| Astrophysical N-body simulations on GRAPE-4 special-purpose computer |
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Conference on High Performance Networking and Computing
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Proceedings of the 1995 ACM/IEEE conference on Supercomputing (CDROM)
table of contents
San Diego, California, United States
Article No. 63
Year of Publication: 1995
ISBN:0-89791-816-9
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Authors
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Junichiro Makino
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Department of Information Science and Graphics, Department of Earth Science and Astronomy, College of Arts and Sciences, University of Tokyo, Tokyo 153, Japan
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Makoto Taiji
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Department of Information Science and Graphics, Department of Earth Science and Astronomy, College of Arts and Sciences, University of Tokyo, Tokyo 153, Japan
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Downloads (6 Weeks): 6, Downloads (12 Months): 14, Citation Count: 3
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ABSTRACT
We report on resent astrophysical N-body simulations performed on the GRAPE-4 (GRAvity PipE 4) system, a special-purpose computer for astrophysical N-body simulations. We first review the astrophysical motivation, the algorithm, the structure of the GRAPE system, and the actual performance. The GRAPE-4 system consists of 1692 pipeline processors. The peak speed of one pipeline processor is 523 Mflops and that of the total system is 884 Gflops. The performance obtained is 529 Gflops for the simulation of two massive black holes in the core of a galaxy with 700,000 stars.
REFERENCES
Note: OCR errors may be found in this Reference List extracted from the full text article. ACM has opted to expose the complete List rather than only correct and linked references.
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CITED BY 3
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Tetsu Narumi , Ryutaro Susukita , Takahiro Koishi , Kenji Yasuoka , Hideaki Furusawa , Atsushi Kawai , Toshikazu Ebisuzaki, 1.34 Tflops molecular dynamics simulation for NaCl with a special-purpose computer: MDM, Proceedings of the 2000 ACM/IEEE conference on Supercomputing (CDROM), p.54-es, November 04-10, 2000, Dallas, Texas, United States
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