Microfluid Nanofluid (2010) 9:1011–1031
DOI 10.1007/s10404-010-0612-5
REVIEW
Molecular dynamics simulation of nanoscale liquid flows
Yuxiu Li • Jinliang Xu • Dongqing Li
Received: 8 February 2010 / Accepted: 25 March 2010 / Published online: 14 April 2010
Springer-Verlag 2010
Abstract Molecular dynamics (MD) simulation is a
powerful tool to investigate the nanoscale fluid flow. In this
article, we review the methods and the applications of MD
simulation in liquid flows in nanochannels. For pressuredriven flows, we focus on the fundamental research and the
rationality of the model hypotheses. For electrokineticdriven flows and the thermal-driven flows, we concentrate
on the principle of generating liquid motion. The slip
boundary condition is one of the marked differences
between the macro- and micro-scale flows and the nanoscale flows. In this article, we review the parameters controlling the degree of boundary slip and the new findings.
MD simulation is based on the Newton’s second law to
simulate the particles’ interactions and consists of several
important processing methods, such as the thermal wall
model, the cut-off radius, and the initial condition. Therefore, we also reviewed the recent improvement in these key
methods to make the MD simulation more rational and
efficient. Finally, we summarized the important discoveries
in this research field and proposed some worthwhile future
research directions.
Y. Li
Guangzhou Institute of Energy Conversion, Chinese Academy
of Sciences, Guangzhou 510640, China
J. Xu
The Beijing Key Laboratory of New and Renewable Energy,
North China Electric Power University, Beijing 102206, China
D. Li (&)
Department of Mechanical and Mechatronics Engineering,
University of Waterloo, Waterloo, ON N2L 3G1, Canada
e-mail:
[email protected]
Keywords Molecular dynamics simulation
Liquid flow Nanochannels Nanofluidics
Understanding the behavior of liquid flow in nano-environments is of important relevance to various applications
such as separation and identification of biological and
chemical species, drug delivery, programmable catalysis,
selective absorption, and bionic energy (Wheeler and
Stroock 2008). Extensive research has been conducted to
understand nanoscale flow physics. Experimentally, nanochannels of various sizes made from different materials
have been fabricated and tested (Stein et al. 2004; Pennathur and Santiago 2005; Raviv et al. 2001; Fan et al. 2003;
Tas et al. 2004; Gogotsi et al. 2001; Stern et al. 1997).
Computationally, Monte Carle and molecular dynamics
(MD) simulations have become the most popular methods
to mimic the nanoscale flow. In this article, we try to
review the studies of nanoscale liquid flow using MD
simulations.
Fluids confined in nanoscale chambers/channels possess
significant different properties from fluids in the macroscale and the microscale. In nanoscale, the competitive
balance of the forces involved in the fluid system often
does not exist. The effects of volume forces which dominate the fluid properties in the large scale are weakened,
and the impacts of surface forces are enhanced. These
result in many special flow phenomena in nanoscale, for
example, the slip boundary condition effect. The hypothesis that the fluid velocity is equal to the wall velocity at
the interface of fluid and solid, the so-called non-slip
boundary condition, is widely accepted because it has been
validated by several experimental and computational
researches in large-scale systems. However, the non-slip
boundary condition is not valid in nanoscale systems. That
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Microfluid Nanofluid (2010) 9:1011–1031
is, the velocity of fluid is not equal to that of the solid wall
in nanoscale systems, which is called the slip boundary
effect.
For studying the fluid flow, the continuum theory usually is applied, based on the hypothesis of continuum
medium. However, this hypothesis may no longer be valid
in nanoscale systems where the molecular free path is
comparable to the characteristic size of the fluid-confined
space, especially for gas. Therefore, the theories based on
the particle movement were developed. The Molecular
dynamics simulation (MDS) is a computer simulation
method that provides a view of the particles’ motion by
computing the interactions of atoms and molecules over a
period of time based on known physics. With the development of nanofluidics, the MDS has become a promising
simulation method for fluid flow in nanoscale channels.
This article is focused on MDS of liquid flows in
nanochannels, and is organized as follows. First, the
method of MDS will be reviewed briefly. In the following
sections, we shall discuss several aspects of MDS of liquid
flows in nanochannels: pressure-driven flow, electric fielddriven flow, thermal-driven flow, liquid–solid interaction,
slip boundary conditions, and improved MD schemes.
Finally, a summary of the past and current research in this
area and comments on several promising research directions will be provided.
1 Introduction of MD
The MDS starts from the integration of the Newton’s
second law. Applying appropriate integral methods, such as
the Gear finite-difference algorithm or Verlet method, the
basic dynamics parameters such as position, velocity, and
interaction force can be determined. The macroscopic
physical properties such as pressure, mean velocity, temperature, particle number density etc. can subsequently be
determined via statistical mechanics. On the basis of the
MD method, the Newtonian equation for each fluid molecule is written as
mi
Nw
N
X
X
~2
dr
~
~
F ijw þ ~
F sou~i
F
þ
¼
ij
dt2 j6¼i;j¼1
j 6¼i;j¼1
ð1Þ
potential model is applied, the interaction force between a
pair of molecules comes from the following relation:
o/ij
Fij ¼
orij
ð2Þ
The LJ potential /ij is given by:
r 12 r6
/ðrÞ ¼ 4e
r
r
ð3Þ
where r is the distance between two molecules, r is a
molecular length scale, and e is an interaction strength
parameter. For example, r = 3.4 9 10-10 m and e =
1.67 9 10-21 J are for liquid argon molecules. The cut-off
distance (beyond this distance, it is assumed that the
molecules do not interact) is usually set to be 2.5r. The
values of the parameters r and e change with the type of
wall and fluid molecules. They are named as rwf and ewf
when Eq. 3 is applied for the potential interaction between
fluid particles and solid wall particles. The cut-off length is
changed to be 2.5rwf, correspondingly.
Finally, combining Eqs. 3 and 2 with Eq. 1 and applying
the shifted potential and shifted force concepts of Haile
(1992), we obtain the basic equation for each fluid particle.
The shifted force technique ensures that the molecular
force between fluid particle i and other fluid particles or
other solid wall particles is reduced to zero once the distance between such fluid particle and other particles
reaches or is beyond the cut-off distance. The main
advantage of doing so is to save a lot of computational time
for the force integration.
N
r13 r7 r 13 r 7 ~rij
P
e
24 r
2 r r 2 rc þ rc
jrij j
j6¼i;j¼1
N
w
13 7 ~
rwf 13 rwf 7
rijw
ewf P
rwf
rwf
þ 24 rwf
2 r
r 2 rcw þ rcw
jrijw j
jw ¼1
ai
þ~
F sou~i ¼ mi~
ð4Þ
The movement of the fluid particles will be predicted by
these basic physics laws. However, solving these equations
with special conditions, such as the boundary conditions
and initial conditions requires specific methods as
explained in the following.
w
where subscript i represents particle i, and ~i is the unit
vector in x-coordinate. The first term of the right-hand side
of Eq. 1 is the molecular force due to Lennard–Jones (LJ)
potential between particle i and other fluid molecules in the
calculation domain, and the second term is the molecular
force between particle i and all the solid wall particles j.
The last term in Eq. 1 represents the external force, which
makes the fluid deviate from the equilibrium, such as
gravity, electric force, or pressure. When a two-body
123
1.1 Thermal wall model
When the fluid flows inside the solid boundary, if a fluid
molecular is quite close to the wall surface, the repulsive
force between the fluid particles and solid molecules will
push the fluid particle away from the wall surfaces. Physically such a force interaction will never let the fluid particles penetrate the wall surfaces. However, in the real
computation, one cannot guarantee that any of the fluid
Microfluid Nanofluid (2010) 9:1011–1031
particles does not travel beyond the wall surfaces. This is
because it is impossible to use an infinitely small time step.
Owing to the above reason, a thermal wall model is
introduced as an accessorial boundary conditions.
During the computational process through the time
series, for most time steps, none of the particles travels
beyond the wall surface. Incidentally, there are some time
steps that have a couple of particles striking the wall surfaces. In this situation, the thermal wall model is used to
ensure that all the fluid particles are confined in the two
parallel walls. In other words, the thermal wall model is to
reallocate velocity vector of the fluid molecules infinitely
closed to the solid wall based on the real physical principle.
Take the fluid confined between two parallel solid walls as
an example. When a fluid molecular strikes a thermal wall
at temperature Tw, all the three components of velocities
are reset to a biased Maxwellian distribution. In the
Cartesian coordinate system, the three velocity components, after the fluid particles strike the wall surfaces, are
given by Alexander and Garcia (1997):
qffiffiffiffiffiffiffiffi
vx ¼ kBmTw wG ;
qffiffiffiffiffiffiffiffi
ð5Þ
vy ¼ kBmTw w0G ;
qffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi
vz ¼ 2kBmTw ln w
The positive sign of vz is for the fluid particles striking
the bottom wall surface, while the negative sign is for the
fluid particles striking the upper wall surface. w is an
uniformly distributed random number in (0,1) and wG, w0G
are Gaussian-distributed random numbers with zero mean
and unit variance. The detailed reentry mechanism at the
thermal wall is described by Tenenbaum et al. (1982).
1.2 Initial conditions
The initial conditions provide the information of the simulation regions to activate the numerical computation.
Taking the crystal fluid confined between two solid walls
as an example, the procedure is summarized as follows:
•
•
•
The solid wall molecules are arranged in terms of FCC
structure, and such an arrangement is not changing
during the whole calculation process, because the two
solid walls are rigid.
