Dynamical evolution of rotating stellar systems: Fokker Planck and N-body

Details Dynamical evolution of rotating stellar systems: Fokker Planck and N-body Dynamical evolution of rotating stellar systems: Fokker Planck and N-body

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007cophc.177..260l&link_type=abstract

Computer Physics Communications, Volume 177, Issue 1-2, p. 260-261.

Physics

Scientific paper

We have carried out comparative study between direct N-body technique and Fokker Planck approach for the dynamical evolution of rotating stellar systems. Because of limitations of computing resources, we have restricted to relatively small N (˜10,000) systems compared to realistic star clusters. We found that these two different approaches generally give very similar results. Some minor differences are found to exist, but they can be understood because Fokker Planck approach has to make some simplifying assumptions.

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