Entropic
Origin
of Ionic
Interactions
in Polar
Solvents
Published
as part of The Journal
of Physical
Chemistry
virtual
special
issue “Pablo
G. Debenedetti
Festschrift”.
Samuel
Varner,
‡
Christopher
Balzer,
‡
and Zhen-Gang
Wang
*
Cite This:
J. Phys.
Chem.
B
2023,
127, 4328−4337
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Supporting
Information
ABSTRACT:
Implicit
solvent models that reduce solvent degrees of
freedom
into effective interaction
potentials
are widely used in the study
of soft materials
and biophysical
systems.
For electrolyte
and
polyelectrolyte
solutions,
coarse-graining
the solvent degrees of freedom
into an effective
dielectric
constant
embeds entropic
contributions
into
the temperature
dependence
of the dielectric
constant.
Properly
accounting
for this electrostatic
entropy is essential
to discern whether
a free energy change is enthalpically
or entropically
driven. We address
the entropic
origin of electrostatic
interactions
in a dipolar solvent and
provide a clarified physical picture of the solvent dielectric
response.
We
calculate
the potential
of mean force (PMF) between
two oppositely
chargedionsinadipolarsolventusingmolecular
dynamics
anddipolarself-consistent
fieldtheory.Wefindwithbothtechniques
that
thePMFisdominated
bytheentropygainfromthedipolerelease,owingtothediminished
orientational
polarization
ofthesolvent.
We also find that the relative contribution
of the entropy to the free energy change is nonmonotonic
with temperature.
We expect
that our conclusions
are applicable
to a broad range of problems
involving
ionic interactions
in polar solvents.
■
INTRODUCTION
A wide variety of simulation
and theoretical
approaches
utilize
implicit solvent models, where the solvent degrees of freedom
arelumpedintoeffectiveinteractions.
1,2
Treating
thesolventas
a background
medium
can significantly
reduce the computa-
tional cost.
3
−
5
In doing so, however,
the solvent degrees of
freedom
become
hidden in effective
interaction
potentials,
which are often specified
in an approximate
manner. Common
methods
inbiological
simulations
includetheaccessible
surface
area (ASA) method and continuum
electrostatic
methods
such
as the generalized
Born model.
6
−
13
Dielectric
materials
with polar molecules
respond
to an
electric field through reorientation
of the dipoles.
14
Generally,
the presence
of an electric field will cause the dipoles to align
and increase the order in the system. The free energy change
during dipole reorganization
is thus composed
of both
energetic
and entropic
contributions.
15
The energy comes
from the electrostatic
interactions
of the dipoles with the
electricfieldandwitheachother,while theentropyarisesfrom
the changes in the orientation
of the dipoles. For a uniform
dielectric
material,
the electrostatic
entropy
contribution
is
encapsulated
in the temperature
dependence
of the dielectric
constant.
16
i
k
j
j
j
y
{
z
z
z
S
F
T
T
VE
VE
T
1
2
1
2
el
2
2
=
=
=
(1)
where
T
is the temperature,
Δ
S
el
is the electrostatic
entropy
change due to the application
of an electric field,
Δ
F
is the
Helmholtz
free energy change,
ε
is the dielectric
constant,
V
is
the system volume, and
E
is the electric field. Capturing
the
entropic
contribution
relies on knowing
the temperature
dependence
of the dielectric
constant.
In solutions
containing
ions and charged macromolecules,
the presence
of charged species generates
the electric field that
polarizes
the solvent.
16
Recently,
this phenomenon
has been
used to explain the apparent
discrepancy
between
experi-
ments
17
−
20
and coarse-grained
molecular
dynamics
simula-
tions
21
−
24
in describing
the driving force for polyelectrolyte
complex
coacervation.
Chen and Wang showed
that the
Coulomb
potential
used in coarse-grained
implicit
solvent
models inherently
includes
an entropic
contribution,
which
they term the electrostatic
entropy.
25
By correctly
accounting
for this electrostatic
entropy
contribution
through
the
temperature
dependence
of the dielectric
constant,
they were
able to predict entropy
driven coacervation
from implicit
solvent molecular
dynamics,
in agreement
with experimental
observations.
