Speaker
Alberto Sesana
(Albert Einstein Institute, Golm)
Description
Massive black hole binaries (MBHBs) are expected to be the loudest gravitational wave (GW) sources in the milli-Hz window which will be probed by the future Laser Interferometer Space Antenna. MBHs are also known to radiate at large luminosities, opening the possibility of future multimessenger observations of MBHBs. I will describe the dynamics of MBHBs, their expected GW and electromagnetic signals and prospects for multimessenger astronomy in the next decade.
Primary author
Alberto Sesana
(Albert Einstein Institute, Golm)
