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add data. done much of methodology and simulation details.

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1 gezelter 3717 \documentclass[11pt]{article}
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26 gezelter 3717 \bibpunct{[}{]}{,}{s}{}{;}
27     \bibliographystyle{aip}
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 skuang 3725
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 gezelter 3717 \end{abstract}
64    
65     \newpage
66    
67     %\narrowtext
68    
69     %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
70     % BODY OF TEXT
71     %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
72    
73     \section{Introduction}
74 skuang 3727 [BACKGROUND FOR INTERFACIAL THERMAL CONDUCTANCE PROBLEM]
75 skuang 3725 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 gezelter 3717
89 skuang 3725 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 skuang 3721 \section{Methodology}
99     \subsection{Algorithm}
100 skuang 3727 [BACKGROUND FOR MD METHODS]
101 skuang 3721 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 skuang 3727 \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 skuang 3721
151 skuang 3727 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     initial configurations generated by Packmol are further equilibrated
245     with the $x$ and $y$ dimensions fixed, only allowing length scale
246     change in $z$ dimension. This is to ensure that the equilibration of
247     liquid phase does not affect the metal crystal structure in $x$ and
248     $y$ dimensions. Further equilibration are run under NVT and then NVE ensembles.
249    
250     After the systems reach equilibrium, NIVS is implemented to impose a
251     periodic unphysical thermal flux between the metal and the liquid
252     phase. Most of our simulations have this flux from the metal to the
253     liquid so that the liquid has a higher temperature and would not
254     freeze due to excessively low temperature. This induced temperature
255     gradient is stablized and the simulation cell is devided evenly into
256     N slabs along the $z$-axis and the temperatures of each slab are
257     recorded. When the slab width $d$ of each slab is the same, the
258     derivatives of $T$ with respect to slab number $n$ can be directly
259     used for $G^\prime$ calculations:
260     \begin{equation}
261     G^\prime = |J_z|\Big|\frac{\partial^2 T}{\partial z^2}\Big|
262     \Big/\left(\frac{\partial T}{\partial z}\right)^2
263     = |J_z|\Big|\frac{1}{d^2}\frac{\partial^2 T}{\partial n^2}\Big|
264     \Big/\left(\frac{1}{d}\frac{\partial T}{\partial n}\right)^2
265     = |J_z|\Big|\frac{\partial^2 T}{\partial n^2}\Big|
266     \Big/\left(\frac{\partial T}{\partial n}\right)^2
267     \label{derivativeG2}
268     \end{equation}
269    
270    
271 skuang 3725 \subsection{Force Field Parameters}
272 skuang 3721
273     The Au-Au interactions in metal lattice slab is described by the
274     quantum Sutton-Chen (QSC) formulation.\cite{PhysRevB.59.3527} The QSC
275     potentials include zero-point quantum corrections and are
276     reparametrized for accurate surface energies compared to the
277     Sutton-Chen potentials\cite{Chen90}.
278    
279     Straight chain {\it n}-hexane and aromatic toluene are respectively
280     used as solvents. For hexane, both United-Atom\cite{TraPPE-UA.alkanes}
281     and All-Atom\cite{OPLSAA} force fields are used for comparison; for
282     toluene, United-Atom\cite{TraPPE-UA.alkylbenzenes} force fields are
283     used with rigid body constraints applied. (maybe needs more details
284     about rigid body)
285    
286     Buatnethiol molecules are used as capping agent for some of our
287     simulations. United-Atom\cite{TraPPE-UA.thiols} and All-Atom models
288     are respectively used corresponding to the force field type of
289     solvent.
290    
291     To describe the interactions between metal Au and non-metal capping
292     agent and solvent, we refer to Vlugt\cite{vlugt:cpc2007154} and derive
293     other interactions which are not parametrized in their work. (can add
294     hautman and klein's paper here and more discussion; need to put
295     aromatic-metal interaction approximation here)
296    
297 skuang 3725 [TABULATED FORCE FIELD PARAMETERS NEEDED]
298    
299     \section{Results}
300     \subsection{Toluene Solvent}
301    
302 skuang 3727 The results (Table \ref{AuThiolToluene}) show a
303 skuang 3725 significant conductance enhancement compared to the gold/water
304     interface without capping agent and agree with available experimental
305     data. This indicates that the metal-metal potential, though not
306     predicting an accurate bulk metal thermal conductivity, does not
307     greatly interfere with the simulation of the thermal conductance
308     behavior across a non-metal interface. The solvent model is not
309     particularly volatile, so the simulation cell does not expand
310     significantly under higher temperature. We did not observe a
311     significant conductance decrease when the temperature was increased to
312     300K. The results show that the two definitions used for $G$ yield
313     comparable values, though $G^\prime$ tends to be smaller.
