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authorJaron Kent-Dobias <jaron@kent-dobias.com>2022-10-21 15:55:17 +0200
committerJaron Kent-Dobias <jaron@kent-dobias.com>2022-10-21 15:55:17 +0200
commitd28e08b7e4637b5a44434f2909f6213818a3834b (patch)
tree43f95e981881c3ca293aedaf6a963c3a7a4ce4a7
parent0e641b3cf916deefef4752d87a860104ef783816 (diff)
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No mu^* in this version.
-rw-r--r--frsb_kac-rice_letter.tex8
1 files changed, 4 insertions, 4 deletions
diff --git a/frsb_kac-rice_letter.tex b/frsb_kac-rice_letter.tex
index b4ba867..f216171 100644
--- a/frsb_kac-rice_letter.tex
+++ b/frsb_kac-rice_letter.tex
@@ -221,11 +221,11 @@ find the complexity everywhere. This is how the data in what follows was produce
\includegraphics[width=\columnwidth]{figs/316_complexity_contour_1_letter.pdf}
\caption{
- Complexity of the $3+16$ model in the energy $E$ and stability $\mu^*$
+ Complexity of the $3+16$ model in the energy $E$ and stability $\mu$
plane. The right shows a detail of the left. Below the yellow marginal line
- the complexity counts saddles of increasing index as $\mu^*$ decreases.
+ the complexity counts saddles of increasing index as $\mu$ decreases.
Above the yellow marginal line the complexity counts minima of increasing
- stability as $\mu^*$ increases.
+ stability as $\mu$ increases.
} \label{fig:2rsb.contour}
\end{figure}
@@ -333,7 +333,7 @@ model stall in a place where minima are exponentially subdominant.
\includegraphics[width=\columnwidth]{figs/24_phases_letter.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
+ stability $\mu$ plane. The region shaded gray shows where the RS solution
is correct, while the region shaded red shows that where the FRSB solution
is correct. The white region shows where the complexity is zero.
} \label{fig:frsb.phases}