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author | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2022-09-02 16:56:56 +0200 |
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committer | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2022-09-02 16:56:56 +0200 |
commit | 78216a25b1314e2bf6e13ec846fcd313dde09eb8 (patch) | |
tree | 70fc28b60b613093f24c13df435d7e99b0581894 | |
parent | 8c04cb9cb7b67b27f6604a32a50f5bada2ef62a7 (diff) | |
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-rw-r--r-- | frsb_kac-rice.tex | 44 |
1 files changed, 22 insertions, 22 deletions
diff --git a/frsb_kac-rice.tex b/frsb_kac-rice.tex index 875d5a9..bdcbe58 100644 --- a/frsb_kac-rice.tex +++ b/frsb_kac-rice.tex @@ -969,7 +969,7 @@ sampling a landscape at high energies, high index saddles may show a sign of replica symmetry breaking when minima or inherent states do not. \begin{figure} - \includegraphics[width=\textwidth]{figs/316_complexity.pdf} + \includegraphics[width=\textwidth]{316_complexity.pdf} \caption{ Complexity of dominant saddles (blue), marginal minima (yellow), and @@ -984,10 +984,10 @@ replica symmetry breaking when minima or inherent states do not. \begin{figure} \centering \hspace{-1em} - \includegraphics{figs/316_complexity_contour_1.pdf} + \includegraphics{316_complexity_contour_1.pdf} \hspace{-1em} - \includegraphics{figs/316_complexity_contour_2.pdf} - \raisebox{3em}{\includegraphics[width=0.27\textwidth]{figs/316_complexity_contour_leg.pdf}} + \includegraphics{316_complexity_contour_2.pdf} + \raisebox{3em}{\includegraphics[width=0.27\textwidth]{316_complexity_contour_leg.pdf}} \caption{ Complexity of the $3+16$ model in the energy $E$ and stability $\mu^*$ @@ -1018,7 +1018,7 @@ model stall in a place where minima are exponentially subdominant. \begin{figure} \centering - \includegraphics[width=\textwidth]{figs/316_detail.pdf} + \includegraphics[width=\textwidth]{316_detail.pdf} \caption{ Detail of the `phases' of the $3+16$ model complexity as a function of @@ -1058,14 +1058,14 @@ point in the complexity of high-index saddles in worth further study. \begin{figure} \centering - \includegraphics{figs/316_comparison_q.pdf}\hfill - \includegraphics{figs/316_comparison_rd.pdf}\hfill - \includegraphics{figs/316_comparison_r1.pdf}\hfill - \raisebox{1em}{\includegraphics[width=0.24\textwidth]{figs/316_comparison_legend.pdf}} \vspace{0.5em}\\ - \includegraphics{figs/316_comparison_x.pdf}\hfill - \includegraphics{figs/316_comparison_dd.pdf}\hfill - \includegraphics{figs/316_comparison_d1.pdf}\hfill - \includegraphics{figs/316_comparison_b.pdf} + \includegraphics{316_comparison_q.pdf}\hfill + \includegraphics{316_comparison_rd.pdf}\hfill + \includegraphics{316_comparison_r1.pdf}\hfill + \raisebox{1em}{\includegraphics[width=0.24\textwidth]{316_comparison_legend.pdf}} \vspace{0.5em}\\ + \includegraphics{316_comparison_x.pdf}\hfill + \includegraphics{316_comparison_dd.pdf}\hfill + \includegraphics{316_comparison_d1.pdf}\hfill + \includegraphics{316_comparison_b.pdf} \caption{ Comparison of the saddle point parameters for the $3+16$ model along @@ -1116,7 +1116,7 @@ insight into lower-energy symmetry breaking in more general contexts. \begin{figure} \centering - \includegraphics[width=\textwidth]{figs/24_complexity.pdf} + \includegraphics[width=\textwidth]{24_complexity.pdf} \caption{ The complexity $\Sigma$ of the mixed $2+4$ spin model as a function of distance $\Delta E=E-E_0$ of the ground state. The @@ -1130,7 +1130,7 @@ insight into lower-energy symmetry breaking in more general contexts. \begin{figure} \centering - \includegraphics[width=\textwidth]{figs/24_phases.pdf} + \includegraphics[width=\textwidth]{24_phases.pdf} \caption{ `Phases' of the complexity for the $2+4$ model in the energy $E$ and stability $\mu^*$ plane. The region shaded gray shows where the RS solution @@ -1148,13 +1148,13 @@ goes to zero with finite slopes. \begin{figure} \raggedright - \hspace{1em}\includegraphics{figs/24_opt_qx.pdf} + \hspace{1em}\includegraphics{24_opt_qx.pdf} \hspace{0.5em} - \includegraphics{figs/24_opt_xMax.pdf} + \includegraphics{24_opt_xMax.pdf} \\\vspace{1em} - \includegraphics{figs/24_opt_rx.pdf} + \includegraphics{24_opt_rx.pdf} \hspace{1em} - \includegraphics{figs/24_opt_dx.pdf} + \includegraphics{24_opt_dx.pdf} \caption{ $x_\textrm{max}$ as a function of $E$ for several trajectories of interest, @@ -1257,11 +1257,11 @@ exponentially many stationary points. A cartoon of this picture is shown in Fig. \begin{figure} \centering - \includegraphics{figs/cartoon_RS.pdf} + \includegraphics{cartoon_RS.pdf} \hfill - \includegraphics{figs/cartoon_1RSB.pdf} + \includegraphics{cartoon_1RSB.pdf} \hfill - \includegraphics{figs/cartoon_2RSB.pdf} + \includegraphics{cartoon_2RSB.pdf} \caption{ A cartoon visualizing how to interpret replica symmetry breaking solutions |