Using Computation to Understand Why Black Holes Shine
Recently the Event Horizon Telescope (EHT) collaboration reported observing the shadow of a supermassive black hole at the center of a nearby galaxy called M87. But black holes are supposed to be so compact that light cannot escape from them. So how was it possible to observe radio waves coming from the vicinity of the black hole in M87? The answer lies in the dynamics of matter that is accreting into the black hole.


