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The interdependence of intra-aggregate and inter-aggregate forces
J.N. Israelachvili, D. Sornette
To cite this version:
J.N. Israelachvili, D. Sornette. The interdependence of intra-aggregate and inter-aggregate forces.
Journal de Physique, 1985, 46 (12), pp.2125-2136. �10.1051/jphys:0198500460120212500�. �jpa-
00210161�
The interdependence of intra-aggregate and inter-aggregate forces
J. N. Israelachvili
Department of Applied Mathematics, Institute of Advanced Studies, Research School of Physical Sciences, GPO Box 4, Canberra Act 2601, Australia
and D. Sornette
Laboratoire de Physique de la Matière Condensée (*), Université des Sciences, Parc Valrose, 06034 Nice Cedex, France
(Reçu le 6 mai 1985, accepté le 20 août 1985)
Résumé. 2014 Nous examinons l’interdépendance des forces responsables de l’association d’amphiphiles pour former des agrégats tels que micelles, microémulsions et bicouches et des forces s’exerçant entre de telles structures à courte distance. Nous présentons d’abord une analyse de l’origine et de la nature des forces d’hydratation entre têtes polaires qui prédominent à très courte portée. Un développement Landau-Ginzburg permet de relier naturellement la force d’hydratation
ausein d’un même agrégat à celle s’exerçant entre deux bicouches. Le potentiel d’interaction unique obtenu permet de démontrer la corrélation entre l’aire par tête polaire d’une bicouche isolée et la force de
répulsion entre bicouches. L’application de cette approche à d’autres systèmes est discutée.
Abstract
2014We examine the interdependence between forces responsible for the self-association of amphiphiles in
aggregates such as micelles, microemulsions and bilayers and the forces occurring between such structures when
they
comeclose together. We first present
atheoretical analysis of the origin and nature of the hydration force which
appears as the most important interaction occurring between head-groups at very short distances. A Landau-
Ginzburg approach allows us to link naturally the hydration force between the head-groups within an aggregate with that between two opposing bilayers. The single interaction potential obtained between amphiphilic head-
groups allows demonstration of
aquantitative correlation between the measured head-groups
areasof isolated
bilayers and the repulsive pressures between bilayers. The relevance of this interdependence to various other
phenomena is discussed.
Classification
Physics Abstracts
82. 70K - 82.65D
1. Introduction
The forces acting between amphiphilic structures (aggregates) such as micelles, bilayers, vesicles and microemulsion droplets in water determine many
important phenomena, for example, their stability to aggregation. in dilute solution, their phase behaviour
in concentrated solution, the thickness of soap films,
etc. By contrast, the forces acting between the same
amphiphilic molecules within these structures deter- mine the type of structure they self-assemble into, their shape, size, polydispersity and phase state, and in particular how these parameters are sensitive to changes in the solution conditions. For unlike solid
(i.e. rigid) colloidal particles, the forces holding amphiphiles together within aggregates are weak
(*) Laboratoire LA 190 Associe
auC.N.R.S.
(viz. van der Waals, screened electrostatic, and sol-
vation forces), which usually results in fluid-like struc- tures that change their size and shape when the solu- tion conditions, temperature, or surfactant concen-
tration is changed. These factors, however, are the same
as those that affect the forces between these structures
(or any colloidal particles in general).
The purpose of this paper is to investigate how the
intermolecular forces within amphiphilic aggregates
are correlated with the forces betweel aggregates, how this interdependence manifests itself in practical terms, and how it may be quantified.
While such correlations have been noticed before [1],
no attempts appear to have been made to consider their generality or their theoretical basis. The reasons
for this are twofold. First, the short-range electro- static, hydration and hydrophobic forces involved
are still not sufficiently well understood. Second,
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:0198500460120212500
theories of interparticle and intersurface forces are
often formulated in terms of some smeared-out surface property (rather than between the molecules consti-
tuting the surfaces). For example, a uniform surface
charge density in the case of double-layer forces [2],
or a uniform surface polarization density in the case
of hydration (solvation) forces [3, 4].
Further, the interface itself is usually modelled as a
discontinuous dielectric boundary. By so treating
surfaces as homogeneous planar discontinuities rather than made up of discrete molecular groups (amphi- philic head-groups, for example) it is not readily
apparent how the forces .between these groups can be related to the forces between the surfaces.
