Title: 　Stellar tidal disruption and the discovery of supermassive black hole binaries

     in normal galaxies　　 

　　Speaker:  Fukun Liu (Peking University)　　 

    Time: Thursday, 3:00pm, September 11th　　

　　Location: Lecture Hall, 3rd floor　　 

　　Abstract: AGNs and all massive galaxies are believed to contain supermassive black holes at centre. Because galaxies grow through mergers, the central black holes must come together to form supermassive binaries (SMBHBs) after two galaxies merge. Measurements of SMBHBs can provide us with a statistical measure of how many galaxies are the results of a merger, and thus help to understand the evolution of the universe. In addition, SMBHBs are destined to merge in a burst of strong gravitational wave radiations: those that still elude detection and for which scientists are building more and more sensitive telescopes. A couple of SMBHBs have been directly detected in AGNs. Until recently, however, clear evidence of an example of a close SMB has been lacking. In particular, most binaries may form at gas-poor galactic nuclei but are extremely challenging to find them because they are truly dark. In this colloquium, I will talk about our long-lasting theoretical investigations about how to discover and measure SMBHBs with stellar tidal disruptions and show the discovery of the first pair of SMBHB in normal galaxies. At the end of my talk, I will discuss how many similar systems we expect to detect in the near future.