Dynamical 3-Space Gravity Theory: Effects on Polytropic Solar Models
Richard D May, Reginald T Cahill (Flinders University, Australia)

TL;DR
This paper discusses a dynamical 3-space gravity theory that explains various gravitational phenomena without dark matter or energy, and applies it to model the Sun's internal structure using polytropic models.
Contribution
It introduces a new gravity theory based on a velocity formalism and applies it to solar modeling, providing alternative explanations for gravitational effects.
Findings
Predicted solar density, pressure, and temperature profiles.
Explains galaxy rotation curves without dark matter.
Accounts for bore hole g anomalies and black hole masses.
Abstract
Numerous experiments and observations have confirmed the existence of a dynamical 3-space, detectable directly by light-speed anisotropy experiments, and indirectly by means of novel gravitational effects, such as bore hole g anomalies, predictable black hole masses, flat spiral-galaxy rotation curves, and the expansion of the universe, all without dark matter and dark energy. The dynamics for this 3-space follows from a unique generalisation of Newtonian gravity, once that is cast into a velocity formalism. This new theory of gravity is applied to the sun to compute new density, pressure and temperature profiles, using polytrope modelling of the equation of state for the matter. These results should be applied to a re-analysis of solar neutrino production, and to stellar evolution in general.
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Black Holes and Theoretical Physics