Note however, that these formulations are the result of mean field approximations and are not due
to an inherent assumption where one disregards the
direct interaction between the ionic head groups at the surface (1).
In this paper we adopt another approach where right from the start we assume that the forces between individual head-groups within aggregates are the same
as those that give rise to the net force between the aggregates. In other words, a single interaction
potential is postulated to describe both.
This work can be considered as an attempt to generalize to neutral systems what has been established for charged systems.
In section 2 we proceed with a theoretical discussion of the problem, and in particular we derive a simple expression for the repulsive hydration potential
between two head-groups. In section 3 we apply this potential in a detailed quantitative analysis of lecithin
bilayers, while in the final section 4 we discuss the broader implications of the results and show that there are many other systems to which the « principle
of interdependence » applies.
2. Nature of the interactions within and between aggregates.
2.1 THEORETICAL BACKGROUND. - First we consi- der the interaction forces between amphiphiles (sur- factants, lipids) within aggregates that determine the type of structure that they self-assemble into. This has been well described and reviewed in the literature
[ 1, 5] and only the essential features will be given here.
For amphiphiles whose hydrocarbon chains are in
the fluid state (i.e. surfactants above their Krafft point)
their optimum head-.group area ao is determined by a
balance of two « opposing forces » (6) acting mainly
in the interfacial head-group region. The attractive
(hydrophobic) energy contribution per molecule may be expressed as ya where a is the head-group area and
where y, the hydrocarbon-water interfacial (hydro- phobic) free energy, is in the range 20-50 mJ/m2
[1, 7-9]. The repulsive energy contribution per head-
(’) As pointed out by
areferee.
group may be expressed approximately as cla, where c
is a constant. The total energy per molecule is therefore ya + cla. This has a minimum value at a = ao
=ffi,
which gives the « optimal area » per head-group [1, 9].
For fluid hydrocarbon chains the optimal area should
be independent of the number of chains or the chain
length, as is indeed found experimentally [10, 12]
since the van der Waals attraction between chains
gives a very small contribution compared to these
two terms.
The optimal head-group area is a very important
parameter since (when it is taken together with the
chain volume and chain length) it determines the types of aggregates that are formed and many of their
physical and thermodynamic properties [1, 5, 9].
From the preceding paragraph it is also apparent that the head-group area ao is mainly determined by the repulsive forces between head-groups, since the attrac-
tive component y is more or less constant [7-9] while
the repulsive component c can vary greatly depending
on the nature of the head-group and the solution conditions. Let us therefore consider these repulsive
forces in more detail.
The repulsive forces between adjacent head-groups
within a fluid micelle, bilayer or monolayer, which
determine their head-group area, include electrostatic,
steric and solvation (hydration) interactions. Since all these interactions are occurring over very short distances (a few Angstroms, corresponding to the mean spacing between head-groups) their theoretical model-
ling is still at a rudimentary stage. Simple equations for
the lateral electrostatic (double-layer) pressure within the interfacial region of a single monolayer or bilayer
have been derived by Payens [ 13] and Forsyth et al. [ 14]
on the assumption of a smeared out surface charge,
and their interplay with the attractive interfacial force has been analysed by Parsegian [7] and by Wenner-
str6m and Jonsson [8]. The steric repulsion, which depends primarily on the sizes of molecules or mole- cular groups which may be modelled by hard spheres,
discs or cylinders [ 15] was first considered by Lang-
muir [16]. However, the important role of water of hydration in determining the effective head-group size, and/or its contribution to the inter head-group pair potential, does not appear to have been considered in the literature and is still unresolved.
Turning our attention now to inter-aggregate forces
we notice that the repulsive forces are fundamentally
the same as those between adjacent head-groups
discussed above, viz. repulsive electrostatic, steric and hydration forces. Consequently, one should expect a
correlation between intrabilayer and interbilayer for-
ces. For example, we might expect larger head-group
areas to be accompanied by larger repulsions between bilayers. This is borne out by experiments : the large hydration of the lecithin head-group results in a large
surface area of N 70 A2 as well as a large swelling in
fully hydrated lecithin multibilayers. By contrast the
head-group repulsion in phosphatidylethanolamines
is much less, which leads to a smaller head-group area
of 45-55 A2 and a much reduced swelling, viz. 10 A compared to about 25 A for lecithin [ 17,18]. We shall
consider other systems where such correlations occur
later. Here we proceed with a consideration of the three major types of repulsive inter-aggregate forces.
