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
Unique-IP document downloads: 102 times
Add your own feedback and questions here:
You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.