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Astrophysical N-body simulations on GRAPE-4 special-purpose computer
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Source Conference on High Performance Networking and Computing archive
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
Authors
Junichiro Makino  Department of Information Science and Graphics, Department of Earth Science and Astronomy, College of Arts and Sciences, University of Tokyo, Tokyo 153, Japan
Makoto Taiji  Department of Information Science and Graphics, Department of Earth Science and Astronomy, College of Arts and Sciences, University of Tokyo, Tokyo 153, Japan
Sponsors
IEEE-CS : Computer Society
SIGARCH: ACM Special Interest Group on Computer Architecture
Publisher
ACM  New York, NY, USA
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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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Collaborative Colleagues:
Junichiro Makino: colleagues
Makoto Taiji: colleagues