Analysis of the Non-singular Wyman-Schwarzschild Metric
Neil Cornish
TL;DR
This paper investigates a non-singular version of the Schwarzschild metric within Non-Singular Gravity, showing that it eliminates black holes, singularities, and Hawking radiation by ensuring finite curvatures and redshifts.
Contribution
It introduces an analytic framework for a non-singular Schwarzschild-like metric, removing singularities and black hole features in gravitational models.
Findings
All curvatures are finite, indicating no singularities.
Redshifts remain finite, preventing event horizon formation.
The spacetime lacks black holes and Hawking radiation.
Abstract
The analog of the Schwarzschild metric is explored in the context of Non-Singular Gravity. Analytic results are developed describing redshifts, curvatures and topological features of the spacetime. All curvatures and redshifts are finite so there are no Black Holes, no singularities and no Hawking radiation.
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