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- W3100206626 abstract "In the framework of a model based on the gravitational field of the Kerr black hole, we turn to investigate the kinematic behavior of extragalactic jets. We analytically calculate the observable velocities and accelerations along any geodesic. Then, by numerical calculations, we apply our results to a geodesic, typical of the M87 jet, and probe our results by confrontation to recent observations. A transition from non-relativistic to ultrarelativistic speeds at subparsec scale is highlighted. This transition comes sooner and more abruptly than in models based on magnetic paradigm, which indicates that we need a weaker magnetic field to explain observed synchrotron radiation. We attribute the ejection phenomenon to the repulsive effect of the gravitomagnetic Kerr field." @default.
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- W3100206626 date "2017-02-20" @default.
- W3100206626 modified "2023-10-09" @default.
- W3100206626 title "Observable acceleration of jets by a Kerr black hole" @default.
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- W3100206626 doi "https://doi.org/10.1007/s10714-017-2208-9" @default.
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