Spherical super-Eddington accretion onto a black hole has two analytic solution branches, an isothermal one and a power-law one, and neither branch is luminous enough to explain the observed failed supernova candidates.
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Super-Eddington accretion onto black holes and its application to fallback accretion
Spherical super-Eddington accretion onto a black hole has two analytic solution branches, an isothermal one and a power-law one, and neither branch is luminous enough to explain the observed failed supernova candidates.