JournalsaihpcVol. 5, No. 3pp. 287–295

Non-collision orbits for a class of Keplerian-like potentials

  • Antonio Ambrosetti

    Scuola Normale Superiore, Piazza dei Cavalieri, 56100 Pisa, Italy

  • Vittorio Coti Zelati

    CEREMADE, Université de Paris-Dauphine, Place du M.-de-Lattre-de-Tassigny, 75775 Paris Cedex 16, France
Non-collision orbits for a class of Keplerian-like potentials cover
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Abstract

We prove the existence of non-collision orbits with large period for a class of Keplerian-like dynamical systems.

Résumé

Nous prouvons l’existence d’orbites de non-collision avec grand period pour une classe de systèmes dynamiques de type keplerien.

Cite this article

Antonio Ambrosetti, Vittorio Coti Zelati, Non-collision orbits for a class of Keplerian-like potentials. Ann. Inst. H. Poincaré Anal. Non Linéaire 5 (1988), no. 3, pp. 287–295

DOI 10.1016/S0294-1449(16)30347-X