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Orbital stability of the restricted three body problem in General Relativity

We consider the problem of orbital stability of the motion of a test particle in the restricted three-body problem, by using the orbital moment and its time derivative. We show that it is possible to get some insight into the stability properties of the motion of test particles, without knowing the exact solutions of the motion equations.

preprint2015arXivOpen access
M. AbishevH. QuevedoS. ToktarbayB. Zhami
gr-qc
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Open access4 authors1 topic
Imported metadata coverageMissing code, dataset, citation and institution fields are tracked without dominating the paper.Details
Citations: 0Reviews: 0Saves: 0Code: not linkedDataset: not linkedInstitutions: 0

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M. AbishevH. QuevedoS. ToktarbayB. Zhami

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