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1 gezelter 3808 \documentclass[11pt]{article}
2     \usepackage{amsmath}
3     \usepackage{amssymb}
4 gezelter 3818 \usepackage{times}
5     \usepackage{mathptm}
6 jmichalk 3802 \usepackage{setspace}
7 gezelter 3818 \usepackage{float}
8 gezelter 3808 \usepackage{caption}
9 jmichalk 3817
10 gezelter 3808 %\usepackage{tabularx}
11     \usepackage{graphicx}
12     \usepackage{multirow}
13     %\usepackage{booktabs}
14     %\usepackage{bibentry}
15     %\usepackage{mathrsfs}
16     \usepackage[square, comma, sort&compress]{natbib}
17     \usepackage{url}
18     \pagestyle{plain} \pagenumbering{arabic} \oddsidemargin 0.0cm
19     \evensidemargin 0.0cm \topmargin -21pt \headsep 10pt \textheight
20     9.0in \textwidth 6.5in \brokenpenalty=10000
21 jmichalk 3802
22 gezelter 3808 % double space list of tables and figures
23 gezelter 3820 %\AtBeginDelayedFloats{\renewcomand{\baselinestretch}{1.66}}
24 gezelter 3808 \setlength{\abovecaptionskip}{20 pt}
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26    
27 gezelter 3820 \bibpunct{}{}{,}{s}{}{;}
28 gezelter 3808 \bibliographystyle{achemso}
29    
30     \begin{document}
31    
32    
33 jmichalk 3802 %%
34     %Introduction
35     % Experimental observations
36     % Previous work on Pt, CO, etc.
37     %
38     %Simulation Methodology
39     % FF (fits and parameters)
40     % MD (setup, equilibration, collection)
41     %
42     % Analysis of trajectories!!!
43     %Discussion
44     % CO preferences for specific locales
45     % CO-CO interactions
46     % Differences between Au & Pt
47     % Causes of 2_layer reordering in Pt
48     %Summary
49     %%
50    
51     %Title
52 gezelter 3818 \title{Molecular Dynamics simulations of the surface reconstructions
53     of Pt(557) and Au(557) under exposure to CO}
54    
55 jmichalk 3816 \author{Joseph R. Michalka, Patrick W. McIntyre and J. Daniel
56 gezelter 3808 Gezelter\footnote{Corresponding author. \ Electronic mail: gezelter@nd.edu} \\
57     Department of Chemistry and Biochemistry,\\
58     University of Notre Dame\\
59     Notre Dame, Indiana 46556}
60 gezelter 3818
61 jmichalk 3802 %Date
62 gezelter 3818 \date{Dec 15, 2012}
63    
64 jmichalk 3802 %authors
65 gezelter 3808
66 jmichalk 3802 % make the title
67 jmichalk 3817 \maketitle
68 jmichalk 3802
69 gezelter 3808 \begin{doublespace}
70 jmichalk 3802
71 gezelter 3808 \begin{abstract}
72 jmichalk 3802
73 gezelter 3808 \end{abstract}
74 jmichalk 3802
75 gezelter 3808 \newpage
76    
77    
78 jmichalk 3802 \section{Introduction}
79     % Importance: catalytically active metals are important
80     % Sub: Knowledge of how their surface structure affects their ability to catalytically facilitate certain reactions is growing, but is more reactionary than predictive
81     % 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)
82     % Theory can explore temperatures and pressures which are difficult to work with in experiments
83     % Sub: Also, easier to observe what is going on and provide reasons and explanations
84     %
85    
86 gezelter 3808 Industrial catalysts usually consist of small particles exposing
87     different atomic terminations that exhibit a high concentration of
88     step, kink sites, and vacancies at the edges of the facets. These
89 jmichalk 3810 sites are thought to be the locations of catalytic
90 gezelter 3808 activity.\cite{ISI:000083038000001,ISI:000083924800001} There is now
91     significant evidence to demonstrate that solid surfaces are often
92     structurally, compositionally, and chemically {\it modified} by
93     reactants under operating conditions.\cite{Tao2008,Tao:2010,Tao2011}
94     The coupling between surface oxidation state and catalytic activity
95     for CO oxidation on Pt, for instance, is widely
96     documented.\cite{Ertl08,Hendriksen:2002} Despite the well-documented
97     role of these effects on reactivity, the ability to capture or predict
98     them in atomistic models is currently somewhat limited. While these
99     effects are perhaps unsurprising on the highly disperse, multi-faceted
100     nanoscale particles that characterize industrial catalysts, they are
101     manifest even on ordered, well-defined surfaces. The Pt(557) surface,
102     for example, exhibits substantial and reversible restructuring under
103     exposure to moderate pressures of carbon monoxide.\cite{Tao:2010}
104 jmichalk 3802
105 gezelter 3808 This work is part of an ongoing effort to understand the causes,
106     mechanisms and timescales for surface restructuring using molecular
107     simulation methods. Since the dynamics of the process is of
108     particular interest, we utilize classical molecular dynamic methods
109     with force fields that represent a compromise between chemical
110     accuracy and the computational efficiency necessary to observe the
111     process of interest.
