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, th...
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| Principais autores: | , |
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| 格式: | Artigo |
| 語言: | Inglês |
| 出版: |
IOP Publishing
2024-01-01
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| 叢編: | The Astrophysical Journal |
| 主題: | |
| 在線閱讀: | https://doi.org/10.3847/1538-4357/ad7fec |
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