Non-singular inhomogeneous stiff fluid cosmology

Details Non-singular inhomogeneous stiff fluid cosmology Non-singular inhomogeneous stiff fluid cosmology

2009-05-29

arxiv.org/abs/0905.4835v1

Published in Encuentros Relativistas Espa\~noles, Some Topics on General Relativity and Gravitational Radiation. Eds: J.A. Mir

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 pp. Proceedings of ERE'96

Scientific paper

In this talk we show a stiff fluid solution of the Einstein equations for a
cylindrically symmetric spacetime. The main features of this metric are that it
is non-separable in comoving coordinates for the congruence of the worldlineS
of the fluid and that it yields regular curvature invariants.

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