HAL Id: jpa-00232116
https://hal.archives-ouvertes.fr/jpa-00232116
Submitted on 1 Jan 1982
HAL is a multi-disciplinary open access
archive for the deposit and dissemination of
sci-entific research documents, whether they are
pub-lished or not. The documents may come from
teaching and research institutions in France or
abroad, or from public or private research centers.
L’archive ouverte pluridisciplinaire HAL, est
destinée au dépôt et à la diffusion de documents
scientifiques de niveau recherche, publiés ou non,
émanant des établissements d’enseignement et de
recherche français ou étrangers, des laboratoires
publics ou privés.
What is the static Edwards-Anderson order parameter
in the mean-field theory of spin glasses ?
H.-J. Sommers
To cite this version:
H.-J. Sommers.
What is the static Edwards-Anderson order parameter in the mean-field
the-ory of spin glasses ?.
Journal de Physique Lettres, Edp sciences, 1982, 43 (21), pp.719-725.
�10.1051/jphyslet:019820043021071900�. �jpa-00232116�
L-719
What
is
the static
Edwards-Anderson
order
parameter
in the
mean-field
theory
of
spin
glasses ?
H.-J. Sommers
Institut
Laue-Langevin,
156X, 38042 Grenoble Cedex, France(Reçu le 29 juin 1982, accepte le 17 septembre 1982)
Résumé. 2014 Nous présentons une preuve, par la méthode des
répliques,
de laproposition
suivante : la valeur moyennequadratique
du spin local dans le modèle de verre de spin deSherrington
etKirkpatrick
est égale au minimum q(0) des paramètres d’ordre q(x) de Parisi. Ceci correspond àl’interprétation dynamique
deSompolinsky
concernant q(x). On montre que q(0) obéit à une loide
puissance q(0) ~
b2/3 pour de faibles champsappliqués b
et pour des domaines de températures 0 T Tc. De plus on calcule l’aimantation en champ faible à toutestempératures.
Les calculs sont basés sur une relation exacte pour lasusceptibilité
locale renormalisée,qui
remplace l’hypothèsede Parisi et Toulouse.
Abstract. 2014 We
present a
replica
derivation for the claim that theaveraged
square of the localspin
expectation
value in thelong-range spin
glass model is equal to the minimum,q(0)
of Parisi’s orderparameters
q(x).
This corresponds to thedynamic interpretation
of q(x) due toSompolinsky.
We show that q(0)obeys
a power lawq(0) ~
b2/3 for low external fields b and all temperatures 0 T Tc. Furthermore we calculate the low fieldmagnetization
for all temperatures. The calculations arebased on an exact relation for the renormalized local
susceptibility
which replaces the Parisi-Toulousehypothesis.
LE
JOURNAL
DE
PHYSIQUE - LETTRES
J. Physique - LETTRES 43 ( 1982) L-719 - L-725 Classification Physics Abstracts 75.40 1 er NOVEMBRE 1982, ]
Edwards and Anderson
[1] suggested originally
the timepersistent
part of the localspin
cor-relation as the
spin glass
order parameterWe consider for
simplicity
anIsing
model(Si =
±1).
The bar denotes theconfiguration
averagewith respect to the random
exchange
interactions and the brackets denote the thermal ordyna-mical average. In the mean-field
approximation
madeby
Edwards and Anderson andSher-rington
andKirkpatrick
[2]
q
wasreplaced by
the static Edwards-Anderson order parameterEdwards and Anderson
implicitly
assumed theequivalence
of both definitions since for verylong
times thedynamical
correlations shoulddecay. q
is the order parameter which can be calculatedby
Monte-Carlo computer simulations[3].
Unfortunately
the definition(1)
seems to beL-720 JOURNAL DE PHYSIQUE - LETTRES
ill-defined for
long-range spin
glasses.
Sompolinsky
[4] suggested
a continuum of order parameterswhere LX are relaxation times
arranged
in adecreasing
order(0
x1)
which all go toinfinity
in the
thermodynamic
limit butq(x)
remains a monotonous function between 0 and 1.Sompo-linsky
introduced a second order parameterd (x)
where~( 1 -
~(1)
+J(x))
is the localsuscepti-bility
on a timescalerx.
