,

given

in reference [14]. Some useful identities are,

~j

P

ele(

"

Pôab, (2.4a)

1=1

~j

p-1

e(e$'

=

pâli»

1.

(2.4b)

a=1

~j

P

e(

= 0.

(2.4c)

1=1

We next add an additional Potts

spin

at a site 0. The vector

configurational magnetic

field

acting

on site 0

(the (N +1)~h spin)

due to the

original N-spms

is,

N

hi

=

fl ~j

Jokska.

(2.5)

k=1

If the

N-spin

system is m the state

a(N)

then

by

definition the number of

configurations, dN(EN),

of the

N-spm

system with energy between EN and EN +dEN is,

dN(EN

=

e~(~N)dEN

=

exp[fIEN flF~(NjÎdEN (2.6)

The

magnetic

field

given by equation (2.5)

is

specified by

a

probability distribution, P(h)dh,

equal

to the

probability

that

choosing

at random any relevant

configuration

in

a(N)

the value of

(5)

ha is in the interval

(ha,

ha+dha

). By

definition

P(h)

is

independent

of EN which is determined

by J,j

with 1,

j #

o.

By

trie central limit theorem

P(h)

is Gaussian with parameters,

N

(h()~(Nj

"

fl~jJ0k (Ska)ce(Nj

k=1

(2.7a)

N

"

à~J0kfilÎÎ~~

" ~Î~~~>

k=1

~~~

(h~

~

h"~~~)

~

hC

b

OE(N)j

b

~

~(N)

~ fl~

~

~°kJ0£

jska

lllj~~~) jS~~

~OE(N)j

k,£=1

~ £b

N

OE(N)

Î ~ ~~~

'~~ÎÎ~~) (Skb m~)~~)

~~ ~~~

~~~ OE(N)

" Plôab qab] "

Pôab Ii ql'

The second

equality

in

equation (2.7b) (p

w

fl~J~)

follows from trie

clustering

property of

a pure state,

a(N),

and trie third

equality

is due to linear response in a

surgie valley

with

zero net

magnetization, equation (2.3).

In

equation (2.7b),

qab is trie Edwards-Anderson order parameter,

~ab

~

D2~~~~~Î~~~

~~ab> (~.~C)

i=1

which in a frozen state, with

equation (2.3),

must be

diagonal

in trie vector labels a, b.

To each

configuration

of trie

N-spin

system there exists p

configurations

of trie

(N +1) spin

system. Trie energy of trie

(N +1) spin

system is

EN+i

=

EN hasoa.

For fixed

EN+i,

h and

So

trie number of

configurations

is,

(h ha(Nj)

2

dN

(EN+i, h,

So " exp

-fifre(Nj

+

fIEN+i

+ h

So dEN+iDh. (2.8a)

21L(1

q)

IV

l)

with Db

=

~~~

~~ ~

db.

Integrating

over h and

summing

over So

gives, by definition,

27r

dN(EN+i

" exp

-flF~(

N+i) +

fIEN+i dEN+1, (2.8b)

with

Fa(

N+ij trie free energy of trie

(N

+

1)-spin

system,

FOE(N+i) =

Fa(N) ~(P l)(1 q) j1°g~exP (lll~~~e~j (2.8C)

1

To derive trie TAP

equations

for trie PG we use that

equation (2.8a) implies

that trie

probability

that trie

(N +1)

spin system bas a certain value So and field h

acting

on So is, for fixed

EN+1, j~

~oe(N) )2

~~~'~°~

~~~~

2p(1- q)

~

~°Î

~~'~~

(6)

N°7 THE CAVITY APPROACH FOR METASTABLE GLASSY STATES 781

with K a normalization constant. From finis

result,

trie average

magnetization

in trie state

a(N +1)

is,

(S0a)a(N+i~

OE

m()~~~~

#

~j /DhP(h, 50)S0a

~~~

~jeÎeXPÎh~~~~e~Î (2.10a)

