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1 \documentclass[11pt]{article}
2 \usepackage{amsmath}
3 \usepackage{amssymb}
4 \usepackage{times}
5 \usepackage{mathptm}
6 \usepackage{setspace}
7 \usepackage{float}
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10 %\usepackage{tabularx}
11 \usepackage{graphicx}
12 \usepackage{multirow}
13 %\usepackage{booktabs}
14 %\usepackage{bibentry}
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21 9.0in \textwidth 6.5in \brokenpenalty=10000
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23 % double space list of tables and figures
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30 \bibliographystyle{achemso}
31
32 \begin{document}
33
34
35 %%
36 %Introduction
37 % Experimental observations
38 % Previous work on Pt, CO, etc.
39 %
40 %Simulation Methodology
41 % FF (fits and parameters)
42 % MD (setup, equilibration, collection)
43 %
44 % Analysis of trajectories!!!
45 %Discussion
46 % CO preferences for specific locales
47 % CO-CO interactions
48 % Differences between Au & Pt
49 % Causes of 2_layer reordering in Pt
50 %Summary
51 %%
52
53 %Title
54 \title{Molecular Dynamics simulations of the surface reconstructions
55 of Pt(557) and Au(557) under exposure to CO}
56
57 \author{Joseph R. Michalka, Patrick W. McIntyre and J. Daniel
58 Gezelter\footnote{Corresponding author. \ Electronic mail: gezelter@nd.edu} \\
59 Department of Chemistry and Biochemistry,\\
60 University of Notre Dame\\
61 Notre Dame, Indiana 46556}
62
63 %Date
64 \date{Dec 15, 2012}
65
66 %authors
67
68 % make the title
69 \maketitle
70
71 \begin{doublespace}
72
73 \begin{abstract}
74
75 \end{abstract}
76
77 \newpage
78
79
80 \section{Introduction}
81 % Importance: catalytically active metals are important
82 % Sub: Knowledge of how their surface structure affects their ability to catalytically facilitate certain reactions is growing, but is more reactionary than predictive
83 % Sub: Designing catalysis is the future, and will play an important role in numerous processes (ones that are currently seen to be impractical, or at least inefficient)
84 % Theory can explore temperatures and pressures which are difficult to work with in experiments
85 % Sub: Also, easier to observe what is going on and provide reasons and explanations
86 %
87
88 Industrial catalysts usually consist of small particles exposing
89 different atomic terminations that exhibit a high concentration of
90 step, kink sites, and vacancies at the edges of the facets. These
91 sites are thought to be the locations of catalytic
92 activity.\cite{ISI:000083038000001,ISI:000083924800001} There is now
93 significant evidence to demonstrate that solid surfaces are often
94 structurally, compositionally, and chemically {\it modified} by
95 reactants under operating conditions.\cite{Tao2008,Tao:2010,Tao2011}
96 The coupling between surface oxidation state and catalytic activity
97 for CO oxidation on Pt, for instance, is widely
98 documented.\cite{Ertl08,Hendriksen:2002} Despite the well-documented
99 role of these effects on reactivity, the ability to capture or predict
100 them in atomistic models is currently somewhat limited. While these
101 effects are perhaps unsurprising on the highly disperse, multi-faceted
102 nanoscale particles that characterize industrial catalysts, they are
103 manifest even on ordered, well-defined surfaces. The Pt(557) surface,
104 for example, exhibits substantial and reversible restructuring under
105 exposure to moderate pressures of carbon monoxide.\cite{Tao:2010}
106
107 This work is part of an ongoing effort to understand the causes,
108 mechanisms and timescales for surface restructuring using molecular
109 simulation methods. Since the dynamics of the process is of
110 particular interest, we utilize classical molecular dynamic methods
111 with force fields that represent a compromise between chemical
112 accuracy and the computational efficiency necessary to observe the
113 process of interest.
114
115 Since restructuring occurs as a result of specific interactions of the catalyst
116 with adsorbates, two metals systems exposed to the same adsorbate, CO,
117 were examined in this work. The Pt(557) surface has already been shown to
118 reconstruct under certain conditions. The Au(557) surface, because of gold's
119 weaker interaction with CO, is less likely to undergo such a large reconstruction.
