On the intrinsic labeling of space-times: a characterization of the Kerr solution

Details On the intrinsic labeling of space-times: a characterization of the Kerr solution On the intrinsic labeling of space-times: a characterization of the Kerr solution

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1122..268f&link_type=abstract

PHYSICS AND MATHEMATICS OF GRAVITATION: Proceedings of the Spanish Relativity Meeting 2008. AIP Conference Proceedings, Volume

Mathematics

Electrooptical Effects, Riemannian Geometries, Approximation Methods, Equations Of Motion

Scientific paper

The interest of obtaining an intrinsic (depending solely on the metric
tensor) and fully explicit characterization of a space-time is pointed
out. We give the necessary and sufficient (local) conditions for a
metric tensor to be the Kerr solution. These conditions exclusively
involve concomitants of the Weyl tensor.

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