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authorJaron Kent-Dobias <jaron@kent-dobias.com>2021-03-12 16:38:17 +0100
committerJaron Kent-Dobias <jaron@kent-dobias.com>2021-03-12 16:38:17 +0100
commit43ed1805b695086eb1eb7218fc483557a6df82be (patch)
tree8cc9b2fa2b846cc65bc824d3b6a54b3a4e18068e
parent9aa887b6e9cf240de5efbd26411d6a2aad834366 (diff)
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Changed some notation to be more clear.
-rw-r--r--bezout.tex32
1 files changed, 13 insertions, 19 deletions
diff --git a/bezout.tex b/bezout.tex
index eaa98ce..458b448 100644
--- a/bezout.tex
+++ b/bezout.tex
@@ -51,7 +51,7 @@ review see \cite{Castellani_2005_Spin-glass}) defined by the energy
H_0 = \frac1{p!}\sum_{i_1\cdots i_p}^NJ_{i_1\cdots i_p}z_{i_1}\cdots z_{i_p},
\end{equation}
where $J$ is a symmetric tensor whose elements are real Gaussian variables and
-$z\in\mathbb R^N$ is constrained to the sphere $z^2=N$. This problem has been
+$z\in\mathbb R^N$ is constrained to the sphere $z^Tz=N$. This problem has been
studied in the algebra \cite{Cartwright_2013_The} and probability literature
\cite{Auffinger_2012_Random, Auffinger_2013_Complexity}. It has been attacked
from several angles: the replica trick to compute the Boltzmann--Gibbs
@@ -68,7 +68,7 @@ In this paper we extend the study to complex variables: we shall take
$z\in\mathbb C^N$ and $J$ to be a symmetric tensor whose elements are
\emph{complex} normal, with $\overline{|J|^2}=p!/2N^{p-1}$ and
$\overline{J^2}=\kappa\overline{|J|^2}$ for complex parameter $|\kappa|<1$. The
-constraint remains $z^2=N$.
+constraint remains $z^Tz=N$.
The motivations for this paper are of two types. On the practical side, there
are indeed situations in which complex variables appear naturally in disordered
@@ -98,27 +98,26 @@ of Lagrange multipliers: introducing $\epsilon\in\mathbb C$, our energy is
\begin{equation} \label{eq:constrained.hamiltonian}
H = H_0+\frac p2\epsilon\left(N-\sum_i^Nz_i^2\right).
\end{equation}
-One might balk at the constraint $z^2=N$---which could appropriately be called
-a \emph{hyperbolic} constraint---by comparison with $|z|^2=N$. The reasoning
+One might balk at the constraint $z^Tz=N$---which could appropriately be called
+a \emph{hyperbolic} constraint---by comparison with $z^\dagger z=N$. The reasoning
behind the choice is twofold.
First, we seek draw conclusions from our model that would be applicable to
generic holomorphic functions without any symmetry. Samples of $H_0$ nearly
provide this, save for a single anomaly: the value of the energy and its
gradient at any point $z$ correlate along the $z$ direction, with
-$\overline{H_0\partial_iH_0}\propto\kappa(z^2)^{p-1}z_i$ and
-$\overline{H_0(\partial_iH_0)^*}\propto|z|^{2(p-1)}z_i$. Besides being a
+$\overline{H_0\partial_iH_0}\propto \overline{H_0(\partial_iH_0)^*}\propto z_i$. Besides being a
spurious correlation, in each sample there is also a `radial' gradient of
magnitude proportional to the energy, since $z\cdot\partial H_0=pH_0$. This
anomalous direction must be neglected if we are to draw conclusions about
-generic functions, and the constraint surface $z^2=N$ is the unique surface
+generic functions, and the constraint surface $z^Tz=N$ is the unique surface
whose normal is parallel to $z$ and which contains the configuration space of
the real $p$-spin model as a subspace.
Second, taking the constraint to be the level set of a holomorphic function
means the resulting configuration space is a \emph{bone fide} complex manifold,
and therefore permits easy generalization of the integration techniques
-referenced above. The same cannot be said for the space defined by $|z|^2=N$,
+referenced above. The same cannot be said for the space defined by $z^\dagger z=N$,
which is topologically the $(2N-1)$-sphere and cannot admit a complex
structure.
@@ -128,10 +127,10 @@ related problems have similar properties but are concerned with subspaces on
which the energy is bounded. (In fact, identifying the appropriate subspace on
which to define one's model often requires the study of critical points in the
whole space.) Where it might be a problem, we introduce the additional
-constraint $|z|^2\leq Nr^2$. The resulting configuration space is a complex
+constraint $z^\dagger z\leq Nr^2$. The resulting configuration space is a complex
manifold with boundary. We shall see that the `radius' $r$ proves an insightful
knob in our present problem, revealing structure as it is varied. Note
-that---combined with the constraint $z^2=N$---taking $r=1$ reduces the problem
+that---combined with the constraint $z^Tz=N$---taking $r=1$ reduces the problem
to that of the ordinary $p$-spin.
The critical points are of $H$ given by the solutions to the set of equations
@@ -211,8 +210,7 @@ be averaged independently. The $\delta$-functions are converted to exponentials
by the introduction of auxiliary fields $\hat z=\hat x+i\hat y$. The average
of those factors over $J$ can then be performed. A generalized
Hubbard--Stratonovich allows a change of variables from the $4N$ original
-and auxiliary fields to eight bilinears defined by $Na=|z|^2$, $N\hat a=|\hat
-z|^2$, $N\hat c=\hat z^2$, $Nb=\hat z^*z$, and $Nd=\hat zz$ (and their
+and auxiliary fields to eight bilinears defined by $Na=z^\dagger z$, $N\hat a=\hat z^\dagger\hat z$, $N\hat c=\hat z^T\hat z$, $Nb=\hat z^\dagger z$, and $Nd=\hat z^Tz$ (and their
conjugates). The result, to leading order in $N$, is
\begin{equation} \label{eq:saddle}
\overline{\mathcal N}(\kappa,\epsilon,r)
@@ -244,10 +242,7 @@ where $\theta=\frac12\arg\kappa$ and
\begin{equation}
C_{\pm}=\frac{a^p(1+p(a^2-1))\mp a^2|\kappa|}{a^{2p}\pm(p-1)a^p(a^2-1)|\kappa|-a^2|\kappa|^2}.
\end{equation}
-This leaves a single parameter, $a$, which dictates the magnitude of $|z|^2$,
-or alternatively the magnitude $y^2$ of the imaginary part. The latter vanishes
-as $a\to1$, where (as we shall see) one recovers known results for the real
-$p$-spin.
+This leaves a single parameter, $a$, which dictates the norm of $z$.
The Hessian $\partial\partial H=\partial\partial H_0-p\epsilon I$ is equal to
the unconstrained Hessian with a constant added to its diagonal. The eigenvalue
@@ -385,9 +380,8 @@ in supersymmetric quiver theories \cite{Manschot_2012_From}.
\includegraphics{fig/complexity.pdf}
\caption{
The complexity of the 3-spin model at $\epsilon=0$ as a function of
- the maximum `radius' $r=|z_{\mathrm{max}}|/\sqrt N$ at several values of
- $\kappa$. The dashed line shows $\frac12\log(p-1)$, while the dotted shows
- $\log(p-1)$.
+ the maximum `radius' $r$ at several values of $\kappa$. The dashed line
+ shows $\frac12\log(p-1)$, while the dotted shows $\log(p-1)$.
} \label{fig:complexity}
\end{figure}