112    
113 jmichalk 3811 Since restructuring occurs as a result of specific interactions of the catalyst
114     with adsorbates, two metals systems exposed to the same adsorbate, CO,
115     were examined in this work. The Pt(557) surface has already been shown to
116 jmichalk 3812 reconstruct under certain conditions. The Au(557) surface, because of gold's
117     weaker interaction with CO, is less likely to undergo such a large reconstruction.
118 jmichalk 3811 %Platinum molecular dynamics
119     %gold molecular dynamics
120 jmichalk 3802
121    
122    
123     \section{Simulation Methods}
124 gezelter 3808 The challenge in modeling any solid/gas interface problem is the
125     development of a sufficiently general yet computationally tractable
126     model of the chemical interactions between the surface atoms and
127     adsorbates. Since the interfaces involved are quite large (10$^3$ -
128     10$^6$ atoms) and respond slowly to perturbations, {\it ab initio}
129     molecular dynamics
130     (AIMD),\cite{KRESSE:1993ve,KRESSE:1993qf,KRESSE:1994ul} Car-Parrinello
131     methods,\cite{CAR:1985bh,Izvekov:2000fv,Guidelli:2000fy} and quantum
132     mechanical potential energy surfaces remain out of reach.
133     Additionally, the ``bonds'' between metal atoms at a surface are
134     typically not well represented in terms of classical pairwise
135     interactions in the same way that bonds in a molecular material are,
136     nor are they captured by simple non-directional interactions like the
137     Coulomb potential. For this work, we have been using classical
138     molecular dynamics with potential energy surfaces that are
139     specifically tuned for transition metals. In particular, we use the
140     EAM potential for Au-Au and Pt-Pt interactions, while modeling the CO
141     using a model developed by Straub and Karplus for studying
142     photodissociation of CO from myoglobin.\cite{Straub} The Au-CO and Pt-CO
143     cross interactions were parameterized as part of this work.
144    
145     \subsection{Metal-metal interactions}
146     Many of the potentials used for classical simulation of transition
147     metals are based on a non-pairwise additive functional of the local
148     electron density. The embedded atom method (EAM) is perhaps the best
149     known of these
150     methods,\cite{Daw84,Foiles86,Johnson89,Daw89,Plimpton93,Voter95a,Lu97,Alemany98}
151     but other models like the Finnis-Sinclair\cite{Finnis84,Chen90} and
152     the quantum-corrected Sutton-Chen method\cite{QSC,Qi99} have simpler
153     parameter sets. The glue model of Ercolessi {\it et al.} is among the
154     fastest of these density functional approaches.\cite{Ercolessi88} In
155     all of these models, atoms are conceptualized as a positively charged
156     core with a radially-decaying valence electron distribution. To
157     calculate the energy for embedding the core at a particular location,
158     the electron density due to the valence electrons at all of the other
159     atomic sites is computed at atom $i$'s location,
160     \begin{equation*}
161     \bar{\rho}_i = \sum_{j\neq i} \rho_j(r_{ij})
162     \end{equation*}
163     Here, $\rho_j(r_{ij})$ is the function that describes the distance
164     dependence of the valence electron distribution of atom $j$. The
165     contribution to the potential that comes from placing atom $i$ at that
166     location is then
167     \begin{equation*}
168     V_i = F[ \bar{\rho}_i ] + \sum_{j \neq i} \phi_{ij}(r_{ij})
169     \end{equation*}
170     where $F[ \bar{\rho}_i ]$ is an energy embedding functional, and
171     $\phi_{ij}(r_{ij})$ is an pairwise term that is meant to represent the
172     overlap of the two positively charged cores.
