4 |
|
\usepackage{setspace} |
5 |
|
\usepackage{endfloat} |
6 |
|
\usepackage{caption} |
7 |
+ |
|
8 |
|
%\usepackage{tabularx} |
9 |
|
\usepackage{graphicx} |
10 |
|
\usepackage{multirow} |
51 |
|
%Title |
52 |
|
\title{Investigation of the Pt and Au 557 Surface Reconstructions |
53 |
|
under a CO Atmosphere} |
54 |
< |
\author{Joseph R. Michalka, Patrick W. MacIntyre and J. Daniel |
54 |
> |
\author{Joseph R. Michalka, Patrick W. McIntyre and J. Daniel |
55 |
|
Gezelter\footnote{Corresponding author. \ Electronic mail: gezelter@nd.edu} \\ |
56 |
|
Department of Chemistry and Biochemistry,\\ |
57 |
|
University of Notre Dame\\ |
208 |
|
mechanical predictions (-2.46 D~\AA)\cite{QuadrupoleCOCalc}. |
209 |
|
%CO Table |
210 |
|
\begin{table}[H] |
211 |
< |
\caption{Positions, $\sigma$, $\epsilon$ and charges for CO geometry and self-interactions\cite{Straub}. Distances are in \AA~, energies are in kcal/mol, and charges are in $e$.} |
211 |
> |
\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 |
|
\centering |
215 |
|
\begin{tabular}{| c | c | ccc |} |
216 |
|
\hline |
282 |
|
the bare crystal systems were initially run in the Canonical ensemble at |
283 |
|
800~K and 1000~K respectively for 100 ps. Various amounts of CO were |
284 |
|
placed in the vacuum region, which upon full adsorption to the surface |
285 |
< |
corresponded to 5\%, 25\%, 33\%, and 50\% coverages. These systems |
286 |
< |
were again allowed to reach thermal equilibrium before being run in the |
285 |
> |
corresponded to 5\%, 25\%, 33\%, and 50\% coverages. Because of the |
286 |
> |
high temperature and the difference in binding energies, the platinum systems |
287 |
> |
very rarely had CO that was not adsorbed to the surface whereas the gold systems |
288 |
> |
often had a substantial minority of CO away from the surface. |
289 |
> |
These systems were again allowed to reach thermal equilibrium before being run in the |
290 |
|
microcanonical ensemble. All of the systems examined in this work were |
291 |
|
run for at least 40 ns. A subset that were undergoing interesting effects |
292 |
|
have been allowed to continue running with one system approaching 200 ns. |
329 |
|
& Calc. & Exp. \\ |
330 |
|
\hline |
331 |
|
\textbf{Pt-CO} & -1.9 & -1.4~\cite{Kelemen:1979}-- -1.9~\cite{Yeo} \\ |
332 |
< |
\textbf{Au-CO} & -0.39 & -0.44~\cite{TPD_Gold_CO} \\ |
332 |
> |
\textbf{Au-CO} & -0.39 & -0.40~\cite{TPD_Gold} \\ |
333 |
|
\hline |
334 |
|
\end{tabular} |
335 |
|
\end{table} |
342 |
|
% Just results, leave discussion for discussion section |
343 |
|
\section{Results} |
344 |
|
\subsection{Diffusion} |
345 |
< |
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 been running continuously. The lowered diffusion constant at longer run times will be examined in-depth in the discussion section. |
345 |
> |
An ideal metal surface displaying a low-energy facet, a (111) face for |
346 |
> |
instance, is unlikely to experience much surface diffusion because of |
347 |
> |
the large energy barrier associated with atoms 'lifting' from the top |
348 |
> |
layer to then be able to explore the surface. Rougher surfaces, those |
349 |
> |
that already contain numerous adatoms, step edges, and kinks, should |
350 |
> |
have concomitantly higher surface diffusion rates. Tao et al. showed |
351 |
> |
that the platinum 557 surface undergoes two separate reconstructions |
352 |
> |
upon CO adsorption. \cite{Tao:2010} The first reconstruction involves a |
353 |
> |
doubling of the step edge height which is accomplished by a doubling |
354 |
> |
of the plateau length. The second reconstruction led to the formation of |
355 |
> |
triangular motifs stretching across the lengthened plateaus. |
356 |
|
|
357 |
+ |
As shown in Figure 2, over a period of approximately 100 ns, the surface |
358 |
+ |
has reconstructed from a 557 surface by doubling the step height and |
359 |
+ |
step length. Focusing on only the platinum, or gold, atoms that were |
360 |
+ |
deemed mobile on the surface, an analysis of the surface diffusion was |
361 |
+ |
performed. A particle was considered mobile once it had traveled more |
362 |
+ |
than 2~\AA between snapshots. This immediately eliminates all of the |
363 |
+ |
bulk metal and greatly limits the number of surface atoms examined. |
364 |
+ |
Since diffusion on a surface is strongly affected by overcoming energy |
365 |
+ |
barriers, the diffusion parallel to the step edge axis was determined |
366 |
+ |
separately from the diffusion perpendicular to the step edge. The results |
367 |
+ |
at various coverages on both platinum and gold are shown in Table 4. |
368 |
+ |
|
369 |
+ |
%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. |
370 |
+ |
|
371 |
+ |
\begin{figure}[H] |
372 |
+ |
\includegraphics[scale=0.6]{DiffusionComparison_error.png} |
373 |
+ |
\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. } |
374 |
+ |
\end{figure} |
375 |
+ |
|
376 |
|
%Table of Diffusion Constants |
377 |
|
%Add gold?M |
378 |
|
\begin{table}[H] |
397 |
|
|
398 |
|
%Discussion |
399 |
|
\section{Discussion} |
400 |
< |
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. |
400 |
> |
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. |
401 |
|
|
402 |
|
\subsection{Diffusion} |
403 |
|
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?) |
406 |
|
%Evolution of surface |
407 |
|
\begin{figure}[H] |
408 |
|
\includegraphics[scale=0.5]{ProgressionOfDoubleLayerFormation_yellowCircle.png} |
409 |
< |
\caption{Four snapshots at various times a) 258 ps b) 19 ns c) 31.2 ns 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.} |
409 |
> |
\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.} |
410 |
|
\end{figure} |
411 |
|
|
412 |
|
|
413 |
|
|
414 |
|
|
415 |
|
%Peaks! |
416 |
+ |
\begin{figure}[H] |
417 |
|
\includegraphics[scale=0.25]{doublePeaks_noCO.png} |
418 |
+ |
\caption{} |
419 |
+ |
\end{figure} |
420 |
|
\section{Conclusion} |
421 |
|
|
422 |
|
|