~

i

~jexp[h~(~)e~]

'

1

and trie average

magnetic

field

is,

N

(h ~~ J~~~~~~~~~

~ °~~~~~

~~~

~~

(2.10b)

=

hÎ~~~

+

pli q)m()~~~~

To relate this to

previous

TAP work for trie PG (3] we use,

equations (2.4a)

and

(2.10a)

to

obtain,

h[(~l

=

£

e~

log il

+

e(m()~~~~j j2 lia)

p

~

~

In

deriving equation (2.lia)

trie

identity

[3]

exp

- £ log

~

~~~~~~~~~

=

£

exp[e~

h~(~) (2.

Il

b)

1 i'

i

was used. With

equations (2.10)

and

(2.Il)

we recover trie TAP

equations

used before. Al-

though

non needed in Section 3 trie

underlying

TAP free energy [3] is, suppress trie

o(N +1) index,

àFTAP

"

~(l

+

m,ae~)

ÎOg ~ ~~~~~

iiJ,>m,~m~~

ljp~

i~ji

~~~.

12.12~

1<j

These results reduce to trie free energy for trie usual SK mortel for p

= 2.

3. Fluctuations Due to

Many

Solutions: Self-Consistent

Equation

for qab

In this section we first quote trie known result for the number of

statistically

similar but incon- gruent metastable states in the PG above the true

equilibrium phase

transition temperature.

We then argue that this result is easy to understand and that it is

probably generic

for a class of

problems. Following

finis, we determine trie statistical properties of trie

magnetic

field which acts on trie

(N +1)

spin due to trie fact that trie

magnetizations

are

specified by

a

probability

measure and because there are many

statistically

similar metastable states.

Finally,

we use

these results to derive a self-consistent

equation

for trie Edwards-Anderson order parameter for trie PG. Trie final result is in agreement with trie

equation

of state derived

by

orner methods.

(7)

3.1. NUMBER OF METASTABLE STATES. In reference [4] ii was shown that for trie PG trie number of

statistically

similar metastable states in a

N-spin

system with free energy FN above the

equilibrium phase

transition temperature was extensive [3] and

given by,

dN(FN)

" ~~P

~~N ~~Î~

2àN ~~~ ~~~

~~~

(~'~~

=

exp[fIFN flF(]dFN.

Here

F(

is the canonical free energy in the

N-spm

system,

ÉN

is the component

averaged

free energy for

N-spins

and

AN

z~J

0(N)

is the variance in the

weighted

free energy distribution about

ÉN

Î15]. Note that the last term in the first

equality

in equation

(3.1)

is of relative

magnitude

zero unless FN

ÉN

z~J

0(N). Restricting

ourselves to states with free energy close to

ÉN,

we have the second

equality

in

equation (3.1).

In

general F( # ÉN

if there is an

extensive solution

degcneracy.

We next

interpret

equation

(3.1)

and argue it is

generic

for a Mass of

problems.

The systems

we have considered with ramdam first-order

phase

transitions have an extensive number of metastable states that are

statistically

similar but

incongruent.

In terms of

overlap

functions

(cf. below)

these states have zero

overlap. By

the central limit theorem this

implies

that

the

weighted

distribution of free energy states must be Gaussian. The

weighted

distribution

is defined

by examining

the

partition

function which is

given by

a sum over ail

statistically

similar states,

~N "

~

eXPÎ~~~OEÎ

"

/

d~N

~~j@~ eXPÎ~~~NÎ. (3.~)