For simplicity we shall only talk about the forces between planar bilayers (while recognizing that the
same forces occur between micelles, vesicles, etc.).
The repulsive electrostatic double-layer force bet-
ween colloidal surfaces, lipid bilayers and across soap films is now well understood theoretically and it has
been measured in all three cases [19]. The importance
of steric repulsion between fluid bilayers is still
controversial [20], Huh [21] applied the theory of
Dolan and Edwards [22] to the interactions between oil in water microemulsion droplets where the pro-
truding hydrophilic head-groups on each surface
were considered to act as short polymer chains interacting via a repulsive osmotic (entropic) steric
interaction. Other steric contributions to the net
repulsion between bilayers would arise from local thermal fluctuations in bilayer thickness and head-
group area [23], and long wavelength elastic undu- lations of bilayers [24, 25]. Again, the effect of water of hydration in increasing the effective excluded volume of head-groups and in modulating the undu-
lation forces is to enhance their magnitude and
range [25].
Finally, we briefly mention the various theories that have been proposed to account for the strong exponentially repulsive « hydration >> force measured between lecithin bilayers [26]. The mean field theory
of Marcelja and Radic [3] later extended by Gruen and Marcelja [4] considers hydration forces in general as
due to the decaying polarization of water molecules
away from a surface, although a more realistic mole- cular dynamics simulation of this system [27] shows
that an oscillatory force is expected when the discrete molecular nature of water is taken into account Jonsson and Wennerstrom [28] proposed a highly specific theory (for lecithin bilayers alone) based on
the interactions of the zwitterionic (dipolar) head-
groups on one surface with their electrostatic images
« reflected >> by the other. Somette and Ostrowsky [24, 25] have extended a previous calculation by
Helfrich [29] and have derived general expressions
for the steric repulsion contribution arising from the
thermal undulation of elastic bilayers in the presence of other interactions. Note that these three very different theories each predict an exponential, or near- exponential short-range repulsion of magnitude and
range close to that measured, and we may also mention that the theory of Dolan and Edwards [22] also predicts
a short-range exponential steric repulsion between bilayers with freely mobile protruding head-groups.
(The one consolation for this state of affairs is that it is quite common in the history of science to find
completely different theories « explaining >> one obser-
vation
-a phenomenon that is known as the « inva- riance of current theories to current experimental
results ».)
However, we can make the qualitative remark that this uniformity of exponential behaviour in all theories
only reflects the existence of a well defined correlation
length (not necessarily the same for all theories) leading unambiguously to exponential decaying cor-
relation functions.
We shall return to consider the likelihood of these interactions again at the end of this paper. Here,
we shall continue with a more detailed analysis of the origin and nature of the hydration force since (i) it is
the least understood and yet appears to be the most
important (at least in contributing to the short-range repulsion between hydrophilic head-groups), and (ii) we require some formulation that naturally links
up the hydration force between head-groups (within
a bilayer) with that between two opposing bilayers.
2.2 A SIMPLE MODEL FOR THE HYDRATION INTERACTION BETWEEN HEAD-GROUPS.
-The physical origin of
this so-called hydration or structural force is not yet fully understood. It has long been recognized that
water is an associated liquid which has rather unique
solvent properties [30].
A qualitative concept, developed from the beginning
of colloid and surface science, underlines the impor-
tance of the modification of solvent structure near a
solute molecule. This perturbation propagates over
some distance from the solute molecule. When a
second solute molecule approaches, the total per- turbation of the solvent structure is changed, leading
to an indirect solvent mediated solute-solute inter- action.