120 %Platinum molecular dynamics
121 %gold molecular dynamics
122
123
124
125 \section{Simulation Methods}
126 The challenge in modeling any solid/gas interface problem is the
127 development of a sufficiently general yet computationally tractable
128 model of the chemical interactions between the surface atoms and
129 adsorbates. Since the interfaces involved are quite large (10$^3$ -
130 10$^6$ atoms) and respond slowly to perturbations, {\it ab initio}
131 molecular dynamics
132 (AIMD),\cite{KRESSE:1993ve,KRESSE:1993qf,KRESSE:1994ul} Car-Parrinello
133 methods,\cite{CAR:1985bh,Izvekov:2000fv,Guidelli:2000fy} and quantum
134 mechanical potential energy surfaces remain out of reach.
135 Additionally, the ``bonds'' between metal atoms at a surface are
136 typically not well represented in terms of classical pairwise
137 interactions in the same way that bonds in a molecular material are,
138 nor are they captured by simple non-directional interactions like the
139 Coulomb potential. For this work, we have been using classical
140 molecular dynamics with potential energy surfaces that are
141 specifically tuned for transition metals. In particular, we use the
142 EAM potential for Au-Au and Pt-Pt interactions, while modeling the CO
143 using a model developed by Straub and Karplus for studying
144 photodissociation of CO from myoglobin.\cite{Straub} The Au-CO and Pt-CO
145 cross interactions were parameterized as part of this work.
146
147 \subsection{Metal-metal interactions}
148 Many of the potentials used for classical simulation of transition
149 metals are based on a non-pairwise additive functional of the local
150 electron density. The embedded atom method (EAM) is perhaps the best
151 known of these
152 methods,\cite{Daw84,Foiles86,Johnson89,Daw89,Plimpton93,Voter95a,Lu97,Alemany98}
153 but other models like the Finnis-Sinclair\cite{Finnis84,Chen90} and
154 the quantum-corrected Sutton-Chen method\cite{QSC,Qi99} have simpler
155 parameter sets. The glue model of Ercolessi {\it et al.} is among the
156 fastest of these density functional approaches.\cite{Ercolessi88} In
157 all of these models, atoms are conceptualized as a positively charged
158 core with a radially-decaying valence electron distribution. To
159 calculate the energy for embedding the core at a particular location,
160 the electron density due to the valence electrons at all of the other
161 atomic sites is computed at atom $i$'s location,
162 \begin{equation*}
163 \bar{\rho}_i = \sum_{j\neq i} \rho_j(r_{ij})
164 \end{equation*}
165 Here, $\rho_j(r_{ij})$ is the function that describes the distance
166 dependence of the valence electron distribution of atom $j$. The
167 contribution to the potential that comes from placing atom $i$ at that
168 location is then
169 \begin{equation*}
170 V_i = F[ \bar{\rho}_i ] + \sum_{j \neq i} \phi_{ij}(r_{ij})
171 \end{equation*}
172 where $F[ \bar{\rho}_i ]$ is an energy embedding functional, and
173 $\phi_{ij}(r_{ij})$ is an pairwise term that is meant to represent the
174 overlap of the two positively charged cores.
175
176 The {\it modified} embedded atom method (MEAM) adds angular terms to
177 the electron density functions and an angular screening factor to the
178 pairwise interaction between two
179 atoms.\cite{BASKES:1994fk,Lee:2000vn,Thijsse:2002ly,Timonova:2011ve}
180 MEAM has become widely used to simulate systems in which angular
181 interactions are important (e.g. silicon,\cite{Timonova:2011ve} bcc
182 metals,\cite{Lee:2001qf} and also interfaces.\cite{Beurden:2002ys})
