Dynamic Article LinksC<Soft Matter
Cite this: Soft Matter, 2012, 8, 5180
www.rsc.org/softmatter PAPER
Dow
nloa
ded
by F
lori
da S
tate
Uni
vers
ity o
n 12
Mar
ch 2
013
Publ
ishe
d on
26
Mar
ch 2
012
on h
ttp://
pubs
.rsc
.org
| do
i:10.
1039
/C2S
M07
425G
View Article Online / Journal Homepage / Table of Contents for this issue
Decay of interfacial fluid ordering probed by X-ray reflectivity
Kim Nyg�ard†* and Oleg Konovalov
Received 20th December 2011, Accepted 14th March 2012
DOI: 10.1039/c2sm07425g
To what extent is the ordering of fluids at interfaces governed by the bulk structure of the fluid? In order
to address this question, we have studied a dense, charge-stabilized colloidal suspension at the fluid–air
interface and at two different solid–fluid interfaces using specular X-ray reflectivity. The experimental
data are well described by a simple model of a stratified fluid, with the wall–particle potential mainly
affecting the position of the first particle layer with respect to the interface. The decay of the fluid’s
density profile can for all the studied interfaces be described by a characteristic wavelength and a decay
length, both of which are independently determined from the bulk phase using small-angle X-ray
scattering. This latter finding is consistent with theoretical predictions and recent surface-force
experiments.
1 Introduction
Studies on the asymptotic decay of pair correlations in fluids
were pioneered by Fisher and Widom in the late 1960s.1 In their
seminal paper, they predicted a sharp line in the phase diagram of
simple one-component fluids, known as the Fisher–Widom line,
at which the asymptotic decay of the total pair correlation
function changes from purely exponential to oscillatory expo-
nential. Later it was realized that this also has strong implica-
tions for the density profiles of inhomogeneous fluids, whether at
a single interface or in confinement. In particular, for a fluid
exhibiting short-ranged (i.e., finite or exponentially decaying)
interaction potentials, the asymptotic decay of the density profile
is governed by the leading complex (conjugate) poles of the bulk
total pair correlation function.2 In other words, the decay of the
fluid’s density profile is determined by the decay of its bulk
structure.
The theoretically predicted connection between the fluid’s
density profile and its bulk pair correlations is a general
phenomenon, and is not limited to the aforementioned one-
component fluids exhibiting short-ranged interaction potentials.
For example, upon considering binary mixtures instead of one-
component fluids, this property manifests as the so-called
structural crossover; for mixtures with a sufficiently large size
asymmetry, there exists a crossover line in the phase diagram
separating which of the fluid components govern the decay of the
density profile.3 Recently, the structural crossover was directly
observed in the total pair correlation function of bulk binary
colloidal mixtures.4 Moreover, the analysis of the decay of
correlations in fluids in terms of leading poles has also been
European Synchrotron Radiation Facility, BP 220, F-38043 Grenoble,France
† Present address: Department of Chemistry and Molecular Biology,University of Gothenburg, Sweden. E-mail: [email protected]
5180 | Soft Matter, 2012, 8, 5180–5186
extended to fluids exhibiting additional long-ranged (i.e., power-
law) interactions, such as Coulomb or dispersion interactions.5
From an experimental point of view, studies on the decay of
interfacial fluid ordering are scarce. Recently, Klapp et al.
addressed this question in a series of papers6–8 by combining
surface-force experiments on charge-stabilized colloidal suspen-
sions using the colloidal-probe atomic-force microscope (CP-
AFM), small-angle X-ray and neutron scattering on the bulk
fluid, and theoretical modeling. In these studies, which were
carried out on fluids in narrow confinement rather than on fluids
at single interfaces, they obtained the first experimental evidence
for the decay of the fluid’s density profile being governed by the
decay of its bulk structure, as predicted by theory. Moreover,
they found the ‘‘asymptotic limit’’ of the density profile to be
valid already for confining slit widths of approximately twice the
particle diameter. This latter finding is surprising and therefore
warrants experimental verification using complementary
techniques.
In this paper, we complement the aforementioned surface-
force studies by probing the ordering of a colloidal suspension at
the fluid–air and at two different solid–fluid interfaces using
specular X-ray reflectivity (XRR). Three particular differences
between our approach and that of Klapp et al. should be
mentioned. First, we carry out experiments at single fluid inter-
faces rather than in narrow confinement, i.e., we carry out
experiments in a geometry where the asymptotic limit is well
defined. Second, we perform scattering experiments, and are
therefore probing the structure of the fluid instead of the ensuing
structural force. Third, we study the effect of different wall–
particle interaction potentials on the ordering of the fluid, rather
than the influence of different particle–particle interaction
potentials. The results of the present study can be summarized as
follows: (i) the XRR data can be described using a simple model
of a stratified fluid, with the wall–particle interaction potential
This journal is ª The Royal Society of Chemistry 2012
Dow
nloa
ded
by F
lori
da S
tate
Uni
vers
ity o
n 12
Mar
ch 2
013
Publ
ishe
d on
26
Mar
ch 2
012
on h
ttp://
pubs
.rsc
.org
| do
i:10.
