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Constrained Annealing for Spin Glasses

Giovanni Paladin, Michele Pasquini, Maurizio Serva

To cite this version:

Giovanni Paladin, Michele Pasquini, Maurizio Serva. Constrained Annealing for Spin Glasses. Journal

de Physique I, EDP Sciences, 1995, 5 (3), pp.337-354. �10.1051/jp1:1995130�. �jpa-00247059�

(2)

Classification Physics Abstracts

05.50 02.50 75.10N

Constrained AnneaEng for Spin Glasses

Giovanni

Paladin(~),

Michele

Pasquini(1)

and Maurizio

Serva(2)

(~) Dipartimento di Fisica, Università dell'Aquila, 1-67100 Coppito, L'Aquila, Italy (~) Dipartimento di Matematica, Università dell'Aquùa, 1-67100 Coppito, L'Aquila, Italy

(Received

3 October 1994, accepted 29 November 1994)

Abstract. The quenched free energy of spin glasses con be estimated by means of annealed averages where the frustration or other self-averaging variables of disorder are constrained to their average value. We discuss the case of d-dimensional Ising mortels with random nearest

neighbour coupling, and for +J spin glasses we introduce a new method to obtain constrained annealed averages without recurring to Lagrange multipliers- It requires to perform quenched

averages either

on small volumes in

an analytic way, or on finite size strips via products of random transfer matrices. We thus give a sequence of converging lower bounds for the quenched

free energy of 2d spm glasses-

l. Introduction

Disordered systems are made of random variables which relax to

equilibrium

on very diiferent time scales. For instance in the standard models of

spin glass,

the spins arrange themselves

to minimize the free energy while the random

couplings

are assumed to be frozen in their initial

values,

since their evolution time is much

longer.

As a consequence, one should consider diiferent kinds of averages:

quenched

averages for the frozen

variables,

and annealed averages for the fast variables.

However,

it,is much easier to compute annealed averages, which

#ve

lower bounds of the

quenched

free energy, the

physically

relevant

quantity.

These bounds

are often very poor

estimates,

since in annealed averages the main contribution comes from a set of disorder realizations which bave zero

probability

in trie

thermodynarniclimit.

In those

realizations,

trie

quenched

random variables are

arranged

in order to minimize trie free energy, at diiference with a

typical sample

of trie system where

they

are frozen in a

given

realization.

Trie idea of constrained

annealing

is to

perform

annealed averages where trie random vari- ables are

partly

frozen

by

trie requirement of

satisfying appropriate

constraints, related to some

disorder

self-avera#ng

variables. Trie standard way to

impose

a constraint is

by

a

Lagrange multiplier. By

that

method,

trie constrained annealed average allows one to introduce a sort of Gibbs

thermodynamic potential, depending

on trie temperature and on trie

Lagrange

mul-

tipliers

which

play

the role of trie chernical

potential

in

ordinary

statistical mechanics [1]. In the

thermodynamic

limit, the values of the

multipliers

that maximize the Gibbs

potential

are

those ones that select the realizations with a correct value of the disorder intensive

variables,

@ Les Editions de Physique 1995

(3)

and,

at trie same

time,

that minimize the diiference between trie mean free energy

density

and its annealed

approximations.

Constrained

annealing

for disordered systems bas been

proposed

and

applied

in

particular

contexts

by

many authors

(see [2-6]).

A

general

formulation of trie method and its

physical

meaning

can be found in [1].

Trie purpose of this paper is to show that it is

possible

to

perform

constrained annealed averages without

Lagrange multipliers,

m d-dimensional

spin glasses

with dichotomic random

couplings

in terms of a

quenched

average over a finite size

sub-system.

This is often

possible

either m an

analytic

or m a numeric way.

Using

our

method,

we are able to obtain very

good

lower bounds of trie

quenched

free energy of two dimensional spin

glasses.

Trie summary of trie paper is trie

following:

In section 2, we recall some basic facts about spm

glasses.

We also

classify

the set of trie constraints necessary to recover trie

quenched

free energy

by

annealed averages. In section 3,

we

study

trie

Ising

model with

couplings

which con assume trie values J~j = +1 with

equal probability (the

sc-called +J spin

glass).

In section 4, we introduce our method to obtain

constrained annealed averages without

recurring

to

Lagrange multipliers

in trie +J spin

glass.

In section 5, we

apply

trie method to

loops

of infinite

length using

trie

Lyapunov

exponent of

product

of random transfer matrices. We are thus able to get accurate estimates of trie free

energy in two dimensions.

