ViewVC Help
View File | Revision Log | Show Annotations | View Changeset | Root Listing
root/group/interfacial/interfacial.tex
(Generate patch)

Comparing interfacial/interfacial.tex (file contents):
Revision 3725 by skuang, Mon May 9 19:08:08 2011 UTC vs.
Revision 3759 by skuang, Fri Jul 29 21:06:30 2011 UTC

# Line 22 | Line 22
22   \setlength{\abovecaptionskip}{20 pt}
23   \setlength{\belowcaptionskip}{30 pt}
24  
25 < %\renewcommand\citemid{\ } % no comma in optional referenc note
26 < \bibpunct{[}{]}{,}{s}{}{;}
27 < \bibliographystyle{aip}
25 > %\renewcommand\citemid{\ } % no comma in optional reference note
26 > \bibpunct{[}{]}{,}{n}{}{;}
27 > \bibliographystyle{achemso}
28  
29   \begin{document}
30  
# Line 45 | Line 45 | We have developed a Non-Isotropic Velocity Scaling alg
45  
46   \begin{abstract}
47  
48 < We have developed a Non-Isotropic Velocity Scaling algorithm for
49 < setting up and maintaining stable thermal gradients in non-equilibrium
50 < molecular dynamics simulations. This approach effectively imposes
51 < unphysical thermal flux even between particles of different
52 < identities, conserves linear momentum and kinetic energy, and
53 < minimally perturbs the velocity profile of a system when compared with
54 < previous RNEMD methods. We have used this method to simulate thermal
55 < conductance at metal / organic solvent interfaces both with and
56 < without the presence of thiol-based capping agents.  We obtained
57 < values comparable with experimental values, and observed significant
58 < conductance enhancement with the presence of capping agents. Computed
59 < power spectra indicate the acoustic impedance mismatch between metal
60 < and liquid phase is greatly reduced by the capping agents and thus
61 < leads to higher interfacial thermal transfer efficiency.
48 > With the Non-Isotropic Velocity Scaling algorithm (NIVS) we have
49 > developed, an unphysical thermal flux can be effectively set up even
50 > for non-homogeneous systems like interfaces in non-equilibrium
51 > molecular dynamics simulations. In this work, this algorithm is
52 > applied for simulating thermal conductance at metal / organic solvent
53 > interfaces with various coverages of butanethiol capping
54 > agents. Different solvents and force field models were tested. Our
55 > results suggest that the United-Atom models are able to provide an
56 > estimate of the interfacial thermal conductivity comparable to
57 > experiments in our simulations with satisfactory computational
58 > efficiency. From our results, the acoustic impedance mismatch between
59 > metal and liquid phase is effectively reduced by the capping
60 > agents, and thus leads to interfacial thermal conductance
61 > enhancement. Furthermore, this effect is closely related to the
62 > capping agent coverage on the metal surfaces and the type of solvent
63 > molecules, and is affected by the models used in the simulations.
64  
65   \end{abstract}
66  
# Line 71 | Line 73 | leads to higher interfacial thermal transfer efficienc
73   %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
74  
75   \section{Introduction}
76 + Due to the importance of heat flow in nanotechnology, interfacial
77 + thermal conductance has been studied extensively both experimentally
78 + and computationally.\cite{cahill:793} Unlike bulk materials, nanoscale
79 + materials have a significant fraction of their atoms at interfaces,
80 + and the chemical details of these interfaces govern the heat transfer
81 + behavior. Furthermore, the interfaces are
82 + heterogeneous (e.g. solid - liquid), which provides a challenge to
83 + traditional methods developed for homogeneous systems.
84  
85 < Interfacial thermal conductance is extensively studied both
86 < experimentally and computationally, and systems with interfaces
87 < present are generally heterogeneous. Although interfaces are commonly
88 < barriers to heat transfer, it has been
89 < reported\cite{doi:10.1021/la904855s} that under specific circustances,
90 < e.g. with certain capping agents present on the surface, interfacial
91 < conductance can be significantly enhanced. However, heat conductance
92 < of molecular and nano-scale interfaces will be affected by the
93 < chemical details of the surface and is challenging to
94 < experimentalist. The lower thermal flux through interfaces is even
95 < more difficult to measure with EMD and forward NEMD simulation
96 < methods. Therefore, developing good simulation methods will be
97 < desirable in order to investigate thermal transport across interfaces.
85 > Experimentally, various interfaces have been investigated for their
86 > thermal conductance. Cahill and coworkers studied nanoscale thermal
87 > transport from metal nanoparticle/fluid interfaces, to epitaxial
88 > TiN/single crystal oxides interfaces, to hydrophilic and hydrophobic
89 > interfaces between water and solids with different self-assembled
90 > monolayers.\cite{Wilson:2002uq,PhysRevB.67.054302,doi:10.1021/jp048375k,PhysRevLett.96.186101}
91 > Wang {\it et al.} studied heat transport through
92 > long-chain hydrocarbon monolayers on gold substrate at individual
93 > molecular level,\cite{Wang10082007} Schmidt {\it et al.} studied the
94 > role of CTAB on thermal transport between gold nanorods and
95 > solvent,\cite{doi:10.1021/jp8051888} and Juv\'e {\it et al.} studied
96 > the cooling dynamics, which is controlled by thermal interface
97 > resistence of glass-embedded metal
98 > nanoparticles.\cite{PhysRevB.80.195406} Although interfaces are
99 > normally considered barriers for heat transport, Alper {\it et al.}
100 > suggested that specific ligands (capping agents) could completely
101 > eliminate this barrier
102 > ($G\rightarrow\infty$).\cite{doi:10.1021/la904855s}
103  
104 < Recently, we have developed the Non-Isotropic Velocity Scaling (NIVS)
104 > Theoretical and computational models have also been used to study the
105 > interfacial thermal transport in order to gain an understanding of
106 > this phenomena at the molecular level. Recently, Hase and coworkers
107 > employed Non-Equilibrium Molecular Dynamics (NEMD) simulations to
108 > study thermal transport from hot Au(111) substrate to a self-assembled
109 > monolayer of alkylthiol with relatively long chain (8-20 carbon
110 > atoms).\cite{hase:2010,hase:2011} However, ensemble averaged
111 > measurements for heat conductance of interfaces between the capping
112 > monolayer on Au and a solvent phase have yet to be studied with their
113 > approach. The comparatively low thermal flux through interfaces is
114 > difficult to measure with Equilibrium
115 > MD\cite{doi:10.1080/0026897031000068578} or forward NEMD simulation
116 > methods. Therefore, the Reverse NEMD (RNEMD)
117 > methods\cite{MullerPlathe:1997xw,kuang:164101} would have the
118 > advantage of applying this difficult to measure flux (while measuring
119 > the resulting gradient), given that the simulation methods being able
120 > to effectively apply an unphysical flux in non-homogeneous systems.
121 > Garde and coworkers\cite{garde:nl2005,garde:PhysRevLett2009} applied
122 > this approach to various liquid interfaces and studied how thermal
123 > conductance (or resistance) is dependent on chemistry details of
124 > interfaces, e.g. hydrophobic and hydrophilic aqueous interfaces.
125 >
126 > Recently, we have developed a Non-Isotropic Velocity Scaling (NIVS)
127   algorithm for RNEMD simulations\cite{kuang:164101}. This algorithm
128   retains the desirable features of RNEMD (conservation of linear
129   momentum and total energy, compatibility with periodic boundary
130   conditions) while establishing true thermal distributions in each of
131 < the two slabs. Furthermore, it allows more effective thermal exchange
132 < between particles of different identities, and thus enables extensive
133 < study of interfacial conductance.
131 > the two slabs. Furthermore, it allows effective thermal exchange
132 > between particles of different identities, and thus makes the study of
133 > interfacial conductance much simpler.
134  
135 + The work presented here deals with the Au(111) surface covered to
136 + varying degrees by butanethiol, a capping agent with short carbon
137 + chain, and solvated with organic solvents of different molecular
138 + properties. Different models were used for both the capping agent and
139 + the solvent force field parameters. Using the NIVS algorithm, the
140 + thermal transport across these interfaces was studied and the
141 + underlying mechanism for the phenomena was investigated.
142 +
143   \section{Methodology}
144 < \subsection{Algorithm}
145 < There have been many algorithms for computing thermal conductivity
146 < using molecular dynamics simulations. However, interfacial conductance
147 < is at least an order of magnitude smaller. This would make the
148 < calculation even more difficult for those slowly-converging
149 < equilibrium methods. Imposed-flux non-equilibrium
150 < methods\cite{MullerPlathe:1997xw} have the flux set {\it a priori} and
151 < the response of temperature or momentum gradients are easier to
152 < measure than the flux, if unknown, and thus, is a preferable way to
153 < the forward NEMD methods. Although the momentum swapping approach for
154 < flux-imposing can be used for exchanging energy between particles of
155 < different identity, the kinetic energy transfer efficiency is affected
156 < by the mass difference between the particles, which limits its
157 < application on heterogeneous interfacial systems.
