Stable Circular orbit in the Equatorial plane of Black hole
Shobha Lal
Broschiertes Buch

Stable Circular orbit in the Equatorial plane of Black hole

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A detailed study of the properties of time -like and Null geodesics, specially of stable circular orbits, in the charge free Kerr metric have been presented by Bardeen, has been made. In the case of Bardeen, the three direct orbits radius of marginally stable circular, radius of marginally bound orbit and radius for circular photon orbit, all seems to concide with the event horizon in extreme Kerr black hole. He has also obtained the three orbits rms= 6m, rmb=4m and rph=3m for schwarzs child metric. But in his case there are no circular orbits corresponding to rms=6m rmb=4m, and rph=3m, concid...