Black hole uniqueness from a hidden symmetry of Einstein's gravity

Details Black hole uniqueness from a hidden symmetry of Einstein's gravity Black hole uniqueness from a hidden symmetry of Einstein's gravity

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984gregr..16..211m&link_type=abstract

General Relativity and Gravitation (ISSN 0001-7701), vol. 16, March 1984, p. 211-215.

Mathematics

Group Theory

25

Black Holes (Astronomy), Gravitation Theory, Maxwell Equation, Relativity, Uniqueness Theorem, Einstein Equations, Group Theory, Kerr Effects, Rotating Matter, Symmetry

Scientific paper

A theorem is proven that the only possible exterior solution for a pseudostationary, rotating, electrovacuum black hole with nondegenerate event horizon is the Kerr-Newman solution with M sq - J sq /M sq - Q sq greater than 0. A special role played in the proof of this theorem by the hidden symmetry group Su(1, 2) of Einstein's equations is established.

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