In this paper we give some positive and negative results about the contact property for the energy levels Σcof a symplectic magnetic field on S2. In the first part we focus on the case of the area form on a surface of revolution. We state a sufficient condition for an energy level to be of contact type and give an example where the contact property fails. If the magnetic curvature is positive, the dynamics and the action of invariant measures can be numerically computed. The collected data hint at the conjecture that an energy level of a symplectic magnetic field with positive magnetic curvature should be of contact type. In the second part we show that, for a small energy c, there exist a convex hypersurface Nc in C2 and a double cover Nc !Σc such that the pull-back of the characteristic distribution on Σc is the standard characteristic distribution on Nc. As a corollary, we prove that there are either two or infinitely many periodic orbits on Σc. The second alternative holds if there exists a contractible prime periodic orbit.

The contact property for symplectic magnetic fields on S2 / Benedetti, G.. - In: ERGODIC THEORY & DYNAMICAL SYSTEMS. - ISSN 0143-3857. - 760:3(2014), pp. 682-713. [10.1017/etds.2014.82]

The contact property for symplectic magnetic fields on S2

Benedetti G.
2014-01-01

Abstract

In this paper we give some positive and negative results about the contact property for the energy levels Σcof a symplectic magnetic field on S2. In the first part we focus on the case of the area form on a surface of revolution. We state a sufficient condition for an energy level to be of contact type and give an example where the contact property fails. If the magnetic curvature is positive, the dynamics and the action of invariant measures can be numerically computed. The collected data hint at the conjecture that an energy level of a symplectic magnetic field with positive magnetic curvature should be of contact type. In the second part we show that, for a small energy c, there exist a convex hypersurface Nc in C2 and a double cover Nc !Σc such that the pull-back of the characteristic distribution on Σc is the standard characteristic distribution on Nc. As a corollary, we prove that there are either two or infinitely many periodic orbits on Σc. The second alternative holds if there exists a contractible prime periodic orbit.
2014
760
3
682
713
Benedetti, G.
File in questo prodotto:
Non ci sono file associati a questo prodotto.

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.11767/150916
 Attenzione

Attenzione! I dati visualizzati non sono stati sottoposti a validazione da parte dell'ateneo

Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus ND
  • ???jsp.display-item.citation.isi??? ND
social impact