Further,
they rationalized
this entropic
driving
force as arising from the solvent reorganization
using the
example
of two oppositely
charged ions forming an ion pair.
Received:
January 27, 2023
Revised:
March 30, 2023
Published:
May 9,
2023
Article
pubs.acs.org/JPCB
© 2023
The Authors.
Published
by
American
Chemical
Society
4328
https://doi.org/10.1021/acs.jpcb.3c00588
J. Phys.
Chem.
B
2023,
127, 4328
−
4337
The entropic
contributions
to the potential
of mean force have
also been addressed
in other studies which used molecular
dynamics
26
and the extended
reference
interaction
site model
(RISM).
27
However,
these studies were restricted
to water,
which has specific properties
and interactions
with different
types of ions.
The effective
interaction
potential,
or potential
of mean
force (PMF),
between
ions in solution
is a result of the
combined
effects of direct ion
−
ion
interactions
and
interactions
of ions with the solvent. At the most basic level,
one can assume the solvent has a uniform
temperature-
dependent
dielectric
constant.
In the Debye approximation,
28
for the process of bringing
two ions from infinity to a distance
r
, we have
F
q q
r
4
(1
)
i
j
0
=
+
(2)
T
S
T
F
T
q q
r
4
(1
)
i
j
0
2
=
=
+
(3)
U
F
T
S
q q
r
4
1
(1
)
i
j
0
2
=
+
=
+
(4)
where
q
i
and
q
j
are the charges on the ions,
U
is the internal
energy,
v
3
2
0
is a dimensionless
measure
of the dipole
strength,
μ
̅
is the dipole moment,
β
= 1/
k
B
T
, and
v
is the
molecular
volume
of the solvent.
Thus, the electrostatic
entropy will dominate
the PMF when
ξ
> 1. A similar result
can be obtained
using a more complete
dielectric
theory, such
as Onsager’s
theory.
29,30
While this is a satisfying
result, it is
phenomenological
and does not provide
a clear molecular
picture, since the solvent degrees of freedom
are not explicitly
included.
Inthisstudy,weaddresstheconceptofelectrostatic
entropy
and demonstrate
its generality
by studying
two ions in a
dipolar
fluid. Using dipolar
self-consistent
field theory
(DSCFT)
and molecular
dynamics
simulations,
we analyze
the PMF between
two oppositely
charged,
monovalent
ions
immersed
in a dipolar solvent, explicitly
accounting
for the
solvent degrees of freedom.
We separate
the PMF into its
entropic
and energetic
contributions
to determine
the
conditions
where the electrostatic
entropy dominates.
Finally,
we connect the entropic
driving force to the release of dipoles
as the ions approach
one another,
quantified
through
the
decrease
in the solvent polarization.
While solvent reorganiza-
tion has long been recognized
as a source of entropy
in
physical processes,
especially
in the context of binding of small
molecules
to proteins
and multivalent
ions to charged
macromolecules
in water,
31
−
33
the phenomenon
is often
presented
as solvent-
or system-specific,
where other effects
suchashydrogen
bondingmaydominate.
Ourresultshighlight
the generality
of the electrostatic
entropy and the importance
of properly
accounting
for the solvent degrees of freedom
in
studying
charge-containing
systems.
■
METHODS
Simulation
Model.
To model two ions in a dipolar fluid,
we use a Stockmayer
fluid model based on work by Shock et
al.
34
Thesolventparticlespossesspermanent
pointdipoles
μ
at
their center of mass, while the ions are described
as point
charges
with no dipole (Figure
S1). The nonelectrostatic
nonbonded
potential
energyforallbeadtypesisdescribed
bya
truncated
and shifted Lennard-Jones
(LJ) potential,
35
l
m
o
o
o
o
o
o
o
n
o
o
o
o
o
o
o
Ä
Ç
Å
Å
Å
Å
Å
Å
Å
Å
Å
Å
i
k
j
j
j
y
{
z
z
z
i
k
j
j
j
y
{
z
z
z
É
Ö
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
U
r
r
r
r
r
(
)
4
1
4
2
0
2
ij
LJ
ij
ij
ij
ij
ij
12
6
1 /6
1 /6
=
+
>
(5)
where
ij
i
j
=
,
ij
i
j
=
for all pairs, and
r
is the distance
between
beads
i
and
j
. With a cutoff of 2
1/6
σ
ij
, the LJ potential
is purely repulsive
and
ε
ij
is relatively
unimportant.