The initial positions of fluid molecules are structured
according to FCC. However, the fluid molecules will be
melting once the applied force acts on the fluid
molecules.
Randomly distributed velocities in the fluid region are
assumed to activate the calculation. However, in order
to make sure that the steady state can be easily reached
after some reasonable time, the randomly distributed
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velocities should satisfy that the total kinetic temperature is equal to the kinetic energy in the fluid
calculation domain:
N
3
1 X
NkB Tfluid ¼ m
ð6Þ
v2i;x þ v2i;y þ v2i;z
2
2 i¼1
•
Values for the initial acceleration ai(0) are determined
in terms of the positions ri(0) by computing the force on
each atom, and applying the Newton’s second law. If
the Gear finite-difference algorithm is used as the
integral method, the higher derivatives are also needed.
These higher derivatives are assumed to be zero for the
initial time step to activate the calculation.
iv
v
x000
i ð0Þ ¼ xi ð0Þ ¼ xi ð0Þ ¼ 0
000
iv
v
ð7Þ
yi ð0Þ ¼ yi ð0Þ ¼ yi ð0Þ ¼ 0
iv
v
z000
ð0Þ
¼
z
ð0Þ
¼
z
ð0Þ
¼
0
i
i
i
For other types of fluid and the solid walls, the solidstate molecular structure should be used as the initial
position.
1.3 Periodic boundary conditions
Because of the limitation of the computational ability, it is
impossible to simulate all of the molecules in the flow
system. In order to solve this problem, a feasible method
involves the use of the periodic boundary conditions. In
this method, a unit cell or computational domain far from
the system’s edge is considered. The flow field in the whole
system is the periodic recurrence of the flow field of this
unit cell. When a molecule passes through one face of the
unit cell, it reappears on the opposite face with the same
velocity. Take the confined fluid flow between two parallel
plates as an example. In the Cartesian coordinate system,
the periodic boundary conditions are applied in x and y
directions, and the length of the unit cell is Lx in x direction. When a fluid particle is leaving the boundary at x = 0
or x = Lx, another fluid molecule will enter the unit cell at
x = Lx or x = 0. The particle entering the unit cell has the
same velocity as the fluid molecule that is leaving the
calculation domain. This principle ensures that the total
fluid molecule number in the unit cell is constant.
As mentioned above, the unit cell is a small part of the
real fluid flow system. When we use the periodic boundary
condition, we assume that the real fluid flow system is the
periodical repetition of the unit cell. Therefore, when we
compute the molecular interaction force, the image force
shall be included. For instance, fluid particle i has the
molecular interaction with particle j in the unit cell.
However, particle j located at (xj, yj, zj) has a series of
image particles outside of the unit cell located at (xj ± nLx,
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Microfluid Nanofluid (2010) 9:1011–1031
yj ± mLy, Lz) where n and m are integers ranging from 1 to
infinity. In order to reduce the computational time for the
force calculation of particle i with any particle j in the unit
cell and its particle images, Eq. 1 is corrected in terms of
Haile (1992):
~
F ij ¼
aX
x ¼1
aX
y ¼1
~ij aLÞ
d/ij ðr
drij
a ¼1 a ¼1
x
represents the direction normal to the solid walls. We
define the function Hn(zi) such that
Hn zi;j ¼ 1 if ðn 1ÞDz\zi \nDz;
ð9Þ
otherwise
Hn ðzi;j Þ ¼ 0
ð8Þ
y
where L is Lx in x direction, and Ly in y direction. a is the
cell translation vector. Eq. 7 accumulates forces for molecule i interacting with molecule j inside the fluid calculation domain and its images outside of the unit cell. Note
that Eq. 7 is also valid for the force integration between
particle i with any solid wall particle jw and its images
outside of two solid wall regions.
A minimum-image criterion has been developed to the
calculation of Eqs. 7 and 1. For a cubic container in three
dimensions, the minimum image criterion applies separately to each Cartesian component of the pair separation
vector. For the x component, we use xij ? xij - axLx where
ax = 0 if -0.5Lx B xij B 0.5Lx, ax = -1 if xij B -0.5Lx,
and ax = 1 if xij C 0.5Lx (Haile 1992). Similar treatment
should be used for yij.
where the subscript j represents the j time step.
Then, the average non-dimensional number density in
nth bin from JN time step to JM time step is
qn r3 ¼
JM X
N
X
r3
Hn zi;j
ADzðJM JN þ 1Þ j¼JN i¼1
123
ð11Þ
where zi is the coordinate of the midpoint of the nth bin,
and A is the area expressed as Lx 9 Ly. JN and JM are,
respectively, the starting and the ending time steps of the
parameter averaging. The integrated time interval from JN
time step to JM time step is larger than 150s. Longer time
interval also results in no change in the results of the
parameter averaging. The bin average velocity from JN
time step to JM time step is given by
uðzi Þ ¼
1
ðJ M J N þ 1 Þ
1.4 Parameter averaging
By integrating the Newton’s second law equation temporally and spatially, the position, velocity, and acceleration
of the molecules are obtained. All of these values are for
individual molecules. However, what we are interested in
are the macro quantities of the bulk fluid, such as the density, velocity, and pressure. Therefore, statistical thermodynamics must be used to complete the transformation from
the micro quantities to the macro quantities. The following
summarizes the process of the parameter averaging.
Temporally, the appropriate integral methods, such as
the Gear finite-difference algorithm, are employed for the
dynamics simulation of the molecular system. The time
step is chosen from Dt = 0.005s to Dt = 0.0005s
depending on the amplitudepofffiffiffiffiffiffiffiffi
the applied force, where s is
the LJ reduced time s ¼ r m=e: For a large driven force
or a large shear rate, the fluid particle has a small characteristic time response to the large applied force. Spatially,
the unit cell is divided into many bins. The number of bins
is dependent on the fluid molecule numbers. For larger
number system, more bins are divided. The macroscopic
parameters, such as the number density, mean velocity,
temperatures, are defined in the center of each bin. These
parameters can be obtained via statistical mechanics, and
the detailed procedures are summarized as follows. Taking
the confined flow in two parallel plates as an example, we
calculate these parameters as a function of Z, where Z
ð10Þ
PN
JM X
N
X
i¼1 Hn ðzi;j Þ j¼JN
Hn ðzi;j Þvxi;j
i¼1
ð12Þ
where vxij is the velocity in x component of particle i at j
time step. Using Eq. 13, we compute the bin temperature as
Tðzi Þ ¼
1
P
3kB ðJM JN þ 1Þ Ni¼1 Hn ðzi;j Þ
JM X
N
h
i2
X
Hn ðzi;j Þmi vai;j ua ðzi Þ
ð13Þ
j¼JN i¼1
where the superscript a represents x, y or z. At steady state,
uy(zi) and uz(zi) are zero for all the bins.
2 Pressure-driven flows
Pressurized flow is a general mode of flow in nanochannels. Two fundamental physical processes are involved
here, namely, the filtration of fluids into the nanochannel
and the transport of fluids inside nanochannel. In the filtration process, the flow resistance and the structure change
of the liquid are key factors. In the transport process, the
bulk average velocity and molecular structure of liquid are
focal points. There are many reported research studies of
modeling and numerical simulation of the pressure-driven
transport processes in nanochannels. The validity of the
continuum theory in nanoscale is examined by comparing
the result of MDS with those using Navier–Stokes (NS)
equations.
Microfluid Nanofluid (2010) 9:1011–1031
2.1 Infiltration flow
The fundamental infiltration and defiltration mechanisms
of nanofluidics are distinct from that of bulk phases. For
smaller channel sizes, such as several nanometers, the
relationship between molecular structure and the flow
velocity is concerned. Thomas and McGauthey (2009)
simulated pressure-driven water flow through 0.83–1.66-nm
diameter armchair single-walled carbon nanotubes
(SWCNTs) in the NVT ensemble. TIP5P potential was
used to model the interactions between water molecules
(Mahoney and Jorgensen 2000). The interaction of wall
molecules and carbon atoms was modeled using LJ
potential of Werder et al. (2003). In order to maintain the
temperature of the system, a Berendsen thermostat in the
velocity components transverse to the flow direction was
employed. The authors found that employing the thermostat to all the three directions did not affect the predictions
about the flow. The authors drew two conclusions. First,
unlike the continuum theory, the flow enhancement in
subcontinuum systems may not increase monotonically
with the decrease in flow area. On the contrary, when the
flow cross-sectional area is comparable to the size of
the liquid molecules, confinement-induced changes to the
liquid structure may reduce the flow enhancement. The
authors identified the critical diameter of the flow cross
section, which is between 1.25 and 1.39 nm, just as shown
in Fig. 1. Second, the liquid structure and liquid flow are
dependent when the characteristic flow time scale is comparable to the molecular structure relaxation time. As
Fig. 1 a Relationship between average flow velocity and applied
pressure gradient for the 75-nm-long CNTs. b Variation in flow
enhancement factor with CNT diameter. The dashed line between
D = 1.25 nm and D = 1.39 nm delineates continuum and subcontinuum flow regimes (Thomas and
McGauthey 2009). Note: By Darcy
Dp
law, the flow velocity v ¼ c Dp
L ; where L means the pressure
gradient, and c means the hydraulic conductivity. There exist three
factors causing the actual hydraulic conductivity to exceed that
calculated from the Poiseuille relation, which is the liquid slip at the
solid–liquid boundary, confinement-induced reductions in the liquid
viscosity, and subcontinuum changes to the liquid structure. Flow
enhancement factor means that the ratio of actual c and the no-slip
Poiseuille c
1015
shown in Fig. 2, the water molecular structure varies
according to the CNT diameter, from single-file molecular
chains (0.83 nm), tilted pentagonal rings (0.97 nm),
stacked pentagonal rings (1.10 nm), stacked hexagonal
rings (1.25 nm), and to disordered bulklike water (1.39 and
1.66 nm). The authors established the relationship between
the molecular structure and the flow enhancement. In the
subcontinuum scale (D B 1.25 nm), the transport of molecules in these structured subcontinuum systems is contingent upon the movement of nearby layers. A layer of
water molecules that fills an energetically stable CNT
surface site can impede the movement of other layers. Such
localized limitations on transport will reduce velocity and
lower the overall flow enhancement.
