Choked accretion onto a Kerr black hole

The choked accretion model consists of a purely hydrodynamical mechanism in which, by setting an equatorial to polar density contrast, spherically symmetric flow transitions inflow-outflow configuration. This scenario has been studied the case (non-rotating) Schwarzschild black hole as central accretor, well non-relativistic limit. In this article, we generalize these previous works studying perfect fluid onto (rotating) Kerr hole. We first describe using steady-state, irrotational analytic solution ultrarelativistic fluid, obeying stiff equation state. then use numerical simulations order explore more general Analyzing effects hole's rotation on flow, find particular that morphology prevails for all possible values spin parameter, showing robustness model.