Left panel: debris mass fallback time t _fb for tidal disruption of 300M _⊙ (M ₃₀₀, red) and 30M _⊙ (M ₃₀, blue) Pop III stars with Z = 10⁻⁵ (Z ₋₅, solid lines) and Z = 10⁻⁹ (Z ₋₉, dashed lines) compared to a regular 1M _⊙ star (black solid line). Right panel: Eddington ratio of the peak debris mass fallback rate ﹩{\dot{M}}_{\mathrm{fb},\mathrm{peak}}﹩ for the same stars as in the left panel. Pop III stars have shorter fallback times and much higher peak mass fallback rates compared to Pop I star TDEs.