This artist’s concept shows a supermassive black hole surrounded by a disk of gas. Embedded in this disk are two smaller black holes that may have merged together to form a new black hole. Credit: Caltech/R. Hurt (IPAC)
In a first, astronomers may have seen light from the merger of two black holes, providing opportunities to learn about these mysterious dark objects.
This artist’s concept shows a supermassive black hole surrounded by a disk of gas. Embedded in this disk are two smaller black holes that may have merged together to form a new black hole.
When two black holes spiral around each other and ultimately collide, they send out gravitational waves — ripples in space and time that can be detected with extremely sensitive instruments on Earth. Since black holes and black hole mergers are completely dark, these events are invisible to telescopes and other light-detecting instruments used by astronomers. However, theorists have come up with ideas about how a black hole merger could produce a light signal by causing nearby material to radiate.
Now, scientists using Caltech’s Zwicky Transient Facility (ZTF) located at Palomar Observatory near San Diego may have spotted what could be just such a scenario. If confirmed, it would be the first known light flare from a pair of colliding black holes.
The merger was identified on May 21, 2019, by two gravitational wave detectors – the National Science Foundation’s Laser Interferometer Gravitational-wave Observatory, or LIGO, and the European Virgo detector – in an event called GW190521g. That detection allowed the ZTF scientists to look for light signals from the location where the gravitational wave signal originated. These gravitational wave detectors have also spotted mergers between dense cosmic objects called neutron stars, and astronomers have identified light emissions from those collisions.
i found the arxiv preprint, but the model isn’t of a merger producing light but of it kicking the merged black hole through the galaxy supermassive black hole accretion disk to produce a light flare.
“Nearby gas is accelerated around the BH, producing a shocked Bondi tail [e.g., 57–59] which both acts as a drag on the BH and accretes onto it. We approximate the Bondi-Hoyle-Lyttleton (BHL) luminosity …” [ https://arxiv.org/pdf/2006.14122.pdf ].
They then predict a similar flare “when the kicked BBH re-encounters the disk on timescale … “.