arXiv:1406.1246v1 [cond-mat.soft] 5 Jun 2014
Theory of Polymer Chains in Poor Solvent: Single-Chain Stru
cture, Solution
Thermodynamics and
Θ
Point
Rui Wang and Zhen-Gang Wang
Division of Chemistry and Chemical Engineering,
California Institute of Technology, Pasadena, CA 91125, US
A
Using the language of the Flory
χ
parameter, we develop a theory that unifies the treatment of t
he
single-chain structure and the solution thermodynamics of
polymers in poor solvents. The structure
of a globule and its melting thermodynamics is examined usin
g the self-consistent filed theory. Our
results show that the chain conformation involves three sta
tes prior to the globule-to-coil transition:
the
fully-collapsed globule
, the
swollen globule
and the
molten globule
, which are distinguished by
the core density and the interfacial thickness. By examinin
g the chain-length dependence of the
melting of the swollen globule, we find universal scaling beh
avior in the chain properties near the
Θ point. The information of density profile and free energy of
the globule is used in the dilute
solution thermodynamics to study the phase equilibrium of p
olymer solution. Our results show
different scaling behavior of the solubility of polymers in t
he dilute solution compared to the F-H
theory, both in the
χ
dependence and the chain-length dependence. From the persp
ectives of single
chain structure and solution thermodynamics, our results v
erifies the consistency of the Θ point
defined by different criteria in the limit of infinite chain len
gth: the disappearance of the second
viral coefficient, the abrupt change in chain size and the crit
ical point in the phase diagram of the
polymer solution. Our results show
χ
Θ
= 0
.
5 (for the case of equal monomer and solvent volume),
which coincides with the value predicted from the F-H theory
.
I. INTRODUCTION
Flory-Huggins (F-H) theory is the cornerstone for poly-
mer solution thermodynamics
1
. The theory assumes
random mixing of ideal chains with solvent molecules,
and describes the polymer-solvent interaction by a phe-
nomenological parameter
χ
. Above the critical
χ
(or
equivalently below the critical temperature), the F-H
theory predicts phase separation of a polymer solution
into a polymer-concentrated phase and polymer-dilute
phase. From the F-H theory, des Cloizeaux and Jannink
2
found that the equilibrium polymer concentration in
the dilute phase well below the critical point scales as
ln
φ
∼−
(
χ
−
1
2
)
2
N
. The critical
χ
for polymer chains of
length
N
is given by
1
2
+
N
−
1
/
2
, and has the asymptotic
value of
1
2
as
N
approaches infinity. It is accepted that,
in the limit of infinite chain length, the critical point for
the phase separation of the polymer solution coincides
with the Θ point for the coil-to-globule transition of a
single chain
3–7
. Thus,
χ
Θ
=
1
2
in the framework of F-H
theory in the limit of infinite chain length.
The phase diagram calculated by the F-H theory shows
poor agreement with experiments and simulation for the
dilute phase and near the critical point: the F-H theory
predicts a much lower equilibrium polymer concentration
and a lower critical
χ
8–12
. An obvious fact that is not cap-
tured by the F-H theory is the large localized density fluc-
tuation in the dilute solution. The instantaneous picture
of the solution has much higher polymer density where
the chains are located and pure solvents elsewhere, which
is significantly different from the random-mixing picture
envisioned in the F-H theory. For polymers in poor sol-
vents, such localized density fluctuation takes the form
of single-chain globules and multichain clusters
13
. By
accounting for the large localized fluctuation, we showed
in previous work
14
that the solubility of the polymer in
the poor solvent is enhanced by several orders of magni-
tude relative to the prediction of the F-H theory – the
logarithm of the solubility scales with
N
2
/
3
rather than
N
as predicted from the F-H theory. The critical
χ
in
the phase diagram for polymers of finite chain length was
also shown to be pushed to higher values than
1
2
+
N
−
1
/
2
,
consistent with computer simulation and experiment re-
sults.
Another important fact not reflected in the F-H theory
is the change in chain conformation according to differ-
ent solvent qualities
15–23
. With increasing
χ
, an isolated
polymer chain will undergo the coil-to-globule transition
from the swollen coil (
R
g
∼
N
3
/
5
) in good solvent to
the ideal coil (
R
g
∼
N
1
/
2
) at the Θ condition, and fur-
ther to the collapsed globule (
R
g
∼
N
1
/
3
) as the sol-
vent becomes poorer. The coil-to-globule transition is a
unique property of macromolecules that is different from
the small molecules: even one macromolecule can form
a mesoscopic phase
13,24–26
. It is a fundamental problem
relevant to many interesting phenomena, such as protein
folding
27
, DNA packing
28
, gel network collapse
29
, and
interpolymer complexation
30
. The coil-to-globule transi-
tion of a flexible polymer is of second-order
25,31
: in the
limit of infinite chain length, there is a well-defined tran-
sition temperature known as the Θ point; whereas for the
chain of finite length, the transition occurs within the Θ
region of the width proportional to
N
−
1
/
2
. De Gennes
31
pointed out that the Θ point is a tricritical point, so
mean-field theory can be applied except for logarithmic
corrections
32,33
. For polymer chains with sufficient stiff-
ness, the coil-to-globule transition is predicted to become
first-order
23,34
.
