Properties of kinematic singularities

Details Properties of kinematic singularities Properties of kinematic singularities

2009-07-09

arxiv.org/abs/0907.1620v3

Class.Quant.Grav.26:215008,2009

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

13 pages. Published version. One sentence from version 2 corrected

Scientific paper

10.1088/0264-9381/26/21/215008

The locally rotationally symmetric tilted perfect fluid Bianchi type V cosmological model provides examples of future geodesically complete spacetimes that admit a `kinematic singularity' at which the fluid congruence is inextendible but all frame components of the Weyl and Ricci tensors remain bounded. We show that for any positive integer n there are examples of Bianchi type V spacetimes admitting a kinematic singularity such that the covariant derivatives of the Weyl and Ricci tensors up to the n-th order also stay bounded. We briefly discuss singularities in classical spacetimes.

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