Newtonion Quantum Gravity, WIMPs and Celestial Mechanics -- Summary of Results
Richard Durran, Andrew Neate, Aubrey Truman

TL;DR
This paper explores semi-classical quantum gravity in Newtonian settings, providing explicit solutions for various potentials, and discusses implications for planetary systems, galaxy evolution, and observable quantum effects in celestial mechanics.
Contribution
It introduces explicit solutions and a general implicit method for semi-classical equations in Newtonian quantum gravity, extending to multiple potentials and celestial phenomena.
Findings
Explicit solutions for isotropic harmonic oscillator potentials.
Insight into semi-classical orbit behavior near classical orbits.
Potential observable effects in planetary ring systems and galaxy evolution.
Abstract
We discuss the leading term in the semi-classical asymptotics of Newtonian quantum gravity for the Kepler problem. For dark matter, ice or dust particles in the gravitational field of a star or massive planet this explains how rapidly planets or ring systems can be formed by considering semi-classical equations for the asymptotic of the relevant Schrodinger wave function. We extend this treatment to isotropic harmonic oscillator potentials in two and three dimensions finding explicit solutions, with important applications to the Trojan asteroids. More detailed results on the restricted 3-body problem are in a forthcoming paper. Further in two dimensions, we find the explicit solutions for Newton's corresponding revolving orbits, explaining planetary perihelion advance in these terms. A general implicit approach to solving our equations is given using Cauchy characteristic curves giving…
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Pulsars and Gravitational Waves Research
