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Spinodal phase separation in complex fluids
F. Schmid, R. Blossey
To cite this version:
F. Schmid, R. Blossey. Spinodal phase separation in complex fluids. Journal de Physique II, EDP
Sciences, 1994, 4 (7), pp.1195-1207. �10.1051/jp2:1994194�. �jpa-00248037�
Classification Physics Abstracts
64.70J 64.75 82.70
Spinodal phase separation in complex fluids
F. Schmid
(I)
and R.Blossey (~)
(') Department
ofPhysics
FM-15,University
ofwashington,
Seattle wA 98195, U-S-A- (2) Institut fur TheoretischePhysik
IV, Heinrich-Heine-Universitit Ddsseldorf, Universithts-strasse1, 40225 Dusseldorf,
Germany
(Received 27 September 1993, revised 28 January 1994,
accepted
25 March 1994)Abstract. we study the early stages of the phase separation of an
amphiphilic
system into twofluids, one structured and the other not, in the context of a one-component
order-parameter
model.A
generalization
of theLanger
Bar-on Millerapproximation permits
the calculation of the time evolution of the structure function in the mixture. Near the structured-fluid side of the coexistence, we find that thespinodal
is much moreclearly
observable and is closer to the binodal than on the unstructured side.1. Introduction.
Phase
separation
occurs when abinary
system(e.g.
a mixture of two fluids orpolymers)
isquenched
from astable, homogeneous one-phase
state into thetwo-phase region
of itsphase diagram [11.
Theearly-stage dynamics
of theunmixing
process has been studied first in thecontext of
simple,
mean-field like theories[2, 31.
Thepicture emerging
from thisdistinguishes
between two very different
regimes.
If the initial statqright
after thequench
isthermodynami- cally metastable, phase separation
mustbegin
with the nucleation ofdroplets
of thepreferred
stable
phase.
When the size of such adroplet
exceeds a critical value, it will grow and the metastable statedecays.
The nucleation process itself is mediatedby
thermal fluctuations and isgenerally
described in terms of thedroplet
nucleation rate r e~ ~, wheree is the excess free energy of the critical
droplet.
In this firstregime, phase separation
is ahighly inhomogeneous
and stochastic process. On the other hand,
phase separation
from athermodynamically
unstable initial state is
govemed by
thegrowth
of the unstable fluctuations(spinodal
decomposition).
Theearly-stage demixing
isessentially homogeneous, leading
to the formation of acomplex
interconnectedtwo-phase
structure. In mean-fieldtheory,
bothregimes
are
separated by
a well-definedspinodal.
This
simple,
classicalpicture
succeeds inqualitatively describing
manyexperimental
features of
early-stage phase separation. Unfortunately,
it fails as soon as fluctuations have to be included. Inparticular,
the concept of aspinodal
isgenerally
considered to bemeaningless
beyond
mean-fieldtheory [11.
The main reason for this lies in the fact that the unstablefluctuations close to the
spinodal
have verylong wavelengths
andconsequently
grow veryslowly
in time. Therefore the dominant mechanism forphase separation
remains nucleationeven
beyond
the classicalspinodal.
Asharp spinodal
cannot be detectedby experiment
orby
simulation.
Experimentally,
theearly
stages ofphase separation
have beenfrequently
studied in metallicalloys [41. Unfortunately,
the observation insimple binary
fluids is rather difficult due to the very short time scales on which relaxation occurs. In order to circumvent thisdifficulty,
experiments
have been conducted in situations where time scales are enhanced, as is e.g. thecase for
quenches
at the critical concentration[51.
Another strategy has been to chooseexperimental
systems whichby
themselves havelong
relaxationtimes,
such aspolymer
solutions
[6, 71, equal
mass solutions [81 orcomplex
fluids such as non-ionic micellarsolutions
[91.
These latter systems areespecially interesting
because of the new effects that can beexpected
due to the intemal structure of thehomogeneous phases.
