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In this talk, i will present some new advances in the theory of Tidal Disruption Events (TDE). TDEs occur when a star approaches a SMBH close enough to be torn apart by the black hole tidal field. The rapid accretion of the stellar debris produce a luminous, possibly super-Eddington flare, lighting up an otherwise quiescent black hole. In this talk, I will present some recent results concerning the formation and early evolution of an accretion disc formed by the stellar debris. The structure ofdoi:10.5281/zenodo.163790 fatcat:f2yzjpzed5cqfhn6wec3nosoye