183 MEAM presents significant additional computational costs, however.
184
185 The EAM, Finnis-Sinclair, MEAM, and the Quantum Sutton-Chen potentials
186 have all been widely used by the materials simulation community for
187 simulations of bulk and nanoparticle
188 properties,\cite{Chui:2003fk,Wang:2005qy,Medasani:2007uq}
189 melting,\cite{Belonoshko00,sankaranarayanan:155441,Sankaranarayanan:2005lr}
190 fracture,\cite{Shastry:1996qg,Shastry:1998dx} crack
191 propagation,\cite{BECQUART:1993rg} and alloying
192 dynamics.\cite{Shibata:2002hh} All of these potentials have their
193 strengths and weaknesses. One of the strengths common to all of the
194 methods is the relatively large library of metals for which these
195 potentials have been
196 parameterized.\cite{Foiles86,PhysRevB.37.3924,Rifkin1992,mishin99:_inter,mishin01:cu,mishin02:b2nial,zope03:tial_ap,mishin05:phase_fe_ni}
197
198 \subsection{CO}
199 Since one explanation for the strong surface CO repulsion on metals is
200 the large linear quadrupole moment of carbon monoxide, the model
201 chosen for this molecule exhibits this property in an efficient
202 manner. We used a model first proposed by Karplus and Straub to study
203 the photodissociation of CO from myoglobin.\cite{Straub} The Straub and
204 Karplus model is a rigid three site model which places a massless M
205 site at the center of mass along the CO bond. The geometry used along
206 with the interaction parameters are reproduced in Table 1. The effective
207 dipole moment, calculated from the assigned charges, is still
208 small (0.35 D) while the linear quadrupole (-2.40 D~\AA) is close
209 to the experimental (-2.63 D~\AA)\cite{QuadrupoleCO} and quantum
210 mechanical predictions (-2.46 D~\AA)\cite{QuadrupoleCOCalc}.
211 %CO Table
212 \begin{table}[H]
213 \caption{Positions, $\sigma$, $\epsilon$ and charges for CO geometry
214 and self-interactions\cite{Straub}. Distances are in \AA~, energies are
215 in kcal/mol, and charges are in $e$.}
216 \centering
217 \begin{tabular}{| c | c | ccc |}
218 \hline
219 \multicolumn{5}{|c|}{\textbf{Self-Interactions}}\\
220 \hline
221 & {\it z} & $\sigma$ & $\epsilon$ & q\\
222 \hline
223 \textbf{C} & -0.6457 & 0.0262 & 3.83 & -0.75 \\
224 \textbf{O} & 0.4843 & 0.1591 & 3.12 & -0.85 \\
225 \textbf{M} & 0.0 & - & - & 1.6 \\
226 \hline
227 \end{tabular}
228 \end{table}
229
230 \subsection{Cross-Interactions}
231
232 One hurdle that must be overcome in classical molecular simulations
233 is the proper parameterization of the potential interactions present
234 in the system. Since the adsorption of CO onto a platinum surface has been
235 the focus of many experimental \cite{Yeo, Hopster:1978, Ertl:1977, Kelemen:1979}
236 and theoretical studies \cite{Beurden:2002ys,Pons:1986,Deshlahra:2009,Feibelman:2001,Mason:2004}
237 there is a large amount of data in the literature to fit too. We started with parameters
238 reported by Korzeniewski et al. \cite{Pons:1986} and then
239 modified them to ensure that the Pt-CO interaction favored
240 an atop binding position for the CO upon the Pt surface. This
241 constraint led to the binding energies being on the higher side
242 of reported values. Following the method laid out by Korzeniewski,
243 the Pt-C interaction was fit to a strong Lennard-Jones 12-6
244 interaction to mimic binding, while the Pt-O interaction
245 was parameterized to a Morse potential with a large $r_o$
246 to contribute a weak repulsion. The resultant potential-energy
247 surface suitably recovers the calculated Pt-C bond length ( 1.6\AA)\cite{Beurden:2002ys} and affinity
248 for the atop binding position.\cite{Deshlahra:2012, Hopster:1978}
249
250 %where did you actually get the functionals for citation?
251 %scf calculations, so initial relaxation was of the four layers, but two layers weren't kept fixed, I don't think
252 %same cutoff for slab and slab + CO ? seems low, although feibelmen had values around there...
253 The Au-C and Au-O cross-interactions were fit using Lennard-Jones and
254 Morse potentials, respectively, to reproduce Au-CO binding energies.
255
256 The fits were refined against gas-surface calculations using DFT with
257 a periodic supercell plane-wave basis approach, as implemented in the
258 {\sc Quantum ESPRESSO} package.\cite{QE-2009} Electron cores are
259 described with the projector augmented-wave (PAW)
260 method,\cite{PhysRevB.50.17953,PhysRevB.59.1758} with plane waves
261 included to an energy cutoff of 20 Ry. Electronic energies are
262 computed with the PBE implementation of the generalized gradient
263 approximation (GGA) for gold, carbon, and oxygen that was constructed
264 by Rappe, Rabe, Kaxiras, and Joannopoulos.\cite{Perdew_GGA,RRKJ_PP}
265 Ionic relaxations were performed until the energy difference between
266 subsequent steps was less than 0.0001 eV. In testing the CO-Au
267 interaction, Au(111) supercells were constructed of four layers of 4
268 Au x 2 Au surface planes and separated from vertical images by six
269 layers of vacuum space. The surface atoms were all allowed to relax.
