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-rw-r--r--frsb_kac-rice.bib10
-rw-r--r--frsb_kac-rice.tex44
-rw-r--r--frsb_kac-rice_letter.tex12
3 files changed, 28 insertions, 38 deletions
diff --git a/frsb_kac-rice.bib b/frsb_kac-rice.bib
index 6a2b5e8..b11ad6c 100644
--- a/frsb_kac-rice.bib
+++ b/frsb_kac-rice.bib
@@ -926,13 +926,3 @@ complexity},
url = {https://doi.org/10.1103%2Fphysrevlett.110.118101},
doi = {10.1103/physrevlett.110.118101}
}
-
-@article{ros2021dynamical,
- title={Dynamical instantons and activated processes in mean-field glass models},
- author={Ros, Valentina and Biroli, Giulio and Cammarota, Chiara},
- journal={SciPost Physics},
- volume={10},
- number={1},
- pages={002},
- year={2021}
-}
diff --git a/frsb_kac-rice.tex b/frsb_kac-rice.tex
index 3d59148..f21864f 100644
--- a/frsb_kac-rice.tex
+++ b/frsb_kac-rice.tex
@@ -996,7 +996,7 @@ 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
@@ -1011,10 +1011,10 @@ 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 $\mu^*$
@@ -1045,7 +1045,7 @@ 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
@@ -1085,14 +1085,14 @@ 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
@@ -1143,7 +1143,7 @@ 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
@@ -1157,7 +1157,7 @@ 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
@@ -1175,13 +1175,13 @@ 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,
@@ -1284,11 +1284,11 @@ 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
diff --git a/frsb_kac-rice_letter.tex b/frsb_kac-rice_letter.tex
index c7ef913..bdcec74 100644
--- a/frsb_kac-rice_letter.tex
+++ b/frsb_kac-rice_letter.tex
@@ -263,8 +263,8 @@ find the complexity everywhere. This is how the data in what follows was produce
\begin{figure}
\centering
\hspace{-1em}
- \includegraphics[width=\columnwidth]{figs/316_complexity_contour_1_letter.pdf}
- \includegraphics[width=\columnwidth]{figs/316_detail_letter_legend.pdf}
+ \includegraphics[width=\columnwidth]{316_complexity_contour_1_letter.pdf}
+ \includegraphics[width=\columnwidth]{316_detail_letter_legend.pdf}
\caption{
Complexity of the $3+16$ model in the energy $E$ and stability $\mu$
@@ -278,8 +278,8 @@ find the complexity everywhere. This is how the data in what follows was produce
\begin{figure}
\centering
- \includegraphics[width=\columnwidth]{figs/316_detail_letter.pdf}
- \includegraphics[width=\columnwidth]{figs/316_detail_letter_legend.pdf}
+ \includegraphics[width=\columnwidth]{316_detail_letter.pdf}
+ \includegraphics[width=\columnwidth]{316_detail_letter_legend.pdf}
\caption{
Detail of the `phases' of the $3+16$ model complexity as a function of
@@ -382,8 +382,8 @@ model stall in a place where minima are exponentially subdominant.
\begin{figure}
\centering
- \includegraphics[width=\columnwidth]{figs/24_phases_letter.pdf}
- \includegraphics[width=\columnwidth]{figs/24_detail_letter_legend.pdf}
+ \includegraphics[width=\columnwidth]{24_phases_letter.pdf}
+ \includegraphics[width=\columnwidth]{24_detail_letter_legend.pdf}
\caption{
`Phases' of the complexity for the $2+4$ model in the energy $E$ and
stability $\mu$ plane. Solid lines show the prediction of 1RSB complexity,