Attractors and orbit-flip homoclinic orbits for star flows
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Abstract:
We study star flows on closed $3$-manifolds and prove that they either have a finite number of attractors or can be $C^1$ approximated by vector fields with orbit-flip homoclinic orbits.References
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Additional Information
- C. A. Morales
- Affiliation: Instituto de Matemática, Universidade Federal do Rio de Janeiro, P. O. Box 68530, 21945-970 Rio de Janeiro, Brazil
- MR Author ID: 611238
- ORCID: 0000-0002-4808-6902
- Email: morales@impa.br
- Received by editor(s): July 28, 2001
- Received by editor(s) in revised form: November 3, 2011
- Published electronically: April 12, 2013
- Additional Notes: The author was partially supported by CNPq, FAPERJ and PRONEX-Brazil.
- Communicated by: Bryna Kra
- © Copyright 2013
American Mathematical Society
The copyright for this article reverts to public domain 28 years after publication. - Journal: Proc. Amer. Math. Soc. 141 (2013), 2783-2791
- MSC (2010): Primary 37D20; Secondary 37C10
- DOI: https://doi.org/10.1090/S0002-9939-2013-11535-2
- MathSciNet review: 3056568