On singularity-free spacetimes.

Computer Science

Scientific paper

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Cosmology: Space-Time

Scientific paper

The authors consider here the metric for the singularity-free family of fluid models. The metric is unique for cylindrically symmetric space-time with metric potentials being separable functions of radial and time coordinates in the comoving coordinates. It turns out that fluid models separate out into two classes, with ρ ≠ μp in general but ρ = 3ρ in particular and p = ρ. It is shown that in both the cases radial heat flow can be incorporated without disturbing the singularity-free character of the spacetime. The geodesics of the singularity-free metric are studied and the geodesic completeness is established. Several previously known solutions are derived as particular cases.

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