270 Supercell calculations were performed nonspin-polarized, and energies
271 were converged to within 0.03 meV per Au atom with a 4 x 4 x 4
272 Monkhorst-Pack\cite{Monkhorst:1976,PhysRevB.13.5188} {\bf k}-point
273 sampling of the first Brillouin zone. The relaxed gold slab was then
274 used in numerous single point calculations with CO at various heights
275 (and angles relative to the surface) to allow fitting of the empirical
276 force field.
277
278 %Hint at future work
279 The fit parameter sets employed in this work are shown in Table 2 and their
280 reproduction of the binding energies are displayed in Table 3. Currently,
281 charge transfer is not being treated in this system, however, that is a goal
282 for future work as the effect has been seen to affect binding energies and
283 binding site preferences. \cite{Deshlahra:2012}
284
285
286
287
288 \subsection{Construction and Equilibration of 557 Metal interfaces}
289
290 Our model systems are composed of approximately 4000 metal atoms
291 cut along the 557 plane so that they are periodic in the {\it x} and {\it y}
292 directions exposing the 557 plane in the {\it z} direction. Runs at various
293 temperatures ranging from 300~K to 1200~K were started with the intent
294 of viewing relative stability of the surface when CO was not present in the
295 system. Owing to the different melting points (1337~K for Au and 2045~K for Pt),
296 the bare crystal systems were initially run in the Canonical ensemble at
297 800~K and 1000~K respectively for 100 ps. Various amounts of CO were
298 placed in the vacuum region, which upon full adsorption to the surface
299 corresponded to 5\%, 25\%, 33\%, and 50\% coverages. Because of the
300 high temperature and the difference in binding energies, the platinum systems
301 very rarely had CO that was not adsorbed to the surface whereas the gold systems
302 often had a substantial minority of CO away from the surface.
303 These systems were again allowed to reach thermal equilibrium before being run in the
304 microcanonical ensemble. All of the systems examined in this work were
305 run for at least 40 ns. A subset that were undergoing interesting effects
306 have been allowed to continue running with one system approaching 200 ns.
307 All simulations were run using the open source molecular dynamics package, OpenMD. \cite{Ewald, OOPSE}
308
309
310
311
312
313
314 %\subsection{System}
315 %Once equilibration was reached, the systems were exposed to various sub-monolayer coverage of CO: $0, \frac{1}{10}, \frac{1}{4}, \frac{1}{3},\frac{1}{2}$. The CO was started many \AA~above the surface with random velocity and rotational velocity vectors sampling from a Gaussian distribution centered on the temperature of the equilibrated metal block. Full adsorption occurred over the period of approximately 10 ps for Pt, while the binding energy between Au and CO is smaller and led to an incomplete adsorption. The metal-metal interactions were treated using the Embedded Atom Method while the Pt-CO and Au-CO interactions were fit to experimental data and quantum calculations. The raised temperature helped shorten the length of the simulations by allowing the activation barrier of reconstruction to be more easily overcome. A few runs at lower temperatures showed the very beginnings of reconstructions, but their simulation lengths limited their usefulness.
