Star Decompositions of a Cyclic Polygon
Tomoki Nakamigawa
TL;DR
This work studies star decompositions of cyclic polygons, introducing a framework of cycle decompositions built from diagonals and stars. It proves that any two maximal star decompositions of a common cyclic polygon are connected by a finite sequence of diagonal flips, and establishes a precise count of diagonals in a maximal decomposition as $p - \frac{(n-2r)(n-2r-1)}{2}$, where $p$ is the total number of diagonals, $n$ the vertex count, and $r$ the rotation number. The paper also discusses existence conditions for star decompositions and provides exact counts for special families like $P_n^k$, linking to Catalan-related structures and Dick-path fans. These results extend combinatorial triangulation concepts to generalized star decompositions, with implications for pseudo-triangulations and related geometric complexes.
Abstract
Let $V$ be a set of vertices on a circumference in the plane. Let $E$ be a set of directed line segments linking two vertices of $V$. If $E$ forms a set of closed cycles and for all two adjacent edges $uv$ and $vw$, the vertices $u$, $v$, $w$ are arranged in anti-clockwise order, we call $P(V,E)$ a cyclic polygon. A star decomposition $\mathcal{S}$ of a cyclic polygon $P$ is a set of star polygons partitioning the region of $P$ with some additional diagonals. A star decomposition $\mathcal{S}$ is called maximal if there is no other star decomposition $\mathcal{S}'$ such that a set of diagonals of $\mathcal{S}$ is a proper subset of that of $\mathcal{S}'$. In this paper, it is shown that for any two maximal star decompositions $\mathcal{S}_1$ and $\mathcal{S}_2$ of a common cyclic polygon, $\mathcal{S}_1$ can be transformed into $\mathcal{S}_2$ by a finite sequence of diagonal flips. It is also shown that if a cyclic polygon $P$ admits a star decomposition, the number of diagonals contained in a maximal star decomposition of $P$ is $p - (n-2r)(n-2r-1)/2$, where $p$ is the number of all possible diagonals of $P$, $n$ is the number of vertices of $P$, and $r$ is the rotation number of $P$.