144 > \subsection{Imposd-Flux Methods in MD Simulations}
145 > Steady state MD simulations have an advantage in that not many
146 > trajectories are needed to study the relationship between thermal flux
147 > and thermal gradients. For systems with low interfacial conductance,
148 > one must have a method capable of generating or measuring relatively
149 > small fluxes, compared to those required for bulk conductivity. This
150 > requirement makes the calculation even more difficult for
151 > slowly-converging equilibrium methods.\cite{Viscardy:2007lq} Forward
152 > NEMD methods impose a gradient (and measure a flux), but at interfaces
153 > it is not clear what behavior should be imposed at the boundaries
154 > between materials.  Imposed-flux reverse non-equilibrium
155 > methods\cite{MullerPlathe:1997xw} set the flux {\it a priori} and
156 > the thermal response becomes an easy-to-measure quantity.  Although
157 > M\"{u}ller-Plathe's original momentum swapping approach can be used
158 > for exchanging energy between particles of different identity, the
159 > kinetic energy transfer efficiency is affected by the mass difference
160 > between the particles, which limits its application on heterogeneous
161 > interfacial systems.
162  
163 < The non-isotropic velocity scaling (NIVS)\cite{kuang:164101} approach in
164 < non-equilibrium MD simulations is able to impose relatively large
165 < kinetic energy flux without obvious perturbation to the velocity
166 < distribution of the simulated systems. Furthermore, this approach has
163 > The non-isotropic velocity scaling (NIVS) \cite{kuang:164101} approach
164 > to non-equilibrium MD simulations is able to impose a wide range of
165 > kinetic energy fluxes without obvious perturbation to the velocity
166 > distributions of the simulated systems. Furthermore, this approach has
167   the advantage in heterogeneous interfaces in that kinetic energy flux
168   can be applied between regions of particles of arbitary identity, and
169 < the flux quantity is not restricted by particle mass difference.
169 > the flux will not be restricted by difference in particle mass.
170  
171   The NIVS algorithm scales the velocity vectors in two separate regions
172   of a simulation system with respective diagonal scaling matricies. To
173   determine these scaling factors in the matricies, a set of equations
174   including linear momentum conservation and kinetic energy conservation
175 < constraints and target momentum/energy flux satisfaction is
176 < solved. With the scaling operation applied to the system in a set
177 < frequency, corresponding momentum/temperature gradients can be built,
178 < which can be used for computing transportation properties and other
179 < applications related to momentum/temperature gradients. The NIVS
131 < algorithm conserves momenta and energy and does not depend on an
132 < external thermostat.
175 > constraints and target energy flux satisfaction is solved. With the
176 > scaling operation applied to the system in a set frequency, bulk
177 > temperature gradients can be easily established, and these can be used
178 > for computing thermal conductivities. The NIVS algorithm conserves
179 > momenta and energy and does not depend on an external thermostat.
180  
181 < (wondering how much detail of algorithm should be put here...)
181 > \subsection{Defining Interfacial Thermal Conductivity ($G$)}
182  
183 < \subsection{Force Field Parameters}
184 < Our simulation systems consists of metal gold lattice slab solvated by
185 < organic solvents. In order to study the role of capping agents in
186 < interfacial thermal conductance, butanethiol is chosen to cover gold
187 < surfaces in comparison to no capping agent present.
183 > For an interface with relatively low interfacial conductance, and a
184 > thermal flux between two distinct bulk regions, the regions on either
185 > side of the interface rapidly come to a state in which the two phases
186 > have relatively homogeneous (but distinct) temperatures. The
187 > interfacial thermal conductivity $G$ can therefore be approximated as:
188 > \begin{equation}
189 >  G = \frac{E_{total}}{2 t L_x L_y \left( \langle T_\mathrm{hot}\rangle -
190 >    \langle T_\mathrm{cold}\rangle \right)}
191 > \label{lowG}
192 > \end{equation}
193 > where ${E_{total}}$ is the total imposed non-physical kinetic energy
194 > transfer during the simulation and ${\langle T_\mathrm{hot}\rangle}$
195 > and ${\langle T_\mathrm{cold}\rangle}$ are the average observed
196 > temperature of the two separated phases.  For an applied flux $J_z$
197 > operating over a simulation time $t$ on a periodically-replicated slab
198 > of dimensions $L_x \times L_y$, $E_{total} = J_z *(t)*(2 L_x L_y)$.
199  
142 The Au-Au interactions in metal lattice slab is described by the
143 quantum Sutton-Chen (QSC) formulation.\cite{PhysRevB.59.3527} The QSC
144 potentials include zero-point quantum corrections and are
145 reparametrized for accurate surface energies compared to the
146 Sutton-Chen potentials\cite{Chen90}.
147
148 Straight chain {\it n}-hexane and aromatic toluene are respectively
149 used as solvents. For hexane, both United-Atom\cite{TraPPE-UA.alkanes}
150 and All-Atom\cite{OPLSAA} force fields are used for comparison; for
151 toluene, United-Atom\cite{TraPPE-UA.alkylbenzenes} force fields are
152 used with rigid body constraints applied. (maybe needs more details
153 about rigid body)
154
155 Buatnethiol molecules are used as capping agent for some of our
156 simulations. United-Atom\cite{TraPPE-UA.thiols} and All-Atom models
157 are respectively used corresponding to the force field type of
158 solvent.
159
160 To describe the interactions between metal Au and non-metal capping
161 agent and solvent, we refer to Vlugt\cite{vlugt:cpc2007154} and derive
162 other interactions which are not parametrized in their work. (can add
163 hautman and klein's paper here and more discussion; need to put
164 aromatic-metal interaction approximation here)
165
166 [TABULATED FORCE FIELD PARAMETERS NEEDED]
167
168 \section{Computational Details}
169 \subsection{System Geometry}
170 Our simulation systems consists of a lattice Au slab with the (111)
171 surface perpendicular to the $z$-axis, and a solvent layer between the
172 periodic Au slabs along the $z$-axis. To set up the interfacial
173 system, the Au slab is first equilibrated without solvent under room
174 pressure and a desired temperature. After the metal slab is
175 equilibrated, United-Atom or All-Atom butanethiols are replicated on
176 the Au surface, each occupying the (??) among three Au atoms, and is
177 equilibrated under NVT ensemble. According to (CITATION), the maximal
178 thiol capacity on Au surface is $1/3$ of the total number of surface
179 Au atoms.
180
181 \cite{packmol}
182
183 \subsection{Simulation Parameters}
184
200   When the interfacial conductance is {\it not} small, there are two
201 < ways to define $G$. If we assume the temperature is discretely
202 < different on two sides of the interface, $G$ can be calculated with
203 < the thermal flux applied $J$ and the temperature difference measured
204 < $\Delta T$ as:
201 > ways to define $G$. One common way is to assume the temperature is
202 > discrete on the two sides of the interface. $G$ can be calculated
203 > using the applied thermal flux $J$ and the maximum temperature
204 > difference measured along the thermal gradient max($\Delta T$), which
205 > occurs at the Gibbs deviding surface (Figure \ref{demoPic}). This is
206 > known as the Kapitza conductance, which is the inverse of the Kapitza
207 > resistance.
208   \begin{equation}
209 < G=\frac{J}{\Delta T}
209 >  G=\frac{J}{\Delta T}
210   \label{discreteG}
211   \end{equation}
212 < We can as well assume a continuous temperature profile along the
213 < thermal gradient axis $z$ and define $G$ as the change of bulk thermal
214 < conductivity $\lambda$ at a defined interfacial point:
212 >
213 > \begin{figure}
214 > \includegraphics[width=\linewidth]{method}
215 > \caption{Interfacial conductance can be calculated by applying an
216 >  (unphysical) kinetic energy flux between two slabs, one located
217 >  within the metal and another on the edge of the periodic box.  The
218 >  system responds by forming a thermal response or a gradient.  In
219 >  bulk liquids, this gradient typically has a single slope, but in
220 >  interfacial systems, there are distinct thermal conductivity
221 >  domains.  The interfacial conductance, $G$ is found by measuring the
222 >  temperature gap at the Gibbs dividing surface, or by using second
223 >  derivatives of the thermal profile.}
224 > \label{demoPic}
225 > \end{figure}
226 >
227 > The other approach is to assume a continuous temperature profile along
228 > the thermal gradient axis (e.g. $z$) and define $G$ at the point where
229 > the magnitude of thermal conductivity ($\lambda$) change reaches its
230 > maximum, given that $\lambda$ is well-defined throughout the space:
231   \begin{equation}
232   G^\prime = \Big|\frac{\partial\lambda}{\partial z}\Big|
233           = \Big|\frac{\partial}{\partial z}\left(-J_z\Big/
234             \left(\frac{\partial T}{\partial z}\right)\right)\Big|
235 <         = J_z\Big|\frac{\partial^2 T}{\partial z^2}\Big|
235 >         = |J_z|\Big|\frac{\partial^2 T}{\partial z^2}\Big|
236           \Big/\left(\frac{\partial T}{\partial z}\right)^2
237   \label{derivativeG}
238   \end{equation}
239 < With the temperature profile obtained from simulations, one is able to
239 >
240 > With temperature profiles obtained from simulation, one is able to
241   approximate the first and second derivatives of $T$ with finite
242 < difference method and thus calculate $G^\prime$.
