Large-Scale Simulations of Clusters of Galaxies
Astrophysics
2009-10-31 v1
Abstract
We discuss some of the computational challenges encountered in simulating the evolution of clusters of galaxies. Eulerian adaptive mesh refinement (AMR) techniques can successfully address these challenges but are currently being used by only a few groups. We describe our publicly available AMR code, FLASH, which uses an object-oriented framework to manage its AMR library, physics modules, and automated verification. We outline the development of the FLASH framework to include collisionless particles, permitting it to be used for cluster simulation.
Keywords
Cite
@article{arxiv.astro-ph/0011502,
title = {Large-Scale Simulations of Clusters of Galaxies},
author = {P. M. Ricker and A. C. Calder and L. J. Dursi and B. Fryxell and D. Q. Lamb and P. MacNeice and K. Olson and R. Rosner and F. X. Timmes and J. W. Truran and H. M. Tufo and M. Zingale},
journal= {arXiv preprint arXiv:astro-ph/0011502},
year = {2009}
}
Comments
3 pages, 3 figures, to appear in Proceedings of the VII International Workshop on Advanced Computing and Analysis Techniques in Physics Research (ACAT 2000), Fermilab, Oct. 16-20, 2000