摘要We discuss two kinds of magnetic connection (MC) in the black hole (BH) accretion disc: the magnetic connection between the BH and the disc (MCHD) and that between the plunging region and the disc (MCPD). The magnetic field configuration is produced by an electric current flowing at the inner edge of the disc. It turns out that the transfer direction of energy and angular omentum depends on the BH spin and a parameter λ for adjusting the angular velocities of the plunging matter, which corresponds to at most five regions in the disc. The effect of MCPD results in a much steeper emissivity than a standard accretion disc in the inner disc, however it fails to reach the observation range 4.3--5.5 in several objects, such as Seyfert 1 galaxy MCG-6-30-15, microquasars XTE J1650-500 and GX 399-4.
Abstract：We discuss two kinds of magnetic connection (MC) in the black hole (BH) accretion disc: the magnetic connection between the BH and the disc (MCHD) and that between the plunging region and the disc (MCPD). The magnetic field configuration is produced by an electric current flowing at the inner edge of the disc. It turns out that the transfer direction of energy and angular omentum depends on the BH spin and a parameter λ for adjusting the angular velocities of the plunging matter, which corresponds to at most five regions in the disc. The effect of MCPD results in a much steeper emissivity than a standard accretion disc in the inner disc, however it fails to reach the observation range 4.3--5.5 in several objects, such as Seyfert 1 galaxy MCG-6-30-15, microquasars XTE J1650-500 and GX 399-4.
(Galactic nuclei (including black holes), circumnuclear matter, and bulges)
引用本文:
LI Yang(李洋);WANG Ding-Xiong(汪定雄)$^{**}$;GANZhao-Ming. Two Kinds of Magnetic Connection in Black-Hole Accretion Disc[J]. 中国物理快报, 2007, 24(5): 1421-1424.
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2007, Vol. 24 
