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HAL Id: jpa-00247366

https://hal.archives-ouvertes.fr/jpa-00247366

Submitted on 1 Jan 1997

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Energy-Energy Correlations in Square and Cubic Ising Models

Roland Netz, Ingo Gersonde

To cite this version:

Roland Netz, Ingo Gersonde. Energy-Energy Correlations in Square and Cubic Ising Models. Journal

de Physique I, EDP Sciences, 1997, 7 (7), pp.827-832. �10.1051/jp1:1997204�. �jpa-00247366�

(2)

Short Communication

Energy-Energy Correlations in Square and Cubic Ising Models

Roland R. Netz

(~,~'*) and Ingo

H.

Gersonde (~)

(~)

Department

of

Physics,

Box 351560,

University

of

Washington, Seattle,

WA 98195-1560, USA

(~) Service de

Physique Th60rique, CEA-Saclay,

91191 Gif sur Yvette, France

(Received

9

September

1997, ret,ised 4

February1997,

accepted 6

May 1997)

PACS.05.70.Jk Critical

point phenomena

PACS.64.60.Fr

Equilibrium properties

near critical points, critical exponents

PACS.02.70.Lq

Monte Carlo and statistical methods

Abstract. Cluster-Monte-Carlo simulations are used to calculate the structure factors as- sociated with

order-parameter

and energy correlations for square and cubic

Ising

models, from which the

corresponding

correlation lengths ( and (E,

respectively,

are determined. The am-

plitude

ratio ~KE +

((/(~

is

asymptotically

universal but

strongly

influenced

by

the crossover from mean-field behavior. The

numerically

determined XE therefore does not reach its universal

asymptotic

value but agrees well with

e-expansion predictions including

corrections to

scaling.

The consequences for experiments on near-critical fluids and colloidal systems are

briefly

dis- cussed.

On

approaching

a continuous

symmetry-breaking phase transition,

the order parameter field

#(r) characterizing

the ordered state exhibits

diverging

correlated fluctuations. The structure factor

G(q, t),

which is the Fourier transform ofthe bilinear correlation function

Giq, tl

C~

/ d~r e~~'~1410)41r)1, il)

has been of central interest in the

study

of critical

phenomena [il.

In an

experiment

where

a

scattering probe (such

as

X-rays

or

neutrons) couples

to the order

parameter,

the result-

ing scattering intensity

is

proportional

to

G(q,t),

which allows accurate tests of theoretical

predictions [2].

The local energy

density

is

proportional

to the square of the order

parameter, #~(r),

and therefore shows

strong

fluctuations

sufficiently

close to a critical

transition,

too. In this article

we discuss the structure factor

GE(q,t)

of connected energy-energy

correlations,

GE(~,~)

C~

/ ~~r

e~~

~(~~(0)~~(r))C. (~)

(* Author for

correspondence (e-mail: netztlmpikg-teltow.mpg.de)

Present address: Max-Planck-Institut fir Kolloid und

Grenzflhchenforschung,

Kantstr. 55, 14513 Teltow,

Germany

©

Les

#ditions

de

Physique

1997

(3)

828 JOURNAL DE

PHYSIQUE

I N°7

To measure

GE (q, t) experimentally

one needs a

scattering probe

which does not

couple

to

the order

parameter

field itself but

only

to the square of it. One such

example

is sound

adsorption

in near-critical fluids or solids

[3,4].

A different mechanism is

provided by systems

with

distinct, coupled

order parameters;

scattering

from a

secondary

order

parameter

which shows critical behavior

only

due to a

coupling

to the square of the

primary (critical)

order

parameter

should then be

proportional

to

GE (q, t). Experimental

realizations include colloidal

particles

in near-critical

liquid binary

mixtures

[5,

6] and the so-called sponge

phase

found in microemulsions

[7].

One of the

early

theoretical successes consisted of

postulating

[8]

land

later

deriving [9])

for the structure factor

ii

the

scaling

form

Gjq,tj

=

xlt)glq~f~), 13j

valid in the

asymptotic regime, I.e.,

for small

temperatures

t and for wave vectors much smaller than the inverse lattice constant a,

I-e-,

q «

a~~.

Unless at a critical

point,

defined

by

t =

0,

the

scaling

function

g(x)

can

always

be

expanded

as a

jower

series of its

argument.

For small

arguments,

the inverse

scaling

function is

commonly approximated by

g~~lq~f~)

= i +

q~f~

+

Olq~f~),

14)

which defines the correlation

length (

as the second

spatial

moment of the correlation func- tion. Close

enough

to

criticality,

the

susceptibility

and correlation

length

can be written as

tit)

=

xot~~

and

fit)

=

(ot~~, respectively.

The

amplitudes

xo and

to

are non-universal

parameters depending

on details of the

interaction,

etc. The exponents +t and u are universal and determined

by

the dimensionalities of space and order

parameter

field.

