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- W2618320830 abstract "We implement the koral code to perform two sets of very long general relativistic radiation magnetohydrodynamic simulations of an axisymmetric optically thin magnetized flow around a non-rotating black hole: one with a new term in the electromagnetic field tensor due to the radiation pressure felt by the plasma electrons on the comoving frame of the electron–proton plasma, and one without. The source of the radiation is the accretion flow itself. Without the new term, the system evolves to a standard accretion flow due to the development of the magneto-rotational instability. With the new term, however, the system eventually evolves to a magnetically arrested disc state in which a large-scale jet-like magnetic field threads the black hole horizon. Our results confirm the secular action of the Cosmic Battery in accretion flows around astrophysical black holes." @default.
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- W2618320830 date "2017-09-04" @default.
- W2618320830 modified "2023-10-17" @default.
- W2618320830 title "Numerical simulations of the Cosmic Battery in accretion flows around astrophysical black holes" @default.
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- W2618320830 doi "https://doi.org/10.1093/mnras/stx2249" @default.
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