Solving the dark matter problem through dynamic interactions
Werner A. Hofer

TL;DR
This paper proposes a new model for dark matter based on dynamic interactions similar to magnetic fields, aiming to explain galactic rotation discrepancies without invoking unknown particles.
Contribution
It introduces a novel interaction-based model that accounts for galactic rotation curves and planetary orbit variations, challenging traditional dark matter particle hypotheses.
Findings
Model explains galactic rotation curves without dark matter particles
Interactions produce observable effects in planetary orbits
Fundamental constant characterizes the interaction strength
Abstract
Owing to the renewed interest in dark matter after the upgrade of the large hadron collider and its dedication to dark matter research it is timely to reassess the whole problem. Considering dark matter is one way to reconcile the discrepancy between the velocity of matter in the outer regions of galaxies and the observed galactic mass. So far, no credible candidate for dark matter has been identified. Here, we develop a model accounting for observations by rotations and interactions between rotating objects analogous to magnetic fields and interactions with moving charges. The magnitude of these fields is described by a fundamental constant of the order 10-41kg-1. The same interactions can be observed in the solar system where they lead to small changes in planetary orbits.
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