Astrophysics

    

The Viscous Coupling of Rotating Bodies by Tidal Forces a Proposal for an Extension of Newtonian Dynamics (End)

Authors: Thorsten Hilker

This work presents an approach to extending classical gravitational dynamics by modeling tidal forces between rotating celestial bodies as a viscous, velocity-dependent coupling. Using concrete examples (Earth—Moon, Earth—Sun, Mars—Phobos), it is shown that this coupling can explain observed distance changes. The application of this concept demonstrates the evolution of galactic rotation curves in a simulation without dark matter, thus offering an introduction to a potentially fundamental complement to Newtonian physics.

Comments: 16 Pages. In German (Note by viXra Admin: Please submit article written with AI assistance to ai.viXra.org)

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[v1] 2025-08-30 23:05:08

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