Hederived,
with thehelp
of certainassumptions,
a selfconsistenttheory
which turned out to beequivalent
to thetheory
of Parisi[5]
withJ’(x) = - xq’(x)
subject
to- d
’(x)jq’(x) being
monotonic. However in the Parisitheory
the definition of x isslightly
different so thatq(x)
is constant outside a certain interval where it increasesmonotonicly.
The definition of theboundary
values is invariant. Thus we have two well defined limitsq(O)
and~(1).
It wassuggested
[6, 7]
that~(1)
isequal
to q since this accounts well for the results of computer simu-lations[8].
However,
it has beenpointed
outby
Young
andKirkpatrick
([9],
hereafter referredto as
YK)
that thisinterpretation
is wrong sincethey
determinednumerically
aninequality
for the internal energy per
spin,
u,which is violated
by
theParisi-Sompolinsky
solutionif q = ~(1),
since LJ’(x)
0.We are
considering
anIsing
model of Ninteracting
spins
in externalfields bi
with theHamil-tonian
where the
long-range
interactions have the distributionInequality
(4)
can beproved
rigorously following
Bray
and Moore[10]
The second
equality
followsby partial integration,
theinequality
followsdecomposing Si Sj >
2
into
Xij
+
Si ~
S~ ~
andusing
thepositivity
of the matrix Xij andof ( ~ ((
~ )~ 2013 ~ ~ ~)) .
.B’
/According
to thetheory
ofSompolinsky ~(1)
is thequantity
that is calculated incomputer
simulationsand q = q(0).
The last claim has never been written down but it is the naturalconse-quence of
Sompolinsky’s theory.
Wepresent
below areplica
derivation of this statement which also reflectswhy
thereplica
derivation of the localsusceptibility
does notgive
the result which is obtained for finite Nby varying only
the one local field at the site considered. Thereplica
derivationgives
the renormalized localsusceptibility
discussed below.YK claimed
that q
cannot besimply expressed by
q(x).
Howeverthey calculated q using
a restricted ensemble ofspins having
apositive projection
onto themagnetization,
sincethen q
as function of the external field bextrapolates
linearly
to a finite value for & -~ 0.However,
there exist many
possibilities
of such restricted ensembles which allgive
different results for b --> 0(a
few have beenpresented
by
YK).
They
seem tocorrespond
to the different relaxation times ofSompolinsky.
The linearextrapolation
for & -~ 0 maycorrespond
to a certainq(x).
One calculation of YK without restriction is wellcompatible
with a power lawdependence of q
for & -~ 0. It shows that the linear
extrapolation
calculated with the restricted ensemble mentionedabove starts at a field which is an order of
magnitude
greater than the field where themagnetization
rapidly
goes to zero. We will show below thatq(O)
has a power lawdependence
for all temperatures T > 0 below the critical
temperature
T~.
This has been shownby
Parisi[6]
for T ~T~.
Besides it follows thatq(O) =
0 for b = 0 which coincides with the result ofMor-genstem and Binder in two and three dimensions
[11].
Thus thespin glass phase
is critical for alltemperatures
0 T7~.
The above critical index is universal andtemperature
independent.
Sompolinsky
andZippelius [12]
obtained a temperaturedependent
critical index for the lowfrequency
behaviour of thedynamical spin
correlation.However,
the connection of thedynamical
theory
with the fullequilibrium theory
is notquite
clear because of the ill-defined limits fort ~ oo
(Eq. (1)).
The above critical index(Eq. (8))
is based on an exact relation for the renormalized localsusceptibility
which is valid for alltemperatures
and external fields in thespin glass phase
and has been derivedby
the author from theSompolinsky equations.
Itreplaces
the Parisi-Toulousehypothesis [13]
and theBray-Moore
criterion for a soft mode[14].
Furthermore wecalculate the
magnetization
andsusceptibility
for low fields andexplain
the difference between localsusceptibility,
renormalized localsusceptibility
and totalsusceptibility.
We start with a
replica
derivationof q = q(O).