2. Constraints for d-Dimensional

Spin

Glasses

Spin glasses

are trie

challenge

of constrained

annealing.

In that case, trie relevant variables to be constrained should be related to frustration [7], as first remarked

by

Toulouse and Vannimenus in 1976 [5]. As far as we

know,

there are

only

Montecarlo

simulations,

see e.g.

[8,9],

which used

that idea while no

analytic

calculations bave been

performed

on that

ground.

However, it is

possible

to get

analytic

results m dimension d > 2 with constraints connected to frustration.

Let us consider d-dimensional

Ising

models with nearest

neighbour couplings

J~j which are

independent identically

distributed

(1.i.d.)

random

variables,

in absence of externat

magnetic

field. Trie

partition

function is

zN

=

~ fl expjpJ~jaiajj (2.1)

lai i J

where trie

product

runs

over1, j

which are nearest

neighbours. Using

standard relations of trie

hyperbohc functions, (2.1)

becomes

ZN "

~ fl cosh(flJ~j) il

+ a~aj

tanin(flJ~j) (2.2)

lai '>J

This form is useful since shows that trie non-trivial part of trie partition function is

given by

fl,

~

il

+ a~aj

tanin(flJ~j

)]. A

typical

term m that

product

is a~ajaj ai

tanin(flJ,j tanin(flJji)

where trie bonds

(1, j ), ( j,1)

can form either a closed or an open line on trie lattice. If trie bonds form an open

line,

at least two distinct spin variables survive as factor of trie

product

of the various

tanh(flJ,j ),

and the related term

gives

a zero contribution to the partition function,

after

jerformmg

the sum over the a

configurations.

As a consequence, one bas to consider

only

trie terms

corresponding

to bonds which form a closed fine

(where

trie

product

of trie a's is

equal

to

unity

smce

they

appear

twice)

so that

(2.2)

con be written as a sum over all trie

possible loops

LÎ~~, where T > 4 indicates trie

length

of trie

loop

(T bas to be

even)

and s labels

(4)

diiferent

loops

with the same

length:

ZN

"

eÉ.,>

~" ~°~~~~"~

2'~

l

+

~j fl tanh(flJ,j) (2.3)

lL[~>j j~,jjeL[~>

It follows that in a system with a finite number N of

spins,

the free energy of a disorder realization is

given by

y~ = in z~ = B +

fl~ (t(4)

~(Rj ~~

~)

flN fl

' '

where R is the maximum

possible length

of a

loop

in the system

(R

< const

N),

and

B = In 2 +

~j

In

cosh(flJ~j (2.4a)

~

>,J

and

~~~~~~~' '~~~~~

Î

~~

~

~

~Î~~

(2.4b)

jL[~>j This function

depends

on the new set of variables

t(~) =

fl tanh(flJ~j) (2.4c)

j~ ~j~~(r>

given by products

which run on the

loops

LÎ~~, 1-e-

plaquettes

of

larger

and

larger perimeter

at

increasing

T. For instance, the

loop

L(~) is the

elementary plaquette

of four bonds. Let us

stress that a

loop

L(~) can be built up as a set of two

(or more)

distinct and separate

loops

L(~'l

and L(~2) with

Ti + T2 " T. In the

following

we often label a

coupling by only

one label

mstead of two ones, 1.e. Jki is denoted

by Jk,

since there is no risk of

ambiguity

on a closed line.

As the number of the nearest

neighbour couplmgs

in a

hypercubic

d-dimensional lattice is dN, in the

thermodynamic

limit the

quenched

free energy reads

f

e lim @ " d In

cosh(flJ~j

+ F + In 2

(2.5)

N-CC

fl

where

F = lim

j lui

1

+

~j

tÎ~~

(2.6)

~~~°

j~(r>j

The reduction of the

partition

function

(2.1)

into

(2.3)

is the

procedure

used in the Kac and Ward solution of the 2d

Ising

model without disorder.

Equation (2.5)

is fundamental since it shows that the

quenched

free energy

depends only

on the distributions of the variables

t(~),

apart the mean value In

cosh(flJ,j).

The relevant variables to be fixed to their ~r~ean value m a constrained annealed average of the free energy

are

related,

with

increasing difliculty 1)

In cosh

flJ~j

2) t(~l

=

tanh(flJi) tanh(flJ2) tanh(flJ3) tanh(flJ4)

3)

t~~l with T > 6

(considering only

connected

loops).

(5)

Fixint

all the constraints

corresponding

to those

quantities

in an annealed average is

equiv-

alent to solve the system with

quenched

disorder. This can be understood

noting

that in

(2.6)

we have a sum over ail the

possible

tÎ~~. Because of the law of the

large

numbers the rescaled

sum of the t-variables

corresponding

to the same

topological

kind of

loops self-averages

to its

quenched

mean value.

