Authors: Ben Steber
The Eddington-Finkelstein as a pair of coordinates have selectively allowed for solutions to the Schwarzschild metric which include singularity as well as a permeable event horizon. The author will demonstrate that the coordinates reduce to identities which remove tortoise coordinates from the field. Special Relativistic and General Relativistic principles will demonstrate the inaccessibility of the Event Horizon by massive particles, resulting in the removal of singularity. The Einstein-Rosen solution will establish a field free of singularities resulting in a drastically new model for the structure of black holes.
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[v1] 2015-01-06 21:58:21
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