242 > difference methods and calculate $G^\prime$. In what follows, both
243 > definitions have been used, and are compared in the results.
244  
245 < In what follows, both definitions are used for calculation and comparison.
245 > To investigate the interfacial conductivity at metal / solvent
246 > interfaces, we have modeled a metal slab with its (111) surfaces
247 > perpendicular to the $z$-axis of our simulation cells. The metal slab
248 > has been prepared both with and without capping agents on the exposed
249 > surface, and has been solvated with simple organic solvents, as
250 > illustrated in Figure \ref{gradT}.
251  
252 < \section{Results}
253 < \subsection{Toluene Solvent}
252 > With the simulation cell described above, we are able to equilibrate
253 > the system and impose an unphysical thermal flux between the liquid
254 > and the metal phase using the NIVS algorithm. By periodically applying
255 > the unphysical flux, we obtained a temperature profile and its spatial
256 > derivatives. Figure \ref{gradT} shows how an applied thermal flux can
257 > be used to obtain the 1st and 2nd derivatives of the temperature
258 > profile.
259  
260 < The simulations follow a protocol similar to the previous gold/water
261 < interfacial systems. The results (Table \ref{AuThiolToluene}) show a
262 < significant conductance enhancement compared to the gold/water
263 < interface without capping agent and agree with available experimental
264 < data. This indicates that the metal-metal potential, though not
265 < predicting an accurate bulk metal thermal conductivity, does not
266 < greatly interfere with the simulation of the thermal conductance
267 < behavior across a non-metal interface. The solvent model is not
222 < particularly volatile, so the simulation cell does not expand
223 < significantly under higher temperature. We did not observe a
224 < significant conductance decrease when the temperature was increased to
225 < 300K. The results show that the two definitions used for $G$ yield
226 < comparable values, though $G^\prime$ tends to be smaller.
260 > \begin{figure}
261 > \includegraphics[width=\linewidth]{gradT}
262 > \caption{A sample of Au-butanethiol/hexane interfacial system and the
263 >  temperature profile after a kinetic energy flux is imposed to
264 >  it. The 1st and 2nd derivatives of the temperature profile can be
265 >  obtained with finite difference approximation (lower panel).}
266 > \label{gradT}
267 > \end{figure}
268  
269 + \section{Computational Details}
270 + \subsection{Simulation Protocol}
271 + The NIVS algorithm has been implemented in our MD simulation code,
272 + OpenMD\cite{Meineke:2005gd,openmd}, and was used for our simulations.
273 + Metal slabs of 6 or 11 layers of Au atoms were first equilibrated
274 + under atmospheric pressure (1 atm) and 200K. After equilibration,
275 + butanethiol capping agents were placed at three-fold hollow sites on
276 + the Au(111) surfaces. These sites are either {\it fcc} or {\it
277 +  hcp} sites, although Hase {\it et al.} found that they are
278 + equivalent in a heat transfer process,\cite{hase:2010} so we did not
279 + distinguish between these sites in our study. The maximum butanethiol
280 + capacity on Au surface is $1/3$ of the total number of surface Au
281 + atoms, and the packing forms a $(\sqrt{3}\times\sqrt{3})R30^\circ$
282 + structure\cite{doi:10.1021/ja00008a001,doi:10.1021/cr9801317}. A
283 + series of lower coverages was also prepared by eliminating
284 + butanethiols from the higher coverage surface in a regular manner. The
285 + lower coverages were prepared in order to study the relation between
286 + coverage and interfacial conductance.
287 +
288 + The capping agent molecules were allowed to migrate during the
289 + simulations. They distributed themselves uniformly and sampled a
290 + number of three-fold sites throughout out study. Therefore, the
291 + initial configuration does not noticeably affect the sampling of a
292 + variety of configurations of the same coverage, and the final
293 + conductance measurement would be an average effect of these
294 + configurations explored in the simulations.
295 +
296 + After the modified Au-butanethiol surface systems were equilibrated in
297 + the canonical (NVT) ensemble, organic solvent molecules were packed in
298 + the previously empty part of the simulation cells.\cite{packmol} Two
299 + solvents were investigated, one which has little vibrational overlap
300 + with the alkanethiol and which has a planar shape (toluene), and one
301 + which has similar vibrational frequencies to the capping agent and
302 + chain-like shape ({\it n}-hexane).
303 +
304 + The simulation cells were not particularly extensive along the
305 + $z$-axis, as a very long length scale for the thermal gradient may
306 + cause excessively hot or cold temperatures in the middle of the
307 + solvent region and lead to undesired phenomena such as solvent boiling
308 + or freezing when a thermal flux is applied. Conversely, too few
309 + solvent molecules would change the normal behavior of the liquid
310 + phase. Therefore, our $N_{solvent}$ values were chosen to ensure that
311 + these extreme cases did not happen to our simulations. The spacing
312 + between periodic images of the gold interfaces is $45 \sim 75$\AA.
313 +
314 + The initial configurations generated are further equilibrated with the
315 + $x$ and $y$ dimensions fixed, only allowing the $z$-length scale to
316 + change. This is to ensure that the equilibration of liquid phase does
317 + not affect the metal's crystalline structure. Comparisons were made
318 + with simulations that allowed changes of $L_x$ and $L_y$ during NPT
319 + equilibration. No substantial changes in the box geometry were noticed
320 + in these simulations. After ensuring the liquid phase reaches
321 + equilibrium at atmospheric pressure (1 atm), further equilibration was
322 + carried out under canonical (NVT) and microcanonical (NVE) ensembles.
323 +
324 + After the systems reach equilibrium, NIVS was used to impose an
325 + unphysical thermal flux between the metal and the liquid phases. Most
326 + of our simulations were done under an average temperature of
327 + $\sim$200K. Therefore, thermal flux usually came from the metal to the
328 + liquid so that the liquid has a higher temperature and would not
329 + freeze due to lowered temperatures. After this induced temperature
330 + gradient had stablized, the temperature profile of the simulation cell
331 + was recorded. To do this, the simulation cell is devided evenly into
332 + $N$ slabs along the $z$-axis. The average temperatures of each slab
333 + are recorded for 1$\sim$2 ns. When the slab width $d$ of each slab is
334 + the same, the derivatives of $T$ with respect to slab number $n$ can
335 + be directly used for $G^\prime$ calculations: \begin{equation}
336 +  G^\prime = |J_z|\Big|\frac{\partial^2 T}{\partial z^2}\Big|
337 +         \Big/\left(\frac{\partial T}{\partial z}\right)^2
338 +         = |J_z|\Big|\frac{1}{d^2}\frac{\partial^2 T}{\partial n^2}\Big|
339 +         \Big/\left(\frac{1}{d}\frac{\partial T}{\partial n}\right)^2
340 +         = |J_z|\Big|\frac{\partial^2 T}{\partial n^2}\Big|
341 +         \Big/\left(\frac{\partial T}{\partial n}\right)^2
342 + \label{derivativeG2}
343 + \end{equation}
344 +
345 + All of the above simulation procedures use a time step of 1 fs. Each
346 + equilibration stage took a minimum of 100 ps, although in some cases,
347 + longer equilibration stages were utilized.
348 +
349 + \subsection{Force Field Parameters}
350 + Our simulations include a number of chemically distinct components.
351 + Figure \ref{demoMol} demonstrates the sites defined for both
352 + United-Atom and All-Atom models of the organic solvent and capping
353 + agents in our simulations. Force field parameters are needed for
354 + interactions both between the same type of particles and between
355 + particles of different species.
