38 |
|
\begin{doublespace} |
39 |
|
|
40 |
|
\begin{abstract} |
41 |
< |
|
41 |
> |
We present a new method for introducing stable non-equilibrium |
42 |
> |
velocity and temperature distributions in molecular dynamics |
43 |
> |
simulations of heterogeneous systems. This method extends some |
44 |
> |
earlier Reverse Non-Equilibrium Molecular Dynamics (RNEMD) methods |
45 |
> |
which use momentum exchange swapping moves that can create |
46 |
> |
non-thermal velocity distributions (and which are difficult to use |
47 |
> |
for interfacial calculations). By using non-isotropic velocity |
48 |
> |
scaling (NIVS) on the molecules in specific regions of a system, it |
49 |
> |
is possible to impose momentum or thermal flux between regions of a |
50 |
> |
simulation and stable thermal and momentum gradients can then be |
51 |
> |
established. The scaling method we have developed conserves the |
52 |
> |
total linear momentum and total energy of the system. To test the |
53 |
> |
methods, we have computed the thermal conductivity of model liquid |
54 |
> |
and solid systems as well as the interfacial thermal conductivity of |
55 |
> |
a metal-water interface. We find that the NIVS-RNEMD improves the |
56 |
> |
problematic velocity distributions that develop in other RNEMD |
57 |
> |
methods. |
58 |
|
\end{abstract} |
59 |
|
|
60 |
|
\newpage |
65 |
|
% BODY OF TEXT |
66 |
|
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% |
67 |
|
|
52 |
– |
|
53 |
– |
|
68 |
|
\section{Introduction} |
69 |
|
The original formulation of Reverse Non-equilibrium Molecular Dynamics |
70 |
|
(RNEMD) obtains transport coefficients (thermal conductivity and shear |
71 |
|
viscosity) in a fluid by imposing an artificial momentum flux between |
72 |
|
two thin parallel slabs of material that are spatially separated in |
73 |
|
the simulation cell.\cite{MullerPlathe:1997xw,ISI:000080382700030} The |
74 |
< |
artificial flux is typically created by periodically ``swapping'' either |
75 |
< |
the entire momentum vector $\vec{p}$ or single components of this |
76 |
< |
vector ($p_x$) between molecules in each of the two slabs. If the two |
77 |
< |
slabs are separated along the $z$ coordinate, the imposed flux is either |
78 |
< |
directional ($j_z(p_x)$) or isotropic ($J_z$), and the response of a |
79 |
< |
simulated system to the imposed momentum flux will typically be a |
80 |
< |
velocity or thermal gradient (Fig. \ref{thermalDemo}). The transport |
81 |
< |
coefficients (shear viscosity and thermal conductivity) are easily |
82 |
< |
obtained by assuming linear response of the system, |
74 |
> |
artificial flux is typically created by periodically ``swapping'' |
75 |
> |
either the entire momentum vector $\vec{p}$ or single components of |
76 |
> |
this vector ($p_x$) between molecules in each of the two slabs. If |
77 |
> |
the two slabs are separated along the $z$ coordinate, the imposed flux |
78 |
> |
is either directional ($j_z(p_x)$) or isotropic ($J_z$), and the |
79 |
> |
response of a simulated system to the imposed momentum flux will |
80 |
> |
typically be a velocity or thermal gradient (Fig. \ref{thermalDemo}). |
81 |
> |
The shear viscosity ($\eta$) and thermal conductivity ($\lambda$) are |
82 |
> |
easily obtained by assuming linear response of the system, |
83 |
|
\begin{eqnarray} |
84 |
|
j_z(p_x) & = & -\eta \frac{\partial v_x}{\partial z}\\ |
85 |
|
J_z & = & \lambda \frac{\partial T}{\partial z} |
87 |
|
RNEMD has been widely used to provide computational estimates of thermal |
88 |
|
conductivities and shear viscosities in a wide range of materials, |
89 |
|
from liquid copper to monatomic liquids to molecular fluids |
90 |
< |
(e.g. ionic liquids).\cite{ISI:000246190100032} |
90 |
> |
(e.g. ionic liquids).\cite{Bedrov:2000-1,Bedrov:2000,Muller-Plathe:2002,ISI:000184808400018,ISI:000231042800044,Maginn:2007,Muller-Plathe:2008,ISI:000258460400020,ISI:000258840700015,ISI:000261835100054} |
91 |
|
|
92 |
|
\begin{figure} |
93 |
|
\includegraphics[width=\linewidth]{thermalDemo} |
94 |
< |
\caption{Demostration of thermal gradient estalished by RNEMD |
95 |
< |
method. Physical thermal flow directs from high temperature region |