Generalizing

the

scaling hypothesis

to the

biquadratic

correlation function

GE(q,t),

one

writes the

biquadratic

structure factor

(2)

in

analogy

to

(3)

and

(4)

as

GE iq, t)

=

Cit)gE iq~fi)

~f

~ ~~

ji)j

j~~ j~

,

is)

which defines the energy correlation function

(E

as the second moment of the energy-energy correlation function. In the

asymptotic limit,

the

specific

heat and the energy correlation

length obey-

the

asymptotic

laws

C(t)

=

Cot~°

and

(E It)

=

(E,ot~~E, respectively. Here,

o is the universal

specific

heat exponent and uE is the

exponent

of the energy correlation

length

which could in

general

be different from u.

Within the

e-expansion technique (where

e

= 4 d measures the deviation from the upper

critical dimension

four)

the energy-energy correlation function

GE(q, t)

can be calculated for the standard

#~ theory using

a double

expansion

in e and the

quartic coupling strength [ii.

The actual calculation is rather

long

and

technical,

but among the results one finds that the two correlation

lengths

scale with the Same

exponents,

I.e.

u/uE

= 1+

fJ(e~ [10].

A different conclusion was

initially

drawn from

X-ray scattering

results for similar

biquadratic

correlations at a smectic-nematic transition in a

liquid crystal sj,stem [11],

but later reconciled with the

above theoretical result

[12].

Furthermore, the ratio of the correlation

lengths asymptotically approaches

a universal

amplitude

ratio

[10]

j2

~

~~ (~

6~

~

~~~~~'

~~~

Although

the

equality

of the two correlation

lengths,

I.e. u

= uE, has

only

been

proved

up to the first order in e, we note that a naive

scaling theory

would

suggest

that this

equality

is exact.

(4)

Also,

it could be

speculated

that the relation

(6),

which has been calculated up to

e~, might

hold to all orders in e, and thus be

applicable

at all dimensionalities. This could of course

only

be substantiated

by higher-loop

calculations. As is well

known,

the

specific

heat is

strongly

influenced

by

the crossover from mean-field to

asymptotic

critical behavior

[13].

It therefore

might

be hard to observe the

asymptotic

correlation

length

ratio

(6)

in an

experiment

or a

simulation.

Defining

the effective

temperature-dependent exponents +te~(t)

e d In

x(t) Id

In t and ae~

it)

e d In

C(t) Id

Int one derives to

Die)

the relation

[10]

x~jt)

-

(

=

je~((~ j7)

which holds

beyond

the

asymptotic regime

since it includes corrections to

scaling.

It is this

expression

which would be measurable

experimentally

and which we test in this article.

In our simulations we use the standard

Ising model,

defined

by

the Hamiltonian

~

IT

=

-J£j~~~

s~sj with si = ~1 and the sum

running

over

nearest-neighbor pairs

on square or cubic lattices. We

empliy

a Cluster-Monte-Carlo

algorithm [14],

which has

recently

been

successfully

used to calculate bilinear correlation functions

[15].

Figure

I shows results for square lattices of linear size up to L

=

200; subaveraging

over

progressively larger

time intervals has been used to calculate statistical errors

(which

are

always

smaller than the

symbol size).

The

susceptibility

x

(solid circles, Fig. la)

compares well with exact

results,

+t =

7/4

and to

= 0.962582

[16] (solid line).

The

specific

heat C

(open circles), predicted

to exhibit

logarithmic

behavior

(a

=

0)

indicated

by

the broken line with

zero

slope,

has not

quite

reached the

asymptotic scaling regime,

in accord with theoretical

expectations [13].

For the calculation of correlation functions

along

a certain direction

(here

chosen to coincide with a lattice

principal direction)

we

separate

the

spatial

coordinates into the

parallel, rii

e r Q, and

perpendicular part,

ri % r

ripe,

and rewrite

equation ii)

as

G(q, t)

«

V~~

drjie~o~"

dr(j ~ d~~~r[#(r(j,r [) ~ d~~~r14(r(j

+

rip,ri) ), (8)

thereby minimizing

the numerical effort.

Figure

16 shows the inverse

scaling

functions

g~~

and

50gj~

as a function of

q2

for t

= 0.11438.

According

to

(4)

and

is),

the

corresponding squared

correlation

lengths

are determined

by

the

slopes

for small momentum

(solid lines).

As seen in the

figure,

the energy-energy

scaling

function

(open circles) extrapolates

not as

nicely

to a

straight

line at the

origin

as the bilinear correlation function

(closed circles) does,

and the extraction of the energy correlation

length

is harder. This is in full accord with the field-theoretic

calculation,

which

predicts higher-order

terms in the

expansion

of the

scaling

function in

(5)

to be

larger

than for the bilinear

scaling

function

[10].