1039
/C2S
M07
425G
View Article Online
predominantly influencing the distance between the first particle
layer and the interface. (ii) The decay of the fluid’s density profile
can be described by a characteristic wavelength and a decay
length, both of which are independently obtained from the bulk
phase using small-angle X-ray scattering (SAXS). This latter
observation is consistent with theoretical predictions and
corroborates the above mentioned CP-AFM results.
The rest of the paper is organized as follows. In Section 2 we
provide a brief review of pair correlations and density profiles in
homogeneous and inhomogeneous fluids as well as their
connection with our experimental data. The experimental part is
described in Section 3. The results are presented and discussed in
Section 4, while the conclusions and an outlook are given in
Section 5.
2 Theory
2.1 Pair correlations
The pair correlations, and hence the local structure, of simple
fluids are governed by the Ornstein–Zernike (OZ) equation.9 For
uniform and isotropic one-component fluids, the OZ equation
reads
h(r) ¼ c(r) + n0Ðh(r0)c(|r � r0|)dr0, (1)
with h(r) ¼ g(r) � 1 denoting the total pair correlation function,
g(r) the pair distribution function, c(r) the direct correlation
function, and n0 the bulk number density. The distance between
two particles is denoted by r. Eqn (1) is exact, but a closure
approximation between h(r), c(r), and the particle–particle
interaction potential u(r) is needed to solve it. The reader is
referred to ref. 9 for a review of the most common closure
relations.
In the case of inhomogeneous fluids, the lack of translational
invariance normal to the interface induces anisotropy of the pair
correlations.10,11 This phenomenon has been known for a long
time within inhomogeneous liquid-state theory, both for fluids at
single interfaces12–14 and in confinement.15–18 The anisotropy of
the pair correlations has also recently been verified experimen-
tally by SAXS for hard-sphere19 and charged20 colloidal
suspensions in confinement. However, with increasing distance
from the interface this feature is less prominent, and hence the
number density profile n(z) can be approximated in a simple
manner using the so-called wall–particle or singlet OZ
equation,21,22
hwpðzÞ ¼ cwpðzÞ þ 2pn0
ðN�N
hwpðtÞdtðNjz�tj
scðsÞds; (2)
in which the anisotropy of the pair correlations is neglected. In
eqn (2), z denotes the distance normal to the interface, hwp(z) the
wall–particle total correlation function, and cwp(z) the wall–
particle direct correlation function. Similar as for eqn (1), the
singlet OZ equation needs to be complemented by a closure
approximation. From eqn (2), the number density profile of the
fluid is recovered using the relation n(z)¼ n0[hwp(z) + 1]. It should
be noted that, in contrast to eqn (1), the singlet OZ equation is
not formally exact and it has been reported to exhibit qualitative
discrepancies close to the interface in comparison with more
This journal is ª The Royal Society of Chemistry 2012
sophisticated theories.13 Nevertheless, for the purpose of dis-
cussing the asymptotic limit of n(z), it suffices to consider the
singlet OZ approximation.
The connection between h(r) and hwp(z) becomes particularly
obvious in reciprocal space, with
h(q) ¼ c(q)/[1 � n0c(q)] (3)
being the three-dimensional (3D) Fourier transform of eqn (1)
and
~hwp(q) ¼ ~cwp(q)/[1 � n0c(q)] (4)
the one-dimensional (1D) Fourier transform of eqn (2).2 Here,
and throughout this article, f (q) denotes the 3D Fourier trans-
form of the spherically symmetric function f(r), while ~f (q) depicts
the 1D Fourier transform of f(z). Notably, for short-ranged
wall–particle interaction potentials, ~hwp(q) is governed by the
same complex leading poles as the bulk quantity h(q). It follows
that, beyond the Fisher–Widom line,1 the asymptotic limit of the
number density profile is given by2
n(z) � n0 / Aexp(�a0 z)cos(a1z � Q). (5)
Here, the decay length x¼ a0�1 and the characteristic wavelength
L ¼ 2pa1�1 are bulk properties of the fluid,23 whereas the
parameters A and Q depend on the wall–particle interaction
potential. We emphasize that eqn (5) is not a result of the singlet
OZ approximation, but holds also within formally exact theo-
ries.24 Although the asymptotic limit of the number density
profile n(z) might at first seem a rather abstract quantity, recent
surface-force experiments on charge-stabilized colloidal suspen-
sions in confinement have suggested eqn (5) to hold already for
confining slit widths of approximately twice the particle diam-
eter.6–8 Moreover, theoretical studies in the bulk phase have
shown the leading-pole analysis to be valid at surprisingly short
distances of a few particle diameters.2,25
2.2 Small-angle X-ray scattering
SAXS probes electron density variations from nanometre to
mesoscopic length scales.26 In the case of bulk colloidal suspen-
sions composed of spherical particles, SAXS yields the total pair
correlation function as follows. Within the monodisperse
approximation, the scattered intensity is given by
I(q) f h|F(q)|2iS(q), (6)
with q¼ 2k sinq denoting the scattering vector modulus, k¼ 2p/l
the wave vector modulus, l the X-ray wavelength, 2q the scat-
tering angle, F(q) the particle form factor, and the brackets h.ithe averaging over a distribution of particle sizes. The interpar-
ticle interactions are contained in the static structure factor,
S(q) ¼ 1 + n0h(q), (7)
which provides a connection between the SAXS data and the
bulk pair correlations of the fluid.
