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28
29 \begin{document}
30
31 \title{Simulating interfacial thermal conductance at metal-solvent
32 interfaces: the role of chemical capping agents}
33
34 \author{Shenyu Kuang and J. Daniel
35 Gezelter\footnote{Corresponding author. \ Electronic mail: gezelter@nd.edu} \\
36 Department of Chemistry and Biochemistry,\\
37 University of Notre Dame\\
38 Notre Dame, Indiana 46556}
39
40 \date{\today}
41
42 \maketitle
43
44 \begin{doublespace}
45
46 \begin{abstract}
47
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
67 \newpage
68
69 %\narrowtext
70
71 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
72 % BODY OF TEXT
73 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
74
75 \section{Introduction}
76 Interfacial thermal conductance is extensively studied both
77 experimentally and computationally, due to its importance in nanoscale
78 science and technology. Reliability of nanoscale devices depends on
79 their thermal transport properties. Unlike bulk homogeneous materials,
80 nanoscale materials features significant presence of interfaces, and
81 these interfaces could dominate the heat transfer behavior of these
82 materials. Furthermore, these materials are generally heterogeneous,
83 which challenges traditional research methods for homogeneous systems.
84
85 Heat conductance of molecular and nano-scale interfaces will be
86 affected by the chemical details of the surface. Experimentally,
87 various interfaces have been investigated for their thermal
88 conductance properties. Wang {\it et al.} studied heat transport
89 through long-chain hydrocarbon monolayers on gold substrate at
90 individual molecular level\cite{Wang10082007}; Schmidt {\it et al.}
91 studied the role of CTAB on thermal transport between gold nanorods
92 and solvent\cite{doi:10.1021/jp8051888}; Juv\'e {\it et al.} studied
93 the cooling dynamics, which is controlled by thermal interface
94 resistence of glass-embedded metal
95 nanoparticles\cite{PhysRevB.80.195406}. Although interfaces are
96 commonly barriers for heat transport, Alper {\it et al.} suggested
97 that specific ligands (capping agents) could completely eliminate this
98 barrier ($G\rightarrow\infty$)\cite{doi:10.1021/la904855s}.
99
100 Theoretical and computational studies were also engaged in the
101 interfacial thermal transport research in order to gain an
102 understanding of this phenomena at the molecular level. Hase and
103 coworkers employed Non-Equilibrium Molecular Dynamics (NEMD)
104 simulations to study thermal transport from hot Au(111) substrate to a
105 self-assembled monolayer of alkylthiolate with relatively long chain
106 (8-20 carbon atoms)\cite{hase:2010,hase:2011}. However,
107 emsemble average measurements for heat conductance of interfaces
108 between the capping monolayer on Au and a solvent phase has yet to be
109 studied. The relatively low thermal flux through interfaces is
110 difficult to measure with Equilibrium MD or forward NEMD simulation
111 methods. Therefore, the Reverse NEMD (RNEMD) methods would have the
112 advantage of having this difficult to measure flux known when studying
113 the thermal transport across interfaces, given that the simulation
114 methods being able to effectively apply an unphysical flux in
115 non-homogeneous systems.
116
117 Recently, we have developed the Non-Isotropic Velocity Scaling (NIVS)
118 algorithm for RNEMD simulations\cite{kuang:164101}. This algorithm
119 retains the desirable features of RNEMD (conservation of linear
120 momentum and total energy, compatibility with periodic boundary
121 conditions) while establishing true thermal distributions in each of
122 the two slabs. Furthermore, it allows more effective thermal exchange
123 between particles of different identities, and thus enables extensive
124 study of interfacial conductance under steady states.
125
126 Our work presented here investigated the Au(111) surface with various
127 coverage of butanethiol, a capping agent with shorter carbon chain,
128 solvated with organic solvents of different molecular shapes. And
129 different models were used for both the capping agent and the solvent
130 force field parameters. With the NIVS algorithm applied, the thermal
131 transport through these interfacial systems was studied and the
132 underlying mechanism for this phenomena was investigated.
133
134 [WHY STUDY AU-THIOL SURFACE; MAY CITE SHAOYI JIANG]
135
136 \section{Methodology}
137 \subsection{Algorithm}
138 [BACKGROUND FOR MD METHODS]
139 There have been many algorithms for computing thermal conductivity
140 using molecular dynamics simulations. However, interfacial conductance
141 is at least an order of magnitude smaller. This would make the
142 calculation even more difficult for those slowly-converging
143 equilibrium methods. Imposed-flux non-equilibrium
144 methods\cite{MullerPlathe:1997xw} have the flux set {\it a priori} and
145 the response of temperature or momentum gradients are easier to
146 measure than the flux, if unknown, and thus, is a preferable way to
147 the forward NEMD methods. Although the momentum swapping approach for
148 flux-imposing can be used for exchanging energy between particles of
149 different identity, the kinetic energy transfer efficiency is affected
150 by the mass difference between the particles, which limits its
151 application on heterogeneous interfacial systems.
152
153 The non-isotropic velocity scaling (NIVS)\cite{kuang:164101} approach in
154 non-equilibrium MD simulations is able to impose relatively large
155 kinetic energy flux without obvious perturbation to the velocity
156 distribution of the simulated systems. Furthermore, this approach has
157 the advantage in heterogeneous interfaces in that kinetic energy flux
158 can be applied between regions of particles of arbitary identity, and
159 the flux quantity is not restricted by particle mass difference.