For all of
our systems,
we set
ε
i
=
ε
j
= 1.
The electrostatic
interactions
are composed
of charge
−
charge, charge
−
dipole,
and dipole
−
dipole
interactions.
The
standard
Coulomb
potential
describes
the charge
−
charge
interactions
between
the two ions,
U
r
q q
r
(
)
1
4
ij
qq
i
j
0
=
(6)
where
ε
0
is vacuum permittivity
and
q
is the charge on each
ion. The charge
−
dipole
and dipole
−
dipole
interactions
are,
respectfully,
given as
U
q
r
r
r
(
)
1
4
(
)
q
q
q
0
3
=
·
|
|
(7)
where
|
r
q
μ
|
is the center of mass distance
between
the charge
and the solvent dipole, and
U
r
r
r
r
r
(
)
1
4
3
4
(
)(
)
ij
i
j
i
j
0
3
0
5
=
·
|
|
·
·
|
|
(8)
where
|
r
μμ
|
isthecenterofmassdistancebetween
pointdipoles
μ
i
and
μ
j
.We reiterate that onlythe ionscarry charge. Alllong-
range electrostatic
interactions
are computed
using a standard
Ewald summation.
The solvent dipoles reorient due to the torque arising from
charge
−
dipole
or dipole
−
dipole
interactions.
We use a
Langevin
thermostat
that takes into account
the angular
degrees of freedom
of the solvent. The LJ size parameter
σ
s
is
used to describe
the spherical
diameter
required
to update the
angular velocity via the solvent bead’s moment
of inertia.
Throughout
the work, we consider
a coarse-grained
model
solvent based on water.
34
Namely,
the number density is
ρ
=
0.03344/Å
3
at
T
= 300 K, with diameter
σ
s
= 3.0 Å and mass
18.015
g
mol
. Water has a gas-phase
dipole moment
of 1.85 D;
however,
we vary the magnitude
of the dipole moment
to
highlight
the role of the dipoles, ranging from
μ
̅
= 0
−
2 D. For
simplicity,
we treat the anion and cation as monovalent
ions
±
1
e
with the same size parameter
as the solvent,
σ
+
=
σ
−
=
σ
s
.
For all simulations,
we use reduced units with the length scale
1
σ
= 3 Å, energy scale 1
ε
= 2.49 kJ/mol, and mass scale 1
m
=
18.015 g/mol that give a corresponding
time scale
m
2
=
.
The PMF between
two ions is calculated
using the adaptive
biasing force (ABF) method.
36,37
The ion separation
distance
isdividedinto8windows
intherangeof0.75
σ
to8.5
σ
. Ineach
window,
the system was equilibrated
for 5
×
10
6
timesteps
(
δ
t
= 0.005
τ
) and production
of 10
7
timesteps.
Each simulation
consists
of 5000 solvent
particles,
corresponding
to a
simulation
box length of 17.69
σ
. We use the GPU
38,39
and
Colvars
40
packages
in
LAMMPS
41
for simulations
and
OVITO
42
for
The Journal
of Physical
Chemistry
B
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Article
https://doi.org/10.1021/acs.jpcb.3c00588
J. Phys.
Chem.
B
2023,
127, 4328
−
4337
4329
visualizations.
Example
LAMMPS
and Colvars
scripts for
calculating
the PMF are available
at https://github.com/
chrisbalzer/Stockmayer-Two-Ions.
Field-Theoretic
Model.
In recent years, several groups
have developed
statistical
field theories that explicitly
account
for solvent polarization
and the dielectric
response.
43
−
47
Here,
we adapt a dipolar self-consistent
field theory that was
previously
developed
and used to study ion solvation
energy
and electron transfer reorganization
energy.