In this study, the SAXS data is modeled as follows. The size
polydispersity of the spherical particles is included using the
Soft Matter, 2012, 8, 5180–5186 | 5181
Dow
nloa
ded
by F
lori
da S
tate
Uni
vers
ity o
n 12
Mar
ch 2
013
Publ
ishe
d on
26
Mar
ch 2
012
on h
ttp://
pubs
.rsc
.org
| do
i:10.
1039
/C2S
M07
425G
View Article Online
Schultz distribution.27 The structure factor S(q), in turn, is
determined within the rescaled mean spherical approximation
(RMSA),28,29 with the repulsive particle–particle interaction
potential u(r) being of hard-core Yukawa-type,
buðrÞ ¼8<:
N if r\2R0;
Z2lB
�expðkR0Þð1þ kR0Þ
�2expð�krÞ
rif r. 2R0:
(8)
Here R0 is the average particle radius, Z the number of
elementary charges per particle, lB the Bjerrum length, k�1 the
Debye screening length, and b ¼ (kBT)�1 with kB Boltzmann’s
constant and T the absolute temperature.
Table 1 The complex refractive index nc ¼ 1 � d � ib for the materialsand incident X-ray energies h-u of the present XRR study.38 The densitiesr are also shown
Material r/g cm�3 h-u/keV d b
H2O 1.0 8.0 3.6 � 10�6 1.3 � 10�8
H2O 1.0 22.1 4.7 � 10�7 2.5 � 10�10
SiO2 2.0 8.0 6.6 � 10�6 8.6 � 10�8
SiO2 2.0 22.1 8.5 � 10�7 1.6 � 10�9
Si 2.3 22.1 9.8 � 10�7 3.2 � 10�9
2.3 Specular X-ray reflectivity
The density profile of the fluid normal to the interface can be
determined using XRR.30 Within the kinematic approximation,
XRR data are given by
R(q) f q2RF(q)|~re(q)|2. (9)
Here q denotes the scattering vector modulus,31 RF(q) the Fresnel
reflectivity of an ideal, sharp interface, and iq~re(q) the Fourier
transform of dre(z)/dz, with re(z) being the electron density
profile. The kinematic approximation fails close to the critical
angle for total reflection, and therefore we use the exact,
dynamical reflection formalism of Parratt32 throughout this
study. Nevertheless, the main result of eqn (9) remains, i.e.,
deviations of R(q)/RF(q) from unity are due to density variations
of the fluid normal to the interface.33
Since R(q) is the reflected intensity rather than the amplitude,
it can not be Fourier inverted directly to yield the density
profile. Instead, XRR data are typically analyzed by compar-
ison with model density profiles. Here, we model the number
density profile as a stratified fluid, following previous XRR
studies of ordering at liquid–air34 and solid–liquid interfaces.35
Although simple, this approach provides a straightforward
means to address the decay of n(z). Within this model, an
oscillatory n(z) close to and a constant n(z) far from the inter-
face are constructed using an array of Gaussian peaks, the root-
mean-square width of which diverge with increasing distance
from the interface. More specifically, we model the number
density profile as
nðzÞ ¼XNm¼0
n0dffiffiffiffiffiffi2p
psm
exp
"�ðz� z0 �mdÞ2
2s2m
#; (10)
with z0 denoting the position of the first particle layer with
respect to the interface and d the distance between adjacent
layers. Although the distance between the particle layers may
vary, as exemplified by a recent XRR study on a molecular
liquid confined between mica crystals,36 we decided to adopt
a constant interlayer distance d in order to minimize the
number of free parameters. The diverging peak width is given
by sm ¼ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffis20 þmhsi2
q, with s0 and hsi being empirical
constants. In order to calculate the reflectivity R(q) corre-
sponding to the model, we transform the number density
profile n(z) into a silica concentration profile, C(z) ¼ (4pR30/3)
n(z)5P(z), with (4pR30/3)n(z) denoting the particle volume
5182 | Soft Matter, 2012, 8, 5180–5186
fraction profile, 5 the convolution operator, and P(z) the
projection of the particle shape.37 In essence, the convolu-
tion with P(z) takes into account that XRR is sensitive to
the electron density (or, equivalently, the refractive index)
profile, whereas n(z) is a distribution of particle centers.
Finally, we determine a complex refractive index profile
nc(z) ¼ 1 � d(z) �ib(z) from C(z) using tabulated optical
constants of the material constituents (see Table 1),38 which
is then used as an input for determining the model R(q)
using Parratt’s recursion formalism.32 Throughout this study,
we include the interface roughness sr in a standard manner
by describing the profile of the interface using an error
function.
3 Experimental details
3.1 Samples
As a model system, we used a commercially available, charge-
stabilized colloidal suspension of spherical SiO2 particles
dispersed in H2O (Ludox SM-30, Sigma-Aldrich). The colloidal
suspension was used as received. It had a nominal particle mass
fraction xM ¼ 0.30 and a pH of 10. We note that the same
brand of colloidal suspensions were used in the CP-AFM
experiments of Klapp et al.,6–8 although at lower particle
concentrations and pH.