96 |
< |
to low temperature region. Unphysical thermal transfer counteracts |
97 |
< |
it and maintains a steady thermal gradient.} |
94 |
> |
\caption{RNEMD methods impose an unphysical transfer of momentum or |
95 |
> |
kinetic energy between a ``hot'' slab and a ``cold'' slab in the |
96 |
> |
simulation box. The molecular system responds to this imposed flux |
97 |
> |
by generating a momentum or temperature gradient. The slope of the |
98 |
> |
gradient can then be used to compute transport properties (e.g. |
99 |
> |
shear viscosity and thermal conductivity).} |
100 |
|
\label{thermalDemo} |
101 |
|
\end{figure} |
102 |
|
|
103 |
< |
RNEMD is preferable in many ways to the forward NEMD methods because |
104 |
< |
it imposes what is typically difficult to measure (a flux or stress) |
105 |
< |
and it is typically much easier to compute momentum gradients or |
106 |
< |
strains (the response). For similar reasons, RNEMD is also preferable |
107 |
< |
to slowly-converging equilibrium methods for measuring thermal |
108 |
< |
conductivity and shear viscosity (using Green-Kubo relations or the |
109 |
< |
Helfand moment approach of Viscardy {\it et |
103 |
> |
RNEMD is preferable in many ways to the forward NEMD |
104 |
> |
methods\cite{ISI:A1988Q205300014,hess:209,Vasquez:2004fk,backer:154503,ISI:000266247600008} |
105 |
> |
because it imposes what is typically difficult to measure (a flux or |
106 |
> |
stress) and it is typically much easier to compute momentum gradients |
107 |
> |
or strains (the response). For similar reasons, RNEMD is also |
108 |
> |
preferable to slowly-converging equilibrium methods for measuring |
109 |
> |
thermal conductivity and shear viscosity (using Green-Kubo |
110 |
> |
relations\cite{daivis:541,mondello:9327} or the Helfand moment |
111 |
> |
approach of Viscardy {\it et |
112 |
|
al.}\cite{Viscardy:2007bh,Viscardy:2007lq}) because these rely on |
113 |
|
computing difficult to measure quantities. |
114 |
|
|
118 |
|
typically samples from the same manifold of states in the |
119 |
|
microcanonical ensemble. |
120 |
|
|
121 |
< |
Recently, Tenney and Maginn\cite{ISI:000273472300004} have discovered |
121 |
> |
Recently, Tenney and Maginn\cite{Maginn:2010} have discovered |
122 |
|
some problems with the original RNEMD swap technique. Notably, large |
123 |
|
momentum fluxes (equivalent to frequent momentum swaps between the |
124 |
|
slabs) can result in ``notched'', ``peaked'' and generally non-thermal |
132 |
|
(conservation of linear momentum and total energy, compatibility with |
133 |
|
periodic boundary conditions) while establishing true thermal |
134 |
|
distributions in each of the two slabs. In the next section, we |
135 |
< |
develop the method for determining the scaling constraints. We then |
135 |
> |
present the method for determining the scaling constraints. We then |
136 |
|
test the method on both single component, multi-component, and |
137 |
|
non-isotropic mixtures and show that it is capable of providing |
138 |
|
reasonable estimates of the thermal conductivity and shear viscosity |
139 |
|
in these cases. |
140 |
|
|
141 |
|
\section{Methodology} |
142 |
< |
We retain the basic idea of Muller-Plathe's RNEMD method; the periodic |
143 |
< |
system is partitioned into a series of thin slabs along a particular |
142 |
> |
We retain the basic idea of M\"{u}ller-Plathe's RNEMD method; the |
143 |
> |
periodic system is partitioned into a series of thin slabs along one |
144 |
|
axis ($z$). One of the slabs at the end of the periodic box is |
145 |
|
designated the ``hot'' slab, while the slab in the center of the box |
146 |
|
is designated the ``cold'' slab. The artificial momentum flux will be |
148 |
|
hot slab. |
149 |
|
|
150 |
|
Rather than using momentum swaps, we use a series of velocity scaling |
151 |
< |
moves. For molecules $\{i\}$ located within the cold slab, |
151 |
> |
moves. For molecules $\{i\}$ located within the cold slab, |
152 |
|
\begin{equation} |
153 |
|
\vec{v}_i \leftarrow \left( \begin{array}{ccc} |
154 |
|
x & 0 & 0 \\ |
168 |
|
\end{equation} |
169 |
|
|
170 |
|
Conservation of linear momentum in each of the three directions |