Moreover,

in the

appendix

we shall prove that this result holds even in a finite volume system for a +J

spin glass:

the

quenched

free energy can be obtained

by

a minimization of the

logarithm

of the annealed average of a

Grand-partition

function with respect to the

Lagrange multipliers

related to the variables tÎ~~ over ail the

possible loops

of the finite system. For a

generic

distribution of the

couplings,

an extension of this statement is

possible.

In one dimension there are no

loops,

so that the constraint related to

point 1)

is suflicient to obtain the exact solution. In

general,

we expect that many

physical

features of a

spin glass

can be

reproduced already by considering

the first two

points.

The case of random

couplings

J~j = +1 with

equal probability

is

particularly simple

in this respect, since the variable In cosh

flJ,j

is a constant and thus can be

ignored. Moreover,

one

immediately

sees that

(2.4c)

becomes

t(~) =

tanh~(fl) fl

J~j

(2.7)

j, jj~ ~(r>

implying

that the

quenched

free energy

only depends

on the values of the

product

of

J,j

on

closed fines of bonds. The non trivial part of the free energy yN m

(2.4)

is thus

FN

"

ln(1

+ x4

tanh~ là)

+ x6

tanh~(fl)

+ .)

(2.8)

N

where the coefficients

(x4,

x6;.

)

are

non-mdependent

random

quantities.

As a consequence, the

quenched

free energy is

f

=

fl (d

In cosh

fl

+ In 2 + limN-no éÎ

ln(1

+ x4

tanh~ (pi

+ x6

tanh~ (fl)

+

(2.9)

In the annealed model, the last non-trivial term of

(2.9)

vanishes since n

= o for ail i's

(each

x, is a sum of

products

of

independent

random

couphngs).

In the limit of

high

temperature

-

o),

the diiference between annealed free energy and

quenched

free energy thus is of order

tanh~ fl

~J

fl4.

More

important,

the

simplest

relevant constraint in the +J

spin glass

is the frustration

Jp

on the

elementary

square

plaquette

of four

couphngs Ji, J2, J3, J4,

that is

Jp

= -JiJ2J3J4

(2.lo)

since t(~)

=

-Jp tanh~ fl.

3. +J

Spin

Glasses

In this section we consider a d-dimensional spin

glass

with 1.i.d. nearest

neighbour couplings

which assume two

possible

value

J,j

= +1 with

equal probability.

From

(2.9),

one sees that the annealed free energy

density

is

(6)

In one

dimension,

there are no

loops

and

fa

is

equal

to the

quenched

free energy

density f,

since In

coshflJ,j

is a constant, at diiference with the Gaussian case where that variable is random and has to be constrained in order to recover

f [loi.

In section

2,

we have recalled standard results which show that it is necessary to constrain variables associated to the

loop

variable

t(~),

in order to

improve (3.1).

As first noted

by

Toulouse and Vannimenus [Si, one

has to consider the intensive variable

a~r=

j j (

13.2) j~j,>j

which has zero mean

value,

Wi " o. Let us remark that it is a

self-averaging quantity,

that is

limN-co

ON

" o for almost ail disorder realizations. The related constrained annealed average

