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Direct N-body simulation on supercomputers

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The Use of Supercomputers in Stellar Dynamics

Part of the book series: Lecture Notes in Physics ((LNP,volume 267))

Abstract

We have analyzed the effect of vectorization on several schemes of direct N-body integration. We find that an Aarseth-type code with a neighbour scheme, which is the fastest on a scalar processor, is still the fastest on vector processors for large N. For N=1000, the overall gain in speed is found to be a factor of 10 both in theory and experiment. In the presence of hard binaries, however, the gain is reduced significantly.

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References

  • Aarseth, S. J. (1985), in Multiple Time Scales, eds J. U. Brackbill and B. I. Cohen (Academic Press, New York), p 377.

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  • Aarseth, S. J. (1963), Mon. Not. Roy. Astron. Soc., 126, 223.

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  • Ahmad, A. and Cohen, L. (1973), J. Comp. Phys., 12, 389.

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  • Makino, J. and Hut, P. (1986), in preparation.

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Piet Hut Stephen L. W. McMillan

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© 1986 Springer-Verlag

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Makino, J. (1986). Direct N-body simulation on supercomputers. In: Hut, P., McMillan, S.L.W. (eds) The Use of Supercomputers in Stellar Dynamics. Lecture Notes in Physics, vol 267. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0116405

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  • DOI: https://doi.org/10.1007/BFb0116405

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-17196-6

  • Online ISBN: 978-3-540-47361-9

  • eBook Packages: Springer Book Archive

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