Thereplica
method consists ofaveraging
Tr W" with a
positive integer n and W
=exp( - #H)
andtrying
to obtainlog
Tr W from thecontinuation ~ -~ 0. We may also
directly
calculate derivatives of the free energyby
thereplica
method. A crucial
point
is that Tr W" can be written as anintegral
overvariables
~,
0 a
/3 n,
which can be evaluated for N -~ ooby
saddlepoint integration.
Let us dividethe n
replicas { a }
into two groups{
CXI}, {
a2 }
with n 1, n2replicas
Assume now that the local external field
bil~
in the first group is different from the fieldb~2~
inthe second group. Then
The index a or a 1, a2 indicates which
replica
thespin S a belongs
to.S~ ~ 1, Sl ~ 2
mean theexpectation
values in the fieldsb~l~, i
respectively.
The traces should be normalized so thatTr 1 = 1. W" in
equation (10)
meansactually M~’. W 2
with different fields in the two groups.We have
explicitly
used the fact thatb~ 1 ~
isindependent
of a 1 andbi (2)
isindependent
of (X2. ThusTr Wn
Sf1 Sf2
is a constant.L-722 JOURNAL DE
PHYSIQUE -
LETTRESWe are interested in the limit N -+ oo. The r.h.s. of
equation
( 11 )
can be evaluatedby
the methodof
steepest
descents if weinterchange
the limits n -+ 0 and N -+ oo. This is the standard way toproceed.
The result becomesproportional
to the normalization factor Tr Wn which goes to 1for n --~ 0. We use the fact
that ! ~~ ~ 2
isindependent
of i. Then it is easy to see(e.g.
by
the methodof Ref
[7])
that the result iswhere
q~~a2
means the value at thestationary point.
This statement is not trivial in the case ofreplica
symmetry
breaking,
sinceequation (12)
isonly
validif qa ~ a~
is constant for abelonging
to the first group and
(t2 to
the second group.qa 1 ~~
is not maximized as claimedby
Thou-less et al.
[7].
For asystem
of tworeplicas
equation (12)
coincides with the orderparameter
definition of Blandin et al.
[15, 16].
The two fieldsbi 1 ~
andb~z~
haveonly
been introduced for thepartition
of thereplicas
into two groups. Furtherreplica
symmetry
breaking
isproduced
by
interchanging
the limits n -+ 0 and N -~ oo.Now we look for a
replica
symmetry
breaking
solution which contains apartition
such that(12)
is
independent
of (t1
and a2. Furthermoreqa~a=
should beindependent
of the choice of thepartition
if several
partitions
with the desiredproperty
exist. The solution should go to Parisi’s solution for~
-+b~~~
and indeed Parisi’s solution has theproperties
which are needed. Thesymmetry
breaking
scheme of Parisi consists in thefollowing.
The zerostep
isqa~ -
qo for C( =1=~3.
In a firststep
the nreplicas
are divided intonlm,
groupsof ml
replicas
with a new q,within
each group as indicated infigure
1. In a nextstep
the sameprocedure
isapplied
tothe q
matrices
and so on.We see from
figure
1 that theonly
possibility
fordividing
thereplicas
into two groups with thedesired
property
is thatnlm,
andn2/ml
areintegers.
Thus weget
for the Parisi solution in thelimit n -+ 0
In our
approach
thepartition
(nl, n2)
isgiven
first and then the limit N ~--~ oo istaken,
whichproduces
the stablereplica
symmetry
breaking
scheme. Therefore thepartition
is notcompletely
arbitrary
if we start from Parisi’s solution.We can use the same method to find the averages of
higher
powers ofSi > :
Fig.
1. - Schematic form of the matrixqa~ after the first iteration step of Parisi. One
possible partition
which must be constant with
respect
to a 1, (X2’ ..., oe~.Again
theonly
possibility
is that thedecom-position
of thereplicas
into m groups must be commensurate with the first iteration step of Parisi. Itimmediately
followswhere
mo(y) is
obtained from all the next iterationsteps
in the same way as in Parisi’s work[17].
Thus
where
4J(y,
x)
obeys
the Parisi differentialequation
with the
boundary
conditionEquation
(15)
is similar to theSherrington-Kirkpatrick
case. Theonly
difference is thatmo(Y) =1= tgh
y.mo( y)
is renormalized due to the interactionaccording
toequation (17)
and isthus
additionally
a functional ofq’(x).
