Exponentially Amplified Magnetic Field Eliminates Disk Fragmentation around Population III Protostars
Exponentially Amplified Magnetic Field Eliminates Disk Fragmentation around Population III Protostars
One critical remaining issue to unclear the initial mass function of the first (Population III) stars is the final fate of secondary protostars formed in the accretion disk, specifically whether they merge or survive. We focus on the magnetic effects on the first star formation under the cosmological magnetic field. …