We extend the static interior Schwarzschild solution to a
collapsing model by applying geometrical methods. We examine the field
quantities and field equations in the comoving and non-comoving observer
systems. The collapsing stellar object contracts asymptotically to its minimum
extent and needs an infinitely long time to arrive at the final state. The
event horizon of the exterior Schwarzschild solution is not reached or even
crossed. A geometric model of ECOs (eternally collapsing objects) is presented.
Author (s) Details Rainer Burghardt
Independent Researcher, Austria
View Book :- http://bp.bookpi.org/index.php/bpi/catalog/book/193
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