~

N

Equations (3.1)

and

(3.2)

give a

weighted

free energy distribution

P(FN), P(FN)

z~J

~~~~~~

exp[-fIFNÎ, (3.3)

dFN

with an average free energy

ÉN

=

~f~exp[-flf~j /ZN

and a canonical free energy

flfjj

=

-logZN.

The

density

of states

given by

~ equation

(3.1)

is the unique

density

consistent with the above stated

requirements.

Finally,

we note that the cavity

approach

in the next subsection shows that

Fjj

does non

depend

on the

ordering

into the metastable

glassy

states. This has been

interpreted

else- where

[3,4, 7j.

The crucial point is that

dynamical

mean-field

theory predicts freezing

into a

metastable

glassy

state for T < TA because the extensive solution

degeneracy implies

that with

probability

one the initial

configuration

of the

N-spm

system will be in a

glassy

metastable

state. Because nucleation ont of a metastable state is

impossible

in a mean-field model it will

stay m a

particular

metastable state forever. In non-metastable models one expects

droplet

fluctuations to cause activated transitions to the lower free energy

paramagnetic

state and to other metastable

glassy

states (3j.

3.2. SITE FLUCTUATIONS DUE TO THE PRESENCE OF MANY STATES. We denote the

free energy states of the

N-spin

system

by

the label a

= 1, 2,.

,

M and the

corresponding magnetic

fields

acting

on the

(N +1)

spin

by (h~(/~1).

An average of our

observable,

0, over

solutions is defined

by [lj

1°)r(N)

"

ù É

1°)a(N) 13.4)

~=i

(8)

N°7 THE CAVITY APPROACH FOR METASTABLE GLASSY STATES 783

Note that this is an

unweighted

average because we bave

already

restricted ourselves to states with similar free

energies.

The solution

averaged magnetic

field at site 0

is,

N

/~o(N)) ~ jj

j

jy~~

/~r(N) j~

~)

~ r~~/~ °~ ~~ r(N) " a

k=1

By

definition the field

hÎ~~~

fluctuates

only

due to the random

(Jok).

For our case there are

many states

(M

+~

e/~)

that are ail

incongruent,

~ÎÎ ~Î ~Îa~$

~ ~°~

~

# ~' (3.~)

~

Denoting

the disorder average

by

],

equations (3.5)

and

(3.6) yield,

j/~r(N)j

~ ~

(3.7) [/~r(Nj/~r(Njj

~ ~ ~

or

equivalently, hÎ~~~

= 0. With equation

(3.5) this,

in tum, seems to

imply (mka)r(N)

" 0

(self-consistent

arguments

yield ((mka)r(N)(

z~J

N~~/~).

A similar result was used in our

previous

work on structural

glasses

[Si where the

analog

of Jok is non-random and the

only

average is over the solution

degeneracy.

The solution average of the square of the

magnetic

field at site 0 is,

(h[(/~)h)~~~)

= pqab =

pqôab. (3.8)

r(N)

Because the states are uncorrelated we can take

h]~~~

e hia to be a Gaussian random variable

with vanance

given by equation (3.8)

in an ensemble of

N-spin

states. The number of free

energy states with

N-partiales

with field hi

acting

on the

(N +1) spin

is,

dN(FN,

hi

" exp

(fIFN flF[ h( /2~1q) dFNDhi, (3.9)

jp 1j

with Dhi

=

(~~)

~ dhi The distribution m the variables

FN+i

and hi is

given by,

27r

~

j~ (FN+i,

hi

=

/dN(FN, h)à[FN+i

FN

àF(h)]

~+i

=

Dlli

exP

fl FN+i

flfi Ill/2Pq

+

iog ~llie~ 13.1°)

+i iv i)ii )1

~

where we have used equation

(2.8c)

with

h°(/~)

- hi

Integrating equatiou (3.10)

over hi must

yield,

~~l~N+1)

" ~XP

ÎfI~N+i fIFÎÙ+iÎ dFN+1 (3.lia)

(9)

From

equation (3.10)

we obtain,

~~N+1 ~7c/~

2fl

~

jp i)ji

q)

fl log /Dhexp [-hÎ/2~1q) ~je~~~~

1

(3.llb)

" ~Î~

~~~

~~

~°~~

As

already

mentioned, this result

implies

that the canonical free energy does not

depend

on trie

glassy ordering

characterized

by

q.