171 |
< |
($\alpha = x,y,z$) ties the values of the hot and cold bin scaling |
171 |
> |
($\alpha = x,y,z$) ties the values of the hot and cold scaling |
172 |
|
parameters together: |
173 |
|
\begin{equation} |
174 |
|
P_h^\alpha + P_c^\alpha = \alpha^\prime P_h^\alpha + \alpha P_c^\alpha |
202 |
|
similar manner to the linear momenta (Eq. \ref{eq:momentumdef}). |
203 |
|
Substituting in the expressions for the hot scaling parameters |
204 |
|
($\alpha^\prime$) from Eq. (\ref{eq:hotcoldscaling}), we obtain the |
205 |
< |
{\it constraint ellipsoid equation}: |
205 |
> |
{\it constraint ellipsoid}: |
206 |
|
\begin{equation} |
207 |
|
\sum_{\alpha = x,y,z} a_\alpha \alpha^2 + b_\alpha \alpha + c_\alpha = 0 |
208 |
|
\label{eq:constraintEllipsoid} |
216 |
|
c_\alpha & = & K_h^\alpha p_\alpha^2 + 2 K_h^\alpha p_\alpha - K_c^\alpha |
217 |
|
\label{eq:constraintEllipsoidConsts} |
218 |
|
\end{eqnarray} |
219 |
< |
This ellipsoid equation defines the set of cold slab scaling |
220 |
< |
parameters which can be applied while preserving both linear momentum |
221 |
< |
in all three directions as well as kinetic energy. |
219 |
> |
This ellipsoid (Eq. \ref{eq:constraintEllipsoid}) defines the set of |
220 |
> |
cold slab scaling parameters which can be applied while preserving |
221 |
> |
both linear momentum in all three directions as well as total kinetic |
222 |
> |
energy. |
223 |
|
|
224 |
|
The goal of using velocity scaling variables is to transfer linear |
225 |
|
momentum or kinetic energy from the cold slab to the hot slab. If the |
234 |
|
x^2 K_c^x + y^2 K_c^y + z^2 K_c^z = K_c^x + K_c^y + K_c^z - J_z\Delta t |
235 |
|
\label{eq:fluxEllipsoid} |
236 |
|
\end{equation} |
237 |
< |
The spatial extent of the {\it thermal flux ellipsoid equation} is |
238 |
< |
governed both by a targetted value, $J_z$ as well as the instantaneous |
239 |
< |
values of the kinetic energy components in the cold bin. |
237 |
> |
The spatial extent of the {\it thermal flux ellipsoid} is governed |
238 |
> |
both by a targetted value, $J_z$ as well as the instantaneous values |
239 |
> |
of the kinetic energy components in the cold bin. |
240 |
|
|
241 |
|
To satisfy an energetic flux as well as the conservation constraints, |
242 |
< |
it is sufficient to determine the points ${x,y,z}$ which lie on both |
243 |
< |
the constraint ellipsoid (Eq. \ref{eq:constraintEllipsoid}) and the |
244 |
< |
flux ellipsoid (Eq. \ref{eq:fluxEllipsoid}), i.e. the intersection of |
245 |
< |
the two ellipsoids in 3-dimensional space. |
242 |
> |
we must determine the points ${x,y,z}$ which lie on both the |
243 |
> |
constraint ellipsoid (Eq. \ref{eq:constraintEllipsoid}) and the flux |
244 |
> |
ellipsoid (Eq. \ref{eq:fluxEllipsoid}), i.e. the intersection of the |
245 |
> |
two ellipsoids in 3-dimensional space. |
246 |
|
|
247 |
|
\begin{figure} |
248 |
|
\includegraphics[width=\linewidth]{ellipsoids} |
249 |
< |
\caption{Scaling points which maintain both constant energy and |
250 |
< |
constant linear momentum of the system lie on the surface of the |
251 |
< |
{\it constraint ellipsoid} while points which generate the target |
252 |
< |
momentum flux lie on the surface of the {\it flux ellipsoid}. The |
253 |
< |
velocity distributions in the cold bin are scaled by only those |
254 |
< |
points which lie on both ellipsoids.} |
249 |
> |
\caption{Illustration from the perspective of a space having cold |
250 |
> |
slab scaling coefficients as its coordinates. Scaling points which |
251 |
> |
maintain both constant energy and constant linear momentum of the |
252 |
> |
system lie on the surface of the {\it constraint ellipsoid} while |
253 |
> |
points which generate the target momentum flux lie on the surface of |
254 |
> |
the {\it flux ellipsoid}. The velocity distributions in the cold bin |
255 |
> |
are scaled by only those points which lie on both ellipsoids.} |
256 |
|
\label{ellipsoids} |
257 |
|
\end{figure} |
258 |
|
|
259 |
< |
One may also define momentum flux (say along the $x$-direction) as: |
259 |
> |
One may also define {\it momentum} flux (say along the $x$-direction) as: |
260 |
|
\begin{equation} |
