Robust numerical computation of the 3D scalar potential field of the cubic Galileon gravity model at solar system scales

1 code implementation • 2 Mar 2020 • Nicholas C. White, Sandra M. Troian, Jeffrey B. Jewell, Curt J. Cutler, Sheng-wey Chiow, Nan Yu

Here we present a numerical method based on finite differences for solution of the static CGG scalar field for a 2D axisymmetric Sun-Earth system and a 3D Cartesian Sun-Earth-Moon system.

Computational Physics