An intrinsic characterization of the Kerr metric

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

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15 pages; v2: necessary conditions added to theorems 1 and 2, other minor changes

Scientific paper

10.1088/0264-9381/26/7/075013

We give the necessary and sufficient (local) conditions for a metric tensor
to be the Kerr solution. These conditions exclusively involve explicit
concomitants of the Riemann tensor.

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