Einstein-Grossmann geometry for frequency shifts of retrograde and direct orbits
Igor Bulyzhenkov

TL;DR
This paper explores how Einstein's geodesics in a rotating metric predict measurable frequency shifts and differences in orbital speeds for direct and retrograde orbits, extending classical gravity models.
Contribution
It introduces a novel application of Einstein-Grossmann geometry to explain frequency shifts and orbital differences in rotating gravitational systems.
Findings
Predicts Zeeman-like frequency shifts in Keplerian orbits
Shows measurable differences in orbital speeds of direct and retrograde orbits
Demonstrates the influence of metric gyro-potentials on orbital dynamics
Abstract
The metric gyro-potential of rotating distributions creates centripetal forces that can override Newtonian attraction on the inner and near-zone orbits. Einstein's geodesics in four metric potentials predict Zeeman-like shifts of Keplerian frequencies and measurable differences in the orbital speeds of direct and retrograde circulations.
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Taxonomy
TopicsSpacecraft Dynamics and Control · Astrophysics and Star Formation Studies · Astro and Planetary Science
