Abstract
We present a review of the influence of cosmic repulsion and external magnetic fields on accretion disks rotating around rotating black holes and on jets associated with these rotating configurations. We consider both geometrically thin and thick disks. We show that the vacuum energy represented by the relic cosmological constant strongly limits extension of the accretion disks that is for supermassive black holes comparable to extension of largest galaxies, and supports collimation of jets at large distances from the black hole. We further demonstrate that an external magnetic field crucially influences the fate of ionized Keplerian disks causing creation of winds and jets, enabling simultaneously acceleration of ultra-high energy particles with energy up to 10 21 eV around supermassive black holes with M ∼ 10 10 M ⊙ surrounded by sufficiently strong magnetic field with B ∼ 10 4 G. We also show that the external magnetic fields enable existence of “levitating” off-equatorial clouds or tori, along with the standard equatorial toroidal structures, if these carry a non-vanishing, appropriately distributed electric charge.
Subject
General Physics and Astronomy
Reference154 articles.
1. Launching of Active Galactic Nuclei Jets;Tchekhovskoy,2015
2. The Lense-Thirring Effect and Accretion Disks around Kerr Black Holes
3. Foundations of Black Hole Accretion Disk Theory
4. Astrophysics of black holes;Novikov,1973
5. The analytic theory of fluid disks orbiting the Kerr black hole;Kozlowski;Astron. Astrophys.,1978
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