A
complex
fluid can exhibit disorderedphases
that, whilebeing homogeneous
on amicroscopic
scale, areinternally
structured. The structure shows up as apeak
at non-zerowavevector in the static structure factor of
scattering [101.
Aprominent example
of acomplex
fluid is the microemulsion
phase
in oil-water-surfactant mixtures which contains aninterpene- trating
network of oil-water interfaces[lll. Only recently
has there been some theoreticalinterest in the
dynamics
in such systems : the relaxation after aquench
into theone-phase region
of the microemulsion has been studied[121
as well as thedynamics
of oil-waterseparation
in the presence ofamphiphiles [131.
However, since the internal structure of acomplex
fluid indicates a built-inaffinity
towards fluctuations of a certainwavelength,
it shouldparticularly
affect thespinodal decomposition
in anunmixing
process.It is this
question
we address in the present paper. Westudy
theearly
stages ofphase separation
into twophases,
one of which isintemally
structured while the other is not, within aGinzburg-Landau-type
model system for acomplex
fluid. Inparticular,
we are interested in thechanges
in thetime-dependent
structure factor as the average concentration isvaried,
and thespinodal
on both the structured and the non-structured side of thephase diagram
is crossed.Our
approach generalizes
the method ofLanger,
Bar-on and Miller[171
forsimple binary
systems, which accounts for small fluctuations. Forcomparison,
we alsostudy
the system in mean-fieldtheory.
Our paper isorganized
as follows : we introduce the model in section 2 anddevelop
thetheory
in section 3. Section 4 presents in detail the results for both the mean-fieldtheory
and theLanger
Bar-on Millerapproximation.
We summarize in section 5.2. The model.
A temary
oil-water-amphiphile
mixture is mostnaturally
studied with a two-fieldGinzburg-
Landau functional
[141,
?l~, 4fl
=
d3r(c(A~)2
+go(v~
)2 +w(~
+v(~,
~i~(v~)2)
,
(1)
where go
~0,
c~0.~
denotes the difference between oil and waterdensity,
and#r is the surfactant
density.
The last term in(I)
accounts for theamphiphilic properties
of thesurfactant, favoring
it to sit at the internal oil-water interfaces. ThusI
~ 0 is related to the
strength
of theamphiphile. W(#
is a double-wellpotential
with minima at the oil- and water- richphases.
Since the surfactant does not cluster and itsdensity
is small even in themicroemulsion
phase,
weexpand
J up to second order in#r.
We getV
(#r, #
m vj(#
#r p #r + v~(#
) #r~, wherev~(#
m 0 for all accessible values of 2#
and p is the chemicalpotential driving
the surfactantdensity
#r.At
early
times of thephase separation
process, whentypical length
scales are stillsmall,
energy and momentum transport in the fluid are fastcompared
to theunmixing
process. Thedynamics
can then be describedby Langevin equations
for the conserved fields # and~. We further
simplify
thedynamics by assuming
that the surfactant relaxes much faster than oil or water, I.e. itsdensity
follows thechanges
in the difference of oil and waterdensity adiabatically. Although
this lastassumption
is notnecessarily
realistic in ageneral experimental situation,
we expect that thesimplified
model still contains the main characteris- tics ofphase separation
in asimple/complex-fluid
mixture. We note that, theresulting
model(2) being
thesimplest possible
model withtwo-phase
coexistence of asimple
and a structuredfluid,
itsstudy
shouldgive qualitative insight
into the effect of internal structure onphase
separation
in any such system, notjust
in ternary mixtures.Following
ourassumption,
we canintegrate
out the field #rquasistatically [lsl
which leads to an effectiveone-order-parameter
functional[161,
>1#1
=
d3r jc(A#
)2 +g(# )(v#
)2 +fj# )j
,
(2)
where
g(#
)= go I (p vi
)/v~
and~
k~
Tf
(#=
w
(#
)(v
v)~/2
v~j
in(v~/k~ T)
(Higher
orders in VW have beenneglected
inEq. (2)
as inEq.
