From 93e5b0121a82ec60c2d97a257342a4d9d9a93a08 Mon Sep 17 00:00:00 2001
From: Jaron Kent-Dobias <jaron@kent-dobias.com>
Date: Wed, 13 Jul 2022 13:01:30 +0200
Subject: Updated Jorge's references

---
 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 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
-- 
cgit v1.2.3-70-g09d2

