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Direct collisional simulation of 10 000 particles past core collapse | | Rainer Spurzem
; Sverre J. Aarseth
; | | Date: |
1 May 1996 | | Subject: | astro-ph | | Affiliation: | Institut fuer Astronomie und Astrophysik, Univ. Kiel, Germany), Sverre J. Aarseth (Institute of Astronomy, Cambridge, UK | | Abstract: | A collisional $N$-body simulation using NBODY5 on a single CRAY YMP processor is followed well into the post-collapse regime. This is presently one of the largest particle numbers of all such models published, but some data for an even larger $N$ produced by using special-purpose computers have recently been presented. In contrast to previous ensemble-averaged $N$-body simulations the noise here is low enough to just compare this one single run with the expectations from statistical models based on the Fokker-Planck approximation. Agreement is as good as could be expected for the case of the evolution of the Lagrangian radii, radial and tangential velocity dispersions and various core quantities. We briefly discuss approximate models to understand number and energy of escapers and the question of gravothermal core oscillations; although the system exhibits post-collapse oscillations they turn out to be directly binary driven and we cannot prove the existence of a gravothermal expansion at this particle number. Finally in a detailed examination of the wandering of the density centre we find in contrast to some previous studies a clear long-time period of the order of about 14 half-mass crossing times. | | Source: | arXiv, astro-ph/9605003 | | Services: | Forum | Review | PDF | Favorites | |
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