173 jmichalk 3807
174 gezelter 3808 The {\it modified} embedded atom method (MEAM) adds angular terms to
175     the electron density functions and an angular screening factor to the
176     pairwise interaction between two
177     atoms.\cite{BASKES:1994fk,Lee:2000vn,Thijsse:2002ly,Timonova:2011ve}
178     MEAM has become widely used to simulate systems in which angular
179     interactions are important (e.g. silicon,\cite{Timonova:2011ve} bcc
180     metals,\cite{Lee:2001qf} and also interfaces.\cite{Beurden:2002ys})
181     MEAM presents significant additional computational costs, however.
182 jmichalk 3807
183 gezelter 3808 The EAM, Finnis-Sinclair, MEAM, and the Quantum Sutton-Chen potentials
184     have all been widely used by the materials simulation community for
185     simulations of bulk and nanoparticle
186     properties,\cite{Chui:2003fk,Wang:2005qy,Medasani:2007uq}
187     melting,\cite{Belonoshko00,sankaranarayanan:155441,Sankaranarayanan:2005lr}
188     fracture,\cite{Shastry:1996qg,Shastry:1998dx} crack
189     propagation,\cite{BECQUART:1993rg} and alloying
190     dynamics.\cite{Shibata:2002hh} All of these potentials have their
191     strengths and weaknesses. One of the strengths common to all of the
192     methods is the relatively large library of metals for which these
193     potentials have been
194     parameterized.\cite{Foiles86,PhysRevB.37.3924,Rifkin1992,mishin99:_inter,mishin01:cu,mishin02:b2nial,zope03:tial_ap,mishin05:phase_fe_ni}
195    
196 jmichalk 3802 \subsection{CO}
197 gezelter 3808 Since one explanation for the strong surface CO repulsion on metals is
198     the large linear quadrupole moment of carbon monoxide, the model
199     chosen for this molecule exhibits this property in an efficient
200     manner. We used a model first proposed by Karplus and Straub to study
201     the photodissociation of CO from myoglobin.\cite{Straub} The Straub and
202     Karplus model is a rigid three site model which places a massless M
203 jmichalk 3812 site at the center of mass along the CO bond. The geometry used along
204     with the interaction parameters are reproduced in Table 1. The effective
205     dipole moment, calculated from the assigned charges, is still
206 jmichalk 3810 small (0.35 D) while the linear quadrupole (-2.40 D~\AA) is close
207 jmichalk 3812 to the experimental (-2.63 D~\AA)\cite{QuadrupoleCO} and quantum
208     mechanical predictions (-2.46 D~\AA)\cite{QuadrupoleCOCalc}.