Given that the F-H theory provides a poor description
2
of polymers in poor solvent, on consideration of both
the over-simplified physical picture in the theory and the
demonstrated inconsistency with experiments and simu-
lation, it is natural to question the validity of the Θ value
of
χ
predicted by the F-H theory. The
χ
parameter is a
general language for describing single chains, polymer so-
lutions, blends and block copolymers. The value of
χ
Θ
is
crucially important in polymer science and engineering,
because it serves as the benchmark to categorize differ-
ent polymer-solvent pairs. However, existing theories for
coil-to-globule transition are usually couched in the lan-
guage of either the viral coefficients
34–37
or the expansion
factor
31,38,39
, which makes it difficult to directly connect
the single chain behavior to the solution properties. Fur-
thermore, the second virial coefficient used in the study
of the single-chain behavior in previous work was ob-
tained from the F-H free energy of the homogeneous bulk
phase; the connection between this second virial coeffi-
cient and the effective two-body interaction at the level
of the single-chain Hamiltonian has not be elucidated. In
addition, the consistency of the Θ point defined by the
different criteria concerning different properties – the sec-
ond viral coefficient in dilute polymer solution, the single-
chain conformation, and the critical point in the phase
diagram of polymer solution in the limit of infinite chain
length – has not been theoretically verified. On the other
hand, computer simulation of the Θ point is challenging
due to the limitation of chain length
22,40,41
and numerical
accuracy. On the experimental side, there are ambigui-
ties in the structure of single-chain globule. For example,
by measuring the temperature dependence of the chain
size for an isolated polymer in aqueous solution, Wu and
Wang
17,18
suggested that the chain conformation before
the globule-to-coil transition involves two globule states:
a
fully-collapsed globule
and a
molten globule
, where, in
their words, quantitative description of the molten glob-
ule is still a challenge. They also found it surprising that
a fully-collapsed globule still contains 66% solvent inside
its volume.
The globule state of polymers has been theoretically
studied extensively by Grosberg and coworkers
13,34–37,42
.
Using the Lifshitz theory
25
, these authors have sys-
tematically elucidated the globule structure, globule-to-
coil transition, globule-globule interaction and the phase
equilibrium in dilute solution. The Lifshitz theory as-
sumes ground-state dominance and uses a virial expan-
sion of the local interactions. For both these two as-
sumptions to be satisfied, the globule must on one hand
have a sharp interface and on the other hand have low
monomer volume fraction in the core. The combination
of these two assumptions excludes a significant portion of
the parameter space in the globule state. In addition, the
globule structure in a poor solvent and the melting ther-
modynamics of a globule near the Θ point are studied
by using two different theoretical formulations, the for-
mer by using the Lifshitz theory and the later by using
Flory expansion factor. To complete the knowledge on
the globule state of polymers, it is desirable to develop a
theory that can describe the structural change of a glob-
ule in the full parameter space of the poor solvent, and
can unify the globule structure and the globule melting
in a single theoretical framework. In this regard, we note
that Ref.
42
showed that the expansion factor calculated
using the F-H free energy has a large discrepancy with
that obtained using the virial expansion. However, the
density profile of the globule and the surface energy or
its connection to solubility were not examined.
In an earlier paper, we developed a new theory in
the language of the F-H
χ
parameter that can unify
the description of the single chain structure and the so-
lution thermodynamics for polymers in poor solvent
14
.
There, we focused on the equilibrium cluster distribu-
tion, the solubility limit, and nucleation in the supersat-
urated state. In the current work, we apply the theory
to examine in detail the structure and properties of a
single-chain globule. In our theory, we employ the full
self-consistent field theory (SCFT) and treat the solu-
tion as incompressible, thus allowing us to describe both
a high-density globule and melting of the globule as the Θ
point is approached. From the chain-length dependence
of globule melting characteristics, we investigate the scal-
ing behavior and determine the value of
χ
Θ
by extrapo-
lating to the limit of infinite chain length. Because our
theory is capable of describing the phase equilibrium in
dilute polymer solutions, we also determine
χ
Θ
from the
solubility of polymers based on the intrinsic connection
between the single chain structure and solution property.
II. THEORY
The system of polymers in poor solvent is a collection
of globules and clusters. We study this structure of large
localized density fluctuation by focusing on a subvolume
of the entire solution that contains only one globule or
one multi-chain cluster
14,43,44
. The density profile and
free energy of the globule and clusters are obtained by
applying self-consistent field theory (SCFT) in the sub-
volume. This information is then used in the framework
of dilute solution thermodynamics to reconstruct the so-
lution behavior of the full system. To distinguish between
the composition within a single globule/cluster and the
overall bulk composition in the solution, we use the nota-
tion
ρ
and
φ
, respectively, to denote the volume fraction
of polymer in the globule/cluster and in the solution.
A. Self-consistent Field Theory for an isolated
globule/cluster
We consider a subvolume
V
consisting of
m
polymer
chains and
n
solvent molecules.
m
= 1 specifies the
single-chain globule. We treat the subvolume as a semi-
canonical ensemble: the number of polymers in the sub-
volume is fixed, whereas the solvent is connected with a
reservoir of pure solvent outside that maintains chemical
3
potential
μ
s
. (Here
μ
s
is defined relative to that of the
pure solvent.) The polymers are assumed to be Gaussian
chains of
N
Kuhn segments (with Kuhn length
b
). For
simplicity, the volume of the solvent molecule and the
chain segment are assumed to be the same
v
. The local
polymer-solvent interaction is described by the Flory
χ
parameter, and the solution is treated as incompressible.
