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arXiv 2109.00611math-phmath.MP
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Noncommutative Kepler Dynamics: symmetry groups and bi-Hamiltonian structures

Mahouton Norbert Hounkonnou, Mahougnon Justin Landalidji, Melanija Mitrovic

英文摘要:

Integrals of motion are constructed from noncommutative (NC) Kepler dynamics, generating $SO(3),$ $SO(4),$ and $SO(1,3)$ 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.

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