Detecting coalescences of intermediate-mass black holes in globular clusters with the Einstein Telescope
arXiv:0912.4925 · doi:10.1142/9789814374552_0300
Abstract
We discuss the capability of a third-generation ground-based detector such as the Einstein Telescope to detect mergers of intermediate-mass black holes that may have formed through runaway stellar collisions in globular clusters. We find that detection rates of 500 events per year are plausible.