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...
Saved in:
| Main Authors: | Akshay Singh, Damien Bégué, Asaf Pe’er |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astrophysical Journal Letters |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/2041-8213/adb749 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Global Resistive Magnetohydrodynamic Accretion Flows around Spinning Active Galactic Nuclei: Impact of Resistivity on the Magnetically Arrested Disk State
by: Ramiz Aktar, et al.
Published: (2025-01-01) -
Radiation Magnetohydrodynamic Simulation of Sub-Eddington Circumbinary Disk around an Equal-mass Massive Black Hole Binary
by: Vishal Tiwari, et al.
Published: (2025-01-01) -
Distinguishability of a Naked Singularity from a Black Hole in Dynamics and Radiative Signatures
by: Indu K. Dihingia, et al.
Published: (2024-01-01) -
Emergence of cHz Quasiperiodic Oscillations from a Low-angular-momentum Flow onto a Supermassive Black Hole
by: Indu K. Dihingia, et al.
Published: (2025-01-01) -
Magnetic Flux Transport in Advection-dominated Accretion Flow toward the Formation of a Magnetically Arrested Disk
by: Jia-Wen Li, et al.
Published: (2024-01-01)