A substitute for the singular Green kernel in the Newtonian potential of celestial bodies
Jean-Marc Hur\'e, Andreas Dieckmann

TL;DR
The paper introduces an analytical method to replace the singular Green kernel in Newtonian gravity with a regularized kernel, improving the accuracy and efficiency of modeling gravitational potentials in celestial bodies.
Contribution
It presents a novel regularization technique using a 'cool kernel' and a 'hyperkernel' to handle singularities in gravitational potential calculations for continuous mass distributions.
Findings
The method effectively regularizes the Green kernel inside sources.
It maintains the correct asymptotic behavior of the potential.
Demonstrated accuracy with a flat circular disc model.
Abstract
The "point mass singularity" inherent in Newton's law for gravitation represents a major difficulty in accurately determining the potential and forces inside continuous bodies. Here we report a simple and efficient analytical method to bypass the singular Green kernel 1/|r-r'| inside the source without altering the nature of the interaction. We build an equivalent kernel made up of a "cool kernel", which is fully regular (and contains the long-range -GM/r asymptotic behavior), and the gradient of a "hyperkernel", which is also regular. Compared to the initial kernel, these two components are easily integrated over the source volume using standard numerical techniques. The demonstration is presented for three-dimensional distributions in cylindrical coordinates, which are well-suited to describing rotating bodies (stars, discs, asteroids, etc.) as commonly found in the Universe. An…
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