Application of the logarithmic Hamiltonian algorithm to the circular restricted three-body problem with some post-Newtonian terms
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  • 作者:Xiang-Ning Su ; Xin Wu ; Fu-Yao Liu
  • 关键词:Celestial mechanics ; Symplectic integrator ; Circular restricted three ; body problem ; Chaos
  • 刊名:Astrophysics and Space Science
  • 出版年:2016
  • 出版时间:January 2016
  • 年:2016
  • 卷:361
  • 期:1
  • 全文大小:1,465 KB
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  • 作者单位:Xiang-Ning Su (1)
    Xin Wu (1)
    Fu-Yao Liu (2)

    1. Department of Physics & Institute of Astronomy, Nanchang University, Nanchang, 330031, China
    2. School of Mathematics and Information, Shanghai Lixin University of Commerce, Shanghai, 201600, China
  • 刊物类别:Physics and Astronomy
  • 刊物主题:Physics
    Astronomy
  • 出版者:Springer Netherlands
  • ISSN:1572-946X
文摘
An implementation of a fourth-order symplectic algorithm to the logarithmic Hamiltonian of the Newtonian circular restricted three-body problem in an inertial frame is detailed. The logarithmic Hamiltonian algorithm produces highly accurate results, comparable to the non-logarithmic one. Its numerical performance is independent of an orbital eccentricity. However, it is not when some post-Newtonian terms are included in this problem. Although the numerical accuracy becomes somewhat poorer as the orbital eccentricity gets larger, it is still much higher than that of the non-logarithmic Hamiltonian algorithm. As a result, the present code can drastically eliminate the overestimation of Lyapunov exponents and the spurious rapid growth of fast Lyapunov indicators for high-eccentricity orbits in the Newtonian or post-Newtonian circular restricted three-body problem.

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