Black Hole Mergers in Nuclear Star Clusters
How frequent are black hole mergers in the centers of galaxies?
How frequent are black hole mergers in the centers of galaxies?
During the search for an elusive electromagnetic counterpart to the newest gravitational wave in town, GW170104, a very special supernova was uncovered. Here we discuss its classification and whether it is linked to the origin of GW170104 .
Today’s paper talks about the not-yet-observed electromagnetic counterparts to gravitational waves
Echoes after the initial gravitational wave signal are the “smoking gun” signature of exotic compact objects (ECOs).
Detecting electromagnetic and gravitational signals from a single astrophysical event will be revolutionary, but how do we find the former when we don’t know exactly where the latter is?
If a low-frequency gravitational wave detector, like LISA, existed 5 years ago, we would have been able to predict that LIGO would detect a binary merger on September 14, 2015 at 09:50:45 plus or minus a few seconds.