356 +
357 + \begin{figure}
358 + \includegraphics[width=\linewidth]{structures}
359 + \caption{Structures of the capping agent and solvents utilized in
360 +  these simulations. The chemically-distinct sites (a-e) are expanded
361 +  in terms of constituent atoms for both United Atom (UA) and All Atom
362 +  (AA) force fields.  Most parameters are from
363 +  Refs. \protect\cite{TraPPE-UA.alkanes,TraPPE-UA.alkylbenzenes,TraPPE-UA.thiols}
364 +  (UA) and \protect\cite{OPLSAA} (AA). Cross-interactions with the Au
365 +  atoms are given in Table \ref{MnM}.}
366 + \label{demoMol}
367 + \end{figure}
368 +
369 + The Au-Au interactions in metal lattice slab is described by the
370 + quantum Sutton-Chen (QSC) formulation.\cite{PhysRevB.59.3527} The QSC
371 + potentials include zero-point quantum corrections and are
372 + reparametrized for accurate surface energies compared to the
373 + Sutton-Chen potentials.\cite{Chen90}
374 +
375 + For the two solvent molecules, {\it n}-hexane and toluene, two
376 + different atomistic models were utilized. Both solvents were modeled
377 + using United-Atom (UA) and All-Atom (AA) models. The TraPPE-UA
378 + parameters\cite{TraPPE-UA.alkanes,TraPPE-UA.alkylbenzenes} are used
379 + for our UA solvent molecules. In these models, sites are located at
380 + the carbon centers for alkyl groups. Bonding interactions, including
381 + bond stretches and bends and torsions, were used for intra-molecular
382 + sites closer than 3 bonds. For non-bonded interactions, Lennard-Jones
383 + potentials are used.
384 +
385 + By eliminating explicit hydrogen atoms, the TraPPE-UA models are
386 + simple and computationally efficient, while maintaining good accuracy.
387 + However, the TraPPE-UA model for alkanes is known to predict a slighly
388 + lower boiling point than experimental values. This is one of the
389 + reasons we used a lower average temperature (200K) for our
390 + simulations. If heat is transferred to the liquid phase during the
391 + NIVS simulation, the liquid in the hot slab can actually be
392 + substantially warmer than the mean temperature in the simulation. The
393 + lower mean temperatures therefore prevent solvent boiling.
394 +
395 + For UA-toluene, the non-bonded potentials between intermolecular sites
396 + have a similar Lennard-Jones formulation. The toluene molecules were
397 + treated as a single rigid body, so there was no need for
398 + intramolecular interactions (including bonds, bends, or torsions) in
399 + this solvent model.
400 +
401 + Besides the TraPPE-UA models, AA models for both organic solvents are
402 + included in our studies as well. The OPLS-AA\cite{OPLSAA} force fields
403 + were used. For hexane, additional explicit hydrogen sites were
404 + included. Besides bonding and non-bonded site-site interactions,
405 + partial charges and the electrostatic interactions were added to each
406 + CT and HC site. For toluene, a flexible model for the toluene molecule
407 + was utilized which included bond, bend, torsion, and inversion
408 + potentials to enforce ring planarity.
409 +
410 + The butanethiol capping agent in our simulations, were also modeled
411 + with both UA and AA model. The TraPPE-UA force field includes
412 + parameters for thiol molecules\cite{TraPPE-UA.thiols} and are used for
413 + UA butanethiol model in our simulations. The OPLS-AA also provides
414 + parameters for alkyl thiols. However, alkyl thiols adsorbed on Au(111)
415 + surfaces do not have the hydrogen atom bonded to sulfur. To derive
416 + suitable parameters for butanethiol adsorbed on Au(111) surfaces, we
417 + adopt the S parameters from Luedtke and Landman\cite{landman:1998} and
418 + modify the parameters for the CTS atom to maintain charge neutrality
419 + in the molecule.  Note that the model choice (UA or AA) for the capping
420 + agent can be different from the solvent. Regardless of model choice,
421 + the force field parameters for interactions between capping agent and
422 + solvent can be derived using Lorentz-Berthelot Mixing Rule:
423 + \begin{eqnarray}
424 +  \sigma_{ij} & = & \frac{1}{2} \left(\sigma_{ii} + \sigma_{jj}\right) \\
425 +  \epsilon_{ij} & = & \sqrt{\epsilon_{ii}\epsilon_{jj}}
426 + \end{eqnarray}
427 +
428 + To describe the interactions between metal (Au) and non-metal atoms,
429 + we refer to an adsorption study of alkyl thiols on gold surfaces by
430 + Vlugt {\it et al.}\cite{vlugt:cpc2007154} They fitted an effective
431 + Lennard-Jones form of potential parameters for the interaction between
432 + Au and pseudo-atoms CH$_x$ and S based on a well-established and
433 + widely-used effective potential of Hautman and Klein for the Au(111)
434 + surface.\cite{hautman:4994} As our simulations require the gold slab
435 + to be flexible to accommodate thermal excitation, the pair-wise form
436 + of potentials they developed was used for our study.
437 +
438 + The potentials developed from {\it ab initio} calculations by Leng
439 + {\it et al.}\cite{doi:10.1021/jp034405s} are adopted for the
440 + interactions between Au and aromatic C/H atoms in toluene. However,
441 + the Lennard-Jones parameters between Au and other types of particles,
442 + (e.g. AA alkanes) have not yet been established. For these
443 + interactions, the Lorentz-Berthelot mixing rule can be used to derive
444 + effective single-atom LJ parameters for the metal using the fit values
445 + for toluene. These are then used to construct reasonable mixing
446 + parameters for the interactions between the gold and other atoms.
447 + Table \ref{MnM} summarizes the ``metal/non-metal'' parameters used in
448 + our simulations.
449 +
450   \begin{table*}
451    \begin{minipage}{\linewidth}
452      \begin{center}
453 <      \caption{Computed interfacial thermal conductivity ($G$ and
454 <        $G^\prime$) values for the Au/butanethiol/toluene interface at
455 <        different temperatures using a range of energy fluxes.}
456 <      
235 <      \begin{tabular}{cccc}
453 >      \caption{Non-bonded interaction parameters (including cross
454 >        interactions with Au atoms) for both force fields used in this
455 >        work.}      
456 >      \begin{tabular}{lllllll}
457          \hline\hline
458 <        $\langle T\rangle$ & $J_z$ & $G$ & $G^\prime$ \\
459 <        (K) & (GW/m$^2$) & \multicolumn{2}{c}{(MW/m$^2$/K)} \\
458 >        & Site  & $\sigma_{ii}$ & $\epsilon_{ii}$ & $q_i$ &
459 >        $\sigma_{Au-i}$ & $\epsilon_{Au-i}$ \\
460 >        & & (\AA) & (kcal/mol) & ($e$) & (\AA) & (kcal/mol) \\
461          \hline
462 <        200 & 1.86 & 180 & 135 \\
463 <            & 2.15 & 204 & 113 \\
464 <            & 3.93 & 175 & 114 \\
465 <        300 & 1.91 & 143 & 125 \\
466 <            & 4.19 & 134 & 113 \\
462 >        United Atom (UA)
463 >        &CH3  & 3.75  & 0.1947  & -      & 3.54   & 0.2146  \\
464 >        &CH2  & 3.95  & 0.0914  & -      & 3.54   & 0.1749  \\
465 >        &CHar & 3.695 & 0.1003  & -      & 3.4625 & 0.1680  \\
466 >        &CRar & 3.88  & 0.04173 & -      & 3.555  & 0.1604  \\
467 >        \hline
468 >        All Atom (AA)
469 >        &CT3  & 3.50  & 0.066   & -0.18  & 3.365  & 0.1373  \\
470 >        &CT2  & 3.50  & 0.066   & -0.12  & 3.365  & 0.1373  \\
471 >        &CTT  & 3.50  & 0.066   & -0.065 & 3.365  & 0.1373  \\
472 >        &HC   & 2.50  & 0.030   &  0.06  & 2.865  & 0.09256 \\
473 >        &CA   & 3.55  & 0.070   & -0.115 & 3.173  & 0.0640  \\
474 >        &HA   & 2.42  & 0.030   &  0.115 & 2.746  & 0.0414  \\
475 >        \hline
476 >        Both UA and AA
477 >        & S   & 4.45  & 0.25    & -      & 2.40   & 8.465   \\
478          \hline\hline
479        \end{tabular}
480 <      \label{AuThiolToluene}
480 >      \label{MnM}
481      \end{center}
482    \end{minipage}
483   \end{table*}
484  
252 \subsection{Hexane Solvent}
485  
486 < Using the united-atom model, different coverages of capping agent,
487 < temperatures of simulations and numbers of solvent molecules were all
488 < investigated and Table \ref{AuThiolHexaneUA} shows the results of
489 < these computations. The number of hexane molecules in our simulations
490 < does not affect the calculations significantly. However, a very long
491 < length scale for the thermal gradient axis ($z$) may cause excessively
492 < hot or cold temperatures in the middle of the solvent region and lead
493 < to undesired phenomena such as solvent boiling or freezing, while too
262 < few solvent molecules would change the normal behavior of the liquid
263 < phase. Our $N_{hexane}$ values were chosen to ensure that these
264 < extreme cases did not happen to our simulations.
