Thick Accretion Disk and Its Super Eddington Luminosity around a Spinning Black Hole

In the general accretion disk model theory, surrounding an astronomical object comprises fluid rings obeying Keplerian motion. However, we should consider relativistic and rotational effects as close in toward center of spinning compact massive objects such a black hole or neutron star. this study, explore geometry inner portion context Mukhopadhyay’s pseudo-Newtonian potential approximation for full relativity theory. We found that shape “puffs up” becomes thicker luminosity could exceed Eddington near surface hole.