con be

regarded

as the

Grand-partition

function

iiN(à>

ÎL) ~

ZN

e~'~""N

In the

thermodynamic

limit the

Lagrange multiplier

p that maximizes

~~~'~~

ÀÎCO flÎÎ

~~ ~~

~'~~

fixes the frustration on square

plaquettes

to its mean value. Moreover it is

simple

to show the

foiiowing inequality:

f

~

Ill

~ ~°~~

girl, PI

In our case, we have to compute

QN(fl, Al

"

~exp(~j flJ,ja,aj ~j pJp) (3.3)

(a) i,j j

~l')j

Taking

into account that the

coupiings

are dichotomic with

equal probabiiity,

one con

perform

the gauge transformation J~j -

Jjja~aj

which leaves

unchanged

the free energy of a disorder realization of the system as well as

Jp,

1-e-

Jp

-

Jp.

As a consequence,

(3.3)

becomes

iiN(à,

ÎL)

"

~~ eXp(~ flÀj ~ pJp) (3.4)

1,j

j~l')j

This expression

(which

is

meaningful

for any dimension d >

2)

cannot be

computed exactly including

all the

possible

square

plaquettes

LÎ~I of the d-dimensional lattice. It can be shown that the

problem

is

equivalent

to solve a d-dimensional gauge model without

disorder,

whose

solution is not known for d > 2.

However, an exact solution can be achieved if we restrict the sum

(3.4) only

on a part

(of

order

N)

of the

plaquettes.

In other terms the constraint is

imposed

over a fraction of the

plaquettes,

that is we are able to

partially

fix the

plaquette

frustration to its mean value.

As a consequence, the annealed system exhibits a "residual" frustration related to the non- constrained

plaquettes.

Let us consider the 2d model. It is convenient to limit ourselves to consider one half of the

plaquettes,

which must be chosen in such a way that

they

do not share any

coupling,

as it

happens

for the black squares of a chessboard. With this restriction

(3.4)

contains a sum over

(7)

-1

_j .-.-.-.-.-.-.-. d=2

j=±1

~=--,

f'~ /~

i /

~ /

Î

~ /

/ /

/ f sq

Î / f~~

~

/ f cr

ac

0 0.5 1-5 2

Fig. 1. +J spin glass m 2d: the annealed free energy fa

(dashed

fine) and the constrained free ener- gies fil

(fuit

fine) and fil

(dot-dashed

fine) versus temperature T

=

1là.

The constraints

are imposed, respectively, on

N/2

independent plaquettes and on

N/8

independent crosses of rive plaquettes.

products

of

N/2 independent

variables

(corresponding

to trie

N/2

black

plaquettes)

and trie

Grand-partition

function can be rewritten as:

QN

(à)

"

2'~ (exp(fl(Ji

+ J2 +

J3

+

J4)

+

pJi J2J3J4 ))

~~~

(3.5)

where Ji

,

J2

,

J3

,

J4 are trie

couplings

of one of trie

plaquettes.

After

maximizing

with respect

to p trie Gibbs

potential

[1], one obtains

f])

= In 2 + In cosh

2fl

+

In(

3 +

cosh4fl ) (3.6)

fl

2 4 4

The functions

fa

and

fil

of trie 2d spin

glass

are shown in

Figure

1. At diiference with trie annealed case trie entropy of trie constrained annealed system never becomes

negative.

We bave thus obtained a real

qualitative

improvement.

It is also

interesting

to consider trie heat capacity C which can be

explicitly computed.

For

fl

- co one has

C

~J

fl~e~~P (3.7)

The argument of the

exponential

has been

conjectured

in

Ill]

for the

quenched

model and it is diiferent from the exact one-dimension result where the argument is

-2fl.

Note that the

annealed system also

gives

C

~J

exp(-2fl).

Finally,

since we have fixed

only

one half of the

single plaquette frustration,

it is reasonable to ask what is the residual frustration #a~ Since the black

plaquettes

have zero

frustration,

this

quantity

will be one half of the frustration of a white

plaquette.

The four

couphngs forming

a white

plaquette

are

independent

smce

they

are not

coupled by

the

Lagrange multiplier.

Therefore, the white

plaquette

frustration can be written as « /

»~,

and the

global

frustration #a~ reads:

#a~ = ~ « Jj

»~ (3.8)

2

(8)

/ / /

/

~

'( o.

(

/

j

É j j]1

/

/

~

/ 0

ig. . -

+J pin

lass

for the mortel. The

constraint is imposed on N/2

plaquettes.

where « . » is an verage on the Gibbs measure associated

(3-3).