As solid surfaces, we prepared two polished, single crystalline
Si wafers with different surface termination. First, a Si wafer with
a native oxide layer was used without further preparation. It had
a hydrophilic surface termination, with the contact angle of
water being y ¼ 31 � 1�. Second, a Si wafer was coated with
dimethyldichlorosilane [Si(CH3)2Cl2, Sigma-Aldrich], leading to
a weakly hydrophilic surface termination with the water contact
angle y ¼ 78 � 1�.Two points about the electron density contrasts of the surface
layers on the Si substrate need to be mentioned: (i) the electron
density of dimethyldichlorosilane in the liquid phase, re ¼ 320
nm�3, is close to that of liquid water, re ¼ 330 nm�3. Conse-
quently, we expect Si(CH3)2Cl2 and H2O to be practically
indistinguishable in the XRR experiment. (ii) The electron
densities of Si (re ¼ 700 nm�3) and the native oxide layer may be
very similar, depending on the porosity of the latter (a density of
r ¼ 2.3 g cm�3 for the latter would correspond to an electron
density re ¼ 690 nm�3). Since we observed signatures of neither
the dimethyldichlorosilane nor the native oxide layer in R(q) for
the probed q regime, we have not included these layers explicitly
in the XRR modeling.
This journal is ª The Royal Society of Chemistry 2012
Fig. 1 Bulk SAXS data. Only every fourth data point is shown for
clarity. The error bars of the experimental data are smaller than the
symbol size. The solid line depicts a model of polydisperse spherical
particles, with hard-core Yukawa-type particle–particle interactions
included within the RMSA.
Dow
nloa
ded
by F
lori
da S
tate
Uni
vers
ity o
n 12
Mar
ch 2
013
Publ
ishe
d on
26
Mar
ch 2
012
on h
ttp://
pubs
.rsc
.org
| do
i:10.
1039
/C2S
M07
425G
View Article Online
3.2 Experiments
The SAXS experiment was carried out at beamline ID02 at the
European Synchrotron Radiation Facility (ESRF). Details
about the beamline have been reported elsewhere.39 The incident
X-ray beam had an energy of h-u ¼ 12.5 keV (wavelength l ¼1.00 �A) and the scattered X-rays were collected 1.3 m behind the
sample using the two-dimensional FReLoN CCD detector. The
preliminary data treatment (masking and radial integration) was
done using software available at the beamline. We corrected for
parasitic scattering by subtracting the scattering pattern obtained
from a water sample. The SAXS experiment was carried out at
room temperature, T ¼ 295 K.
The XRR experiments were carried out at beamline ID10B at
the ESRF. Details about the beamline can be found elsewhere.40
Wemade use of two different setups: (i) for XRR experiments on
the fluid–air interface, we used an incident X-ray beam with an
energy of h-u ¼ 8.0 keV (l ¼ 1.55 �A) and a beam size of 1.0 mm
(H) � 0.1 mm (V) at the sample position (H and V denote
horizontal and vertical, respectively). In order to tilt the
incoming beam with respect to the fluid surface, we used
a Ge(111) deflector crystal available at the beamline. (ii) In order
to penetrate through 25 mm of the bulk colloidal suspension, the
XRR experiments on the buried solid–fluid interfaces were
carried out using an incident X-ray energy of h-u ¼ 22.1 keV (l ¼0.56 �A). In this experiment, the beam size at the sample position
was 1.0 mm (H)� 12 mm (V), and the experiment was carried out
by rotating the sample with respect to the incident X-ray beam.
In both setups, the sample-to-detector distance was about
600 mm and we collected the specularly reflected X-rays and the
parasitic background scattering simultaneously using the linear
(1D) VANTEC-1 detector. All the XRR experiments were
carried out at room temperature, T ¼ 295 K.
In the case of the XRR data collected from solid–fluid inter-
faces, the subtraction of parasitic scattering warrants special
attention. In the present study, the X-ray beam traversed
approximately 25 mm in the bulk colloidal suspension, either
prior to or after being reflected from the interface. Consequently,
the main contribution to the parasitic background scattering is
SAXS from the bulk fluid, which exhibits a strong maximum in
S(q) in the same q range as the interesting features in R(q).
Gratifyingly, we have carefully modeled the parasitic scattering
in this q regime prior to subtraction, and found the intensity of
the parasitic scattering to be less than 5% of the intensity of the
specular reflection.
