Many late-time TDE plateaus can be reproduced by initially wide disks formed with redistributed angular momentum, while the same model with super-Eddington outflows explains AT2018cow's late emission with a 10-100 solar-mass black hole.
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Viscously Spreading Accretion Disks around Black Holes: Implications for TDEs, LFBOTs and other Transients
Many late-time TDE plateaus can be reproduced by initially wide disks formed with redistributed angular momentum, while the same model with super-Eddington outflows explains AT2018cow's late emission with a 10-100 solar-mass black hole.