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Field theory and polymer size distribution for branched polymers
T.C. Lubensky, J. Isaacson
To cite this version:
T.C. Lubensky, J. Isaacson. Field theory and polymer size distribution for branched polymers. Journal
de Physique, 1981, 42 (2), pp.175-188. �10.1051/jphys:01981004202017500�. �jpa-00208998�
Field theory and polymer size distribution for branched polymers
T. C. Lubensky and J. Isaacson
Dept. of Physics, University of Pennsylvania, Philadelphia, Pa. 19104, U.S.A.
(Reçu le 21 juillet 1980, accepté le 27 octobre 1980)
Résumé.
2014On donne une description de la statistique des chaînes polymériques basée sur des ensembles à l’équi-
libre dont les contraintes sont le nombre de dimères, de trimères et de polymères et celui des extrémités. On montre que cette description correspond exactement à une théorie des champs avec laquelle la distribution des tailles des polyméres peut être calculée. La théorie des champs, dans l’approximation de champ moyen en l’absence d’interactions répulsives, donne le seuil de gélation et la distribution des tailles des polymères en accord avec
ceux calculés par Flory et Stockmayer. On étudie les modifications de la théorie de Flory-Stockmayer dues à
l’addition d’interactions répulsives. Pour les ensembles à l’equilibre avec contraintes étudiés ici, les propriétés critiques de gélation et de percolation sont identiques.
Abstract.
2014The statistics of crosslinked polymer chains, produced by condensation of polyfunctional units, is
described by constrained equilibrium ensembles with fugacities controlling dimer, trimer, endpoint and polymer
number. It is shown that this description can be reproduced identically by a statistical field theory from which polymer size distribution functions can be calculated. The field theory, in the mean field approximation in the
absence of repulsive interactions, gives critical probabilities and polymer size distribution functions identical to those of Flory and Stockmayer. Modifications to the Flory-Stockmayer theory resulting from repulsive interactions
are studied. Within the context of the constrained equilibrium ensembles studied here, the critical properties of gelation and percolation are identical.
Classification
Physics Abstracts
05.90
-36.20
-61.40
-82.35
1. Introduction. - A gel is a polymer network
formed from crosslinked polymer chains [1, 2, 3].
The polymer solution before sufficient crosslinking
to produce a gel has occurred is a sol. The sol-gel
transition has been of interest to polymer scientists
for many years. The first theories of this transition
were formulated by Flory [4] and Stockmayer [5]
over thirty years ago and remain today the standards to which other theories are compared. Percolation is the formation of an infinite network in a random medium [6, 7]. It is most precisely defined in terms of a model in which sites (bonds) on a lattice are occupied with probability p and absent with pro-
bability 1
-p. Clusters are defined as groups of
adjacent occupied sites (or adjacent sites connected
by occupied bonds). Percolation occurs at a critical
probability, Pc, when an infinite cluster is formed.
It is now well established that percolation is precisely analogous to a second order thermodynamic phase
transition and is characterized by critical exponents and scaling functions [8, 9, 10]. Several authors have
pointed out the analogy between gelation and percola-
tion [6, 11, 12, 13, 14] and have noted that gelation
should be described by the same set of critical expo- nents as percolation. The purpose of this paper is to
explore this analogy in détail by showing that both
the classical gelation results of Flory and Stockmayer
and the modern critical percolation results can be
obtained from a model of reacting branched and unbranched polymer units. Our primary interest
will be to derive in some detail the field theory used
in reference [13], to reproduce the classical results,
and to explore how they are modified by the presence of repulsive interactions between polymer units.
Since the critical properties of percolation and branch- ed polymers have been studied in detail elsewhere [ 15, 16, 17], we will summarize, only briefly, the types of critical behaviour predicted by the field theory in the
last section. Those interested in more detail are referred to the original papers.
The development of a model for the sol-gel transi-
tion is complicated by the fact that there are many types of gels and many different paths to gelation.
