Strong-Field Behavior in the Graviton Wave Model

This document provides a comprehensive derivation of the strongfield behavior in the Graviton Wave Model (GWM) using a tensor wave field approach.The GWM, originally based on a scalar wave potential, is extended to a tensor fieldto replicate General Relativity’s (GR) predictions in strong gravitational fields, suchas those near black holes. We derive the tensor wave equation, solve it for a pointmass, and demonstrate how it reproduces GR’s key strong-field effects, including lightbending, orbital dynamics, and event horizon behavior.