dc.contributor.author |
Sharp, P.W. |
en |
dc.date.accessioned |
2009-08-28T03:23:22Z |
en |
dc.date.available |
2009-08-28T03:23:22Z |
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dc.date.issued |
2001-07 |
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dc.identifier.citation |
Department of Mathematics - Research Reports-468 (2001) |
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dc.identifier.issn |
1173-0889 |
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dc.identifier.uri |
http://hdl.handle.net/2292/5160 |
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dc.description.abstract |
N-body simulations of the Solar System are a rich source of initial value problems for ordinary differential equations. The problems range from the simulation of two bodies requiring a few milliseconds of CPU time to large simulations of a hundred thousand bodies or more requiring CPU time counted in months. We describe five N-body models and use them with long intervals of integration to compare the integrators DIVA, STEP, RKNINT and RKSUITE. |
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dc.publisher |
Department of Mathematics, The University of Auckland, New Zealand |
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dc.relation.ispartofseries |
Research Reports - Department of Mathematics |
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dc.rights.uri |
https://researchspace.auckland.ac.nz/docs/uoa-docs/rights.htm |
en |
dc.source.uri |
http://www.math.auckland.ac.nz/Research/Reports/view.php?id=468 |
en |
dc.title |
Long initial value test problems from simulations of the Solar System |
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dc.type |
Technical Report |
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dc.subject.marsden |
Fields of Research::230000 Mathematical Sciences::230100 Mathematics |
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dc.rights.holder |
The author(s) |
en |