English

Noncommutative Kepler Dynamics: symmetry groups and bi-Hamiltonian structures

Mathematical Physics 2021-09-03 v1 math.MP

Abstract

Integrals of motion are constructed from noncommutative (NC) Kepler dynamics, generating SO(3),SO(3), SO(4),SO(4), and SO(1,3)SO(1,3) dynamical symmetry groups. The Hamiltonian vector field is derived in action-angle coordinates, and the existence of a hierarchy of bi-Hamiltonian structures is highlighted. Then, a family of Nijenhuis recursion operators is computed and discussed.

Keywords

Cite

@article{arxiv.2109.00611,
  title  = {Noncommutative Kepler Dynamics: symmetry groups and bi-Hamiltonian structures},
  author = {Mahouton Norbert Hounkonnou and Mahougnon Justin Landalidji and Melanija Mitrovic},
  journal= {arXiv preprint arXiv:2109.00611},
  year   = {2021}
}
R2 v1 2026-06-24T05:36:35.362Z