One ~ ~~~ ~~ ~~~

~~

~ ~~ ~

2~ôÎ~ ~'~~

where p* is

alue

which

aximizes

total umber of ouplings is 2N. Since ri(4) " 9(4,

Îl~(4)1

and

since

the

derivative

Using the xpression (3.6) for fil we

can

compute the residual

~~~

~ Î

~~

~ ~~~ ~ Î Î~~~Î~~ ~ 4 ~ÎÎÎ~Î2fI)1~

At

ture #a~ =

3~ o.158.

This

esult

indicates trie

non vanishing residual

frustration.

An alogous

xpression can be found from trie

annealed

free

energy

fa. In this

case ail

plaquettes can bave negative rustration and

#a =

-

« Ji »~ =

-th~(fl)

(3.12) here

trie is in

trie

Gibbs

measure

generated

#a(T = o) = -1 since at zero temperature triespins are aligned and trie

is

Both #a and #a~ are reported in Figure 2.

Trie

fact that in

trie

constrained annealed

model trie residual rustration does

not

anish indicates that trie

free energy estimate could be improved by further

constraints

as we shall

discuss section.

(9)

4. Constraints without

Lagrange Multipliers

As far as we

know,

up to now constrained

annealing

bas been

performed only using Lagrange multipliers.

This is a strong

limitation,

since in most cases it is too diflicult to derive

analitically

an annealed average

using

more than one constraint. Trie

spin glass

with dichotomic

couplings

bas some

algebraic

features which

permit

us to introduce an alternative

method,

in order to obtain constrained annealed averages

avoiding

in this way trie

problem

of trie minimization of trie

Lagrange multipliers.

Let us consider a d-dimensional lattice of N points: trie total number of trie

couplings

is

dN,

but trie system can be

fully

described

by

a lower number of

independent

random variables. In fact trie non-trivial part of trie

quenched

free energy

(2.6)

is a function of trie variables (tÎ~~

),

see

(2.4c)

,

defined on trie closed

loops

of trie lattice.

Indeed,

from a

topological point

of view any closed

loop

LÎ~~ can be

thought

as trie union of some

elementary

square

plaquettes,

say a

number

k,

so that trie related variable

tl~l

can be written as:

k

t(~) =

tanh~(fl) fl

J)~)

(4.1)

1=1

where we bave introduced trie frustrations

Jp

=

fl)~~

J, = +1 with

equal probability

of trie k

plaquettes (trie

index1 runs over trie four sites of each

square).

Let us stress that a

loop

can

be either connected or

disconnected,

1-e- it is not necessary that trie

plaquettes

are

neighbours.

Notice that trie

plaquette

frustration was

previously

defined with a minus

sign (sec (2.lo)),

but

in this context we

neglect

it to

simplify

trie notation.

Moreover,

we dot not assume

periodic

boundary

conditions in this section.

In other terms, we con consider trie

plaquette

frustrations as trie random variables of trie system, instead of trie

coùphngs,

with no loss of

generality.

We shall see that trie number of

frustrations necessary for a fuit

description

of trie system is

always

lower than

dN,

trie total number of

couplings.

For instance, in

2d,

there are 2N

couplings,

while trie number of

plaquette

frustrations is of order N when N - co.

However,

trie 2d case exhibits a

special feature,

since ail trie

possible plaquette

frustrations turn out to be a set of

independent

random variables

([et

us recall that we do not assume

periodic boundary condition).

In trie

general

case d > 3, this statement is no

longer

valid.

Indeed,

[et us consider a cube in a d-dimensionai iattice: a moment of reflection shows that trie

product

of trie reiated six

plaquette

frustrations bas to be 1, so that

only

rive frustrations are

mdependent

random variables. As a consequence, for d > 3 trie

change

of random variables from trie

couplings

to trie

plaquette

frustrations invoives

oniy

a subset of

them,

[et us say

N*,

chosen in such a way that

they

are

independent

random variables and that

they

can build up every

possible

closed

loop

on trie lattice.

Let us illustrate this

change

of random variables for a 3d lattice of N

points,

where we can introduce three

integer

coordinates

(x,y, z).

A square

plaquette

has three diiferent orienta- tions,

belonging

to a x = const

plane,

or y

= const, or z = const. In the

thermodynamic

limit

one has

Nl/~ planes

for each orientation, and each

plane

is a set of

N~/~ plaquettes,

for a total number of 3N

plaquettes

in the whole lattice.

Consider a cube of six

plaquettes,

with one of them on the z

= o

plane.

As

previously discussed,

one of the J's cannot

belong

to the subset of

plaquette

frustrations that describe trie whole system, [et us say trie

Îrustration

of trie

plaquette

on trie z = 1

plane.

Let us

now consider trie other cube

sharing

this

"neglected" plaquette. By introducing

as random variables of the system the frustrations which are related to the four

plaquettes

that share a

coupling

with the

plaquette

on the z

= 1

plane,

we have to

neglect

the sixth frustration of the

(10)

plaquette

on the z

= 2

plane,

since the

product

of ail the

plaquette

frustrations of these two

nearest

neighbour

cubes is fixed to

(the

presence of the

plaquette

on z

= 1 in trie

product

is

irrelevant,

since it appears

twice).

These arguments con be

easily repeated,

so that trie subset of

plaquette

frustrations that

fully

describes trie whole system can be found as follows: one bas to consider two distinct orientations and to take into account ail trie

plaquettes

with these

orientations,

for a total number of 2N.

Moreover,

trie third orientation

gives only

a

plane

of

N~/~ plaquettes (trie

z

= o

plane

in our

example),

so that in the

thermodynamic

limit trie number of

independent

random frustrations N* that

fully

describe trie systems grows as 2N.

Trie

generalization

of this result is immediate: in trie

thermodynamic

limit trie d-dimensional lattice of N points

(with

d >

3)

is built up

by

N distinct

plaquettes,

since is trie number of diiferent orientations for a

plane

m trie

lattice,

but

only

a number N*

= 2N

of

plaquette

frustrations is necessary to describe trie system. In fact trie

change

of random variables involves

only

the frustrations of the

plaquettes

with two well-defined orientations

(2N plaquettes), together

with a

plane

of

plaquettes

for each one of trie other

orientations,

but

m trie

thermodynamic

limit trie main contribution to N* comes from trie former term.

Using

this subset of

plaquettes,

whose related frustrations are all

independent

random

variables,

it

is

possible

to build up every

possible

closed

loop

on trie d-dimensional lattice.

In conclusion the described

change

of variables

permits

us to reduce trie number of

indepen-

dent random variables necessary to describe trie system, from dN

couplings

to N*

frustrations,

with N*

= N for d

= 2 or N*

= 2N for d > 3. In trie

following,

if not

diiferently specified,

trie term "frustration"

always

indicates one of trie N* random variables of trie system.

Recalling (4.1),

equation

(2-6)

becomes:

N*

F = lim

In[1

+

~j ~j $"~ $'~~ tanh~~'" '"k)(fl)] (4.2)