A complete statistical mechanical treatment of
homogeneous water is extremely difficult (and all
the more so for inhomogeneous water) : indeed, the
structure of water is not determined by hard core
contacts and smooth attractive forces. Instead, water
constitutes an open structure akin to an imperfect
random tetrahedral network with oxygen atoms at the vertices and hydrogen atoms placed along the 0-0
bonds in configurations satisfying the ice rule, forming
the so-called hydrogen bonds. As a result, water forms
a structure where both position and orientation of
nearby water molecules are correlated. Theoretically,
one has thus to take into account both the transla- tional and orientational degrees of freedom and
analyse the way they are coupled
Some attempts have been made to derive general Landau-Ginzburg formalisms by expanding the
Ornstein-Zernike equation in the weak coupling limit
with the additional hypothesis that the interaction
potential between water molecules is short-ranged [31].
Marcelja et al. [31 have obtained an expression for the
free-energy density in terms of the density order
parameter. Realizing the incompleteness of this
approach, they have also proposed a generalized
Pople model for water focusing on an orientational order parameter, namely the average of the cosine of the angle measuring the deviation of either the lone
pair direction or of the OH bond from 0-0 line.
They also obtained in this case a Landau-Ginzburg expansion very similar to the density order parameter.
A similar formalism had been proposed previously by Marcelja and Radic [3] who considered the orientation effects of a planar membrane which polarizes the surrounding medium. This case may be simplified if
one assumes that the dominant effect of the pertur- bation of water structure is orientational ordering
of molecular dipoles and that the density variation
and dipolar polarization are decoupled.
The free energy expansion describing the solvent perturbation then reads
where Eo is the applied electric field, P
=XE, D
=sE and ~ is the corresponding correlation length.
This first approach has been subsequently put on a
firmer basis [4, 32] by showing that equation (1),
which implies a fixed local linear relation between the electric field and the dielectric polarization P, may be derived from a statistical ice-model of water with
Bjerrum defects.
The advantages of this type of approach are : a) The very difficult problem of determining the
translational and orientational correlation functions is replaced by the search for a continuous order parameter profile subjected to the condition that it minimizes the total free energy expressed as a Landau expansion. This LG expansion is extremely general
and has a wider validity than expected naively from
its derivation. It is essentially equivalent to the assumption of the Ornstein-Zernike form for the order parameter correlation function i.e.
where is the order parameter correlation length.
b) The unknown region where the interaction is strong (near a solute particle for example) which corresponds to a breakdown of the validity of the
weak coupling limit is subsumed in the boundary
conditions that one has to implement to the Euler- Lagrange equations derived from the minimization of the total free energy. Provided one can experi- mentally determine the boundary conditions (this
may be the difficult point) the problem is well-defined.
The continuous limit of the free energy density in
the LG expansion neglects the discrete nature of the solvent and should be ideally used only when relevant distances are larger than the molecular size. In this
limit, the variation of, say, an exponential sinusoidal
correlation function is averaged to an exponential.
However, even if the correlation length and molecular
separation are comparable we can still expect a qualitative description [31]. In the case of light solute particles or fluctuating fluid membranes, one expects
a smearing out of the molecular discrete structure of the solvent when averaging over time (or alternatively
over statistical configurations) with the result that the continuous description then becomes more rele- vant and appropriate.
We may then summarize the possible options for describing the solvation interaction between solute
particles as follows :
Conceptually, the notion of a disruption of water
structure by the presence of a solute molecule (or macroscopic body or surface) seems well established.
The difficulty remains in determining what is (are)
the relevant order parameter(s). The most likely
candidates may be the solvent density, the hydrogen
bonds density and the polarization density. The two
first order parameters are scalar whereas the last one
is a vector. This recognition already leads to an interesting conclusion : when applied to solute-solute
interactions, the LG formalism with a single scalar
order parameter can be shown to be unable to dis-
tinguish clearly between the case of non-polar and polar solutes, and always predicts an attraction [31].
One could argue that this results from the restriction to quadratic expansions of the free energy as a function of the order parameter as in equation (1). Indeed,
for large solute particles, it has been recognized that
the next quartic term, as well as a surface energy
density replacing the fixed boundary conditions usually imposed, are essential.
This surface free-energy which describes both the
change in coupling of the order parameter induced
by the presence of the surface and a possible surface
chemical potential, together with the bulk free energy
density, leads to the qualitatively correct description
of the very rich behaviour such as prewetting, first-
order and second-order wetting transitions [33].
