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Cited by 318

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High order symplectic integrators for perturbed Hamiltonian systems

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Laskar, Jacques, Robutel, Philippe·2001·Celestial Mechanics and Dynamical Astronomy

Abstract

A family of symplectic integrators adapted for the integration of perturbed Hamiltonian systems of the form H = A + εB was given in (McLachlan, 1995). We give here a constructive proof that for all integer p, such integrator exists, with only positive steps, and with a remainder of order O(τpε + τ2ε2), where τ is the stepsize of the integrator. Moreover, we compute the analytical expressions of the leading terms of the remainders at all orders. We show also that for a large class of systems, a corrector step can be performed such that the remainder becomes O(τpε +τ4ε2). The performances of these integrators are compared for the simple pendulum and the planetary three-body problem of Sun–Jupiter–Saturn.

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Metadata

Authors
Laskar, J., & Robutel, P.
Venue
Celestial Mechanics and Dynamical Astronomy
Published
2001-05
Volume
80
Issue
1
Pages
39-62
ISSN
  • 0923-2958 (ISSN-L)
  • 1572-9478
OpenAlex
W1749808203
Cited by
318
References
13
FWCI
5.74
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: High order symplectic integrators for perturbed Hamiltonian systems. https://app.cochat.ai/papers/10.1023/a:1012098603882
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Laskar, J., & Robutel, P. (2001). High order symplectic integrators for perturbed Hamiltonian systems. Celestial Mechanics and Dynamical Astronomy. https://doi.org/10.1023/a%3A1012098603882

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