In most infiltration studies, the liquid molecules were
placed in vacuum nanotubes or nanochannels (Hummer
et al. 2001; Holt et al. 2006). The absolute vacuum condition is difficult to achieve in real experiments. In a bulk
liquid, the gas nanophase that typically consists of a few to
several hundred gas molecules often has secondary influence on the liquid motion, in part due to the low gas
molecule density that is usually a few orders of magnitude
smaller than that of liquids. However, in a nanochannel,
due to the radial confinement, the effective gas molecular
density significantly increases. If the nanotube diameter is
smaller than a few nanometers, then a single gas molecule
could make it difficult for the infiltrated liquid molecules to
bypass it. Qiao et al. (2007) showed that the gas molecules
in relatively large nanochannels could be dissolved in the
liquid during pressure-induced infiltration. However, the
important role of gas phase was ignored in the previous
studies. The authors found that the gas molecules tend to
form clusters in relatively small nanochannels, which
triggers liquid defiltration at a reduced pressure. The
authors studied a cluster of 12 carbon dioxide molecules in
water confined by CNTs of four different radii. The CO2
cluster was placed in the middle of a long open-ended tube
and surrounded by water molecules, and the MD simulations were carried out at a constant temperature with a
constant pressure, using a condensed-phased optimized
molecular potential for atomistic simulation studies (Sun
et al. 1998). The MDS in this article not only shows the
dependence of the defiltration behavior on the pore size and
the pore surface properties, but also reveals the inherent
interactions between gas and liquid phases, where the
effective gas solubility highly depends on the characteristic
length scale. In a nanochannel, even a single gas molecule
can significantly promote the liquid infiltration and may
make the confined liquid unstable. The low effective gas
solubility in a small nanochannel leads to the formation of
trapped gas clusters during infiltration and the outflow
behavior during defiltration, whereas the liquid–solid
interaction is dominant after the gas phase is dissolved in
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1016
Microfluid Nanofluid (2010) 9:1011–1031
Fig. 2 a Water structures inside
the 0.83–1.66-nm-diameter
CNTs. Carbon atoms are
removed for clarity, and the
chirality vector for each CNT is
provided. b Axial distribution
function (ADF), structure
relaxation time s, and extent of
the ADF, Lt, for each CNT.
c P(n, tc), the probability that
n molecules cross the system
midplane over the characteristic
flow time tc, and the CNT
permeability a is provided for
pressure gradient with
4 9 1014 Pa/m (Thomas and
McGauthey 2009)
larger nanopores or after the gas phase is diffused out of
small nanopores.
Qiao et al. (2009) performed MDS of water flowing in
silicon dioxide nanochannel by using the COMPASS force
field. They considered a straight nanochannel with a
diameter of 0.83 nm. One end of the nanochannel was
closed. The effective pressure was computed from the state
function of water, and the redistribution of water molecules
with pressure variation reflects the adiabatic pressure-driven infiltration. The authors analyzed the resistance as
and when the water molecules enter the nanochannel. The
123
energy barrier that the water molecules need to overcome
in order to enter the nanochannel includes two parts. First
part is the change of the free energy of the infiltrated
molecules due to each water molecule losing two hydrogen
bonds when it enters the nanochannel. Second part is the
van der Waals and electrostatic interactions between water
molecules and nanochannel atoms. After the infiltration
occurred, the driving pressure is still increased almost
linearly with the volume difference, which implied that the
continued infiltration had to overcome not only the initial
energy barrier but also a certain resistance that varied with
Microfluid Nanofluid (2010) 9:1011–1031
the infiltration volume. It is referred to as column resistance. In a nanopore with the diameter comparable with the
liquid molecule size, most of the infiltrated water molecules are in direct contact with the solid surface, which
caused column resistance.
Liu et al. (2009) use MD to explore insights into the
complex behaviors of liquid infiltration into cone-shaped
nanopores. The new contribution of this article is the study
of flow in nanochannels with a varying cross-section, while
most previous studies of nanofluidics were limited to
nanochannels with an invariant cross-section. The liquid
and the solid are water and carbon nanocone, respectively.
The authors used a series of existed molecular model,
potential parameters, and experimental value for building
CNTS and CNCS model. The authors used the LAMMPS
(Plimpton 1995) (large-scale atomic/molecular massively
parallel simulator) package, with the NVT ensemble and
the temperature fixed at 300 K. Water molecules are
modeled by the rigid extended simple point charge potential SPC/E (Berendsen et al. 1987), while the carbon–
oxygen LJ parameters are extracted from the experimental
low-coverage isotherm data of oxygen adsorption on
graphite. The following are the findings of this article.
Under ambient conditions, the applied pressure needs to be
higher than a critical infiltration pressure so that water
molecules may flow into a nanotube, and such an infiltration pressure is higher for smaller nanotubes. Spontaneous
infiltration initiates when the apex angle of nanocone is
large despite the hydrophobic nature of the solid phase.
However, water cannot wet the entire nanocone. Furthermore, with the same blunt cone angle, a long nanocone and
a short nanocone may exhibit distinct wetting properties.
Enlarging the apex angle always leads to a lower pressure
for liquid to reach the same pore size, and hence the easier
infiltration.
2.2 Special statistical method for low speed flows
In Sect. 1.4, we introduced the transformation method from
the micro quantities to the macro quantities. In the MDS
method, the total velocity of molecules consists of the
thermal motions velocity and the liquid flow velocity
caused by the externally applied forces. The total liquid
flow velocity is calculated by summing up the thermal
motion velocity and the external force-driven flow velocity,
temporally and spatially. In general, the thermal motion
velocity of molecules is on the order of several hundred
meters per second. Theoretically, if the time averaging is
performed for infinitely long time, then the summation of
the random thermal motion velocity will be zero. However,
in practice, the time averaging is conducted over a limited
period of time, and hence the summation of the random
thermal motion velocity may not be zero. Therefore, when
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the external force-driven flow velocity is \1 m/s, the
thermal motion velocity will affect the average value dramatically so that the MDS method cannot extract the true
bulk liquid flow velocity. In these cases, the bulk liquid
flow velocity is overestimated. This has been verified by
the error theory and simulation analyses (Zhang and Li
2007). In order to extract the true liquid bulk flow velocity
caused by the externally applied forces, Zhang and Ely
(2004) proposed a new linearized algorithm, where the
total flow velocity is the linear accumulation of the flow
velocity increment of each time step. In each time step,
using the linear development of the particle interaction
force function in MDS method, the force increment associated with the external force can be separated from the
total increment of the particle interaction force. Then, the
increment of the flow velocity can be calculated. The total
flow velocity is the accumulation of the increments over all
time steps. When the interval of time step is smaller than
10-16 s, the algorithm is convergent. This interval of time
step is smaller than that applied in the conventional MDS
method.
2.3 Special applications
Conventional injection involved in spray combustion
devices has been widely studied. In recent years, numerous
studies have attempted to predict nanoscale jet breakup by
using non-equilibrium MD (Branam 2005; Ludwig 2004;
Micci et al. 2000; Moseler and Landman 2000; Shin 2006).
Kim (2007) developed a non-equilibrium MD code and
applied it to simulate nanojetting and electrowetting phenomena. The liquid and solid are argon and platinum,
respectively. The sum of the LJ potential and the Coulomb
potential was adopted. For liquid–solid interaction, the LJ
potential was modified by the intermolecular parameters,
a and b, between liquid and solid. In this study, the
nanojetting mechanism from droplet ejection, breakup,
wetting, and the drying process was identified by the
simulation, with a = 0.5 and b = 0.5. Three types of
typical wetting phenomena were simulated to understand
the effects of intermolecular forces on the surface tension
and contact angle. Three different wettabilities (full wetting, intermediate wetting, and no wetting) are obtained
under three potential parameters condition of b = 1.0,
b = 0.25, and b = 0.1. In addition, a conceptual nanopumping system was simulated using the electrowetting
phenomenon. For the homogeneous flow in nanotube, the
author found that those wall effects become more serious
as the diameter decreases from 12 to 3 nm. For flow in a
charged nanotube, the negative surface charges attract the
counterions to the wall surface. On the other hand, repulsive forces are induced between fluid and wall particles,
causing the slip flow at wall surface. Therefore, the authors
123
1018
drew a conclusion that the sign of wall surface charge
determines the flow resistance that is inversely proportional
to flow rate while applying the same driving force.
3 Electric field-driven flows
Pressure-driven flows in nanochannels need a large pressure gradient, which is difficult to achieve experimentally.
