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Dynamical Simulations: Methods and Comparisons

D. C. Heggie·M. Giersz·R. Spurzem·K. Takahashi
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Abstract

We review recent progress in computational methods for studying the dynamical evolution of large star clusters. After describing some highlights of a new comparison of different models, including N-body models, we mention in detail recent developments in three codes which allow models with anisotropic distributions of velocity to be studied: (i) a Fokker-Planck code using finite differences, (ii) a Monte Carlo code and (iii) a gaseous model code.

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D. C. Heggie, M. Giersz, R. Spurzem, K. Takahashi. 1997-11-17. Dynamical Simulations: Methods and Comparisons. https://arxiv.org/abs/astro-ph/9711191

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