Title:
Modeling accretion disks, winds and jets in tidal disruption events

Abstract:
Tidal disruption events happen in the centers of galaxies, 
where stars that pass too close by are destroyed by 
the tidal force from the central supermassive black holes. 
A large amount of stellar material is fed to the black hole in 
only a few years, forming a transient accretion disk, winds and 
sometimes even a relativistic jet. When the stellar material is 
accreted onto the black hole at a rate exceeding 
the Eddington accretion rate, a super-Eddington disk forms, 
which can launch strong winds and jets. As the accretion rate drops, 
the disk morphology, wind and jet power can all change accordingly. 
I will talk about our most recent modeling about the disks, winds and 
jets in tidal disruption events .