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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 We have developed a Non-Isotropic Velocity Scaling algorithm for
49 setting up and maintaining stable thermal gradients in non-equilibrium
50 molecular dynamics simulations. This approach effectively imposes
51 unphysical thermal flux even between particles of different
52 identities, conserves linear momentum and kinetic energy, and
53 minimally perturbs the velocity profile of a system when compared with
54 previous RNEMD methods. We have used this method to simulate thermal
55 conductance at metal / organic solvent interfaces both with and
56 without the presence of thiol-based capping agents. We obtained
57 values comparable with experimental values, and observed significant
58 conductance enhancement with the presence of capping agents. Computed
59 power spectra indicate the acoustic impedance mismatch between metal
60 and liquid phase is greatly reduced by the capping agents and thus
61 leads to higher interfacial thermal transfer efficiency.
62
63 \end{abstract}
64
65 \newpage
66
67 %\narrowtext
68
69 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
70 % BODY OF TEXT
71 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
72
73 \section{Introduction}
74 [BACKGROUND FOR INTERFACIAL THERMAL CONDUCTANCE PROBLEM]
75 Interfacial thermal conductance is extensively studied both
76 experimentally and computationally, and systems with interfaces
77 present are generally heterogeneous. Although interfaces are commonly
78 barriers to heat transfer, it has been
79 reported\cite{doi:10.1021/la904855s} that under specific circustances,
80 e.g. with certain capping agents present on the surface, interfacial
81 conductance can be significantly enhanced. However, heat conductance
82 of molecular and nano-scale interfaces will be affected by the
83 chemical details of the surface and is challenging to
84 experimentalist. The lower thermal flux through interfaces is even
85 more difficult to measure with EMD and forward NEMD simulation
86 methods. Therefore, developing good simulation methods will be
87 desirable in order to investigate thermal transport across interfaces.
88
89 Recently, we have developed the Non-Isotropic Velocity Scaling (NIVS)
90 algorithm for RNEMD simulations\cite{kuang:164101}. This algorithm
91 retains the desirable features of RNEMD (conservation of linear
92 momentum and total energy, compatibility with periodic boundary
93 conditions) while establishing true thermal distributions in each of
94 the two slabs. Furthermore, it allows more effective thermal exchange
95 between particles of different identities, and thus enables extensive
96 study of interfacial conductance.
97
98 \section{Methodology}
99 \subsection{Algorithm}
100 [BACKGROUND FOR MD METHODS]
101 There have been many algorithms for computing thermal conductivity
102 using molecular dynamics simulations. However, interfacial conductance
103 is at least an order of magnitude smaller. This would make the
104 calculation even more difficult for those slowly-converging
105 equilibrium methods. Imposed-flux non-equilibrium
106 methods\cite{MullerPlathe:1997xw} have the flux set {\it a priori} and
107 the response of temperature or momentum gradients are easier to
108 measure than the flux, if unknown, and thus, is a preferable way to
109 the forward NEMD methods. Although the momentum swapping approach for
110 flux-imposing can be used for exchanging energy between particles of
111 different identity, the kinetic energy transfer efficiency is affected
112 by the mass difference between the particles, which limits its
113 application on heterogeneous interfacial systems.
114
115 The non-isotropic velocity scaling (NIVS)\cite{kuang:164101} approach in
116 non-equilibrium MD simulations is able to impose relatively large
117 kinetic energy flux without obvious perturbation to the velocity
118 distribution of the simulated systems. Furthermore, this approach has
119 the advantage in heterogeneous interfaces in that kinetic energy flux
120 can be applied between regions of particles of arbitary identity, and
121 the flux quantity is not restricted by particle mass difference.
122
123 The NIVS algorithm scales the velocity vectors in two separate regions
124 of a simulation system with respective diagonal scaling matricies. To
125 determine these scaling factors in the matricies, a set of equations
126 including linear momentum conservation and kinetic energy conservation
127 constraints and target momentum/energy flux satisfaction is
128 solved. With the scaling operation applied to the system in a set
129 frequency, corresponding momentum/temperature gradients can be built,
130 which can be used for computing transportation properties and other
131 applications related to momentum/temperature gradients. The NIVS
132 algorithm conserves momenta and energy and does not depend on an
133 external thermostat.
