Chaotic magnetic disconnections trigger flux eruptions in accretion flows channeled onto magnetically saturated Kerr black holes

Context. Magnetized accretion flow onto a black hole (BH) may lead to the accumulation of poloidal magnetic flux across its horizon, which for high BH spin can power far-reaching relativistic jets. The BH magnetic flux is subject to a saturation mechanism by means of magnetic flux eruptions involvin...

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Bibliographic Details
Published inAstronomy and astrophysics (Berlin) Vol. 692; p. A37
Main Authors Nalewajko, Krzysztof, Kapusta, Mateusz, Janiuk, Agnieszka
Format Journal Article
LanguageEnglish
Published 01.12.2024
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