From d944977b38915e8fe51ef1cca68b95d0a8107217 Mon Sep 17 00:00:00 2001
From: Jaron Kent-Dobias <jaron@kent-dobias.com>
Date: Tue, 29 Oct 2024 14:00:55 +0100
Subject: Wording tweak.

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

diff --git a/marginal.tex b/marginal.tex
index 1f1143c..30d3dce 100644
--- a/marginal.tex
+++ b/marginal.tex
@@ -1394,7 +1394,7 @@ Unlike in the spherical and multispherical spin glasses, the value $\mu^*$
 defined in \eqref{eq:mu.star} giving the typical value of
 $\frac1N\operatorname{Tr}\partial\partial H$ is not always zero. Instead
 $\mu^*=-f'(0)$, nonzero where there is a linear term in $V$. Fixing the trace
-of the Hessian is therefore equivalent to setting $\omega=\mu+f'(0)$.
+of the Hessian is therefore equivalent to constraining the value of the Lagrange multiplier $\omega=\mu+f'(0)$.
 
 
 The derivation of the marginal complexity for this model is complicated, but
-- 
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