Hostname: page-component-78c5997874-xbtfd Total loading time: 0 Render date: 2024-11-06T01:19:08.456Z Has data issue: false hasContentIssue false
  • English
  • Français

Grape-4: A Teraflops Machine for N-Body Simulations

Published online by Cambridge University Press:  25 May 2016

Makoto Taiji ,
Junichiro Makino ,
Toshiyuki Fukushige ,
Toshikazu Ebisuzaki  and
Daiichiro Sugimoto
Makoto Taiji
Affiliation:
Department of Earth Science and Astronomy
Junichiro Makino
Affiliation:
†Department of Graphics and Information Science, College of Arts and Sciences, University of Tokyo, Komaba 3-8-1, Meguro, Tokyo 153, Japan, Internet : [email protected]
Toshiyuki Fukushige
Affiliation:
Department of Earth Science and Astronomy
Toshikazu Ebisuzaki
Affiliation:
Department of Earth Science and Astronomy
Daiichiro Sugimoto
Affiliation:
Department of Earth Science and Astronomy

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have developed a massively parallel special-purpose computer system for N-body simulations, GRAPE-4 (GRAvity-PipE 4). The GRAPE-4 system is designed for high-accuracy simulations of dense stellar systems. The GRAPE-4 calculates gravitational forces, their derivatives in time and potential energies. It has a hardware for prediction of positions and velocities, which is used for the individual timestep scheme. Using multi-chip module technology, we integrated 1692 chips of 640 megaflops performance. The peak speed of GRAPE-4 is 1.08 teraflops.

Type
Large N-body Simulation
Information
Symposium - International Astronomical Union , Volume 174: Dynamical Evolution of Stars Clusters , 1996 , pp. 141 - 150
Copyright
Copyright © Kluwer 1996 

References

The viewgraphs of the presentation are available at “http://butterfly.c.u-tokyo.ac.jp:8080/pub/people/taiji/grape4”.Google Scholar
Aarseth, S. J. 1995. In this volume. Google Scholar
Barnes, J., and Hut, P. (1986) Nature, 324, 446.Google Scholar
Brieu, P. P., Summers, F. J., and Ostriker, J. P. 1995. Astrophys. J., in press.Google Scholar
Ebisuzaki, T., Makino, J., Fukushige, T., Taiji, M., Sugimoto, D., Ito, T., and Okumura, S. K. (1993) Publ. Astron. Soc. Japan, 45, 269, and references therein.Google Scholar
Greengard, L., and Rokhlin, V. (1987) J. Comp. Phys., 73, 325–348.CrossRefGoogle Scholar
Hockney, R. W., and Eastwood, J. W. (1988) Computer Simulation Using Particles. Bristol: Adam Hilger.Google Scholar
Makino, J. (1991a) Astrophys. J., 369, 200.CrossRefGoogle Scholar
Makino, J. (1991b) Publ. Astron. Soc. Japan, 43, 621–638.Google Scholar
Makino, J., and Aarseth, S. J. (1992) Publ. Astron. Soc. Japan, 44, 141.Google Scholar
Makino, J., Kokubo, E., and Taiji, M. (1993) Publ. Astron. Soc. Japan, 45, 349.Google Scholar
McMillan, S. L. W., and Aarseth, S. J. (1993) Astrophys. J., 414, 200.Google Scholar
Sugimoto, D., Chikada, Y., Makino, J., Ito, T., Ebisuzaki, T., and Umemura, M. (1990) Nature, 345, 33.CrossRefGoogle Scholar
Taiji, M., Makino, J., Ebisuzaki, T., and Sugimoto, D. (1994a) Pages 280-287 of: Proceedings of the 8th International Parallel Processing Symposium. Los Alamitos: IEEE Computer Society Press.Google Scholar
Taiji, M., Makino, J., Kokubo, E., Ebisuzaki, T., and Sugimoto, D. (1994b) Pages 302-311 of: Proceedings of the 27th Hawaii International Conference on System Sciences. Los Alamitos: IEEE Computer Society Press.Google Scholar
Taiji, M., Makino, J., Ebisuzaki, T., and Sugimoto, D. 1996. Publ. Astron. Soc. Japan, to be submitted.Google Scholar