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authorJaron Kent-Dobias <jaron@kent-dobias.com>2022-07-08 12:33:30 +0200
committerJaron Kent-Dobias <jaron@kent-dobias.com>2022-07-08 12:33:30 +0200
commit95dac43e6bb643e1cb64167671627f277208d4d1 (patch)
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parent2f4b812d1c458e6d3fedde8f661315c3affe6d32 (diff)
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More pedogogical introduction to the model.
-rw-r--r--frsb_kac-rice.tex10
1 files changed, 7 insertions, 3 deletions
diff --git a/frsb_kac-rice.tex b/frsb_kac-rice.tex
index 70c61f2..a22b7b2 100644
--- a/frsb_kac-rice.tex
+++ b/frsb_kac-rice.tex
@@ -69,9 +69,13 @@ For definiteness, we consider the mixed $p$-spin spherical model, whose Hamilton
is defined for vectors $\mathbf s\in\mathbb R^N$ confined to the sphere
$\|\mathbf s\|^2=N$. The coupling coefficients $J$ are taken at random, with
zero mean and variance $\overline{(J^{(p)})^2}=a_pp!/2N^{p-1}$ chosen so that
-the energy is typically extensive. This implies that the covariance of the
-energy with itself depends only on the dot product (or overlap) between two
-configurations. In particular, one has
+the energy is typically extensive. The factors $a_p$ in the variances are
+freely chosen constants that define the particular model. For instance, the
+so-called `pure' models have $a_p=1$ for some $p$ and all others zero.
+
+The variance of the couplings implies that the covariance of the energy with
+itself depends only on the dot product (or overlap) between two configurations.
+In particular, one has
\begin{equation}
\overline{H(\mathbf s_1)H(\mathbf s_2)}=Nf\left(\frac{\mathbf s_1\cdot\mathbf s_2}N\right)
\end{equation}