A nonmetric theory of gravitation that is nonsingular at the Schwarzschild radius
James W. Douglass

TL;DR
This paper proposes a nonmetric gravitational theory that avoids singularities at the Schwarzschild radius, predicts that black holes are not black, and aligns with general relativity in weak fields but differs near black hole horizons.
Contribution
It introduces a new gravitational theory based on relativistic processes that eliminates singularities and predicts observable differences near black hole horizons.
Findings
The theory is a weak-field approximation to general relativity.
It predicts no singularity at the Schwarzschild radius.
Photons escape with a specific redshift, making black holes not black.
Abstract
A gravitational theory is formulated by considering the physical processes underlying relativistic dilation of time and contraction of space. It is shown that the point mass solution of general relativity's field equation - the Schwarzschild metric - is a weak-field approximation to the more general Lagrangian resulting here. Unlike general relativity the resulting theory does not exhibit a singularity at the Schwarzschild radius and furthermore shows that photons escape from that radius with a red shift of e^0.5 - 1. Consequently black holes are not black. Experimental confirmations of general relativity that have been conducted in the weak field domain may also be considered as confirmations of the theory presented here since the two theories provide nearly identical predictions there. Testable differentiation of these two theories will require observations in the near vicinity of the…
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Pulsars and Gravitational Waves Research
