Chaos in a quasar model with a disk and a massive nucleus

Astronomy and Astrophysics – Astronomy

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Galaxies: Kinematics And Dynamics

Scientific paper

We present a quasar model with a rotating disk and a massive nucleus. We use this model in order to characterize the motion in the model (regular or chaotic) and to connect the extent of the chaotic regions to the physical parameters of the model. Numerical experiments suggest that, there are connections between the extent of the chaotic areas and the parameters of the system. Furthermore, it is shown that the form of numerically found relationships can be expressed analytically. Comparison to previous work is also made.

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