Authors: Thierry De Mees
Black holes and fast spinning stars attract the surrounding objects in a different way than Newtonian gravity. As shown by my work on Gravitomagnetism , the spin of fast spinning stars and black holes is far the most important factor in the behavior of nearby objects. This paper shows that the accretion disc of any black hole is orbiting in prograde way. Moreover, it is explained that the accretion disc’s turbulence, curvature and quantity of the vortexes are predominant factors for the gravitational strength of a black hole. The measurement of the spin of a black hole depends mainly on this factor, and to a lesser extent, to a few other factors.
Comments: 3 Pages.
[v1] 2017-02-17 04:01:32
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