TL;DR
This paper examines the equations of a relativistic causal Newtonian gravity law applied to solar system planets, assuming a stationary Sun and non-interacting planets, to explore gravitational dynamics.
Contribution
It introduces a relativistic causal Newtonian gravity framework for planetary motion, focusing on simplified conditions with a fixed Sun and no planetary interactions.
Findings
Derived equations for planetary motion under the new gravity law.
Analyzed the approximation where the Sun is stationary.
Provided insights into relativistic effects in Newtonian gravity.
Abstract
The equations of the relativistic causal Newton gravity law for the planets of the solar system are studied in the approximation when the Sun rests at the coordinates origin and the planets do not iteract between each other.
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Taxonomy
TopicsRelativity and Gravitational Theory · Cosmology and Gravitation Theories · Geophysics and Gravity Measurements