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more results and discussions, added conclusions and abstract

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