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Star flows: a characterization via Lyapunov functions

Abstract

We say that a differentiable flow or vector field XX is star on a compact invariant set Ξ›\Lambda of the Riemannian manifold M if there exist neighborhoods U∈X1(M)\mathcal{U} \in \mathfrak{X}^1(M) of XX and UβŠ‚MU \subset M of Ξ›\Lambda for which every closed orbit in UU of every vector field YY in U\mathcal{U} is hyperbolic. In this work, it is presented a characterization of star condition for flows based on Lyapunov functions. It is obtained conditions to strong homogeneity for singular sets for a C1C^1 flow by using the notion of infinitesimal Lyapunov functions. As an application we obtain some results related to singular hyperbolic sets for flows.Comment: 22 pages, 1 figure. It were done many changes in the text and included more details into the proof of a main theorem. Proposition 4.3 stated to linear cocycles. arXiv admin note: text overlap with arXiv:1611.04072, arXiv:1201.255

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