486 > \section{Results}
487 > There are many factors contributing to the measured interfacial
488 > conductance; some of these factors are physically motivated
489 > (e.g. coverage of the surface by the capping agent coverage and
490 > solvent identity), while some are governed by parameters of the
491 > methodology (e.g. applied flux and the formulas used to obtain the
492 > conductance). In this section we discuss the major physical and
493 > calculational effects on the computed conductivity.
494  
495 < Table \ref{AuThiolHexaneUA} enables direct comparison between
267 < different coverages of capping agent, when other system parameters are
268 < held constant. With high coverage of butanethiol on the gold surface,
269 < the interfacial thermal conductance is enhanced
270 < significantly. Interestingly, a slightly lower butanethiol coverage
271 < leads to a moderately higher conductivity. This is probably due to
272 < more solvent/capping agent contact when butanethiol molecules are
273 < not densely packed, which enhances the interactions between the two
274 < phases and lowers the thermal transfer barrier of this interface.
275 < % [COMPARE TO AU/WATER IN PAPER]
495 > \subsection{Effects due to capping agent coverage}
496  
497 < It is also noted that the overall simulation temperature is another
498 < factor that affects the interfacial thermal conductance. One
499 < possibility of this effect may be rooted in the decrease in density of
500 < the liquid phase. We observed that when the average temperature
501 < increases from 200K to 250K, the bulk hexane density becomes lower
502 < than experimental value, as the system is equilibrated under NPT
283 < ensemble. This leads to lower contact between solvent and capping
284 < agent, and thus lower conductivity.
497 > A series of different initial conditions with a range of surface
498 > coverages was prepared and solvated with various with both of the
499 > solvent molecules. These systems were then equilibrated and their
500 > interfacial thermal conductivity was measured with the NIVS
501 > algorithm. Figure \ref{coverage} demonstrates the trend of conductance
502 > with respect to surface coverage.
503  
504 < Conductivity values are more difficult to obtain under higher
505 < temperatures. This is because the Au surface tends to undergo
506 < reconstructions in relatively high temperatures. Surface Au atoms can
507 < migrate outward to reach higher Au-S contact; and capping agent
508 < molecules can be embedded into the surface Au layer due to the same
509 < driving force. This phenomenon agrees with experimental
510 < results\cite{doi:10.1021/j100035a033,doi:10.1021/la026493y}. A surface
293 < fully covered in capping agent is more susceptible to reconstruction,
294 < possibly because fully coverage prevents other means of capping agent
295 < relaxation, such as migration to an empty neighbor three-fold site.
504 > \begin{figure}
505 > \includegraphics[width=\linewidth]{coverage}
506 > \caption{Comparison of interfacial thermal conductivity ($G$) values
507 >  for the Au-butanethiol/solvent interface with various UA models and
508 >  different capping agent coverages at $\langle T\rangle\sim$200K.}
509 > \label{coverage}
510 > \end{figure}
511  
512 < %MAY ADD MORE DATA TO TABLE
512 > In partially covered surfaces, the derivative definition for
513 > $G^\prime$ (Eq. \ref{derivativeG}) becomes difficult to apply, as the
514 > location of maximum change of $\lambda$ becomes washed out.  The
515 > discrete definition (Eq. \ref{discreteG}) is easier to apply, as the
516 > Gibbs dividing surface is still well-defined. Therefore, $G$ (not
517 > $G^\prime$) was used in this section.
518 >
519 > From Figure \ref{coverage}, one can see the significance of the
520 > presence of capping agents. When even a small fraction of the Au(111)
521 > surface sites are covered with butanethiols, the conductivity exhibits
522 > an enhancement by at least a factor of 3.  Cappping agents are clearly
523 > playing a major role in thermal transport at metal / organic solvent
524 > surfaces.
525 >
526 > We note a non-monotonic behavior in the interfacial conductance as a
527 > function of surface coverage. The maximum conductance (largest $G$)
528 > happens when the surfaces are about 75\% covered with butanethiol
529 > caps.  The reason for this behavior is not entirely clear.  One
530 > explanation is that incomplete butanethiol coverage allows small gaps
531 > between butanethiols to form. These gaps can be filled by transient
532 > solvent molecules.  These solvent molecules couple very strongly with
533 > the hot capping agent molecules near the surface, and can then carry
534 > away (diffusively) the excess thermal energy from the surface.
535 >
536 > There appears to be a competition between the conduction of the
537 > thermal energy away from the surface by the capping agents (enhanced
538 > by greater coverage) and the coupling of the capping agents with the
539 > solvent (enhanced by interdigitation at lower coverages).  This
540 > competition would lead to the non-monotonic coverage behavior observed
541 > here.
542 >
543 > Results for rigid body toluene solvent, as well as the UA hexane, are
544 > within the ranges expected from prior experimental
545 > work.\cite{Wilson:2002uq,cahill:793,PhysRevB.80.195406} This suggests
546 > that explicit hydrogen atoms might not be required for modeling
547 > thermal transport in these systems.  C-H vibrational modes do not see
548 > significant excited state population at low temperatures, and are not
549 > likely to carry lower frequency excitations from the solid layer into
550 > the bulk liquid.
551 >
552 > The toluene solvent does not exhibit the same behavior as hexane in
553 > that $G$ remains at approximately the same magnitude when the capping
554 > coverage increases from 25\% to 75\%.  Toluene, as a rigid planar
555 > molecule, cannot occupy the relatively small gaps between the capping
556 > agents as easily as the chain-like {\it n}-hexane.  The effect of
557 > solvent coupling to the capping agent is therefore weaker in toluene
558 > except at the very lowest coverage levels.  This effect counters the
559 > coverage-dependent conduction of heat away from the metal surface,
560 > leading to a much flatter $G$ vs. coverage trend than is observed in
561 > {\it n}-hexane.
562 >
563 > \subsection{Effects due to Solvent \& Solvent Models}
564 > In addition to UA solvent and capping agent models, AA models have
565 > also been included in our simulations.  In most of this work, the same
566 > (UA or AA) model for solvent and capping agent was used, but it is
567 > also possible to utilize different models for different components.
568 > We have also included isotopic substitutions (Hydrogen to Deuterium)
569 > to decrease the explicit vibrational overlap between solvent and
570 > capping agent. Table \ref{modelTest} summarizes the results of these
571 > studies.
