Double-Period Gravitational Dynamics from a Multifractal Perspective of Motion

Assimilating complex systems to multifractal-type objects reveals continuous and non-differentiable curve dynamics, aligning with the Multifractal Theory of Motion. Two scenarios, a Schrödinger-type and a Madelung-type multifractal scenario, are possible in this setting. If the Madelung scenario employs maximized information entropy for a distribution density, then Newtonian and oscillator-type forces can be determined. In the presence of these forces and a matter background, we analyze the two-body problem. The obtained results are as follows: a generalized Hubble-type law, a dependence of Newton’s constant on the epoch and background density, a generalization of Lorentz transform (involving the Hubble constant, Newton’s constant, the speed of light, and cosmic matter density), etc. Moreover, in the same scenario, the functionality of a diffusion-type equation implies instabilities, such as period doubling, through an SL(2R) invariance. Thus, multiple infragalactic and extragalactic instabilities are exemplified.