Typically, gels are classified as weak (reversible)
or strong (irreversible) [2]. In weak gels, bonds can
break and reform. Thus, weak gels will have a vanish- ing zero frequency shear modulus, but a possibly significant finite frequency shear modulus. Weak
gels can often be created and destroyed by raising and lowering the temperature. In strong gels, bonds do
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01981004202017500
not break once they have formed. These gels will
have a non-vanishing zero frequency shear modulus.
The distinction between strong and weak gels is
useful but is probably only one of time scale. A strong gel may lose its shear modulus only at frequencies
below inverse days or weeks whereas a weak gel may show no significant shear modulus even at frequencies
of inverse seconds or higher. It is worth noting that
weak and strong gels are analogous respectively
to annealed and quenched random systems [18].
The network topology remains unchanged (quenched
or frozen-in) in the presence of external strains iri strong gels but relaxes in weak gels [19]. The theory
we present here will be applicable with proper inter-
pretation to both strong and weak gels.
A common path to the gel phase is that of conden- sation of polyfunctional units [1]. In this path, bifunc-
tional and polyfunctional units react in solution, eventually producing a gel. An alternate path is that
of vulcanization in which crosslinking units are added
to a solution or melt of linear polymers. In this paper,
we will concentrate on gelation by condensation
polymerization of bifunctional units which we call dimers and denote by A-A (Fig. la) and trifunctional units which we call trimers and denote by RA3 (Fig. lb). However our results can be shown to apply
to condensation with branched units of higher func- tionality. For simplicity, we will assume that all
.
reactive end groups, A, on both dimers and trimers
are identical. In this method of gel formation, average number densities, c2 > and C3)’ of dimers and trimers are introduced into solution. Before any reactions have occurred, there is a concentration
of unreacted or free ends groups. As time proceeds,
the concentration ( C1 > of free ends diminishes until
at long times, an equilibrium or quasi-equilibrium
state is reached. In strong gels, the final state is always
in the gel phase whereas in weak gels, it may be in the sol or gel phase depending on the temperature.
Fig. 1.
-a) A-A dimer; b) RA3 trimer.
Strictly speaking, the sol-gel transition (except
in the thermally driven transition in weak gels) is a dynamical transition that occurs at a critical time after reactions are allowed to begin. Thus many treatments of the sol-gel transition solve approximate
kinetic equations describing the chemical reactions among polymeric species [20, 21]. An alternate ap-
proach is to attempt to describe the system at each instant in time in terms of a statistical ensemble
characterized by densities (or chemical potentials)
of observable quantities. This approach has the virtue of simplicity, but there is no proof that it correctly
describes what actually goes on near the sol-gel tran-
sition. In particular, due to kinetic constraints, the system may get trapped in some region of phase space and be unable to probe all states satisfying specified
constraints as required by an equilibrium ensemble.
Nevertheless, the constrained equilibrium ensembles yield a very rich behaviour and should provide a qualitative if not quantitative description of the sol-
gel transition. It is straightforward, with modern
techniques, to incorporate repulsive interactions among dimers and trimers using the equilibrium
ensemble approach, but not so straightforward using
kinetic equations. In this paper, we will use the former
approach. The simplest and physically most reasonable
ensemble is one in which all states with given dimer,
trimer and endpoint densities c2, c3 and ci(t) occur
with equal probability. This is equivalent to a con-
strained equilibrium ensemble (which we will describe in a grand canonical formulation) with fixed average
Cl(t) >1 ( c2 > and C3). When repulsive inter-
actions and loop formation are neglected, the kinetic equations and the equilibrium ensemble equations
can be solved exactly and yield identical polymer size
distribution functions at equivalent densities of un-
reacted end groups. This result gives some confidence
that the equilibrium ensembles provides a realistic description of the sol-gel transition in strong as well
as weak gels even when loops and repulsions are
included. One can think of other constraints that
might be applied. Most are unphysical or mathema- tically intractable. We mention only one in which
the average total polymer concentration cp > as well
as ( ci ), C2 ) and C3 ) is fixed. This ensemble, though probably unphysical, is important in that
it can lead to significant variation of the critical exponents associated with gelation. In this paper,
we will describe the sol-gel transition, both that which
occurs as a function of time and that in weak gels
which is thermally accessed, in terms of these
constrained equilibrium ensembles.