572 >
573   \begin{table*}
574    \begin{minipage}{\linewidth}
575      \begin{center}
301      \caption{Computed interfacial thermal conductivity ($G$ and
302        $G^\prime$) values for the Au/butanethiol/hexane interface
303        with united-atom model and different capping agent coverage
304        and solvent molecule numbers at different temperatures using a
305        range of energy fluxes.}
576        
577 <      \begin{tabular}{cccccc}
577 >      \caption{Computed interfacial thermal conductance ($G$ and
578 >        $G^\prime$) values for interfaces using various models for
579 >        solvent and capping agent (or without capping agent) at
580 >        $\langle T\rangle\sim$200K. (D stands for deuterated solvent
581 >        or capping agent molecules; ``Avg.'' denotes results that are
582 >        averages of simulations under different applied thermal flux
583 >        values $(J_z)$. Error estimates are indicated in
584 >        parentheses.)}
585 >      
586 >      \begin{tabular}{llccc}
587          \hline\hline
588 <        Thiol & $\langle T\rangle$ & & $J_z$ & $G$ & $G^\prime$ \\
589 <        coverage (\%) & (K) & $N_{hexane}$ & (GW/m$^2$) &
588 >        Butanethiol model & Solvent & $J_z$ & $G$ & $G^\prime$ \\
589 >        (or bare surface) & model & (GW/m$^2$) &
590          \multicolumn{2}{c}{(MW/m$^2$/K)} \\
591          \hline
592 <        0.0   & 200 & 200 & 0.96 & 43.3 & 42.7 \\
593 <              &     &     & 1.91 & 45.7 & 42.9 \\
594 <              &     & 166 & 0.96 & 43.1 & 53.4 \\
595 <        88.9  & 200 & 166 & 1.94 & 172  & 108  \\
596 <        100.0 & 250 & 200 & 0.96 & 81.8 & 67.0 \\
597 <              &     & 166 & 0.98 & 79.0 & 62.9 \\
598 <              &     &     & 1.44 & 76.2 & 64.8 \\
599 <              & 200 & 200 & 1.92 & 129  & 87.3 \\
600 <              &     &     & 1.93 & 131  & 77.5 \\
601 <              &     & 166 & 0.97 & 115  & 69.3 \\
602 <              &     &     & 1.94 & 125  & 87.1 \\
592 >        UA    & UA hexane    & Avg. & 131(9)    & 87(10)    \\
593 >              & UA hexane(D) & 1.95 & 153(5)    & 136(13)   \\
594 >              & AA hexane    & Avg. & 131(6)    & 122(10)   \\
595 >              & UA toluene   & 1.96 & 187(16)   & 151(11)   \\
596 >              & AA toluene   & 1.89 & 200(36)   & 149(53)   \\
597 >        \hline
598 >        AA    & UA hexane    & 1.94 & 116(9)    & 129(8)    \\
599 >              & AA hexane    & Avg. & 442(14)   & 356(31)   \\
600 >              & AA hexane(D) & 1.93 & 222(12)   & 234(54)   \\
601 >              & UA toluene   & 1.98 & 125(25)   & 97(60)    \\
602 >              & AA toluene   & 3.79 & 487(56)   & 290(42)   \\
603 >        \hline
604 >        AA(D) & UA hexane    & 1.94 & 158(25)   & 172(4)    \\
605 >              & AA hexane    & 1.92 & 243(29)   & 191(11)   \\
606 >              & AA toluene   & 1.93 & 364(36)   & 322(67)   \\
607 >        \hline
608 >        bare  & UA hexane    & Avg. & 46.5(3.2) & 49.4(4.5) \\
609 >              & UA hexane(D) & 0.98 & 43.9(4.6) & 43.0(2.0) \\
610 >              & AA hexane    & 0.96 & 31.0(1.4) & 29.4(1.3) \\
611 >              & UA toluene   & 1.99 & 70.1(1.3) & 65.8(0.5) \\
612          \hline\hline
613        \end{tabular}
614 <      \label{AuThiolHexaneUA}
614 >      \label{modelTest}
615      \end{center}
616    \end{minipage}
617   \end{table*}
618  
619 < For the all-atom model, the liquid hexane phase was not stable under NPT
620 < conditions. Therefore, the simulation length scale parameters are
621 < adopted from previous equilibration results of the united-atom model
334 < at 200K. Table \ref{AuThiolHexaneAA} shows the results of these
335 < simulations. The conductivity values calculated with full capping
336 < agent coverage are substantially larger than observed in the
337 < united-atom model, and is even higher than predicted by
338 < experiments. It is possible that our parameters for metal-non-metal
339 < particle interactions lead to an overestimate of the interfacial
340 < thermal conductivity, although the active C-H vibrations in the
341 < all-atom model (which should not be appreciably populated at normal
342 < temperatures) could also account for this high conductivity. The major
343 < thermal transfer barrier of Au/butanethiol/hexane interface is between
344 < the liquid phase and the capping agent, so extra degrees of freedom
345 < such as the C-H vibrations could enhance heat exchange between these
346 < two phases and result in a much higher conductivity.
619 > To facilitate direct comparison between force fields, systems with the
620 > same capping agent and solvent were prepared with the same length
621 > scales for the simulation cells.
622  
623 + On bare metal / solvent surfaces, different force field models for
624 + hexane yield similar results for both $G$ and $G^\prime$, and these
625 + two definitions agree with each other very well. This is primarily an
626 + indicator of weak interactions between the metal and the solvent, and
627 + is a typical case for acoustic impedance mismatch between these two
628 + phases.  
629 +
630 + For the fully-covered surfaces, the choice of force field for the
631 + capping agent and solvent has a large impact on the calulated values
632 + of $G$ and $G^\prime$.  The AA thiol to AA solvent conductivities are
633 + much larger than their UA to UA counterparts, and these values exceed
634 + the experimental estimates by a large measure.  The AA force field
635 + allows significant energy to go into C-H (or C-D) stretching modes,
636 + and since these modes are high frequency, this non-quantum behavior is
637 + likely responsible for the overestimate of the conductivity.  Compared
638 + to the AA model, the UA model yields more reasonable conductivity
639 + values with much higher computational efficiency.
640 +
641 + \subsubsection{Are electronic excitations in the metal important?}
642 + Because they lack electronic excitations, the QSC and related embedded
643 + atom method (EAM) models for gold are known to predict unreasonably
644 + low values for bulk conductivity
645 + ($\lambda$).\cite{kuang:164101,ISI:000207079300006,Clancy:1992} If the
646 + conductance between the phases ($G$) is governed primarily by phonon
647 + excitation (and not electronic degrees of freedom), one would expect a
648 + classical model to capture most of the interfacial thermal
649 + conductance.  Our results for $G$ and $G^\prime$ indicate that this is
650 + indeed the case, and suggest that the modeling of interfacial thermal
651 + transport depends primarily on the description of the interactions
652 + between the various components at the interface.  When the metal is
653 + chemically capped, the primary barrier to thermal conductivity appears
654 + to be the interface between the capping agent and the surrounding
655 + solvent, so the excitations in the metal have little impact on the
656 + value of $G$.
657 +
658 + \subsection{Effects due to methodology and simulation parameters}
659 +
660 + We have varied the parameters of the simulations in order to
661 + investigate how these factors would affect the computation of $G$.  Of
662 + particular interest are: 1) the length scale for the applied thermal
663 + gradient (modified by increasing the amount of solvent in the system),
664 + 2) the sign and magnitude of the applied thermal flux, 3) the average
665 + temperature of the simulation (which alters the solvent density during
666 + equilibration), and 4) the definition of the interfacial conductance
667 + (Eqs. (\ref{discreteG}) or (\ref{derivativeG})) used in the
668 + calculation.
669 +
670 + Systems of different lengths were prepared by altering the number of
671 + solvent molecules and extending the length of the box along the $z$
672 + axis to accomodate the extra solvent.  Equilibration at the same
673 + temperature and pressure conditions led to nearly identical surface
674 + areas ($L_x$ and $L_y$) available to the metal and capping agent,
675 + while the extra solvent served mainly to lengthen the axis that was
676 + used to apply the thermal flux.  For a given value of the applied
677 + flux, the different $z$ length scale has only a weak effect on the
678 + computed conductivities (Table \ref{AuThiolHexaneUA}).
679 +
680 + \subsubsection{Effects of applied flux}
681 + The NIVS algorithm allows changes in both the sign and magnitude of
682 + the applied flux.  It is possible to reverse the direction of heat
683 + flow simply by changing the sign of the flux, and thermal gradients
684 + which would be difficult to obtain experimentally ($5$ K/\AA) can be
685 + easily simulated.  However, the magnitude of the applied flux is not
686 + arbitary if one aims to obtain a stable and reliable thermal gradient.
687 + A temperature gradient can be lost in the noise if $|J_z|$ is too
688 + small, and excessive $|J_z|$ values can cause phase transitions if the
689 + extremes of the simulation cell become widely separated in
690 + temperature.  Also, if $|J_z|$ is too large for the bulk conductivity
691 + of the materials, the thermal gradient will never reach a stable
692 + state.  
693 +
694 + Within a reasonable range of $J_z$ values, we were able to study how
695 + $G$ changes as a function of this flux.  In what follows, we use
696 + positive $J_z$ values to denote the case where energy is being
697 + transferred by the method from the metal phase and into the liquid.
698 + The resulting gradient therefore has a higher temperature in the
699 + liquid phase.  Negative flux values reverse this transfer, and result
700 + in higher temperature metal phases.  The conductance measured under
701 + different applied $J_z$ values is listed in Tables
702 + \ref{AuThiolHexaneUA} and \ref{AuThiolToluene}. These results do not
703 + indicate that $G$ depends strongly on $J_z$ within this flux
704 + range. The linear response of flux to thermal gradient simplifies our
705 + investigations in that we can rely on $G$ measurement with only a
706 + small number $J_z$ values.  
