HAL Id: jpa-00210354
https://hal.archives-ouvertes.fr/jpa-00210354
Submitted on 1 Jan 1986
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.
On the stability of polydisperse colloidal crystals
J.L. Barrat, J.P. Hansen
To cite this version:
J.L. Barrat, J.P. Hansen. On the stability of polydisperse colloidal crystals. Journal de Physique, 1986, 47 (9), pp.1547-1553. �10.1051/jphys:019860047090154700�. �jpa-00210354�
On the stability of polydisperse colloidal crystals
J. L. Barrat and J. P. Hansen
Laboratoire de Physique Théorique des Liquides (*),
Université Pierre et Marie Curie, 75252 Paris Cedex 05, France
(Reçu le 24 février 1986, accepté le 16 mai 1986)
Résumé. 2014 Le formalisme de la fonctionnelle de la densité est appliqué à l’étude de la stabilité mécanique et thermodynamique de cristaux colloidaux polydisperses. Les particules colloidales sont assimilées à des sphères
dures avec une distribution continue, p(03C3), de diamètres additifs. On montre que de telles solutions solides cessent d’être stables au-delà d’un degré de polydispersité critique, qui dépend de la forme de p(03C3), mais est toujours de
l’ordre de 20 %. Le problème de la détermination de la courbe de coexistence fluide-solide est brièvement évoqué.
Abstract 2014 The recently developed density functional theory of freezing is applied to an investigation of the
mechanical and thermodynamic stability of polydisperse colloidal crystals. The colloidal particles are modelled by hard spheres with a continuous distribution p(03C3) of additive diameters. It is shown that such solid solutions
cease to be stable beyond a critical degree of polydispersity, which depends somewhat on the shape of p(03C3), but is always of the order of 20 %. The problem of determining the fluid-solid coexistence curve is also briefly examined
Classification Physics Abstracts
05.20 - 64.70D - 82.70
1. Introduction.
Dispersions
of colloidalparticles,
like silica orpoly-
styrenespheres,
are known toundergo
a « disorder-order » transition from a disordered fluid
phase
to anordered
crystal
structure when the volume fraction of theparticles
or theelectrolyte
concentration in the solvent are varied[1].
Theresulting phase diagram
formonodisperse suspensions
has beenextensively
ana-lysed theoretically [1 ], generally
on the basis of the standard DLVO model for the interactions between colloidalparticles
incharge-stabilized dispersions [2].
However rather little effort has gone into
assessing
theinfluence of the unavoidable
polydispersity
ofparticle
diameters on the fluid-solid
phase
transition and onthe
stability
of the colloidalcrystal.
Theonly
availableinformation comes from the molecular
dynamics
simulations of small
samples
of 108 colloidalparticles
due to Dickinson and co-workers
[3].
The mainconclusion of that work is that
polydispersity
favours disorder, as one wouldintuitively
expect, and that the orderedphase disappears altogether
above a certaincritical
degree
ofpolydispersity.
For atriangular
dis-tribution of diameters, an
extrapolation
of the simu- lation datapredicts
the criticaldegree
ofpolydisper- sity
to be about 27% [4].
In this paper we examine the
stability
ofpolydis-
perse «solid solutions » in the framework of the modem
density
functionaltheory
offreezing [5].
Thepolydisperse generalization
of thetheory
is formulated in section 2 andspecialized
to the case of hardsphere
mixtures in section 3. This
specialization
is necessarysince detailed theoretical information on the
pair
structure of
multicomponent
fluids, a fundamentalingredient
in thedensity
functionaltheory,
is availableonly
for the hardsphere
model[6].
Results on thestability
of thepolydisperse
solidphase
aregiven
insection 4 for
triangular
andrectangular
distributions of diameters and variousdegrees
ofpolydispersity.
The theoretical
problems
associated with the deter- mination of fluid-solid coexistence ofpolydisperse
systems are
finally
discussed in section 5.2. Density functional formulation.
We consider a
polydisperse suspension
ofspherical
colloidal
particles
with diameters a distributed accord-ing
to agiven
normalized distributionp(a).