I)).
Hence, one is left withjust
one
equation
of motion for the oil-waterdensity
#d~~b
(r,
t =AV~ ~~~
+ i(r, t),(3)
where the Gaussian white noise f satisfies the
fluctuation-dissipation
relation<~(r, t) ~(r', t')j
=
2
k~ TAV~ 8(r r') 8(t t'). (4)
The static
properties
of model(2)
have been studiedextensively [141
in various contexts. Inmean-field
theory,
thehomoge fiases
aregiven by
the minima of the functionf(#
). The value of y= g
(# )/
, 2cf"(#
there determines thedegree
of internal structure of the fluid forlarge positive
values of y the system behavesjust
as anordinary
fluid. At thedisorder line y
= I, correlation functions
begin
to showoscillatory
behaviorbeyond
theLifshitz line y =0, the structure functions exhibit a
peak
at nonzero q.Finally,
aty = I, the
homogeneous phase
becomes unstable with respect todensity
fluctuations of acertain
wavelength,
and the lamellarphase
is stable. Here we are interested in a situation attwo-phase
coexistence, where one hasphase separation
into a structured and a non-structuredphase.
Hencef(#
has two minima and g(#
ispositive
at one, e.g, the water richphase,
andnegative
at the other, e-g- the microemulsion.3.
Theory
of the structure factor.Based on the model
(2), (3)
we now establish theequations
for the evolution in time of thestructure factor.
Equation (3)
leads to the Fokker-Planckequation
for the distributionfunctional p
[~
;tl,
d~p
d~r
~~i~
15)
~
~ (~)
JOUR~AL DE PHYSIQUE u -T 4 N'7 JULY 1994
with the
probability
current3j~ tl
#
AV~[H(r)
p +k~
T~((
,
(6)
where
1I(r)=
~~=2cA~#-2gA#-fg(V#)~+ff. (7)
From
(5)
we find that the structurefactor, ((k)m ($ (k) / (- k)), obeys
J~i(k)
=
Ak21(»(k) I (- k)j
+(»(~ k) I (k)j1
+ 2Ak~ Tk2
,
(8)
where indicates a Fourier transform and the brackets
(.. )
denote the average with respect to thejoint probability
functional p[$ tl.
In order to solve these
equations,
weadopt
the route takenby Langer,
Bar-on and Miller[171,
and factorize p in a convenient way : let p~~J denote then-point
distribution functionp)~~, r~(iij,
,
u~)
=
(&(u(rj) u~).. (u(r~) u~))
,
where
u(r)
= #
(r) (#)
are the fluctuations in the field #(r).
Weexpand
theexpression
p
~"~(uj, u~)/[1I)~
j p
~'~(u, )I
up to second order in the u~ and obtainp)]~ r~(l~l,
,
l~n) ~
In
p ~~~(l~,)ii
+jj y(r~,
r~)11,l~j
(9)
, , <j
Here y is related to the structure function
by y(r,,r~)(u~)~=S(r~ -r~).
For n =2equation (9)
recovers the ansatz for thetwo-point
distribution functional p ~~ usedby Langer
et al.However,
asopposed
to the model forsimple binary
mixtures treated there, theright
handside of
equation (8)
involves alsothree-point
correlations functions.With the ansatz
(8)
and(9),
the time derivative of the structure functiond~((k)
can beexpressed
as a function of((k)
and p ~'~ alone.Using equations (5)
and(6),
we find?iP
~~'(u
)= A
jj
k~e~'~
~l( fi(k
~ +k~
T ~~(# (r
u)
,
(10)
k
~~ ~ll~
which also involves
only
the structure function and p I'J. Thus, the set of
equations (8)
and(10)
is closed.They
will be solvednumerically
in thefollowing
section. Inpractice
we use the~°~~~~~~~
k/T~~~ ~~
~ ~~ ~~~ ~~~~~~k/T ~~~ ~~'
~° ~~~~ ~ ~~ ~~~~~~~~ ~°~positive
4 andpositive
fornegative
4.Furthermore,
we fix c= I and
k~
TA=
I thus
k~
Tsetting
the units of time and space. In thecomplex
fluidphase,
theequilibrium
structure function((k)
hasa maximum at k
=
/
=
0.92 at # = 1.7.
