Simulating Galaxy Clusters
Michael L. Norman
TL;DR
This review discusses methods and recent advances in simulating galaxy clusters, covering theoretical models, numerical techniques, and observational comparisons to understand cluster formation and properties.
Contribution
It provides a comprehensive overview of galaxy cluster simulation techniques, recent physics incorporations, and their implications for astrophysical research.
Findings
Validation through Santa Barbara cluster comparison project
Advances in modeling turbulence and AGN feedback
Progress in simulating statistical cluster samples
Abstract
This pedagogical review of galaxy cluster simulations is based on three lectures given at the 2008 Enrico Fermi Summer School entitled "Astrophysics of Galaxy Clusters". It covers the standard cosmological framework, growth of perturbations in the linear regime, analytic models for nonlinear perturbation growth, statistics of galaxy cluster populations, virial scaling relations, overview of numerical methods, simulating gas in galaxy clusters, basic results on adiabatic clusters (Santa Barbara cluster comparison project), effect of additional physics, recent progress in galaxy clustering modeling (Galcons, turbulence, AGN jets, cluster-wide B-fields), simulating statistical samples and lightcones, and simulated SZE surveys.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Gamma-ray bursts and supernovae