134
135 \subsection{Defining Interfacial Thermal Conductivity $G$}
136 For interfaces with a relatively low interfacial conductance, the bulk
137 regions on either side of an interface rapidly come to a state in
138 which the two phases have relatively homogeneous (but distinct)
139 temperatures. The interfacial thermal conductivity $G$ can therefore
140 be approximated as:
141 \begin{equation}
142 G = \frac{E_{total}}{2 t L_x L_y \left( \langle T_\mathrm{hot}\rangle -
143 \langle T_\mathrm{cold}\rangle \right)}
144 \label{lowG}
145 \end{equation}
146 where ${E_{total}}$ is the imposed non-physical kinetic energy
147 transfer and ${\langle T_\mathrm{hot}\rangle}$ and ${\langle
148 T_\mathrm{cold}\rangle}$ are the average observed temperature of the
149 two separated phases.
150
151 When the interfacial conductance is {\it not} small, two ways can be
152 used to define $G$.
153
154 One way is to assume the temperature is discretely different on two
155 sides of the interface, $G$ can be calculated with the thermal flux
156 applied $J$ and the maximum temperature difference measured along the
157 thermal gradient max($\Delta T$), which occurs at the interface, as:
158 \begin{equation}
159 G=\frac{J}{\Delta T}
160 \label{discreteG}
161 \end{equation}
162
163 The other approach is to assume a continuous temperature profile along
164 the thermal gradient axis (e.g. $z$) and define $G$ at the point where
165 the magnitude of thermal conductivity $\lambda$ change reach its
166 maximum, given that $\lambda$ is well-defined throughout the space:
167 \begin{equation}
168 G^\prime = \Big|\frac{\partial\lambda}{\partial z}\Big|
169 = \Big|\frac{\partial}{\partial z}\left(-J_z\Big/
170 \left(\frac{\partial T}{\partial z}\right)\right)\Big|
171 = |J_z|\Big|\frac{\partial^2 T}{\partial z^2}\Big|
172 \Big/\left(\frac{\partial T}{\partial z}\right)^2
173 \label{derivativeG}
174 \end{equation}
175
176 With the temperature profile obtained from simulations, one is able to
177 approximate the first and second derivatives of $T$ with finite
178 difference method and thus calculate $G^\prime$.
179
180 In what follows, both definitions are used for calculation and comparison.
181
182 [IMPOSE G DEFINITION INTO OUR SYSTEMS]
183 To facilitate the use of the above definitions in calculating $G$ and
184 $G^\prime$, we have a metal slab with its (111) surfaces perpendicular
185 to the $z$-axis of our simulation cells. With or withour capping
186 agents on the surfaces, the metal slab is solvated with organic
187 solvents, as illustrated in Figure \ref{demoPic}.
188
189 \begin{figure}
190 \includegraphics[width=\linewidth]{demoPic}
191 \caption{A sample showing how a metal slab has its (111) surface
192 covered by capping agent molecules and solvated by hexane.}
193 \label{demoPic}
194 \end{figure}
195
196 With a simulation cell setup following the above manner, one is able
197 to equilibrate the system and impose an unphysical thermal flux
198 between the liquid and the metal phase with the NIVS algorithm. Under
199 a stablized thermal gradient induced by periodically applying the
200 unphysical flux, one is able to obtain a temperature profile and the
201 physical thermal flux corresponding to it, which equals to the
202 unphysical flux applied by NIVS. These data enables the evaluation of
203 the interfacial thermal conductance of a surface. Figure \ref{gradT}
204 is an example how those stablized thermal gradient can be used to
205 obtain the 1st and 2nd derivatives of the temperature profile.