Since the final result is rather
technical,
werelegate
it to theappendix
and conclude thissection with a few comments on the
validity
of theapproximation (9). Technically,
thecalculation breaks down as soon as the
higher
moments(u")
of the fluctuation field become toolarge compared
to the first ones. The fluctuations uobviously
have to be small, sinceequation (9)
h anexpansion
in u. This limits theapplicability
of ourapproach
toearly
times. Amore serious
shortcoming
ofequation (9)
is that it does not include effects ofinhomogeneities
and assumes correlations to be
independent
of whether fluctuations occur in the same ordifferent domains.
Therefore,
theapproximation
will not be able to treatphase separation correctly
wherever nucleation effects areimportant.
In thespinodal regime, however,
the systemdecomposes homogeneously
and our treatment willprovide
anappropriate description.
4. Results.
Having
established the basicequations,
we are nowready
to present the results for the structure function. Tobegin with,
we discuss the Gaussianapproximation,
in whichonly
theleading
order in the fluctuations u is
kept
inequation (15)
and(16).
The structure function is found toobey
theequation
d~((k)
= 2
Ak~ ((k)A(k)
+ 2
Ak~ Tk~ (11)
with
A(k)~ 2ck4+2k2g(~)+ f"(~). (12)
Equations (I
I) and(12) correspond
to the Cahn-Hilliard-Cookapproximation
for the structurefactor
[2,181.
Within thisapproximation,
fluctuation modes with different wavevectorsdecouple
and each relaxesexponentially
with its own characteristic time 1/~(k
)=
2 Ak~A
jk).
The mode becomes unstable when
~(k)
becomesnegative. Suppose
now that thequench
experiment
starts at somehomogeneous
concentration ~bo and then the system isbrought rapidly
into the coexistenceregion.
If~
(k
ispositive
for all k, the system reaches a metastablehomogeneous
state after sometime,
which canonly decay by
nucleation processes for which there is no mechanism in thetheory
we use.As soon as
~ becomes
negative
for some k, thecorresponding
mode growsexponentially
and initiates the
unmixing
process. In asimple binary
fluid where g ~0,
the classicalspinodal
that separates the nucleation and
spinodal decomposition regimes
isgiven by f"(4
o = 0. The
maximum
growth
rate w~ = max[-
1/~(k )I drops
to zero withvanishing slope
as thespinodal
k
is
approached (Fig.
la, 4 ~ 0 and g(4
cc##
and the unstable modes are those with smallwavevector k
(Fig.
lb, # ~0).
Therefore, unstable modes grow veryslowly
close to thespinodal
and will neverprovide
the dominant mechanism forphase separation.
As discussed in the Introduction, thisimplies
that inpractice
the nucleation and thespinodal decomposition regimes
cannotclearly
beseparated
and thespinodal
ismeaningless.
The situation is different in a
complex
fluid with g~ 0. Here, modes with finite wavevector k~
= g
(#o)/2
c become unstable before theordinary spinodal
is reached.Spinodal
decom-position
occurs as soon asf"(~bo)
<gi~bo)~/2
c(13)
is fulfilled. The consequences are illustrated in
figures
la and 16-Compared
to thesimple
fluid side at40
~ 0, twoimportant changes
occur on thecomplex
fluid side(40
~ 0).First,
thespinodal
is shifted towards the binodal at 4 = 1, theregion
ofspinodal decomposition
isenlarged.