261 |
|
(1-x) P_c^x = j_z(p_x)\Delta t |
262 |
|
\label{eq:fluxPlane} |
263 |
|
\end{equation} |
264 |
< |
The above {\it momentum flux equation} is essentially a plane which is |
265 |
< |
perpendicular to the $x$-axis, with its position governed both by a |
266 |
< |
target value, $j_z(p_x)$ as well as the instantaneous value of the |
247 |
< |
momentum along the $x$-direction. |
264 |
> |
The above {\it momentum flux plane} is perpendicular to the $x$-axis, |
265 |
> |
with its position governed both by a target value, $j_z(p_x)$ as well |
266 |
> |
as the instantaneous value of the momentum along the $x$-direction. |
267 |
|
|
268 |
< |
Similarly, to satisfy a momentum flux as well as the conservation |
269 |
< |
constraints, it is sufficient to determine the points ${x,y,z}$ which |
270 |
< |
lie on both the constraint ellipsoid (Eq. \ref{eq:constraintEllipsoid}) |
271 |
< |
and the flux plane (Eq. \ref{eq:fluxPlane}), i.e. the intersection of |
272 |
< |
an ellipsoid and a plane in 3-dimensional space. |
268 |
> |
In order to satisfy a momentum flux as well as the conservation |
269 |
> |
constraints, we must determine the points ${x,y,z}$ which lie on both |
270 |
> |
the constraint ellipsoid (Eq. \ref{eq:constraintEllipsoid}) and the |
271 |
> |
flux plane (Eq. \ref{eq:fluxPlane}), i.e. the intersection of an |
272 |
> |
ellipsoid and a plane in 3-dimensional space. |
273 |
|
|
274 |
< |
To summarize, by solving respective equation sets, one can determine |
275 |
< |
possible sets of scaling variables for cold slab. And corresponding |
276 |
< |
sets of scaling variables for hot slab can be determine as well. |
274 |
> |
In both the momentum and energy flux scenarios, valid scaling |
275 |
> |
parameters are arrived at by solving geometric intersection problems |
276 |
> |
in $x, y, z$ space in order to obtain cold slab scaling parameters. |
277 |
> |
Once the scaling variables for the cold slab are known, the hot slab |
278 |
> |
scaling has also been determined. |
279 |
|
|
280 |
+ |
|
281 |
|
The following problem will be choosing an optimal set of scaling |
282 |
|
variables among the possible sets. Although this method is inherently |
283 |
|
non-isotropic, the goal is still to maintain the system as isotropic |
285 |
|
energies in different directions could become as close as each other |
286 |
|
after each scaling. Simultaneously, one would also like each scaling |
287 |
|
as gentle as possible, i.e. ${x,y,z \rightarrow 1}$, in order to avoid |
288 |
< |
large perturbation to the system. Therefore, one approach to obtain the |
289 |
< |
scaling variables would be constructing an criteria function, with |
288 |
> |
large perturbation to the system. Therefore, one approach to obtain |
289 |
> |
the scaling variables would be constructing an criteria function, with |
290 |
|
constraints as above equation sets, and solving the function's minimum |
291 |
|
by method like Lagrange multipliers. |
292 |
|
|
336 |
|
periodic boundary condition, and devided into ${N = 20}$ slabs. In each swap, |
337 |
|
the top slab ${(n = 1)}$ exchange the most negative $x$ momentum with the |
338 |
|
most positive $x$ momentum in the center slab ${(n = N/2 + 1)}$. Referred |
339 |
< |
to Tenney {\it et al.}\cite{ISI:000273472300004}, a series of swapping |
339 |
> |
to Tenney {\it et al.}\cite{Maginn:2010}, a series of swapping |
340 |
|
frequency were chosen. According to each result from swapping |
341 |
|
RNEMD, scaling RNEMD simulations were run with the target momentum |
342 |
|
flux set to produce a similar momentum flux, and consequently shear |
397 |
|
Another series of our simulation is the calculation of interfacial |
398 |
|
thermal conductivity of a Au/H$_2$O system. Respective calculations of |
399 |
|
liquid water (Extended Simple Point Charge model) and crystal gold |
400 |
< |
(Quantum Sutton-Chen potential) thermal conductivity were performed |
401 |
< |
and compared with current results to ensure the validity of |
402 |
< |
NIVS-RNEMD. After that, a mixture system was simulated. |
400 |
> |
thermal conductivity were performed and compared with current results |
401 |
> |