However, it has been shown [34] that one always
expects an attractive contribution for the solvation interaction between like-solute particles in the case
of symmetric boundary conditions (i.e. identical on
the two solute particles). This result holds as long as
the scalar order parameters (say, molecular density
and hydrogen bonds density) are decoupled. This assumption is clearly questionable considering the highly correlated local orientational and translational order of liquid water. Indeed, it can be shown for the
case of two coupled, scalar, order parameters, that there exits suitable choices of the free energy density
and (symmetric) boundary conditions which lead to a
repulsive interaction.
Thus, within the hypothesis that the interaction between solute particles results from the disruption
of the density and hydrogen bonding of water mole- cules, we might conclude that the observed repulsion
can only emerge when fully taking into account of the
coupling between the two scalar order parameters.
The alternative description in terms of the vector polarization order parameter is richer since it embo- dies in a sense the density and hydrogen bonding description (to be precise, a full description of the
solvent is only attainable by defining all multipole
densities and not only the polarization profile) and
allows a simple treatment in terms of a single three-
dimensional order parameter.
In the following to be specific we use this repre- sentation. Let us consider a film of water bounded by
two infinite planes from which polar heads protrude
and occupy on the average the equilibrium area ao.
We assume that the planes are placed at the hydro- phobic-water interfaces and that the water molecules do not penetrate in the hydrocarbon core [35]. The
water disturbance can then be decomposed into two contributions, the hydrocarbon-water and the polar-
heads-water interactions. We assume for simplicity
and as a first approximation, that the structure of
water is mainly due to its interaction with the polar
heads. This hypothesis is clearly wrong when no polar
or ionic species are fixed on the surface as is the case
for hydrophobic surfaces immersed in water [36].
In this context, a new type of inter-aggregate force
has been measured, namely a rather long-range
attractive hydrophobic interaction which may be partly rationalized within the Marcelja’s type of models with a scalar order parameter and symmetric boundary conditions.
In the presence of polar or ionic species bounded
to the surfaces, we expect the electrostatic interaction to dominate.
We may now write the form of the generic total
Landau free-energy of the water solvent as :
where Vd is the water volume bounded by the two planes and the polar heads. Pj(r) is the j th component
of the polarization at r and f (P) is the free-energy density of a bulk solvent having a uniform polarization
P. The polarization profile actually carried by the
solvent minimizes Fd ~ P } and thus satisfies the Euler-
Lagrange equations :
This equation must be implemented by either a
surface energy term or surface boundary conditions.
Since we only want here to convey the main ideas,
we assume for simplicity that the polar-heads are spherical with radius R The more general case is
treated in the Appendix but the main qualitative
results are not changed by this hypothesis.
We further assume that the polar-head group- water interaction is modelled by a spherically sym- metric radial boundary condition (see Fig. 1). The polarization of a water molecule in contact with a
head-group is thus taken radial and of amplitude,
say Po (2).
Finally, as is often done in many-body problems,
we simplify the treatment by considering only two- body interactions and assume pairwise additivity of
forces. This last hypothesis is usually valid for large
distances or weak interactions but has been shown to
yield incorrect results for short distances, in a number
of cases [37].
Now, the interaction between two polar-heads is computed using a differential method. If the distance d between the two head-groups is increased by bd by introducing a fluid slice of thickness bd in the vicinity
of the medium plane between the head-groups, the
total free-energy of the solvent will change by the
Fig. 1.
-Configuration of two spherical polar heads sepa- rated by
adistance d + bd. The azimuthal angle T, not
represented,
measuresthe deviation of the plane Sl rS2
with respect to the reference xOy.
(2) This approximation is valid
aslong
asthe « extra=
polation
»length A is shorter than the correlation length ~.
(The extrapolation length is defined
asthe ratio between the coefficient of the gradient term and the coefficient of the
quadratic term of the surface free energy [44].) The physical
status of the extrapolation length
canbe clarified by relating
it to the range and anisotropy of the microscopic interactions in the bulk and
nearthe surfaces [44].