4 Results and discussion
4.1 Bulk structure
In Fig. 1, we present the SAXS data obtained from the bulk
colloidal suspension (collected up to qmax ¼ 4.5 nm�1). Also
shown is the best model of polydisperse spherical particles
interacting via hard-core Yukawa-type forces within the RMSA,
as determined by fitting the model of Section 2.2 to the experi-
mental data in the range 0.2 nm�1 # q # 2.0 nm�1. In the low-q
regime, the model fails to describe the experimental data, an
effect which we attribute to a minor fraction of aggregated
colloidal particles. For larger q, the experimental data and the
model are in reasonable agreement, the latter providing the
This journal is ª The Royal Society of Chemistry 2012
average particle radius R0 ¼ 5.15 � 0.04 nm, the particle size
polydispersity DR0/R0 ¼ 0.21 � 0.02, the Debye screening length
k�1¼ 3.40� 0.12 nm, and the particle volume fraction f¼ 0.18�0.01. The volume fraction corresponds to the number density
n0 ¼ 0.34D0�3, with D0 ¼ 2R0 denoting the average particle
diameter. The error bars reported here have been determined
from a 10% increase in the error metric
ð1=NÞPNi¼1
½IeðqiÞ � ImðqiÞ�2=I2e ðqiÞ, with Ie(q) and Im(q) denoting
the experimental and model SAXS data, respectively. We note
that the average particle size R0 and polydispersity DR0/R0 are in
good agreement with the values recently reported by Zeng et al.8
for the same brand of Ludox SM-30 colloids. The value of the
Debye screening length implies Z z 26 elementary charges per
particle. This is roughly a factor of four larger than Z ¼ 6
reported in ref. 8, an effect which we attribute to the following
two phenomena: (i) the colloidal suspension of the present study
has a larger pH compared to that of Zeng et al., leading to
a higher surface charge on the particles, and (ii) the RMSA
overestimates Z (see, e.g., ref. 41). Finally, the nominal particle
mass fraction xM ¼ 0.30 and the obtained bulk number density
n0 ¼ 0.34D0�3 imply an average density rSiO2
¼ 2.0 g cm�3 for our
colloidal SiO2. In the subsequent modeling of the XRR data, we
use these values for n0 and rSiO2as fixed parameters.
4.2 Interfacial density profiles
The XRR data collected from the fluid–air and the two solid–
fluid interfaces are presented in Fig. 2. Although not shown here,
all the reflectivity curves R(q) have been collected up to at least
qmax ¼ 2.5 nm�1. The XRR data from the solid–fluid interfaces
do not exhibit total reflection at small q, in contrast to the data
from the fluid–air interface. We attribute this unfortunate effect
to a minor bending of the solid substrates used in the present
experiment. Nevertheless, it does not affect the results of the
experiment, which are based on features in the XRR data at
larger q values.
Soft Matter, 2012, 8, 5180–5186 | 5183
Fig. 2 XRR data collected from the silica colloidal suspension at three
different interfaces: air, a weakly hydrophilic surface, and a hydrophilic
surface. The curves are vertically offset and only every fourth data point
is shown for clarity. The experimental error bars are smaller than the
symbol size. The solid lines depict the best fits using the stratified fluid
model of eqn (10).
Fig. 3 The silica concentration profiles C(z) obtained by fitting eqn (10)
to the XRR data in Fig. 2.
Dow
nloa
ded
by F
lori
da S
tate
Uni
vers
ity o
n 12
Mar
ch 2
013
Publ
ishe
d on
26
Mar
ch 2
012
on h
ttp://
pubs
.rsc
.org
| do
i:10.
1039
/C2S
M07
425G
View Article Online
Also shown in Fig. 2 are the best fits to the experimental data
using the stratified fluid model of eqn (10). The XRR data from
the fluid–air and solid–fluid interfaces were modeled in the range
0.15 nm�1 # q # 3.5 nm�1 and 0.24 nm�1 # q # 2.5 nm�1,
respectively. In general, the agreement between the experimental
and the model R(q) is good, although the model exhibits weak
oscillations at large q which are not present in the experimental
data. We attribute this minor difference to size polydispersity of
the colloidal particles, which is expected to induce size segrega-
tion in the density profile42 and which is not properly taken into
account in the model. Indeed, such a weak large-q oscillation in
R(q) was observed in a previous XRR study on the fluid–air
interface of a colloidal suspension containing spherical particles
with a smaller size polydispersity of DR0/R0 ¼ 0.13.43
The best fit parameters of the modeling in Fig. 2 are presented
in Table 2. The values obtained for the distance d between
adjacent layers as well as the layer roughness s0 and hsi agreewell for all three models. This is also reflected in the corre-
sponding density profiles presented in Fig. 3, which coincide
Table 2 Fit parameters of eqn (10) to the XRR data of Fig. 2: the positiod between adjacent layers, empirical layer roughness s0 and hsi, and the inter
particle diameter D0. The error bars are determined from a 10% increase in
denoting the experimental and model reflectivity curve, respectively
Interface z0/D0 d/D0
Air 1.19 � 0.02 1.32 � 0.03Weakly hydrophilic 1.46 � 0.02 1.38 � 0.07Hydrophilic 1.11 � 0.02 1.39 � 0.03
5184 | Soft Matter, 2012, 8, 5180–5186
within the accuracy of the present XRR experiments. This
finding will be discussed in more detail in Section 4.3. Here, we
will instead focus on the other parameters of the model. First, we
note that the surface roughness sr obtained for the fluid–air
interface is in good agreement with the capillary-wave-induced
surface roughness of water, 3.24 � 0.05 �A.44 The solid–fluid
interfaces, in turn, exhibit a somewhat larger surface roughness.
Second, andmore interestingly, the distance z0 of the first particle
layer from the interface is found to depend on the wall–particle
potential. In order to explain the values of z0 quantitatively, we
would need to carry out extensive simulations or theoretical
calculations, taking into account both wall–particle and many-
body particle–particle interactions. Since this is beyond the scope
of the present study, we instead provide a brief, qualitative
discussion below.