48
−
50
Alternatively,
we could have used the Ornstein
−
Zernike
integral equation
theory with the hypernetted-chain
(HNC) approximation,
or
the extended
RISM equation
which have both been used to
study the potential
of mean force between
ions at infinite
dilution.
27,51
−
54
The purpose of the theoretical
model is not to
compare
or validate the simulation,
but rather to provide an
alternative
approach
for studying
the ionic interaction
in
dipolar fluids to emphasize
the generality
of the presented
behavior.
We believe any theory which can capture the solvent
orientational
polarization
inthevicinityofions cancapturethe
presented
results, which includes allof the mentioned
theories.
Weconsider
twoionsatfixedseparation
immersed
inadipolar
solvent. The solvent dipole is composed
of a permanent
dipole
μ
andaninduceddipole
p
. Theinduceddipoleisrelatedtothe
electronic
degrees
of freedom.
This contribution
is not
essential
for this work, but we include it for completeness
as
it does not add much complexity
to the theory or calculations.
The ions are modeled
as Gaussian
smeared
charges inside a
spherical
solute cavity, where the solvent is excluded.
The use
of smeared
charges is for convenience,
to avoid the diverging
self-energy.
The cavities
are modeled
using a spherically
symmetric
cavity function.
55
−
57
The ions are treated as fixed
external charges to the solvent in this field theory. See Figure
S2foranexampleofthesystemsetup.Themicroscopic
charge
density in the system is given by the contributions
from the
two ions and the solvent dipoles.
r
r
r
r
(
)
(
)
(
)
(
)
c
or
el
=
+
+
(9)
Here,
r
r
r
(
)
(
)
(
)
c
1
2
=
+
is the total charge density of the
ions, modeled
as Gaussian
smeared
charges,
i
k
j
j
j
j
j
y
{
z
z
z
z
z
i
k
j
j
j
j
j
y
{
z
z
z
z
z
i
k
j
j
j
j
j
y
{
z
z
z
z
z
i
k
j
j
j
j
j
y
{
z
z
z
z
z
z e
b
b
z
e
b
b
r
r
R
r
R
(
)
1
2
exp
2
1
2
exp
2
c
1
1
2
3/ 2
1
2
1
2
2
2
2
3/ 2
2
2
2
2
=
|
|
+
|
|
(10)
where
z
i
are the ion valencies,
b
i
are the radii of the charge
spread,
R
i
are the ion positions,
and
e
is the elementary
charge.
r
(
)
or
and
r
(
)
el
are the charge densities
due to the permanent
and induced
dipoles of the solvent, respectively.
The charge
density due to theorientational
and electronic
contributions
of
the solvent can be expressed
in terms of their dipole moments
as
r
r
r
(
)
(
)
i
N
i
i
or
1
=
·
=
(11)
p
r
r
r
(
)
(
)
i
N
i
i
el
1
=
·
=
(12)
where
N
is the number
of solvent molecules,
μ
i
is the
permanent
dipole moment
onmolecule
i
, and
p
i
is theinduced
dipole moment
on molecule
i
. In the energy, we only consider
the Coulomb
interactions
between
all charges, and a harmonic
penalty associated
with the induced dipoles
p
p
U
r
r
r
r
r
r
r
(
,
,
)
1
2
d
d
(
)
(
)
4
2
N
N
N
i
N
i
0
1
2
=
|
|
+
| |
=
(13)
where
α
is the polarizability.
We work in the grand canonical
ensemble
with volume
V
, temperature
T
, and solvent chemical
potential
μ
. We assume the system is incompressible.
The
grand canonical
partition
function
is given by
p
e
N
vn
e
r
r
r
1
d
d
d
(
)
(
)
1
N
N
i
N
i
i
i
U
0
1
0
=
!
[
+
]
=
=
(14)
where
n
̂
is the solvent density operator,
φ
0
is the volume
fraction occupied
by the ions, and
η
is a factor similar to the
cube of the thermal wavelength,
which has no thermodynamic
consequence.
