Analysis of the Non-singular Wyman-Schwarzschild Metric
arXiv:gr-qc/9408009 · doi:10.1142/S0217732394003476
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.
14 pages, RevTeX, 6 Figures available on request, UTPT-94-16