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-rw-r--r--2-point.bib14
-rw-r--r--2-point.tex2
2 files changed, 16 insertions, 0 deletions
diff --git a/2-point.bib b/2-point.bib
index 6fb83bd..60d64cc 100644
--- a/2-point.bib
+++ b/2-point.bib
@@ -403,3 +403,17 @@ Spherical Spin Glasses},
doi = {10.21468/scipostphys.15.3.109}
}
+@article{Kent-Dobias_2023_When,
+ author = {Kent-Dobias, Jaron},
+ title = {When is the average number of saddle points typical?},
+ journal = {Europhysics Letters},
+ publisher = {IOP Publishing},
+ year = {2023},
+ month = {8},
+ number = {6},
+ volume = {143},
+ pages = {61003},
+ url = {https://doi.org/10.1209%2F0295-5075%2Facf521},
+ doi = {10.1209/0295-5075/acf521}
+}
+
diff --git a/2-point.tex b/2-point.tex
index 5f9bda8..acbba87 100644
--- a/2-point.tex
+++ b/2-point.tex
@@ -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)