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authorJaron Kent-Dobias <jaron@kent-dobias.com>2022-09-02 16:56:56 +0200
committerJaron Kent-Dobias <jaron@kent-dobias.com>2022-09-02 16:56:56 +0200
commit78216a25b1314e2bf6e13ec846fcd313dde09eb8 (patch)
tree70fc28b60b613093f24c13df435d7e99b0581894
parent8c04cb9cb7b67b27f6604a32a50f5bada2ef62a7 (diff)
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-rw-r--r--frsb_kac-rice.tex44
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