206
207 \begin{figure}
208 \includegraphics[width=\linewidth]{gradT}
209 \caption{The 1st and 2nd derivatives of temperature profile can be
210 obtained with finite difference approximation.}
211 \label{gradT}
212 \end{figure}
213
214 \section{Computational Details}
215 \subsection{System Geometry}
216 In our simulations, Au is used to construct a metal slab with bare
217 (111) surface perpendicular to the $z$-axis. Different slab thickness
218 (layer numbers of Au) are simulated. This metal slab is first
219 equilibrated under normal pressure (1 atm) and a desired
220 temperature. After equilibration, butanethiol is used as the capping
221 agent molecule to cover the bare Au (111) surfaces evenly. The sulfur
222 atoms in the butanethiol molecules would occupy the three-fold sites
223 of the surfaces, and the maximal butanethiol capacity on Au surface is
224 $1/3$ of the total number of surface Au atoms[CITATION]. A series of
225 different coverage surfaces is investigated in order to study the
226 relation between coverage and conductance.
227
228 [COVERAGE DISCRIPTION] However, since the interactions between surface
229 Au and butanethiol is non-bonded, the capping agent molecules are
230 allowed to migrate to an empty neighbor three-fold site during a
231 simulation. Therefore, the initial configuration would not severely
232 affect the sampling of a variety of configurations of the same
233 coverage, and the final conductance measurement would be an average
234 effect of these configurations explored in the simulations. [MAY NEED FIGURES]
235
236 After the modified Au-butanethiol surface systems are equilibrated
237 under canonical ensemble, Packmol\cite{packmol} is used to pack
238 organic solvent molecules in the previously vacuum part of the
239 simulation cells, which guarantees that short range repulsive
240 interactions do not disrupt the simulations. Two solvents are
241 investigated, one which has little vibrational overlap with the
242 alkanethiol and plane-like shape (toluene), and one which has similar
243 vibrational frequencies and chain-like shape ({\it n}-hexane). The
244 spacing filled by solvent molecules, i.e. the gap between periodically
245 repeated Au-butanethiol surfaces should be carefully chosen so that it
246 would not be too short to affect the liquid phase structure, nor too
247 long, leading to over cooling (freezing) or heating (boiling) when a
248 thermal flux is applied. In our simulations, this spacing is usually
249 $35 \sim 60$\AA.
250
251 The initial configurations generated by Packmol are further
252 equilibrated with the $x$ and $y$ dimensions fixed, only allowing
253 length scale change in $z$ dimension. This is to ensure that the
254 equilibration of liquid phase does not affect the metal crystal
255 structure in $x$ and $y$ dimensions. Further equilibration are run
256 under NVT and then NVE ensembles.
257
258 After the systems reach equilibrium, NIVS is implemented to impose a
259 periodic unphysical thermal flux between the metal and the liquid
260 phase. Most of our simulations are under an average temperature of
261 $\sim$200K. Therefore, this flux usually comes from the metal to the
262 liquid so that the liquid has a higher temperature and would not
263 freeze due to excessively low temperature. This induced temperature
264 gradient is stablized and the simulation cell is devided evenly into
265 N slabs along the $z$-axis and the temperatures of each slab are
266 recorded. When the slab width $d$ of each slab is the same, the
267 derivatives of $T$ with respect to slab number $n$ can be directly
268 used for $G^\prime$ calculations:
269 \begin{equation}
270 G^\prime = |J_z|\Big|\frac{\partial^2 T}{\partial z^2}\Big|
271 \Big/\left(\frac{\partial T}{\partial z}\right)^2
272 = |J_z|\Big|\frac{1}{d^2}\frac{\partial^2 T}{\partial n^2}\Big|
273 \Big/\left(\frac{1}{d}\frac{\partial T}{\partial n}\right)^2
274 = |J_z|\Big|\frac{\partial^2 T}{\partial n^2}\Big|
275 \Big/\left(\frac{\partial T}{\partial n}\right)^2
276 \label{derivativeG2}
277 \end{equation}
278
279 \subsection{Force Field Parameters}
280 Our simulations include various components. Therefore, force field
281 parameter descriptions are needed for interactions both between the
282 same type of particles and between particles of different species.
