Speaker
SHURUI ZHANG
(ICRANet)
Description
Compact objects or stars in nuclear clusters can interact with AGN disks during their motion, exchanging energy and angular momentum, and eventually settling into disk-plane motion. Additionally, the outer regions of AGN disks may undergo gravitational collapse, forming stars that evolve into compact objects and migrate inward. By studying the accretion and dynamics of various compact objects (white dwarfs, neutron stars, and black holes) in AGN disks, their respective fates and the resulting multi-wavelength and multi-messenger signals are investigated.
Author
SHURUI ZHANG
(ICRANet)