Accretion into Black Hole, and Formation of Magnetically Arrested Accretion Disks
The exact time-dependent solution is obtained for a magnetic field growth during a spherically symmetric accretion into a black hole (BH) with a Schwarzschild metric. Magnetic field is increasing with time, changing from the initially uniform into a quasi-radial field. Equipartition between magnetic...
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| Format: | Article |
| Language: | English |
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MDPI AG
2019-06-01
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| Series: | Universe |
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| Online Access: | https://www.mdpi.com/2218-1997/5/6/146 |