209 jmichalk 3802 %CO Table
210     \begin{table}[H]
211 jmichalk 3817 \caption{Positions, $\sigma$, $\epsilon$ and charges for CO geometry
212     and self-interactions\cite{Straub}. Distances are in \AA~, energies are
213     in kcal/mol, and charges are in $e$.}
214 jmichalk 3802 \centering
215 jmichalk 3810 \begin{tabular}{| c | c | ccc |}
216 jmichalk 3802 \hline
217 jmichalk 3810 \multicolumn{5}{|c|}{\textbf{Self-Interactions}}\\
218 jmichalk 3802 \hline
219 jmichalk 3814 & {\it z} & $\sigma$ & $\epsilon$ & q\\
220 jmichalk 3802 \hline
221 jmichalk 3814 \textbf{C} & -0.6457 & 0.0262 & 3.83 & -0.75 \\
222     \textbf{O} & 0.4843 & 0.1591 & 3.12 & -0.85 \\
223     \textbf{M} & 0.0 & - & - & 1.6 \\
224 jmichalk 3802 \hline
225     \end{tabular}
226     \end{table}
227 gezelter 3808
228 jmichalk 3802 \subsection{Cross-Interactions}
229    
230 jmichalk 3811 One hurdle that must be overcome in classical molecular simulations
231 jmichalk 3812 is the proper parameterization of the potential interactions present
232     in the system. Since the adsorption of CO onto a platinum surface has been
233     the focus of many experimental \cite{Yeo, Hopster:1978, Ertl:1977, Kelemen:1979}
234     and theoretical studies \cite{Beurden:2002ys,Pons:1986,Deshlahra:2009,Feibelman:2001,Mason:2004}
235     there is a large amount of data in the literature to fit too. We started with parameters
236     reported by Korzeniewski et al. \cite{Pons:1986} and then
237 jmichalk 3811 modified them to ensure that the Pt-CO interaction favored
238 jmichalk 3812 an atop binding position for the CO upon the Pt surface. This
239     constraint led to the binding energies being on the higher side
240     of reported values. Following the method laid out by Korzeniewski,
241     the Pt-C interaction was fit to a strong Lennard-Jones 12-6
242     interaction to mimic binding, while the Pt-O interaction
243     was parameterized to a Morse potential with a large $r_o$
244     to contribute a weak repulsion. The resultant potential-energy
245     surface suitably recovers the calculated Pt-C bond length ( 1.6\AA)\cite{Beurden:2002ys} and affinity
246 jmichalk 3811 for the atop binding position.\cite{Deshlahra:2012, Hopster:1978}
247    
248 jmichalk 3812 %where did you actually get the functionals for citation?
249     %scf calculations, so initial relaxation was of the four layers, but two layers weren't kept fixed, I don't think
250     %same cutoff for slab and slab + CO ? seems low, although feibelmen had values around there...
251 gezelter 3818 The Au-C and Au-O cross-interactions were fit using Lennard-Jones and
252     Morse potentials, respectively, to reproduce Au-CO binding energies.
253 jmichalk 3811
254 gezelter 3818 The fits were refined against gas-surface calculations using DFT with
255     a periodic supercell plane-wave basis approach, as implemented in the
256     {\sc Quantum ESPRESSO} package.\cite{QE-2009} Electron cores are
257     described with the projector augmented-wave (PAW)
258     method,\cite{PhysRevB.50.17953,PhysRevB.59.1758} with plane waves
259     included to an energy cutoff of 20 Ry. Electronic energies are
260     computed with the PBE implementation of the generalized gradient
261     approximation (GGA) for gold, carbon, and oxygen that was constructed
262     by Rappe, Rabe, Kaxiras, and Joannopoulos.\cite{Perdew_GGA,RRKJ_PP}
263     Ionic relaxations were performed until the energy difference between
264     subsequent steps was less than 0.0001 eV. In testing the CO-Au
265     interaction, Au(111) supercells were constructed of four layers of 4
266     Au x 2 Au surface planes and separated from vertical images by six
267     layers of vacuum space. The surface atoms were all allowed to relax.
268     Supercell calculations were performed nonspin-polarized, and energies
269     were converged to within 0.03 meV per Au atom with a 4 x 4 x 4
270     Monkhorst-Pack\cite{Monkhorst:1976,PhysRevB.13.5188} {\bf k}-point
271     sampling of the first Brillouin zone. The relaxed gold slab was then
272     used in numerous single point calculations with CO at various heights
273     (and angles relative to the surface) to allow fitting of the empirical
274     force field.