The semi-canonical partition function can be written
as:
Ξ =
∞
∑
n
=0
e
βμ
s
n
m
!
n
!
v
Nm
+
n
m
∏
j
=1
∫
ˆ
D
{
R
j
}
n
∏
k
=1
∫
d
r
k
δ
(ˆ
ρ
p
+ ˆ
ρ
s
−
1) exp
[
−
χ
v
∫
d
r
ˆ
ρ
p
(
r
)ˆ
ρ
s
(
r
)
]
(1)
where
∫
ˆ
D
{
R
j
}
denotes integration over all chain config-
urations weighted by the Gaussian-chain statistics, and
∫
d
r
k
denotes integration over the solvent degrees of free-
dom. ˆ
ρ
s
(
r
) and ˆ
ρ
p
(
r
) are the local instantaneous volume
fraction of solvent and polymer, respectively. The par-
tition function Eq. 1 cannot be exactly evaluated due
to both the energetic interaction and the incompressibil-
ity constraint. We make the self-consistent field (SCF)
approximation, which involves (1) decoupling the inter-
acting system into a noninteracting chains in fluctuat-
ing fields by a identity transformation using functional
integration over the fluctuating fields, (2) replacing the
functional integration over the fluctuating fields by the
saddle point approximation. For systematic derivation
and numerical details we refer readers to the standard
literature
45,46
. The free energy of the system is then:
βF
m
=
∫
d
r
1
v
[
χρ
p
(1
−
ρ
p
)
−
ω
p
ρ
p
−
ω
s
(1
−
ρ
p
)]
−
m
ln
Q
p
−
e
βμ
s
Q
s
+ ln (
m
!)
(2)
Q
p
is the single-chain partition function in the field
ω
p
,
given by
Q
p
=
1
v
∫
d
r
q
(
r
, N
), where
q
(
r
, τ
) is the chain
propagator determined by the diffusion equation:
[
∂
∂τ
−
b
2
6
∇
2
r
+
ω
p
]
q
(
r
, τ
) = 0
(3)
with initial condition
q
(
r
,
0) = 1.
Q
s
is the single parti-
cle partition function of solvent in the field
ω
s
, given by
Q
s
=
1
v
∫
d
r
exp(
−
ω
s
). The density profile
φ
p
(
r
) and the
fields
ω
p
(
r
) and
ω
s
(
r
) are determined by the following
self-consistent equations:
ω
p
(
r
)
−
ω
s
(
r
) =
χ
[1
−
2
ρ
p
(
r
)]
(4
a
)
ρ
p
(
r
) =
m
Q
p
∫
N
0
dτq
(
r
, τ
)
q
(
r
, N
−
τ
)
(4
b
)
1
−
ρ
p
(
r
) =
e
βμ
s
exp(
−
ω
s
(
r
))
(4
c
)
By solving equations 3 and 4 iteratively
47
, we obtain
the equilibrium density profile and free energy of a glob-
ule/cluster in the subvolume.
B. Effective Two-body Interaction
If the polymer density in the subvolume is low, it is
convenient to integrate over the solvent degrees of free-
dom, which leads to effective interaction between two
polymer segments. Applying the identity transformation
for ˆ
ρ
s
together with local incompressibility, we recast the
partition function in Eq. 1 into:
Ξ =
1
m
!
v
Nm
∫
Dω
s
m
∏
j
=1
∫
ˆ
D
{
R
j
}
exp
[
−
∫
d
r
1
v
[
χ
ˆ
ρ
p
(1
−
ˆ
ρ
p
)
−
ω
s
(1
−
ˆ
ρ
p
)] +
e
βμ
s
Q
s
]
(5)
Because of the high volume fraction of the solvent, the
fluctuation of the field
ω
s
is small, and the functional
integration over
ω
s
in Eq 5 can be replaced by the saddle
point value, which yields
Ξ =
1
m
!
v
Nm
m
∏
j
=1
∫
ˆ
D
{
R
j
}
exp [
−
βH
]
where
H
is the Hamiltonian in the form of
βH
=
∫
d
r
1
v
[
χ
ˆ
ρ
p
(1
−
ˆ
ρ
p
) + (1
−
ˆ
ρ
p
)(ln(1
−
ˆ
ρ
p
)
−
1)]
−
βμ
s
v
(1
−
ˆ
ρ
p
)
(6)
Taking the reference such that
H
is zero in the reser-
voir of pure solvent outside the subvolume, we obtain
βμ
s
=
−
1. Eq 6 can then be written in the form of viral
expansion in terms of instantaneous volume fraction of
polymer segments as
βH
=
∫
d
r
1
v
[
(
χ
−
1)ˆ
ρ
p
+
(
1
2
−
χ
)
ˆ
ρ
2
p
+
1
6
ˆ
ρ
3
p
+
···
]
(7)
from which we identify the effective two-body interac-
tion as
1
2
−
χ
. Although this is the identical expression of
the effective two-body interaction commonly used in the
literature, the correspondence between the effective two-
body interaction and the F-H
χ
parameter in the previous
theories
1,3,13
was constructed for the
homogeneous, bulk
polymer solution; to our knowledge, this connection has
not been established at the level of single-chain Hamilto-
nian. Here we have provided an explicit demonstration,
based on a saddle-point approximation which amounts to
neglecting the concentration fluctuation of the solvent,
that the expression is valid at the single-chain level. If
one further includes the short-length-scale concentration
fluctuations, the
χ
parameter should more properly be
interpreted as the effective interaction parameter instead
of the bare interaction parameter
48,49
. Renormalization
group theory
4
showed that the second viral coefficient
of the polymer solution has corrections from the three-
body interaction. Grosberg and Kuznetsov
34
pointed out
4
that this correction vanishes in the limit of infinite chain
length. Therefore, both the effective two-body interac-
tion and the second viral coefficient vanish at
χ
Θ
=
1
2
for
infinitely long chain.
C. Phase Equilibrium
The density profile and free energy of the globule and
clusters obtained from SCFT can be included into the
framework of dilute solution thermodynamics to recon-
struct the bulk dilute polymer solution. The free energy
density of the entire solution with volume
V
t
, including
the translational entropy of clusters, can be written as
βF/V
t
=
∞
∑
m
=1
[
C
m
βF
m
+
C
m
(ln
φ
m
−
1)]
(8)
where
C
m
and
φ
m
are respectively the concentration and
volume fraction of the cluster with association number
m
(called
m
-cluster henceforth) in the solution.
