Periodicity characterization by capacities for star-shaped domains
Jean Gutt, Vinicius G. B. Ramos, Shira Tanny
TL;DR
The paper advances the spectral classification of Reeb flows on boundaries of star-shaped domains by establishing that Besse flows correspond to blocks of equal equivariant symplectic-homology capacities, with the block length determined by the Morse–Bott data of the period orbit manifold. Using Morse–Bott indices, mean indices, and the $S^1$-equivariant SH barcode, the authors prove dynamic convexity for Besse domains and show that the SH spectrum aligns with the periods of the flow; this yields concrete criteria: a common equality of the first $n$ capacities implies Zoll, while a single orbit period yields a structured capacity chain of length $n$ and a precise index relation $k= frac12(\mu_-(S_\mathcal{T})-n+1)$. The work also identifies the Morse–Bott fixed-point sets $Y_T$ as ${\mathbb{F}}_2$-homology spheres and proves a diagonal SH barcode, enabling a complete spectral characterization in terms of capacities. Collectively, the results extend Ginzburg–Gürel–Mazzucchelli’s framework to general star-shaped domains (beyond convex cases) and provide a robust toolkit for understanding Zoll/Besse phenomena via symplectic-homology invariants.
Abstract
We complete the spectral characterization of Besse and Zoll Reeb flows on the standard contact sphere $S^{2n-1}$ initiated by Ginzburg-Gürel-Mazzucchelli. Roughly speaking, it states that a Reeb flow on the boundary of any star-shaped domain in $\mathbb{R}^{2n}$ is Besse if and only if it has $n$ coinciding Ekeland-Hofer capacities, and that it is Zoll if and only if the first $n$ capacities coincide.
