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Solving the Three-Body Problem via the Dual Rotational Current Model

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Zenodo2026-01-08 更新2026-05-26 收录
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https://zenodo.org/doi/10.5281/zenodo.18186480
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This paper presents a deterministic solution to the Three-Body Problem based exclusively on the ”Dual Rotational Current Model.” Unlike classical mechanics which relies on point- mass attraction leading to chaotic variables, this model treats celestial bodies as nodes of concentrated magnetic currents within a symmetrical helical medium. By applying the principles of flux density and dual torque balance, trajectory prediction becomes a matter of calculating the geometric equilibrium of the vacuum fabric.
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Zenodo
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2026-01-08
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