Monte Carlo Simulations of Globular Cluster Dynamics
Astrophysics
2007-05-23 v1
Abstract
We have developed a new parallel supercomputer code based on Henon's Monte Carlo method for simulating the dynamical evolution of globular clusters. This new code allows us to calculate the evolution of a cluster containing a realistic number of stars (N ~ 10^5 - 10^6) in about a day of computing time. The discrete, star-by-star representation of the cluster in the simulation allows us to treat naturally a number of important processes, including single and binary star evolution, all dynamical interactions of single stars and primordial binaries, and tidal interactions with the Galaxy.
Cite
@article{arxiv.astro-ph/0006205,
title = {Monte Carlo Simulations of Globular Cluster Dynamics},
author = {F. A. Rasio},
journal= {arXiv preprint arXiv:astro-ph/0006205},
year = {2007}
}
Comments
7 pages, with 2 postscript figures, to appear in Dynamics of Star Clusters and the Milky Way, eds. R. Spurzem et al. (ASP Conference Series)