In a complete treatment of statistical properties
of polymers in solution, polymer-solvent interactions have to be properly treated. In this paper, we will consider good athermal solvents in which the repulsive
interaction between polymeric units and the solvent
can be characterized by a single temperature inde- pendent short range potential u. The formalism we develop can, however, easily be extended to include solvent dynamical variables and to allow for different interactions between dimers and trimers. Thus, it is possible to generalize the present theory to discuss solvent-gel phase separation [22] or even to include
the possibility of dimer-trimer phase separation.
One important result of this paper is that the gel point
depends on u even in mean field theory in agreement
with Coniglio et al. [22].
The theory presented here, which follows earlier work of the authors [ 13], is a direct extension to branch- ed polymers of the work of de Gennes [23] and des
Cloizeaux [24] on linear polymers. It is similar in
spirt to earlier work by Edwards and Freed [25].
We develop, in terms of an ns component field tfJij,
a field theory whose partition function reduces to the partition function of the constrained equilibrium
ensembles describing the approach to gelation. We
note that these ensembles by their nature are poly- disperse. Although the presence of polydispersity is
sometimes considered a shortcoming of the field theoretic method of describing to the statistics of linear polymers [26], it is precisely what is required
for the polyfunctional condensation path to gelation.
For other paths, such as that of vulcanization from
a monodisperse melt of linear polymers, polydispersity
will be a problem. Presumably the methods of Schàfer and Witten [27] can be extended to treat other that
equilibrium distributions of branched polymers.
This paper consists of six sections besides the introduction. In section 2, we discuss the grand canor
nical formulation of the equilibrium ensembles for
reacting chemical species. In section 3, we discuss polymer size distribution functions for the equilibrium partition function and the generating function for the
polymer size distribution. In section 5, we study mean
field theory. In section 6, we review results published
elsewhere on critical properties of gels, and dilute
branched polymers obtained via renormalization group calculations. Finally in section 7, we summarize
our results.
2. Grand canonical ensemble. - As discussed in the introduction, we wish principally to discuss the process of gelation whereby dimers and trimers are
allowed to undergo chemical reactions. As the chemi- cal reaction progresses, large and complex polymeric
’ species are made. Eventually a sample traversing polymer is produced. We envision that the system
can be described instantaneously by a constrained
equilibrium ensemble in which the chemical potential
for reactive endgroups is fixed. In this case, the statisti- cal properties of the system can be described by a grand canonical ensemble with chemical potentials
for the various chemical species, J. For simplicity
we will restrict our attention to systems with only
dimers and trimers. A molecular species J is then specified by the number of dimers, n2, trimers, n3, and unreactive end groups, nl, and by its topology, r :
where we introduced the notation n,,, for the set (nl, n2, n3). Altematively using the relation
valid for each polymer where n, is the number of loops
in the polymer, we can write
For a solution in which the concentration of each chemical species is controlled, we must introduce a
chemical potential J.l( (J) for each u. Let N p( (J) be the
number of polymers of species J. We then have
where Tr signifies a trace over all dynamic variables,
H is the Hamiltonian of the system, and
Since we are primarily interested in the distribution of polymer sizes, we introduce the concept of a state, G, of the system specified only by the number of
polymers of each species can then be decomposed
into a sum for all possible states G :
where
and
where Z(G) is the classical partition function for the state G and S,, is a symmetry factor for species J.
In this paper we will be concerned exclusively with indistinguishable reactive endgroups. Monomers can
thus be visualized as (A-A) units and trimers as RA3
units shown in figure 1. Symmetry factors for various
simple polymers are shown in figure 2. In another
paper [28], we will discuss ARB2 trimers units and
Fig. 2.
-This figure shows asymmetry factors for various simple
polymers.
A-B dimers in which only reactions between A and B
endgroups are allowed.