160
161 The NIVS algorithm scales the velocity vectors in two separate regions
162 of a simulation system with respective diagonal scaling matricies. To
163 determine these scaling factors in the matricies, a set of equations
164 including linear momentum conservation and kinetic energy conservation
165 constraints and target momentum / energy flux satisfaction is
166 solved. With the scaling operation applied to the system in a set
167 frequency, corresponding momentum / temperature gradients can be
168 built, which can be used for computing transport properties and other
169 applications related to momentum / temperature gradients. The NIVS
170 algorithm conserves momenta and energy and does not depend on an
171 external thermostat.
172
173 \subsection{Defining Interfacial Thermal Conductivity $G$}
174 For interfaces with a relatively low interfacial conductance, the bulk
175 regions on either side of an interface rapidly come to a state in
176 which the two phases have relatively homogeneous (but distinct)
177 temperatures. The interfacial thermal conductivity $G$ can therefore
178 be approximated as:
179 \begin{equation}
180 G = \frac{E_{total}}{2 t L_x L_y \left( \langle T_\mathrm{hot}\rangle -
181 \langle T_\mathrm{cold}\rangle \right)}
182 \label{lowG}
183 \end{equation}
184 where ${E_{total}}$ is the imposed non-physical kinetic energy
185 transfer and ${\langle T_\mathrm{hot}\rangle}$ and ${\langle
186 T_\mathrm{cold}\rangle}$ are the average observed temperature of the
187 two separated phases.
188
189 When the interfacial conductance is {\it not} small, two ways can be
190 used to define $G$.
191
192 One way is to assume the temperature is discretely different on two
193 sides of the interface, $G$ can be calculated with the thermal flux
194 applied $J$ and the maximum temperature difference measured along the
195 thermal gradient max($\Delta T$), which occurs at the interface, as:
196 \begin{equation}
197 G=\frac{J}{\Delta T}
198 \label{discreteG}
199 \end{equation}
200
201 The other approach is to assume a continuous temperature profile along
202 the thermal gradient axis (e.g. $z$) and define $G$ at the point where
203 the magnitude of thermal conductivity $\lambda$ change reach its
204 maximum, given that $\lambda$ is well-defined throughout the space:
205 \begin{equation}
206 G^\prime = \Big|\frac{\partial\lambda}{\partial z}\Big|
207 = \Big|\frac{\partial}{\partial z}\left(-J_z\Big/
208 \left(\frac{\partial T}{\partial z}\right)\right)\Big|
209 = |J_z|\Big|\frac{\partial^2 T}{\partial z^2}\Big|
210 \Big/\left(\frac{\partial T}{\partial z}\right)^2
211 \label{derivativeG}
212 \end{equation}
213
214 With the temperature profile obtained from simulations, one is able to
215 approximate the first and second derivatives of $T$ with finite
216 difference method and thus calculate $G^\prime$.
217
218 In what follows, both definitions are used for calculation and comparison.
219
220 [IMPOSE G DEFINITION INTO OUR SYSTEMS]
221 To facilitate the use of the above definitions in calculating $G$ and
222 $G^\prime$, we have a metal slab with its (111) surfaces perpendicular
223 to the $z$-axis of our simulation cells. With or withour capping
224 agents on the surfaces, the metal slab is solvated with organic
225 solvents, as illustrated in Figure \ref{demoPic}.
226
227 \begin{figure}
228 \includegraphics[width=\linewidth]{demoPic}
229 \caption{A sample showing how a metal slab has its (111) surface
230 covered by capping agent molecules and solvated by hexane.}
231 \label{demoPic}
232 \end{figure}
233
234 With a simulation cell setup following the above manner, one is able
235 to equilibrate the system and impose an unphysical thermal flux
236 between the liquid and the metal phase with the NIVS algorithm. Under
237 a stablized thermal gradient induced by periodically applying the
238 unphysical flux, one is able to obtain a temperature profile and the
239 physical thermal flux corresponding to it, which equals to the
240 unphysical flux applied by NIVS. These data enables the evaluation of
241 the interfacial thermal conductance of a surface. Figure \ref{gradT}
242 is an example how those stablized thermal gradient can be used to
243 obtain the 1st and 2nd derivatives of the temperature profile.
244
245 \begin{figure}
246 \includegraphics[width=\linewidth]{gradT}
247 \caption{The 1st and 2nd derivatives of temperature profile can be
248 obtained with finite difference approximation.}
249 \label{gradT}
250 \end{figure}
251
252 [MAY INCLUDE POWER SPECTRUM PROTOCOL]
253
254 \section{Computational Details}
255 \subsection{Simulation Protocol}
256 Our MD simulation code, OpenMD\cite{Meineke:2005gd,openmd}, has the
257 NIVS algorithm integrated and was used for our simulations. In our
258 simulations, Au is used to construct a metal slab with bare (111)
259 surface perpendicular to the $z$-axis. Different slab thickness (layer
260 numbers of Au) are simulated. This metal slab is first equilibrated
261 under normal pressure (1 atm) and a desired temperature. After
262 equilibration, butanethiol is used as the capping agent molecule to
263 cover the bare Au (111) surfaces evenly. The sulfur atoms in the
264 butanethiol molecules would occupy the three-fold sites of the
265 surfaces, and the maximal butanethiol capacity on Au surface is $1/3$
266 of the total number of surface Au atoms[CITATIONs]. A series of
267 different coverage surfaces is investigated in order to study the
268 relation between coverage and conductance.
