A Multiple Time Step Symplectic Algorithm for Integrating Close Encounters

We present a new symplectic algorithm that has the desirable properties of the sophisticated but highly efficient numerical algorithms known as mixed variable symplectic (MVS) methods and that, in addition, can handle close encounters between objects. This technique is based on a variant of the standard MVS methods, but it handles close encounters by employing a multiple time step technique. When the bodies are well separated, the algorithm has the speed of MVS methods, and whenever two bodies suffer a mutual encounter, the time step for the relevant bodies is recursively subdivided to whatever level is required. We demonstrate the power of this method using several tests of the technique. We believe that this algorithm will be a valuable tool for the study of planetesimal dynamics and planet formation.

[1]  J. Lissauer,et al.  Orbital Stability of the Uranian Satellite System , 1997 .

[2]  S. Ida,et al.  Lunar accretion from an impact-generated disk , 1997, Nature.

[3]  Harold F. Levison,et al.  The Long-Term Dynamical Behavior of Short-Period Comets , 1993 .

[4]  Robert D. Skeel,et al.  Does variable step size ruin a symplectic integrator , 1992 .

[5]  J. M. Sanz-Serna,et al.  Numerical Hamiltonian Problems , 1994 .

[6]  H. Yoshida Construction of higher order symplectic integrators , 1990 .

[7]  M. Moutsoulas,et al.  Theory of orbits , 1968 .

[8]  Jack Wisdom,et al.  Dynamical Stability in the Outer Solar System and the Delivery of Short Period Comets , 1993 .

[9]  Robert D. Skeel,et al.  Dangers of multiple time step methods , 1993 .

[10]  R. Ruth,et al.  Fourth-order symplectic integration , 1990 .

[11]  Harold F. Levison,et al.  The Dynamical Structure of the Kuiper Belt , 1995 .

[12]  J. Wisdom,et al.  Symplectic maps for the N-body problem. , 1991 .

[13]  R. Ruth A Can0nical Integrati0n Technique , 1983, IEEE Transactions on Nuclear Science.

[14]  S. Tremaine,et al.  Symplectic integrators for solar system dynamics , 1992 .

[15]  Victor Szebehely,et al.  Theory of Orbits. , 1967 .

[16]  S. Tremaine,et al.  Long-Term Planetary Integration With Individual Time Steps , 1994, astro-ph/9403057.

[17]  J. Lissauer,et al.  Accretion rates of protoplanets , 1990 .

[18]  Jack Wisdom,et al.  Lie-Poisson integrators for rigid body dynamics in the solar system , 1994 .