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author | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2022-07-13 00:35:31 +0200 |
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committer | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2022-07-13 00:35:31 +0200 |
commit | f31a46c260294a51d9215b5c66c828453ac1bfd6 (patch) | |
tree | ad400e37da8342252baa785c6e4aa89de10266ad | |
parent | b33e99bdbd3add4b040bd325171ae3785e43e3fa (diff) | |
download | PRE_107_064111-f31a46c260294a51d9215b5c66c828453ac1bfd6.tar.gz PRE_107_064111-f31a46c260294a51d9215b5c66c828453ac1bfd6.tar.bz2 PRE_107_064111-f31a46c260294a51d9215b5c66c828453ac1bfd6.zip |
Some tweaks for a4paper.
-rw-r--r-- | frsb_kac-rice.tex | 20 |
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} |