(IBM, 2004) Lake, G.; Quinn, T.; Richardson, D. C.; Stadel, J.
We describe the keys to meeting the challenges of N-body
simulation: adaptive potential solvers, adaptive integration,
and volume renormalization. With these techniques and a
dedicated teraflop facility, simulation can keep pace with
observations of the universe. We also describe some problems
in simulating the formation and stability of planetary systems.
