Non-singular inhomogeneous stiff fluid cosmology
General Relativity and Quantum Cosmology
2009-06-01 v1
Abstract
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.
Keywords
Cite
@article{arxiv.0905.4835,
title = {Non-singular inhomogeneous stiff fluid cosmology},
author = {L. Fernández-Jambrina},
journal= {arXiv preprint arXiv:0905.4835},
year = {2009}
}
Comments
4 pp. Proceedings of ERE'96