316
317
318 %Table of Parameters
319 %Pt Parameter Set 9
320 %Au Parameter Set 35
321 \begin{table}[H]
322 \caption{Best fit parameters for metal-adsorbate interactions. Distances are in \AA~and energies are in kcal/mol}
323 \centering
324 \begin{tabular}{| c | cc | c | ccc |}
325 \hline
326 \multicolumn{7}{| c |}{\textbf{Cross-Interactions} }\\
327 \hline
328 & $\sigma$ & $\epsilon$ & & $r$ & $D$ & $\gamma$ \\
329 \hline
330 \textbf{Pt-C} & 1.3 & 15 & \textbf{Pt-O} & 3.8 & 3.0 & 1 \\
331 \textbf{Au-C} & 1.9 & 6.5 & \textbf{Au-O} & 3.8 & 0.37 & 0.9\\
332
333 \hline
334 \end{tabular}
335 \end{table}
336
337 %Table of energies
338 \begin{table}[H]
339 \caption{Adsorption energies in eV}
340 \centering
341 \begin{tabular}{| c | cc |}
342 \hline
343 & Calc. & Exp. \\
344 \hline
345 \textbf{Pt-CO} & -1.9 & -1.4~\cite{Kelemen:1979}-- -1.9~\cite{Yeo} \\
346 \textbf{Au-CO} & -0.39 & -0.40~\cite{TPD_Gold} \\
347 \hline
348 \end{tabular}
349 \end{table}
350
351
352
353
354
355
356 % Just results, leave discussion for discussion section
357 \section{Results}
358 \subsection{Diffusion}
359 An ideal metal surface displaying a low-energy facet, a (111) face for
360 instance, is unlikely to experience much surface diffusion because of
361 the large energy barrier associated with atoms 'lifting' from the top
362 layer to then be able to explore the surface. Rougher surfaces, those
363 that already contain numerous adatoms, step edges, and kinks, should
364 have concomitantly higher surface diffusion rates. Tao et al. showed
365 that the platinum 557 surface undergoes two separate reconstructions
366 upon CO adsorption. \cite{Tao:2010} The first reconstruction involves a
367 doubling of the step edge height which is accomplished by a doubling
368 of the plateau length. The second reconstruction led to the formation of
369 triangular motifs stretching across the lengthened plateaus.
370
371 As shown in Figure 2, over a period of approximately 100 ns, the surface
372 has reconstructed from a 557 surface by doubling the step height and
373 step length. Focusing on only the platinum, or gold, atoms that were
374 deemed mobile on the surface, an analysis of the surface diffusion was
375 performed. A particle was considered mobile once it had traveled more
376 than 2~\AA between snapshots. This immediately eliminates all of the
377 bulk metal and greatly limits the number of surface atoms examined.
378 Since diffusion on a surface is strongly affected by overcoming energy
379 barriers, the diffusion parallel to the step edge axis was determined
380 separately from the diffusion perpendicular to the step edge. The results
381 at various coverages on both platinum and gold are shown in Table 4.
382
383 %While an ideal metallic surface is unlikely to experience much surface diffusion, high-index surfaces have large numbers of low-coordinated atoms which have a much easier time overcoming the energetic barriers limiting diffusion, leading to easier surface reconstructions. Surface movement was divided between the parallel ($\parallel$) and perpendicular ($\perp$) directions relative to the step edge. We were then able to calculate diffusion constants as a function of CO coverage. As can be seen in Table 4, the presence and amount of CO directly affects the diffusion constants of surface platinum atoms. The presence of two 50\% coverage systems is to show how the diffusion process is affected by time. The majority of the systems were run for approximately 50 ns while the half monolayer system has been running continuously. The lowered diffusion constant at longer run times will be examined in-depth in the discussion section.