269
270 [COVERAGE DISCRIPTION]
271 In the initial configurations for each coverage precentage,
272 butanethiols were distributed evenly on the Au(111) surfaces. However,
273 since the interaction descriptions between surface Au and butanethiol
274 is non-bonded in our simulations, the capping agent molecules are
275 allowed to migrate to an empty neighbor three-fold site during a
276 simulation. Therefore, the initial configuration would not severely
277 affect the sampling of a variety of configurations of the same
278 coverage, and the final conductance measurement would be an average
279 effect of these configurations explored in the simulations. [MAY NEED FIGURES]
280
281 After the modified Au-butanethiol surface systems are equilibrated
282 under canonical ensemble, organic solvent molecules are packed in the
283 previously vacuum part of the simulation cells and guarantees that
284 short range repulsive interactions do not disrupt the
285 simulations\cite{packmol}. Two solvents are investigated, one which
286 has little vibrational overlap with the alkanethiol and plane-like
287 shape (toluene), and one which has similar vibrational frequencies and
288 chain-like shape ({\it n}-hexane). [MAY EXPLAIN WHY WE CHOOSE THEM]
289
290 The spacing filled by solvent molecules, i.e. the gap between
291 periodically repeated Au-butanethiol surfaces should be carefully
292 chosen. A very long length scale for the thermal gradient axis ($z$)
293 may cause excessively hot or cold temperatures in the middle of the
294 solvent region and lead to undesired phenomena such as solvent boiling
295 or freezing when a thermal flux is applied. Conversely, too few
296 solvent molecules would change the normal behavior of the liquid
297 phase. Therefore, our $N_{solvent}$ values were chosen to ensure that
298 these extreme cases did not happen to our simulations. And the
299 corresponding spacing is usually $35 \sim 60$\AA.
300
301 The initial configurations generated by Packmol are further
302 equilibrated with the $x$ and $y$ dimensions fixed, only allowing
303 length scale change in $z$ dimension. This is to ensure that the
304 equilibration of liquid phase does not affect the metal crystal
305 structure in $x$ and $y$ dimensions. Further equilibration are run
306 under NVT and then NVE ensembles.
307
308 After the systems reach equilibrium, NIVS is implemented to impose a
309 periodic unphysical thermal flux between the metal and the liquid
310 phase. Most of our simulations are under an average temperature of
311 $\sim$200K. Therefore, this flux usually comes from the metal to the
312 liquid so that the liquid has a higher temperature and would not
313 freeze due to excessively low temperature. This induced temperature
314 gradient is stablized and the simulation cell is devided evenly into
315 N slabs along the $z$-axis and the temperatures of each slab are
316 recorded. When the slab width $d$ of each slab is the same, the
317 derivatives of $T$ with respect to slab number $n$ can be directly
318 used for $G^\prime$ calculations:
319 \begin{equation}
320 G^\prime = |J_z|\Big|\frac{\partial^2 T}{\partial z^2}\Big|
321 \Big/\left(\frac{\partial T}{\partial z}\right)^2
322 = |J_z|\Big|\frac{1}{d^2}\frac{\partial^2 T}{\partial n^2}\Big|
323 \Big/\left(\frac{1}{d}\frac{\partial T}{\partial n}\right)^2
324 = |J_z|\Big|\frac{\partial^2 T}{\partial n^2}\Big|
325 \Big/\left(\frac{\partial T}{\partial n}\right)^2
326 \label{derivativeG2}
327 \end{equation}
328
329 \subsection{Force Field Parameters}
330 Our simulations include various components. Therefore, force field
331 parameter descriptions are needed for interactions both between the
332 same type of particles and between particles of different species.
333
334 The Au-Au interactions in metal lattice slab is described by the
335 quantum Sutton-Chen (QSC) formulation\cite{PhysRevB.59.3527}. The QSC
336 potentials include zero-point quantum corrections and are
337 reparametrized for accurate surface energies compared to the
338 Sutton-Chen potentials\cite{Chen90}.
339
340 Figure \ref{demoMol} demonstrates how we name our pseudo-atoms of the
341 organic solvent molecules in our simulations.
