Properties of the accretions for m _NS = 1.4M _⊙, r _NS = 10 km NSs with different magnetic fields and indices s. Each panel synchronously shows relative magnitude between the inner truncation radius r _m and the otherwise inner disk boundary r _in = 10r _g , i.e., r _m/10r _g , by contour lines, and comparison between the energy released via the accreted mass hitting the NS surface L _acc and the energy released from the circum-NS disk L _w. L _acc is always larger than L _w, indicating that the NS-accretion liberated energy dominates the energy injection into the outflow.