707 +
708   \begin{table*}
709    \begin{minipage}{\linewidth}
710      \begin{center}
351      
711        \caption{Computed interfacial thermal conductivity ($G$ and
712 <        $G^\prime$) values for the Au/butanethiol/hexane interface
713 <        with all-atom model and different capping agent coverage at
714 <        200K using a range of energy fluxes.}
712 >        $G^\prime$) values for the 100\% covered Au-butanethiol/hexane
713 >        interfaces with UA model and different hexane molecule numbers
714 >        at different temperatures using a range of energy
715 >        fluxes. Error estimates indicated in parenthesis.}
716        
717 <      \begin{tabular}{cccc}
717 >      \begin{tabular}{ccccccc}
718          \hline\hline
719 <        Thiol & $J_z$ & $G$ & $G^\prime$ \\
720 <        coverage (\%) & (GW/m$^2$) & \multicolumn{2}{c}{(MW/m$^2$/K)} \\
719 >        $\langle T\rangle$ & $N_{hexane}$  & $\rho_{hexane}$ &
720 >        $J_z$ & $G$ & $G^\prime$ \\
721 >        (K) &  & (g/cm$^3$) & (GW/m$^2$) &
722 >        \multicolumn{2}{c}{(MW/m$^2$/K)} \\
723          \hline
724 <        0.0   & 0.95 & 28.5 & 27.2 \\
725 <              & 1.88 & 30.3 & 28.9 \\
726 <        100.0 & 2.87 & 551  & 294  \\
727 <              & 3.81 & 494  & 193  \\
724 >        200 & 266 &  0.672 & -0.96 & 102(3)    & 80.0(0.8) \\
725 >            & 200 &  0.688 &  0.96 & 125(16)   & 90.2(15)  \\
726 >            &     &        &  1.91 & 139(10)   & 101(10)   \\
727 >            &     &        &  2.83 & 141(6)    & 89.9(9.8) \\
728 >            & 166 &  0.681 &  0.97 & 141(30)   & 78(22)    \\
729 >            &     &        &  1.92 & 138(4)    & 98.9(9.5) \\
730 >        \hline
731 >        250 & 200 &  0.560 &  0.96 & 75(10)    & 61.8(7.3) \\
732 >            &     &        & -0.95 & 49.4(0.3) & 45.7(2.1) \\
733 >            & 166 &  0.569 &  0.97 & 80.3(0.6) & 67(11)    \\
734 >            &     &        &  1.44 & 76.2(5.0) & 64.8(3.8) \\
735 >            &     &        & -0.95 & 56.4(2.5) & 54.4(1.1) \\
736 >            &     &        & -1.85 & 47.8(1.1) & 53.5(1.5) \\
737          \hline\hline
738        \end{tabular}
739 <      \label{AuThiolHexaneAA}
739 >      \label{AuThiolHexaneUA}
740      \end{center}
741    \end{minipage}
742   \end{table*}
743  
744 < %subsubsection{Vibrational spectrum study on conductance mechanism}
745 < To investigate the mechanism of this interfacial thermal conductance,
746 < the vibrational spectra of various gold systems were obtained and are
747 < shown as in the upper panel of Fig. \ref{vibration}. To obtain these
748 < spectra, one first runs a simulation in the NVE ensemble and collects
749 < snapshots of configurations; these configurations are used to compute
750 < the velocity auto-correlation functions, which is used to construct a
751 < power spectrum via a Fourier transform. The gold surfaces covered by
752 < butanethiol molecules exhibit an additional peak observed at a
382 < frequency of $\sim$170cm$^{-1}$, which is attributed to the vibration
383 < of the S-Au bond. This vibration enables efficient thermal transport
384 < from surface Au atoms to the capping agents. Simultaneously, as shown
385 < in the lower panel of Fig. \ref{vibration}, the large overlap of the
386 < vibration spectra of butanethiol and hexane in the all-atom model,
387 < including the C-H vibration, also suggests high thermal exchange
388 < efficiency. The combination of these two effects produces the drastic
389 < interfacial thermal conductance enhancement in the all-atom model.
744 > The sign of $J_z$ is a different matter, however, as this can alter
745 > the temperature on the two sides of the interface. The average
746 > temperature values reported are for the entire system, and not for the
747 > liquid phase, so at a given $\langle T \rangle$, the system with
748 > positive $J_z$ has a warmer liquid phase.  This means that if the
749 > liquid carries thermal energy via convective transport, {\it positive}
750 > $J_z$ values will result in increased molecular motion on the liquid
751 > side of the interface, and this will increase the measured
752 > conductivity.
753  
754 + \subsubsection{Effects due to average temperature}
755 +
756 + We also studied the effect of average system temperature on the
757 + interfacial conductance.  The simulations are first equilibrated in
758 + the NPT ensemble at 1 atm.  The TraPPE-UA model for hexane tends to
759 + predict a lower boiling point (and liquid state density) than
760 + experiments.  This lower-density liquid phase leads to reduced contact
761 + between the hexane and butanethiol, and this accounts for our
762 + observation of lower conductance at higher temperatures as shown in
763 + Table \ref{AuThiolHexaneUA}.  In raising the average temperature from
764 + 200K to 250K, the density drop of ~20\% in the solvent phase leads to
765 + a ~65\% drop in the conductance.
766 +
767 + Similar behavior is observed in the TraPPE-UA model for toluene,
768 + although this model has better agreement with the experimental
769 + densities of toluene.  The expansion of the toluene liquid phase is
770 + not as significant as that of the hexane (8.3\% over 100K), and this
771 + limits the effect to ~20\% drop in thermal conductivity  (Table
772 + \ref{AuThiolToluene}).
773 +
774 + Although we have not mapped out the behavior at a large number of
775 + temperatures, is clear that there will be a strong temperature
776 + dependence in the interfacial conductance when the physical properties
777 + of one side of the interface (notably the density) change rapidly as a
778 + function of temperature.
779 +
780 + \begin{table*}
781 +  \begin{minipage}{\linewidth}
782 +    \begin{center}
783 +      \caption{Computed interfacial thermal conductivity ($G$ and
784 +        $G^\prime$) values for a 90\% coverage Au-butanethiol/toluene
785 +        interface at different temperatures using a range of energy
786 +        fluxes. Error estimates indicated in parenthesis.}
787 +      
788 +      \begin{tabular}{ccccc}
789 +        \hline\hline
790 +        $\langle T\rangle$ & $\rho_{toluene}$ & $J_z$ & $G$ & $G^\prime$ \\
791 +        (K) & (g/cm$^3$) & (GW/m$^2$) & \multicolumn{2}{c}{(MW/m$^2$/K)} \\
792 +        \hline
793 +        200 & 0.933 &  2.15 & 204(12) & 113(12) \\
794 +            &       & -1.86 & 180(3)  & 135(21) \\
795 +            &       & -3.93 & 176(5)  & 113(12) \\
796 +        \hline
797 +        300 & 0.855 & -1.91 & 143(5)  & 125(2)  \\
798 +            &       & -4.19 & 135(9)  & 113(12) \\
799 +        \hline\hline
800 +      \end{tabular}
801 +      \label{AuThiolToluene}
802 +    \end{center}
803 +  \end{minipage}
804 + \end{table*}
805 +
806 + Besides the lower interfacial thermal conductance, surfaces at
807 + relatively high temperatures are susceptible to reconstructions,
808 + particularly when butanethiols fully cover the Au(111) surface. These
809 + reconstructions include surface Au atoms which migrate outward to the
810 + S atom layer, and butanethiol molecules which embed into the surface
811 + Au layer. The driving force for this behavior is the strong Au-S
812 + interactions which are modeled here with a deep Lennard-Jones
813 + potential. This phenomenon agrees with reconstructions that have beeen
814 + experimentally
815 + observed.\cite{doi:10.1021/j100035a033,doi:10.1021/la026493y}.  Vlugt
816 + {\it et al.} kept their Au(111) slab rigid so that their simulations
817 + could reach 300K without surface
818 + reconstructions.\cite{vlugt:cpc2007154} Since surface reconstructions
819 + blur the interface, the measurement of $G$ becomes more difficult to
820 + conduct at higher temperatures.  For this reason, most of our
821 + measurements are undertaken at $\langle T\rangle\sim$200K where
822 + reconstruction is minimized.
823 +
824 + However, when the surface is not completely covered by butanethiols,
825 + the simulated system appears to be more resistent to the
826 + reconstruction. O ur Au / butanethiol / toluene system had the Au(111)
827 + surfaces 90\% covered by butanethiols, but did not see this above
828 + phenomena even at $\langle T\rangle\sim$300K.  That said, we did
829 + observe butanethiols migrating to neighboring three-fold sites during
830 + a simulation.  Since the interface persisted in these simulations,
831 + were able to obtain $G$'s for these interfaces even at a relatively
832 + high temperature without being affected by surface reconstructions.
833 +
834 + \section{Discussion}
835 +
836 + The primary result of this work is that the capping agent acts as an
837 + efficient thermal coupler between solid and solvent phases.  One of
838 + the ways the capping agent can carry out this role is to down-shift
839 + between the phonon vibrations in the solid (which carry the heat from
840 + the gold) and the molecular vibrations in the liquid (which carry some
841 + of the heat in the solvent).
