Ultra high energy cosmic ray generation in black hole magnetosphere: testing by polarimetric observations

作者: M. Y. Piotrovich , Y. N. Gnedin , S. D. Buliga , T. M. Natsvlishvili

DOI: 10.1007/S10509-014-2043-3

关键词: Supermassive black holeCosmic rayIntermediate-mass black holeSpin-flipActive galactic nucleusAstrophysicsAccretion (astrophysics)PhysicsMagnetosphereUltra-high-energy cosmic rayAstronomy

摘要: We develop the method that allows to estimate ultra high energy cosmic ray (UHECR) production in active galactic nuclei (AGNs). used model developed by Neronov et al. (New J. Phys. 11:065015, 2009) and estimated magnetic field strength near innermost stable orbit an accretion disk at horizon radius of a supermassive black hole (SMBH) using data polarimetric observations broad lines emission. It kinetic power relativistic jet base Blandford–Znajek mechanism. In result we for number AGNs with known values SMBH spins.

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