Numerical Spherically Symmetric Static Solution of the RTG Equations Outside the Matter

TL;DR

This paper presents a numerical solution to the RTG equations for a static, spherically symmetric spacetime outside matter, analyzing its properties and boundary conditions.

Contribution

It provides the first numerical external solution for the RTG equations in the static spherically symmetric case with natural boundary conditions.

Findings

Properties of the numerical solution are discussed.

The solution satisfies natural boundary conditions.

Insights into the behavior of RTG equations in spherical symmetry.

Abstract

There was obtained a numerical external solution for the exact system of the RTG equations with some natural boundary conditions in the static spherically symmetric case. The properties of the solution are discussed.