Title:
(Provisional) General relativistic simulations of tidal disruption events

Abstract:
(Provisional) I will discuss some recent results of 
our full General Relativistic Smoothed Particle Hydrodynamics simulations of 
tidal disruption events around Schwarzschild and Kerr black holes. 
We simulate disruption of stars on both eccentric and parabolic orbits with 
different penetration factors. We are able to follow the disruption and 
the fallback phase, and to simulate self-consistently the formation and 
inflation of an expanding Eddington bubble. We compute the photosphere of 
the bubble and its lightcurve, resulting in optical-UV luminosity 
remarkably close to observations.