F
m
is
the free energy of the
m
-cluster calculated by SCFT (ob-
tained as an excess free energy in the subvolume with
respect to the pure solvent). In Eq 8, we ignore the in-
teraction between different clusters on the assumption
that the solution is sufficiently dilute. The equilibrium
concentration of
m
-clusters can be obtained by minimiza-
tion of the free energy density in Eq 8 subject to fixed
total polymer concentration
∑
∞
m
=1
mC
m
, which results
in the following cluster distribution:
φ
m
= (
φ
1
)
m
exp(
−
β
∆
F
m
)
(9)
where ∆
F
m
≡
F
m
−
mF
1
is the free energy of formation
of the
m
-cluster from m single chain globule.
To study the coexistence between the polymer-poor
phase and the polymer-rich phase, we use Eq 8 with Eq.
9 to account for the large localized density fluctuation
in the polymer-poor solution, whereas the polymer-rich
phase is described by the F-H theory. The phase bound-
ary is determined by the respective equality of the chem-
ical potential of the polymer and the solvent in the two
coexisting phases, which results in
−
∞
∑
m
=1
φ
m
mN
=
(
1
−
1
N
)
φ
H
+ ln(1
−
φ
H
) +
χφ
2
H
(10a)
βF
1
+ ln
φ
1
= ln
φ
H
−
1 + (1
−
N
)(1
−
φ
H
)
+
χN
(1
−
φ
H
)
2
(10b)
where
φ
H
is the equilibrium volume fraction of polymers
in the polymer-rich phase and
φ
m
is the equilibrium vol-
ume fraction of the
m
-cluster in the dilute phase given
by Eq 9. The total volume fraction of polymers in the
dilute phase,
φ
L
, is given by
φ
L
=
∑
∞
m
=1
φ
m
.
III. GLOBULE STRUCTURE
In the poor solvent, a single polymer chain adopts a
compact globular structure due to the unfavorable inter-
action between the polymer segments and the solvent.
The increase in local segment density is countered by ex-
cluded volume (modeled by the incompressibility in our
theory) which prevents the globule from collapsing into
unbounded high density. Figure 1 shows the density pro-
file of a globule for different values of
χ
calculated by
SCFT. Clearly the globule can be divided into a core re-
gion with uniform density (denoted by
ρ
0
) and a surface
region. The globule core resembles a liquid droplet that
contains a number of uncorrelated parts of the chain. By
taking uniform fields
ω
p
and
ω
s
in equations 2-4, we ob-
tain the free energy in the globule core to be
βF
c
=
N
ρ
0
[
χρ
0
(1
−
ρ
0
) + (1
−
ρ
0
) ln(1
−
ρ
0
)] (11)
which is the Flory-Huggins free energy without the trans-
lational entropy of the polymer due to the fixed center of
mass. In the limit of large
N
, the Laplace pressure due to
curvature can be neglected, and the polymer density of
the globule core can be obtained approximately by bal-
ancing the osmotic pressure inside the globule with that
of the pure solvent outside (
≈
0), which yields
ρ
0
as the
nontrivial root of the following equation
50
ρ
0
+ ln(1
−
ρ
0
) +
χρ
2
0
= 0
(12)
For
χ
close to 0.5, Eq 12 has the symptomatic solution of
ρ
0
≈
3(
χ
−
0
.
5). As shown in Figure 1, the core density
becomes lower with the decreasing
χ
, which increases the
size of the globule as a result of swelling. At the same
time, the interfacial region becomes thicker and more dif-
fuse. We see from Figure 2 that the thickness of the in-
terfacial region scales with the Kuhn length
b
as pointed
out by Grosberg and Khokhlov
13
and is independent of
the chain stiffness parameter
p
=
b
3
/v
. Because the de-
pendence on
p
is relatively straightforward, in most of
the subsequent discussions, we choose a specific
p
corre-
sponding to
v
= 4
πb
3
/
3.
Based on the density profile, we can define the radius
of gyration (
R
g
), the core radius (
R
0
) and the surface
diffuseness (
h
) to characterize the globule size, which are
given as:
R
g
=
(
∫
∞
0
r
2
ρ
(
r
)4
πr
2
dr
∫
∞
0
ρ
(
r
)4
πr
2
dr
)
1
/
2
(13a)
R
0
= (3
/
5)
1
/
2
[3
Nv/
(4
πρ
0
)]
1
/
3
(13b)
h
=
R
g
−
R
0
(13c)
R
0
is the radius of gyration for a uniform sphere with
polymer density
ρ
0
that contains the same total amount
of chain segments as in the globule; in other words,
r
=
(5
/
3)
1
/
2
R
0
is the location of the Gibbs dividing surface.
h
describes the deviation of the globule from the uniform
sphere, thus characterizing the diffuseness of the globule
surface. It should be noted that
h
is not a linear measure
of the true thickness of the globule surface (denoted by
h
T
) within which the polymer density changes from
ρ
0
5
0
1
2
3
0.0
0.2
0.4
0.6
0.8
1.0
=0.54
=0.77
(r)
r/(N
1/3
b)
=2.0
FIG. 1. Density profile of a globule for three values of
χ
with
N
= 10
4
and
v
= 4
πb
3
/
3.
ρ
(
r
) is the local volume fraction
of polymer with
r
the radial axis starting from the globule
center.
0
1
2
0.0
0.2
0.4
0.6
0.8
1.0
0.0
0.2
0.4
0.6
0.8
(r)
r/(N
1/3
b)
b
3
/v
5
1
3/(4
)
(r)
FIG. 2. Effect of the chain stiffness parameter
p
=
b
3
/v
on
the density profile of a globule with the same Kuhn length.
χ
= 0
.
