Amplification and Saturation of Turbulent Magnetic Fields in Collapsing Primordial Gas Clouds

Amplification and Saturation of Turbulent Magnetic Fields in Collapsing Primordial Gas Clouds

Recent numerical studies suggest that magnetic fields play an important role in primordial star formation in the early Universe. However, the detailed evolution of the magnetic field in the collapse phase still has uncertainties because of the complicated physics associated with turbulence in a coll...

Full description

Bibliographic Details
Main Authors: Sho Higashi, Hajime Susa, Christoph Federrath, Gen Chiaki
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Early universe
Magnetohydrodynamical simulations
Collapsing clouds
Population III stars
Magnetic fields
Hydrodynamics
Online Access:https://doi.org/10.3847/1538-4357/ad2066

Internet

https://doi.org/10.3847/1538-4357/ad2066

Similar Items