Edward Schaefer

Flat Background General Relativity

Flat Background Relativity assumes that solving the Einstein Field Equations (EFE) is not the final step in finding the metrics of spacetime. Instead its overall premise is that the physical metrics of spacetime are distortions of the EFE solutions in the direction of changing maximal clock rate such that their background metric becomes flat. Gravitational length contraction, the construction of background metrics from foreground metrics such as the EFE solutions, and how to find the distortion that flattens the background are described. The distortion of the Schwarzschild Solution is examined, and it is shown that the equations of motion for the distorted geometry prohibit entry into the Schwarzschild black hole coordinates.
Back to ECGM6 Program