283
284 The Au-Au interactions in metal lattice slab is described by the
285 quantum Sutton-Chen (QSC) formulation.\cite{PhysRevB.59.3527} The QSC
286 potentials include zero-point quantum corrections and are
287 reparametrized for accurate surface energies compared to the
288 Sutton-Chen potentials\cite{Chen90}.
289
290 For both solvent molecules, straight chain {\it n}-hexane and aromatic
291 toluene, United-Atom (UA) and All-Atom (AA) models are used
292 respectively. The TraPPE-UA
293 parameters\cite{TraPPE-UA.alkanes,TraPPE-UA.alkylbenzenes} are used
294 for our UA solvent molecules. In these models, pseudo-atoms are
295 located at the carbon centers for alkyl groups. By eliminating
296 explicit hydrogen atoms, these models are simple and computationally
297 efficient, while maintains good accuracy. However, the TraPPE-UA for
298 alkanes is known to predict a lower boiling point than experimental
299 values. Considering that after an unphysical thermal flux is applied
300 to a system, the temperature of ``hot'' area in the liquid phase would be
301 significantly higher than the average, to prevent over heating and
302 boiling of the liquid phase, the average temperature in our
303 simulations should be much lower than the liquid boiling point. [NEED MORE DISCUSSION]
304 For UA-toluene model, rigid body constraints are applied, so that the
305 benzene ring and the methyl-C(aromatic) bond are kept rigid. This
306 would save computational time.[MORE DETAILS NEEDED]
307
308 Besides the TraPPE-UA models, AA models for both organic solvents are
309 included in our studies as well. For hexane, the OPLS
310 all-atom\cite{OPLSAA} force field is used. [MORE DETAILS]
311 For toluene, the United Force Field developed by Rapp\'{e} {\it et
312 al.}\cite{doi:10.1021/ja00051a040} is adopted.[MORE DETAILS]
313
314 The capping agent in our simulations, the butanethiol molecules can
315 either use UA or AA model. The TraPPE-UA force fields includes
316 parameters for thiol molecules\cite{TraPPE-UA.thiols} and are used in
317 our simulations corresponding to our TraPPE-UA models for solvent.
318 and All-Atom models [NEED CITATIONS]
319 However, the model choice (UA or AA) of capping agent can be different
320 from the solvent. Regardless of model choice, the force field
321 parameters for interactions between capping agent and solvent can be
322 derived using Lorentz-Berthelot Mixing Rule.
323
324 To describe the interactions between metal Au and non-metal capping
325 agent and solvent, we refer to Vlugt\cite{vlugt:cpc2007154} and derive
326 other interactions which are not yet finely parametrized. [can add
327 hautman and klein's paper here and more discussion; need to put
328 aromatic-metal interaction approximation here]\cite{doi:10.1021/jp034405s}
329
330 [TABULATED FORCE FIELD PARAMETERS NEEDED]
331
332
333 [SURFACE RECONSTRUCTION PREVENTS SIMULATION TEMP TO GO HIGHER]
334
335
336 \section{Results}
337 [REARRANGEMENT NEEDED]
338 \subsection{Toluene Solvent}
339
340 The results (Table \ref{AuThiolToluene}) show a
341 significant conductance enhancement compared to the gold/water
342 interface without capping agent and agree with available experimental
343 data. This indicates that the metal-metal potential, though not
344 predicting an accurate bulk metal thermal conductivity, does not
345 greatly interfere with the simulation of the thermal conductance
346 behavior across a non-metal interface. The solvent model is not
347 particularly volatile, so the simulation cell does not expand
348 significantly under higher temperature. We did not observe a
349 significant conductance decrease when the temperature was increased to
350 300K. The results show that the two definitions used for $G$ yield
351 comparable values, though $G^\prime$ tends to be smaller.
