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Spin-glasses have long been considered the paradigm of many variable `complex
landscapes,' a subject that includes neural networks and optimization problems,
-most notably constraint satisfaction. The most tractable family of these
+most notably constraint satisfaction \cite{Mezard_2009_Information}. The most tractable family of these
are the mean-field spherical $p$-spin models \cite{Crisanti_1992_The} (for a
review see \cite{Castellani_2005_Spin-glass}) defined by the energy
\begin{equation} \label{eq:bare.hamiltonian}
@@ -72,35 +72,37 @@ constraint remains $z^2=N$.
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
-problems: such is the case in which they are \emph{phases}, as in random laser
-problems \cite{Antenucci_2015_Complex}. Quiver Hamiltonians---used to model
-black hole horizons in the zero-temperature limit---also have a Hamiltonian
-very close to ours \cite{Anninos_2016_Disordered}.
-
-There is however a more fundamental reason for this study: we know from
-experience that extending a real problem to the complex plane often uncovers
-underlying simplicity that is otherwise hidden. Consider, for example, the
-procedure of starting from a simple, known Hamiltonian $H_{00}$ and studying
-$\lambda H_{00} + (1-\lambda H_{0} )$, evolving adiabatically from $\lambda=0$
-to $\lambda=1$, as is familiar from quantum annealing. The $H_{00}$ is a
-polynomial of degree $p$ chosen to have simple, known saddles. Because we are
-working in complex variables, and the saddles are simple all the way (we shall
-confirm this), we may follow a single one from $\lambda=0$ to $\lambda=1$,
-while with real variables minima of functions appear and disappear, and this
-procedure is not possible. The same idea may be implemented by performing
-diffusion in the $J$s and following the roots, in complete analogy with Dyson's
-stochastic dynamics \cite{Dyson_1962_A}.
-
-The spherical constraint is enforced using the method of Lagrange multipliers:
-introducing $\epsilon\in\mathbb C$, our energy is
+problems: such is the case in which the variables are \emph{phases}, as in
+random laser problems \cite{Antenucci_2015_Complex}. Quiver Hamiltonians---used
+to model black hole horizons in the zero-temperature limit---also have a
+Hamiltonian very close to ours \cite{Anninos_2016_Disordered}. A second reason
+is that, as we know from experience, extending a real problem to the complex
+plane often uncovers underlying simplicity that is otherwise hidden, sheding
+light on the original real problem, e.g., as in the radius of convergence of a
+series.
+
+Deforming an integral in $N$ real variables to a surface of dimension $N$ in
+$2N$-dimensional complex space has turned out to be necessary for correctly
+defining and analyzing path integrals with complex action (see
+\cite{Witten_2010_A, Witten_2011_Analytic}), and as a useful palliative for the
+sign problem \cite{Cristoforetti_2012_New, Tanizaki_2017_Gradient,
+Scorzato_2016_The}. In order to do this correctly, the features of landscape
+of the action in complex space---like the relative position of its
+saddles---must be understood. Such landscapes are in general not random: here
+we propose to follow the strategy of computer science of understanding the
+generic features of random instances, expecting that this sheds light on the
+practical, nonrandom problems.
+
+Returning to our problem, the spherical constraint is enforced using the method
+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}
- We choose to
-constrain our model by $z^2=N$ rather than $|z|^2=N$ in order to preserve the
-analyticity of $H$. The nonholomorphic constraint also has a disturbing lack of
-critical points nearly everywhere: if $H$ were so constrained, then
-$0=\partial^* H=-p\epsilon z$ would only be satisfied for $\epsilon=0$.
+We choose to constrain our model by $z^2=N$ rather than $|z|^2=N$ in order to
+preserve the analyticity of $H$. The nonholomorphic constraint also has a
+disturbing lack of critical points nearly everywhere: if $H$ were so
+constrained, then $0=\partial^* H=-p\epsilon z$ would only be satisfied for
+$\epsilon=0$.
The critical points are of $H$ given by the solutions to the set of equations
\begin{equation} \label{eq:polynomial}
@@ -108,12 +110,11 @@ The critical points are of $H$ given by the solutions to the set of equations
= p\epsilon z_i
\end{equation}
for all $i=\{1,\ldots,N\}$, which for fixed $\epsilon$ is a set of $N$
-equations of degree $p-1$, to which one must add the constraint.
-In this sense
+equations of degree $p-1$, to which one must add the constraint. In this sense
this study also provides a complement to the work on the distribution of zeroes
of random polynomials \cite{Bogomolny_1992_Distribution}, which are for $N=1$
-and $p\to\infty$.
-We see from \eqref{eq:polynomial} that at any critical point, $\epsilon=H/N$, the average energy.
+and $p\to\infty$. We see from \eqref{eq:polynomial} that at any critical
+point, $\epsilon=H/N$, the average energy.
Since $H$ is holomorphic, any critical point of $\operatorname{Re}H$ is also a
critical point of $\operatorname{Im}H$. The number of critical points of $H$ is
@@ -444,18 +445,23 @@ the complex case. The relationship between the threshold, i.e., where the gap
appears, and the dynamics of, e.g., a minimization algorithm or physical
dynamics, are a problem we hope to address in future work.
-This paper provides a first step for the study of a complex landscape with
-complex variables. The next obvious one is to study the topology of the
-critical points and gradient lines of constant phase. We anticipate that the
-threshold level, where the system develops a mid-spectrum gap, will play a
-crucial role as it does in the real case.
+ This paper provides a first step towards the study of a complex landscape with
+ complex variables. The next obvious one is to study the topology of the
+ critical points, the sets reached following gradient descent (the
+ Lefschetz thimbles), and ascent (the anti-thimbles) \cite{Witten_2010_A,
+ Witten_2011_Analytic, Cristoforetti_2012_New, Behtash_2017_Toward,
+ Scorzato_2016_The}, which act as constant-phase integrating `contours.'
+ Locating and counting the saddles that are joined by gradient lines---the
+ Stokes points, which play an important role in the theory---is also well within
+ reach of the present-day spin-glass literature techniques. We anticipate
+ that the threshold level, where the system develops a mid-spectrum gap, will
+ play a crucial role as it does in the real case.
\begin{acknowledgments}
We wish to thank Alexander Altland, Satya Majumdar and Gregory Schehr for a useful suggestions.
JK-D and JK are supported by the Simons Foundation Grant No.~454943.
\end{acknowledgments}
-\bibliographystyle{apsrev4-2}
\bibliography{bezout}
\end{document}