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At most exponential growth of periodic orbits for star flows

C. A. Morales, E. Rego, X. Wen

math.DSarXiv:2608.30119

Abstract

We prove that on any closed manifold there exists a C1 open and dense subset of star flows for which the periodic orbits grow at most expo- nentially. We also explain how our methods apply to the sectional-hyperbolic attractors including the Lorenz polynomial equation.

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