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Accretion onto black holes is an efficient mechanism in converting the gasmass-energy into energetic outputs as radiation, wind and jet. Tidal disruptionevents, in which stars are tidally torn apart and then accreted ontosupermassive black holes, offer unique opportunities of studying the accretionphysics as well as the wind and jet launching physics across differentaccretion regimes. In this review, we systematically describe and discuss themodels that have been developed to study the accretion flows and jets in tidaldisruption events. A good knowledge of these physics is not only needed forunderstanding the emissions of the observed events, but also crucial forprobing the general relativistic space-time around black holes and thedemographics of supermassive black holes via tidal disruption events.

The Physics of Accretion Discs, Winds And Jets in Tidal Disruption Events