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A Canonical Transformation to Eliminate Resonant Perturbations. I.
被引:0
|作者:
Deme, Barnabas
[1
]
Kocsis, Bence
[1
,2
]
机构:
[1] Eotvos Lorand Univ, Inst Phys, Pazmany PS 1-A, H-1117 Budapest, Hungary
[2] Clarendon Lab, Rudolf Peierls Ctr Theoret Phys, Parks Rd, Oxford OX1 3PU, England
来源:
基金:
欧洲研究理事会;
关键词:
EVOLUTION;
SYSTEMS;
MOTION;
D O I:
10.3847/1538-3881/abfb6d
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We study dynamical systems that admit action-angle variables at leading order, which are subject to nearly resonant perturbations. If the frequencies characterizing the unperturbed system are not in resonance, the long-term dynamical evolution may be integrated by orbit-averaging over the high-frequency angles, thereby evolving the orbit-averaged effect of the perturbations. It is well known that such integrators may be constructed via a canonical transformation, which eliminates the high-frequency variables from the orbit-averaged quantities. An example of this algorithm in celestial mechanics is the von Zeipel transformation. However, if the perturbations are inside or close to a resonance, i.e., the frequencies of the unperturbed system are commensurate; these canonical transformations are subject to divergences. We introduce a canonical transformation that eliminates the high-frequency phase variables in the Hamiltonian without encountering divergences. This leads to a well-behaved symplectic integrator. We demonstrate the algorithm through two examples: a resonantly perturbed harmonic oscillator and the gravitational three-body problem in mean motion resonance.
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页数:11
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