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• W2045861251 abstract "A jet acceleration model for extracting energy from disk-corona surrounding a rotating black hole (BH) is proposed. In the disk-corona scenario, we obtain the ratio of the power dissipated in the corona to the total for such disk-corona system by solving the disk dynamics equations. The analytical expression of the jet power is derived based on the electronic circuit theory of the magnetosphere. It is shown that jet power increases with the increasing BH spin, and concentrates in the inner region of the disk-corona. In addition, we use a sample consisting of 37 radio loud quasars to explore their jet production mechanism, and show that our jet formation mechanism can simulate almost all sources with high power jet, which fails to be explained by the Blandford-Znajek (BZ) process." @default.
• W2045861251 created "2016-06-24" @default.
• W2045861251 creator A5002139901 @default.
• W2045861251 creator A5089507526 @default.
• W2045861251 date "2012-03-25" @default.
• W2045861251 modified "2023-10-18" @default.
• W2045861251 title "Jet magnetically accelerated from disk-corona around a rotating black hole" @default.
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• W2045861251 doi "https://doi.org/10.1007/s11433-012-4705-x" @default.
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