The solvent
density
operator
is given by
n
r
r
r
(
)
(
)
i
N
i
1
=
=
. The local volume fraction due to the
two ions, is modeled
by the superposition
of two cavity
functions,
Ä
Ç
Å
Å
Å
Å
Å
Å
Å
Å
Å
Å
Å
É
Ö
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ä
Ç
Å
Å
Å
Å
Å
Å
Å
Å
Å
Å
Å
É
Ö
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
m
c
m
c
r
r
R
r
R
(
)
1
1
2
tanh
1
2
tanh
0
1
2
2
2
1
2
=
+
|
|
+
|
|
(15)
where
σ
i
is the diameter
of the two ions,
m
is a positive
parameter
for shifting the boundary
of the cavity, and
c
is a
positive
parameter
for tuning the width of the interface
between
the ion and the solvent. In practice,
any reasonable
choice of
m
and
c
will yield the same qualitative
results. We
choose
c
= 0.01 for a rapid but continuous
decay near the ion
boundary,
and we choose
m
= 0.95 such that the ion volume
fraction practically
decays to zero by
σ
i
.
We take advantage
of the Fourier representation
of a delta
functional
to introduce
the incompressibility
field
w
vn
w
i
w
vn
r
r
r
r
r
(
)
(
)
1
exp
d
(
)
(
)
1
0
0
{
}
[
+
] =
[
+
]
(16)
To turn the partition
function
into a field theory, we introduce
coarse-grained
density fields
ρ
or
and
ρ
el
through the identities
w
i
w
r
r
r
r
r
1
(
)
(
)
exp
d
(
)
(
)
or
or
or
or
or
or
or
or
{
}
=
[
]
=
[
]
(17)
w
i
w
r
r
r
r
r
1
(
)
(
)
exp
d
(
)
(
)
el
el
el
el
el
el
el
el
{
}
=
[
]
=
[
]
(18)
where
w
or
and
w
el
are auxiliary
fields introduced
through the
Fourier representation
of the delta functional.
In eqs 16
−
18,
The Journal
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Chemistry
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J. Phys.
Chem.
B
2023,
127, 4328
−
4337
4330
the notation
[···]
denotes functional
integration.
Applying
these identities
to the partition
function
results in
l
m
o
o
o
n
o
o
o
|
}
o
o
o
~
o
o
o
p
p
w
w
w
e
N
i
w
i
w
i
w
vn
r
r
r
r
r
r
r
r
r
r
r
r
r
r
r
r
r
r
r
1
d
d
d
exp
2
2
d
d
(
)
(
)
4
d
(
)
(
)
(
)
d
(
)
(
)
(
)
d
(
)
(
)
(
)
1
N
N
i
N
i
i
i
i
N
i
or
el
or
el
0
1
1
2
0
or
or
or
el
el
el
0
=
!
×
| |
|
|
+
[
] +
[
]
+
[
+
]
=
=
=
(19)
where
r
r
r
r
(
)
(
)
(
)
(
)
c
or
el
=
+
+
. Through
these identity
transformations,
the particle
−
particle
interactions
are turned
into particles
interacting
with fluctuating
fields. The particle
degrees of freedom
can be easily integrated
out to yield the
single-particle
partition
function,
Q
[
w
,
w
or
,
w
el
], given by
i
k
j
j
j
j
y
{
z
z
z
z
l
m
o
o
n
o
o
Ä
Ç
Å
Å
Å
Å
Å
Å
Å
Å
Å
É
Ö
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
|
}
o
o
~
o
o
Q
w
w
ivw
w
r
r
r
4
2
d
sin(
)
exp
(
)
2
(
)
2
3 /2
or
or
el
2
=
|
|
|
|
×
|
|
(20)
The transformed
grand canonical
partition
function
is now
written as
w
w
w
e
H
or
el
or
el
=
(21)
where the Hamiltonian,
H
=
H
[
w
,
w
or
,
w
el
,
ρ
or
,
ρ
el
], is a
functional
of the field variables
only and is given by
H
i
w
i
w
i
w
e
Q
w
w
w
r
r
r
r
r
r
r
r
r
r
r
r
r
r
r
d
(
)
(
)
d
(
)
(
)
2
d
d
(
)
(
)
4
d
(
) 1
(
)
,
,
or
or
el
el
0
0
or
el
=
+
|
|
+
[
]
[
]
(22)
The integrals
in the partition
function
cannot be evaluated
in
closed form, so we use the saddle-point
configuration
as an
approximation
to the full partition
function.
