Electromagnetic Excitation of Rotating Black Holes and Relativistic Jets

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dc.creatorBurinskii, A.
dc.creatorElizalde, E.
dc.creatorHildebrandt, S. R.
dc.creatorMagli, G.
dc.date2006-10-02
dc.date.accessioned2026-07-07T07:26:49Z
dc.date.available2026-07-07T07:26:49Z
dc.descriptionWe show that electromagnetic excitations of rotating black holes can lead to the appearance of narrow singular beams which break up the black hole horizon forming a tube-like region which connects the interior and exterior. It is argued that this effect may be at the origin of jet formation.
dc.description4 pages, 2 figs. Talk at the Int. Conf. on Gravitation, Cosmology, Astrophysics and Nonstationary Gas Dynamics, dedicated to Prof. K.P. Staniukovich's 90th birthday, Moscow, 2-6 March 2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0610036
dc.identifierhttp://arxiv.org/abs/astro-ph/0610036
dc.identifierGrav.Cosmol. 12 (2006) 115
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/117165
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleElectromagnetic Excitation of Rotating Black Holes and Relativistic Jets
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