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add more references, done much of the introduction.

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