When A is not small compared to ~, the physical behaviour
at surfaces is governed by the interplay of these two charac-
teristic lengths. One can then show that expression (14) for
the interaction energy between spherical head groups
(derived in the limit h - 0), is still valid if ~ is replaced by j
function of ~ and ,1,. For d - ~, ~ takes
asimple form :
amount
which can be expressed as :
The notation Vd, Pd ... illustrates the fact that the volume of integration and the polarization profile
of the solvent are functions of
As shown on figure 1, we divide the volume into three parts, Vj, V2 and the slab of thickness 03B4d at x = 0
Then equation (6) reads
where x
=0 denotes the position of the central plane. We have used Vd
=V 1 + V2. The first integral can be
transformed using the fact that Pd +,5d(r) is only slightly different from Pd(r) :
The first term in the r.h.s. of equation (8) is nothing more than the functional derivative of Fd { P } with respect
to P at fixed volume Vd, and is zero as seen on inspection of the Euler-Lagrange equation (4).
The second term arises from the integration by part and the sign derives from the choice of the sense of the x-axis and recalling that the slab (3) is not in Yd. Equation (7) can then be written as :
Developing
allows to express 6F to first order in bd as :
The first term in the r.h.s. of equation (10) does not
contribute to equation (11) since it cancels out with the two contributions from x
=± 6dl2.
The pressure resulting from the interaction between the head-groups is simply
and F is computed up to an additive constant by integrating equation (11).
The calculation now requires the form of the polari-
zation profile P(x, r 1-) and of its first derivative. This is done in the appendix taking a specific model for the
free energy density [31 ] :
and using a superposition approximation which
amounts to saying that P(x, r.1) and its first derivatives
are given by the sum of their values computed for
isolated head-groups. We finally obtain
where d is the distance between the two head-groups
and where A is given by
R is the radius of a polar head (Fig.1 ).
We can now use this formulation equation (14), for
the hydration force, to link up the solvation force between head-groups (within a bilayer) with that
between two opposing bilayers.
3. Lecithin multilayer interactions.
Let us consider the hydration interaction between two
parallel bilayers. Within our model, an important contribution comes from the interaction between
pairs of head-groups, one sited in one bilayer the
second on the other one. Using the assumption of pairwise additivity, the total interaction energy per unit surface can be estimated by summing all pair
interactions between a given head-group on one
membrane and all head-groups on the other one :
ao is the equilibrium head-group area and p and r are
defined in figure 2. Using d 2 + p2
=r2, we obtain,
for the hydration interaction free energy per unit area
between two bilayers.
Now, we can estimate consistently ao by generalizing
the thermodynamic approach briefly recalled in § 2. l.
Arguing that the optimal head-group area ao is
determined by the balance between an attractive
hydrophobic energy and a repulsive energy which
Fig. 2.
-Schematic drawing of two opposing bilayers
adistance d apart whose head-groups occupy
amean (optimall
area
ao. Each head-group is assumed to interact with all
other head-groups via the
samepotential function of equa- tion (14) regardless of whether these head-groups
arein the
same
bilayer or the opposite bilayer.
origin is mainly of hydration nature, we write the free energy per head-group as :
where a is the hard-core diameter of a head-group.
The integral in equation (18) gives the sum of all pair hydration interactions between all head-groups in a bilayer and the head-group at the origin. Its expression
in equation (18) corresponds to the zeroth order term in a development of the free energy in powers of the
fluctuating part of the density [31]. ao is then given by
which yields
we can now replace expression (20) for ao in equation (17) and obtain :
where
The corresponding pressure is
with
Equations (22) and (23) constitute our main result Note that the repulsion between bilayers does not depend explicitely on the amplitude A of the hydration
forces between head-groups, but implicitely through
the dependence of the range ~ on A (or conversely through the dependence of A on ~ as seen for example
in Eq. (15)). Indeed, since G ~ A (Eq. (17)) and ao
ao - (Eq. (20)), it is clear that G should not
depend explicitely on A. In other words, this result
qualitatively says that when A increases (due to ion binding for example), ao increases so that the surface
density of head-groups decreases leading to an unchanged inter-bilayer interaction energy, if we
neglect the change of ~. Note however that for our
approach to be consistent, we should have added the energy given by equation (17) to the free-
energy per polar heads. This gives a correction of
d-(1
amplitude (2 e ~ ) times the hydration force comput- ed in equation (18) which is negligeable as long as
-r is larger than a few units.
