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| author | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2022-07-08 14:09:23 +0200 |
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| committer | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2022-07-08 14:09:23 +0200 |
| commit | f3de26844a01eb909501f3e73b60e2626f91b40c (patch) | |
| tree | cc13af984007536c7658a77fb54ab167b0ccc2d1 | |
| parent | 95dac43e6bb643e1cb64167671627f277208d4d1 (diff) | |
| download | PRE_107_064111-f3de26844a01eb909501f3e73b60e2626f91b40c.tar.gz PRE_107_064111-f3de26844a01eb909501f3e73b60e2626f91b40c.tar.bz2 PRE_107_064111-f3de26844a01eb909501f3e73b60e2626f91b40c.zip | |
Small wording change.
| -rw-r--r-- | frsb_kac-rice.tex | 3 |
1 files changed, 2 insertions, 1 deletions
diff --git a/frsb_kac-rice.tex b/frsb_kac-rice.tex index a22b7b2..09c3042 100644 --- a/frsb_kac-rice.tex +++ b/frsb_kac-rice.tex @@ -327,7 +327,8 @@ where the function $\mathcal D$ is defined by \end{aligned} \end{equation} It follows that by fixing the trace of the Hessian, we have effectively fixed -the value of $\mu$ in all replicas to $\mu^*$, and therefore the index as well. +the value of $\mu$ in all replicas to $\mu^*$, and therefore the index of +saddles in all replicas as well. What we have described is the {\em typical} spectrum for given $\mu$. What about the deviations of the spectrum -- we are particularly interested in the |