Statistics of Small-N Simulations

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dc.creatorHeggie, Douglas C.
dc.date1995-11-27
dc.date.accessioned2026-07-07T02:20:29Z
dc.date.available2026-07-07T02:20:29Z
dc.descriptionWe first review the reasons for carrying out statistical analysis of results from large numbers of N-body simulations, including a summary of previous work. Then we describe some results about the behaviour of N-body systems which have been acquired by this technique. Finally we concentrate on the problems associated with the scaling of N-body data with N, with particular regard to the dissolution of systems in a tidal field when mass is lost by stellar evolution.
dc.description10 pages uuencoded compressed postscript; to appear in P. Hut and J. Makino, eds, Dynamical Evolution of Star Clusters - Confrontation of Theory and Observations, Proc. IAU Symposium 174
dc.identifierhttps://arxiv.org/abs/astro-ph/9511124
dc.identifierhttp://arxiv.org/abs/astro-ph/9511124
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10224
dc.subjectAstrophysics
dc.titleStatistics of Small-N Simulations
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