Evolution of massive Population III stars with rotation and magnetic fields

Aims. We present a new grid of massive Population III (Pop III) star models including the effects of rotation on the stellar structure and chemical mixing, and magnetic torques for the transport of angular momentum. This grid covers the range of mass from 10 to 1000 M⊙, and rotational velocity from zero to 100% of the critical rotation on the zero-age main sequence. Based on the grid, we also present a phase diagram for the expected final fates (i.e., core-collapse supernova, gamma-ray bursts (GRBs) and pair-instability supernovae of diverse types) of rotating massive Pop III stars.