No CrossRef data available.
Article contents
The First Ten Years of GRAPE
Published online by Cambridge University Press: 26 May 2016
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.
GRAPE is a project for a special-purpose computer dedicated to classical many-body problems. Its primary use is for gravitational many-body problem of stellar systems. It was initiated in 1989, and now its performance is in the range of 100 Tera-flops equivalent. As an introduction to this symposium, development of the GRAPE project is reviewed, where motivation to it is the main concern of this paper rather than the computer itself.
- Type
- Introduction
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2003
References
Aarseth, S. J.
1985, in Multiple Time Scales, ed. Brackhill, J. U. & Cohen, B. I. (New York: Academic Press), 377
Google Scholar
Ebisuzaki, T., Makino, J., Fukushige, T., Taiji, M., Sugimoto, D., Ito, T., & Okumura, S.-K.
1993, PASJ, 45, 269
Google Scholar
Hachisu, I., Nakada, Y., Nomoto, K. & Sugimoto, D.
1978, Progr. Theoret. Phys. (Kyoto), 1978, 393
CrossRefGoogle Scholar
Sugimoto, D.
1986, in IAU Symp. 113, Dynamics of Star Clusters, eds. Goodman, J. and Hut, P. (Dordrecht: Reidel), 207
Google Scholar
Sugimoto, D., Eriguchi, Y., & Hachisu, I.
1981, Progr. Theoret. Phys. (Kyoto), Suppl.
70, 154
Google Scholar
Sugimoto, D., Chikada, Y., Makino, J., Ito, T., Ebisuzaki, T., & Umemura, M.
1990, Nature, 345, 33
Google Scholar