314    
315     \begin{table*}
316     \begin{minipage}{\linewidth}
317     \begin{center}
318     \caption{Computed interfacial thermal conductivity ($G$ and
319     $G^\prime$) values for the Au/butanethiol/toluene interface at
320     different temperatures using a range of energy fluxes.}
321    
322     \begin{tabular}{cccc}
323     \hline\hline
324     $\langle T\rangle$ & $J_z$ & $G$ & $G^\prime$ \\
325     (K) & (GW/m$^2$) & \multicolumn{2}{c}{(MW/m$^2$/K)} \\
326     \hline
327     200 & 1.86 & 180 & 135 \\
328     & 2.15 & 204 & 113 \\
329     & 3.93 & 175 & 114 \\
330     300 & 1.91 & 143 & 125 \\
331     & 4.19 & 134 & 113 \\
332     \hline\hline
333     \end{tabular}
334     \label{AuThiolToluene}
335     \end{center}
336     \end{minipage}
337     \end{table*}
338    
339     \subsection{Hexane Solvent}
340    
341     Using the united-atom model, different coverages of capping agent,
342     temperatures of simulations and numbers of solvent molecules were all
343     investigated and Table \ref{AuThiolHexaneUA} shows the results of
344     these computations. The number of hexane molecules in our simulations
345     does not affect the calculations significantly. However, a very long
346     length scale for the thermal gradient axis ($z$) may cause excessively
347     hot or cold temperatures in the middle of the solvent region and lead
348     to undesired phenomena such as solvent boiling or freezing, while too
349     few solvent molecules would change the normal behavior of the liquid
350     phase. Our $N_{hexane}$ values were chosen to ensure that these
351     extreme cases did not happen to our simulations.
352    
353     Table \ref{AuThiolHexaneUA} enables direct comparison between
354     different coverages of capping agent, when other system parameters are
355     held constant. With high coverage of butanethiol on the gold surface,
356     the interfacial thermal conductance is enhanced
357     significantly. Interestingly, a slightly lower butanethiol coverage
358     leads to a moderately higher conductivity. This is probably due to
359     more solvent/capping agent contact when butanethiol molecules are
360     not densely packed, which enhances the interactions between the two
361     phases and lowers the thermal transfer barrier of this interface.
362     % [COMPARE TO AU/WATER IN PAPER]
363    
364     It is also noted that the overall simulation temperature is another
365     factor that affects the interfacial thermal conductance. One
366     possibility of this effect may be rooted in the decrease in density of
367     the liquid phase. We observed that when the average temperature
368     increases from 200K to 250K, the bulk hexane density becomes lower
369     than experimental value, as the system is equilibrated under NPT
370     ensemble. This leads to lower contact between solvent and capping
371     agent, and thus lower conductivity.
372    
373     Conductivity values are more difficult to obtain under higher
374     temperatures. This is because the Au surface tends to undergo
375     reconstructions in relatively high temperatures. Surface Au atoms can
376     migrate outward to reach higher Au-S contact; and capping agent
377     molecules can be embedded into the surface Au layer due to the same
378     driving force. This phenomenon agrees with experimental
379     results\cite{doi:10.1021/j100035a033,doi:10.1021/la026493y}. A surface
380     fully covered in capping agent is more susceptible to reconstruction,
381     possibly because fully coverage prevents other means of capping agent
382     relaxation, such as migration to an empty neighbor three-fold site.
