Principle of Local Conservation of Energy-Momentum
Garret Sobczyk, Tolga Yarman

TL;DR
This paper derives equations of motion based on energy-momentum conservation, suggesting no singularities or blackholes exist, challenging traditional views in gravitational physics.
Contribution
It introduces a new derivation of equations of motion from energy-momentum conservation, eliminating singularities and blackholes in gravitational theory.
Findings
No singularities in the derived equations
Blackholes are not supported by this theory
Consistent with energy-momentum conservation principles
Abstract
Starting with Einstein's theory of special relativity and the principle that whenever a celestial body or an elementary particle, subjected only to the fundamental forces of nature, undergoes a change in its kinetic energy then the mass-energy equivalent of that kinetic energy must be subtracted from the rest-mass of the body or particle, we derive explicit equations of motion for two falling bodies. In the resulting mathematical theory we find that there are no singularities and consequently no blackholes.
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Taxonomy
TopicsAlgebraic and Geometric Analysis · Relativity and Gravitational Theory · Quantum and Classical Electrodynamics
