Jan Eldridge

Since the detection of the first gravitational wave transient in 2015 there has been a small revolution in our understanding of the mass distribution of black holes. But there are still many unknowns and theory is still struggling to understand how the observed distribution is determined. There are also other windows onto black holes that are showing that the GW transient masses are only have the story. I’ll present the main samples of black holes that are available to us today and in the not-too-distant future. Then describe how theoretical work will allow us to understand what physics is in play in determining the birth and evolution of black holes, their ecology within galaxies and the Universe.