Magnetically driven superluminal motion from rotating black holes Solution of the magnetic wind equation in Kerr metric
Magnetically driven superluminal motion from rotating black holes Solution of the magnetic wind equation in Kerr metric
We have investigated magnetically driven superluminal jets originating from rotating black holes. The stationary, general relativistic, magnetohydrodynamic wind equation along collimating magnetic flux surfaces has been solved numerically. Our jet solutions are calculated on a global scale of a spatial range from several to several 1000 gravitational radii. Dierent magnetic …