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|
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\begin{figure}[htbp] |
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\centering |
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< |
%\includegraphics[width=\linewidth]{images/w6fig.pdf} |
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> |
\includegraphics[width=\linewidth]{images/w6_stacked_plot.pdf} |
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|
\caption{Distributions of the bond orientational order parameter |
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($\hat{W}_6$) at different temperatures. The upper, middle, and lower |
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panels are for 20, 30, and 40 \AA\ particles, respectively. The |
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$\mathrm{Wm^{-2}K^{-1}}$), while the right-hand column used a more |
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physically reasonable value of $117 \times 10^{6}$ |
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$\mathrm{Wm^{-2}K^{-1}}$. The peak at $\hat{W}_6 \approx -0.17$ is |
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< |
due to local icosahedral structures.} |
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> |
due to local icosahedral structures. The different curves in each of |
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> |
the panels indicate the distribution of $\hat{W}_6$ values for samples |
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> |
taken at different times along the cooling trajectory. The initial |
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> |
and final temperatures (in K) are indicated on the plots adjacent to |
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> |
their respective distributions.} |
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\label{fig:w6} |
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\end{figure} |
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|
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\begin{figure}[htbp] |
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|
\centering |
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< |
%\includegraphics[width=\linewidth]{images/q6fig.pdf} |
| 183 |
> |
\includegraphics[width=\linewidth]{images/q6_stacked_plot.pdf} |
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|
\caption{Distributions of the bond orientational order parameter |
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($Q_6$) at different temperatures. The curves in the six panels in |
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this figure were computed at identical conditions to the same panels in |
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|
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\begin{figure}[htbp] |
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\centering |
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< |
%\includegraphics[width=\linewidth]{images/ficos.pdf} |
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> |
\includegraphics[width=\linewidth]{images/fraction_icos.pdf} |
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|
\caption{Temperautre dependence of the fraction of atoms with local |
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icosahedral ordering, $f_\textrm{icos}(T)$ for 20, 30, and 40 \AA\ |
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particles cooled at two different values of the interfacial |
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|
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\begin{figure}[htbp] |
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|
\centering |
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< |
%\includegraphics[width=\linewidth]{images/AgVsCu.pdf} |
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> |
\includegraphics[width=\linewidth]{images/w6_stacked_bytype_plot.pdf} |
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|
\caption{Distributions of the bond orientational order parameter |
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($\hat{W}_6$) for the two different elements present in the |
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nanoparticles. This distribution was taken from the fully-cooled 40 |