The new simulations showed that the rotating disks around collapsars can also emit gravitational waves that amplify together, very much like the orbiting compact objects in mergers.
"I thought that the signal would be much messier because the disk is a continuous distribution of gas with material spinning in different orbits," Gottlieb says. "We found that the gravitational waves from these disks are emitted coherently, and they're also rather strong."
Not only is the predicted signal from collapsar disks strong enough to be detected by LIGO, but Gottlieb's calculations suggest that a few events might already be in existing datasets. Proposed
gravitational wave detectors such as the
Cosmic Explorer and
Einstein Telescope could spot dozens a year.