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New perspective about the existence of a supermassive black hole in a quasar with double redshift systems

Authors:

Basil Petropoulos Manos Mavrogiannis

Institution:

1. Research Center for Astronomy and Applied Mathematics, Academy of Athens, Greece

Abstract:

Research of several years has confirmed the general aspect that the most acceptable model in quasars' nuclei is a rotating Kerr black hole.Assuming the Kerr type potential given by the equation:

$V_{{\text{Kerr}}} (r) = 1 - \frac{1}{{r - r_0 }} + \frac{1}{2}\omega ^2 r^2 ,$

Keywords:
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