~~~° ~

k=i i,.. i~

where one considers all trie

products

of k E

Il, N*] elementary plaquettes (trie

indices ii

~

12

~ ~

ik run from 1 to

N*)

and

T(ii,

,

ik)

is trie

length

of trie

loop

built up

by

trie k

plaquettes,

while trie overline represents now trie average over trie frustrations.

In trie

following paragraph,

we consider trie

plaquettes

of trie lattice

only

from a

topolo#cal point

of view, 1.e., trie fact that a frustration of a

plaquette

is a random variable of trie system

(or not)

is irrelevant. At this

point,

we

perform

a

decomposition

of trie set of

plaquettes

into subsets such that each

coupling J,j belongs

to one and

only

one of these subsets. It follows that two distinct subsets can bave in common

only

isolated lattice

points.

For instance, three diiferent

decompositions

of trie bonds of a 2d lattice

(trie

black

regions)

are illustrated in

Figure

3. It is worth

stressing that,

after the

decomposition,

we get a collection of

sub-systems

which

do not cover trie whole

original lattice,

e.g. in

Figure

3a

only

one half of the 2d lattice is

covered. This kind of

decomposition

divides trie

plaquettes

into two classes: trie "black" ones, which are

organized

in groups

correspoiiding

to trie

sub-systems (e.g.

trie crosses in

Fig. 3b),

and trie "white" ones, which do not

belong

to any

sub-system-

Coming

back to trie

frustrations,

note that in

general

there are many "white" or "black"

plaquettes

whose frustration is not a random variable of the system.

At this

point

we can derive an upper estimate Fa~ of the function

(4.2), by treating

ail the random variables of frustration associated to the "white"

plaquettes

as annealed

variables,

1.e.

by averaging

over these variables

only

trie argument of trie

logarithm

m

(4.2),

instead of the

(11)

ai

hi

Cl

Fig. 3- Ising mortel with nearest neighbour interactions on a 2d lattice: decompositions of the set of the couplings in independent subsets

(the

black

areas): a)

squares,

b)

crosses and c) elongated crosses.

logarithm

itself:

~~ lôj

Fa~ = lim

ln[1

+

~j ~j 1"~ l'~~~'~~ tanh~~'" "~)(fl)] (4.3)

~~~° ~

k=i i, i~

where R~'°) and R~~) represent trie averages over trie frustrations related to,

respectively,

trie "white" and the "black" squares. In

(4.3) only

the terms

l~~~ l'~~

with all "black"

frustrations do not vanish after

performmg

the "white" average:

p~~

(b)

Fa~ = lim

jIn[1

+

~j ~j l~~~ l~~~ tanh~~~'

~~)

(fl)] (4.4)

~~~°

k=i ii. .>k

where now trie indices ii, .,ik run

only

over trie N~ "black" frustrations. It should be re- marked that after

performmg

trie "white" average, trie

surviving loops

do not connect diiferent

sub-systems.

In other terms, any

loop appearing

in trie average

(4.4)

can be

decomposed

into a set of

"sub-loops",

each of them limited to a

single sub-system.

This

implies

that tanh~~~i> >~k~(fl) con be

factorized,

1-e-,

T(ii,

.,

ik)

is trie sum of trie

lengths

of trie vanous

"sub-loops".

