$ cargo run --release parameters/test.yaml
- Dormand–Prince 5(4) method (1980).
- [TODO] Fehlberg ERK7(8) (1968).
ref. "Hairer, Ernst; Nørsett, Syvert Paul; Wanner, Gerhard (1993), Solving ordinary differential equations I: Nonstiff problems, Berlin, New York".
- Simon F. Portegies Zwart (Leiden Observatory), Tjarda C.N. Boekholt (Clarendon Laboratory, Oxford), Emiel Por (STScI), Adrian S. Hamers (MPI), Steve L.W. McMillan (Drexel), Chaos in self-gravitating many-body systems: Lyapunov time dependence of N and the influence of general relativity
- I use (4) formula of page 5.
- Yousuke Itoh, Post-Newtonian equations of motion for relativistic compact binaries (2013)
- Yousuke Itoh, Post-Newtonian approximation and gravitational waves from compact binaries (2017)
- The literature mentions 3.5PN.
- Sergei Kopeikin, Yi Xie, Post-Newtonian Reference Frames for Advanced Theory of the Lunar Motion and a New Generation of Lunar Laser Ranging
- Kei Yamada, Triangular solution to the general relativistic three-body problem
- Yi Xie, Sergei Kopeikin, Post-Newtonian Mechanics of the Earth-Moon System
- Sverre J. Aarseth, Post-Newtonian N-body simulations
- Luc Blanchet, Post-Newtonian theory and the two-body problem