Letp =
N/ Y
be the total number ofparticles
per unit volume. It will prove convenient to introduce the fol-lowing
moments of the distribution of diameters :(*) Unite associ6e au C.N.R.S.
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:019860047090154700
1548
In
particular
the volume (orpacking)
fraction of theparticles
is :In the uniform fluid
phase
the localdensity Pa(r)
ofparticles
of diameters a iseverywhere equal
topO
=pp(a),
while thisdensity
has theperiodicity
of thecrystal
lattice in the solidphase. Denoting by Rj(l j
N) the lattice sites of agiven crystal
struc-ture, we assume the
density p,,(r)
in the solid solutionto be the sum of Gaussians centred on the
Ri :
Equation (3)
constitutes the obviousgeneralization
of the local densities used earlier to
study
thefreezing
of hard
spheres [7]
and of theirbinary
mixtures[8].
A local
density
of the form(3)
means thatparticles
ofspecies (i.e. diameter) a
are, on average, distributedat random on the N site of the
crystal
lattice.A convenient
starting point
of thedensity
func-tional
theory
is thefollowing
exactexpression
for thedifference between the Helmholtz free energy densities of the solid and fluid
phases
taken at the samedensity
and temperature, and for identical distributions of diameters :
with :
where P
=I lkB T
and Caa, denotes the direct correla- tion function betweenparticles
ofspecies
a and a’cor-responding
to a system with local densities :Equation (4)
is thestraighforward generalization
of theone and two-component
expressions
used in earliertheories of
freezing [7, 8].
The first term on the r.h.s. ofequation (4a)
is the ideal part of the free energy, while the interaction part involves acoupling-constant integration
over a linearpath
inone-particle density
space, in the manner first introduced
by
Saam andEbner
[9] (an
exhaustivepresentation
ofdensity
func-tional
techniques
isgiven
in the excellent reviewby
Evans
[10]).
Equation (4)
is exact; thepair
correlations embodied in the Caa,(r, r’; { pl’ })
are, however, ingeneral
unknown.
Systematic approximations
are obtainedby making
aTaylor expansion
of these functions around their uniform fluid valuescaa,(I
r - r’ I;{p2})
corresponding
to A = 0. Ifonly
the lowest order term is retained,caa,(r,
r’) ---caa,(I
r - r’ I;{p2}); higher
order terms of the
expansion
in powers of A involve three andmore-body
direct correlation functions of the uniform fluid, about which very little is known. For that reason theexpansion
is limited to lowest order, but, in an attempt to accountapproximately
for theneglected higher
order terms, the direct correlation functionscaa’
are taken to be those of an « effective » fluidhaving
the samecomposition { po },
and a totaldensity
padjusted
such that theposition
of the firstpeak
in the total fluid structure factor :coincide with the first
reciprocal
lattice vector of thesolid The
partial
structure factorsS,,,(k) appearing
in
equation
(5) are related to the Fourier transformsëaa,(k)
of the direct correlation functionsby
the usualOrnstein-Zernike
equations :
4
where
’haa,(k)
is the Fourier transform of thepair
correlation function
haa,(r)
=gaa,(r) -
1.With the above
prescription
forZ_,,
theapproxi-
mate free energy difference is now
given by
equa- tion(4a).
Thisexpression
is then minimized with respect to the widths a,, of the Gaussiansappearing
in the local
density (3),
for agiven
distribution ofdiameters, a
given
temperature T and agiven
totaldensity
p. The scenario which is observedalong
an isotherm, in similar studies of one or two-component systems(characterized by
one or two Gaussian widthsao)
isgenerally
thefollowing [7, 8].
Below somethreshold
density
p., the free energy f exhibits asingle
minimum for cx,, = 0,
corresponding
to a stable fluidphase.
Above p., f exhibits two minima, one forao = 0
(fluid)
and a second one for a. > 0; thissecond minimum is associated with a solid
phase
whereparticles
are localized around the latticesites { Ri }.
In a certain range of densities P- p pb, this second minimum is
higher
than the minimum cor-responding
to the fluidphase, signalling
that the solid ismechanically,
but notthermodynamically
stable(metastable
solidphase).