to ensure the validity of NIVS-RNEMD. After that, a mixture system was |
402 |
> |
simulated. |
403 |
|
|
404 |
|
For thermal conductivity calculation of bulk water, a simulation box |
405 |
|
consisting of 1000 molecules were first equilibrated under ambient |
411 |
|
process was similar to Lennard-Jones fluid system. |
412 |
|
|
413 |
|
Thermal conductivity calculation of bulk crystal gold used a similar |
414 |
< |
protocol. The face-centered cubic crystal simulation box consists of |
414 |
> |
protocol. Two types of force field parameters, Embedded Atom Method |
415 |
> |
(EAM) and Quantum Sutten-Chen (QSC) force field were used |
416 |
> |
respectively. The face-centered cubic crystal simulation box consists of |
417 |
|
2880 Au atoms. The lattice was first allowed volume change to relax |
418 |
|
under ambient temperature and pressure. Equilibrations in canonical and |
419 |
|
microcanonical ensemble were followed in order. With the simulation |
482 |
|
|
483 |
|
\begin{figure} |
484 |
|
\includegraphics[width=\linewidth]{thermalGrad} |
485 |
< |
\caption{Temperature gradients under various kinetic energy flux of |
486 |
< |
thermal conductivity simulations} |
485 |
> |
\caption{NIVS-RNEMD method introduced similar temperature gradients |
486 |
> |
compared to ``swapping'' method under various kinetic energy flux in |
487 |
> |
thermal conductivity simulations.} |
488 |
|
\label{thermalGrad} |
489 |
|
\end{figure} |
490 |
|
|
495 |
|
that under relatively high unphysical kinetic energy flux, speed and |
496 |
|
velocity distribution of molecules in slabs where swapping occured |
497 |
|
could deviate from Maxwell-Boltzmann distribution. Figure |
498 |
< |
\ref{histSwap} illustrates how these distributions deviate from an |
498 |
> |
\ref{thermalHist} a) illustrates how these distributions deviate from an |
499 |
|
ideal distribution. In high temperature slab, probability density in |
500 |
|
low speed is confidently smaller than ideal curve fit; in low |
501 |
|
temperature slab, probability density in high speed is smaller than |
516 |
|
interference. Consequently, swapping RNEMD has a relatively narrow |
517 |
|
choice of swapping rate to satisfy these above restrictions. |
518 |
|
|
494 |
– |
\begin{figure} |
495 |
– |
\includegraphics[width=\linewidth]{histSwap} |
496 |
– |
\caption{Speed distribution for thermal conductivity using swapping |
497 |
– |
RNEMD. Shown is from the simulation with 250 fs exchange interval.} |
498 |
– |
\label{histSwap} |
499 |
– |
\end{figure} |
500 |
– |
|
519 |
|
Comparatively, NIVS-RNEMD has a speed distribution closer to the ideal |
520 |
< |
curve fit (Figure \ref{histScale}). Essentially, after scaling, a |
520 |
> |
curve fit (Figure \ref{thermalHist} b). Essentially, after scaling, a |
521 |
|
Gaussian distribution function would remain Gaussian. Although a |
522 |
|
single scaling is non-isotropic in all three dimensions, our scaling |
523 |
|
coefficient criteria could help maintian the scaling region as |
530 |
|
to the distribution of velocity and speed in the exchange regions. |
531 |
|
|
532 |
|
\begin{figure} |
533 |
< |
\includegraphics[width=\linewidth]{histScale} |
534 |
< |
\caption{Speed distribution for thermal conductivity using scaling |
535 |
< |
RNEMD. Shown is from the simulation with an equilvalent thermal flux |
536 |
< |
as an 250 fs exchange interval swapping simulation.} |
537 |
< |
\label{histScale} |
533 |
> |
\includegraphics[width=\linewidth]{thermalHist} |
534 |
> |
\caption{Speed distribution for thermal conductivity using a) |
535 |
> |
``swapping'' and b) NIVS- RNEMD methods. Shown is from the |
536 |
> |
simulations with an exchange or equilvalent exchange interval of 250 |
537 |
> |
fs. In circled areas, distributions from ``swapping'' RNEMD |
538 |
> |
simulation have deviation from ideal Maxwell-Boltzmann distribution |
539 |
> |
(curves fit for each distribution).} |
540 |
> |
\label{thermalHist} |
541 |
|
\end{figure} |
542 |
|
|
543 |
|
\subsubsection{SPC/E Water} |
544 |
|
Our results of SPC/E water thermal conductivity are comparable to |
545 |
< |
Bedrov {\it et al.}\cite{ISI:000090151400044}, which employed the |
545 |
> |
