Rotating dust clouds in general relativity

Details Rotating dust clouds in general relativity Rotating dust clouds in general relativity

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008gregr..40..191b&link_type=abstract

General Relativity and Gravitation, Volume 40, Issue 1, pp.191-198

Physics

Rotating Dust, Angular Momentum

Scientific paper

We present an exact solution of Einstein’s equations representing interpenetrating clouds of rotating dust. The solution is a member of the van Stockum class; it contains singularities at the centres of the clouds. These are sources of the angular momentum which is displayed by the metric at infinity. It is not clear whether the rotating dust contributes to the angular momentum. In the case of two clouds there is a conical singularity between the central ones. For three clouds the conical singularity may be absent.

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