342
343 \begin{figure}
344 \includegraphics[width=\linewidth]{demoMol}
345 \caption{Denomination of atoms or pseudo-atoms in our simulations: a)
346 UA-hexane; b) AA-hexane; c) UA-toluene; d) AA-toluene.}
347 \label{demoMol}
348 \end{figure}
349
350 For both solvent molecules, straight chain {\it n}-hexane and aromatic
351 toluene, United-Atom (UA) and All-Atom (AA) models are used
352 respectively. The TraPPE-UA
353 parameters\cite{TraPPE-UA.alkanes,TraPPE-UA.alkylbenzenes} are used
354 for our UA solvent molecules. In these models, pseudo-atoms are
355 located at the carbon centers for alkyl groups. By eliminating
356 explicit hydrogen atoms, these models are simple and computationally
357 efficient, while maintains good accuracy. However, the TraPPE-UA for
358 alkanes is known to predict a lower boiling point than experimental
359 values. Considering that after an unphysical thermal flux is applied
360 to a system, the temperature of ``hot'' area in the liquid phase would be
361 significantly higher than the average, to prevent over heating and
362 boiling of the liquid phase, the average temperature in our
363 simulations should be much lower than the liquid boiling point. [MORE DISCUSSION]
364 For UA-toluene model, rigid body constraints are applied, so that the
365 benzene ring and the methyl-CRar bond are kept rigid. This would save
366 computational time.[MORE DETAILS]
367
368 Besides the TraPPE-UA models, AA models for both organic solvents are
369 included in our studies as well. For hexane, the OPLS-AA\cite{OPLSAA}
370 force field is used. [MORE DETAILS]
371 For toluene, the United Force Field developed by Rapp\'{e} {\it et
372 al.}\cite{doi:10.1021/ja00051a040} is adopted.[MORE DETAILS]
373
374 The capping agent in our simulations, the butanethiol molecules can
375 either use UA or AA model. The TraPPE-UA force fields includes
376 parameters for thiol molecules\cite{TraPPE-UA.thiols} and are used for
377 UA butanethiol model in our simulations. The OPLS-AA also provides
378 parameters for alkyl thiols. However, alkyl thiols adsorbed on Au(111)
379 surfaces do not have the hydrogen atom bonded to sulfur. To adapt this
380 change and derive suitable parameters for butanethiol adsorbed on
381 Au(111) surfaces, we adopt the S parameters from Luedtke and
382 Landman\cite{landman:1998} and modify parameters for its neighbor C
383 atom for charge balance in the molecule. Note that the model choice
384 (UA or AA) of capping agent can be different from the
385 solvent. Regardless of model choice, the force field parameters for
386 interactions between capping agent and solvent can be derived using
387 Lorentz-Berthelot Mixing Rule:[EQN'S]
388
389
390 To describe the interactions between metal Au and non-metal capping
391 agent and solvent particles, we refer to an adsorption study of alkyl
392 thiols on gold surfaces by Vlugt {\it et
393 al.}\cite{vlugt:cpc2007154} They fitted an effective Lennard-Jones
394 form of potential parameters for the interaction between Au and
395 pseudo-atoms CH$_x$ and S based on a well-established and widely-used
396 effective potential of Hautman and Klein\cite{hautman:4994} for the
397 Au(111) surface. As our simulations require the gold lattice slab to
398 be non-rigid so that it could accommodate kinetic energy for thermal
399 transport study purpose, the pair-wise form of potentials is
400 preferred.
401
402 Besides, the potentials developed from {\it ab initio} calculations by
403 Leng {\it et al.}\cite{doi:10.1021/jp034405s} are adopted for the
404 interactions between Au and aromatic C/H atoms in toluene.[MORE DETAILS]
405
406 However, the Lennard-Jones parameters between Au and other types of
407 particles in our simulations are not yet well-established. For these
408 interactions, we attempt to derive their parameters using the Mixing
409 Rule. To do this, the ``Metal-non-Metal'' (MnM) interaction parameters
410 for Au is first extracted from the Au-CH$_x$ parameters by applying
411 the Mixing Rule reversely. Table \ref{MnM} summarizes these ``MnM''
412 parameters in our simulations.
413
414 \begin{table*}
415 \begin{minipage}{\linewidth}
416 \begin{center}
417 \caption{Lennard-Jones parameters for Au-non-Metal
418 interactions in our simulations.}
419
420 \begin{tabular}{ccc}
421 \hline\hline
422 Non-metal atom & $\sigma$ & $\epsilon$ \\
423 (or pseudo-atom) & \AA & kcal/mol \\
424 \hline
425 S & 2.40 & 8.465 \\
426 CH3 & 3.54 & 0.2146 \\
427 CH2 & 3.54 & 0.1749 \\
428 CT3 & 3.365 & 0.1373 \\
429 CT2 & 3.365 & 0.1373 \\
430 CTT & 3.365 & 0.1373 \\
431 HC & 2.865 & 0.09256 \\
432 CHar & 3.4625 & 0.1680 \\
433 CRar & 3.555 & 0.1604 \\
434 CA & 3.173 & 0.0640 \\
435 HA & 2.746 & 0.0414 \\
436 \hline\hline
437 \end{tabular}
438 \label{MnM}
439 \end{center}
440 \end{minipage}
441 \end{table*}
442
443
444 \section{Results and Discussions}
445 [MAY HAVE A BRIEF SUMMARY]
446 \subsection{How Simulation Parameters Affects $G$}
447 [MAY NOT PUT AT FIRST]
448 We have varied our protocol or other parameters of the simulations in
449 order to investigate how these factors would affect the measurement of
450 $G$'s. It turned out that while some of these parameters would not
451 affect the results substantially, some other changes to the
452 simulations would have a significant impact on the measurement
453 results.
454
455 In some of our simulations, we allowed $L_x$ and $L_y$ to change
456 during equilibrating the liquid phase. Due to the stiffness of the Au
457 slab, $L_x$ and $L_y$ would not change noticeably after
458 equilibration. Although $L_z$ could fluctuate $\sim$1\% after a system
459 is fully equilibrated in the NPT ensemble, this fluctuation, as well
460 as those comparably smaller to $L_x$ and $L_y$, would not be magnified
461 on the calculated $G$'s, as shown in Table \ref{AuThiolHexaneUA}. This
462 insensivity to $L_i$ fluctuations allows reliable measurement of $G$'s
463 without the necessity of extremely cautious equilibration process.
