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| author | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2022-07-08 12:24:18 +0200 |
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| committer | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2022-07-08 12:24:18 +0200 |
| commit | 2f4b812d1c458e6d3fedde8f661315c3affe6d32 (patch) | |
| tree | 95a01cfc24302476d7cde56b667ef4481d3cf282 /frsb_kac-rice.tex | |
| parent | 9ecc2e2aba085c2624db01a1c1f55dfbb2424451 (diff) | |
| download | PRE_107_064111-2f4b812d1c458e6d3fedde8f661315c3affe6d32.tar.gz PRE_107_064111-2f4b812d1c458e6d3fedde8f661315c3affe6d32.tar.bz2 PRE_107_064111-2f4b812d1c458e6d3fedde8f661315c3affe6d32.zip | |
Fixed typo.
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 eeac95e..70c61f2 100644 --- a/frsb_kac-rice.tex +++ b/frsb_kac-rice.tex @@ -38,7 +38,7 @@ of small temperature for the lowest states, as it should. To understand the importance of this computation, consider the following situation. When one solves the problem of spheres in large dimensions, one finds that there is a transition at a given temperature to a one-step symmetry breaking (1RSB) phase at a Kauzmann temperature, and, at a lower temperature, -another transition to a full RSB phase (see \cite{Gross_1985_Mean-field, Gardner_1985_Spin}, the o-called `Gardner' phase \cite{Charbonneau_2014_Fractal}). +another transition to a full RSB phase (see \cite{Gross_1985_Mean-field, Gardner_1985_Spin}, the so-called `Gardner' phase \cite{Charbonneau_2014_Fractal}). Now, this transition involves the lowest, equilibrium states. Because they are obviously unreachable at any reasonable timescale, an often addressed question to ask is: what is the Gardner transition line for higher than equilibrium |