Even for an uncharged interface, such as the fluid–air inter-
face, we expect two electrostatic contributions to the wall–
particle interaction potential:45 (i) a repulsion due to image
charges induced by the dielectric discontinuity at the interface
and (ii) a repulsion due to distortions close to the interface of the
electrical double layer surrounding the charged particle. Conse-
quently, we expect the charged colloidal particles to be repelled
from the fluid–air interface, in agreement with our observation.
This effect was also observed in a previous XRR study on the
ordering of a charge-stabilized colloidal suspension at the fluid–
air interface.43 In the case of the hydrophilic surface, we must
consider the following two effects:45 first, the repulsion due to
image charges will be weaker than that at the fluid–air interface,
because of a smaller jump in the dielectric constant across the
n z0 of the first particle layer with respect to the interface, the distanceface roughness sr. Except for sr, all values are given in units of the average
the error metric ð1=NÞPNi¼1
½ReðqiÞ � RmðqiÞ�2=R2eðqiÞ, with Re(q) and Rm(q)
s0/D0 hsi/D0 sr/�A
0.18 � 0.02 0.36 � 0.03 3.1 � 0.20.17 � 0.02 0.38 � 0.08 5.9 � 0.30.21 � 0.02 0.34 � 0.03 6.3 � 0.2
This journal is ª The Royal Society of Chemistry 2012
Fig. 4 Decay of the model density profiles of Table 2. The dashed line is
Dow
nloa
ded
by F
lori
da S
tate
Uni
vers
ity o
n 12
Mar
ch 2
013
Publ
ishe
d on
26
Mar
ch 2
012
on h
ttp://
pubs
.rsc
.org
| do
i:10.
1039
/C2S
M07
425G
View Article Online
interface. Second, we expect an additional electrostatic wall–
particle repulsion of the Yukawa-type, due to the negative
surface charges on both the solid surface and the particles. These
two effects are competing, as evidenced by z0 being practically
equal for the fluid–air and hydrophilic surface–fluid interfaces.
Surprisingly, in the case of the weakly hydrophilic surface, for
which we expect weaker Yukawa-type repulsions than for the
hydrophilic surface, z0 reaches its maximum value. Such a large
z0 can not be explained only by steric repulsions due to the
dimethyldichlorosilane coating. We have verified these results for
the two solid–fluid interfaces using an effective hard-sphere hard-
wall model within the singlet OZ approximation of eqn (2) using
the Percus–Yevick closure,21 ruling out the possibility that the
behavior of z0 is specific to the model of eqn (10). For the
moment, the behavior of z0 in the case of the weakly hydrophilic
surface remains unexplained.
a linear fit to the data for the hydrophilic surface.4.3 Decay of interfacial density profiles
Finally, we turn to the main topic of this paper, i.e., the decay of
density profiles at fluid interfaces. It should be mentioned that
this topic has also been touched upon in previous XRR experi-
ments. In particular, Yu et al. adopted a model akin to eqn (5), in
order to explain XRR data for a molecular liquid at a solid
surface.46 Recently, one of us also rationalized the decay of
interfacial ordering for confined reverse micelles using this
model.47 However, to our knowledge this is the first XRR (or,
more generally, X-ray scattering) study, in which the decay of
interfacial fluid ordering and its connection with the decay of
bulk pair correlations is explicitly addressed.
First, we discuss the characteristic wavelength L, which is
straightforwardly obtained from the model of eqn (10) as the
distance between adjacent layers, L ¼ d. This should be
compared to the average particle distance in the bulk phase, db.
The latter quantity is most readily determined as the distance
between adjacent peaks in the bulk total pair correlation function
h(r), which in turn is obtained from the model of Fig. 1 by
Fourier inverting eqn (7). Using this approach, we obtain db ¼1.34D0 for interparticle distances beyond the second peak in h(r),
in good agreement with the values of d given in Table 2. Alter-
natively, we can use d0b z 2p/q0 following Zeng et al.,8 with q0
denoting the position of the first peak in S(q). It should be noted,
however, that while the relation between the interparticle
distance and the first peak position in S(q) is exact when the
system exhibits long-range order, i.e., in the limit of Bragg
diffraction, it holds only approximately for disordered systems
such as fluids. Indeed, from the model of Fig. 1 we estimate d0b z
1.26D0. Finally, we note that db < 2(R0 + k�1) ¼ 1.66D0. This
latter observation corroborates the previous finding8 that the
spatial extent of the electrical double layers, �2(R0 + k�1), does
not provide a good estimate of the characteristic wavelengthL in
this system.
Next, we consider the decay length x, which is not as
straightforwardly determined from the model of eqn (10) as the
characteristic wavelength L. In order to determine x, we present
in Fig. 4 the peak values of log([n(z) � n0]/n0) for the three model
density profiles of Table 2. Also shown is a linear fit to the model
obtained for the hydrophilic surface, which (i) illustrates the
exponential decay of the stratified fluid model of eqn (10) and (ii)
This journal is ª The Royal Society of Chemistry 2012
provides an estimate of x. From Fig. 4, we determine the decay
lengths xa ¼ 0.99D0, xwh ¼ 0.99D0, and xh ¼ 1.27D0 for the data
collected at the interfaces between the fluid and air, the weakly
hydrophilic surface, and the hydrophilic surface, respectively.
