4.7 Article

Modification of logarithmic Hamiltonians and application of explicit symplectic-like integrators

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 469, Issue 3, Pages 3031-3041

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stx1059

Keywords

chaos; methods: numerical; celestial mechanics; planets and satellites: dynamical evolution and stability

Funding

  1. National Natural Science Foundation of China [11533004]
  2. Natural Science Foundation of Jiangxi Province [20153BCB22001]

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We modify the logarithmic Hamiltonian of Mikkola and Tanikawa by adding a constant (or function) to both the kinetic energy and the force function. Explicit symplectic algorithms are available when the logarithmic Hamiltonian has two separable parts of coordinates and momenta. However, they are not if the logarithmic Hamiltonian is inseparable. Fortunately, they are still efficient by manipulating the logarithmic Hamiltonian as a new separable Hamiltonian in an extended phase space. In fact, they belong to symplectic-like integrators. The choice of mixing maps affects the performance of the considered symplectic-like integrators. It is shown that two maps about sequent permutations of coordinates and momenta are inferior to a map with mid-point permutations in some cases. The choice of the constant (or function) added also exerts some influence on the performance of the algorithms. As a result, with the help of the mid-point permutations and a suitable choice for the constant (or function) included, the logarithmic Hamiltonian methods bring an increase in accuracy compared to the non-logarithmic ones, particularly for highly eccentric orbits.

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