464
465 As stated in our computational details, the spacing filled with
466 solvent molecules can be chosen within a range. This allows some
467 change of solvent molecule numbers for the same Au-butanethiol
468 surfaces. We did this study on our Au-butanethiol/hexane
469 simulations. Nevertheless, the results obtained from systems of
470 different $N_{hexane}$ did not indicate that the measurement of $G$ is
471 susceptible to this parameter. For computational efficiency concern,
472 smaller system size would be preferable, given that the liquid phase
473 structure is not affected.
474
475 Our NIVS algorithm allows change of unphysical thermal flux both in
476 direction and in quantity. This feature extends our investigation of
477 interfacial thermal conductance. However, the magnitude of this
478 thermal flux is not arbitary if one aims to obtain a stable and
479 reliable thermal gradient. A temperature profile would be
480 substantially affected by noise when $|J_z|$ has a much too low
481 magnitude; while an excessively large $|J_z|$ that overwhelms the
482 conductance capacity of the interface would prevent a thermal gradient
483 to reach a stablized steady state. NIVS has the advantage of allowing
484 $J$ to vary in a wide range such that the optimal flux range for $G$
485 measurement can generally be simulated by the algorithm. Within the
486 optimal range, we were able to study how $G$ would change according to
487 the thermal flux across the interface. For our simulations, we denote
488 $J_z$ to be positive when the physical thermal flux is from the liquid
489 to metal, and negative vice versa. The $G$'s measured under different
490 $J_z$ is listed in Table \ref{AuThiolHexaneUA} and [REF]. These
491 results do not suggest that $G$ is dependent on $J_z$ within this flux
492 range. The linear response of flux to thermal gradient simplifies our
493 investigations in that we can rely on $G$ measurement with only a
494 couple $J_z$'s and do not need to test a large series of fluxes.
495
496 %ADD MORE TO TABLE
497 \begin{table*}
498 \begin{minipage}{\linewidth}
499 \begin{center}
500 \caption{Computed interfacial thermal conductivity ($G$ and
501 $G^\prime$) values for the 100\% covered Au-butanethiol/hexane
502 interfaces with UA model and different hexane molecule numbers
503 at different temperatures using a range of energy fluxes.}
504
505 \begin{tabular}{cccccccc}
506 \hline\hline
507 $\langle T\rangle$ & & $L_x$ & $L_y$ & $L_z$ & $J_z$ &
508 $G$ & $G^\prime$ \\
509 (K) & $N_{hexane}$ & \multicolumn{3}{c}{(\AA)} & (GW/m$^2$) &
510 \multicolumn{2}{c}{(MW/m$^2$/K)} \\
511 \hline
512 200 & 266 & 29.86 & 25.80 & 113.1 & -0.96 &
513 102() & 80.0() \\
514 & 200 & 29.84 & 25.81 & 93.9 & 1.92 &
515 129() & 87.3() \\
516 & & 29.84 & 25.81 & 95.3 & 1.93 &
517 131() & 77.5() \\
518 & 166 & 29.84 & 25.81 & 85.7 & 0.97 &
519 115() & 69.3() \\
520 & & & & & 1.94 &
521 125() & 87.1() \\
522 250 & 200 & 29.84 & 25.87 & 106.8 & 0.96 &
523 81.8() & 67.0() \\
524 & 166 & 29.87 & 25.84 & 94.8 & 0.98 &
525 79.0() & 62.9() \\
526 & & 29.84 & 25.85 & 95.0 & 1.44 &
527 76.2() & 64.8() \\
528 \hline\hline
529 \end{tabular}
530 \label{AuThiolHexaneUA}
531 \end{center}
532 \end{minipage}
533 \end{table*}
534
535 Furthermore, we also attempted to increase system average temperatures
536 to above 200K. These simulations are first equilibrated in the NPT
537 ensemble under normal pressure. As stated above, the TraPPE-UA model
538 for hexane tends to predict a lower boiling point. In our simulations,
539 hexane had diffculty to remain in liquid phase when NPT equilibration
540 temperature is higher than 250K. Additionally, the equilibrated liquid
541 hexane density under 250K becomes lower than experimental value. This
542 expanded liquid phase leads to lower contact between hexane and
543 butanethiol as well.[MAY NEED FIGURE] And this reduced contact would
544 probably be accountable for a lower interfacial thermal conductance,
545 as shown in Table \ref{AuThiolHexaneUA}.
546
547 A similar study for TraPPE-UA toluene agrees with the above result as
548 well. Having a higher boiling point, toluene tends to remain liquid in
549 our simulations even equilibrated under 300K in NPT
550 ensembles. Furthermore, the expansion of the toluene liquid phase is
551 not as significant as that of the hexane. This prevents severe
552 decrease of liquid-capping agent contact and the results (Table
553 \ref{AuThiolToluene}) show only a slightly decreased interface
554 conductance. Therefore, solvent-capping agent contact should play an
555 important role in the thermal transport process across the interface
556 in that higher degree of contact could yield increased conductance.