352
353 \begin{table*}
354 \begin{minipage}{\linewidth}
355 \begin{center}
356 \caption{Computed interfacial thermal conductivity ($G$ and
357 $G^\prime$) values for the Au/butanethiol/toluene interface at
358 different temperatures using a range of energy fluxes.}
359
360 \begin{tabular}{cccc}
361 \hline\hline
362 $\langle T\rangle$ & $J_z$ & $G$ & $G^\prime$ \\
363 (K) & (GW/m$^2$) & \multicolumn{2}{c}{(MW/m$^2$/K)} \\
364 \hline
365 200 & 1.86 & 180 & 135 \\
366 & 2.15 & 204 & 113 \\
367 & 3.93 & 175 & 114 \\
368 300 & 1.91 & 143 & 125 \\
369 & 4.19 & 134 & 113 \\
370 \hline\hline
371 \end{tabular}
372 \label{AuThiolToluene}
373 \end{center}
374 \end{minipage}
375 \end{table*}
376
377 \subsection{Hexane Solvent}
378
379 Using the united-atom model, different coverages of capping agent,
380 temperatures of simulations and numbers of solvent molecules were all
381 investigated and Table \ref{AuThiolHexaneUA} shows the results of
382 these computations. The number of hexane molecules in our simulations
383 does not affect the calculations significantly. However, a very long
384 length scale for the thermal gradient axis ($z$) may cause excessively
385 hot or cold temperatures in the middle of the solvent region and lead
386 to undesired phenomena such as solvent boiling or freezing, while too
387 few solvent molecules would change the normal behavior of the liquid
388 phase. Our $N_{hexane}$ values were chosen to ensure that these
389 extreme cases did not happen to our simulations.
390
391 Table \ref{AuThiolHexaneUA} enables direct comparison between
392 different coverages of capping agent, when other system parameters are
393 held constant. With high coverage of butanethiol on the gold surface,
394 the interfacial thermal conductance is enhanced
395 significantly. Interestingly, a slightly lower butanethiol coverage
396 leads to a moderately higher conductivity. This is probably due to
397 more solvent/capping agent contact when butanethiol molecules are
398 not densely packed, which enhances the interactions between the two
399 phases and lowers the thermal transfer barrier of this interface.
400 % [COMPARE TO AU/WATER IN PAPER]
401
402 It is also noted that the overall simulation temperature is another
403 factor that affects the interfacial thermal conductance. One
404 possibility of this effect may be rooted in the decrease in density of
405 the liquid phase. We observed that when the average temperature
406 increases from 200K to 250K, the bulk hexane density becomes lower
407 than experimental value, as the system is equilibrated under NPT
408 ensemble. This leads to lower contact between solvent and capping
409 agent, and thus lower conductivity.
410
411 Conductivity values are more difficult to obtain under higher
412 temperatures. This is because the Au surface tends to undergo
413 reconstructions in relatively high temperatures. Surface Au atoms can
414 migrate outward to reach higher Au-S contact; and capping agent
415 molecules can be embedded into the surface Au layer due to the same
416 driving force. This phenomenon agrees with experimental
417 results\cite{doi:10.1021/j100035a033,doi:10.1021/la026493y}. A surface
418 fully covered in capping agent is more susceptible to reconstruction,
419 possibly because fully coverage prevents other means of capping agent
420 relaxation, such as migration to an empty neighbor three-fold site.
421
422 %MAY ADD MORE DATA TO TABLE
423 \begin{table*}
424 \begin{minipage}{\linewidth}
425 \begin{center}
426 \caption{Computed interfacial thermal conductivity ($G$ and
427 $G^\prime$) values for the Au/butanethiol/hexane interface
428 with united-atom model and different capping agent coverage
429 and solvent molecule numbers at different temperatures using a
430 range of energy fluxes.}
431
432 \begin{tabular}{cccccc}
433 \hline\hline
434 Thiol & $\langle T\rangle$ & & $J_z$ & $G$ & $G^\prime$ \\
435 coverage (\%) & (K) & $N_{hexane}$ & (GW/m$^2$) &
436 \multicolumn{2}{c}{(MW/m$^2$/K)} \\
437 \hline
438 0.0 & 200 & 200 & 0.96 & 43.3 & 42.7 \\
439 & & & 1.91 & 45.7 & 42.9 \\
440 & & 166 & 0.96 & 43.1 & 53.4 \\
