A method of symplectic integrations with adaptive time-steps for individual Hamiltonians in the planetary N-body problem

Details A method of symplectic integrations with adaptive time-steps for individual Hamiltonians in the planetary N-body problem A method of symplectic integrations with adaptive time-steps for individual Hamiltonians in the planetary N-body problem

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007cemda..98..191e&link_type=abstract

Celestial Mechanics and Dynamical Astronomy, Volume 98, Issue 3, pp.191-202

Astronomy and Astrophysics

Astronomy

6

Scientific paper

A new algorithm is developed for long-term integrations of the N-body problem. The method uses symplectic integrations of the Hamiltonian equations of motion for each body. This allows one to employ individual adaptive time-steps in computations. The efficiency of this technique is demonstrated by several tests performed for typical problems of Solar System dynamics.

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