The saddle point
is found by extremizing
the Hamiltonian
with respect to all the
fieldvariables.
58
Thegrandfreeenergyisgivenby
β
Ω
=
−
ln
Ξ
≈
−
ln
Ξ*
, where
Ξ*
is the saddle-point
contribution
to the
partition
function.
Extremizing
the free energy results in a set
of self-consistent
equations
that can be solved to find the
equilibrium
field configurations,
and therefore
observables
such as the free energy and the electric field. Since the saddle-
pointsforthe
w
fieldslieontheimaginary
axis,toavoidtheuse
of imaginary
numbers,
we define real potentials
β
u
=
−
iw
and
βφ
=
iw
or
=
iw
el
(
w
or
=
w
el
at equilibrium).
The set of self-
consistent
equations
obtained
fromextremizing
Ω
withrespect
to
w
,
ρ
or
(and
ρ
el
),
w
or
, and
w
el
respectively,
is given by
e
r
r
r
1
(
)
sinh(
(
) )
(
)
vu
r
r
0
(
)
(
/ 2)
(
)
2
=
|
|
|
|
+
|
|
(23)
r
r
r
r
(1
(
)
(
))
(
)
(
)
c
0
or
el
·[
+
+
] =
(24)
v
e
G
r
r
(
)
(
(
)
)
vu
r
r
or
2
0
(
)
(
/ 2)
(
)
2
=
|
|
+
|
|
(25)
v
r
r
(
)
1
(
)
el
0
0
=
[
]
(26)
where
G
(
x
) = [1/tanh(
x
)
−
1/
x
] sinh(
x
)/
x
2
. Additionally,
we
have defined the orientational
electric susceptibility,
χ
or
, and
the electronic
electric susceptibility,
χ
el
. For convenience,
The
Poisson equation,
eq 24, is written in a way that separates
the
ion charge density from the bound solvent charge density
(reflected
in
χ
or
and
χ
el
). Equation
24 can be rewritten
as
D
r
(
)
c
·
=
(27)
where
D
=
−
ε
0
[1 +
χ
or
(
r
) +
χ
el
(
r
)]
∇
φ
(
r
)
is the electric
displacement.
Conveniently,
the electric displacement
can be
determined
solely from the location
of the free charges.
We
simplify
the solution
to eq 27 by assuming
that the total
electric displacement
is the superposition
of the electric
displacement
due to each of the ions. (The superposition
principle
is used as an approximation
to avoid solving the full
Poisson
equation.
In general it does not hold exactly for
nonlinear
dielectrics.
Theapproximation
becomes
lessaccurate
for strong interactions,
and in particular
when the ions are at
close approach.
49
) The displacement
at a distance
r
i
from an
isolated Gaussian
smeared
charge
i
is
Ä
Ç
Å
Å
Å
Å
Å
Å
Å
Å
Å
Å
Å
i
k
j
j
j
j
j
y
{
z
z
z
z
z
i
k
j
j
j
j
j
y
{
z
z
z
z
z
É
Ö
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
ez
r
r
b
r
b
r
b
D
r
r
(
)
4
erf
2
2
exp
2
i
i
i
i
i
i
i
i
i
i
2
2
2
=
(28)
where
r
i
=
r
−
R
i
, and
r
i
is the unit vector in the direction
of
r
i
.
The equilibrium
electric field is found by iterating
D
(
r
) =
−
ε
(
r
)
∇
φ
(
r
)
usingeqs23, 25, and26tocalculate
thedielectric
function
ε
(
r
) =
ε
0
[1 +
χ
or
(
r
) +
χ
el
(
r
)]. For all self-consistent
calculations,
we iterate until the maximum
difference
in the
electric field between
two consecutive
steps is less than 10
−
13
.