275    
276 jmichalk 3812 %Hint at future work
277     The fit parameter sets employed in this work are shown in Table 2 and their
278     reproduction of the binding energies are displayed in Table 3. Currently,
279     charge transfer is not being treated in this system, however, that is a goal
280     for future work as the effect has been seen to affect binding energies and
281     binding site preferences. \cite{Deshlahra:2012}
282 jmichalk 3811
283    
284    
285 jmichalk 3812
286 gezelter 3808 \subsection{Construction and Equilibration of 557 Metal interfaces}
287 jmichalk 3802
288 jmichalk 3813 Our model systems are composed of approximately 4000 metal atoms
289     cut along the 557 plane so that they are periodic in the {\it x} and {\it y}
290     directions exposing the 557 plane in the {\it z} direction. Runs at various
291     temperatures ranging from 300~K to 1200~K were started with the intent
292     of viewing relative stability of the surface when CO was not present in the
293     system. Owing to the different melting points (1337~K for Au and 2045~K for Pt),
294     the bare crystal systems were initially run in the Canonical ensemble at
295     800~K and 1000~K respectively for 100 ps. Various amounts of CO were
296     placed in the vacuum region, which upon full adsorption to the surface
297 jmichalk 3816 corresponded to 5\%, 25\%, 33\%, and 50\% coverages. Because of the
298     high temperature and the difference in binding energies, the platinum systems
299     very rarely had CO that was not adsorbed to the surface whereas the gold systems
300     often had a substantial minority of CO away from the surface.
301     These systems were again allowed to reach thermal equilibrium before being run in the
302 jmichalk 3813 microcanonical ensemble. All of the systems examined in this work were
303     run for at least 40 ns. A subset that were undergoing interesting effects
304     have been allowed to continue running with one system approaching 200 ns.
305     All simulations were run using the open source molecular dynamics package, OpenMD. \cite{Ewald, OOPSE}
306 jmichalk 3802
307    
308 gezelter 3808
309    
310    
311    
312 jmichalk 3802 %\subsection{System}
313     %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.
314    
315    
316     %Table of Parameters
317     %Pt Parameter Set 9
318     %Au Parameter Set 35
319     \begin{table}[H]
320     \caption{Best fit parameters for metal-adsorbate interactions. Distances are in \AA~and energies are in kcal/mol}
321     \centering
322     \begin{tabular}{| c | cc | c | ccc |}
323     \hline
324     \multicolumn{7}{| c |}{\textbf{Cross-Interactions} }\\
325     \hline
326     & $\sigma$ & $\epsilon$ & & $r$ & $D$ & $\gamma$ \\
327     \hline
328     \textbf{Pt-C} & 1.3 & 15 & \textbf{Pt-O} & 3.8 & 3.0 & 1 \\
329     \textbf{Au-C} & 1.9 & 6.5 & \textbf{Au-O} & 3.8 & 0.37 & 0.9\\
330    
331     \hline
332     \end{tabular}
333     \end{table}
334    
335     %Table of energies
336     \begin{table}[H]
337 jmichalk 3805 \caption{Adsorption energies in eV}
338 jmichalk 3802 \centering
339     \begin{tabular}{| c | cc |}
340     \hline
341     & Calc. & Exp. \\
342     \hline
343 jmichalk 3811 \textbf{Pt-CO} & -1.9 & -1.4~\cite{Kelemen:1979}-- -1.9~\cite{Yeo} \\
344 jmichalk 3817 \textbf{Au-CO} & -0.39 & -0.40~\cite{TPD_Gold} \\
345 jmichalk 3802 \hline
346     \end{tabular}
347     \end{table}
348    
349    
350    
351    
352    
353    
354     % Just results, leave discussion for discussion section
355     \section{Results}
356     \subsection{Diffusion}
357 jmichalk 3817 An ideal metal surface displaying a low-energy facet, a (111) face for
358     instance, is unlikely to experience much surface diffusion because of
359     the large energy barrier associated with atoms 'lifting' from the top
360     layer to then be able to explore the surface. Rougher surfaces, those
361     that already contain numerous adatoms, step edges, and kinks, should
362     have concomitantly higher surface diffusion rates. Tao et al. showed
363     that the platinum 557 surface undergoes two separate reconstructions
364     upon CO adsorption. \cite{Tao:2010} The first reconstruction involves a
365     doubling of the step edge height which is accomplished by a doubling
366     of the plateau length. The second reconstruction led to the formation of
367     triangular motifs stretching across the lengthened plateaus.