Bedrov {\it et al.}\cite{Bedrov:2000}, which employed the |
546 |
|
previous swapping RNEMD method for their calculation. Bedrov {\it et |
547 |
< |
al.}\cite{ISI:000090151400044} argued that exchange of the molecule |
547 |
> |
al.}\cite{Bedrov:2000} argued that exchange of the molecule |
548 |
|
center-of-mass velocities instead of single atom velocities in a |
549 |
|
molecule conserves the total kinetic energy and linear momentum. This |
550 |
|
principle is adopted in our simulations. Scaling is applied to the |
560 |
|
|
561 |
|
\begin{figure} |
562 |
|
\includegraphics[width=\linewidth]{spceGrad} |
563 |
< |
\caption{Temperature gradients for SPC/E water thermal conductivity.} |
563 |
> |
\caption{Temperature gradients in SPC/E water thermal conductivity |
564 |
> |
simulations.} |
565 |
|
\label{spceGrad} |
566 |
|
\end{figure} |
567 |
|
|
576 |
|
\begin{tabular}{cccc} |
577 |
|
\hline |
578 |
|
$\langle dT/dz\rangle$(K/\AA) & & $\lambda$(W/m/K) & \\ |
579 |
< |
& This work & Previous simulations\cite{ISI:000090151400044} & |
579 |
> |
& This work & Previous simulations\cite{Bedrov:2000} & |
580 |
|
Experiment$^a$\\ |
581 |
|
\hline |
582 |
|
0.38 & 0.816(0.044) & & 0.64\\ |
590 |
|
\end{table*} |
591 |
|
|
592 |
|
\subsubsection{Crystal Gold} |
593 |
< |
Our results of gold thermal conductivity using QSC force field are |
594 |
< |
shown in Table \ref{AuThermal}. Although our calculation is smaller |
595 |
< |
than experimental value by an order of more than 100, this difference |
596 |
< |
is mainly attributed to the lack of electron interaction |
597 |
< |
representation in our force field parameters. Richardson {\it et |
598 |
< |
al.}\cite{ISI:A1992HX37800010} using similar force field parameters |
599 |
< |
in their metal thermal conductivity calculations. The EMD method they |
600 |
< |
employed in their simulations produced comparable results to |
601 |
< |
ours. Therefore, it is confident to conclude that NIVS-RNEMD is |
602 |
< |
applicable to metal force field system. |
593 |
> |
Our results of gold thermal conductivity using two force fields are |
594 |
> |
shown separately in Table \ref{qscThermal} and \ref{eamThermal}. In |
595 |
> |
these calculations,the end and middle slabs were excluded in thermal |
596 |
> |
gradient regession and only used as heat source and drain in the |
597 |
> |
systems. Our yielded values using EAM force field are slightly larger |
598 |
> |
than those using QSC force field. However, both series are |
599 |
> |
significantly smaller than experimental value by an order of more than |
600 |
> |
100. It has been verified that this difference is mainly attributed to |
601 |
> |
the lack of electron interaction representation in these force field |
602 |
> |
parameters. Richardson {\it et al.}\cite{Clancy:1992} used EAM |
603 |
> |
force field parameters in their metal thermal conductivity |
604 |
> |
calculations. The Non-Equilibrium MD method they employed in their |
605 |
> |
simulations produced comparable results to ours. As Zhang {\it et |
606 |
> |
al.}\cite{ISI:000231042800044} stated, thermal conductivity values |
607 |
> |
are influenced mainly by force field. Therefore, it is confident to |
608 |
> |
conclude that NIVS-RNEMD is applicable to metal force field system. |
609 |
|
|
610 |
|
\begin{figure} |
611 |
|
\includegraphics[width=\linewidth]{AuGrad} |
612 |
< |
\caption{Temperature gradients for crystal gold thermal conductivity.} |
612 |
> |
\caption{Temperature gradients for thermal conductivity calculation of |
613 |
> |
crystal gold using QSC force field.} |
614 |
|
\label{AuGrad} |
615 |
|
\end{figure} |
616 |
|
|
619 |
|
\begin{center} |
620 |
|
|
621 |
|
\caption{Calculation results for thermal conductivity of crystal gold |
622 |
< |
at ${\langle T\rangle}$ = 300K at various thermal exchange rates. Errors of |
623 |
< |
calculations in parentheses. } |
622 |
> |
using QSC force field at ${\langle T\rangle}$ = 300K at various |
623 |
> |
thermal exchange rates. Errors of calculations in parentheses. } |
624 |
|
|
625 |
|
\begin{tabular}{cc} |
626 |
|
\hline |
631 |
|
5.14 & 1.15(0.01)\\ |
632 |
|
\hline |
633 |
|
\end{tabular} |
634 |
< |
\label{AuThermal} |
634 |
> |