557
558 [ADD Lxyz AND ERROR ESTIMATE TO TABLE]
559 \begin{table*}
560 \begin{minipage}{\linewidth}
561 \begin{center}
562 \caption{Computed interfacial thermal conductivity ($G$ and
563 $G^\prime$) values for a 90\% coverage Au-butanethiol/toluene
564 interface at different temperatures using a range of energy
565 fluxes.}
566
567 \begin{tabular}{cccc}
568 \hline\hline
569 $\langle T\rangle$ & $J_z$ & $G$ & $G^\prime$ \\
570 (K) & (GW/m$^2$) & \multicolumn{2}{c}{(MW/m$^2$/K)} \\
571 \hline
572 200 & -1.86 & 180() & 135() \\
573 & 2.15 & 204() & 113() \\
574 & -3.93 & 175() & 114() \\
575 300 & -1.91 & 143() & 125() \\
576 & -4.19 & 134() & 113() \\
577 \hline\hline
578 \end{tabular}
579 \label{AuThiolToluene}
580 \end{center}
581 \end{minipage}
582 \end{table*}
583
584 Besides lower interfacial thermal conductance, surfaces in relatively
585 high temperatures are susceptible to reconstructions, when
586 butanethiols have a full coverage on the Au(111) surface. These
587 reconstructions include surface Au atoms migrated outward to the S
588 atom layer, and butanethiol molecules embedded into the original
589 surface Au layer. The driving force for this behavior is the strong
590 Au-S interactions in our simulations. And these reconstructions lead
591 to higher ratio of Au-S attraction and thus is energetically
592 favorable. Furthermore, this phenomenon agrees with experimental
593 results\cite{doi:10.1021/j100035a033,doi:10.1021/la026493y}. Vlugt
594 {\it et al.} had kept their Au(111) slab rigid so that their
595 simulations can reach 300K without surface reconstructions. Without
596 this practice, simulating 100\% thiol covered interfaces under higher
597 temperatures could hardly avoid surface reconstructions. However, our
598 measurement is based on assuming homogeneity on $x$ and $y$ dimensions
599 so that measurement of $T$ at particular $z$ would be an effective
600 average of the particles of the same type. Since surface
601 reconstructions could eliminate the original $x$ and $y$ dimensional
602 homogeneity, measurement of $G$ is more difficult to conduct under
603 higher temperatures. Therefore, most of our measurements are
604 undertaken at $\langle T\rangle\sim$200K.
605
606 However, when the surface is not completely covered by butanethiols,
607 the simulated system is more resistent to the reconstruction
608 above. Our Au-butanethiol/toluene system did not see this phenomena
609 even at $\langle T\rangle\sim$300K. The Au(111) surfaces have a 90\% coverage of
610 butanethiols and have empty three-fold sites. These empty sites could
611 help prevent surface reconstruction in that they provide other means
612 of capping agent relaxation. It is observed that butanethiols can
613 migrate to their neighbor empty sites during a simulation. Therefore,
614 we were able to obtain $G$'s for these interfaces even at a relatively
615 high temperature without being affected by surface reconstructions.
616
617 \subsection{Influence of Capping Agent Coverage on $G$}
618 To investigate the influence of butanethiol coverage on interfacial
619 thermal conductance, a series of different coverage Au-butanethiol
620 surfaces is prepared and solvated with various organic
621 molecules. These systems are then equilibrated and their interfacial
622 thermal conductivity are measured with our NIVS algorithm. Table
623 \ref{tlnUhxnUhxnD} lists these results for direct comparison between
624 different coverages of butanethiol. To study the isotope effect in
625 interfacial thermal conductance, deuterated UA-hexane is included as
626 well.
627
628 It turned out that with partial covered butanethiol on the Au(111)
629 surface, the derivative definition for $G$ (Eq. \ref{derivativeG}) has
630 difficulty to apply, due to the difficulty in locating the maximum of
631 change of $\lambda$. Instead, the discrete definition
632 (Eq. \ref{discreteG}) is easier to apply, as max($\Delta T$) can still
633 be well-defined. Therefore, $G$'s (not $G^\prime$) are used for this
634 section.
635
636 From Table \ref{tlnUhxnUhxnD}, one can see the significance of the
637 presence of capping agents. Even when a fraction of the Au(111)
638 surface sites are covered with butanethiols, the conductivity would
639 see an enhancement by at least a factor of 3. This indicates the
640 important role cappping agent is playing for thermal transport
641 phenomena on metal/organic solvent surfaces.
642
643 Interestingly, as one could observe from our results, the maximum
644 conductance enhancement (largest $G$) happens while the surfaces are
645 about 75\% covered with butanethiols. This again indicates that
646 solvent-capping agent contact has an important role of the thermal
647 transport process. Slightly lower butanethiol coverage allows small
648 gaps between butanethiols to form. And these gaps could be filled with
649 solvent molecules, which acts like ``heat conductors'' on the
650 surface. The higher degree of interaction between these solvent
651 molecules and capping agents increases the enhancement effect and thus
652 produces a higher $G$ than densely packed butanethiol arrays. However,
653 once this maximum conductance enhancement is reached, $G$ decreases
654 when butanethiol coverage continues to decrease. Each capping agent
655 molecule reaches its maximum capacity for thermal
656 conductance. Therefore, even higher solvent-capping agent contact
657 would not offset this effect. Eventually, when butanethiol coverage
658 continues to decrease, solvent-capping agent contact actually
659 decreases with the disappearing of butanethiol molecules. In this
660 case, $G$ decrease could not be offset but instead accelerated.
