Direct Collapse Accretion Disks within Dark Matter Halos: Saturation of the Magnetorotational Instability and the Field Expulsion

We have used high-resolution zoom-in simulations of direct collapse to supermassive black hole (SMBH) seeds within dark mater halos in the presence of magnetic fields generated during the collapse, down to 10 −5 pc or 2 au. We confirm an efficient amplification of magnetic field during collapse, the...

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Bibliographic Details
Published inThe Astrophysical journal Vol. 976; no. 1; pp. 85 - 98
Main Authors Luo, Yang, Shlosman, Isaac
Format Journal Article
LanguageEnglish
Published Philadelphia The American Astronomical Society 01.11.2024
IOP Publishing
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