In the extreme case where g -2,
I.e. very close to the transition to the lamellarphase,
thespinodal
and the binodalnearly
coincide. Theincipient instability
of the structured fluid to the lamellarphase
appears tocatalyse
thephase separation.
The secondchange
is evenmore dramatic. In contrast to a
simple
fluid mixture, here the most unstable fluctuation at thespinodal
has finitewavelength
and the maximumgrowth
ratew~ drops
to zero with a finite and rather steepslope.
Therefore theregion
in which nucleation process compete withspinodal
0. 8
0.6
o.4
0.2
"p
o
-0.2
0. 4
0. 6
-0.8
-1 -0.5 0 0.5 1
~$0 a)
o. 9
0. 8
0.7
0.6
j~ 0.5
P 0.4
o.3
0. 2
o. i
o
-i -o.5 o o.5 1
~b0 b)
Fig.
I. Cahn-Hilliardapproximation
: a) growth rate w~ = max [- I/r(k)] and b) wave vector iL~ of the most unstable fluctuation after a quench into the two-phase region with 1.7. i's order parameter ~o.
decomposition
should be much smaller and thespinodal
should be better defined. As aconsequence, the concept of a
spinodal
is useful evenbeyond
the Cahn-Hilliard-Cookapproximation
in acomplex
fluid and it may bepossible
to locate itexperimentally.
We now
proceed
to the full treatment,considering
model(2)
with#
=
1.7 and
accounting
for fluctuations as described in the
previous
section and in theappendix.
Figure
2 shows the structure function at different times for bothspinodals,
on the normal-fluid side
(4,~
=0.58)
and on thecomplex-fluid
side(~~~
=0.8).
In both cases, thestructure function
develops
apeak
it grows faster on thecomplex-fluid
side of thephase
diagram,
and thecorresponding
wavevector kchanges
less in time. Thus, the system on the0. 6
t = i.o
o.5
o.4
§(k)
~ ~
0. 2
o.i t =
o
0.5 1 1.5 2
k
a)1.8
t =
1.6
1. 4
1. 2
ijk)
10.8
0. 6
0.4
0.2
0.2
=
o
0.5 1 1.5 2
k
b)Fig.
2. Structurefunction'(
(i) for different times between t= 0. I and t I. al at ~o 0.58, b) at
~o 0.8.
complex-fluid
side is driven towards alamellar-phase-like
intermediate structure which mediates thephase separation
:spinodal decomposition
in acomplex
fluid hasqualitatively
avery different character than in a
simple
fluid.Nevertheless,
if onejust
looks at((k), locating
thespinodal
on thecomplex-fluid
side remains as difficult as on thesimple-fluid
side. The structure functionschange only slightly
as40
crosses thespinodal.
It proves useful to consider the time derivatived~(
instead. Whilenothing special
appears tohappen
at thespinodal
on thesimple-fluid
side(Fig.
3), its behaviorchanges qualitatively
as thespinodal
on thecomplex-fluid
side ispassed
in the nucleationregime, d~(
decreases in time, in thespinodal regime,
it decreases first and then increasesagain.
These tworegimes
areclearly
distinct(Fig. 4).
1. 2
= o.1
~ ~ 0.2
d§(k) i
°.60. 4
0.2 t =
o
0.5 1 1.5 2
k
a)1. 2
1
= o.1
dS(k)
0.8dt
0.60. 4
0.2 =
o
0.5 1 1.5 2
k
b)Fig. 3. Time derivative of the structure function for different times a) at ~o " 0.55, b) at
~~ 0.6.
Another useful
quantity
to examine is thelogarithmic
derivative of the structure functiond~(/(.
In the Cahn-Hilliard-Cookapproximation (11),
it issimply given by
~~~~~ l.
~ t
((k)
t~(k) (14)
1- 0 j j
with h
(x)-
I -x + x~ Hence,[d~S(k)/S(k) I/t] roughly gives
the character-2 12
istic
growth
rate, 1/~(k),
of a mode k.Figure
5 shows the maximum value of thisquantity
for different times as a function of 4. One
easily
identifies aspinodal
on thecomplex-fluid
side of thephase diagram.