The large scatter in these values is striking, considering the small
variation in s0 and hsi in Table 2. The scatter shows the sensi-
tivity of the decay length x, and hence the difficulty in experi-
mentally determining it for inhomogeneous fluids. Nonetheless,
the obtained values do provide an estimate of x, which we can
compare to the bulk counterpart xb. In order to determine the
bulk decay length xb from the SAXS data, we apply a similar
analysis as in Fig. 4 on the model h(r) of Fig. 1 (not shown). For
interparticle distances beyond the second peak in h(r), the
exponential decay of the bulk total pair correlation function can
be described by a single decay length, xb ¼ 0.79D0. We primarily
attribute the deviations between xb and x to the modeling of
Fig. 2. Nevertheless, xb is in reasonable agreement with the
inhomogeneous counterparts x presented above, considering the
difficulties in determining the latter values as mentioned above.
Here, a few important points need to be mentioned: (i) we have
so far in the discussion neglected the van der Waals contribution
to the particle–particle interaction potential u(r). It is long
ranged, and we therefore expect it to ultimately govern the
asymptotic decay of h(r) and n(z).5 However, the short-ranged
hard-core Yukawa-type contribution to u(r) will dominate at
short and intermediate distances, and it is this decay that we are
concerned with in the present paper. (ii) Based on theoretical
studies of bulk fluids, the contribution from at least two of the
slowest decaying poles are needed to accurately describe h(r) at
short distances.2,25 Moreover, we do not determine the charac-
teristic wavelength L and the decay length x from the slowest
decaying complex poles of eqn (3), but rather from simplified
modeling. Consequently, the present quantities should be
considered as approximations to (or effective counterparts of)
L ¼ 2pa1�1 and x ¼ a0
�1 introduced in Section 2.1.
5 Conclusions and outlook
In summary, we have carried out XRR experiments on a charge-
stabilized colloidal suspension at the fluid–air and at two
different solid–fluid interfaces, in order to address the question:
Soft Matter, 2012, 8, 5180–5186 | 5185
Dow
nloa
ded
by F
lori
da S
tate
Uni
vers
ity o
n 12
Mar
ch 2
013
Publ
ishe
d on
26
Mar
ch 2
012
on h
ttp://
pubs
.rsc
.org
| do
i:10.
1039
/C2S
M07
425G
View Article Online
to what extent is the decay of interfacial fluid ordering deter-
mined by the bulk structure of the fluid? Our experiments provide
support for a bulk-like decay of the density profile already at
short distances from the interface. This finding is consistent with
theoretical predictions and corroborates recent surface-force
experiments on a similar colloidal suspension under confinement.
The above result raises the obvious question: how can we
reconcile the bulk-like decay of the fluid’s density profile close to
the interface with the anisotropy of its pair correlations alluded
to in Section 2.1? In order to answer this question, we would need
to go beyond the effective characteristic wavelength and decay
length probed in this study. Instead, we propose a theoretical
study of the fluid’s density profile n(z) and its characteristic
parameters L and x, while systematically varying the strength of
the anisotropy in the pair correlation functions. In practice, such
a study could be carried out, e.g., on an inhomogeneous hard-
sphere fluid as a function of particle concentration.
Acknowledgements
We thank Manuel Fern�andez and Theyencheri Narayanan for
assistance with the SAXS experiment and Angelo Accardo for
help with the contact angle measurements.
Notes and references
1 M. E. Fisher and B. Widom, J. Chem. Phys., 1969, 50, 3756–3772.
2 R. Evans, R. J. F. Leote de Carvalho, J. R. Henderson andD. C. Hoyle, J. Chem. Phys., 1994, 100, 591–603.
3 C. Grodon, M. Dijkstra, R. Evans and R. Roth, Mol. Phys., 2005,103, 3009–3023.
4 J. Baumgartl, R. P. A. Dullens, M. Dijkstra, R. Roth andC. Bechinger, Phys. Rev. Lett., 2007, 98, 198303.
5 R. J. F. Leote de Carvalho, R. Evans, D. C. Hoyle andJ. R. Henderson, J. Phys.: Condens. Matter, 1994, 6, 9275–9294.
6 S. H. L. Klapp, Y. Zeng, D. Qu and R. von Klitzing, Phys. Rev. Lett.,2008, 100, 118303.
7 S. H. L. Klapp, S. Gradner, Y. Zeng and R. vonKlitzing, SoftMatter,2010, 6, 2330–2336.
8 Y. Zeng, S. Grandner, C. L. P. Oliveira, A. F. Th€unemann, O. Paris,J. S. Pedersen, S. H. L. Klapp and R. von Klitzing, Soft Matter, 2011,7, 10899–10909.
