On the Density of Periodic Measures for Star Vector Fields
Qimai Sun, Guangwa Wang, Wanlou Wu
TL;DR
The paper proves that for a $C^1$ star vector field $X$ on a compact $d$-manifold, every ergodic hyperbolic invariant measure not supported on singularities can be approximated in the weak$^*$ topology by periodic measures. The authors develop Lyapunov-norm techniques and Lyapunov charts in the presence of singularities, leveraging the scaled linear Poincaré flow $\psi_t^*$ and its dominated splitting to obtain a shadowing framework (Liao shadowing) for quasi-hyperbolic strings. They then perform a case analysis on the Lyapunov spectrum: if all exponents share the same sign, the measure is supported on a periodic orbit; if not, a dominated splitting coincides with the Oseledets splitting, enabling the construction of a periodic orbit that approximates the given ergodic measure in the weak$^*$ sense. This extends Katok’s density result from $C^{1+\alpha}$ diffeomorphisms to $C^1$ star vector fields, addressing singularities and higher-dimensional settings.
Abstract
In this paper, we prove that every ergodic hyperbolic invariant measure of a $C^1$ star vector field can be approximated by periodic measures in weak$^*$ topology. This extends a classical result of Katok \cite{Ka} for $C^{1+α}(α>0)$ diffeomorphisms to $C^1$ star vector field of any dimension.
