A Potential Barrier Halting Spherically Symmetric Relativistic Gravitational Collapse
Geodesic pathways of radially inbound photons in a Schwarzschild space-time approach the critical radius of a collapsed star asymptotically for asymptotic observers. Inbound null geodesics in a matching Vaidya space-time, however, pass through a temporary inflection point when time dilation diverges and then reach the critical radius within a...
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