However for smaller separation, the coupling
between bilayers as well as the correction terms involv-
ing the higher order contributions in power of the
fluctuating part of the density should become relevant and equation (22) should no more be valid. Let us now
examine quantitatively equations (22)-(23). We can
extract an order of magnitude for the pressure ampli-
tude no by taking y
=50
which yields 1011 dynes/cm’.
This is well within the experimental range [18].
Moreover, our model predicts that the pressure
amplitude is related to the hydration range ~ as shown
in equation (23). To test this feature, we have plotted
in figure 3, Log Ho as a function of 1 /~ which should
obey the following scaling form :
The grouping of the experimental points taken
from reference [18] on a straight line is rather remar-
kable considering the crudeness and level of approxi-
mation of the model.
The prediction (23) verified quite accurately in figure 3 thus presents strong evidence for the quanti-
tative correlation between the forces determining the
structure within a bilayer and those occurring between adjacent bilayers. This can be stated alternatively as
follows :
The decay length ~ varies from system to system in a way that correlates with the area per polar group.
However, in the Landau-Ginzburg theory presented
Fig. 3. - Plot of log 77o against I/j (where 1Io is in
dynes/cm2 and ~ in A) for eight different lecithins, egg PE, and lecithin-cholesterol mixtures, each in the fluid-state,
at 25 °C. The experimental data is from reference [18],
table I, which gives the repulsive hydration pressures
J7(J)
=no e-"/4 for these lipid bilayer systems (as well
asfor three other lipids, two in the frozen state and one at 50 °C - not included in this plot). The slope of the straight line yields
anestimate of the hard-core radius
(1 ’"8 A.
in § 2.2, ~ is identified as the correlation length and
should be constant for a given solvent at a given temperature (at constant pressure). This apparent
inconsistency is clarified in note (2) where the ~ used in equation (14) is argued to be related to the true correla- tion length and also to another characteristic « extra-
polation » length, function of surface quantities.
However, explaining in details the precise origin
of the change of the decay length ~ with each lipid system, would take us outside the scope of the paper and does not seem feasible without a careful analysis
of the direct water correlation functions in the bulk and near the disturbing surfaces.
An idea, analogous to the one discussed in this
paper, has been put forward very recently in the
context of phase separation of micellar solutions [38].
Regarding intermicellar interactions as resulting from pairwise interactions between amphiphiles of different micelles the authors of reference [38] have been able to demonstrate the existence of a link between self- association and phase separation via low-order mo-
ments of the micelle distribution using a classical thermodynamic approach.
Let us finally mention that our development in
section 3 can be applied also in the presence of other types of interactions (and not only hydration) as long
as they are short-ranged (i.e. showing exponential decay) and that the pairwise additivity approxima-
tion holds.
4. Discussion.
In the preceding sections we have argued that there are
good theoretical reasons for expecting the properties
of individual amphiphilic aggregates to be correlated with the forces between the aggregates. We have also shown that for lecithin and mixed lecithin bilayers
this manifests itself as a correlation between the head- group areas of isolated bilayers and the repulsive
pressure between two bilayers, and further that a single
interaction potential between amphiphilic head-
groups can account for both. In this case the correlation
was surprisingly good (Fig. 3) and it is unlikely that
such quantitative agreement would occur for other systems. Since the possible presence of other relevant interactions of different and longer range (double- layers forces...) may break down the simplicity of the previous analysis. However, we should expect at least qualitative correlations between various aggregate
properties and inter-aggregate forces and we now
consider some of these.
(i) We have already noted (Sect. 2) the correlation between the head-group area and amount of swelling
of lecithins (PC) and phosphatidylethanolamines (PE). We should also expect that the adhesion of two PE bilayers is greater than that of PC bilayers. This
indeed is the case [23].
