Flares on the Black Holes

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dc.creatorGruzinov, Andrei
dc.date1999-08-10
dc.date.accessioned2026-07-07T02:32:47Z
dc.date.available2026-07-07T02:32:47Z
dc.descriptionA Kerr black hole can flare quasi-periodically, if it is magnetically connected to the accretion disk. The flares extract the rotational energy of the hole. The flaring occurs because the hole twists the magnetic field lines beyond the threshold of the screw instability.
dc.description8 pages, submitted to ApJ
dc.identifierhttps://arxiv.org/abs/astro-ph/9908101
dc.identifierhttp://arxiv.org/abs/astro-ph/9908101
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14585
dc.subjectAstrophysics
dc.titleFlares on the Black Holes
dc.typetext

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