The equilibrium
free energy can be simplified
by plugging
the saddle-point
equations
into the Hamiltonian,
Ä
Ç
Å
Å
Å
Å
Å
Å
Å
Å
Å
Å
É
Ö
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
Ñ
|
}
o
o
~
o
o
vn
v
vn
v
vn
r
r
r
r
r
r
r
r
r
d
1
2
(1
2
(
)
(
))
(
)
(
)
ln
sinh(
(
) )
(
)
(
)
1
ln(
(
))
0
or
el
2
{
=
+
+
|
|
|
|
|
|
[
]
(29)
where
vn
(
r
) = 1
−
φ
0
(
r
) is the coarse-grained
solvent volume
fraction.
The system is rotationally
symmetric
about the axis
connecting
the ions, allowing
the integral in eq 29 to be
calculated
in cylindrical
coordinates
with variation
restricted
to
the
r
,
z
-plane. We use a large enough domain to avoid cutting
off the long-range
tail of the electric field from the ions.
When calculating
the PMF, the quantity
of interest is the
difference
between
the free energy at separation
r
and that at
infinite separation.
We call this difference
ΔΩ
=
Ω
(
r
)
−
Ω
(
∞
). The entropic
contribution
to
ΔΩ
can be calculated
with the derivative
i
k
j
j
j
y
{
z
z
z
S
T
V
,
=
(30)
Note that the change in grand free energy is equal to the
change in Helmholtz
free energy for this process
as the
chemical
potential
and particle number do not change when
bringing
the ions together
at a fixed
T
and
V
due to the
The Journal
of Physical
Chemistry
B
pubs.acs.org/JPCB
Article
https://doi.org/10.1021/acs.jpcb.3c00588
J. Phys.
Chem.
B
2023,
127, 4328
−
4337
4331
incompressibility
constraint.
Mathematically,
we can write the
following
U
TS
N
U
TS
N
U
U
T
S
S
F
(
)
(
)
(
)
=
[
]
=
=
(31)
where the subscript
∞
denotes
a quantity
at infinite ion
separation.
We then decompose
ΔΩ
into entropic
and
energetic
contributions
by calculating
Δ
S
with eq 30 and
internal energy with
Δ
U
=
Δ
F
+
T
Δ
S
=
ΔΩ
+
T
Δ
S
.
■
RESULTS
AND
DISCUSSION
We start with a discussion
of the behavior
of the PMF for
bringing
two oppositely
charged monovalent
ions together
in a
dipolar solvent; this is shown in Figure 1. Both panels show
that increasing
the dipole moment
of the solvent decreases
the
attraction
between
the two ions. This behavior
can be easily
understood
as due to the increase
in the effective
dielectric
constant
with the dipole moment.
The diverging
behavior
below
r
= 1
σ
in Figure 1b is due to the diverging
LJ potential
from simulation.
Above
r
= 1
σ
, we see close agreement
between
theDSCFTandsimulation
resultsatlowto moderate
dipole moment;
a direct comparison
is given in Figure S3 in
the Supporting
Information.
At higher dipole moments
(insets
of Figure 1), oscillations
appear in the PMFs for simulations,
Figure
1.
PMFsforvariousdipolemoments
calculated
from(a)DSCFTand(b)molecular
dynamics
simulation
with
σ
=3Å,
T
=300K,
q
1
=
−
q
2
=
e
,
v
= 30 Å
3
. The insets of both panels show PMFs for larger dipole moments.
For reference,
μ
̅
= 1.85D corresponds
to the gas-phase
dipole
moment
of water.
Figure
2.
PMFs decomposed
into their energetic
and entropic
contributions
with solvent dipoles of (a, b)
μ
̅
= 0 D and (c, d)
μ
̅
= 1 D. The PMFs
are calculated
from DSCFT in (a) and (c) and MD simulation
in (b) and (d). Other parameters
are the same as in Figure 1.
The Journal
of Physical
Chemistry
B
pubs.acs.org/JPCB
Article
https://doi.org/10.1021/acs.jpcb.3c00588
J. Phys.
Chem.
B
2023,
127, 4328
−
4337
4332