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astro-ph1999
Direct N-body Simulations
R. Spurzem
Special high-accuracy direct force summation N-body algorithms and their relevance for the simulation of the dynamical evolution of star clusters and other gravitating N-body syste…
astro-ph1999
AHA-GRAPE: Adaptive Hydrodynamic Architecture - GRAvity PipE
T. Kuberka, A. Kugel, R. Maenner +3
In astrophysics numerical star cluster simulations and hydrodynamical methods like SPH require computational performance in the petaflop range. The GRAPE family of ASIC-based accel…