From 78216a25b1314e2bf6e13ec846fcd313dde09eb8 Mon Sep 17 00:00:00 2001
From: Jaron Kent-Dobias <jaron@kent-dobias.com>
Date: Fri, 2 Sep 2022 16:56:56 +0200
Subject: APS doesn't allow subdirectories.

---
 frsb_kac-rice.tex | 44 ++++++++++++++++++++++----------------------
 1 file changed, 22 insertions(+), 22 deletions(-)

(limited to 'frsb_kac-rice.tex')

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
-- 
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