To facilitate contact with the field theory to be presented in the next section, it is convenient at this
point to think of a ball and spring model for the
polymers that are formed as a result of reactions between A’s. Each ball in the interior of the polymer
will consist of a reacted pair of A’s whereas each terminal ball will consist of a single A as shown in figure 3. We will assume that classical statistics can be applied to each ball and measure all lengths
relative to the thermal wavelength
-of the interior A pairs, which we take to have twice
the mass, MA, of the external, A’s. We then have
where x(G)’ represents the co-ordinates of all A engroups, A bound pairs and central R groups, U(G)
the potential energy, N1(G) the total number of free ends and N3(G) the total number of trimers in state G. U can be decomposed into a part, Ub, measur- ing the elastic energy of links between A’s and links between A’s and the core group R, a part Ue measur- ing the energy of a free A relative to a bound A and
a part, Ur measuring the repulsive energy between
nearby groups :
As is customary, we assume short range repulsion
and write
where p(x ; G) is the density of A’s in G. Strictly speaking, pUr should include contributions from the central R groups. In this paper, we will assume that these contributions can be included by choosing u correctly. We note, however, that they play a central
role in any phase separation between dimers and trimers that might occur.
Fig. 3. - This figure shows a typical polymer. The large interior ball, labelled AA, is a bound A pair. The balls labelled R are core
groups and the smaller terminal balls represent single A endpoints.
Individual trimers are described by a potential
energy V 3(Yb Y2, Y3) where yi is the distance of
endgroup i from the core group. The potential bet-
ween A’s with separation y (either bound pairs or
free ends) not on a trimer are described by V2( y).
Finally we will choose the zero of energy so that a
free A has a positive potential V 1 relative to an A in a
bound pair. Assuming that bonds remain indepen- dent, Y2 and V3 remain unchanged as a result of
interactions between A’s, and we can write
where N2(G) is the number of dimers in G, and
The factors of 2 - d/2 and (MR/2 M A)d/2 in equations
(2.14a) and (2. 14c) result from the different masses
of the central R group and free A’s from the bound A
pairs.
When u is zero, Zrep is QNp(G) where Q is the volume
of the system and Np(G) the number of distinct poly-
mers in G. We therefore write
where Zrep
=1 when u
=0. Combining equations (2.6)-(2.15), we obtain
where
C(G) is the number of configurations in state G.
The partition function z in equation (2.15) allows
a specification of the concentration of each chemical
species, (1. In the usual situation, only the concentra-
tions of dimers and trimers are specified, and the system seeks chemical equilibrium with respect to all possible chemical reactions. In général, molecules (1 and (1’ can interact to produce a third molecule (1".
Q" can have an arbitrary topology, but the reaction must conserve dimer and trimer number and reduce the number of free ends by two. In equilibrium, we
must, therefore, have
for all possible Q, u’ and a". In addition, there must
be equilibrium with respect to reactions on a single polymer which change the number of free ends by
two :
M(nl, n2, n3; u)
=M(n, - 2, n2, n3; 6’) (2.19)
for all a and u’. Equations (2.18) and (2.19) imply
that
in equilibrium. Thus, as expected the initial concen-
tration of dimers and trimers are all that are needed to specify the final equilibrium ensemble.
In order to discuss the approach to the gel point,
we need to consider a sequence of ensembles in which the concentration of endgroups and/or polymers is
allowed to vary. This we do by introducing chemical potentials III and yp for end groups and polymers,
which allows us to fix ( cl ) and cp ). The grand partition function is then
In this equation, we have set
and
where Z’ signifies a sum over all states with
G
and
Alternatively, the number of free ends can be re-
expressed in terms of the number of loops via equa- tion (2.2) to yield
where NI(G) is the total number of loops in G and
From ’,-70 we can calculate averages of functions of the various densities. Let
and
Then we can express equilibrium averages over the states G as :
and
where the derivatives are taken keeping other fields constant. Fluctuations in densities can also be cal- culated :
where ôN,,,
=N(X - N(X) and 8Np
=Np - Np ).
