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| author | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2023-11-28 16:36:42 +0100 |
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| committer | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2023-11-28 16:36:42 +0100 |
| commit | f4c4f40405bf306880edeb8ceb43a7469b54bb92 (patch) | |
| tree | 62de100a9ce18bd6ffb550c5bc63b345933af528 | |
| parent | 6ffa6f15dbac91e6853c3aad20a0fa6d342005c2 (diff) | |
| download | SciPostPhys_16_001-f4c4f40405bf306880edeb8ceb43a7469b54bb92.tar.gz SciPostPhys_16_001-f4c4f40405bf306880edeb8ceb43a7469b54bb92.tar.bz2 SciPostPhys_16_001-f4c4f40405bf306880edeb8ceb43a7469b54bb92.zip | |
Began response to one point.
| -rw-r--r-- | response.md | 2 |
1 files changed, 2 insertions, 0 deletions
diff --git a/response.md b/response.md index 351a221..f6fcfbf 100644 --- a/response.md +++ b/response.md @@ -90,6 +90,8 @@ The suggestion of the referee was good and was implemented in the new manuscript > saddle with mu\<mu, but with energies smaller than the threshold energy", so? > What is the implication? This misses a conclusion. +These low-lying saddles represent large-deviations from the typical complexity + > Sec.3.1, the author comments on the similarity with the pure model, without > explaining what is similar. What should we expect on the p-spin? At least the > relevant aspects. It would also be useful to plot a version of Fig.3 for the |