On thesimple-fluid
side, the exact location is still difficult todetermine,
2 5
= o.1
2
dir(k)
1.5dt
1
oos
t - i.o
0
0.5 1 1.5 2
k
a)2 5
= o. 1
2
tiS(k)
1.5tit
i
o.5
t " lo
o
0.5 1 1.5 2
k
b)2.5
= o. 1
2
dir(k)
15dt
i
o.5
~
o
0.5 1 1.5 2
k
c)Fig. 4. Time deRvative of the s~ucture function at different times a) at
#o=
0.75,b)
at~o = 0.8, c) at ~o
= 0.85.
1
t=0.1-
0.9 t=0.2
;,
~ ~ tm0.4 '.
t=0. 6 '.
0~7 t=0.8
/
"t=1 0 / _;- .,,
max[~~/~~)-
~~ l'/~' ""
k S t " "~~'~
0.4
0. 3
0. 2
o. i
-o.i
-i -o.5 o o.5 1
~b0
Fig. 5.
max
~II
I/t vs ~o at different times
~
especially
since the curves areexpected
to smear out due to nucleation events. We note thatfigure
5 isstrikingly
similar tofigure
I the main features ofspinodil decomposition
incomplex
fluids arealready
evident in the Cahn-Hilliard-Cookapproximation.
Thequantitative
behavior however
changes
as one includes fluctuations sinced~((k)
ceases to behaveexponentially
in time aspredicted by
theapproximation.
On thecomplex-fluid
side of thephase diagram,
it may even be nonmonotonic in time, as is evident e.g. infigure
4a.5.
Summary
and discussion.In the present work we have discussed
early-stage spinodal decomposition
within asimple
model for a
complex
fluid. We have studied the time evolution of the structure functionI(k)
in mean-field(Cahn-Hilliard-Cook) theory
and included fluctuations in aLanger
Bar-on Miller type
approximation.
Our main results can be summarized as follows :I)
the presence of intemal structure in the fluid shrinks themetastability region
of thephase diagram.
In fact, for anideally
strongamphiphile
thespinodal approaches
the binodal,leaving
no nucleation
regime
at all ;it)
in contrast tosimple fluids,
the unstable fluctuations at thespinodal
have a definitewavelength
iii)
in contrast tosimple fluids,
incomplex
fluids the maximumgrowth
rate(the
maximumof
d~(/(- I/t) drops
tozero at the
spinodal
with a finiteslope, making
thespinodal considerably
moresharply
defined than in asimple
fluid. This should be found inexperiments
as well as in simulations '~
iv)
ingeneral,
the results of thesimple
Gaussiantheory (Cahn-Hilliard-Cook)
are in remarkablequalitative
agreement with the nonlineartheory.
However, the linearizedtheory
does notpredict
the non-monotonousgrowth
behavior ofd~i
which can be found on thecomplex-fluid
side of thephase diagram.
We
explain
the secondpoint
in somewhat more detail. While the unstable fluctuations in asimple
fluid have allwavelengths
up to a minimum value, we find that in acomplex
fluid thereis a restriction of these modes to a band of finite
wavelength,
with this bandnarrowing
down to zero width as the classicalspinodal
curve is reached. Motivatedby
this wetentatively
like tointerpret
our results in terms of an intermediate state which mediates thephase separation
on thecomplex
fluid side. As is reflectedby
its internal structure, thecomplex
fluid shows someaffinity
to a modulated, I-e- lamellarphase. Deeper
in thetwo-phase
coexistenceregion
thehomogeneous phase
becomesincreasingly
unstable to bothphase separation
and to the formation of a modulated structure. On a short time-scale theshort-wavelength
localordering
wins the
competition
with thelong-wavelength phase separation.
In some respects this issimilar to the
phenomenon
of simultaneousordering
andphase separation commonly
found inmetallic
alloys [191.