661
662 A comparison of the results obtained from differenet organic solvents
663 can also provide useful information of the interfacial thermal
664 transport process. The deuterated hexane (UA) results do not appear to
665 be much different from those of normal hexane (UA), given that
666 butanethiol (UA) is non-deuterated for both solvents. These UA model
667 studies, even though eliminating C-H vibration samplings, still have
668 C-C vibrational frequencies different from each other. However, these
669 differences in the infrared range do not seem to produce an observable
670 difference for the results of $G$. [MAY NEED FIGURE]
671
672 Furthermore, results for rigid body toluene solvent, as well as other
673 UA-hexane solvents, are reasonable within the general experimental
674 ranges[CITATIONS]. This suggests that explicit hydrogen might not be a
675 required factor for modeling thermal transport phenomena of systems
676 such as Au-thiol/organic solvent.
677
678 However, results for Au-butanethiol/toluene do not show an identical
679 trend with those for Au-butanethiol/hexane in that $G$'s remain at
680 approximately the same magnitue when butanethiol coverage differs from
681 25\% to 75\%. This might be rooted in the molecule shape difference
682 for plane-like toluene and chain-like {\it n}-hexane. Due to this
683 difference, toluene molecules have more difficulty in occupying
684 relatively small gaps among capping agents when their coverage is not
685 too low. Therefore, the solvent-capping agent contact may keep
686 increasing until the capping agent coverage reaches a relatively low
687 level. This becomes an offset for decreasing butanethiol molecules on
688 its effect to the process of interfacial thermal transport. Thus, one
689 can see a plateau of $G$ vs. butanethiol coverage in our results.
690
691 [NEED ERROR ESTIMATE, MAY ALSO PUT J HERE]
692 \begin{table*}
693 \begin{minipage}{\linewidth}
694 \begin{center}
695 \caption{Computed interfacial thermal conductivity ($G$) values
696 for the Au-butanethiol/solvent interface with various UA
697 models and different capping agent coverages at $\langle
698 T\rangle\sim$200K using certain energy flux respectively.}
699
700 \begin{tabular}{cccc}
701 \hline\hline
702 Thiol & \multicolumn{3}{c}{$G$(MW/m$^2$/K)} \\
703 coverage (\%) & hexane & hexane(D) & toluene \\
704 \hline
705 0.0 & 46.5() & 43.9() & 70.1() \\
706 25.0 & 151() & 153() & 249() \\
707 50.0 & 172() & 182() & 214() \\
708 75.0 & 242() & 229() & 244() \\
709 88.9 & 178() & - & - \\
710 100.0 & 137() & 153() & 187() \\
711 \hline\hline
712 \end{tabular}
713 \label{tlnUhxnUhxnD}
714 \end{center}
715 \end{minipage}
716 \end{table*}
717
718 \subsection{Influence of Chosen Molecule Model on $G$}
719 [MAY COMBINE W MECHANISM STUDY]
720
721 In addition to UA solvent/capping agent models, AA models are included
722 in our simulations as well. Besides simulations of the same (UA or AA)
723 model for solvent and capping agent, different models can be applied
724 to different components. Furthermore, regardless of models chosen,
725 either the solvent or the capping agent can be deuterated, similar to
726 the previous section. Table \ref{modelTest} summarizes the results of
727 these studies.
728
729 [MORE DATA; ERROR ESTIMATE]
730 \begin{table*}
731 \begin{minipage}{\linewidth}
732 \begin{center}
733
734 \caption{Computed interfacial thermal conductivity ($G$ and
735 $G^\prime$) values for interfaces using various models for
736 solvent and capping agent (or without capping agent) at
737 $\langle T\rangle\sim$200K.}
738
739 \begin{tabular}{ccccc}
740 \hline\hline
741 Butanethiol model & Solvent & $J_z$ & $G$ & $G^\prime$ \\
742 (or bare surface) & model & (GW/m$^2$) &
743 \multicolumn{2}{c}{(MW/m$^2$/K)} \\
744 \hline
745 UA & AA hexane & 1.94 & 135() & 129() \\
746 & & 2.86 & 126() & 115() \\
747 & AA toluene & 1.89 & 200() & 149() \\
748 AA & UA hexane & 1.94 & 116() & 129() \\
749 & AA hexane & 3.76 & 451() & 378() \\
750 & & 4.71 & 432() & 334() \\
751 & AA toluene & 3.79 & 487() & 290() \\
752 AA(D) & UA hexane & 1.94 & 158() & 172() \\
753 bare & AA hexane & 0.96 & 31.0() & 29.4() \\
754 \hline\hline
755 \end{tabular}
756 \label{modelTest}
757 \end{center}
758 \end{minipage}
759 \end{table*}
760
761 To facilitate direct comparison, the same system with differnt models
762 for different components uses the same length scale for their
763 simulation cells. Without the presence of capping agent, using
764 different models for hexane yields similar results for both $G$ and
765 $G^\prime$, and these two definitions agree with eath other very
766 well. This indicates very weak interaction between the metal and the
767 solvent, and is a typical case for acoustic impedance mismatch between
768 these two phases.
