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authorJaron Kent-Dobias <jaron@kent-dobias.com>2022-07-13 00:35:31 +0200
committerJaron Kent-Dobias <jaron@kent-dobias.com>2022-07-13 00:35:31 +0200
commitf31a46c260294a51d9215b5c66c828453ac1bfd6 (patch)
treead400e37da8342252baa785c6e4aa89de10266ad /frsb_kac-rice.tex
parentb33e99bdbd3add4b040bd325171ae3785e43e3fa (diff)
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Some tweaks for a4paper.
Diffstat (limited to 'frsb_kac-rice.tex')
-rw-r--r--frsb_kac-rice.tex20
1 files changed, 10 insertions, 10 deletions
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}