Large-Scale Simulations of Clusters of Galaxies

2); (2) NASA/GSFC); A. C. Calder (1); B. Fryxell (1); D. Q. Lamb (1); F. X. Timmes (1); H. M. Tufo (1); J. W. Truran (1); K. Olson (1; L. J. Dursi (1)

arxiv: astro-ph/0011502 · v1 · submitted 2000-11-27 · 🌌 astro-ph

Large-Scale Simulations of Clusters of Galaxies

P. M. Ricker (1) , A. C. Calder (1) , L. J. Dursi (1) , B. Fryxell (1) , D. Q. Lamb (1) , P. MacNeice (2) , K. Olson (1 , 2)

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R. Rosner (1) F. X. Timmes (1) J. W. Truran (1) H. M. Tufo (1) M. Zingale (1) ((1) Univ. of Chicago (2) NASA/GSFC)

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keywords challengesclustersflashframeworkgalaxiesusedadaptiveaddress

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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.

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Large-Scale Simulations of Clusters of Galaxies

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