The averages in equations (2.30bj and (2.31) involve
the total densities of dimers, trimers and endpoints, including those that might be members of the infi- nite molecule that is the gel. At a phase sepa- ration transition, some components of X(X,p would diverge. In this paper, we will not consider phase separation and will assume that gaz is small.
3. Polymer size distribution. - The gel transition
involves the formation of a sample traversing or
infinite molecule. As the transition is approached, larger and larger polymers form, and it is natural to
study the distribution of polymer sizes. Let cp( f n., } ; G)
be the density of polymers in the state G containing { na } units of type a. The state G occurs with proba- bility
so that the average value of any function O(G) of
the state G is determined by
In particular, the generating function for the polymer
size distribution can be written as
where the sum is over na
=0 to oo for every a. If
each h,,, is taken to be positive (even infinitesimal),
the term with n,,,
=oo is excluded from the sum. Thus f ({ ha }) generates statistics of finite polymers only.
f ({ ha }) can be used to determine moments of cp({ na } ; G) on finite polymers. In particular
The prime on the average brackets ( >’) emphasizes
that the averages are only over finite polymers.
S.,, is a generalization to multi-component molecules
of the mean square cluster size of percolation theory.
( cp y, y and Sa,fJ all depend on the fugacities s
and f wa } via their dependence on P(G). Alternati- vely they can be taken to depend on the total concen, tration )> and ( cp > with the aid of equa- tions (2.30). In most instances, there is no restriction
on the number of polymers formed so that s
=1
and ( cl >, C2 > and C3) are the only indepen-
dent variables.
The probability, p, that any pair of A units has reacted is just the total number of free ends that have reacted divided by the initial number of free
ends (eq. (1.1)) [1]. This is trivially given by
As time proceeds, p increases until the gel first forms when p
=Pc. p - Pc is a convenient measure of the distance from the gel point. In analogy with perco-
lation, we expect the moments of cp(j na }, G) to
display characteristic singularities near po. The den-
sity p,,, of units of type a in the infinité cluster grows
continuously from zero in the gel phase as [7]
The mean square cluster size in finite clusters diverges
both above and below Pc as
and the average number of finite clusters has the free energy singularity
The correlation length exponent vp can be intro- duced by looking at spatial correlations of units within a given polymers. For percolation, the hyper-
scaling relation d vp
=2 - ap where d is the spatial dimensionality holds.
More generally, one expects f ({ ha }) to scale like
a free energy density [10]
where Jp
=fi, + yp and where we have used thé result from section 4 that the crossover exponent for all values of a is the same. Equation (3.9) leads to
the familiar scaling relation
where d - (f3p + yp) and r
=2 + AP p f3 P and where for
simplicity we have h2 = h3 = 0 (similar expressions
hold for other cp(n2) > and ( cp(n3) > hold). We will
discuss the validity and limitations of this formula in section 6.
4. Perturbation theory and field theory. - Lt is
clear that a graphical perturbation theory for can
be developed along the lines discussed by Fixman [29]
for linear polymers in solution. As for linear polymers,
the fundamental propagator is that associated with
a free linear polymer :
where P n2(X, x’) is the probability that a free linear polymer with n2 dimers has one end-point at x and
the other at x’. Note that this sum includes point polymers with n2
=0. The Fourier transform of Gf
is easily evaluated yielding
where
The propagator Gf is represented graphically by a
dark line. As usual repulsive interactions are repre- sented by a dotted line with endpoints at xi and x2 that carries a factor u l5(Xl - x2). Three point branches
are represented by a wavy three leg vertex and carry
a factor
where xo is the co-ordinate of the central R group
and w3(x, x’, x") is defined so that
With these preliminaries, we can evaluate the parti-
tion function E, which includes all possible contri-
butions from point polymers (i.e. no dimers or tri- mers) with the aid of the following diagrammatic
rules.
1. Draw all possible graphs containing an arbi- trary number of polymers, 3-point branches and repulsive encounters. Sample graphs are shown in figure 4.