77 and
N
= 10
4
. The insert shows the overlap of the
interfacial region when the density profiles are shifted.
to 0. Dobrynin and Rubinstein
51
pointed out that the
surface thickness of the globule has a length scale of one
thermal blob
h
T
∼
b/ρ
0
. For a globule with a large
uniform core (i.e.,
h
T
/R
0
≪
1), it can be shown that the
surface diffuseness scales as
h
∼
h
2
T
/R
0
.
52
In this work,
we choose
h
rather than
h
T
to characterize the globule
surface because
h
is defined based on
R
g
, which is an
experimentally measurable quantity.
With the definition of
R
0
and
h
, we can separately
examine the volume contribution and the surface con-
tribution to the globule size. The core density and the
globule size as a function of
χ
for polymer with
N
= 10
4
are shown in Figure 3. When
χ
is well above 0
.
5,
R
g
coin-
cides with
R
0
while
h
remains very small and is negligible
compared to
R
0
. The globule surface is of the thickness
of one thermal blob (
h
T
∼
b/ρ
0
,
h
∼
bρ
−
5
/
3
0
N
−
1
/
3
), and
the entire globule is space-filled by
∼
ρ
2
0
N
thermal blobs.
In this regime, the globule can be envisioned as a uniform
sphere: the increase of the globule size as
χ
decreases is
due to the swelling of the globule core (see Figure 3b),
given by
R
g
≈
R
0
∼
(
Nv/ρ
0
)
1
/
3
. As
χ
approaches 0
.
5,
R
g
increases rapidly and deviates from
R
0
. At the same
time,
h
increases sharply and becomes comparable to
R
0
.
The thermal blob expands, reaching a size comparable
to the whole globule. The rapid increase of the globule
size in this regime indicates melting of the globule, which
takes place by both the swelling of the globule core and
the widening of the interface.
The
χ
dependence of the globule size and core density
shown in Figure 3 suggests that the single chain con-
formation prior to the globule-to-coil transition involves
three states: the
fully-collapsed globule
, the
swollen glob-
ule
and the
molten globule
, in the order of decreasing
χ
. For large
χ
(
χ >
1), the globule is fully-collapsed,
with core density close to one and a sharp interface:
ρ
0
≈
1,
h
T
/R
0
∼
N
−
1
/
3
and
h/R
0
∼
N
−
2
/
3
. The fully-
collapsed globule can further transform to the ordered
solid-globule as pointed out by Zhou et al.
53
, which is
out of the scope of this work. In the intermediate regime,
where
χ
−
0
.
5
≪
1 but (
χ
−
χ
Θ
)
N
1
/
2
≫
1, the globule is
swollen. The core density is significantly lower than one,
while the interfacial thickness is still narrow compared to
the core radius:
ρ
0
<<
1,
h
T
/R
0
∼
[
(
χ
−
χ
Θ
)
N
1
/
2
]
−
2
/
3
,
h/R
0
∼
[
(
χ
−
χ
Θ
)
N
1
/
2
]
−
4
/
3
. Finally in the Θ regime,
where (
χ
−
χ
Θ
)
N
1
/
2
∼
O
(1) or less, the globule is molten,
with a very dilute core, comparable to a Gaussian coil,
and an interfacial thickness comparable to the core ra-
dius:
ρ
0
∼
(
χ
−
χ
Θ
)
∼
N
−
1
/
2
,
h
T
/R
0
∼
O
(1), and
h/R
0
∼
O
(1).
That the globule structure may involve more than one
states has been suggested before. Wu and Wang
17,18
pro-
posed that the globule structure involves two states: the
fully-collapsed globule and the molten globule, based on
the consideration that the ratio between the radius of
gyration and hydrodynamic radius for the fully-collapsed
globule is (3
/
5)
1
/
2
whereas this ratio for the molten glob-
ule is smaller than (3
/
5)
1
/
2
(this criterion is equivalent
to whether the globule has a sharp or diffuse surface).
However, the “fully-collapsed” globule observed in their
experiment contains 66% solvent inside the globule vol-
ume, which is more properly considered as the swollen
globule in our definition. If we choose
χ
= 1 as the cri-
terion for separating the swollen globule from the fully-
collapsed globule, then the range of the swollen globule is
roughly between
χ
Θ
and
χ
= 1 for large
N
; this can cor-
respond to a large temperature window in experiments.
The swollen state for the infinitely long chain persists all
the way to the Θ point, as we discuss below.
6
FIG. 3. a) Radius of gyration (
R
g
), core radius (
R
0
) and in-
terfacial diffuseness (
h
) and b) core density(
ρ
0
) of the globule
as a function of
χ
with
N
= 10
4
. The schematic inserted in
a) represents the three states in globule structure: the
fully-
collapse globule
, the
swollen globule
and the
molten globule
.
It is instructive to note an analogy between the swollen
globule and the semidilute polymer solution in good sol-
vent. The existence of both these states is due to the
long chain length. Indeed the molten globule, the swollen
globule and the fully-collapsed globule can be consid-
ered the respective analogues of the dilute, semi dilute,
and concentrated solutions. Just as there is no clear-
cut boundary between the semidilute and concentrated
solutions, the distinction between a swollen globule and
fully collapse globule is not a sharp one. And just as
the concentration range for the dilute regime becomes
narrower as the chain length increases, so the region of
the molten globule shrinks with increasing chain length.
Likewise, with decreasing chain length, the window for
the existence of the swollen globule shrinks, and eventu-
ally disappears for very short chains.
We should emphasize that the density profile of the
globule is calculated using the flexible Gaussian chain
model. If the thickness of the globule surface becomes
comparable to the Kuhn length, which happens for very
large
χ
, the chain segments can become oriented by the
interface. In that case, the flexible Gaussian chain is no
longer a valid description and chain rigidity and local ne-
matic order may have to be accounted for explicitly
54
.
However, we find that for
χ
= 1
.