Therefore, other driving forces, such as a surface tension
difference (de Gennes et al. 2003), a chemical gradient
(Chaudhury and Whitesides 1992), a temperature gradient
(Linke et al. 2006), and electric field (Kuo et al. 2001;
Mitchell et al. 2000; Daiguji et al. 2004; Ermakov et al.
1998; Freund 2002; Qiao and Aluru 2003) have been
considered.
3.1 Fundamental research
Electroosmotic flow is an important fluid transport mechanism in nanofluidic system. In general, there is an electrical double layer (EDL) near the solid–liquid interface
when an ionic solution is in contact with a charged solid
surface. If an external electrical field is applied in the
direction tangential to the surface, the fluid will be dragged
by the moving ions in the EDL and an electroosmotic flow
is generated. The key parameters of the electroosmotic flow
in nanochannels are the zeta potential, the density distribution of the solution and ions, and the velocity profile in
the channels. There are several other factors affecting the
above physical parameters, such as the surface roughness,
the hydrophobicity of the solid wall, the external electric
field strength, the charge density, and the polarity of the
surface charges.
In the MDS of electroosmotic flow, the Coulomb
potential should be added to the LJ potential for the
charged particle pair. The general expression is
"
#
r 12
r 6
qi qj
Vðri;j Þ ¼ e
þ
ð14Þ
þ e0
rij
rij
rij
where qi, qj are the charge of the charged particle pair. In
general, the electrostatic interactions were computed using
the particle-mesh Ewald (PME) method (Darden et al.
1993) for the Coulomb interactions.
For electroosmostic flow, the charged atoms were driven
by the electric filed force. Therefore, the Newton’s Second
Law should be written as follows:
N
X
o/ rij
mai ¼
þ Eqi
ð15Þ
orij
j¼1;j6¼i
Modeling and simulation of electroosmotic flow in
nanometer scale channels can address many fundamental
123
Microfluid Nanofluid (2010) 9:1011–1031
issues currently encountered during the design of
nanofluidic systems (Kuo et al. 2001). By far, the most
popular method to simulate the electro-osmotic flow is
based on the classical continuum theories, such as the
combination of Poisson–Boltzmann (PB) equation for the
ion distribution and NS equations for the fluid transport
(Mitchell et al. 2000; Daiguji et al. 2004; Ermakov et al.
1998). However, some important information dominated in
nanoscale would be ignored while using the continuum
method. For instance, the ions are modeled as point
charges, and the water is modeled as a dielectric continuum
in the PB equation. The molecular nature of the ions and
the discreteness of the water molecules are not accounted
for in the PB equation (Darden et al. 1993). Several articles
have shown the discrepancies between the MD results and
the continuum ones.
The MDS can provide a qualitative understanding of the
various physical processes without the assumptions built
into the continuum theory. Freund (2002) found the profile
differences of the ion density and the water velocity near
the walls derived from the two methods. Qiao and Aluru
(2003, 2005) published a series of articles on this topic.
They modified the PB equation by adding MDS and simulated more realistic model systems. They found that the
direction of electro-osmotic flows is opposite to that predicted by the continuum equation under the condition that
ions have the same sign of charge as the walls. They also
found that the ionic distribution is different in positively
and negatively charged channel walls due to different
hydrogen bond patterns. Moreover, this phenomenon cannot be observed by using continuum method. Joly et al.
(2004) reported that the zeta potential increased when the
slip near hydrophobic walls existed. Therefore, the continuum theory may be invalid at smaller nanoscale systems.
In any case, MDS is a powerful tool to investigate the flow
and ion distribution in nanoscale.
Qiao and Aluru (2005) investigated the influence of the
finite size of the ions and the water molecules on the ion
distribution, and the effect of surface–fluid interactions on
the electroosmotic transport. The simulation system consists of a slab of KCl solution sandwiched between two
oppositely charged channel walls. The models in this
article are approximately the same as that used in Darden’s
study (Darden et al. 1993). The ions distribution in nanochannels is not coincident with the Boltzmann distribution.
Figure 3 shows the distinct results derived from the continuum method and the MD simulation. For Cl- ions, the
first concentration peak is about 81% higher compared to
the PB theory prediction, and the concentration does not
decrease monotonically to its value in the channel center as
PB equation predicts. For K? ions, the concentration is
substantially different from that of the Cl- ion concentration. Particularly, the K? ion concentration appears to have
Microfluid Nanofluid (2010) 9:1011–1031
Fig. 3 K? ion and water concentration profiles across the channel
(Qiao and Aluru 2005)
two distinct peaks. The authors explained that the first peak
is related to the interaction of K? ion and the walls. The
second peak is mainly caused by the interaction between
the ion and its hydration water molecules. In an electrolyte
solution, the water molecules near an ion are loosely
bonded to the ion due to the strong charge–dipole interactions between the ion and the water molecules. These
water molecules are called hydration water. Because of this
interaction, the water distribution will affect the ion distribution. It is well known that the water density oscillates
near the wall, and so there is the second peak of ions. For
water and ion transport, the MD results showed that the
electro-osmotic velocity in a negatively charged channel is
much higher than that in a positively charged channel. The
authors calculated the water viscosity and found that the
viscosity is much higher near a positively charged surface
compared to that near a negatively charged surface. The
authors established the relationship between the water
molecular structure, especially the hydrogen bonding, and
the various properties. The hydrogen bonding is referred as
the H–H bonding between two water molecules. In the
positively charged surface, the number of hydrogen bonding is much larger than that in the negatively charged
surface. The larger the number of the hydrogen bondings,
the higher the water viscosity.
Kim and Darve (2006) studied the effects of solid surface roughness on the density profile, the zeta potential, the
ionic distribution, and the velocity profile. One of the key
issues in electroosmotic flow related to the roughness was
proposed in this article: The zeta potential is influenced by
the roughness. It should be noted that the surface potential
and the zeta potential are different. The zeta potential is
defined as the electrostatic potential at the slip plane. In
electrokinetic theory, the surface potential is approximated
1019
by the zeta potential because it is impossible to measure the
surface potential. The zeta potential would deviate significantly from the surface potential when the influence of
surface roughness increases so that the location of the slip
plane is changed. The structure of electric double layers on
charged rough walls was also addressed in several books
(Bikerman 1970; Dukhin and Derjaguin 1974). In the
computational model (Darden et al. 1993), the authors
applied several simplified processes, which may influence
the reliability of the conclusion. Their key assumptions are
listed as follows. The walls were modeled as a simple cubic
crystal structure and fixed at each lattice site. When constructing rough wall channels, the extra partial layers of
wall atoms were added only in two-dimensional direction.
Only counterions were included for simplicity and computational efficiency. The authors combined several existed
models together to simulate the effect of the roughness to
electro-osmotic flow. The sodium ions were modeled as
point charges with the LJ potentials. For water molecules,
the authors used the extended simple point charge model
[SPC/E (Berendsen et al. 1984)]. The GROMACS code
(Spoel et al. 2004) with GROMOS-96 force field was used
except for wall atoms. For the interactions of wall atoms
with other types of atoms, the authors applied the LorentzBerthelot combination rule. For the calculation of electrostatic potentials, the PME method (Darden et al. 1993) was
used. In order to constrain water molecules, the SETTLE
algorithm (Miyamoto and Kollman 1992) was used. Very
high electric field strength (0.1 V/nm) was applied for
avoiding relatively large thermal noises which result in
large statistical errors. Because of the layering of water
molecules and the finite-size effect of ions and walls, the
ionic distribution deviates from the Boltzmann distribution.
The polarization density, expression of the structure of
water molecules and ions, was computed. The polarization
density component in the direction normal to the wall
dominates over the other components. This result indicated
that there existed the preferred orientation of water molecules. For rough walls, the preferred orientation is more
evident inside the groove. With the use of the velocity
autocorrelation function, the residence time and the diffusion coefficient showed that the diffusion of water and ions
in the direction normal to the wall is reduced near the wall
and further reduces inside the groove. The zeta potential
would decrease as the period of surface roughness
decreases or the amplitude of surface roughness increases.
3.2 Pumping application
Fluid can be transported by electric or magnetic fields if
there are ions or magnetic quanta in the fluid. However,
pure water is charge-neutral and has no magnetic moment.
Understanding and controlling the water transportation
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Microfluid Nanofluid (2010) 9:1011–1031
Fig. 4 Introduction to the main
system. The three circles on the
right side of the cylindrical
channel represent the charges
that drive the water flow
through the nanochannel. a Side
view of the main system. b Top
view of the same arrangement
(Gong et al. 2007)
through nanochannels is of great importance for designing
novel molecular devices and has wide applications
(Whitesides 2006; Whitby and Quirk 2007; Regan et al.
2004; Service 2006; Holt et al. 2006; Bourlon et al. 2007;
Besteman et al. 2003; Ghosh et al. 2003).
