Dissipation of Magnetic Flux in Primordial Gas Clouds
Dissipation of Magnetic Flux in Primordial Gas Clouds
We report the strength of seed magnetic flux of accretion disk surrounding the PopIII stars. The magnetic field in accretion disk might play an important role in the transport of angular momentum because of the turbulence induced by Magneto-Rotational Instability (MRI). On the other hand, since the primordial star-forming clouds …