From f31a46c260294a51d9215b5c66c828453ac1bfd6 Mon Sep 17 00:00:00 2001
From: Jaron Kent-Dobias <jaron@kent-dobias.com>
Date: Wed, 13 Jul 2022 00:35:31 +0200
Subject: Some tweaks for a4paper.

---
 frsb_kac-rice.tex | 20 ++++++++++----------
 1 file changed, 10 insertions(+), 10 deletions(-)

(limited to 'frsb_kac-rice.tex')

diff --git a/frsb_kac-rice.tex b/frsb_kac-rice.tex
index 3cc1ba6..11d5822 100644
--- a/frsb_kac-rice.tex
+++ b/frsb_kac-rice.tex
@@ -1,4 +1,4 @@
-\documentclass[fleqn]{article}
+\documentclass[fleqn,a4paper]{article}
 
 \usepackage[utf8]{inputenc} % why not type "Bézout" with unicode?
 \usepackage[T1]{fontenc} % vector fonts plz
@@ -1007,7 +1007,7 @@ 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{figs/316_complexity.pdf}
+  \includegraphics[width=\textwidth]{figs/316_complexity.pdf}
 
   \caption{
     Complexity of dominant saddles (blue), marginal minima (yellow), and
@@ -1025,7 +1025,7 @@ replica symmetry breaking when minima or inherent states do not.
   \includegraphics{figs/316_complexity_contour_1.pdf}
   \hspace{-1em}
   \includegraphics{figs/316_complexity_contour_2.pdf}
-  \raisebox{3em}{\includegraphics{figs/316_complexity_contour_leg.pdf}}
+  \raisebox{3em}{\includegraphics[width=0.27\textwidth]{figs/316_complexity_contour_leg.pdf}}
 
   \caption{
     Complexity of the $3+16$ model in the energy $E$ and stability $\mu^*$
@@ -1056,7 +1056,7 @@ model stall in a place where minima are exponentially subdominant.
 
 \begin{figure}
   \centering
-  \includegraphics{figs/316_detail.pdf}
+  \includegraphics[width=\textwidth]{figs/316_detail.pdf}
 
   \caption{
     Detail of the `phases' of the $3+16$ model complexity as a function of
@@ -1098,8 +1098,8 @@ point in the complexity of high-index saddles in worth further study.
   \centering
   \includegraphics{figs/316_comparison_q.pdf}\hfill
   \includegraphics{figs/316_comparison_rd.pdf}\hfill
-  \includegraphics{figs/316_comparison_r1.pdf}\hspace{1em}
-  \includegraphics{figs/316_comparison_legend.pdf} \vspace{0.5em}\\
+  \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
@@ -1154,7 +1154,7 @@ insight into lower-energy symmetry breaking in more general contexts.
 
 \begin{figure}
   \centering
-  \includegraphics{figs/24_complexity.pdf}
+  \includegraphics[width=\textwidth]{figs/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
@@ -1168,7 +1168,7 @@ insight into lower-energy symmetry breaking in more general contexts.
 
 \begin{figure}
   \centering
-  \includegraphics{figs/24_phases.pdf}
+  \includegraphics[width=\textwidth]{figs/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
@@ -1186,8 +1186,8 @@ goes to zero with finite slopes.
 
 \begin{figure}
   \raggedright
-  \hspace{2em}\includegraphics{figs/24_opt_q(x).pdf}
-  \hspace{1em}
+  \hspace{1em}\includegraphics{figs/24_opt_q(x).pdf}
+  \hspace{0.5em}
   \includegraphics{figs/24_opt_xMax.pdf}
   \\\vspace{1em}
   \includegraphics{figs/24_opt_r(x).pdf}
-- 
cgit v1.2.3-70-g09d2