Gong et al. (2007) proposed a design for a molecular
water pump on the basis of MD simulations. Figure 4
shows the principle of the design. The model system is the
uncapped armchair SWCNT. Three positive charges were
arranged outside of the nanotube along the longitudinal
direction, two of which were of symmetrical distribution
versus the mid-point of the nanotube length. The third
charge is positioned at the bottom of the nanotube. The
water dipole orientation angle along the length of the
channel follows the regular distribution: the water dipoles
near the bottom end point down, whereas the water dipoles
near the top end point up, showing a bipolar order. Such
bipolar structure could produce biased electrostatic potential, which could push water molecules through the nanochannel. The authors compared the effectiveness of other
systems (such as only one charge at the end of the nanotube) with the above system (called the main system) by
analyzing the water dipole orientation angle and corresponding potential structure. For the main system, the
change of the water dipoles orientation was slower than the
other systems. Correspondingly, there was less deep
potential well, and hence, the water permeation across the
channel was easier. Meanwhile, it should be noted that the
single-file structure of water inside the channel was crucial
to the water dipole orientation distribution being shielded
from thermal fluctuations. For wider channels, the thermal
fluctuations will reduce the regular bipole distribution,
which smoothes the asymmetries of the potentials and
weakens the pumping abilities.
3.3 Particle separation or screening
Selectivity in ion transport through nanochannels is an
important branch of nanofluidics and has important applications. Banerjee et al. (2007) used MDS methods to
demonstrate the utility of CNTs for water and ion separation
123
from a salt solution. Water was modeled using the simple
point charge (SPC) model (Berendsen et al. 1981), ions
using the so-called primitive intermolecular potential model
(Chandrasekhar et al. 1984; Jorgensen et al. 1982), and
CNTs using the parameters provided in Turner et al. (2002).
The new contribution of this study is to describe the role of
alternating spatial or temporal charge patterns in accomplishing the controlled intake of either ions or polar solvents
such as water. The results showed that when spatially or
temporally alternate charge patterns were applied to CNTs,
the ion intake is minimal while allowing water passing
through the CNTs. The implication is that CNTs could be
used for the preferential intake of water molecules as waterpurifying devices (or conversely as ion concentrators for the
solutions external to CNTs).
The CNTs have been used for various sensing applications (Mashl et al. 2003; Li et al. 2004; Saito et al. 1992;
Benedict et al. 1995; Chen et al. 2005; Li and Lin 2006),
such as chemical sensors, for selective detection of nitrogen oxide and ammonia (Mahar et al. 2007). Xu and Aluru
(2008) investigated the screening effects of semiconducting and metallic single-walled CNTs (SWCNTs) when the
water molecules and various charged ions pass through the
nanotubes. It is shown that metallic SWCNTs have much
stronger screening abilities than semiconducting SWCNTs.
The authors thought that relatively fewer efforts have been
invested to study the polarizability and the screening
effects of CNTs under electric fields generated by water
dipoles and charged ions inside SWCNTs. In this article,
the structure of water and ions inside the SWCNTs is
obtained by performing MD simulations. The results from
MD simulations are then used in tight-binding (TB) simulations to investigate the screening effects of metallic and
semiconducting SWCNTs. The authors considered 5.3 nm
long hydrogen-terminated metallic and semiconducting
CNTs attached to reservoirs at both ends. Both the CNTs
have similar diameters but different electric properties.
This article demonstrated how to integrate the MD method
with self-consistent TB (tight binding) calculations and
ab initio methods. In the MD simulations, the initial systems were equilibrated for 100 ps under a constant pressure
Microfluid Nanofluid (2010) 9:1011–1031
of 1 bar and then switched to NVT ensemble (the number
of particles (N), the volume (V), of each system in the
ensemble are the same, and the ensemble has a welldefined temperature (T), determined by the temperature of
the heat bath.). Non-equilibrium MD simulations were
performed for ion transport to obtain the coordinates of
water molecules and the ions at intervals of 1 ps for TB
simulation.
Yang (2007) studied water structure in negatively
charged model cylindrical nanopores, as well as the partitioning of positive ions of increasing size into the pore
interior by using MD simulations. The authors used a piece
of (5,5) armchair CNT pore comprising 100 carbons as a
model cylindrical pore. Charges were distributed uniformly
on the pore atoms. The aim of this article is not to model
specifically a CNT but to use its cylindrical geometry as a
model for a cylindrical pore. Simulations were performed
using AMBER6.0, TIP3P model of water, and LJ
description of carbon. Ions were represented as LJ spheres
with ion charge placed at the center. Ion–water and ion–
carbon LJ interactions were calculated using Lorentz–
Berthelot mixing rules. The PME method was used to
calculate the electrostatic interactions with grid spacing of
1 Å. Temperature and pressure were maintained at 300 K
and 1 atm, respectively, using the Berendsen method. A
time step of 1 fs was used in the simulations. This study
found that the nanopores display selectivity toward partitioning of the larger cations over that for the smaller ions.
The absence of the equilibrium kinetic simulations shows
that the partitioning is significantly slower for Na ions
compared to that for K and Cs ions, especially for lower
charge densities on the pore. Thermodynamic and kinetic
studies collectively suggest the presence of a barrier for
partitioning of cations into the nanopore interior. Such a
barrier is expected to slow down the flow rates of ions
through nanopores.
4 Thermally driven flow
When particles are added into a quiescent fluid that is
subjected to a temperature gradient, they tend to migrate
toward the cold end. The phenomenon is called thermophoresis. The origin of the thermophoretic force was first
suggested by Maxwell (1879). The mechanism of the
phenomenon is as follows. Since the molecules from the
hotter region have a higher momentum tangential to the
surface than those from the colder region, the total interaction may result in the thrust on the wall or the particle
toward the cold region. In contrast to gases, the theory and
the experiment of thermophoresis in liquids are far from
well established even in the simplest case of a neutral
particle in a non-conducting liquid. The difficulty for
1021
thermophoresis in liquids lies in the fact that there may be
some mechanism responsible for the thermophoretic flow
other than the kinetic interaction. Nevertheless, thermophoresis has practical implications in the fields such as the
bore stability in the oil industry, the particle accumulation
in a thermal boundary layer, and the transport of polymeric
molecules in the microchannels.
Han (2005) studied thermophoresis by MD. The authors
believed that the kinetic theory on rarefied gases cannot
predict a finite thermophoretic velocity observed in the
liquids. Moreover, the intermolecular interaction potential
plays a dominant role in the liquid state. Since the liquid
atoms were under the influence of other particles’ potential
and the fluid may become inhomogeneous at the solid–
liquid interface, it is desirable to understand the dynamics
in the solid–liquid interfacial region more clearly. A rigid
and neutral particle with diameters of about 1 lm was
immersed in quiescent non-conducting liquid. The temperature difference of 1 K is applied over a distance of
100 lm. The authors divided the computation domain into
two sub domains: quiescent liquid domain far from the
particle and creeping flow domain close to the particle.
Thus, the computational cost would be reduced dramatically. In the quiescent liquid domain, analytical method
was used. In the domain near the particle, MD method was
used. By combining the two methods, it is shown that the
temperature gradient applied to the non-conducting liquid
induced the pressure gradient tangential to the neutral
particle surface. The model didn’t consider any charge or
charged materials, whose effects may be very significant in
some cases. The dependence of the EDL as well as other
properties on temperature must be accounted for in many
cases. The phenomena may closely depend on the characteristics of the liquid structures developed in the interfacial region according to the given conditions. In the
colder region, a higher bulk density and the stronger
influence of the solid over the thermal mobility induce a
higher rate of increase of density and a higher tangential
pressure. As a result, a negative gradient of the tangential
pressure with respect to temperature is developed and the
particle moves to the cold end.
Two years later, Han (2008) published another article.
This article focused on the potential applications based on
thermophoresis, such as pumping operation. Figure 5
shows the principle of the pump. Owing to the presence of
solid, there always exists a pressure difference as shown by
the dashed line in Fig. 5a. The pressure difference collectively results in an unbalanced force occurring only in the
interfacial region Fig. 5b). The author studied four different types of systems using MD simulation. The four systems differed mainly in the channel configuration and the
way that the gradient was applied. The author found some
technical obstacles when designing the device and found
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Microfluid Nanofluid (2010) 9:1011–1031
Fig. 5 Illustration of the origin of thermophoretic force: a MD results of the tangential pressures with respect to the distance from the solid
surface; b the integrated effect of the unbalanced pressure occurring near the surface (Han 2008)
the solution for the difficulties. First, it was found that it is
difficult in imposing a sufficiently large temperature gradient in the small scale. In this case, the features like
thermal-contact-resistance at the interface need to be
included in design considerations. The second was a limited flow-development under an increased viscous drag in
the narrow channel. The first difficulty may be overcome
by connecting a single pumping unit of a modest gradient
with another in sequence. Assembling a large number of
the units would provide a necessary pumping power with
less limitation. The main idea of the novel design is as
follows. The signs of the temperature gradient and the
thermophoretic force alternate periodically. However, the
author produced a significant amount of thermophoretic
force using a weakly interaction wall or fluid in the region
of temperature gradient of a certain sing (for example,
minus in this case). Then, a larger amount of flow is
developed by the forces in the region where the temperature gradient is of the opposite sign (plus in this case), and
the net flow would be of a significant amount. The major
part of the simulation system consists of liquid argon and
platinum wall. The argon atoms interact with each others
through the LJ potential. A harmonic potential was used for
the atom–atom interactions in the Pt lattice. The thermally
insulating slip wall was introduced, and their atoms were
fixed in space in the same FCC lattice and interacted with
fluid atoms through only the repulsive potential. When the
temperature of the Pt walls needed to be controlled, the
scheme based on the so-called ghost particle was used,
which let the energy in and out to maintain a constant
temperature. The ghost particles are located in boundaries
of the simulation system and play the role of a thermal
reservoir. By using the readjusting temperature method,
only the velocity components in y and z directions, which
are normal to the flow, are involved in the scaling to
minimize the influence on particle drift.
