A cylindrically symmetric solution of Einstein's equations describing gravitational collapse of stiff fluid.

Mathematics – Mathematical Physics

Scientific paper

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Scientific paper

This article presents a one-parameter solution of Einstein's equations that describes a stiff fluid in gravitational collapse with cylindrical symmetry. Two numerical examples of the physical parameters are given to describe (1) the collapse of a stiff fluid initially of nuclear density and of radius ≡20 km and (2) the contraction to a singularity of a cosmological distribution of stiff matter.

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