For a kappa-deformed, RG-improved Schwarzschild black hole, the peak energy flux and disk temperature increase relative to classical Schwarzschild, while the ISCO radius shrinks from 6M to about 5.24M.
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Effect of Noncommutative Geometry on Accretion Disks around RGI-Schwarzschild Black Hole
For a kappa-deformed, RG-improved Schwarzschild black hole, the peak energy flux and disk temperature increase relative to classical Schwarzschild, while the ISCO radius shrinks from 6M to about 5.24M.