Equation (3.116)

is trie

expected

result for a

paramagnetic

PG if one takes into account that trie J's in

Fjj

~~ are normalized to

(N +1)~~,

while those in

Fjj

are normalized to N~~.

A self-consistent

equation

for trie Edwards-Anderson order parameter can be obtained

by noting

that equation

(3,10)

gives trie distribution of hi for fixed

FN+1~

P(h)Dh

= K exp

-

~~

+

log £

e~i~~

Dhi, (3.12)

~l~~

1

with K

being

a normalization constant. From equations

(2.10a), (2.

Il and

(3.12)

trie equation of state is,

/Dhima(hi )mb(hi

exp

-

~~

£ log

~

~~~~~~~~ )j

21Lq P

~ P

~~~ ~~~~

/Dhi

exp

(- £ log

~

~~~~~~~

~~ ~~~~

211q P

~ P

with

ma(hi given by,

hia

"

~j

e$

log

(1 +

e(mb(hi

)j

(3.13b)

P ~

Equations (3.13)

are closed

equations

for q and are m agreement with trie results from orner static and

dynamical approaches (3,4].

4. Discussion

In this paper we bave

provided

very

general

arguments for trie

origin

of

glassy

behavior in systems that

undergo

random first-order transitions. Dur results

emphasize

that trie slow

dy-

namics

resulting

in

glass-like

relaxation in a

myriad

of

seemingly

unrelated systems can be understood from one central concept. This crucial idea is

that,

whenever one bas a froc en- ergy

landscape

such that there are extensive numbers of basins of attraction

corresponding

to

(macroscopically) statistically

similar but

incongruent

metastable states, then trie system gen-

erates intrinsic randomness because one is forced to average over trie solution

degeneracy.

This situation can

naturally

arise even for Hamiltonians which do non

explicitly

contain

quenched

random interactions. Trie

glassy

behavior results from this

self-generated

randomness. Dur arguments bave been buttressed

using

trie Potts

glass

as a concrete

example.

However trie

similarity

of trie results with our

previous

work

involving

model fluid Hamiltonians [Si that do not

explicitly

contain any randomness shows that trie

conceptual

aspects of our work should be

applicable

to a wide

variety

of systems. We also note that similar argument can be used to

obtain

analogous

results for trie J~-spin

glass

model

(16j.

(10)

N°7 THE CAVITY APPROACH FOR METASTABLE GLASSY STATES 785

These ideas can be used to understand trie recent novel work

(8-loi by several'groups

who bave discovered that

glassy

behavior can be observed even in model Hamiltonians that do not contain

explicitly

contain

quenched

disorder. In ail these cases trie systems gel frozen into

one of trie

possible

metastable states below a characteristic temperature. In reference

iii]

an

explicit computation

of trie solution

degeneracy

for one of these niodels bas been

done,

and

a

dynamical phase

transition bas been related to trie emergence of an extensive number of

statistically

similar states.

A crucial

point

that is worth

making

is that ail our results follow from trie Gaussian distri- bution of free

energies.

This is to be contrasted with trie SK

model,

where trie free

energies

are

exponentially

distributed below a threshold value

[18j.

Thus unlike trie SK

model,

alI trie consequences of trie law of

large

numbers are valid in our case. It is

perhaps

for this reason that trie behavior we bave discovered niay be

generic

for a

variety

of classical disordered systems.

Furthermore,

it appears natural that these concepts con be used to

provide

a framework for

understanding dynamical

behavior in structural

glasses (19j.

It is also important to

emphasize

that trie

major

consequences

resulting

from solution de- generacy do non require trie

