Abstract
The Blandford-Znajek (BZ) mechanism describes a physical process for the energy extraction from a spinning black hole (BH), which is believed to power a great variety of astrophysical sources, such as active galactic nuclei (AGNs) and Gamma ray bursts (GRBs). The only known analytic solution to the BZ mechanism is a split monopole perturbation solution up to , where is the spin parameter of a Kerr black hole. In this paper, we extend the monopole solution to higher order . We carefully investigate the structure of the BH magnetosphere, including the angular velocity of magnetic field lines , the toroidal magnetic field as well as the poloidal electric current . In addition, the relevant energy extraction rate and the stability of this high-order monopole perturbation solution are also examined.
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