368 jmichalk 3802
369 jmichalk 3817 As shown in Figure 2, over a period of approximately 100 ns, the surface
370     has reconstructed from a 557 surface by doubling the step height and
371     step length. Focusing on only the platinum, or gold, atoms that were
372     deemed mobile on the surface, an analysis of the surface diffusion was
373     performed. A particle was considered mobile once it had traveled more
374     than 2~\AA between snapshots. This immediately eliminates all of the
375     bulk metal and greatly limits the number of surface atoms examined.
376     Since diffusion on a surface is strongly affected by overcoming energy
377     barriers, the diffusion parallel to the step edge axis was determined
378     separately from the diffusion perpendicular to the step edge. The results
379     at various coverages on both platinum and gold are shown in Table 4.
380    
381     %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.
382    
383 jmichalk 3816 \begin{figure}[H]
384     \includegraphics[scale=0.6]{DiffusionComparison_error.png}
385     \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. }
386     \end{figure}
387    
388 jmichalk 3802 %Table of Diffusion Constants
389     %Add gold?M
390     \begin{table}[H]
391 jmichalk 3814 \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}
392 jmichalk 3802 \centering
393 jmichalk 3814 \begin{tabular}{| c | cc | cc | c |}
394 jmichalk 3802 \hline
395 jmichalk 3814 \textbf{System Coverage} & $\mathbf{D}_{\parallel}$ & $\mathbf{D}_{\perp}$ & $\mathbf{D}_{\parallel}$ & $\mathbf{D}_{\perp}$ & \textbf{Time (ns)}\\
396 jmichalk 3802 \hline
397 jmichalk 3814 &\multicolumn{2}{c|}{\textbf{Platinum}}&\multicolumn{2}{c|}{\textbf{Gold}} & \\
398 jmichalk 3802 \hline
399 jmichalk 3814 50\% & 4.32 $\pm$ 0.02 & 1.185 $\pm$ 0.008 & 1.72 $\pm$ 0.02 & 0.455 $\pm$ 0.006 & 40 \\
400     33\% & 5.18 $\pm$ 0.03 & 1.999 $\pm$ 0.005 & 1.95 $\pm$ 0.02 & 0.337 $\pm$ 0.004 & 40 \\
401     25\% & 5.01 $\pm$ 0.02 & 1.574 $\pm$ 0.004 & 1.26 $\pm$ 0.03 & 0.377 $\pm$ 0.006 & 40 \\
402     5\% & 3.61 $\pm$ 0.02 & 0.355 $\pm$ 0.002 & 1.84 $\pm$ 0.03 & 0.169 $\pm$ 0.004 & 40 \\
403     0\% & 3.27 $\pm$ 0.02 & 0.147 $\pm$ 0.004 & 1.50 $\pm$ 0.02 & 0.194 $\pm$ 0.002 & 40 \\
404 jmichalk 3802 \hline
405     \end{tabular}
406     \end{table}
407    
408    
409    
410     %Discussion
411     \section{Discussion}
412 jmichalk 3816 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.
413 jmichalk 3802
414     \subsection{Diffusion}
415     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?)
416     \\
417     \\
418     %Evolution of surface
419     \begin{figure}[H]
420     \includegraphics[scale=0.5]{ProgressionOfDoubleLayerFormation_yellowCircle.png}
421 jmichalk 3817 \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.}
422 jmichalk 3802 \end{figure}
423    
424    
425    
426    
427     %Peaks!
428 jmichalk 3816 \begin{figure}[H]
429 jmichalk 3802 \includegraphics[scale=0.25]{doublePeaks_noCO.png}
430 jmichalk 3816 \caption{}
431     \end{figure}
432 jmichalk 3802 \section{Conclusion}
433    
434    
435 gezelter 3808 \section{Acknowledgments}
436     Support for this project was provided by the National Science
437     Foundation under grant CHE-0848243 and by the Center for Sustainable
438     Energy at Notre Dame (cSEND). Computational time was provided by the
439     Center for Research Computing (CRC) at the University of Notre Dame.
440 jmichalk 3802
441 gezelter 3808 \newpage
442     \bibliography{firstTryBibliography}
443     \end{doublespace}
444     \end{document}