We now derive the low field
properties
using
a relation which has been derivedby
the authorfrom the
Sompolinsky
equations
This
equation
is valid for all external fields and itrepresents
the correct formulation of theParisi-. Toulouse
hypothesis
[ 13] :
theaveraged
square of the renormalized localsusceptibility
is constant.It corrects also the
Bray-Moore
criterion for a soft mode[14].
However,
one can show that ananalogous
equation
exists for all x, for x = 1 it takes the form ofBray
and Moore.Equation (19)
follows from the
selfconsistency
equation
forq(x)
differentiated withrespect
tox.for
x -+ 0(in
theSompolinsky formulation).
A more detailed derivation will bepublished
elsewhere. Inaddition we have
equation
(13)
Expanding
bothequations
with respect toPb
=fib
+/~Jz q(0)
weget :
and
~(0)
turns out to be of order(Pb)2/3.
Wemultiply equation (21)
with(pb)~
subtract both equa-tions and take into accountonly
terms up to the order(Pb)2.
Performing
thesimple
GaussianL-724 JOURNAL DE PHYSIQUE - LETTRES
In the last
equation
we mayreplace
mo3~(o)
by
the value forb --+ 0,
i.e.neglecting
thecorrec-tions of
q’(x)
due to the external field. Thus we haveproved
the powerlaw,
equation
(8),
for all0 T
Tc.
The coefficient is determinedby
the Parisi solution for b = 0. For T -~T~
we havewhich coincides with the Parisi result
[6].
Let us now
expand
themagnetization
for b -~ 0From
equation (21)
we findmo(o)
up to the desired order.Introducing
this intoequation
(25)
we obtainUp
to this order we findThis is the usual relation between the
magnetization
and thesusceptibility
for low fields.However,
because of thesingular
behaviour,
equation (23),
this is not the totalsusceptibility
Parisi
[6]
did notdistinguish
between the twosusceptibilities. mo
is the renormalized localsusceptibility,
it is the derivative of themagnetization
with respect to the external field for fixed order parametersq(O), q’(x).
Thus it does not contain the criticaldependence
on themagnetic
field. For fixed order
parameters
it can beexpanded
in powers of the external field. On the otherhand,
for the totalsusceptibility
thedependence
of the order parameters on the external fieldis needed. The unrenormalized local
susceptibility obeys
asimple
Curie law for b = 0 sinceq(O)
=0,
however this is not amacroscopic thermodynamic
quantity
in thespin glass phase.
From the
replica
calculation it iseasily
seen thatThe above
replica
derivation shows that theright
hand side isonly equal
to theunrenor-malized local
susceptibility, ~ Si )/b~bi
= 1 -( Si
)2
if~
is constant, i.e. withoutreplica
References
[1]
EDWARDS, S. F. and ANDERSON, P. W,, J.Phys.
F 5 (1975) 965.[2]
SHERRINGTON, D. and KIRKPATRICK, S.,Phys.
Rev. Lett. 35 (1975) 1792.[3]
KIRKPATRICK, S. and SHERRINGTON, D.,Phys.
Rev. B 17(1978)
4384.[4]
SOMPOLINSKY, H.,Phys.
Rev. Lett. 47 (1981) 935.[5]
DE DOMINICIS, C., GABAY, M. and DUPLANTIER, B., J.Phys,
A 15 (1982) L47.[6]
PARISI, G., J. Phys. A 13 (1980) 1887.[7]
THOULESS, D. J., DE ALMEIDA, J. R. L. and KOSTERLITZ, J. M., J.Phys. C
13(1980)
3771.[8]
PARISI,G.,
Philos. Mag. B 41 (1980) 677.[9]
YOUNG, A. P., KIRKPATRICK, S., Phys. Rev. B 25(1982)
440.[10]
BRAY, A. J., MOORE, M. A., J.Phys. C
13(1980)
419.[11] MORGENSTERN, I. and BINDER, K.,
Phys.
Rev. Lett. 43 (1979) 1615,Phys.
Rev. B 22 (1980) 288, Z.Phys.
B 39 (1980) 227.