123
5 Slip boundary condition
The flow behavior at the submicron scale strongly depends
on the boundary conditions at the solid–liquid interface. A
number of experimental studies showed that the no-slip
boundary condition is not valid in the submicron scale. The
most popular Navier model relates the slip velocity and the
shear rate with a proportionality coefficient, the slip length,
which is determined by the linear extrapolation of the fluid
velocity profile to zero. Many key parameters, such as
wettability, surface roughness, coupled fluid structure, and
shear rate, have effect on the magnitude of the slip length.
There are extensive literature reporting research studies in
this area (Churaev et al. 1984; Cottin-Bizonne et al. 2002;
Joly et al. 2006; Pit et al. 2000; Schmatko et al. 2005;
Bonaccurso et al. 2003; Sanchez-Reyes and Archer
2003; Schmatko et al. 2006, Vinogradova and Yakubov
2006; Migler et al. 1993; Horn et al. 2000; Craig et al.
2001; Choi et al. 2003; Koplik et al. 1989; Thompson and
Robbins 1990; Thompson et al. 1995; Thompson and
Troian 1997; Jabbarzadeh et al. 1999; Barrat and Bocquet
1999; Cieplak et al. 2001; Priezjev and Troian 2004; Galea
and Attard 2004; Priezjev 2007; Khare et al. 1996; Koike
and Yoneya 1998; Niavarani and Priezjev 2008a, b).
Niavarani and Priezjev (2008a, b) investigated the slip
phenomena in thin polymer films confined by flat or periodically corrugated surfaces by MD and continuum simulations. The LJ potential was employed for the wall–fluid
interaction. In addition to the LJ potential, the neighboring
monomers in the polymer chain interact with the finite
extensible nonlinear elastic potential. In this study, to avoid
a bias in the flow direction, the random force and the friction
term were added to the equation of motion in the y direction.
By using this method, the system will not be heated by the
friction, which is not reasonable. The findings of this article
are as follows. For atomically flat walls, the slip length
Microfluid Nanofluid (2010) 9:1011–1031
passes through a shallow minimum at low shear rates and
then increases rapidly at higher shear rates. In the case of
periodic surface heterogeneities with the wavelength larger
than the radius of gyration, the effective slip length decays
monotonically with increase in the corrugation amplitude.
At low Reynolds numbers, the inertial effects on slip
boundary conditions are negligible. When the corrugation
wavelengths are comparable to the radius of gyration,
polymer chains stretch in the direction of shear flow above
the crests of the surface corrugation, while the chains
located in the grooves elongate perpendicular to the flow.
As we all know, the substance consists of molecules
which are arranged according to a certain kind of spatial
structure. The arrangement of the molecules will form
different crystal planes where the properties vary. From a
microscopic point of view, the lattice arrangement of wall
atoms at the liquid–solid interface will influence the liquid
hydrodynamic characteristics. The surface orientation or
lattice plane is a solid wall characterized by its Miller
indices, which can be referred as a control parameter in
nanochannel flows. Soong et al. (2007) studied Couette and
Poideuille flows and explored the effects of wall lattice–
fluid interactions on the hydrodynamic characteristics in
nanochannels. The liquid confined between two parallel
planes is argon and LJ potential was used to model the
potential between fluid–fluid and fluid–wall atoms. The
thermostat was applied only to the wall atoms and the fluid
particles within the thin layer closest to the walls. There
exists another method which applied the thermostat to the
molecules in the entire fluid region. The authors employed
a hypothetical solid wall of FCC lattice structure with a
nonlinear spring model of interaction between wall atoms.
Taking the FCC crystal as an example, as shown in Fig. 6,
one can see that the molecules’ arrangement is different in
1023
different orientations. For FCC crystal lattice, there exist
three types of surface orientation: h111i, h100i and h110i.
The surface orientation will affect the flow behavior. Figure 7a and b shows the Couette and Poiseuille flows of the
usual LJ fluids. For both flows, among the three lattice
planes, the flow with a channel wall of the surface h100i is
the most insensitive to the variation of the flow orientation.
Khare et al. (1997) had compared the two approaches and
recommended the former one. By using this method, the
computational cost will be reduced. The MD results
revealed that the flow orientation with respect to the wall
lattice structure had very remarkable influence on the fluid
slippage and in turn the velocity profile and the flow rate.
With increasing wall–fluid interaction potential or wall
density, the density layering could be enhanced. Among
the three surface orientations, the slip length for the
smoothest wall, FCC (111) is the largest, especially at a
high wall density. By employing the wall surface FCC
(110) as a model, it was found that flow along the molecular trenches of the surface led to the largest slip length.
The MD simulations disclose that the influences of the flow
orientation are quite distinct for various lattice planes. The
fluid slippage and the flow rate will be different if the
channel walls are of different lattice planes and/or the fluid
flows over the wall at a different orientation angle.
Yang (2006) carried out non-equilibrium MD simulations to investigate the effect of surface roughness and
interface wettability on the nano-rheology and slip boundary condition in nanoscale. The roughness of the wall was
performed by decorating the wall with periodic nanostrips
of a certain height and width in x and y direction. The
simulation results showed that the surface roughness suppresses the fluid slip for both of the hydrophilic and
hydrophobic surfaces of nanochannels. For smooth and
Fig. 6 Flow channel model,
surface orientation, and flow
orientation. a Nanochannel
model, b face-centered cubic
crystal lattice; c surface
orientation or crystal plane;
d flow orientation (Soong 2007)
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1024
Microfluid Nanofluid (2010) 9:1011–1031
Fig. 8 Snapshots of liquid argon flowing through nanochannels.
a Hydrophobic surface; b hydrophilic surface (Yang 2006)
Fig. 7 Effects of flow orientation on a Couette and b Poiseuille flow
velocity distributions (Soong 2007)
hydrophobic surfaces, an air gap or nanobubble was found
to appear at the fluid–solid interface, which resulted in the
apparent slip velocity. The velocities of fluid molecules are
enhanced with the driving force, while the nanostructures of
fluid densities are independent of the driving force. The
results showed that the slip length increased with the
average fluid number density for hydrophobic nanochannels, while the effect of the average fluid number density on
the slip length is not obvious for hydrophilic walls. The
advantage of this model lies in that the wall molecules are
not fixed, and the interactions among the wall molecules
were determined by the LJ force and spring force. The
surface wettability or wall–fluid interaction was adjusted by
the length scale in LJ potential. In order to keep the temperature of the system constant, a Gaussian isokinetic
thermostat is used to adjust the wall temperature to a constant value at each time step. For a nanochannel with a
hydrophobic surface, as shown in Fig. 8a, an air gap or
nanobubble exists near the fluid–solid interface. The
experimental results of Tyrell and Attard (2001) were
similar to the simulated results. For flow through a nanochannel with a hydrophilic surface, due to the strong solid–
liquid interactions, Fig. 8b shows that the fluid molecules
are orderly adsorbed in the vicinity of the solid interface.
Priezjev and Troian (2006) investigated the influence of
surface roughness on the slip behavior of a Newtonian
liquid under a steady planar shear by employing three
123
different approaches, Stokes flow calculations, MD, and a
statistical mechanical models. The LJ potential was adopted in this article to simulate the interaction between the
particles. Each wall consists of two layers the atomic sites
of which defined the (111) plane of a face-centered cubic
(FCC) lattice. The equations of motion governing the
coordinate and momentum values of the ith particle were
integrated using a standard fifth-order Gear predictor–corrector scheme. The fluid was subjected to steady planar
shear by translating the upper flat wall at a constant speed
along the x-axis. The lower wavy wall remained stationary.
The wavy wall was constructed by vertically displacing all
particles within the (111) plane of the FCC lattice by a
distance varying with a sine wave. The thermal reservoir
and driven force were absent for the x- and z- components.
By using this simplification, the computational cost can be
reduced. However, this method cannot deal with the high
shear rate condition. Therefore, in this article the shear rate
never exceeded 0.033 s-1. The authors found a key
parameter ka, where k is the wave-number, and a is the
amplitude of a sinusoid wave. For Newtonian liquids
subjecting to steady planar shear, the slip length decreased
monotonically with increasing values of ka. A no-slip or
even a negative-slip boundary condition could be obtained
for sufficiently large values of ka. In small ka and large k,
the authors found MD as a better method than Stokes
method. The potential energy exerted by the wavy wall
exhibits two competing wavelengths, one set by the lattice
sites comprising a flat crystalline wall and the other set by
the topological modulation describing a periodically
roughened wall. In this study, the authors combined three
methods spanning multiple length scales ranging from
Microfluid Nanofluid (2010) 9:1011–1031
molecular to macroscopic dimensions and provided a
detailed picture of the influence of periodic roughness on
the slip length.
Martini et al. (2008) tried to explore the molecular
mechanisms of liquid slip. The MDS data and the results
from an analytical model which support two mechanisms
of flow slip were presented in this article. The authors
distinguished two types of slip under the conditions of low
levels of force and high levels of force. At low levels of
force, the potential field generated by the solid creates a
ground state which the liquid atoms preferentially occupy.