0 (with the core den-
sity
ρ
0
= 0
.
7) the interfacial width is
h
T
= 5
b
and is
h
T
= 10
b
for
χ
= 0
.
77 (with the core density
ρ
0
= 0
.
52).
The interfacial width decreases to the Kuhn length at
about
χ
= 2
.
0, corresponding to a core density
ρ
0
= 0
.
93.
Therefore, there is a significant range of parameter space
in which the Gaussian chain model remains valid.
IV. DETERMINING
χ
Θ
FROM THE
SINGLE-CHAIN GLOBULE
The globule structure obtained by our SCFT calcula-
tion is valid under the condition that the surface energy
of the globule is much larger than
kT
; otherwise shape
fluctuation must be taken into account and the assump-
tion of spherical symmetry becomes questionable. This
condition is equivalent to the requirement that the num-
ber of thermal blobs
ρ
2
0
N
must be large, i.e.,
ρ
2
0
N
≫
1.
To satisfy this requirement, the globule state should be
within the parameter space (
χ
−
χ
Θ
)
N
1
/
2
≫
1, i.e., the
chain should be in the fully-collapsed or swollen globule.
(Equation 17b provides a more quantitative Ginzburg cri-
terion.) This requirement would at first seem to prevent
us from applying the theory to the close vicinity of the Θ
point. However, as the chain length increases, the width
of the Θ region (in
χ
) shrinks and the transition becomes
increasingly sharper
23,31,34
. In other words, the state of
the swollen globule persists closer to the Θ point. In the
limit of infinitely long chain, the swollen globule persists
all the way to the Θ point. Therefore, the chain length
dependence of the melting of the swollen globule can be
used to probe the width of the Θ region and the location
of the Θ point.
0.5
1.0
1.5
2.0
0.00
0.02
0.04
0.06
0.08
0.10
h/R
0
N
10
3
2
10
3
5
10
3
10
4
FIG. 4. The ratio between the surface diffuseness and the core
radius (
h/R
0
) as a function of
χ
for different chain length.
Figure 4 shows the ratio between the surface thickness
and the core radius of the globule (
h/R
0
) as a function
of
χ
for several different chain lengths. As
χ
decreases
close to 0.5,
h/R
0
exhibits a rapid rise as a result of the
melting of the globule; this rise is sharper for larger
N
.
7
From Figure 4, we can define the onset of the melting
(denoted by
χ
N
(
λ
)) as the value of
χ
at which
h/R
0
reaches a threshold
λ
.
χ
N
(
λ
) thus represents the onset
of the globule-to-coil transition as well as the boundary of
the Θ region on the globule side. Clearly,
χ
N
(
λ
) depends
on chain length. Figure 5 shows the linear relation of
χ
N
(
λ
) versus
N
−
1
/
2
for three different levels of
λ
; this
linearity demonstrates that the width of the Θ region
is proportional to
N
−
1
/
2
, in agreement with the results
from the scaling argument
31
and simulation
22
.
0.00
0.01
0.02
0.03
0.50
0.55
0.60
0.65
0.70
=5%
=7%
=9%
N
(
)
N
-1/2
FIG. 5. The onset of globule melting
χ
N
(
λ
) plotted vs
N
−
1
/
2
for three different
λ
. Points represent the results calculated
by SCFT. Straight lines are the linear fit to the points. Three
lines intersect to a common point as
N
→ ∞
, which yields
χ
Θ
= 0
.
5.
As
N
increases,
χ
N
(
λ
) for the different choices of the
threshold
λ
become closer, indicating that the transition
becomes sharper for longer polymer chains. Extrapolat-
ing
χ
N
(
λ
) versus
N
−
1
/
2
to the limit of
N
→ ∞
,
χ
N
(
λ
)
for different
λ
’s converge to a common point that is inde-
pendent of the choice of
λ
, indicating that the transition
is infinitely sharp as
N
→ ∞
. From the perspective
of single-chain conformation, Θ point is defined as the
abrupt change in chain size from globule to coil for an
infinitely long chain. The common intersection shown in
Figure 5 yields
χ
Θ
= 0
.
50. This value coincides with the
result of F-H theory and is also consistent with the van-
ishing of the second viral coefficient derived in Sec II. We
comment that the coincidence of
χ
Θ
= 0
.
50 with the pre-
diction of the F-H theory is not a trivial result, nor does
it mean that the F-H theory itself is valid. Indeed, the
F-H theory is a poor description of the dilute solution,
including the solution near the Θ point. However, if we
focus on the core of an isolated globule, it is a homoge-
neous region containing many uncorrelated blobs of the
chain, sharing the same physical picture as the F-H the-
ory. In the limit of the infinite chain length, the swollen
globule state persists all the way to the Θ point where
the effective two-body interaction vanishes.
1
10
100
1E-3
0.01
0.1
h/R
0
(
-
)N
1/2
N
10
3
2
10
3
5
10
3
10
4
FIG. 6. Universal behavior in the scaling region. log-log pl
ot
of
h/R
0
vs (
χ
−
χ
Θ
)
N
1
/
2
.
Using
χ
Θ
,
h/R
0
can now be plotted as a function of
the scaling variable (
χ
−
χ
Θ
)
N
1
/
2
. Figure 6 shows that
h/R
0
for different chain lengths collapse onto each when
plotted against (
χ
−
χ
Θ
)
N
1
/
2
, confirming the universal
behavior near the Θ point:
h/R
0
=
f
[
(
χ
−
χ
Θ
)
N
1
/
2
]
(14)
where
f
is a universal function. In the range
(
χ
−
χ
Θ
)
N
1
/
2
>
10 (where the globule is in the swollen
state with low core density), the slope of the log-log
plot is
−
1
.
