From 2f4b812d1c458e6d3fedde8f661315c3affe6d32 Mon Sep 17 00:00:00 2001
From: Jaron Kent-Dobias <jaron@kent-dobias.com>
Date: Fri, 8 Jul 2022 12:24:18 +0200
Subject: Fixed typo.

---
 frsb_kac-rice.tex | 2 +-
 1 file changed, 1 insertion(+), 1 deletion(-)

(limited to 'frsb_kac-rice.tex')

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
-- 
cgit v1.2.3-70-g09d2