replica analysis.

In

fact,

trie

only

relevant order parameter in trie temperature range TK < T < TA is trie self

overlap

between trie

replicas, narnely

trie

dynarni-

cal Edwards-Anderson order parameter.

This,

agam, is in contrast with trie much studied SK model in which there is no

analogue

ofTA

Description

of trie

spin glass phase

in trie SK model

requires

trie fuit broken

replica

symmetry treatment.

Further

insight

into trie nature of trie states m trie range TK < T < TA may be obtained

by mferring

trie barrier

height separating

two states. From

equation (3.1)

it is obvions

(3,7j

that trie free

energies separating

any states o and

fl typically

dilfer

by @.

Trie free energy of

activation between two genenc metastable states may be estimated as follows. Elsewhere [20j

we showed that, at least close to

TK,

trie activation borner àF* scales as, [20]

àF*

+~

t~~"~. (4.1)

In finite range

models,

there exists a natural finite size correlation

length, (

+~

t~". In a correlation volume, trie number of spms N scales

(~. Making

these substitutions in

equation (4.1)

gives

àF*

+~

N~/"~ (4.2)

For random first-order transitions, du = 2

Id,

which

implies

that àF*

+~

@,

1-e-, trie barrier between states is

comparable

to their dilference in free energy. In trie usual SK model àF* is

estimated (21] to scale as

N~H.

Trie

same arguments bave been used

recently

to estimate lime scales for

folding

of

proteins

[22] which are

mesoscopic.

Trie success of finis

application

further

underscores trie

ubiquity

of

complex

energy

Iandscapes

m a wide vanety of systems.

Acknowledgments

This work was

supported by

trie National Science Foundation under grant numbers DMR-92- l7496 and CH&93-07884.

(11)

References

iii

Onsager L., J. Am. Ghem. Soc. 58

(1936)

1486.

[2] Mézard M., Parisi G. and Virasaro M., Europhys. Lent. 1

(1986)

77; Mézard M., Parisi G. and Virasaro M.A., Spin Glass Theory and Beyond

(World

Scientific, Singapore, 1987) p. 65.

[3] Kirkpatrick T.R. and Wolynes P-G-, Phys. Rev. B 36 (1987) 8552.

[4] Thirumalai D. and Kirkpatrick T.R., Phys. Rev. B 38

(1988)

4881.

[5] Kirkpatrick T.R. and Thirumalai D., J. Phys. A 22

(1989)

L149.

[6] Huse D.A. and Fisher D.S., J. Phys. A 20

(1997)

L997.

[7] Kirkpatrick T.R. and Thirumalai D., Phys. Rev. A 37

(1988)

4439.

[8] Chandra P., Coleman P. and Ritchey I., J. Phys. 13

(1993)

591.

[9] Kisker J., Rieger H. and Schreckenberg M., J. Phys. A 27 (1994) L853.

[10] Bouchaud J-P- and Mézard M., J. Phys. I France 4

(1994)

1109.

[Il]

Franz S. and Hertz J., Phys. Rev. Lent. 74 (1995) 2114.

[12] Baldassari A., Gugliandolo L.F., Kurchan J. and Parisi G., preprint

(1994).

[13] Elderfield D. and Sherrington D., J. Phys. G16

(1983)

873.

[14] A review of regular Potts models can be found in: Wu F-Y-, Rev. Mod. Phys. 54

(1982)

235.

[15] For a discussion of the various free energies that anse m system with many macroscopic states, consult: Palmer R-G-, Adv. Phys. 31

(1985)

6691.

[16] Kirkpatrick T.R. and Thirumalai D., Phys. Rev. Lent. 58 (1987) 2091; Phys. Rev. B 36

(1987)

5388. See aise, Rieger H., Phys. Rev. B 46

(1992)

14665.

[17] Parisi G. and Potters M., preprint

(Cond.

Mat.

9503009).

[18] Mézard M., Parisi G. and Virasaro M.A., J. Phys. Lent. 46 (1985) L217.

[19] Kirkpatrick T.R. and Thirumalai D., to be published.

[20] Kirkpatrick T.R., Thirumalai D. and Wolynes P-G-, Phys. Rev. A 40

(1989)

1045.

[21] McKenzie N-D- and Young A.P., Phys. Rev. Lent. 49

(1982)

301.

[22] Thirumalai D., preprint

(1995).

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