769
770 As for Au(111) surfaces completely covered by butanethiols, the choice
771 of models for capping agent and solvent could impact the measurement
772 of $G$ and $G^\prime$ quite significantly. For Au-butanethiol/hexane
773 interfaces, using AA model for both butanethiol and hexane yields
774 substantially higher conductivity values than using UA model for at
775 least one component of the solvent and capping agent, which exceeds
776 the upper bond of experimental value range. This is probably due to
777 the classically treated C-H vibrations in the AA model, which should
778 not be appreciably populated at normal temperatures. In comparison,
779 once either the hexanes or the butanethiols are deuterated, one can
780 see a significantly lower $G$ and $G^\prime$. In either of these
781 cases, the C-H(D) vibrational overlap between the solvent and the
782 capping agent is removed. [MAY NEED FIGURE] Conclusively, the
783 improperly treated C-H vibration in the AA model produced
784 over-predicted results accordingly. Compared to the AA model, the UA
785 model yields more reasonable results with higher computational
786 efficiency.
787
788 However, for Au-butanethiol/toluene interfaces, having the AA
789 butanethiol deuterated did not yield a significant change in the
790 measurement results.
791 . , so extra degrees of freedom
792 such as the C-H vibrations could enhance heat exchange between these
793 two phases and result in a much higher conductivity.
794
795
796 Although the QSC model for Au is known to predict an overly low value
797 for bulk metal gold conductivity[CITE NIVSRNEMD], our computational
798 results for $G$ and $G^\prime$ do not seem to be affected by this
799 drawback of the model for metal. Instead, the modeling of interfacial
800 thermal transport behavior relies mainly on an accurate description of
801 the interactions between components occupying the interfaces.
802
803 \subsection{Mechanism of Interfacial Thermal Conductance Enhancement
804 by Capping Agent}
805 %OR\subsection{Vibrational spectrum study on conductance mechanism}
806
807 [MAY INTRODUCE PROTOCOL IN METHODOLOGY/COMPUTATIONAL DETAIL, EQN'S]
808
809 To investigate the mechanism of this interfacial thermal conductance,
810 the vibrational spectra of various gold systems were obtained and are
811 shown as in the upper panel of Fig. \ref{vibration}. To obtain these
812 spectra, one first runs a simulation in the NVE ensemble and collects
813 snapshots of configurations; these configurations are used to compute
814 the velocity auto-correlation functions, which is used to construct a
815 power spectrum via a Fourier transform.
816
817 The gold surfaces covered by
818 butanethiol molecules, compared to bare gold surfaces, exhibit an
819 additional peak observed at a frequency of $\sim$170cm$^{-1}$, which
820 is attributed to the vibration of the S-Au bond. This vibration
821 enables efficient thermal transport from surface Au atoms to the
822 capping agents. Simultaneously, as shown in the lower panel of
823 Fig. \ref{vibration}, the large overlap of the vibration spectra of
824 butanethiol and hexane in the all-atom model, including the C-H
825 vibration, also suggests high thermal exchange efficiency. The
826 combination of these two effects produces the drastic interfacial
827 thermal conductance enhancement in the all-atom model.
828
829 [MAY NEED TO CONVERT TO JPEG]
830 \begin{figure}
831 \includegraphics[width=\linewidth]{vibration}
832 \caption{Vibrational spectra obtained for gold in different
833 environments (upper panel) and for Au/thiol/hexane simulation in
834 all-atom model (lower panel).}
835 \label{vibration}
836 \end{figure}
837
838 [COMPARISON OF TWO G'S; AU SLAB WIDTHS; ETC]
839 % The results show that the two definitions used for $G$ yield
840 % comparable values, though $G^\prime$ tends to be smaller.
841
842 \section{Conclusions}
843 The NIVS algorithm we developed has been applied to simulations of
844 Au-butanethiol surfaces with organic solvents. This algorithm allows
845 effective unphysical thermal flux transferred between the metal and
846 the liquid phase. With the flux applied, we were able to measure the
847 corresponding thermal gradient and to obtain interfacial thermal
848 conductivities. Our simulations have seen significant conductance
849 enhancement with the presence of capping agent, compared to the bare
850 gold/liquid interfaces. The acoustic impedance mismatch between the
851 metal and the liquid phase is effectively eliminated by proper capping
852 agent. Furthermore, the coverage precentage of the capping agent plays
853 an important role in the interfacial thermal transport process.
854
855 Our measurement results, particularly of the UA models, agree with
856 available experimental data. This indicates that our force field
857 parameters have a nice description of the interactions between the
858 particles at the interfaces. AA models tend to overestimate the
859 interfacial thermal conductance in that the classically treated C-H
860 vibration would be overly sampled. Compared to the AA models, the UA
861 models have higher computational efficiency with satisfactory
862 accuracy, and thus are preferable in interfacial thermal transport
863 modelings.
864
865 Vlugt {\it et al.} has investigated the surface thiol structures for
866 nanocrystal gold and pointed out that they differs from those of the
867 Au(111) surface\cite{vlugt:cpc2007154}. This difference might lead to
868 change of interfacial thermal transport behavior as well. To
869 investigate this problem, an effective means to introduce thermal flux
870 and measure the corresponding thermal gradient is desirable for
871 simulating structures with spherical symmetry.
872
873
874 \section{Acknowledgments}
875 Support for this project was provided by the National Science
876 Foundation under grant CHE-0848243. Computational time was provided by
877 the Center for Research Computing (CRC) at the University of Notre
878 Dame. \newpage
879
880 \bibliography{interfacial}
881
882 \end{doublespace}
883 \end{document}
884