Prefer a chat interface with context about you and your work?
Magnetohydrodynamics of Population III Star Formation
The evolution of collapsing primordial clouds and the formation of Population III (Pop III) protostars are investigated with threeādimensional ideal MHD simulations. We follow the collapse of parsecāsized primordial clouds down to the formation of protostars on subāAU scales. Pop III protostar formation is characterized by the ratio of rotational ā¦