At stillhigher
densities(P > Pb),
the second minimumdrops
below the fluidminimum and the solid becomes the
thermodynami- cally
stablephase.
The fluid-solid coexistence isdetermined, as usual,
by equating
the pressures P andchemical
potentials
of bothphases.
In sections 3 and 4 we show that the bifurcation scenario whichwe have
just
described also occurs in apolydisperse
system of hard spheres; in section 5 we
point
out thedifficulties encountered if one attempts to determine the fluid-solid coexistence curve
[1 ].
3. The
polydisperse
hardsphere
model.In order to calculate the free energy difference
(4a) explicitly,
detailed expressions for the direct correla- tion functionscaa,(r)
of thepolydisperse
fluidphase
are
required
Such information is at presentonly
available for
polydisperse
mixtures of additive hardspheres.
Indeed,using
Baxter’s reduction of the Oms- tein-Zemikeequations
forfinite-range potentials [12],
Blum and Stell
[6]
were able to calculate thepartial
structure factors
Saa,(k)
of such mixtures in the Percus- Yevick(PY) approximation,
which is known to bereasonably
accurate for dense hardsphere
fluids. Thisapproximation supplements
the set of Omstein-Zemike
equations (6b) by
the closure relations :Equation (7a)
expresses the exactrequirement
thathard
spheres
of diameters a and Q’ must notoverlap,
while
equation (7b)
is the PYapproximation.
Theresults of Blum and Stell
[6]
can be used to obtain thefollowing
solutions forcaa,(r)
inside the hard cores(with a’
> a) :where x = r -
Å.aa’
and the coefficients a, band d canbe
expressed
in terms of the moments(1),
of thepack- ing
fractionq and of 4
= 1 - qaccording
to :The total structure factor, which is
required
to deter-mine the
density
of the effective fluid, asexplained
insection 2, is
finally
calculated fromequations
(6)and
(5). Examples
are shown infigure
1 fortriangular
and
rectangular
distributions of diameters.The lattice sites
{ Rj }
inequation (3)
are chosen tobe those of an FCC lattice, which is the stable structure for a
monodisperse
hardsphere
solid[7,
13]. Thiscompletes
thespecification
of theingredients
of our calculation, the results of which will bepresented
in thefollowing
section.Before that we
briefly
pause to examine the relevance of thepolydisperse
hardsphere
model for thestudy
of colloidal
crystals. Polydispersity
is an unavoidable characteristic of colloids and should hence be taken into account in any realistic calculation of thephase diagram.
The hardsphere
model is of course a crudeoversimplification
of the DLVO interaction between colloidalparticles,
which includes, besides a hard corerepulsion,
a screened Coulomb interaction and a vander Waals attraction. If the latter is
neglected,
andunder strong
screening
conditions(i.e.
in the presence of addedsalt),
the DLVOpotential
may bereasonably
well
approximated by
an effective hardsphere
interac-tion with
state-dependent
diameters, as isroutinely
done in the
theory
ofsimple liquids [14].
It should benoted that the FCC structure has been
predicted
to bethe stable one in the strong
screening regime, by
cal-culations based on a
repulsive
screened Coulombinteraction
[15]. Experimentally, charge-stabilized
col-loidal
crystals
are observed in theopposite,
weakscreening
limit, butcrystallization
ofuncharged
col-loidal
particles
has also been observed[17],
and the present hardsphere
modelapplies directly
to that case.Fig. 1. - Static structure factors (5) of the monodisperse
hard sphere fluid (full curve) and of polydisperse hard sphere fluids with triangular (dashes) and rectangular (dots)
distributions of diameters, versus reduced wavenumber,
at a packing fraction 17 = 0.5. The polydispersity parameter has the value 6 =.0.15 in the two polydisperse cases. The
structure factors are calculated in the PY approximation [6].
