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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Published in | The Astrophysical journal Vol. 976; no. 1; pp. 85 - 98 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
Philadelphia
The American Astronomical Society
01.11.2024
IOP Publishing |
Subjects | |
Online Access | Get full text |
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