As a consequence, trie whole argument of trie

logarithm

m

(4.4)

is factorized

(12)

among ail trie

sub-systems,

and it

immediately

follows:

Fa~ =

~

In

il

+

~j ~j l~~~ l~~~ tanh~~~"""~~)(fl)] (4.5)

'lJ

Îi

i~ ~~

where trie average is

performed

over trie np "black"

plaquette

frustrations that

belong

to a

single sub-system,

and where nj is trie number of

couplings

in trie

sub-system,

so that

é

represents trie total number of

sub-systems,

rescaled with N in trie

thermodynamic limil.

Recalling (2.5),

from

(4.5)

trie lower estimate

fa~

of trie

quenched

free energy

yields:

fl fa~

= d In

cosh(fl)

+ ~

ln[1

+

~j ~ l~'~ l~~~ tanh~~'i'

""k)

(fl)]

+ lu 2

(4.6)

"J

~i

1, .>~

It is

preferable

to choose a

topolo#cal decomposition

of trie system such that trie np "black"

frustrations

fully

describe trie

single sub-system.

In this context Fa~ is

practically equivalent

to the

quenched

free energy of the

sub-system,

a part a factor

proportional

to In cosh

fl.

If np

is not too

large,

the

computation

of Fa~ can be

performed analitically

or

numerically.

Trie correct

multiplicative

factors to transform trie

quenched

free energy of a

sub-system

to

trie

global

constrained free energy

(4.6)

can also be obtained

by

a

simple

argument. Indeed trie

partition

function Z~z~ of a

sub-system

made of ns

spins

and nj

couplings

is trie sum of 2'~S

terms which are given

by

trie

product

of nj

exponentials

while trie

global

constrained Grand-

partition

function

QN

of a system with N

spins

and dN

couplings

is trie sum of 2'~ terms which are given

by

trie

product

of dN

exponentials.

In order to compare two

quantities

of

order one, one bas to write trie

followmg equality:

2~~ilN )~/~~~~

= 2~"~

z»~ )~/"'

so that

1 ~ ns

(4

7)

/

=

--(1-

d

")

ln2 + d

-fsub

~~

fl

"J "J

This formula is

completely equivalent

to

(4.6),

but bas trie

davantage

that trie

quenched

free energy

fsu~

of trie

sub-system explicitly

appears. Trie

ground

state energy can be estimated

by

trie saddle

point

method when

fl

- co m trie

quenched

average of Zn~

Ea~(T

=

o)

= ~ max

H((J)) (4.8)

nj j«j

where trie maximum is taken over ail trie a

configurations

for each disorder realization. One

can also obtains trie residual entropy as

Sa~(T

=

o)

=

(1 ~d)

In 2 + In

deg((J)) (4.9)

"J

where

deg((J))

is trie number of disorder

configurations

which bave energy

H((J)) equal

to

Ea~(T

=

o).

Let us

briefly

resume trie

discussion,

m order to

clarify

trie

meaning

of trie result.

Using

a

topological decomposition

of trie system into

independent sub-systems,

we bave derived a lower estimate of trie

quenched

free energy that

depends

from trie

quenched

free energy of trie

single sub-system.

As discussed in trie

appendix,

trie

quenched

free energy of a

sub-system

can be obtained

by

a minimization of an annealed average of trie

Grand-partition

function

(13)

with

Lagrange multipliers

over ail its

possible loops. Using

our

procedure,

we are able to get trie annealed average

fa~

of trie

global

system where trie constraints are

imposed

over ail trie

possible

rescaled sums of frustration on ail trie

loops

that appear in trie various

sub-systems.

To illustrate our

method,

we

apply

it in trie case of Section 3, 1-e- trie

decomposition

of a

2d

spin glass

in "white" and "black" square

plaquettes,

like in a

chessboard,

see

Figure

3a.

In this case ail trie N

plaquette

frustrations represent a set of

independent

random

variables,

i e. N* = N. One half of them is related to "white"

plaquettes,

so that

they

are treated as annealed

variables,

while trie other half related to "black"

plaquettes

as

quenched

variables.

We also bave nj = 4 and np = 1, so that

(4.6)

becomes:

fl f])

= 2 In

cosh(fl)

+

ln[1 tanh~(fl)]

+ In 2

(4.lo)

It is easy to check that after trivial

algebraic manipulations

one gets

again (3.6).

Trie

ground

state energy and trie zero temperature entropy can be

directly computed

from

(4.lo),

and

respectively

are:

E])(T

=

o)

= -1.5

S])(T

=

o)

= o

(4.Il)

The method of constrained annealed averages without

multipliers

can be

applied

to non-

elementary sub-systems

in an easy numerical way, since one bas not to introduce a set of

corresponding Lagrange multipliers.