1550
4. Results.
We have carried out
explicit
free energy calculationsto determine the
density
range ofstability
and meta-stability
ofpolydisperse
hardsphere
systems withtriangular
andrectangular
distributions of diameters.Since we are
dealing
with hardspheres,
the results areindependent
of temperature. Thetriangular
distribu-tion is defined
by :
while the
rectangular
distribution isgiven by :
where 6 characterizes the
dispersion (2
6-a is the total width of eachdistribution)
and 7F =’1/’0
is the mean diameter,equal
to the median value in these symme- tric distributions. The calculations can in fact beeasily
carried out for any choice
of p( 0),
butonly
the distri- butions(l0a)
and (lOb) will be considered in the fol-lowing.
With these choices, and the forms(3)
and(8)
for the local densities and direct correlation functions, the
integrations
inequation (4a)
can be carried outanalytically,
thusgreatly simplifying
the minimizationpr’ocedure
with respect to the a,,. This minimization is mosteasily
carried out inpractice by discretizing
thedistributions
(l0a)
or(lOb)
andseeking
the minimumof Af with respect to n width parameters a;
by
a stan-dard
simplex algorithm.
The results turn out to bepractically independent
of n whenever n ;Z-, 10. In themonodisperse
case (ð = 0), we recover the results of Baus and Colot[7] :
the bifurcation occurs at apacking fraction tj
= 0.504beyond
which a secondminimum with rx #= 0
(metastable solid)
appears besides the fluid minimum (a = 0, Af =0).
Thesecond minimum
drops
below the fluid minimum for 11 = 0.548beyond
which the solid isthermodynami- cally
stable up to thevicinity
of closepacking ( r
=0.74)
where the second minimum
disappears abruptly.
A
qualitatively
similar behaviour is still observed when 6 isgradually
increased from zero. However theabrupt vanishing
of the second minimum takesplace
for
increasingly
lower values of thepacking
frac-tion
(2),
due to theoverlap
of thelargest spheres
athigh
densities; moreprecisely
the minimum of the free energy surface vanishes in the direction of the width parameter aQ associated with thelargest spheres.
Indeed, two
spheres
touch as soon as 0’ + a’ =aJ2,
where a =
(4/p)1/3
is the FCC lattice constant. Sincethe range of the direct correlation function
caa,(r)
is( 6
+c’)/2 (cf.
Eq.(7b)),
thecorresponding
contribu-tion to
Af
inequation (4a),
i.e.increases
sharply.
In themonodisperse
case this leadsto the
rapid
vanishing of the second minimum around j7 = 0.74, as mentioned earlier. In thepolydisperse
case, the contribution (11) is weighted
by
theproduct
p( 0-)p(a’)
whichcorresponds roughly
to theprobabi- lity
offinding
twospheres
of diameters a and Q’ onneighbouring
sites; thisweight
factorexplains why stability
is not lost as soon as ama. =Z(1
+b)
>al.,,12-,
and alsowhy
thetriangular
distribution has awider range of
stability
than therectangular
one.The
destabilizing
role of thelarge spheres
becomesvery apparent if the
expression (11)
is rewritten inreciprocal
lattice space. The local densities can beexpanded as sums over the vectors G of the
reciprocal
lattice
according
to :Substituting (12)
into(11)
we arrive at thefollowing
contribution of a (1 (1’
pair
to the free energy :A
typical
situation is shown infigure
2; the contribu- tion to (13) due to thelargest spheres
islarge
andposi-
tive at the second
reciprocal
lattice vector, which makes a sizeable contribution(large amplitude a,G)
to the local
density p,,(r).
As 6 is increased, the desta-Fig. 2. - Three partial direct correlation functions
(k)
(dashes),
-a C,,,,,(k)
(full curve) and"’êa2a2(k)
(dots) correspond- ing to the pairs of largest (a, =aj .and
smallest ( 62 = O"min) spheres in a polydisperse fluid mixture with a rectangulardistribution of diameters, and 6 = 0.15. The effective packing
fraction is fleff = 0.5 and corresponds to a solid solution
of tj = 0.56 according to the structure factor criterion explained in the text. The moduli of the first three reciprocal
lattice vectors of the FFC structure,
are indicated by arrows.
