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This article is cited in 5 scientific papers (total in 5 papers)
Noncommutative Kepler dynamics: symmetry groups and bi-Hamiltonian structures
M. N. Hounkonnoua, M. J. Landalidjia, M. Mitrovićb a University of Abomey-Calavi, Cotonou, Republic of Benin
b Faculty of Mechanical Engineering, Department of Mathematics and Informatics, University
of Niš, Serbia
Abstract:
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.
Keywords:
Bi-Hamiltonian structure, noncommutative phase space, recursion
operator, Kepler dynamics, dynamical symmetry groups.
Received: 03.12.2020 Revised: 03.12.2020
Citation:
M. N. Hounkonnou, M. J. Landalidji, M. Mitrović, “Noncommutative Kepler dynamics: symmetry groups and bi-Hamiltonian structures”, TMF, 207:3 (2021), 403–423; Theoret. and Math. Phys., 207:3 (2021), 751–769
Linking options:
https://www.mathnet.ru/eng/tmf10017https://doi.org/10.4213/tmf10017 https://www.mathnet.ru/eng/tmf/v207/i3/p403
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Abstract page: | 237 | Full-text PDF : | 63 | References: | 28 | First page: | 11 |
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