In the situation westudy,
however, thespinodal decomposition
leads to twohomogeneous phases.
To be morespecific
localordering
to some extentalready
takesplace beyond
thebinodal,
in the stablecomplex fluid,
since the internal structure has to establish itself.However,
theinstability
of fluctuations withordering
wavevectorpoints
towards a much stronger
ordering tendency
within thespinodal,
in the unstableregion.
Thus, the local order has to decreaseagain
in the later stages ofphase separation. Unfortunately,
due to ourapproximations
these are not within reach of ourstudy.
To
conclude,
we have shown that the internal structure in acomplex
fluidgives
rise to anumber of new,
interesting
effects inspinodal decomposition.
We expect that it wouldlikewise affect the nucleation and the
decomposition
at intermediate stages. A verycomplex demixing
behavior has forexample recently
beenreported
in thincopolymer
films[71.
Acknowledgements.
We wish to
acknowledge
Michael Schick forsuggesting
theproblem
and for valuable discussions. F. S. has received financial support from the DeutscheForschungsgemeinschaft.
R. B. wishes to thank the
University
ofWashington
for itshospitality during
a stay andacknowledges
supportby
the DFG under SFB 237. This work was alsosupported
in partby
Grant No. DMR9220733 of the NSF.
Appendix.
We
give
the result for the set ofcoupled equations
for the structure functionI
(k(Eq. 8))
and theone-point
distribution functional p ~''(Eq. (5))
t~
d~((k)
= 2
Ak~ ilk
A(k)
+a~
j
dq
q~S(q
A2(u~) (p
+ 2 a +2 ar
o
+
a~ (u~)k~
a + 2 Ak~ Tk~ (15)
d~p I'
'(u
= A
~
p
~'
'(u
F (u)
+k~
T~(
~~ ~~,
(16)
du a du
where
j lm»
(
(kF (u ~
= u dk
~ k A
(k
)2
ar~
o
(u~)
~m4
~(~
~
+ dk
~ k A~
[2 b(u
+ut~(u
)1 2ar~
o
(u-)
A[
u(p + a ) +(A~ Al
b(u)+ A~
t~(u
+ A2tap/ju(u)
and
with
a =
(ugj (u3j/ (u2j
2 dG(~ )/d~
= g(~
p
=((u~ t~(u )))/ (u~)
A~=
~ 5 k$~~
b(")
~
(~g)
(~~~(~~) )
1~4 ~k$ax
c~(u)
=f(u) (f(u)j u(uf(u)j/(u2j
In the derivation of the
equations,
the sum over wave vectors3~..
haseverywhere
been~
im~~
~ ~ ~ ~~~replaced by
theintegral (2
ar)-
dkk ; k~~~ =(6
ar la is an upper cutoff in whicho
a is a
coarse-graining length,
a free parameter of thetheory,
chosen to be of the order of the bulk correlationlength.
Instead of
solving
thepartial equation (16) directly,
we chose to consider the set ofordinary equations
for thehigher
moments(u~),
which can be derived from them. In order to control the arbitrariness involved in the choice of thecoarse-graining length
a and the number ofmoments included, we varied both and studied the effect on the results. Not
surprisingly,
thevalues for the
higher
momentsdepend
on a. The structure function itself remainsindependent
of a until the
higher
moments becomelarge compared
to thefirst,
and the calculation breaksdown. This
happens
the sooner, the smaller one chooses the value of a. On the other handa has to be small
enough
so that the structuresdeveloping during spinodal decomposition
are apparent. We foundk~~,
=
2.0 to be a reasonable choice for our model.
Furthermore,
theinclusion of eleven moments was found to be
sufficient,
since results varyonly
very littlebeyond
this value.References
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[lsl Note that in this treatment the total surfactant concentration is not conserved:
(~)
=
~~
(
[p + I (V~ )~ vi (~)l/v~).
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~)
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