bilizing
contributions of thelarger spheres
to the freeenergy lead to a
vanishing
of the minimum for decreas-ing
values of q, as shown infigures
3(triangular
dis-tribution)
and 4(rectangular
distribution of diame-ters). This second minimum, associated with the solid,
vanishes
completely (i.e,
for all values of’1) beyond
6 = 0.16 for a rectangular distribution and
beyond
b N 0.21 for a
triangular
distribution of diameters; thelatter result is
roughly compatible
with Dickinson’s moleculardynamics
data[3,
4] discussed in the intro- duction.Beyond
these criticaldegrees
ofpolydisper- sity,
a solid solution isalways thermodynamically
andmechanically
unstable; this means that upon com-pression
of asufficiently polydisperse
colloidal sus-Fig. 3. - Range of stability of the polydisperse solid solution,
with a triangular distribution of diameters, in the plane of packing faction 17 versus polydispersity parameter 6.
The dashed curve delimits the region of mechanical stability,
while the full curve corresponds to the onset of thermody-
namic stability; the two types of stability vanish simul-
taneously at large values of 17 (upper. part of the stability range).
Fig. 4. - Same as figure 3, but for a rectangular distribution of diameters.
pension,
one should observe eitherglass
formationor
phase separation
into crystals with different com-positions.
So far our calculation has allowed us to mark the boundaries of
stability
of thepolydisperse
solid solu- tion. Theproblem
ofdetermining
the fluid-solid coexistence curve in apolydisperse
system is muchmore tedious in
practice,
and isbriefly
examined in thefollowing
section.5. Comments on the fluid-solid phase equilibrium
The
difficulty
instudying
theequilibrium
betweentwo phases of a
polydisperse
system lies in the fact that thecomposition (i.e.
the distribution ofdiameters)
is not, in
general,
the same in the twocoexisting phases.
If we denote the twophases by
A and B and thecorresponding
distributionsby PA( a)
andPB( a),
chemical
equilibrium
between A and B involves inprinciple
an infinite set ofcoupled equations,
express-ing
theequality
of chemicalpotentials
over the wholerange of diameters :
If some
easily
tractable(e.g. analytical)
form isavailable for the chemical
potentials,
theproblem
isusually
solvedby
discretization, i.e.by modelling
the
polydisperse
systemby
an n-component mixture,and
by solving
theresulting n coupled equations
[11, 16]. Such aprocedure
cannot beimplemented
in anypractical
way in the present case, because the varia- tional nature of our calculation renders the methodnumerically
untractable.The
problem
can besimplified
furtherby imposing
that the distributions PA and pB be members of a
given family p( a ; z) depending
on asingle
parameter z ; forexample
z could be taken to be theposition
of the top ofan
asymmetrical triangular
distribution, as shownin
figure
5.By
ajudicious
choice of thesingle
parameterone may
hope
to retain the essential features of thephase
coexistence, for instance thepossibility of having
a solid
phase
richer inlarge spheres
than the fluid, as isthe case in
binary
mixtures of hardspheres [8].
The compositions of thecoexisting phases
are now charac-terized
by
the values of thesingle
parameter z, zA and zB say.Equilibrium
between the twophases
must beexpressed
in a wayinvolving only
zA and zB. The total freeenthalpy
of the system is :where gA’ and gB
are the freeenthalpies
perparticle
in both
phases,
with distributionsPA( (1)
=P(a; ZI)
and
PB( (1)
=p(a; zB) respectively.
The total number ofparticles
of diameter 6 is :1552
Fig. 5. - Examples of asymmetric triangular distributions of diameters characterized by a single parameter z.
The
equilibrium
condition dG = 0 and the conserva-tion
equations dN( 0’)
= 0 take the form :As a consequence of the constraint
imposed
on the dis-tributions
p(a),
the conservationequations
(18) cannot be satisfiedsimultaneously.
Instead we look for anapproximate
solution that violates the conservation conditions(18)
asweakly
aspossible.
To this end weretain the
global
conditiondNA
= -dNB
and weseek two functions
A(zA, zB)
andp(zA, zB)
such that :and such that
be minimum with respect to variations of A and Jl.