9 J.-P. Hansen and I. R. McDonald, Theory of Simple Liquids,Academic Press, Amsterdam, 3rd edn, 2006.
10 J. K. Percus, The Equilibrium Theory of Classical Fluids, New York,1964, pp. II.33–II.170.
11 S. Sokolowski, J. Chem. Phys., 1980, 73, 3507–3508.12 R. Kjellander and S. Mar�celja, Chem. Phys. Lett., 1984, 112, 49–53.13 M. Plischke and D. Henderson, J. Chem. Phys., 1986, 84, 2846–2852.14 B. G€otzelmann, A. Haase and S. Dietrich, Phys. Rev. E, 1996, 53,
3456–3467.15 R. Kjellander and S. Mar�celja, J. Chem. Phys., 1988, 88, 7138–7146.16 R. Kjellander and S. Sarman, J. Chem. Soc., Faraday Trans., 1991, 87,
1869–1881.
5186 | Soft Matter, 2012, 8, 5180–5186
17 B. G€otzelmann and S. Dietrich, Phys. Rev. E, 1997, 55, 2993–3005.18 D. Henderson, S. Sokolowski and D. Wasan, J. Stat. Phys., 1997, 89,
233–247.19 K. Nyg�ard, R. Kjellander, S. Sarman, S. Chodankar, E. Perret,
J. Buitenhuis and J. F. van der Veen, Phys. Rev. Lett., 2012, 108,037802.
20 K. Nyg�ard, D. K. Satapathy, J. Buitenhuis, E. Perret, O. Bunk,C. David and J. F. van der Veen, Europhys. Lett., 2009, 86, 66001.
21 D. Henderson, F. F. Abraham and J. A. Barker,Mol. Phys., 1976, 31,1291–1295.
22 Here, we have for brevity reproduced only one of several equivalentversions of the singlet OZ equation.
23 More specifically, a0 and a1 are obtained from the lowest lyingcomplex conjugate pole p ¼ �a1 + i a0 of eqn (3).
24 J. R. Henderson and Z. A. Sabeur, J. Chem. Phys., 1992, 97, 6750–6758.
25 J. Ulander and R. Kjellander, J. Chem. Phys., 1998, 109, 9508–9522.26 O. Glatter and O. Kratky, Small Angle X-ray Scattering, Academic
Press, London, 1982.27 M. Kotlarchyk and S.-H. Chen, J. Chem. Phys., 1983, 79, 2461–2469.28 J. B. Hayter and J. Penfold, Mol. Phys., 1981, 42, 109–118.29 J.-P. Hansen and J. B. Hayter, Mol. Phys., 1982, 46, 651–656.30 J. Daillant and A. Gibaud, X-ray and Neutron Reflectivity: Principles
and Applications, Springer, Berlin Heidelberg, 2009.31 In line with eqn (4), we denote the scattering vector modulus simply
with q. However, while the bulk S(q) is an isotropic quantity, R(q)is defined normal to the interface.
32 L. G. Parratt, Phys. Rev., 1954, 95, 359–369.33 The effects of capillary waves or roughness of the solid surface have
for simplicity been neglected in this discussion. However, they areincluded in the modeling of the XRR data.
34 O. M. Magnussen, B. M. Ocko, M. J. Regan, K. Penanen,P. S. Pershan and M. Deutsch, Phys. Rev. Lett., 1995, 74, 4444–4447.
35 W. J. Huisman, J. F. Peters, M. J. Zwanenburg, S. A. de Vries,T. E. Derry, D. Abernathy and J. F. van der Veen, Nature, 1997,390, 379–381.
36 E. Perret, K. Nyg�ard, D. K. Satapathy, T. E. Balmer, O. Bunk,M. Heuberger and J. F. van der Veen, J. Phys.: Condens. Matter,2010, 22, 235102.
37 M. C. Gerstenberg, J. S. Pedersen andG. S. Smith,Phys. Rev. E, 1998,58, 8028–8031.
38 B. L. Henke, E. M. Gullikson and J. C. Davis, At. Data Nucl. DataTables, 1993, 54, 181–342.
39 T. Narayanan, O. Diat and P. B€osecke, Nucl. Instrum. Methods Phys.Res., Sect. A, 2001, 467–468, 1005–1009.
40 D.-M. Smilgies, N. Boudet, B. Struth and O. Konovalov, J.Synchrotron Radiat., 2005, 12, 329–339.
41 M. Heinen, P. Holmqvist, A. J. Banchio and G. N€agele, J. Chem.Phys., 2011, 134, 044532.
42 I. Pagonabarraga, M. E. Cates and G. J. Ackland, Phys. Rev. Lett.,2000, 84, 911–914.
43 A. Madsen, O. Konovalov, A. Robert and G. Gr€ubel, Phys. Rev. E,2001, 64, 061406.
44 A. Braslau, M. Deutsch, P. S. Pershan, A. H. Weiss, J. Als-Nielsenand J. Bohr, Phys. Rev. Lett., 1985, 54, 114–117.
45 H. H. von Gr€unberg and E. C. Mbamala, J. Phys.: Condens. Matter,2001, 13, 4801–4834.
46 C.-J. Yu, A. G. Richter, J. Kmetko, A. Datta and P. Dutta, Europhys.Lett., 2000, 50, 487–493.
47 K. Nyg�ard, D. K. Satapathy, E. Perret, C. Padeste, O. Bunk, C. Davidand J. F. van der Veen, Soft Matter, 2010, 6, 4536–4539.
This journal is ª The Royal Society of Chemistry 2012