441 88.9 & 200 & 166 & 1.94 & 172 & 108 \\
442 100.0 & 250 & 200 & 0.96 & 81.8 & 67.0 \\
443 & & 166 & 0.98 & 79.0 & 62.9 \\
444 & & & 1.44 & 76.2 & 64.8 \\
445 & 200 & 200 & 1.92 & 129 & 87.3 \\
446 & & & 1.93 & 131 & 77.5 \\
447 & & 166 & 0.97 & 115 & 69.3 \\
448 & & & 1.94 & 125 & 87.1 \\
449 \hline\hline
450 \end{tabular}
451 \label{AuThiolHexaneUA}
452 \end{center}
453 \end{minipage}
454 \end{table*}
455
456 For the all-atom model, the liquid hexane phase was not stable under NPT
457 conditions. Therefore, the simulation length scale parameters are
458 adopted from previous equilibration results of the united-atom model
459 at 200K. Table \ref{AuThiolHexaneAA} shows the results of these
460 simulations. The conductivity values calculated with full capping
461 agent coverage are substantially larger than observed in the
462 united-atom model, and is even higher than predicted by
463 experiments. It is possible that our parameters for metal-non-metal
464 particle interactions lead to an overestimate of the interfacial
465 thermal conductivity, although the active C-H vibrations in the
466 all-atom model (which should not be appreciably populated at normal
467 temperatures) could also account for this high conductivity. The major
468 thermal transfer barrier of Au/butanethiol/hexane interface is between
469 the liquid phase and the capping agent, so extra degrees of freedom
470 such as the C-H vibrations could enhance heat exchange between these
471 two phases and result in a much higher conductivity.
472
473 \begin{table*}
474 \begin{minipage}{\linewidth}
475 \begin{center}
476
477 \caption{Computed interfacial thermal conductivity ($G$ and
478 $G^\prime$) values for the Au/butanethiol/hexane interface
479 with all-atom model and different capping agent coverage at
480 200K using a range of energy fluxes.}
481
482 \begin{tabular}{cccc}
483 \hline\hline
484 Thiol & $J_z$ & $G$ & $G^\prime$ \\
485 coverage (\%) & (GW/m$^2$) & \multicolumn{2}{c}{(MW/m$^2$/K)} \\
486 \hline
487 0.0 & 0.95 & 28.5 & 27.2 \\
488 & 1.88 & 30.3 & 28.9 \\
489 100.0 & 2.87 & 551 & 294 \\
490 & 3.81 & 494 & 193 \\
491 \hline\hline
492 \end{tabular}
493 \label{AuThiolHexaneAA}
494 \end{center}
495 \end{minipage}
496 \end{table*}
497
498 %subsubsection{Vibrational spectrum study on conductance mechanism}
499 To investigate the mechanism of this interfacial thermal conductance,
500 the vibrational spectra of various gold systems were obtained and are
501 shown as in the upper panel of Fig. \ref{vibration}. To obtain these
502 spectra, one first runs a simulation in the NVE ensemble and collects
503 snapshots of configurations; these configurations are used to compute
504 the velocity auto-correlation functions, which is used to construct a
505 power spectrum via a Fourier transform. The gold surfaces covered by
506 butanethiol molecules exhibit an additional peak observed at a
507 frequency of $\sim$170cm$^{-1}$, which is attributed to the vibration
508 of the S-Au bond. This vibration enables efficient thermal transport
509 from surface Au atoms to the capping agents. Simultaneously, as shown
510 in the lower panel of Fig. \ref{vibration}, the large overlap of the
511 vibration spectra of butanethiol and hexane in the all-atom model,
512 including the C-H vibration, also suggests high thermal exchange
513 efficiency. The combination of these two effects produces the drastic
514 interfacial thermal conductance enhancement in the all-atom model.
515
516 \begin{figure}
517 \includegraphics[width=\linewidth]{vibration}
518 \caption{Vibrational spectra obtained for gold in different
519 environments (upper panel) and for Au/thiol/hexane simulation in
520 all-atom model (lower panel).}
521 \label{vibration}
522 \end{figure}
523 % 600dpi, letter size. too large?
524
525
526 \section{Acknowledgments}
527 Support for this project was provided by the National Science
528 Foundation under grant CHE-0848243. Computational time was provided by
529 the Center for Research Computing (CRC) at the University of Notre
530 Dame. \newpage
531
532 \bibliography{interfacial}
533
534 \end{doublespace}
535 \end{document}
536