Dynamics of a test particle around two massive bodies in decay circular orbits

DOI10.1007/S10714-014-1798-8zbMath1305.83025OpenAlexW1992466860MaRDI QIDQ481740

Xin Wu, Guoqing Huang

Publication date: 12 December 2014

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10714-014-1798-8

zbMATH Keywords

chaoscircular restricted three-body problemorbital decay

Mathematics Subject Classification ID

Three-body problems (70F07) Dynamical systems in other branches of physics (quantum mechanics, general relativity, laser physics) (37N20) Equations of motion in general relativity and gravitational theory (83C10) Gravitational waves (83C35)

Related Items (3)

Uniqueness of First Order Post-Newtonian Collinear Solutions for Three-Body Problem under a Scalar-Tensor Theory ⋮ Reliability of Lyapunov characteristic exponents computed by the two-particle method ⋮ Effects of manifold correction methods on chaos indicators

Cites Work

• Fast Lyapunov indicators. Application to asteroidal motion
• Computation of Lyapunov exponents in general relativity
• Gravitational Waves from a Pseudo-Newtonian Kerr Field with Halos
• Binary black hole initial data for numerical general relativity based on post-Newtonian data
• Lyapunov timescales and black hole binaries
• Solar System Dynamics

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