2. With each dark line associate a factor Gf(x, x’),
Fig. 4. - This figure shows some sample polymer graphs. Figure (a) represents a repulsive encounter in a linear polymer. Figure (b) is
a repulsive encounter between two legs of a branched polymer.
Figure (c) is a repulsive encounter between two branched polymers.
with each dotted line a factor u b(x - x’) and with
each 3-legged vertex a factor w3(x, x’, x").
3. Integrate over all co-ordinates.
4. Multiply each graph by a factor SNp(G) and l(G)
where Np(G) and N1(G) are the number of polymers
and free ends in graph G.
5. Divide each graph by the appropriate set of symmetry factors (S(1) to avoid double counting of
polymers.
.6. Sum contributions from all possible graphs.
The above rules yield the following contributions
to É from the graph shown in figure 5
Fig. 5.
-This figure shows the graphical representation of equa- tion (4.4).
Precisely the same set of diagrammatic rules [30] can be generated by the field theoretical representation for 5 introduced in reference [16]. Here we will introduce a generalized field theory in terms of an ns compo- nent field t/li,j (i
=1, ..., n ; j
=1,
...,s) with anisotropic potentials that will allow us to calculate both E and f
First we introduce the notation
Then, we have
where L is decomposed into a sum over four parts
L2 describes a Gaussian chain with a bond weight factor depending on the direction in the space of j indices :
where
L3 describes trimers :
where
L1 describes free ends :
Finally Lrep describes the repulsive interaction between A units :
It is straightforward to verify that
so that 8(s, s, { wa, wa }) is identical to 8(s, { wa, wa }) calculated from the perturbation rules just described.
Since the sum in equation (4.1) includes the term with n2
=0, both Ê"s count
N·point polymers consisting
Nof two
unreacted A’s at the same point in space. These can be removed by dividing ---’boy S(W2
=W3
=0), we therefore
define
where the w, without curly brackets signifies { W¡, W2
=0, W3
=0 }. From equation (4.8), it is clear that both
E and :E can be expanded in powers of (s - k) : 1
Note Fo does not depend of { Wa }. Fo(k
=s)
=Fo(s)
is clearly identical to equation (2.28) whereas the cluster generating function is
Thus both thermodynamic and cluster functions can
be obtained from the same field theoretical partition
function.
The expectation values of fluctuating fields or
order parameters play a central role in field theories
such as thàt described by equations (4.5) and (4.6).
Order parameters become non-zero as a result of external fields or as a result of a spontaneous broken symmetry. In our case the linear external field is in the 1-direction in the i-indices. It treats, however,
the first k components in the j index differently from
the remaining (s
-k). We, therefore, have
This, however is not the most useful choice of varia- bles. If hl = h2 = h3
=0, the (1, 1, 1, ..., 1) direction
in the j-indices is special, and it is convenient to
introduce an orthonormal transformation to a co-
ordinate system with one axis along this direction via the vector di satisfying [31]
The field t/J i,j can be expressed in the new co-ordinate system. Since the 1-direction in the i-index is special,
we write
Similarly the coupling to w 1 can be re-expressed as
where
It is thus clear that when °°°1°°1 # Wl, wl is composed
k
of a term along 1= 0 and one along £ alj. Introduc-
j=1
ing unit vectors
we have
where
and
We can similarly décomposez iPI > into parts
along e, and d, :
’
where we also derme
Unless otherwise specified, we will assume Qo and Ql
are evaluated at k
=s. Using the above définitions,
it is easy to see that
We are now in a position to relate field theoretical order parameters to the densities introduced in the
previous two sections. We will denote any quantity
evaluated at w2
=W3
=0 with a superscript zero.