\label{qscThermal} |
635 |
|
\end{center} |
636 |
|
\end{minipage} |
637 |
|
\end{table*} |
638 |
|
|
610 |
– |
\subsection{Interfaciel Thermal Conductivity} |
611 |
– |
After valid simulations of homogeneous water and gold systems using |
612 |
– |
NIVS-RNEMD method, calculation of gold/water interfacial thermal |
613 |
– |
conductivity was followed. It is found out that the interfacial |
614 |
– |
conductance is low due to a hydrophobic surface in our system. Figure |
615 |
– |
\ref{interfaceDensity} demonstrates this observance. Consequently, our |
616 |
– |
reported results (Table \ref{interfaceRes}) are of two orders of |
617 |
– |
magnitude smaller than our calculations on homogeneous systems. |
618 |
– |
|
639 |
|
\begin{figure} |
640 |
< |
\includegraphics[width=\linewidth]{interfaceDensity} |
641 |
< |
\caption{Density profile for interfacial thermal conductivity |
642 |
< |
simulation box.} |
643 |
< |
\label{interfaceDensity} |
640 |
> |
\includegraphics[width=\linewidth]{eamGrad} |
641 |
> |
\caption{Temperature gradients for thermal conductivity calculation of |
642 |
> |
crystal gold using EAM force field.} |
643 |
> |
\label{eamGrad} |
644 |
|
\end{figure} |
645 |
+ |
|
646 |
+ |
\begin{table*} |
647 |
+ |
\begin{minipage}{\linewidth} |
648 |
+ |
\begin{center} |
649 |
+ |
|
650 |
+ |
\caption{Calculation results for thermal conductivity of crystal gold |
651 |
+ |
using EAM force field at ${\langle T\rangle}$ = 300K at various |
652 |
+ |
thermal exchange rates. Errors of calculations in parentheses. } |
653 |
+ |
|
654 |
+ |
\begin{tabular}{cc} |
655 |
+ |
\hline |
656 |
+ |
$\langle dT/dz\rangle$(K/\AA) & $\lambda$(W/m/K)\\ |
657 |
+ |
\hline |
658 |
+ |
1.24 & 1.24(0.06)\\ |
659 |
+ |
2.06 & 1.37(0.04)\\ |
660 |
+ |
2.55 & 1.41(0.03)\\ |
661 |
+ |
\hline |
662 |
+ |
\end{tabular} |
663 |
+ |
\label{eamThermal} |
664 |
+ |
\end{center} |
665 |
+ |
\end{minipage} |
666 |
+ |
\end{table*} |
667 |
|
|
668 |
+ |
|
669 |
+ |
\subsection{Interfaciel Thermal Conductivity} |
670 |
+ |
After simulations of homogeneous water and gold systems using |
671 |
+ |
NIVS-RNEMD method were proved valid, calculation of gold/water |
672 |
+ |
interfacial thermal conductivity was followed. It is found out that |
673 |
+ |
the low interfacial conductance is probably due to the hydrophobic |
674 |
+ |
surface in our system. Figure \ref{interface} (a) demonstrates mass |
675 |
+ |
density change along $z$-axis, which is perpendicular to the |
676 |
+ |
gold/water interface. It is observed that water density significantly |
677 |
+ |
decreases when approaching the surface. Under this low thermal |
678 |
+ |
conductance, both gold and water phase have sufficient time to |
679 |
+ |
eliminate temperature difference inside respectively (Figure |
680 |
+ |
\ref{interface} b). With indistinguishable temperature difference |
681 |
+ |
within respective phase, it is valid to assume that the temperature |
682 |
+ |
difference between gold and water on surface would be approximately |
683 |
+ |
the same as the difference between the gold and water phase. This |
684 |
+ |
assumption enables convenient calculation of $G$ using |
685 |
+ |
Eq. \ref{interfaceCalc} instead of measuring temperatures of thin |
686 |
+ |
layer of water and gold close enough to surface, which would have |
687 |
+ |
greater fluctuation and lower accuracy. Reported results (Table |
688 |
+ |
\ref{interfaceRes}) are of two orders of magnitude smaller than our |
689 |
+ |
calculations on homogeneous systems, and thus have larger relative |
690 |
+ |
errors than our calculation results on homogeneous systems. |
691 |
+ |
|
692 |
|
\begin{figure} |
693 |
< |
\includegraphics[width=\linewidth]{interfaceGrad} |
694 |
< |
\caption{Temperature profiles for interfacial thermal conductivity |
695 |
< |
simulation box.} |
696 |
< |
\label{interfaceGrad} |
693 |
> |
\includegraphics[width=\linewidth]{interface} |
694 |
> |
\caption{Simulation results for Gold/Water interfacial thermal |
695 |
> |
conductivity: (a) Significant water density decrease is observed on |
696 |
> |
crystalline gold surface. (b) Temperature profiles for a series of |
697 |
> |
