Radiative (solid lines) and kinetic (dashed lines) efficiency defined as in Equation (11). The blue lines are A122Edd1_LR, and the red lines are A122Edd1. The efficiencies may slightly exceed 1.0 because of the conversion between kinetic energy and gravitational potential. The low-resolution run A122Edd1_LR produces more radiation luminosity than A122Edd1 and less kinetic energy.