Cosmological Simulations of AGN Feedback in Groups and Clusters

Details Cosmological Simulations of AGN Feedback in Groups and Clusters Cosmological Simulations of AGN Feedback in Groups and Clusters

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011scgg.conf...49s&link_type=abstract

"Structure in Clusters and Groups of Galaxies in the Chandra Era, 2011 Chandra Science Workshop held July 12-14, 2011. Edited by

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I will review numerical techniques employed to simulate black hole formation, accretion and feedback processes in cosmological simulations of structure formation. In particular, I will discuss how black holes co-evolve with forming groups and clusters of galaxies from high redshifts to the present epoch, and how AGN feedback modifies gaseous and stellar properties in the central regions of these systems. I will also elaborate on various shortcomings of the widely used cosmological codes illustrating how they affect simulated properties of galaxy clusters and to which extent this reflects on our understanding of feedback processes in cluster cores.

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