(ii) All the examples so far have involved zwitte-
rionic head-groups. There are many other examples
involving both cationic, anionic and non-ionic head- groups where a reduction in head-group area results in increased inter-aggregate adhesion (due to a reduction
in inter-aggregate repulsion). Thus the head-group
area of the nonionic lipid DGDG is greater than that of MGDG, which correlates with the shorter-range repulsion and stronger adhesion of MGDG bilayers [39]. Analogous correlations occur in anionic lipid bilayers where in general a decrease in pH or addition
of divalent cations reduces the electrostatic head- group repulsion and hence the surface area per lipid,
and also leads to reduced bilayers swelling in multilayer phases and to increased adhesion of vesicles.
(iii) Note that any general correlation between
head-group area and inter-aggregate adhesion is
particularly interesting for self-assembly considerations since smaller head-group areas usually lead to larger
vesicles or inverted micellar structures (for doubled-
chained lipids), or larger micelles (for single-chained surfactants) [1]. Thus, aliphatic alcohols which are
often used as co-surfactants in microemulsion systems have a very small head-area (ao 20 A2). This causes
oil in water microemulsion droplets to increase in size when alcohol is added. Recently, Pashley and Mc Guiggan (private communication) have measured the
adhesion forces between adsorbed surfactant bilayers
and found that the adhesion increases significantly as
more pentanol is incorporated in the bilayers.
(iv) As a final example, the aggregation number of
anionic alkyl sulphate micelles increases as the elec-
trolyte is changed from LiCl -+ NaCl -> CsCI [40].
This implies a reduced head-group area which probably
arises from the reduced hydration repulsion of the
bound counterions as we go from Li + to Cs + . This correlates with the increasing adhesion between oil-in- water emulsion droplets, stabilized by alkyl sulphate monolayers, as monitored by the contact angles
between them [41]. Similar correlations occur for CTABr and CTACI micelles.
We conclude that many apparently unrelated properties of amphiphilic systems are correlated (interdependent), and that these correlations have
some sound theoretical basis. In the absence of a more
rigorous general theory to describe these correlations
quantitatively we propose that this phenomenon be
called the Principle of Interdependence of amphiphilic
systems.
The Principle of Interdependence should help in testing the validity of theories of hydration forces
between surfaces, since any such theory should be
at least consistent with interdependence. We may note in passing that the theory of double-layer forces is inherently consistent in this regard [13]. However, it
is not yet clear whether the theory of Jonsson and Wennerstrom [28] or that of Somette and Ostrowsky [25] satisfy the Principle of Interdependence since
neither tell us anything about the lateral interactions between amphiphiles. On the other hand any theory
of the entropic (steric) interaction between head-groups
must obviously satisfy the Principle, as does the
extension of Marcelja’s theory discussed in section 2 and applied in section 3.
It is also possible that the hydration force between
head-groups involves a combination of some of these effects. Thus, it is very likely that the intrinsic hydration
force is oscillatory, possibly superimposed on a
monotonic repulsion [42], and that the thermal fluctuations of head-groups and bilayers smear out the oscillatory nature of the force-law leaving a purely
monotonic repulsion that is enhanced by the thermal fluctuations (i.e. a combination of hydration and steric
effects [20, 23, 25]. However, these interesting develop-
ments take us outside the scope of this paper.
Appendix A.
In this appendix, we give the main steps leading to equation (14) in the text. As seen from equation (11),
in order to compute 6F/64 one has to estimate first the
polarization profile P(x, rl) and its first derivatives for the problem of two spherical head-groups distant
from d imposing a radial uniform water polarization Po on their boundary.
We first solve the case of a single sphere for the particular choice f(p) = 1 P 1. This form for the free energy density yields a linear differential equation
which allows in a second step to solve the two-spheres problem using a superposition approximation.
The Euler-Lagrange equation (4) then reads :
which must be solved with the boundary conditions
where R is the radius of the head-group.
The problem being spherically symmetric, it is
convenient to use spherical coordinates.
In this basis, equation (A .1) reduces to :
where Pr is the radial component of P, the other two angular component being zero.
Integration of (A. 2) is straightforward and gives :
Using the superposition principle, the two sphere
problem is solved immediately and within this approxi-
mation the polarization profile is given by :
The notations are defined in figure 1.
We are now interested in computing surface inte-
grals of P2 and its derivatives in the mid-plane x
=0.
For x
=0, 81 = 02 and ri = r2, expression (A. 4)
reduces to
Let us first estimate the integral
Using
and
we obtain
I I I I