English

Performance Analysis of Direct N-Body Algorithms on Special-Purpose Supercomputers

Astrophysics 2008-11-26 v1

Abstract

Direct-summation N-body algorithms compute the gravitational interaction between stars in an exact way and have a computational complexity of O(N^2). Performance can be greatly enhanced via the use of special-purpose accelerator boards like the GRAPE-6A. However the memory of the GRAPE boards is limited. Here, we present a performance analysis of direct N-body codes on two parallel supercomputers that incorporate special-purpose boards, allowing as many as four million particles to be integrated. Both computers employ high-speed, Infiniband interconnects to minimize communication overhead, which can otherwise become significant due to the small number of "active" particles at each time step. We find that the computation time scales well with processor number; for 2*10^6 particles, efficiencies greater than 50% and speeds in excess of 2 TFlops are reached.

Keywords

Cite

@article{arxiv.astro-ph/0608125,
  title  = {Performance Analysis of Direct N-Body Algorithms on Special-Purpose Supercomputers},
  author = {Stefan Harfst and Alessia Gualandris and David Merritt and Rainer Spurzem and Simon Portegies Zwart and Peter Berczik},
  journal= {arXiv preprint arXiv:astro-ph/0608125},
  year   = {2008}
}

Comments

34 pages, 15 figures, submitted to New Astronomy

R2 v1 2026-07-22T09:11:03.721Z