383    
384     %MAY ADD MORE DATA TO TABLE
385     \begin{table*}
386     \begin{minipage}{\linewidth}
387     \begin{center}
388     \caption{Computed interfacial thermal conductivity ($G$ and
389     $G^\prime$) values for the Au/butanethiol/hexane interface
390     with united-atom model and different capping agent coverage
391     and solvent molecule numbers at different temperatures using a
392     range of energy fluxes.}
393    
394     \begin{tabular}{cccccc}
395     \hline\hline
396     Thiol & $\langle T\rangle$ & & $J_z$ & $G$ & $G^\prime$ \\
397     coverage (\%) & (K) & $N_{hexane}$ & (GW/m$^2$) &
398     \multicolumn{2}{c}{(MW/m$^2$/K)} \\
399     \hline
400     0.0 & 200 & 200 & 0.96 & 43.3 & 42.7 \\
401     & & & 1.91 & 45.7 & 42.9 \\
402     & & 166 & 0.96 & 43.1 & 53.4 \\
403     88.9 & 200 & 166 & 1.94 & 172 & 108 \\
404     100.0 & 250 & 200 & 0.96 & 81.8 & 67.0 \\
405     & & 166 & 0.98 & 79.0 & 62.9 \\
406     & & & 1.44 & 76.2 & 64.8 \\
407     & 200 & 200 & 1.92 & 129 & 87.3 \\
408     & & & 1.93 & 131 & 77.5 \\
409     & & 166 & 0.97 & 115 & 69.3 \\
410     & & & 1.94 & 125 & 87.1 \\
411     \hline\hline
412     \end{tabular}
413     \label{AuThiolHexaneUA}
414     \end{center}
415     \end{minipage}
416     \end{table*}
417    
418     For the all-atom model, the liquid hexane phase was not stable under NPT
419     conditions. Therefore, the simulation length scale parameters are
420     adopted from previous equilibration results of the united-atom model
421     at 200K. Table \ref{AuThiolHexaneAA} shows the results of these
422     simulations. The conductivity values calculated with full capping
423     agent coverage are substantially larger than observed in the
424     united-atom model, and is even higher than predicted by
425     experiments. It is possible that our parameters for metal-non-metal
426     particle interactions lead to an overestimate of the interfacial
427     thermal conductivity, although the active C-H vibrations in the
428     all-atom model (which should not be appreciably populated at normal
429     temperatures) could also account for this high conductivity. The major
430     thermal transfer barrier of Au/butanethiol/hexane interface is between
431     the liquid phase and the capping agent, so extra degrees of freedom
432     such as the C-H vibrations could enhance heat exchange between these
433     two phases and result in a much higher conductivity.
434    
435     \begin{table*}
436     \begin{minipage}{\linewidth}
437     \begin{center}
438    
439     \caption{Computed interfacial thermal conductivity ($G$ and
440     $G^\prime$) values for the Au/butanethiol/hexane interface
441     with all-atom model and different capping agent coverage at
442     200K using a range of energy fluxes.}
443    
444     \begin{tabular}{cccc}
445     \hline\hline
446     Thiol & $J_z$ & $G$ & $G^\prime$ \\
447     coverage (\%) & (GW/m$^2$) & \multicolumn{2}{c}{(MW/m$^2$/K)} \\
448     \hline
449     0.0 & 0.95 & 28.5 & 27.2 \\
450     & 1.88 & 30.3 & 28.9 \\
451     100.0 & 2.87 & 551 & 294 \\
452     & 3.81 & 494 & 193 \\
453     \hline\hline
454     \end{tabular}
455     \label{AuThiolHexaneAA}
456     \end{center}
457     \end{minipage}
458     \end{table*}
459    
460     %subsubsection{Vibrational spectrum study on conductance mechanism}
461     To investigate the mechanism of this interfacial thermal conductance,
462     the vibrational spectra of various gold systems were obtained and are
463     shown as in the upper panel of Fig. \ref{vibration}. To obtain these
464     spectra, one first runs a simulation in the NVE ensemble and collects
465     snapshots of configurations; these configurations are used to compute
466     the velocity auto-correlation functions, which is used to construct a
467     power spectrum via a Fourier transform. The gold surfaces covered by
468     butanethiol molecules exhibit an additional peak observed at a
469     frequency of $\sim$170cm$^{-1}$, which is attributed to the vibration
470     of the S-Au bond. This vibration enables efficient thermal transport
471     from surface Au atoms to the capping agents. Simultaneously, as shown
472     in the lower panel of Fig. \ref{vibration}, the large overlap of the
473     vibration spectra of butanethiol and hexane in the all-atom model,
474     including the C-H vibration, also suggests high thermal exchange
475     efficiency. The combination of these two effects produces the drastic
476     interfacial thermal conductance enhancement in the all-atom model.
477    
478     \begin{figure}
479     \includegraphics[width=\linewidth]{vibration}
480     \caption{Vibrational spectra obtained for gold in different
481     environments (upper panel) and for Au/thiol/hexane simulation in
482     all-atom model (lower panel).}
483     \label{vibration}
484     \end{figure}
485     % 600dpi, letter size. too large?
486    
487    
488 gezelter 3717 \section{Acknowledgments}
489     Support for this project was provided by the National Science
490     Foundation under grant CHE-0848243. Computational time was provided by
491     the Center for Research Computing (CRC) at the University of Notre
492     Dame. \newpage
493    
494     \bibliography{interfacial}
495    
496     \end{doublespace}
497     \end{document}
498