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DTSTART;TZID=America/Chicago:20260130T153000
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CREATED:20250919T154927Z
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UID:10435356-1769787000-1769792400@uwm.edu
SUMMARY:Physics Colloquium - Chris Fragile
DESCRIPTION:What Are We Learning About Super-Eddington Accretion Disks From Simulations?\nProfessor Chris Fragile\nDepartment of Physics & Astronomy\, College of Charleston \nAccretion of gas onto black holes is one of the most important processes shaping our Universe. Understanding extremely high rates of accretion (dubbed ‘super-Eddington’) is vital to explaining the challenging observation that supermassive black holes (SMBHs) are fully formed at redshifts >7. It is also important to understanding astrophysical objects such as tidal disruption events (TDEs) and ultra-luminous X-ray sources (ULXs). \nIn this talk\, I will present the results of some recent super-Eddington disk simulations and discuss some of the interesting things we are learning.
URL:https://uwm.edu/physics/event/physics-colloquium-chris-fragile/
LOCATION:Chemistry 108\, 2050 E Kenwood Blvd\, Milwaukee\, WI\, 53201\, United States
CATEGORIES:Physics Colloquia
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