384
385 \begin{figure}[H]
386 \includegraphics[scale=0.6]{DiffusionComparison_error.png}
387 \caption{Diffusion parallel to the step edge will always be higher than that perpendicular to the edge because of the lower energy barrier associated with going from approximately 7 nearest neighbors to 5, as compared to the 3 of an adatom. Additionally, the observed maximum and subsequent decrease for the Pt system suggests that the CO self-interactions are playing a significant role with regards to movement of the platinum atoms around and more importantly across the surface. }
388 \end{figure}
389
390 %Table of Diffusion Constants
391 %Add gold?M
392 \begin{table}[H]
393 \caption{Platinum and gold diffusion constants parallel and perpendicular to the 557 step edge. As the coverage increases, the diffusion constants parallel and perpendicular to the step edge both initially increase and then decrease slightly. Units are \AA\textsuperscript{2}/ns}
394 \centering
395 \begin{tabular}{| c | cc | cc | c |}
396 \hline
397 \textbf{System Coverage} & $\mathbf{D}_{\parallel}$ & $\mathbf{D}_{\perp}$ & $\mathbf{D}_{\parallel}$ & $\mathbf{D}_{\perp}$ & \textbf{Time (ns)}\\
398 \hline
399 &\multicolumn{2}{c|}{\textbf{Platinum}}&\multicolumn{2}{c|}{\textbf{Gold}} & \\
400 \hline
401 50\% & 4.32 $\pm$ 0.02 & 1.185 $\pm$ 0.008 & 1.72 $\pm$ 0.02 & 0.455 $\pm$ 0.006 & 40 \\
402 33\% & 5.18 $\pm$ 0.03 & 1.999 $\pm$ 0.005 & 1.95 $\pm$ 0.02 & 0.337 $\pm$ 0.004 & 40 \\
403 25\% & 5.01 $\pm$ 0.02 & 1.574 $\pm$ 0.004 & 1.26 $\pm$ 0.03 & 0.377 $\pm$ 0.006 & 40 \\
404 5\% & 3.61 $\pm$ 0.02 & 0.355 $\pm$ 0.002 & 1.84 $\pm$ 0.03 & 0.169 $\pm$ 0.004 & 40 \\
405 0\% & 3.27 $\pm$ 0.02 & 0.147 $\pm$ 0.004 & 1.50 $\pm$ 0.02 & 0.194 $\pm$ 0.002 & 40 \\
406 \hline
407 \end{tabular}
408 \end{table}
409
410
411
412 %Discussion
413 \section{Discussion}
414 Comparing the results from simulation to those reported previously by Tao et al. the similarities in the platinum and CO system are quite strong. As shown in figure 1, the simulated platinum system under a CO atmosphere will restructure slightly by doubling the terrace heights. The restructuring appears to occur slowly, one to two platinum atoms at a time. Looking at individual snapshots, these adatoms tend to either rise on top of the plateau or break away from the step edge and then diffuse perpendicularly to the step direction until reaching another step edge. This combination of growth and decay of the step edges appears to be in somewhat of a state of dynamic equilibrium. However, once two previously separated edges meet as shown in figure 1.B, this point tends to act as a focus or growth point for the rest of the edge to meet up, akin to that of a zipper. From the handful of cases where a double layer was formed during the simulation, measuring from the initial appearance of a growth point, the double layer tends to be fully formed within $\sim$~35 ns.
415
416 \subsection{Diffusion}
417 As shown in the results section, the diffusion parallel to the step edge tends to be much faster than that perpendicular to the step edge. Additionally, the coverage of CO appears to play a slight role in relative rates of diffusion, as shown in Table 4. Thus, the bottleneck of the double layer formation appears to be the initial formation of this growth point, which seems to be somewhat of a stochastic event. Once it appears, parallel diffusion, along the now slightly angled step edge, will allow for a faster formation of the double layer than if the entire process were dependent on only perpendicular diffusion across the plateaus. Thus, the larger $D_{\perp}$, the more likely a growth point is to be formed. One driving force behind this reconstruction appears to be the lowering of surface energy that occurs by doubling the terrace widths. (I'm not really proving this... I have the surface flatness to show it, but surface energy?)
418 \\
419 \\
420 %Evolution of surface
421 \begin{figure}[H]
422 \includegraphics[scale=0.5]{ProgressionOfDoubleLayerFormation_yellowCircle.png}
423 \caption{Four snapshots of the $\frac{1}{2}$ monolayer system at various times a) 258 ps b) 19 ns c) 31.2 ns and d) 86.1 ns. Slight disruption of the surface occurs fairly quickly. However, the doubling of the layers seems to be very dependent on the initial linking of two separate step edges. The focal point in b, appears to be a growth spot for the rest of the double layer.}
424 \end{figure}
425
426
427
428
429 %Peaks!
430 \begin{figure}[H]
431 \includegraphics[scale=0.25]{doublePeaks_noCO.png}
432 \caption{}
433 \end{figure}
434 \section{Conclusion}
435
436
437 \section{Acknowledgments}
438 Support for this project was provided by the National Science
439 Foundation under grant CHE-0848243 and by the Center for Sustainable
440 Energy at Notre Dame (cSEND). Computational time was provided by the
441 Center for Research Computing (CRC) at the University of Notre Dame.
442
443 \newpage
444 \bibliography{firstTryBibliography}
445 \end{doublespace}
446 \end{document}