Polynomial Maximal Surfaces in H^{2,2} and Spherical Polygons

Abstract

We study the moduli space of complete maximal surfaces in pseudo-hyperbolic space $\mathbf{H}^{2,2}$ with polygonal asymptotic boundary a lightlike $(n+4)$-gon in the Einstein universe $\mathbf{Ein}^{1,2}$, up to the action of $\mathsf{SO}_0(2,3)$. Importantly, this space $M_{n+4}(\mathbf{H}^{2,2})$ is disconnected for $n\geq 2$. We introduce a \emph{turning invariant} $Θ$ that classifies the components in terms of the geometry of the boundary polygons in the Einstein universe $\mathbf{Ein}^{1,2}$, which is related to \emph{spherical polygons} in $\mathbb{S}^2$. We provide a geometric parametrization of the moduli space $M_{n+4}(\mathbf{H}^{2,2})$ via holomorphic data, namely a pair of polynomials $α$, $β$. These polynomials appear in relation to certain components of the complexified second fundamental form of the corresponding surface. We then relate the holomorphic data $α,β$ with the turning invariant $Θ$. This leads to characterizations of the \emph{Hitchin component} of polygonal maximal surfaces studied by Tamburelli-Wolf.