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A Multi-Particle Regularisation Technique*

Published online by Cambridge University Press:  12 April 2016

D. C. Heggie
D. C. Heggie*
Affiliation:
Institute of Theoretical Astronomy, Cambridge

Abstract

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Certain features of a practical regularisation method, in which the potential or kinetic energy is used as a time-regularising function, are described. For two-body encounters the method is less powerful than Kustaanheimo-Stiefel regularisation, but it has wider applicability.

Information

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 10: Gravitational N-Body Problem , November 1971, pp. 35 - 39
Copyright
Copyright © Reidel 1971

Footnotes

*

This work was carried out during tenure by the author of a Studentship from the U.K. Science Research Council.

References

Aarseth, S. J.: 1968, Bull. Astron. 3, 124.Google Scholar
Aarseth, S. J.: 1970, Astron. Astrophys. 9, 64.Google Scholar
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Peters, C. F.: 1968, Bull. Astron. 3, 167.Google Scholar