Algorithmic regularization with velocity-dependent forces
Abstract
Algorithmic regularization uses a transformation of the equations of motion such that the leapfrog algorithm produces exact trajectories for two-body motion as well as regular results in numerical integration of the motion of strongly interacting few-body systems. That algorithm alone is not sufficiently accurate and one must use the extrapolation method for improved precision. This requires that the basic leapfrog algorithm be time-symmetric, which is not directly possible in the case of velocity-dependent forces, but is usually obtained with the help of the implicit mid-point method. Here, we suggest an alternative explicit algorithmic regularization algorithm which can handle velocity-dependent forces. This is done with the help of a generalized mid-point method to obtain the required time symmetry, thus eliminating the need for the implicit mid-point method and allowing the use of extrapolation.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- October 2006
- DOI:
- 10.1111/j.1365-2966.2006.10854.x
- arXiv:
- arXiv:astro-ph/0605054
- Bibcode:
- 2006MNRAS.372..219M
- Keywords:
-
- stellar dynamics: methods: N-body simulations: celestial mechanics;
- stellar dynamics;
- methods: N-body simulations;
- celestial mechanics;
- Astrophysics
- E-Print:
- 5 pages, 2 figures. Uses mn2e.cls