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HEP - ASTRO SEMINAR | Galaxy Clusters: Laboratories for Extreme Plasma Physics

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Monday, September 29, 2014
12:00 AM
335 West Hall

Galaxy clusters are the most massive virialized objects in the universe, and have the potential to be highly accurate probes of cosmological parameters. A fundamental challenge for cluster cosmology is to estimate the masses of these objects using observational proxies such as X-ray luminosity and temperature, which are complicated by the merger history of clusters and the microphysical properties of the intracluster medium.  These effects, while frustrating to cosmologists, provide a rich laboratory for exploring the plasma physical processes that are occurring in these massive objects.  In this talk I will present recent efforts to understand the effects that several plasma processes - including conduction, cosmic ray acceleration, and condensation - have on the observable properties of galaxy clusters.

 

Speaker:
Physics
Randall Lab and Homer A. Neal Lab
450 Church Street
Ann Arbor, MI 48109-1040
734.764.4437
734.763.9694
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