4, close to the exponent
−
4
/
3 we have ob-
tained in Sec III by using the scaling argument. The uni-
versal behavior of the single chain conformation around
the Θ point, initially predicted by de Gennes
31
, is usu-
ally difficult to achieve in the globule state in computer
simulation
22
due to the limitation of chain length. For
short chains, the swollen globule either is not well-defined
or cannot persist to a very dilute core, thus making the
window for observing the scaling regime unclear or too
small. Here, by applying SCFT to long chains (
N >
10
3
),
we are able to more definitively examine this scaling
regime in the globule state.
V. DETERMINING
χ
Θ
FROM SOLUTION
THERMODYNAMICS
The single chain structure will of course affect the so-
lution properties. The compaction of chain segments
into a globule significantly reduces the polymer-solvent
contact, which leads to enhancement of the solubility of
polymer in poor solvent by several orders of magnitude
compared to the prediction of the F-H theory as shown
in our earlier paper
14
. The governing equation for the
8
phase equilibrium of polymers in poor solvent is given
by Eq 10 in Sec IIC. In Eq 10a, the osmotic pressure for
long polymer chain in the dilute solution is very small
(
∑
∞
m
=1
φ
m
/mN
≈
0). Thus, from the similarity between
Eq 10a and Eq 12, we obtain for the volume fraction of
the polymer-rich phase,
φ
H
≈
ρ
0
(15)
On the other hand, based on our analysis of the globule
structure in Sec III, the free energy of the single chain
globule in Eq 10b can be divided into the volume con-
tribution and the surface contribution as
F
1
=
F
c
+
F
s
.
It can be shown that this definition is consistent with
the definition based on the monomeric osmotic pressure
across the interface used in Ref.
13
. By substituting
F
c
in the form of Eq 11 into Eq 10b, and making use of Eq
12 and Eq 15, we obtain the relation between the equi-
librium volume fraction of polymers in the dilute phase
and the surface energy of the globule
ln
φ
L
≈−
βF
s
+ ln
ρ
0
−
ρ
0
=
−
γA
+ ln
ρ
0
−
ρ
0
(16)
from which we identify the surface tension
γ
.
A
=
(36
π
)
1
/
3
(
Nv/ρ
0
)
2
/
3
is the surface area of the globule.
Noting that the natural dimension of the surface ten-
sion is
b/v
(
kT
is taken to be 1), a dimensionless surface
tension can be defined as
γv
2
/
3
which thus contains an
overall
p
1
/
3
dependence; this is the origin of the
p
1
/
3
in
Eqs. 17a and 17b. Eq 16 indicates that, the excess free
energy of a globule is due to its surface energy, and not
due to (uniform) mixing of polymer segments and sol-
vents assumed in the F-H theory. Equations 15 and 16
reveal the intrinsic connection between the macroscopic
phase behavior of the polymer solution and the micro-
scopic structure and property of the single globule. This
connection also allow us to extract information of single
chain globule from solution thermodynamics.
The linear relation between ln
φ
L
and
N
2
/
3
is con-
firmed by numerically solving Eq. 10 as shown in Figure
7. From the slope of ln
φ
L
versus
N
2
/
3
, we can extract the
surface tension of a single globule. Figure 8 shows that
for
χ
much larger than
χ
Θ
,
γ
decreases linearly with
χ
as
γv
2
/
3
= 0
.
11
χ
−
0
.
07. This linear dependence on
χ
agrees with the result of Weber and Helfand for the in-
terfacial tension of a planar interface
55
. As
χ
decreases,
γ
deviates from the linear behavior and approaches zero.
The disappearance of the surface tension of the globule
serves as another definition of the Θ point. By extrapo-
lating the numerical data to the limit of
γ
= 0, Figure 8
yields
χ
Θ
= 0
.
50, which coincides with previous results
obtained from other definitions. Figure 8 also shows that,
γ
follows a quadratic form
γv
2
/
3
= 0
.
52(
χ
−
0
.
5)
2
for
χ
−
χ
Θ
≪
1. The quadratic form of
γ
near the Θ point is
in agreement with scaling prediction by Lifshitz et al.
25
.
In the framework of F-H theory, des Cloizeaux and
Jannink obtained
φ
L
=
3
e
(
χ
−
1
2
)
exp
[
−
3
2
(
χ
−
1
2
)
2
N
]
.
By substituting the expression of
γ
and
ρ
0
into Eq 16, our
400
500
600
700
-150
-100
-50
0
=0.6
=0.7
=0.8
ln
L
N
2/3
=0.9
FIG. 7. Linear relation between ln
φ
L
and
N
2
/
3
. Points rep-
resent the numerical results based on Eq 10. Straight lines
are the linear fit of the points.
0.5
0.6
0.7
0.8
0.9
1.0
0.00
0.01
0.02
0.03
0.04
0.05
This work
Large
Near the
point
v
2 /3
FIG. 8. Dimensionless surface tension of the globule
γv
2
/
3
as
a function of
χ
. Extrapolating the numerical data to
γ
= 0
reveals
χ
Θ
= 0
.
5.
γ
is fitted linearly for large
χ
as
γv
2
/
3
=
0
.
11
χ
−
0
.
07, and fitted by a quadratic function 0
.
52(
χ
−
0
.
5)
2
near the Θ point.
theory yields the equilibrium volume fraction of polymers
in the dilute phase as
φ
L
=
1
e
exp
[
−
p
1
/
3
(0
.
89
χ
−
0
.
53)
N
2
/
3
]
for large χ
(17a)
φ
L
= 3(
χ
−
0
.
5) exp
[
−
1
.
93
p
1
/
3
(
χ
−
0
.
5)
4
/
3
N
2
/
3
]
for χ
−
χ
Θ
≪
1
(17b)
where we have inserted the dependence on the stiffness
parameter
p
=
b
3
/v
. We note that an equation similar
9
to Eq 17b has been given in Ref.