To access even smaller q values one would need to take

larger system sizes,

which increases the

computational

effort.

The

resulting

bilinear correlation

length ( (circles, Fig. 1c)

is much smaller than the system size

(so

that finite-size effects can be

neglected)

and agrees well with series

expansion estimates,

u = 0.632 and

to

= 0.495

ii?] (solid line).

The correlation

length

ratio

XE (for

which the error bars would be hard to

estimate)

is

plotted

in

Figure

id. With o

= 0 the

predicted asymptotic

value is

XE

=

0, according

to

(6)

and

using

the

working hypothesis

that the e

expansion

results

are also valid in dimension two, I.e. for e = 2. The actual values for

,KE, though being

very

small,

are far from zero and in contrast to the

asymptotic prediction

agree rather well with the effective

exponent

ratio determined

by (7) (solid line).

The effective exponents +te~ and ae~ are determined from our data

by fitting

the

double-logarithmic

data in

Figure

la to a

polynomial

of fifth order.

(5)

830 JOURNAL DE

PHYSIQUE

I N°7

x

a)

c

<2°

js0gi

°

'

~ ~

_

,~ ~~

0

' 0 2 4 6 8 lo

0.03 0.< 0.3 2

t

~l

20

C) ~

,~ E

I.

.

(6)

~~~

a)

~~ 60

~0g/

~

~f

-c--_

~

o I

° ~

~~~

~

~ ~ 40 o

.

<00

o

o

g-1

~

b)

20 ~

0

<0 0.06

C) XE

j

.

~ .

d)

2

~~~

(7)

832 JOURNAL DE

PHYSIQUE

I N°7

References

[ii

Wilson

K.G., Phys.

Rev. Lett. 28

(1972) 540;

see also Ma

S.K.,

Modern

Theory

of Critical Phenomena

(Benjamin, Reading, 1976).

[2] Als-Nielsen

J.,

in "Phase Transitions and Critical

Phenomena",

C. Domb and M.S.

Green,

Eds.

(Academic, London, 1976)

Vol.

5a;

Collins

M-F-, Magnetic

Critical

Scattering (Ox-

ford

University Press,

New

York, 1989).

(3]

Hohenberg

P-C- and

Halperin B-I-,

Rev. Mod.

Phys.

49

(1977)

435.

(4] Garland

C.W.,

Eden D. and Mistura

L., Phys.

Rev. Lett. 25

(1970) l161;

Mueller

P.E.,

Eden

D.,

Garland C.W. and Williamson

R.C., Phys.

Rev. A 6

(1972)

2272.

(5] Netz

R.R., Phys.

Rev. Lett. 76

(1996)

3646.

[6]

Gallagher

P.D. and Maher

J.V., Phys.

Rev. A 46

(1992) 2012;

to observe the

biquadratic

structure

factor,

the colloidal

particles

must be indifferent to the concentration difference between the

binary component,

i.e., must not

prefer

one component over the other.

[7]

Gompper

G. and Schick

M.,

in Phase Transitions and Critical

Phenomena,

C. Domb and J.L.

Lebowitz,

Eds.

(Academic, London, 1994),

Vol. 16.

[8] Kadanoff

L.P., Physics

2

(1966)

263.

[9] Fisher M.E. and Burford

R-J-, Phys.

Rev. 156

(1967) 583;

Fisher M.E. and

Aharony A., Phys.

Rev. B lo

(1974)

2818.

[10]

Netz R.R. and

Aharony A., Phys.

Rev. E 55

(1997)

2267.

[11]

Wu

L., Young M-J-,

Shao

Y.,

Garland

C-W-, Birgeneau

R.J. and

Heppke G., Phys.

Rev.

Lett. 72

(1994)

376.

[12] Aharony A., Birgeneau R.J.,

Garland

C.W.,

Kim

Y.-J.,

Lebedev

V.V.,

Netz R.R. and

Young M.J., Phys.

Rev. Lett. 74

(1995)

5064.

[13]

Rudnick J. and Nelson

D.R., Phys.

Rev. B13

(1976)

2208.

[14]

Swendsen R.H. and

Wang J.-S., Phys.

Rev. Lett. 58

(1987) 86;

Wolff

U.,

ibid. 62

(1989)

361.

[15]

For an extensive discussion of technical

points,

consult

Ruge C.,

Zhu P. and

Wagner F., Physica

A 209

(1994)

431.

[16]

Barouch

E., Mccoy

B.M. and Wu

T.T., Phys.

Rev. Lett. 31

(1973)

1409.

[17]

Liu A.J. and Fisher

M.E., Physica

A 156

(1989)

35.

[18] Ferrenberg

A.M. and Landau

D-P-, Phys.

Rev. B 44

(1991) 5081;

Baillie

C.F.,

Hawick K-A- and

Pawley G.S.,

ibid. 45

(1992)

10438.

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