Using the expression
we easily obtain
Similarly, we fmd
and
When w1= w1, pi = SW1(Q.i - Qf). Since there can
be no infinite cluster when w2
=W3
=0, we conclude
that Ql(wl
=Wl)
=0. Thus Q1 is proportional to
the density of endpoints in the infinite cluster
Because of the complicated broken symmetries
in the problem,
has five independent components for k # 1 and four independent components for k
=1 :
where ,11) and P(,,, are the projection operators and
Note that pIf) reduces to zero when k
=1. It is
now a straightforward exercise to show that
and
Since neither Go nor Gl have long range correlations,
it is clear that Gl is the divergent susceptibility asso-
ciated with gelation and Go with phase separation.
We close this rather formal section by defining the Legendre transformed generating function which , we will employ in the next two sections :
where it is understood that T also depends on w2,
w2, W3 and w3. r can be expanded in powers of
(s
-k) just as F yielding
The equation of state relating ( tJ¡’ > to wi is
From this, we can determine Qo and Q1 evaluated at
s = k via
Thus when k = s, Qo is a function only of wl, w2 and W3 and does not couple to Qi. Inverse correlation functions can also be calculated from r
5. Mean field theory. - In this section, we will study the properties of the gel transition in mean field
theory. This theory reduces identically to the Flory
theory [1] when uAp
=0. When uAp > 0, the gel point is shifted from the Flory value but, as expected,
the mean field critical exponents remain unchanged.
uAp
=0 corresponds either to having no repulsive
interactions between dimers or to the dilute limit.
(If uAp
=0 and 3 body interactions are included, Flory’s result is again not obtained.) Mean field
theory consists of neglecting spatial variations off
in the partition sum of equation (4.5). Using equa- tions (4.6) and (4.12), we obtain
where r
=1 - w2 from which we find
and
where,
and
The inverse correlation function are also easily cal-
culated. We find
where
L2 and i3 differ by terms of order (s
-k). Thus, in
mean field theory,
and
indicating that the gel point is determined by
The quantity (Qolwl) is finite and well defined for all values of wi : for wi - 0, it becomes Gl (eq. (4.27))
whereas for riz oo it saturates because of equa- tion (4.23). Therefore, usQ’ is zero if and only if uA p --_ uA p w 2 1
=0. This fact will be used for future classification of critical behaviour. Note that if
us > 0, r 0 is always greater than t’ indicating that
fluctuations in the total density (for example leading
to phase separation) are unimportant at the gel
transition. Note also that t° is determined by the total
densities ( ca ) independently of the existence of
large or infinite polymers.
The mean field equation of state determining Qo
and Q1 are
where
H 1 = (Wl - w 1) + (W2 - W2) QO + 21W3 W3) Q2 0 (Fl has a term linear in Q1. We have incorporated
this term into H -L so that I’(’) 1 is not equal q to Dr aQ 1V
Equation (5. 8b) is easily solved for Q1 to yield
Using equation (5.1), we then obtain
When uAp
=0, the equations for Ql and Q2 decouple, and it is more convenient to deal with these variable instead of Qo and Q1. For future refe- rence, we quote only the results for Q2(UAP
=0) :
Near the gel point, t°
=0, { hx }
=0, we can write
the singular part of j’ in a scaling form
Using t Î - ( p - Pc) (which we will verify in more
detail shortly) and comparing equations (5.12), (5.13), (3. 6), (3. 7) and (3.9) we obtain the usual mean field critical exponents for percolation
The density of high polymers can be obtained by Laplace transforming f 5;ng
This implies that r
=5/2 in mean field theory.
We now tum to a determination of the gel point.