In order to improve

(4-la)

and

(4.Il),

we bave considered

a

partition

of trie 2d lattice into

independent

crosses of np = 5 square

plaquettes,

as shown

m

Figure

3b. We thus obtain a constrained annealed average where ail trie relevant variables

on trie non connected

loops

inside trie crosses are frozen. Since nj = 16, from

(4.6)

trie free energy is

easily evaluated,

and is shown in

Figure

1. Trie

ground

state energy and trie residual entropy are

respectively

E([(T

=

0)

= -1.484375

S([(T

=

o)

= 0.00882...

(4.12)

The next step is to considered trie

elongated

cross of trie type shown in

Figure

3c

(np

= 8 and nj =

24).

In this case we get

E[[~(T

=

o)

= -1.477865

S~~(T

=

o)

= 0.0130...

(4.13)

At

increasing

trie size of trie subsets of trie

decomposition,

trie convergence to trie

quenched ground

state energy Eo is rather slow as trie numerical result of

Ill] #ves

Eo " -1.404 + 0.002 and So

" o.075 +

o.oo4). However,

trie main

qualitative

feature

(positive

residual

entropy)

is

reproduced by

our approximations.

We bave also

applied

our

technique

to trie +J spin

glass

in three dimensions. From a

topological point

of view, a 3d lattice with N

points

can be

thought

as trie union of distinct cubes distributed in such a way that two of them bave

only

one lattice

point

in common

(trie

3d

equivalent

of trie 2d

chessboard).

In trie

thermodynamic

limit their number is N. Let us stress that in this case trie six

plaquettes

of each cube represent trie "black"

re#on)for

a total of

~N,

while there

are

~N

"white"

plaquettes

between cubes.

2 2

It is easy to realize that there exists a

diiferent,

but

equivalent, change

of random variables with respect to trie one

previously described,

which involves np = 5 "black"

plaquette

frustra- tions for each cube

(trie neglected plaquette

must be

always

trie

same), together

with other

plaquette

frustrations in trie "white" areas, for a total of 2N

independent

random variables.

After

performing

trie "white" annealed average, trie

problem

is reduced to trie calculation of

(14)

/ / / / / /

~ -2.

t /

~ /

/ / /

/

-f~

/ ~ cube

~

0 0.5 1-5 2 2.5 3

T

Fig. 4- +J spin glass in 3d: the annealed free energy fa

(dashed fine)

and constrained free energy

f(i~~ (fuit

fine versus T

=

1là.

the

quenched

free energy of a

single

cube. In this case we obtain a constrained annealed av- erage of the free energy of the

global

system

f(f~~,

where the constraints are

imposed

over the

products

of the

J,j's

on all the closed

loops

of bonds in the

~N independent

cubes. The

4

resulting f(f~~

has a very

long analytic expression

and is

plotted

in

Figure

4, where it is also drawn for comparison the annealed free energy.

Unfortunately,

the residual entropy is still

negative,

thus

indicating

that in three dimensions more constraints are necessary to get a fair

approximation

of the

quenched

system at low temperature- However, trie free energy should be

a

non-decreasing

function of trie temperature, so that trie

ground

state energy can be estimated

as trie supremum of an annealed

approximation although

trie free energy bas

negative

deriva- tive at low temperature [5]. Our constraints on all trie

loops

inside trie alternated cubes allows to estimate

Eo(d

=

3)

> -1.917 which

improves

trie lower bounds

given by

trie supremum of trie annealed free energy, Eo > -1.956.

5. Constrained Annealed

Averages

on Infinite

Loops

The method introduced in trie previous section could allow us to obtain very accurate estimates

(lower bounds)

of trie

quenched

free energy. Indeed trie main limitation we bave met is that trie number of

plaquettes

np of trie

sub-system

should be not too

large

m order to

perform

an

analytic

calculation of its

quenched

free energy. For instance m 2d we bave

stopped

trie estimates at trie

elongated

cross with np = 8

plaquettes.

However, we can consider infinite

loops by estimating

trie free energy of

sub-systems

of infinite size

only

in one

direction,

via trie

Lyapunov

exponent of trie

product

of random transfer matrices [12].

To

simplify,

[et us consider

again

trie two-dimensional

Ising

model with

J;j

= +1 with

equal

probability, although

our discussion can be extended to three and

higher

dimensions. Trie idea is to find an

independent decomposition

of trie 2d lattice m

strips

of size L. We then compute trie

quenched

free energy of trie strip as trie

Lyapunov

exponent of trie infinite

product

of

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