Liquid atoms hop through this energy landscape from one
equilibrium site to another. Visual evidence of the trajectories of individual atoms on the solid surface supports the
view of localized hopping, independent of the dynamics
outside a local neighborhood. The authors call this defect
slip. At higher levels of force, the entire layer slips together, obviating the need for localized defects and resulting
in the instantaneous motion of all atoms adjacent to the
solid. The appearance of global slip leads to an increase in
the number of slipping atoms and consequently an increase
in the slip length. The wall atoms were tethered to its lattice
site by a linear spring, which is more realistic. The model
adopted a united atom model allowing both bond bending
and torsion into consideration. A key factor that differentiates this study from others previously reported is that the
fluid density was determined using a grand canonical
Monte Carlo simulation. The advantage of this method lies
in that as the chemical potential, rather than particle
number, is fixed, the liquid is allowed to reach equilibrium
if the channel were filled from a reservoir at the given
temperature.
6 Other liquid–solid interactions
In addition to the slip flow boundary conditions, a key
topic in the studies of liquid flow in nanochannels by
MDS is how the interaction between the fluid molecules
and the solid walls will affect the liquid flow. Xu and
Chen (2006) presented a MDS of molecules translocation
through CNTs in vacuum and in aqueous environment.
The authors compared the dynamic characteristics
between the rigid molecules (C60 molecule and a finite
segment of SWNT with a smaller diameter than the outer
channel) and semi-flexible molecules (single-stranded and
double-stranded DNA oligonucleotide molecules). The
authors found that for rigid molecules the van der Waals
interaction between the molecules and the CNT channel
can induce rapid molecular oscillation inside the CNT
channel in vacuum with little dissipation. The dynamics
of spontaneous insertion into the water-solvated CNT
channels was found to depend sensitively on the details of
1025
the interplay between van der Waals, hydrophobic and
hydrogen bonding interactions in the hybrid nanotubewater molecule system. The authors used the AMBER99
force field to model atomic interactions in the buckyball
molecule, the SWNT channel, and the ssDNA and dsDNA
molecules. For studying nanotube molecule interaction,
the carbon atoms of the nanotube and C60 molecule were
modeled as uncharged LJ particles, corresponding to sp2
carbon–carbon bond length and bond angle in the SWNT
and C60 molecules were maintained by applying harmonic potentials. For simulating the encapsulation process
in aqueous environment, the CNT and the CNT- molecule
complex were solvated in a water reservoir using the well
known TIP3P water model. The study method was applied
to evaluate electrostatic interactions, and sodium ions
were added as counter ions to compensate negative net
charges on the DNA molecules. Atomic interactions
between the ssDNA and dsDNA molecules and the water
solvent were modeled using the AMBER99 force field.
The results showed that in the absence of water solvation,
the van der Waals interaction between the molecule and
the nanotube wall can induce a rapid spontaneous
encapsulation of the molecule inside the nanotube channel. The encapsulation process is strongly impeded for
nanotubes dissolved in water due to the competition
between the van der Waals, hydrophobic and hydrogen
bonding interactions in the nanotube/eater/molecule
complex.
Sofos et al. (2009) calculated the transport properties of
liquid argon flowing through a nanochannel formed by
krypton walls. In this study, wall atoms are constrained by
LJ potential and an elastic spring potential, unlike other
articles where the wall atoms are fixed. This approach can
simulate more accurately the condition of wall atoms. An
external driving force was applied along the x direction to
every fluid particle. The magnitude of the external applied
force was selected in order to avoid non-linear variations in
fluid temperature induced by the flow. The wall atoms
absorb the increase in kinetic energy of the fluid atoms and
Nose–Hoover thermostats at the thermal walls were
employed in order to keep the system’s temperature constant. The authors used two independent thermostats, one
for the upper wall and another for the lower wall in order to
achieve better thermostat of the wall atoms. The results
show clearly the existence of a critical width of the nanochannel, below which the transport properties are affected
in comparison with bulk properties. The authors explained
the phenomenon as follows. For small width values, diffusion coefficient is highly anisotropic, the component
normal to the wall being the smaller one. For the same
width range, diffusivities are higher in the central layers
than those close to the walls. Diffusivity is isotropic in
planes parallel to the walls. The calculation of the diffusion
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1026
coefficients in distinct layers parallel to walls revealed that
diffusion is higher in layers close to the center of the
channel and decreases for the layers adjacent to the walls.
Shear viscosity values are affected by the channel width.
The smaller the channel width, the larger its value. The
existence of this critical width is attributed to the interaction of the fluid with the walls since at smaller channel
widths the effect of the interactions of the walls on the fluid
extends practically to all the fluid molecules in the channel,
modifying considerably the fluid properties in comparison
to the bulk.
Sofos (2009) used NEMD to investigate the effect of
periodic wall roughness on the flow of liquid argon through
krypton nanochannels. The particle interactions were
described by the LJ potential. The lower wall of the
channel is smooth. The rough upper wall is constructed by
‘‘adding’’ extra wall atoms to form periodically spaced
rectangular protrusions. The wall atoms are bound on FCC
sites and remain in their original positions by an elastic
spring force. The temperature is kept constant at with the
application of Nose–Hoover thermostats. The authors presented a potential energy map that shows the existence of
low and high potential energy regions inside the rectangular cavities. The potential energy field varies with the
length of the grooves and affects the trapping of fluid atoms
inside a roughness cavity. The number density contour
plots show that fluid atoms tend to be localized inside
rough wall cavities. As the cavities become narrower, this
localization increases. The maximum value of streaming
velocity in the center of the channel is not significantly
affected by the presence of roughness. Velocity profiles are
suppressed in the upper half of the channel where the rough
wall is present. The result showed that as the wall cavities
become narrower velocity values inside the cavities
decrease and fluid atoms tend to be trapped inside them. As
a result, slip on the boundary diminishes as fluid atoms are
trapped inside the cavities.
7 Improvement in MD method
The MDS method, as a distinguished flow physics simulation method from other simulation methods, can provide
direct numerical experiments at atomistic level with various physical conditions. However, MDS scheme, as a
numerical method, adopts some hypotheses which induce
some deviations of the simulation results from the real
physical process. Furthermore, limited by the computational ability, MDS method can only be applied for nanoscale systems. Therefore, how to introduce the rational
assumptions which reflect the true physical process and
decrease the computational consumption is the main
research direction in order to improve MDS method.
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Microfluid Nanofluid (2010) 9:1011–1031
7.1 Thermal wall models for viscous dissipation effect
Owing to the large velocity gradient, heat generated in
nanochannels by viscous dissipation cannot be neglected.
In the real physical process heat generated by viscous
dissipation would be conducted through the wall so that the
system can keep a constant temperature. Therefore, in MD
simulation, there are several special methods must be
adopted in the MDS to keep the constant temperature
(Andersen 1980; Berendsen et al. 1984; Nose 1984, 2002;
Hoover 1985). A relaxing method (Buckingham 1938) was
developed by coupling an external bath at a constant
temperature to the system and modifying the velocities at
each iteration through a differential feedback mechanism.
This method was widely used. However, it does not produce canonical probability distribution in momentum space
during simulations although it can maintain constant temperature. Nose–Hoover thermostat (Errington and Panagiotopoulos 1999; Zhang and Ely 2004; Galliero et al.
2006) is the most popular method, which can sustain the
canonical ensemble distribution both in configuration and
momentum space. This method generates canonical temperature fluctuations by affecting intermolecular forces
from extended ensemble system. However, because the
wall molecules are fixed, the results which derived from
Nose–Hoover model show almost unphysical uniform
temperature distribution.
Kim et al. (2008) developed a novel thermal wall model
by which the nature of thermal transport at the wall–fluid
interface could be considered. The main idea of this
method is as follows. The wall molecules were in balance
places with thermal oscillations. Thermal oscillations of
wall molecules influence the fluid by absorbing or supplying momentum and energy to fluid molecules via
intermolecular interactions. The resulting force on a molecule of the wall consists of two parts. The first part is the
interaction between fluid molecules and wall molecules,
which can be described by LJ potential. The second part is
the interaction with the wall molecules, which is the lattice
bond springs attached to the wall molecules at their lattice
positions. The forces between molecules depend on interparticles distances. Hence, thermal oscillations of wall
molecules affect the forces acting on the fluid molecules
through the variation of their position as well. In this way,
the dissipation heat could be conducted to the walls. Walls
were utilized as heat baths to maintain thermal equilibrium
of the fluid. Then, for interactive thermal wall model,
velocity scaling thermostat to each wall layer separately
qffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi
Tassignedwall
with parameter glayer ¼
Tlayerwall at every time step was
applied to keep the walls temperature constant. Because
only the fluid flow and thermal properties were concerned,
the thermostat applied on the walls does not influence the
Microfluid Nanofluid (2010) 9:1011–1031
results. The temperature profiles derived from this method
were compared with that derived from the Nose–Hoover
thermostat method. The results of this method show distinct differences. When the interaction potential is weak or
the wall has a large crystal bonding stiffness, temperature
jumps at the wall–fluid interface were observed. However,
because one cannot apply the infinitely small time interval
in simulation, there exist possibilities that the fluid molecules would penetrate into the solid walls, which violate
the true physics. This article did not say how to deal with
this situation. If no special method is applied to ensure the
fluid molecules would not entry the walls domain, then the
law of conservation of mass will not be satisfied.
Jakobtorweihen et al. (2006) described a novel algorithm that includes the effect of host lattice flexibility into
MD simulations that traditionally use rigid lattices. This
method uses a Lowe-Andersen thermostat for interface–
fluid collisions to consider the most important aspects of
flexibility. This method was applied for different guest
molecules, temperatures, and types of CNTs. It has a crucial influence on the diffusive dynamics of the guest molecules. In this article, a CNT is modeled as a flexible
framestudy as described by Walther et al. (2003). Bond
vibrations were modeled with a Morse potential. Bond
bending was controlled by a harmonic cosine potential.