Total densities can be obtained as discussed in section 3
by differentiation of Fo with respect to the appropriate fuagacities. In mean field theory, we have
where it is understood that Qo satisfies the equation
of state equation (5.8a). Thus, we have
These equations plus the équations of state for Qo
and Q’ 0 are sufficient to determine wi, w2, W3, 6o
and Q’ in terms of cl ), C2 ), C3 > and u. We
can, therefore determine the gel point to
=0 in
terms of initial densities and cl >. The general solu-
tion is somewhat complicated, and we will concen-
trate on the special case us
=0. In this case, Qo z wi and ( Cl )
=SW1(QO - wl). The equations can easily
be solved for the probability that an end group is on a
three functional unit,
and the probability that a reaction has taken place (eq. (3.5)),
Similarly we find
The gel transition is usually studied in terms of the
probability, a, that a branch originating at a given
trimer terminates at another trimer. Flory calculated a
for the dimer-trimer mixture we are considering and
found
Using equations (5.16), (5.17) and (5.7) (evaluated
at u
=0), we obtain
where Pc = (1 + p)-1 is the critical reaction proba- bility. Equation (5.20) shows that the gel point
occurs at a
=1/2 in agreement with Flory. When
us > 0, there is no compact way of writing t° in
terms of densities only. It is, however, instructive to write it in the following form
In the absence of the QI term, this expression agrees with that of reference [13] where point polymers were
included. Eliminating the point polymers causes the gel point to occur at a higher density of reacted end groups (smaller ( cp >).
We close this section with two observations. First,
it is clear that not only ( c 1 ) - ( ci 1’ but also C2 ) - C2)’ and C3 ) - C3)’ should grow continuously from zero above the gel point. This can easily be seen within the context 4f mean field theory.
We find when { ha }
=0
showing, as expected that both of the quantities grow
as (p - Pcfp for p > Pc. Second, as already remarked,
the mean field theory presented here is identical to the Flory theory when uAp
=0. To emphasize this,
we calculate the probability P1(n2, n3) that an arbi- trary selected unreacted endgroup is attached to a
polymer with n2 dimers and n3 trimers :
is just the coefficient of e - hl e - h3
in the expansion of
This is easily calculated using equation (5.12). We
obtain
which (using eq. (5.18)) is identical to equation (A. 2)
in Chap. IX of Flory’s book.
6. Beyond mean field theory. - It is now well
established that mean field theory breaks down below a critical dimension, dc. Critical behaviour in the vicinity of dc - e can be studied using the s-expan- sion which often suggests the type of scaling behaviour
to be expected for a general dimension. Different critical behaviours are associated with different renor-
malization group fixed points.
To calculate critical properties in the E-expansion,
one begins with the partition function defined in equations (4.5) and (4.6). Since tfJi,j) will always
have a non-vanishing value, we shift tfJ i,j via
The components of ({Ji,j with i > 1 are non-critical in the vicinity of the gel point (since their inverse propagators have no contributions from
We, therefore, eliminate them by integration and obtain a new action L’ that is only a
function of qJ lj or
In principal L’ should have potentials renormalized
by the non-critical degrees of freedom. We will ignore
this problem and write using the summation conven-
tion on repeated indices
where Lo
=QFMF and ri,l, apart from a constant rescaling factor is defined in equation (5.3) to (5.5)
FMF is the mean field free energy (eq. (5.1)) evaluated
at the actual values of Qo and Ql. Strictly speaking,
there should be additional third and fourth order terms, but they are irrelevant to our present discussion.
Even in cases where only units of functionality higher than three are present the reduced action
(eq. (6.3)) has the same symmetry as equation (6.3)
with an explicit third order term. Thus all critical behaviour as described below apply equally well to systems with higher functional units. All of the fixed
points and associated critical behaviour arising from
a s-expansion analysis of the above field theory have
been studied in references [15, 16 and 17]. Here we
will summarize the types of behaviour that can be
expected.
The symmetries of the fixed points are determined by the number of components of qi which are cri-
tical. These in tum are determined by which of thç potentials’ (appropriately shifted to include effects of interactions) 1"0’ 1" , i2 and 1"3 go to zero. We now list the various symmetry critical points that occur.
6.1 DILUTE BRANCHED POLYMERS (ANIMALS).
-All components of ({J’ are simultaneously critical. This
occurs only when uAp
=0. This critical point has dc
=8, and its properties within the E-expansion
were analysed in detail in reference [16]. There have
been also extensive series and Monte Carlo studies of statistics of animals [32-35]. The polymer size dis-
tribution behaves as
where is a constant and, 9 is a critical exponent that varies from 5/2 for d > de to unity for d
=2 [32].
1