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| author | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2022-07-13 13:01:30 +0200 |
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| committer | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2022-07-13 13:01:30 +0200 |
| commit | 93e5b0121a82ec60c2d97a257342a4d9d9a93a08 (patch) | |
| tree | 77b7279ed9b2c1b5e6c50e9bac7a0510686ce4c3 /frsb_kac-rice.tex | |
| parent | 4b9e19bbd81a390236b413a25f24770027d4d32c (diff) | |
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Updated Jorge's references
Diffstat (limited to 'frsb_kac-rice.tex')
| -rw-r--r-- | frsb_kac-rice.tex | 2 |
1 files changed, 1 insertions, 1 deletions
diff --git a/frsb_kac-rice.tex b/frsb_kac-rice.tex index c31cb62..1a576a3 100644 --- a/frsb_kac-rice.tex +++ b/frsb_kac-rice.tex @@ -1411,7 +1411,7 @@ saddles of random mean-field landscapes, including systems with many steps of RSB. For systems with full RSB, we find that minima are exponentially subdominant with respect to saddles at all energy densities above the ground state. The solution contains valuable geometric information that has yet to be -extracted in all detail, for example considering several copies of the system \cite{cavagna1997structure}, or the extension to complex variables \cite{kent2021complex,kent2022analytic}. +extracted in all detail, for example considering several copies of the system \cite{Cavagna_1997_Structure}, or the extension to complex variables \cite{Kent-Dobias_2021_Complex, Kent-Dobias_2022_Analytic}. A first and very important application of the method here is to perform the calculation for high dimensional spheres, where it would give us a clear |