And bond torsions with a twofold torsion potential. However, in this study no intermolecular carbon–carbon interactions were considered. Intermolecular interactions were
modeled with the shifted and truncated LJ 12–6 potential.
The fluid molecules were modeled as united atoms. In
order to avoid flexible host matrix simulations and ensure
that transport occurs under a fluid–solid thermal equilibrium, the authors used the so-called fluid–solid thermal
diffuse scattering (TDS) algorithm. Simulations with this
new algorithm lead to the same self-diffusion coefficients
and give the same heat transfer across the rigid interface as
across a flexible interface. The results showed that the
flexibility of a smooth pore cannot be neglected in the low
loading regime. The small vibrations of the carbon atoms
have a significant influence on the self-diffusion at low
loading in CNTs. The loading dependence of self-diffusion
for helium in a (20.0) CNT at 300 K was also investigated.
Owing to an increased relative roughness (smaller molecule) of the CNT surface, the flexibility influence is less
than that in the case of methane.
7.2 Potentials
The LJ 12–6 potential is by far the most widely used
potential for the intermolecular interactions in MD simulations. It allows a relatively quick computation of the
interaction in MD. Furthermore, it has been shown to be
able to reveal most of the features experimentally found in
1027
fluid states though it formulation is simple. However, the
LJ 12–6 potential is a many-body empirical potential, other
than a true representation of two-body interactions between
argon atoms (Stone 1996). The LJ 12–6 potential represents the decay of repulsive interaction by an inverse 12
power dependence on intermolecular separation distance
whereas intermolecular repulsion decays exponentially. In
addition to LJ 12–6 potential, the general three-parameter
LJ a–6 potentials and three-parameter exponential a–6
potentials (Buckingham 1938) which uses an exponential
formulation of the repulsive part of the potential, have
shown the improved efficiency over the standard LJ
potential for thermodynamic (Errington and Panagiotopoulos 1999) and even for dynamic properties such as viscosity (Zhang and Ely 2004).
Galliero et al. (2006) tried to find more rational potential
formulation.
h iA general form of LJ potential is proposed as:
a
b
e rr þ rr ; the exponential values of a, b can be varied,
for example from 12 to 22, to obtain better potential formulations. They computed the viscosity and the pressure of
spherical fluid particles interacting through LJ a–6 and
exponential a–6 potentials by using MD simulation. They
intended to test the ability of the various potentials to
reproduce simultaneously the pressure and the viscosity of
the same simple real fluids in various thermodynamic
states. They found that LJ potentials and exponential
potentials both can lead to accurate results by using the
appropriate exponent a. However, the exponential potentials results are not superior to the LJ ones. Furthermore,
the authors found that the best results were obtained by the
LJ 12–6 and the exponential 14-6 potentials for each type
of the real fluid that they simulated.
7.3 Reduction of the computation consumption
It is well known that the applications of MDS were limited
mainly because of the required large computation power.
Considering the LJ 12–6 potential, the interaction between
each two molecules decays vary fast to zero when their
distance gets larger than several times of the equilibrium
separation distance. Therefore, cut-off radium, which is
usually about three times of the equilibrium distance, is
defined so that the neighboring atoms outside this radius
will be ignored. The identification of neighboring atoms
and the calculation of inter-atomic distance and force
consume most of the calculation time. Therefore, how to
select the rational cut-off radius in order to reduce the
computational consumption has attracted many attentions.
Several algorithms about select rational cut-off radius, such
as Verlet list, cell-linked list and their combinations
(Frenkel and Smit 2002), have been proposed. Furthermore, several improved algorithms of identifying the
neighboring atoms have been proposed (Mason 2005; Yao
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1028
et al. 2004; Heinz and Hunenberger 2004; Sutmann and
Stegailov 2006; Maximova and Keasar 2006). However,
these algorithms are either valid only for specific systems
or lack of validation.
Wang et al. (2007) developed an estimation formula of
the computation time for each MD algorithm calculation so
as to find an optimized performance for each algorithm.
With the formula proposed in this article, the best algorithm can be chosen based on different total number of
atoms, system average density and system average temperature for the MD simulation. The new contribution of
this study is to reduce the computation time by define
appropriate Verlet radius, the cut-off radius and the average
number density of atoms in a system, respectively. In order
to establish the list in recording the neighboring atoms
around each atom more efficiently during the MDS process, a commonly applied skill is to use a large radius
called, the Verlet radius, and the sphere with the Verlet
radius is called the interaction sphere. This list will be
updated for every K time-steps. As shown in Fig. 9, if the
list recording the neighboring atoms is established by
radius R and will be repeatedly used in the following k
time-steps, then time would be defined so that after (k - 1)t
steps some neighboring atoms, which are initially located
on the sphere with radius R and may penetrate the sphere,
can be contained by such a list in the beginning. The
Verlet-cell list algorithm combines the advantages of
Verlet list and cell-linked list. In the beginning of each listupdating interval, it requires N operations to assign each
atom to a certain cell. It also requires operations to calculate and judge the inter-atomic distance between the
central atoms and neighboring atoms in surrounding cells
and operations to establish the neighbor list with neighboring atoms inside the interaction sphere. Using this
algorithm, the reduction factor is the same as Verlet list,
while t is much smaller.
Fig. 9 Illustration of the cut-off radius Rc and Verlet radius Rv as
well as the corresponding number densities of atoms N00 and N0 (Wang
et al. 2007)
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Microfluid Nanofluid (2010) 9:1011–1031
8 Summary
In this article, we reviewed physics of liquid flows in
nanochannels simulated by MD method, including the
fundamentals of MD simulation, flows under different
driving forces, the boundary conditions, and the improved
algorisms of MD methods. It is worthwhile to comment on
the key issues which may be the promising research
directions in the studies of the liquid flows in nanochannels
by MD simulation.
In the research of electro-osmotic flow in nanochannels,
several conclusions are different from the classical PB
theory, such as the laying density profile near the walls, the
zeta potential varied with the walls roughness, and the
diffusion decreased by the influence of roughness. Furthermore, the ions distribution predicted by MDS departs
from the Boltzmann distribution, which is the base of the
PB theory. The MD simulations reveal that fluid molecules
near the wall are positioned with the preferred orientation,
which cannot be predicted by the PB theory but can explain
the various thermodynamic properties of the liquids in
nanochannels. These conclusions may not reflect exactly
the real physics, because some simplifying assumptions are
used in MDS models. Nevertheless, the results tell us that
the PB equations at least should be modified when used to
solve the nanoscale fluid flow problems. The MDS method
is a powerful tool to probe the distributions and structures
of molecules and ions in nanoscale, which are the dominate
factors controlling the thermodynamic parameters. Therefore, in the electroosmotic flow research, studying the
structure and distribution of molecules and ions in nanochannels will be an important direction.
Carbon nanotubes with charges can be used to develop
the next generation devices for pumping, sensing and
particle screening applications. The study of the potential
CNT applications and the liquid molecular structure in
CNTs are promising directions. The previous studies
showed that the water molecular would have a dipole
structure in the charged nanotubes. CNTs with charges in
the proper positions can be used as the liquid pump and
MDS has been applied to prove its feasibility. In addition,
the structure of water and ions inside the CNTs has significant effects on the effectiveness of particle screening
and partition.
Thermophoresis has practical implications in the fields
such as the bore stability in the oil industry, the particle
accumulation in a thermal boundary layer, and the transport of polymeric molecules in the nanochannels. The
studies of thermophoresis by using MD simulations are still
in the early stage. For the application of using thermophoresis as a pumping method, studies showed that the
obstacle is the small driven force. Although a cascaded
method was proposed to overcome the above difficulty,
Microfluid Nanofluid (2010) 9:1011–1031
however, thermophoresis is not a promising direction to
drive the liquid in nanochannels compared to the electrokinetically driven flow.
For the improved MD scheme, the focus is how to
reflect the realistic flow physics and use less computer
power. The key issues involve building better potential
functions, the thermal wall model, and the cut-off radius.
The rational potential function is the most important issue
in the MD simulation. By far, the LJ 12–6 potential is the
most popular potential function, which has been verified by
lots of studies. However, as an empirical formula, it can
only cover limited types of molecules interactions. Different types of interactions and potential expressions are
urgently needed. Quantum method starts from the sub-atom
level structure to predict the properties of atom level.
Therefore, quantum theory may be used to develop the
molecular interaction potential functions.
The thermal wall model becomes more important
because of the large thermal dissipation in nanoscale. The
simulation will fail if the thermal wall model is not
appropriate. By far, the most successful thermostatic model
is the Nose model. It can keep the system temperature
constant. However, recent studies show that if the wall
molecules are fixed in Nose, then it may induce the
velocity and temperature profile deviation from the realistic
physics status. Oscillation wall molecules’model was proposed in the new studies. The dissipation heat could be
dispersed from the liquid to the oscillated wall molecules.
Then,thermostatic is applied to the wall molecules. The
result of this model is more close to the realistic process.
Acknowledgements The study is supported by the National Natural
Science Foundation of China with the contract number 50906088, and
the National Natural Science Foundation of China with the contract
number 50825603. The authors wish to thank the support of the
Natural Sciences and Engineering Research Council through a
research grant to D. Li.
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