13
(Eq. 26.8). However,
our Eq. 17b provides the numerical prefactor (1.93) in
the scaling dependence in the exponential, which was not
provided in Ref.
13
. Eq. 17a is a completely new result.
These equations show very different scaling behavior of
the solubility of polymers in poor solvent predicted by
our theory compared to the F-H theory
2
, both in the
χ
dependence and in the
N
dependence.
The exponent in Eq. 17b can be considered as a quan-
titative Ginzburg criterion for the validity of applying the
SCFT, i.e., SCFT is applicable if
p
1
/
3
(
χ
−
0
.
5)
4
/
3
N
2
/
3
>
1. Thus increasing the stiffness parameter
p
allows a
closer approach to the Θ point. This conclusion is con-
sistent with results from computer simulation by Withers
et al.
33
.
From Eq 17b, we obtain the slope of the phase bound-
ary near the Θ point as
∂φ
L
∂χ
=
[
3
−
7
.
74
p
1
/
3
(
χ
−
0
.
5)
4
/
3
N
2
/
3
]
exp
[
−
1
.
93
p
1
/
3
(
χ
−
0
.
5)
4
/
3
N
2
/
3
]
(18)
Consistent with the validity of the SCFT, Eq 18 is valid
in the swollen globule state, which can persist all the way
to the Θ point for infinitely long chain. In the limit of
N
→ ∞
,
∂φ
L
/∂χ
= 0 if
χ >
0
.
5. However,
∂φ
L
/∂χ
jumps to a finite value at
χ
= 0
.
5, which suggests that
χ
= 0
.
5 is the critical point in the phase diagram of a
polymer solution in the limit of infinite chain length
56
.
This establishes the Θ point defined from the perspective
of solution thermodynamics.
These results confirm that the Θ point defined as the
abrupt change in chain size from globule to coil and as
the critical point in the phase diagram are consistent with
each other in the limit of infinite chain length. This con-
sistency reveals the intrinsic connection between the sin-
gle chain structure and its solution properties. From the
perspective of solution thermodynamics our results sug-
gest an alternative experimental determination of the Θ
point from measuring the slope of ln
φ
L
versus
N
2
/
3
at
different temperatures. Since this approach is based on
finite polymer concentrations, it may be more easily con-
ducted than the single-chain measurement.
VI. CONCLUSIONS
In this work, we have presented a theory that uni-
fies the study of the single-chain structure and solution
thermodynamics for polymers in poor solvents, using the
language of the Flory-Huggins parameter. Our theory
captures the large localized density fluctuation in dilute
polymer solutions and the change in chain conformation
with the solvent quality that are missing in the F-H the-
ory. The structure of a globule is studied by SCFT, which
affords a more accurate description of the density profile
of the globule and its free energy for finite chain lengths.
By relaxing the assumption of the virial expansion of
the local interaction as assumed in previous theories, our
theory can be applied to globules with relatively high
monomer density, which facilitates the calculation of the
surface tension of the globule and the solubility of poly-
mers in dilute solution for large values of
χ
. On the other
hand, by avoiding the ground state dominance approx-
imation, the SCFT is capable to describe globules with
diffuse interfaces. These advantages allow us to study the
globule structure and the thermodynamics of the globule
melting in a unified theoretical framework. The chain-
length dependence of the globule melting provides the
essential information on the approach to the Θ point.
We briefly summarize the key new results of this work.
First, we show that the chain conformation involves three
globular states prior to the globule-to-coil transition: the
fully-collapsed globule
, the
swollen globule
and the
molten
globule
; this identification clarifies the ambiguity in the
experimental studies of the globule structure. Second, we
provide numerical verification of the universal behavior
as a function of the scaling variable (
χ
−
χ
Θ
)
N
1
/
2
near the
Θ point, which has not been achieved by previous com-
puter simulation in the globule state due to the limitation
of the chain length. Third, we provide new results for the
solubility of the polymers in dilute solution compared to
the results of des Cloizeaux and Jannink based on the F-
H theory. The large
χ
result is completely new while the
result near the Θ point provides the missing numerical
prefactor in previous work. Fourth, we demonstrate the
consistency of the Θ points defined by the different crite-
ria in the limit of infinite chain length: the disappearance
of the second viral coefficient in the dilute polymer solu-
tion, the abrupt change in chain size from globule to coil
and the critical point in the phase diagram of polymer
solution. Fifth, we find
χ
Θ
= 0
.
5 from all three differ-
ent criteria, which
coincides
with the prediction of F-H
theory. Lastly, although the expression itself is known
and widely used in the literature, we provide the explicit
derivation that shows the effective two-body interaction
in the
single-chain Hamiltonian
is given by 0
.
5
−
χ
.
Although
χ
Θ
= 0
.
5 can be directly obtained through
the viral expansion of the local Hamiltonian if the
polymer-solvent interaction is parameterized by the Flory
χ
parameter, the two methods we present in this pa-
per, that is tracking the chain-length dependence of the
melting of the globule and tracking the chain-length de-
pendence of the solubility of polymer solution, are more
general approaches in determining the Θ point. For ex-
ample, the approaches can also be used for heteropoly-
mers. Moreover, the consistency of the Θ point defined
by the different criteria allows us to choose a convenient
way to measure the Θ point in experiment. Our results
suggest that the Θ point can be determined by measuring
the slope of ln
φ
L
versus
N
2
/
3
for different temperatures,
which is a finite-concentration instead of a single-chain
measurement.
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Strictly speaking, the critical point corresponds to
∂φ
L
/∂χ
→ ∞
. However, since our method is only valid
in the swollen globule regime, we are unable to reach the
critical point. Therefore, rather than a divergence, we ob-
tain a discontinuity.