Authors: R. Wayte
Gravitational collapse of diffuse material has been investigated using a new solution of Einstein's equations of general relativity. This replaces the theory of black-hole formation developed for the standard vacuum solution of Schwarzschild. The bodies which now form have reasonable physical properties, such as nuclear hard core density in collapsed stars, or 104kg/l in galactic centres, and only 1kg/l in quasars. Accreting material converts to kinetic energy and radiation, so that a singularity cannot be produced.
Comments: 7 pages, Research artical submitted to PMC Physics A
[v1] 29 Oct 2010
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