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@@ -213,6 +213,8 @@ are not aware of any result guaranteeing this for the complexity away from the
ground state, but we check that our replica-symmetric solutions satisfy the
saddle point equations at {\oldstylenums1}\textsc{rsb}.
+\cite{Kent-Dobias_2023_When}
+
To enforce the spherical constraint at stationary points, we make use of a Lagrange multiplier $\omega$. This results in the extremal problem
\begin{equation}
H(\mathbf s)+\frac\omega2(\|\mathbf s\|^2-N)