Population III star formation in the presence of turbulence, magnetic
fields and ionizing radiation feedback
Population III star formation in the presence of turbulence, magnetic
fields and ionizing radiation feedback
Turbulence, magnetic fields and radiation feedback are key components that shape the formation of stars, especially in the metal-free environments at high redshifts where Population III stars form. Yet no 3D numerical simulations exist that simultaneously take all of these into account. We present the first suite of radiation-magnetohydrodynamics (RMHD) …