Singularity-Free Collapse through Local Inflation

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dc.creatorMonroe, Hunter
dc.date2005-06-21
dc.date2005-07-07
dc.date.accessioned2026-07-07T02:18:02Z
dc.date.available2026-07-07T02:18:02Z
dc.descriptionIn common relativistic models of gravitational collapse, the interior experiences a bubble-like local inflation, allowing radii to diverge rather than converge toward a singularity. This proves a conjecture of Shatskiy. At the horizon, the solution locally resembles the neck of a wormhole from the exterior to the interior. The implied limiting curvature is at the horizon not the Planck level.
dc.description11 pages. Paper prepared in honor of the retirement of L.R. King. This version shortens introduction
dc.identifierhttps://arxiv.org/abs/astro-ph/0506506
dc.identifierhttp://arxiv.org/abs/astro-ph/0506506
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9339
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleSingularity-Free Collapse through Local Inflation
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