Radiative Cooling Changes the Dynamics of Magnetically Arrested Disks
We study magnetically arrested disks (MADs) around rotating black holes (BHs) under the influence of radiative cooling. We introduce a critical value of the mass accretion rate ${\dot{M}}_{{\rm{crit}}}$ for which the cooling by the synchrotron process efficiently radiates the thermal energy of the d...
| 發表在: | The Astrophysical Journal Letters |
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| Main Authors: | , , |
| 格式: | Article |
| 語言: | 英语 |
| 出版: |
IOP Publishing
2025-01-01
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| 主題: | |
| 在線閱讀: | https://doi.org/10.3847/2041-8213/adb749 |