simulations. Temperatures of different slabs in the same phase show |
698 |
> |
no significant differences.} |
699 |
> |
\label{interface} |
700 |
|
\end{figure} |
701 |
|
|
702 |
|
\begin{table*} |
732 |
|
momentum flux would theoretically result in swap method. All the scale |
733 |
|
method results were from simulations that had a scaling interval of 10 |
734 |
|
time steps. The average molecular momentum gradients of these samples |
735 |
< |
are shown in Figure \ref{shearGrad}. |
735 |
> |
are shown in Figure \ref{shear} (a) and (b). |
736 |
|
|
737 |
|
\begin{table*} |
738 |
|
\begin{minipage}{\linewidth} |
759 |
|
\end{table*} |
760 |
|
|
761 |
|
\begin{figure} |
762 |
< |
\includegraphics[width=\linewidth]{shearGrad} |
763 |
< |
\caption{Average momentum gradients of shear viscosity simulations} |
764 |
< |
\label{shearGrad} |
762 |
> |
\includegraphics[width=\linewidth]{shear} |
763 |
> |
\caption{Average momentum gradients in shear viscosity simulations, |
764 |
> |
using (a) ``swapping'' method and (b) NIVS-RNEMD method |
765 |
> |
respectively. (c) Temperature difference among x and y, z dimensions |
766 |
> |
observed when using NIVS-RNEMD with equivalent exchange interval of |
767 |
> |
500 fs.} |
768 |
> |
\label{shear} |
769 |
|
\end{figure} |
770 |
|
|
698 |
– |
\begin{figure} |
699 |
– |
\includegraphics[width=\linewidth]{shearTempScale} |
700 |
– |
\caption{Temperature profile for scaling RNEMD simulation.} |
701 |
– |
\label{shearTempScale} |
702 |
– |
\end{figure} |
771 |
|
However, observations of temperatures along three dimensions show that |
772 |
|
inhomogeneity occurs in scaling RNEMD simulations, particularly in the |
773 |
< |
two slabs which were scaled. Figure \ref{shearTempScale} indicate that with |
773 |
> |
two slabs which were scaled. Figure \ref{shear} (c) indicate that with |
774 |
|
relatively large imposed momentum flux, the temperature difference among $x$ |
775 |
|
and the other two dimensions was significant. This would result from the |
776 |
|
algorithm of scaling method. From Eq. \ref{eq:fluxPlane}, after |
792 |
|
|
793 |
|
\section{Conclusions} |
794 |
|
NIVS-RNEMD simulation method is developed and tested on various |
795 |
< |
systems. Simulation results demonstrate its validity of thermal |
796 |
< |
conductivity calculations. NIVS-RNEMD improves non-Boltzmann-Maxwell |
797 |
< |
distributions existing in previous RNEMD methods, and extends its |
798 |
< |
applicability to interfacial systems. NIVS-RNEMD has also limited |
799 |
< |
application on shear viscosity calculations, but under high momentum |
800 |
< |
flux, it could cause temperature difference among different |
801 |
< |
dimensions. Modification is necessary to extend the applicability of |
802 |
< |
NIVS-RNEMD in shear viscosity calculations. |
795 |
> |
systems. Simulation results demonstrate its validity in thermal |
796 |
> |
conductivity calculations, from Lennard-Jones fluid to multi-atom |
797 |
> |
molecule like water and metal crystals. NIVS-RNEMD improves |
798 |
> |
non-Boltzmann-Maxwell distributions, which exist in previous RNEMD |
799 |
> |
methods. Furthermore, it develops a valid means for unphysical thermal |
800 |
> |
transfer between different species of molecules, and thus extends its |
801 |
> |
applicability to interfacial systems. Our calculation of gold/water |
802 |
> |
interfacial thermal conductivity demonstrates this advantage over |
803 |
> |
previous RNEMD methods. NIVS-RNEMD has also limited application on |
804 |
> |
shear viscosity calculations, but could cause temperature difference |
805 |
> |
among different dimensions under high momentum flux. Modification is |
806 |
> |
necessary to extend the applicability of NIVS-RNEMD in shear viscosity |
807 |
> |
calculations. |
808 |
|
|
809 |
|
\section{Acknowledgments} |
810 |
|
Support for this project was provided by the National Science |
812 |
|
the Center for Research Computing (CRC) at the University of Notre |
813 |
|
Dame. \newpage |
814 |
|
|
815 |
< |
\bibliographystyle{jcp2} |
815 |
> |
\bibliographystyle{aip} |
816 |
|
\bibliography{nivsRnemd} |
817 |
+ |
|
818 |
|
\end{doublespace} |
819 |
|
\end{document} |
820 |
|
|