The solution is :
À(ZA’ ZB) =
By
inserting equation (19)
into theequilibrium
condi-tion
(17),
andby separately equating
to zero the coef-ficients of
dzA
anddzB,
we arrive at a set of two equa- tions for zA and zB :It can be
easily
checked that in the case of abinary
mixture, where the distribution isentirely
characte-rized
by
thecomposition
parameter x =N -
z,the set of
equations (23)
reduces to the usual double tangent construction; in that case the minimum value of 6S isexactly
0.It is worth
noting
that the ideal gastermslp2 Log x (p2 A;),
which involve theparticle
masses ma in thede
Broglie
thermalwavelengths Aa,
cancel in equa- tions (23) if we express these masses as ma =a a’,
where a is
proportional
to the massdensity
of the mate-rial of which the colloidal
particles
are made. Thus equations (23) involveonly
T, P, zA and zB and may be solved toyield
forexample,
the value of the para- meter zB of thecrystal phase
which is formed when the temperature T is lowered at constant zA and P.In the present context such a calculation of the fluid- solid coexistence,
although
feasible inprinciple,
re-mains very cumbersome, and we made no attempt to
carry it
through,
but we believe that the method whichwe have
just
outlined may be useful in related pro- blems wherepolydispersity
is animportant
factor.Acknowledgments.
The calculations were carried out on the VAX 750 of Ecole Normale
Sup6rieure
with the support of the GRECO «Exp6rimentation Numérique».
References
[1] For reviews, see PIERA0143SKI, P., Contemp. Phys. 24 (1983) 25 and the proceedings of the Winter
Workshop on Colloidal Crystals, edited by P. Pie-
ra0144ski and F. Rothen, J. Physique Colloq. 46 (1985) C3.
[2] VERWEY, E. J. W. and OVERBECK, J. Th. G., Theory of Stability of Lyophobic Colloids (Elsevier, Ams- terdam) 1948.
[3] DICKINSON, E., Faraday Discuss. R. Soc. Chem. 65
(1978) 127.
DICKINSON, E., PARKER, R. and LAL, M., Chem. Phys.
Lett. 79 (1981) 578.
[4] DICKINSON, E. and PARKER, R., J. Physique Lett. 46 (1985) L-229.
[5] RAMAKRISHNAN, T. U. and YUSSOUFF, M., Phys. Rev.
B 19 (1979) 2775.
[6] BLUM, L. and STELL, G., J. Chem. Phys. 71 (1979) 42 and 72 (1980) 2212. See also VRIJ, A., J. Chem.
Phys. 71 (1979) 3267.
[7] BAUS, M. and COLOT, J. L., J. Phys. C 18 (1985) L 365
and Mol. Phys. 55 (1985) 653.
[8] BARRAT, J. L., BAUS, M. and HANSEN, J. P., Phys. Rev.
Lett. 56 (1986) 1063.
[9] SAAM, W. F. and EBNER, C., Phys. Rev. A 15 (1977)
2566.
[10] EVANS, R., Adv. Phys. 28 (1979) 143.
[11] SALACUSE, J. L. and STELL, G., J. Chem. Phys. 77 (1982) 3714.
[12] BAXTER, R. J., J. Chem. Phys. 52 (1970) 4559.
[13] COLOT, J. L. and BAUS, M., Molec. Phys. (in press).
[14] VICTOR, J. M. and HANSEN, J. P., J. Chem. Soc. Fara-
day Trans. II 81 (1985) 43.
[15] HONE, D., ALEXANDER, S., CHAIKIN, P. M. and PIN- cus, P., J. Chem. Phys. 79 (1983) 1474 ; HONE, D., J. Physique Colloq. 46 (1985) C3-21.
[16] DICKINSON, E., J. Chem. Soc. Faraday Trans. II 76
(1980) 1458.
[17] NIEUWENHUIS, E. A. and VRIJ, A., J. Coll. Int. Sci.
72 (1979) 321.
DE KRUIF, C. G., ROUW, P. W., JANSEN, J. W. and VRIJ, A., J. Physique Colloq. 46 (1985) C3-295.