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authorJaron Kent-Dobias <jaron@kent-dobias.com>2024-10-29 14:00:55 +0100
committerJaron Kent-Dobias <jaron@kent-dobias.com>2024-10-29 14:00:55 +0100
commitd944977b38915e8fe51ef1cca68b95d0a8107217 (patch)
tree6570f29a30794032f8259207d41ea26642cf2dbb
parent79309cd70841ecc1a0c34776ab962785c1e6ebce (diff)
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Wording tweak.
-rw-r--r--marginal.tex2
1 files changed, 1 insertions, 1 deletions
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