842 +
843 + To investigate the mechanism of interfacial thermal conductance, the
844 + vibrational power spectrum was computed. Power spectra were taken for
845 + individual components in different simulations. To obtain these
846 + spectra, simulations were run after equilibration in the
847 + microcanonical (NVE) ensemble and without a thermal
848 + gradient. Snapshots of configurations were collected at a frequency
849 + that is higher than that of the fastest vibrations occuring in the
850 + simulations. With these configurations, the velocity auto-correlation
851 + functions can be computed:
852 + \begin{equation}
853 + C_A (t) = \langle\vec{v}_A (t)\cdot\vec{v}_A (0)\rangle
854 + \label{vCorr}
855 + \end{equation}
856 + The power spectrum is constructed via a Fourier transform of the
857 + symmetrized velocity autocorrelation function,
858 + \begin{equation}
859 +  \hat{f}(\omega) =
860 +  \int_{-\infty}^{\infty} C_A (t) e^{-2\pi it\omega}\,dt
861 + \label{fourier}
862 + \end{equation}
863 +
864 + \subsection{The role of specific vibrations}
865 + The vibrational spectra for gold slabs in different environments are
866 + shown as in Figure \ref{specAu}. Regardless of the presence of
867 + solvent, the gold surfaces which are covered by butanethiol molecules
868 + exhibit an additional peak observed at a frequency of
869 + $\sim$165cm$^{-1}$.  We attribute this peak to the S-Au bonding
870 + vibration. This vibration enables efficient thermal coupling of the
871 + surface Au layer to the capping agents. Therefore, in our simulations,
872 + the Au / S interfaces do not appear to be the primary barrier to
873 + thermal transport when compared with the butanethiol / solvent
874 + interfaces.
875 +
876   \begin{figure}
877   \includegraphics[width=\linewidth]{vibration}
878 < \caption{Vibrational spectra obtained for gold in different
879 <  environments (upper panel) and for Au/thiol/hexane simulation in
880 <  all-atom model (lower panel).}
881 < \label{vibration}
878 > \caption{Vibrational power spectra for gold in different solvent
879 >  environments.  The presence of the butanethiol capping molecules
880 >  adds a vibrational peak at $\sim$165cm$^{-1}$. The butanethiol
881 >  spectra exhibit a corresponding peak.}
882 > \label{specAu}
883   \end{figure}
398 % 600dpi, letter size. too large?
884  
885 + Also in this figure, we show the vibrational power spectrum for the
886 + bound butanethiol molecules, which also exhibits the same
887 + $\sim$165cm$^{-1}$ peak.
888  
889 + \subsection{Overlap of power spectra}
890 + A comparison of the results obtained from the two different organic
891 + solvents can also provide useful information of the interfacial
892 + thermal transport process.  In particular, the vibrational overlap
893 + between the butanethiol and the organic solvents suggests a highly
894 + efficient thermal exchange between these components.  Very high
895 + thermal conductivity was observed when AA models were used and C-H
896 + vibrations were treated classically.  The presence of extra degrees of
897 + freedom in the AA force field yields higher heat exchange rates
898 + between the two phases and results in a much higher conductivity than
899 + in the UA force field.
900 +
901 + The similarity in the vibrational modes available to solvent and
902 + capping agent can be reduced by deuterating one of the two components
903 + (Fig. \ref{aahxntln}).  Once either the hexanes or the butanethiols
904 + are deuterated, one can observe a significantly lower $G$ and
905 + $G^\prime$ values (Table \ref{modelTest}).
906 +
907 + \begin{figure}
908 + \includegraphics[width=\linewidth]{aahxntln}
909 + \caption{Spectra obtained for all-atom (AA) Au / butanethiol / solvent
910 +  systems. When butanethiol is deuterated (lower left), its
911 +  vibrational overlap with hexane decreases significantly.  Since
912 +  aromatic molecules and the butanethiol are vibrationally dissimilar,
913 +  the change is not as dramatic when toluene is the solvent (right).}
914 + \label{aahxntln}
915 + \end{figure}
916 +
917 + For the Au / butanethiol / toluene interfaces, having the AA
918 + butanethiol deuterated did not yield a significant change in the
919 + measured conductance. Compared to the C-H vibrational overlap between
920 + hexane and butanethiol, both of which have alkyl chains, the overlap
921 + between toluene and butanethiol is not as significant and thus does
922 + not contribute as much to the heat exchange process.
923 +
924 + Previous observations of Zhang {\it et al.}\cite{hase:2010} indicate
925 + that the {\it intra}molecular heat transport due to alkylthiols is
926 + highly efficient.  Combining our observations with those of Zhang {\it
927 +  et al.}, it appears that butanethiol acts as a channel to expedite
928 + heat flow from the gold surface and into the alkyl chain.  The
929 + acoustic impedance mismatch between the metal and the liquid phase can
930 + therefore be effectively reduced with the presence of suitable capping
931 + agents.
932 +
933 + Deuterated models in the UA force field did not decouple the thermal
934 + transport as well as in the AA force field.  The UA models, even
935 + though they have eliminated the high frequency C-H vibrational
936 + overlap, still have significant overlap in the lower-frequency
937 + portions of the infrared spectra (Figure \ref{uahxnua}).  Deuterating
938 + the UA models did not decouple the low frequency region enough to
939 + produce an observable difference for the results of $G$ (Table
940 + \ref{modelTest}).
941 +
942 + \begin{figure}
943 + \includegraphics[width=\linewidth]{uahxnua}
944 + \caption{Vibrational spectra obtained for normal (upper) and
945 +  deuterated (lower) hexane in Au-butanethiol/hexane
946 +  systems. Butanethiol spectra are shown as reference. Both hexane and
947 +  butanethiol were using United-Atom models.}
948 + \label{uahxnua}
949 + \end{figure}
950 +
951 + \section{Conclusions}
952 + The NIVS algorithm has been applied to simulations of
953 + butanethiol-capped Au(111) surfaces in the presence of organic
954 + solvents. This algorithm allows the application of unphysical thermal
955 + flux to transfer heat between the metal and the liquid phase. With the
956 + flux applied, we were able to measure the corresponding thermal
957 + gradients and to obtain interfacial thermal conductivities. Under
958 + steady states, 2-3 ns trajectory simulations are sufficient for
959 + computation of this quantity.
960 +
961 + Our simulations have seen significant conductance enhancement in the
962 + presence of capping agent, compared with the bare gold / liquid
963 + interfaces. The acoustic impedance mismatch between the metal and the
964 + liquid phase is effectively eliminated by a chemically-bonded capping
965 + agent. Furthermore, the coverage precentage of the capping agent plays
966 + an important role in the interfacial thermal transport
967 + process. Moderately low coverages allow higher contact between capping
968 + agent and solvent, and thus could further enhance the heat transfer
969 + process, giving a non-monotonic behavior of conductance with
970 + increasing coverage.
971 +
972 + Our results, particularly using the UA models, agree well with
973 + available experimental data.  The AA models tend to overestimate the
974 + interfacial thermal conductance in that the classically treated C-H
975 + vibrations become too easily populated. Compared to the AA models, the
976 + UA models have higher computational efficiency with satisfactory
977 + accuracy, and thus are preferable in modeling interfacial thermal
978 + transport.
979 +
980 + Of the two definitions for $G$, the discrete form
981 + (Eq. \ref{discreteG}) was easier to use and gives out relatively
982 + consistent results, while the derivative form (Eq. \ref{derivativeG})
983 + is not as versatile. Although $G^\prime$ gives out comparable results
984 + and follows similar trend with $G$ when measuring close to fully
985 + covered or bare surfaces, the spatial resolution of $T$ profile
986 + required for the use of a derivative form is limited by the number of
987 + bins and the sampling required to obtain thermal gradient information.
988 +
989 + Vlugt {\it et al.} have investigated the surface thiol structures for
990 + nanocrystalline gold and pointed out that they differ from those of
991 + the Au(111) surface.\cite{landman:1998,vlugt:cpc2007154} This
992 + difference could also cause differences in the interfacial thermal
993 + transport behavior. To investigate this problem, one would need an
994 + effective method for applying thermal gradients in non-planar
995 + (i.e. spherical) geometries.
996 +
997   \section{Acknowledgments}
998   Support for this project was provided by the National Science
999   Foundation under grant CHE-0848243. Computational time was provided by
1000   the Center for Research Computing (CRC) at the University of Notre
1001 < Dame.  \newpage
1001 > Dame.
1002 > \newpage
1003  
1004   \bibliography{interfacial}
1005  

Diff Legend

Removed lines
+ Added lines
< Changed lines
> Changed lines